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
270.6126 53.6991 0.0102 32.9356 17.1308 1.0418809 18.675 TRIG_01031297
Foreground time interval of the image:
-0.180 9.877 (delta_t = 10.057 [sec])
Background time interval of the image:
-172.323 -0.180 (delta_t = 172.143 [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 0.512000
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 0.512000
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 0.512000
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 -0.180 sec. to 106.404 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.15137 ( -0.0723534 0.0717559 )
Norm@50keV : 3.82737E-03 ( -0.00014398 0.000143704 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 53.77 using 59 bins.
Reduced chi-squared = 0.943333
# Null hypothesis probability of 5.97e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 106.6 sec: 0.446423 ( -0.017757 0.017845 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.19882e-06 ( -1.68433e-07 1.68919e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.180 sec. to 106.404 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.14996 ( -0.134024 0.069541 )
Epeak [keV] : 9999.36 ( -9999.36 -9999.36 )
Norm@50keV : 3.83356E-03 ( -0.000143509 0.000581442 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 53.87 using 59 bins.
Reduced chi-squared = 0.961964
# Null hypothesis probability of 5.56e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 106.6 sec: 0.446291 ( -0.017781 0.017822 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.2327e-06 ( -2.03888e-07 1.33333e-07 ) ergs/cm2
Band function
Time interval is from -0.180 sec. to 106.404 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] : 20.8642 ( )
R^2/D10^2 : 1.75299E-02 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 213.48 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.19e-20 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.541e-07 1.215e-08
25- 50 7.889e-07 4.269e-08
50-150 2.558e-06 1.567e-07
15-150 3.501e-06 1.578e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.362 ( )
Norm : 1.88751 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared 152.61 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.16e-10 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.010e-07 2.169e-08
25- 50 9.638e-07 4.280e-08
50-150 2.114e-06 9.168e-08
15-150 3.579e-06 1.412e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 8.95309 (-1.32374 1.46558)
R1^2/D10^2 : 0.177367 (-0.064087 0.116391)
kT2 [keV] : 41.7699 (-7.63368 14.507)
R2^2/D10^2 : 1.73056E-03 (-0.000946228 0.00144043)
------------------------------------------------------------
#Fit statistic : Chi-Squared 59.50 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.15e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.345e-07 5.378e-08
25- 50 8.983e-07 9.391e-08
50-150 3.032e-06 5.922e-07
15-150 4.265e-06 6.183e-07
Peak spectrum fit
Power-law model
Time interval is from 43.156 sec. to 44.156 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.731095 ( -0.128652 0.125566 )
Norm@50keV : 2.58130E-02 ( -0.00178501 0.00177421 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 62.14 using 59 bins.
Reduced chi-squared = 1.09018
# Null hypothesis probability of 2.98e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 2.97702 ( -0.19973 0.19989 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.10771e-07 ( -2.34946e-08 2.3655e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 43.156 sec. to 44.156 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.724203 ( -0.230774 0.125792 )
Epeak [keV] : 9998.79 ( -9998.96 -9998.96 )
Norm@50keV : 2.60102E-02 ( -0.00177119 0.0114368 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 62.16 using 59 bins.
Reduced chi-squared = 1.11
# Null hypothesis probability of 2.66e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 2.98167 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 3.12047e-07 ( 0 0 ) ergs/cm2
Band function
Time interval is from 43.156 sec. to 44.156 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] : 26.9605 (-2.8149 3.34558)
R^2/D10^2 : 6.06127E-02 (-0.0169184 0.0224882)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 97.34 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.98e-04 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.343e-09 1.124e-09
25- 50 4.322e-08 4.605e-09
50-150 2.296e-07 2.575e-08
15-150 2.801e-07 2.650e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.363 ( )
Norm : 11.0489 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared 171.07 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.48e-13 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.751e-08 2.760e-09
25- 50 5.292e-08 9.200e-09
50-150 1.161e-07 4.480e-08
15-150 1.965e-07 6.752e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 8.19546 (-2.47447 3.59262)
R1^2/D10^2 : 1.03821 (-0.659871 2.36257)
kT2 [keV] : 42.2790 (-9.16703 25.8642)
R2^2/D10^2 : 1.57071E-02 (-0.0109587 0.018012)
------------------------------------------------------------
#Fit statistic : Chi-Squared 62.59 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.25e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.631e-08 7.171e-09
25- 50 4.752e-08 1.660e-08
50-150 2.530e-07 9.072e-08
15-150 3.168e-07 8.780e-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: 0.850516 ( -0.17787 0.169178 )
Norm@50keV : 6.54229E-03 ( -0.000625899 0.00061362 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 79.17 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.77e-02 with 57 degrees of freedom
Photon flux (15-150 keV) in 10.06 sec: 0.750995 ( -0.0701619 0.0704679 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.53259e-07 ( -6.83445e-08 6.86698e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.853030 ( -0.188536 0.162165 )
Epeak [keV] : 9999.36 ( -9999.36 -9999.36 )
Norm@50keV : 6.60039E-03 ( -0.000583191 0.00174925 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 79.25 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.22e-02 with 56 degrees of freedom
Photon flux (15-150 keV) in 10.06 sec: 0.753192 ( -0.0729 0.068238 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.50883e-07 ( -6.6391e-08 7.16272e-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) = 8.56e-07
S(50-100 keV) = 1.55e-06
T90 vs. Hardness ratio plot
T90 = 92.5279998779297 sec.
Hardness ratio (energy fluence ratio) = 1.81075
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.52196
Count Ratio (50-100 keV) / (15-25 keV) = 1.45978
Mask shadow pattern
IMX = 6.190710664771016E-01, IMY = -1.908159232915664E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.512000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.512000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.512000
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:
-172.323410 -0.180000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.4860 35.2162 5.3 53.2 5.5 1.3532 2.2 7.7 Her X-1
299.5344 35.2546 3.2 28.1 -37.6 0.8248 3.6 4.2 Cyg X-1
308.0770 40.9573 1.8 19.5 -42.4 1.2415 6.4 1.5 Cyg X-3
326.3194 38.3500 4.8 16.6 -88.7 0.5140 2.4 7.2 Cyg X-2
258.9029 24.7013 3.4 58.5 -6.4 4.2918 3.4 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-0.180000 9.876590
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.4656 35.2288 10.2 53.2 5.5 0.1499 1.1 6.8 Her X-1
299.4507 35.0931 6.7 28.3 -37.7 0.0761 1.7 9.4 Cyg X-1
308.3064 40.9579 8.0 19.4 -42.8 -0.0600 -1.4 8.9 Cyg X-3
326.3618 38.4064 107.3 16.6 -88.8 -0.0047 -0.1 10.3 Cyg X-2
270.6126 53.6990 0.6 32.9 17.1 1.0420 18.7 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
63.076610 409.576610
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.4598 35.3651 2.7 21.5 -2.1 1.5494 4.2 1.4 Her X-1
299.5407 35.3510 15.2 27.3 -99.8 0.3615 0.8 9.3 Cyg X-1
307.9794 40.9762 2.6 27.9 -118.6 1.9086 4.4 6.1 Cyg X-3
326.2394 38.3853 3.0 40.3 -131.3 2.2807 3.9 5.0 Cyg X-2
222.4621 27.3666 3.3 43.8 32.5 2.2948 3.5 ------ UNKNOWN
270.6546 53.6353 2.4 0.0 -83.9 1.4908 4.8 ------ UNKNOWN
Plot creation:
Sat Jul 30 07:17:50 EDT 2022