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<ri:Resource created="2024-10-23T09:52:19Z" status="active" updated="2025-05-19T09:50:00Z" version="1.2" xmlns:cs="http://www.ivoa.net/xml/ConeSearch/v1.0" xmlns:ri="http://www.ivoa.net/xml/RegistryInterface/v1.0" xmlns:vr="http://www.ivoa.net/xml/VOResource/v1.0" xmlns:vs="http://www.ivoa.net/xml/VODataService/v1.1" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.ivoa.net/xml/ConeSearch/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/ConeSearch.xsd http://www.ivoa.net/xml/VOResource/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/VOResource.xsd http://www.ivoa.net/xml/VODataService/v1.1 http://vo.ari.uni-heidelberg.de/docs/schemata/VODataService.xsd" xsi:type="vs:CatalogService"><title>Ly{alpha} absorbers redshifts</title><shortName>J/MNRAS/509/1536</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/509/1536</identifier><altIdentifier>doi:10.26093/cds/vizier.75091536</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Maitra S.</name></creator><creator><name>Srianand R.</name></creator><creator><name>Gaikwad P.</name></creator><date role="Updated">2025-02-12T20:11:56Z</date><date role="Created">2024-10-23T09:52:19Z</date><contact><name>CDS support team</name><address>CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France</address><email>cds-question@unistra.fr</email></contact></curation><content><subject>quasars</subject><subject>redshifted</subject><subject>h-i-line-emission</subject><description>We present redshift-space two-point ({xi}), three-point ({dzeta}), and reduced three- point (Q) correlation of Ly{alpha} absorbers (Voigt profile components having HI column density, N_HI_&gt;10^13.5^cm^-2^) over three redshift bins spanning 1.7&lt;z&lt;3.5 using high-resolution spectra of 292 quasars. We detect positive {xi} up to 8h^-1^cMpc in all three redshift bins. The strongest detection of {dzeta}=1.81+/-0.59 (with Q=0.68+/-0.23) is in z=1.7-2.3 bin at 1-2h^-1^cMpc. The measured {xi} and {dzeta} values show an increasing trend with N_HI_, while Q remains relatively independent of N_HI_. We find {xi} and {dzeta} to evolve strongly with redshift. Using simulations, we find that {xi} and {dzeta} seen in real space may be strongly amplified by peculiar velocities in redshift space. Simulations suggest that while feedback, thermal and pressure smoothing effects influence the clustering of Ly{alpha} absorbers at small scales, i.e. &lt;0.5h^-1^cMpc, the HI photoionization rate ({GAMMA}_HI_) has a strong influence at all scales. The strong redshift evolution of {xi} and {dzeta} (for a fixed N_HI_ cut-off) is driven by the redshift evolution of the relationship between _HI_ and baryon overdensity. Our simulation using best- fitting {GAMMA}_HI_(z) measurements produces consistent clustering signals with observations at z~2 but underpredicts the clustering at higher redshifts. One possible remedy is to have higher values of {GAMMA}_HI_ at higher redshifts. Alternatively the discrepancy could be related to non-equilibrium and inhomogeneous conditions prevailing during He ii reionization not captured by our simulations.</description><source format="bibcode">2022MNRAS.509.1536M</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/509/1536</referenceURL><type>Catalog</type><contentLevel>Research</contentLevel><relationship><relationshipType>IsServedBy</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/TAP">TAP VizieR generic service</relatedResource></relationship><relationship><relationshipType>IsServedBy</relationshipType><relatedResource>Conesearch service</relatedResource></relationship></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface xsi:type="vr:WebBrowser"><accessURL use="full">https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/509/1536</accessURL><mirrorURL title="VizieR at IUCAA: Pune, 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