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</div> <div class="control"> <button class="button is-small is-link">Go</button> </div> </div> </form> </div> </div> <ol class="breathe-horizontal" start="1"> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/2405.00669">arXiv:2405.00669</a> <span> [<a href="https://arxiv.org/pdf/2405.00669">pdf</a>, <a href="https://arxiv.org/format/2405.00669">other</a>] </span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Cosmology and Nongalactic Astrophysics">astro-ph.CO</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Data Analysis, Statistics and Probability">physics.data-an</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Computation">stat.CO</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1051/0004-6361/202450617">10.1051/0004-6361/202450617 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> Euclid preparation. LIII. LensMC, weak lensing cosmic shear measurement with forward modelling and Markov Chain Monte Carlo sampling </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&query=Euclid+Collaboration"> Euclid Collaboration</a>, <a href="/search/physics?searchtype=author&query=Congedo%2C+G">G. Congedo</a>, <a href="/search/physics?searchtype=author&query=Miller%2C+L">L. Miller</a>, <a href="/search/physics?searchtype=author&query=Taylor%2C+A+N">A. N. Taylor</a>, <a href="/search/physics?searchtype=author&query=Cross%2C+N">N. Cross</a>, <a href="/search/physics?searchtype=author&query=Duncan%2C+C+A+J">C. A. J. Duncan</a>, <a href="/search/physics?searchtype=author&query=Kitching%2C+T">T. Kitching</a>, <a href="/search/physics?searchtype=author&query=Martinet%2C+N">N. Martinet</a>, <a href="/search/physics?searchtype=author&query=Matthew%2C+S">S. Matthew</a>, <a href="/search/physics?searchtype=author&query=Schrabback%2C+T">T. Schrabback</a>, <a href="/search/physics?searchtype=author&query=Tewes%2C+M">M. Tewes</a>, <a href="/search/physics?searchtype=author&query=Welikala%2C+N">N. Welikala</a>, <a href="/search/physics?searchtype=author&query=Aghanim%2C+N">N. Aghanim</a>, <a href="/search/physics?searchtype=author&query=Amara%2C+A">A. Amara</a>, <a href="/search/physics?searchtype=author&query=Andreon%2C+S">S. Andreon</a>, <a href="/search/physics?searchtype=author&query=Auricchio%2C+N">N. Auricchio</a>, <a href="/search/physics?searchtype=author&query=Baldi%2C+M">M. Baldi</a>, <a href="/search/physics?searchtype=author&query=Bardelli%2C+S">S. Bardelli</a>, <a href="/search/physics?searchtype=author&query=Bender%2C+R">R. Bender</a>, <a href="/search/physics?searchtype=author&query=Bodendorf%2C+C">C. Bodendorf</a>, <a href="/search/physics?searchtype=author&query=Bonino%2C+D">D. Bonino</a>, <a href="/search/physics?searchtype=author&query=Branchini%2C+E">E. Branchini</a>, <a href="/search/physics?searchtype=author&query=Brescia%2C+M">M. Brescia</a>, <a href="/search/physics?searchtype=author&query=Brinchmann%2C+J">J. Brinchmann</a>, <a href="/search/physics?searchtype=author&query=Camera%2C+S">S. Camera</a> , et al. (217 additional authors not shown) </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="2405.00669v4-abstract-short" style="display: inline;"> LensMC is a weak lensing shear measurement method developed for Euclid and Stage-IV surveys. It is based on forward modelling in order to deal with convolution by a point spread function (PSF) with comparable size to many galaxies; sampling the posterior distribution of galaxy parameters via Markov Chain Monte Carlo; and marginalisation over nuisance parameters for each of the 1.5 billion galaxies… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2405.00669v4-abstract-full').style.display = 'inline'; document.getElementById('2405.00669v4-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="2405.00669v4-abstract-full" style="display: none;"> LensMC is a weak lensing shear measurement method developed for Euclid and Stage-IV surveys. It is based on forward modelling in order to deal with convolution by a point spread function (PSF) with comparable size to many galaxies; sampling the posterior distribution of galaxy parameters via Markov Chain Monte Carlo; and marginalisation over nuisance parameters for each of the 1.5 billion galaxies observed by Euclid. We quantified the scientific performance through high-fidelity images based on the Euclid Flagship simulations and emulation of the Euclid VIS images; realistic clustering with a mean surface number density of 250 arcmin$^{-2}$ ($I_{\rm E}<29.5$) for galaxies, and 6 arcmin$^{-2}$ ($I_{\rm E}<26$) for stars; and a diffraction-limited chromatic PSF with a full width at half maximum of $0.^{\!\prime\prime}2$ and spatial variation across the field of view. LensMC measured objects with a density of 90 arcmin$^{-2}$ ($I_{\rm E}<26.5$) in 4500 deg$^2$. The total shear bias was broken down into measurement (our main focus here) and selection effects (which will be addressed elsewhere). We found measurement multiplicative and additive biases of $m_1=(-3.6\pm0.2)\times10^{-3}$, $m_2=(-4.3\pm0.2)\times10^{-3}$, $c_1=(-1.78\pm0.03)\times10^{-4}$, $c_2=(0.09\pm0.03)\times10^{-4}$; a large detection bias with a multiplicative component of $1.2\times10^{-2}$ and an additive component of $-3\times10^{-4}$; and a measurement PSF leakage of $伪_1=(-9\pm3)\times10^{-4}$ and $伪_2=(2\pm3)\times10^{-4}$. When model bias is suppressed, the obtained measurement biases are close to Euclid requirement and largely dominated by undetected faint galaxies ($-5\times10^{-3}$). Although significant, model bias will be straightforward to calibrate given the weak sensitivity. LensMC is publicly available at https://gitlab.com/gcongedo/LensMC <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('2405.00669v4-abstract-full').style.display = 'none'; document.getElementById('2405.00669v4-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 2 December, 2024; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 1 May, 2024; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> May 2024. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">28 pages, 18 figures, and 2 tables</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> A&A 691, A319 (2024) </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/0712.1548">arXiv:0712.1548</a> <span> [<a href="https://arxiv.org/pdf/0712.1548">pdf</a>] </span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Astrophysics">astro-ph</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="General Relativity and Quantum Cosmology">gr-qc</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="High Energy Physics - Phenomenology">hep-ph</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Space Physics">physics.space-ph</span> </div> </div> <p class="title is-5 mathjax"> Science with the new generation high energy gamma- ray experiments </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&query=Alvarez%2C+M">M. Alvarez</a>, <a href="/search/physics?searchtype=author&query=D%27Armiento%2C+D">D. D'Armiento</a>, <a href="/search/physics?searchtype=author&query=Agnetta%2C+G">G. Agnetta</a>, <a href="/search/physics?searchtype=author&query=Alberdi%2C+A">A. Alberdi</a>, <a href="/search/physics?searchtype=author&query=Antonelli%2C+A">A. Antonelli</a>, <a href="/search/physics?searchtype=author&query=Argan%2C+A">A. Argan</a>, <a href="/search/physics?searchtype=author&query=Assis%2C+P">P. Assis</a>, <a href="/search/physics?searchtype=author&query=Baltz%2C+E+A">E. A. Baltz</a>, <a href="/search/physics?searchtype=author&query=Bambi%2C+C">C. Bambi</a>, <a href="/search/physics?searchtype=author&query=Barbiellini%2C+G">G. Barbiellini</a>, <a href="/search/physics?searchtype=author&query=Bartko%2C+H">H. Bartko</a>, <a href="/search/physics?searchtype=author&query=Basset%2C+M">M. Basset</a>, <a href="/search/physics?searchtype=author&query=Bastieri%2C+D">D. Bastieri</a>, <a href="/search/physics?searchtype=author&query=Belli%2C+P">P. Belli</a>, <a href="/search/physics?searchtype=author&query=Benford%2C+G">G. Benford</a>, <a href="/search/physics?searchtype=author&query=Bergstrom%2C+L">L. Bergstrom</a>, <a href="/search/physics?searchtype=author&query=Bernabei%2C+R">R. Bernabei</a>, <a href="/search/physics?searchtype=author&query=Bertone%2C+G">G. Bertone</a>, <a href="/search/physics?searchtype=author&query=Biland%2C+A">A. Biland</a>, <a href="/search/physics?searchtype=author&query=Biondo%2C+B">B. Biondo</a>, <a href="/search/physics?searchtype=author&query=Bocchino%2C+F">F. Bocchino</a>, <a href="/search/physics?searchtype=author&query=Branchini%2C+E">E. Branchini</a>, <a href="/search/physics?searchtype=author&query=Brigida%2C+M">M. Brigida</a>, <a href="/search/physics?searchtype=author&query=Bringmann%2C+T">T. Bringmann</a>, <a href="/search/physics?searchtype=author&query=Brogueira%2C+P">P. Brogueira</a> , et al. (175 additional authors not shown) </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="0712.1548v1-abstract-short" style="display: inline;"> This Conference is the fifth of a series of Workshops on High Energy Gamma- ray Experiments, following the Conferences held in Perugia 2003, Bari 2004, Cividale del Friuli 2005, Elba Island 2006. This year the focus was on the use of gamma-ray to study the Dark Matter component of the Universe, the origin and propagation of Cosmic Rays, Extra Large Spatial Dimensions and Tests of Lorentz Invaria… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('0712.1548v1-abstract-full').style.display = 'inline'; document.getElementById('0712.1548v1-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="0712.1548v1-abstract-full" style="display: none;"> This Conference is the fifth of a series of Workshops on High Energy Gamma- ray Experiments, following the Conferences held in Perugia 2003, Bari 2004, Cividale del Friuli 2005, Elba Island 2006. This year the focus was on the use of gamma-ray to study the Dark Matter component of the Universe, the origin and propagation of Cosmic Rays, Extra Large Spatial Dimensions and Tests of Lorentz Invariance. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('0712.1548v1-abstract-full').style.display = 'none'; document.getElementById('0712.1548v1-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 4 December, 2007; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> December 2007. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">328 pages, 7.8Mb, Proceedings of the 5th SCINEGHE Workshop, June 18-20, 2007 http://www.roma2.infn.it/SciNeGHE07/</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Frascati Physics Series vol.45 (2007) A.Lionetto, A.Morselli editors ISBN 978-88-86409-54-0 </p> </li> </ol> <div class="is-hidden-tablet">  <span class="help" style="display: inline-block;"><a href="https://github.com/arXiv/arxiv-search/releases">Search v0.5.6 released 2020-02-24</a>  </span> </div> </div> </main> <footer> <div class="columns is-desktop" role="navigation" aria-label="Secondary">  <div class="column"> <div class="columns"> <div class="column"> <ul class="nav-spaced"> <li><a href="https://info.arxiv.org/about">About</a></li> <li><a href="https://info.arxiv.org/help">Help</a></li> </ul> </div> <div class="column"> <ul class="nav-spaced"> <li> <svg xmlns="http://www.w3.org/2000/svg" viewBox="0 0 512 512" class="icon filter-black" role="presentation"><title>contact arXiv</title><desc>Click here to contact arXiv</desc><path d="M502.3 190.8c3.9-3.1 9.7-.2 9.7 4.7V400c0 26.5-21.5 48-48 48H48c-26.5 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