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
60.5556 -50.2446 0.0263 19.5270 -69.3260 0.4516108 7.354 TRIG_00965484
Foreground time interval of the image:
-0.512 16.789 (delta_t = 17.301 [sec])
Background time interval of the image:
-239.512 -0.512 (delta_t = 239.000 [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
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 -0.512 sec. to 19.488 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.11733 ( -0.418263 0.481696 )
Norm@50keV : 1.23946E-03 ( -0.000397747 0.000378088 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 43.65 using 59 bins.
Reduced chi-squared = 0.765789
# Null hypothesis probability of 9.03e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 20 sec: 0.196701 ( -0.039995 0.040024 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.30766e-07 ( -6.22156e-08 6.6695e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.512 sec. to 19.488 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.57162 ( -1.282 0.244805 )
Epeak [keV] : 198.699 ( )
Norm@50keV : 7.10627E-04 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared 42.81 using 59 bins.
Reduced chi-squared = 0.764464
# Null hypothesis probability of 9.03e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 20 sec: 0.156090 ( -0.0565071 0.074096 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.82448e-07 ( -1.10558e-07 1.82776e-07 ) ergs/cm2
Band function
Time interval is from -0.512 sec. to 19.488 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] : 7.16181 (-1.64692 2.14126)
R^2/D10^2 : 0.327473 (-0.212138 0.623559)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 49.90 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.36e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.523e-08 2.452e-08
25- 50 7.903e-08 3.826e-08
50-150 1.421e-08 1.033e-08
15-150 1.485e-07 6.709e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 47.4466 (-23.318 78.2451)
Norm : 1.13420 (-0.385763 0.723724)
------------------------------------------------------------
#Fit statistic : Chi-Squared 45.42 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.65e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.477e-08 1.676e-08
25- 50 7.717e-08 2.846e-08
50-150 7.125e-08 4.530e-08
15-150 2.032e-07 8.078e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.99318 (-1.57399 1.85233)
R1^2/D10^2 : 0.620265 (-0.447855 1.4107)
kT2 [keV] : 77.5699 (-75.6965 -98.5808)
R2^2/D10^2 : 1.11358E-04 (-6.38871e-05 0.00249238)
------------------------------------------------------------
#Fit statistic : Chi-Squared 40.54 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.27e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.013e-08 3.459e-08
25- 50 6.677e-08 3.875e-08
50-150 1.423e-07 9.577e-08
15-150 2.692e-07 1.424e-07
Peak spectrum fit
Power-law model
Time interval is from -0.512 sec. to 0.488 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.48238 ( -0.431521 0.445604 )
Norm@50keV : 5.75025E-03 ( -0.00160642 0.00158344 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 44.77 using 59 bins.
Reduced chi-squared = 0.785439
# Null hypothesis probability of 8.80e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.714538 ( -0.191964 0.19232 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.47142e-08 ( -1.63603e-08 1.68556e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.512 sec. to 0.488 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.265333 ( -2.68119 1.51817 )
Epeak [keV] : 68.7967 ( -23.6805 -68.7967 )
Norm@50keV : 2.47084E-02 ( -0.0247084 0.52205 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 43.36 using 59 bins.
Reduced chi-squared = 0.774286
# Null hypothesis probability of 8.91e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.687666 ( -0.196083 0.19642 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.03002e-08 ( -1.66095e-08 1.80359e-08 ) ergs/cm2
Band function
Time interval is from -0.512 sec. to 0.488 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] : 14.8569 (-4.07297 5.58234)
R^2/D10^2 : 8.82116E-02 (-0.0594967 0.180993)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 44.75 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.81e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.083e-09 2.501e-09
25- 50 1.608e-08 9.795e-09
50-150 2.405e-08 1.500e-08
15-150 4.421e-08 2.199e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.363 (-199.363 -199.363)
Norm : 2.95313 (-0.780975 0.930354)
------------------------------------------------------------
#Fit statistic : Chi-Squared 44.19 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.93e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.354e-09 4.288e-09
25- 50 1.415e-08 8.595e-09
50-150 3.102e-08 1.880e-08
15-150 5.252e-08 3.096e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.05350 (-6.09119 -6.09119)
R1^2/D10^2 : 0.883465 (-0.880581 -0.880581)
kT2 [keV] : 19.3354 (-19.3754 -19.3754)
R2^2/D10^2 : 2.91864E-02 (-0.0290833 0.141889)
------------------------------------------------------------
#Fit statistic : Chi-Squared 43.02 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.79e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.487e-09 3.746e-09
25- 50 1.480e-08 7.515e-09
50-150 2.902e-08 1.800e-08
15-150 5.031e-08 2.860e-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: 2.11846 ( -0.401217 0.461112 )
Norm@50keV : 1.35807E-03 ( -0.00042231 0.00040363 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 41.91 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.33e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 17.3 sec: 0.215627 ( -0.0431665 0.0431883 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.18696e-07 ( -5.74194e-08 6.14781e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.42333 ( -1.85111 0.198314 )
Epeak [keV] : 157.631 ( )
Norm@50keV : 9.23034E-04 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared 41.53 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.25e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 17.3 sec: 0.215244 ( -0.042922 0.043122 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.18881e-07 ( -6.69588e-08 5.95328e-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) = 7.18e-08
S(50-100 keV) = 6.62e-08
T90 vs. Hardness ratio plot
T90 = 16 sec.
Hardness ratio (energy fluence ratio) = 0.922006
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 0.725094
Count Ratio (50-100 keV) / (15-25 keV) = 0.304899
Mask shadow pattern
IMX = 1.252090946347269E-01, IMY = 3.318117338568732E-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:
-239.512000 -0.512000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.5369 -40.5455 1.6 39.0 51.3 4.3505 7.2 0.7 Vela X-1
170.3296 -60.4467 10.5 36.5 99.6 -0.6844 -1.1 10.6 Cen X-3
186.8066 -62.8850 6.3 39.7 111.9 1.6613 1.8 8.0 GX 301-2
151.9471 -66.4892 2.6 26.4 98.3 1.6877 4.4 ------ UNKNOWN
93.6940 -9.3473 2.7 57.6 -11.0 4.9364 4.2 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-0.512000 16.788590
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.5210 -40.6905 5.8 38.9 51.4 0.2494 2.0 8.2 Vela X-1
170.4362 -60.6734 8.1 36.4 100.0 0.1840 1.4 4.7 Cen X-3
186.9356 -62.7399 7.8 39.8 111.8 0.2840 1.5 7.9 GX 301-2
178.4574 -57.8453 2.6 41.2 102.1 1.0220 4.4 ------ UNKNOWN
94.5950 -27.8991 3.1 39.2 -7.0 0.2639 3.7 ------ UNKNOWN
60.5557 -50.2446 1.6 19.5 -69.3 0.4491 7.3 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
57.788590 898.988600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
309.0769 -62.7506 3.9 54.8 167.4 9.7764 3.0 ------ UNKNOWN
13.4701 -60.4045 3.2 27.9 -173.4 2.6384 3.6 ------ UNKNOWN
2.7497 -37.7794 2.7 42.3 -139.8 5.8876 4.4 ------ UNKNOWN
Plot creation:
Wed May 5 20:16:23 EDT 2021