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
20.8341 27.7220 0.0235 14.7395 -14.7838 0.6958510 8.179 TRIG_01000255
Foreground time interval of the image:
30.164 69.840 (delta_t = 39.676 [sec])
Background time interval of the image:
-143.699 30.164 (delta_t = 173.863 [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
8 ms binning
From T100_start-3 s to T100_start+3 s
2 ms binning
From T100_start-1 s to T100_start+1 s
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 30.164 sec. to 69.840 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.54960 ( -0.342528 0.396749 )
Norm@50keV : 7.63774E-04 ( -0.00022885 0.000233972 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 50.77 using 59 bins.
Reduced chi-squared = 0.890702
# Null hypothesis probability of 7.06e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 39.68 sec: 0.154740 ( -0.025303 0.02536 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.07356e-07 ( -6.57926e-08 7.07657e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 30.164 sec. to 69.840 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.696954 ( -3.59785 1.31087 )
Epeak [keV] : 21.1615 ( -20.289 7.72568 )
Norm@50keV : 1.48962E-02 ( -0.0157064 7.14099 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 48.56 using 59 bins.
Reduced chi-squared = 0.867143
# Null hypothesis probability of 7.49e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 39.68 sec: 0.149686 ( -0.0246 0.025095 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.58185e-07 ( -5.59758e-08 8.18479e-08 ) ergs/cm2
Band function
Time interval is from 30.164 sec. to 69.840 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] : 6.27132 (-1.00528 1.18902)
R^2/D10^2 : 0.476301 (-0.246901 0.526842)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 50.09 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.30e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.050e-07 3.301e-08
25- 50 1.151e-07 3.649e-08
50-150 1.259e-08 8.183e-09
15-150 2.326e-07 6.537e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 26.3901 (-8.31133 13.7581)
Norm : 1.40621 (-0.430496 0.688058)
------------------------------------------------------------
#Fit statistic : Chi-Squared 48.76 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.73e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.057e-07 2.309e-08
25- 50 1.121e-07 3.016e-08
50-150 5.154e-08 3.349e-08
15-150 2.694e-07 7.801e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.09482 (-5.14758 1.85843)
R1^2/D10^2 : 0.926221 (-0.895646 -0.895646)
kT2 [keV] : 13.5503 (-14.1138 -14.1138)
R2^2/D10^2 : 7.80910E-03 (-0.00643241 0.624769)
------------------------------------------------------------
#Fit statistic : Chi-Squared 47.78 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.44e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.084e-07 6.262e-08
25- 50 1.092e-07 5.887e-08
50-150 5.445e-08 3.327e-08
15-150 2.720e-07 1.464e-07
Peak spectrum fit
Power-law model
Time interval is from 59.440 sec. to 60.440 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.19005 ( -1.11809 1.77313 )
Norm@50keV : 1.97185E-03 ( -0.00197067 0.00147387 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 56.32 using 59 bins.
Reduced chi-squared = 0.98807
# Null hypothesis probability of 5.00e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.324762 ( -0.154211 0.154048 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.85089e-08 ( -1.13391e-08 1.37783e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 59.440 sec. to 60.440 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.98699 ( )
Epeak [keV] : 25.9604 ( )
Norm@50keV : 2.24315E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared 56.42 using 59 bins.
Reduced chi-squared = 1.0075
# Null hypothesis probability of 4.59e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.296347 ( -0.296347 0.161191 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.80443e-08 ( -1.6856e-08 1.09051e-08 ) ergs/cm2
Band function
Time interval is from 59.440 sec. to 60.440 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] : 6.51328 (-3.27602 6.66419)
R^2/D10^2 : 0.779974 (-0.775798 17.3111)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 57.90 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.42e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.902e-09 3.037e-09
25- 50 5.814e-09 3.983e-09
50-150 7.369e-10 7.515e-10
15-150 1.145e-08 7.770e-09
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 41.5936 (-41.9919 -41.9919)
Norm : 1.99408 (-1.27063 7.38263)
------------------------------------------------------------
#Fit statistic : Chi-Squared 56.98 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.76e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.638e-09 2.989e-09
25- 50 6.204e-09 4.185e-09
50-150 5.006e-09 4.585e-09
15-150 1.585e-08 1.087e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.61945 (-3.25386 4.46504)
R1^2/D10^2 : 1.34610 (-1.37384 91.3637)
kT2 [keV] : 200.000 (-200 -200)
R2^2/D10^2 : 5.64889E-05 (-2.82457e-05 0.000465737)
------------------------------------------------------------
#Fit statistic : Chi-Squared 55.11 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.71e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.216e-09 3.288e-09
25- 50 4.929e-09 3.245e-09
50-150 1.542e-08 1.047e-08
15-150 2.556e-08 1.384e-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: 2.54960 ( -0.342528 0.396749 )
Norm@50keV : 7.63774E-04 ( -0.00022885 0.000233972 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 50.77 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.06e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 39.68 sec: 0.154717 ( -0.0253006 0.0253573 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.07276e-07 ( -6.57827e-08 7.08236e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.693945 ( -3.59573 1.54136 )
Epeak [keV] : 21.1732 ( -21.0252 7.71363 )
Norm@50keV : 1.49716E-02 ( -0.01573 7.1414 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 48.56 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.49e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 39.68 sec: 0.149641 ( -0.024584 0.025073 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.582e-07 ( -5.60623e-08 8.28844e-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) = 1.02e-07
S(50-100 keV) = 6.98e-08
T90 vs. Hardness ratio plot
T90 = 36.1959998607635 sec.
Hardness ratio (energy fluence ratio) = 0.684314
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 0.682981
Count Ratio (50-100 keV) / (15-25 keV) = 0.0953286
Mask shadow pattern
IMX = 2.543736476525352E-01, IMY = 6.713140143594612E-02
TIME vs. PHA plot around the trigger time
TIME vs. DetID plot around the trigger time
100 us light curve (15-350 keV)
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:
-143.699400 30.164000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
34.3986 50.8998 2.8 39.4 -0.8 1.1911 4.2 ------ UNKNOWN
30.9102 47.9233 2.5 35.9 -2.8 1.2567 4.5 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
30.164000 69.840000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
21.1331 -40.1339 1.9 53.1 165.8 2.1541 6.0 ------ UNKNOWN
20.8341 27.7220 1.4 14.7 -14.8 0.6959 8.2 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
153.500600 864.200600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6405 22.0295 1.1 56.6 -10.5 23.4354 10.0 1.0 Crab
326.1782 38.2412 5.8 46.4 -153.4 -2.6695 -2.0 4.8 Cyg X-2
11.3576 -6.4888 3.4 35.4 105.3 4.0270 3.4 ------ UNKNOWN
56.3477 4.9141 3.1 40.7 26.3 3.6720 3.8 ------ UNKNOWN
326.2221 18.5741 2.4 50.7 -179.1 7.9622 4.9 ------ UNKNOWN
36.5873 57.7850 3.1 32.1 -75.4 3.5047 3.7 ------ UNKNOWN
84.3766 46.7581 3.6 52.5 -40.6 9.3959 3.2 ------ UNKNOWN
319.8768 51.7604 3.2 50.9 -135.4 11.6592 3.6 ------ UNKNOWN
74.3280 56.0888 2.8 47.2 -53.5 11.4071 4.2 ------ UNKNOWN
Plot creation:
Sat Jul 30 07:31:34 EDT 2022