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
248.4678 -47.3839 0.0173 22.9 -167.0 1.4758 11.1 TRIG_01160641
------------------------------------------
Foreground time interval of the image:
0.000 64.000 (delta_t = 64.000 [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
Time interval is from -79.640 sec. to -78.104 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 -79.640 sec. to -78.104 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 -79.640 sec. to -78.104 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 -79.660 sec. to -78.660 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 -79.660 sec. to -78.660 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 -79.660 sec. to -78.660 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) = 1.69e-07
S(50-100 keV) = 7.60e-08
T90 vs. Hardness ratio plot
T90 = 1.3439998626709 sec.
Hardness ratio (energy fluence ratio) = 0.449704
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 0.535288
Count Ratio (50-100 keV) / (15-25 keV) = -0.0392621
Mask shadow pattern
IMX = -4.119780819429618E-01, IMY = 9.477355811627441E-02
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:
0.000000 64.000000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
170.1620 -60.6396 7.0 23.3 39.9 0.2369 1.6 4.6 Cen X-3
186.7812 -62.9063 7.8 15.4 45.8 0.1977 1.5 8.8 GX 301-2
244.9610 -15.6639 2.0 52.2 170.7 3.2035 5.7 1.8 Sco X-1
255.8247 -37.8484 10.3 33.9 -165.7 0.1679 1.1 7.7 4U 1700-377
256.6082 -36.3012 0.0 35.5 -165.8 -0.3270 -2.0 11.1 GX 349+2
262.8937 -24.6937 4.2 48.3 -165.0 0.8152 2.8 7.0 GX 1+4
264.7249 -44.4570 27.5 31.2 -148.9 -0.0705 -0.4 0.9 4U 1735-44
270.2820 -25.0423 100.4 50.5 -156.6 0.0370 0.1 2.2 GX 5-1
270.1771 -25.7081 4.3 49.9 -156.4 -0.8277 -2.7 7.1 GRS 1758-258
275.7761 -30.3447 16.2 47.8 -147.8 -0.2244 -0.7 7.8 H1820-303
263.1328 -33.8058 8.7 40.0 -159.5 0.2732 1.3 7.4 GX 354-0
248.4678 -47.3839 1.0 22.9 -167.0 1.4759 11.1 ------ UNKNOWN
256.5061 -20.5333 2.4 50.3 -174.1 1.6500 4.8 ------ UNKNOWN
317.0580 -84.1639 2.5 25.6 -51.2 0.7269 4.7 ------ UNKNOWN
348.6221 -83.9288 3.0 28.5 -47.9 0.6651 3.9 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
508.600590 963.143400
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
170.1486 -60.5250 5.7 44.9 27.3 -2.1297 -2.0 7.7 Cen X-3
186.6677 -62.7152 4.8 36.8 26.7 2.8229 2.4 3.3 GX 301-2
244.9648 -15.6417 0.8 31.9 157.8 15.2183 15.1 0.9 Sco X-1
255.9651 -37.8602 0.9 11.0 -163.1 9.3995 12.7 1.4 4U 1700-377
256.5082 -36.2817 7.8 12.6 -164.6 1.2021 1.5 9.2 GX 349+2
263.0860 -24.6379 5.3 25.5 -163.6 1.8437 2.2 7.7 GX 1+4
264.9640 -44.3143 0.0 11.9 -114.6 0.5684 0.7 12.5 4U 1735-44
268.2689 -1.4428 129.5 49.0 -169.1 0.1620 0.1 6.0 SW J1753.5-0127
270.2006 -25.1268 4.9 28.1 -150.4 2.0172 2.4 5.4 GX 5-1
270.2810 -25.7454 3.1 27.6 -149.6 3.1656 3.8 1.2 GRS 1758-258
273.9056 -13.9596 32.3 39.5 -154.9 0.4853 0.4 7.4 GX 17+2
275.9643 -30.2258 13.0 27.2 -135.0 0.8292 0.9 8.7 H1820-303
285.1304 -24.8793 4.7 36.6 -130.6 -3.2728 -2.5 5.7 HT1900.1-2455
263.0580 -33.7103 4.7 17.5 -151.7 -1.8204 -2.4 8.2 GX 354-0
225.6558 -33.6236 2.6 22.0 104.7 4.2359 4.4 ------ UNKNOWN
248.4980 -47.4205 1.1 0.0 -24.6 8.8689 10.9 ------ UNKNOWN
59.9386 -79.7612 2.9 52.8 -17.6 8.9967 4.0 ------ UNKNOWN
287.0275 -21.3385 2.6 40.4 -132.2 6.5731 4.5 ------ UNKNOWN
294.3972 -24.2153 3.1 43.0 -121.8 9.3080 3.7 ------ UNKNOWN
349.5639 -69.1177 3.8 50.1 -42.8 13.4948 3.0 ------ UNKNOWN
309.3535 -45.4884 3.1 40.9 -85.0 12.1881 3.8 ------ UNKNOWN
Plot creation:
Tue Mar 21 07:09:07 EDT 2023