Access to Astronomical Catalogues

← Click to display the menu
J/A+A/455/813    BeppoSAX catalog of GRB X-ray afterglows   (De Pasquale+, 2006)

The BeppoSAX catalog of GRB X-ray afterglow observations. De Pasquale M., Piro L., Gendre B., Amati L., Antonelli L.A., Costa E., Feroci M., Frontera F., Nicastro L., Soffitta P., in't Zand J. <Astron. Astrophys. 455, 813 (2006)> =2006A&A...455..813D
ADC_Keywords: Gamma rays ; X-ray sources Keywords: X-rays: general - gamma-rays: bursts - catalogs Abstract: We present the catalog of X-ray afterglow observed by BeppoSAX from the launch of the satellite to the end of the mission. Thirty-three X-ray afterglows out of 39 observations were securely identified based on their fading behavior. We have extracted the continuum parameters (decay index, spectral index, flux, absorption) for all available afterglows. We point out a possible correlation between the X-ray afterglow luminosity and the energy emitted during the prompt gamma-ray event. Description: This catalog gives the list of gamma-ray bursts observed by the BeppoSAX narrow fields instruments. We list for convenience bursts discovered by BeppoSAX or discovered by another mission but which X-ray afterglow was observed by BeppoSAX (table1.dat). We also list the properties of these bursts (table2.dat). Other informations, such as the spectral and temporal properties of the afterglow, extended to the XMM-Newton and Chandra results can be obtained at http://grb.iasf-roma.inaf.it/ File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table1.dat 77 55 GRBs localized and/or observed by BeppoSAX table2.dat 56 53 Properties of the prompt emission of BeppoSAX GRB refs.dat 154 27 References
See also: IX/20 : The Fourth BATSE Burst Revised Catalog (Paciesas+ 1999) J/A+A/427/87 : List of GRBs (Gorosabel+, 2004) J/A+A/362/799 : The BeppoSAX 2-10 keV Survey (Giommi+, 2000) http://grb.iasf-roma.inaf.it/ : IASF-Roma Gamma-Ray Burst group Home Page Byte-by-byte Description of file: table1.dat
Bytes Format Units Label Explanations
1- 10 A10 --- Name GRB name 12- 13 I2 h RAh Right ascension (J2000) 15- 16 I2 min RAm Right ascension (J2000) 18- 19 I2 s RAs Right ascension (J2000) 21 A1 --- DE- Declination sign (J2000) 22- 23 I2 deg DEd Declination (J2000) 25- 26 I2 arcmin DEm Declination (J2000) 28- 29 I2 arcsec DEs Declination (J2000) 31- 36 A6 --- LOC Localization instrument (1) 38- 43 F6.1 h 1TS ? First TOO start time 45- 50 F6.1 h 1TE ? First TOO end time 52- 56 F5.1 ks GTI ? Sum of of the Good Time Interval (GTI) 58- 62 F5.1 h 2TS ? Other TOO start time (2) 64- 68 F5.1 h 2TE ? Other TOO end time 70 A1 --- Opt Optical afterglow detection (3) 72- 77 F6.4 --- Z ? GRB redshift (4)
Note (1): Instrument as follows: NFI = BeppoSAX Narrow Field Instruments WFC = BeppoSAX Wide Field Camera (IPN) = InterPlanetary Network (RXTE) = RXTE All Sky Monitor In parenthesis, non-BeppoSAX instrument. In such a case, the localization displayed has been provided by NFI. Note (2): GRB 980425 was also observed between Nov. 10.75 and Nov. 12.0 Note (3): Detection flag as follows: N = No optical afterglow detection 0 = No optical studies Y = Optical afterglow detection S = Optical afterglow detection and supernova association Note (4): For GRB 000214 a redshift range was derived : 0.37-0.47. The median value is indicated in the table.
Byte-by-byte Description of file: table2.dat
Bytes Format Units Label Explanations
1- 10 A10 --- Name GRB name (1) 12 A1 --- XRF [YN] X-ray rich or X-ray flash event 14- 17 I4 s Gdu ? 40-700keV duration 19- 22 I4 s Xdu ? 2-10keV duration 24- 29 F6.2 nJ/m2 Gflu ? 40-700keV fluence 31- 35 F5.2 nJ/m2 e_Gflu ? 40-700keV fluence error 37- 42 F6.3 nJ/m2 Xflu ? 2-10keV fluence (2) 43- 47 F5.3 nJ/m2 e_Xflu ? 2-10keV fluence error 49- 56 A8 --- Ref References, in refs.dat file
Note (1): Individual notes on GRB: * GRB 991106 may not be a GRB. See Cornelisse et al. (2002A&A...392..885C). The 40-700keV fluence is a conservative 3 sigma limit based on GCN 448. * GRB 020410 2-10keV duration and fluence are lower limits * GRB 020427 40-700keV fluence is an upper limit Note (2): When not available, values of 2-10keV fluences have been calculated from the 2-26keV fluences and assuming the spectral parameters reported in the references.
Byte-by-byte Description of file: refs.dat
Bytes Format Units Label Explanations
1- 2 I2 --- Ref Reference code 4- 22 A19 --- BibCode BibCode 24- 39 A16 --- Aut Author's name 42-154 A113 --- Com Comments
Acknowledgements: Bruce Gendre, Bruce.Gendre(at)iasf-roma.inaf.it
(End) Patricia Vannier [CDS] 09-Nov-2006
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

catalogue service

© UDS/CNRS

Contact