Special notes of this burst
Image
Pre-slew 15.0-350.0 keV image (Event data)
# RAcent DECcent POSerr Theta Phi Peak Cts SNR Name
86.7883 51.2581 0.0056 9.7185 -123.4694 1.9600793 34.366 TRIG_00323542
Foreground time interval of the image:
-10.544 15.733 (delta_t = 26.277 [sec])
Background time interval of the image:
-239.368 -10.544 (delta_t = 228.824 [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)
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 -10.544 sec. to 68.008 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.66327 ( -0.0970922 0.0983887 )
Norm@50keV : 2.16604E-03 ( -0.000121392 0.000120561 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 53.29 using 59 PHA bins.
# Reduced chi-squared = 0.9349 for 57 degrees of freedom
# Null hypothesis probability = 6.150331e-01
Photon flux (15-150 keV) in 78.55 sec: 0.284086 ( -0.0147845 0.0147929 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.58034e-06 ( -9.4586e-08 9.55647e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -10.544 sec. to 68.008 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.933345 ( -0.499846 0.446562 )
Epeak [keV] : 67.9643 ( -11.4482 35.0092 )
Norm@50keV : 5.23531E-03 ( -0.00215133 0.00426319 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 45.02 using 59 PHA bins.
# Reduced chi-squared = 0.8040 for 56 degrees of freedom
# Null hypothesis probability = 8.531460e-01
Photon flux (15-150 keV) in 78.55 sec: 0.271332 ( -0.016563 0.016542 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.46182e-06 ( -1.14125e-07 1.17032e-07 ) ergs/cm2
Band function
Time interval is from -10.544 sec. to 68.008 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.944903 ( -0.486952 0.673806 )
beta : -2.31040 ( 2.35848 0.513624 )
Epeak [keV] : 67.4291 ( -15.3548 31.1333 )
Norm@50keV : 5.19483E-03 ( -0.00260166 0.00824573 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 44.58 using 59 PHA bins.
# Reduced chi-squared = 0.8106 for 55 degrees of freedom
# Null hypothesis probability = 8.411666e-01
Photon flux (15-150 keV) in 78.55 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] : 13.0227 (-0.777803 0.836464)
R^2/D10^2 : 5.06904E-02 (-0.010222 0.012701)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 87.51 using 59 PHA bins.
# Reduced chi-squared = 1.535 for 57 degrees of freedom
# Null hypothesis probability = 5.790302e-03
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.432e-07 1.402e-08
25- 50 4.942e-07 3.016e-08
50-150 5.304e-07 6.068e-08
15-150 1.168e-06 7.423e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 137.986 (-31.5257 43.9615)
Norm : 1.17763 (-0.0713708 0.0858962)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 46.65 using 59 PHA bins.
# Reduced chi-squared = 0.8184 for 57 degrees of freedom
# Null hypothesis probability = 8.344724e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.391e-07 1.964e-08
25- 50 4.377e-07 4.010e-08
50-150 8.337e-07 2.755e-07
15-150 1.510e-06 3.071e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 4.13934 (-1.09224 1.87947)
R1^2/D10^2 : 1.75314 (-1.34317 6.30596)
kT2 [keV] : 16.0446 (-1.60153 2.73788)
R2^2/D10^2 : 2.13702E-02 (-0.0103532 0.0109636)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 46.92 using 59 PHA bins.
# Reduced chi-squared = 0.8531 for 55 degrees of freedom
# Null hypothesis probability = 7.725855e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.368e-07 8.811e-08
25- 50 4.353e-07 6.437e-08
50-150 6.793e-07 1.035e-07
15-150 1.351e-06 1.881e-07
Peak spectrum fit
Power-law model
Time interval is from -2.796 sec. to -1.796 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.15635 ( -0.24889 0.245487 )
Norm@50keV : 6.72627E-03 ( -0.00101527 0.00101445 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 65.45 using 59 PHA bins.
# Reduced chi-squared = 1.148 for 57 degrees of freedom
# Null hypothesis probability = 2.068168e-01
Photon flux (15-150 keV) in 1 sec: 0.785012 ( -0.118812 0.11894 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.91074e-08 ( -1.18147e-08 1.20403e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -2.796 sec. to -1.796 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -0.785206 ( -2.26676 1.46573 )
Epeak [keV] : 71.5133 ( -14.847 67.3837 )
Norm@50keV : 6.20449E-02 ( -0.0621911 0.628588 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 59.82 using 59 PHA bins.
# Reduced chi-squared = 1.068 for 56 degrees of freedom
# Null hypothesis probability = 3.386568e-01
Photon flux (15-150 keV) in 1 sec: 0.722307 ( -0.130837 0.129349 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.87242e-08 ( -1.25668e-08 1.41308e-08 ) ergs/cm2
Band function
Time interval is from -2.796 sec. to -1.796 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 1.15960 ( -1.65547 2.40283 )
beta : -2.49001 ( 2.4509 1.0361 )
Epeak [keV] : 66.4924 ( -17.9507 48.1806 )
Norm@50keV : 9.72498E-02 ( -0.0899507 1.25824 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 59.06 using 59 PHA bins.
# Reduced chi-squared = 1.074 for 55 degrees of freedom
# Null hypothesis probability = 3.295172e-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] : 16.9548 (-2.49255 3.1221)
R^2/D10^2 : 6.55311E-02 (-0.0282734 0.0458275)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 60.04 using 59 PHA bins.
# Reduced chi-squared = 1.053 for 57 degrees of freedom
# Null hypothesis probability = 3.660959e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.839e-09 1.092e-09
25- 50 1.695e-08 4.090e-09
50-150 3.476e-08 9.840e-09
15-150 5.555e-08 1.210e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 ( )
Norm : 3.17038 (-0.486503 0.486494)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 70.11 using 59 PHA bins.
# Reduced chi-squared = 1.230 for 57 degrees of freedom
# Null hypothesis probability = 1.138885e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.894e-09 4.493e-09
25- 50 1.519e-08 8.560e-09
50-150 3.330e-08 1.864e-08
15-150 5.638e-08 3.156e-08
Double BB
R1^2/D10^2 : 5.48504E-05 ( )
kT2 [keV] : 15.1387 (-15.1312 3.74051)
R2^2/D10^2 : 8.59322E-02 (-0.0396943 -0.0860977)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 59.53 using 59 PHA bins.
#Fit statistic : Chi-Squared = 58.68 using 59 PHA bins.
#Fit statistic : Chi-Squared = 58.46 using 59 PHA bins.
# Reduced chi-squared = 1.082 for 55 degrees of freedom
# Reduced chi-squared = 1.067 for 55 degrees of freedom
# Reduced chi-squared = 1.063 for 55 degrees of freedom
# Null hypothesis probability = 3.144143e-01
# Null hypothesis probability = 3.420723e-01
# Null hypothesis probability = 3.494443e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.692e-09 2.461e-09
25- 50 1.637e-08 8.154e-09
50-150 3.624e-08 2.054e-08
15-150 5.730e-08 3.239e-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: 1.43622 ( -0.0815316 0.0817485 )
Norm@50keV : 4.29894E-03 ( -0.000209199 0.000208742 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 92.27 using 59 PHA bins.
# Reduced chi-squared = 1.619 for 57 degrees of freedom
# Null hypothesis probability = 2.151582e-03
Photon flux (15-150 keV) in 26.28 sec: 0.528002 ( -0.0252615 0.0252713 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.08388e-06 ( -5.87926e-08 5.9217e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 9.68394E-02 ( -0.498594 0.446681 )
Epeak [keV] : 66.9496 ( -7.11725 11.614 )
Norm@50keV : 2.14439E-02 ( -0.00877605 0.017251 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 60.11 using 59 PHA bins.
# Reduced chi-squared = 1.073 for 56 degrees of freedom
# Null hypothesis probability = 3.294349e-01
Photon flux (15-150 keV) in 26.28 sec: 0.493208 ( -0.027412 0.027442 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.49412e-07 ( -6.81151e-08 7.02491e-08 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 0.273914 ( -0.609355 0.970261 )
beta : -2.25869 ( -0.833651 0.383118 )
Epeak [keV] : 59.0690 ( -10.9349 10.0287 )
Norm@50keV : 3.55819E-02 ( -0.0198646 0.105211 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 55.92 using 59 PHA bins.
# Reduced chi-squared = 1.017 for 55 degrees of freedom
# Null hypothesis probability = 4.400084e-01
Photon flux (15-150 keV) in 26.28 sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 9.75256e-07 ( -9.75072e-07 -6.84357e-08 ) ergs/cm2
S(25-50 keV) vs. S(50-100 keV) plot
S(25-50 keV) = 4.21e-07
S(50-100 keV) = 5.32e-07
T90 vs. Hardness ratio plot
T90 = 66.3400000035763 sec.
Hardness ratio (energy fluence ratio) = 1.26366
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.30492
Count Ratio (50-100 keV) / (15-25 keV) = 0.757414
Mask shadow pattern
IMX = -9.445175407291447E-02, IMY = 1.428667928175362E-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:
-239.368000 -10.544000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6309 22.0185 0.2 24.2 -10.4 10.0944 53.4 0.3 Crab
22.7287 43.9526 2.4 36.8 116.0 2.1583 4.8 ------ UNKNOWN
73.1758 -10.1712 2.5 55.5 11.3 4.6149 4.6 ------ UNKNOWN
123.7990 47.6596 2.1 33.0 -103.2 1.8692 5.6 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-10.544000 15.732600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6762 21.8678 5.5 24.4 -10.4 -0.1238 -2.1 9.1 Crab
3.7223 57.1245 2.3 44.2 141.1 0.8618 5.0 ------ UNKNOWN
86.7883 51.2581 0.3 9.7 -123.5 1.9601 34.4 ------ UNKNOWN
139.7625 66.5909 2.4 39.4 -136.9 0.4554 4.8 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
47.132600 962.687700
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6347 22.0229 0.2 29.4 -0.4 39.3628 70.8 0.5 Crab
34.9233 36.0651 2.6 39.5 81.7 9.7241 4.4 ------ UNKNOWN
45.5069 39.4657 2.3 30.8 77.4 4.9567 5.0 ------ UNKNOWN
98.4724 24.6325 2.8 28.1 -29.4 2.2071 4.2 ------ UNKNOWN
103.9515 24.6574 2.9 29.7 -39.2 2.3968 4.0 ------ UNKNOWN
Plot creation:
Sun May 31 06:37:48 EDT 2015