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<ri:Resource created="2016-05-20T13:46:58Z" 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>Jet angles and gamma-ray energetics estimations</title><shortName>J/ApJ/818/18</shortName><identifier>ivo://CDS.VizieR/J/ApJ/818/18</identifier><altIdentifier>doi:10.26093/cds/vizier.18180018</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Goldstein A.</name></creator><creator><name>Connaughton V.</name></creator><creator><name>Briggs M.S.</name></creator><creator><name>Burns E.</name></creator><date role="Updated">2017-11-29T11:48:18Z</date><date role="Created">2016-05-20T13:46:58Z</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>astronomical-models</subject><description>We present a method to estimate the jet opening angles of long duration gamma-ray bursts (GRBs) using the prompt gamma-ray energetics and an inversion of the Ghirlanda relation, which is a correlation between the time-integrated peak energy of the GRB prompt spectrum and the collimation-corrected energy in gamma-rays. The derived jet opening angles using this method and detailed assumptions match well with the corresponding inferred jet opening angles obtained when a break in the afterglow is observed. Furthermore, using a model of the predicted long GRB redshift probability distribution observable by the Fermi Gamma-ray Burst Monitor (GBM), we estimate the probability distributions for the jet opening angle and rest-frame energetics for a large sample of GBM GRBs for which the redshifts have not been observed. Previous studies have only used a handful of GRBs to estimate these properties due to the paucity of observed afterglow jet breaks, spectroscopic redshifts, and comprehensive prompt gamma-ray observations, and we potentially expand the number of GRBs that can be used in this analysis by more than an order of magnitude. In this analysis, we also present an inferred distribution of jet breaks which indicates that a large fraction of jet breaks are not observable with current instrumentation and observing strategies. We present simple parameterizations for the jet angle, energetics, and jet break distributions so that they may be used in future studies.</description><source format="bibcode">2016ApJ...818...18G</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/818/18</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/A+A/588/A135">J/A+A/588/A135 : Fermi/GBM GRB time-resolved spectral catalog (Yu+, 2016)</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/ApJ/811/93">J/ApJ/811/93 : Fermi/GBM GRB minimum timescales (Golkhou+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/218/11">J/ApJS/218/11 : The 5yr Fermi/GBM magnetar burst catalog (Collazzi+, 2015)</relatedResource><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/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/208/21">J/ApJS/208/21 : The BATSE 5B GRB spectral catalog (Goldstein+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/207/39">J/ApJS/207/39 : IPN supplement to the Fermi GBM (Hurley+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/774/114">J/ApJ/774/114 : GRB 081007 and GRB 090424 light curves (Jin+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/763/15">J/ApJ/763/15 : Fermi GRB analysis. 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