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Image
Pre-slew 15.0-350.0 keV image (Event data)
# RAcent DECcent POSerr Theta Phi Peak Cts SNR Name
350.6460 5.7877 0.0085 34.6571 39.5558 1.6594723 22.602 TRIG_00148833
Foreground time interval of the image:
59.584 81.501 (delta_t = 21.917 [sec])
Background time interval of the image:
-299.000 59.584 (delta_t = 358.584 [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 72.000000
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 72.000000
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 72.000000
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 59.584 sec. to 165.124 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.39244 ( -0.10632 0.106045 )
Norm@50keV : 2.11957E-03 ( -0.000121878 0.00012183 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 49.58 using 59 PHA bins.
# Reduced chi-squared = 0.8699 for 57 degrees of freedom
# Null hypothesis probability = 7.466557e-01
Photon flux (15-150 keV) in 105.5 sec: 0.257684 ( -0.0156683 0.0157249 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.16408e-06 ( -1.35504e-07 1.36245e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from 59.584 sec. to 165.124 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.38911 ( -0.358903 0.141575 )
Epeak [keV] : 9999.20 ( )
Norm@50keV : 2.12730E-03 ( -0.000122238 0.00106612 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 49.59 using 59 PHA bins.
# Reduced chi-squared = 0.8855 for 56 degrees of freedom
# Null hypothesis probability = 7.147080e-01
Photon flux (15-150 keV) in 105.5 sec: 0.257627 ( -0.015411 0.015546 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.16412e-06 ( -1.41824e-07 1.35093e-07 ) ergs/cm2
Band function
Time interval is from 59.584 sec. to 165.124 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.12657 ( 1.12656 1.12656 )
beta : -1.39242 ( -0.106258 0.106342 )
Epeak [keV] : 34.9571 ( -34.9597 -34.9597 )
Norm@50keV : 4.17219E-03 ( -0.00173627 511.663 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 49.58 using 59 PHA bins.
# Reduced chi-squared = 0.9015 for 55 degrees of freedom
# Null hypothesis probability = 6.809022e-01
Photon flux (15-150 keV) in 105.5 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] : 17.7508 ( )
R^2/D10^2 : 1.63406E-02 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 123.91 using 59 PHA bins.
# Reduced chi-squared = 2.1739 for 57 degrees of freedom
# Null hypothesis probability = 7.282594e-07
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.092e-07 1.280e-08
25- 50 4.999e-07 4.399e-08
50-150 1.139e-06 1.111e-07
15-150 1.748e-06 1.329e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 ( )
Norm : 1.06973 (-0.0617661 0.0617569)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 59.22 using 59 PHA bins.
# Reduced chi-squared = 1.039 for 57 degrees of freedom
# Null hypothesis probability = 3.945626e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.811e-07 1.915e-08
25- 50 5.407e-07 4.315e-08
50-150 1.186e-06 2.034e-07
15-150 2.008e-06 2.653e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.64703 (-1.34033 1.84204)
R1^2/D10^2 : 0.533006 (-0.337028 1.1202)
kT2 [keV] : 25.5298 (-3.54709 5.91645)
R2^2/D10^2 : 4.20323E-03 (-0.00215512 0.00292116)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 53.54 using 59 PHA bins.
# Reduced chi-squared = 0.9735 for 55 degrees of freedom
# Null hypothesis probability = 5.304847e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.669e-07 8.841e-08
25- 50 4.739e-07 8.356e-08
50-150 1.385e-06 2.274e-07
15-150 2.126e-06 2.801e-07
Peak spectrum fit
Power-law model
Time interval is from 147.108 sec. to 148.108 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.23417 ( -0.211519 0.208983 )
Norm@50keV : 8.11185E-03 ( -0.000947142 0.000945399 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 46.18 using 59 PHA bins.
# Reduced chi-squared = 0.8102 for 57 degrees of freedom
# Null hypothesis probability = 8.466251e-01
Photon flux (15-150 keV) in 1 sec: 0.956997 ( -0.112379 0.112512 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.15264e-08 ( -1.09392e-08 1.10615e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 147.108 sec. to 148.108 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.40047 ( -0.299427 0.202002 )
Epeak [keV] : 132.114 ( -9999.36 -9999.36 )
Norm@50keV : 1.68063E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 45.88 using 59 PHA bins.
# Reduced chi-squared = 0.8193 for 56 degrees of freedom
# Null hypothesis probability = 8.306485e-01
Photon flux (15-150 keV) in 1 sec: 0.958048 ( -0.113184 0.111422 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.15961e-08 ( -1.09992e-08 1.06798e-08 ) ergs/cm2
Band function
Time interval is from 147.108 sec. to 148.108 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 4.73891 ( -4.73891 -4.73891 )
beta : -1.28925 ( -0.240925 0.231238 )
Epeak [keV] : 23.8889 ( -23.8889 7.71786 )
Norm@50keV : 572.117 ( -66.2332 2.62108e+06 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 45.74 using 59 PHA bins.
# Reduced chi-squared = 0.8317 for 55 degrees of freedom
# Null hypothesis probability = 8.087344e-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] : 16.9594 (-3.20522 4.35048)
R^2/D10^2 : 7.20375E-02 (-0.0372683 0.0726331)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 75.01 using 59 PHA bins.
# Reduced chi-squared = 1.316 for 57 degrees of freedom
# Null hypothesis probability = 5.509435e-02
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.223e-09 1.063e-09
25- 50 1.865e-08 3.475e-09
50-150 3.826e-08 9.130e-09
15-150 6.113e-08 1.080e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 ( )
Norm : 3.89612 (-0.459969 0.459959)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 53.43 using 59 PHA bins.
# Reduced chi-squared = 0.9374 for 57 degrees of freedom
# Null hypothesis probability = 6.096230e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 9.700e-09 5.440e-09
25- 50 1.866e-08 1.024e-08
50-150 4.092e-08 2.265e-08
15-150 6.929e-08 3.777e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 8.33709 (-1.92777 2.35576)
R1^2/D10^2 : 0.595567 (-0.330673 0.836633)
kT2 [keV] : 56.6554 (-24.2738 -56.6555)
R2^2/D10^2 : 1.71339E-03 (-0.00146577 0.00471043)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 42.25 using 59 PHA bins.
# Reduced chi-squared = 0.7681 for 55 degrees of freedom
# Null hypothesis probability = 8.962094e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.249e-09 3.307e-09
25- 50 1.851e-08 6.593e-09
50-150 5.963e-08 3.199e-08
15-150 8.639e-08 3.942e-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: 1.36905 ( -0.121054 0.120292 )
Norm@50keV : 5.26702E-03 ( -0.00036455 0.000364484 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 81.32 using 59 PHA bins.
# Reduced chi-squared = 1.427 for 57 degrees of freedom
# Null hypothesis probability = 1.890536e-02
Photon flux (15-150 keV) in 21.92 sec: 0.637063 ( -0.0464034 0.0465209 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.12287e-06 ( -8.38806e-08 8.42129e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.946520 ( -0.571858 0.467547 )
Epeak [keV] : 132.331 ( -48.0469 -132.342 )
Norm@50keV : 8.40067E-03 ( -0.00329328 0.00710352 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 79.29 using 59 PHA bins.
# Reduced chi-squared = 1.416 for 56 degrees of freedom
# Null hypothesis probability = 2.198231e-02
Photon flux (15-150 keV) in 21.92 sec: 0.624400 ( -0.04904 0.048856 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.09423e-06 ( -9.25177e-08 9.16103e-08 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.716480 ( -0.596887 1.34459 )
beta : -1.65802 ( 1.64906 0.308224 )
Epeak [keV] : 95.1060 ( -39.4707 329.53 )
Norm@50keV : 1.12822E-02 ( -0.00647574 131.596 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 78.50 using 59 PHA bins.
# Reduced chi-squared = 1.427 for 55 degrees of freedom
# Null hypothesis probability = 2.043063e-02
Photon flux (15-150 keV) in 21.92 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) = 5.07e-07
S(50-100 keV) = 7.72e-07
T90 vs. Hardness ratio plot
T90 = 88.1240000128746 sec.
Hardness ratio (energy fluence ratio) = 1.52268
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.26087
Count Ratio (50-100 keV) / (15-25 keV) = 1.10484
Mask shadow pattern
IMX = 5.330146659035959E-01, IMY = -4.402563902034786E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 72.000000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 72.000000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 72.000000
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:
-299.000000 59.584000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
299.5925 35.2004 0.3 31.1 156.9 12.8958 40.5 0.1 Cyg X-1
308.0973 40.9182 1.0 23.4 166.2 2.4185 11.6 2.1 Cyg X-3
325.9843 38.3560 4.9 9.9 153.0 0.5280 2.4 9.1 Cyg X-2
273.4155 28.5039 2.2 54.1 161.1 5.8975 5.2 ------ UNKNOWN
308.0689 37.6590 1.4 23.9 158.2 1.8756 8.1 ------ UNKNOWN
34.7657 62.6406 3.0 41.0 -83.4 4.4559 3.8 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
59.584000 81.500600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
299.4096 35.0919 175.8 31.3 156.8 -0.0036 -0.1 11.0 Cyg X-1
308.0245 41.1050 18.0 23.5 166.7 -0.0292 -0.6 9.9 Cyg X-3
326.2868 38.1431 1059.1 9.7 151.6 -0.0004 -0.0 12.0 Cyg X-2
350.6461 5.7877 0.5 34.7 39.6 1.6596 22.6 ------ UNKNOWN
297.1953 37.6910 2.7 32.3 162.5 0.2190 4.3 ------ UNKNOWN
291.0749 46.7117 2.8 35.3 179.8 0.2306 4.1 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
140.100590 303.111900
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
308.0062 40.8971 5.7 51.8 172.6 0.7448 2.0 5.8 Cyg X-3
326.1943 38.1347 0.0 39.2 -177.7 -0.3381 -2.0 11.3 Cyg X-2
356.5260 -38.3625 2.2 44.5 26.7 1.3801 5.2 ------ UNKNOWN
329.3347 12.7007 2.9 22.1 143.0 0.5110 4.0 ------ UNKNOWN
310.4249 47.5852 2.7 54.1 -179.3 1.6677 4.3 ------ UNKNOWN
Plot creation:
Sun May 31 16:07:51 EDT 2015