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
219.0055 33.0584 0.0081 24.2678 -1.9162 1.7823304 23.796 TRIG_01016881
Foreground time interval of the image:
-10.440 15.789 (delta_t = 26.229 [sec])
Background time interval of the image:
-239.112 -10.440 (delta_t = 228.672 [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 1.024000
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 1.024000
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 1.024000
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 -10.440 sec. to 218.472 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.39934 ( -0.0285561 0.0284721 )
Norm@50keV : 1.02253E-02 ( -0.000155511 0.000155235 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 27.67 using 59 bins.
Reduced chi-squared = 0.485439
# Null hypothesis probability of 1.00e+00 with 57 degrees of freedom
Photon flux (15-150 keV) in 228.9 sec: 1.24509 ( -0.02245 0.02252 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.26223e-05 ( -3.32988e-07 3.32665e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -10.440 sec. to 218.472 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.33398 ( -0.115509 0.0867241 )
Epeak [keV] : 621.736 ( -621.79 -621.79 )
Norm@50keV : 1.08773E-02 ( -0.000397896 0.00122201 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 26.71 using 59 bins.
Reduced chi-squared = 0.476964
# Null hypothesis probability of 1.00e+00 with 56 degrees of freedom
Photon flux (15-150 keV) in 228.9 sec: 1.23758 ( -0.02563 0.02439 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.25479e-05 ( -3.55408e-07 3.51604e-07 ) ergs/cm2
Band function
Time interval is from -10.440 sec. to 218.472 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] : 20.0124 ( )
R^2/D10^2 : 5.14068E-02 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 954.33 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.01e-163 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 9.083e-07 3.067e-08
25- 50 4.526e-06 1.122e-07
50-150 1.344e-05 2.850e-07
15-150 1.887e-05 2.781e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.363 ( )
Norm : 5.31753 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared 193.59 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.07e-17 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.031e-06 5.723e-08
25- 50 5.830e-06 1.076e-07
50-150 1.279e-05 2.403e-07
15-150 2.165e-05 3.949e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 8.41008 (-0.489366 0.511618)
R1^2/D10^2 : 0.635232 (-0.113962 0.14555)
kT2 [keV] : 32.9816 (-1.87917 2.23796)
R2^2/D10^2 : 7.81589E-03 (-0.00156154 0.00176558)
------------------------------------------------------------
#Fit statistic : Chi-Squared 37.68 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.64e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.212e-06 1.347e-07
25- 50 5.503e-06 1.614e-07
50-150 1.464e-05 4.052e-07
15-150 2.235e-05 5.207e-07
Peak spectrum fit
Power-law model
Time interval is from 68.864 sec. to 69.864 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.17878 ( -0.0456232 0.0455613 )
Norm@50keV : 0.166048 ( -0.00406879 0.00406738 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 38.36 using 59 bins.
Reduced chi-squared = 0.672982
# Null hypothesis probability of 9.73e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 1.22138 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 1.69508e-06 ( -4.53229e-08 4.54039e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 68.864 sec. to 69.864 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.09671 ( -0.190242 0.0683688 )
Epeak [keV] : 588.514 ( -998.921 -998.921 )
Norm@50keV : 0.180491 ( -0.0188975 0.0328621 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 38.58 using 59 bins.
Reduced chi-squared = 0.688929
# Null hypothesis probability of 9.63e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 19.3885 ( -0.5422 0.5041 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.69075e-06 ( -4.79678e-08 4.71309e-08 ) ergs/cm2
Band function
Time interval is from 68.864 sec. to 69.864 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] : 20.0948 ( )
R^2/D10^2 : 0.870920 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 370.65 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.56e-47 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.767e-08 3.465e-09
25- 50 3.381e-07 1.180e-08
50-150 1.013e-06 4.335e-08
15-150 1.419e-06 4.400e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.363 ( )
Norm : 81.3064 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared 240.34 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.28e-24 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.025e-07 5.400e-09
25- 50 3.895e-07 1.055e-08
50-150 8.542e-07 2.180e-08
15-150 1.446e-06 3.950e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 8.81159 (-0.912524 0.982563)
R1^2/D10^2 : 7.73840 (-2.06405 3.11705)
kT2 [keV] : 36.8494 (-4.10943 5.92318)
R2^2/D10^2 : 0.104333 (-0.0381513 0.0483207)
------------------------------------------------------------
#Fit statistic : Chi-Squared 45.79 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.07e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.350e-07 1.235e-08
25- 50 3.666e-07 1.995e-08
50-150 1.193e-06 9.500e-08
15-150 1.695e-06 1.100e-07
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: 1.28117 ( -0.10057 0.0999212 )
Norm@50keV : 4.65163E-03 ( -0.000284095 0.000284061 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 86.88 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.56e-03 with 57 degrees of freedom
Photon flux (15-150 keV) in 26.23 sec: 0.553072 ( -0.0347298 0.0347796 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.21134e-06 ( -8.09969e-08 8.13466e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.155506 ( -0.546594 0.483967 )
Epeak [keV] : 84.6570 ( -12.8098 26.2657 )
Norm@50keV : 1.64943E-02 ( -0.00679587 0.0134318 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 68.73 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.18e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 26.23 sec: 0.528469 ( -0.036336 0.036326 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.12317e-06 ( -8.96384e-08 9.01578e-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) = 5.31e-06
S(50-100 keV) = 8.06e-06
T90 vs. Hardness ratio plot
T90 = 107.599999904633 sec.
Hardness ratio (energy fluence ratio) = 1.51789
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.45069
Count Ratio (50-100 keV) / (15-25 keV) = 1.1845
Mask shadow pattern
IMX = 4.505885202684413E-01, IMY = 1.507483326274372E-02
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.024000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.024000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.024000
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:
-239.112000 -10.440000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.3068 35.4287 7.7 27.0 -72.7 0.5093 1.5 9.0 Her X-1
197.4932 48.1564 2.7 20.7 57.5 1.2077 4.3 ------ UNKNOWN
323.1135 45.9647 5.2 55.2 -145.1 3.2348 2.2 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-10.440000 15.788600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.5318 35.2882 25.6 27.2 -72.9 -0.0446 -0.4 4.9 Her X-1
169.9945 57.5781 2.4 31.2 94.7 0.5649 4.8 ------ UNKNOWN
219.0055 33.0584 0.5 24.3 -1.9 1.7822 23.8 ------ UNKNOWN
247.8556 29.9497 2.1 29.5 -57.3 0.5217 5.6 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
63.188590 715.982000
720.888000 963.006100
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.5415 35.2105 51.0 29.4 -130.2 -0.2971 -0.2 8.9 Her X-1
191.2839 -13.7707 3.3 53.8 8.0 9.1435 3.5 ------ UNKNOWN
219.0020 33.0404 0.3 0.0 -66.7 31.6984 35.8 ------ UNKNOWN
226.1683 -10.8418 2.2 44.4 -36.1 9.1825 5.3 ------ UNKNOWN
289.0790 40.2559 4.2 55.2 -145.1 14.9515 2.8 ------ UNKNOWN
237.4893 -11.5700 3.1 48.0 -50.7 14.9246 3.7 ------ UNKNOWN
Plot creation:
Sat Jul 30 07:19:24 EDT 2022