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diff --git a/docs/dev/_images/sphx_glr_plot_sine_temporal_thumb.png b/docs/dev/_images/sphx_glr_plot_sine_temporal_thumb.png
diff --git a/docs/dev/_images/sphx_glr_simulate_3d_001.png b/docs/dev/_images/sphx_glr_simulate_3d_001.png
diff --git a/docs/dev/_images/sphx_glr_simulate_3d_002.png b/docs/dev/_images/sphx_glr_simulate_3d_002.png
diff --git a/docs/dev/_images/sphx_glr_simulate_3d_thumb.png b/docs/dev/_images/sphx_glr_simulate_3d_thumb.png
diff --git a/docs/dev/_images/sphx_glr_spectral_analysis_rad_max_005.png b/docs/dev/_images/sphx_glr_spectral_analysis_rad_max_005.png
diff --git a/docs/dev/_modules/gammapy/analysis/config.html b/docs/dev/_modules/gammapy/analysis/config.html
@@ -188,7 +188,7 @@
 
             $("#version_switcher_menu").append(node);
             // replace dropdown button text with the preferred display name of
-            // this version, rather than using sphinx's 1.2.dev927+g7d6757ef7 variable.
+            // this version, rather than using sphinx's 1.2.dev937+g87a9b7512 variable.
             // also highlight the dropdown entry for the currently-viewed
             // version's entry
             if (entry.version == "dev") {

diff --git a/docs/dev/_modules/gammapy/analysis/core.html b/docs/dev/_modules/gammapy/analysis/core.html
@@ -188,7 +188,7 @@
 
             $("#version_switcher_menu").append(node);
             // replace dropdown button text with the preferred display name of
-            // this version, rather than using sphinx's 1.2.dev927+g7d6757ef7 variable.
+            // this version, rather than using sphinx's 1.2.dev937+g87a9b7512 variable.
             // also highlight the dropdown entry for the currently-viewed
             // version's entry
             if (entry.version == "dev") {

diff --git a/docs/dev/_modules/gammapy/astro/darkmatter/profiles.html b/docs/dev/_modules/gammapy/astro/darkmatter/profiles.html
diff --git a/docs/dev/_modules/gammapy/astro/darkmatter/spectra.html b/docs/dev/_modules/gammapy/astro/darkmatter/spectra.html
@@ -188,7 +188,7 @@
 
             $("#version_switcher_menu").append(node);
             // replace dropdown button text with the preferred display name of
-            // this version, rather than using sphinx's 1.2.dev927+g7d6757ef7 variable.
+            // this version, rather than using sphinx's 1.2.dev937+g87a9b7512 variable.
             // also highlight the dropdown entry for the currently-viewed
             // version's entry
             if (entry.version == "dev") {
@@ -290,12 +290,12 @@ <h1>Source code for gammapy.astro.darkmatter.spectra</h1><div class="highlight">
 <span class="sd">    to the nearest available value. The spectra will be available as</span>
 <span class="sd">    `~gammapy.modeling.models.TemplateNDSpectralModel` for a chosen dark matter mass and</span>
 <span class="sd">    annihilation channel. Using a `~gammapy.modeling.models.TemplateNDSpectralModel`</span>
-<span class="sd">    allows the interpolation beween different dark matter masses.</span>
+<span class="sd">    allows the interpolation between different dark matter masses.</span>
 
 <span class="sd">    Parameters</span>
 <span class="sd">    ----------</span>
 <span class="sd">    mDM : `~astropy.units.Quantity`</span>
-<span class="sd">        Dark matter particle mass as rest mass energy</span>
+<span class="sd">        Dark matter particle mass as rest mass energy.</span>
 <span class="sd">    channel: str</span>
 <span class="sd">        Annihilation channel. List available channels with `~gammapy.spectrum.PrimaryFlux.allowed_channels`.</span>
 
@@ -404,7 +404,7 @@ <h1>Source code for gammapy.astro.darkmatter.spectra</h1><div class="highlight">
 
     <span class="nd">@property</span>
     <span class="k">def</span> <span class="nf">channel</span><span class="p">(</span><span class="bp">self</span><span class="p">):</span>
-<span class="w">        </span><span class="sd">&quot;&quot;&quot;Annihilation channel (str).&quot;&quot;&quot;</span>
+<span class="w">        </span><span class="sd">&quot;&quot;&quot;Annihilation channel as a string.&quot;&quot;&quot;</span>
         <span class="k">return</span> <span class="bp">self</span><span class="o">.</span><span class="n">_channel</span>
 
     <span class="nd">@channel</span><span class="o">.</span><span class="n">setter</span>
@@ -417,6 +417,7 @@ <h1>Source code for gammapy.astro.darkmatter.spectra</h1><div class="highlight">
             <span class="bp">self</span><span class="o">.</span><span class="n">_channel</span> <span class="o">=</span> <span class="n">channel</span>
 
 <div class="viewcode-block" id="PrimaryFlux.evaluate"><a class="viewcode-back" href="../../../../api/gammapy.astro.darkmatter.PrimaryFlux.html#gammapy.astro.darkmatter.PrimaryFlux.evaluate">[docs]</a>    <span class="k">def</span> <span class="nf">evaluate</span><span class="p">(</span><span class="bp">self</span><span class="p">,</span> <span class="n">energy</span><span class="p">,</span> <span class="o">**</span><span class="n">kwargs</span><span class="p">):</span>
+<span class="w">        </span><span class="sd">&quot;&quot;&quot;Evaluate the primary flux.&quot;&quot;&quot;</span>
         <span class="n">mass</span> <span class="o">=</span> <span class="p">{</span><span class="s2">&quot;mass&quot;</span><span class="p">:</span> <span class="bp">self</span><span class="o">.</span><span class="n">mDM</span><span class="p">}</span>
         <span class="n">kwargs</span><span class="o">.</span><span class="n">update</span><span class="p">(</span><span class="n">mass</span><span class="p">)</span>
 
@@ -455,30 +456,31 @@ <h1>Source code for gammapy.astro.darkmatter.spectra</h1><div class="highlight">
 <span class="sd">    Parameters</span>
 <span class="sd">    ----------</span>
 <span class="sd">    mass : `~astropy.units.Quantity`</span>
-<span class="sd">        Dark matter mass</span>
+<span class="sd">        Dark matter mass.</span>
 <span class="sd">    channel : str</span>
-<span class="sd">        Annihilation channel for `~gammapy.astro.darkmatter.PrimaryFlux`, e.g. &quot;b&quot; for &quot;bbar&quot;. See `PrimaryFlux.channel_registry` for more.</span>
+<span class="sd">        Annihilation channel for `~gammapy.astro.darkmatter.PrimaryFlux`, e.g. &quot;b&quot; for &quot;bbar&quot;.</span>
+<span class="sd">        See `PrimaryFlux.channel_registry` for more.</span>
 <span class="sd">    scale : float</span>
-<span class="sd">        Scale parameter for model fitting</span>
+<span class="sd">        Scale parameter for model fitting.</span>
 <span class="sd">    jfactor : `~astropy.units.Quantity`</span>
 <span class="sd">        Integrated J-Factor needed when `~gammapy.modeling.models.PointSpatialModel`</span>
-<span class="sd">        spatial model is used</span>
+<span class="sd">        is used.</span>
 <span class="sd">    z: float</span>
-<span class="sd">        Redshift value</span>
+<span class="sd">        Redshift value.</span>
 <span class="sd">    k: int</span>
-<span class="sd">        Type of dark matter particle (k:2 Majorana, k:4 Dirac)</span>
+<span class="sd">        Type of dark matter particle (k:2 Majorana, k:4 Dirac).</span>
 
 <span class="sd">    Examples</span>
 <span class="sd">    --------</span>
 <span class="sd">    This is how to instantiate a `DarkMatterAnnihilationSpectralModel` model::</span>
 
-<span class="sd">        from astropy import units as u</span>
-<span class="sd">        from gammapy.astro.darkmatter import DarkMatterAnnihilationSpectralModel</span>
+<span class="sd">        &gt;&gt;&gt; import astropy.units as u</span>
+<span class="sd">        &gt;&gt;&gt; from gammapy.astro.darkmatter import DarkMatterAnnihilationSpectralModel</span>
 
-<span class="sd">        channel = &quot;b&quot;</span>
-<span class="sd">        massDM = 5000*u.Unit(&quot;GeV&quot;)</span>
-<span class="sd">        jfactor = 3.41e19 * u.Unit(&quot;GeV2 cm-5&quot;)</span>
-<span class="sd">        modelDM = DarkMatterAnnihilationSpectralModel(mass=massDM, channel=channel, jfactor=jfactor)  # noqa: E501</span>
+<span class="sd">        &gt;&gt;&gt; channel = &quot;b&quot;</span>
+<span class="sd">        &gt;&gt;&gt; massDM = 5000*u.Unit(&quot;GeV&quot;)</span>
+<span class="sd">        &gt;&gt;&gt; jfactor = 3.41e19 * u.Unit(&quot;GeV2 cm-5&quot;)</span>
+<span class="sd">        &gt;&gt;&gt; modelDM = DarkMatterAnnihilationSpectralModel(mass=massDM, channel=channel, jfactor=jfactor)  # noqa: E501</span>
 
 <span class="sd">    References</span>
 <span class="sd">    ----------</span>
@@ -521,6 +523,7 @@ <h1>Source code for gammapy.astro.darkmatter.spectra</h1><div class="highlight">
         <span class="k">return</span> <span class="n">flux</span></div>
 
 <div class="viewcode-block" id="DarkMatterAnnihilationSpectralModel.to_dict"><a class="viewcode-back" href="../../../../api/gammapy.astro.darkmatter.DarkMatterAnnihilationSpectralModel.html#gammapy.astro.darkmatter.DarkMatterAnnihilationSpectralModel.to_dict">[docs]</a>    <span class="k">def</span> <span class="nf">to_dict</span><span class="p">(</span><span class="bp">self</span><span class="p">,</span> <span class="n">full_output</span><span class="o">=</span><span class="kc">False</span><span class="p">):</span>
+<span class="w">        </span><span class="sd">&quot;&quot;&quot;Convert to dictionary.&quot;&quot;&quot;</span>
         <span class="n">data</span> <span class="o">=</span> <span class="nb">super</span><span class="p">()</span><span class="o">.</span><span class="n">to_dict</span><span class="p">(</span><span class="n">full_output</span><span class="o">=</span><span class="n">full_output</span><span class="p">)</span>
         <span class="n">data</span><span class="p">[</span><span class="s2">&quot;spectral&quot;</span><span class="p">][</span><span class="s2">&quot;channel&quot;</span><span class="p">]</span> <span class="o">=</span> <span class="bp">self</span><span class="o">.</span><span class="n">channel</span>
         <span class="n">data</span><span class="p">[</span><span class="s2">&quot;spectral&quot;</span><span class="p">][</span><span class="s2">&quot;mass&quot;</span><span class="p">]</span> <span class="o">=</span> <span class="bp">self</span><span class="o">.</span><span class="n">mass</span><span class="o">.</span><span class="n">to_string</span><span class="p">()</span>
@@ -531,17 +534,17 @@ <h1>Source code for gammapy.astro.darkmatter.spectra</h1><div class="highlight">
 
 <div class="viewcode-block" id="DarkMatterAnnihilationSpectralModel.from_dict"><a class="viewcode-back" href="../../../../api/gammapy.astro.darkmatter.DarkMatterAnnihilationSpectralModel.html#gammapy.astro.darkmatter.DarkMatterAnnihilationSpectralModel.from_dict">[docs]</a>    <span class="nd">@classmethod</span>
     <span class="k">def</span> <span class="nf">from_dict</span><span class="p">(</span><span class="bp">cls</span><span class="p">,</span> <span class="n">data</span><span class="p">):</span>
-<span class="w">        </span><span class="sd">&quot;&quot;&quot;Create spectral model from dict</span>
+<span class="w">        </span><span class="sd">&quot;&quot;&quot;Create spectral model from a dictionary.</span>
 
 <span class="sd">        Parameters</span>
 <span class="sd">        ----------</span>
 <span class="sd">        data : dict</span>
-<span class="sd">            Dict with model data</span>
+<span class="sd">            Dictionary with model data.</span>
 
 <span class="sd">        Returns</span>
 <span class="sd">        -------</span>
 <span class="sd">        model : `DarkMatterAnnihilationSpectralModel`</span>
-<span class="sd">            Dark matter annihilation spectral model</span>
+<span class="sd">            Dark matter annihilation spectral model.</span>
 <span class="sd">        &quot;&quot;&quot;</span>
         <span class="n">data</span> <span class="o">=</span> <span class="n">data</span><span class="p">[</span><span class="s2">&quot;spectral&quot;</span><span class="p">]</span>
         <span class="n">data</span><span class="o">.</span><span class="n">pop</span><span class="p">(</span><span class="s2">&quot;type&quot;</span><span class="p">)</span>
@@ -563,28 +566,29 @@ <h1>Source code for gammapy.astro.darkmatter.spectra</h1><div class="highlight">
 <span class="sd">    Parameters</span>
 <span class="sd">    ----------</span>
 <span class="sd">    mass : `~astropy.units.Quantity`</span>
-<span class="sd">        Dark matter mass</span>
+<span class="sd">        Dark matter mass.</span>
 <span class="sd">    channel : str</span>
-<span class="sd">        Annihilation channel for `~gammapy.astro.darkmatter.PrimaryFlux`, e.g. &quot;b&quot; for &quot;bbar&quot;. See `PrimaryFlux.channel_registry` for more.</span>
+<span class="sd">        Annihilation channel for `~gammapy.astro.darkmatter.PrimaryFlux`, e.g. &quot;b&quot; for &quot;bbar&quot;.</span>
+<span class="sd">        See `PrimaryFlux.channel_registry` for more.</span>
 <span class="sd">    scale : float</span>
 <span class="sd">        Scale parameter for model fitting</span>
 <span class="sd">    jfactor : `~astropy.units.Quantity`</span>
 <span class="sd">        Integrated J-Factor needed when `~gammapy.modeling.models.PointSpatialModel`</span>
-<span class="sd">        spatial model is used</span>
+<span class="sd">        is used.</span>
 <span class="sd">    z: float</span>
-<span class="sd">        Redshift value</span>
+<span class="sd">        Redshift value.</span>
 
 <span class="sd">    Examples</span>
 <span class="sd">    --------</span>
 <span class="sd">    This is how to instantiate a `DarkMatterAnnihilationSpectralModel` model::</span>
 
-<span class="sd">        from astropy import units as u</span>
-<span class="sd">        from gammapy.astro.darkmatter import DarkMatterDecaySpectralModel</span>
+<span class="sd">        &gt;&gt;&gt; import astropy.units as u</span>
+<span class="sd">        &gt;&gt;&gt; from gammapy.astro.darkmatter import DarkMatterDecaySpectralModel</span>
 
-<span class="sd">        channel = &quot;b&quot;</span>
-<span class="sd">        massDM = 5000*u.Unit(&quot;GeV&quot;)</span>
-<span class="sd">        jfactor = 3.41e19 * u.Unit(&quot;GeV cm-2&quot;)</span>
-<span class="sd">        modelDM = DarkMatterDecaySpectralModel(mass=massDM, channel=channel, jfactor=jfactor)  # noqa: E501</span>
+<span class="sd">        &gt;&gt;&gt; channel = &quot;b&quot;</span>
+<span class="sd">        &gt;&gt;&gt; massDM = 5000*u.Unit(&quot;GeV&quot;)</span>
+<span class="sd">        &gt;&gt;&gt; jfactor = 3.41e19 * u.Unit(&quot;GeV cm-2&quot;)</span>
+<span class="sd">        &gt;&gt;&gt; modelDM = DarkMatterDecaySpectralModel(mass=massDM, channel=channel, jfactor=jfactor)  # noqa: E501</span>
 
 <span class="sd">    References</span>
 <span class="sd">    ----------</span>
@@ -633,17 +637,17 @@ <h1>Source code for gammapy.astro.darkmatter.spectra</h1><div class="highlight">
 
 <div class="viewcode-block" id="DarkMatterDecaySpectralModel.from_dict"><a class="viewcode-back" href="../../../../api/gammapy.astro.darkmatter.DarkMatterDecaySpectralModel.html#gammapy.astro.darkmatter.DarkMatterDecaySpectralModel.from_dict">[docs]</a>    <span class="nd">@classmethod</span>
     <span class="k">def</span> <span class="nf">from_dict</span><span class="p">(</span><span class="bp">cls</span><span class="p">,</span> <span class="n">data</span><span class="p">):</span>
-<span class="w">        </span><span class="sd">&quot;&quot;&quot;Create spectral model from dict</span>
+<span class="w">        </span><span class="sd">&quot;&quot;&quot;Create spectral model from dictionary.</span>
 
 <span class="sd">        Parameters</span>
 <span class="sd">        ----------</span>
 <span class="sd">        data : dict</span>
-<span class="sd">            Dict with model data</span>
+<span class="sd">            Dictionary with model data.</span>
 
 <span class="sd">        Returns</span>
 <span class="sd">        -------</span>
 <span class="sd">        model : `DarkMatterDecaySpectralModel`</span>
-<span class="sd">            Dark matter decay spectral model</span>
+<span class="sd">            Dark matter decay spectral model.</span>
 <span class="sd">        &quot;&quot;&quot;</span>
         <span class="n">data</span> <span class="o">=</span> <span class="n">data</span><span class="p">[</span><span class="s2">&quot;spectral&quot;</span><span class="p">]</span>
         <span class="n">data</span><span class="o">.</span><span class="n">pop</span><span class="p">(</span><span class="s2">&quot;type&quot;</span><span class="p">)</span>

diff --git a/docs/dev/_modules/gammapy/astro/darkmatter/utils.html b/docs/dev/_modules/gammapy/astro/darkmatter/utils.html
@@ -188,7 +188,7 @@
 
             $("#version_switcher_menu").append(node);
             // replace dropdown button text with the preferred display name of
-            // this version, rather than using sphinx's 1.2.dev927+g7d6757ef7 variable.
+            // this version, rather than using sphinx's 1.2.dev937+g87a9b7512 variable.
             // also highlight the dropdown entry for the currently-viewed
             // version's entry
             if (entry.version == "dev") {
@@ -281,13 +281,13 @@ <h1>Source code for gammapy.astro.darkmatter.utils</h1><div class="highlight"><p
 <span class="sd">    Parameters</span>
 <span class="sd">    ----------</span>
 <span class="sd">    geom : `~gammapy.maps.WcsGeom`</span>
-<span class="sd">        Reference geometry</span>
+<span class="sd">        Reference geometry.</span>
 <span class="sd">    profile : `~gammapy.astro.darkmatter.profiles.DMProfile`</span>
-<span class="sd">        Dark matter profile</span>
+<span class="sd">        Dark matter profile.</span>
 <span class="sd">    distance : `~astropy.units.Quantity`</span>
-<span class="sd">        Distance to convert angular scale of the map</span>
+<span class="sd">        Distance to convert angular scale of the map.</span>
 <span class="sd">    annihilation: bool, optional</span>
-<span class="sd">        Decay or annihilation (default: True)</span>
+<span class="sd">        Decay or annihilation. Default is True.</span>
 <span class="sd">    &quot;&quot;&quot;</span>
 
     <span class="k">def</span> <span class="fm">__init__</span><span class="p">(</span><span class="bp">self</span><span class="p">,</span> <span class="n">geom</span><span class="p">,</span> <span class="n">profile</span><span class="p">,</span> <span class="n">distance</span><span class="p">,</span> <span class="n">annihilation</span><span class="o">=</span><span class="kc">True</span><span class="p">):</span>