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<ri:Resource created="2015-12-10T16:22:09Z" 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>373 GRBs between 0.008&lt;z&lt;6.7</title><shortName>J/ApJ/807/76</shortName><identifier>ivo://CDS.VizieR/J/ApJ/807/76</identifier><altIdentifier>doi:10.26093/cds/vizier.18070076</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Li M.-H.</name></creator><creator><name>Lin H.-N.</name></creator><date role="Updated">2017-12-22T05:32:16Z</date><date role="Created">2015-12-10T16:22:09Z</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>gamma-ray-astronomy</subject><subject>redshifted</subject><description>In this paper, we examine the spatial distribution of gamma-ray bursts (GRBs) using a sample of 373 objects. We subdivide the GRB data into two redshift intervals over the redshift range 0&lt;z&lt;6.7. We measure the two-point correlation function, {xi}(r), of the GRBs. In determining the separation distance of the GRB pairs, we consider two representative cosmological models: a cold dark matter universe plus a cosmological constant {Lambda}, with ({Omega}_m_,{Omega}_{Lambda}_)=(0.28,0.72), and an Einstein-de Sitter universe, with ({Omega}_m_,{Omega}_{Lambda}_)=(1,0). We find a z-decreasing correlation of the GRB distribution, which is in agreement with the predictions of the current structure formation theory. We fit a power-law model {xi}(r)=(r/r0)^-{gamma}^ to the measured {xi}(r) and obtain an amplitude and slope of r_0_=1235.2+/-342.6h^-1^Mpc and {gamma}=0.80+/-0.19, respectively (1{sigma} confidence level), over the scales r=200-10^4^h^-1^Mpc. Our results provide a supplement to the measurement of matter correlation on large scales, while the matter distribution below 200h^-1^Mpc is usually described by the correlation function of galaxies.</description><source format="bibcode">2015ApJ...807...76L</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/807/76</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/J/ApJS/216/32">J/ApJS/216/32 : Localizations of GRBs with Fermi GBM (Connaughton+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/581/A125">J/A+A/581/A125 : UV/Optical/NIR spectroscopy GRB hosts (Kruehler+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/573/A81">J/A+A/573/A81 : Spectral properties of energetic GRBs (Yu+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/568/A75">J/A+A/568/A75 : GRB 130925A GROND light curves (Greiner+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/568/A19">J/A+A/568/A19 : Photometry of 3 {gamma}-ray burst supernovae (Cano+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/572/A12">J/A+A/572/A12 : GRB 140506A spectra (Fynbo+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/562/A29">J/A+A/562/A29 : GRB 100814A GROND and UVOT light curves (Nardini+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/211/13">J/ApJS/211/13 : The second Fermi/GBM GRB catalog (4yr) (von Kienlin+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/208/20">J/ApJS/208/20 : Nine-year WMAP point source catalogs (Bennett+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/560/A70">J/A+A/560/A70 : GRB 100621A unusual afterglow (Greiner+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/557/A18">J/A+A/557/A18 : GRB 120815A afterglow spectra (Kruehler+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/199/18">J/ApJS/199/18 : The Fermi GBM catalog (Paciesas+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/426/2">J/MNRAS/426/2 : GRB 091018 Optical/NIR photometry (Wiersema+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/744/141">J/ApJ/744/141 : Shapes of GRB light curves (Bhat+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/730/119">J/ApJ/730/119 : HST/WFC3 obs. of Cepheids in SN Ia hosts (Riess+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/535/A57">J/A+A/535/A57 : g'r'i'z'JH light curves of GRB 091127 (Filgas+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/531/A39">J/A+A/531/A39 : g'r'i'z'JHKs light curves of GRB 081029 (Nardini+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/406/2473">J/MNRAS/406/2473 : Photometry of GRB 071025 (Perley+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/720/862">J/ApJ/720/862 : Afterglow light curve of GRB 090926A (Rau+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/508/593">J/A+A/508/593 : GRB 080710 bright optical/NIR afterglow (Kruehler+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/384/404">J/ApJ/384/404 : Redshifts of a nearby rich clusters of gal. 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