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
38.5420 -38.0825 0.0122 37.5651 14.6842 1.7893121 15.790 TRIG_01328546
Foreground time interval of the image:
-9.424 28.525 (delta_t = 37.949 [sec])
Background time interval of the image:
-239.576 -9.424 (delta_t = 230.152 [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 2.048000
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 2.048000
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 2.048000
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 -9.424 sec. to 68.560 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.98418 ( -0.121523 0.12523 )
Norm@50keV : 2.59503E-03 ( -0.000207602 0.000204933 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 64.52 using 59 bins.
Reduced chi-squared = 1.13193
# Null hypothesis probability of 2.30e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 77.98 sec: 0.386479 ( -0.026481 0.026507 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.86502e-06 ( -1.42064e-07 1.43443e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -9.424 sec. to 68.560 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.33816 ( -0.589297 0.511905 )
Epeak [keV] : 44.4086 ( -12.1265 17.2538 )
Norm@50keV : 5.98416E-03 ( -0.00285132 0.00684271 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 59.73 using 59 bins.
Reduced chi-squared = 1.06661
# Null hypothesis probability of 3.42e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 77.98 sec: 0.376457 ( -0.027593 0.027605 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.76146e-06 ( -1.60895e-07 1.63597e-07 ) ergs/cm2
Band function
Time interval is from -9.424 sec. to 68.560 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] : 10.2839 (-0.808138 0.882569)
R^2/D10^2 : 0.160855 (-0.043989 0.0600753)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 98.57 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.25e-04 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.726e-07 3.189e-08
25- 50 7.048e-07 5.513e-08
50-150 3.986e-07 7.428e-08
15-150 1.376e-06 1.076e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 69.9311 (-13.0802 18.0833)
Norm : 1.89788 (-0.204622 0.233848)
------------------------------------------------------------
#Fit statistic : Chi-Squared 59.64 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.80e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.797e-07 3.665e-08
25- 50 6.039e-07 4.191e-08
50-150 7.751e-07 1.266e-07
15-150 1.759e-06 1.571e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.58203 (-1.21091 1.24886)
R1^2/D10^2 : 0.648201 (-0.284664 0.648937)
kT2 [keV] : 21.4939 (-5.01693 9.54267)
R2^2/D10^2 : 6.09741E-03 (-0.00459452 0.00719792)
------------------------------------------------------------
#Fit statistic : Chi-Squared 57.46 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.84e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.696e-07 8.851e-08
25- 50 6.123e-07 1.321e-07
50-150 7.913e-07 3.746e-07
15-150 1.773e-06 5.340e-07
Peak spectrum fit
Power-law model
Time interval is from -0.096 sec. to 0.904 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.86161 ( -0.311543 0.346803 )
Norm@50keV : 8.61496E-03 ( -0.00197148 0.00191409 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 57.80 using 59 bins.
Reduced chi-squared = 1.01404
# Null hypothesis probability of 4.46e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 1.21674 ( -0.248712 0.24905 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.92155e-08 ( -1.77714e-08 1.79495e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.096 sec. to 0.904 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.793695 ( -1.77644 1.27274 )
Epeak [keV] : 56.3274 ( -56.3274 -56.3274 )
Norm@50keV : 3.06379E-02 ( -0.030638 0.217857 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 55.81 using 59 bins.
Reduced chi-squared = 0.996607
# Null hypothesis probability of 4.82e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 1.19004 ( -0.25328 0.25212 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.74123e-08 ( -1.81703e-08 1.84196e-08 ) ergs/cm2
Band function
Time interval is from -0.096 sec. to 0.904 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] : 13.0502 (-2.77993 3.36301)
R^2/D10^2 : 0.227094 (-0.130408 0.315429)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 59.86 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.72e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.202e-09 3.072e-09
25- 50 2.837e-08 8.780e-09
50-150 3.061e-08 1.314e-08
15-150 6.718e-08 2.207e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 94.4712 (-41.5287 -94.4681)
Norm : 5.55728 (-1.36481 1.79486)
------------------------------------------------------------
#Fit statistic : Chi-Squared 56.20 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.05e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.452e-08 3.792e-09
25- 50 2.481e-08 7.690e-09
50-150 3.890e-08 2.416e-08
15-150 7.823e-08 3.327e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 4.23781 (-3.38156 5.92412)
R1^2/D10^2 : 7.96701 (-7.60054 3.57515)
kT2 [keV] : 16.5526 (-4.57214 11.8479)
R2^2/D10^2 : 8.15830E-02 (-0.0700402 0.215334)
------------------------------------------------------------
#Fit statistic : Chi-Squared 55.18 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.68e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.410e-08 7.870e-09
25- 50 2.389e-08 1.272e-08
50-150 3.856e-08 2.407e-08
15-150 7.655e-08 4.187e-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: 2.05794 ( -0.158719 0.166451 )
Norm@50keV : 2.87074E-03 ( -0.000320422 0.000314642 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 58.82 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.09e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 37.95 sec: 0.442492 ( -0.0394277 0.0394459 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.00849e-06 ( -1.03563e-07 1.04996e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.27459 ( -0.876287 0.699888 )
Epeak [keV] : 37.8998 ( -29.7531 14.0471 )
Norm@50keV : 8.25425E-03 ( -0.004978 0.0192915 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 55.10 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.09e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 37.95 sec: 0.431341 ( -0.040607 0.04062 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.38226e-07 ( -1.1722e-07 1.21334e-07 ) 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) = 5.59e-07
S(50-100 keV) = 5.65e-07
T90 vs. Hardness ratio plot
T90 = 63.7839999198914 sec.
Hardness ratio (energy fluence ratio) = 1.01073
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.17016
Count Ratio (50-100 keV) / (15-25 keV) = 0.597086
Mask shadow pattern
IMX = 7.440107916344209E-01, IMY = -1.949689904494813E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 2.048000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 2.048000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 2.048000
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:
-239.576000 -9.424000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
357.8936 35.2481 2.4 49.1 161.8 4.5719 4.9 ------ UNKNOWN
1.1096 39.9055 2.3 50.4 168.6 4.9394 5.0 ------ UNKNOWN
64.2016 33.5344 3.1 44.7 -122.0 5.0020 3.7 ------ UNKNOWN
63.0618 38.0265 3.3 47.3 -127.3 6.1673 3.5 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-9.424000 28.524590
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
38.5420 -38.0825 0.7 37.6 14.7 1.7894 15.8 ------ UNKNOWN
15.6597 50.3241 3.5 53.4 -173.3 0.6710 3.3 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
108.724590 786.224580
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
359.5775 -4.0881 2.1 49.1 161.8 12.7493 5.5 246.6 UNKNOWN
25.9377 -57.2600 3.1 20.9 57.2 3.3951 3.7 ------ UNKNOWN
2.8322 0.1353 2.3 50.4 168.6 12.6510 5.0 170.1 UNKNOWN
70.6544 -66.8447 2.9 34.0 15.9 4.3794 4.0 ------ UNKNOWN
125.1321 -57.6872 2.5 56.9 -1.7 10.6510 4.6 ------ UNKNOWN
71.3944 -18.8315 2.1 34.4 -76.9 7.8373 5.6 ------ UNKNOWN
Plot creation:
Sun Mar 1 23:37:26 EST 2026