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diff --git a/docs/dev/.doctrees/api/gammapy.astro.darkmatter.BurkertProfile.doctree b/docs/dev/.doctrees/api/gammapy.astro.darkmatter.BurkertProfile.doctree
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diff --git a/docs/dev/_modules/gammapy/analysis/config.html b/docs/dev/_modules/gammapy/analysis/config.html
@@ -66,7 +66,7 @@
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-  <meta name="docsearch:version" content="2.0.dev452+g4492f4b7c" />
+  <meta name="docsearch:version" content="2.0.dev456+g82fae34f9" />
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diff --git a/docs/dev/_modules/gammapy/analysis/core.html b/docs/dev/_modules/gammapy/analysis/core.html
@@ -66,7 +66,7 @@
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-  <meta name="docsearch:version" content="2.0.dev452+g4492f4b7c" />
+  <meta name="docsearch:version" content="2.0.dev456+g82fae34f9" />
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diff --git a/docs/dev/_modules/gammapy/astro/darkmatter/profiles.html b/docs/dev/_modules/gammapy/astro/darkmatter/profiles.html
@@ -66,7 +66,7 @@
     <link rel="search" title="Search" href="../../../../search.html" />
   <meta name="viewport" content="width=device-width, initial-scale=1"/>
   <meta name="docsearch:language" content="en"/>
-  <meta name="docsearch:version" content="2.0.dev452+g4492f4b7c" />
+  <meta name="docsearch:version" content="2.0.dev456+g82fae34f9" />
   </head>
 
 
@@ -459,6 +459,7 @@
   <h1>Source code for gammapy.astro.darkmatter.profiles</h1><div class="highlight"><pre>
 <span></span><span class="c1"># Licensed under a 3-clause BSD style license - see LICENSE.rst</span>
 <span class="sd">&quot;&quot;&quot;Dark matter profiles.&quot;&quot;&quot;</span>
+
 <span class="kn">import</span><span class="w"> </span><span class="nn">abc</span>
 <span class="kn">import</span><span class="w"> </span><span class="nn">html</span>
 <span class="kn">import</span><span class="w"> </span><span class="nn">numpy</span><span class="w"> </span><span class="k">as</span><span class="w"> </span><span class="nn">np</span>
@@ -586,14 +587,16 @@ <h1>Source code for gammapy.astro.darkmatter.profiles</h1><div class="highlight"
 <span class="k">class</span><span class="w"> </span><span class="nc">ZhaoProfile</span><span class="p">(</span><span class="n">DMProfile</span><span class="p">):</span>
 <span class="w">    </span><span class="sa">r</span><span class="sd">&quot;&quot;&quot;Zhao Profile.</span>
 
-<span class="sd">    This is taken from equation 1 from Zhao (1996). It is a generalization of the NFW profile. The volume density</span>
+<span class="sd">    It is a generalization of the NFW profile. The volume density</span>
 <span class="sd">    is parametrized with a double power-law. Scale radii smaller than the scale radius are described with a slope of</span>
 <span class="sd">    :math:`-\gamma` and scale radii larger than the scale radius are described with a slope of :math:`-\beta`.</span>
 <span class="sd">    :math:`\alpha` is a measure for the width of the transition region.</span>
 
 <span class="sd">    .. math::</span>
 <span class="sd">        \rho(r) = \rho_s \left(\frac{r_s}{r}\right)^\gamma \left(1 + \left(\frac{r}{r_s}\right)^\frac{1}{\alpha} \right)^{(\gamma - \beta) \alpha}</span>
 
+<span class="sd">    Equation (1) from [1]_.</span>
+
 <span class="sd">    Parameters</span>
 <span class="sd">    ----------</span>
 <span class="sd">    r_s : `~astropy.units.Quantity`</span>
@@ -609,8 +612,10 @@ <h1>Source code for gammapy.astro.darkmatter.profiles</h1><div class="highlight"
 
 <span class="sd">    References</span>
 <span class="sd">    ----------</span>
-<span class="sd">    * `1996MNRAS.278..488Z &lt;https://ui.adsabs.harvard.edu/abs/1996MNRAS.278..488Z&gt;`_</span>
-<span class="sd">    * `2011JCAP...03..051C &lt;https://ui.adsabs.harvard.edu/abs/2011JCAP...03..051C&gt;`_</span>
+<span class="sd">    .. [1] `Zhao (1996), &quot;Analytical models for galactic nuclei&quot;</span>
+<span class="sd">      &lt;https://ui.adsabs.harvard.edu/abs/1996MNRAS.278..488Z&gt;`_</span>
+<span class="sd">    * `Marco et al. (2011), &quot;PPPC 4 DM ID: a poor particle physicist cookbook for dark matter indirect detection&quot;</span>
+<span class="sd">      &lt;https://ui.adsabs.harvard.edu/abs/2011JCAP...03..051C&gt;`_</span>
 <span class="sd">    &quot;&quot;&quot;</span>
 
     <span class="n">DEFAULT_SCALE_RADIUS</span> <span class="o">=</span> <span class="mf">24.42</span> <span class="o">*</span> <span class="n">u</span><span class="o">.</span><span class="n">kpc</span>
@@ -667,8 +672,10 @@ <h1>Source code for gammapy.astro.darkmatter.profiles</h1><div class="highlight"
 
 <span class="sd">    References</span>
 <span class="sd">    ----------</span>
-<span class="sd">    * `1997ApJ...490..493 &lt;https://ui.adsabs.harvard.edu/abs/1997ApJ...490..493N&gt;`_</span>
-<span class="sd">    * `2011JCAP...03..051C &lt;https://ui.adsabs.harvard.edu/abs/2011JCAP...03..051C&gt;`_</span>
+<span class="sd">    * `Navarro et al. (1997), &quot;A Universal Density Profile from Hierarchical Clustering&quot;</span>
+<span class="sd">      &lt;https://ui.adsabs.harvard.edu/abs/1997ApJ...490..493N&gt;`_</span>
+<span class="sd">    * `Marco et al. (2011), &quot;PPPC 4 DM ID: a poor particle physicist cookbook for dark matter indirect detection&quot;</span>
+<span class="sd">      &lt;https://ui.adsabs.harvard.edu/abs/2011JCAP...03..051C&gt;`_</span>
 <span class="sd">    &quot;&quot;&quot;</span>
 
     <span class="n">DEFAULT_SCALE_RADIUS</span> <span class="o">=</span> <span class="mf">24.42</span> <span class="o">*</span> <span class="n">u</span><span class="o">.</span><span class="n">kpc</span>
@@ -712,8 +719,10 @@ <h1>Source code for gammapy.astro.darkmatter.profiles</h1><div class="highlight"
 
 <span class="sd">    References</span>
 <span class="sd">    ----------</span>
-<span class="sd">    * `1965TrAlm...5...87E &lt;https://ui.adsabs.harvard.edu/abs/1965TrAlm...5...87E&gt;`_</span>
-<span class="sd">    * `2011JCAP...03..051C &lt;https://ui.adsabs.harvard.edu/abs/2011JCAP...03..051C&gt;`_</span>
+<span class="sd">    * `Einasto (1965), &quot;On the Construction of a Composite Model for the Galaxy and on the Determination of the System</span>
+<span class="sd">      of Galactic Parameters&quot; &lt;https://ui.adsabs.harvard.edu/abs/1965TrAlm...5...87E&gt;`_</span>
+<span class="sd">    * `Marco et al. (2011), &quot;PPPC 4 DM ID: a poor particle physicist cookbook for dark matter indirect detection&quot;</span>
+<span class="sd">      &lt;https://ui.adsabs.harvard.edu/abs/2011JCAP...03..051C&gt;`_</span>
 <span class="sd">    &quot;&quot;&quot;</span>
 
     <span class="n">DEFAULT_SCALE_RADIUS</span> <span class="o">=</span> <span class="mf">28.44</span> <span class="o">*</span> <span class="n">u</span><span class="o">.</span><span class="n">kpc</span>
@@ -759,8 +768,10 @@ <h1>Source code for gammapy.astro.darkmatter.profiles</h1><div class="highlight"
 
 <span class="sd">    References</span>
 <span class="sd">    ----------</span>
-<span class="sd">    * `1991MNRAS.249..523B &lt;https://ui.adsabs.harvard.edu/abs/1991MNRAS.249..523B&gt;`_</span>
-<span class="sd">    * `2011JCAP...03..051C &lt;https://ui.adsabs.harvard.edu/abs/2011JCAP...03..051C&gt;`_</span>
+<span class="sd">    * `Begeman et al. (1991), &quot;Extended rotation curves of spiral galaxies : dark haloes and modified dynamics&quot;</span>
+<span class="sd">      &lt;https://ui.adsabs.harvard.edu/abs/1965TrAlm...5...87E&gt;`_</span>
+<span class="sd">    * `Marco et al. (2011), &quot;PPPC 4 DM ID: a poor particle physicist cookbook for dark matter indirect detection&quot;</span>
+<span class="sd">      &lt;https://ui.adsabs.harvard.edu/abs/2011JCAP...03..051C&gt;`_</span>
 <span class="sd">    &quot;&quot;&quot;</span>
 
     <span class="n">DEFAULT_SCALE_RADIUS</span> <span class="o">=</span> <span class="mf">4.38</span> <span class="o">*</span> <span class="n">u</span><span class="o">.</span><span class="n">kpc</span>
@@ -798,8 +809,10 @@ <h1>Source code for gammapy.astro.darkmatter.profiles</h1><div class="highlight"
 
 <span class="sd">    References</span>
 <span class="sd">    ----------</span>
-<span class="sd">    * `1995ApJ...447L..25B &lt;https://ui.adsabs.harvard.edu/abs/1995ApJ...447L..25B&gt;`_</span>
-<span class="sd">    * `2011JCAP...03..051C &lt;https://ui.adsabs.harvard.edu/abs/2011JCAP...03..051C&gt;`_</span>
+<span class="sd">    * `Burkert (1995), &quot;The Structure of Dark Matter Halos in Dwarf Galaxies&quot;</span>
+<span class="sd">      &lt;https://ui.adsabs.harvard.edu/abs/1965TrAlm...5...87E&gt;`_</span>
+<span class="sd">    * `Marco et al. (2011), &quot;PPPC 4 DM ID: a poor particle physicist cookbook for dark matter indirect detection&quot;</span>
+<span class="sd">      &lt;https://ui.adsabs.harvard.edu/abs/2011JCAP...03..051C&gt;`_</span>
 <span class="sd">    &quot;&quot;&quot;</span>
 
     <span class="n">DEFAULT_SCALE_RADIUS</span> <span class="o">=</span> <span class="mf">12.67</span> <span class="o">*</span> <span class="n">u</span><span class="o">.</span><span class="n">kpc</span>
@@ -839,8 +852,10 @@ <h1>Source code for gammapy.astro.darkmatter.profiles</h1><div class="highlight"
 
 <span class="sd">    References</span>
 <span class="sd">    ----------</span>
-<span class="sd">    * `2004MNRAS.353..624D &lt;https://ui.adsabs.harvard.edu/abs/2004MNRAS.353..624D&gt;`_</span>
-<span class="sd">    * `2011JCAP...03..051C &lt;https://ui.adsabs.harvard.edu/abs/2011JCAP...03..051C&gt;`_</span>
+<span class="sd">    * `Diemand et al. (2004), &quot;Convergence and scatter of cluster density profiles&quot;</span>
+<span class="sd">      &lt;https://ui.adsabs.harvard.edu/abs/1965TrAlm...5...87E&gt;`_</span>
+<span class="sd">    * `Marco et al. (2011), &quot;PPPC 4 DM ID: a poor particle physicist cookbook for dark matter indirect detection&quot;</span>
+<span class="sd">      &lt;https://ui.adsabs.harvard.edu/abs/2011JCAP...03..051C&gt;`_</span>
 <span class="sd">    &quot;&quot;&quot;</span>
 
     <span class="n">DEFAULT_SCALE_RADIUS</span> <span class="o">=</span> <span class="mf">30.28</span> <span class="o">*</span> <span class="n">u</span><span class="o">.</span><span class="n">kpc</span>

diff --git a/docs/dev/_modules/gammapy/astro/darkmatter/spectra.html b/docs/dev/_modules/gammapy/astro/darkmatter/spectra.html
@@ -66,7 +66,7 @@
     <link rel="search" title="Search" href="../../../../search.html" />
   <meta name="viewport" content="width=device-width, initial-scale=1"/>
   <meta name="docsearch:language" content="en"/>
-  <meta name="docsearch:version" content="2.0.dev452+g4492f4b7c" />
+  <meta name="docsearch:version" content="2.0.dev456+g82fae34f9" />
   </head>
 
 
@@ -492,8 +492,10 @@ <h1>Source code for gammapy.astro.darkmatter.spectra</h1><div class="highlight">
 
 <span class="sd">    References</span>
 <span class="sd">    ----------</span>
-<span class="sd">    * `2011JCAP...03..051 &lt;https://ui.adsabs.harvard.edu/abs/2011JCAP...03..051C&gt;`_</span>
-<span class="sd">    * Cirelli et al (2016): http://www.marcocirelli.net/PPPC4DMID.html</span>
+<span class="sd">    * `Marco et al. (2011), &quot;PPPC 4 DM ID: a poor particle physicist cookbook for dark matter indirect detection&quot;</span>
+<span class="sd">      &lt;https://ui.adsabs.harvard.edu/abs/2011JCAP...03..051C&gt;`_</span>
+<span class="sd">    * `Cirelli et al. (2016), &quot;PPPC 4 DM ID: A Poor Particle Physicist Cookbook for Dark Matter Indirect Detection&quot;</span>
+<span class="sd">      &lt;http://www.marcocirelli.net/PPPC4DMID.html&gt;`_</span>
 <span class="sd">    &quot;&quot;&quot;</span>
 
     <span class="n">channel_registry</span> <span class="o">=</span> <span class="p">{</span>
@@ -668,7 +670,8 @@ <h1>Source code for gammapy.astro.darkmatter.spectra</h1><div class="highlight">
 
 <span class="sd">    References</span>
 <span class="sd">    ----------</span>
-<span class="sd">    * `2011JCAP...03..051 &lt;https://ui.adsabs.harvard.edu/abs/2011JCAP...03..051C&gt;`_</span>
+<span class="sd">    `Marco et al. (2011), &quot;PPPC 4 DM ID: a poor particle physicist cookbook for dark matter indirect detection&quot;</span>
+<span class="sd">    &lt;https://ui.adsabs.harvard.edu/abs/2011JCAP...03..051C&gt;`_</span>
 <span class="sd">    &quot;&quot;&quot;</span>
 
     <span class="n">THERMAL_RELIC_CROSS_SECTION</span> <span class="o">=</span> <span class="mf">3e-26</span> <span class="o">*</span> <span class="n">u</span><span class="o">.</span><span class="n">Unit</span><span class="p">(</span><span class="s2">&quot;cm3 s-1&quot;</span><span class="p">)</span>
@@ -787,7 +790,8 @@ <h1>Source code for gammapy.astro.darkmatter.spectra</h1><div class="highlight">
 
 <span class="sd">    References</span>
 <span class="sd">    ----------</span>
-<span class="sd">    * `2011JCAP...03..051 &lt;https://ui.adsabs.harvard.edu/abs/2011JCAP...03..051C&gt;`_</span>
+<span class="sd">    `Marco et al. (2011), &quot;PPPC 4 DM ID: a poor particle physicist cookbook for dark matter indirect detection&quot;</span>
+<span class="sd">    &lt;https://ui.adsabs.harvard.edu/abs/2011JCAP...03..051C&gt;`_</span>
 <span class="sd">    &quot;&quot;&quot;</span>
 
     <span class="n">LIFETIME_AGE_OF_UNIVERSE</span> <span class="o">=</span> <span class="mf">4.3e17</span> <span class="o">*</span> <span class="n">u</span><span class="o">.</span><span class="n">Unit</span><span class="p">(</span><span class="s2">&quot;s&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
@@ -66,7 +66,7 @@
     <link rel="search" title="Search" href="../../../../search.html" />
   <meta name="viewport" content="width=device-width, initial-scale=1"/>
   <meta name="docsearch:language" content="en"/>
-  <meta name="docsearch:version" content="2.0.dev452+g4492f4b7c" />
+  <meta name="docsearch:version" content="2.0.dev456+g82fae34f9" />
   </head>
 
 

diff --git a/docs/dev/_modules/gammapy/astro/population/simulate.html b/docs/dev/_modules/gammapy/astro/population/simulate.html
@@ -66,7 +66,7 @@
     <link rel="search" title="Search" href="../../../../search.html" />
   <meta name="viewport" content="width=device-width, initial-scale=1"/>
   <meta name="docsearch:language" content="en"/>
-  <meta name="docsearch:version" content="2.0.dev452+g4492f4b7c" />
+  <meta name="docsearch:version" content="2.0.dev456+g82fae34f9" />
   </head>