Estimated redshift from machine learning (Ukwatta et al. 2016) - may take a few minute to calcaulte
Image
Pre-slew 15.0-350.0 keV image (Event data)
# RAcent DECcent POSerr Theta Phi Peak Cts SNR Name
18.4948 56.4825 0.0101 9.6831 50.2763 0.7353866 18.910 TRIG_01400964
Foreground time interval of the image:
-2.412 9.804 (delta_t = 12.216 [sec])
Background time interval of the image:
-239.496 -2.412 (delta_t = 237.084 [sec])
Lightcurves
Notes:
- 1) The mask-weighted light curves are using the flight position.
- 2) Multiple plots of different time binning/intervals are shown to cover all scenarios of short/long GRBs, rate/image triggers, and real/false positives.
- 3) 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.
- 4) 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.
- 5) 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 1.024000
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 1.024000
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 1.024000
SN=5 or 10 sec. binning (whichever binning is satisfied first)
SN=5 or 10 sec. binning (T < 200 sec)
Quad-rate summed light curves (from T0-300s to T0+1000s)
Spectral Evolution
Spectra
Notes:
- 1) The fitting includes the systematic errors.
- 2) When the burst includes telescope slew time periods, the fitting uses an average response file made from multiple 5-s response files through out the slew time plus single time preiod for the non-slew times, and weighted by the total counts in the corresponding time period using addrmf. An average response file is needed becuase a spectral fit using 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.
Time averaged spectrum fit using the average DRM
Power-law model
Time interval is from -2.412 sec. to 9.804 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.64486 ( -0.147749 0.150593 )
Norm@50keV : 3.59771E-03 ( -0.000318823 0.000315355 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 69.09 using 59 bins.
Reduced chi-squared = 1.21211
# Null hypothesis probability of 1.31e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 12.22 sec: 0.468997 ( -0.038824 0.038859 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.09149e-07 ( -3.85609e-08 3.90402e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -2.412 sec. to 9.804 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.45681 ( -0.644992 0.283177 )
Epeak [keV] : 137.097 ( -74.0762 -137.111 )
Norm@50keV : 4.52326E-03 ( -0.00122012 0.00523768 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 68.79 using 59 bins.
Reduced chi-squared = 1.22839
# Null hypothesis probability of 1.17e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 12.22 sec: 0.464970 ( -0.040893 0.040692 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.0219e-07 ( -4.42322e-08 4.37349e-08 ) ergs/cm2
Band function
Time interval is from -2.412 sec. to 9.804 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : ( )
beta : ( )
Epeak [keV] : ( )
Norm@50keV : ( )
------------------------------------------------------------
Photon flux (15-150 keV) in 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] : 13.2429 (-1.35261 1.52409)
R^2/D10^2 : 7.96233E-02 (-0.0259256 0.0380289)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 103.10 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.79e-04 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.617e-08 5.750e-09
25- 50 1.271e-07 1.565e-08
50-150 1.424e-07 2.544e-08
15-150 3.057e-07 3.336e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 154.071 (-50.7475 -153.698)
Norm : 1.92955 (-0.176357 0.211545)
------------------------------------------------------------
#Fit statistic : Chi-Squared 69.03 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.32e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.001e-08 7.723e-09
25- 50 1.121e-07 2.464e-08
50-150 2.259e-07 1.049e-07
15-150 3.980e-07 1.682e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.82345 (-1.72417 2.25852)
R1^2/D10^2 : 0.952322 (-0.623928 1.68954)
kT2 [keV] : 21.4069 (-4.44563 10.5455)
R2^2/D10^2 : 1.13421E-02 (-0.00873783 0.0100327)
------------------------------------------------------------
#Fit statistic : Chi-Squared 71.07 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.12e-02 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.207e-08 2.495e-08
25- 50 1.087e-07 3.402e-08
50-150 2.155e-07 8.079e-08
15-150 3.863e-07 1.433e-07
Peak spectrum fit
Power-law model
Time interval is from 0.920 sec. to 1.920 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.26623 ( -0.219354 0.215849 )
Norm@50keV : 8.12317E-03 ( -0.00108171 0.00108158 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 69.47 using 59 bins.
Reduced chi-squared = 1.21877
# Null hypothesis probability of 1.24e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.963355 ( -0.132105 0.132425 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.09618e-08 ( -1.1715e-08 1.18023e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.920 sec. to 1.920 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 6.09061E-02 ( -1.44983 1.06341 )
Epeak [keV] : 85.2651 ( -21.0804 207.138 )
Norm@50keV : 3.06615E-02 ( -0.0306664 0.105766 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 65.66 using 59 bins.
Reduced chi-squared = 1.1725
# Null hypothesis probability of 1.77e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.921838 ( -0.140897 0.139122 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.57757e-08 ( -1.26015e-08 1.27991e-08 ) ergs/cm2
Band function
Time interval is from 0.920 sec. to 1.920 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : ( )
beta : ( )
Epeak [keV] : ( )
Norm@50keV : ( )
------------------------------------------------------------
Photon flux (15-150 keV) in 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] : 17.6356 (-2.34472 2.86086)
R^2/D10^2 : 6.94434E-02 (-0.028164 0.0441193)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 68.34 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.45e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.352e-09 1.198e-09
25- 50 1.982e-08 4.260e-09
50-150 4.449e-08 1.032e-08
15-150 6.866e-08 1.184e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-46.4608 -200)
Norm : 4.02361 (-0.541491 0.541491)
------------------------------------------------------------
#Fit statistic : Chi-Squared 72.65 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.92e-02 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.002e-08 5.665e-09
25- 50 1.927e-08 1.081e-08
50-150 4.227e-08 2.363e-08
15-150 7.157e-08 4.026e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 3.99063 (-3.48622 -4.03266)
R1^2/D10^2 : 4.09585 (-3.95777 -4.04188)
kT2 [keV] : 19.4489 (-3.09796 -19.4637)
R2^2/D10^2 : 4.71106E-02 (-0.043381 0.0406492)
------------------------------------------------------------
#Fit statistic : Chi-Squared 64.55 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.77e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.156e-09 3.099e-09
25- 50 1.830e-08 5.610e-09
50-150 4.741e-08 1.745e-08
15-150 7.286e-08 2.153e-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: 1.64486 ( -0.147749 0.150593 )
Norm@50keV : 3.59771E-03 ( -0.000318823 0.000315355 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 69.09 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.31e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 12.22 sec: 0.468979 ( -0.0388211 0.038856 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.09096e-07 ( -3.86194e-08 3.9034e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.45681 ( -0.644991 0.283181 )
Epeak [keV] : 137.092 ( -74.0764 -137.111 )
Norm@50keV : 4.52331E-03 ( -0.00122012 0.00523767 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 68.79 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.17e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 12.22 sec: 0.464895 ( -0.040813 0.040376 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.02326e-07 ( -4.43158e-08 4.36682e-08 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : ( )
beta : ( )
Epeak [keV] : ( )
Norm@50keV : ( )
------------------------------------------------------------
Photon flux (15-150 keV) in 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) = 1.08e-07
S(50-100 keV) = 1.38e-07
T90 vs. Hardness ratio plot
T90 = 10.7840000391006 sec.
Hardness ratio (energy fluence ratio) = 1.27778
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.1458
Count Ratio (50-100 keV) / (15-25 keV) = 0.776943
Mask shadow pattern
IMX = 1.090464935946764E-01, IMY = -1.312365260240749E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.024000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.024000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.024000
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:
-239.496000 -2.412000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
299.5784 35.1889 0.9 48.6 -177.9 9.4332 12.9 1.0 Cyg X-1
308.0803 41.0146 2.7 40.1 178.8 1.9497 4.3 4.0 Cyg X-3
326.0879 38.1750 5.1 35.0 157.0 1.1326 2.3 9.6 Cyg X-2
55.0912 42.6205 2.5 34.9 19.0 2.0833 4.7 ------ UNKNOWN
320.5393 39.1796 2.8 36.3 164.3 1.8401 4.2 ------ UNKNOWN
278.8281 72.0569 2.6 30.5 -122.1 1.7905 4.5 ------ UNKNOWN
227.9246 71.3108 3.0 41.7 -103.6 4.9935 3.9 ------ UNKNOWN
256.4803 56.3259 2.5 48.2 -129.3 7.1554 4.6 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-2.412000 9.804000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
299.6414 35.1508 10.3 48.6 -178.0 -0.0944 -1.1 3.9 Cyg X-1
308.2008 40.8838 5.9 40.1 178.6 -0.1104 -1.9 5.8 Cyg X-3
326.1873 38.4480 5.0 34.7 157.1 -0.1282 -2.3 7.6 Cyg X-2
18.4947 56.4825 0.6 9.7 50.3 0.7355 18.9 ------ UNKNOWN
281.7274 54.1841 2.0 41.1 -147.3 0.3577 5.6 ------ UNKNOWN
256.6592 56.4938 2.3 48.0 -129.3 0.8635 5.0 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
57.004600 474.504600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
299.6181 35.1824 1.1 55.4 -178.2 16.9576 10.2 1.8 Cyg X-1
308.1891 40.9779 4.8 46.6 -179.4 2.8815 2.4 3.9 Cyg X-3
326.1301 38.1745 12.9 38.7 163.2 0.7628 0.9 9.0 Cyg X-2
Plot creation:
Sun Mar 1 23:20:56 EST 2026