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
22.0856 -11.9254 0.0197 20.8363 53.0294 0.8679399 9.783 TRIG_00775553
Foreground time interval of the image:
12.028 34.196 (delta_t = 22.168 [sec])
Background time interval of the image:
-13.099 12.028 (delta_t = 25.127 [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 12.028 sec. to 34.196 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.44356 ( -0.200632 0.20292 )
Norm@50keV : 2.68908E-03 ( -0.000305544 0.000303363 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 69.42 using 59 PHA bins.
# Reduced chi-squared = 1.218 for 57 degrees of freedom
# Null hypothesis probability = 1.251110e-01
Photon flux (15-150 keV) in 22.17 sec: 0.330873 ( -0.03696 0.03703 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.7125e-07 ( -7.23704e-08 7.32987e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 12.028 sec. to 34.196 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.30323 ( )
Epeak [keV] : 253.945 ( )
Norm@50keV : 3.15706E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 69.33 using 59 PHA bins.
# Reduced chi-squared = 1.238 for 56 degrees of freedom
# Null hypothesis probability = 1.086373e-01
Photon flux (15-150 keV) in 22.17 sec: 0.328567 ( -0.039362 0.038652 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.65062e-07 ( -8.07833e-08 7.78706e-08 ) ergs/cm2
Band function
Time interval is from 12.028 sec. to 34.196 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] : 15.9237 (-2.0868 2.49459)
R^2/D10^2 : 3.06356E-02 (-0.0120897 0.0192148)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 85.45 using 59 PHA bins.
# Reduced chi-squared = 1.499 for 57 degrees of freedom
# Null hypothesis probability = 8.696507e-03
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.565e-08 7.815e-09
25- 50 1.494e-07 2.511e-08
50-150 2.643e-07 5.882e-08
15-150 4.493e-07 7.183e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-60.5077 -200)
Norm : 1.35532 (-0.14901 0.14901)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 70.39 using 59 PHA bins.
# Reduced chi-squared = 1.235 for 57 degrees of freedom
# Null hypothesis probability = 1.096415e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.483e-08 4.179e-08
25- 50 1.439e-07 7.731e-08
50-150 3.157e-07 1.727e-07
15-150 5.345e-07 2.914e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 2.90913 (-1.18255 1.96558)
R1^2/D10^2 : 14.6360 (-13.5889 129.096)
kT2 [keV] : 18.9827 (-2.94315 4.16582)
R2^2/D10^2 : 1.56729E-02 (-0.00787164 0.0122874)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 66.89 using 59 PHA bins.
# Reduced chi-squared = 1.216 for 55 degrees of freedom
# Null hypothesis probability = 1.305512e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.460e-08 3.287e-08
25- 50 1.249e-07 2.773e-08
50-150 3.133e-07 7.977e-08
15-150 5.128e-07 1.181e-07
Peak spectrum fit
Power-law model
Time interval is from 31.416 sec. to 32.416 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.65999 ( -0.330967 0.353295 )
Norm@50keV : 7.22888E-03 ( -0.00158985 0.00153741 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 54.57 using 59 PHA bins.
# Reduced chi-squared = 0.9574 for 57 degrees of freedom
# Null hypothesis probability = 5.667224e-01
Photon flux (15-150 keV) in 1 sec: 0.947083 ( -0.179113 0.179137 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.71754e-08 ( -1.5342e-08 1.58536e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 31.416 sec. to 32.416 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.16929 ( -1.51679 1.11304 )
Epeak [keV] : 77.6203 ( -37.0242 -77.6184 )
Norm@50keV : 1.33710E-02 ( -0.0133713 0.0748494 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 54.10 using 59 PHA bins.
# Reduced chi-squared = 0.9661 for 56 degrees of freedom
# Null hypothesis probability = 5.471054e-01
Photon flux (15-150 keV) in 1 sec: 0.930393 ( -0.183583 0.183637 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.42407e-08 ( -1.63887e-08 1.72992e-08 ) ergs/cm2
Band function
Time interval is from 31.416 sec. to 32.416 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] : 12.8708 (-3.05138 4.01087)
R^2/D10^2 : 0.180342 (-0.110875 0.294934)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 60.76 using 59 PHA bins.
# Reduced chi-squared = 1.066 for 57 degrees of freedom
# Null hypothesis probability = 3.420622e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.337e-09 2.231e-09
25- 50 2.159e-08 7.300e-09
50-150 2.248e-08 9.896e-09
15-150 5.040e-08 1.649e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 145.049 (-78.6397 -142.391)
Norm : 3.91503 (-0.792036 1.12816)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 54.15 using 59 PHA bins.
# Reduced chi-squared = 0.9500 for 57 degrees of freedom
# Null hypothesis probability = 5.826240e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.008e-08 5.685e-09
25- 50 1.860e-08 1.048e-08
50-150 3.620e-08 2.227e-08
15-150 6.488e-08 3.802e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.22145 (-2.51514 3.42672)
R1^2/D10^2 : 2.87145 (-2.38003 53.4986)
kT2 [keV] : 20.0481 (-6.17478 14.6669)
R2^2/D10^2 : 3.04956E-02 (-0.0263655 0.0529037)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 53.08 using 59 PHA bins.
# Reduced chi-squared = 0.9652 for 55 degrees of freedom
# Null hypothesis probability = 5.481539e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.064e-08 6.135e-09
25- 50 1.779e-08 8.915e-09
50-150 3.540e-08 2.180e-08
15-150 6.383e-08 3.371e-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: 1.44356 ( -0.200632 0.20292 )
Norm@50keV : 2.68908E-03 ( -0.000305544 0.000303363 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 69.42 using 59 PHA bins.
# Reduced chi-squared = 1.218 for 57 degrees of freedom
# Null hypothesis probability = 1.251110e-01
Photon flux (15-150 keV) in 22.17 sec: 0.330866 ( -0.036958 0.0370281 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.71172e-07 ( -7.23602e-08 7.33078e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.30175 ( -0.905867 1.23019 )
Epeak [keV] : 249.038 ( -254.282 -254.282 )
Norm@50keV : 3.16088E-03 ( -0.00138249 0.00547149 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 69.34 using 59 PHA bins.
# Reduced chi-squared = 1.238 for 56 degrees of freedom
# Null hypothesis probability = 1.086190e-01
Photon flux (15-150 keV) in 22.17 sec: 0.328530 ( -0.039353 0.038499 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.65284e-07 ( -8.08185e-08 7.80362e-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) = 1.37e-07
S(50-100 keV) = 2.02e-07
T90 vs. Hardness ratio plot
T90 = 20.9159999489784 sec.
Hardness ratio (energy fluence ratio) = 1.47445
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.17403
Count Ratio (50-100 keV) / (15-25 keV) = 1.14072
Mask shadow pattern
IMX = 2.288884879572669E-01, IMY = -3.040696127955854E-01
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:
-13.099400 12.028000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
12.028000 34.196000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
22.0856 -11.9254 1.2 20.8 53.0 0.8678 9.8 ------ UNKNOWN
351.9142 52.8389 2.2 56.9 176.6 2.5095 5.3 ------ UNKNOWN
50.1920 40.4765 2.5 37.8 -133.0 0.5349 4.7 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
175.300590 963.090000
1503.000000 1503.200600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
2.1113 22.8774 2.3 39.9 103.9 10.8400 5.1 ------ UNKNOWN
23.2210 15.4319 2.1 27.3 135.7 4.0826 5.6 ------ UNKNOWN
334.7687 -33.0711 3.5 48.0 9.2 3.4101 3.3 ------ UNKNOWN
326.9806 -44.0337 4.2 56.9 -2.0 6.9574 2.8 ------ UNKNOWN
339.2112 -44.8871 2.6 49.2 -7.2 4.9064 4.5 ------ UNKNOWN
64.7543 5.1296 2.5 45.7 -156.1 4.6662 4.6 ------ UNKNOWN
70.6902 4.2278 2.7 51.0 -152.2 6.4170 4.3 ------ UNKNOWN
Plot creation:
Fri Oct 20 14:57:46 EDT 2017