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
198.2840 44.5104 0.0069 31.2901 3.6820 7.0618146 27.895 TRIG_01040123
Foreground time interval of the image:
-51.604 80.701 (delta_t = 132.305 [sec])
Background time interval of the image:
-239.000 -51.604 (delta_t = 187.396 [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
8 ms binning
From T100_start-3 s to T100_start+3 s
2 ms binning
From T100_start-1 s to T100_start+1 s
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 -51.604 sec. to 310.200 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.83892 ( -0.0632978 0.0638578 )
Norm@50keV : 2.60642E-03 ( -8.77849e-05 8.74199e-05 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 63.96 using 59 bins.
Reduced chi-squared = 1.12211
# Null hypothesis probability of 2.45e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 361.8 sec: 0.364742 ( -0.012166 0.012207 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.67358e-06 ( -2.94839e-07 2.96344e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -51.604 sec. to 310.200 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.49822 ( -0.276781 0.259822 )
Epeak [keV] : 70.1791 ( -13.1395 67.1912 )
Norm@50keV : 3.89212E-03 ( -0.0010035 0.0014699 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 58.88 using 59 bins.
Reduced chi-squared = 1.05143
# Null hypothesis probability of 3.71e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 361.8 sec: 0.354852 ( -0.014117 0.01419 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.36351e-06 ( -3.72375e-07 3.7341e-07 ) ergs/cm2
Band function
Time interval is from -51.604 sec. to 310.200 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] : 12.3278 ( )
R^2/D10^2 : 7.36398E-02 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 239.82 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.79e-24 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.579e-07 4.993e-08
25- 50 2.786e-06 1.017e-07
50-150 2.591e-06 1.776e-07
15-150 6.235e-06 2.080e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 98.9505 (-11.9264 14.808)
Norm : 1.57636 (-0.077826 0.0841941)
------------------------------------------------------------
#Fit statistic : Chi-Squared 60.23 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.60e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.491e-06 1.094e-07
25- 50 2.572e-06 1.069e-07
50-150 4.143e-06 1.002e-06
15-150 8.206e-06 1.053e-06
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.80344 (-0.787988 0.817266)
R1^2/D10^2 : 0.464332 (-0.146798 0.252608)
kT2 [keV] : 22.8418 (-2.90321 4.10621)
R2^2/D10^2 : 5.48380E-03 (-0.00255787 0.00394519)
------------------------------------------------------------
#Fit statistic : Chi-Squared 64.47 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.79e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.400e-06 1.708e-07
25- 50 2.586e-06 1.930e-07
50-150 4.199e-06 5.852e-07
15-150 8.186e-06 7.381e-07
Peak spectrum fit
Power-law model
Time interval is from 173.532 sec. to 174.532 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.60344 ( -0.212681 0.220315 )
Norm@50keV : 1.17916E-02 ( -0.0015132 0.00147508 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 36.46 using 59 bins.
Reduced chi-squared = 0.639649
# Null hypothesis probability of 9.84e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 1.51694 ( -0.17032 0.17037 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.10245e-07 ( -1.5307e-08 1.5607e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 173.532 sec. to 174.532 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.60529 ( -0.216881 0.218372 )
Epeak [keV] : 9999.22 ( -9999.35 -9999.35 )
Norm@50keV : 1.18055E-02 ( -0.0102398 0.0083955 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 36.47 using 59 bins.
Reduced chi-squared = 0.65125
# Null hypothesis probability of 9.80e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 1.51916 ( -0.17508 0.1696 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.94576e-08 ( -1.57804e-08 1.25606e-08 ) ergs/cm2
Band function
Time interval is from 173.532 sec. to 174.532 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] : 13.6537 (-2.14347 2.57303)
R^2/D10^2 : 0.227338 (-0.102376 0.186602)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 67.51 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.61e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.971e-09 1.821e-09
25- 50 3.253e-08 5.280e-09
50-150 3.941e-08 1.052e-08
15-150 8.091e-08 1.372e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.095 (-99.3703 -199.041)
Norm : 6.13102 (-0.691384 0.810388)
------------------------------------------------------------
#Fit statistic : Chi-Squared 38.36 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.73e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.527e-08 8.490e-09
25- 50 2.937e-08 1.601e-08
50-150 6.438e-08 3.531e-08
15-150 1.090e-07 5.960e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 4.53834 (-1.36715 1.9129)
R1^2/D10^2 : 9.30937 (-6.64519 32.8737)
kT2 [keV] : 22.8529 (-5.31384 10.4113)
R2^2/D10^2 : 3.26890E-02 (-0.0232067 0.0303695)
------------------------------------------------------------
#Fit statistic : Chi-Squared 36.37 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.75e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.822e-08 8.899e-09
25- 50 2.449e-08 8.349e-09
50-150 6.565e-08 2.926e-08
15-150 1.084e-07 4.432e-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: 1.76221 ( -0.0854165 0.0864725 )
Norm@50keV : 3.31288E-03 ( -0.000159842 0.00015882 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 48.10 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.93e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 132.3 sec: 0.449990 ( -0.020492 0.0205298 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.04161e-06 ( -2.01637e-07 2.03078e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.45245 ( -0.365213 0.334764 )
Epeak [keV] : 83.0216 ( -22.8251 -83.0262 )
Norm@50keV : 4.81064E-03 ( -0.00154281 0.00260315 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 45.64 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.37e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 132.3 sec: 0.440817 ( -0.022646 0.022657 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.91423e-06 ( -2.4412e-07 2.44768e-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) = 2.48e-06
S(50-100 keV) = 2.77e-06
T90 vs. Hardness ratio plot
T90 = 238.707999944687 sec.
Hardness ratio (energy fluence ratio) = 1.11694
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.19138
Count Ratio (50-100 keV) / (15-25 keV) = 0.7023
Mask shadow pattern
IMX = 6.065185159620234E-01, IMY = -3.903051617941981E-02
TIME vs. PHA plot around the trigger time
TIME vs. DetID plot around the trigger time
100 us light curve (15-350 keV)
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:
-239.000000 -51.604000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
202.7667 59.9884 2.5 40.8 -17.7 1.5997 4.6 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-51.604000 80.700600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
175.5618 20.4470 2.5 12.7 79.7 1.0020 4.6 ------ UNKNOWN
198.2840 44.5104 0.4 31.3 3.7 7.0622 27.9 ------ UNKNOWN
118.9701 -8.0084 1.9 57.0 -168.5 4.3799 5.9 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
143.100580 963.079600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.5214 35.2130 42.2 43.3 -15.4 -0.3085 -0.3 8.4 Her X-1
189.0896 13.1473 2.8 32.3 99.3 4.4754 4.1 ------ UNKNOWN
206.3113 24.4028 2.7 21.2 61.6 3.1989 4.2 ------ UNKNOWN
231.5521 22.3752 3.9 35.1 20.5 2.9257 2.9 ------ UNKNOWN
129.3012 26.8724 3.1 56.9 179.2 14.1139 3.7 ------ UNKNOWN
198.2924 44.5135 1.0 0.1 -17.4 8.1825 11.7 ------ UNKNOWN
262.0989 18.4819 5.9 58.7 -3.0 10.7181 2.0 ------ UNKNOWN
252.6738 37.7645 3.4 40.8 -17.6 3.7089 3.4 ------ UNKNOWN
275.1210 41.0542 3.4 54.4 -32.9 13.6477 3.4 ------ UNKNOWN
113.2853 67.0510 2.4 47.9 -129.1 15.6057 4.8 ------ UNKNOWN
Plot creation:
Sat Jul 30 07:08:15 EDT 2022