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
16.3642 16.5373 0.0049 52.0287 -21.5613 65.8487229 39.142 TRIG_01013243
Foreground time interval of the image:
-15.888 64.112 (delta_t = 80.000 [sec])
Background time interval of the image:
-64.787 -15.888 (delta_t = 48.899 [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 -15.888 sec. to 64.112 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.43475 ( -0.0301378 0.0300528 )
Norm@50keV : 5.87778E-02 ( -0.000995505 0.000994116 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 41.82 using 59 bins.
Reduced chi-squared = 0.733684
# Null hypothesis probability of 9.34e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 80 sec: 7.21670 ( -0.1462 0.14677 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.51315e-05 ( -7.30802e-07 7.30163e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -15.888 sec. to 64.112 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.32336 ( -0.124266 0.0898119 )
Epeak [keV] : 379.489 ( -166.024 -379.982 )
Norm@50keV : 6.52175E-02 ( -0.00661928 0.00782546 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 39.39 using 59 bins.
Reduced chi-squared = 0.703393
# Null hypothesis probability of 9.55e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 80 sec: 3.53302 ( -0.27854 0.41676 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.49614e-05 ( -7.54547e-07 7.5264e-07 ) ergs/cm2
Band function
Time interval is from -15.888 sec. to 64.112 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] : 20.0703 ( )
R^2/D10^2 : 0.295689 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 844.31 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.35e-140 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.834e-06 6.840e-08
25- 50 9.158e-06 2.400e-07
50-150 2.736e-05 6.160e-07
15-150 3.835e-05 6.560e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.363 ( )
Norm : 30.7806 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared 154.35 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.56e-11 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.132e-06 1.232e-07
25- 50 1.180e-05 2.320e-07
50-150 2.587e-05 5.200e-07
15-150 4.380e-05 9.280e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 9.12357 (-0.575062 0.600779)
R1^2/D10^2 : 2.89050 (-0.533781 0.692836)
kT2 [keV] : 35.1036 (-2.41889 3.00309)
R2^2/D10^2 : 3.48391E-02 (-0.00845495 0.00987972)
------------------------------------------------------------
#Fit statistic : Chi-Squared 55.60 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.52e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.259e-06 2.576e-07
25- 50 1.137e-05 3.480e-07
50-150 2.883e-05 1.044e-06
15-150 4.446e-05 1.284e-06
Peak spectrum fit
Power-law model
Time interval is from 23.612 sec. to 24.612 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.74652 ( -0.101919 0.103787 )
Norm@50keV : 0.133576 ( -0.00833673 0.00829755 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 49.21 using 59 bins.
Reduced chi-squared = 0.863333
# Null hypothesis probability of 7.59e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 18.0394 ( -1.1323 1.1346 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.23299e-06 ( -7.9032e-08 7.93005e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 23.612 sec. to 24.612 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.37120 ( -0.443034 0.403578 )
Epeak [keV] : 85.6267 ( -22.9349 -85.6268 )
Norm@50keV : 0.205916 ( -0.0745458 0.133715 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 46.72 using 59 bins.
Reduced chi-squared = 0.834286
# Null hypothesis probability of 8.07e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 17.7512 ( -1.1717 1.1748 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.21143e-06 ( -8.35575e-08 8.32129e-08 ) ergs/cm2
Band function
Time interval is from 23.612 sec. to 24.612 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] : 13.5199 (-0.993716 1.07875)
R^2/D10^2 : 2.83227 (-0.695175 0.917637)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 113.39 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.31e-05 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.097e-07 1.216e-08
25- 50 3.936e-07 3.060e-08
50-150 4.651e-07 5.355e-08
15-150 9.683e-07 7.160e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 119.122 (-23.5375 46.1474)
Norm : 78.1321 (-6.51508 6.06892)
------------------------------------------------------------
#Fit statistic : Chi-Squared 47.08 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.23e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.036e-07 2.005e-08
25- 50 3.637e-07 2.545e-08
50-150 6.467e-07 1.848e-07
15-150 1.214e-06 2.034e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.45728 (-1.40732 1.46713)
R1^2/D10^2 : 16.9784 (-7.43898 17.4625)
kT2 [keV] : 26.0132 (-5.05867 9.16867)
R2^2/D10^2 : 0.181431 (-0.12206 0.251888)
------------------------------------------------------------
#Fit statistic : Chi-Squared 49.01 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.02e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.821e-07 3.770e-08
25- 50 3.696e-07 6.595e-08
50-150 6.536e-07 2.047e-07
15-150 1.205e-06 2.686e-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: 1.43475 ( -0.0301378 0.0300528 )
Norm@50keV : 5.87778E-02 ( -0.000995505 0.000994116 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 41.82 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.34e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 80 sec: 7.21655 ( -0.146178 0.146752 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.51255e-05 ( -7.30401e-07 7.3038e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.32351 ( -0.124283 0.0898591 )
Epeak [keV] : 379.943 ( -166.021 -379.988 )
Norm@50keV : 6.52083E-02 ( -0.00661925 0.00782546 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 39.39 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.55e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 80 sec: 7.14596 ( -0.16265 0.16278 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.49786e-05 ( -7.544e-07 7.5352e-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) = 1.08e-05
S(50-100 keV) = 1.60e-05
T90 vs. Hardness ratio plot
T90 = 48 sec.
Hardness ratio (energy fluence ratio) = 1.48148
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.64473
Count Ratio (50-100 keV) / (15-25 keV) = 1.52907
Mask shadow pattern
IMX = 1.191606335249240E+00, IMY = 4.708600849302003E-01
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:
-64.787400 -15.888000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6412 22.0336 0.7 22.4 91.8 2.2309 16.4 1.2 Crab
84.7449 26.3161 0.8 26.2 86.7 2.4201 15.3 ------ UNKNOWN
21.5259 15.7663 3.4 47.0 -21.8 0.7208 3.4 ------ UNKNOWN
67.5302 -35.4626 2.8 40.8 -127.5 0.9369 4.2 ------ UNKNOWN
10.4449 12.4666 3.2 57.5 -27.0 2.5209 3.7 ------ UNKNOWN
73.5303 -43.5646 4.2 49.1 -133.4 1.4418 2.8 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-15.888000 64.112000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.4850 22.0597 4.9 22.3 91.5 -1.0470 -2.3 8.7 Crab
81.9503 40.5093 3.5 37.3 68.9 2.1667 3.3 ------ UNKNOWN
55.4331 50.9856 2.8 46.9 40.5 3.9919 4.2 ------ UNKNOWN
113.0326 7.4604 3.3 44.5 136.4 3.2678 3.6 ------ UNKNOWN
113.6999 -10.7283 2.6 48.0 161.2 3.5870 4.4 ------ UNKNOWN
90.7644 8.6557 2.4 22.6 131.8 2.0142 4.9 ------ UNKNOWN
79.9221 8.8076 4.1 12.1 124.2 1.0963 2.9 ------ UNKNOWN
70.1673 8.8767 4.1 4.0 79.4 1.0914 2.8 ------ UNKNOWN
15.2071 36.5044 2.5 57.6 2.0 9.6282 4.5 ------ UNKNOWN
116.7305 -27.2148 3.1 57.0 179.1 7.2170 3.7 ------ UNKNOWN
67.8460 -12.7408 2.3 18.1 -127.1 2.2652 5.0 ------ UNKNOWN
76.1814 -21.9285 2.8 28.3 -144.0 2.2308 4.1 ------ UNKNOWN
16.3642 16.5373 0.3 52.0 -21.6 65.8426 39.1 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
626.412590 962.222000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
139.2370 -32.3417 3.7 56.8 -1.8 4.1336 3.1 ------ UNKNOWN
154.7482 -30.6369 3.6 56.5 -17.7 4.0381 3.2 ------ UNKNOWN
168.2581 1.0350 2.6 34.9 -56.0 2.4006 4.5 ------ UNKNOWN
Plot creation:
Sat Jul 30 07:23:45 EDT 2022