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
245.0481 -15.7602 0.0139 17.9 55.6 1.8499 13.8 TRIG_01212132
------------------------------------------
Foreground time interval of the image:
0.000 15.390 (delta_t = 15.390 [sec])
16.000 52.150 (delta_t = 36.150 [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
Time interval is from 77.032 sec. to 145.608 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 77.032 sec. to 145.608 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 77.032 sec. to 145.608 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
Peak spectrum fit
Power-law model
Time interval is from 126.512 sec. to 127.512 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 126.512 sec. to 127.512 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 126.512 sec. to 127.512 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) = 7.36e-08
S(50-100 keV) = 5.70e-09
T90 vs. Hardness ratio plot
T90 = 62.9199998378754 sec.
Hardness ratio (energy fluence ratio) = 0.0774457
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 0.129375
Count Ratio (50-100 keV) / (15-25 keV) = -0.0168677
Mask shadow pattern
IMX = 1.818553940636338E-01, IMY = -2.659371451096094E-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:
-14.499400 15.390000
16.000000 52.150000
53.000000 73.200590
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
245.0550 -15.7543 0.8 17.9 55.7 3.0572 15.1 8.1 Sco X-1
254.7071 35.4400 0.0 49.2 147.2 0.8063 1.2 13.5 Her X-1
256.0538 -37.8890 7.9 25.6 -10.3 -0.2821 -1.5 4.2 4U 1700-377
256.4568 -36.3563 4.0 24.1 -10.0 0.5443 2.9 4.1 GX 349+2
262.9771 -24.8274 5.3 11.7 -22.2 0.3751 2.2 5.2 GX 1+4
264.7739 -44.6128 8.7 31.6 -25.6 -0.2575 -1.3 9.9 4U 1735-44
268.2291 -1.4053 5.6 12.7 179.6 0.3557 2.0 8.8 SW J1753.5-0127
270.1918 -24.8906 120.3 13.5 -51.4 0.0164 0.1 12.4 GX 5-1
270.4370 -25.8386 3.7 14.4 -50.3 0.5398 3.2 9.3 GRS 1758-258
274.0959 -14.2288 0.0 10.6 -106.1 0.2661 1.6 12.7 GX 17+2
275.8947 -30.2673 12.0 20.8 -55.7 0.1808 1.0 6.2 H1820-303
284.8498 -24.9600 3.3 23.5 -80.1 -0.6957 -3.5 10.4 HT1900.1-2455
288.7068 11.0153 6.1 34.9 -156.1 0.4065 1.9 6.8 GRS 1915+105
263.1680 -33.8518 5.2 20.8 -23.3 0.3885 2.2 9.0 GX 354-0
264.5984 19.0573 2.7 32.2 158.8 1.0273 4.3 ------ UNKNOWN
296.8850 -53.2882 2.4 48.2 -49.9 3.8293 4.9 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
0.000000 15.390000
16.000000 52.150000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
245.0482 -15.7602 0.8 17.9 55.6 1.8499 13.8 8.2 Sco X-1
254.6296 35.3445 5.9 49.1 147.1 0.8879 2.0 8.4 Her X-1
255.9764 -37.9116 11.1 25.7 -10.1 -0.1381 -1.0 4.1 4U 1700-377
256.4233 -36.3531 3.1 24.1 -9.9 0.4767 3.8 4.2 GX 349+2
262.9227 -24.7537 6.6 11.7 -21.9 0.2075 1.7 4.7 GX 1+4
264.7945 -44.6156 6.5 31.6 -25.6 -0.2407 -1.8 10.2 4U 1735-44
268.2224 -1.4211 6.4 12.6 179.6 0.2080 1.8 8.9 SW J1753.5-0127
270.2487 -25.0021 7.8 13.6 -51.4 -0.1684 -1.5 5.0 GX 5-1
270.4405 -25.8306 3.7 14.4 -50.3 0.3628 3.2 9.1 GRS 1758-258
274.0959 -14.2288 0.0 10.6 -106.1 0.1784 1.5 12.7 GX 17+2
275.8413 -30.2233 8.8 20.7 -55.6 0.1635 1.3 9.7 H1820-303
285.1626 -24.9550 5.5 23.8 -80.4 0.2994 2.1 7.2 HT1900.1-2455
288.7162 10.9146 11.5 34.8 -155.9 0.1438 1.0 5.2 GRS 1915+105
263.0711 -34.0231 10.3 20.9 -23.0 0.1223 1.1 12.0 GX 354-0
229.6481 -36.8791 2.4 38.3 22.1 0.9582 4.8 ------ UNKNOWN
264.5623 19.0938 2.8 32.2 158.7 0.6640 4.2 ------ UNKNOWN
275.0149 19.6997 2.4 34.8 176.1 0.7084 4.7 ------ UNKNOWN
287.7809 8.7302 2.1 32.7 -154.1 0.7283 5.5 ------ UNKNOWN
301.1787 17.6822 2.0 48.4 -152.1 1.4563 5.8 ------ UNKNOWN
309.0811 21.6745 3.1 56.8 -150.8 2.3073 3.7 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
133.500600 243.067300
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
244.9628 -15.6408 0.6 0.1 130.1 4.2892 20.3 1.0 Sco X-1
254.4573 35.3426 864.7 51.8 177.8 -0.0078 -0.0 0.0 Her X-1
256.1693 -37.8359 8.0 24.2 -33.9 0.3126 1.4 8.7 4U 1700-377
256.4268 -36.3720 5.6 23.0 -36.1 0.4430 2.1 3.1 GX 349+2
263.1516 -24.6985 3.9 19.2 -71.3 -0.6895 -2.9 8.3 GX 1+4
264.8452 -44.5743 5.4 33.4 -38.1 0.5594 2.1 8.6 4U 1735-44
268.5197 -1.3635 7.1 27.3 -131.5 0.3769 1.6 10.6 SW J1753.5-0127
270.2499 -25.1709 3.8 25.4 -76.1 0.7393 3.1 5.8 GX 5-1
270.3951 -25.7511 3.8 25.7 -74.9 0.7663 3.2 5.0 GRS 1758-258
273.9047 -13.9694 3.6 28.0 -101.8 0.8974 3.2 7.1 GX 17+2
275.7467 -30.5078 0.0 31.7 -68.8 1.2748 3.9 12.5 H1820-303
285.0739 -24.9478 1601.6 38.5 -81.5 -0.0038 -0.0 2.6 HT1900.1-2455
262.9857 -33.7943 3.0 24.3 -50.6 0.8671 3.8 2.4 GX 354-0
273.2084 33.7933 2.1 56.3 -163.9 3.7417 5.6 ------ UNKNOWN
Plot creation:
Thu Feb 1 03:03:27 EST 2024