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
161.0388 32.1063 0.0107 10.4531 -162.7648 2.5773292 17.951 TRIG_01164980
Foreground time interval of the image:
-34.136 38.077 (delta_t = 72.213 [sec])
Background time interval of the image:
-239.224 -34.136 (delta_t = 205.088 [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 4.096000
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 4.096000
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 4.096000
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 -34.136 sec. to 100.920 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.64066 ( -0.101131 0.102242 )
Norm@50keV : 2.26286E-03 ( -0.000139385 0.000138556 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 62.60 using 59 bins.
Reduced chi-squared = 1.09825
# Null hypothesis probability of 2.84e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 135.1 sec: 0.294581 ( -0.017131 0.017145 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.84633e-06 ( -1.86855e-07 1.88579e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -34.136 sec. to 100.920 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.959623 ( -0.482533 0.429504 )
Epeak [keV] : 70.4133 ( -13.181 42.4359 )
Norm@50keV : 5.24150E-03 ( -0.00211875 0.00420445 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 54.81 using 59 bins.
Reduced chi-squared = 0.97875
# Null hypothesis probability of 5.20e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 135.1 sec: 0.285134 ( -0.01809 0.018084 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.66119e-06 ( -2.16432e-07 2.19032e-07 ) ergs/cm2
Band function
Time interval is from -34.136 sec. to 100.920 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] : 12.6041 (-0.868159 0.951313)
R^2/D10^2 : 6.02911E-02 (-0.0140887 0.0180268)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 99.90 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.85e-04 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.744e-07 2.911e-08
25- 50 9.135e-07 6.410e-08
50-150 9.006e-07 1.126e-07
15-150 2.089e-06 1.479e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 145.836 (-35.7451 51.5621)
Norm : 1.21970 (-0.0800617 0.0963101)
------------------------------------------------------------
#Fit statistic : Chi-Squared 56.14 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.07e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.242e-07 3.479e-08
25- 50 7.830e-07 8.038e-08
50-150 1.528e-06 5.290e-07
15-150 2.735e-06 6.073e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 8.03216 (-1.31279 1.32234)
R1^2/D10^2 : 0.215023 (-0.0790508 0.153003)
kT2 [keV] : 27.0741 (-6.21804 12.3771)
R2^2/D10^2 : 2.56009E-03 (-0.00184908 0.00446585)
------------------------------------------------------------
#Fit statistic : Chi-Squared 50.96 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.30e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.821e-07 7.086e-08
25- 50 8.477e-07 1.547e-07
50-150 1.490e-06 6.590e-07
15-150 2.719e-06 7.641e-07
Peak spectrum fit
Power-law model
Time interval is from 1.412 sec. to 2.412 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.36761 ( -0.3089 0.317272 )
Norm@50keV : 7.93802E-03 ( -0.00161299 0.00160433 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 58.37 using 59 bins.
Reduced chi-squared = 1.02404
# Null hypothesis probability of 4.25e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.959863 ( -0.192459 0.192737 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.72343e-08 ( -1.7193e-08 1.74832e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 1.412 sec. to 2.412 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -1.06728 ( -3.51049 1.83113 )
Epeak [keV] : 67.4664 ( -13.0517 42.714 )
Norm@50keV : 0.109110 ( -0.112822 3.3634 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 52.37 using 59 bins.
Reduced chi-squared = 0.935179
# Null hypothesis probability of 6.13e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.877890 ( -0.21178 0.20664 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.53411e-08 ( -1.85209e-08 1.42085e-08 ) ergs/cm2
Band function
Time interval is from 1.412 sec. to 2.412 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] : 16.8721 (-2.91318 3.64989)
R^2/D10^2 : 8.25357E-02 (-0.0406506 0.0744918)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 52.18 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.56e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.795e-09 1.983e-09
25- 50 2.109e-08 7.150e-09
50-150 4.276e-08 1.554e-08
15-150 6.864e-08 2.112e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.363 (-90.0059 -199.363)
Norm : 3.98215 (-0.788477 0.788477)
------------------------------------------------------------
#Fit statistic : Chi-Squared 57.80 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.46e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 9.916e-09 5.925e-09
25- 50 1.908e-08 1.091e-08
50-150 4.183e-08 2.414e-08
15-150 7.083e-08 4.168e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 2.43449 (-2.45416 16.5464)
R1^2/D10^2 : 62.6408 (-56.8446 -56.8446)
kT2 [keV] : 17.7641 (-3.24317 4.36722)
R2^2/D10^2 : 6.70437E-02 (-0.0664769 0.0391251)
------------------------------------------------------------
#Fit statistic : Chi-Squared 50.22 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.58e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.081e-09 2.697e-09
25- 50 1.966e-08 8.326e-09
50-150 4.446e-08 2.035e-08
15-150 7.120e-08 2.608e-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: 1.64670 ( -0.128308 0.130674 )
Norm@50keV : 2.29093E-03 ( -0.000187505 0.000185978 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 62.54 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.86e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 72.21 sec: 0.298813 ( -0.0225732 0.0225858 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.53906e-06 ( -1.33849e-07 1.35414e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.478376 ( -0.746969 0.627635 )
Epeak [keV] : 59.1105 ( -8.8298 19.3652 )
Norm@50keV : 9.80506E-03 ( -0.00525344 0.0149653 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 51.08 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.61e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 72.21 sec: 0.284343 ( -0.023777 0.02376 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.38402e-06 ( -1.48211e-07 1.54074e-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) = 7.51e-07
S(50-100 keV) = 9.63e-07
T90 vs. Hardness ratio plot
T90 = 111.947999954224 sec.
Hardness ratio (energy fluence ratio) = 1.28229
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.4158
Count Ratio (50-100 keV) / (15-25 keV) = 0.839634
Mask shadow pattern
IMX = -1.762085707032564E-01, IMY = 5.466435392643043E-02
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 4.096000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 4.096000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 4.096000
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:
-239.224000 -34.136000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
174.7132 7.8649 2.5 29.3 127.2 2.2598 4.7 ------ UNKNOWN
221.0907 68.7092 2.4 41.2 -23.3 2.6019 4.8 ------ UNKNOWN
119.9545 56.0931 2.7 39.4 -91.8 5.7377 4.2 ------ UNKNOWN
119.5392 64.7229 2.9 41.3 -78.8 5.4382 4.1 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-34.136000 38.076590
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
189.0577 -0.2863 2.4 40.5 105.7 3.0409 4.8 ------ UNKNOWN
179.8089 19.2726 2.1 19.0 109.7 0.9370 5.5 ------ UNKNOWN
203.6270 47.4348 2.1 25.2 8.0 0.8387 5.7 ------ UNKNOWN
194.6365 44.9114 2.3 18.6 10.2 0.7361 5.0 ------ UNKNOWN
161.0388 32.1064 0.6 10.5 -162.8 2.5765 17.9 ------ UNKNOWN
138.4734 40.4544 2.8 26.4 -119.9 0.8414 4.1 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
79.676600 962.886000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
204.0854 17.1520 2.4 41.6 64.5 16.4995 4.9 ------ UNKNOWN
188.5688 13.0582 2.4 31.6 84.7 11.0419 4.8 ------ UNKNOWN
132.3088 1.1142 3.4 41.1 -169.1 7.0926 3.4 ------ UNKNOWN
150.8505 81.5009 2.5 49.5 -38.0 21.2138 4.6 ------ UNKNOWN
Plot creation:
Fri Jun 16 09:08:43 EDT 2023