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
201.3113 25.6239 0.0147 25.3208 -151.9481 1.8900647 13.074 TRIG_01280056
Foreground time interval of the image:
-63.136 34.645 (delta_t = 97.781 [sec])
Background time interval of the image:
-239.056 -63.136 (delta_t = 175.920 [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 4.096000
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 4.096000
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 4.096000
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 -63.136 sec. to 218.208 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.62411 ( -0.188932 0.192729 )
Norm@50keV : 6.42983E-04 ( -7.12043e-05 7.00916e-05 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 62.96 using 59 bins.
Reduced chi-squared = 1.10456
# Null hypothesis probability of 2.74e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 281.3 sec: 8.32582E-02 ( -0.0085896 0.0086034 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.68702e-06 ( -2.00056e-07 2.02494e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -63.136 sec. to 218.208 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.62913 ( -0.19618 0.187791 )
Epeak [keV] : 9999.36 ( -9999.35 -9999.36 )
Norm@50keV : 6.43321E-04 ( -0.000249105 0.000401045 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 62.97 using 59 bins.
Reduced chi-squared = 1.12446
# Null hypothesis probability of 2.43e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 281.3 sec: 8.32551E-02 ( -0.008597 0.0085979 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.68659e-06 ( -2.00211e-07 2.02443e-07 ) ergs/cm2
Band function
Time interval is from -63.136 sec. to 218.208 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] : 13.5219 (-2.1404 2.63978)
R^2/D10^2 : 1.27176E-02 (-0.00586944 0.0108742)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 102.74 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.96e-04 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.385e-07 2.989e-08
25- 50 4.974e-07 7.848e-08
50-150 5.879e-07 1.238e-07
15-150 1.224e-06 1.871e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 181.684 (-75.8447 -181.445)
Norm : 0.336682 (-0.0358854 0.0431951)
------------------------------------------------------------
#Fit statistic : Chi-Squared 65.16 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.14e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.386e-07 1.321e-07
25- 50 4.538e-07 2.423e-07
50-150 9.641e-07 5.304e-07
15-150 1.656e-06 8.876e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.84236 (-1.33472 1.60427)
R1^2/D10^2 : 0.200287 (-0.119106 0.368447)
kT2 [keV] : 27.9265 (-6.75191 13.6899)
R2^2/D10^2 : 8.46773E-04 (-0.000599814 0.00134754)
------------------------------------------------------------
#Fit statistic : Chi-Squared 61.51 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.54e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.760e-07 1.159e-07
25- 50 4.126e-07 1.295e-07
50-150 1.043e-06 5.020e-07
15-150 1.732e-06 6.512e-07
Peak spectrum fit
Power-law model
Time interval is from 1.556 sec. to 2.556 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.930293 ( -0.516423 0.447196 )
Norm@50keV : 5.18943E-03 ( -0.00135007 0.0012785 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 58.81 using 59 bins.
Reduced chi-squared = 1.03175
# Null hypothesis probability of 4.09e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.595897 ( -0.150571 0.151414 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.75732e-08 ( -1.43278e-08 1.43767e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 1.556 sec. to 2.556 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.941807 ( -0.753484 0.434345 )
Epeak [keV] : 9999.36 ( -9999.36 -9999.36 )
Norm@50keV : 5.23858E-03 ( -0.0012242 0.00805731 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 58.83 using 59 bins.
Reduced chi-squared = 1.05054
# Null hypothesis probability of 3.72e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.595880 ( -0.150685 0.151283 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.75771e-08 ( -1.43556e-08 1.43661e-08 ) ergs/cm2
Band function
Time interval is from 1.556 sec. to 2.556 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] : 28.4696 (-9.9604 23.2802)
R^2/D10^2 : 9.48442E-03 (-0.00939005 0.0260057)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 65.14 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.15e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.241e-09 7.880e-10
25- 50 7.489e-09 4.477e-09
50-150 4.368e-08 2.550e-08
15-150 5.241e-08 3.085e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-72.5222 -200)
Norm : 2.48387 (-0.619327 0.619327)
------------------------------------------------------------
#Fit statistic : Chi-Squared 64.70 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.26e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.189e-09 3.691e-09
25- 50 1.191e-08 7.130e-09
50-150 2.611e-08 1.512e-08
15-150 4.420e-08 2.668e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 8.10134 (-3.90176 6.83685)
R1^2/D10^2 : 0.357712 (-0.298234 3.32375)
kT2 [keV] : 65.9258 (-45.5436 -69.6769)
R2^2/D10^2 : 9.73120E-04 (-0.000763035 0.00625812)
------------------------------------------------------------
#Fit statistic : Chi-Squared 57.29 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.90e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.654e-09 3.096e-09
25- 50 1.048e-08 5.885e-09
50-150 4.557e-08 2.409e-08
15-150 6.071e-08 3.064e-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: 1.56124 ( -0.156073 0.157967 )
Norm@50keV : 1.35624E-03 ( -0.00012504 0.000124086 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 47.85 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.01e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 97.78 sec: 0.172257 ( -0.0154326 0.0154573 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.24646e-06 ( -1.2445e-07 1.25596e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.39302 ( -0.613821 0.309832 )
Epeak [keV] : 178.483 ( -178.482 -178.482 )
Norm@50keV : 1.65438E-03 ( -0.000562324 0.00168417 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 47.59 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.81e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 97.78 sec: 0.170968 ( -0.016 0.015797 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.23094e-06 ( -6.88176e-08 1.3522e-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) = 4.42e-07
S(50-100 keV) = 5.74e-07
T90 vs. Hardness ratio plot
T90 = 218.111999988556 sec.
Hardness ratio (energy fluence ratio) = 1.29864
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.04545
Count Ratio (50-100 keV) / (15-25 keV) = 0.784496
Mask shadow pattern
IMX = -4.175576600804364E-01, IMY = 2.225047426076106E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 4.096000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 4.096000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 4.096000
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:
-239.056000 -63.136000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
180.8333 -37.8027 2.6 44.9 -9.8 1.6485 4.4 ------ UNKNOWN
212.8918 38.3743 2.2 41.2 -156.6 1.9574 5.2 ------ UNKNOWN
203.8480 -45.7546 2.8 55.9 -29.8 5.1248 4.1 ------ UNKNOWN
230.2548 24.3532 3.0 48.1 -129.2 3.9254 3.9 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-63.136000 34.644600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
154.1209 -17.8547 2.7 38.1 36.3 1.0532 4.3 ------ UNKNOWN
201.3113 25.6239 0.9 25.3 -151.9 1.8896 13.1 ------ UNKNOWN
206.2216 -4.5894 2.3 25.6 -76.3 0.8496 5.0 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
96.044590 963.058300
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.3997 35.4475 5.4 46.2 -136.1 -5.5506 -2.1 6.9 Her X-1
255.9716 30.2195 2.7 48.1 -129.2 21.0531 4.3 ------ UNKNOWN
Plot creation:
Fri Jun 20 01:55:38 EDT 2025