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
235.7457 -37.2326 0.0055 30.1407 -151.6118 7.0614982 34.876 TRIG_01015728
Foreground time interval of the image:
-2.068 97.364 (delta_t = 99.432 [sec])
Background time interval of the image:
-239.632 -2.068 (delta_t = 237.564 [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 1.024000
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 1.024000
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 1.024000
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 -2.068 sec. to 97.364 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.87756 ( -0.0811261 0.0821029 )
Norm@50keV : 4.26524E-03 ( -0.000193647 0.000192383 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 47.02 using 59 bins.
Reduced chi-squared = 0.824912
# Null hypothesis probability of 8.24e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 99.43 sec: 0.606395 ( -0.026342 0.026414 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.89931e-06 ( -1.76097e-07 1.77005e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -2.068 sec. to 97.364 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.72688 ( -0.324039 0.311201 )
Epeak [keV] : 84.7894 ( -26.0645 -84.79 )
Norm@50keV : 5.11729E-03 ( -0.00153225 0.00239426 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 46.31 using 59 bins.
Reduced chi-squared = 0.826964
# Null hypothesis probability of 8.19e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 99.43 sec: 0.600161 ( -0.029039 0.029078 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.83979e-06 ( -2.12205e-07 2.10422e-07 ) ergs/cm2
Band function
Time interval is from -2.068 sec. to 97.364 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] : 11.6057 ( )
R^2/D10^2 : 0.153392 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 183.33 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.51e-15 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.330e-07 3.251e-08
25- 50 1.309e-06 6.562e-08
50-150 1.036e-06 1.058e-07
15-150 2.778e-06 1.293e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 91.9205 (-13.5764 17.6962)
Norm : 2.67459 (-0.176765 0.195157)
------------------------------------------------------------
#Fit statistic : Chi-Squared 50.73 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.08e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.943e-07 5.200e-08
25- 50 1.180e-06 5.568e-08
50-150 1.820e-06 4.927e-07
15-150 3.694e-06 4.847e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.86366 (-0.775291 0.7961)
R1^2/D10^2 : 0.837417 (-0.268366 0.45511)
kT2 [keV] : 25.8884 (-4.12145 6.07786)
R2^2/D10^2 : 5.64405E-03 (-0.00294519 0.00519597)
------------------------------------------------------------
#Fit statistic : Chi-Squared 45.97 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.02e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.813e-07 8.069e-08
25- 50 1.183e-06 1.039e-07
50-150 1.954e-06 4.335e-07
15-150 3.819e-06 5.573e-07
Peak spectrum fit
Power-law model
Time interval is from 66.712 sec. to 67.712 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.59460 ( -0.111434 0.112768 )
Norm@50keV : 3.44685E-02 ( -0.00238807 0.00237525 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 42.82 using 59 bins.
Reduced chi-squared = 0.751228
# Null hypothesis probability of 9.18e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 4.42213 ( -0.29566 0.2959 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.22612e-07 ( -2.395e-08 2.41249e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 66.712 sec. to 67.712 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.939289 ( -0.516183 0.4603 )
Epeak [keV] : 77.5780 ( -16.3598 67.7537 )
Norm@50keV : 7.60060E-02 ( -0.0317919 0.0640536 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 36.65 using 59 bins.
Reduced chi-squared = 0.654464
# Null hypothesis probability of 9.79e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 4.31080 ( -0.30595 0.30585 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.06606e-07 ( -2.63854e-08 2.65748e-08 ) ergs/cm2
Band function
Time interval is from 66.712 sec. to 67.712 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] : 13.6663 (-1.06696 1.17089)
R^2/D10^2 : 0.694753 (-0.178485 0.236826)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 76.33 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.46e-02 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.746e-08 3.555e-09
25- 50 9.969e-08 8.160e-09
50-150 1.210e-07 1.690e-08
15-150 2.482e-07 1.940e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 165.632 (-45.0331 -166.13)
Norm : 18.2180 (-1.31185 1.44402)
------------------------------------------------------------
#Fit statistic : Chi-Squared 37.93 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.76e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.636e-08 4.230e-09
25- 50 8.713e-08 1.720e-08
50-150 1.789e-07 7.581e-08
15-150 3.124e-07 9.665e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.96327 (-1.47689 1.71834)
R1^2/D10^2 : 4.60310 (-2.2611 5.56912)
kT2 [keV] : 22.9331 (-4.19611 7.60144)
R2^2/D10^2 : 8.12206E-02 (-0.0540057 0.0565388)
------------------------------------------------------------
#Fit statistic : Chi-Squared 35.21 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.83e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.341e-08 1.372e-08
25- 50 9.033e-08 1.867e-08
50-150 1.728e-07 6.832e-08
15-150 3.066e-07 9.265e-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: 1.87756 ( -0.0811261 0.0821029 )
Norm@50keV : 4.26524E-03 ( -0.000193647 0.000192383 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 47.02 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.24e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 99.43 sec: 0.606359 ( -0.0263382 0.02641 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.89866e-06 ( -1.76104e-07 1.77025e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.72688 ( -0.324039 0.311201 )
Epeak [keV] : 84.7889 ( -26.0598 -84.79 )
Norm@50keV : 5.11729E-03 ( -0.00153225 0.00239426 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 46.31 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.19e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 99.43 sec: 0.600030 ( -0.02902 0.028938 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.84084e-06 ( -2.12273e-07 2.11159e-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) = 1.13e-06
S(50-100 keV) = 1.23e-06
T90 vs. Hardness ratio plot
T90 = 87.231999874115 sec.
Hardness ratio (energy fluence ratio) = 1.0885
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.17821
Count Ratio (50-100 keV) / (15-25 keV) = 0.650196
Mask shadow pattern
IMX = -5.108070927266599E-01, IMY = 2.760563595252863E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.024000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.024000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.024000
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:
-239.632000 -2.068000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
170.4615 -60.5101 11.6 27.3 98.6 0.4773 1.0 8.0 Cen X-3
186.7243 -62.6972 6.9 19.9 106.1 0.6108 1.7 4.8 GX 301-2
245.0279 -15.6776 3.3 52.2 -141.0 4.8995 3.5 3.6 Sco X-1
255.9692 -38.0278 0.0 31.9 -120.4 0.2004 0.4 11.0 4U 1700-377
256.3666 -36.4495 19.4 33.5 -120.7 0.2662 0.6 3.7 GX 349+2
264.6077 -44.3578 4.8 28.2 -103.8 1.0087 2.4 8.0 4U 1735-44
262.9445 -33.8608 115.6 37.5 -113.1 0.0710 0.1 2.7 GX 354-0
206.4748 -67.7876 2.4 10.3 100.2 1.3694 4.9 ------ UNKNOWN
208.3508 -24.4514 2.3 45.7 172.1 3.4312 4.9 ------ UNKNOWN
235.6190 -44.8199 3.0 22.6 -151.3 1.1267 3.9 ------ UNKNOWN
241.8985 -12.3998 3.8 55.2 -145.1 5.0738 3.0 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-2.068000 97.364000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
170.4606 -60.5098 4.0 27.3 98.6 -0.7512 -2.9 8.0 Cen X-3
186.3867 -62.7817 8.0 19.9 105.6 0.2917 1.4 7.4 GX 301-2
244.9855 -15.6618 19.1 52.2 -141.1 -0.4606 -0.6 1.3 Sco X-1
255.8953 -37.7308 11.1 32.1 -120.7 0.2750 1.0 8.1 4U 1700-377
256.3052 -36.4147 6.7 33.5 -120.8 -0.4774 -1.7 6.3 GX 349+2
265.0192 -44.4224 34.4 28.2 -103.2 0.0859 0.3 12.0 4U 1735-44
262.7847 -33.8249 9.0 37.5 -113.3 0.5169 1.3 10.2 GX 354-0
235.7458 -37.2326 0.3 30.1 -151.6 7.0618 34.9 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
495.768630 542.538000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
350.6208 19.9527 2.5 50.1 15.0 23.4856 4.5 ------ UNKNOWN
286.4815 -58.1544 2.9 49.2 -133.1 41.6602 3.9 ------ UNKNOWN
Plot creation:
Sat Jul 30 07:21:03 EDT 2022