Estimated redshift from machine learning (Ukwatta et al. 2016) - may take a few minutes to calcaulte
Image
Pre-slew 15-350 keV image (Event data; bkg subtracted)
# RAcent DECcent POSerr Theta Phi Peak Cts SNR Name
300.3678 +35.1427 0.0125 0.2 -95.2 3.0679 15.4 TRIG_01205110
------------------------------------------
Foreground time interval of the image:
0.000 128.000 (delta_t = 128.000 [sec])
Background time interval of the image:
Lightcurves
Notes:
- 1) All plots contain as much data as has been downloaded to date.
- 2) The mask-weighted light curves are using the flight position.
- 3) Multiple plots of different time binning/intervals are shown to cover all scenarios of short/long GRBs, rate/image triggers, and real/false positives.
- 4) For all the mask-weighted lightcurves, the y-axis units are counts/sec/det where a det is 0.4 x 0.4 = 0.16 sq cm.
- 5) The verticle lines correspond to following: green dotted lines are T50 interval, black dotted lines are T90 interval, blue solid line(s) is a spacecraft slew start time, and orange solid line(s) is a spacecraft slew end time.
- 6) Time of each bin is in the middle of the bin.
1 s binning
From T0-310 s to T0+310 s
From T100_start - 20 s to T100_end + 30 s
Full time interval
64 ms binning
Full time interval
From T100_start to T100_end
From T0-5 sec to T0+5 sec
16 ms binning
From T100_start-5 s to T100_start+5 s
8 ms binning
From T100_start-3 s to T100_start+3 s
2 ms binning
From T100_start-1 s to T100_start+1 s
SN=5 or 10 sec. binning (whichever binning is satisfied first)
SN=5 or 10 sec. binning (T < 200 sec)
Spectra
Notes:
- 1) The fitting includes the systematic errors.
- 2) For long bursts, a spectral fit of the pre-slew DRM will introduce some errors in both a spectral shape and a normalization if the PHA file contains a lot of the slew/post-slew time interval.
- 3) For fits to more complicated models (e.g. a power-law over a cutoff power-law), the BAT team has decided to require a chi-square improvement of more than 6 for each extra dof.
- 4) For short bursts (T90<1sec), the specrtum is also fit with Blackbody, OTTB, and Double Blackbody.
Time averaged spectrum fit using the pre-slew DRM
Power-law model
Multiple GTIs in the spectrum
tstart tstop
352.028000 391.300000
392.000000 432.000000
434.000000 462.420000
464.000000 588.908000
Usage: bat_spec_fit_sys_xspec12.sh (pha file) (response file) (script folder) (folder of taka's xspec lmodel)
This script tries to add the systematic column to the PHA
file before doing the fitting
script folder: /local/data/BATtools/battools/bin/GRB_spec_fit_v2
folder of taka's xspec lmodel: /local/data/bat1/prebascript/xspec_taka_lmodel
Cutoff power-law model
Multiple GTIs in the spectrum
tstart tstop
352.028000 391.300000
392.000000 432.000000
434.000000 462.420000
464.000000 588.908000
Usage: bat_spec_fit_cutoff_sys_xspec12.sh (pha file) (response file) (script folder) (folder of taka's xspec lmodel)
This script tries to add the systematic column to the PHA
file before doing the fitting
script folder: /local/data/bat2/BATtools/battools/bin/GRB_spec_fit_v2
folder of taka's xspec lmodel: /local/data/bat1/prebascript/xspec_taka_lmodel
Band function
Multiple GTIs in the spectrum
tstart tstop
352.028000 391.300000
392.000000 432.000000
434.000000 462.420000
464.000000 588.908000
Usage: bat_spec_fit_band_sys.sh (pha file) (response file) (script folder) (folder of taka's xspec lmodel)
This script tries to add the systematic column to the PHA
file before doing the fitting
script folder: /local/data/bat2/BATtools/battools/bin/GRB_spec_fit_v2
folder of taka's xspec lmodel: /local/data/bat1/prebascript/xspec_taka_lmodel
Single BB
Usage: bat_spec_fit_bb_sys.sh (pha file) (response file)
This script tries to add the systematic column to the PHA
file before doing the fitting
Thermal bremsstrahlung (OTTB)
Usage: bat_spec_fit_brems_sys.sh (pha file) (response file)
This script tries to add the systematic column to the PHA
file before doing the fitting
Double BB
Usage: bat_spec_fit_2bb_sys.sh (pha file) (response file)
This script tries to add the systematic column to the PHA
file before doing the fitting
Peak spectrum fit
Power-law model
Time interval is from 587.680 sec. to 588.680 sec.
Usage: bat_spec_fit_sys_xspec12.sh (pha file) (response file) (script folder) (folder of taka's xspec lmodel)
This script tries to add the systematic column to the PHA
file before doing the fitting
script folder: /local/data/BATtools/battools/bin/GRB_spec_fit_v2
folder of taka's xspec lmodel: /local/data/bat1/prebascript/xspec_taka_lmodel
Cutoff power-law model
Time interval is from 587.680 sec. to 588.680 sec.
Usage: bat_spec_fit_cutoff_sys_xspec12.sh (pha file) (response file) (script folder) (folder of taka's xspec lmodel)
This script tries to add the systematic column to the PHA
file before doing the fitting
script folder: /local/data/bat2/BATtools/battools/bin/GRB_spec_fit_v2
folder of taka's xspec lmodel: /local/data/bat1/prebascript/xspec_taka_lmodel
Band function
Time interval is from 587.680 sec. to 588.680 sec.
Usage: bat_spec_fit_band_sys.sh (pha file) (response file) (script folder) (folder of taka's xspec lmodel)
This script tries to add the systematic column to the PHA
file before doing the fitting
script folder: /local/data/bat2/BATtools/battools/bin/GRB_spec_fit_v2
folder of taka's xspec lmodel: /local/data/bat1/prebascript/xspec_taka_lmodel
Single BB
Usage: bat_spec_fit_bb_sys.sh (pha file) (response file)
This script tries to add the systematic column to the PHA
file before doing the fitting
Thermal bremsstrahlung (OTTB)
Usage: bat_spec_fit_brems_sys.sh (pha file) (response file)
This script tries to add the systematic column to the PHA
file before doing the fitting
Double BB
Usage: bat_spec_fit_2bb_sys.sh (pha file) (response file)
This script tries to add the systematic column to the PHA
file before doing the fitting
Pre-slew spectrum (Pre-slew PHA with pre-slew DRM)
Power-law model
Cutoff power-law model
Band function
S(25-50 keV) vs. S(50-100 keV) plot
S(25-50 keV) = 4.50e-07
S(50-100 keV) = 3.57e-07
T90 vs. Hardness ratio plot
T90 = 211.019999980927 sec.
Hardness ratio (energy fluence ratio) = 0.793333
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 0.907324
Count Ratio (50-100 keV) / (15-25 keV) = 0.37229
Mask shadow pattern
IMX = -3.315584289980598E-04, IMY = 3.626473530940569E-03
TIME vs. PHA plot around the trigger time
TIME vs. DetID plot around the trigger time
100 us light curve (15-350 keV)
Spacecraft aspect plot
Bright source in the pre-burst/pre-slew/post-slew images
Pre-burst image of 15-350 keV band
Time interval of the image:
-239.000000 -56.680000
-56.000000 135.800600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.3865 35.4622 14.6 37.2 -10.2 0.5900 0.8 8.0 Her X-1
288.8730 11.0503 49.7 26.5 -88.0 0.1520 0.2 7.7 GRS 1915+105
299.8104 35.2576 29.2 0.5 -32.9 0.2111 0.4 11.3 Cyg X-1
308.0039 41.1153 18.0 8.3 109.3 -0.3477 -0.6 10.9 Cyg X-3
325.9412 38.3271 5.2 20.6 139.9 1.2710 2.2 10.9 Cyg X-2
332.0283 22.4858 2.4 30.3 172.3 2.8230 4.8 ------ UNKNOWN
300.4046 35.1517 0.7 0.2 -102.9 8.8198 17.3 ------ UNKNOWN
243.4640 40.1199 2.2 44.6 -0.3 4.9549 5.1 ------ UNKNOWN
329.7939 9.1726 2.0 37.4 -167.0 3.7973 5.7 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
0.000000 128.000000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.5042 35.2223 12.0 37.2 -10.6 -0.2695 -1.0 7.6 Her X-1
288.6195 10.8491 0.0 26.7 -87.6 -0.1469 -0.6 12.0 GRS 1915+105
299.7745 35.1714 11.4 0.6 -41.0 0.2059 1.0 9.2 Cyg X-1
308.1042 40.9519 92.0 8.2 110.5 -0.0257 -0.1 0.3 Cyg X-3
326.0207 38.2712 5.6 20.6 140.0 0.4680 2.0 7.7 Cyg X-2
316.0393 66.2294 2.6 32.2 77.5 1.8325 4.5 ------ UNKNOWN
332.0388 22.4828 2.7 30.3 172.3 1.0097 4.3 ------ UNKNOWN
300.3968 35.1364 0.8 0.2 -102.0 3.0836 15.5 ------ UNKNOWN
267.5971 41.1294 3.0 26.3 -1.6 0.8279 3.9 ------ UNKNOWN
329.1174 9.0248 2.1 37.1 -166.0 1.3815 5.5 ------ UNKNOWN
277.9164 18.8075 2.0 25.9 -58.0 1.2366 5.7 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
141.200640 391.300000
392.000000 432.000000
434.000000 462.420000
464.000000 510.800600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.4258 35.4627 8.2 37.1 -9.9 1.0223 1.4 7.4 Her X-1
288.6497 10.9352 12.7 26.4 -87.6 -0.5626 -0.9 8.8 GRS 1915+105
299.5881 35.3662 7.3 0.6 -3.4 -0.8065 -1.6 9.9 Cyg X-1
308.1047 40.9495 2490.2 8.4 110.0 -0.0020 -0.0 0.3 Cyg X-3
326.0055 38.2488 756.1 20.8 139.7 -0.0083 -0.0 9.0 Cyg X-2
315.4745 66.0648 3.1 32.2 77.4 3.7793 3.6 ------ UNKNOWN
243.5265 47.6188 3.3 43.4 10.7 3.1855 3.5 ------ UNKNOWN
240.8868 43.1402 2.1 45.8 4.7 4.8756 5.5 ------ UNKNOWN
329.6726 9.0646 1.8 37.4 -167.0 4.1684 6.5 ------ UNKNOWN
313.4124 3.5761 2.5 33.8 -138.1 3.0070 4.7 ------ UNKNOWN
268.3417 2.9532 3.0 43.8 -64.2 8.0831 3.9 ------ UNKNOWN
311.6189 -11.6815 2.3 48.0 -129.1 11.8133 5.1 ------ UNKNOWN
Plot creation:
Fri Dec 29 10:11:15 EST 2023