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
296.9544 -55.1986 0.0035 32.9613 1.6447 5.1864200 55.175 TRIG_00997024
Foreground time interval of the image:
-1.880 10.833 (delta_t = 12.713 [sec])
Background time interval of the image:
-20.167 -1.880 (delta_t = 18.287 [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 0.064000
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 0.064000
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 0.064000
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 -1.880 sec. to 16.224 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.12451 ( -0.0564127 0.0570624 )
Norm@50keV : 1.72613E-02 ( -0.000547172 0.000544994 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 75.93 using 59 bins.
Reduced chi-squared = 1.33211
# Null hypothesis probability of 4.76e-02 with 57 degrees of freedom
Photon flux (15-150 keV) in 18.1 sec: 2.74922 ( -0.08974 0.09016 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.91064e-06 ( -8.62275e-08 8.63698e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -1.880 sec. to 16.224 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.43858 ( -0.267449 0.25202 )
Epeak [keV] : 39.1364 ( -6.90051 4.71449 )
Norm@50keV : 3.86519E-02 ( -0.00974663 0.0140964 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 52.21 using 59 bins.
Reduced chi-squared = 0.932321
# Null hypothesis probability of 6.19e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 18.1 sec: 2.60241 ( -0.10134 0.1021 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.75384e-06 ( -1.01445e-07 1.01634e-07 ) ergs/cm2
Band function
Time interval is from -1.880 sec. to 16.224 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] : 11.3063 ( )
R^2/D10^2 : 0.730899 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 246.23 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.32e-25 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.551e-07 1.919e-08
25- 50 1.040e-06 3.349e-08
50-150 7.664e-07 5.330e-08
15-150 2.161e-06 6.788e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 64.0181 (-5.11947 5.80562)
Norm : 13.4615 (-0.727018 0.773834)
------------------------------------------------------------
#Fit statistic : Chi-Squared 52.68 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.38e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.183e-07 2.724e-08
25- 50 9.595e-07 2.778e-08
50-150 1.151e-06 7.711e-08
15-150 2.729e-06 8.598e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.59254 (-0.730743 0.728177)
R1^2/D10^2 : 4.12534 (-1.24864 2.18349)
kT2 [keV] : 19.6791 (-2.16007 2.82563)
R2^2/D10^2 : 5.59552E-02 (-0.0247965 0.0384782)
------------------------------------------------------------
#Fit statistic : Chi-Squared 59.57 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.13e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.639e-07 5.692e-08
25- 50 9.680e-07 7.285e-08
50-150 1.153e-06 1.376e-07
15-150 2.684e-06 2.163e-07
Peak spectrum fit
Power-law model
Time interval is from -0.460 sec. to 0.540 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.72946 ( -0.063622 0.0643496 )
Norm@50keV : 8.45686E-02 ( -0.00330055 0.00329412 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 77.38 using 59 bins.
Reduced chi-squared = 1.35754
# Null hypothesis probability of 3.75e-02 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 11.3502 ( -0.4555 0.4564 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.81448e-07 ( -3.13984e-08 3.14574e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.460 sec. to 0.540 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.885037 ( -0.303718 0.285529 )
Epeak [keV] : 69.0452 ( -6.72334 10.6835 )
Norm@50keV : 0.217544 ( -0.0583381 0.086016 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 48.98 using 59 bins.
Reduced chi-squared = 0.874643
# Null hypothesis probability of 7.35e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 10.0130 ( -0.62216 0.7288 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.52991e-07 ( -3.32438e-08 3.32216e-08 ) ergs/cm2
Band function
Time interval is from -0.460 sec. to 0.540 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] : 14.3154 ( )
R^2/D10^2 : 1.48064 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 158.05 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.95e-11 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.394e-08 4.770e-09
25- 50 2.431e-07 1.110e-08
50-150 3.317e-07 2.430e-08
15-150 6.388e-07 2.620e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 131.099 (-18.9442 21.423)
Norm : 47.5501 (-2.24654 2.60096)
------------------------------------------------------------
#Fit statistic : Chi-Squared 54.59 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.66e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.208e-07 8.150e-09
25- 50 2.207e-07 1.310e-08
50-150 4.174e-07 1.080e-07
15-150 7.589e-07 1.111e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.51626 (-1.12146 1.25265)
R1^2/D10^2 : 13.6751 (-5.97 13.4815)
kT2 [keV] : 20.5966 (-2.00448 2.77683)
R2^2/D10^2 : 0.304446 (-0.129102 0.169121)
------------------------------------------------------------
#Fit statistic : Chi-Squared 51.71 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.01e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.107e-07 1.830e-08
25- 50 2.271e-07 2.425e-08
50-150 4.072e-07 4.940e-08
15-150 7.450e-07 7.130e-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: 2.09193 ( -0.0517878 0.0522901 )
Norm@50keV : 2.40316E-02 ( -0.000699049 0.000696998 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 73.89 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.56e-02 with 57 degrees of freedom
Photon flux (15-150 keV) in 12.71 sec: 3.76581 ( -0.116423 0.116945 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.8357e-06 ( -7.84203e-08 7.84807e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.33934 ( -0.248799 0.235671 )
Epeak [keV] : 42.8297 ( -4.89754 3.98023 )
Norm@50keV : 5.74333E-02 ( -0.0134761 0.0188988 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 40.72 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.38e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 12.71 sec: 3.54465 ( -0.13047 0.13146 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.6799e-06 ( -9.0724e-08 9.08511e-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) = 9.07e-07
S(50-100 keV) = 8.31e-07
T90 vs. Hardness ratio plot
T90 = 10.3039999008179 sec.
Hardness ratio (energy fluence ratio) = 0.916207
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.11462
Count Ratio (50-100 keV) / (15-25 keV) = 0.535889
Mask shadow pattern
IMX = 6.481798389224950E-01, IMY = -1.861139071835446E-02
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.064000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.064000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.064000
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:
-20.167400 -1.880000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
264.6766 -44.6046 5.8 51.5 -19.2 0.2819 2.0 9.7 4U 1735-44
277.8521 -36.3838 2.2 55.5 -3.9 0.9583 5.2 ------ UNKNOWN
225.8746 -69.2275 2.3 35.8 -59.6 0.4791 5.1 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-1.880000 10.832580
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
264.6222 -44.3386 9.8 51.8 -19.1 0.2368 1.2 8.5 4U 1735-44
318.9588 -32.5622 2.8 47.4 38.6 1.1122 4.2 ------ UNKNOWN
296.9544 -55.1986 0.2 33.0 1.6 5.1865 55.2 ------ UNKNOWN
84.8023 -30.7376 2.2 56.9 -174.0 2.0951 5.1 ------ UNKNOWN
89.7772 -31.4861 2.2 57.6 -169.0 2.4470 5.1 ------ UNKNOWN
112.8539 -42.3555 2.6 54.0 -143.5 2.0850 4.4 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
64.832590 261.632590
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
255.9334 -37.7384 7.0 32.5 -52.0 0.5600 1.6 6.8 4U 1700-377
256.3171 -36.3949 6.3 33.3 -49.8 -0.6202 -1.9 6.0 GX 349+2
263.1379 -24.6670 97.4 39.3 -30.1 0.0406 0.1 8.5 GX 1+4
264.9540 -44.3885 8.8 23.0 -52.5 0.3665 1.3 9.8 4U 1735-44
268.3201 -1.3328 19.4 58.7 -11.2 -0.8282 -0.6 7.7 SW J1753.5-0127
270.3670 -25.1871 3.6 35.8 -21.0 0.9194 3.2 7.9 GX 5-1
270.2494 -25.7026 4.1 35.3 -21.5 0.8371 2.9 3.8 GRS 1758-258
273.9382 -14.1882 158.6 44.7 -9.7 0.0268 0.1 9.9 GX 17+2
275.7593 -30.2736 5.0 29.1 -17.0 0.5560 2.3 10.3 H1820-303
284.9321 -24.8599 12.5 31.6 1.8 -0.2419 -0.9 6.7 HT1900.1-2455
262.8363 -33.7392 5.6 31.9 -39.1 0.6155 2.1 9.5 GX 354-0
316.0308 -15.5154 2.4 42.3 50.8 2.9834 4.8 ------ UNKNOWN
288.7594 -51.4056 2.3 6.2 -32.6 1.1577 5.1 ------ UNKNOWN
267.3568 -2.3723 2.8 58.0 -12.7 4.6323 4.1 ------ UNKNOWN
114.6253 -69.9600 2.5 54.8 -158.1 3.8315 4.7 ------ UNKNOWN
258.8109 -7.0088 2.4 56.9 -24.1 5.2890 4.9 ------ UNKNOWN
Plot creation:
Thu Oct 20 00:48:30 EDT 2022