J/MNRAS/397/1177    Swift-XRT observations of GRBs             (Evans+, 2009)

Methods and results of an automatic analysis of a complete sample of Swift-XRT observations of GRBs. Evans P.A., Beardmore A.P. Page K.L., Osborne J.P., O'Brien, P.T., Willingale R., Starling R.L.C, Burrows D.N., Godet O., Vetere L., Racusin J., Goad M.R., Wiersema K., Angelini L., Capalbi M., Chincarini G., Gehrels N., Kennea J.A., Margutti R., Morris D.C., Mountford C.J., Pagani C., Perri M., Romano P., Tanvir N. <Mon. Not. R. Astron. Soc. 397, 1177 (2009)> =2009MNRAS.397.1177E 2009MNRAS.397.1177E
ADC_Keywords: X-ray sources ; Gamma rays Keywords: methods: data analysis - catalogues - gamma rays: bursts Abstract: We present a homogeneous X-ray analysis of all 318 Gamma Ray Bursts detected by the X-ray Telescope on the Swift satellite up to 2008 July 23; this represents the largest sample of X-ray GRB data published to date. In Sections 2-3 we detail the methods which the Swift-XRT team has developed to produce the enhanced positions, light curves, hardness ratios and spectra presented in this paper. Software using these methods continues to create such products for all new GRBs observed by the Swift-XRT. We also detail web-based tools allowing users to create these products for any object observed by the XRT, not just GRBs. In Sections 4-6 we present the results of our analysis of GRBs, including probability distribution functions of the temporal and spectral properties of the sample. We demonstrate evidence for a consistent underlying behaviour which can produce a range of light curve morphologies, and attempt to interpret this behaviour in the framework of external forward shock emission. We find several difficulties, in particular that reconciliation of our data with the forward shock model requires energy injection to continue for days to weeks. Description: Position, temporal and spectral parameters for 318 GRBs observed by the Swift X-ray telescope, up to GRB 080723B. The values were determined by automated analysis tools. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file enhpos.dat 40 268 Enhanced X-ray positions for 268 GRBs lcfit.dat 299 295 Temporal decay parameters for 295 XRT GRB light curves avespec.dat 113 320 Time-averaged X-ray spectral parameters for 318 GRBs resspec.dat 511 211 Time resolved spectral parameters for 211 GRBs -------------------------------------------------------------------------------- See also: J/A+AS/129/1 : GRANAT/WATCH catalogue of gamma-ray bursts (Sazonov+ 1998) J/A+A/473/347 : BeppoSAX complete catalogue of GRBs (Vetere+, 2007) J/A+A/427/87 : List of GRBs (Gorosabel+, 2004) Byte-by-byte Description of file: enhpos.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 8 I8 --- TargetID Swift Target ID 9- 11 A3 --- --- [GRB] 13- 19 A7 --- GRB GRB Name (YYMMDDA) 20- 28 F9.5 deg RAdeg Right ascension (J2000.0) 29- 37 F9.5 deg DEdeg Declination (J2000.0) 38- 40 F3.1 arcsec e_Pos Position uncertainty (radius, 90% confidence) -------------------------------------------------------------------------------- Byte-by-byte Description of file: lcfit.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 8 I8 --- TargetID Swift Target ID 9- 11 A3 --- --- [GRB] 13- 19 A7 --- GRB GRB Name (YYMMDDA) 20- 27 E8.4 mW/m2 Flux11 ? 0.3-10keV Flux 11 hours after the trigger 28- 35 E8.4 s Tstart When the XRT observations started, seconds since trigger 36- 43 E8.4 s Tstop When the XRT observations ended, seconds since trigger 44- 49 F6.1 s T90 ? The duration of the GRB, from the Swift data table 50- 55 F6.2 --- alpha1 Power-law decay index of the first light curve segment 57- 62 F6.2 --- E_alpha1 Positive error (90% conf) on alpha1 64- 69 F6.2 --- e_alpha1 Negative error (90% conf) on alpha1 70- 77 E8.4 s tbr1 ? Time of the first break in the decay 79- 86 E8.4 s E_tbr1 ? Positive error (90% conf) on tbr1 88- 95 E8.4 s e_tbr1 ? Negative error (90% conf) on tbr1 96-101 F6.2 --- alpha2 ? Power-law decay index of the second light curve segment 103-108 F6.2 --- E_alpha2 ? Positive error (90% conf) on alpha2 110-115 F6.2 --- e_alpha2 ? Negative error (90% conf) on alpha2 116-123 E8.4 s tbr2 ? Time of the second br in the decay 125-132 E8.4 s E_tbr2 ? Positive error (90% conf) on tbr2 134-141 E8.4 s e_tbr2 ? Negative error (90% conf) on tbr2 142-147 F6.2 --- alpha3 ? Power-law decay index of the third light curve segment 149-154 F6.2 --- E_alpha3 ? Positive error (90% conf) on alpha3 156-161 F6.2 --- e_alpha3 ? Negative error (90% conf) on alpha3 162-169 E8.4 s tbr3 ? Time of the third br in the decay 171-178 E8.4 s E_tbr3 ? Positive error (90% conf) on tbr3 180-187 E8.4 s e_tbr3 ? Negative error (90% conf) on tbr3 188-193 F6.2 --- alpha4 ? Power-law decay index of the fourth light curve segment 195-200 F6.2 --- E_alpha4 ? Positive error (90% conf) on alpha4 202-207 F6.2 --- e_alpha4 ? Negative error (90% conf) on alpha4 208-215 E8.4 s tbr4 ? Time of the fourth br in the decay 217-224 E8.4 s E_tbr4 ? Positive error (90% conf) on tbr4 226-233 E8.4 s e_tbr4 ? Negative error (90% conf) on tbr4 234-239 F6.2 --- alpha5 ? Power-law decay index of the fifth light curve segment 241-246 F6.2 --- E_alpha5 ? Positive error (90% conf) on alpha5 248-253 F6.2 --- e_alpha5 ? Negative error (90% conf) on alpha5 254-261 E8.4 s tbr5 ? Time of the fifth br in the decay 263-270 E8.4 s E_tbr5 ? Positive error (90% conf) on tbr5 272-279 E8.4 s e_tbr5 ? Negative error (90% conf) on tbr5 280-285 F6.2 --- alpha6 ? Power-law decay index of the sixth light curve segment 287-292 F6.2 --- E_alpha6 ? Positive error (90% conf) on alpha6 294-299 F6.2 --- e_alpha6 ? Negative error (90% conf) on alpha6 -------------------------------------------------------------------------------- Byte-by-byte Description of file: avespec.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 8 I8 --- TargetID Swift Target ID 9- 11 A3 --- --- [GRB] 13- 19 A7 --- GRB GRB Name (YYMMDDA) 20- 27 E8.2 cm-2 NH Galactic column density, from Kalberla et al. 2005 28- 31 F4.2 --- z ? Redshift, from the GCN circulars 32- 39 E8.2 cm-2 WTNH ? Intrinsic column density for the WT mode spectrum 41- 48 E8.2 cm-2 E_WTNH ? Positive error on WTNH 50- 57 E8.2 cm-2 e_WTNH ? Negative error on WTNH 58- 62 F5.2 --- WTbeta ? Spectral index for the WT mode spectrum 64- 67 F4.2 --- E_WTbeta ? Positive error on WTbeta 69- 72 F4.2 --- e_WTbeta ? Negative error on WTbeta 73- 80 E8.2 cm-2 PCNH ? Intrinsic column density for the PC mode spectrum 82- 89 E8.2 cm-2 E_PCNH ? Positive error on PCNH 91- 98 E8.2 cm-2 e_PCNH ? Negative error on PCNH 99-103 F5.2 --- PCbeta ? Spectral index for the PC mode spectrum 105-108 F4.2 --- E_PCbeta ? Positive error on PCbeta 110-113 F4.2 --- e_PCbeta ? Negative error on PCbeta -------------------------------------------------------------------------------- Byte-by-byte Description of file: resspec.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 8 I8 --- TargetID Swift Target ID 9- 11 A3 --- --- [GRB] 13- 19 A7 --- GRB GRB Name (YYMMDDA) 20- 27 E8.2 cm-2 WTNH1 ? Intrinsic column density for the WT mode spectrum of the first power-law segment of the light curve 29- 36 E8.2 cm-2 E_WTNH1 ? Positive error on WTNH1 38- 45 E8.2 cm-2 e_WTNH1 ? Negative error on WTNH1 46- 50 F5.2 --- WTbeta1 ? Spectral index for the WT mode spectrum of the first power-law segment of the light curve 52- 55 F4.2 --- E_WTbeta1 ? Positive error on WTbeta1 57- 60 F4.2 --- e_WTbeta1 ? Negative error on WTbeta1 61- 68 E8.2 cm-2 PCNH1 ? Intrinsic column density for the PC mode spectrum of the first power-law segment of the light curve 70- 77 E8.2 cm-2 E_PCNH1 ? Positive error on PCNH1 79- 86 E8.2 cm-2 e_PCNH1 ? Negative error on PCNH1 87- 91 F5.2 --- PCbeta1 ? Spectral index for the PC mode spectrum of the first power-law segment of the light curve 93- 96 F4.2 --- E_PCbeta1 ? Positive error on PCbeta1 98-101 F4.2 --- e_PCbeta1 ? Negative error on PCbeta1 102-109 E8.2 cm-2 WTNH2 ? Intrinsic column density for the WT mode spectrum of the second power-law segment of the light curve 111-118 E8.2 cm-2 E_WTNH2 ? Positive error on WTNH2 120-127 E8.2 cm-2 e_WTNH2 ? Negative error on WTNH2 128-132 F5.2 --- WTbeta2 ? Spectral index for the WT mode spectrum of the second power-law segment of the light curve 134-137 F4.2 --- E_WTbeta2 ? Positive error on WTbeta2 139-142 F4.2 --- e_WTbeta2 ? Negative error on WTbeta2 143-150 E8.2 cm-2 PCNH2 ? Intrinsic column density for the PC mode spectrum of the second power-law segment of the light curve 151 A1 --- --- [±] 152-159 E8.2 cm-2 E_PCNH2 ? Positive error on PCNH2 160 A1 --- --- [±] 161-168 E8.2 cm-2 e_PCNH2 ? Negative error on PCNH2 169-173 F5.2 --- PCbeta2 ? Spectral index for the PC mode spectrum of the second power-law segment of the light curve 174 A1 --- --- [±] 175-178 F4.2 --- E_PCbeta2 ? Positive error on PCbeta2 179 A1 --- --- [±] 180-183 F4.2 --- e_PCbeta2 ? Negative error on PCbeta2 184-191 E8.2 cm-2 WTNH3 ? Intrinsic column density for the WT mode spectrum of the third power-law segment of the light curve 193-200 E8.2 cm-2 E_WTNH3 ? Positive error on WTNH3 202-209 E8.2 cm-2 e_WTNH3 ? Negative error on WTNH3 210-214 F5.2 --- WTbeta3 ? Spectral index for the WT mode spectrum of the third power-law segment of the light curve 216-219 F4.2 --- E_WTbeta3 ? Positive error on WTbeta3 221-224 F4.2 --- e_WTbeta3 ? Negative error on WTbeta3 225-232 E8.2 cm-2 PCNH3 ? Intrinsic column density for the PC mode spectrum of the third power-law segment of the light curve 234-241 E8.2 cm-2 E_PCNH3 ? Positive error on PCNH3 243-250 E8.2 cm-2 e_PCNH3 ? Negative error on PCNH3 251-255 F5.2 --- PCbeta3 ? Spectral index for the PC mode spectrum of the third power-law segment of the light curve 257-260 F4.2 --- E_PCbeta3 ? Positive error on PCbeta3 262-265 F4.2 --- e_PCbeta3 ? Negative error on PCbeta3 266-273 E8.2 cm-2 WTNH4 ? Intrinsic column density for the WT mode spectrum of the fourth power-law segment of the light curve 275-282 E8.2 cm-2 E_WTNH4 ? Positive error on WTNH4 284-291 E8.2 cm-2 e_WTNH4 ? Negative error on WTNH4 292-296 F5.2 --- WTbeta4 ? Spectral index for the WT mode spectrum of the fourth power-law segment of the light curve 298-301 F4.2 --- E_WTbeta4 ? Positive error on WTbeta4 303-306 F4.2 --- e_WTbeta4 ? Negative error on WTbeta4 307-314 E8.2 cm-2 PCNH4 ? Intrinsic column density for the PC mode spectrum of the fourth power-law segment of the light curve 316-323 E8.2 cm-2 E_PCNH4 ? Positive error on PCNH4 325-332 E8.2 cm-2 e_PCNH4 ? Negative error on PCNH4 333-337 F5.2 --- PCbeta4 ? Spectral index for the PC mode spectrum of the fourth power-law segment of the light curve 339-342 F4.2 --- E_PCbeta4 ? Positive error on PCbeta4 344-347 F4.2 --- e_PCbeta4 ? Negative error on PCbeta4 348-355 E8.2 cm-2 WTNH5 ? Intrinsic column density for the WT mode spectrum of the fifth power-law segment of the light curve 357-364 E8.2 cm-2 E_WTNH5 ? Positive error on WTNH5 366-373 E8.2 cm-2 e_WTNH5 ? Negative error on WTNH5 374-378 F5.2 --- WTbeta5 ? Spectral index for the WT mode spectrum of the fifth power-law segment of the light curve 380-383 F4.2 --- E_WTbeta5 ? Positive error on WTbeta5 385-388 F4.2 --- e_WTbeta5 ? Negative error on WTbeta5 389-396 E8.2 cm-2 PCNH5 ? Intrinsic column density for the PC mode spectrum of the fifth power-law segment of the light curve 398-405 E8.2 cm-2 E_PCNH5 ? Positive error on PCNH5 407-414 E8.2 cm-2 e_PCNH5 ? Negative error on PCNH5 415-419 F5.2 --- PCbeta5 ? Spectral index for the PC mode spectrum of the fifth power-law segment of the light curve 421-424 F4.2 --- E_PCbeta5 ? Positive error on PCbeta5 426-429 F4.2 --- e_PCbeta5 ? Negative error on PCbeta5 430-437 E8.2 cm-2 WTNH6 ? Intrinsic column density for the WT mode spectrum of the sixth power-law segment of the light curve 439-446 E8.2 cm-2 E_WTNH6 ? Positive error on WTNH6 448-455 E8.2 cm-2 e_WTNH6 ? Negative error on WTNH6 456-460 F5.2 --- WTbeta6 ? Spectral index for the WT mode spectrum of the sixth power-law segment of the light curve 462-465 F4.2 --- E_WTbeta6 ? Positive error on WTbeta6 467-470 F4.2 --- e_WTbeta6 ? Negative error on WTbeta6 471-478 E8.2 cm-2 PCNH6 ? Intrinsic column density for the PC mode spectrum of the sixth power-law segment of the light curve 480-487 E8.2 cm-2 E_PCNH6 ? Positive error on PCNH6 489-496 E8.2 cm-2 e_PCNH6 ? Negative error on PCNH6 497-501 F5.2 --- PCbeta6 ? Spectral index for the PC mode spectrum of the sixth power-law segment of the light curve 503-506 F4.2 --- E_PCbeta6 ? Positive error on PCbeta6 508-511 F4.2 --- e_PCbeta6 ? Negative error on PCbeta6 -------------------------------------------------------------------------------- Acknowledgements: Phil Evans, pae9(at)star.le.ac.uk
(End) Patricia Vannier [CDS] 23-Mar-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