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Image
Pre-slew 15.0-350.0 keV image (Event data)
# RAcent DECcent POSerr Theta Phi Peak Cts SNR Name
42.3212 9.7902 0.0232 22.7628 -5.3589 0.7769026 8.238 TRIG_00652643
Foreground time interval of the image:
14.008 73.101 (delta_t = 59.093 [sec])
Background time interval of the image:
-239.000 14.008 (delta_t = 253.008 [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 64.000000
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 64.000000
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 64.000000
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 14.008 sec. to 73.448 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.72964 ( -0.266247 0.278934 )
Norm@50keV : 8.55671E-04 ( -0.000151343 0.000147524 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 45.06 using 59 PHA bins.
# Reduced chi-squared = 0.7906 for 57 degrees of freedom
# Null hypothesis probability = 8.736079e-01
Photon flux (15-150 keV) in 59.44 sec: 0.114845 ( -0.0175479 0.017553 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.69904e-07 ( -8.50188e-08 8.72876e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 14.008 sec. to 73.448 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.16434 ( -1.50325 1.06335 )
Epeak [keV] : 64.0867 ( -24.5636 -64.1083 )
Norm@50keV : 1.78690E-03 ( -0.00178565 0.0109456 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 44.38 using 59 PHA bins.
# Reduced chi-squared = 0.7925 for 56 degrees of freedom
# Null hypothesis probability = 8.687236e-01
Photon flux (15-150 keV) in 59.44 sec: 0.112454 ( -0.0182972 0.018218 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.42115e-07 ( -9.77051e-08 1.03571e-07 ) ergs/cm2
Band function
Time interval is from 14.008 sec. to 73.448 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.929449 ( 0.916953 4.95212 )
beta : -2.14258 ( 2.14668 0.629286 )
Epeak [keV] : 53.8502 ( -52.3603 54.0538 )
Norm@50keV : 2.52104E-03 ( -0.00154829 74.2813 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 44.08 using 59 PHA bins.
# Reduced chi-squared = 0.8015 for 55 degrees of freedom
# Null hypothesis probability = 8.541950e-01
Photon flux (15-150 keV) in 59.44 sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 4.45961e-07 ( 0 0 ) ergs/cm2
Single BB
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 11.5400 (-1.91208 2.34078)
R^2/D10^2 : 3.25214E-02 (-0.0161115 0.0308265)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 51.20 using 59 PHA bins.
# Reduced chi-squared = 0.8983 for 57 degrees of freedom
# Null hypothesis probability = 6.913628e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.422e-08 1.723e-08
25- 50 1.628e-07 3.902e-08
50-150 1.269e-07 4.553e-08
15-150 3.439e-07 8.289e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 109.407 (-47.3699 -109.562)
Norm : 0.500537 (-0.0871929 0.122099)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 44.39 using 59 PHA bins.
# Reduced chi-squared = 0.7787 for 57 degrees of freedom
# Null hypothesis probability = 8.883991e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.771e-08 1.644e-08
25- 50 1.367e-07 4.873e-08
50-150 2.328e-07 1.425e-07
15-150 4.472e-07 1.937e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.88123 (-3.43725 6.11371)
R1^2/D10^2 : 0.221301 (-0.183202 8.40769)
kT2 [keV] : 18.3485 (-6.70003 -18.6499)
R2^2/D10^2 : 4.39914E-03 (-0.00404928 0.0223271)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 45.03 using 59 PHA bins.
# Reduced chi-squared = 0.8187 for 55 degrees of freedom
# Null hypothesis probability = 8.290768e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.623e-08 4.289e-08
25- 50 1.382e-07 7.082e-08
50-150 2.065e-07 1.252e-07
15-150 4.209e-07 2.189e-07
Peak spectrum fit
Power-law model
Time interval is from 17.676 sec. to 18.676 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.29508 ( -0.849725 1.36373 )
Norm@50keV : 1.82461E-03 ( -0.00182457 0.0012245 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 57.69 using 59 PHA bins.
# Reduced chi-squared = 1.012 for 57 degrees of freedom
# Null hypothesis probability = 4.493780e-01
Photon flux (15-150 keV) in 1 sec: 0.317995 ( -0.131781 0.131859 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.74197e-08 ( -9.33851e-09 1.0676e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 17.676 sec. to 18.676 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.88267 ( )
Epeak [keV] : 13.5113 ( )
Norm@50keV : 3.05799E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 57.85 using 59 PHA bins.
# Reduced chi-squared = 1.033 for 56 degrees of freedom
# Null hypothesis probability = 4.066547e-01
Photon flux (15-150 keV) in 1 sec: 0.317130 ( -0.13106 0.132454 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.74048e-08 ( -9.39784e-09 1.05174e-08 ) ergs/cm2
Band function
Time interval is from 17.676 sec. to 18.676 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.63143 ( 1.63351 1.63351 )
beta : -2.27153 ( 2.28202 0.835494 )
Epeak [keV] : 10.3082 ( -9.63288 -9.63288 )
Norm@50keV : 6.77132E-03 ( -0.00708129 1.4233e+06 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 57.70 using 59 PHA bins.
# Reduced chi-squared = 1.049 for 55 degrees of freedom
# Null hypothesis probability = 3.757840e-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] : 8.72007 (-5.47647 8.52166)
R^2/D10^2 : 0.237766 (-0.235402 39.6038)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 60.74 using 59 PHA bins.
# Reduced chi-squared = 1.066 for 57 degrees of freedom
# Null hypothesis probability = 3.425825e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.717e-09 2.405e-09
25- 50 6.760e-09 4.465e-09
50-150 1.909e-09 1.644e-09
15-150 1.239e-08 8.060e-09
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 45.0412 (-45.0566 -45.0566)
Norm : 1.90465 (-1.02744 5.28347)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 58.19 using 59 PHA bins.
# Reduced chi-squared = 1.021 for 57 degrees of freedom
# Null hypothesis probability = 4.313039e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.536e-09 2.856e-09
25- 50 6.265e-09 3.945e-09
50-150 5.493e-09 4.969e-09
15-150 1.629e-08 1.136e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 3.20662 (-2.29967 4.34134)
R1^2/D10^2 : 14.3807 (-13.9785 17557.5)
kT2 [keV] : 15.1235 (-7.97038 -15.1408)
R2^2/D10^2 : 2.26240E-02 (-0.022399 0.397868)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 56.95 using 59 PHA bins.
# Reduced chi-squared = 1.035 for 55 degrees of freedom
# Null hypothesis probability = 4.024801e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.101e-09 2.778e-09
25- 50 5.066e-09 3.006e-09
50-150 6.768e-09 4.816e-09
15-150 1.693e-08 8.875e-09
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: 1.74049 ( -0.267915 0.281211 )
Norm@50keV : 8.49224E-04 ( -0.00015208 0.000148172 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 45.11 using 59 PHA bins.
# Reduced chi-squared = 0.7915 for 57 degrees of freedom
# Null hypothesis probability = 8.724518e-01
Photon flux (15-150 keV) in 59.09 sec: 0.114429 ( -0.0176013 0.0176059 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.63299e-07 ( -8.45336e-08 8.68434e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.14017 ( -1.53672 1.08167 )
Epeak [keV] : 61.7030 ( -21.2296 -61.7207 )
Norm@50keV : 1.86209E-03 ( -0.000595414 0.0121669 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 44.37 using 59 PHA bins.
# Reduced chi-squared = 0.7923 for 56 degrees of freedom
# Null hypothesis probability = 8.689875e-01
Photon flux (15-150 keV) in 59.09 sec: 0.111921 ( -0.0183415 0.018277 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.34055e-07 ( -9.68083e-08 1.03438e-07 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.910596 ( 0.895707 5.86449 )
beta : -2.16911 ( 2.17386 0.642571 )
Epeak [keV] : 52.5577 ( -50.8353 52.522 )
Norm@50keV : 2.61447E-03 ( -0.00292459 67.7366 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 44.06 using 59 PHA bins.
# Reduced chi-squared = 0.8011 for 55 degrees of freedom
# Null hypothesis probability = 8.546450e-01
Photon flux (15-150 keV) in 59.09 sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 4.38604e-07 ( 0 0 ) ergs/cm2
S(25-50 keV) vs. S(50-100 keV) plot
S(25-50 keV) = 1.29e-07
S(50-100 keV) = 1.55e-07
T90 vs. Hardness ratio plot
T90 = 51.6640000343323 sec.
Hardness ratio (energy fluence ratio) = 1.20155
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.17945
Count Ratio (50-100 keV) / (15-25 keV) = 0.662141
Mask shadow pattern
IMX = 4.177627969290901E-01, IMY = 3.918811376565548E-02
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 64.000000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 64.000000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 64.000000
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 14.008000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
326.0368 38.2599 10.6 51.4 155.9 -1.1193 -1.1 7.4 Cyg X-2
48.7411 -17.6242 3.3 49.7 9.5 1.8864 3.5 ------ UNKNOWN
316.9616 69.7563 3.1 57.6 -165.4 3.9815 3.7 ------ UNKNOWN
53.7399 53.1691 0.6 32.6 -112.6 7.0350 19.9 ------ UNKNOWN
76.2402 -2.9214 3.0 56.3 -28.3 4.1094 3.9 ------ UNKNOWN
72.2319 49.9186 4.7 41.1 -98.6 2.6501 2.5 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
14.008000 73.100590
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
326.1527 38.3562 17.0 51.3 156.0 0.2642 0.7 2.3 Cyg X-2
42.3212 9.7902 1.4 22.8 -5.4 0.7770 8.2 ------ UNKNOWN
30.2037 50.5087 2.0 23.3 -137.5 0.5156 5.8 ------ UNKNOWN
26.8492 62.2195 2.4 34.9 -142.8 0.5504 4.8 ------ UNKNOWN
54.0461 59.8173 2.3 37.4 -120.6 0.8386 5.1 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
121.900600 963.099900
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
17.5804 -30.2479 4.6 46.6 45.9 5.8396 2.5 ------ UNKNOWN
23.2911 55.3310 1.9 48.0 -178.5 7.2101 6.3 ------ UNKNOWN
64.1406 -3.9208 2.2 25.7 -42.8 2.7021 5.3 ------ UNKNOWN
53.7682 53.1567 0.6 44.4 -154.2 19.6758 20.0 ------ UNKNOWN
64.6762 34.9739 3.2 32.4 -128.5 2.5593 3.7 ------ UNKNOWN
73.9061 59.5407 3.7 55.1 -145.1 11.6362 3.6 ------ UNKNOWN
74.0506 59.6794 5.1 55.3 -145.2 9.2359 3.0 ------ UNKNOWN
85.6659 -2.6128 2.6 44.9 -60.2 9.9703 4.4 ------ UNKNOWN
Plot creation:
Wed Sep 30 11:09:32 EDT 2015