Click here for the BAT GCN circular template
Image
Pre-slew 15.0-350.0 keV image (Event data)
# RAcent DECcent POSerr Theta Phi Peak Cts SNR Name
121.3528 37.2630 0.0098 39.9715 -108.5032 19.3648902 19.689 TRIG_00282066
Foreground time interval of the image:
-4.696 417.864 (delta_t = 422.560 [sec])
Background time interval of the image:
-239.000 -4.696 (delta_t = 234.304 [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 64.000000
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 64.000000
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 64.000000
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 -4.696 sec. to 417.864 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.63995 ( -0.0915319 0.0920371 )
Norm@50keV : 2.75173E-03 ( -0.000145791 0.000145314 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 47.69 using 59 PHA bins.
# Reduced chi-squared = 0.8367 for 57 degrees of freedom
# Null hypothesis probability = 8.053735e-01
Photon flux (15-150 keV) in 422.6 sec: 0.358128 ( -0.0191716 0.0192051 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.08264e-05 ( -6.06477e-07 6.08975e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -4.696 sec. to 417.864 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.43918 ( -0.357111 0.248206 )
Epeak [keV] : 137.694 ( )
Norm@50keV : 3.48654E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 46.63 using 59 PHA bins.
# Reduced chi-squared = 0.8327 for 56 degrees of freedom
# Null hypothesis probability = 8.095078e-01
Photon flux (15-150 keV) in 422.6 sec: 0.354543 ( -0.020022 0.020029 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.0663e-05 ( -6.72399e-07 6.67793e-07 ) ergs/cm2
Band function
Time interval is from -4.696 sec. to 417.864 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 4.96006 ( -4.67666 -4.96006 )
beta : -1.73841 ( -0.12122 0.106329 )
Epeak [keV] : 24.6647 ( -3.06101 2.6627 )
Norm@50keV : 333.766 ( -16.9831 616.893 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 39.47 using 59 PHA bins.
# Reduced chi-squared = 0.7177 for 55 degrees of freedom
# Null hypothesis probability = 9.433056e-01
Photon flux (15-150 keV) in 422.6 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] : 13.8300 ( )
R^2/D10^2 : 5.12549E-02 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 146.51 using 59 PHA bins.
# Reduced chi-squared = 2.5704 for 57 degrees of freedom
# Null hypothesis probability = 8.112258e-10
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.761e-07 8.431e-08
25- 50 3.219e-06 2.227e-07
50-150 4.028e-06 4.116e-07
15-150 8.123e-06 5.135e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 160.469 (-35.8651 -160.274)
Norm : 1.46664 (-0.0881944 0.0976521)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 47.10 using 59 PHA bins.
# Reduced chi-squared = 0.8263 for 57 degrees of freedom
# Null hypothesis probability = 8.221817e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.582e-06 1.204e-07
25- 50 2.961e-06 2.681e-07
50-150 6.005e-06 1.935e-06
15-150 1.055e-05 2.371e-06
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.98492 (-0.941788 1.04978)
R1^2/D10^2 : 0.428672 (-0.16357 0.28926)
kT2 [keV] : 27.4229 (-4.39541 6.88303)
R2^2/D10^2 : 3.42154E-03 (-0.00183511 0.003182)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 41.75 using 59 PHA bins.
# Reduced chi-squared = 0.7591 for 55 degrees of freedom
# Null hypothesis probability = 9.060988e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.596e-06 2.715e-07
25- 50 2.997e-06 4.192e-07
50-150 6.143e-06 1.531e-06
15-150 1.074e-05 1.794e-06
Peak spectrum fit
Power-law model
Time interval is from 2.620 sec. to 3.620 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.616839 ( -0.486739 0.419424 )
Norm@50keV : 1.17333E-02 ( -0.00346556 0.00325317 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 47.69 using 59 PHA bins.
# Reduced chi-squared = 0.8367 for 57 degrees of freedom
# Null hypothesis probability = 8.053777e-01
Photon flux (15-150 keV) in 1 sec: 1.36721 ( -0.345462 0.35457 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.48844e-07 ( -3.35724e-08 3.35963e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 2.620 sec. to 3.620 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -1.39551E-02 ( -4.29074 0.946137 )
Epeak [keV] : 231.963 ( -337.035 -337.035 )
Norm@50keV : 1.89414E-02 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 47.43 using 59 PHA bins.
# Reduced chi-squared = 0.8470 for 56 degrees of freedom
# Null hypothesis probability = 7.855515e-01
Photon flux (15-150 keV) in 1 sec: 1.32628 ( -0.370963 0.18896 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.48595e-07 ( -3.4206e-08 3.3885e-08 ) ergs/cm2
Band function
Time interval is from 2.620 sec. to 3.620 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.845395 ( 0.845395 0.845395 )
beta : -0.616840 ( -0.419434 0.48636 )
Epeak [keV] : 18.8119 ( -18.8119 -18.8119 )
Norm@50keV : 1.58619E-02 ( -0.00729474 142328 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 47.69 using 59 PHA bins.
# Reduced chi-squared = 0.8671 for 55 degrees of freedom
# Null hypothesis probability = 7.472871e-01
Photon flux (15-150 keV) in 1 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] : 33.0912 (-8.67543 16.7306)
R^2/D10^2 : 1.65144E-02 (-0.0109729 0.0237353)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 47.92 using 59 PHA bins.
# Reduced chi-squared = 0.8406 for 57 degrees of freedom
# Null hypothesis probability = 7.988050e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.658e-09 1.384e-09
25- 50 1.704e-08 8.739e-09
50-150 1.260e-07 6.396e-08
15-150 1.457e-07 7.425e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 ( )
Norm : 5.78742 (-1.50159 1.50122)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 61.64 using 59 PHA bins.
# Reduced chi-squared = 1.081 for 57 degrees of freedom
# Null hypothesis probability = 3.137791e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.441e-08 8.670e-09
25- 50 2.772e-08 1.662e-08
50-150 6.079e-08 3.700e-08
15-150 1.029e-07 6.265e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.35621 (-5.14968 -5.14968)
R1^2/D10^2 : 1.39029 (-2.28368 37.5886)
kT2 [keV] : 36.1678 (-10.5228 -36.2413)
R2^2/D10^2 : 1.24579E-02 (-0.0124786 0.0191238)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 46.65 using 59 PHA bins.
# Reduced chi-squared = 0.8482 for 55 degrees of freedom
# Null hypothesis probability = 7.810061e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.675e-09 4.619e-09
25- 50 1.832e-08 1.010e-08
50-150 1.253e-07 7.335e-08
15-150 1.503e-07 8.300e-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: 1.63995 ( -0.0915319 0.0920371 )
Norm@50keV : 2.75173E-03 ( -0.000145791 0.000145314 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 47.69 using 59 PHA bins.
# Reduced chi-squared = 0.8367 for 57 degrees of freedom
# Null hypothesis probability = 8.053735e-01
Photon flux (15-150 keV) in 422.6 sec: 0.358128 ( -0.0191716 0.0192051 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.08264e-05 ( -6.06477e-07 6.08975e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.43918 ( -0.357111 0.248206 )
Epeak [keV] : 137.694 ( )
Norm@50keV : 3.48654E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 46.63 using 59 PHA bins.
# Reduced chi-squared = 0.8327 for 56 degrees of freedom
# Null hypothesis probability = 8.095078e-01
Photon flux (15-150 keV) in 422.6 sec: 0.354543 ( -0.020022 0.020029 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.0663e-05 ( -6.72399e-07 6.67793e-07 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 4.96006 ( -4.67666 -4.96006 )
beta : -1.73841 ( -0.12122 0.106329 )
Epeak [keV] : 24.6647 ( -3.06101 2.6627 )
Norm@50keV : 333.766 ( -16.9831 616.893 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 39.47 using 59 PHA bins.
# Reduced chi-squared = 0.7177 for 55 degrees of freedom
# Null hypothesis probability = 9.433056e-01
Photon flux (15-150 keV) in 422.6 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) = 2.86e-06
S(50-100 keV) = 3.67e-06
T90 vs. Hardness ratio plot
T90 = 365.27999997139 sec.
Hardness ratio (energy fluence ratio) = 1.28322
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.29907
Count Ratio (50-100 keV) / (15-25 keV) = 0.969134
Mask shadow pattern
IMX = -2.660250002177185E-01, IMY = 7.949191657710479E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 64.000000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 64.000000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 64.000000
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:
-239.000000 -4.696000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
211.8144 28.4434 2.1 35.9 97.9 1.9517 5.5 ------ UNKNOWN
276.8477 63.6733 2.5 49.4 16.2 2.0630 4.6 ------ UNKNOWN
171.2249 -0.4899 2.9 52.6 166.2 2.3368 4.0 ------ UNKNOWN
201.8755 50.2013 2.7 16.8 66.8 0.7206 4.3 ------ UNKNOWN
114.8842 41.8789 3.8 41.1 -98.2 2.6255 3.1 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-4.696000 417.864000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
136.7430 43.0152 2.5 27.1 -112.7 1.9277 4.6 ------ UNKNOWN
58.1749 70.2846 2.9 49.6 -42.0 5.1622 4.0 ------ UNKNOWN
121.3529 37.2631 0.6 40.0 -108.5 19.3673 19.7 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
910.300600 963.055700
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
170.3506 -60.5754 18.8 47.0 -52.4 -0.2213 -0.6 3.0 Cen X-3
186.4277 -62.8653 5.9 39.1 -51.8 0.2677 2.0 8.5 GX 301-2
244.9771 -15.6501 0.4 34.3 67.2 4.6936 28.4 0.6 Sco X-1
255.9520 -37.8573 2.4 10.9 87.1 0.3693 4.7 1.8 4U 1700-377
256.4036 -36.4965 4.0 12.3 88.6 0.2280 2.9 4.7 GX 349+2
262.9269 -24.7356 4.2 24.7 101.7 0.2965 2.7 4.5 GX 1+4
264.8191 -44.5973 7.5 7.6 145.4 0.1122 1.5 9.4 4U 1735-44
270.2761 -25.2221 4.8 26.2 116.9 0.2731 2.4 8.6 GX 5-1
270.4381 -25.7011 9.6 25.8 117.6 0.1491 1.4 7.7 GRS 1758-258
274.1325 -14.0146 6.5 38.0 115.7 0.4044 1.8 7.5 GX 17+2
275.7922 -30.5245 0.0 23.8 133.0 -0.1006 -1.0 11.7 H1820-303
284.9244 -25.0597 11.2 33.0 140.2 0.1384 1.0 10.3 HT1900.1-2455
262.9601 -33.9841 8.8 15.8 108.6 0.1061 1.3 9.1 GX 354-0
210.6532 -52.7964 1.9 28.2 -29.8 0.4834 6.2 ------ UNKNOWN
341.6461 -87.5355 2.9 41.1 -98.1 1.5453 3.9 ------ UNKNOWN
Plot creation:
Sun May 31 09:58:39 EDT 2015