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Image
Pre-slew 15.0-350.0 keV image (Event data)
# RAcent DECcent POSerr Theta Phi Peak Cts SNR Name
119.6655 32.8565 0.0026 15.0644 -63.2484 3.4454502 74.426 TRIG_00294835
Foreground time interval of the image:
-3.052 7.532 (delta_t = 10.584 [sec])
Background time interval of the image:
-239.248 -3.052 (delta_t = 236.196 [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 0.512000
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 0.512000
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 0.512000
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 -3.052 sec. to 7.532 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.08201 ( -0.0426832 0.0425053 )
Norm@50keV : 2.10697E-02 ( -0.000479065 0.000477953 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 32.74 using 59 PHA bins.
# Reduced chi-squared = 0.5744 for 57 degrees of freedom
# Null hypothesis probability = 9.959144e-01
Photon flux (15-150 keV) in 10.58 sec: 2.44016 ( -0.0586126 0.0581387 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.34421e-06 ( -5.49755e-08 5.50319e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -3.052 sec. to 7.532 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.02224 ( -0.158315 0.075213 )
Epeak [keV] : 990.275 ( -994.013 -994.013 )
Norm@50keV : 2.23154E-02 ( -0.000497796 0.00355428 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 32.53 using 59 PHA bins.
# Reduced chi-squared = 0.5808 for 56 degrees of freedom
# Null hypothesis probability = 9.949287e-01
Photon flux (15-150 keV) in 10.58 sec: 2.43707 ( -0.05664 0.06 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.33904e-06 ( -5.68358e-08 5.92374e-08 ) ergs/cm2
Band function
Time interval is from -3.052 sec. to 7.532 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.725949 ( 0.722667 0.722667 )
beta : -1.10680 ( 1.10849 0.0610276 )
Epeak [keV] : 136.519 ( -145.448 325.782 )
Norm@50keV : 3.36989E-02 ( -0.0117823 0 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 31.81 using 59 PHA bins.
# Reduced chi-squared = 0.5784 for 55 degrees of freedom
# Null hypothesis probability = 9.948376e-01
Photon flux (15-150 keV) in 10.58 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] : 22.4138 ( )
R^2/D10^2 : 7.89054E-02 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 370.07 using 59 PHA bins.
# Reduced chi-squared = 6.4924 for 57 degrees of freedom
# Null hypothesis probability = 2.001963e-47
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.695e-08 3.486e-09
25- 50 4.114e-07 1.481e-08
50-150 1.544e-06 5.449e-08
15-150 2.033e-06 5.449e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.363 ( )
Norm : 10.4217 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 404.88 using 59 PHA bins.
# Reduced chi-squared = 7.1031 for 57 degrees of freedom
# Null hypothesis probability = 6.449534e-54
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.746e-07 6.771e-09
25- 50 5.282e-07 1.386e-08
50-150 1.158e-06 2.751e-08
15-150 1.961e-06 5.290e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 9.09479 (-0.952826 1.04577)
R1^2/D10^2 : 0.807192 (-0.219391 0.329401)
kT2 [keV] : 38.1662 (-3.88888 5.56976)
R2^2/D10^2 : 1.27515E-02 (-0.00430666 0.00516767)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 41.43 using 59 PHA bins.
# Reduced chi-squared = 0.7532 for 55 degrees of freedom
# Null hypothesis probability = 9.121743e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.645e-07 1.370e-08
25- 50 4.750e-07 2.645e-08
50-150 1.706e-06 1.090e-07
15-150 2.346e-06 1.296e-07
Peak spectrum fit
Power-law model
Time interval is from -0.356 sec. to 0.644 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.767647 ( -0.0526889 0.0522742 )
Norm@50keV : 7.31767E-02 ( -0.00216072 0.00215139 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 35.82 using 59 PHA bins.
# Reduced chi-squared = 0.6283 for 57 degrees of freedom
# Null hypothesis probability = 9.873832e-01
Photon flux (15-150 keV) in 1 sec: 8.42190 ( -0.242212 0.242318 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.66985e-07 ( -2.7094e-08 2.71378e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.356 sec. to 0.644 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.686332 ( -0.194096 0.100059 )
Epeak [keV] : 999.229 ( -999.552 -999.552 )
Norm@50keV : 7.90531E-02 ( -0.002222 0.0155896 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 35.52 using 59 PHA bins.
# Reduced chi-squared = 0.6344 for 56 degrees of freedom
# Null hypothesis probability = 9.851297e-01
Photon flux (15-150 keV) in 1 sec: 8.40064 ( -0.25008 0.24101 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.65579e-07 ( -2.7871e-08 2.6056e-08 ) ergs/cm2
Band function
Time interval is from -0.356 sec. to 0.644 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 5.00000 ( -5 -5 )
beta : -0.784527 ( -0.0544346 0.0547416 )
Epeak [keV] : 26.0983 ( -25.9444 4.81059 )
Norm@50keV : 3105.11 ( -87.067 6.35281e+06 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 34.09 using 59 PHA bins.
# Reduced chi-squared = 0.6197 for 55 degrees of freedom
# Null hypothesis probability = 9.880265e-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] : 26.4812 ( )
R^2/D10^2 : 0.181936 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 201.92 using 59 PHA bins.
# Reduced chi-squared = 3.5424 for 57 degrees of freedom
# Null hypothesis probability = 4.421815e-18
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.148e-08 1.160e-09
25- 50 1.254e-07 5.600e-09
50-150 6.451e-07 2.795e-08
15-150 7.920e-07 2.555e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.363 ( )
Norm : 32.3226 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 612.63 using 59 PHA bins.
# Reduced chi-squared = 10.748 for 57 degrees of freedom
# Null hypothesis probability = 4.168288e-94
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.049e-08 2.605e-09
25- 50 1.548e-07 4.850e-09
50-150 3.396e-07 1.030e-08
15-150 5.749e-07 1.870e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 9.65979 (-1.58066 1.92415)
R1^2/D10^2 : 1.80671 (-0.667554 1.20111)
kT2 [keV] : 43.9776 (-6.17211 11.2735)
R2^2/D10^2 : 3.74239E-02 (-0.0171186 0.0204993)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 40.16 using 59 PHA bins.
# Reduced chi-squared = 0.7302 for 55 degrees of freedom
# Null hypothesis probability = 9.334346e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.261e-08 5.925e-09
25- 50 1.412e-07 1.170e-08
50-150 6.898e-07 7.080e-08
15-150 8.737e-07 6.750e-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: 1.08201 ( -0.0426832 0.0425053 )
Norm@50keV : 2.10697E-02 ( -0.000479065 0.000477953 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 32.74 using 59 PHA bins.
# Reduced chi-squared = 0.5744 for 57 degrees of freedom
# Null hypothesis probability = 9.959144e-01
Photon flux (15-150 keV) in 10.58 sec: 2.44016 ( -0.0586126 0.0581387 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.34421e-06 ( -5.49755e-08 5.50319e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.02224 ( -0.158315 0.075213 )
Epeak [keV] : 990.275 ( -994.013 -994.013 )
Norm@50keV : 2.23154E-02 ( -0.000497796 0.00355428 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 32.53 using 59 PHA bins.
# Reduced chi-squared = 0.5808 for 56 degrees of freedom
# Null hypothesis probability = 9.949287e-01
Photon flux (15-150 keV) in 10.58 sec: 2.43707 ( -0.05664 0.06 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.33904e-06 ( -5.68358e-08 5.92374e-08 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.725949 ( 0.722667 0.722667 )
beta : -1.10680 ( 1.10849 0.0610276 )
Epeak [keV] : 136.519 ( -145.448 325.782 )
Norm@50keV : 3.36989E-02 ( -0.0116406 0 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 31.81 using 59 PHA bins.
# Reduced chi-squared = 0.5784 for 55 degrees of freedom
# Null hypothesis probability = 9.948376e-01
Photon flux (15-150 keV) in 10.58 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) = 4.58e-07
S(50-100 keV) = 8.65e-07
T90 vs. Hardness ratio plot
T90 = 4.30000001192093 sec.
Hardness ratio (energy fluence ratio) = 1.88865
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.65955
Count Ratio (50-100 keV) / (15-25 keV) = 1.65675
Mask shadow pattern
IMX = 1.211522604034570E-01, IMY = 2.403453886967238E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.512000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.512000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.512000
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:
-239.248000 -3.052000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6305 22.0182 0.3 24.5 51.8 10.1283 45.4 0.3 Crab
76.5971 9.8420 2.5 38.3 48.7 1.8025 4.5 ------ UNKNOWN
102.4794 -16.3022 1.9 56.4 4.2 5.6935 6.0 ------ UNKNOWN
133.2913 29.5943 2.9 26.7 -72.9 0.9119 3.9 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-3.052000 7.532000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.7687 22.0906 11.2 24.3 51.7 0.0583 1.0 8.8 Crab
93.8715 34.6733 2.6 9.1 60.3 0.1899 4.5 ------ UNKNOWN
119.6655 32.8565 0.2 15.1 -63.2 3.4454 74.4 ------ UNKNOWN
115.2856 -8.8203 2.4 50.1 -12.3 0.5560 4.9 ------ UNKNOWN
137.8438 40.2680 2.2 26.3 -98.4 0.3065 5.2 ------ UNKNOWN
192.6699 64.4124 2.7 54.3 -144.5 1.0375 4.3 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
50.452600 962.838100
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6263 22.0143 0.3 33.6 69.3 36.9734 37.9 0.4 Crab
71.3060 58.2211 2.8 41.0 132.0 5.5920 4.1 ------ UNKNOWN
83.5241 53.4070 2.6 32.8 128.5 3.8614 4.5 ------ UNKNOWN
86.7982 44.1821 2.4 27.8 112.5 3.7723 4.9 ------ UNKNOWN
92.0993 4.5546 2.5 38.2 37.1 3.7503 4.6 ------ UNKNOWN
149.2800 73.1483 3.3 43.0 -179.0 2.8592 3.5 ------ UNKNOWN
136.0712 34.7215 2.7 13.8 -113.4 2.0115 4.2 ------ UNKNOWN
Plot creation:
Sun May 31 08:55:25 EDT 2015