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
72.2503 7.2158 0.0159 5.2505 -65.0454 1.4939900 12.162 TRIG_01032183
Foreground time interval of the image:
-15.512 67.589 (delta_t = 83.101 [sec])
Background time interval of the image:
-239.512 -15.512 (delta_t = 224.000 [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 -15.512 sec. to 80.488 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.84622 ( -0.223366 0.235439 )
Norm@50keV : 9.07576E-04 ( -0.000137411 0.000133529 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 83.08 using 59 bins.
Reduced chi-squared = 1.45754
# Null hypothesis probability of 1.37e-02 with 57 degrees of freedom
Photon flux (15-150 keV) in 96 sec: 0.127381 ( -0.015202 0.015203 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.01311e-07 ( -1.19347e-07 1.22645e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -15.512 sec. to 80.488 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.83569 ( -1.04404 0.829999 )
Epeak [keV] : 532.943 ( -9988.61 -9988.62 )
Norm@50keV : 9.20720E-04 ( -0.000136974 0.00192961 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 83.08 using 59 bins.
Reduced chi-squared = 1.48357
# Null hypothesis probability of 1.09e-02 with 56 degrees of freedom
Photon flux (15-150 keV) in 96 sec: 0.127377 ( -0.015834 0.015203 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.46193e-07 ( -1.4954e-07 1.16272e-07 ) ergs/cm2
Band function
Time interval is from -15.512 sec. to 80.488 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] : 9.73573 (-1.30897 1.55634)
R^2/D10^2 : 6.55540E-02 (-0.0281698 0.047824)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 97.29 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.06e-04 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.203e-07 2.526e-08
25- 50 2.879e-07 5.237e-08
50-150 1.390e-07 4.616e-08
15-150 5.471e-07 1.034e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 85.1699 (-30.6826 68.3722)
Norm : 0.585538 (-0.0979837 0.129079)
------------------------------------------------------------
#Fit statistic : Chi-Squared 83.91 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.17e-02 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.464e-07 2.573e-08
25- 50 2.445e-07 3.706e-08
50-150 3.596e-07 1.855e-07
15-150 7.505e-07 2.035e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.71970 (-1.79299 1.66294)
R1^2/D10^2 : 0.137097 (-0.0685309 0.0878915)
kT2 [keV] : 52.6715 (-30.961 -52.6715)
R2^2/D10^2 : 1.48842E-04 (-0.000133229 0.00204439)
------------------------------------------------------------
#Fit statistic : Chi-Squared 81.39 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.19e-02 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.421e-07 4.598e-08
25- 50 2.571e-07 8.789e-08
50-150 4.429e-07 2.362e-07
15-150 8.421e-07 3.235e-07
Peak spectrum fit
Power-law model
Time interval is from 7.988 sec. to 8.988 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.64594 ( -0.487861 0.532885 )
Norm@50keV : 3.87681E-03 ( -0.00129383 0.00123844 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 45.00 using 59 bins.
Reduced chi-squared = 0.789474
# Null hypothesis probability of 8.75e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.505559 ( -0.146358 0.14639 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.60753e-08 ( -1.22828e-08 1.28496e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 7.988 sec. to 8.988 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.839565 ( -2.90191 1.39206 )
Epeak [keV] : 65.0401 ( -52.1155 -65.0399 )
Norm@50keV : 1.07753E-02 ( -0.0107755 0.360292 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 44.53 using 59 bins.
Reduced chi-squared = 0.795179
# Null hypothesis probability of 8.65e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.493638 ( -0.149705 0.149451 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.36574e-08 ( -1.23657e-08 1.4079e-08 ) ergs/cm2
Band function
Time interval is from 7.988 sec. to 8.988 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] : 13.2240 (-3.99483 5.54213)
R^2/D10^2 : 9.04219E-02 (-0.0903565 0.23509)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 46.43 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.40e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.352e-09 2.111e-09
25- 50 1.176e-08 7.145e-09
50-150 1.313e-08 8.665e-09
15-150 2.824e-08 1.736e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 150.638 (-98.6292 -145.996)
Norm : 2.09341 (-0.632712 1.00199)
------------------------------------------------------------
#Fit statistic : Chi-Squared 44.67 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.82e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.219e-09 3.158e-09
25- 50 9.923e-09 6.010e-09
50-150 2.106e-08 1.259e-08
15-150 3.620e-08 2.177e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 4.60234 (-4.52049 10.8019)
R1^2/D10^2 : 2.17080 (-2.19074 10.8525)
kT2 [keV] : 17.3013 (-6.05879 -17.2002)
R2^2/D10^2 : 2.91318E-02 (-0.0295611 0.134271)
------------------------------------------------------------
#Fit statistic : Chi-Squared 43.99 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.56e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.512e-09 3.178e-09
25- 50 9.910e-09 5.425e-09
50-150 1.709e-08 1.127e-08
15-150 3.251e-08 1.810e-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: 1.81610 ( -0.21459 0.225226 )
Norm@50keV : 1.01603E-03 ( -0.000146637 0.000142794 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 81.09 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.97e-02 with 57 degrees of freedom
Photon flux (15-150 keV) in 83.1 sec: 0.140889 ( -0.01636 0.0163606 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.76911e-07 ( -1.11804e-07 1.14697e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.70218 ( -0.972501 0.525774 )
Epeak [keV] : 110.025 ( -111.031 -111.045 )
Norm@50keV : 1.18284E-03 ( -0.000740836 0.00315728 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 81.04 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.60e-02 with 56 degrees of freedom
Photon flux (15-150 keV) in 83.1 sec: 0.140230 ( -0.016988 0.016813 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.66079e-07 ( -1.37474e-07 1.23581e-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) = 2.29e-07
S(50-100 keV) = 2.55e-07
T90 vs. Hardness ratio plot
T90 = 80 sec.
Hardness ratio (energy fluence ratio) = 1.11354
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.11968
Count Ratio (50-100 keV) / (15-25 keV) = 0.528725
Mask shadow pattern
IMX = 3.877095071584416E-02, IMY = 8.331681337943837E-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:
-239.512000 -15.512000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6511 22.0146 0.3 17.5 27.6 9.5857 35.1 1.0 Crab
74.0320 -20.5541 2.4 26.4 -165.5 1.2649 4.7 ------ UNKNOWN
46.6734 -41.8727 4.8 55.1 -144.9 4.8850 2.4 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-15.512000 67.588600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6996 22.0340 6.4 17.5 27.7 -0.2393 -1.8 3.9 Crab
73.6632 43.4436 2.1 37.9 3.3 1.0649 5.4 ------ UNKNOWN
77.9158 -12.9506 2.3 18.6 -174.3 0.6718 5.1 ------ UNKNOWN
72.2503 7.2157 0.9 5.3 -65.0 1.4939 12.2 ------ UNKNOWN
39.7428 -16.1475 2.3 43.1 -113.4 2.4307 4.9 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
91.588610 928.988610
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6601 22.0208 0.8 18.4 47.7 33.7064 15.2 1.5 Crab
101.8574 2.9257 2.7 29.8 109.1 12.3977 4.3 ------ UNKNOWN
41.7647 55.5876 3.0 54.1 -8.5 22.5806 3.8 ------ UNKNOWN
30.8701 45.8224 3.3 52.5 -23.3 22.7887 3.5 ------ UNKNOWN
40.0926 -18.0578 3.6 40.6 -116.7 20.2243 3.2 ------ UNKNOWN
24.8602 26.5700 2.6 48.9 -48.6 46.1594 4.4 ------ UNKNOWN
Plot creation:
Sat Jul 30 07:15:32 EDT 2022