build based on ce01268

dev/.documenter-siteinfo.json

@@ -1 +1 @@
-{"documenter":{"julia_version":"1.6.7","generation_timestamp":"2024-03-27T15:24:44","documenter_version":"1.3.0"}}
+{"documenter":{"julia_version":"1.6.7","generation_timestamp":"2024-03-28T08:48:31","documenter_version":"1.3.0"}}

dev/bc2016/index.html

@@ -29,4 +29,4 @@
   }{
     \sum_{j}
     \Gamma\bigl([\MR(\rho,t,\omega)\cdot\Vx_\lambda]_{j}\bigr)^2
-  } \, ,\]</p><p>which is a normalized correlation between the <span>$\Gamma$</span>-corrected images.</p><p>To compensate for different pixel sizes, the image <span>$x$</span> or <span>$x$</span> which has the larger pixel size is interpolated so that both images have the same (smallest) pixel size.</p><p>Separable linear interpolation with a triangle kernel is applied for magnifying and fine shifting the images.</p><p>The criterion is minimized for a translation between each images (for each spectral channel).</p><p>In every spectral channel, the brightness of the restored images is scaled so that the total flux per channel is the same as in the reference image.</p><p>Because the resolution of the reference image may change (see above) the score is the ratio between the sum for all spectral channels of the scores between the restored images and the reference images divided by the sum for all spectral channels of the scores between a zero image and the reference images.</p><section class="footnotes is-size-7"><ul><li class="footnote" id="footnote-Sanchez2016"><a class="tag is-link" href="#citeref-Sanchez2016">Sanchez2016</a><blockquote><p>J. Sanchez-Bermudez, É. Thiébaut, K.-H. Hofmann, M. Heininger, D. Schertl, G. Weigelt, F. Millour, A. Schutz, A. Ferrari, M. Vannier, D. Mary, J. Young &amp; F. Malbet, F., <em>The 2016 interferometric imaging beauty contest</em> in Optical and Infrared Interferometry and Imaging V, SPIE International Conference, <strong>9907</strong>, 99071D (2016) <a href="https://doi.org/10.1117/12.2231982">doi</a>.</p></blockquote></li></ul></section></article><nav class="docs-footer"><a class="docs-footer-prevpage" href="../general/">« General image metrics</a><div class="flexbox-break"></div><p class="footer-message">Powered by <a href="https://github.com/JuliaDocs/Documenter.jl">Documenter.jl</a> and the <a href="https://julialang.org/">Julia Programming Language</a>.</p></nav></div><div class="modal" id="documenter-settings"><div class="modal-background"></div><div class="modal-card"><header class="modal-card-head"><p class="modal-card-title">Settings</p><button class="delete"></button></header><section class="modal-card-body"><p><label class="label">Theme</label><div class="select"><select id="documenter-themepicker"><option value="auto">Automatic (OS)</option><option value="documenter-light">documenter-light</option><option value="documenter-dark">documenter-dark</option></select></div></p><hr/><p>This document was generated with <a href="https://github.com/JuliaDocs/Documenter.jl">Documenter.jl</a> version 1.3.0 on <span class="colophon-date" title="Wednesday 27 March 2024 15:24">Wednesday 27 March 2024</span>. Using Julia version 1.6.7.</p></section><footer class="modal-card-foot"></footer></div></div></div></body></html>
+  } \, ,\]</p><p>which is a normalized correlation between the <span>$\Gamma$</span>-corrected images.</p><p>To compensate for different pixel sizes, the image <span>$x$</span> or <span>$x$</span> which has the larger pixel size is interpolated so that both images have the same (smallest) pixel size.</p><p>Separable linear interpolation with a triangle kernel is applied for magnifying and fine shifting the images.</p><p>The criterion is minimized for a translation between each images (for each spectral channel).</p><p>In every spectral channel, the brightness of the restored images is scaled so that the total flux per channel is the same as in the reference image.</p><p>Because the resolution of the reference image may change (see above) the score is the ratio between the sum for all spectral channels of the scores between the restored images and the reference images divided by the sum for all spectral channels of the scores between a zero image and the reference images.</p><section class="footnotes is-size-7"><ul><li class="footnote" id="footnote-Sanchez2016"><a class="tag is-link" href="#citeref-Sanchez2016">Sanchez2016</a><blockquote><p>J. Sanchez-Bermudez, É. Thiébaut, K.-H. Hofmann, M. Heininger, D. Schertl, G. Weigelt, F. Millour, A. Schutz, A. Ferrari, M. Vannier, D. Mary, J. Young &amp; F. Malbet, F., <em>The 2016 interferometric imaging beauty contest</em> in Optical and Infrared Interferometry and Imaging V, SPIE International Conference, <strong>9907</strong>, 99071D (2016) <a href="https://doi.org/10.1117/12.2231982">doi</a>.</p></blockquote></li></ul></section></article><nav class="docs-footer"><a class="docs-footer-prevpage" href="../general/">« General image metrics</a><div class="flexbox-break"></div><p class="footer-message">Powered by <a href="https://github.com/JuliaDocs/Documenter.jl">Documenter.jl</a> and the <a href="https://julialang.org/">Julia Programming Language</a>.</p></nav></div><div class="modal" id="documenter-settings"><div class="modal-background"></div><div class="modal-card"><header class="modal-card-head"><p class="modal-card-title">Settings</p><button class="delete"></button></header><section class="modal-card-body"><p><label class="label">Theme</label><div class="select"><select id="documenter-themepicker"><option value="auto">Automatic (OS)</option><option value="documenter-light">documenter-light</option><option value="documenter-dark">documenter-dark</option></select></div></p><hr/><p>This document was generated with <a href="https://github.com/JuliaDocs/Documenter.jl">Documenter.jl</a> version 1.3.0 on <span class="colophon-date" title="Thursday 28 March 2024 08:48">Thursday 28 March 2024</span>. Using Julia version 1.6.7.</p></section><footer class="modal-card-foot"></footer></div></div></div></body></html>

dev/general/index.html

@@ -6,4 +6,4 @@
   \min_{\alpha,\beta} \Vert \alpha\,\MR\cdot\Vx + \beta\,\One - \Vy\Vert
 }{
   \min_{\beta} \Vert \beta\,\One - \Vy \Vert
-}\]</p><p>where <span>$\Zero$</span> is an image of the same size as <span>$\Vy$</span> but filled with zeros.</p><section class="footnotes is-size-7"><ul><li class="footnote" id="footnote-Gomes2016"><a class="tag is-link" href="#citeref-Gomes2016">Gomes2016</a><blockquote><p>N. Gomes, P. J. V. Garcia &amp; É. Thiébaut, <em>Assessing the quality of restored images in optical long-baseline interferometry</em> in Monthly Notices of the Royal Astronomical Society, vol. <strong>465</strong>, pp. 3823-3839 (2016).</p></blockquote></li></ul></section></article><nav class="docs-footer"><a class="docs-footer-prevpage" href="../">« Image metrics</a><a class="docs-footer-nextpage" href="../bc2016/">The 2016&#39; Interferometric Beauty Contest »</a><div class="flexbox-break"></div><p class="footer-message">Powered by <a href="https://github.com/JuliaDocs/Documenter.jl">Documenter.jl</a> and the <a href="https://julialang.org/">Julia Programming Language</a>.</p></nav></div><div class="modal" id="documenter-settings"><div class="modal-background"></div><div class="modal-card"><header class="modal-card-head"><p class="modal-card-title">Settings</p><button class="delete"></button></header><section class="modal-card-body"><p><label class="label">Theme</label><div class="select"><select id="documenter-themepicker"><option value="auto">Automatic (OS)</option><option value="documenter-light">documenter-light</option><option value="documenter-dark">documenter-dark</option></select></div></p><hr/><p>This document was generated with <a href="https://github.com/JuliaDocs/Documenter.jl">Documenter.jl</a> version 1.3.0 on <span class="colophon-date" title="Wednesday 27 March 2024 15:24">Wednesday 27 March 2024</span>. Using Julia version 1.6.7.</p></section><footer class="modal-card-foot"></footer></div></div></div></body></html>
+}\]</p><p>where <span>$\Zero$</span> is an image of the same size as <span>$\Vy$</span> but filled with zeros.</p><section class="footnotes is-size-7"><ul><li class="footnote" id="footnote-Gomes2016"><a class="tag is-link" href="#citeref-Gomes2016">Gomes2016</a><blockquote><p>N. Gomes, P. J. V. Garcia &amp; É. Thiébaut, <em>Assessing the quality of restored images in optical long-baseline interferometry</em> in Monthly Notices of the Royal Astronomical Society, vol. <strong>465</strong>, pp. 3823-3839 (2016).</p></blockquote></li></ul></section></article><nav class="docs-footer"><a class="docs-footer-prevpage" href="../">« Image metrics</a><a class="docs-footer-nextpage" href="../bc2016/">The 2016&#39; Interferometric Beauty Contest »</a><div class="flexbox-break"></div><p class="footer-message">Powered by <a href="https://github.com/JuliaDocs/Documenter.jl">Documenter.jl</a> and the <a href="https://julialang.org/">Julia Programming Language</a>.</p></nav></div><div class="modal" id="documenter-settings"><div class="modal-background"></div><div class="modal-card"><header class="modal-card-head"><p class="modal-card-title">Settings</p><button class="delete"></button></header><section class="modal-card-body"><p><label class="label">Theme</label><div class="select"><select id="documenter-themepicker"><option value="auto">Automatic (OS)</option><option value="documenter-light">documenter-light</option><option value="documenter-dark">documenter-dark</option></select></div></p><hr/><p>This document was generated with <a href="https://github.com/JuliaDocs/Documenter.jl">Documenter.jl</a> version 1.3.0 on <span class="colophon-date" title="Thursday 28 March 2024 08:48">Thursday 28 March 2024</span>. Using Julia version 1.6.7.</p></section><footer class="modal-card-foot"></footer></div></div></div></body></html>