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LSSTDESC · Oct 6, 2024 · f446e94 · f446e94
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diff --git a/doc/1BasicFunctionality.html b/doc/1BasicFunctionality.html
@@ -7538,7 +7538,8 @@
 <li><strong>A19</strong>. The original NaMaster paper (Alonso et al. 2019 <a href="https://arxiv.org/abs/1809.09603">https://arxiv.org/abs/1809.09603</a>).</li>
 <li><strong>G19</strong>. Garcia-Garcia et al. 2019 (<a href="https://arxiv.org/abs/1906.11765">https://arxiv.org/abs/1906.11765</a>), which introduces the basic approximation used by NaMaster to estimate covariance matrix.</li>
 <li><strong>N20</strong>. Nicola et al. 2020 (<a href="https://arxiv.org/abs/2010.09717">https://arxiv.org/abs/2010.09717</a>), which refined these approximations and described in detail the procedure to estimate cosmic shear power spectra.</li>
-<li><strong>W24</strong>. Wolz et al. 2024 (TBD), which introduced the formalism for catalog-based $C_\ell$s.</li>
+<li><strong>W24</strong>. Wolz et al. 2024 (<a href="https://arxiv.org/abs/2407.21013">https://arxiv.org/abs/2407.21013</a>), which introduced the formalism for catalog-based $C_\ell$s.</li>
+<li><strong>A24</strong>. Alonso 2024 (TBD), which generalised the estimator to anisotropic weights.</li>
 </ul>
 </div>
 </div>

diff --git a/doc/1BasicFunctionality.ipynb b/doc/1BasicFunctionality.ipynb
@@ -22,7 +22,8 @@
     "- **A19**. The original NaMaster paper (Alonso et al. 2019 https://arxiv.org/abs/1809.09603).\n",
     "- **G19**. Garcia-Garcia et al. 2019 (https://arxiv.org/abs/1906.11765), which introduces the basic approximation used by NaMaster to estimate covariance matrix.\n",
     "- **N20**. Nicola et al. 2020 (https://arxiv.org/abs/2010.09717), which refined these approximations and described in detail the procedure to estimate cosmic shear power spectra.\n",
-    "- **W24**. Wolz et al. 2024 (TBD), which introduced the formalism for catalog-based $C_\\ell$s."
+    "- **W24**. Wolz et al. 2024 (https://arxiv.org/abs/2407.21013), which introduced the formalism for catalog-based $C_\\ell$s.\n",
+    "- **A24**. Alonso 2024 (TBD), which generalised the estimator to anisotropic weights."
    ]
   },
   {

diff --git a/doc/2Spin.html b/doc/2Spin.html
@@ -7538,7 +7538,8 @@
 <li><strong>A19</strong>. The original NaMaster paper (Alonso et al. 2019 <a href="https://arxiv.org/abs/1809.09603">https://arxiv.org/abs/1809.09603</a>).</li>
 <li><strong>G19</strong>. Garcia-Garcia et al. 2019 (<a href="https://arxiv.org/abs/1906.11765">https://arxiv.org/abs/1906.11765</a>), which introduces the basic approximation used by NaMaster to estimate covariance matrix.</li>
 <li><strong>N20</strong>. Nicola et al. 2020 (<a href="https://arxiv.org/abs/2010.09717">https://arxiv.org/abs/2010.09717</a>), which refined these approximations and described in detail the procedure to estimate cosmic shear power spectra.</li>
-<li><strong>W24</strong>. Wolz et al. 2024 (TBD), which introduced the formalism for catalog-based $C_\ell$s.</li>
+<li><strong>W24</strong>. Wolz et al. 2024 (<a href="https://arxiv.org/abs/2407.21013">https://arxiv.org/abs/2407.21013</a>), which introduced the formalism for catalog-based $C_\ell$s.</li>
+<li><strong>A24</strong>. Alonso 2024 (TBD), which generalised the estimator to anisotropic weights.</li>
 </ul>
 </div>
 </div>

diff --git a/doc/2Spin.ipynb b/doc/2Spin.ipynb
@@ -22,7 +22,8 @@
     "- **A19**. The original NaMaster paper (Alonso et al. 2019 https://arxiv.org/abs/1809.09603).\n",
     "- **G19**. Garcia-Garcia et al. 2019 (https://arxiv.org/abs/1906.11765), which introduces the basic approximation used by NaMaster to estimate covariance matrix.\n",
     "- **N20**. Nicola et al. 2020 (https://arxiv.org/abs/2010.09717), which refined these approximations and described in detail the procedure to estimate cosmic shear power spectra.\n",
-    "- **W24**. Wolz et al. 2024 (TBD), which introduced the formalism for catalog-based $C_\\ell$s."
+    "- **W24**. Wolz et al. 2024 (https://arxiv.org/abs/2407.21013), which introduced the formalism for catalog-based $C_\\ell$s.\n",
+    "- **A24**. Alonso 2024 (TBD), which generalised the estimator to anisotropic weights."
    ]
   },
   {

diff --git a/doc/3Covariances.html b/doc/3Covariances.html
@@ -7540,7 +7540,8 @@
 <li><strong>A19</strong>. The original NaMaster paper (Alonso et al. 2019 <a href="https://arxiv.org/abs/1809.09603">https://arxiv.org/abs/1809.09603</a>).</li>
 <li><strong>G19</strong>. Garcia-Garcia et al. 2019 (<a href="https://arxiv.org/abs/1906.11765">https://arxiv.org/abs/1906.11765</a>), which introduces the basic approximation used by NaMaster to estimate covariance matrix.</li>
 <li><strong>N20</strong>. Nicola et al. 2020 (<a href="https://arxiv.org/abs/2010.09717">https://arxiv.org/abs/2010.09717</a>), which refined these approximations and described in detail the procedure to estimate cosmic shear power spectra.</li>
-<li><strong>W24</strong>. Wolz et al. 2024 (TBD), which introduced the formalism for catalog-based $C_\ell$s.</li>
+<li><strong>W24</strong>. Wolz et al. 2024 (<a href="https://arxiv.org/abs/2407.21013">https://arxiv.org/abs/2407.21013</a>), which introduced the formalism for catalog-based $C_\ell$s.</li>
+<li><strong>A24</strong>. Alonso 2024 (TBD), which generalised the estimator to anisotropic weights.</li>
 </ul>
 </div>
 </div>

diff --git a/doc/3Covariances.ipynb b/doc/3Covariances.ipynb
@@ -24,7 +24,8 @@
     "- **A19**. The original NaMaster paper (Alonso et al. 2019 https://arxiv.org/abs/1809.09603).\n",
     "- **G19**. Garcia-Garcia et al. 2019 (https://arxiv.org/abs/1906.11765), which introduces the basic approximation used by NaMaster to estimate covariance matrix.\n",
     "- **N20**. Nicola et al. 2020 (https://arxiv.org/abs/2010.09717), which refined these approximations and described in detail the procedure to estimate cosmic shear power spectra.\n",
-    "- **W24**. Wolz et al. 2024 (TBD), which introduced the formalism for catalog-based $C_\\ell$s."
+    "- **W24**. Wolz et al. 2024 (https://arxiv.org/abs/2407.21013), which introduced the formalism for catalog-based $C_\\ell$s.\n",
+    "- **A24**. Alonso 2024 (TBD), which generalised the estimator to anisotropic weights."
    ]
   },
   {

diff --git a/doc/4Catalogs.html b/doc/4Catalogs.html
@@ -7542,7 +7542,8 @@
 <li><strong>A19</strong>. The original NaMaster paper (Alonso et al. 2019 <a href="https://arxiv.org/abs/1809.09603">https://arxiv.org/abs/1809.09603</a>).</li>
 <li><strong>G19</strong>. Garcia-Garcia et al. 2019 (<a href="https://arxiv.org/abs/1906.11765">https://arxiv.org/abs/1906.11765</a>), which introduces the basic approximation used by NaMaster to estimate covariance matrix.</li>
 <li><strong>N20</strong>. Nicola et al. 2020 (<a href="https://arxiv.org/abs/2010.09717">https://arxiv.org/abs/2010.09717</a>), which refined these approximations and described in detail the procedure to estimate cosmic shear power spectra.</li>
-<li><strong>W24</strong>. Wolz et al. 2024 (TBD), which introduced the formalism for catalog-based $C_\ell$s.</li>
+<li><strong>W24</strong>. Wolz et al. 2024 (<a href="https://arxiv.org/abs/2407.21013">https://arxiv.org/abs/2407.21013</a>), which introduced the formalism for catalog-based $C_\ell$s.</li>
+<li><strong>A24</strong>. Alonso 2024 (TBD), which generalised the estimator to anisotropic weights.</li>
 </ul>
 </div>
 </div>

diff --git a/doc/4Catalogs.ipynb b/doc/4Catalogs.ipynb
@@ -26,7 +26,8 @@
     "- **A19**. The original NaMaster paper (Alonso et al. 2019 https://arxiv.org/abs/1809.09603).\n",
     "- **G19**. Garcia-Garcia et al. 2019 (https://arxiv.org/abs/1906.11765), which introduces the basic approximation used by NaMaster to estimate covariance matrix.\n",
     "- **N20**. Nicola et al. 2020 (https://arxiv.org/abs/2010.09717), which refined these approximations and described in detail the procedure to estimate cosmic shear power spectra.\n",
-    "- **W24**. Wolz et al. 2024 (TBD), which introduced the formalism for catalog-based $C_\\ell$s."
+    "- **W24**. Wolz et al. 2024 (https://arxiv.org/abs/2407.21013), which introduced the formalism for catalog-based $C_\\ell$s.\n",
+    "- **A24**. Alonso 2024 (TBD), which generalised the estimator to anisotropic weights."
    ]
   },
   {