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Image
Pre-slew 15.0-350.0 keV image (Event data)
# RAcent DECcent POSerr Theta Phi Peak Cts SNR Name
317.9481 -65.3892 0.0096 41.1648 -113.0263 6.0373332 19.647 TRIG_00436981
Foreground time interval of the image:
-12.308 13.013 (delta_t = 25.321 [sec])
Background time interval of the image:
-179.787 -12.308 (delta_t = 167.479 [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 1.024000
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 1.024000
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 1.024000
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)
The mask-weighted light curves based on cleaned DPHs
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 -12.308 sec. to 137.268 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.53739 ( -0.0340034 0.0339927 )
Norm@50keV : 1.87345E-02 ( -0.000315896 0.000315879 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 47.29 using 59 PHA bins.
# Reduced chi-squared = 0.8297 for 57 degrees of freedom
# Null hypothesis probability = 8.168520e-01
Photon flux (15-150 keV) in 149.6 sec: 2.36307 ( -0.0468084 0.0470627 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.64331e-05 ( -4.58312e-07 4.58623e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -12.308 sec. to 137.268 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.29530 ( -0.146605 0.142079 )
Epeak [keV] : 163.069 ( -40.6571 143.061 )
Norm@50keV : 2.39738E-02 ( -0.00315892 0.00376403 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 38.73 using 59 PHA bins.
# Reduced chi-squared = 0.6916 for 56 degrees of freedom
# Null hypothesis probability = 9.619380e-01
Photon flux (15-150 keV) in 149.6 sec: 2.30923 ( -0.0552 0.05557 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.59583e-05 ( -5.39458e-07 5.36166e-07 ) ergs/cm2
Band function
Time interval is from -12.308 sec. to 137.268 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.977886 ( -0.39001 0.82691 )
beta : -1.63492 ( 1.63564 0.0731071 )
Epeak [keV] : 81.2326 ( -36.6007 129.315 )
Norm@50keV : 3.64957E-02 ( -0.0136389 0.0926265 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 36.83 using 59 PHA bins.
# Reduced chi-squared = 0.6696 for 55 degrees of freedom
# Null hypothesis probability = 9.716648e-01
Photon flux (15-150 keV) in 149.6 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] : 16.8190 ( )
R^2/D10^2 : 0.168366 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 617.29 using 59 PHA bins.
# Reduced chi-squared = 10.830 for 57 degrees of freedom
# Null hypothesis probability = 4.993882e-95
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.455e-06 5.131e-08
25- 50 6.384e-06 1.601e-07
50-150 1.285e-05 3.665e-07
15-150 2.069e-05 3.964e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 ( )
Norm : 9.59601 (-0.161591 0.161586)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 47.26 using 59 PHA bins.
# Reduced chi-squared = 0.8292 for 57 degrees of freedom
# Null hypothesis probability = 8.176136e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.575e-06 7.256e-08
25- 50 6.878e-06 1.399e-07
50-150 1.508e-05 3.134e-07
15-150 2.554e-05 5.012e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 8.13385 (-0.593626 0.618358)
R1^2/D10^2 : 1.37844 (-0.289971 0.398378)
kT2 [keV] : 28.9525 (-2.17258 2.72499)
R2^2/D10^2 : 1.98366E-02 (-0.00544887 0.00659137)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 52.76 using 59 PHA bins.
# Reduced chi-squared = 0.9593 for 55 degrees of freedom
# Null hypothesis probability = 5.605331e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.895e-06 1.915e-07
25- 50 6.914e-06 2.244e-07
50-150 1.574e-05 7.637e-07
15-150 2.555e-05 8.826e-07
Peak spectrum fit
Power-law model
Time interval is from 57.344 sec. to 58.344 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.13044 ( -0.037753 0.0376752 )
Norm@50keV : 0.181506 ( -0.00373229 0.00373014 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 62.31 using 59 PHA bins.
# Reduced chi-squared = 1.093 for 57 degrees of freedom
# Null hypothesis probability = 2.931317e-01
Photon flux (15-150 keV) in 1 sec: 21.1200 ( -0.456599 0.45722 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.87966e-06 ( -4.1093e-08 4.11434e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 57.344 sec. to 58.344 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.879392 ( -0.158694 0.153319 )
Epeak [keV] : 264.006 ( -78.7528 298.355 )
Norm@50keV : 0.232504 ( -0.0319049 0.0382509 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 54.37 using 59 PHA bins.
# Reduced chi-squared = 0.9709 for 56 degrees of freedom
# Null hypothesis probability = 5.367888e-01
Photon flux (15-150 keV) in 1 sec: 20.8083 ( -0.4895 0.4909 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.85866e-06 ( 0 0 ) ergs/cm2
Band function
Time interval is from 57.344 sec. to 58.344 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.603655 ( -0.368132 0.603655 )
beta : -1.24205 ( 1.24205 0.0866791 )
Epeak [keV] : 125.345 ( -97.3994 251.195 )
Norm@50keV : 0.332665 ( -0.119705 0.724501 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 52.61 using 59 PHA bins.
# Reduced chi-squared = 0.9566 for 55 degrees of freedom
# Null hypothesis probability = 5.663073e-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] : 21.0537 ( )
R^2/D10^2 : 0.834092 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 413.08 using 59 PHA bins.
# Reduced chi-squared = 7.2471 for 57 degrees of freedom
# Null hypothesis probability = 1.843331e-55
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.977e-08 3.000e-09
25- 50 3.592e-07 1.080e-08
50-150 1.187e-06 4.000e-08
15-150 1.616e-06 4.000e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.363 ( )
Norm : 89.1488 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 425.46 using 59 PHA bins.
# Reduced chi-squared = 7.4643 for 57 degrees of freedom
# Null hypothesis probability = 8.479422e-58
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.220e-07 5.050e-09
25- 50 4.270e-07 9.200e-09
50-150 9.365e-07 2.010e-08
15-150 1.586e-06 3.600e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 9.15011 (-0.934336 1.01437)
R1^2/D10^2 : 6.77528 (-1.733 2.57442)
kT2 [keV] : 35.2415 (-3.28882 4.58165)
R2^2/D10^2 : 0.132742 (-0.0432437 0.0516005)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 61.49 using 59 PHA bins.
# Reduced chi-squared = 1.118 for 55 degrees of freedom
# Null hypothesis probability = 2.548379e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.346e-07 1.055e-08
25- 50 3.951e-07 1.940e-08
50-150 1.330e-06 7.800e-08
15-150 1.860e-06 7.900e-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: 1.50324 ( -0.10744 0.108425 )
Norm@50keV : 1.57477E-02 ( -0.00100001 0.000996608 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 74.07 using 59 PHA bins.
# Reduced chi-squared = 1.299 for 57 degrees of freedom
# Null hypothesis probability = 6.387890e-02
Photon flux (15-150 keV) in 25.32 sec: 1.96765 ( -0.123228 0.123369 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.78058e-06 ( -2.63214e-07 2.65194e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.593239 ( -0.573731 0.503126 )
Epeak [keV] : 76.2813 ( -13.0852 34.8872 )
Norm@50keV : 4.53699E-02 ( -0.0197905 0.0421358 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 63.64 using 59 PHA bins.
# Reduced chi-squared = 1.136 for 56 degrees of freedom
# Null hypothesis probability = 2.254377e-01
Photon flux (15-150 keV) in 25.32 sec: 1.87816 ( -0.13233 0.13213 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.51006e-06 ( -2.9946e-07 3.02802e-07 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.605085 ( -0.488069 0.485076 )
beta : -9.35838 ( 9.36932 19.3693 )
Epeak [keV] : 76.8055 ( -10.3681 33.6843 )
Norm@50keV : 4.46846E-02 ( -0.0186929 0.0101595 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 63.64 using 59 PHA bins.
# Reduced chi-squared = 1.157 for 55 degrees of freedom
# Null hypothesis probability = 1.983914e-01
Photon flux (15-150 keV) in 25.32 sec: 1.87899 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 3.54477e-06 ( 0 0 ) ergs/cm2
S(25-50 keV) vs. S(50-100 keV) plot
S(25-50 keV) = 6.66e-06
S(50-100 keV) = 9.17e-06
T90 vs. Hardness ratio plot
T90 = 80.823999941349 sec.
Hardness ratio (energy fluence ratio) = 1.37688
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.35645
Count Ratio (50-100 keV) / (15-25 keV) = 1.02058
Mask shadow pattern
IMX = -3.420041356545789E-01, IMY = 8.046851815051855E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.024000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.024000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.024000
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:
-179.787400 -12.308000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
342.1958 2.5998 2.2 38.8 14.0 1.5511 5.3 ------ UNKNOWN
69.0727 -52.1747 2.8 52.7 175.9 2.7444 4.1 ------ UNKNOWN
358.6283 -58.8375 2.7 26.2 -136.9 0.9756 4.3 ------ UNKNOWN
87.3973 -68.6526 3.2 59.1 -162.9 5.0676 3.6 ------ UNKNOWN
312.4914 -62.4418 3.0 41.9 -107.4 4.4073 3.8 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-12.308000 13.012600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
72.8992 -48.3885 2.4 55.8 171.9 1.9412 4.7 ------ UNKNOWN
313.4901 0.3490 3.1 54.4 -19.9 0.9574 3.8 ------ UNKNOWN
314.3108 -4.2725 2.4 50.7 -23.7 1.0180 4.8 ------ UNKNOWN
317.9483 -65.3892 0.6 41.2 -113.0 6.0381 19.3 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
73.812600 194.012590
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
186.8155 -62.7898 6.4 46.9 -129.1 1.3786 1.8 4.5 GX 301-2
256.0218 -37.7280 11.2 44.7 -60.4 0.7911 1.0 7.2 4U 1700-377
264.6546 -44.5252 4.8 35.4 -57.8 -0.6526 -2.4 5.9 4U 1735-44
270.1458 -25.0627 8.2 50.3 -37.9 1.0285 1.4 7.6 GX 5-1
270.3760 -25.8793 0.0 49.5 -38.1 0.1896 0.3 9.1 GRS 1758-258
275.9096 -30.3871 5.1 43.4 -34.5 -0.6727 -2.3 1.4 H1820-303
285.1491 -24.9823 9.8 45.5 -20.8 0.3499 1.2 7.2 HT1900.1-2455
263.0939 -33.9498 23.0 45.1 -50.7 0.3342 0.5 8.7 GX 354-0
303.9516 -19.3267 3.6 47.0 4.6 1.0350 3.2 ------ UNKNOWN
317.9326 -65.3867 0.4 0.0 -81.7 4.5841 27.3 ------ UNKNOWN
275.8700 -38.7881 2.9 35.9 -40.4 0.9317 4.0 ------ UNKNOWN
248.5502 -68.5458 2.2 25.9 -105.6 1.0455 5.2 ------ UNKNOWN
274.7889 -35.8937 3.2 38.8 -39.4 0.9033 3.6 ------ UNKNOWN
Plot creation:
Sat May 30 23:37:19 EDT 2015