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
232.1121 11.1697 0.0087 22.5397 81.1883 2.7260442 22.200 TRIG_01070157
Foreground time interval of the image:
-12.880 32.653 (delta_t = 45.533 [sec])
Background time interval of the image:
-239.248 -12.880 (delta_t = 226.368 [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 4.096000
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 4.096000
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 4.096000
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 -12.880 sec. to 100.016 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.48252 ( -0.151333 0.151939 )
Norm@50keV : 1.82886E-03 ( -0.000165379 0.000164466 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 46.97 using 59 bins.
Reduced chi-squared = 0.824035
# Null hypothesis probability of 8.26e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 112.9 sec: 0.227263 ( -0.020063 0.02008 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.96473e-06 ( -1.95258e-07 1.97609e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -12.880 sec. to 100.016 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.15800 ( -0.676487 0.404282 )
Epeak [keV] : 123.105 ( -55.1353 -123.149 )
Norm@50keV : 2.71842E-03 ( -0.00101955 0.00339179 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 46.11 using 59 bins.
Reduced chi-squared = 0.823393
# Null hypothesis probability of 8.24e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 112.9 sec: 0.224256 ( -0.020904 0.020809 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.90355e-06 ( -2.26972e-07 2.25686e-07 ) ergs/cm2
Band function
Time interval is from -12.880 sec. to 100.016 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] : 14.0039 (-1.5092 1.74128)
R^2/D10^2 : 3.27095E-02 (-0.0111005 0.0163709)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 72.19 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.48e-02 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.530e-07 2.727e-08
25- 50 5.691e-07 7.101e-08
50-150 7.350e-07 1.323e-07
15-150 1.457e-06 1.885e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-58.8296 -200)
Norm : 0.931579 (-0.080921 0.080921)
------------------------------------------------------------
#Fit statistic : Chi-Squared 46.44 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.40e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.619e-07 5.984e-08
25- 50 5.039e-07 1.555e-07
50-150 1.105e-06 4.999e-07
15-150 1.871e-06 8.606e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 8.29219 (-2.47673 2.82921)
R1^2/D10^2 : 0.147581 (-0.0840349 0.286162)
kT2 [keV] : 33.5153 (-13.1225 -33.8987)
R2^2/D10^2 : 1.17852E-03 (-0.00103852 0.00542754)
------------------------------------------------------------
#Fit statistic : Chi-Squared 45.23 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.24e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.343e-07 7.608e-08
25- 50 5.357e-07 1.703e-07
50-150 1.174e-06 5.918e-07
15-150 1.944e-06 7.936e-07
Peak spectrum fit
Power-law model
Time interval is from 0.924 sec. to 1.924 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.02566 ( -0.33856 0.318031 )
Norm@50keV : 1.06391E-02 ( -0.00179552 0.00178066 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 52.67 using 59 bins.
Reduced chi-squared = 0.924035
# Null hypothesis probability of 6.38e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 1.22670 ( -0.21148 0.21219 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.1403e-07 ( -2.08742e-08 2.10746e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.924 sec. to 1.924 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.03203 ( -0.352536 0.309207 )
Epeak [keV] : 9999.36 ( -9999.36 -9999.36 )
Norm@50keV : 1.07101E-02 ( -0.00177265 0.00997529 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 52.69 using 59 bins.
Reduced chi-squared = 0.940893
# Null hypothesis probability of 6.01e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 1.22646 ( -0.21156 0.21208 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.14525e-07 ( 0 0 ) ergs/cm2
Band function
Time interval is from 0.924 sec. to 1.924 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] : 24.4803 (-6.34 10.0075)
R^2/D10^2 : 2.99647E-02 (-0.0188242 0.0463528)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 64.33 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.35e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.154e-09 1.255e-09
25- 50 1.770e-08 6.483e-09
50-150 7.887e-08 3.094e-08
15-150 9.973e-08 3.709e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-50.2826 -200)
Norm : 5.03477 (-0.869293 0.869293)
------------------------------------------------------------
#Fit statistic : Chi-Squared 61.06 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.32e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.254e-08 7.360e-09
25- 50 2.412e-08 1.384e-08
50-150 5.289e-08 3.002e-08
15-150 8.954e-08 5.070e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.20911 (-2.92728 5.01614)
R1^2/D10^2 : 1.69657 (-1.46098 6.28055)
kT2 [keV] : 40.0453 (-14.755 -40.2993)
R2^2/D10^2 : 6.63060E-03 (-0.0061895 0.0180149)
------------------------------------------------------------
#Fit statistic : Chi-Squared 52.01 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.90e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.048e-08 6.180e-09
25- 50 1.914e-08 1.023e-08
50-150 9.057e-08 5.142e-08
15-150 1.202e-07 6.430e-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: 1.20238 ( -0.113825 0.11219 )
Norm@50keV : 3.76566E-03 ( -0.000248726 0.000248718 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 64.28 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.37e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 45.53 sec: 0.442161 ( -0.0301658 0.0302084 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.73827e-06 ( -1.26016e-07 1.26639e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.688326 ( -0.512059 0.452432 )
Epeak [keV] : 132.237 ( -42.3792 467.082 )
Norm@50keV : 6.73755E-03 ( -0.00264725 0.00510048 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 60.46 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.18e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 45.53 sec: 0.433027 ( -0.031289 0.031267 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.67223e-06 ( -1.374e-07 1.40902e-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) = 4.82e-07
S(50-100 keV) = 6.90e-07
T90 vs. Hardness ratio plot
T90 = 77.6319998502731 sec.
Hardness ratio (energy fluence ratio) = 1.43154
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.27517
Count Ratio (50-100 keV) / (15-25 keV) = 0.924463
Mask shadow pattern
IMX = 6.357669069512054E-02, IMY = -4.101261862489640E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 4.096000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 4.096000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 4.096000
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:
-239.248000 -12.880000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.4338 35.2019 10.5 47.9 46.6 -1.1790 -1.1 8.5 Her X-1
214.2745 -41.8131 2.9 52.5 170.4 2.9341 3.9 ------ UNKNOWN
207.7517 -36.7888 2.8 47.3 176.7 2.4347 4.1 ------ UNKNOWN
187.0102 -40.8221 2.5 55.2 -164.5 3.4845 4.6 ------ UNKNOWN
168.8244 -10.6683 2.5 45.3 -121.4 4.6593 4.5 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-12.880000 32.652600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.3326 35.4610 69.8 47.9 46.3 0.0742 0.2 9.4 Her X-1
232.1121 11.1698 0.5 22.5 81.2 2.7260 22.2 ------ UNKNOWN
230.1933 28.4142 1.9 26.7 39.9 0.7183 6.0 ------ UNKNOWN
229.4525 62.7041 2.8 54.3 6.5 1.3651 4.1 ------ UNKNOWN
180.9339 2.2447 2.3 29.2 -109.2 0.6677 4.9 ------ UNKNOWN
168.8473 -11.5161 2.0 45.7 -122.5 2.3465 6.0 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
181.252600 193.652610
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
299.6717 35.1715 2.5 48.6 144.8 0.8624 4.6 4.4 Cyg X-1
308.0879 40.9613 633.6 40.1 141.5 0.0020 0.0 1.1 Cyg X-3
325.9914 38.4240 4.9 34.9 120.1 -0.2079 -2.4 10.5 Cyg X-2
46.2453 17.4499 2.7 54.0 8.7 0.6831 4.2 ------ UNKNOWN
250.6698 50.2747 2.4 55.0 -166.6 0.6855 4.8 ------ UNKNOWN
Plot creation:
Mon Oct 24 05:21:25 EDT 2022