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
232.9430 +0.7888 0.0319 24.1 -50.3 1.0056 6.1 TRIG_01347265
------------------------------------------
Foreground time interval of the image:
-15.104 34.996 (delta_t = 50.100 [sec])
35.896 59.197 (delta_t = 23.301 [sec])
Background time interval of the image:
-87.603 -42.284 (delta_t = 45.319 [sec])
-41.104 -15.104 (delta_t = 26.000 [sec])
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 5.504000
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 5.504000
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 5.504000
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
-15.104000 34.996000
35.896000 64.896000
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.65804 ( -0.671213 0.704645 )
Norm@50keV : 5.59864E-04 ( -0.000183461 0.0001651 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 49.48 using 59 PHA bins.
# Reduced chi-squared = 0.8681 for 57 degrees of freedom
# Null hypothesis probability = 7.500963e-01
Photon flux (15-150 keV) in 79.1 sec: 7.33045E-02 ( -0.0217027 0.0217908 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.11463e-07 ( -1.3362e-07 1.37618e-07 ) ergs/cm2
Cutoff power-law model
Multiple GTIs in the spectrum
tstart tstop
-15.104000 34.996000
35.896000 64.896000
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.24416 ( -1.10038 1.11676 )
Epeak [keV] : 90.5977 ( )
Norm@50keV : 2.79052E-04 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 48.05 using 59 PHA bins.
# Reduced chi-squared = 0.8581 for 56 degrees of freedom
# Null hypothesis probability = 7.661073e-01
Photon flux (15-150 keV) in 79.1 sec: 7.41974E-02 ( -0.0223797 0.0210419 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.04989e-07 ( -1.26463e-07 1.44647e-07 ) ergs/cm2
Band function
Multiple GTIs in the spectrum
tstart tstop
-15.104000 34.996000
35.896000 64.896000
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.33676 ( 1.33706 1.33706 )
beta : -1.65698 ( 1.65845 0.671167 )
Epeak [keV] : 21.7789 ( -21.7943 -21.7943 )
Norm@50keV : 1.26814E-03 ( -0.00127202 266.589 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 49.48 using 59 PHA bins.
# Reduced chi-squared = 0.8996 for 55 degrees of freedom
# Null hypothesis probability = 6.847166e-01
Photon flux (15-150 keV) in 79.1 sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 0 ( 0 0 ) ergs/cm2
Single BB
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 17.8044 (-10.6741 23.9778)
R^2/D10^2 : 3.89502E-03 (-0.00364907 0.0970812)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 58.45 using 59 PHA bins.
# Reduced chi-squared = 1.025 for 57 degrees of freedom
# Null hypothesis probability = 4.218945e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.962e-08 1.301e-08
25- 50 9.000e-08 5.790e-08
50-150 2.065e-07 1.358e-07
15-150 3.161e-07 1.949e-07
Thermal bremsstrahlung (OTTB)
XSPEC12>exit
XSPEC: quit
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.344 (-199.354 -199.354)
Norm : 0.287395 (-0.081513 0.137044)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.661e-08 3.501e-08
25- 50 1.089e-07 6.601e-08
50-150 2.388e-07 1.416e-07
15-150 4.043e-07 2.401e-07
Double BB
XSPEC12>exit
XSPEC: quit
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 4.43858 (-2.06046 3.90681)
R1^2/D10^2 : 0.743047 (-0.687935 23.0737)
kT2 [keV] : 41.4875 (-22.2905 -41.6053)
R2^2/D10^2 : 2.70775E-04 (-0.000262872 0.00238255)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 9.119e-08 5.335e-08
25- 50 7.358e-08 3.799e-08
50-150 3.200e-07 1.921e-07
15-150 4.847e-07 2.429e-07
Peak spectrum fit
Power-law model
Time interval is from 8.396 sec. to 9.396 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.654321 ( -1.1356 1.05345 )
Norm@50keV : 2.38026E-03 ( -0.00238026 0.00153388 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 50.16 using 59 PHA bins.
# Reduced chi-squared = 0.8801 for 57 degrees of freedom
# Null hypothesis probability = 7.273128e-01
Photon flux (15-150 keV) in 1 sec: 0.276252 ( -0.15884 0.176245 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.96685e-08 ( -1.55979e-08 1.56768e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 8.396 sec. to 9.396 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -0.988718 ( -0.234502 -0.234502 )
Epeak [keV] : 127.092 ( -276.504 -276.504 )
Norm@50keV : 8.47782E-03 ( -0.00834771 40.7194 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 50.02 using 59 PHA bins.
# Reduced chi-squared = 0.8933 for 56 degrees of freedom
# Null hypothesis probability = 6.993592e-01
Photon flux (15-150 keV) in 1 sec: 0.251054 ( -0.156044 0.195919 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.8298e-08 ( -2.8298e-08 1.66266e-08 ) ergs/cm2
Band function
Time interval is from 8.396 sec. to 9.396 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -10.00000 ( 10 10 )
beta : -0.654319 ( -1.05344 1.53441 )
Epeak [keV] : 15.6671 ( -15.6671 -15.6671 )
Norm@50keV : 0.323511 ( -0.323511 0.208486 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 50.16 using 59 PHA bins.
# Reduced chi-squared = 0.9121 for 55 degrees of freedom
# Null hypothesis probability = 6.595715e-01
Photon flux (15-150 keV) in 1 sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 0 ( 0 0 ) ergs/cm2
Single BB
XSPEC: quit
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 29.5050 (-14.1573 -29.505)
R^2/D10^2 : 4.49294E-03 (-0.00449294 0.0295978)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.182e-10 4.042e-10
25- 50 3.787e-09 2.460e-09
50-150 2.344e-08 1.520e-08
15-150 2.784e-08 1.851e-08
Thermal bremsstrahlung (OTTB)
XSPEC12>exit
XSPEC: quit
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.356 (-199.36 -199.36)
Norm : 1.23632 (-0.732168 0.732047)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.378e-09 1.800e-09
25- 50 4.575e-09 3.417e-09
50-150 1.003e-08 7.340e-09
15-150 1.699e-08 1.161e-08
Double BB
XSPEC12>exit
XSPEC: quit
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 1.83648 (-1.83083 190.969)
R1^2/D10^2 : 379.843 (-385.336 1.27166e+07)
kT2 [keV] : 30.9607 (-15.0641 -30.9588)
R2^2/D10^2 : 3.85291E-03 (-0.00378505 0.0191321)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.169e-09 4.324e-10
25- 50 3.568e-09 2.293e-09
50-150 2.366e-08 1.609e-08
15-150 2.940e-08 1.790e-08
Pre-slew spectrum (Pre-slew PHA with pre-slew DRM)
Power-law model
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.66590 ( -0.62194 0.66604 )
Norm@50keV : 6.12520E-04 ( -0.000189778 0.000171721 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 57.28 using 59 PHA bins.
# Reduced chi-squared = 1.005 for 57 degrees of freedom
# Null hypothesis probability = 4.646970e-01
Photon flux (15-150 keV) in 73.4 sec: 8.04117E-02 ( -0.0225455 0.0226536 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.17442e-07 ( -1.28722e-07 1.32022e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.71207 ( )
Epeak [keV] : 9999.33 ( )
Norm@50keV : 6.07258E-04 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 57.30 using 59 PHA bins.
# Reduced chi-squared = 1.023 for 56 degrees of freedom
# Null hypothesis probability = 4.266762e-01
Photon flux (15-150 keV) in 73.4 sec: 8.11073E-02 ( -0.0229745 0.0220197 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.12013e-07 ( -1.22974e-07 1.37883e-07 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.33132 ( 1.3323 1.3323 )
beta : -1.66589 ( 1.66635 0.621974 )
Epeak [keV] : 23.6837 ( -23.2616 -23.2616 )
Norm@50keV : 1.38549E-03 ( -0.00138867 0.0296566 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 57.28 using 59 PHA bins.
# Reduced chi-squared = 1.041 for 55 degrees of freedom
# Null hypothesis probability = 3.905753e-01
Photon flux (15-150 keV) in 73.4 sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 0 ( 0 0 ) ergs/cm2
S(25-50 keV) vs. S(50-100 keV) plot
S(25-50 keV) = 1.09e-07
S(50-100 keV) = 1.39e-07
T90 vs. Hardness ratio plot
T90 = 48 sec.
Hardness ratio (energy fluence ratio) = 1.27523
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 0.628261
Count Ratio (50-100 keV) / (15-25 keV) = 0.538268
Mask shadow pattern
IMX = 2.852948919588382E-01, IMY = 3.434709698992672E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 5.504000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 5.504000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 5.504000
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:
-87.603410 -42.284000
-41.104000 -15.104000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
245.0027 -15.6463 0.4 5.7 -94.0 4.9201 29.8 1.4 Sco X-1
254.3407 35.2138 5.1 50.7 2.5 -0.9032 -2.3 9.6 Her X-1
256.1431 -37.7751 154.0 22.8 168.3 -0.0127 -0.1 8.5 4U 1700-377
256.4550 -36.4390 5.0 21.6 166.8 0.3806 2.3 1.3 GX 349+2
262.8707 -24.6068 25.3 14.5 130.1 -0.0745 -0.5 11.2 GX 1+4
264.5523 -44.3348 19.1 31.1 159.9 -0.1268 -0.6 10.7 4U 1735-44
268.2309 -1.5945 0.0 22.0 51.6 0.3320 1.7 11.8 SW J1753.5-0127
270.2203 -24.9425 5.9 20.4 119.8 0.3836 2.0 8.9 GX 5-1
270.4765 -25.8662 0.0 21.0 121.9 0.3373 1.7 12.0 GRS 1758-258
273.8403 -13.9119 164.0 22.2 88.0 0.0157 0.1 12.2 GX 17+2
275.7631 -30.4210 5.5 27.2 126.6 -0.5306 -2.1 9.0 H1820-303
285.1518 -24.9894 6.8 33.4 111.1 -0.5572 -1.7 7.5 HT1900.1-2455
262.8142 -33.7585 10.0 21.2 150.7 0.2063 1.2 9.8 GX 354-0
291.5669 -47.9267 2.3 46.6 142.0 3.3247 5.1 ------ UNKNOWN
238.3207 -49.4632 2.3 35.6 -166.9 1.0008 5.1 ------ UNKNOWN
224.5485 -16.5395 2.8 25.4 -97.2 0.8152 4.1 ------ UNKNOWN
221.2003 -28.7370 2.7 30.5 -122.0 0.9298 4.2 ------ UNKNOWN
223.4014 29.1091 2.2 51.9 -32.0 2.9805 5.2 ------ UNKNOWN
210.4021 -12.4782 2.8 39.4 -92.0 2.8046 4.1 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-15.104000 34.996000
35.896000 59.196580
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
244.9657 -15.5210 1.9 5.7 -92.8 0.8986 6.1 7.2 Sco X-1
254.4264 35.2901 18.7 50.8 2.6 0.2744 0.6 3.5 Her X-1
256.1599 -37.6893 11.8 22.7 168.2 -0.1549 -1.0 12.4 4U 1700-377
256.3339 -36.4282 5.3 21.5 167.0 -0.3344 -2.2 4.9 GX 349+2
263.1180 -24.8041 6.6 14.8 130.2 0.2855 1.7 6.9 GX 1+4
264.6904 -44.3064 10.8 31.1 159.7 -0.2077 -1.1 8.9 4U 1735-44
268.3134 -1.5953 4.1 22.0 51.7 -0.5158 -2.8 9.2 SW J1753.5-0127
270.4468 -25.0681 4.8 20.7 119.9 0.4222 2.4 8.9 GX 5-1
270.4415 -25.5822 5.9 20.9 121.2 0.3397 1.9 12.2 GRS 1758-258
274.0963 -13.8900 3.3 22.5 88.0 0.7174 3.5 10.2 GX 17+2
275.7513 -30.2565 6.3 27.2 126.3 -0.3788 -1.8 11.2 H1820-303
285.1866 -24.9442 12.0 33.4 111.0 0.2948 1.0 8.3 HT1900.1-2455
263.1669 -33.9680 0.0 21.6 150.4 -0.1056 -0.7 11.9 GX 354-0
251.4514 -22.6716 2.4 7.3 175.1 0.7125 4.8 ------ UNKNOWN
238.6475 -43.4358 2.2 29.9 -163.0 0.8469 5.3 ------ UNKNOWN
232.9430 0.7888 1.9 24.1 -50.3 1.0057 6.0 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
119.396590 311.316000
312.896000 379.216000
380.896000 395.886000
401.896000 403.396600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
244.9802 -15.6428 0.3 20.2 138.1 18.3982 33.6 0.2 Sco X-1
254.3334 35.4804 8.0 39.9 20.7 -1.2283 -1.4 10.3 Her X-1
255.9813 -37.8432 165.5 44.0 147.0 -0.1142 -0.1 0.3 4U 1700-377
256.2994 -36.4830 15.9 43.1 145.6 1.1778 0.7 7.5 GX 349+2
262.8797 -24.8816 4.7 38.6 127.0 -3.6936 -2.4 10.8 GX 1+4
268.2612 -1.3155 181.5 35.3 86.6 -0.0849 -0.1 10.4 SW J1753.5-0127
262.8229 -33.9000 8.6 44.5 137.3 -2.5667 -1.3 9.2 GX 354-0
206.6677 -26.6467 2.4 37.4 -145.9 3.7398 4.9 ------ UNKNOWN
209.4381 30.4247 2.6 37.2 -41.6 3.4143 4.5 ------ UNKNOWN
191.3767 -17.0209 2.3 44.8 -122.2 10.9629 4.9 ------ UNKNOWN
Plot creation:
Sat Sep 6 05:59:34 EDT 2025