- ``CALDB`` (example: ``CALDB = 1dc``)
- ``IRF`` (example: ``IRF = South_z20_50h``)
- This method is useful specifically if you want to load data simulated
- with `ctobssim`_.
-
- .. _ctobssim: http://cta.irap.omp.eu/ctools/users/reference_manual/ctobssim.html
-
Parameters
----------
events_paths : list of str or `~pathlib.Path`
@@ -1296,7 +1291,6 @@ Source code for gammapy.data.data_store
yield dict(HDU_TYPE="bkg", HDU_CLASS="bkg_3d", HDU_NAME="BACKGROUND", **info)
-# TODO: load IRF file, and infer HDU_CLASS from IRF file contents!
class CalDBIRF:
"""Helper class to work with IRFs in CALDB format."""
diff --git a/docs/dev/_modules/gammapy/irf/edisp/map.html b/docs/dev/_modules/gammapy/irf/edisp/map.html
index 6175fdd40b8..0b3b70d2b91 100644
--- a/docs/dev/_modules/gammapy/irf/edisp/map.html
+++ b/docs/dev/_modules/gammapy/irf/edisp/map.html
@@ -574,7 +574,7 @@ Source code for gammapy.irf.edisp.map
--------
::
- # Energy dispersion map for CTA data
+ # Energy dispersion map for CTAO data
import numpy as np
from astropy import units as u
from astropy.coordinates import SkyCoord
diff --git a/docs/dev/_modules/gammapy/irf/effective_area.html b/docs/dev/_modules/gammapy/irf/effective_area.html
index 0c11b899503..6fce7fe1b0b 100644
--- a/docs/dev/_modules/gammapy/irf/effective_area.html
+++ b/docs/dev/_modules/gammapy/irf/effective_area.html
@@ -536,6 +536,7 @@
Source code for gammapy.irf.effective_area
# Licensed under a 3-clause BSD style license - see LICENSE.rst
+import warnings
import numpy as np
import astropy.units as u
from astropy.visualization import quantity_support
@@ -544,6 +545,7 @@ Source code for gammapy.irf.effective_area
from gammapy.maps.axes import UNIT_STRING_FORMAT
from gammapy.visualization.utils import add_colorbar
from .core import IRF
+from gammapy.utils.deprecation import GammapyDeprecationWarning
__all__ = ["EffectiveAreaTable2D"]
@@ -792,7 +794,7 @@ Source code for gammapy.irf.effective_area
energy_axis_true : `MapAxis`, optional
Energy binning, analytic function is evaluated at log centers.
Default is None.
- instrument : {'HESS', 'HESS2', 'CTA'}
+ instrument : {'HESS', 'HESS2', 'CTAO'}
Instrument name. Default is 'HESS'.
Returns
@@ -805,9 +807,15 @@ Source code for gammapy.irf.effective_area
pars = {
"HESS": [6.85e9, 0.0891, 5e5],
"HESS2": [2.05e9, 0.0891, 1e5],
- "CTA": [1.71e11, 0.0891, 1e5],
+ "CTAO": [1.71e11, 0.0891, 1e5],
}
+ if instrument == "CTA":
+ instrument = "CTAO"
+ warnings.warn(
+ "Since v1.3, the value 'CTA' is replaced by 'CTAO' for the argument instrument.",
+ GammapyDeprecationWarning,
+ )
if instrument not in pars.keys():
ss = f"Unknown instrument: {instrument}\n"
ss += f"Valid instruments: {list(pars.keys())}"
diff --git a/docs/dev/_modules/gammapy/makers/map.html b/docs/dev/_modules/gammapy/makers/map.html
index 3488a149b38..398dcca835a 100644
--- a/docs/dev/_modules/gammapy/makers/map.html
+++ b/docs/dev/_modules/gammapy/makers/map.html
@@ -573,7 +573,7 @@ Source code for gammapy.makers.map
Background evaluation oversampling factor in energy.
background_interp_missing_data : bool, optional
Interpolate missing values in background 3d map.
- Default is True, have to be set to True for CTA IRF.
+ Default is True, have to be set to True for CTAO IRF.
background_pad_offset : bool, optional
Pad one bin in offset for 2d background map.
This avoids extrapolation at edges and use the nearest value.
diff --git a/docs/dev/_modules/gammapy/modeling/models/spectral_cosmic_ray.html b/docs/dev/_modules/gammapy/modeling/models/spectral_cosmic_ray.html
index 6589190b9f1..786f2d8c5a0 100644
--- a/docs/dev/_modules/gammapy/modeling/models/spectral_cosmic_ray.html
+++ b/docs/dev/_modules/gammapy/modeling/models/spectral_cosmic_ray.html
@@ -539,7 +539,7 @@ Source code for gammapy.modeling.models.spectral_cosmic_ray
"""Simple models for cosmic ray spectra at Earth.
For measurements, the "Database of Charged Cosmic Rays (CRDB)" is a great resource:
-
http://lpsc.in2p3.fr/cosmic-rays-db/
+
https://lpsc.in2p3.fr/crdb/
"""
import numpy as np
from astropy import units as u
@@ -576,7 +576,7 @@
Source code for gammapy.modeling.models.spectral_cosmic_ray
def
create_cosmic_ray_spectral_model(particle="proton"):
"""Cosmic a cosmic ray spectral model at Earth.
-
These are the spectra assumed in this CTA study:
+
These are the spectra assumed in this CTAO study:
Table 3 in https://ui.adsabs.harvard.edu/abs/2013APh....43..171B
The spectrum given is a differential flux ``dnde`` in units of
diff --git a/docs/dev/_sources/development/dev_howto.rst.txt b/docs/dev/_sources/development/dev_howto.rst.txt
index 4f4d210c893..86450c64b9a 100644
--- a/docs/dev/_sources/development/dev_howto.rst.txt
+++ b/docs/dev/_sources/development/dev_howto.rst.txt
@@ -70,9 +70,12 @@ Notes:
Gammapy names defined here, to the names used in the formats.
Of course, where formats are not set in stone yet, we advocate and encourage
the use of the names chosen here.
-* Finally, we realise that eventually probably CTA will define this, and Gammapy
- is only a prototype. So if CTA chooses something else, probably we will follow
- suite and do one more backward-incompatible change at some point to align with CTA.
+* Finally, CTAO has proposed a full data model associated to the needed quantities. And
+ the community is working to create a data format for very-high-energy data produced by gamma-ray
+ and neutrino experiments within the open initiative `Very-high-energy Open Data Format`_. This format
+ aims to respect the CTAO data model, to respect the `FAIR principles`_ and to follow as much as
+ possible the `IVOA`_ recommendations. In order to handle past, current and old formats,
+ Gammapy should follow the `FAIR4RS principles`_ by proposing a user-friendly interface.
Clobber or overwrite?
+++++++++++++++++++++
diff --git a/docs/dev/_sources/development/release.rst.txt b/docs/dev/_sources/development/release.rst.txt
index 09774995204..bf558988b55 100644
--- a/docs/dev/_sources/development/release.rst.txt
+++ b/docs/dev/_sources/development/release.rst.txt
@@ -90,9 +90,8 @@ Steps for the day to announce the release:
(decide on a case by case basis, if it's relevant to the group of people):
* https://groups.google.com/forum/#!forum/astropy-dev
- * https://lists.nasa.gov/mailman/listinfo/open-gamma-ray-astro
- * CTA DATA list (cta-wp-dm@cta-observatory.org)
- * hess-analysis
+ * CTAO AS WG list (cta-wg-as [at] cta-observatory [dot] org)
+ * hess-forum list (hess-forum [at] lsw.uni-heidelberg [dot] de)
#. Make sure the release milestone and issue is closed on GitHub
#. Update these release notes with any useful infos / steps that you learned
while making the release (ideally try to script / automate the task or check,
diff --git a/docs/dev/_sources/index.rst.txt b/docs/dev/_sources/index.rst.txt
index 2fe2c37e2ed..1339b7d8163 100644
--- a/docs/dev/_sources/index.rst.txt
+++ b/docs/dev/_sources/index.rst.txt
@@ -18,7 +18,7 @@ Gammapy
Gammapy is a community-developed, open-source Python package for gamma-ray
-astronomy built on Numpy, Scipy and Astropy. **It is the core library for the** `CTA`_ **Science Tools**
+astronomy built on Numpy, Scipy and Astropy. **It is the core library for the** `CTAO`_ **Science Tools**
but can also be used to analyse data from existing imaging atmospheric Cherenkov telescopes
(IACTs), such as `H.E.S.S.`_, `MAGIC`_ and `VERITAS`_. It also provides some support
for `Fermi-LAT`_ and `HAWC`_ data analysis.
diff --git a/docs/dev/_sources/sg_execution_times.rst.txt b/docs/dev/_sources/sg_execution_times.rst.txt
index d7fa9ebb350..e03c6ef51ef 100644
--- a/docs/dev/_sources/sg_execution_times.rst.txt
+++ b/docs/dev/_sources/sg_execution_times.rst.txt
@@ -6,7 +6,7 @@
Computation times
=================
-**09:53.580** total execution time for 84 files **from all galleries**:
+**10:02.876** total execution time for 84 files **from all galleries**:
.. container::
@@ -33,254 +33,254 @@ Computation times
- Time
- Mem (MB)
* - :ref:`sphx_glr_tutorials_api_priors.py` (``../examples/tutorials/api/priors.py``)
- - 01:21.171
+ - 01:27.538
- 0.0
* - :ref:`sphx_glr_tutorials_analysis-1d_spectral_analysis.py` (``../examples/tutorials/analysis-1d/spectral_analysis.py``)
- - 00:44.699
+ - 00:44.094
- 0.0
* - :ref:`sphx_glr_tutorials_analysis-3d_analysis_3d.py` (``../examples/tutorials/analysis-3d/analysis_3d.py``)
- - 00:37.983
+ - 00:37.871
- 0.0
* - :ref:`sphx_glr_tutorials_analysis-time_light_curve_flare.py` (``../examples/tutorials/analysis-time/light_curve_flare.py``)
- - 00:34.207
+ - 00:33.442
- 0.0
* - :ref:`sphx_glr_tutorials_api_astro_dark_matter.py` (``../examples/tutorials/api/astro_dark_matter.py``)
- - 00:28.155
+ - 00:27.997
- 0.0
- * - :ref:`sphx_glr_tutorials_analysis-time_Time_resolved_spectroscopy.py` (``../examples/tutorials/analysis-time/Time_resolved_spectroscopy.py``)
- - 00:21.382
+ * - :ref:`sphx_glr_tutorials_analysis-3d_event_sampling.py` (``../examples/tutorials/analysis-3d/event_sampling.py``)
+ - 00:26.961
- 0.0
- * - :ref:`sphx_glr_tutorials_analysis-3d_flux_profiles.py` (``../examples/tutorials/analysis-3d/flux_profiles.py``)
- - 00:21.171
+ * - :ref:`sphx_glr_tutorials_analysis-time_light_curve_simulation.py` (``../examples/tutorials/analysis-time/light_curve_simulation.py``)
+ - 00:21.166
- 0.0
- * - :ref:`sphx_glr_tutorials_analysis-2d_detect.py` (``../examples/tutorials/analysis-2d/detect.py``)
- - 00:20.870
+ * - :ref:`sphx_glr_tutorials_analysis-time_Time_resolved_spectroscopy.py` (``../examples/tutorials/analysis-time/Time_resolved_spectroscopy.py``)
+ - 00:21.126
- 0.0
- * - :ref:`sphx_glr_tutorials_analysis-3d_energy_dependent_estimation.py` (``../examples/tutorials/analysis-3d/energy_dependent_estimation.py``)
- - 00:19.804
+ * - :ref:`sphx_glr_tutorials_analysis-2d_detect.py` (``../examples/tutorials/analysis-2d/detect.py``)
+ - 00:20.552
- 0.0
- * - :ref:`sphx_glr_tutorials_analysis-time_light_curve_simulation.py` (``../examples/tutorials/analysis-time/light_curve_simulation.py``)
- - 00:18.165
+ * - :ref:`sphx_glr_tutorials_analysis-3d_flux_profiles.py` (``../examples/tutorials/analysis-3d/flux_profiles.py``)
+ - 00:20.547
- 0.0
- * - :ref:`sphx_glr_tutorials_analysis-3d_event_sampling.py` (``../examples/tutorials/analysis-3d/event_sampling.py``)
- - 00:17.717
+ * - :ref:`sphx_glr_tutorials_analysis-3d_energy_dependent_estimation.py` (``../examples/tutorials/analysis-3d/energy_dependent_estimation.py``)
+ - 00:19.657
- 0.0
* - :ref:`sphx_glr_tutorials_analysis-3d_cta_data_analysis.py` (``../examples/tutorials/analysis-3d/cta_data_analysis.py``)
- - 00:17.287
+ - 00:16.841
- 0.0
* - :ref:`sphx_glr_tutorials_starting_analysis_1.py` (``../examples/tutorials/starting/analysis_1.py``)
- - 00:15.384
+ - 00:15.326
- 0.0
* - :ref:`sphx_glr_tutorials_api_makers.py` (``../examples/tutorials/api/makers.py``)
- - 00:15.214
+ - 00:15.013
- 0.0
* - :ref:`sphx_glr_tutorials_api_datasets.py` (``../examples/tutorials/api/datasets.py``)
- - 00:14.906
+ - 00:13.751
- 0.0
* - :ref:`sphx_glr_tutorials_analysis-2d_ring_background.py` (``../examples/tutorials/analysis-2d/ring_background.py``)
- - 00:12.115
+ - 00:12.100
- 0.0
* - :ref:`sphx_glr_tutorials_api_fitting.py` (``../examples/tutorials/api/fitting.py``)
- - 00:11.540
+ - 00:11.367
- 0.0
* - :ref:`sphx_glr_tutorials_api_model_management.py` (``../examples/tutorials/api/model_management.py``)
- - 00:10.396
+ - 00:10.361
- 0.0
* - :ref:`sphx_glr_tutorials_analysis-3d_simulate_3d.py` (``../examples/tutorials/analysis-3d/simulate_3d.py``)
- - 00:10.129
+ - 00:09.965
- 0.0
* - :ref:`sphx_glr_tutorials_analysis-1d_spectral_analysis_hli.py` (``../examples/tutorials/analysis-1d/spectral_analysis_hli.py``)
- - 00:08.080
+ - 00:07.829
- 0.0
* - :ref:`sphx_glr_tutorials_starting_analysis_2.py` (``../examples/tutorials/starting/analysis_2.py``)
- - 00:07.749
+ - 00:07.665
- 0.0
* - :ref:`sphx_glr_tutorials_analysis-time_light_curve.py` (``../examples/tutorials/analysis-time/light_curve.py``)
- - 00:07.519
+ - 00:07.502
- 0.0
* - :ref:`sphx_glr_tutorials_analysis-1d_spectrum_simulation.py` (``../examples/tutorials/analysis-1d/spectrum_simulation.py``)
- - 00:07.312
- - 0.0
- * - :ref:`sphx_glr_tutorials_data_hawc.py` (``../examples/tutorials/data/hawc.py``)
- - 00:07.256
+ - 00:07.149
- 0.0
* - :ref:`sphx_glr_tutorials_analysis-1d_ebl.py` (``../examples/tutorials/analysis-1d/ebl.py``)
- - 00:07.003
+ - 00:06.985
- 0.0
* - :ref:`sphx_glr_tutorials_api_estimators.py` (``../examples/tutorials/api/estimators.py``)
- - 00:06.947
+ - 00:06.718
+ - 0.0
+ * - :ref:`sphx_glr_tutorials_data_hawc.py` (``../examples/tutorials/data/hawc.py``)
+ - 00:06.689
- 0.0
* - :ref:`sphx_glr_tutorials_analysis-3d_analysis_mwl.py` (``../examples/tutorials/analysis-3d/analysis_mwl.py``)
- - 00:06.759
+ - 00:06.606
- 0.0
* - :ref:`sphx_glr_tutorials_data_fermi_lat.py` (``../examples/tutorials/data/fermi_lat.py``)
- - 00:06.673
+ - 00:06.263
- 0.0
* - :ref:`sphx_glr_tutorials_analysis-time_pulsar_analysis.py` (``../examples/tutorials/analysis-time/pulsar_analysis.py``)
- - 00:06.579
+ - 00:06.235
- 0.0
* - :ref:`sphx_glr_tutorials_api_catalog.py` (``../examples/tutorials/api/catalog.py``)
- - 00:06.157
+ - 00:06.077
- 0.0
* - :ref:`sphx_glr_tutorials_analysis-2d_modeling_2D.py` (``../examples/tutorials/analysis-2d/modeling_2D.py``)
- - 00:05.661
- - 0.0
- * - :ref:`sphx_glr_tutorials_data_cta.py` (``../examples/tutorials/data/cta.py``)
- - 00:05.525
+ - 00:05.541
- 0.0
* - :ref:`sphx_glr_tutorials_analysis-1d_sed_fitting.py` (``../examples/tutorials/analysis-1d/sed_fitting.py``)
- - 00:05.362
+ - 00:05.263
- 0.0
- * - :ref:`sphx_glr_tutorials_analysis-1d_spectral_analysis_rad_max.py` (``../examples/tutorials/analysis-1d/spectral_analysis_rad_max.py``)
- - 00:04.474
+ * - :ref:`sphx_glr_tutorials_data_cta.py` (``../examples/tutorials/data/cta.py``)
+ - 00:05.234
- 0.0
* - :ref:`sphx_glr_tutorials_analysis-1d_extended_source_spectral_analysis.py` (``../examples/tutorials/analysis-1d/extended_source_spectral_analysis.py``)
- - 00:04.330
+ - 00:04.301
+ - 0.0
+ * - :ref:`sphx_glr_tutorials_analysis-1d_spectral_analysis_rad_max.py` (``../examples/tutorials/analysis-1d/spectral_analysis_rad_max.py``)
+ - 00:04.195
- 0.0
* - :ref:`sphx_glr_tutorials_api_observation_clustering.py` (``../examples/tutorials/api/observation_clustering.py``)
- - 00:03.955
+ - 00:03.875
- 0.0
* - :ref:`sphx_glr_tutorials_api_irfs.py` (``../examples/tutorials/api/irfs.py``)
- - 00:03.852
+ - 00:03.804
- 0.0
* - :ref:`sphx_glr_tutorials_data_hess.py` (``../examples/tutorials/data/hess.py``)
- - 00:03.605
- - 0.0
- * - :ref:`sphx_glr_tutorials_api_models.py` (``../examples/tutorials/api/models.py``)
- - 00:03.150
+ - 00:03.259
- 0.0
* - :ref:`sphx_glr_tutorials_analysis-3d_event_sampling_nrg_depend_models.py` (``../examples/tutorials/analysis-3d/event_sampling_nrg_depend_models.py``)
- - 00:02.958
+ - 00:02.891
- 0.0
* - :ref:`sphx_glr_tutorials_api_maps.py` (``../examples/tutorials/api/maps.py``)
- - 00:02.746
+ - 00:02.716
+ - 0.0
+ * - :ref:`sphx_glr_tutorials_api_models.py` (``../examples/tutorials/api/models.py``)
+ - 00:02.624
- 0.0
* - :ref:`sphx_glr_tutorials_scripts_survey_map.py` (``../examples/tutorials/scripts/survey_map.py``)
- - 00:02.511
+ - 00:02.499
- 0.0
* - :ref:`sphx_glr_tutorials_api_mask_maps.py` (``../examples/tutorials/api/mask_maps.py``)
- - 00:02.337
+ - 00:02.315
- 0.0
* - :ref:`sphx_glr_tutorials_starting_overview.py` (``../examples/tutorials/starting/overview.py``)
- - 00:01.267
+ - 00:01.360
- 0.0
* - :ref:`sphx_glr_user-guide_model-gallery_spectral_plot_absorbed.py` (``../examples/models/spectral/plot_absorbed.py``)
- - 00:01.001
+ - 00:01.055
- 0.0
* - :ref:`sphx_glr_tutorials_analysis-1d_cta_sensitivity.py` (``../examples/tutorials/analysis-1d/cta_sensitivity.py``)
- - 00:00.833
- - 0.0
- * - :ref:`sphx_glr_tutorials_analysis-time_Variability_estimation.py` (``../examples/tutorials/analysis-time/Variability_estimation.py``)
- - 00:00.659
+ - 00:00.825
- 0.0
* - :ref:`sphx_glr_user-guide_model-gallery_temporal_plot_constant_temporal.py` (``../examples/models/temporal/plot_constant_temporal.py``)
- - 00:00.579
+ - 00:00.752
+ - 0.0
+ * - :ref:`sphx_glr_tutorials_analysis-time_Variability_estimation.py` (``../examples/tutorials/analysis-time/Variability_estimation.py``)
+ - 00:00.596
- 0.0
* - :ref:`sphx_glr_user-guide_model-gallery_spectral_plot_template_spectral.py` (``../examples/models/spectral/plot_template_spectral.py``)
- - 00:00.449
+ - 00:00.446
- 0.0
* - :ref:`sphx_glr_user-guide_model-gallery_spectral_plot_naima.py` (``../examples/models/spectral/plot_naima.py``)
- - 00:00.430
+ - 00:00.419
- 0.0
* - :ref:`sphx_glr_user-guide_model-gallery_spatial_plot_constant.py` (``../examples/models/spatial/plot_constant.py``)
- - 00:00.352
+ - 00:00.369
- 0.0
* - :ref:`sphx_glr_user-guide_model-gallery_spectral_plot_exp_cutoff_powerlaw_norm_spectral.py` (``../examples/models/spectral/plot_exp_cutoff_powerlaw_norm_spectral.py``)
- - 00:00.345
+ - 00:00.343
- 0.0
- * - :ref:`sphx_glr_user-guide_model-gallery_spectral_plot_broken_powerlaw.py` (``../examples/models/spectral/plot_broken_powerlaw.py``)
+ * - :ref:`sphx_glr_user-guide_model-gallery_spectral_plot_powerlaw.py` (``../examples/models/spectral/plot_powerlaw.py``)
- 00:00.331
- 0.0
- * - :ref:`sphx_glr_user-guide_model-gallery_spectral_plot_compound.py` (``../examples/models/spectral/plot_compound.py``)
- - 00:00.327
+ * - :ref:`sphx_glr_user-guide_model-gallery_spectral_plot_powerlaw2.py` (``../examples/models/spectral/plot_powerlaw2.py``)
+ - 00:00.324
- 0.0
* - :ref:`sphx_glr_user-guide_model-gallery_spectral_plot_smooth_broken_powerlaw.py` (``../examples/models/spectral/plot_smooth_broken_powerlaw.py``)
- - 00:00.327
- - 0.0
- * - :ref:`sphx_glr_user-guide_model-gallery_spectral_plot_powerlaw2.py` (``../examples/models/spectral/plot_powerlaw2.py``)
- - 00:00.326
+ - 00:00.321
- 0.0
- * - :ref:`sphx_glr_user-guide_model-gallery_spectral_plot_powerlaw.py` (``../examples/models/spectral/plot_powerlaw.py``)
+ * - :ref:`sphx_glr_user-guide_model-gallery_spectral_plot_broken_powerlaw.py` (``../examples/models/spectral/plot_broken_powerlaw.py``)
- 00:00.321
- 0.0
- * - :ref:`sphx_glr_user-guide_model-gallery_spatial_plot_disk.py` (``../examples/models/spatial/plot_disk.py``)
- - 00:00.317
+ * - :ref:`sphx_glr_user-guide_model-gallery_spectral_plot_compound.py` (``../examples/models/spectral/plot_compound.py``)
+ - 00:00.320
- 0.0
- * - :ref:`sphx_glr_user-guide_model-gallery_spectral_plot_logparabola_norm_spectral.py` (``../examples/models/spectral/plot_logparabola_norm_spectral.py``)
- - 00:00.299
+ * - :ref:`sphx_glr_user-guide_model-gallery_spatial_plot_disk.py` (``../examples/models/spatial/plot_disk.py``)
+ - 00:00.319
- 0.0
* - :ref:`sphx_glr_user-guide_model-gallery_spectral_plot_powerlaw_norm_spectral.py` (``../examples/models/spectral/plot_powerlaw_norm_spectral.py``)
- 00:00.274
- 0.0
+ * - :ref:`sphx_glr_user-guide_model-gallery_spectral_plot_logparabola_norm_spectral.py` (``../examples/models/spectral/plot_logparabola_norm_spectral.py``)
+ - 00:00.271
+ - 0.0
* - :ref:`sphx_glr_user-guide_model-gallery_spectral_plot_constant_spectral.py` (``../examples/models/spectral/plot_constant_spectral.py``)
- - 00:00.242
+ - 00:00.239
- 0.0
* - :ref:`sphx_glr_user-guide_model-gallery_spatial_plot_template.py` (``../examples/models/spatial/plot_template.py``)
- 00:00.229
- 0.0
- * - :ref:`sphx_glr_user-guide_model-gallery_spectral_plot_piecewise_norm_spectral.py` (``../examples/models/spectral/plot_piecewise_norm_spectral.py``)
- - 00:00.227
- - 0.0
* - :ref:`sphx_glr_user-guide_model-gallery_spectral_plot_super_exp_cutoff_powerlaw_4fgl.py` (``../examples/models/spectral/plot_super_exp_cutoff_powerlaw_4fgl.py``)
- - 00:00.226
+ - 00:00.228
+ - 0.0
+ * - :ref:`sphx_glr_user-guide_model-gallery_spectral_plot_piecewise_norm_spectral.py` (``../examples/models/spectral/plot_piecewise_norm_spectral.py``)
+ - 00:00.225
- 0.0
* - :ref:`sphx_glr_user-guide_model-gallery_spatial_plot_gen_gauss.py` (``../examples/models/spatial/plot_gen_gauss.py``)
- 00:00.224
- 0.0
* - :ref:`sphx_glr_user-guide_model-gallery_spectral_plot_super_exp_cutoff_powerlaw_4fgl_dr1.py` (``../examples/models/spectral/plot_super_exp_cutoff_powerlaw_4fgl_dr1.py``)
- - 00:00.223
+ - 00:00.219
- 0.0
* - :ref:`sphx_glr_user-guide_model-gallery_spectral_plot_super_exp_cutoff_powerlaw_3fgl.py` (``../examples/models/spectral/plot_super_exp_cutoff_powerlaw_3fgl.py``)
- - 00:00.222
+ - 00:00.219
- 0.0
* - :ref:`sphx_glr_user-guide_model-gallery_spectral_plot_gauss_spectral.py` (``../examples/models/spectral/plot_gauss_spectral.py``)
- - 00:00.221
+ - 00:00.217
- 0.0
* - :ref:`sphx_glr_user-guide_model-gallery_spatial_plot_gauss.py` (``../examples/models/spatial/plot_gauss.py``)
- - 00:00.215
+ - 00:00.211
- 0.0
* - :ref:`sphx_glr_user-guide_model-gallery_spectral_plot_exp_cutoff_powerlaw.py` (``../examples/models/spectral/plot_exp_cutoff_powerlaw.py``)
- - 00:00.209
+ - 00:00.206
- 0.0
* - :ref:`sphx_glr_user-guide_model-gallery_spectral_plot_logparabola.py` (``../examples/models/spectral/plot_logparabola.py``)
- - 00:00.208
+ - 00:00.204
- 0.0
* - :ref:`sphx_glr_user-guide_model-gallery_spectral_plot_exp_cutoff_powerlaw_3fgl.py` (``../examples/models/spectral/plot_exp_cutoff_powerlaw_3fgl.py``)
- - 00:00.206
+ - 00:00.203
- 0.0
* - :ref:`sphx_glr_user-guide_model-gallery_spatial_plot_point.py` (``../examples/models/spatial/plot_point.py``)
- - 00:00.203
+ - 00:00.201
- 0.0
* - :ref:`sphx_glr_user-guide_model-gallery_temporal_plot_powerlaw_temporal.py` (``../examples/models/temporal/plot_powerlaw_temporal.py``)
- - 00:00.193
+ - 00:00.195
- 0.0
* - :ref:`sphx_glr_user-guide_model-gallery_spatial_plot_shell.py` (``../examples/models/spatial/plot_shell.py``)
- - 00:00.186
+ - 00:00.185
- 0.0
* - :ref:`sphx_glr_user-guide_model-gallery_spatial_plot_shell2.py` (``../examples/models/spatial/plot_shell2.py``)
- 00:00.177
- 0.0
* - :ref:`sphx_glr_user-guide_model-gallery_spatial_plot_piecewise_norm_spatial.py` (``../examples/models/spatial/plot_piecewise_norm_spatial.py``)
- - 00:00.146
+ - 00:00.143
- 0.0
* - :ref:`sphx_glr_user-guide_model-gallery_temporal_plot_template_phase_temporal.py` (``../examples/models/temporal/plot_template_phase_temporal.py``)
- - 00:00.123
+ - 00:00.129
- 0.0
* - :ref:`sphx_glr_user-guide_model-gallery_temporal_plot_template_temporal.py` (``../examples/models/temporal/plot_template_temporal.py``)
- 00:00.121
- 0.0
* - :ref:`sphx_glr_user-guide_model-gallery_temporal_plot_generalized_gaussian_temporal.py` (``../examples/models/temporal/plot_generalized_gaussian_temporal.py``)
- - 00:00.114
+ - 00:00.111
- 0.0
- * - :ref:`sphx_glr_user-guide_model-gallery_temporal_plot_gaussian_temporal.py` (``../examples/models/temporal/plot_gaussian_temporal.py``)
+ * - :ref:`sphx_glr_user-guide_model-gallery_temporal_plot_sine_temporal.py` (``../examples/models/temporal/plot_sine_temporal.py``)
- 00:00.110
- 0.0
- * - :ref:`sphx_glr_user-guide_model-gallery_temporal_plot_expdecay_temporal.py` (``../examples/models/temporal/plot_expdecay_temporal.py``)
- - 00:00.110
+ * - :ref:`sphx_glr_user-guide_model-gallery_temporal_plot_gaussian_temporal.py` (``../examples/models/temporal/plot_gaussian_temporal.py``)
+ - 00:00.109
- 0.0
- * - :ref:`sphx_glr_user-guide_model-gallery_temporal_plot_sine_temporal.py` (``../examples/models/temporal/plot_sine_temporal.py``)
- - 00:00.108
+ * - :ref:`sphx_glr_user-guide_model-gallery_temporal_plot_expdecay_temporal.py` (``../examples/models/temporal/plot_expdecay_temporal.py``)
+ - 00:00.109
- 0.0
* - :ref:`sphx_glr_user-guide_model-gallery_temporal_plot_linear_temporal.py` (``../examples/models/temporal/plot_linear_temporal.py``)
- - 00:00.104
+ - 00:00.106
- 0.0
diff --git a/docs/dev/_sources/tutorials/analysis-1d/cta_sensitivity.rst.txt b/docs/dev/_sources/tutorials/analysis-1d/cta_sensitivity.rst.txt
index 35b65565003..5274abf4534 100644
--- a/docs/dev/_sources/tutorials/analysis-1d/cta_sensitivity.rst.txt
+++ b/docs/dev/_sources/tutorials/analysis-1d/cta_sensitivity.rst.txt
@@ -21,12 +21,12 @@
Point source sensitivity
========================
-Estimate the CTA sensitivity for a point-like IRF at a fixed zenith angle and fixed offset.
+Estimate the CTAO sensitivity for a point-like IRF at a fixed zenith angle and fixed offset.
Introduction
------------
-This notebook explains how to estimate the CTA sensitivity for a
+This notebook explains how to estimate the CTAO sensitivity for a
point-like IRF at a fixed zenith angle and fixed offset, using the full
containment IRFs distributed for the CTA 1DC. The significance is
computed for a 1D analysis (ON-OFF regions) with the Li&Ma formula.
@@ -119,7 +119,7 @@ Check setup
Gammapy package:
- version : 1.3.dev1143+ge26e20052
+ version : 1.3.dev1180+gb03e9b8c7
path : /home/runner/work/gammapy-docs/gammapy-docs/gammapy/.tox/build_docs/lib/python3.9/site-packages/gammapy
@@ -195,7 +195,7 @@ degree.
Load IRFs and prepare dataset
-----------------------------
-We extract the 1D IRFs from the full 3D IRFs provided by CTA.
+We extract the 1D IRFs from the full 3D IRFs provided by CTAO.
.. GENERATED FROM PYTHON SOURCE LINES 86-97
@@ -339,7 +339,7 @@ minimal significance of 5 per bin. The excess must also be larger than 5% of the
We assume an alpha of 0.2 (ratio between ON and OFF area). We then run the sensitivity estimator.
-These are the conditions imposed in standard CTA sensitivity computations.
+These are the conditions imposed in standard CTAO sensitivity computations.
.. GENERATED FROM PYTHON SOURCE LINES 157-165
diff --git a/docs/dev/_sources/tutorials/analysis-1d/ebl.rst.txt b/docs/dev/_sources/tutorials/analysis-1d/ebl.rst.txt
index 4cc66e6eba4..d95607951a5 100644
--- a/docs/dev/_sources/tutorials/analysis-1d/ebl.rst.txt
+++ b/docs/dev/_sources/tutorials/analysis-1d/ebl.rst.txt
@@ -352,7 +352,7 @@ compound model.
SkyModel
- Name : YgI3kZSF
+ Name : Wqkl5UsP
Datasets names : None
Spectral model type : CompoundSpectralModel
Spatial model type :
@@ -367,7 +367,7 @@ compound model.
SkyModel
- Name : O4vAZEUJ
+ Name : dr-wsdJg
Datasets names : None
Spectral model type : PowerLawSpectralModel
Spatial model type :
diff --git a/docs/dev/_sources/tutorials/analysis-1d/extended_source_spectral_analysis.rst.txt b/docs/dev/_sources/tutorials/analysis-1d/extended_source_spectral_analysis.rst.txt
index 6f33859439a..1a00aaa0865 100644
--- a/docs/dev/_sources/tutorials/analysis-1d/extended_source_spectral_analysis.rst.txt
+++ b/docs/dev/_sources/tutorials/analysis-1d/extended_source_spectral_analysis.rst.txt
@@ -164,7 +164,7 @@ Check setup
Gammapy package:
- version : 1.3.dev1143+ge26e20052
+ version : 1.3.dev1180+gb03e9b8c7
path : /home/runner/work/gammapy-docs/gammapy-docs/gammapy/.tox/build_docs/lib/python3.9/site-packages/gammapy
diff --git a/docs/dev/_sources/tutorials/analysis-1d/sed_fitting.rst.txt b/docs/dev/_sources/tutorials/analysis-1d/sed_fitting.rst.txt
index b6127303219..2233eee183b 100644
--- a/docs/dev/_sources/tutorials/analysis-1d/sed_fitting.rst.txt
+++ b/docs/dev/_sources/tutorials/analysis-1d/sed_fitting.rst.txt
@@ -162,7 +162,7 @@ attribute:
Table length=5
-
+
| e_ref | e_min | e_max | dnde | dnde_errp | dnde_errn | dnde_ul | sqrt_ts | is_ul |
|---|
| GeV | GeV | GeV | 1 / (cm2 GeV s) | 1 / (cm2 GeV s) | 1 / (cm2 GeV s) | 1 / (cm2 GeV s) | | |
|---|
| float64 | float64 | float64 | float64 | float64 | float64 | float64 | float32 | bool |
|---|
diff --git a/docs/dev/_sources/tutorials/analysis-1d/sg_execution_times.rst.txt b/docs/dev/_sources/tutorials/analysis-1d/sg_execution_times.rst.txt
index da9322aa951..28fed85fb86 100644
--- a/docs/dev/_sources/tutorials/analysis-1d/sg_execution_times.rst.txt
+++ b/docs/dev/_sources/tutorials/analysis-1d/sg_execution_times.rst.txt
@@ -6,7 +6,7 @@
Computation times
=================
-**01:22.094** total execution time for 8 files **from tutorials/analysis-1d**:
+**01:20.640** total execution time for 8 files **from tutorials/analysis-1d**:
.. container::
@@ -33,26 +33,26 @@ Computation times
- Time
- Mem (MB)
* - :ref:`sphx_glr_tutorials_analysis-1d_spectral_analysis.py` (``spectral_analysis.py``)
- - 00:44.699
+ - 00:44.094
- 0.0
* - :ref:`sphx_glr_tutorials_analysis-1d_spectral_analysis_hli.py` (``spectral_analysis_hli.py``)
- - 00:08.080
+ - 00:07.829
- 0.0
* - :ref:`sphx_glr_tutorials_analysis-1d_spectrum_simulation.py` (``spectrum_simulation.py``)
- - 00:07.312
+ - 00:07.149
- 0.0
* - :ref:`sphx_glr_tutorials_analysis-1d_ebl.py` (``ebl.py``)
- - 00:07.003
+ - 00:06.985
- 0.0
* - :ref:`sphx_glr_tutorials_analysis-1d_sed_fitting.py` (``sed_fitting.py``)
- - 00:05.362
- - 0.0
- * - :ref:`sphx_glr_tutorials_analysis-1d_spectral_analysis_rad_max.py` (``spectral_analysis_rad_max.py``)
- - 00:04.474
+ - 00:05.263
- 0.0
* - :ref:`sphx_glr_tutorials_analysis-1d_extended_source_spectral_analysis.py` (``extended_source_spectral_analysis.py``)
- - 00:04.330
+ - 00:04.301
+ - 0.0
+ * - :ref:`sphx_glr_tutorials_analysis-1d_spectral_analysis_rad_max.py` (``spectral_analysis_rad_max.py``)
+ - 00:04.195
- 0.0
* - :ref:`sphx_glr_tutorials_analysis-1d_cta_sensitivity.py` (``cta_sensitivity.py``)
- - 00:00.833
+ - 00:00.825
- 0.0
diff --git a/docs/dev/_sources/tutorials/analysis-1d/spectral_analysis.rst.txt b/docs/dev/_sources/tutorials/analysis-1d/spectral_analysis.rst.txt
index e489070b4d3..30c29ac6636 100644
--- a/docs/dev/_sources/tutorials/analysis-1d/spectral_analysis.rst.txt
+++ b/docs/dev/_sources/tutorials/analysis-1d/spectral_analysis.rst.txt
@@ -206,7 +206,7 @@ Check setup
Gammapy package:
- version : 1.3.dev1143+ge26e20052
+ version : 1.3.dev1180+gb03e9b8c7
path : /home/runner/work/gammapy-docs/gammapy-docs/gammapy/.tox/build_docs/lib/python3.9/site-packages/gammapy
@@ -1216,7 +1216,7 @@ tutorial.
.. rst-class:: sphx-glr-timing
- **Total running time of the script:** (0 minutes 44.699 seconds)
+ **Total running time of the script:** (0 minutes 44.094 seconds)
.. _sphx_glr_download_tutorials_analysis-1d_spectral_analysis.py:
diff --git a/docs/dev/_sources/tutorials/analysis-1d/spectral_analysis_hli.rst.txt b/docs/dev/_sources/tutorials/analysis-1d/spectral_analysis_hli.rst.txt
index 13fec9316eb..be683fd7574 100644
--- a/docs/dev/_sources/tutorials/analysis-1d/spectral_analysis_hli.rst.txt
+++ b/docs/dev/_sources/tutorials/analysis-1d/spectral_analysis_hli.rst.txt
@@ -150,7 +150,7 @@ Check setup
Gammapy package:
- version : 1.3.dev1143+ge26e20052
+ version : 1.3.dev1180+gb03e9b8c7
path : /home/runner/work/gammapy-docs/gammapy-docs/gammapy/.tox/build_docs/lib/python3.9/site-packages/gammapy
@@ -350,8 +350,8 @@ Here is what the configuration for our analysis looks like:
parameters:
selection_optional: all
metadata:
- creator: Gammapy 1.3.dev1143+ge26e20052
- date: '2024-10-11T08:29:44.930944'
+ creator: Gammapy 1.3.dev1180+gb03e9b8c7
+ date: '2024-10-11T10:01:30.751715'
origin: null
@@ -571,8 +571,8 @@ One can export/import the `~gammapy.analysis.AnalysisConfig` to/from a YAML file
parameters:
selection_optional: all
metadata:
- creator: Gammapy 1.3.dev1143+ge26e20052
- date: '2024-10-11T08:29:44.955101'
+ creator: Gammapy 1.3.dev1180+gb03e9b8c7
+ date: '2024-10-11T10:01:30.775845'
origin: null
@@ -1107,8 +1107,8 @@ This is how we can write the model back to file again:
unit: TeV
covariance: model-best-fit_covariance.dat
metadata:
- creator: Gammapy 1.3.dev1143+ge26e20052
- date: '2024-10-11T08:29:48.384963'
+ creator: Gammapy 1.3.dev1180+gb03e9b8c7
+ date: '2024-10-11T10:01:34.151913'
origin: null
diff --git a/docs/dev/_sources/tutorials/analysis-1d/spectral_analysis_rad_max.rst.txt b/docs/dev/_sources/tutorials/analysis-1d/spectral_analysis_rad_max.rst.txt
index d6c10352a32..6b0aac6beba 100644
--- a/docs/dev/_sources/tutorials/analysis-1d/spectral_analysis_rad_max.rst.txt
+++ b/docs/dev/_sources/tutorials/analysis-1d/spectral_analysis_rad_max.rst.txt
@@ -206,7 +206,7 @@ Check setup
Gammapy package:
- version : 1.3.dev1143+ge26e20052
+ version : 1.3.dev1180+gb03e9b8c7
path : /home/runner/work/gammapy-docs/gammapy-docs/gammapy/.tox/build_docs/lib/python3.9/site-packages/gammapy
@@ -749,10 +749,10 @@ provide a good distribution of the background.
result = super().__array_ufunc__(function, method, *arrays, **kwargs)
model type name value unit ... min max frozen link prior
--------- ---- --------- ---------- -------------- ... --- --- ------ ---- -----
- simulated amplitude 4.3947e-11 cm-2 s-1 TeV-1 ... nan nan False
+ simulated amplitude 4.1819e-11 cm-2 s-1 TeV-1 ... nan nan False
simulated reference 1.0000e+00 TeV ... nan nan True
- simulated alpha 2.5055e+00 ... nan nan False
- simulated beta 1.5758e-01 ... nan nan False
+ simulated alpha 2.6903e+00 ... nan nan False
+ simulated beta 2.3367e-01 ... nan nan False
diff --git a/docs/dev/_sources/tutorials/analysis-1d/spectrum_simulation.rst.txt b/docs/dev/_sources/tutorials/analysis-1d/spectrum_simulation.rst.txt
index 04de2aafd0a..2922e90ebc4 100644
--- a/docs/dev/_sources/tutorials/analysis-1d/spectrum_simulation.rst.txt
+++ b/docs/dev/_sources/tutorials/analysis-1d/spectrum_simulation.rst.txt
@@ -44,12 +44,12 @@ using Poisson probability distribution.
This can be done to check the feasibility of a measurement, to test
whether fitted parameters really provide a good fit to the data etc.
-Here we will see how to perform a 1D spectral simulation of a CTA
+Here we will see how to perform a 1D spectral simulation of a CTAO
observation, in particular, we will generate OFF observations following
-the template background stored in the CTA IRFs.
+the template background stored in the CTAO IRFs.
**Objective: simulate a number of spectral ON-OFF observations of a
-source with a power-law spectral model with CTA using the CTA 1DC
+source with a power-law spectral model with CTAO using the CTA 1DC
response, fit them with the assumed spectral model and check that the
distribution of fitted parameters is consistent with the input values.**
@@ -142,7 +142,7 @@ Check setup
Gammapy package:
- version : 1.3.dev1143+ge26e20052
+ version : 1.3.dev1180+gb03e9b8c7
path : /home/runner/work/gammapy-docs/gammapy-docs/gammapy/.tox/build_docs/lib/python3.9/site-packages/gammapy
@@ -411,14 +411,14 @@ dealing with simulations based on observations of real off counts.
SpectrumDatasetOnOff
--------------------
- Name : bCK5aw7p
+ Name : 2n3Wh7vX
- Total counts : 279
- Total background counts : 22.80
- Total excess counts : 256.20
+ Total counts : 328
+ Total background counts : 24.60
+ Total excess counts : 303.40
- Predicted counts : 303.74
- Predicted background counts : 22.37
+ Predicted counts : 306.36
+ Predicted background counts : 24.99
Predicted excess counts : 281.37
Exposure min : 2.53e+08 m2 s
@@ -428,7 +428,7 @@ dealing with simulations based on observations of real off counts.
Number of fit bins : 9
Fit statistic type : wstat
- Fit statistic value (-2 log(L)) : 9.90
+ Fit statistic value (-2 log(L)) : 6.83
Number of models : 1
Number of parameters : 3
@@ -446,7 +446,7 @@ dealing with simulations based on observations of real off counts.
amplitude : 2.50e-12 +/- 0.0e+00 1 / (cm2 s TeV)
reference (frozen): 1.000 TeV
- Total counts_off : 114
+ Total counts_off : 123
Acceptance : 9
Acceptance off : 45
diff --git a/docs/dev/_sources/tutorials/analysis-2d/detect.rst.txt b/docs/dev/_sources/tutorials/analysis-2d/detect.rst.txt
index 712861eb89c..6769bbc0c64 100644
--- a/docs/dev/_sources/tutorials/analysis-2d/detect.rst.txt
+++ b/docs/dev/_sources/tutorials/analysis-2d/detect.rst.txt
@@ -124,7 +124,7 @@ Check setup
Gammapy package:
- version : 1.3.dev1143+ge26e20052
+ version : 1.3.dev1180+gb03e9b8c7
path : /home/runner/work/gammapy-docs/gammapy-docs/gammapy/.tox/build_docs/lib/python3.9/site-packages/gammapy
@@ -425,7 +425,7 @@ normalisation factor:
SkyModel
- Name : xKQKPkcV
+ Name : zTE1BNIs
Datasets names : None
Spectral model type : PowerLawSpectralModel
Spatial model type : PointSpatialModel
@@ -624,7 +624,7 @@ Here’s some suggestions what to do next:
.. rst-class:: sphx-glr-timing
- **Total running time of the script:** (0 minutes 20.870 seconds)
+ **Total running time of the script:** (0 minutes 20.552 seconds)
.. _sphx_glr_download_tutorials_analysis-2d_detect.py:
diff --git a/docs/dev/_sources/tutorials/analysis-2d/modeling_2D.rst.txt b/docs/dev/_sources/tutorials/analysis-2d/modeling_2D.rst.txt
index 08b2b083ddc..367c3107aa0 100644
--- a/docs/dev/_sources/tutorials/analysis-2d/modeling_2D.rst.txt
+++ b/docs/dev/_sources/tutorials/analysis-2d/modeling_2D.rst.txt
@@ -124,7 +124,7 @@ Check setup
Gammapy package:
- version : 1.3.dev1143+ge26e20052
+ version : 1.3.dev1180+gb03e9b8c7
path : /home/runner/work/gammapy-docs/gammapy-docs/gammapy/.tox/build_docs/lib/python3.9/site-packages/gammapy
@@ -165,7 +165,7 @@ Creating the config file
Now, we create a config file for out analysis. You may load this from
disc if you have a pre-defined config file.
-Here, we use 3 simulated CTA runs of the galactic center.
+Here, we use 3 simulated CTAO runs of the galactic center.
.. GENERATED FROM PYTHON SOURCE LINES 69-76
@@ -342,8 +342,8 @@ analysis as *3D*, and define the geometry of the analysis.
parameters:
selection_optional: all
metadata:
- creator: Gammapy 1.3.dev1143+ge26e20052
- date: '2024-10-11T08:30:26.582357'
+ creator: Gammapy 1.3.dev1180+gb03e9b8c7
+ date: '2024-10-11T10:02:11.313439'
origin: null
diff --git a/docs/dev/_sources/tutorials/analysis-2d/ring_background.rst.txt b/docs/dev/_sources/tutorials/analysis-2d/ring_background.rst.txt
index 33a019cfee3..1783cc9b138 100644
--- a/docs/dev/_sources/tutorials/analysis-2d/ring_background.rst.txt
+++ b/docs/dev/_sources/tutorials/analysis-2d/ring_background.rst.txt
@@ -125,7 +125,7 @@ Check setup
Gammapy package:
- version : 1.3.dev1143+ge26e20052
+ version : 1.3.dev1180+gb03e9b8c7
path : /home/runner/work/gammapy-docs/gammapy-docs/gammapy/.tox/build_docs/lib/python3.9/site-packages/gammapy
@@ -325,8 +325,8 @@ MSH 1552
parameters:
selection_optional: all
metadata:
- creator: Gammapy 1.3.dev1143+ge26e20052
- date: '2024-10-11T08:30:32.416068'
+ creator: Gammapy 1.3.dev1180+gb03e9b8c7
+ date: '2024-10-11T10:02:17.016713'
origin: null
@@ -476,8 +476,8 @@ create the config
parameters:
selection_optional: all
metadata:
- creator: Gammapy 1.3.dev1143+ge26e20052
- date: '2024-10-11T08:30:32.473564'
+ creator: Gammapy 1.3.dev1180+gb03e9b8c7
+ date: '2024-10-11T10:02:17.073732'
origin: null
@@ -776,7 +776,7 @@ to be a standard normal distribution.
.. rst-class:: sphx-glr-timing
- **Total running time of the script:** (0 minutes 12.115 seconds)
+ **Total running time of the script:** (0 minutes 12.100 seconds)
.. _sphx_glr_download_tutorials_analysis-2d_ring_background.py:
diff --git a/docs/dev/_sources/tutorials/analysis-2d/sg_execution_times.rst.txt b/docs/dev/_sources/tutorials/analysis-2d/sg_execution_times.rst.txt
index 134e740ea86..c89d61bb124 100644
--- a/docs/dev/_sources/tutorials/analysis-2d/sg_execution_times.rst.txt
+++ b/docs/dev/_sources/tutorials/analysis-2d/sg_execution_times.rst.txt
@@ -6,7 +6,7 @@
Computation times
=================
-**00:38.646** total execution time for 3 files **from tutorials/analysis-2d**:
+**00:38.193** total execution time for 3 files **from tutorials/analysis-2d**:
.. container::
@@ -33,11 +33,11 @@ Computation times
- Time
- Mem (MB)
* - :ref:`sphx_glr_tutorials_analysis-2d_detect.py` (``detect.py``)
- - 00:20.870
+ - 00:20.552
- 0.0
* - :ref:`sphx_glr_tutorials_analysis-2d_ring_background.py` (``ring_background.py``)
- - 00:12.115
+ - 00:12.100
- 0.0
* - :ref:`sphx_glr_tutorials_analysis-2d_modeling_2D.py` (``modeling_2D.py``)
- - 00:05.661
+ - 00:05.541
- 0.0
diff --git a/docs/dev/_sources/tutorials/analysis-3d/analysis_3d.rst.txt b/docs/dev/_sources/tutorials/analysis-3d/analysis_3d.rst.txt
index 1fc1ebff839..d9dd1c29921 100644
--- a/docs/dev/_sources/tutorials/analysis-3d/analysis_3d.rst.txt
+++ b/docs/dev/_sources/tutorials/analysis-3d/analysis_3d.rst.txt
@@ -96,7 +96,7 @@ Check setup
Gammapy package:
- version : 1.3.dev1143+ge26e20052
+ version : 1.3.dev1180+gb03e9b8c7
path : /home/runner/work/gammapy-docs/gammapy-docs/gammapy/.tox/build_docs/lib/python3.9/site-packages/gammapy
@@ -295,8 +295,8 @@ the analysis, we will programmatically build a config file from scratch.
parameters:
selection_optional: all
metadata:
- creator: Gammapy 1.3.dev1143+ge26e20052
- date: '2024-10-11T08:30:44.740422'
+ creator: Gammapy 1.3.dev1180+gb03e9b8c7
+ date: '2024-10-11T10:02:29.341815'
origin: null
AnalysisConfig
@@ -409,8 +409,8 @@ the analysis, we will programmatically build a config file from scratch.
parameters:
selection_optional: all
metadata:
- creator: Gammapy 1.3.dev1143+ge26e20052
- date: '2024-10-11T08:30:44.748175'
+ creator: Gammapy 1.3.dev1180+gb03e9b8c7
+ date: '2024-10-11T10:02:29.349613'
origin: null
@@ -1065,21 +1065,21 @@ Data reduction
Dataset 0:
Type : MapDataset
- Name : tnFttnKH
+ Name : X-JIar1n
Instrument : CTA
Models :
Dataset 1:
Type : MapDataset
- Name : Cdd-kKNp
+ Name : -mXcSLBO
Instrument : CTA
Models :
Dataset 2:
Type : MapDataset
- Name : o86DlVQX
+ Name : pQ5z7iuR
Instrument : CTA
Models :
@@ -1112,7 +1112,7 @@ You can access each one by name or by index, eg:
MapDataset
----------
- Name : tnFttnKH
+ Name : X-JIar1n
Total counts : 40481
Total background counts : 36014.51
@@ -1180,9 +1180,9 @@ map, omit the region argument.
name counts excess ... n_fit_bins stat_type stat_sum
...
-------- ------ ------------------ ... ---------- --------- --------
- tnFttnKH 40481 4466.4930435940405 ... 693940 cash nan
- Cdd-kKNp 40525 4510.505523195905 ... 693940 cash nan
- o86DlVQX 40235 4220.480554966147 ... 693940 cash nan
+ X-JIar1n 40481 4466.4930435940405 ... 693940 cash nan
+ -mXcSLBO 40525 4510.505523195905 ... 693940 cash nan
+ pQ5z7iuR 40235 4220.480554966147 ... 693940 cash nan
Models
Component 0: SkyModel
@@ -1203,8 +1203,8 @@ map, omit the region argument.
Component 1: FoVBackgroundModel
- Name : tnFttnKH-bkg
- Datasets names : ['tnFttnKH']
+ Name : X-JIar1n-bkg
+ Datasets names : ['X-JIar1n']
Spectral model type : PowerLawNormSpectralModel
Parameters:
norm : 1.000 +/- 0.00
@@ -1213,8 +1213,8 @@ map, omit the region argument.
Component 2: FoVBackgroundModel
- Name : Cdd-kKNp-bkg
- Datasets names : ['Cdd-kKNp']
+ Name : -mXcSLBO-bkg
+ Datasets names : ['-mXcSLBO']
Spectral model type : PowerLawNormSpectralModel
Parameters:
norm : 1.000 +/- 0.00
@@ -1223,8 +1223,8 @@ map, omit the region argument.
Component 3: FoVBackgroundModel
- Name : o86DlVQX-bkg
- Datasets names : ['o86DlVQX']
+ Name : pQ5z7iuR-bkg
+ Datasets names : ['pQ5z7iuR']
Spectral model type : PowerLawNormSpectralModel
Parameters:
norm : 1.000 +/- 0.00
@@ -1339,8 +1339,8 @@ Check best-fit parameters and error estimates:
Component 1: FoVBackgroundModel
- Name : tnFttnKH-bkg
- Datasets names : ['tnFttnKH']
+ Name : X-JIar1n-bkg
+ Datasets names : ['X-JIar1n']
Spectral model type : PowerLawNormSpectralModel
Parameters:
norm : 1.118 +/- 0.01
@@ -1349,8 +1349,8 @@ Check best-fit parameters and error estimates:
Component 2: FoVBackgroundModel
- Name : Cdd-kKNp-bkg
- Datasets names : ['Cdd-kKNp']
+ Name : -mXcSLBO-bkg
+ Datasets names : ['-mXcSLBO']
Spectral model type : PowerLawNormSpectralModel
Parameters:
norm : 1.119 +/- 0.01
@@ -1359,8 +1359,8 @@ Check best-fit parameters and error estimates:
Component 3: FoVBackgroundModel
- Name : o86DlVQX-bkg
- Datasets names : ['o86DlVQX']
+ Name : pQ5z7iuR-bkg
+ Datasets names : ['pQ5z7iuR']
Spectral model type : PowerLawNormSpectralModel
Parameters:
norm : 1.111 +/- 0.01
@@ -1489,7 +1489,7 @@ Exercises
.. rst-class:: sphx-glr-timing
- **Total running time of the script:** (0 minutes 37.983 seconds)
+ **Total running time of the script:** (0 minutes 37.871 seconds)
.. _sphx_glr_download_tutorials_analysis-3d_analysis_3d.py:
diff --git a/docs/dev/_sources/tutorials/analysis-3d/analysis_mwl.rst.txt b/docs/dev/_sources/tutorials/analysis-3d/analysis_mwl.rst.txt
index a2b68d30770..6f6723cd037 100644
--- a/docs/dev/_sources/tutorials/analysis-3d/analysis_mwl.rst.txt
+++ b/docs/dev/_sources/tutorials/analysis-3d/analysis_mwl.rst.txt
@@ -123,7 +123,7 @@ Check setup
Gammapy package:
- version : 1.3.dev1143+ge26e20052
+ version : 1.3.dev1180+gb03e9b8c7
path : /home/runner/work/gammapy-docs/gammapy-docs/gammapy/.tox/build_docs/lib/python3.9/site-packages/gammapy
diff --git a/docs/dev/_sources/tutorials/analysis-3d/cta_data_analysis.rst.txt b/docs/dev/_sources/tutorials/analysis-3d/cta_data_analysis.rst.txt
index a9d9d087386..73112269581 100644
--- a/docs/dev/_sources/tutorials/analysis-3d/cta_data_analysis.rst.txt
+++ b/docs/dev/_sources/tutorials/analysis-3d/cta_data_analysis.rst.txt
@@ -27,11 +27,11 @@ Introduction
------------
**This notebook shows an example how to make a sky image and spectrum
-for simulated CTA data with Gammapy.**
+for simulated CTAO data with Gammapy.**
The dataset we will use is three observation runs on the Galactic
Center. This is a tiny (and thus quick to process and play with and
-learn) subset of the simulated CTA dataset that was produced for the
+learn) subset of the simulated CTAO dataset that was produced for the
first data challenge in August 2017.
.. GENERATED FROM PYTHON SOURCE LINES 21-26
@@ -118,7 +118,7 @@ Check setup
Gammapy package:
- version : 1.3.dev1143+ge26e20052
+ version : 1.3.dev1180+gb03e9b8c7
path : /home/runner/work/gammapy-docs/gammapy-docs/gammapy/.tox/build_docs/lib/python3.9/site-packages/gammapy
@@ -818,7 +818,7 @@ profile to compute the flux and flux error.
Table length=5
-
+
| e_ref | e_min | e_max | dnde | dnde_err | ts | sqrt_ts | npred | npred_excess | stat | stat_null | counts | success |
|---|
| TeV | TeV | TeV | 1 / (cm2 s TeV) | 1 / (cm2 s TeV) | | | | | | | | |
|---|
| float64 | float64 | float64 | float64 | float64 | float64 | float64 | float64[1] | float32[1] | float64 | float64 | float64[1] | bool |
|---|
@@ -904,7 +904,7 @@ Exercises
What next?
----------
-- This notebook showed an example of a first CTA analysis with Gammapy,
+- This notebook showed an example of a first CTAO analysis with Gammapy,
using simulated 1DC data.
- Let us know if you have any questions or issues!
@@ -912,7 +912,7 @@ What next?
.. rst-class:: sphx-glr-timing
- **Total running time of the script:** (0 minutes 17.287 seconds)
+ **Total running time of the script:** (0 minutes 16.841 seconds)
.. _sphx_glr_download_tutorials_analysis-3d_cta_data_analysis.py:
diff --git a/docs/dev/_sources/tutorials/analysis-3d/energy_dependent_estimation.rst.txt b/docs/dev/_sources/tutorials/analysis-3d/energy_dependent_estimation.rst.txt
index 021954020bb..53f4e60d448 100644
--- a/docs/dev/_sources/tutorials/analysis-3d/energy_dependent_estimation.rst.txt
+++ b/docs/dev/_sources/tutorials/analysis-3d/energy_dependent_estimation.rst.txt
@@ -126,7 +126,7 @@ Check setup
Gammapy package:
- version : 1.3.dev1143+ge26e20052
+ version : 1.3.dev1180+gb03e9b8c7
path : /home/runner/work/gammapy-docs/gammapy-docs/gammapy/.tox/build_docs/lib/python3.9/site-packages/gammapy
@@ -482,7 +482,7 @@ Plotting the results
.. rst-class:: sphx-glr-timing
- **Total running time of the script:** (0 minutes 19.804 seconds)
+ **Total running time of the script:** (0 minutes 19.657 seconds)
.. _sphx_glr_download_tutorials_analysis-3d_energy_dependent_estimation.py:
diff --git a/docs/dev/_sources/tutorials/analysis-3d/event_sampling.rst.txt b/docs/dev/_sources/tutorials/analysis-3d/event_sampling.rst.txt
index cabea0e7fd5..dbfb597f67e 100644
--- a/docs/dev/_sources/tutorials/analysis-3d/event_sampling.rst.txt
+++ b/docs/dev/_sources/tutorials/analysis-3d/event_sampling.rst.txt
@@ -174,7 +174,7 @@ Check setup
Gammapy package:
- version : 1.3.dev1143+ge26e20052
+ version : 1.3.dev1180+gb03e9b8c7
path : /home/runner/work/gammapy-docs/gammapy-docs/gammapy/.tox/build_docs/lib/python3.9/site-packages/gammapy
@@ -1077,7 +1077,7 @@ Exercises
.. rst-class:: sphx-glr-timing
- **Total running time of the script:** (0 minutes 17.717 seconds)
+ **Total running time of the script:** (0 minutes 26.961 seconds)
.. _sphx_glr_download_tutorials_analysis-3d_event_sampling.py:
diff --git a/docs/dev/_sources/tutorials/analysis-3d/event_sampling_nrg_depend_models.rst.txt b/docs/dev/_sources/tutorials/analysis-3d/event_sampling_nrg_depend_models.rst.txt
index 84411ad169b..8df35384b09 100644
--- a/docs/dev/_sources/tutorials/analysis-3d/event_sampling_nrg_depend_models.rst.txt
+++ b/docs/dev/_sources/tutorials/analysis-3d/event_sampling_nrg_depend_models.rst.txt
@@ -125,7 +125,7 @@ Check setup
Gammapy package:
- version : 1.3.dev1143+ge26e20052
+ version : 1.3.dev1180+gb03e9b8c7
path : /home/runner/work/gammapy-docs/gammapy-docs/gammapy/.tox/build_docs/lib/python3.9/site-packages/gammapy
@@ -457,7 +457,7 @@ passed through the map.
Define an observation and make a dataset
~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~
-In the following, we define an observation of 1 hr with CTA in the
+In the following, we define an observation of 1 hr with CTAO in the
alpha-configuration for the south array, and we also create a dataset
to be passed to the event sampler. The full `SkyModel` created above
is passed to the dataset.
diff --git a/docs/dev/_sources/tutorials/analysis-3d/flux_profiles.rst.txt b/docs/dev/_sources/tutorials/analysis-3d/flux_profiles.rst.txt
index 998e603a7bd..63164bb52f7 100644
--- a/docs/dev/_sources/tutorials/analysis-3d/flux_profiles.rst.txt
+++ b/docs/dev/_sources/tutorials/analysis-3d/flux_profiles.rst.txt
@@ -131,7 +131,7 @@ Check setup
Gammapy package:
- version : 1.3.dev1143+ge26e20052
+ version : 1.3.dev1180+gb03e9b8c7
path : /home/runner/work/gammapy-docs/gammapy-docs/gammapy/.tox/build_docs/lib/python3.9/site-packages/gammapy
@@ -374,11 +374,11 @@ We can see the full configuration by printing the estimator object:
--------------------
energy_edges : [ 10. 2000.] GeV
- fit :
+ fit :
n_jobs : None
n_sigma : 1
n_sigma_ul : 2
- norm : Parameter(name='norm', value=1.0, factor=1.0, scale=1.0, unit=Unit(dimensionless), min=nan, max=nan, frozen=False, prior=None, id=0x7fcdbe622130)
+ norm : Parameter(name='norm', value=1.0, factor=1.0, scale=1.0, unit=Unit(dimensionless), min=nan, max=nan, frozen=False, prior=None, id=0x7f4fd4b3cbb0)
null_value : 0
parallel_backend : None
reoptimize : False
@@ -826,7 +826,7 @@ And now plot the points together with the likelihood profiles:
.. rst-class:: sphx-glr-timing
- **Total running time of the script:** (0 minutes 21.171 seconds)
+ **Total running time of the script:** (0 minutes 20.547 seconds)
.. _sphx_glr_download_tutorials_analysis-3d_flux_profiles.py:
diff --git a/docs/dev/_sources/tutorials/analysis-3d/sg_execution_times.rst.txt b/docs/dev/_sources/tutorials/analysis-3d/sg_execution_times.rst.txt
index 5c61928aef8..be6af331d03 100644
--- a/docs/dev/_sources/tutorials/analysis-3d/sg_execution_times.rst.txt
+++ b/docs/dev/_sources/tutorials/analysis-3d/sg_execution_times.rst.txt
@@ -6,7 +6,7 @@
Computation times
=================
-**02:13.808** total execution time for 8 files **from tutorials/analysis-3d**:
+**02:21.339** total execution time for 8 files **from tutorials/analysis-3d**:
.. container::
@@ -33,26 +33,26 @@ Computation times
- Time
- Mem (MB)
* - :ref:`sphx_glr_tutorials_analysis-3d_analysis_3d.py` (``analysis_3d.py``)
- - 00:37.983
+ - 00:37.871
+ - 0.0
+ * - :ref:`sphx_glr_tutorials_analysis-3d_event_sampling.py` (``event_sampling.py``)
+ - 00:26.961
- 0.0
* - :ref:`sphx_glr_tutorials_analysis-3d_flux_profiles.py` (``flux_profiles.py``)
- - 00:21.171
+ - 00:20.547
- 0.0
* - :ref:`sphx_glr_tutorials_analysis-3d_energy_dependent_estimation.py` (``energy_dependent_estimation.py``)
- - 00:19.804
- - 0.0
- * - :ref:`sphx_glr_tutorials_analysis-3d_event_sampling.py` (``event_sampling.py``)
- - 00:17.717
+ - 00:19.657
- 0.0
* - :ref:`sphx_glr_tutorials_analysis-3d_cta_data_analysis.py` (``cta_data_analysis.py``)
- - 00:17.287
+ - 00:16.841
- 0.0
* - :ref:`sphx_glr_tutorials_analysis-3d_simulate_3d.py` (``simulate_3d.py``)
- - 00:10.129
+ - 00:09.965
- 0.0
* - :ref:`sphx_glr_tutorials_analysis-3d_analysis_mwl.py` (``analysis_mwl.py``)
- - 00:06.759
+ - 00:06.606
- 0.0
* - :ref:`sphx_glr_tutorials_analysis-3d_event_sampling_nrg_depend_models.py` (``event_sampling_nrg_depend_models.py``)
- - 00:02.958
+ - 00:02.891
- 0.0
diff --git a/docs/dev/_sources/tutorials/analysis-3d/simulate_3d.rst.txt b/docs/dev/_sources/tutorials/analysis-3d/simulate_3d.rst.txt
index 5932d7e56f4..46fdd086d3a 100644
--- a/docs/dev/_sources/tutorials/analysis-3d/simulate_3d.rst.txt
+++ b/docs/dev/_sources/tutorials/analysis-3d/simulate_3d.rst.txt
@@ -303,9 +303,9 @@ the `selection` of the maps that you want to produce
Name : dataset-simu
- Total counts : 170109
+ Total counts : 170025
Total background counts : 161250.95
- Total excess counts : 8858.05
+ Total excess counts : 8774.05
Predicted counts : 169871.64
Predicted background counts : 161250.95
@@ -318,7 +318,7 @@ the `selection` of the maps that you want to produce
Number of fit bins : 804492
Fit statistic type : cash
- Fit statistic value (-2 log(L)) : 562258.99
+ Fit statistic value (-2 log(L)) : 561885.48
Number of models : 2
Number of parameters : 11
@@ -537,12 +537,12 @@ Compare the injected and fitted models:
Spatial model type : GaussianSpatialModel
Temporal model type :
Parameters:
- index : 3.013 +/- 0.02
+ index : 3.022 +/- 0.02
amplitude : 1.01e-11 +/- 3.3e-13 1 / (cm2 s TeV)
reference (frozen): 1.000 TeV
- lon_0 : 0.201 +/- 0.01 deg
+ lon_0 : 0.197 +/- 0.01 deg
lat_0 : 0.096 +/- 0.01 deg
- sigma : 0.298 +/- 0.00 deg
+ sigma : 0.303 +/- 0.00 deg
e (frozen): 0.000
phi (frozen): 0.000 deg
@@ -572,12 +572,12 @@ Get the errors on the fitted parameters from the parameter table
type name value unit ... max frozen link prior
---- --------- ---------- -------------- ... --------- ------ ---- -----
- index 3.0132e+00 ... nan False
- amplitude 1.0059e-11 cm-2 s-1 TeV-1 ... nan False
+ index 3.0222e+00 ... nan False
+ amplitude 1.0051e-11 cm-2 s-1 TeV-1 ... nan False
reference 1.0000e+00 TeV ... nan True
- lon_0 2.0138e-01 deg ... nan False
- lat_0 9.6064e-02 deg ... 9.000e+01 False
- sigma 2.9839e-01 deg ... nan False
+ lon_0 1.9666e-01 deg ... nan False
+ lat_0 9.5761e-02 deg ... 9.000e+01 False
+ sigma 3.0341e-01 deg ... nan False
e 0.0000e+00 ... 1.000e+00 True
phi 0.0000e+00 deg ... nan True
norm 1.0000e+00 ... nan True
@@ -588,11 +588,6 @@ Get the errors on the fitted parameters from the parameter table
-.. rst-class:: sphx-glr-timing
-
- **Total running time of the script:** (0 minutes 10.129 seconds)
-
-
.. _sphx_glr_download_tutorials_analysis-3d_simulate_3d.py:
.. only:: html
diff --git a/docs/dev/_sources/tutorials/analysis-time/Time_resolved_spectroscopy.rst.txt b/docs/dev/_sources/tutorials/analysis-time/Time_resolved_spectroscopy.rst.txt
index 6dee6ab8a91..e7ddfc3ef0b 100644
--- a/docs/dev/_sources/tutorials/analysis-time/Time_resolved_spectroscopy.rst.txt
+++ b/docs/dev/_sources/tutorials/analysis-time/Time_resolved_spectroscopy.rst.txt
@@ -275,238 +275,238 @@ modelled.
Dataset 0:
Type : SpectrumDatasetOnOff
- Name : dqj7OCOt
+ Name : NiQZ4ry2
Instrument : HESS
Models :
Dataset 1:
Type : SpectrumDatasetOnOff
- Name : IuqqlS6d
+ Name : vqjXpIdP
Instrument : HESS
Models :
Dataset 2:
Type : SpectrumDatasetOnOff
- Name : zybaXCrP
+ Name : dyMZ9coR
Instrument : HESS
Models :
Dataset 3:
Type : SpectrumDatasetOnOff
- Name : t3X_lqk4
+ Name : 8xmVEej2
Instrument : HESS
Models :
Dataset 4:
Type : SpectrumDatasetOnOff
- Name : Drq3iIdo
+ Name : 85Zdag8M
Instrument : HESS
Models :
Dataset 5:
Type : SpectrumDatasetOnOff
- Name : oHjZxCgK
+ Name : UGeBFzTk
Instrument : HESS
Models :
Dataset 6:
Type : SpectrumDatasetOnOff
- Name : k2qlefkU
+ Name : Vd5qKleU
Instrument : HESS
Models :
Dataset 7:
Type : SpectrumDatasetOnOff
- Name : Y3Tybbz8
+ Name : 9f-K2Z0A
Instrument : HESS
Models :
Dataset 8:
Type : SpectrumDatasetOnOff
- Name : cmn7uMUy
+ Name : iBp2fXaH
Instrument : HESS
Models :
Dataset 9:
Type : SpectrumDatasetOnOff
- Name : IcD0Fs8r
+ Name : h90YWjxn
Instrument : HESS
Models :
Dataset 10:
Type : SpectrumDatasetOnOff
- Name : uQu94Q85
+ Name : Jcm1BeoC
Instrument : HESS
Models :
Dataset 11:
Type : SpectrumDatasetOnOff
- Name : Sgzyu_un
+ Name : 9k5GaK3O
Instrument : HESS
Models :
Dataset 12:
Type : SpectrumDatasetOnOff
- Name : FHqp5P2a
+ Name : Wa8Jxt7n
Instrument : HESS
Models :
Dataset 13:
Type : SpectrumDatasetOnOff
- Name : HOX1lSkv
+ Name : ahWhUVcg
Instrument : HESS
Models :
Dataset 14:
Type : SpectrumDatasetOnOff
- Name : 9TIUrtyj
+ Name : iPNbqlev
Instrument : HESS
Models :
Dataset 15:
Type : SpectrumDatasetOnOff
- Name : wV3fdmcq
+ Name : OuyApKFP
Instrument : HESS
Models :
Dataset 16:
Type : SpectrumDatasetOnOff
- Name : tHIZ3J_y
+ Name : RF47DVOT
Instrument : HESS
Models :
Dataset 17:
Type : SpectrumDatasetOnOff
- Name : Cd7aIGC1
+ Name : TQ_RB2xH
Instrument : HESS
Models :
Dataset 18:
Type : SpectrumDatasetOnOff
- Name : y-wvy6QT
+ Name : nNJG0ula
Instrument : HESS
Models :
Dataset 19:
Type : SpectrumDatasetOnOff
- Name : xhrPjoTk
+ Name : AaS585B_
Instrument : HESS
Models :
Dataset 20:
Type : SpectrumDatasetOnOff
- Name : wI5bx3R4
+ Name : Aw_vqXrZ
Instrument : HESS
Models :
Dataset 21:
Type : SpectrumDatasetOnOff
- Name : u-XbpT7u
+ Name : HFlgxHdy
Instrument : HESS
Models :
Dataset 22:
Type : SpectrumDatasetOnOff
- Name : 0nEJ-_kP
+ Name : yaEezWwp
Instrument : HESS
Models :
Dataset 23:
Type : SpectrumDatasetOnOff
- Name : syqVZIjW
+ Name : S_T9qRu-
Instrument : HESS
Models :
Dataset 24:
Type : SpectrumDatasetOnOff
- Name : yuStLMOW
+ Name : 6mnBDRFY
Instrument : HESS
Models :
Dataset 25:
Type : SpectrumDatasetOnOff
- Name : XfMW_aU2
+ Name : Vjs8V2_r
Instrument : HESS
Models :
Dataset 26:
Type : SpectrumDatasetOnOff
- Name : nTwpP0gs
+ Name : 9_8FW5W3
Instrument : HESS
Models :
Dataset 27:
Type : SpectrumDatasetOnOff
- Name : 93g21J34
+ Name : XyI7F1GI
Instrument : HESS
Models :
Dataset 28:
Type : SpectrumDatasetOnOff
- Name : py-xXhuo
+ Name : jEgqTth-
Instrument : HESS
Models :
Dataset 29:
Type : SpectrumDatasetOnOff
- Name : Dg4XeSeE
+ Name : Wkqz_A7n
Instrument : HESS
Models :
Dataset 30:
Type : SpectrumDatasetOnOff
- Name : yfEQie9j
+ Name : v0pC1bcZ
Instrument : HESS
Models :
Dataset 31:
Type : SpectrumDatasetOnOff
- Name : ACi5Ugo8
+ Name : Z_j6iSF8
Instrument : HESS
Models :
Dataset 32:
Type : SpectrumDatasetOnOff
- Name : jvlAXiw-
+ Name : W6_g1hPS
Instrument : HESS
Models :
Dataset 33:
Type : SpectrumDatasetOnOff
- Name : azCzxhr4
+ Name : aYXklO6J
Instrument : HESS
Models :
@@ -929,7 +929,7 @@ Exercises
.. rst-class:: sphx-glr-timing
- **Total running time of the script:** (0 minutes 21.382 seconds)
+ **Total running time of the script:** (0 minutes 21.126 seconds)
.. _sphx_glr_download_tutorials_analysis-time_Time_resolved_spectroscopy.py:
diff --git a/docs/dev/_sources/tutorials/analysis-time/Variability_estimation.rst.txt b/docs/dev/_sources/tutorials/analysis-time/Variability_estimation.rst.txt
index 3067c248cf7..a99ffb77f8a 100644
--- a/docs/dev/_sources/tutorials/analysis-time/Variability_estimation.rst.txt
+++ b/docs/dev/_sources/tutorials/analysis-time/Variability_estimation.rst.txt
@@ -438,7 +438,7 @@ with the original light curve start and end points.
.. code-block:: none
-
+
diff --git a/docs/dev/_sources/tutorials/analysis-time/light_curve.rst.txt b/docs/dev/_sources/tutorials/analysis-time/light_curve.rst.txt
index c963f9c4b5d..b3e3ab53a78 100644
--- a/docs/dev/_sources/tutorials/analysis-time/light_curve.rst.txt
+++ b/docs/dev/_sources/tutorials/analysis-time/light_curve.rst.txt
@@ -132,7 +132,7 @@ Check setup
Gammapy package:
- version : 1.3.dev1143+ge26e20052
+ version : 1.3.dev1180+gb03e9b8c7
path : /home/runner/work/gammapy-docs/gammapy-docs/gammapy/.tox/build_docs/lib/python3.9/site-packages/gammapy
diff --git a/docs/dev/_sources/tutorials/analysis-time/light_curve_flare.rst.txt b/docs/dev/_sources/tutorials/analysis-time/light_curve_flare.rst.txt
index 236dabf5c86..41997a91602 100644
--- a/docs/dev/_sources/tutorials/analysis-time/light_curve_flare.rst.txt
+++ b/docs/dev/_sources/tutorials/analysis-time/light_curve_flare.rst.txt
@@ -149,7 +149,7 @@ Check setup
Gammapy package:
- version : 1.3.dev1143+ge26e20052
+ version : 1.3.dev1180+gb03e9b8c7
path : /home/runner/work/gammapy-docs/gammapy-docs/gammapy/.tox/build_docs/lib/python3.9/site-packages/gammapy
@@ -626,7 +626,7 @@ Here, we rebin 4 adjacent bins together, to get 30 min bins
.. rst-class:: sphx-glr-timing
- **Total running time of the script:** (0 minutes 34.207 seconds)
+ **Total running time of the script:** (0 minutes 33.442 seconds)
.. _sphx_glr_download_tutorials_analysis-time_light_curve_flare.py:
diff --git a/docs/dev/_sources/tutorials/analysis-time/light_curve_simulation.rst.txt b/docs/dev/_sources/tutorials/analysis-time/light_curve_simulation.rst.txt
index ebb92e0d5f2..22d4466eb47 100644
--- a/docs/dev/_sources/tutorials/analysis-time/light_curve_simulation.rst.txt
+++ b/docs/dev/_sources/tutorials/analysis-time/light_curve_simulation.rst.txt
@@ -167,7 +167,7 @@ Check setup
Gammapy package:
- version : 1.3.dev1143+ge26e20052
+ version : 1.3.dev1180+gb03e9b8c7
path : /home/runner/work/gammapy-docs/gammapy-docs/gammapy/.tox/build_docs/lib/python3.9/site-packages/gammapy
@@ -413,16 +413,16 @@ quick look into our datasets.
name counts excess ... n_fit_bins stat_type stat_sum
...
--------- ------ ------------------ ... ---------- --------- -------------------
- dataset-0 828 807.6812310184489 ... 9 cash -6642.086210032157
- dataset-1 353 343.76419591747674 ... 9 cash -2254.1954009303604
- dataset-2 278 268.3947637541758 ... 9 cash -1589.0039992789837
- dataset-3 364 349.2227134679628 ... 9 cash -2358.492346502915
- dataset-4 189 174.22271346796282 ... 9 cash -995.3847936004798
- dataset-5 167 148.52839183495354 ... 9 cash -811.0332843024476
- dataset-6 34 19.22271346796283 ... 9 cash -65.98862211011613
- dataset-7 38 18.78952750835169 ... 9 cash -89.08811786589854
- dataset-8 29 13.114416978060046 ... 9 cash -53.923361548601605
- dataset-9 41 23.636688324856333 ... 9 cash -87.87723932823582
+ dataset-0 830 809.6812310184489 ... 9 cash -6642.047923092727
+ dataset-1 341 331.76419591747674 ... 9 cash -2127.3614605107423
+ dataset-2 323 313.3947637541758 ... 9 cash -2022.9576749783714
+ dataset-3 330 315.2227134679628 ... 9 cash -2020.1188859247495
+ dataset-4 212 197.22271346796282 ... 9 cash -1160.1822508893981
+ dataset-5 176 157.52839183495354 ... 9 cash -902.7032124181009
+ dataset-6 34 19.22271346796283 ... 9 cash -64.93180377532649
+ dataset-7 45 25.78952750835169 ... 9 cash -73.95429248223132
+ dataset-8 18 2.1144169780600457 ... 9 cash -10.450785462745976
+ dataset-9 33 15.636688324856333 ... 9 cash -60.633254644563365
@@ -572,10 +572,10 @@ that ``t_ref`` should be fixed by default for the
Name : dataset_lc
Number of total flux points : 30
- Number of fit bins : 24
+ Number of fit bins : 22
Fit statistic type : chi2
- Fit statistic value (-2 log(L)) : 1524.09
+ Fit statistic value (-2 log(L)) : 1541.35
Number of models : 1
Number of parameters : 5
@@ -623,10 +623,10 @@ Fit the dataset
type name value unit error min max frozen link prior
---- --------- ---------- -------------- --------- --- --- ------ ---- -----
- index 2.9834e+00 2.780e-02 nan nan False
- amplitude 1.0194e-11 cm-2 s-1 TeV-1 3.477e-13 nan nan False
+ index 2.9532e+00 2.725e-02 nan nan False
+ amplitude 1.0390e-11 cm-2 s-1 TeV-1 3.492e-13 nan nan False
reference 1.0000e+00 TeV 0.000e+00 nan nan True
- t0 5.9005e+00 h 2.237e-01 nan nan False
+ t0 5.9005e+00 h 2.249e-01 nan nan False
t_ref 5.8909e+04 d 0.000e+00 nan nan True
@@ -739,10 +739,10 @@ Perform a joint fit
type name value unit error min max frozen link prior
---- --------- ---------- -------------- --------- --- --- ------ ---- -----
- index 2.9983e+00 3.161e-02 nan nan False
- amplitude 1.0341e-11 cm-2 s-1 TeV-1 3.600e-13 nan nan False
+ index 2.9838e+00 3.120e-02 nan nan False
+ amplitude 1.0556e-11 cm-2 s-1 TeV-1 3.601e-13 nan nan False
reference 1.0000e+00 TeV 0.000e+00 nan nan True
- t0 5.7898e+00 h 2.000e-01 nan nan False
+ t0 5.7745e+00 h 1.936e-01 nan nan False
t_ref 5.8909e+04 d 0.000e+00 nan nan True
@@ -768,7 +768,7 @@ Exercises
.. rst-class:: sphx-glr-timing
- **Total running time of the script:** (0 minutes 18.165 seconds)
+ **Total running time of the script:** (0 minutes 21.166 seconds)
.. _sphx_glr_download_tutorials_analysis-time_light_curve_simulation.py:
diff --git a/docs/dev/_sources/tutorials/analysis-time/pulsar_analysis.rst.txt b/docs/dev/_sources/tutorials/analysis-time/pulsar_analysis.rst.txt
index 43fadd71df1..106d22844d8 100644
--- a/docs/dev/_sources/tutorials/analysis-time/pulsar_analysis.rst.txt
+++ b/docs/dev/_sources/tutorials/analysis-time/pulsar_analysis.rst.txt
@@ -117,7 +117,7 @@ Check setup
Gammapy package:
- version : 1.3.dev1143+ge26e20052
+ version : 1.3.dev1180+gb03e9b8c7
path : /home/runner/work/gammapy-docs/gammapy-docs/gammapy/.tox/build_docs/lib/python3.9/site-packages/gammapy
@@ -674,7 +674,7 @@ Finally, we can run an `~gammapy.estimators.ExcessMapEstimator` to compute the e
.. GENERATED FROM PYTHON SOURCE LINES 334-348
-Note that here we are lacking statistic because we only use one run of CTA.
+Note that here we are lacking statistic because we only use one run of CTAO.
Phase-resolved spectrum
-----------------------
diff --git a/docs/dev/_sources/tutorials/analysis-time/sg_execution_times.rst.txt b/docs/dev/_sources/tutorials/analysis-time/sg_execution_times.rst.txt
index 118fafac69e..0fee51cbb7d 100644
--- a/docs/dev/_sources/tutorials/analysis-time/sg_execution_times.rst.txt
+++ b/docs/dev/_sources/tutorials/analysis-time/sg_execution_times.rst.txt
@@ -6,7 +6,7 @@
Computation times
=================
-**01:28.511** total execution time for 6 files **from tutorials/analysis-time**:
+**01:30.067** total execution time for 6 files **from tutorials/analysis-time**:
.. container::
@@ -33,20 +33,20 @@ Computation times
- Time
- Mem (MB)
* - :ref:`sphx_glr_tutorials_analysis-time_light_curve_flare.py` (``light_curve_flare.py``)
- - 00:34.207
- - 0.0
- * - :ref:`sphx_glr_tutorials_analysis-time_Time_resolved_spectroscopy.py` (``Time_resolved_spectroscopy.py``)
- - 00:21.382
+ - 00:33.442
- 0.0
* - :ref:`sphx_glr_tutorials_analysis-time_light_curve_simulation.py` (``light_curve_simulation.py``)
- - 00:18.165
+ - 00:21.166
+ - 0.0
+ * - :ref:`sphx_glr_tutorials_analysis-time_Time_resolved_spectroscopy.py` (``Time_resolved_spectroscopy.py``)
+ - 00:21.126
- 0.0
* - :ref:`sphx_glr_tutorials_analysis-time_light_curve.py` (``light_curve.py``)
- - 00:07.519
+ - 00:07.502
- 0.0
* - :ref:`sphx_glr_tutorials_analysis-time_pulsar_analysis.py` (``pulsar_analysis.py``)
- - 00:06.579
+ - 00:06.235
- 0.0
* - :ref:`sphx_glr_tutorials_analysis-time_Variability_estimation.py` (``Variability_estimation.py``)
- - 00:00.659
+ - 00:00.596
- 0.0
diff --git a/docs/dev/_sources/tutorials/api/astro_dark_matter.rst.txt b/docs/dev/_sources/tutorials/api/astro_dark_matter.rst.txt
index 2028d253954..6d630566b62 100644
--- a/docs/dev/_sources/tutorials/api/astro_dark_matter.rst.txt
+++ b/docs/dev/_sources/tutorials/api/astro_dark_matter.rst.txt
@@ -106,7 +106,7 @@ Check setup
Gammapy package:
- version : 1.3.dev1143+ge26e20052
+ version : 1.3.dev1180+gb03e9b8c7
path : /home/runner/work/gammapy-docs/gammapy-docs/gammapy/.tox/build_docs/lib/python3.9/site-packages/gammapy
@@ -478,7 +478,7 @@ Finally flux maps for decay can be produced like this:
.. rst-class:: sphx-glr-timing
- **Total running time of the script:** (0 minutes 28.155 seconds)
+ **Total running time of the script:** (0 minutes 27.997 seconds)
.. _sphx_glr_download_tutorials_api_astro_dark_matter.py:
diff --git a/docs/dev/_sources/tutorials/api/catalog.rst.txt b/docs/dev/_sources/tutorials/api/catalog.rst.txt
index 5880fa01714..4971013c3a6 100644
--- a/docs/dev/_sources/tutorials/api/catalog.rst.txt
+++ b/docs/dev/_sources/tutorials/api/catalog.rst.txt
@@ -118,7 +118,7 @@ Check setup
Gammapy package:
- version : 1.3.dev1143+ge26e20052
+ version : 1.3.dev1180+gb03e9b8c7
path : /home/runner/work/gammapy-docs/gammapy-docs/gammapy/.tox/build_docs/lib/python3.9/site-packages/gammapy
diff --git a/docs/dev/_sources/tutorials/api/datasets.rst.txt b/docs/dev/_sources/tutorials/api/datasets.rst.txt
index bd6fb537a85..a63a8617838 100644
--- a/docs/dev/_sources/tutorials/api/datasets.rst.txt
+++ b/docs/dev/_sources/tutorials/api/datasets.rst.txt
@@ -103,7 +103,7 @@ Check setup
Gammapy package:
- version : 1.3.dev1143+ge26e20052
+ version : 1.3.dev1180+gb03e9b8c7
path : /home/runner/work/gammapy-docs/gammapy-docs/gammapy/.tox/build_docs/lib/python3.9/site-packages/gammapy
@@ -297,7 +297,7 @@ To see the geometry of each map, we can use:
.. code-block:: none
- {'geom': , 'geom_exposure': , 'geom_psf': , 'geom_edisp': }
+ {'geom': , 'geom_exposure': , 'geom_psf': , 'geom_edisp': }
@@ -1883,7 +1883,7 @@ Or slice all datasets by a given energy range:
.. rst-class:: sphx-glr-timing
- **Total running time of the script:** (0 minutes 14.906 seconds)
+ **Total running time of the script:** (0 minutes 13.751 seconds)
.. _sphx_glr_download_tutorials_api_datasets.py:
diff --git a/docs/dev/_sources/tutorials/api/estimators.rst.txt b/docs/dev/_sources/tutorials/api/estimators.rst.txt
index bc9d39d2e29..eb365a354ce 100644
--- a/docs/dev/_sources/tutorials/api/estimators.rst.txt
+++ b/docs/dev/_sources/tutorials/api/estimators.rst.txt
@@ -551,7 +551,7 @@ Typically, it is the best fit model:
SkyModel
- Name : wYsZT8AS
+ Name : J04Tt_Fm
Datasets names : None
Spectral model type : PowerLawSpectralModel
Spatial model type :
diff --git a/docs/dev/_sources/tutorials/api/fitting.rst.txt b/docs/dev/_sources/tutorials/api/fitting.rst.txt
index 3a06fbc0ff6..448a5df98c1 100644
--- a/docs/dev/_sources/tutorials/api/fitting.rst.txt
+++ b/docs/dev/_sources/tutorials/api/fitting.rst.txt
@@ -107,7 +107,7 @@ Check setup
Gammapy package:
- version : 1.3.dev1143+ge26e20052
+ version : 1.3.dev1180+gb03e9b8c7
path : /home/runner/work/gammapy-docs/gammapy-docs/gammapy/.tox/build_docs/lib/python3.9/site-packages/gammapy
@@ -1119,7 +1119,7 @@ in.
.. rst-class:: sphx-glr-timing
- **Total running time of the script:** (0 minutes 11.540 seconds)
+ **Total running time of the script:** (0 minutes 11.367 seconds)
.. _sphx_glr_download_tutorials_api_fitting.py:
diff --git a/docs/dev/_sources/tutorials/api/makers.rst.txt b/docs/dev/_sources/tutorials/api/makers.rst.txt
index a3eb13dc139..ad37d5daa3e 100644
--- a/docs/dev/_sources/tutorials/api/makers.rst.txt
+++ b/docs/dev/_sources/tutorials/api/makers.rst.txt
@@ -98,7 +98,7 @@ Check setup
Gammapy package:
- version : 1.3.dev1143+ge26e20052
+ version : 1.3.dev1180+gb03e9b8c7
path : /home/runner/work/gammapy-docs/gammapy-docs/gammapy/.tox/build_docs/lib/python3.9/site-packages/gammapy
@@ -174,7 +174,7 @@ object. This is illustrated in the following example:
MapDataset
----------
- Name : Nj35nLaI
+ Name : AMw5riZy
Total counts : 0
Total background counts : 0.00
@@ -345,7 +345,7 @@ observational data using the `~gammapy.makers.MapDatasetMaker`:
MapDataset
----------
- Name : g1hz85F8
+ Name : UftOlEWP
Total counts : 2016
Total background counts : 1866.72
@@ -597,7 +597,7 @@ dataset per observation is stacked into a larger map.
MapDataset
----------
- Name : NJF1frkD
+ Name : HTbP0aHQ
Total counts : 7972
Total background counts : 7555.42
@@ -672,30 +672,30 @@ allow to use multiple processes on run.
Dataset 0:
Type : MapDataset
- Name : 3AyTdMXN
+ Name : cj-kBoNZ
Instrument : HESS
- Models : ['3AyTdMXN-bkg']
+ Models : ['cj-kBoNZ-bkg']
Dataset 1:
Type : MapDataset
- Name : n7MOliCm
+ Name : 5_Wwdc5s
Instrument : HESS
- Models : ['n7MOliCm-bkg']
+ Models : ['5_Wwdc5s-bkg']
Dataset 2:
Type : MapDataset
- Name : Oz_zRyNs
+ Name : HPcD7_1w
Instrument : HESS
- Models : ['Oz_zRyNs-bkg']
+ Models : ['HPcD7_1w-bkg']
Dataset 3:
Type : MapDataset
- Name : QR_nggnK
+ Name : ynurRGl_
Instrument : HESS
- Models : ['QR_nggnK-bkg']
+ Models : ['ynurRGl_-bkg']
@@ -957,7 +957,7 @@ use `get_by_coord`
.. rst-class:: sphx-glr-timing
- **Total running time of the script:** (0 minutes 15.214 seconds)
+ **Total running time of the script:** (0 minutes 15.013 seconds)
.. _sphx_glr_download_tutorials_api_makers.py:
diff --git a/docs/dev/_sources/tutorials/api/maps.rst.txt b/docs/dev/_sources/tutorials/api/maps.rst.txt
index b428cc79df7..ca479725068 100644
--- a/docs/dev/_sources/tutorials/api/maps.rst.txt
+++ b/docs/dev/_sources/tutorials/api/maps.rst.txt
@@ -130,7 +130,7 @@ Check setup
Gammapy package:
- version : 1.3.dev1143+ge26e20052
+ version : 1.3.dev1180+gb03e9b8c7
path : /home/runner/work/gammapy-docs/gammapy-docs/gammapy/.tox/build_docs/lib/python3.9/site-packages/gammapy
diff --git a/docs/dev/_sources/tutorials/api/mask_maps.rst.txt b/docs/dev/_sources/tutorials/api/mask_maps.rst.txt
index e053ddf17a2..b815ac7d555 100644
--- a/docs/dev/_sources/tutorials/api/mask_maps.rst.txt
+++ b/docs/dev/_sources/tutorials/api/mask_maps.rst.txt
@@ -163,7 +163,7 @@ Check setup
Gammapy package:
- version : 1.3.dev1143+ge26e20052
+ version : 1.3.dev1180+gb03e9b8c7
path : /home/runner/work/gammapy-docs/gammapy-docs/gammapy/.tox/build_docs/lib/python3.9/site-packages/gammapy
diff --git a/docs/dev/_sources/tutorials/api/model_management.rst.txt b/docs/dev/_sources/tutorials/api/model_management.rst.txt
index e8c55474cce..a92dba6480e 100644
--- a/docs/dev/_sources/tutorials/api/model_management.rst.txt
+++ b/docs/dev/_sources/tutorials/api/model_management.rst.txt
@@ -136,7 +136,7 @@ Check setup
Gammapy package:
- version : 1.3.dev1143+ge26e20052
+ version : 1.3.dev1180+gb03e9b8c7
path : /home/runner/work/gammapy-docs/gammapy-docs/gammapy/.tox/build_docs/lib/python3.9/site-packages/gammapy
@@ -1567,7 +1567,7 @@ associated models, ie, with yaml and fits files. eg:
.. rst-class:: sphx-glr-timing
- **Total running time of the script:** (0 minutes 10.396 seconds)
+ **Total running time of the script:** (0 minutes 10.361 seconds)
.. _sphx_glr_download_tutorials_api_model_management.py:
diff --git a/docs/dev/_sources/tutorials/api/models.rst.txt b/docs/dev/_sources/tutorials/api/models.rst.txt
index 7c2f6e67f9a..1ec12e8cece 100644
--- a/docs/dev/_sources/tutorials/api/models.rst.txt
+++ b/docs/dev/_sources/tutorials/api/models.rst.txt
@@ -95,7 +95,7 @@ Check setup
Gammapy package:
- version : 1.3.dev1143+ge26e20052
+ version : 1.3.dev1180+gb03e9b8c7
path : /home/runner/work/gammapy-docs/gammapy-docs/gammapy/.tox/build_docs/lib/python3.9/site-packages/gammapy
@@ -1198,7 +1198,7 @@ generated:
.. code-block:: none
- Yq6N6Dy3
+ TaIMLVwq
@@ -1392,7 +1392,7 @@ existing FITS file:
SkyModel
- Name : arA_C38k
+ Name : 6u_OBXEK
Datasets names : None
Spectral model type : PowerLawNormSpectralModel
Spatial model type : TemplateSpatialModel
@@ -1530,7 +1530,7 @@ multiple model components, Gammapy has a `~gammapy.modeling.models.Models` class
Component 1: SkyModel
- Name : arA_C38k
+ Name : 6u_OBXEK
Datasets names : None
Spectral model type : PowerLawNormSpectralModel
Spatial model type : TemplateSpatialModel
@@ -1616,7 +1616,7 @@ To see which models are available you can use the ``.names`` attribute:
.. code-block:: none
- ['my-source', 'arA_C38k']
+ ['my-source', '6u_OBXEK']
@@ -1717,7 +1717,7 @@ format:
value: 2.0
unit: d
scale: utc
- - name: arA_C38k
+ - name: 6u_OBXEK
type: SkyModel
spectral:
type: PowerLawNormSpectralModel
@@ -1786,8 +1786,8 @@ format:
unit: d
scale: utc
metadata:
- creator: Gammapy 1.3.dev1143+ge26e20052
- date: '2024-10-11T08:36:16.315310'
+ creator: Gammapy 1.3.dev1180+gb03e9b8c7
+ date: '2024-10-11T10:08:07.202917'
origin: null
@@ -1864,8 +1864,8 @@ amplitudes:
.. code-block:: none
- Parameter(name='index', value=2.3, factor=2.3, scale=1.0, unit=Unit(dimensionless), min=1.0, max=5.0, frozen=False, prior=None, id=0x7fcdd50a4a60)
- Parameter(name='index', value=2.3, factor=2.3, scale=1.0, unit=Unit(dimensionless), min=1.0, max=5.0, frozen=False, prior=None, id=0x7fcdd50a4a60)
+ Parameter(name='index', value=2.3, factor=2.3, scale=1.0, unit=Unit(dimensionless), min=1.0, max=5.0, frozen=False, prior=None, id=0x7f4fd525a6d0)
+ Parameter(name='index', value=2.3, factor=2.3, scale=1.0, unit=Unit(dimensionless), min=1.0, max=5.0, frozen=False, prior=None, id=0x7f4fd525a6d0)
@@ -1904,7 +1904,7 @@ In the YAML files the shared parameter is flagged by the additional
value: 2.3
min: 1.0
max: 5.0
- link: index@4oIhnYmE
+ link: index@xQxKkcrV
- name: amplitude
value: 2.7e-12
unit: cm-2 s-1 TeV-1
@@ -1920,7 +1920,7 @@ In the YAML files the shared parameter is flagged by the additional
value: 2.3
min: 1.0
max: 5.0
- link: index@4oIhnYmE
+ link: index@xQxKkcrV
- name: amplitude
value: 1.0e-12
unit: cm-2 s-1 TeV-1
@@ -1928,8 +1928,8 @@ In the YAML files the shared parameter is flagged by the additional
value: 1.0
unit: TeV
metadata:
- creator: Gammapy 1.3.dev1143+ge26e20052
- date: '2024-10-11T08:36:16.500393'
+ creator: Gammapy 1.3.dev1180+gb03e9b8c7
+ date: '2024-10-11T10:08:07.385517'
origin: null
diff --git a/docs/dev/_sources/tutorials/api/observation_clustering.rst.txt b/docs/dev/_sources/tutorials/api/observation_clustering.rst.txt
index a5682c067e2..e4e9c2839f9 100644
--- a/docs/dev/_sources/tutorials/api/observation_clustering.rst.txt
+++ b/docs/dev/_sources/tutorials/api/observation_clustering.rst.txt
@@ -201,7 +201,7 @@ be adjusted according to each specific science case.
.. code-block:: none
- {'group_high_zenith': , 'group_low_zenith': }
+ {'group_high_zenith': , 'group_low_zenith': }
@@ -481,7 +481,7 @@ Finally, ``observations.group_by_label`` creates a dictionary containing ``t``
.. code-block:: none
- {'group_1': , 'group_2': }
+ {'group_1': , 'group_2': }
diff --git a/docs/dev/_sources/tutorials/api/priors.rst.txt b/docs/dev/_sources/tutorials/api/priors.rst.txt
index e0620c2107a..105f97238ab 100644
--- a/docs/dev/_sources/tutorials/api/priors.rst.txt
+++ b/docs/dev/_sources/tutorials/api/priors.rst.txt
@@ -135,7 +135,7 @@ Check setup
Gammapy package:
- version : 1.3.dev1143+ge26e20052
+ version : 1.3.dev1180+gb03e9b8c7
path : /home/runner/work/gammapy-docs/gammapy-docs/gammapy/.tox/build_docs/lib/python3.9/site-packages/gammapy
@@ -371,8 +371,8 @@ The parameters table will mention the type of prior associated to each model
model type name value ... max frozen link prior
----------- ---- --------- ---------- ... --- ------ ---- -------------
- prior-model index 2.1652e+00 ... nan False GaussianPrior
- prior-model amplitude 7.8406e-12 ... nan False
+ prior-model index 2.1128e+00 ... nan False GaussianPrior
+ prior-model amplitude 9.6402e-12 ... nan False
prior-model reference 1.0000e+00 ... nan True
@@ -781,14 +781,14 @@ The only parameter is ``sigma`` and the evaluation method return the squared inv
{'spectral': {'type': 'PowerLawSpectralModel', 'parameters': [{'name': 'index', 'value': 2.0, 'prior': {'type': 'MyCustomPrior', 'parameters': [{'name': 'sigma', 'value': 0.5, 'unit': ''}], 'weight': 1}}, {'name': 'amplitude', 'value': 1e-12, 'unit': 'cm-2 s-1 TeV-1'}, {'name': 'reference', 'value': 1.0, 'unit': 'TeV'}]}}
- [<__main__.MyCustomPrior object at 0x7fcdb1654940>, None, None]
+ [<__main__.MyCustomPrior object at 0x7f4fd5374a30>, None, None]
.. rst-class:: sphx-glr-timing
- **Total running time of the script:** (1 minutes 21.171 seconds)
+ **Total running time of the script:** (1 minutes 27.538 seconds)
.. _sphx_glr_download_tutorials_api_priors.py:
diff --git a/docs/dev/_sources/tutorials/api/sg_execution_times.rst.txt b/docs/dev/_sources/tutorials/api/sg_execution_times.rst.txt
index 1d627c8342d..e2a0b3ff9a0 100644
--- a/docs/dev/_sources/tutorials/api/sg_execution_times.rst.txt
+++ b/docs/dev/_sources/tutorials/api/sg_execution_times.rst.txt
@@ -6,7 +6,7 @@
Computation times
=================
-**03:10.525** total execution time for 13 files **from tutorials/api**:
+**03:14.156** total execution time for 13 files **from tutorials/api**:
.. container::
@@ -33,41 +33,41 @@ Computation times
- Time
- Mem (MB)
* - :ref:`sphx_glr_tutorials_api_priors.py` (``priors.py``)
- - 01:21.171
+ - 01:27.538
- 0.0
* - :ref:`sphx_glr_tutorials_api_astro_dark_matter.py` (``astro_dark_matter.py``)
- - 00:28.155
+ - 00:27.997
- 0.0
* - :ref:`sphx_glr_tutorials_api_makers.py` (``makers.py``)
- - 00:15.214
+ - 00:15.013
- 0.0
* - :ref:`sphx_glr_tutorials_api_datasets.py` (``datasets.py``)
- - 00:14.906
+ - 00:13.751
- 0.0
* - :ref:`sphx_glr_tutorials_api_fitting.py` (``fitting.py``)
- - 00:11.540
+ - 00:11.367
- 0.0
* - :ref:`sphx_glr_tutorials_api_model_management.py` (``model_management.py``)
- - 00:10.396
+ - 00:10.361
- 0.0
* - :ref:`sphx_glr_tutorials_api_estimators.py` (``estimators.py``)
- - 00:06.947
+ - 00:06.718
- 0.0
* - :ref:`sphx_glr_tutorials_api_catalog.py` (``catalog.py``)
- - 00:06.157
+ - 00:06.077
- 0.0
* - :ref:`sphx_glr_tutorials_api_observation_clustering.py` (``observation_clustering.py``)
- - 00:03.955
+ - 00:03.875
- 0.0
* - :ref:`sphx_glr_tutorials_api_irfs.py` (``irfs.py``)
- - 00:03.852
- - 0.0
- * - :ref:`sphx_glr_tutorials_api_models.py` (``models.py``)
- - 00:03.150
+ - 00:03.804
- 0.0
* - :ref:`sphx_glr_tutorials_api_maps.py` (``maps.py``)
- - 00:02.746
+ - 00:02.716
+ - 0.0
+ * - :ref:`sphx_glr_tutorials_api_models.py` (``models.py``)
+ - 00:02.624
- 0.0
* - :ref:`sphx_glr_tutorials_api_mask_maps.py` (``mask_maps.py``)
- - 00:02.337
+ - 00:02.315
- 0.0
diff --git a/docs/dev/_sources/tutorials/data/cta.rst.txt b/docs/dev/_sources/tutorials/data/cta.rst.txt
index 3901983597a..2769ecd217c 100644
--- a/docs/dev/_sources/tutorials/data/cta.rst.txt
+++ b/docs/dev/_sources/tutorials/data/cta.rst.txt
@@ -18,60 +18,60 @@
.. _sphx_glr_tutorials_data_cta.py:
-CTA with Gammapy
-================
+CTAO with Gammapy
+=================
-Access and inspect CTA data and instrument response functions (IRFs) using Gammapy.
+Access and inspect CTAO data and instrument response functions (IRFs) using Gammapy.
Introduction
------------
-The `Cherenkov Telescope Array
-(CTA) `__ is the next generation
+The `Cherenkov Telescope Array Observatory (CTAO) `__ is the next generation
ground-based observatory for gamma-ray astronomy. Gammapy is the core
-library for the Cherenkov Telescope Array (CTA) science tools
+library for the Cherenkov Telescope Array Observatory (CTAO) science tools
(`2017ICRC…35..766D `__
and `CTAO Press
-Release `__).
+Release `__).
-CTA will start taking data in the coming years. For now, to learn how to
-analyse CTA data and to use Gammapy, if you are a member of the CTA
-consortium, you can use the simulated dataset from the CTA first data
-challenge which ran in 2017 and 2018.
+CTAO will start taking data in the coming years. For now, to learn how to
+analyse CTAO data and to use Gammapy, if you are a member of the CTAO
+consortium, you can use the simulated dataset from:
-- https://forge.in2p3.fr/projects/data-challenge-1-dc-1/wiki (CTA
- internal)
+- the CTA first data challenge which ran in 2017 and 2018 (https://forge.in2p3.fr/projects/data-challenge-1-dc-1/wiki),
+- the CTAO Science Data Challenge of 2024 (https://ctaoobservatory.sharepoint.com/:f:/r/sites/share-open-data/Shared%20Documents/Reference%20datasets/Internal%20Science%20Data%20Challenge?csf=1&web=1&e=gNuFzI)
Gammapy fully supports the FITS data formats (events, IRFs) used in CTA
-1DC. The XML sky model format is not supported, but are also not needed
+1DC and SDC. The XML sky model format is not supported, but are also not needed
to analyse the data, you have to specify your model via the Gammapy YAML
model format, or Python code, as shown below.
-You can use Gammapy to simulate CTA data and evaluate CTA performance
-using the CTA response files available here:
+You can also use Gammapy to simulate CTAO data and evaluate CTAO performance
+using the CTAO response files. Two sets of responses are available for different
+array layouts:
-- https://www.cta-observatory.org/science/cta-performance/
+- the Omega configuration (prod3b, 2016): https://zenodo.org/records/5163273,
+- the Alpha configuration (prod5, 2021): https://zenodo.org/records/5499840.
+
+They are all fully supported by Gammapy.
-The current FITS format `CTA-Performance-prod3b-v2-FITS.tar` is fully
-supported by Gammapy, as shown below.
Tutorial overview
-----------------
-This notebook shows how to access CTA data and instrument response
+This notebook shows how to access CTAO data and instrument response
functions (IRFs) using Gammapy, and gives some examples how to quick
-look the content of CTA files, especially to see the shape of CTA IRFs.
+look the content of CTAO files, especially to see the shape of CTAO IRFs.
At the end of the notebooks, we give several links to other tutorial
-notebooks that show how to simulate CTA data and how to evaluate CTA
-observability and sensitivity, or how to analyse CTA data.
+notebooks that show how to simulate CTAO data and how to evaluate CTAO
+observability and sensitivity, or how to analyse CTAO data.
-Note that the FITS data and IRF format currently used by CTA is the one
+Note that the FITS data and IRF format currently used by CTAO is the one
documented at https://gamma-astro-data-formats.readthedocs.io/, and is
-also used by H.E.S.S. and other imaging atmospheric Cherenkov telescopes
+also used by H.E.S.S. and other Imaging Atmospheric Cherenkov Telescopes
(IACTs). So if you see other Gammapy tutorials using e.g. H.E.S.S.
-example data, know that they also apply to CTA, all you have to do is to
-change the loaded data or IRFs to CTA.
+example data, know that they also apply to CTAO, all you have to do is to
+change the loaded data or IRFs to CTAO.
Setup
-----
@@ -131,7 +131,7 @@ Check setup
Gammapy package:
- version : 1.3.dev1143+ge26e20052
+ version : 1.3.dev1180+gb03e9b8c7
path : /home/runner/work/gammapy-docs/gammapy-docs/gammapy/.tox/build_docs/lib/python3.9/site-packages/gammapy
@@ -183,18 +183,18 @@ survey data you are interested in: Galactic plane survey `gps.tar.gz`
After download, follow the instructions how to `untar` the files, and
set a `CTADATA` environment variable to point to the data.
-For convenience, since the 1DC data files are large, and not publicly
+**For convenience**, since the 1DC data files are large and not publicly
available to anyone, we have taken a tiny subset of the CTA 1DC data,
four observations with the southern array from the GPS survey, pointing
-near the Galactic center, and included them at `$GAMMAPY_DATA/cta-1dc`
+near the Galactic center, and **included them at `$GAMMAPY_DATA/cta-1dc`**
which you get via `gammapy download datasets`.
Files
~~~~~
Next we will show a quick overview of the files and how to load them,
-and some quick look plots showing the shape of the CTA IRFs. How to do
-CTA simulations and analyses is shown in other tutorials, see links at
+and some quick look plots showing the shape of the CTAO IRFs. How to do
+CTAO simulations and analyses is shown in other tutorials, see links at
the end of this notebook.
@@ -350,9 +350,9 @@ We can load events data via the data store and observation, or
equivalently via the `~gammapy.data.EventList` class by specifying the
EVENTS filename.
-The quick-look `events.peek()` plot below shows that CTA has a field
+The quick-look `events.peek()` plot below shows that CTAO has a field
of view of a few degrees, and two energy thresholds, one significantly
-below 100 GeV where the CTA large-size telescopes (LSTs) detect events,
+below 100 GeV where the CTAO large-size telescopes (LSTs) detect events,
and a second one near 100 GeV where the mid-sized telescopes (MSTs)
start to detect events.
@@ -462,7 +462,7 @@ And show a summary plot:
IRFs
----
-The CTA instrument response functions (IRFs) are given as FITS files in
+The CTAO instrument response functions (IRFs) are given as FITS files in
the `caldb` folder, the following IRFs are available:
- effective area
@@ -472,12 +472,12 @@ the `caldb` folder, the following IRFs are available:
Notes:
-- The IRFs contain the energy and offset dependence of the CTA response
-- CTA 1DC was based on an early version of the CTA FITS responses
+- The IRFs contain the energy and offset dependence of the CTAO response
+- CTA 1DC was based on an early version of the CTAO FITS responses
produced in 2017, improvements have been made since.
- The point spread function was approximated by a Gaussian shape
- The background is from hadronic and electron air shower events that
- pass CTA selection cuts. It was given as a function of field of view
+ pass CTAO selection cuts. It was given as a function of field of view
coordinates, although it is radially symmetric.
- The energy dispersion in CTA 1DC is noisy at low energy, leading to
unreliable spectral points for some analyses.
@@ -523,7 +523,7 @@ Notes:
/home/runner/work/gammapy-docs/gammapy-docs/gammapy/.tox/build_docs/lib/python3.9/site-packages/astropy/units/core.py:2097: UnitsWarning: '1/s/MeV/sr' did not parse as fits unit: Numeric factor not supported by FITS If this is meant to be a custom unit, define it with 'u.def_unit'. To have it recognized inside a file reader or other code, enable it with 'u.add_enabled_units'. For details, see https://docs.astropy.org/en/latest/units/combining_and_defining.html
warnings.warn(msg, UnitsWarning)
- {'aeff': , 'psf': , 'edisp': , 'bkg': }
+ {'aeff': , 'psf': , 'edisp': , 'bkg': }
@@ -781,35 +781,35 @@ understands.
-.. GENERATED FROM PYTHON SOURCE LINES 358-369
+.. GENERATED FROM PYTHON SOURCE LINES 358-368
-CTA performance files
----------------------
+Latest CTAO performance files
+-----------------------------
-CTA 1DC is useful to learn how to analyse CTA data. But to do
-simulations and studies for CTA now, you should get the most recent CTA
-IRFs in FITS format from
-https://www.cta-observatory.org/science/cta-performance/
+CTA 1DC is useful to learn how to analyse CTAO data. But to do
+simulations and studies for CTAO now, you should get the most recent CTAO
+IRFs in FITS format from https://www.ctao.org/for-scientists/performance/.
-If you want to run the download and examples in the next code cells,
-remove the # to uncomment.
+If you want to use other response files, the following code cells (remove the # to uncomment)
+explain how to proceed. This example is made with the Alpha configuration (Prod5).
-.. GENERATED FROM PYTHON SOURCE LINES 369-383
+.. GENERATED FROM PYTHON SOURCE LINES 368-383
.. code-block:: Python
- # !curl -O https://www.cta-observatory.org/wp-content/uploads/2019/04/CTA-Performance-prod3b-v2-FITS.tar.gz
-
- # !tar xf CTA-Performance-prod3b-v2-FITS.tar.gz
+ # !curl -o cta-prod5-zenodo-fitsonly-v0.1.zip https://zenodo.org/records/5499840/files/cta-prod5-zenodo-fitsonly-v0.1.zip
+ # !unzip cta-prod5-zenodo-fitsonly-v0.1.zip
+ # !ls fits/
- # !ls caldb/data/cta/prod3b-v2/bcf
+ # !tar xf fits/CTA-Performance-prod5-v0.1-South-40deg.FITS.tar.gz -C fits/.
+ # !ls fits/*.fits.gz
- # irfs1 = load_irf_dict_from_file("caldb/data/cta/prod3b-v2/bcf/South_z20_50h/irf_file.fits")
+ # irfs1 = load_irf_dict_from_file("fits/Prod5-South-40deg-SouthAz-14MSTs37SSTs.180000s-v0.1.fits.gz")
# irfs1["aeff"].plot_energy_dependence()
- # irfs2 = load_irf_dict_from_file("caldb/data/cta/prod3b-v2/bcf/South_z40_50h/irf_file.fits")
+ # irfs2 = load_irf_dict_from_file("fits/Prod5-South-40deg-SouthAz-14MSTs37SSTs.1800s-v0.1.fits.gz")
# irfs2["aeff"].plot_energy_dependence()
@@ -832,11 +832,11 @@ Exercises
- Use `~gammapy.data.EventList.pointing_radec` to find the pointing position of this
observation, and use `astropy.coordinates.SkyCoord` methods to find
the field of view offset of the highest-energy event.
-- What is the effective area and PSF 68% containment radius of CTA at 1
+- What is the effective area and PSF 68% containment radius of CTAO at 1
TeV for the `South_z20_50h` configuration used for the CTA 1DC
simulation?
-- Get the latest CTA FITS performance files from
- https://www.cta-observatory.org/science/cta-performance/ and run the
+- Get the latest CTAO FITS performance files from
+ https://www.ctao.org/for-scientists/performance/ and run the
code example above. Make an effective area ratio plot of 40 deg
zenith versus 20 deg zenith for the `South_z40_50h` and
`South_z20_50h` configurations.
@@ -866,7 +866,7 @@ Next steps
:doc:`/tutorials/starting/analysis_1` and
:doc:`/tutorials/starting/analysis_2` or any other
Gammapy analysis tutorial.
-- Learn how to evaluate CTA observability and sensitivity with
+- Learn how to evaluate CTAO observability and sensitivity with
:doc:`/tutorials/analysis-3d/simulate_3d`,
:doc:`/tutorials/analysis-1d/spectrum_simulation`
or :doc:`/tutorials/analysis-1d/cta_sensitivity`.
diff --git a/docs/dev/_sources/tutorials/data/fermi_lat.rst.txt b/docs/dev/_sources/tutorials/data/fermi_lat.rst.txt
index 787db6116ba..febd79764eb 100644
--- a/docs/dev/_sources/tutorials/data/fermi_lat.rst.txt
+++ b/docs/dev/_sources/tutorials/data/fermi_lat.rst.txt
@@ -140,7 +140,7 @@ Check setup
Gammapy package:
- version : 1.3.dev1143+ge26e20052
+ version : 1.3.dev1180+gb03e9b8c7
path : /home/runner/work/gammapy-docs/gammapy-docs/gammapy/.tox/build_docs/lib/python3.9/site-packages/gammapy
diff --git a/docs/dev/_sources/tutorials/data/hawc.rst.txt b/docs/dev/_sources/tutorials/data/hawc.rst.txt
index a9560212fc2..458c9957afc 100644
--- a/docs/dev/_sources/tutorials/data/hawc.rst.txt
+++ b/docs/dev/_sources/tutorials/data/hawc.rst.txt
@@ -47,7 +47,7 @@ proceeding.
Once the data has been reduced to a MapDataset, there are no differences
in the way that HAWC data is handled with respect to data from any other
-observatory, such as H.E.S.S. or CTA.
+observatory, such as H.E.S.S. or CTAO.
HAWC data access and reduction
@@ -108,7 +108,7 @@ Check setup
Gammapy package:
- version : 1.3.dev1143+ge26e20052
+ version : 1.3.dev1180+gb03e9b8c7
path : /home/runner/work/gammapy-docs/gammapy-docs/gammapy/.tox/build_docs/lib/python3.9/site-packages/gammapy
diff --git a/docs/dev/_sources/tutorials/data/hess.rst.txt b/docs/dev/_sources/tutorials/data/hess.rst.txt
index 8be2f223987..1820344468e 100644
--- a/docs/dev/_sources/tutorials/data/hess.rst.txt
+++ b/docs/dev/_sources/tutorials/data/hess.rst.txt
@@ -29,7 +29,7 @@ current `open data level 3
format `__.
The H.E.S.S. data is private, and H.E.S.S. analysis is mostly documented
-and discussed at https://hess-confluence.desy.de/ and in
+and discussed in the internal Wiki pages and in
H.E.S.S.-internal communication channels. However, in 2018, a small
sub-set of archival H.E.S.S. data was publicly released, called the
`H.E.S.S. DL3
@@ -45,9 +45,8 @@ simple exploration of the data with the creation of theta-squared plot.
H.E.S.S. members can find details on the DL3 FITS production on this
`Confluence
-page `__
-and access more detailed tutorials in this
-`repository `__
+page `__
+and access more detailed tutorials in the BitBucket `hess-open-tools` repository.
DL3 DR1
-------
@@ -55,7 +54,7 @@ DL3 DR1
This is how to access data and IRFs from the H.E.S.S. data level 3, data
release 1.
-.. GENERATED FROM PYTHON SOURCE LINES 40-51
+.. GENERATED FROM PYTHON SOURCE LINES 39-50
.. code-block:: Python
@@ -77,12 +76,12 @@ release 1.
-.. GENERATED FROM PYTHON SOURCE LINES 52-54
+.. GENERATED FROM PYTHON SOURCE LINES 51-53
Check setup
-----------
-.. GENERATED FROM PYTHON SOURCE LINES 54-60
+.. GENERATED FROM PYTHON SOURCE LINES 53-59
.. code-block:: Python
@@ -111,7 +110,7 @@ Check setup
Gammapy package:
- version : 1.3.dev1143+ge26e20052
+ version : 1.3.dev1180+gb03e9b8c7
path : /home/runner/work/gammapy-docs/gammapy-docs/gammapy/.tox/build_docs/lib/python3.9/site-packages/gammapy
@@ -144,7 +143,7 @@ Check setup
-.. GENERATED FROM PYTHON SOURCE LINES 61-69
+.. GENERATED FROM PYTHON SOURCE LINES 60-68
A useful way to organize the relevant files are the index tables. The
observation index table contains information on each particular run,
@@ -155,11 +154,11 @@ the directory in which they can be found, in this case
`$GAMMAPY_DATA/hess-dl3-dr1`:
-.. GENERATED FROM PYTHON SOURCE LINES 71-72
+.. GENERATED FROM PYTHON SOURCE LINES 70-71
Create and get info on the data store
-.. GENERATED FROM PYTHON SOURCE LINES 72-77
+.. GENERATED FROM PYTHON SOURCE LINES 71-76
.. code-block:: Python
@@ -193,11 +192,11 @@ Create and get info on the data store
-.. GENERATED FROM PYTHON SOURCE LINES 78-79
+.. GENERATED FROM PYTHON SOURCE LINES 77-78
Preview an excerpt from the observation table
-.. GENERATED FROM PYTHON SOURCE LINES 79-82
+.. GENERATED FROM PYTHON SOURCE LINES 78-81
.. code-block:: Python
@@ -221,11 +220,11 @@ Preview an excerpt from the observation table
-.. GENERATED FROM PYTHON SOURCE LINES 83-84
+.. GENERATED FROM PYTHON SOURCE LINES 82-83
Get a single observation
-.. GENERATED FROM PYTHON SOURCE LINES 84-87
+.. GENERATED FROM PYTHON SOURCE LINES 83-86
.. code-block:: Python
@@ -239,11 +238,11 @@ Get a single observation
-.. GENERATED FROM PYTHON SOURCE LINES 88-89
+.. GENERATED FROM PYTHON SOURCE LINES 87-88
Select and peek events
-.. GENERATED FROM PYTHON SOURCE LINES 89-92
+.. GENERATED FROM PYTHON SOURCE LINES 88-91
.. code-block:: Python
@@ -262,11 +261,11 @@ Select and peek events
-.. GENERATED FROM PYTHON SOURCE LINES 93-94
+.. GENERATED FROM PYTHON SOURCE LINES 92-93
Peek the effective area
-.. GENERATED FROM PYTHON SOURCE LINES 94-97
+.. GENERATED FROM PYTHON SOURCE LINES 93-96
.. code-block:: Python
@@ -292,11 +291,11 @@ Peek the effective area
-.. GENERATED FROM PYTHON SOURCE LINES 98-99
+.. GENERATED FROM PYTHON SOURCE LINES 97-98
Peek the energy dispersion
-.. GENERATED FROM PYTHON SOURCE LINES 99-102
+.. GENERATED FROM PYTHON SOURCE LINES 98-101
.. code-block:: Python
@@ -315,11 +314,11 @@ Peek the energy dispersion
-.. GENERATED FROM PYTHON SOURCE LINES 103-104
+.. GENERATED FROM PYTHON SOURCE LINES 102-103
Peek the psf
-.. GENERATED FROM PYTHON SOURCE LINES 104-106
+.. GENERATED FROM PYTHON SOURCE LINES 103-105
.. code-block:: Python
@@ -337,11 +336,11 @@ Peek the psf
-.. GENERATED FROM PYTHON SOURCE LINES 107-108
+.. GENERATED FROM PYTHON SOURCE LINES 106-107
Peek the background rate
-.. GENERATED FROM PYTHON SOURCE LINES 108-111
+.. GENERATED FROM PYTHON SOURCE LINES 107-110
.. code-block:: Python
@@ -360,7 +359,7 @@ Peek the background rate
-.. GENERATED FROM PYTHON SOURCE LINES 112-118
+.. GENERATED FROM PYTHON SOURCE LINES 111-117
Theta squared event distribution
--------------------------------
@@ -369,7 +368,7 @@ As a quick look plot it can be helpful to plot the quadratic offset
(theta squared) distribution of the events.
-.. GENERATED FROM PYTHON SOURCE LINES 118-133
+.. GENERATED FROM PYTHON SOURCE LINES 117-132
.. code-block:: Python
@@ -400,7 +399,7 @@ As a quick look plot it can be helpful to plot the quadratic offset
-.. GENERATED FROM PYTHON SOURCE LINES 134-142
+.. GENERATED FROM PYTHON SOURCE LINES 133-141
Exercises
---------
@@ -411,13 +410,13 @@ Exercises
background IRF.
-.. GENERATED FROM PYTHON SOURCE LINES 145-152
+.. GENERATED FROM PYTHON SOURCE LINES 144-151
Next steps
----------
Now you know how to access and work with H.E.S.S. data. All other
-tutorials and documentation apply to H.E.S.S. and CTA or any other IACT
+tutorials and documentation apply to H.E.S.S. and CTAO or any other IACT
that provides DL3 data and IRFs in the standard format.
diff --git a/docs/dev/_sources/tutorials/data/sg_execution_times.rst.txt b/docs/dev/_sources/tutorials/data/sg_execution_times.rst.txt
index 664b7b56494..de66aeeb866 100644
--- a/docs/dev/_sources/tutorials/data/sg_execution_times.rst.txt
+++ b/docs/dev/_sources/tutorials/data/sg_execution_times.rst.txt
@@ -6,7 +6,7 @@
Computation times
=================
-**00:23.059** total execution time for 4 files **from tutorials/data**:
+**00:21.446** total execution time for 4 files **from tutorials/data**:
.. container::
@@ -33,14 +33,14 @@ Computation times
- Time
- Mem (MB)
* - :ref:`sphx_glr_tutorials_data_hawc.py` (``hawc.py``)
- - 00:07.256
+ - 00:06.689
- 0.0
* - :ref:`sphx_glr_tutorials_data_fermi_lat.py` (``fermi_lat.py``)
- - 00:06.673
+ - 00:06.263
- 0.0
* - :ref:`sphx_glr_tutorials_data_cta.py` (``cta.py``)
- - 00:05.525
+ - 00:05.234
- 0.0
* - :ref:`sphx_glr_tutorials_data_hess.py` (``hess.py``)
- - 00:03.605
+ - 00:03.259
- 0.0
diff --git a/docs/dev/_sources/tutorials/index.rst.txt b/docs/dev/_sources/tutorials/index.rst.txt
index fa609617354..fc5283f019e 100644
--- a/docs/dev/_sources/tutorials/index.rst.txt
+++ b/docs/dev/_sources/tutorials/index.rst.txt
@@ -141,7 +141,7 @@ event lists according to different criteria, as well as to get a quick look of t
.. raw:: html
-
+
.. only:: html
@@ -152,7 +152,7 @@ event lists according to different criteria, as well as to get a quick look of t
.. raw:: html
-
CTA with Gammapy
+
CTAO with Gammapy
@@ -241,7 +241,7 @@ time-dependent analysis with light-curves.
.. raw:: html
-
+
.. only:: html
diff --git a/docs/dev/_sources/tutorials/scripts/sg_execution_times.rst.txt b/docs/dev/_sources/tutorials/scripts/sg_execution_times.rst.txt
index 7a260c3e989..8bb569250f1 100644
--- a/docs/dev/_sources/tutorials/scripts/sg_execution_times.rst.txt
+++ b/docs/dev/_sources/tutorials/scripts/sg_execution_times.rst.txt
@@ -6,7 +6,7 @@
Computation times
=================
-**00:02.511** total execution time for 1 file **from tutorials/scripts**:
+**00:02.499** total execution time for 1 file **from tutorials/scripts**:
.. container::
@@ -33,5 +33,5 @@ Computation times
- Time
- Mem (MB)
* - :ref:`sphx_glr_tutorials_scripts_survey_map.py` (``survey_map.py``)
- - 00:02.511
+ - 00:02.499
- 0.0
diff --git a/docs/dev/_sources/tutorials/starting/analysis_1.rst.txt b/docs/dev/_sources/tutorials/starting/analysis_1.rst.txt
index 97936c3062a..26eab45b488 100644
--- a/docs/dev/_sources/tutorials/starting/analysis_1.rst.txt
+++ b/docs/dev/_sources/tutorials/starting/analysis_1.rst.txt
@@ -138,7 +138,7 @@ Check setup
Gammapy package:
- version : 1.3.dev1143+ge26e20052
+ version : 1.3.dev1180+gb03e9b8c7
path : /home/runner/work/gammapy-docs/gammapy-docs/gammapy/.tox/build_docs/lib/python3.9/site-packages/gammapy
@@ -310,8 +310,8 @@ Here is what the configuration for our analysis looks like:
parameters:
selection_optional: all
metadata:
- creator: Gammapy 1.3.dev1143+ge26e20052
- date: '2024-10-11T08:27:53.021569'
+ creator: Gammapy 1.3.dev1180+gb03e9b8c7
+ date: '2024-10-11T09:59:41.447240'
origin: null
@@ -628,8 +628,8 @@ One can export/import the `~gammapy.modeling.AnalysisConfig` to/from a YAML file
parameters:
selection_optional: all
metadata:
- creator: Gammapy 1.3.dev1143+ge26e20052
- date: '2024-10-11T08:27:53.048716'
+ creator: Gammapy 1.3.dev1180+gb03e9b8c7
+ date: '2024-10-11T09:59:41.473779'
origin: null
@@ -1183,8 +1183,8 @@ This is how we can write the model back to file again:
unit: TeV
covariance: model-best-fit_covariance.dat
metadata:
- creator: Gammapy 1.3.dev1143+ge26e20052
- date: '2024-10-11T08:28:01.911387'
+ creator: Gammapy 1.3.dev1180+gb03e9b8c7
+ date: '2024-10-11T09:59:50.284234'
origin: null
@@ -1337,7 +1337,7 @@ You can see how to perform a 1D spectral analysis of the same data in
.. rst-class:: sphx-glr-timing
- **Total running time of the script:** (0 minutes 15.384 seconds)
+ **Total running time of the script:** (0 minutes 15.326 seconds)
.. _sphx_glr_download_tutorials_starting_analysis_1.py:
diff --git a/docs/dev/_sources/tutorials/starting/analysis_2.rst.txt b/docs/dev/_sources/tutorials/starting/analysis_2.rst.txt
index a775591b76c..146a8689aca 100644
--- a/docs/dev/_sources/tutorials/starting/analysis_2.rst.txt
+++ b/docs/dev/_sources/tutorials/starting/analysis_2.rst.txt
@@ -154,7 +154,7 @@ Check setup
Gammapy package:
- version : 1.3.dev1143+ge26e20052
+ version : 1.3.dev1180+gb03e9b8c7
path : /home/runner/work/gammapy-docs/gammapy-docs/gammapy/.tox/build_docs/lib/python3.9/site-packages/gammapy
diff --git a/docs/dev/_sources/tutorials/starting/overview.rst.txt b/docs/dev/_sources/tutorials/starting/overview.rst.txt
index 71e340c8efb..eae65b64331 100644
--- a/docs/dev/_sources/tutorials/starting/overview.rst.txt
+++ b/docs/dev/_sources/tutorials/starting/overview.rst.txt
@@ -137,7 +137,7 @@ Check setup
Gammapy package:
- version : 1.3.dev1143+ge26e20052
+ version : 1.3.dev1180+gb03e9b8c7
path : /home/runner/work/gammapy-docs/gammapy-docs/gammapy/.tox/build_docs/lib/python3.9/site-packages/gammapy
diff --git a/docs/dev/_sources/tutorials/starting/sg_execution_times.rst.txt b/docs/dev/_sources/tutorials/starting/sg_execution_times.rst.txt
index 081a836e261..51f51a9d858 100644
--- a/docs/dev/_sources/tutorials/starting/sg_execution_times.rst.txt
+++ b/docs/dev/_sources/tutorials/starting/sg_execution_times.rst.txt
@@ -6,7 +6,7 @@
Computation times
=================
-**00:24.400** total execution time for 3 files **from tutorials/starting**:
+**00:24.351** total execution time for 3 files **from tutorials/starting**:
.. container::
@@ -33,11 +33,11 @@ Computation times
- Time
- Mem (MB)
* - :ref:`sphx_glr_tutorials_starting_analysis_1.py` (``analysis_1.py``)
- - 00:15.384
+ - 00:15.326
- 0.0
* - :ref:`sphx_glr_tutorials_starting_analysis_2.py` (``analysis_2.py``)
- - 00:07.749
+ - 00:07.665
- 0.0
* - :ref:`sphx_glr_tutorials_starting_overview.py` (``overview.py``)
- - 00:01.267
+ - 00:01.360
- 0.0
diff --git a/docs/dev/_sources/user-guide/astro/darkmatter/index.rst.txt b/docs/dev/_sources/user-guide/astro/darkmatter/index.rst.txt
index 2509f74c846..daf81c33cbb 100644
--- a/docs/dev/_sources/user-guide/astro/darkmatter/index.rst.txt
+++ b/docs/dev/_sources/user-guide/astro/darkmatter/index.rst.txt
@@ -84,7 +84,7 @@ gamLike
`GamLike`_ contains likelihood functions for most leading gamma-ray indirect
searches for dark matter, including Fermi-LAT observations of dwarfs and the
Galactic Centre (GC), HESS observations of the GC, and projected sensitivities
-for CTA observations of the GC. It is released in tandem with the `GAMBIT`_
+for CTAO observations of the GC. It is released in tandem with the `GAMBIT`_
module `DarkBit`_. DarkBit can be used for directly computing observables and
likelihoods, for any combination of parameter values in some underlying
particle model.
diff --git a/docs/dev/_sources/user-guide/howto.rst.txt b/docs/dev/_sources/user-guide/howto.rst.txt
index d7ce187f7d5..a058d500afb 100644
--- a/docs/dev/_sources/user-guide/howto.rst.txt
+++ b/docs/dev/_sources/user-guide/howto.rst.txt
@@ -179,7 +179,7 @@ It is possible to combine Gammapy with astrophysical modeling codes, if they
provide a Python interface. Usually this requires some glue code to be written,
e.g. `~gammapy.modeling.models.NaimaSpectralModel` is an example of a Gammapy
wrapper class around the Naima spectral model and radiation classes, which then
-allows modeling and fitting of Naima models within Gammapy (e.g. using CTA,
+allows modeling and fitting of Naima models within Gammapy (e.g. using CTAO,
H.E.S.S. or Fermi-LAT data).
.. accordion-footer::
@@ -327,7 +327,8 @@ Note that you can create your own style with matplotlib (see
`here `__ and
`here `__)
-The CTA observatory released a document describing best practices for **data visualisation in a way friendly to
+.. TODO: update the link
+The CTAO observatory released a document describing best practices for **data visualisation in a way friendly to
color-blind people**:
`CTAO document `_. To
use them, you should add into your notebooks or scripts the following lines after the Gammapy imports:
diff --git a/docs/dev/_sources/user-guide/model-gallery/spatial/plot_constant.rst.txt b/docs/dev/_sources/user-guide/model-gallery/spatial/plot_constant.rst.txt
index 9404cf8f729..b9e21c707b4 100644
--- a/docs/dev/_sources/user-guide/model-gallery/spatial/plot_constant.rst.txt
+++ b/docs/dev/_sources/user-guide/model-gallery/spatial/plot_constant.rst.txt
@@ -110,8 +110,8 @@ Here is an example YAML file using the model:
type: ConstantSpatialModel
parameters: []
metadata:
- creator: Gammapy 1.3.dev1143+ge26e20052
- date: '2024-10-11T08:27:38.032406'
+ creator: Gammapy 1.3.dev1180+gb03e9b8c7
+ date: '2024-10-11T09:59:26.664097'
origin: null
diff --git a/docs/dev/_sources/user-guide/model-gallery/spatial/plot_disk.rst.txt b/docs/dev/_sources/user-guide/model-gallery/spatial/plot_disk.rst.txt
index cf09e1e834b..deb1083eb7e 100644
--- a/docs/dev/_sources/user-guide/model-gallery/spatial/plot_disk.rst.txt
+++ b/docs/dev/_sources/user-guide/model-gallery/spatial/plot_disk.rst.txt
@@ -232,8 +232,8 @@ Here is an example YAML file using the model:
- name: edge_width
value: 0.01
metadata:
- creator: Gammapy 1.3.dev1143+ge26e20052
- date: '2024-10-11T08:27:38.469500'
+ creator: Gammapy 1.3.dev1180+gb03e9b8c7
+ date: '2024-10-11T09:59:27.102251'
origin: null
diff --git a/docs/dev/_sources/user-guide/model-gallery/spatial/plot_gauss.rst.txt b/docs/dev/_sources/user-guide/model-gallery/spatial/plot_gauss.rst.txt
index c2ca39466a1..61ca01005a7 100644
--- a/docs/dev/_sources/user-guide/model-gallery/spatial/plot_gauss.rst.txt
+++ b/docs/dev/_sources/user-guide/model-gallery/spatial/plot_gauss.rst.txt
@@ -190,8 +190,8 @@ Here is an example YAML file using the model:
value: 0.0
unit: deg
metadata:
- creator: Gammapy 1.3.dev1143+ge26e20052
- date: '2024-10-11T08:27:38.801929'
+ creator: Gammapy 1.3.dev1180+gb03e9b8c7
+ date: '2024-10-11T09:59:27.426205'
origin: null
diff --git a/docs/dev/_sources/user-guide/model-gallery/spatial/plot_gen_gauss.rst.txt b/docs/dev/_sources/user-guide/model-gallery/spatial/plot_gen_gauss.rst.txt
index 3f09d938019..5ec0643c90a 100644
--- a/docs/dev/_sources/user-guide/model-gallery/spatial/plot_gen_gauss.rst.txt
+++ b/docs/dev/_sources/user-guide/model-gallery/spatial/plot_gen_gauss.rst.txt
@@ -182,8 +182,8 @@ Here is an example YAML file using the model:
value: 0.0
unit: deg
metadata:
- creator: Gammapy 1.3.dev1143+ge26e20052
- date: '2024-10-11T08:27:39.145591'
+ creator: Gammapy 1.3.dev1180+gb03e9b8c7
+ date: '2024-10-11T09:59:27.769762'
origin: null
diff --git a/docs/dev/_sources/user-guide/model-gallery/spatial/plot_piecewise_norm_spatial.rst.txt b/docs/dev/_sources/user-guide/model-gallery/spatial/plot_piecewise_norm_spatial.rst.txt
index a42da6499d0..55662a89a0a 100644
--- a/docs/dev/_sources/user-guide/model-gallery/spatial/plot_piecewise_norm_spatial.rst.txt
+++ b/docs/dev/_sources/user-guide/model-gallery/spatial/plot_piecewise_norm_spatial.rst.txt
@@ -141,8 +141,8 @@ Here is an example YAML file using the model:
- -1.785
unit: deg
metadata:
- creator: Gammapy 1.3.dev1143+ge26e20052
- date: '2024-10-11T08:27:39.402378'
+ creator: Gammapy 1.3.dev1180+gb03e9b8c7
+ date: '2024-10-11T09:59:28.022676'
origin: null
diff --git a/docs/dev/_sources/user-guide/model-gallery/spatial/plot_point.rst.txt b/docs/dev/_sources/user-guide/model-gallery/spatial/plot_point.rst.txt
index 71f29a3d874..ad3ccd4c5b9 100644
--- a/docs/dev/_sources/user-guide/model-gallery/spatial/plot_point.rst.txt
+++ b/docs/dev/_sources/user-guide/model-gallery/spatial/plot_point.rst.txt
@@ -133,8 +133,8 @@ Here is an example YAML file using the model:
value: 0.0
unit: deg
metadata:
- creator: Gammapy 1.3.dev1143+ge26e20052
- date: '2024-10-11T08:27:39.725954'
+ creator: Gammapy 1.3.dev1180+gb03e9b8c7
+ date: '2024-10-11T09:59:28.343796'
origin: null
diff --git a/docs/dev/_sources/user-guide/model-gallery/spatial/plot_shell.rst.txt b/docs/dev/_sources/user-guide/model-gallery/spatial/plot_shell.rst.txt
index b9906b68c13..04f6c6e9b32 100644
--- a/docs/dev/_sources/user-guide/model-gallery/spatial/plot_shell.rst.txt
+++ b/docs/dev/_sources/user-guide/model-gallery/spatial/plot_shell.rst.txt
@@ -145,8 +145,8 @@ Here is an example YAML file using the model:
value: 0.2
unit: deg
metadata:
- creator: Gammapy 1.3.dev1143+ge26e20052
- date: '2024-10-11T08:27:40.024408'
+ creator: Gammapy 1.3.dev1180+gb03e9b8c7
+ date: '2024-10-11T09:59:28.638011'
origin: null
diff --git a/docs/dev/_sources/user-guide/model-gallery/spatial/plot_shell2.rst.txt b/docs/dev/_sources/user-guide/model-gallery/spatial/plot_shell2.rst.txt
index 34c05251cfe..b20597494e8 100644
--- a/docs/dev/_sources/user-guide/model-gallery/spatial/plot_shell2.rst.txt
+++ b/docs/dev/_sources/user-guide/model-gallery/spatial/plot_shell2.rst.txt
@@ -157,8 +157,8 @@ Here is an example YAML file using the model:
- name: eta
value: 0.2
metadata:
- creator: Gammapy 1.3.dev1143+ge26e20052
- date: '2024-10-11T08:27:40.321851'
+ creator: Gammapy 1.3.dev1180+gb03e9b8c7
+ date: '2024-10-11T09:59:28.935576'
origin: null
diff --git a/docs/dev/_sources/user-guide/model-gallery/spatial/plot_template.rst.txt b/docs/dev/_sources/user-guide/model-gallery/spatial/plot_template.rst.txt
index b02d651b13d..7a7250cd00b 100644
--- a/docs/dev/_sources/user-guide/model-gallery/spatial/plot_template.rst.txt
+++ b/docs/dev/_sources/user-guide/model-gallery/spatial/plot_template.rst.txt
@@ -129,8 +129,8 @@ Here is an example YAML file using the model:
normalize: true
unit: 1 / sr
metadata:
- creator: Gammapy 1.3.dev1143+ge26e20052
- date: '2024-10-11T08:27:40.671093'
+ creator: Gammapy 1.3.dev1180+gb03e9b8c7
+ date: '2024-10-11T09:59:29.276248'
origin: null
diff --git a/docs/dev/_sources/user-guide/model-gallery/spatial/sg_execution_times.rst.txt b/docs/dev/_sources/user-guide/model-gallery/spatial/sg_execution_times.rst.txt
index 7612b503216..e9583949294 100644
--- a/docs/dev/_sources/user-guide/model-gallery/spatial/sg_execution_times.rst.txt
+++ b/docs/dev/_sources/user-guide/model-gallery/spatial/sg_execution_times.rst.txt
@@ -6,7 +6,7 @@
Computation times
=================
-**00:02.050** total execution time for 9 files **from user-guide/model-gallery/spatial**:
+**00:02.058** total execution time for 9 files **from user-guide/model-gallery/spatial**:
.. container::
@@ -33,10 +33,10 @@ Computation times
- Time
- Mem (MB)
* - :ref:`sphx_glr_user-guide_model-gallery_spatial_plot_constant.py` (``plot_constant.py``)
- - 00:00.352
+ - 00:00.369
- 0.0
* - :ref:`sphx_glr_user-guide_model-gallery_spatial_plot_disk.py` (``plot_disk.py``)
- - 00:00.317
+ - 00:00.319
- 0.0
* - :ref:`sphx_glr_user-guide_model-gallery_spatial_plot_template.py` (``plot_template.py``)
- 00:00.229
@@ -45,17 +45,17 @@ Computation times
- 00:00.224
- 0.0
* - :ref:`sphx_glr_user-guide_model-gallery_spatial_plot_gauss.py` (``plot_gauss.py``)
- - 00:00.215
+ - 00:00.211
- 0.0
* - :ref:`sphx_glr_user-guide_model-gallery_spatial_plot_point.py` (``plot_point.py``)
- - 00:00.203
+ - 00:00.201
- 0.0
* - :ref:`sphx_glr_user-guide_model-gallery_spatial_plot_shell.py` (``plot_shell.py``)
- - 00:00.186
+ - 00:00.185
- 0.0
* - :ref:`sphx_glr_user-guide_model-gallery_spatial_plot_shell2.py` (``plot_shell2.py``)
- 00:00.177
- 0.0
* - :ref:`sphx_glr_user-guide_model-gallery_spatial_plot_piecewise_norm_spatial.py` (``plot_piecewise_norm_spatial.py``)
- - 00:00.146
+ - 00:00.143
- 0.0
diff --git a/docs/dev/_sources/user-guide/model-gallery/spectral/plot_absorbed.rst.txt b/docs/dev/_sources/user-guide/model-gallery/spectral/plot_absorbed.rst.txt
index ceb7e1f691f..06c68975aa7 100644
--- a/docs/dev/_sources/user-guide/model-gallery/spectral/plot_absorbed.rst.txt
+++ b/docs/dev/_sources/user-guide/model-gallery/spectral/plot_absorbed.rst.txt
@@ -185,8 +185,8 @@ Here is an example YAML file using the model:
filename: /home/runner/work/gammapy-docs/gammapy-docs/gammapy-datasets/dev/ebl/ebl_dominguez11.fits.gz
operator: mul
metadata:
- creator: Gammapy 1.3.dev1143+ge26e20052
- date: '2024-10-11T08:27:41.844159'
+ creator: Gammapy 1.3.dev1180+gb03e9b8c7
+ date: '2024-10-11T09:59:30.500622'
origin: null
diff --git a/docs/dev/_sources/user-guide/model-gallery/spectral/plot_broken_powerlaw.rst.txt b/docs/dev/_sources/user-guide/model-gallery/spectral/plot_broken_powerlaw.rst.txt
index 0f907e1addb..dd06cc40994 100644
--- a/docs/dev/_sources/user-guide/model-gallery/spectral/plot_broken_powerlaw.rst.txt
+++ b/docs/dev/_sources/user-guide/model-gallery/spectral/plot_broken_powerlaw.rst.txt
@@ -111,8 +111,8 @@ Here is an example YAML file using the model:
value: 1.0
unit: TeV
metadata:
- creator: Gammapy 1.3.dev1143+ge26e20052
- date: '2024-10-11T08:27:42.317479'
+ creator: Gammapy 1.3.dev1180+gb03e9b8c7
+ date: '2024-10-11T09:59:30.951806'
origin: null
diff --git a/docs/dev/_sources/user-guide/model-gallery/spectral/plot_compound.rst.txt b/docs/dev/_sources/user-guide/model-gallery/spectral/plot_compound.rst.txt
index 205289eb261..cbaf9d20751 100644
--- a/docs/dev/_sources/user-guide/model-gallery/spectral/plot_compound.rst.txt
+++ b/docs/dev/_sources/user-guide/model-gallery/spectral/plot_compound.rst.txt
@@ -126,8 +126,8 @@ Here is an example YAML file using the model:
value: 1.0
operator: add
metadata:
- creator: Gammapy 1.3.dev1143+ge26e20052
- date: '2024-10-11T08:27:42.773695'
+ creator: Gammapy 1.3.dev1180+gb03e9b8c7
+ date: '2024-10-11T09:59:31.379851'
origin: null
diff --git a/docs/dev/_sources/user-guide/model-gallery/spectral/plot_constant_spectral.rst.txt b/docs/dev/_sources/user-guide/model-gallery/spectral/plot_constant_spectral.rst.txt
index dde04296dac..3adb73aad3b 100644
--- a/docs/dev/_sources/user-guide/model-gallery/spectral/plot_constant_spectral.rst.txt
+++ b/docs/dev/_sources/user-guide/model-gallery/spectral/plot_constant_spectral.rst.txt
@@ -92,8 +92,8 @@ Here is an example YAML file using the model:
value: 1.0
unit: cm-2 s-1 TeV-1
metadata:
- creator: Gammapy 1.3.dev1143+ge26e20052
- date: '2024-10-11T08:27:43.142852'
+ creator: Gammapy 1.3.dev1180+gb03e9b8c7
+ date: '2024-10-11T09:59:31.729956'
origin: null
diff --git a/docs/dev/_sources/user-guide/model-gallery/spectral/plot_exp_cutoff_powerlaw.rst.txt b/docs/dev/_sources/user-guide/model-gallery/spectral/plot_exp_cutoff_powerlaw.rst.txt
index 7ceb40b5d15..e0be1b77981 100644
--- a/docs/dev/_sources/user-guide/model-gallery/spectral/plot_exp_cutoff_powerlaw.rst.txt
+++ b/docs/dev/_sources/user-guide/model-gallery/spectral/plot_exp_cutoff_powerlaw.rst.txt
@@ -110,8 +110,8 @@ Here is an example YAML file using the model:
- name: alpha
value: 1.0
metadata:
- creator: Gammapy 1.3.dev1143+ge26e20052
- date: '2024-10-11T08:27:43.469253'
+ creator: Gammapy 1.3.dev1180+gb03e9b8c7
+ date: '2024-10-11T09:59:32.041904'
origin: null
diff --git a/docs/dev/_sources/user-guide/model-gallery/spectral/plot_exp_cutoff_powerlaw_3fgl.rst.txt b/docs/dev/_sources/user-guide/model-gallery/spectral/plot_exp_cutoff_powerlaw_3fgl.rst.txt
index 4588f559e89..3fbfb0d449d 100644
--- a/docs/dev/_sources/user-guide/model-gallery/spectral/plot_exp_cutoff_powerlaw_3fgl.rst.txt
+++ b/docs/dev/_sources/user-guide/model-gallery/spectral/plot_exp_cutoff_powerlaw_3fgl.rst.txt
@@ -109,8 +109,8 @@ Here is an example YAML file using the model:
value: 10.0
unit: TeV
metadata:
- creator: Gammapy 1.3.dev1143+ge26e20052
- date: '2024-10-11T08:27:43.792100'
+ creator: Gammapy 1.3.dev1180+gb03e9b8c7
+ date: '2024-10-11T09:59:32.345959'
origin: null
diff --git a/docs/dev/_sources/user-guide/model-gallery/spectral/plot_exp_cutoff_powerlaw_norm_spectral.rst.txt b/docs/dev/_sources/user-guide/model-gallery/spectral/plot_exp_cutoff_powerlaw_norm_spectral.rst.txt
index 1f0f3967e02..0252fc863c6 100644
--- a/docs/dev/_sources/user-guide/model-gallery/spectral/plot_exp_cutoff_powerlaw_norm_spectral.rst.txt
+++ b/docs/dev/_sources/user-guide/model-gallery/spectral/plot_exp_cutoff_powerlaw_norm_spectral.rst.txt
@@ -146,8 +146,8 @@ Here is an example YAML file using the model:
value: 1.0
operator: mul
metadata:
- creator: Gammapy 1.3.dev1143+ge26e20052
- date: '2024-10-11T08:27:44.255235'
+ creator: Gammapy 1.3.dev1180+gb03e9b8c7
+ date: '2024-10-11T09:59:32.797325'
origin: null
diff --git a/docs/dev/_sources/user-guide/model-gallery/spectral/plot_gauss_spectral.rst.txt b/docs/dev/_sources/user-guide/model-gallery/spectral/plot_gauss_spectral.rst.txt
index 327033b177a..7913a2950ea 100644
--- a/docs/dev/_sources/user-guide/model-gallery/spectral/plot_gauss_spectral.rst.txt
+++ b/docs/dev/_sources/user-guide/model-gallery/spectral/plot_gauss_spectral.rst.txt
@@ -108,8 +108,8 @@ Here is an example YAML file using the model:
value: 0.2
unit: TeV
metadata:
- creator: Gammapy 1.3.dev1143+ge26e20052
- date: '2024-10-11T08:27:44.607609'
+ creator: Gammapy 1.3.dev1180+gb03e9b8c7
+ date: '2024-10-11T09:59:33.129108'
origin: null
diff --git a/docs/dev/_sources/user-guide/model-gallery/spectral/plot_logparabola.rst.txt b/docs/dev/_sources/user-guide/model-gallery/spectral/plot_logparabola.rst.txt
index ba1f525398f..00dc094a15b 100644
--- a/docs/dev/_sources/user-guide/model-gallery/spectral/plot_logparabola.rst.txt
+++ b/docs/dev/_sources/user-guide/model-gallery/spectral/plot_logparabola.rst.txt
@@ -118,8 +118,8 @@ Here is an example YAML file using the model:
- name: beta
value: 0.5
metadata:
- creator: Gammapy 1.3.dev1143+ge26e20052
- date: '2024-10-11T08:27:44.929801'
+ creator: Gammapy 1.3.dev1180+gb03e9b8c7
+ date: '2024-10-11T09:59:33.437280'
origin: null
diff --git a/docs/dev/_sources/user-guide/model-gallery/spectral/plot_logparabola_norm_spectral.rst.txt b/docs/dev/_sources/user-guide/model-gallery/spectral/plot_logparabola_norm_spectral.rst.txt
index f2732f65727..20d0fbbbf7e 100644
--- a/docs/dev/_sources/user-guide/model-gallery/spectral/plot_logparabola_norm_spectral.rst.txt
+++ b/docs/dev/_sources/user-guide/model-gallery/spectral/plot_logparabola_norm_spectral.rst.txt
@@ -135,8 +135,8 @@ Here is an example YAML file using the model:
value: 0.0
operator: mul
metadata:
- creator: Gammapy 1.3.dev1143+ge26e20052
- date: '2024-10-11T08:27:45.343004'
+ creator: Gammapy 1.3.dev1180+gb03e9b8c7
+ date: '2024-10-11T09:59:33.811055'
origin: null
diff --git a/docs/dev/_sources/user-guide/model-gallery/spectral/plot_naima.rst.txt b/docs/dev/_sources/user-guide/model-gallery/spectral/plot_naima.rst.txt
index 5922cf550ef..4e79d568039 100644
--- a/docs/dev/_sources/user-guide/model-gallery/spectral/plot_naima.rst.txt
+++ b/docs/dev/_sources/user-guide/model-gallery/spectral/plot_naima.rst.txt
@@ -169,8 +169,8 @@ Here is an example YAML file using the model:
interp: lin
scale_method: scale10
metadata:
- creator: Gammapy 1.3.dev1143+ge26e20052
- date: '2024-10-11T08:27:45.910796'
+ creator: Gammapy 1.3.dev1180+gb03e9b8c7
+ date: '2024-10-11T09:59:34.342318'
origin: null
diff --git a/docs/dev/_sources/user-guide/model-gallery/spectral/plot_piecewise_norm_spectral.rst.txt b/docs/dev/_sources/user-guide/model-gallery/spectral/plot_piecewise_norm_spectral.rst.txt
index 40252a5bc89..cf70fd315a6 100644
--- a/docs/dev/_sources/user-guide/model-gallery/spectral/plot_piecewise_norm_spectral.rst.txt
+++ b/docs/dev/_sources/user-guide/model-gallery/spectral/plot_piecewise_norm_spectral.rst.txt
@@ -134,8 +134,8 @@ Here is an example YAML file using the model:
unit: TeV
operator: mul
metadata:
- creator: Gammapy 1.3.dev1143+ge26e20052
- date: '2024-10-11T08:27:46.268480'
+ creator: Gammapy 1.3.dev1180+gb03e9b8c7
+ date: '2024-10-11T09:59:34.692427'
origin: null
diff --git a/docs/dev/_sources/user-guide/model-gallery/spectral/plot_powerlaw.rst.txt b/docs/dev/_sources/user-guide/model-gallery/spectral/plot_powerlaw.rst.txt
index d86c64a38a5..2660cbd9f62 100644
--- a/docs/dev/_sources/user-guide/model-gallery/spectral/plot_powerlaw.rst.txt
+++ b/docs/dev/_sources/user-guide/model-gallery/spectral/plot_powerlaw.rst.txt
@@ -104,8 +104,8 @@ Here is an example YAML file using the model:
value: 1.0
unit: TeV
metadata:
- creator: Gammapy 1.3.dev1143+ge26e20052
- date: '2024-10-11T08:27:46.708533'
+ creator: Gammapy 1.3.dev1180+gb03e9b8c7
+ date: '2024-10-11T09:59:35.127536'
origin: null
diff --git a/docs/dev/_sources/user-guide/model-gallery/spectral/plot_powerlaw2.rst.txt b/docs/dev/_sources/user-guide/model-gallery/spectral/plot_powerlaw2.rst.txt
index eb7ace6fe7c..5b852864dbd 100644
--- a/docs/dev/_sources/user-guide/model-gallery/spectral/plot_powerlaw2.rst.txt
+++ b/docs/dev/_sources/user-guide/model-gallery/spectral/plot_powerlaw2.rst.txt
@@ -111,8 +111,8 @@ Here is an example YAML file using the model:
value: 10.0
unit: TeV
metadata:
- creator: Gammapy 1.3.dev1143+ge26e20052
- date: '2024-10-11T08:27:47.154660'
+ creator: Gammapy 1.3.dev1180+gb03e9b8c7
+ date: '2024-10-11T09:59:35.564616'
origin: null
diff --git a/docs/dev/_sources/user-guide/model-gallery/spectral/plot_powerlaw_norm_spectral.rst.txt b/docs/dev/_sources/user-guide/model-gallery/spectral/plot_powerlaw_norm_spectral.rst.txt
index e2976ba382d..8caa647683d 100644
--- a/docs/dev/_sources/user-guide/model-gallery/spectral/plot_powerlaw_norm_spectral.rst.txt
+++ b/docs/dev/_sources/user-guide/model-gallery/spectral/plot_powerlaw_norm_spectral.rst.txt
@@ -132,8 +132,8 @@ Here is an example YAML file using the model:
unit: TeV
operator: mul
metadata:
- creator: Gammapy 1.3.dev1143+ge26e20052
- date: '2024-10-11T08:27:47.550055'
+ creator: Gammapy 1.3.dev1180+gb03e9b8c7
+ date: '2024-10-11T09:59:35.950968'
origin: null
diff --git a/docs/dev/_sources/user-guide/model-gallery/spectral/plot_smooth_broken_powerlaw.rst.txt b/docs/dev/_sources/user-guide/model-gallery/spectral/plot_smooth_broken_powerlaw.rst.txt
index 62b698a1316..95e7fa182d7 100644
--- a/docs/dev/_sources/user-guide/model-gallery/spectral/plot_smooth_broken_powerlaw.rst.txt
+++ b/docs/dev/_sources/user-guide/model-gallery/spectral/plot_smooth_broken_powerlaw.rst.txt
@@ -114,8 +114,8 @@ Here is an example YAML file using the model:
- name: beta
value: 1.0
metadata:
- creator: Gammapy 1.3.dev1143+ge26e20052
- date: '2024-10-11T08:27:47.996746'
+ creator: Gammapy 1.3.dev1180+gb03e9b8c7
+ date: '2024-10-11T09:59:36.383601'
origin: null
diff --git a/docs/dev/_sources/user-guide/model-gallery/spectral/plot_super_exp_cutoff_powerlaw_3fgl.rst.txt b/docs/dev/_sources/user-guide/model-gallery/spectral/plot_super_exp_cutoff_powerlaw_3fgl.rst.txt
index ae274418cbc..f26b83a99a3 100644
--- a/docs/dev/_sources/user-guide/model-gallery/spectral/plot_super_exp_cutoff_powerlaw_3fgl.rst.txt
+++ b/docs/dev/_sources/user-guide/model-gallery/spectral/plot_super_exp_cutoff_powerlaw_3fgl.rst.txt
@@ -125,8 +125,8 @@ Here is an example YAML file using the model:
- name: index_2
value: 2.0
metadata:
- creator: Gammapy 1.3.dev1143+ge26e20052
- date: '2024-10-11T08:27:48.346622'
+ creator: Gammapy 1.3.dev1180+gb03e9b8c7
+ date: '2024-10-11T09:59:36.716755'
origin: null
diff --git a/docs/dev/_sources/user-guide/model-gallery/spectral/plot_super_exp_cutoff_powerlaw_4fgl.rst.txt b/docs/dev/_sources/user-guide/model-gallery/spectral/plot_super_exp_cutoff_powerlaw_4fgl.rst.txt
index 5511514b932..df18a47857a 100644
--- a/docs/dev/_sources/user-guide/model-gallery/spectral/plot_super_exp_cutoff_powerlaw_4fgl.rst.txt
+++ b/docs/dev/_sources/user-guide/model-gallery/spectral/plot_super_exp_cutoff_powerlaw_4fgl.rst.txt
@@ -124,8 +124,8 @@ Here is an example YAML file using the model:
- name: index_2
value: 2.0
metadata:
- creator: Gammapy 1.3.dev1143+ge26e20052
- date: '2024-10-11T08:27:48.693127'
+ creator: Gammapy 1.3.dev1180+gb03e9b8c7
+ date: '2024-10-11T09:59:37.049222'
origin: null
diff --git a/docs/dev/_sources/user-guide/model-gallery/spectral/plot_super_exp_cutoff_powerlaw_4fgl_dr1.rst.txt b/docs/dev/_sources/user-guide/model-gallery/spectral/plot_super_exp_cutoff_powerlaw_4fgl_dr1.rst.txt
index c8ba8f82a02..83bdd9cb36f 100644
--- a/docs/dev/_sources/user-guide/model-gallery/spectral/plot_super_exp_cutoff_powerlaw_4fgl_dr1.rst.txt
+++ b/docs/dev/_sources/user-guide/model-gallery/spectral/plot_super_exp_cutoff_powerlaw_4fgl_dr1.rst.txt
@@ -126,8 +126,8 @@ Here is an example YAML file using the model:
- name: index_2
value: 2.0
metadata:
- creator: Gammapy 1.3.dev1143+ge26e20052
- date: '2024-10-11T08:27:49.031173'
+ creator: Gammapy 1.3.dev1180+gb03e9b8c7
+ date: '2024-10-11T09:59:37.372911'
origin: null
diff --git a/docs/dev/_sources/user-guide/model-gallery/spectral/plot_template_spectral.rst.txt b/docs/dev/_sources/user-guide/model-gallery/spectral/plot_template_spectral.rst.txt
index 651a7d9c07c..478b51212d9 100644
--- a/docs/dev/_sources/user-guide/model-gallery/spectral/plot_template_spectral.rst.txt
+++ b/docs/dev/_sources/user-guide/model-gallery/spectral/plot_template_spectral.rst.txt
@@ -116,7 +116,7 @@ The following shows how to implement extrapolation of a template spectral model:
.. code-block:: none
-
+
@@ -203,8 +203,8 @@ Here is an example YAML file using the model:
- 3.9e-39
unit: 1 / (cm2 MeV s)
metadata:
- creator: Gammapy 1.3.dev1143+ge26e20052
- date: '2024-10-11T08:27:49.594229'
+ creator: Gammapy 1.3.dev1180+gb03e9b8c7
+ date: '2024-10-11T09:59:37.920370'
origin: null
diff --git a/docs/dev/_sources/user-guide/model-gallery/spectral/sg_execution_times.rst.txt b/docs/dev/_sources/user-guide/model-gallery/spectral/sg_execution_times.rst.txt
index 65912997aac..0bfb7867893 100644
--- a/docs/dev/_sources/user-guide/model-gallery/spectral/sg_execution_times.rst.txt
+++ b/docs/dev/_sources/user-guide/model-gallery/spectral/sg_execution_times.rst.txt
@@ -6,7 +6,7 @@
Computation times
=================
-**00:06.414** total execution time for 20 files **from user-guide/model-gallery/spectral**:
+**00:06.385** total execution time for 20 files **from user-guide/model-gallery/spectral**:
.. container::
@@ -33,62 +33,62 @@ Computation times
- Time
- Mem (MB)
* - :ref:`sphx_glr_user-guide_model-gallery_spectral_plot_absorbed.py` (``plot_absorbed.py``)
- - 00:01.001
+ - 00:01.055
- 0.0
* - :ref:`sphx_glr_user-guide_model-gallery_spectral_plot_template_spectral.py` (``plot_template_spectral.py``)
- - 00:00.449
+ - 00:00.446
- 0.0
* - :ref:`sphx_glr_user-guide_model-gallery_spectral_plot_naima.py` (``plot_naima.py``)
- - 00:00.430
+ - 00:00.419
- 0.0
* - :ref:`sphx_glr_user-guide_model-gallery_spectral_plot_exp_cutoff_powerlaw_norm_spectral.py` (``plot_exp_cutoff_powerlaw_norm_spectral.py``)
- - 00:00.345
+ - 00:00.343
- 0.0
- * - :ref:`sphx_glr_user-guide_model-gallery_spectral_plot_broken_powerlaw.py` (``plot_broken_powerlaw.py``)
+ * - :ref:`sphx_glr_user-guide_model-gallery_spectral_plot_powerlaw.py` (``plot_powerlaw.py``)
- 00:00.331
- 0.0
- * - :ref:`sphx_glr_user-guide_model-gallery_spectral_plot_compound.py` (``plot_compound.py``)
- - 00:00.327
+ * - :ref:`sphx_glr_user-guide_model-gallery_spectral_plot_powerlaw2.py` (``plot_powerlaw2.py``)
+ - 00:00.324
- 0.0
* - :ref:`sphx_glr_user-guide_model-gallery_spectral_plot_smooth_broken_powerlaw.py` (``plot_smooth_broken_powerlaw.py``)
- - 00:00.327
- - 0.0
- * - :ref:`sphx_glr_user-guide_model-gallery_spectral_plot_powerlaw2.py` (``plot_powerlaw2.py``)
- - 00:00.326
+ - 00:00.321
- 0.0
- * - :ref:`sphx_glr_user-guide_model-gallery_spectral_plot_powerlaw.py` (``plot_powerlaw.py``)
+ * - :ref:`sphx_glr_user-guide_model-gallery_spectral_plot_broken_powerlaw.py` (``plot_broken_powerlaw.py``)
- 00:00.321
- 0.0
- * - :ref:`sphx_glr_user-guide_model-gallery_spectral_plot_logparabola_norm_spectral.py` (``plot_logparabola_norm_spectral.py``)
- - 00:00.299
+ * - :ref:`sphx_glr_user-guide_model-gallery_spectral_plot_compound.py` (``plot_compound.py``)
+ - 00:00.320
- 0.0
* - :ref:`sphx_glr_user-guide_model-gallery_spectral_plot_powerlaw_norm_spectral.py` (``plot_powerlaw_norm_spectral.py``)
- 00:00.274
- 0.0
- * - :ref:`sphx_glr_user-guide_model-gallery_spectral_plot_constant_spectral.py` (``plot_constant_spectral.py``)
- - 00:00.242
+ * - :ref:`sphx_glr_user-guide_model-gallery_spectral_plot_logparabola_norm_spectral.py` (``plot_logparabola_norm_spectral.py``)
+ - 00:00.271
- 0.0
- * - :ref:`sphx_glr_user-guide_model-gallery_spectral_plot_piecewise_norm_spectral.py` (``plot_piecewise_norm_spectral.py``)
- - 00:00.227
+ * - :ref:`sphx_glr_user-guide_model-gallery_spectral_plot_constant_spectral.py` (``plot_constant_spectral.py``)
+ - 00:00.239
- 0.0
* - :ref:`sphx_glr_user-guide_model-gallery_spectral_plot_super_exp_cutoff_powerlaw_4fgl.py` (``plot_super_exp_cutoff_powerlaw_4fgl.py``)
- - 00:00.226
+ - 00:00.228
+ - 0.0
+ * - :ref:`sphx_glr_user-guide_model-gallery_spectral_plot_piecewise_norm_spectral.py` (``plot_piecewise_norm_spectral.py``)
+ - 00:00.225
- 0.0
* - :ref:`sphx_glr_user-guide_model-gallery_spectral_plot_super_exp_cutoff_powerlaw_4fgl_dr1.py` (``plot_super_exp_cutoff_powerlaw_4fgl_dr1.py``)
- - 00:00.223
+ - 00:00.219
- 0.0
* - :ref:`sphx_glr_user-guide_model-gallery_spectral_plot_super_exp_cutoff_powerlaw_3fgl.py` (``plot_super_exp_cutoff_powerlaw_3fgl.py``)
- - 00:00.222
+ - 00:00.219
- 0.0
* - :ref:`sphx_glr_user-guide_model-gallery_spectral_plot_gauss_spectral.py` (``plot_gauss_spectral.py``)
- - 00:00.221
+ - 00:00.217
- 0.0
* - :ref:`sphx_glr_user-guide_model-gallery_spectral_plot_exp_cutoff_powerlaw.py` (``plot_exp_cutoff_powerlaw.py``)
- - 00:00.209
+ - 00:00.206
- 0.0
* - :ref:`sphx_glr_user-guide_model-gallery_spectral_plot_logparabola.py` (``plot_logparabola.py``)
- - 00:00.208
+ - 00:00.204
- 0.0
* - :ref:`sphx_glr_user-guide_model-gallery_spectral_plot_exp_cutoff_powerlaw_3fgl.py` (``plot_exp_cutoff_powerlaw_3fgl.py``)
- - 00:00.206
+ - 00:00.203
- 0.0
diff --git a/docs/dev/_sources/user-guide/model-gallery/temporal/plot_constant_temporal.rst.txt b/docs/dev/_sources/user-guide/model-gallery/temporal/plot_constant_temporal.rst.txt
index 496032bd1f4..458b2bdbb09 100644
--- a/docs/dev/_sources/user-guide/model-gallery/temporal/plot_constant_temporal.rst.txt
+++ b/docs/dev/_sources/user-guide/model-gallery/temporal/plot_constant_temporal.rst.txt
@@ -111,8 +111,8 @@ Here is an example YAML file using the model:
parameters: []
scale: utc
metadata:
- creator: Gammapy 1.3.dev1143+ge26e20052
- date: '2024-10-11T08:27:50.373108'
+ creator: Gammapy 1.3.dev1180+gb03e9b8c7
+ date: '2024-10-11T09:59:38.860103'
origin: null
diff --git a/docs/dev/_sources/user-guide/model-gallery/temporal/plot_expdecay_temporal.rst.txt b/docs/dev/_sources/user-guide/model-gallery/temporal/plot_expdecay_temporal.rst.txt
index 4d97ec01229..0459286f278 100644
--- a/docs/dev/_sources/user-guide/model-gallery/temporal/plot_expdecay_temporal.rst.txt
+++ b/docs/dev/_sources/user-guide/model-gallery/temporal/plot_expdecay_temporal.rst.txt
@@ -121,8 +121,8 @@ Here is an example YAML file using the model:
unit: d
scale: utc
metadata:
- creator: Gammapy 1.3.dev1143+ge26e20052
- date: '2024-10-11T08:27:50.606922'
+ creator: Gammapy 1.3.dev1180+gb03e9b8c7
+ date: '2024-10-11T09:59:39.083718'
origin: null
diff --git a/docs/dev/_sources/user-guide/model-gallery/temporal/plot_gaussian_temporal.rst.txt b/docs/dev/_sources/user-guide/model-gallery/temporal/plot_gaussian_temporal.rst.txt
index ea68e8645fe..86448f2416d 100644
--- a/docs/dev/_sources/user-guide/model-gallery/temporal/plot_gaussian_temporal.rst.txt
+++ b/docs/dev/_sources/user-guide/model-gallery/temporal/plot_gaussian_temporal.rst.txt
@@ -120,8 +120,8 @@ Here is an example YAML file using the model:
unit: h
scale: utc
metadata:
- creator: Gammapy 1.3.dev1143+ge26e20052
- date: '2024-10-11T08:27:50.840677'
+ creator: Gammapy 1.3.dev1180+gb03e9b8c7
+ date: '2024-10-11T09:59:39.303371'
origin: null
diff --git a/docs/dev/_sources/user-guide/model-gallery/temporal/plot_generalized_gaussian_temporal.rst.txt b/docs/dev/_sources/user-guide/model-gallery/temporal/plot_generalized_gaussian_temporal.rst.txt
index 8275606a559..9c9eebddeee 100644
--- a/docs/dev/_sources/user-guide/model-gallery/temporal/plot_generalized_gaussian_temporal.rst.txt
+++ b/docs/dev/_sources/user-guide/model-gallery/temporal/plot_generalized_gaussian_temporal.rst.txt
@@ -132,8 +132,8 @@ Here is an example YAML file using the model:
value: 0.6666666666666666
scale: utc
metadata:
- creator: Gammapy 1.3.dev1143+ge26e20052
- date: '2024-10-11T08:27:51.075404'
+ creator: Gammapy 1.3.dev1180+gb03e9b8c7
+ date: '2024-10-11T09:59:39.523805'
origin: null
diff --git a/docs/dev/_sources/user-guide/model-gallery/temporal/plot_linear_temporal.rst.txt b/docs/dev/_sources/user-guide/model-gallery/temporal/plot_linear_temporal.rst.txt
index ebd338aee6f..5e5b9829374 100644
--- a/docs/dev/_sources/user-guide/model-gallery/temporal/plot_linear_temporal.rst.txt
+++ b/docs/dev/_sources/user-guide/model-gallery/temporal/plot_linear_temporal.rst.txt
@@ -117,12 +117,12 @@ Here is an example YAML file using the model:
value: 0.5
unit: d-1
- name: t_ref
- value: 60594.2526759211
+ value: 60594.31643099465
unit: d
scale: utc
metadata:
- creator: Gammapy 1.3.dev1143+ge26e20052
- date: '2024-10-11T08:27:51.301305'
+ creator: Gammapy 1.3.dev1180+gb03e9b8c7
+ date: '2024-10-11T09:59:39.742070'
origin: null
diff --git a/docs/dev/_sources/user-guide/model-gallery/temporal/plot_powerlaw_temporal.rst.txt b/docs/dev/_sources/user-guide/model-gallery/temporal/plot_powerlaw_temporal.rst.txt
index 85bd569fc2c..2176872f44a 100644
--- a/docs/dev/_sources/user-guide/model-gallery/temporal/plot_powerlaw_temporal.rst.txt
+++ b/docs/dev/_sources/user-guide/model-gallery/temporal/plot_powerlaw_temporal.rst.txt
@@ -113,15 +113,15 @@ Here is an example YAML file using the model:
- name: alpha
value: -2.0
- name: t_ref
- value: 60594.252678526995
+ value: 60594.31643351969
unit: d
- name: t0
value: 1.0
unit: d
scale: utc
metadata:
- creator: Gammapy 1.3.dev1143+ge26e20052
- date: '2024-10-11T08:27:51.616529'
+ creator: Gammapy 1.3.dev1180+gb03e9b8c7
+ date: '2024-10-11T09:59:40.049560'
origin: null
diff --git a/docs/dev/_sources/user-guide/model-gallery/temporal/plot_sine_temporal.rst.txt b/docs/dev/_sources/user-guide/model-gallery/temporal/plot_sine_temporal.rst.txt
index 487aac99e61..40795141c68 100644
--- a/docs/dev/_sources/user-guide/model-gallery/temporal/plot_sine_temporal.rst.txt
+++ b/docs/dev/_sources/user-guide/model-gallery/temporal/plot_sine_temporal.rst.txt
@@ -119,12 +119,12 @@ Here is an example YAML file using the model:
value: 0.7853981633974483
unit: d-1 rad
- name: t_ref
- value: 60594.2526820428
+ value: 60594.316436978916
unit: d
scale: utc
metadata:
- creator: Gammapy 1.3.dev1143+ge26e20052
- date: '2024-10-11T08:27:51.834275'
+ creator: Gammapy 1.3.dev1180+gb03e9b8c7
+ date: '2024-10-11T09:59:40.263264'
origin: null
diff --git a/docs/dev/_sources/user-guide/model-gallery/temporal/plot_template_phase_temporal.rst.txt b/docs/dev/_sources/user-guide/model-gallery/temporal/plot_template_phase_temporal.rst.txt
index 59e9ab9ebf5..31ccfb41151 100644
--- a/docs/dev/_sources/user-guide/model-gallery/temporal/plot_template_phase_temporal.rst.txt
+++ b/docs/dev/_sources/user-guide/model-gallery/temporal/plot_template_phase_temporal.rst.txt
@@ -127,8 +127,8 @@ Here is an example YAML file using the model:
scale: utc
filename: /home/runner/work/gammapy-docs/gammapy-docs/gammapy-datasets/dev/tests/phasecurve_LSI_DC.fits
metadata:
- creator: Gammapy 1.3.dev1143+ge26e20052
- date: '2024-10-11T08:27:52.078765'
+ creator: Gammapy 1.3.dev1180+gb03e9b8c7
+ date: '2024-10-11T09:59:40.505214'
origin: null
diff --git a/docs/dev/_sources/user-guide/model-gallery/temporal/plot_template_temporal.rst.txt b/docs/dev/_sources/user-guide/model-gallery/temporal/plot_template_temporal.rst.txt
index 877faada713..8a202b0c729 100644
--- a/docs/dev/_sources/user-guide/model-gallery/temporal/plot_template_temporal.rst.txt
+++ b/docs/dev/_sources/user-guide/model-gallery/temporal/plot_template_temporal.rst.txt
@@ -118,8 +118,8 @@ Here is an example YAML file using the model:
format: table
unit: ''
metadata:
- creator: Gammapy 1.3.dev1143+ge26e20052
- date: '2024-10-11T08:27:52.318976'
+ creator: Gammapy 1.3.dev1180+gb03e9b8c7
+ date: '2024-10-11T09:59:40.738213'
origin: null
diff --git a/docs/dev/_sources/user-guide/model-gallery/temporal/sg_execution_times.rst.txt b/docs/dev/_sources/user-guide/model-gallery/temporal/sg_execution_times.rst.txt
index 50762e1d214..399c8597390 100644
--- a/docs/dev/_sources/user-guide/model-gallery/temporal/sg_execution_times.rst.txt
+++ b/docs/dev/_sources/user-guide/model-gallery/temporal/sg_execution_times.rst.txt
@@ -6,7 +6,7 @@
Computation times
=================
-**00:01.561** total execution time for 9 files **from user-guide/model-gallery/temporal**:
+**00:01.743** total execution time for 9 files **from user-guide/model-gallery/temporal**:
.. container::
@@ -33,29 +33,29 @@ Computation times
- Time
- Mem (MB)
* - :ref:`sphx_glr_user-guide_model-gallery_temporal_plot_constant_temporal.py` (``plot_constant_temporal.py``)
- - 00:00.579
+ - 00:00.752
- 0.0
* - :ref:`sphx_glr_user-guide_model-gallery_temporal_plot_powerlaw_temporal.py` (``plot_powerlaw_temporal.py``)
- - 00:00.193
+ - 00:00.195
- 0.0
* - :ref:`sphx_glr_user-guide_model-gallery_temporal_plot_template_phase_temporal.py` (``plot_template_phase_temporal.py``)
- - 00:00.123
+ - 00:00.129
- 0.0
* - :ref:`sphx_glr_user-guide_model-gallery_temporal_plot_template_temporal.py` (``plot_template_temporal.py``)
- 00:00.121
- 0.0
* - :ref:`sphx_glr_user-guide_model-gallery_temporal_plot_generalized_gaussian_temporal.py` (``plot_generalized_gaussian_temporal.py``)
- - 00:00.114
+ - 00:00.111
- 0.0
- * - :ref:`sphx_glr_user-guide_model-gallery_temporal_plot_gaussian_temporal.py` (``plot_gaussian_temporal.py``)
+ * - :ref:`sphx_glr_user-guide_model-gallery_temporal_plot_sine_temporal.py` (``plot_sine_temporal.py``)
- 00:00.110
- 0.0
- * - :ref:`sphx_glr_user-guide_model-gallery_temporal_plot_expdecay_temporal.py` (``plot_expdecay_temporal.py``)
- - 00:00.110
+ * - :ref:`sphx_glr_user-guide_model-gallery_temporal_plot_gaussian_temporal.py` (``plot_gaussian_temporal.py``)
+ - 00:00.109
- 0.0
- * - :ref:`sphx_glr_user-guide_model-gallery_temporal_plot_sine_temporal.py` (``plot_sine_temporal.py``)
- - 00:00.108
+ * - :ref:`sphx_glr_user-guide_model-gallery_temporal_plot_expdecay_temporal.py` (``plot_expdecay_temporal.py``)
+ - 00:00.109
- 0.0
* - :ref:`sphx_glr_user-guide_model-gallery_temporal_plot_linear_temporal.py` (``plot_linear_temporal.py``)
- - 00:00.104
+ - 00:00.106
- 0.0
diff --git a/docs/dev/_sources/user-guide/package.rst.txt b/docs/dev/_sources/user-guide/package.rst.txt
index 242864800ce..d6e0b985cd9 100644
--- a/docs/dev/_sources/user-guide/package.rst.txt
+++ b/docs/dev/_sources/user-guide/package.rst.txt
@@ -42,7 +42,7 @@ the Gammapy API are explained in more detail in the following.
Fig. 1 Data flow and sub-package structure of Gammapy. The folder icons
represent the corresponding sub-packages. The direction of the
the data flow is illustrated with shaded arrows. The top section
- shows the data levels as defined by `CTA`_.
+ shows the data levels as defined by `CTAO`_.
Analysis steps
--------------
diff --git a/docs/dev/_sources/user-guide/references.rst.txt b/docs/dev/_sources/user-guide/references.rst.txt
index 576f673fabf..cd4f5143e89 100644
--- a/docs/dev/_sources/user-guide/references.rst.txt
+++ b/docs/dev/_sources/user-guide/references.rst.txt
@@ -91,7 +91,7 @@ Glossary
GTI
Short for "good time interval": it indicates a continuous time interval of data
- acquisition. In CTA, it also represents a time interval in which the IRFs are
+ acquisition. In the GADF DL3 format, it also represents a time interval in which the IRFs are
supposed to be constant.
IRF
@@ -137,6 +137,10 @@ Glossary
object, the type of plot (e.g. :math:`dN/dE`, :math:`E^2\ dN/dE`) is typically adjusted
through the `sed_type` quantity. See :ref:`sedtypes` for a list of options.
+.. STI
+ Short for "stable time interval": it indicates a continuous time interval of data
+ acquisition for which the instrument response files are supposed to be constant.
+
Stacked Analysis
In a stacked analysis individual observations are reduced to datasets which
are then stacked to produce a single reduced dataset. The latter is then used
diff --git a/docs/dev/_sources/user-guide/utils.rst.txt b/docs/dev/_sources/user-guide/utils.rst.txt
index b9733ad3b50..dcb01e7dcdf 100644
--- a/docs/dev/_sources/user-guide/utils.rst.txt
+++ b/docs/dev/_sources/user-guide/utils.rst.txt
@@ -39,12 +39,12 @@ In Gammapy, `astropy.time.Time` objects are used to represent times:
Note that Astropy chose ``format='isot'`` and ``scale='utc'`` as default and in
Gammapy these are also the recommended format and time scale.
-.. warning::
+.. .. warning::
- Actually what's written here is not true. In CTA it hasn't been decided if
+.. Actually what's written here is not true. In CTAO, it hasn't been decided if
times will be in ``utc`` or ``tt`` (terrestrial time) format.
- Here's a reminder that this needs to be settled / updated:
+.. Here's a reminder that this needs to be settled / updated:
https://github.com/gammapy/gammapy/issues/284
diff --git a/docs/dev/api/gammapy.data.DataStore.html b/docs/dev/api/gammapy.data.DataStore.html
index 96ba819024a..b7304302c76 100644
--- a/docs/dev/api/gammapy.data.DataStore.html
+++ b/docs/dev/api/gammapy.data.DataStore.html
@@ -989,7 +989,7 @@ DataStore
-
For further usage example see CTA with Gammapy tutorial.
+
For further usage example see CTAO with Gammapy tutorial.
Attributes Summary