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
196.6422 3.2776 0.0139 5.4456 89.7705 1.9491461 13.755 TRIG_01175438
Foreground time interval of the image:
-27.784 73.301 (delta_t = 101.085 [sec])
Background time interval of the image:
-275.000 -27.784 (delta_t = 247.216 [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
8 ms binning
From T100_start-3 s to T100_start+3 s
2 ms binning
From T100_start-1 s to T100_start+1 s
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 -27.784 sec. to 107.004 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.35014 ( -0.153983 0.153726 )
Norm@50keV : 1.16885E-03 ( -0.000104842 0.000104435 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 49.39 using 59 bins.
Reduced chi-squared = 0.866491
# Null hypothesis probability of 7.53e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 134.8 sec: 0.140819 ( -0.012675 0.012688 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.539e-06 ( -1.53934e-07 1.55612e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -27.784 sec. to 107.004 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.887185 ( -0.671297 0.569645 )
Epeak [keV] : 122.730 ( -45.6931 -122.73 )
Norm@50keV : 1.98472E-03 ( -0.000871428 0.00217435 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 47.58 using 59 bins.
Reduced chi-squared = 0.849643
# Null hypothesis probability of 7.81e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 134.8 sec: 0.137931 ( -0.01323 0.013205 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.48501e-06 ( -1.69302e-07 1.69921e-07 ) ergs/cm2
Band function
Time interval is from -27.784 sec. to 107.004 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] : 16.6683 (-1.84614 2.12382)
R^2/D10^2 : 1.14560E-02 (-0.00384544 0.00566929)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 69.97 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.16e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.784e-08 1.570e-08
25- 50 3.825e-07 4.893e-08
50-150 7.539e-07 1.318e-07
15-150 1.224e-06 1.374e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-34.5814 -200)
Norm : 0.580957 (-0.0515533 0.0515533)
------------------------------------------------------------
#Fit statistic : Chi-Squared 52.50 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.44e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.950e-07 2.575e-08
25- 50 3.751e-07 9.133e-08
50-150 8.227e-07 4.124e-07
15-150 1.393e-06 5.589e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.46558 (-2.03114 2.78731)
R1^2/D10^2 : 0.154459 (-0.1042 0.374081)
kT2 [keV] : 24.4260 (-4.77811 9.94165)
R2^2/D10^2 : 2.64426E-03 (-0.0018613 0.00237194)
------------------------------------------------------------
#Fit statistic : Chi-Squared 46.91 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.73e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.652e-07 7.891e-08
25- 50 3.589e-07 1.347e-07
50-150 9.486e-07 3.637e-07
15-150 1.473e-06 5.385e-07
Peak spectrum fit
Power-law model
Time interval is from 9.040 sec. to 10.040 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.795654 ( -0.601262 0.522368 )
Norm@50keV : 4.27706E-03 ( -0.00134963 0.00124564 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 59.60 using 59 bins.
Reduced chi-squared = 1.04561
# Null hypothesis probability of 3.81e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.491641 ( -0.141227 0.14307 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.00783e-08 ( -1.40362e-08 1.40884e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 9.040 sec. to 10.040 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.787048 ( -3.09313 -0.710087 )
Epeak [keV] : 1.00000E+04 ( -10000 -10000 )
Norm@50keV : 4.30562E-03 ( -0.00135447 -0.00430633 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 59.61 using 59 bins.
Reduced chi-squared = 1.06446
# Null hypothesis probability of 3.46e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.491476 ( -0.141253 0.143032 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.00553e-08 ( -1.40215e-08 1.40996e-08 ) ergs/cm2
Band function
Time interval is from 9.040 sec. to 10.040 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] : 29.6309 (-9.19086 21.2576)
R^2/D10^2 : 7.51181E-03 (-0.00751326 0.0154208)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 61.48 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.19e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.040e-09 6.560e-10
25- 50 6.380e-09 3.799e-09
50-150 3.976e-08 2.367e-08
15-150 4.718e-08 2.753e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-79.3774 -200)
Norm : 2.02756 (-0.589145 0.589145)
------------------------------------------------------------
#Fit statistic : Chi-Squared 65.84 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.98e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.048e-09 3.135e-09
25- 50 9.711e-09 5.785e-09
50-150 2.130e-08 1.322e-08
15-150 3.606e-08 2.224e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 3.89978 (-2.42721 3.54701)
R1^2/D10^2 : 4.63938 (-4.70086 43.6782)
kT2 [keV] : 35.5205 (-12.2832 40.9381)
R2^2/D10^2 : 4.29194E-03 (-0.00361108 0.00689482)
------------------------------------------------------------
#Fit statistic : Chi-Squared 57.03 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.99e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.486e-09 2.736e-09
25- 50 6.239e-09 3.311e-09
50-150 4.084e-08 2.424e-08
15-150 5.157e-08 2.783e-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: 1.35027 ( -0.149948 0.14963 )
Norm@50keV : 1.38864E-03 ( -0.000121905 0.000121635 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 35.88 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.87e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 101.1 sec: 0.167300 ( -0.0147182 0.0147328 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.3711e-06 ( -1.34832e-07 1.36101e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.914669 ( -0.621689 0.499112 )
Epeak [keV] : 126.425 ( -47.7817 -126.425 )
Norm@50keV : 2.29360E-03 ( -0.000968595 0.00228297 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 34.03 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.91e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 101.1 sec: 0.164181 ( -0.015249 0.015233 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.32581e-06 ( -1.47343e-07 1.47889e-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) = 3.52e-07
S(50-100 keV) = 5.53e-07
T90 vs. Hardness ratio plot
T90 = 104.051999926567 sec.
Hardness ratio (energy fluence ratio) = 1.57102
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.49762
Count Ratio (50-100 keV) / (15-25 keV) = 1.27396
Mask shadow pattern
IMX = 3.817690076934504E-04, IMY = -9.533068798711747E-02
TIME vs. PHA plot around the trigger time
TIME vs. DetID plot around the trigger time
100 us light curve (15-350 keV)
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:
-275.000000 -27.784000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
221.7400 -6.3782 3.5 32.2 77.6 2.5484 3.3 ------ UNKNOWN
239.7130 45.9997 2.4 56.9 2.4 7.0688 4.7 ------ UNKNOWN
144.2993 -21.1214 3.3 54.5 -157.1 4.7235 3.5 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-27.784000 73.300600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
196.6421 3.2776 0.8 5.4 89.8 1.9490 13.8 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
114.500610 289.513000
291.000000 963.012400
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
227.8539 -4.0281 3.8 32.1 77.5 7.7413 3.1 ------ UNKNOWN
226.3339 -7.5675 2.3 31.6 84.7 12.0379 4.9 ------ UNKNOWN
219.7701 8.9129 2.8 23.7 49.8 6.3529 4.1 ------ UNKNOWN
Plot creation:
Sat Sep 30 00:48:40 EDT 2023