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
235.7636 46.0686 0.0172 13.1367 -156.5186 0.3045533 11.211 TRIG_01056426
Foreground time interval of the image:
-1.420 0.928 (delta_t = 2.348 [sec])
Background time interval of the image:
-119.224 -1.420 (delta_t = 117.804 [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 0.512000
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 0.512000
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 0.512000
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 -1.420 sec. to 0.928 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.21642 ( -0.277633 0.277341 )
Norm@50keV : 7.27312E-03 ( -0.0011086 0.00109778 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 58.67 using 59 bins.
Reduced chi-squared = 1.0293
# Null hypothesis probability of 4.14e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 2.348 sec: 0.855746 ( -0.125859 0.125866 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.72484e-07 ( -3.13639e-08 3.23533e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -1.420 sec. to 0.928 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.19306 ( -0.905237 2.57022 )
Epeak [keV] : 9980.86 ( -9999.34 -9999.34 )
Norm@50keV : 7.48632E-03 ( -0.00111629 0.0138709 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 58.75 using 59 bins.
Reduced chi-squared = 1.04911
# Null hypothesis probability of 3.75e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 2.348 sec: 0.862351 ( -0.160819 0.146439 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.75723e-07 ( -3.99857e-08 1.75801e-08 ) ergs/cm2
Band function
Time interval is from -1.420 sec. to 0.928 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] : 14.9169 (-2.86169 4.03634)
R^2/D10^2 : 9.92771E-02 (-0.0539325 0.103871)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 69.72 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.20e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.087e-08 3.342e-09
25- 50 4.297e-08 9.909e-09
50-150 6.490e-08 2.317e-08
15-150 1.187e-07 2.706e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-61.7845 -200)
Norm : 3.39870 (-0.509233 0.509233)
------------------------------------------------------------
#Fit statistic : Chi-Squared 62.46 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.88e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.994e-08 1.135e-08
25- 50 3.836e-08 2.152e-08
50-150 8.412e-08 4.778e-08
15-150 1.424e-07 7.987e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 10.1695 (-2.55741 2.97441)
R1^2/D10^2 : 0.293958 (-0.195893 0.511647)
kT2 [keV] : 200.000 (-200 -200)
R2^2/D10^2 : 1.68992E-04 (-3.56596e-05 0.000732271)
------------------------------------------------------------
#Fit statistic : Chi-Squared 56.07 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.35e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.548e-08 8.311e-09
25- 50 4.095e-08 2.209e-08
50-150 1.272e-07 9.625e-08
15-150 1.836e-07 1.078e-07
Peak spectrum fit
Power-law model
Time interval is from -0.496 sec. to 0.504 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.13629 ( -0.334275 0.327105 )
Norm@50keV : 9.66315E-03 ( -0.00171649 0.00170542 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 89.46 using 59 bins.
Reduced chi-squared = 1.56947
# Null hypothesis probability of 3.89e-03 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 1.12513 ( -0.196245 0.19627 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.9901e-08 ( -2.12942e-08 2.20092e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.496 sec. to 0.504 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.13986 ( -0.343868 0.321894 )
Epeak [keV] : 9999.36 ( -9999.36 -9999.36 )
Norm@50keV : 9.67663E-03 ( -0.00170019 0.0154577 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 89.47 using 59 bins.
Reduced chi-squared = 1.59768
# Null hypothesis probability of 2.98e-03 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 1.13193 ( -0.22569 0.20852 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.43596e-08 ( -1.76194e-08 8.47109e-09 ) ergs/cm2
Band function
Time interval is from -0.496 sec. to 0.504 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] : 16.9650 (-5.00283 8.52474)
R^2/D10^2 : 8.45835E-02 (-0.0827466 0.179053)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 101.47 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.65e-04 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.961e-09 1.909e-09
25- 50 2.191e-08 8.429e-09
50-150 4.500e-08 1.802e-08
15-150 7.187e-08 2.404e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-67.9927 -200)
Norm : 4.41937 (-0.79217 0.79217)
------------------------------------------------------------
#Fit statistic : Chi-Squared 93.73 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.57e-03 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.104e-08 6.475e-09
25- 50 2.124e-08 1.209e-08
50-150 4.658e-08 2.704e-08
15-150 7.886e-08 4.541e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.64736 (-2.25177 3.12988)
R1^2/D10^2 : 0.870527 (-0.592498 2.0578)
kT2 [keV] : 50.3801 (-23.0716 -50.3908)
R2^2/D10^2 : 3.06854E-03 (-0.00274975 0.00751709)
------------------------------------------------------------
#Fit statistic : Chi-Squared 86.29 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.47e-03 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 9.729e-09 5.550e-09
25- 50 2.048e-08 1.120e-08
50-150 7.858e-08 4.250e-08
15-150 1.088e-07 5.805e-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: 1.21642 ( -0.277633 0.277341 )
Norm@50keV : 7.27312E-03 ( -0.0011086 0.00109778 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 58.67 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.14e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 2.348 sec: 0.855741 ( -0.125857 0.125864 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.72463e-07 ( -3.13519e-08 3.2359e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.22261 ( -0.286613 0.272046 )
Epeak [keV] : 9999.36 ( -9999.36 -9999.36 )
Norm@50keV : 7.27690E-03 ( -0.00110874 0.0138845 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 58.68 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.77e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 2.348 sec: 0.855523 ( -0.125802 0.125777 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.71904e-07 ( -3.36306e-08 3.23968e-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) = 3.66e-08
S(50-100 keV) = 6.29e-08
T90 vs. Hardness ratio plot
T90 = 2.13199996948242 sec.
Hardness ratio (energy fluence ratio) = 1.71858
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.70423
Count Ratio (50-100 keV) / (15-25 keV) = 1.22228
Mask shadow pattern
IMX = -2.140563135164859E-01, IMY = 9.299182024394913E-02
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.512000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.512000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.512000
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:
-119.224000 -1.420000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.4493 35.3399 77.7 9.7 102.4 0.0461 0.1 0.4 Her X-1
288.6581 10.8009 40.3 45.0 50.9 -0.2916 -0.3 12.0 GRS 1915+105
299.5846 35.1188 1.7 35.4 12.3 2.9838 6.7 5.0 Cyg X-1
308.3552 40.9913 0.0 38.9 -1.6 0.6659 1.5 11.3 Cyg X-3
326.3185 38.3400 12.4 52.3 -7.5 -0.7147 -0.9 7.0 Cyg X-2
241.1548 9.0906 3.1 37.7 124.0 2.9305 3.8 ------ UNKNOWN
318.9088 23.8788 3.7 55.6 11.7 5.4290 3.1 ------ UNKNOWN
294.6457 35.7818 2.9 31.6 14.9 1.4473 4.0 ------ UNKNOWN
215.2193 28.1630 2.6 35.3 177.2 1.7232 4.4 ------ UNKNOWN
195.4721 14.3918 3.3 58.1 -179.9 7.5448 3.6 ------ UNKNOWN
187.1990 23.8385 3.1 57.6 -165.4 4.9256 3.7 ------ UNKNOWN
320.7240 57.9156 2.4 41.4 -30.5 2.3735 4.8 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-1.420000 0.928000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.2405 35.4579 0.0 9.5 103.4 -0.0189 -0.7 12.7 Her X-1
288.8558 10.8641 6.7 45.0 50.6 0.2047 1.7 5.9 GRS 1915+105
299.5658 35.2697 4.9 35.3 12.1 0.0922 2.3 4.3 Cyg X-1
308.0301 41.1132 4.5 38.6 -1.6 -0.1058 -2.6 10.3 Cyg X-3
326.2174 38.4165 4.0 52.2 -7.5 0.1975 2.9 6.1 Cyg X-2
235.7636 46.0686 1.0 13.1 -156.5 0.3045 11.2 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
49.276600 258.876610
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.5142 35.2525 12.3 17.7 60.3 -0.3420 -0.9 6.1 Her X-1
299.5765 35.1840 1.2 48.3 18.7 7.8622 9.7 1.3 Cyg X-1
308.1805 41.0355 19.5 50.8 7.4 -0.5093 -0.6 5.9 Cyg X-3
189.6407 28.9797 2.6 39.7 -159.5 2.2190 4.6 ------ UNKNOWN
178.7160 13.5939 3.6 57.6 -165.4 5.5054 3.2 ------ UNKNOWN
341.9789 61.1422 2.9 57.5 -27.2 7.4520 3.9 ------ UNKNOWN
Plot creation:
Sat Jul 30 06:58:22 EDT 2022