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Image
Pre-slew 15.0-350.0 keV image (Event data)
# RAcent DECcent POSerr Theta Phi Peak Cts SNR Name
75.0874 14.9566 0.0158 17.1565 121.5554 0.7351997 12.114 TRIG_00181156
Foreground time interval of the image:
-10.596 19.160 (delta_t = 29.756 [sec])
Background time interval of the image:
-299.776 -10.596 (delta_t = 289.180 [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 -10.596 sec. to 19.160 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.52947 ( -0.203657 0.207509 )
Norm@50keV : 1.58174E-03 ( -0.000193943 0.00019165 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 44.27 using 59 PHA bins.
# Reduced chi-squared = 0.7766 for 57 degrees of freedom
# Null hypothesis probability = 8.909251e-01
Photon flux (15-150 keV) in 29.76 sec: 0.199069 ( -0.0230708 0.0230877 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.44486e-07 ( -5.96057e-08 6.05661e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -10.596 sec. to 19.160 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.19403 ( -0.848363 0.508548 )
Epeak [keV] : 116.966 ( -116.966 -116.966 )
Norm@50keV : 2.36017E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 43.66 using 59 PHA bins.
# Reduced chi-squared = 0.7797 for 56 degrees of freedom
# Null hypothesis probability = 8.849915e-01
Photon flux (15-150 keV) in 29.76 sec: 0.196143 ( -0.023959 0.02391 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.32204e-07 ( -6.53559e-08 6.58232e-08 ) ergs/cm2
Band function
Time interval is from -10.596 sec. to 19.160 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.19506 ( -0.427189 0.641548 )
beta : -10.00000 ( 10 20 )
Epeak [keV] : 117.170 ( -48.4958 -117.17 )
Norm@50keV : 2.35694E-03 ( -0.000270001 0.00395759 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 43.66 using 59 PHA bins.
# Reduced chi-squared = 0.7938 for 55 degrees of freedom
# Null hypothesis probability = 8.645748e-01
Photon flux (15-150 keV) in 29.76 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] : 14.6048 (-2.19203 2.61542)
R^2/D10^2 : 2.44436E-02 (-0.0106363 0.0188265)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 61.44 using 59 PHA bins.
# Reduced chi-squared = 1.078 for 57 degrees of freedom
# Null hypothesis probability = 3.201382e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.262e-08 7.501e-09
25- 50 1.264e-07 2.168e-08
50-150 1.813e-07 4.857e-08
15-150 3.403e-07 5.788e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.363 (-84.5855 -199.363)
Norm : 0.812176 (-0.09305 0.0931396)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 43.74 using 59 PHA bins.
# Reduced chi-squared = 0.7673 for 57 degrees of freedom
# Null hypothesis probability = 9.015758e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.019e-08 3.358e-08
25- 50 1.158e-07 6.358e-08
50-150 2.539e-07 1.383e-07
15-150 4.299e-07 2.357e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.83864 (-2.03721 2.54085)
R1^2/D10^2 : 0.376436 (-0.267531 1.7385)
kT2 [keV] : 22.9193 (-5.34609 10.5984)
R2^2/D10^2 : 4.21567E-03 (-0.00312287 0.00468863)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 42.73 using 59 PHA bins.
# Reduced chi-squared = 0.7769 for 55 degrees of freedom
# Null hypothesis probability = 8.859621e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.071e-08 3.253e-08
25- 50 1.106e-07 4.938e-08
50-150 2.580e-07 1.437e-07
15-150 4.292e-07 1.941e-07
Peak spectrum fit
Power-law model
Time interval is from 1.836 sec. to 2.836 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.40603 ( -0.279816 0.281171 )
Norm@50keV : 6.06050E-03 ( -0.00105046 0.00104335 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 42.41 using 59 PHA bins.
# Reduced chi-squared = 0.7440 for 57 degrees of freedom
# Null hypothesis probability = 9.251758e-01
Photon flux (15-150 keV) in 1 sec: 0.739069 ( -0.125905 0.12606 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.84895e-08 ( -1.11465e-08 1.1355e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 1.836 sec. to 2.836 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.606054 ( -1.39214 0.929722 )
Epeak [keV] : 84.4209 ( -30.7367 -84.421 )
Norm@50keV : 1.58190E-02 ( -0.0158189 0.0658649 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 40.84 using 59 PHA bins.
# Reduced chi-squared = 0.7292 for 56 degrees of freedom
# Null hypothesis probability = 9.360799e-01
Photon flux (15-150 keV) in 1 sec: 0.719077 ( -0.125476 0.065161 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.48517e-08 ( -1.21014e-08 1.24396e-08 ) ergs/cm2
Band function
Time interval is from 1.836 sec. to 2.836 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 4.91825 ( -4.91825 -4.91825 )
beta : -1.71323 ( -0.598854 0.389029 )
Epeak [keV] : 31.4471 ( -31.4471 7.89572 )
Norm@50keV : 141.868 ( -23.5756 2.04701e+06 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 39.74 using 59 PHA bins.
# Reduced chi-squared = 0.7226 for 55 degrees of freedom
# Null hypothesis probability = 9.395733e-01
Photon flux (15-150 keV) in 1 sec: 0.722029 ( 6.27797 -0.127473 ) 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] : 15.1080 (-3.02268 3.8668)
R^2/D10^2 : 8.49900E-02 (-0.0463502 0.0998724)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 46.21 using 59 PHA bins.
# Reduced chi-squared = 0.8106 for 57 degrees of freedom
# Null hypothesis probability = 8.459871e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.057e-09 1.370e-09
25- 50 1.623e-08 4.289e-09
50-150 2.528e-08 9.500e-09
15-150 4.557e-08 1.231e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.363 (-87.4912 -199.363)
Norm : 3.05206 (-0.513517 0.513517)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 42.11 using 59 PHA bins.
# Reduced chi-squared = 0.7389 for 57 degrees of freedom
# Null hypothesis probability = 9.297911e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.600e-09 4.370e-09
25- 50 1.462e-08 8.240e-09
50-150 3.206e-08 1.840e-08
15-150 5.428e-08 3.065e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.50217 (-2.99944 4.62432)
R1^2/D10^2 : 0.551900 (-0.417798 2.40885)
kT2 [keV] : 25.0146 (-20.3796 60.3082)
R2^2/D10^2 : 1.12793E-02 (-0.0112495 0.02546)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 39.71 using 59 PHA bins.
# Reduced chi-squared = 0.7220 for 55 degrees of freedom
# Null hypothesis probability = 9.400400e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.558e-09 3.835e-09
25- 50 1.528e-08 8.130e-09
50-150 3.403e-08 1.936e-08
15-150 5.587e-08 2.955e-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: 1.52947 ( -0.203657 0.207509 )
Norm@50keV : 1.58174E-03 ( -0.000193943 0.00019165 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 44.27 using 59 PHA bins.
# Reduced chi-squared = 0.7766 for 57 degrees of freedom
# Null hypothesis probability = 8.909251e-01
Photon flux (15-150 keV) in 29.76 sec: 0.199069 ( -0.0230708 0.0230877 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.44486e-07 ( -5.96057e-08 6.05661e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.19403 ( -0.848363 0.508548 )
Epeak [keV] : 116.966 ( -116.966 -116.966 )
Norm@50keV : 2.36017E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 43.66 using 59 PHA bins.
# Reduced chi-squared = 0.7797 for 56 degrees of freedom
# Null hypothesis probability = 8.849915e-01
Photon flux (15-150 keV) in 29.76 sec: 0.196143 ( -0.023959 0.02391 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.32204e-07 ( -6.53559e-08 6.58232e-08 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.19506 ( -0.427189 0.641548 )
beta : -10.00000 ( 10 20 )
Epeak [keV] : 117.170 ( -48.4958 -117.17 )
Norm@50keV : 2.35694E-03 ( -0.000270001 0.00395759 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 43.66 using 59 PHA bins.
# Reduced chi-squared = 0.7938 for 55 degrees of freedom
# Null hypothesis probability = 8.645748e-01
Photon flux (15-150 keV) in 29.76 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) = 1.12e-07
S(50-100 keV) = 1.55e-07
T90 vs. Hardness ratio plot
T90 = 27.7319999933243 sec.
Hardness ratio (energy fluence ratio) = 1.38393
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.50139
Count Ratio (50-100 keV) / (15-25 keV) = 1.10538
Mask shadow pattern
IMX = -1.615595728491372E-01, IMY = -2.630701998202375E-01
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:
-299.776000 -10.596000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6433 22.0222 0.3 23.4 95.9 11.9561 44.8 0.7 Crab
99.6132 57.8483 2.8 46.9 40.6 3.7603 4.2 ------ UNKNOWN
56.3156 -37.4762 3.2 59.0 -166.2 4.6126 3.6 ------ UNKNOWN
2.2546 39.0918 4.3 50.7 -44.5 3.2389 2.7 ------ UNKNOWN
29.4724 -17.6625 2.7 48.3 -130.0 4.1272 4.2 ------ UNKNOWN
18.8851 6.7559 3.3 40.9 -93.3 4.0025 3.5 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-10.596000 19.160000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.4775 22.1363 6.2 23.3 95.7 -0.1300 -1.9 11.3 Crab
83.7271 52.2945 2.2 36.5 38.1 0.5393 5.3 ------ UNKNOWN
75.0874 14.9566 0.9 17.2 121.6 0.7353 12.1 ------ UNKNOWN
54.1638 66.2189 2.0 44.8 9.5 0.6111 5.7 ------ UNKNOWN
52.3324 27.4198 2.3 8.1 -29.8 0.2589 5.1 ------ UNKNOWN
44.7379 -21.4179 2.8 44.9 -150.0 0.3737 4.1 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
67.324600 302.269900
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6348 22.0211 0.2 10.8 57.0 10.2718 60.9 0.4 Crab
65.4606 42.5598 4.4 28.8 -5.6 0.5004 2.6 ------ UNKNOWN
73.2125 -41.8642 2.8 56.9 -169.2 3.1058 4.2 ------ UNKNOWN
28.1410 60.2034 2.6 56.5 -16.6 3.4306 4.4 ------ UNKNOWN
34.3163 49.6594 2.8 47.9 -25.5 1.6742 4.1 ------ UNKNOWN
23.4614 37.2391 3.1 50.6 -44.6 3.7556 4.2 ------ UNKNOWN
23.2795 37.4221 3.9 50.8 -44.4 3.5611 4.0 ------ UNKNOWN
Plot creation:
Sun May 31 14:12:10 EDT 2015