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
113.9660 -7.9936 0.0187 15.9063 89.7704 2.4961010 10.317 TRIG_01154815
Foreground time interval of the image:
-81.072 16.784 (delta_t = 97.856 [sec])
Background time interval of the image:
-239.600 -81.072 (delta_t = 158.528 [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 2.048000
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 2.048000
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 2.048000
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 -81.072 sec. to 16.784 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.91784 ( -0.225357 0.239715 )
Norm@50keV : 1.39331E-03 ( -0.000223385 0.000217549 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 46.52 using 59 bins.
Reduced chi-squared = 0.81614
# Null hypothesis probability of 8.38e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 97.86 sec: 0.201498 ( -0.024838 0.024838 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.25405e-06 ( -1.9224e-07 1.97983e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -81.072 sec. to 16.784 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.33441 ( -1.071 0.778934 )
Epeak [keV] : 47.2292 ( -45.8543 -47.2292 )
Norm@50keV : 3.04777E-03 ( -0.0030478 0.00968434 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 45.26 using 59 bins.
Reduced chi-squared = 0.808214
# Null hypothesis probability of 8.47e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 97.86 sec: 0.197352 ( -0.025479 0.025551 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.17656e-06 ( -2.08026e-07 2.2698e-07 ) ergs/cm2
Band function
Time interval is from -81.072 sec. to 16.784 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] : 10.5167 (-1.55821 1.78884)
R^2/D10^2 : 7.81392E-02 (-0.0347523 0.064498)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 59.03 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.01e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.749e-07 4.149e-08
25- 50 4.661e-07 8.230e-08
50-150 2.810e-07 9.390e-08
15-150 9.220e-07 1.588e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 74.0484 (-24.6263 47.9942)
Norm : 0.974159 (-0.170341 0.210096)
------------------------------------------------------------
#Fit statistic : Chi-Squared 45.28 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 2.459e-07 4.325e-08
25- 50 3.971e-07 6.312e-08
50-150 5.314e-07 2.779e-07
15-150 1.174e-06 2.445e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 4.42956 (-1.43748 1.8134)
R1^2/D10^2 : 1.30823 (-0.976853 6.56555)
kT2 [keV] : 15.7088 (-3.42159 6.12042)
R2^2/D10^2 : 1.38594E-02 (-0.0102368 0.0237038)
------------------------------------------------------------
#Fit statistic : Chi-Squared 43.76 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.62e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.563e-07 1.317e-07
25- 50 3.771e-07 1.974e-07
50-150 4.947e-07 2.881e-07
15-150 1.128e-06 5.127e-07
Peak spectrum fit
Power-law model
Time interval is from -0.132 sec. to 0.868 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.91109 ( -0.353413 0.389502 )
Norm@50keV : 8.51229E-03 ( -0.00232082 0.0022499 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 63.14 using 59 bins.
Reduced chi-squared = 1.10772
# Null hypothesis probability of 2.68e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 1.22747 ( -0.264896 0.26491 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.82871e-08 ( -2.02641e-08 2.11595e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.132 sec. to 0.868 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.550152 ( -2.90733 1.5399 )
Epeak [keV] : 41.9529 ( -41.9417 78.488 )
Norm@50keV : 5.64273E-02 ( -0.0565738 4.20011 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 60.95 using 59 bins.
Reduced chi-squared = 1.08839
# Null hypothesis probability of 3.02e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 1.19643 ( -0.264396 0.26582 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.90542e-08 ( -1.99193e-08 2.32093e-08 ) ergs/cm2
Band function
Time interval is from -0.132 sec. to 0.868 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] : 9.55905 (-1.9471 2.63346)
R^2/D10^2 : 0.723005 (-0.440599 1.00011)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 62.81 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.78e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.323e-08 6.074e-09
25- 50 3.081e-08 1.242e-08
50-150 1.409e-08 8.163e-09
15-150 5.813e-08 2.038e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 69.7327 (-31.5624 92.5276)
Norm : 6.17610 (-1.70541 2.41289)
------------------------------------------------------------
#Fit statistic : Chi-Squared 61.47 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.19e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.584e-08 5.063e-09
25- 50 2.517e-08 8.560e-09
50-150 3.224e-08 2.469e-08
15-150 7.326e-08 3.601e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.83968 (-7.12113 -7.12113)
R1^2/D10^2 : 1.78598 (-1.65147 -1.65147)
kT2 [keV] : 18.7589 (-20.5402 -20.5402)
R2^2/D10^2 : 2.88302E-02 (-0.0213677 0.900595)
------------------------------------------------------------
#Fit statistic : Chi-Squared 60.39 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.87e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.510e-08 9.290e-09
25- 50 2.669e-08 1.569e-08
50-150 2.724e-08 1.722e-08
15-150 6.902e-08 3.732e-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: 1.91784 ( -0.225357 0.239715 )
Norm@50keV : 1.39331E-03 ( -0.000223385 0.000217549 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 46.52 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.38e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 97.86 sec: 0.201485 ( -0.0248366 0.0248366 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.25382e-06 ( -1.92112e-07 1.98043e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.33439 ( -1.071 0.778933 )
Epeak [keV] : 47.2292 ( -45.7521 -47.2292 )
Norm@50keV : 3.04782E-03 ( -0.00304781 0.00968434 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 45.26 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.47e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 97.86 sec: 0.197313 ( -0.02547 0.025542 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.17688e-06 ( -2.08333e-07 2.27202e-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) = 3.68e-07
S(50-100 keV) = 3.89e-07
T90 vs. Hardness ratio plot
T90 = 91.1999999284744 sec.
Hardness ratio (energy fluence ratio) = 1.05707
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 0.9561
Count Ratio (50-100 keV) / (15-25 keV) = 0.466653
Mask shadow pattern
IMX = 1.141749730817181E-03, IMY = -2.849734827103940E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 2.048000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 2.048000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 2.048000
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:
-239.600000 -81.072000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6254 22.0298 0.9 43.9 14.0 6.2416 13.3 1.0 Crab
135.4708 -40.6720 4.1 36.8 173.0 1.4016 2.8 7.5 Vela X-1
138.2138 1.0800 2.0 41.0 104.0 6.4128 5.7 ------ UNKNOWN
124.0647 -69.1731 2.3 52.9 -151.8 4.7692 5.0 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-81.072000 16.784000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6275 22.1202 5.5 43.9 14.0 0.8718 2.1 6.4 Crab
135.6180 -40.5044 7.3 36.8 172.7 0.4676 1.6 5.1 Vela X-1
113.9659 -7.9936 1.1 15.9 89.8 2.4963 10.3 ------ UNKNOWN
93.4855 10.3446 2.5 29.6 22.2 1.2078 4.6 ------ UNKNOWN
148.0983 -55.0577 2.5 51.0 -174.3 2.4570 4.5 ------ UNKNOWN
84.2404 -11.2161 2.8 18.0 -31.4 0.9204 4.1 ------ UNKNOWN
136.4612 -57.0511 2.5 46.7 -167.3 1.8101 4.6 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
82.900590 962.526800
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6239 22.0147 0.8 42.3 -14.7 34.8150 14.2 0.5 Crab
135.5968 -40.5753 3.4 37.8 -177.7 8.3506 3.4 3.3 Vela X-1
163.5885 -29.9427 2.5 51.3 151.7 46.2118 4.6 ------ UNKNOWN
Plot creation:
Fri Jun 16 09:14:05 EDT 2023