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<ri:Resource created="2020-07-29T14:32:35Z" 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>Swift long gamma-ray bursts</title><shortName>J/ApJS/248/21</shortName><identifier>ivo://CDS.VizieR/J/ApJS/248/21</identifier><altIdentifier>doi:10.26093/cds/vizier.22480021</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Hao J.-M.</name></creator><creator><name>Cao L.</name></creator><creator><name>Lu Y.-J.</name></creator><creator><name>Chu Q.-B.</name></creator><creator><name>Fan J.-H.</name></creator><creator><name>Yuan Y.-F.</name></creator><creator><name>Yuan Y.-H.</name></creator><date role="Updated">2020-10-09T09:49:11Z</date><date role="Created">2020-07-29T14:32:35Z</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>gamma-ray-bursts</subject><subject>redshifted</subject><subject>astronomical-reference-materials</subject><subject>chemical-abundances</subject><description>The exact relationship between the long gamma-ray burst (LGRB) rate and the cosmic star formation rate (CSFR) is essential for using LGRBs as cosmological probes. In this work, we collect a large sample composed of 371 Swift LGRBs with known redshifts and prompt emission properties. We first compare the rest-frame prompt properties of these bursts in different redshift bins, finding negligible redshift evolution of the luminosity of LGRBs with L_iso_&gt;~10^51^erg/s between z~1 and z~4. Then, by utilizing the CSFR obtained from the large-scale cosmological hydrodynamical simulation, the Illustris simulation, we calculate the cumulative redshift distribution of LGRBs under different metallicity thresholds. After comparing with our sample, we find that the predictions with a moderate threshold between 0.3Z_{sun}_&lt;=Z_th_&lt;=1.0Z_{sun}_ are consistent with the sample between redshift 0&lt;z&lt;3, while at higher redshifts, between 3&lt;z&lt;5, all metallicity thresholds fit the data well. When changing to an empirical model based on observations, the predictions show similar results as well. After comparing with the metallicity distribution of the observed LGRB host galaxies between 0&lt;z&lt;1, we confirm that the production of LGRBs in galaxies with super-solar metallicity is suppressed. Nevertheless, considering that a significant fraction of stars are born in sub-solar metallicity environments at z&gt;~3, we suggest that, as a first approximation, LGRBs can be used as direct tracers of the CSFR in this redshift range.</description><source format="bibcode">2020ApJS..248...21H</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/248/21</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/swift">B/swift : Swift Master Catalog (HEASARC, 2004-)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/IX/51">IX/51 : GRB list (1990-2014) (Ruggeri+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/427/87">J/A+A/427/87 : List of GRBs (Gorosabel+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/617/240">J/ApJ/617/240 : Oxygen abundances in the GOODS-North field (Kobulnicky+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/701/824">J/ApJ/701/824 : Afterglows of short and long-duration GRBs (Nysewander+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/711/495">J/ApJ/711/495 : Durations of Swift/BAT GRBs (Butler+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/731/103">J/ApJ/731/103 : Redshift catalog for Swift long GRBs (Xiao+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/431/3608">J/MNRAS/431/3608 : BeppoSAX/GRBM and Fermi/GBM long GRBs (Dichiara+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/800/16">J/ApJ/800/16 : Swift-XRT long GRB durations (Boer+, 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/ApJ/802/103">J/ApJ/802/103 : Model predictions for GRB host galaxies (Trenti+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/820/66">J/ApJ/820/66 : Cosmic evolution of long GRB luminosity (Deng+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/829/7">J/ApJ/829/7 : 3rd Swift/BAT GRB catalog (past ~11yrs) (BAT3) (Lien+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/817/118">J/ApJ/817/118 : SFR-M_*_ relation from ZFOURGE (Tomczak+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/227/7">J/ApJS/227/7 : Long + short GRBs with host galaxies data (Li+, 2016)</relatedResource><relatedResource>http://www.grbhosts.org/ : GRB Host Studies (GHostS) home page</relatedResource><relatedResource>http://www.mpe.mpg.de/~jcg/grbgen.html : Greiner's GRB online table</relatedResource><relatedResource>http://swift.gsfc.nasa.gov/archive/grb_table.html : Swift GRBs home page</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/ApJS/248/21</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJS/248/21</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJS/248/21</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJS/248/21</accessURL><mirrorURL title="VizieR at IUCAA: Pune, 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(1)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="7*">char</dataType></column><column><name>recno</name><description>Record number assigned by the VizieR team. 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