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Image
Pre-slew 15.0-350.0 keV image (Event data)
# RAcent DECcent POSerr Theta Phi Peak Cts SNR Name
0.7282 -37.9244 0.0189 10.3333 123.4695 1.0024224 10.201 TRIG_00423184
Foreground time interval of the image:
-26.352 47.648 (delta_t = 74.000 [sec])
Background time interval of the image:
-502.352 -382.288 (delta_t = 120.064 [sec])
-239.352 -26.352 (delta_t = 213.000 [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 26.880000
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 26.880000
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 26.880000
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 -26.352 sec. to 47.648 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.47839 ( -0.262726 0.267109 )
Norm@50keV : 7.56398E-04 ( -0.000120059 0.000118062 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 58.16 using 59 PHA bins.
# Reduced chi-squared = 1.020 for 57 degrees of freedom
# Null hypothesis probability = 4.322053e-01
Photon flux (15-150 keV) in 74 sec: 9.38899E-02 ( -0.0138282 0.0138324 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.32921e-07 ( -9.36477e-08 9.61512e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -26.352 sec. to 47.648 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.30323 ( )
Epeak [keV] : 181.979 ( )
Norm@50keV : 9.42757E-04 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 58.07 using 59 PHA bins.
# Reduced chi-squared = 1.037 for 56 degrees of freedom
# Null hypothesis probability = 3.988148e-01
Photon flux (15-150 keV) in 74 sec: 9.31712E-02 ( -0.0142211 0.0142808 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.22275e-07 ( -1.1286e-07 1.04733e-07 ) ergs/cm2
Band function
Time interval is from -26.352 sec. to 47.648 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 4.79267 ( -4.79267 -4.79267 )
beta : -1.68502 ( -0.396834 0.336154 )
Epeak [keV] : 27.6481 ( -8.18181 5.999 )
Norm@50keV : 32.0178 ( -4.66825 369080 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 56.42 using 59 PHA bins.
# Reduced chi-squared = 1.026 for 55 degrees of freedom
# Null hypothesis probability = 4.216003e-01
Photon flux (15-150 keV) in 74 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] : 12.9681 (-2.36986 3.1187)
R^2/D10^2 : 1.75103E-02 (-0.00925882 0.0183314)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 68.23 using 59 PHA bins.
# Reduced chi-squared = 1.197 for 57 degrees of freedom
# Null hypothesis probability = 1.465959e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.622e-08 1.410e-08
25- 50 1.588e-07 3.533e-08
50-150 1.685e-07 5.739e-08
15-150 3.735e-07 8.695e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.344 (-95.6781 -199.362)
Norm : 0.383149 (-0.0562354 0.056277)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 58.18 using 59 PHA bins.
# Reduced chi-squared = 1.021 for 57 degrees of freedom
# Null hypothesis probability = 4.317098e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.060e-08 4.077e-08
25- 50 1.358e-07 7.707e-08
50-150 2.978e-07 1.693e-07
15-150 5.043e-07 2.863e-07
Double BB
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 8.07141 (-3.18158 3.86804)
R1^2/D10^2 : 7.03469E-02 ( )
kT2 [keV] : 38.1035 (-17.2771 -38.2831)
R2^2/D10^2 : 3.48639E-04 (-0.000333267 0.00354242)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 57.58 using 59 PHA bins.
#Fit statistic : Chi-Squared = 56.88 using 59 PHA bins.
# Reduced chi-squared = 1.047 for 55 degrees of freedom
# Reduced chi-squared = 1.034 for 55 degrees of freedom
# Null hypothesis probability = 3.800359e-01
# Null hypothesis probability = 4.049409e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.746e-08 4.052e-08
25- 50 1.332e-07 7.381e-08
50-150 2.874e-07 1.730e-07
15-150 4.881e-07 2.683e-07
Peak spectrum fit
Power-law model
Time interval is from 2.648 sec. to 3.648 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.694609 ( -0.911412 0.751056 )
Norm@50keV : 2.52370E-03 ( -0.00114544 0.00103294 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 46.80 using 59 PHA bins.
# Reduced chi-squared = 0.8210 for 57 degrees of freedom
# Null hypothesis probability = 8.304583e-01
Photon flux (15-150 keV) in 1 sec: 0.291840 ( -0.114464 0.116349 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.08804e-08 ( -1.24764e-08 1.27076e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 2.648 sec. to 3.648 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.691681 ( -0.922884 0.75277 )
Epeak [keV] : 9999.36 ( -9999.36 -9999.36 )
Norm@50keV : 2.54593E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 46.80 using 59 PHA bins.
# Reduced chi-squared = 0.8357 for 56 degrees of freedom
# Null hypothesis probability = 8.046741e-01
Photon flux (15-150 keV) in 1 sec: 0.291923 ( -0.126519 0.114625 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.08585e-08 ( -1.23391e-08 1.26447e-08 ) ergs/cm2
Band function
Time interval is from 2.648 sec. to 3.648 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -9.99999 ( 9.99999 9.99999 )
beta : -0.694611 ( -0.751419 0.910562 )
Epeak [keV] : 17.3262 ( -17.3262 -17.3262 )
Norm@50keV : 0.343007 ( -0.155682 0.140392 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 46.80 using 59 PHA bins.
# Reduced chi-squared = 0.8509 for 55 degrees of freedom
# Null hypothesis probability = 7.764824e-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] : 29.2711 (-11.8052 43.4481)
R^2/D10^2 : 4.76650E-03 (-0.00476651 0.0170691)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 47.27 using 59 PHA bins.
# Reduced chi-squared = 0.8294 for 57 degrees of freedom
# Null hypothesis probability = 8.173198e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.486e-10 4.230e-10
25- 50 3.960e-09 2.433e-09
50-150 2.419e-08 1.543e-08
15-150 2.880e-08 1.885e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.360 (-115.726 -199.362)
Norm : 1.15108 (-0.482037 0.482043)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 50.45 using 59 PHA bins.
# Reduced chi-squared = 0.8850 for 57 degrees of freedom
# Null hypothesis probability = 7.176576e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.866e-09 1.906e-09
25- 50 5.514e-09 3.637e-09
50-150 1.209e-08 7.925e-09
15-150 2.047e-08 1.347e-08
Double BB
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 1.26708 (-1.66015 3.002)
R1^2/D10^2 : 1.03051E+04 ( )
kT2 [keV] : 31.0285 (-12.6966 55.4367)
R2^2/D10^2 : 3.98170E-03 (-0.00360698 0.00915891)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 45.64 using 59 PHA bins.
#Fit statistic : Chi-Squared = 45.52 using 59 PHA bins.
# Reduced chi-squared = 0.8298 for 55 degrees of freedom
# Reduced chi-squared = 0.8277 for 55 degrees of freedom
# Null hypothesis probability = 8.116761e-01
# Null hypothesis probability = 8.151492e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.576e-09 5.400e-10
25- 50 3.627e-09 2.221e-09
50-150 2.472e-08 1.589e-08
15-150 2.992e-08 1.826e-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: 1.47839 ( -0.262726 0.267109 )
Norm@50keV : 7.56398E-04 ( -0.000120059 0.000118062 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 58.16 using 59 PHA bins.
# Reduced chi-squared = 1.020 for 57 degrees of freedom
# Null hypothesis probability = 4.322053e-01
Photon flux (15-150 keV) in 74 sec: 9.38899E-02 ( -0.0138282 0.0138324 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.32921e-07 ( -9.36477e-08 9.61512e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.30323 ( )
Epeak [keV] : 181.979 ( )
Norm@50keV : 9.42757E-04 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 58.07 using 59 PHA bins.
# Reduced chi-squared = 1.037 for 56 degrees of freedom
# Null hypothesis probability = 3.988148e-01
Photon flux (15-150 keV) in 74 sec: 9.31712E-02 ( -0.0142211 0.0142808 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.22275e-07 ( -1.1286e-07 1.04733e-07 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 4.79267 ( -4.79267 -4.79267 )
beta : -1.68502 ( -0.396834 0.336154 )
Epeak [keV] : 27.6481 ( -8.18181 5.999 )
Norm@50keV : 32.0178 ( -4.66825 369080 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 56.42 using 59 PHA bins.
# Reduced chi-squared = 1.026 for 55 degrees of freedom
# Null hypothesis probability = 4.216003e-01
Photon flux (15-150 keV) in 74 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) = 1.30e-07
S(50-100 keV) = 1.87e-07
T90 vs. Hardness ratio plot
T90 = 67 sec.
Hardness ratio (energy fluence ratio) = 1.43846
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.33871
Count Ratio (50-100 keV) / (15-25 keV) = 0.879929
Mask shadow pattern
IMX = -1.005538939088317E-01, IMY = -1.520964210415964E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 26.880000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 26.880000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 26.880000
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:
-502.352000 -382.288300
-239.352000 -26.352000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
334.6260 -64.0169 2.7 35.1 67.5 2.0803 4.2 ------ UNKNOWN
353.5620 -48.7015 2.9 18.3 85.3 1.0272 4.0 ------ UNKNOWN
340.9674 6.9398 3.0 54.1 177.0 3.3571 3.8 ------ UNKNOWN
92.1694 -47.2967 3.7 56.1 -14.5 2.7084 3.2 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-26.352000 47.648000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
332.9348 -73.6793 2.1 41.0 54.9 1.6699 5.6 ------ UNKNOWN
0.7282 -37.9244 1.1 10.3 123.5 1.0023 10.2 ------ UNKNOWN
8.6081 -43.3610 2.4 6.9 72.0 0.4364 4.8 ------ UNKNOWN
65.8278 -28.6744 2.3 43.9 -47.3 1.1334 5.0 ------ UNKNOWN
68.4253 -24.4890 3.0 47.9 -50.9 1.5914 3.9 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
365.148610 962.774500
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6387 22.0189 0.3 28.7 -99.5 22.9499 38.0 0.4 Crab
120.4632 -25.1829 3.0 47.1 156.5 4.7194 3.9 ------ UNKNOWN
101.8817 -31.0663 3.9 54.1 177.3 5.0517 3.0 ------ UNKNOWN
80.2306 33.8549 3.2 32.6 -76.6 2.6892 3.6 ------ UNKNOWN
72.8997 -13.6641 2.6 54.0 -143.2 10.7516 4.4 ------ UNKNOWN
70.5453 15.1678 3.2 42.1 -107.2 6.5753 3.6 ------ UNKNOWN
Plot creation:
Sun May 31 01:26:05 EDT 2015