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Image
Pre-slew 15.0-350.0 keV image (Event data)
# RAcent DECcent POSerr Theta Phi Peak Cts SNR Name
222.7994 47.3223 0.0098 17.6623 102.7802 4.4537122 19.529 TRIG_00620090
Foreground time interval of the image:
-42.748 34.573 (delta_t = 77.321 [sec])
Background time interval of the image:
-68.427 -42.748 (delta_t = 25.679 [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 4.096000
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 4.096000
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 4.096000
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 -42.748 sec. to 40.016 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.56169 ( -0.0825818 0.0829011 )
Norm@50keV : 3.56604E-03 ( -0.00016649 0.000166043 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 60.74 using 59 PHA bins.
# Reduced chi-squared = 1.066 for 57 degrees of freedom
# Null hypothesis probability = 3.428718e-01
Photon flux (15-150 keV) in 82.76 sec: 0.452982 ( -0.0212262 0.0212569 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.7738e-06 ( -1.40199e-07 1.40905e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -42.748 sec. to 40.016 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.29492 ( -0.350138 0.299541 )
Epeak [keV] : 129.052 ( -47.6826 -129.064 )
Norm@50keV : 4.88599E-03 ( -0.00139982 0.00243822 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 58.78 using 59 PHA bins.
# Reduced chi-squared = 1.050 for 56 degrees of freedom
# Null hypothesis probability = 3.740161e-01
Photon flux (15-150 keV) in 82.76 sec: 0.446347 ( -0.022659 0.022647 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.7071e-06 ( -1.63732e-07 1.62781e-07 ) ergs/cm2
Band function
Time interval is from -42.748 sec. to 40.016 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 2.76143 ( -4.83869 -3.77428 )
beta : -1.68200 ( -0.122699 0.107298 )
Epeak [keV] : 29.3236 ( -3.94323 5.13811 )
Norm@50keV : 4.52399 ( -4.5232 87.5382 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 52.84 using 59 PHA bins.
# Reduced chi-squared = 0.9607 for 55 degrees of freedom
# Null hypothesis probability = 5.577412e-01
Photon flux (15-150 keV) in 82.76 sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 2.70283e-06 ( -2.70225e-06 -1.46518e-07 ) ergs/cm2
Single BB
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 14.0283 ( )
R^2/D10^2 : 6.26955E-02 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 157.58 using 59 PHA bins.
# Reduced chi-squared = 2.7646 for 57 degrees of freedom
# Null hypothesis probability = 2.281364e-11
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.157e-07 1.953e-08
25- 50 8.037e-07 4.610e-08
50-150 1.042e-06 1.010e-07
15-150 2.062e-06 1.183e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 198.809 (-47.8603 -198.786)
Norm : 1.83658 (-0.0833087 0.0944254)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 58.57 using 59 PHA bins.
# Reduced chi-squared = 1.028 for 57 degrees of freedom
# Null hypothesis probability = 4.176632e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.786e-07 2.143e-08
25- 50 7.281e-07 4.564e-08
50-150 1.595e-06 3.381e-07
15-150 2.702e-06 4.680e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.81961 (-1.18609 1.34444)
R1^2/D10^2 : 0.349265 (-0.132184 0.239056)
kT2 [keV] : 29.6346 (-6.09487 13.0393)
R2^2/D10^2 : 3.36091E-03 (-0.00227271 0.00429895)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 57.70 using 59 PHA bins.
# Reduced chi-squared = 1.049 for 55 degrees of freedom
# Null hypothesis probability = 3.755757e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.526e-07 5.400e-08
25- 50 7.645e-07 9.650e-08
50-150 1.601e-06 4.478e-07
15-150 2.719e-06 5.044e-07
Peak spectrum fit
Power-law model
Time interval is from -4.688 sec. to -3.688 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.39779 ( -0.233809 0.234916 )
Norm@50keV : 9.93605E-03 ( -0.00148986 0.00148416 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 60.30 using 59 PHA bins.
# Reduced chi-squared = 1.058 for 57 degrees of freedom
# Null hypothesis probability = 3.573148e-01
Photon flux (15-150 keV) in 1 sec: 1.20943 ( -0.180112 0.180395 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.605e-08 ( -1.57406e-08 1.59751e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -4.688 sec. to -3.688 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -0.185925 ( -1.42173 1.09753 )
Epeak [keV] : 68.5343 ( -14.0274 45.1199 )
Norm@50keV : 6.26209E-02 ( -0.0626208 0.243531 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 53.67 using 59 PHA bins.
# Reduced chi-squared = 0.9583 for 56 degrees of freedom
# Null hypothesis probability = 5.636667e-01
Photon flux (15-150 keV) in 1 sec: 1.14600 ( -0.184887 0.18552 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.68429e-08 ( -1.59606e-08 1.68781e-08 ) ergs/cm2
Band function
Time interval is from -4.688 sec. to -3.688 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 0.185538 ( -0.92664 1.5552 )
beta : -10.0000 ( 10 5.32907e-15 )
Epeak [keV] : 68.5294 ( -12.7374 45.0031 )
Norm@50keV : 6.26007E-02 ( -0.0626007 0.244307 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 53.67 using 59 PHA bins.
# Reduced chi-squared = 0.9758 for 55 degrees of freedom
# Null hypothesis probability = 5.256467e-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] : 15.6623 (-2.31315 2.77861)
R^2/D10^2 : 0.128057 (-0.0560034 0.0957635)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 55.95 using 59 PHA bins.
# Reduced chi-squared = 0.9815 for 57 degrees of freedom
# Null hypothesis probability = 5.146338e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.525e-09 1.815e-09
25- 50 2.695e-08 6.480e-09
50-150 4.583e-08 1.429e-08
15-150 7.931e-08 1.655e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.362 (-75.3427 -199.363)
Norm : 5.02375 (-0.734935 0.734924)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 59.03 using 59 PHA bins.
# Reduced chi-squared = 1.036 for 57 degrees of freedom
# Null hypothesis probability = 4.011004e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.251e-08 7.090e-09
25- 50 2.406e-08 1.350e-08
50-150 5.278e-08 2.980e-08
15-150 8.935e-08 5.010e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.15808 (-6.81178 -7.27659)
R1^2/D10^2 : 0.638782 (-0.32928 -0.635935)
kT2 [keV] : 19.3319 (-19.4315 -19.4318)
R2^2/D10^2 : 5.14197E-02 (-0.0260134 0.103903)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 53.23 using 59 PHA bins.
# Reduced chi-squared = 0.9678 for 55 degrees of freedom
# Null hypothesis probability = 5.425350e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 9.131e-09 5.080e-09
25- 50 2.596e-08 1.397e-08
50-150 5.173e-08 2.894e-08
15-150 8.682e-08 4.522e-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: 1.54650 ( -0.0820429 0.0823212 )
Norm@50keV : 3.74512E-03 ( -0.000172647 0.000172235 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 57.30 using 59 PHA bins.
# Reduced chi-squared = 1.005 for 57 degrees of freedom
# Null hypothesis probability = 4.639214e-01
Photon flux (15-150 keV) in 77.32 sec: 0.473630 ( -0.0220418 0.0220746 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.72744e-06 ( -1.3643e-07 1.37097e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.30777 ( -0.343544 0.274666 )
Epeak [keV] : 142.856 ( -57.2453 -142.862 )
Norm@50keV : 4.95432E-03 ( -0.00131004 0.00239219 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 55.69 using 59 PHA bins.
# Reduced chi-squared = 0.9944 for 56 degrees of freedom
# Null hypothesis probability = 4.866720e-01
Photon flux (15-150 keV) in 77.32 sec: 0.467354 ( -0.023527 0.023518 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.67008e-06 ( -1.58475e-07 1.57323e-07 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 1.67997 ( -2.76955 -1.68012 )
beta : -1.66019 ( -0.128717 0.115141 )
Epeak [keV] : 31.6818 ( -5.96376 35.7226 )
Norm@50keV : 0.687041 ( -0.687621 97.8444 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 50.49 using 59 PHA bins.
# Reduced chi-squared = 0.9180 for 55 degrees of freedom
# Null hypothesis probability = 6.474000e-01
Photon flux (15-150 keV) in 77.32 sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 2.66269e-06 ( -2.66215e-06 -1.43112e-07 ) ergs/cm2
S(25-50 keV) vs. S(50-100 keV) plot
S(25-50 keV) = 7.07e-07
S(50-100 keV) = 9.57e-07
T90 vs. Hardness ratio plot
T90 = 62.8559999465942 sec.
Hardness ratio (energy fluence ratio) = 1.35361
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.36463
Count Ratio (50-100 keV) / (15-25 keV) = 0.930037
Mask shadow pattern
IMX = -7.043718197915397E-02, IMY = -3.105275447601950E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 4.096000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 4.096000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 4.096000
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:
-68.427400 -42.748000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.3901 35.3282 3.6 24.9 178.4 0.1931 3.2 3.4 Her X-1
200.0386 40.0949 2.8 23.2 52.1 0.2942 4.1 ------ UNKNOWN
191.9873 -5.0274 2.4 47.4 -22.7 0.5682 4.9 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-42.748000 34.572590
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.5958 35.4058 5.3 25.0 178.3 0.4629 2.2 7.8 Her X-1
222.7994 47.3223 0.6 17.7 102.8 4.4537 19.5 ------ UNKNOWN
193.9613 15.2906 2.2 32.4 -0.7 1.2934 5.3 ------ UNKNOWN
286.5168 23.3353 2.5 54.3 -169.8 2.8064 4.7 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
73.572600 799.072580
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.4918 35.3395 1.2 26.4 -141.0 4.8527 9.3 1.7 Her X-1
299.5915 35.2067 4.3 56.6 -174.0 6.0716 2.7 0.3 Cyg X-1
302.3897 71.3980 2.5 42.7 141.3 6.0926 4.5 ------ UNKNOWN
169.4395 13.9046 4.0 55.3 5.1 6.9388 2.9 ------ UNKNOWN
291.7869 43.3734 3.3 47.0 -178.3 3.6307 3.5 ------ UNKNOWN
230.8264 16.4343 2.8 31.5 -81.1 3.0213 4.1 ------ UNKNOWN
245.5546 20.4937 3.1 32.5 -108.7 2.9847 3.8 ------ UNKNOWN
280.7297 18.1097 4.5 55.2 -145.1 9.4243 2.6 ------ UNKNOWN
198.6491 -2.7449 3.1 54.3 -36.1 10.8961 3.8 ------ UNKNOWN
259.8977 14.1300 3.2 45.2 -121.8 7.0812 3.6 ------ UNKNOWN
Plot creation:
Thu May 28 13:57:54 EDT 2015