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
299.2408 +35.4118 0.0285 43.2 -161.5 0.8278 6.7 TRIG_01218903
------------------------------------------
Foreground time interval of the image:
0.000 21.140 (delta_t = 21.140 [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
75.324000 77.500000
79.000000 86.112000
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
75.324000 77.500000
79.000000 86.112000
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
75.324000 77.500000
79.000000 86.112000
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 81.660 sec. to 82.660 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 81.660 sec. to 82.660 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 81.660 sec. to 82.660 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) = 1.28e-07
S(50-100 keV) = 1.83e-07
T90 vs. Hardness ratio plot
T90 = 6.65599989891052 sec.
Hardness ratio (energy fluence ratio) = 1.42969
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 2.84349
Count Ratio (50-100 keV) / (15-25 keV) = 0.818897
Mask shadow pattern
IMX = -8.894240067425627E-01, IMY = 2.969458613156292E-01
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:
-15.999400 21.140000
22.000000 72.300600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
244.8709 -15.6545 0.8 34.6 58.0 5.6305 13.8 6.3 Sco X-1
254.3280 35.2644 5.9 43.6 144.5 1.1395 2.0 7.9 Her X-1
255.9241 -37.7956 63.0 40.3 18.7 0.0587 0.2 4.2 4U 1700-377
256.4161 -36.5399 4.7 39.1 19.3 -0.8148 -2.5 7.1 GX 349+2
262.8874 -24.5672 0.0 26.1 23.4 0.0424 0.2 12.6 GX 1+4
264.8850 -44.5014 8.5 43.3 5.2 0.4287 1.4 6.8 4U 1735-44
268.2405 -1.2848 0.0 9.3 90.2 0.2571 1.4 12.6 SW J1753.5-0127
270.2737 -24.9253 14.3 23.4 8.7 -0.1606 -0.8 9.2 GX 5-1
270.3222 -25.6291 3.6 24.0 8.0 0.6310 3.2 6.9 GRS 1758-258
273.8781 -13.8662 0.0 11.8 9.2 0.5211 2.9 12.6 GX 17+2
275.9248 -30.3720 55.6 27.8 -5.1 -0.0432 -0.2 0.3 H1820-303
285.1498 -24.7800 1897.4 23.4 -25.8 0.0011 0.0 10.5 HT1900.1-2455
288.6583 10.9911 2.0 17.6 -148.6 -1.0448 -5.7 8.7 GRS 1915+105
299.4693 35.3170 6.5 43.2 -161.2 0.5709 1.8 9.1 Cyg X-1
308.1084 41.0199 4.5 51.8 -158.5 1.3285 2.5 4.0 Cyg X-3
263.0016 -33.8182 4.2 34.0 13.9 0.7451 2.8 1.2 GX 354-0
270.6553 51.0555 2.3 54.0 166.9 3.9474 5.0 ------ UNKNOWN
257.8122 -42.3859 2.7 43.5 13.3 1.5205 4.3 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
0.000000 21.140000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
244.8809 -15.6584 1.5 34.6 58.0 1.3287 7.9 5.8 Sco X-1
254.5147 35.2097 6.8 43.5 144.6 -0.3545 -1.7 8.4 Her X-1
256.0951 -38.0313 0.0 40.4 18.4 -0.0679 -0.6 12.3 4U 1700-377
256.3894 -36.5248 4.8 39.1 19.4 -0.3007 -2.4 6.5 GX 349+2
262.8673 -24.7590 15.9 26.2 23.2 0.0616 0.7 7.8 GX 1+4
264.8503 -44.6248 0.0 43.5 5.2 0.2542 2.0 11.5 4U 1735-44
268.4728 -1.6173 4.7 9.0 88.3 -0.1841 -2.4 11.7 SW J1753.5-0127
270.1598 -24.9065 0.0 23.4 8.9 -0.1037 -1.2 12.4 GX 5-1
270.2627 -25.5906 2.4 24.0 8.2 0.3863 4.8 9.4 GRS 1758-258
273.9238 -13.8729 14.5 11.8 9.0 0.0592 0.8 10.9 GX 17+2
275.7705 -30.4178 843.0 27.9 -4.8 0.0011 0.0 8.6 H1820-303
285.1676 -25.0771 0.0 23.7 -25.6 -0.1052 -1.2 11.8 HT1900.1-2455
288.6380 10.8598 7.4 17.5 -148.3 -0.1148 -1.6 10.8 GRS 1915+105
299.4577 35.2520 23.1 43.1 -161.2 0.0609 0.5 7.2 Cyg X-1
308.1623 40.9384 16.6 51.8 -158.4 0.1998 0.7 2.5 Cyg X-3
262.9831 -33.7863 5.9 34.0 13.9 0.2001 2.0 2.9 GX 354-0
250.6412 42.3641 2.8 51.1 146.8 1.5785 4.2 ------ UNKNOWN
270.6903 37.2360 2.3 40.3 163.9 0.6629 5.0 ------ UNKNOWN
282.5395 -2.3931 2.7 5.1 -100.1 0.3018 4.3 ------ UNKNOWN
310.5224 -45.0276 2.1 51.4 -37.4 1.5367 5.5 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
162.200600 243.050000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.4452 35.2181 5.6 36.2 71.0 -0.9431 -2.1 7.5 Her X-1
268.3701 -1.3293 28.6 46.7 12.7 -0.1304 -0.4 7.4 SW J1753.5-0127
274.0413 -13.9416 6.1 54.8 -1.7 1.0344 1.9 6.0 GX 17+2
288.9033 10.9636 6.6 26.2 -8.6 -0.3032 -1.7 6.3 GRS 1915+105
299.4777 35.3370 1.0 0.2 -101.1 1.7580 11.4 9.8 Cyg X-1
307.8662 40.9556 5.9 8.8 -163.9 -0.3054 -2.0 11.1 Cyg X-3
326.1804 38.3729 5.0 21.7 -137.9 0.4053 2.3 3.1 Cyg X-2
275.1097 -5.5848 3.2 46.9 1.8 1.1401 3.7 ------ UNKNOWN
299.3893 -19.7669 1.9 55.2 -32.3 5.8295 6.2 ------ UNKNOWN
339.3831 15.3626 2.9 41.0 -103.3 3.0457 4.0 ------ UNKNOWN
Plot creation:
Wed Mar 6 21:19:38 EST 2024