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
299.7781 +35.2699 0.0127 25.0 163.7 2.0240 15.1 TRIG_01069242
------------------------------------------
Foreground time interval of the image:
0.000 28.950 (delta_t = 28.950 [sec])
30.000 64.000 (delta_t = 34.000 [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
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
143.260000 654.197400
661.000000 714.550000
781.000000 795.544000
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
143.260000 654.197400
661.000000 714.550000
781.000000 795.544000
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
143.260000 654.197400
661.000000 714.550000
781.000000 795.544000
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 606.552 sec. to 607.552 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 606.552 sec. to 607.552 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 606.552 sec. to 607.552 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) = 2.87e-07
S(50-100 keV) = 2.43e-07
T90 vs. Hardness ratio plot
T90 = 395.647999882698 sec.
Hardness ratio (energy fluence ratio) = 0.84669
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 0.987377
Count Ratio (50-100 keV) / (15-25 keV) = 0.453744
Mask shadow pattern
IMX = -4.467291355961386E-01, IMY = -1.302392414578394E-01
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:
-239.000000 -56.213200
-55.000000 28.950000
30.000000 73.100590
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.4614 35.3450 2700.0 57.8 -169.7 0.0038 0.0 0.2 Her X-1
288.7026 11.0700 9.2 48.0 141.7 1.6710 1.3 9.4 GRS 1915+105
299.7492 35.2630 0.5 25.0 163.8 9.5769 23.5 8.6 Cyg X-1
307.9207 40.8716 6.7 17.1 172.7 0.5622 1.7 9.9 Cyg X-3
326.1694 38.1708 8.9 5.3 121.5 0.4140 1.3 9.1 Cyg X-2
301.5082 17.0750 2.6 35.4 133.3 2.5983 4.4 ------ UNKNOWN
308.2509 37.6758 0.6 17.8 162.2 6.2188 18.6 ------ UNKNOWN
17.2567 42.9871 2.9 33.8 -27.8 1.6411 3.9 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
0.000000 28.950000
30.000000 64.000000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.4565 35.2112 17.4 57.9 -169.9 0.3722 0.7 7.9 Her X-1
288.6894 10.8539 9.3 48.2 141.5 -0.6617 -1.2 8.5 GRS 1915+105
299.7607 35.2668 0.8 25.0 163.8 2.0091 15.0 9.2 Cyg X-1
308.0750 40.8065 13.9 17.0 172.4 -0.0896 -0.8 8.9 Cyg X-3
326.0041 38.4741 5.4 5.2 124.7 0.2178 2.1 12.1 Cyg X-2
328.9613 3.1762 1.8 39.1 82.4 2.5195 6.3 ------ UNKNOWN
308.2733 37.6748 1.1 17.7 162.2 1.1296 10.7 ------ UNKNOWN
301.8774 51.0012 2.9 21.5 -156.4 0.4565 4.0 ------ UNKNOWN
20.8152 40.3542 2.5 37.1 -24.8 0.6917 4.6 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
128.100600 466.900640
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.3365 35.2474 4.6 36.7 -131.7 1.5325 2.5 8.2 Her X-1
268.5097 -1.4701 7.0 46.8 169.8 -1.5339 -1.6 8.6 SW J1753.5-0127
288.7808 10.7610 6.6 26.4 149.3 0.7983 1.7 11.1 GRS 1915+105
299.6278 35.2001 0.4 0.0 -174.1 11.0605 32.0 1.8 Cyg X-1
308.0170 40.9937 5.0 8.8 -9.1 0.8400 2.3 4.9 Cyg X-3
326.2971 38.5065 0.0 21.5 18.0 -0.3440 -1.0 12.6 Cyg X-2
319.8021 0.5023 2.1 39.5 91.9 6.2379 5.5 ------ UNKNOWN
308.5190 11.4630 2.7 25.1 103.8 1.9229 4.2 ------ UNKNOWN
271.6673 8.2624 2.5 37.2 174.9 2.3811 4.6 ------ UNKNOWN
308.0779 37.6390 0.8 7.2 12.5 4.8826 14.0 ------ UNKNOWN
252.8874 19.2641 3.1 44.1 -153.9 2.5671 3.7 ------ UNKNOWN
240.8720 11.4322 3.3 58.0 -154.2 7.0085 3.5 ------ UNKNOWN
Plot creation:
Thu Aug 19 15:55:47 EDT 2021