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
36.6021 66.6707 0.0203 41.9154 170.3374 1.2993607 9.408 TRIG_01000613
Foreground time interval of the image:
-2.768 23.872 (delta_t = 26.640 [sec])
Background time interval of the image:
-239.088 -2.768 (delta_t = 236.320 [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 -2.768 sec. to 23.872 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.48355 ( -0.246728 0.246246 )
Norm@50keV : 3.57583E-03 ( -0.000527377 0.000525867 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 40.43 using 59 bins.
Reduced chi-squared = 0.709298
# Null hypothesis probability of 9.53e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 26.64 sec: 0.444471 ( -0.06738 0.067621 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.06285e-07 ( -1.43004e-07 1.44162e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -2.768 sec. to 23.872 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.920801 ( -1.28655 0.753416 )
Epeak [keV] : 95.8954 ( -38.3595 -95.9249 )
Norm@50keV : 6.91033E-03 ( -0.00375115 0.0234671 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 39.53 using 59 bins.
Reduced chi-squared = 0.705893
# Null hypothesis probability of 9.53e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 26.64 sec: 0.435409 ( -0.069693 0.0696 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.727e-07 ( -1.58739e-07 1.56629e-07 ) ergs/cm2
Band function
Time interval is from -2.768 sec. to 23.872 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] : 14.8278 (-2.3501 2.96452)
R^2/D10^2 : 5.37247E-02 (-0.0258355 0.046092)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 46.85 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.29e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.600e-08 1.853e-08
25- 50 2.595e-07 5.816e-08
50-150 3.862e-07 1.118e-07
15-150 7.117e-07 1.487e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.363 (-85.1912 -199.363)
Norm : 1.83755 (-0.267287 0.267366)
------------------------------------------------------------
#Fit statistic : Chi-Squared 39.94 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.58e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.219e-07 6.876e-08
25- 50 2.345e-07 1.310e-07
50-150 5.143e-07 2.836e-07
15-150 8.706e-07 4.823e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 10.2702 (-5.40698 3.63147)
R1^2/D10^2 : 0.151107 (-0.0890057 0.153961)
kT2 [keV] : 45.2548 (-42.9893 -47.9576)
R2^2/D10^2 : 8.12317E-04 (-0.000662242 0.0226669)
------------------------------------------------------------
#Fit statistic : Chi-Squared 38.90 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.51e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 9.244e-08 5.317e-08
25- 50 2.619e-07 1.485e-07
50-150 5.331e-07 2.764e-07
15-150 8.875e-07 4.254e-07
Peak spectrum fit
Power-law model
Time interval is from 0.868 sec. to 1.868 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.66578 ( -0.342401 0.357869 )
Norm@50keV : 1.34234E-02 ( -0.00304333 0.0029909 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 61.41 using 59 bins.
Reduced chi-squared = 1.07737
# Null hypothesis probability of 3.21e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 1.76207 ( -0.38008 0.38098 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.24669e-07 ( -2.92093e-08 2.9668e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.868 sec. to 1.868 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.189064 ( -3.2731 1.70598 )
Epeak [keV] : 56.3185 ( -10.9124 -56.0966 )
Norm@50keV : 8.36988E-02 ( -0.086747 4.73456 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 59.55 using 59 bins.
Reduced chi-squared = 1.06339
# Null hypothesis probability of 3.48e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 1.68166 ( -0.40579 0.39888 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.81008e-08 ( -3.86333e-08 2.33312e-08 ) ergs/cm2
Band function
Time interval is from 0.868 sec. to 1.868 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] : 12.7364 (-2.44918 3.14811)
R^2/D10^2 : 0.370791 (-0.208865 0.439404)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 60.55 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.49e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.276e-08 5.069e-09
25- 50 4.297e-08 1.498e-08
50-150 4.353e-08 2.121e-08
15-150 9.925e-08 3.460e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 136.464 (-72.0281 -134.144)
Norm : 7.41515 (-1.74063 2.48163)
------------------------------------------------------------
#Fit statistic : Chi-Squared 60.43 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.53e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.918e-08 1.108e-08
25- 50 3.505e-08 1.970e-08
50-150 6.643e-08 4.325e-08
15-150 1.207e-07 7.295e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 200.000 (-200 -200)
R1^2/D10^2 : 1.10033E-04 (-0.000110036 -0.000110036)
kT2 [keV] : 11.3176 (-2.05917 3.19046)
R2^2/D10^2 : 0.525266 (-0.309647 0.154931)
------------------------------------------------------------
#Fit statistic : Chi-Squared 58.47 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.49e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.581e-08 7.820e-09
25- 50 4.029e-08 2.335e-08
50-150 4.694e-08 2.748e-08
15-150 1.030e-07 5.605e-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: 1.48355 ( -0.246728 0.246246 )
Norm@50keV : 3.57583E-03 ( -0.000527377 0.000525867 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 40.43 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.53e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 26.64 sec: 0.444460 ( -0.0673749 0.0676175 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.06165e-07 ( -1.42973e-07 1.44226e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.921078 ( -1.28661 0.753343 )
Epeak [keV] : 95.9254 ( -38.3604 -95.9263 )
Norm@50keV : 6.90783E-03 ( -0.00375112 0.0234668 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 39.53 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.53e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 26.64 sec: 0.435361 ( -0.069676 0.069579 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.73019e-07 ( -1.58766e-07 1.56819e-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) = 2.22e-07
S(50-100 keV) = 3.17e-07
T90 vs. Hardness ratio plot
T90 = 22.0800000429153 sec.
Hardness ratio (energy fluence ratio) = 1.42793
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.5647
Count Ratio (50-100 keV) / (15-25 keV) = 1.26806
Mask shadow pattern
IMX = -8.849975337905884E-01, IMY = -1.506806050536204E-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:
-239.088000 -2.768000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6425 22.0059 0.4 12.2 10.6 9.0684 28.4 0.7 Crab
53.0540 3.8135 2.4 40.9 64.1 5.6578 4.8 ------ UNKNOWN
76.3976 -9.6393 3.3 44.2 24.2 1.9405 3.5 ------ UNKNOWN
75.3891 11.6581 2.2 23.5 33.3 1.8169 5.3 ------ UNKNOWN
103.0833 -9.6081 2.6 48.0 -12.3 2.6481 4.5 ------ UNKNOWN
132.9999 36.0478 3.0 40.9 -92.0 5.5266 3.9 ------ UNKNOWN
146.2888 61.3334 2.7 48.0 -129.1 5.7371 4.2 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-2.768000 23.872000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.8285 21.9071 0.0 12.4 9.8 -0.1553 -2.1 12.6 Crab
36.6020 66.6707 1.2 41.9 170.3 1.2996 9.4 ------ UNKNOWN
135.2232 42.7403 2.3 41.5 -102.5 1.4355 5.1 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
87.812590 683.512610
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6119 21.9961 1.4 53.5 16.5 20.0587 8.1 1.6 Crab
308.1847 40.9475 6.8 52.4 -178.4 -3.8866 -1.7 3.4 Cyg X-3
325.9663 38.3318 74.7 47.8 164.4 -0.3052 -0.2 9.7 Cyg X-2
160.5749 67.6818 3.3 40.0 -76.8 8.2271 3.5 ------ UNKNOWN
Plot creation:
Sat Jul 30 07:30:29 EDT 2022