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Added some more important X-ray paper references, and older ones from…
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… the beginning of the field as well.

Signed-off-by: David Turner <[email protected]>
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134 changes: 133 additions & 1 deletion paper/paper.bib
Original file line number Diff line number Diff line change
Expand Up @@ -274,4 +274,136 @@ @ARTICLE{ovigroups
title = "{An X-ray view of galaxy groups in the line of sight of UV-bright quasars - comparing X-ray properties to absorption detection of warm-hot gas}",
keywords = {},
year = {2024, in prep.},
}
}

@ARTICLE{qpedisco,
author = {{Miniutti}, G. and {Saxton}, R.~D. and {Giustini}, M. and {Alexander}, K.~D. and {Fender}, R.~P. and {Heywood}, I. and {Monageng}, I. and {Coriat}, M. and {Tzioumis}, A.~K. and {Read}, A.~M. and {Knigge}, C. and {Gandhi}, P. and {Pretorius}, M.~L. and {Ag{\'\i}s-Gonz{\'a}lez}, B.},
title = "{Nine-hour X-ray quasi-periodic eruptions from a low-mass black hole galactic nucleus}",
journal = {\nat},
keywords = {Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Astrophysics of Galaxies},
year = 2019,
month = sep,
volume = {573},
number = {7774},
pages = {381-384},
doi = {10.1038/s41586-019-1556-x},
archivePrefix = {arXiv},
eprint = {1909.04693},
primaryClass = {astro-ph.HE},
adsurl = {https://ui.adsabs.harvard.edu/abs/2019Natur.573..381M},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{clusterdisco,
author = {{Kellogg}, E. and {Gursky}, H. and {Leong}, C. and {Schreier}, E. and {Tananbaum}, H. and {Giacconi}, R.},
title = "{X-Ray Observations of the Virgo Cluster, NGC 5128, and 3c 273 from the UHURU Satellite}",
journal = {\apjl},
year = 1971,
month = apr,
volume = {165},
pages = {L49},
doi = {10.1086/180714},
adsurl = {https://ui.adsabs.harvard.edu/abs/1971ApJ...165L..49K},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{theOG,
author = {{Giacconi}, Riccardo and {Gursky}, Herbert and {Paolini}, Frank R. and {Rossi}, Bruno B.},
title = "{Evidence for x Rays From Sources Outside the Solar System}",
journal = {\prl},
year = 1962,
month = dec,
volume = {9},
number = {11},
pages = {439-443},
doi = {10.1103/PhysRevLett.9.439},
adsurl = {https://ui.adsabs.harvard.edu/abs/1962PhRvL...9..439G},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{cygx1andfriends,
author = {{Bowyer}, S. and {Byram}, E.~T. and {Chubb}, T.~A. and {Friedman}, H.},
title = "{Cosmic X-ray Sources}",
journal = {Science},
year = 1965,
month = jan,
volume = {147},
number = {3656},
pages = {394-398},
doi = {10.1126/science.147.3656.394},
adsurl = {https://ui.adsabs.harvard.edu/abs/1965Sci...147..394B},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{coup,
author = {{Getman}, K.~V. and {Flaccomio}, E. and {Broos}, P.~S. and {Grosso}, N. and {Tsujimoto}, M. and {Townsley}, L. and {Garmire}, G.~P. and {Kastner}, J. and {Li}, J. and {Harnden}, F.~R., Jr. and {Wolk}, S. and {Murray}, S.~S. and {Lada}, C.~J. and {Muench}, A.~A. and {McCaughrean}, M.~J. and {Meeus}, G. and {Damiani}, F. and {Micela}, G. and {Sciortino}, S. and {Bally}, J. and {Hillenbrand}, L.~A. and {Herbst}, W. and {Preibisch}, T. and {Feigelson}, E.~D.},
title = "{Chandra Orion Ultradeep Project: Observations and Source Lists}",
journal = {\apjs},
keywords = {ISM: Individual: Name: Orion Nebula, ISM: Individual: Alphanumeric: OMC-1, Galaxy: Open Clusters and Associations: Individual: Name: Orion, Stars: Early-Type, Stars: Pre-Main-Sequence, X-Rays: Stars, Astrophysics},
year = 2005,
month = oct,
volume = {160},
number = {2},
pages = {319-352},
doi = {10.1086/432092},
archivePrefix = {arXiv},
eprint = {astro-ph/0410136},
primaryClass = {astro-ph},
adsurl = {https://ui.adsabs.harvard.edu/abs/2005ApJS..160..319G},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{xest,
author = {{G{\"u}del}, M. and {Briggs}, K.~R. and {Arzner}, K. and {Audard}, M. and {Bouvier}, J. and {Feigelson}, E.~D. and {Franciosini}, E. and {Glauser}, A. and {Grosso}, N. and {Micela}, G. and {Monin}, J. -L. and {Montmerle}, T. and {Padgett}, D.~L. and {Palla}, F. and {Pillitteri}, I. and {Rebull}, L. and {Scelsi}, L. and {Silva}, B. and {Skinner}, S.~L. and {Stelzer}, B. and {Telleschi}, A.},
title = "{The XMM-Newton extended survey of the Taurus molecular cloud (XEST)}",
journal = {\aap},
keywords = {stars: formation, stars: pre-main sequence, X-rays: stars, gravitational waves, Astrophysics},
year = 2007,
month = jun,
volume = {468},
number = {2},
pages = {353-377},
doi = {10.1051/0004-6361:20065724},
archivePrefix = {arXiv},
eprint = {astro-ph/0609160},
primaryClass = {astro-ph},
adsurl = {https://ui.adsabs.harvard.edu/abs/2007A&A...468..353G},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{cavities,
author = {{McNamara}, B.~R. and {Wise}, M.~W. and {Nulsen}, P.~E.~J. and {David}, L.~P. and {Carilli}, C.~L. and {Sarazin}, C.~L. and {O'Dea}, C.~P. and {Houck}, J. and {Donahue}, M. and {Baum}, S. and {Voit}, M. and {O'Connell}, R.~W. and {Koekemoer}, A.},
title = "{Discovery of Ghost Cavities in the X-Ray Atmosphere of Abell 2597}",
journal = {\apjl},
keywords = {Galaxies: Cooling Flows, Galaxies: Clusters: General, Galaxies: Intergalactic Medium, Radio Continuum: Galaxies, X-Rays: Galaxies: Clusters, Astrophysics},
year = 2001,
month = dec,
volume = {562},
number = {2},
pages = {L149-L152},
doi = {10.1086/338326},
archivePrefix = {arXiv},
eprint = {astro-ph/0110554},
primaryClass = {astro-ph},
adsurl = {https://ui.adsabs.harvard.edu/abs/2001ApJ...562L.149M},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{accept,
author = {{Cavagnolo}, Kenneth W. and {Donahue}, Megan and {Voit}, G. Mark and {Sun}, Ming},
title = "{Intracluster Medium Entropy Profiles for a Chandra Archival Sample of Galaxy Clusters}",
journal = {\apjs},
keywords = {astronomical data bases: miscellaneous, cooling flows, X-rays: galaxies: clusters, X-rays: general, Astrophysics - Cosmology and Extragalactic Astrophysics},
year = 2009,
month = may,
volume = {182},
number = {1},
pages = {12-32},
doi = {10.1088/0067-0049/182/1/12},
archivePrefix = {arXiv},
eprint = {0902.1802},
primaryClass = {astro-ph.CO},
adsurl = {https://ui.adsabs.harvard.edu/abs/2009ApJS..182...12C},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

17 changes: 14 additions & 3 deletions paper/paper.md
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Expand Up @@ -82,9 +82,20 @@ ability to download pre-processed data from many of the data archives.
![A flowchart giving a brief overview of the [Daxa]{.smallcaps} workflow. \label{fig:flowchart}](figures/daxa_paper_flowchart.pdf)

Almost every sub-field of astronomy, astrophysics, and cosmology has benefited significantly from X-ray coverage over
the last three decades; calibrating weak-lensing mis-centering for galaxy cluster studies [@miscen], identifying
**...COME UP WITH MORE IMPORTANT X-RAY PAPERS**, even probing the irradiation of exoplanets [@xrayirrexo]. The
current workhorse X-ray observatories (_XMM_-Newton [@xmm] and _Chandra_; other telescopes are
the last three decades; the observation of X-ray cavities in galaxy clusters caused by central AGN helped to shed light
on the cooling-flow problem [@cavities]; further X-ray observations allowed for the measurement of spatially-resolved
entropy in hundreds of clusters, dramatically increasing understanding of cooling and heating processes in their
cores; the discovery of quasi-periodic eruptions (QPE) from active galactic nuclei (AGN) [@qpedisco] provided a
high-energy view of young stars and insights into their magnetic fields and stellar winds [@coup, @xest], calibrating
weak-lensing mis-centering for galaxy cluster studies of cosmology [@miscen], and even probing the irradiation of
exoplanets [@xrayirrexo]. Indeed, X-ray telescopes have created many entirely new fields of study; they provided the
first evidence of X-ray sources outside the solar system [@theOG]; discovered the first widely accepted black hole, and
launched the study of supernova remnants [@cygx1andfriends]; and found ionized, volume-filling, gas within the Coma
galaxy cluster (the intra-cluster medium) [@clusterdisco], with the implication that clusters were more than
collections of galaxies. These non-exhaustive lists make evident the importance of X-ray observations to the
astronomy, astrophysics, and cosmology communities.

The current workhorse X-ray observatories (_XMM_-Newton [@xmm] and _Chandra_; other telescopes are
online but are more specialised) are ageing however, with _Chandra_ in particular experiencing a decline in
low-energy sensitivity that might limit science cases; these missions cannot last forever. If we are to enter an
X-ray desert, where the astrophysics community has only limited access to new X-ray observations from specialised
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