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
245.2222 58.1319 0.0074 45.7784 -152.6068 3.0612679 25.669 TRIG_01205319
Foreground time interval of the image:
0.252 17.264 (delta_t = 17.012 [sec])
Background time interval of the image:
-239.376 0.252 (delta_t = 239.628 [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 3.072000
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 3.072000
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 3.072000
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 0.252 sec. to 17.264 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.27724 ( -0.0955486 0.0945992 )
Norm@50keV : 1.26752E-02 ( -0.000704192 0.00070336 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 41.72 using 59 bins.
Reduced chi-squared = 0.73193
# Null hypothesis probability of 9.36e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 17.01 sec: 1.50604 ( -0.08971 0.08997 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.14292e-06 ( -1.24069e-07 1.24304e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.252 sec. to 17.264 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.888209 ( -0.416189 0.378134 )
Epeak [keV] : 162.298 ( -55.8615 1805.85 )
Norm@50keV : 1.90098E-02 ( -0.00598626 0.00985355 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 38.67 using 59 bins.
Reduced chi-squared = 0.690536
# Null hypothesis probability of 9.63e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 17.01 sec: 1.47977 ( -0.09323 0.09348 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.11035e-06 ( -1.29757e-07 1.29223e-07 ) ergs/cm2
Band function
Time interval is from 0.252 sec. to 17.264 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] : 19.3627 (-1.30501 1.43828)
R^2/D10^2 : 7.60639E-02 (-0.0165745 0.0206405)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 93.31 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.72e-03 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 9.469e-08 1.106e-08
25- 50 4.614e-07 3.751e-08
50-150 1.276e-06 1.158e-07
15-150 1.832e-06 1.305e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-10.4946 -200)
Norm : 6.40628 (-0.358365 0.358365)
------------------------------------------------------------
#Fit statistic : Chi-Squared 65.75 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.00e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.714e-07 1.786e-08
25- 50 5.222e-07 3.393e-08
50-150 1.145e-06 1.001e-07
15-150 1.939e-06 2.532e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.27094 (-1.53428 2.00285)
R1^2/D10^2 : 1.07111 (-0.572396 1.39144)
kT2 [keV] : 27.8100 (-3.77393 6.42563)
R2^2/D10^2 : 1.91224E-02 (-0.00996478 0.0133182)
------------------------------------------------------------
#Fit statistic : Chi-Squared 38.74 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.53e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.019e-07 5.992e-08
25- 50 4.825e-07 9.662e-08
50-150 1.423e-06 2.503e-07
15-150 2.108e-06 3.736e-07
Peak spectrum fit
Power-law model
Time interval is from 7.636 sec. to 8.636 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.25692 ( -0.248183 0.240893 )
Norm@50keV : 1.89766E-02 ( -0.00290896 0.00290174 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 47.21 using 59 bins.
Reduced chi-squared = 0.828246
# Null hypothesis probability of 8.19e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 2.24699 ( -0.36542 0.36753 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.89596e-07 ( -2.98574e-08 2.99118e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 7.636 sec. to 8.636 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.348376 ( -1.47532 1.00171 )
Epeak [keV] : 102.234 ( -102.234 -102.234 )
Norm@50keV : 4.95795E-02 ( -0.0495796 0.175344 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 45.22 using 59 bins.
Reduced chi-squared = 0.8075
# Null hypothesis probability of 8.48e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 2.18744 ( -0.37376 0.37569 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.8482e-07 ( -3.17077e-08 3.11234e-08 ) ergs/cm2
Band function
Time interval is from 7.636 sec. to 8.636 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] : 18.3899 (-2.82776 3.71664)
R^2/D10^2 : 0.142233 (-0.0678083 0.113053)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 49.12 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.62e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 9.563e-09 2.996e-09
25- 50 4.493e-08 1.312e-08
50-150 1.109e-07 3.270e-08
15-150 1.654e-07 3.600e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-48.5353 -200)
Norm : 9.61447 (-1.48231 1.48231)
------------------------------------------------------------
#Fit statistic : Chi-Squared 50.77 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.06e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.395e-08 1.346e-08
25- 50 4.608e-08 2.581e-08
50-150 1.011e-07 5.685e-08
15-150 1.711e-07 9.625e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 13.2253 (-6.94041 5.16096)
R1^2/D10^2 : 0.321848 (-0.190118 3.81167)
kT2 [keV] : 50.7079 (-54.6852 -54.6853)
R2^2/D10^2 : 3.06108E-03 (-0.00206643 0.120572)
------------------------------------------------------------
#Fit statistic : Chi-Squared 44.58 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.41e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.464e-08 4.673e-09
25- 50 4.196e-08 1.263e-08
50-150 1.144e-07 3.526e-08
15-150 1.710e-07 3.925e-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: 1.27724 ( -0.0955486 0.0945992 )
Norm@50keV : 1.26752E-02 ( -0.000704192 0.00070336 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 41.72 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.36e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 17.01 sec: 1.50603 ( -0.0897092 0.0899576 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.14265e-06 ( -1.24134e-07 1.24323e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.888210 ( -0.41619 0.378133 )
Epeak [keV] : 162.298 ( -55.8616 1804.93 )
Norm@50keV : 1.90098E-02 ( -0.00598625 0.00985356 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 38.67 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.63e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 17.01 sec: 1.47966 ( -0.0932 0.09345 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.11125e-06 ( -1.29922e-07 1.2931e-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) = 4.71e-07
S(50-100 keV) = 7.77e-07
T90 vs. Hardness ratio plot
T90 = 15.2400000095367 sec.
Hardness ratio (energy fluence ratio) = 1.64968
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.78274
Count Ratio (50-100 keV) / (15-25 keV) = 1.86239
Mask shadow pattern
IMX = -9.123296062587759E-01, IMY = 4.727695310907867E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 3.072000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 3.072000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 3.072000
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:
-239.376000 0.252000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
149.6276 27.4243 3.1 32.2 77.4 2.9041 3.8 ------ UNKNOWN
185.7151 12.0491 2.8 21.5 -9.6 1.5196 4.1 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
0.252000 17.264000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
126.6530 72.5296 2.4 49.3 148.3 1.1498 4.9 ------ UNKNOWN
245.2222 58.1319 0.4 45.8 -152.6 3.0611 25.6 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
126.124610 962.695700
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.4576 35.3424 108.5 23.6 -78.4 0.1406 0.1 0.0 Her X-1
299.5716 35.2236 1.4 42.2 -140.7 17.2011 8.5 1.6 Cyg X-1
308.1447 41.0549 3.1 42.4 -153.9 7.1467 3.8 6.3 Cyg X-3
326.2854 38.2895 4.8 53.9 -165.3 -7.9303 -2.4 5.7 Cyg X-2
172.9260 67.3621 3.0 32.2 77.5 9.6128 3.9 ------ UNKNOWN
293.4868 85.8685 2.1 29.3 127.2 9.0592 5.4 ------ UNKNOWN
240.0722 70.9455 2.4 13.0 113.6 5.5726 4.8 ------ UNKNOWN
203.8846 24.4512 2.4 44.5 -0.3 10.0829 4.9 ------ UNKNOWN
Plot creation:
Sat Mar 9 15:19:49 EST 2024