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Image
Pre-slew 15.0-350.0 keV image (Event data)
# RAcent DECcent POSerr Theta Phi Peak Cts SNR Name
68.9799 -12.6855 0.0195 26.8002 0.8324 0.8242648 9.891 TRIG_00348650
Foreground time interval of the image:
-17.688 28.029 (delta_t = 45.717 [sec])
Background time interval of the image:
-239.272 -17.688 (delta_t = 221.584 [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 2.048000
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 2.048000
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 2.048000
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 -17.688 sec. to 329.352 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.64655 ( -0.26572 0.277596 )
Norm@50keV : 3.54460E-04 ( -5.97004e-05 5.79093e-05 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 62.07 using 59 PHA bins.
# Reduced chi-squared = 1.089 for 57 degrees of freedom
# Null hypothesis probability = 3.002980e-01
Photon flux (15-150 keV) in 347 sec: 4.62313E-02 ( -0.0066545 0.00665517 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.14432e-06 ( -2.03335e-07 2.09389e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -17.688 sec. to 329.352 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.65240 ( -0.272074 0.274324 )
Epeak [keV] : 9999.36 ( -9999.35 -9999.36 )
Norm@50keV : 3.53817E-04 ( -0.000354764 0.000804462 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 62.07 using 59 PHA bins.
# Reduced chi-squared = 1.108 for 56 degrees of freedom
# Null hypothesis probability = 2.686666e-01
Photon flux (15-150 keV) in 347 sec: 4.62254E-02 ( -0.0066614 0.0066443 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.13976e-06 ( -1.91835e-07 2.11809e-07 ) ergs/cm2
Band function
Time interval is from -17.688 sec. to 329.352 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -2.45859 ( 7.24006 2.45859 )
beta : -1.64655 ( -0.277596 0.26572 )
Epeak [keV] : 91.6642 ( -91.6642 -91.6642 )
Norm@50keV : 4.81762E-02 ( -0.00811415 0.00787071 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 62.07 using 59 PHA bins.
# Reduced chi-squared = 1.129 for 55 degrees of freedom
# Null hypothesis probability = 2.387862e-01
Photon flux (15-150 keV) in 347 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] : 12.3848 (-2.44433 3.16011)
R^2/D10^2 : 9.76596E-03 (-0.00537534 0.0117656)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 78.23 using 59 PHA bins.
# Reduced chi-squared = 1.372 for 57 degrees of freedom
# Null hypothesis probability = 3.254299e-02
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.102e-07 3.074e-08
25- 50 3.596e-07 8.628e-08
50-150 3.385e-07 1.188e-07
15-150 8.082e-07 1.893e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 161.938 (-83.1745 -160.329)
Norm : 0.189220 (-0.0284825 0.0391487)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 62.64 using 59 PHA bins.
# Reduced chi-squared = 1.099 for 57 degrees of freedom
# Null hypothesis probability = 2.831593e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.675e-07 9.301e-08
25- 50 3.138e-07 1.704e-07
50-150 6.387e-07 3.739e-07
15-150 1.120e-06 6.354e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.39020 (-1.96561 2.60503)
R1^2/D10^2 : 0.140730 (-0.106503 0.81236)
kT2 [keV] : 23.4926 (-7.36766 19.0311)
R2^2/D10^2 : 8.43948E-04 (-0.000719236 0.00243862)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 61.88 using 59 PHA bins.
# Reduced chi-squared = 1.125 for 55 degrees of freedom
# Null hypothesis probability = 2.440073e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.879e-07 1.027e-07
25- 50 2.835e-07 1.460e-07
50-150 6.626e-07 3.878e-07
15-150 1.134e-06 5.694e-07
Peak spectrum fit
Power-law model
Time interval is from 0.444 sec. to 1.444 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.979010 ( -0.400203 0.365757 )
Norm@50keV : 5.71258E-03 ( -0.00121827 0.00120587 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 57.82 using 59 PHA bins.
# Reduced chi-squared = 1.014 for 57 degrees of freedom
# Null hypothesis probability = 4.449098e-01
Photon flux (15-150 keV) in 1 sec: 0.656986 ( -0.141267 0.14221 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.22453e-08 ( -1.40278e-08 1.41946e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.444 sec. to 1.444 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.33475 ( )
Epeak [keV] : 105.228 ( )
Norm@50keV : 3.30794E-04 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 56.40 using 59 PHA bins.
# Reduced chi-squared = 1.007 for 56 degrees of freedom
# Null hypothesis probability = 4.597684e-01
Photon flux (15-150 keV) in 1 sec: 0.657137 ( -0.143084 0.14107 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.22239e-08 ( -1.50217e-08 1.41761e-08 ) ergs/cm2
Band function
Time interval is from 0.444 sec. to 1.444 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 5.00000 ( -5 -5 )
beta : -1.30676 ( -0.729105 0.54984 )
Epeak [keV] : 38.7631 ( -38.7631 37.4099 )
Norm@50keV : 33.9998 ( -6.97773 1.32226e+06 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 56.57 using 59 PHA bins.
# Reduced chi-squared = 1.029 for 55 degrees of freedom
# Null hypothesis probability = 4.159822e-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] : 20.5012 (-6.33676 11.7429)
R^2/D10^2 : 2.84326E-02 (-0.0208463 0.0658084)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 63.81 using 59 PHA bins.
# Reduced chi-squared = 1.119 for 57 degrees of freedom
# Null hypothesis probability = 2.496438e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.281e-09 1.123e-09
25- 50 1.155e-08 5.205e-09
50-150 3.609e-08 1.663e-08
15-150 4.991e-08 2.402e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 ( )
Norm : 2.67587 (-0.58564 0.585605)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 64.16 using 59 PHA bins.
# Reduced chi-squared = 1.126 for 57 degrees of freedom
# Null hypothesis probability = 2.398836e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.663e-09 4.010e-09
25- 50 1.282e-08 7.665e-09
50-150 2.811e-08 1.680e-08
15-150 4.759e-08 2.809e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 10.7354 (-3.50731 4.86543)
R1^2/D10^2 : 0.171384 (-0.120399 0.257603)
kT2 [keV] : 89.8792 (-58.6445 -89.1087)
R2^2/D10^2 : 4.83025E-04 (-0.000379918 0.00630749)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 55.14 using 59 PHA bins.
# Reduced chi-squared = 1.003 for 55 degrees of freedom
# Null hypothesis probability = 4.694055e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.366e-09 2.684e-09
25- 50 1.333e-08 7.370e-09
50-150 4.597e-08 2.987e-08
15-150 6.366e-08 3.380e-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: 1.62859 ( -0.251813 0.259196 )
Norm@50keV : 1.00784E-03 ( -0.000175768 0.000173277 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 73.12 using 59 PHA bins.
# Reduced chi-squared = 1.283 for 57 degrees of freedom
# Null hypothesis probability = 7.381541e-02
Photon flux (15-150 keV) in 45.72 sec: 0.130684 ( -0.0204563 0.0204607 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.29541e-07 ( -7.87701e-08 8.12069e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -0.971359 ( -2.41851 1.68252 )
Epeak [keV] : 45.9933 ( -7.21844 16.0135 )
Norm@50keV : 3.32139E-02 ( -0.0350329 0.85091 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 64.74 using 59 PHA bins.
# Reduced chi-squared = 1.156 for 56 degrees of freedom
# Null hypothesis probability = 1.979438e-01
Photon flux (15-150 keV) in 45.72 sec: 0.120272 ( -0.02059 0.020942 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.34009e-07 ( -6.77319e-08 8.59595e-08 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 1.16999 ( -1.70546 -1.19861 )
beta : -3.04323 ( 3.04214 1.14847 )
Epeak [keV] : 44.2743 ( -12.2717 14.1343 )
Norm@50keV : 4.59483E-02 ( -0.0525757 9.40346 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 63.96 using 59 PHA bins.
# Reduced chi-squared = 1.163 for 55 degrees of freedom
# Null hypothesis probability = 1.908740e-01
Photon flux (15-150 keV) in 45.72 sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 3.62235e-07 ( 0 0 ) ergs/cm2
S(25-50 keV) vs. S(50-100 keV) plot
S(25-50 keV) = 3.03e-07
S(50-100 keV) = 3.87e-07
T90 vs. Hardness ratio plot
T90 = 315.471999973059 sec.
Hardness ratio (energy fluence ratio) = 1.27723
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.0375
Count Ratio (50-100 keV) / (15-25 keV) = 0.778476
Mask shadow pattern
IMX = 5.050880671116625E-01, IMY = -7.338579258640548E-03
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 2.048000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 2.048000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 2.048000
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:
-239.272000 -17.688000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
92.7612 -79.7030 3.1 46.3 138.4 2.4784 3.7 ------ UNKNOWN
93.4728 -65.1454 2.6 37.3 121.2 1.9716 4.5 ------ UNKNOWN
92.1650 -19.7977 2.3 36.9 41.7 1.7043 5.0 ------ UNKNOWN
3.6258 -71.5276 2.6 44.0 167.9 1.4839 4.5 ------ UNKNOWN
47.1141 -58.3844 2.7 22.9 156.8 0.9182 4.3 ------ UNKNOWN
54.0018 -17.5788 2.3 18.4 -33.3 0.8519 5.1 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-17.688000 28.028590
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
356.0005 -64.9192 2.2 44.6 178.2 0.6541 5.3 ------ UNKNOWN
68.9803 -12.6851 1.1 26.8 0.8 0.8573 10.3 ------ UNKNOWN
337.3791 -50.5791 2.3 55.2 -163.9 1.2418 5.1 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
77.228600 962.772200
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6364 22.0193 0.2 37.5 5.2 34.6351 46.9 0.3 Crab
100.0179 -49.7330 2.6 45.0 134.4 9.9281 4.4 ------ UNKNOWN
87.1015 -44.4410 2.7 35.4 140.0 4.1008 4.2 ------ UNKNOWN
89.3415 -28.0038 3.1 24.4 114.6 2.5860 3.7 ------ UNKNOWN
90.3434 19.6755 2.2 38.6 16.0 4.0403 5.2 ------ UNKNOWN
87.6758 38.1636 3.4 53.8 0.8 6.1229 3.4 ------ UNKNOWN
25.8792 -60.4464 4.8 57.2 -173.8 6.8450 2.4 ------ UNKNOWN
14.0965 -53.6568 3.5 59.4 -163.2 16.2837 3.3 ------ UNKNOWN
40.7354 25.5157 3.4 47.0 -53.1 8.2049 3.4 ------ UNKNOWN
Plot creation:
Sun May 31 04:32:47 EDT 2015