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Image
Pre-slew 15.0-350.0 keV image (Event data)
# RAcent DECcent POSerr Theta Phi Peak Cts SNR Name
346.1200 3.9386 0.0179 36.8819 65.4624 2.7499743 10.759 TRIG_00230711
Foreground time interval of the image:
6.824 86.616 (delta_t = 79.792 [sec])
Background time interval of the image:
-239.000 6.824 (delta_t = 245.824 [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 88.000000
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 88.000000
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 88.000000
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 6.824 sec. to 86.616 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.24360 ( -0.218623 0.236028 )
Norm@50keV : 2.07708E-03 ( -0.000342968 0.000336412 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 52.87 using 59 PHA bins.
# Reduced chi-squared = 0.9275 for 57 degrees of freedom
# Null hypothesis probability = 6.308149e-01
Photon flux (15-150 keV) in 79.79 sec: 0.351943 ( -0.0390857 0.0390861 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.56844e-06 ( -2.14874e-07 2.21752e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from 6.824 sec. to 86.616 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.12925 ( -1.68351 0.88727 )
Epeak [keV] : 28.3217 ( )
Norm@50keV : 1.03768E-02 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 50.41 using 59 PHA bins.
# Reduced chi-squared = 0.9002 for 56 degrees of freedom
# Null hypothesis probability = 6.854829e-01
Photon flux (15-150 keV) in 79.79 sec: 0.338965 ( -0.040996 0.041365 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.3883e-06 ( -2.33114e-07 2.87236e-07 ) ergs/cm2
Band function
Time interval is from 6.824 sec. to 86.616 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.490688 ( -1.77368 0.44513 )
beta : -2.80531 ( 2.78593 0.567696 )
Epeak [keV] : 28.2812 ( -8.92762 7.97392 )
Norm@50keV : 2.92483E-02 ( -0.037382 269.299 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 49.42 using 59 PHA bins.
# Reduced chi-squared = 0.8986 for 55 degrees of freedom
# Null hypothesis probability = 6.867514e-01
Photon flux (15-150 keV) in 79.79 sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 1.45685e-06 ( 0 0 ) ergs/cm2
Single BB
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 8.15404 (-0.919992 1.03452)
R^2/D10^2 : 0.361117 (-0.137983 0.224469)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 56.66 using 59 PHA bins.
# Reduced chi-squared = 0.9941 for 57 degrees of freedom
# Null hypothesis probability = 4.877137e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.512e-07 6.595e-08
25- 50 6.353e-07 1.014e-07
50-150 1.775e-07 6.351e-08
15-150 1.164e-06 1.723e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 42.0607 (-10.6839 16.7139)
Norm : 2.20764 (-0.434381 0.566023)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 50.44 using 59 PHA bins.
# Reduced chi-squared = 0.8849 for 57 degrees of freedom
# Null hypothesis probability = 7.179173e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.111e-07 6.395e-08
25- 50 5.525e-07 8.246e-08
50-150 4.512e-07 1.717e-07
15-150 1.415e-06 2.645e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.15568 (-4.9697 1.27953)
R1^2/D10^2 : 0.555653 (-0.248983 52.2813)
kT2 [keV] : 36.0220 (-27.2834 -37.7868)
R2^2/D10^2 : 5.65647E-04 (-0.000481701 0.00521765)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 49.81 using 59 PHA bins.
# Reduced chi-squared = 0.9056 for 55 degrees of freedom
# Null hypothesis probability = 6.726204e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.810e-07 1.108e-07
25- 50 5.864e-07 1.759e-07
50-150 5.435e-07 3.021e-07
15-150 1.511e-06 4.664e-07
Peak spectrum fit
Power-law model
Time interval is from 27.500 sec. to 28.500 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.09755 ( -0.62289 0.815286 )
Norm@50keV : 5.67378E-03 ( -0.00294643 0.00280951 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 38.10 using 59 PHA bins.
# Reduced chi-squared = 0.6683 for 57 degrees of freedom
# Null hypothesis probability = 9.744983e-01
Photon flux (15-150 keV) in 1 sec: 0.891552 ( -0.34394 0.34395 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.2693e-08 ( -2.35618e-08 2.54348e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 27.500 sec. to 28.500 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -0.127178 ( 0.138269 2.28166 )
Epeak [keV] : 41.8122 ( )
Norm@50keV : 9.82013E-02 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 36.49 using 59 PHA bins.
# Reduced chi-squared = 0.6517 for 56 degrees of freedom
# Null hypothesis probability = 9.798236e-01
Photon flux (15-150 keV) in 1 sec: 0.855179 ( -0.393102 0.348501 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.89368e-08 ( -2.0031e-08 2.45875e-08 ) ergs/cm2
Band function
Time interval is from 27.500 sec. to 28.500 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -6.87921E-02 ( -1.4652 0.53488 )
beta : -10.0000 ( 10 3.55271e-15 )
Epeak [keV] : 41.8080 ( -21.8883 203.339 )
Norm@50keV : 7.75045E-02 ( -0.0774072 45.9881 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 36.50 using 59 PHA bins.
# Reduced chi-squared = 0.6637 for 55 degrees of freedom
# Null hypothesis probability = 9.742167e-01
Photon flux (15-150 keV) in 1 sec: 0.867980 ( 6.13202 -0.377849 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.95095e-08 ( -4.95025e-08 -2.05307e-08 ) ergs/cm2
Single BB
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 11.1352 (-3.43744 4.67031)
R^2/D10^2 : 0.303212 (-0.303212 0.900805)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 36.63 using 59 PHA bins.
# Reduced chi-squared = 0.6427 for 57 degrees of freedom
# Null hypothesis probability = 9.835691e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.874e-09 5.000e-09
25- 50 2.262e-08 1.439e-08
50-150 1.599e-08 1.199e-08
15-150 4.648e-08 3.091e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 57.5546 (-33.0831 -56.8444)
Norm : 4.91609 (-2.2746 4.1787)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 37.05 using 59 PHA bins.
# Reduced chi-squared = 0.6501 for 57 degrees of freedom
# Null hypothesis probability = 9.812769e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.227e-08 7.760e-09
25- 50 1.843e-08 1.184e-08
50-150 2.025e-08 1.617e-08
15-150 5.095e-08 3.517e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 2.80105 (-2.85239 17.3462)
R1^2/D10^2 : 43.5104 (-42.3598 -42.3598)
kT2 [keV] : 12.4761 (-4.10008 -12.5045)
R2^2/D10^2 : 0.177775 (-0.176284 0.653044)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 35.40 using 59 PHA bins.
# Reduced chi-squared = 0.6437 for 55 degrees of freedom
# Null hypothesis probability = 9.815283e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.111e-08 4.951e-09
25- 50 1.990e-08 1.201e-08
50-150 1.853e-08 1.377e-08
15-150 4.955e-08 3.050e-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: 2.24360 ( -0.218623 0.236028 )
Norm@50keV : 2.07708E-03 ( -0.000342968 0.000336412 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 52.87 using 59 PHA bins.
# Reduced chi-squared = 0.9275 for 57 degrees of freedom
# Null hypothesis probability = 6.308149e-01
Photon flux (15-150 keV) in 79.79 sec: 0.351943 ( -0.0390857 0.0390861 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.56844e-06 ( -2.14874e-07 2.21752e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.12925 ( -1.68351 0.88727 )
Epeak [keV] : 28.3217 ( )
Norm@50keV : 1.03768E-02 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 50.41 using 59 PHA bins.
# Reduced chi-squared = 0.9002 for 56 degrees of freedom
# Null hypothesis probability = 6.854829e-01
Photon flux (15-150 keV) in 79.79 sec: 0.338965 ( -0.040996 0.041365 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.3883e-06 ( -2.33114e-07 2.87236e-07 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.490688 ( -2.16955 0.44513 )
beta : -2.80531 ( 2.78593 0.567696 )
Epeak [keV] : 28.2812 ( -8.92762 7.97392 )
Norm@50keV : 2.92483E-02 ( -0.037382 269.421 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 49.42 using 59 PHA bins.
# Reduced chi-squared = 0.8986 for 55 degrees of freedom
# Null hypothesis probability = 6.867514e-01
Photon flux (15-150 keV) in 79.79 sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 1.45685e-06 ( 0 0 ) ergs/cm2
S(25-50 keV) vs. S(50-100 keV) plot
S(25-50 keV) = 5.01e-07
S(50-100 keV) = 4.23e-07
T90 vs. Hardness ratio plot
T90 = 73.7279999554157 sec.
Hardness ratio (energy fluence ratio) = 0.844311
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.2374
Count Ratio (50-100 keV) / (15-25 keV) = 0.372534
Mask shadow pattern
IMX = 3.116029084608269E-01, IMY = -6.825640912998497E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 88.000000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 88.000000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 88.000000
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:
-239.000000 6.824000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
285.1042 -24.9698 10.1 57.6 -26.8 1.4230 1.1 4.7 HT1900.1-2455
14.5430 -7.4317 2.6 33.2 119.8 1.5385 4.4 ------ UNKNOWN
10.2768 -47.8148 2.8 20.9 -143.8 0.6852 4.1 ------ UNKNOWN
309.4091 -35.5550 2.1 34.5 -32.7 1.1734 5.4 ------ UNKNOWN
39.2553 -55.4099 2.7 40.2 -146.8 1.1240 4.2 ------ UNKNOWN
324.1916 -70.8044 4.8 40.9 -92.8 2.2592 2.4 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
6.824000 86.616000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
285.0305 -25.1017 6.2 57.6 -26.9 -0.9907 -1.9 10.9 HT1900.1-2455
356.6368 6.3311 2.3 39.3 82.5 2.1577 5.1 429.9 UNKNOWN
346.1200 3.9386 1.1 36.9 65.5 2.7499 10.8 ------ UNKNOWN
52.9668 -48.5106 2.4 48.1 -157.6 0.9275 4.7 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
190.500600 963.103200
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
326.2631 38.4197 4.0 38.9 -39.7 1.7538 2.9 7.3 Cyg X-2
23.0203 43.3653 3.5 51.1 19.6 6.5386 3.3 ------ UNKNOWN
331.6243 -18.0449 3.3 26.3 -161.9 1.3745 3.5 ------ UNKNOWN
317.0617 -48.4911 2.3 58.3 -172.3 10.4057 4.9 ------ UNKNOWN
306.1538 -43.3880 4.6 59.5 -161.7 9.0493 2.5 ------ UNKNOWN
324.3788 57.6259 3.9 56.3 -28.3 6.4713 2.9 ------ UNKNOWN
311.2437 40.8078 3.1 48.3 -50.0 7.3648 3.7 ------ UNKNOWN
305.0203 7.2351 4.4 41.1 -98.1 6.5298 2.7 ------ UNKNOWN
303.5000 -2.2338 3.5 43.1 -112.1 6.0183 3.3 ------ UNKNOWN
Plot creation:
Sun May 31 11:57:36 EDT 2015