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Anisotropic masks (#217)
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*Anisotropic weighting implemented
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damonge authored Oct 9, 2024
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3 changes: 2 additions & 1 deletion doc/1BasicFunctionality.html
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<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>
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3 changes: 2 additions & 1 deletion doc/1BasicFunctionality.ipynb
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"- **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."
]
},
{
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3 changes: 2 additions & 1 deletion doc/2Spin.html
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<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>
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3 changes: 2 additions & 1 deletion doc/2Spin.ipynb
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"- **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."
]
},
{
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3 changes: 2 additions & 1 deletion doc/3Covariances.html
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<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>
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3 changes: 2 additions & 1 deletion doc/3Covariances.ipynb
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"- **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."
]
},
{
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3 changes: 2 additions & 1 deletion doc/4Catalogs.html
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<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>
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3 changes: 2 additions & 1 deletion doc/4Catalogs.ipynb
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"- **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."
]
},
{
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