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
229.6052 44.4687 0.0162 10.3325 124.7488 2.5193623 11.834 TRIG_01003002
Foreground time interval of the image:
-2.192 73.101 (delta_t = 75.293 [sec])
Background time interval of the image:
-18.099 -2.192 (delta_t = 15.907 [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 64.000000
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 64.000000
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 64.000000
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 -2.192 sec. to 510.784 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.39682 ( -0.14616 0.146333 )
Norm@50keV : 5.91902E-04 ( -4.65111e-05 4.63494e-05 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 66.75 using 59 bins.
Reduced chi-squared = 1.17105
# Null hypothesis probability of 1.77e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 513 sec: 7.20321E-02 ( -0.0056816 0.0056956 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.93628e-06 ( -2.60271e-07 2.62965e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -2.192 sec. to 510.784 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.39852 ( -0.177415 0.142965 )
Epeak [keV] : 9999.29 ( -9999.35 -9999.35 )
Norm@50keV : 5.93646E-04 ( -0.000593716 0.000215289 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 66.77 using 59 bins.
Reduced chi-squared = 1.19232
# Null hypothesis probability of 1.54e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 513 sec: 7.25812E-02 ( -0.0062463 0.0051319 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.93526e-06 ( -2.60918e-07 2.62803e-07 ) ergs/cm2
Band function
Time interval is from -2.192 sec. to 510.784 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] : 16.5545 ( )
R^2/D10^2 : 5.70342E-03 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 121.93 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.27e-06 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.645e-07 2.811e-08
25- 50 7.121e-07 8.413e-08
50-150 1.381e-06 2.083e-07
15-150 2.258e-06 2.252e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-31.6131 -200)
Norm : 0.295306 (-0.0228805 0.0228805)
------------------------------------------------------------
#Fit statistic : Chi-Squared 72.86 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.67e-02 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.772e-07 3.678e-08
25- 50 7.256e-07 2.865e-07
50-150 1.591e-06 6.561e-07
15-150 2.694e-06 7.764e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.95760 (-1.46158 2.05766)
R1^2/D10^2 : 0.135208 (-0.0869215 0.279005)
kT2 [keV] : 29.0388 (-6.13104 13.2262)
R2^2/D10^2 : 7.64239E-04 (-0.000519166 0.000918533)
------------------------------------------------------------
#Fit statistic : Chi-Squared 68.88 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.88e-02 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.765e-07 1.454e-07
25- 50 6.389e-07 1.486e-07
50-150 1.964e-06 6.761e-07
15-150 2.979e-06 7.800e-07
Peak spectrum fit
Power-law model
Time interval is from 7.060 sec. to 8.060 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.00927 ( -0.405116 0.380391 )
Norm@50keV : 5.17039E-03 ( -0.00109769 0.00109191 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 87.96 using 59 bins.
Reduced chi-squared = 1.54316
# Null hypothesis probability of 5.29e-03 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.595563 ( -0.128224 0.128716 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.57327e-08 ( -1.29577e-08 1.31135e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 7.060 sec. to 8.060 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.34499 ( -2.66824 6.16859 )
Epeak [keV] : 112.363 ( )
Norm@50keV : 7.24235E-04 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared 87.82 using 59 bins.
Reduced chi-squared = 1.56821
# Null hypothesis probability of 4.22e-03 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.599405 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 5.58882e-08 ( -1.35824e-08 1.06728e-08 ) ergs/cm2
Band function
Time interval is from 7.060 sec. to 8.060 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] : 22.5964 (-6.50014 10.6291)
R^2/D10^2 : 1.91810E-02 (-0.0130782 0.0366744)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 93.74 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.56e-03 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.790e-09 7.662e-10
25- 50 9.614e-09 4.573e-09
50-150 3.668e-08 1.662e-08
15-150 4.809e-08 1.975e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-67.6985 -200)
Norm : 2.40302 (-0.528183 0.528183)
------------------------------------------------------------
#Fit statistic : Chi-Squared 93.57 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.62e-03 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.983e-09 3.555e-09
25- 50 1.151e-08 6.930e-09
50-150 2.524e-08 1.520e-08
15-150 4.274e-08 2.511e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 9.24310 (-6.46311 8.10795)
R1^2/D10^2 : 0.204716 (-0.159951 16.1498)
kT2 [keV] : 47.6206 (-46.7399 -49.6903)
R2^2/D10^2 : 1.82651E-03 (-0.00157226 0.0174229)
------------------------------------------------------------
#Fit statistic : Chi-Squared 87.94 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.16e-03 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.920e-09 2.311e-09
25- 50 1.100e-08 6.180e-09
50-150 4.220e-08 2.293e-08
15-150 5.712e-08 2.927e-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: 1.06216 ( -0.101028 0.0997358 )
Norm@50keV : 2.22942E-03 ( -0.000125982 0.000125818 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 72.07 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.63e-02 with 57 degrees of freedom
Photon flux (15-150 keV) in 75.29 sec: 0.257734 ( -0.014993 0.0150207 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.7767e-06 ( -1.08223e-07 1.08701e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.446996 ( -0.488991 0.436076 )
Epeak [keV] : 144.885 ( -39.8705 195.804 )
Norm@50keV : 4.16069E-03 ( -0.0014575 0.00253501 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 66.05 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.68e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 75.29 sec: 0.249714 ( -0.016045 0.016013 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.71823e-06 ( -1.18499e-07 1.17784e-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) = 6.87e-07
S(50-100 keV) = 1.05e-06
T90 vs. Hardness ratio plot
T90 = 491.023999929428 sec.
Hardness ratio (energy fluence ratio) = 1.52838
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.1389
Count Ratio (50-100 keV) / (15-25 keV) = 0.969635
Mask shadow pattern
IMX = -1.039163475633133E-01, IMY = -1.498015237863478E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 64.000000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 64.000000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 64.000000
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:
-18.099400 -2.192000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.4299 35.4838 4.4 26.3 173.5 -0.1193 -2.6 8.6 Her X-1
270.6549 61.8681 2.2 39.7 125.9 0.5664 5.2 ------ UNKNOWN
283.9282 38.2153 2.1 48.6 159.9 0.6578 5.4 ------ UNKNOWN
272.1114 2.7338 2.1 57.0 -154.1 1.3691 5.4 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-2.192000 73.100590
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.3849 35.5030 11.3 26.3 173.6 0.2331 1.0 10.3 Her X-1
229.6052 44.4687 1.0 10.3 124.7 2.5185 11.8 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
110.700600 963.060800
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.3886 35.2122 5.3 21.1 -179.3 -1.4241 -2.2 8.5 Her X-1
246.3351 83.8401 3.1 39.7 76.0 9.1562 3.7 ------ UNKNOWN
289.8134 53.4219 3.6 39.3 128.0 5.5007 3.2 ------ UNKNOWN
199.3092 43.7165 3.1 21.6 -8.0 2.4005 3.8 ------ UNKNOWN
154.7637 31.4526 2.6 58.3 -2.1 15.5176 4.5 ------ UNKNOWN
245.9913 -1.2657 2.7 48.0 -129.1 12.2213 4.4 ------ UNKNOWN
Plot creation:
Sat Jul 30 07:27:10 EDT 2022