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J/ApJ/701/824    Afterglows of short and long-duration GRBs  (Nysewander+, 2009)

A comparison of the afterglows of short- and long-duration gamma-ray bursts. Nysewander M., Fruchter A.S., Pe'er A. <Astrophys. J., 701, 824-836 (2009)> =2009ApJ...701..824N
ADC_Keywords: Gamma rays ; X-ray sources ; Photometry Keywords: gamma rays: bursts - radiation mechanisms: non-thermal Abstract: We present a comparative study of the observed properties of the optical and X-ray afterglows of short- and long-duration γ-ray bursts (GRBs). Using a large sample of 37 short and 421 long GRBs, we find a strong correlation between the afterglow brightness measured after 11hr and the observed fluence of the prompt emission. Both the optical (R band) and X-ray flux densities (FR and FX) scale with the γ-ray fluence, Fγ. For bursts with a known redshift, a tight correlation exists between the afterglow flux densities at 11hr (rest frame) and the total isotropic γ-ray energy, Eγ,ISO: FR,X∝Eγ,ISOα, with α∼1. Description: In this study, we include GRBs detected by all satellites, beginning with GRB 970111, the first localization with follow-up observations capable of detecting an afterglow, and ending over a decade later, with GRB 071227. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table1.dat 164 37 Observed prompt and afterglow properties of short-duration GRBs table2.dat 164 420 Observed prompt and afterglow properties of long-duration GRBs refs.dat 130 735 References
See also: J/ApJ/693/1484 : Early optical afterglow catalog (Cenko+, 2009) J/ApJ/686/1209 : Optical properties of GRB afterglows (Melandri+, 2008) J/AJ/133/1027 : Positions for 179 Swift X-ray afterglows (Butler+, 2007) J/A+A/455/813 : BeppoSAX catalog of GRB X-ray afterglows (De Pasquale+, 2006) Byte-by-byte Description of file: table1.dat table2.dat
Bytes Format Units Label Explanations
1- 7 A7 --- GRB GRB designation 9- 18 A10 --- Sat Satellite 20- 21 I2 keV LoCh Lower energy channel 23- 27 I5 keV UpCh Upper energy channel 29- 34 F6.4 --- z ? Redshift 35 A1 --- f_z [ab] Probable (a) or Cluster (b) redshift 37- 44 F8.2 10-10J/m2 Flu Fluence in 10-7erg/cm2 46- 51 F6.2 10-10J/m2 E_Flu ? Upper limit uncertainty in Flu 53- 58 F6.2 10-10J/m2 e_Flu ? Lower limit uncertainty in Flu 60 A1 --- l_logE Limit flag on logE 61- 65 F5.2 [10-7J] logE ? Total isotropic γ-ray energy (erg) 67- 70 F4.2 [10-7J] E_logE ? Upper limit uncertainty in logE 72- 75 F4.2 [10-7J] e_logE ? Lower limit uncertainty in logE 77 A1 --- l_RFlux Limit flag on RFlux 78- 84 F7.1 uJy RFlux ? R band flux density 11 hours after the burst 87- 92 F6.1 uJy E_RFlux ? Upper limit uncertainty in RFlux 95- 99 F5.1 uJy e_RFlux ? Lower limit uncertainty in RFlux 101 A1 --- l_XFlux Limit flag on XFlux 102-108 F7.2 10-17W/m2 XFlux ? The 0.2-10keV X-ray flux 11 hours after the burst (10-14erg/cm2/s) 110-116 F7.2 10-17W/m2 E_XFlux ? Upper limit uncertainty in XFlux 118-124 F7.2 10-17W/m2 e_XFlux ? Lower limit uncertainty in XFlux 126-128 A3 --- n_XFlux [abcd, ] energy range of XFlux (2) 130 A1 --- l_FR/FX Limit flag on FR/FX 131-135 F5.2 --- FR/FX ? Ratio of R band to X-ray fluxes 137-140 F4.2 --- E_FR/FX ? Upper limit uncertainty in FR/FX 142-145 F4.2 --- e_FR/FX ? Lower limit uncertainty in FR/FX 147-164 A18 --- Ref Reference(s) (see refs.dat file)
Note (2): Flag as follows: a = 1.6-10.0keV; b = 2-10keV; c = 0.5-6.0keV; d = Uses estimated NH.
Byte-by-byte Description of file: refs.dat
Bytes Format Units Label Explanations
1- 3 I3 --- Ref Reference number 5- 23 A19 --- BibCode Bibcode 25-130 A106 --- Comm Authors and comment
History: From electronic version of the journal
(End) Greg Schwarz [AAS], Emmanuelle Perret [CDS] 08-Sep-2011
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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