J/MNRAS/418/2202ivo://CDS.VizieR/J/MNRAS/418/2202doi:10.26093/cds/vizier.74182202CDSDainotti M.G.Ostrowski M.Willingale R.2024-07-16T20:12:03Z2012-10-10T17:19:50ZCDS support team

CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France

cds-question@unistra.frgamma-ray-astronomyx-ray-sourcesTo find out the astrophysical processes responsible for gamma-ray burst (GRB), it is crucial to discover and understand the relations between their observational properties. This work was performed in the GRB rest frames using a sample of 62 long Swift GRBs with known redshifts. Following the earlier analysis of the correlation between afterglow luminosity (L^*^a) and break time (T^*^a), we extend it to correlations between the afterglow and the prompt emission GRB physical parameters.2011MNRAS.418.2202Dhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/418/2202CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toJ/A+AS/129/1 : GRANAT/WATCH catalogue of gamma-ray bursts (Sazonov+ 1998)J/ApJS/169/62 : GRB database of spectral lags (Hakkila+, 2007)J/ApJS/195/2 : The second Swift BAT GRB catalog (BAT2) (Sakamoto+, 2011)J/A+A/528/A122 : SwiftFT catalog (Puccetti+, 2011)J/ApJ/701/824 : Afterglows of short and long-duration GRBs (Nysewander+, 2009)J/ApJ/704/1405 : Testing the E_peak_-E_iso_ relation for GRBs (Krimm+, 2009)J/ApJ/711/495 : Durations of Swift/BAT GRBs (Butler+, 2010)J/ApJ/720/1513 : The afterglows of Swift-era GRBs. I. (Kann+, 2010)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/418/2202https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/418/2202http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/418/2202https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/MNRAS/418/2202https://vizier.iucaa.in/viz-bin/votable?-source=J/MNRAS/418/2202http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/MNRAS/418/2202GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/MNRAS/418/2202/table1 (*A data list for GRBs with known redshifts analysed in the paper)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/MNRAS/418/2202/table1?https://vizier.iucaa.in/viz-bin/conesearch/J/MNRAS/418/2202/table1?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/MNRAS/418/2202/table1?GETtext/xml+votable180.050000true306.475417-42.6006080.0055555555555555566/314 500 503 2357 3536 4323 4450 4955 5633 5726 5941 6261 7518 8798 9100 9682 10135 10447 11673 11905 12134 12597 13312 13701 13924 16991 17453 17721 18494 18777 18910 18978 19168 19293 19731 19890 19911 21439 23138 25901 25946 27566 27906 28063 31281 31385 31494 32110 33617 33679 33735 34440 34949 35330 36074 36297 36528 37007 38926 40433 42952 44021-44022 45205 45938 47162 47459 48458 49004https://cdsarc.cds.unistra.fr/viz-bin/moc/J/MNRAS/418/2202?format=asciiGamma-rayX-raydefaultJ/MNRAS/418/2202/table1*A data list for GRBs with known redshifts analysed in the paperzRedshiftsrc.redshiftfloatrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintn_GRB[long IC] class of GRB (1)meta.notecharGRBGRB identification (1)meta.id;meta.maincharbetaX-ray spectral index {beta}_a_ of the emission at afterglow time T*a (2)spect.indexfloate_betarms uncertainty on betastat.errorfloatFXX-ray observed flux not corrected for absorption, FX=Fa*exp(-Tp/Ta) (2)mW.m**-2phot.flux;em.X-raydoublee_FXrms uncertainty on FXmW.m**-2stat.errordoublelogT*90Time interval during which the background-subtracted cumulative counts increase from 5% to 95%log(s)phot.countfloate_logT*90rms uncertainty on logT*90log(s)stat.errorfloatlogT*45Time spanned by the brightest 45% of the total counts above the backgroundlog(s)time;arith.difffloate_logT*45rms uncertainty on logT*45log(s)stat.errorfloatlogT*pFitted transition time in which the exponential decay in the prompt phase changes to a power-law decay (2)log(s)time;arith.difffloate_logT*prms uncertainty on logT*plog(s)stat.errorfloatlogT*aBreak (afterglow) time (2)log(s)time;arith.difffloate_logT*arms uncertainty on logT*alog(s)stat.errorfloatlogL*aX-ray luminosity (2)log(1e-07W)phys.luminosity;em.X-rayfloate_logL*arms uncertainty on logL*alog(1e-07W)stat.errorfloatlogE*iIsotropic energylog(1e-07J)phys.energyfloate_logE*irms uncertainty on logE*ilog(1e-07J)stat.errorfloatlogE*pPeak energy in the {nu}F_{nu}_ spectrumlog(keV)phys.energyfloate_logE*prms uncertainty on logE*plog(keV)stat.errorfloatuValue of the error parameter u defined by u^2^ = e_logT*a^2^ + e_logL*a^2^stat.errorfloatn_u[U] U for the U0.095 subsample ("upper envelope" with fit u<=0.095)meta.notecharSimbadSimbad column added by the CDSmeta.refchar_RARight Ascension (J2000) from SIMBAD (not part of the original data)degpos.eq.ra;meta.main_DEDeclination (J2000) from SIMBAD (not part of the original data)degpos.eq.dec;meta.main