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
39.7779 33.6152 0.0177 38.7215 -8.3340 0.6959546 10.920 TRIG_01202749
Foreground time interval of the image:
-1.120 10.109 (delta_t = 11.229 [sec])
Background time interval of the image:
-56.891 -1.120 (delta_t = 55.771 [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 0.512000
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 0.512000
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 0.512000
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 -1.120 sec. to 51.360 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.60840 ( -0.194839 0.199162 )
Norm@50keV : 2.06673E-03 ( -0.000245323 0.000242588 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 45.70 using 59 bins.
Reduced chi-squared = 0.801754
# Null hypothesis probability of 8.59e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 52.48 sec: 0.266289 ( -0.030204 0.030244 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.01348e-06 ( -1.28355e-07 1.29805e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -1.120 sec. to 51.360 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.19829 ( -0.863032 0.65306 )
Epeak [keV] : 95.9637 ( -37.8162 -95.9637 )
Norm@50keV : 3.36098E-03 ( -0.00149151 0.00574341 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 44.81 using 59 bins.
Reduced chi-squared = 0.800179
# Null hypothesis probability of 8.58e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 52.48 sec: 0.261708 ( -0.031447 0.031338 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.83612e-07 ( -1.38929e-07 1.40149e-07 ) ergs/cm2
Band function
Time interval is from -1.120 sec. to 51.360 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] : 14.1553 (-1.89804 2.23599)
R^2/D10^2 : 3.63513E-02 (-0.0148392 0.0245278)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 62.07 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.00e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.066e-08 1.889e-08
25- 50 3.033e-07 4.760e-08
50-150 4.024e-07 9.305e-08
15-150 7.863e-07 1.299e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 168.651 (-67.9377 -168.651)
Norm : 1.09303 (-0.130531 0.152237)
------------------------------------------------------------
#Fit statistic : Chi-Squared 44.87 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.78e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.457e-07 7.972e-08
25- 50 2.745e-07 1.469e-07
50-150 5.675e-07 3.162e-07
15-150 9.877e-07 5.288e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.02756 (-2.18406 2.95651)
R1^2/D10^2 : 0.872100 (-0.747319 11.3741)
kT2 [keV] : 20.0847 (-4.54428 12.7555)
R2^2/D10^2 : 8.89695E-03 (-0.00775633 0.0146907)
------------------------------------------------------------
#Fit statistic : Chi-Squared 45.42 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.18e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.500e-07 7.651e-08
25- 50 2.564e-07 9.145e-08
50-150 5.449e-07 2.416e-07
15-150 9.513e-07 3.670e-07
Peak spectrum fit
Power-law model
Time interval is from -0.508 sec. to 0.492 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.45358 ( -0.233655 0.234691 )
Norm@50keV : 1.44630E-02 ( -0.00219142 0.00218391 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 54.19 using 59 bins.
Reduced chi-squared = 0.950702
# Null hypothesis probability of 5.81e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 1.78398 ( -0.2716 0.27217 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.38331e-07 ( -2.25306e-08 2.2741e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.508 sec. to 0.492 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 8.06125E-02 ( -1.7218 1.14172 )
Epeak [keV] : 67.0294 ( -16.1528 92.7463 )
Norm@50keV : 7.57985E-02 ( -0.0758352 0.55273 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 49.73 using 59 bins.
Reduced chi-squared = 0.888036
# Null hypothesis probability of 7.10e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 1.71980 ( -0.2797 0.27901 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.26145e-07 ( -2.53799e-08 2.5595e-08 ) ergs/cm2
Band function
Time interval is from -0.508 sec. to 0.492 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] : 14.0944 (-2.06668 2.57528)
R^2/D10^2 : 0.271431 (-0.123632 0.207112)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 52.44 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.47e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.138e-08 3.128e-09
25- 50 4.262e-08 8.915e-09
50-150 5.594e-08 1.720e-08
15-150 1.099e-07 2.177e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.363 (-83.9379 -199.363)
Norm : 7.42928 (-1.10034 1.10042)
------------------------------------------------------------
#Fit statistic : Chi-Squared 52.71 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.37e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.850e-08 1.037e-08
25- 50 3.559e-08 2.005e-08
50-150 7.805e-08 4.377e-08
15-150 1.321e-07 7.440e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 10.7347 (-3.57289 3.33548)
R1^2/D10^2 : 0.547242 (-0.280378 0.814673)
kT2 [keV] : 37.5695 (-35.3047 -42.7583)
R2^2/D10^2 : 4.48320E-03 (-0.00293875 0.0800793)
------------------------------------------------------------
#Fit statistic : Chi-Squared 47.32 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.59e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.396e-08 8.185e-09
25- 50 4.161e-08 2.492e-08
50-150 7.334e-08 3.882e-08
15-150 1.289e-07 6.720e-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: 1.47208 ( -0.213556 0.214261 )
Norm@50keV : 4.29557E-03 ( -0.000569666 0.000567831 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 49.22 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.58e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 11.23 sec: 0.532331 ( -0.0713273 0.0715091 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.5979e-07 ( -6.56117e-08 6.62742e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.291399 ( -1.26778 0.972809 )
Epeak [keV] : 71.6186 ( -16.5132 97.5422 )
Norm@50keV : 1.70794E-02 ( -0.0170794 0.0557731 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 44.77 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.59e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 11.23 sec: 0.509327 ( -0.074222 0.074204 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.25058e-07 ( -7.07366e-08 7.25885e-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) = 2.64e-07
S(50-100 keV) = 3.46e-07
T90 vs. Hardness ratio plot
T90 = 51.1399999856949 sec.
Hardness ratio (energy fluence ratio) = 1.31061
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.18425
Count Ratio (50-100 keV) / (15-25 keV) = 0.988403
Mask shadow pattern
IMX = 7.933018136795843E-01, IMY = 1.162109312197978E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.512000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.512000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.512000
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:
-56.891410 -1.120000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6354 22.0429 0.8 22.3 71.3 2.3435 15.2 1.7 Crab
67.5883 47.9083 2.5 42.6 30.4 1.1321 4.7 ------ UNKNOWN
28.8854 51.6369 2.4 56.6 3.0 2.6738 4.8 ------ UNKNOWN
56.7704 -9.0195 2.4 18.4 -110.2 0.5924 4.7 ------ UNKNOWN
25.6088 15.9678 2.2 43.2 -41.2 1.2926 5.2 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-1.120000 10.108600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.5884 22.1499 5.4 22.4 71.1 0.1240 2.1 8.5 Crab
39.7779 33.6152 1.1 38.7 -8.3 0.6959 10.9 ------ UNKNOWN
40.8928 18.6346 2.4 29.8 -30.1 0.2539 4.8 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
112.708590 714.368000
720.408000 837.726200
840.408000 962.511800
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
78.4881 32.9166 3.4 32.2 77.4 7.7339 3.4 ------ UNKNOWN
42.1788 3.4336 2.4 30.3 172.4 6.4577 4.8 ------ UNKNOWN
Plot creation:
Sat Mar 9 15:20:29 EST 2024