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J/PAZh/35/10     Gamma-ray bursts with known redshifts           (Badjin+, 2009)

Investigation of gamma-ray bursts with known redshifts: Statistical analysis of parameters. Badjin D.A., Beskin G.M., Greco G. <Pis'ma Astron. Zh. 35, 10 (2009)> =2009PAZh...35...10B =2009AstL...35....7B
ADC_Keywords: Gamma rays Keywords: gamma-ray bursts - afterglows Abstract: Observational parameters of the optical and gamma-ray emissions from 58 gamma-ray bursts (GRBs) with discovered afterglows and known redshifts are analyzed. The distributions of these parameters and pair correlations between them are studied. Approximately half of the objects exhibit a relatively slow decrease in the optical flux at initial afterglow phases (with a power-law index in the decay law α<1). Correlations have been found between the luminosities, energies, and durations of the optical and gamma-ray emissions, which can be explained by the presence of universal features in the light curves. A correlation of the peak luminosity for afterglows with the redshift and an anticorrelation of their durations with the redshift have been found for the first time. Against the background of a weak z dependence of the total afterglow energy, this effect can be explained by cosmological evolution of the GRB environment, which determines the rate of optical energy release. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table1.dat 92 58 Parameters of the "observed" sample table2.dat 87 58 Parameter of the "intrinsic" sample
See also: IX/20 : The Fourth BATSE Burst Revised Catalog (Paciesas+ 1999) IX/36 : GRANAT/PHEBUS catalog of cosmic GRB (Terekhov+, 1994-2002) J/A+AS/129/1 : GRANAT/WATCH catalogue of gamma-ray bursts (Sazonov+ 1998) J/ApJS/126/19 : BATSE gamma-ray burst spectral catalog. I. (Preece+, 2000) J/ApJS/134/385 : Supplement to the BATSE GRB catalogs (Kommers+, 2001) J/ApJ/616/1072 : The GUSBAD catalog of gamma-ray bursts (Schmidt+, 2004) J/A+A/438/1175 : First INTEGRAL SPI-ACS Gamma-Ray Burst Catalogue (Rau+, 2005) Byte-by-byte Description of file: table1.dat
Bytes Format Units Label Explanations
1- 7 A7 --- GRB GRB name 8- 11 I4 --- Npt Number of points 13- 18 F6.4 --- z Redshift 20- 25 F6.2 [mW/m2] logFopt Peak optical flux from R band 27- 30 F4.2 [mW/m2] e_logFopt rms uncertainty on logFopt 32- 37 F6.2 [mJ/m2] logSopt Optical fluence [erg/cm2] 39- 42 F4.2 [mJ/m2] e_logSopt rms uncertainty on logSopt 44- 48 F5.2 [d] logt90opt Afterglow duration in the proper frame T90opt 50- 55 F6.3 [d] logtpk Afterglow duration in the proper frame Tpk 57- 61 F5.2 [mW/m2] logFg ?=- Peak gamma-ray flux 63- 66 F4.2 [mW/m2] e_logFg ? rms uncertainty on logFg 68- 72 F5.2 [mJ/m2] logSg ?=- Gamma-ray fluence [erg/cm2] 74- 77 F4.2 [mJ/m2] e_logSg ? rms uncertainty on logSg 79- 82 F4.2 [s] logtg ? Afterglow duration in the proper frame Tg 84- 87 F4.2 --- alpha1 Power-law index of the flux decay with time (F∝t^-α) 89- 92 F4.2 --- e_alpha1 rms uncertainty on alpha
Byte-by-byte Description of file: table2.dat
Bytes Format Units Label Explanations
1- 7 A7 --- GRB GRB name 9- 14 F6.4 --- z Redshift 16- 20 F5.2 [10-7W] logLopt Isotropic equivalent of the peak optical luminosity 22- 25 F4.2 [10-7W] e_logLopt rms uncertainty on logLopt 27- 31 F5.2 [10-7J] logEopt Isotropic equivalent of the total optical energy 33- 36 F4.2 [10-7J] e_logEopt rms uncertainty on logEopt 38- 42 F5.2 [d] logT90opt Afterglow duration ( =t90opt/(1+z)) 44- 49 F6.3 [d] logTpk Afterglow duration ( =tpk/(1+z)) 51- 55 F5.2 [10-7W] logLiso ?=- Isotropic equivalent of the peak gamma-ray luminosity in the energy range 15-150keV 57- 60 F4.2 [10-7W] e_logLiso ? rms uncertainty on logLiso 62- 66 F5.2 [10-7J] logEiso ?=- Isotropic equivalent of the total gamma-ray energy (the energy range 15-150keV in the proper burst frame) 68- 71 F4.2 [10-7J] e_logEiso ? rms uncertainty on logEiso 73- 77 F5.2 [s] logTg ? Afterglow duration ( =tg/(1+z)) 79- 82 F4.2 --- alpha2 Power-law index of the flux decay with time (F∝t^-α) 84- 87 F4.2 --- e_alpha2 rms uncertainty on alpha
History: From electronic version of the journal
(End) Patricia Vannier [CDS] 12-Jan-2009
The document above follows the rules of the Standard Description for Astronomical Catalogues.From this documentation it is possible to generate f77 program to load files into arrays or line by line

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