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<ri:Resource created="2017-01-10T06:54:38Z" 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>GRB light-curve decay indices with Swift</title><shortName>J/ApJ/828/36</shortName><identifier>ivo://CDS.VizieR/J/ApJ/828/36</identifier><altIdentifier>doi:10.26093/cds/vizier.18280036</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Del Vecchio R.</name></creator><creator><name>Dainotti M.G.</name></creator><creator><name>Ostrowski M.</name></creator><date role="Updated">2017-10-13T15:40:48Z</date><date role="Created">2017-01-10T06:54:38Z</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><description>In this work, we study the distribution of temporal power-law decay indices, {alpha}, in the gamma-ray burst (GRB) afterglow phase, fitted for 176 GRBs (139 long GRBs, 12 short GRBs with extended emission, and 25 X-ray flashes) with known redshifts. These indices are compared with the temporal decay index, {alpha}_W_, derived with the light-curve fitting using the Willingale+ (2007ApJ...662.1093W) model. This model fitting yields similar distributions of {alpha}_W_ to the fitted {alpha}, but for individual bursts a difference can be significant. Analysis of ({alpha}, L_a_) distribution, where L_a_ is the characteristic luminosity at the end of the plateau, reveals only a weak correlation of these quantities. However, we discovered a significant regular trend when studying GRB {alpha} values along the Dainotti+ (2013ApJ...774..157D) correlation between L_a_ and the end time of the plateau emission in the rest frame, T_a_^*^, hereafter LT correlation. We note a systematic variation of the {alpha} parameter distribution with luminosity for any selected T_a_^*^. We analyze this systematics with respect to the fitted LT correlation line, expecting that the presented trend may allow us to constrain the GRB physical models. We also attempted to use the derived correlation of {alpha}(T_a_) versus L_a_(T_a_) to diminish the luminosity scatter related to the variations of {alpha} along the LT distribution, a step forward in the effort of standardizing GRBs. A proposed toy model accounting for this systematics applied to the analyzed GRB distribution results in a slight increase of the LT correlation coefficient.</description><source format="bibcode">2016ApJ...828...36D</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/828/36</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/IX/43">IX/43 : 1SXPS Swift X-ray telescope point source catalogue (Evans+ 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/589/A98">J/A+A/589/A98 : Swift GRBs power density spectra (Guidorzi+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/224/20">J/ApJS/224/20 : 10yr of Swift/XRT obs. of GRBs (Yi+, 2016)</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/ApJS/209/20">J/ApJS/209/20 : Swift GRB catalog with X-ray data (Grupe+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/774/157">J/ApJ/774/157 : Swift GRBs with X-ray afterglows and z&lt;9.5 (Dainotti+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/428/729">J/MNRAS/428/729 : GRB Swift X-ray light curves analysis (Margutti+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/418/2202">J/MNRAS/418/2202 : Analysis of {gamma}-ray bursts (Dainotti+, 2011)</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/ApJ/720/1513">J/ApJ/720/1513 : The afterglows of Swift-era GRBs. 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