========================================================================== BAT GROUND-DETECTED GRB DATA PROCESSING REPORT Process Script Ver: batgrbproduct v2.46 Process Start Time: Thu Dec 17 16:33:35 EST 2015 Host Name: bat1 Current Working Dir: /local/data/bat1/alien/Swift_3rdBATcatalog/event/batevent_reproc/trigger531259 ====================================================================== Trigger: 00531259 Segment: 000 BAT Trigger Time: 366868959.252 UTC: 2012-08-17T04:02:29.706 [includes UTCF correction] Where From?: Ground analysis (best_duration.txt) NOTE: BAT trigger time for ground-detected burst is the T100 start time. Analysis Position: [ source = GCN ] RA: 8.310 Dec: -26.428 [deg; J2000] Refined Position: [ source = BAT pre-slew image ] RA: 8.31 Dec: -26.428 [deg; J2000] { 00h 33m 14.4s , -26d -25' -40.8" } +/- 2.43406974085 [arcmin] (estimated 90% radius based on SNR) SNR: 8.53632393016 Angular difference between the analysis and refined position is 0.000000 arcmin Partial Coding Fraction: 0.05175781 [ including projection effects ] Duration (found by FRED-model fit) T90: 0.072 +/- N/A Measured from: 0.00800002 to: 0.08 [s; relative to TRIGTIME] T50: 0.024 +/- N/A Measured from: 0.024 to: 0.048 ====== Table of the duration information ============================= Value tstart tstop T100 0.108 0.000 0.108 T90 0.072 0.008 0.080 T50 0.024 0.024 0.048 Peak 1.000 -0.462 0.538 ====== Spectral Analysis Summary ===================================== Model : spectral model: simple power-law (PL) and cutoff power-law (CPL) Ph_index : photon index: E^{Ph_index} Ph_90err : 90% error of the photon index Epeak : Epeak in keV Epeak_90err: 90% error of Epeak Norm : normalization at 50 keV in both the PL model and CPL model Nomr_90err : 90% error of the normalization chi2 : Chi-Squared dof : degree of freedo === Time-averaged spectral analysis === (Best model with acceptable fit: N/A) Model Ph_index Ph_90err_low Ph_90err_hi Epeak Epeak_90err_low Epeak_90err_hi Norm Nomr_90err_low Norm_90err_hi chi2 dof PL N/A N/A N/A - - - N/A N/A N/A N/A N/A CPL N/A N/A N/A N/A N/A N/A N/A N/A N/A N/A N/A === 1-s peak spectral analysis === (Best model with acceptable fit: N/A) Model Ph_index Ph_90err_low Ph_90err_hi Epeak Epeak_90err_low Epeak_90err_hi Norm Nomr_90err_low Norm_90err_hi chi2 dof PL N/A N/A N/A - - - N/A N/A N/A N/A N/A CPL N/A N/A N/A N/A N/A N/A N/A N/A N/A N/A N/A === Fluence/Peak Flux Summary === Model Band1 Band2 Band3 Band4 Band5 Total 15-25 25-50 50-100 100-350 15-150 15-350 keV Fluence PL N/A N/A N/A N/A N/A N/A erg/cm2
#RAcent DECcent POSerr Theta Phi Peak_Cts SNR Name 8.310 -26.428 0.000 46.005 126.693 0.349 8.536 TRIG_00531259 Image time interval: 0.000 to 0.108 [sec]
Note: The mask-weighted lightcurves have units of either count/det or counts/sec/det, where a det is 0.4 x 0.4 = 0.16 sq cm.
Multiple GTIs in the spectrum tstart tstop Photon index: ( )
Multiple GTIs in the spectrum tstart tstop Photon index: ( )
Time interval is from -0.252 sec. to 2.818 sec. Photon index: ( )
Time interval is from -0.252 sec. to 2.818 sec. Photon index: ( )
T90 = N/A sec. Hardness ratio (energy fluence ratio) = N/A
S(15-50 keV) = N/A S(50-150 keV) = N/A
The dash-dotted line and the dashed line traces the fluences calculated from the Band function with Epeak = 15 and 150 keV, respectively. Both lines assume a canonical values of alpha = -1 and beta = -2.5.
IMX = -0.61887045537, IMY = -0.83050126764
Time interval of the image: -0.252000 2.818000 # RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name # [deg] [deg] ['] [deg] [deg] ['] 170.2118 -60.7761 0.0 45.9 -62.4 -0.0512 -0.6 9.7 Cen X-3 186.8174 -62.7614 7.2 44.8 -51.2 0.0679 1.6 4.4 GX 301-2 264.7748 -44.6053 5.6 53.2 10.6 0.1251 2.1 9.4 4U 1735-44 10.2764 -41.9410 2.4 30.4 128.4 0.1101 4.8 ------ UNKNOWN 55.5938 -33.9169 2.1 44.1 -173.7 0.1486 5.4 ------ UNKNOWN
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