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
299.8254 +35.0696 0.0090 0.0 -147.6 4.7172 21.5 TRIG_01197507
------------------------------------------
Foreground time interval of the image:
-13.000 -1.120 (delta_t = 11.880 [sec])
-1.000 59.140 (delta_t = 60.140 [sec])
61.000 61.928 (delta_t = 0.928 [sec])
64.000 70.200 (delta_t = 6.200 [sec])
72.000 75.900 (delta_t = 3.900 [sec])
78.000 80.470 (delta_t = 2.470 [sec])
83.000 86.400 (delta_t = 3.400 [sec])
88.000 91.090 (delta_t = 3.090 [sec])
94.000 96.810 (delta_t = 2.810 [sec])
98.000 98.310 (delta_t = 0.310 [sec])
99.000 100.036 (delta_t = 1.036 [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
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 64.000000
8 ms binning
From T100_start-3 s to T100_start+3 s
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 64.000000
2 ms binning
From T100_start-1 s to T100_start+1 s
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 64.000000
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
-89.752000 -61.770000
-61.000000 -60.400000
-60.000000 -59.424000
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
-89.752000 -61.770000
-61.000000 -60.400000
-60.000000 -59.424000
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
-89.752000 -61.770000
-61.000000 -60.400000
-60.000000 -59.424000
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 -85.168 sec. to -84.168 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 -85.168 sec. to -84.168 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 -85.168 sec. to -84.168 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) = 1.02e-06
S(50-100 keV) = 1.07e-06
T90 vs. Hardness ratio plot
T90 = 28.0119999647141 sec.
Hardness ratio (energy fluence ratio) = 1.04902
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.39792
Count Ratio (50-100 keV) / (15-25 keV) = 0.655311
Mask shadow pattern
IMX = -6.035991141621187E-04, IMY = 3.836754845310265E-04
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 64.000000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 64.000000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 64.000000
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:
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-13.000000 -1.120000
-1.000000 59.140000
61.000000 61.928300
64.000000 70.200000
72.000000 75.900000
78.000000 80.470000
83.000000 86.400000
88.000000 91.090000
94.000000 96.810000
98.000000 98.310000
99.000000 100.036000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.3975 35.5542 0.0 36.7 -44.8 0.3569 0.9 13.0 Her X-1
288.7837 10.9507 193.3 26.2 -123.9 0.0160 0.1 0.9 GRS 1915+105
299.7874 35.1234 0.6 0.0 -37.3 4.4796 20.2 10.7 Cyg X-1
308.3621 40.8793 3.3 8.9 77.7 0.7323 3.5 12.2 Cyg X-3
325.9597 38.4201 36.2 21.1 104.2 0.0910 0.3 11.6 Cyg X-2
322.1747 62.4023 3.3 30.7 51.1 1.2217 3.5 ------ UNKNOWN
259.3058 74.8671 2.9 44.1 16.8 1.5972 4.0 ------ UNKNOWN
277.7202 50.7090 2.5 22.3 -8.0 1.0370 4.6 ------ UNKNOWN
302.2121 -11.2555 2.5 46.4 -152.3 2.5156 4.5 ------ UNKNOWN
308.9327 -24.2729 2.4 60.0 -158.7 9.5196 4.9 ------ UNKNOWN
296.4616 -19.9479 2.5 55.2 -145.3 7.2077 4.6 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
-119.000000 -106.830000
-104.999600 -96.128100
-95.000000 -86.791900
-84.000000 -79.890000
-78.000000 -75.350000
-71.000000 -62.980000
-61.000000 -60.400000
-60.000000 -43.630000
-40.000000 -37.037500
-36.000000 -32.660000
-31.000000 -16.466100
-13.000000 -6.030000
-6.000000 -1.120000
-1.000000 3.057600
7.000000 7.810000
10.000000 12.780000
15.000000 33.084700
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.4671 35.3923 36.7 26.0 -49.7 -0.0957 -0.3 3.0 Her X-1
289.0168 10.9383 0.0 31.3 -139.4 -0.5792 -1.6 12.9 GRS 1915+105
299.6682 35.0622 9.4 12.2 165.8 0.3067 1.2 9.2 Cyg X-1
307.8684 40.9765 10.8 15.6 131.7 0.2563 1.1 11.1 Cyg X-3
326.2991 38.3793 4.2 30.0 128.3 -0.9835 -2.7 6.9 Cyg X-2
286.9669 42.0817 1.6 0.1 -139.3 1.6950 7.4 ------ UNKNOWN
231.1481 28.8629 2.1 46.5 -43.3 3.4990 5.4 ------ UNKNOWN
Plot creation:
Tue Nov 21 03:59:08 EST 2023