<?xml version="1.0" encoding="UTF-8"?>
<OAI-PMH xmlns="http://www.openarchives.org/OAI/2.0/"
         xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
         xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/ http://www.openarchives.org/OAI/2.0/OAI-PMH.xsd">
<ListRecords>
<oai_dc:dc xmlns="http://www.openarchives.org/OAI/2.0/oai_dc/"
           xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
           xmlns:dc="http://purl.org/dc/elements/1.1/"
           xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
           xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/ http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
   	<dc:title>The effect of intrinsic alignments on weak-lensing statistics in hydrodynamical simulations</dc:title>
   	<dc:creator>Lee, Max E.</dc:creator>
   	<dc:creator>Haiman, Zoltán ; https://orcid.org/0000-0003-3633-5403</dc:creator>
   	<dc:creator>Pandey, Shivam</dc:creator>
   	<dc:creator>Genel, Shy</dc:creator>
   	<dc:subject>ddc:520</dc:subject>
   	<dc:description>The next generation of weak-gravitational-lensing surveys has the potential to place stringent constraints on cosmological parameters. However, their analysis is limited by systematics such as the intrinsic alignments of galaxies, which alter weak-lensing convergence and can lead to biases in cosmological parameter estimations. For the first time, in this work, we investigate the impact of intrinsic alignments on non-Gaussian statistics of the weak-lensing field using galaxy shapes derived from the IllustrisTNG hydrodynamical simulation. We create two catalogs of ray-traced convergence maps: one that includes the measured intrinsic shape of each galaxy and another where all galaxies are randomly rotated to eliminate intrinsic alignments. We compare a range of weak-lensing statistics between the two catalogs, including the shear–shear correlation function, the map-level angular power spectrum, one-point, peak count, and minimum distribution functions, and Minkowski functionals. For each statistic, we assess the level of statistical distinguishability between catalogs for a set of future survey angular areas. Our results reveal strong small-scale correlation in the alignment of galaxies and statistically significant boosts in weak-lensing convergence in both positive and negative directions for high-significance peaks and minima, respectively. We note that our analysis is at a fixed number density of  ˜ 5 arcmin^-2, drawn from a single realization of initial conditions, and does not include observational uncertainties or supersample covariance contributions. Weak-lensing analyses utilizing non-Gaussian statistics must account for intrinsic alignments to avoid significantly compromised cosmological inferences.</dc:description>
   	<dc:publisher>IOP Publishing</dc:publisher>
   	<dc:date>2025</dc:date>
   	<dc:type>info:eu-repo/semantics/article</dc:type>
   	<dc:type>doc-type:article</dc:type>
   	<dc:type>text</dc:type>
   	<dc:type>http://purl.org/coar/resource_type/c_2df8fbb1</dc:type>
   	<dc:identifier>https://research-explorer.ista.ac.at/record/21724</dc:identifier>
   	<dc:identifier>https://research-explorer.ista.ac.at/download/21724/21732</dc:identifier>
   	<dc:source>Lee ME, Haiman Z, Pandey S, Genel S. The effect of intrinsic alignments on weak-lensing statistics in hydrodynamical simulations. &lt;i&gt;The Astrophysical Journal&lt;/i&gt;. 2025;996(1). doi:&lt;a href=&quot;https://doi.org/10.3847/1538-4357/ae1ca7&quot;&gt;10.3847/1538-4357/ae1ca7&lt;/a&gt;</dc:source>
   	<dc:language>eng</dc:language>
   	<dc:relation>info:eu-repo/semantics/altIdentifier/doi/10.3847/1538-4357/ae1ca7</dc:relation>
   	<dc:relation>info:eu-repo/semantics/altIdentifier/issn/0004-637X</dc:relation>
   	<dc:relation>info:eu-repo/semantics/altIdentifier/e-issn/1538-4357</dc:relation>
   	<dc:relation>info:eu-repo/semantics/altIdentifier/arxiv/2504.12460</dc:relation>
   	<dc:rights>info:eu-repo/semantics/openAccess</dc:rights>
</oai_dc:dc>
</ListRecords>
</OAI-PMH>
