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
86.9192 -65.4532 0.0260 21.1227 98.4774 1.0856255 7.360 TRIG_01044032
Foreground time interval of the image:
22.792 73.901 (delta_t = 51.109 [sec])
Background time interval of the image:
-15.699 22.792 (delta_t = 38.491 [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 22.792 sec. to 111.424 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.14412 ( -0.227071 0.245514 )
Norm@50keV : 1.01565E-03 ( -0.000175342 0.000171597 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 57.68 using 59 bins.
Reduced chi-squared = 1.01193
# Null hypothesis probability of 4.50e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 88.63 sec: 0.163372 ( -0.019444 0.019445 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.40448e-07 ( -1.25868e-07 1.30175e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from 22.792 sec. to 111.424 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.25578 ( -1.36938 0.70541 )
Epeak [keV] : 31.4925 ( -9.37503 15.6438 )
Norm@50keV : 3.58696E-03 ( -0.00358731 0.0226514 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 55.56 using 59 bins.
Reduced chi-squared = 0.992143
# Null hypothesis probability of 4.92e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 88.63 sec: 0.158870 ( -0.019907 0.02004 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.60993e-07 ( -1.34249e-07 1.55609e-07 ) ergs/cm2
Band function
Time interval is from 22.792 sec. to 111.424 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] : 8.60625 (-1.11761 1.27273)
R^2/D10^2 : 0.136028 (-0.056856 0.099089)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 64.58 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.29e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.696e-07 3.532e-08
25- 50 3.356e-07 5.389e-08
50-150 1.114e-07 4.166e-08
15-150 6.166e-07 1.027e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 48.7150 (-13.7333 22.8779)
Norm : 0.943588 (-0.180148 0.241766)
------------------------------------------------------------
#Fit statistic : Chi-Squared 55.55 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.30e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.032e-07 3.310e-08
25- 50 2.892e-07 4.321e-08
50-150 2.739e-07 1.020e-07
15-150 7.663e-07 1.353e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 4.87380 (-2.16891 2.77949)
R1^2/D10^2 : 0.784909 (-0.592311 8.74656)
kT2 [keV] : 13.7930 (-4.13309 23.7617)
R2^2/D10^2 : 1.47625E-02 (-0.0144773 0.0609213)
------------------------------------------------------------
#Fit statistic : Chi-Squared 55.75 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.47e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.052e-07 1.124e-07
25- 50 2.864e-07 1.448e-07
50-150 2.431e-07 1.450e-07
15-150 7.348e-07 3.677e-07
Peak spectrum fit
Power-law model
Time interval is from 41.820 sec. to 42.820 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.66756 ( -0.502535 0.546093 )
Norm@50keV : 4.53626E-03 ( -0.0015954 0.00154077 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 45.82 using 59 bins.
Reduced chi-squared = 0.80386
# Null hypothesis probability of 8.56e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.595821 ( -0.187587 0.187722 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.2124e-08 ( -1.50252e-08 1.56045e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 41.820 sec. to 42.820 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.455432 ( -3.21205 1.7488 )
Epeak [keV] : 58.4775 ( -58.4782 -58.4782 )
Norm@50keV : 2.07820E-02 ( -0.0207811 1.05877 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 44.80 using 59 bins.
Reduced chi-squared = 0.8
# Null hypothesis probability of 8.59e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.581422 ( -0.18912 0.189239 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.904e-08 ( -1.44686e-08 1.62632e-08 ) ergs/cm2
Band function
Time interval is from 41.820 sec. to 42.820 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] : 13.1503 (-4.03416 5.70566)
R^2/D10^2 : 0.111901 (-0.11175 0.303721)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 46.09 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.49e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.103e-09 2.589e-09
25- 50 1.431e-08 8.559e-09
50-150 1.575e-08 1.075e-08
15-150 3.416e-08 2.213e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 142.990 (-86.9237 -131.981)
Norm : 2.43544 (-0.838588 1.28881)
------------------------------------------------------------
#Fit statistic : Chi-Squared 45.27 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.69e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.279e-09 3.774e-09
25- 50 1.156e-08 7.065e-09
50-150 2.236e-08 1.457e-08
15-150 4.019e-08 2.555e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.10739 (-5.07681 178.607)
R1^2/D10^2 : 1.58257 (-1.59216 -1.59216)
kT2 [keV] : 17.1162 (-17.0887 -17.0887)
R2^2/D10^2 : 3.57911E-02 (-0.0359271 0.217457)
------------------------------------------------------------
#Fit statistic : Chi-Squared 44.48 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.44e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.319e-09 3.614e-09
25- 50 1.236e-08 6.800e-09
50-150 2.001e-08 1.381e-08
15-150 3.869e-08 2.125e-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: 2.10867 ( -0.261203 0.286146 )
Norm@50keV : 1.22667E-03 ( -0.000243163 0.000236376 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 58.38 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.24e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 51.11 sec: 0.193817 ( -0.0267387 0.0267401 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.83002e-07 ( -1.01163e-07 1.0515e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.17750 ( -1.72828 0.93285 )
Epeak [keV] : 33.7868 ( -31.7279 -33.7912 )
Norm@50keV : 4.53767E-03 ( -0.00454528 0.0484911 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 56.93 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.40e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 51.11 sec: 0.188129 ( -0.027565 0.027747 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.27333e-07 ( -1.05481e-07 1.28726e-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) = 2.63e-07
S(50-100 keV) = 2.38e-07
T90 vs. Hardness ratio plot
T90 = 71.0759999752045 sec.
Hardness ratio (energy fluence ratio) = 0.904943
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 0.933131
Count Ratio (50-100 keV) / (15-25 keV) = 0.354592
Mask shadow pattern
IMX = -5.695155266419270E-02, IMY = -3.821016374942349E-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:
-15.699400 22.792000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
22.792000 73.900600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
86.9193 -65.4532 1.6 21.1 98.5 1.0858 7.3 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
117.300600 963.147900
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.4526 -40.5070 3.8 36.9 39.6 3.4563 3.0 4.5 Vela X-1
170.3418 -60.6207 26.6 35.3 90.4 0.6311 0.4 0.8 Cen X-3
186.3189 -62.8209 10.5 38.9 102.0 -2.1218 -1.1 9.8 GX 301-2
183.1067 -59.0897 2.5 40.8 96.4 11.0182 4.7 ------ UNKNOWN
157.0866 -76.5499 3.9 23.4 114.4 2.5945 3.0 ------ UNKNOWN
128.7830 -63.4427 3.0 17.9 70.7 2.8374 3.8 ------ UNKNOWN
57.4225 -77.6226 4.1 14.9 172.0 1.5553 2.8 ------ UNKNOWN
330.0819 -45.0329 2.9 59.2 -164.9 20.4140 3.9 ------ UNKNOWN
Plot creation:
Sat Jul 30 07:05:58 EDT 2022