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Image
Pre-slew 15.0-350.0 keV image (Event data)
# RAcent DECcent POSerr Theta Phi Peak Cts SNR Name
197.2755 49.8380 0.0055 29.0584 105.7265 15.2761995 34.670 TRIG_00596901
Foreground time interval of the image:
-130.128 108.912 (delta_t = 239.040 [sec])
Background time interval of the image:
-239.184 -130.128 (delta_t = 109.056 [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)
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 -130.128 sec. to 108.912 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.33513 ( -0.0565238 0.0563251 )
Norm@50keV : 4.00113E-03 ( -0.000121131 0.000121108 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 47.91 using 59 PHA bins.
# Reduced chi-squared = 0.8406 for 57 degrees of freedom
# Null hypothesis probability = 7.988438e-01
Photon flux (15-150 keV) in 239 sec: 0.480573 ( -0.0157931 0.0158307 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.37129e-06 ( -3.01742e-07 3.02254e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -130.128 sec. to 108.912 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.16322 ( -0.227853 0.192918 )
Epeak [keV] : 271.029 ( )
Norm@50keV : 4.79027E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 46.09 using 59 PHA bins.
# Reduced chi-squared = 0.8231 for 56 degrees of freedom
# Null hypothesis probability = 8.247693e-01
Photon flux (15-150 keV) in 239 sec: 0.475257 ( -0.017046 0.017082 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.27573e-06 ( -3.29055e-07 3.27406e-07 ) ergs/cm2
Band function
Time interval is from -130.128 sec. to 108.912 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 0.538455 ( -2.63701 -0.971278 )
beta : -1.38093 ( 1.3774 0.0720924 )
Epeak [keV] : 38.4787 ( -17.2603 68.9579 )
Norm@50keV : 7.82767E-02 ( -0.0779836 135.108 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 44.17 using 59 PHA bins.
# Reduced chi-squared = 0.8031 for 55 degrees of freedom
# Null hypothesis probability = 8.519720e-01
Photon flux (15-150 keV) in 239 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] : 18.3665 ( )
R^2/D10^2 : 2.75830E-02 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 253.13 using 59 PHA bins.
# Reduced chi-squared = 4.4409 for 57 degrees of freedom
# Null hypothesis probability = 1.561813e-26
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.423e-07 2.713e-08
25- 50 2.076e-06 9.596e-08
50-150 5.110e-06 2.521e-07
15-150 7.628e-06 2.784e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 ( )
Norm : 2.02324 (-0.0616795 0.0616502)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 95.99 using 59 PHA bins.
# Reduced chi-squared = 1.684 for 57 degrees of freedom
# Null hypothesis probability = 9.471389e-04
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.204e-06 3.860e-08
25- 50 2.317e-06 7.349e-08
50-150 5.082e-06 1.637e-07
15-150 8.603e-06 2.605e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 8.06154 (-1.01494 1.14347)
R1^2/D10^2 : 0.274679 (-0.0917722 0.152828)
kT2 [keV] : 31.3675 (-3.76473 5.66625)
R2^2/D10^2 : 3.75944E-03 (-0.00158621 0.00209742)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 51.10 using 59 PHA bins.
# Reduced chi-squared = 0.9290 for 55 degrees of freedom
# Null hypothesis probability = 6.245724e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 9.104e-07 1.114e-07
25- 50 2.221e-06 1.654e-07
50-150 6.132e-06 5.760e-07
15-150 9.263e-06 7.481e-07
Peak spectrum fit
Power-law model
Time interval is from 44.188 sec. to 45.188 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.19415 ( -0.189737 0.186939 )
Norm@50keV : 1.83307E-02 ( -0.00205655 0.00205563 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 70.77 using 59 PHA bins.
# Reduced chi-squared = 1.242 for 57 degrees of freedom
# Null hypothesis probability = 1.038299e-01
Photon flux (15-150 keV) in 1 sec: 2.14989 ( -0.24505 0.24526 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.86281e-07 ( -2.33939e-08 2.35765e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 44.188 sec. to 45.188 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.980418 ( -0.879528 0.381062 )
Epeak [keV] : 244.833 ( -245.16 -245.16 )
Norm@50keV : 2.34978E-02 ( -0.00928074 0.0408045 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 70.54 using 59 PHA bins.
# Reduced chi-squared = 1.260 for 56 degrees of freedom
# Null hypothesis probability = 9.142196e-02
Photon flux (15-150 keV) in 1 sec: 2.13777 ( -0.24922 0.24875 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.83637e-07 ( -2.6244e-08 2.5247e-08 ) ergs/cm2
Band function
Time interval is from 44.188 sec. to 45.188 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 4.99727 ( -14.9695 -4.99727 )
beta : -1.33952 ( -0.273992 0.22761 )
Epeak [keV] : 29.2537 ( -9.3612 15.4321 )
Norm@50keV : 607.342 ( -67.6291 16936.5 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 68.05 using 59 PHA bins.
# Reduced chi-squared = 1.237 for 55 degrees of freedom
# Null hypothesis probability = 1.112991e-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] : 16.5140 (-2.19956 2.75452)
R^2/D10^2 : 0.188847 (-0.0767221 0.117615)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 84.21 using 59 PHA bins.
# Reduced chi-squared = 1.477 for 57 degrees of freedom
# Null hypothesis probability = 1.105324e-02
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.057e-08 2.676e-09
25- 50 4.567e-08 7.010e-09
50-150 8.807e-08 1.932e-08
15-150 1.443e-07 2.410e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 ( )
Norm : 8.79761 (-1.00679 1.00676)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 79.58 using 59 PHA bins.
# Reduced chi-squared = 1.396 for 57 degrees of freedom
# Null hypothesis probability = 2.576581e-02
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.190e-08 1.191e-08
25- 50 4.213e-08 2.337e-08
50-150 9.241e-08 5.130e-08
15-150 1.564e-07 8.610e-08
Double BB
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 11.9859 (-2.0947 2.6595)
R1^2/D10^2 : 0.454702 (-0.234068 0.400118)
kT2 [keV] : 200.000 ( )
R2^2/D10^2 : 3.15609E-04 (-0.000108797 8.96615e-05)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 65.20 using 59 PHA bins.
#Fit statistic : Chi-Squared = 64.89 using 59 PHA bins.
# Reduced chi-squared = 1.185 for 55 degrees of freedom
# Reduced chi-squared = 1.180 for 55 degrees of freedom
# Null hypothesis probability = 1.633396e-01
# Null hypothesis probability = 1.699972e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.451e-08 4.914e-09
25- 50 4.653e-08 1.798e-08
50-150 1.237e-07 9.434e-08
15-150 1.848e-07 1.189e-07
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: 1.33513 ( -0.0565238 0.0563251 )
Norm@50keV : 4.00113E-03 ( -0.000121131 0.000121108 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 47.91 using 59 PHA bins.
# Reduced chi-squared = 0.8406 for 57 degrees of freedom
# Null hypothesis probability = 7.988438e-01
Photon flux (15-150 keV) in 239 sec: 0.480573 ( -0.0157931 0.0158307 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.37129e-06 ( -3.01742e-07 3.02254e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.16322 ( -0.227853 0.192918 )
Epeak [keV] : 271.029 ( )
Norm@50keV : 4.79027E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 46.09 using 59 PHA bins.
# Reduced chi-squared = 0.8231 for 56 degrees of freedom
# Null hypothesis probability = 8.247693e-01
Photon flux (15-150 keV) in 239 sec: 0.475257 ( -0.017046 0.017082 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.27573e-06 ( -3.29055e-07 3.27406e-07 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 0.369300 ( -2.06256 -0.368849 )
beta : -1.38222 ( 1.38223 0.074495 )
Epeak [keV] : 40.3486 ( -17.2136 114.478 )
Norm@50keV : 5.78850E-02 ( -0.0577116 135.13 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 44.16 using 59 PHA bins.
# Reduced chi-squared = 0.8029 for 55 degrees of freedom
# Null hypothesis probability = 8.521447e-01
Photon flux (15-150 keV) in 239 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) = 2.13e-06
S(50-100 keV) = 3.37e-06
T90 vs. Hardness ratio plot
T90 = 134.143999993801 sec.
Hardness ratio (energy fluence ratio) = 1.58216
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.50528
Count Ratio (50-100 keV) / (15-25 keV) = 1.33307
Mask shadow pattern
IMX = -1.506037702459664E-01, IMY = -5.348419615468998E-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:
-239.184000 -130.128000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
299.6060 35.2186 3.1 57.9 -3.7 2.4521 3.8 1.3 Cyg X-1
308.1073 40.9268 7.3 53.8 -13.1 0.4787 1.6 1.6 Cyg X-3
208.3018 43.4473 2.3 35.7 92.0 1.2829 5.0 ------ UNKNOWN
178.3745 47.6249 1.9 32.0 130.0 1.0461 6.2 ------ UNKNOWN
107.8648 34.1629 2.6 56.4 -157.3 2.0159 4.4 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-130.128000 108.912000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
299.4853 35.2502 5.2 57.8 -3.6 -3.8068 -2.2 5.9 Cyg X-1
308.2230 40.8962 6.2 53.8 -13.2 -1.4951 -1.9 6.1 Cyg X-3
251.1208 36.9666 2.7 47.1 44.0 5.0581 4.2 ------ UNKNOWN
204.0112 45.2785 2.2 33.7 97.2 3.1161 5.1 ------ UNKNOWN
197.2755 49.8380 0.3 29.1 105.7 15.2752 34.7 ------ UNKNOWN
152.1501 64.6322 3.1 19.1 173.8 0.9845 3.7 ------ UNKNOWN
109.6900 52.1668 2.9 38.7 -152.5 1.4767 4.0 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
300.316630 962.840300
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
352.7413 -72.6630 2.6 46.6 45.9 6.2959 4.5 ------ UNKNOWN
332.4196 26.4436 4.3 59.0 -166.2 6.1791 2.7 ------ UNKNOWN
359.8621 10.0084 3.6 36.2 -137.6 1.7709 3.2 ------ UNKNOWN
Plot creation:
Sat May 30 13:45:05 EDT 2015