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<ri:Resource created="2025-08-29T07:31:20Z" status="active" updated="2025-09-01T07:18:35Z" 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>Pulses from Fermi-GBM gamma-ray bursts</title><shortName>J/ApJ/949/110</shortName><identifier>ivo://CDS.VizieR/J/ApJ/949/110</identifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Tak D.</name></creator><creator><name>Uhm Z.L.</name></creator><creator><name>Racusin J.</name></creator><creator><name>Zhang B.</name></creator><creator><name>Guiriec S.</name></creator><creator><name>Kocevski D.,Zhang B.-B.</name></creator><creator><name>McEnery J.</name></creator><date role="Updated">2025-09-01T07:18:35Z</date><date role="Created">2025-08-29T07:31:20Z</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><description>We perform a detailed analysis of broad pulses in bright gamma-ray bursts (GRBs) to understand the evolution of GRB broad pulses. Using the temporal and spectral properties, we test the high-latitude emission (HLE) scenario in the decaying phase of broad pulses. The HLE originates from the curvature effect of a relativistic spherical jet, where higher-latitude photons are delayed and softer than the observer's line-of-sight emission. The signature of HLE has not yet been identified undisputedly during the prompt emission of GRBs. The HLE theory predicts a specific relation, F_{nu},Ep_{propto}E_p_^2^, between the peak energy Ep in {nu}F{nu} spectra and the spectral flux F{nu} measured at Ep, F_{nu},Ep_. We search for evidence of this relation in 2157 GRBs detected by the Gamma-ray Burst Monitor on board the Fermi Gamma-ray Space Telescope from 2008 to 2017. After imposing unbiased selection criteria in order to minimize contamination in a signal by background and overlaps of pulses, we build a sample of 32 broad pulses in 32 GRBs. We perform a time-resolved spectral analysis on each of these 32 broad pulses and find that the evolution of 18 pulses (56%) is clearly consistent with the HLE relation. For the 18 broad pulses, the exponent {delta} in the relation of F_{nu},Ep_{propto}Ep^{delta}^ is distributed as a Gaussian function with a median and width of 1.99 and 0.34, respectively. This result provides a constraint on the emission radius of GRBs with the HLE signature.</description><source format="bibcode">2023ApJ...949..110T</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/949/110</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/ApJ/740/104">J/ApJ/740/104 : BATSE GRB pulse catalog - preliminary data (Hakkila+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/756/112">J/ApJ/756/112 : Fermi/GBM GRB time-resolved spectral analysis (Lu+, 2012)</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/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/ApJ/865/153">J/ApJ/865/153 : Analysis of Fermi GRB data. 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