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<ri:Resource created="2018-06-29T09:42:39Z" 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>HeII photoionization rates of quasars</title><shortName>J/ApJ/847/81</shortName><identifier>ivo://CDS.VizieR/J/ApJ/847/81</identifier><altIdentifier>doi:10.26093/cds/vizier.18470081</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Schmidt T.M.</name></creator><creator><name>Worseck G.</name></creator><creator><name>Hennawi J.F.</name></creator><creator><name>Prochaska J.X.</name></creator><creator><name>Crighton N.H.M.</name></creator><date role="Updated">2020-02-03T08:45:25Z</date><date role="Created">2018-06-29T09:42:39Z</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>intergalactic-medium</subject><subject>redshifted</subject><subject>visible-astronomy</subject><subject>spectroscopy</subject><subject>ultraviolet-astronomy</subject><subject>surveys</subject><description>The HeII transverse proximity effect-enhanced HeII Ly{alpha} transmission in a background sightline caused by the ionizing radiation of a foreground quasar-offers a unique opportunity to probe the morphology of quasar-driven HeII reionization. We conduct a comprehensive spectroscopic survey to find z~3 quasars in the foreground of 22 background quasar sightlines with Hubble Space Telescope/COS HeII Ly{alpha} transmission spectra. With our two-tiered survey strategy, consisting of a deep pencil-beam survey and a shallow wide-field survey, we discover 131 new quasars, which we complement with known SDSS/BOSS quasars in our fields. Using a restricted sample of 66 foreground quasars with inferred HeII photoionization rates greater than the expected UV background at these redshifts ({Gamma}_QSO_^HeII^&gt;5x10^-16^s^-1^) we perform the first statistical analysis of the HeII transverse proximity effect. Our results show qualitative evidence for a large object-to-object variance: among the four foreground quasars with the highest {Gamma}_QSO_^HeII^ only one (previously known) quasar is associated with a significant HeII transmission spike. We perform a stacking analysis to average down these fluctuations, and detect an excess in the average HeII transmission near the foreground quasars at 3{sigma} significance. This statistical evidence for the transverse proximity effect is corroborated by a clear dependence of the signal strength on {Gamma}_QSO_^HeII^. Our detection places a purely geometrical lower limit on the quasar lifetime of t_Q_&gt;25Myr. Improved modeling would additionally constrain quasar obscuration and the mean free path of HeII-ionizing photons.</description><source format="bibcode">2017ApJ...847...81S</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/847/81</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><relationship><relationshipType>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/B/hst">B/hst : HST Archived Exposures Catalog (STScI, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/294">II/294 : The SDSS Photometric Catalog, Release 7 (Adelman-McCarthy+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/V/147">V/147 : The SDSS Photometric Catalogue, Release 12 (Alam+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/592/728">J/ApJ/592/728 : Lyman break galaxies at redshift z~3 (Steidel+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/651/61">J/ApJ/651/61 : Optically thick absorbers near luminous QSO (Hennawi+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/166/470">J/ApJS/166/470 : SDSS-Spitzer type I QSOs IR photometry (Richards+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/133/2222">J/AJ/133/2222 : Clustering of high-redshift QSOs from SDSS (Shen+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/391/1457">J/MNRAS/391/1457 : Lyman{alpha} forest in QSO pairs (Kirkman+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/690/20">J/ApJ/690/20 : Models of AGN and black hole populations (Shankar+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/716/348">J/ApJ/716/348 : The XMM-Newton survey of the COSMOS field (Brusa+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/728/23">J/ApJ/728/23 : GALEX UV-bright high-redshift quasars (Worseck+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/772/26">J/ApJ/772/26 : AGN with WISE. 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