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Image
Pre-slew 15.0-350.0 keV image (Event data)
# RAcent DECcent POSerr Theta Phi Peak Cts SNR Name
324.9880 -61.4612 0.0081 33.5054 148.3565 4.1721371 23.682 TRIG_00635289
Foreground time interval of the image:
-4.516 76.877 (delta_t = 81.393 [sec])
Background time interval of the image:
-361.323 -345.494 (delta_t = 15.829 [sec])
-239.624 -4.516 (delta_t = 235.108 [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
8 ms binning
From T100_start-3 s to T100_start+3 s
2 ms binning
From T100_start-1 s to T100_start+1 s
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 -4.516 sec. to 115.004 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.05709 ( -0.119035 0.12247 )
Norm@50keV : 2.21867E-03 ( -0.000173524 0.00017127 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 69.30 using 59 PHA bins.
# Reduced chi-squared = 1.216 for 57 degrees of freedom
# Null hypothesis probability = 1.271279e-01
Photon flux (15-150 keV) in 119.5 sec: 0.341843 ( -0.021646 0.021664 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.45412e-06 ( -1.76824e-07 1.78831e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -4.516 sec. to 115.004 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.52847 ( -0.632929 0.490059 )
Epeak [keV] : 36.3007 ( -32.0254 14.1157 )
Norm@50keV : 4.51577E-03 ( -0.00218165 0.00611378 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 66.47 using 59 PHA bins.
# Reduced chi-squared = 1.187 for 56 degrees of freedom
# Null hypothesis probability = 1.597807e-01
Photon flux (15-150 keV) in 119.5 sec: 0.333591 ( -0.023225 0.023133 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.31035e-06 ( -2.22294e-07 2.28365e-07 ) ergs/cm2
Band function
Time interval is from -4.516 sec. to 115.004 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 0.874371 ( -1.34619 0.138296 )
beta : -2.30260 ( -0.430298 0.217663 )
Epeak [keV] : 28.1108 ( -6.69329 8.69303 )
Norm@50keV : 0.242320 ( -0.240088 191.345 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 61.27 using 59 PHA bins.
# Reduced chi-squared = 1.114 for 55 degrees of freedom
# Null hypothesis probability = 2.612264e-01
Photon flux (15-150 keV) in 119.5 sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 2.34134e-06 ( -2.3405e-06 -1.88177e-07 ) ergs/cm2
Single BB
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 9.39975 (-0.663973 0.720495)
R^2/D10^2 : 0.196741 (-0.0499084 0.0663837)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 103.94 using 59 PHA bins.
# Reduced chi-squared = 1.8236 for 57 degrees of freedom
# Null hypothesis probability = 1.459124e-04
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.130e-07 4.499e-08
25- 50 9.381e-07 6.752e-08
50-150 4.081e-07 7.445e-08
15-150 1.759e-06 1.261e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 59.3242 (-10.5324 13.8705)
Norm : 1.78629 (-0.19646 0.209629)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 66.62 using 59 PHA bins.
# Reduced chi-squared = 1.169 for 57 degrees of freedom
# Null hypothesis probability = 1.796254e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.355e-07 4.774e-08
25- 50 8.122e-07 5.832e-08
50-150 9.154e-07 1.484e-07
15-150 2.263e-06 1.703e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.28796 (-1.18626 1.06197)
R1^2/D10^2 : 0.453292 (-0.168433 0.358755)
kT2 [keV] : 31.6233 (-12.615 60.763)
R2^2/D10^2 : 1.17583E-03 (-0.00105787 0.00545835)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 62.43 using 59 PHA bins.
# Reduced chi-squared = 1.135 for 55 degrees of freedom
# Null hypothesis probability = 2.291281e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.023e-07 7.385e-08
25- 50 8.454e-07 1.236e-07
50-150 1.062e-06 5.024e-07
15-150 2.409e-06 6.047e-07
Peak spectrum fit
Power-law model
Time interval is from 66.616 sec. to 67.616 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.03878 ( -0.353454 0.384229 )
Norm@50keV : 7.38764E-03 ( -0.00192383 0.00186068 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 57.88 using 59 PHA bins.
# Reduced chi-squared = 1.015 for 57 degrees of freedom
# Null hypothesis probability = 4.425228e-01
Photon flux (15-150 keV) in 1 sec: 1.12837 ( -0.226701 0.226759 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.82899e-08 ( -1.61007e-08 1.67498e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 66.616 sec. to 67.616 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.12092 ( -5.44801 0.99119 )
Epeak [keV] : 34.9960 ( )
Norm@50keV : 2.80657E-02 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 57.22 using 59 PHA bins.
# Reduced chi-squared = 1.022 for 56 degrees of freedom
# Null hypothesis probability = 4.297140e-01
Photon flux (15-150 keV) in 1 sec: 1.09947 ( -0.242106 0.23496 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.04681e-08 ( -2.01586e-08 2.23808e-08 ) ergs/cm2
Band function
Time interval is from 66.616 sec. to 67.616 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 5.00000 ( -6.86138 -5 )
beta : -2.42763 ( -1.28306 0.515948 )
Epeak [keV] : 24.6691 ( -7.85815 6.29948 )
Norm@50keV : 1493.09 ( -293.092 16716.7 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 54.74 using 59 PHA bins.
# Reduced chi-squared = 0.9952 for 55 degrees of freedom
# Null hypothesis probability = 4.847022e-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] : 8.24506 (-1.46436 1.88006)
R^2/D10^2 : 1.15182 (-0.651896 1.36969)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 58.27 using 59 PHA bins.
# Reduced chi-squared = 1.022 for 57 degrees of freedom
# Null hypothesis probability = 4.282377e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.447e-08 5.727e-09
25- 50 2.666e-08 8.320e-09
50-150 7.724e-09 4.717e-09
15-150 4.886e-08 1.646e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 54.8623 (-23.3721 60.6281)
Norm : 6.22958 (-1.90564 2.80509)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 57.20 using 59 PHA bins.
# Reduced chi-squared = 1.003 for 57 degrees of freedom
# Null hypothesis probability = 4.678258e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.541e-08 4.025e-09
25- 50 2.279e-08 6.945e-09
50-150 2.401e-08 1.432e-08
15-150 6.221e-08 1.953e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.21516 (-1.7481 1.88486)
R1^2/D10^2 : 1.76813 (-1.04599 3.02322)
kT2 [keV] : 46.6728 (-31.8801 -46.8902)
R2^2/D10^2 : 1.30896E-03 (-0.00126653 0.0540703)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 53.41 using 59 PHA bins.
# Reduced chi-squared = 0.9711 for 55 degrees of freedom
# Null hypothesis probability = 5.355335e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.557e-08 8.001e-09
25- 50 2.445e-08 1.406e-08
50-150 3.068e-08 1.911e-08
15-150 7.071e-08 3.263e-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: 1.91753 ( -0.110454 0.112915 )
Norm@50keV : 3.04393E-03 ( -0.00021707 0.00021485 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 69.42 using 59 PHA bins.
# Reduced chi-squared = 1.218 for 57 degrees of freedom
# Null hypothesis probability = 1.251763e-01
Photon flux (15-150 keV) in 81.39 sec: 0.440122 ( -0.0273644 0.0273896 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.27819e-06 ( -1.58764e-07 1.60228e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.07969 ( -0.61274 0.527122 )
Epeak [keV] : 46.6898 ( -6.95136 13.0836 )
Norm@50keV : 9.07852E-03 ( -0.00446548 0.0111514 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 61.50 using 59 PHA bins.
# Reduced chi-squared = 1.098 for 56 degrees of freedom
# Null hypothesis probability = 2.857965e-01
Photon flux (15-150 keV) in 81.39 sec: 0.423993 ( -0.029099 0.029071 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.09306e-06 ( -1.87189e-07 1.93269e-07 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.279339 ( -0.852154 4.17082 )
beta : -2.35104 ( -0.69108 0.328279 )
Epeak [keV] : 38.2364 ( -11.5095 10.5574 )
Norm@50keV : 3.06085E-02 ( -0.0321581 33.1142 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 57.83 using 59 PHA bins.
# Reduced chi-squared = 1.052 for 55 degrees of freedom
# Null hypothesis probability = 3.710673e-01
Photon flux (15-150 keV) in 81.39 sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 2.13912e-06 ( -2.13855e-06 -1.7647e-07 ) ergs/cm2
S(25-50 keV) vs. S(50-100 keV) plot
S(25-50 keV) = 7.51e-07
S(50-100 keV) = 7.22e-07
T90 vs. Hardness ratio plot
T90 = 87.4439999461174 sec.
Hardness ratio (energy fluence ratio) = 0.961385
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.19187
Count Ratio (50-100 keV) / (15-25 keV) = 0.469531
Mask shadow pattern
IMX = -5.635977089525922E-01, IMY = -3.473171845361346E-01
TIME vs. PHA plot around the trigger time
TIME vs. DetID plot around the trigger time
100 us light curve (15-350 keV)
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:
-361.323400 -345.494000
-239.624000 -4.516000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
89.3449 -41.5212 3.5 50.2 37.1 3.5575 3.3 ------ UNKNOWN
52.8517 -55.2038 3.3 23.8 50.3 0.8726 3.6 ------ UNKNOWN
302.7552 -33.6303 2.5 56.7 179.1 5.9724 4.7 ------ UNKNOWN
49.9936 -23.8887 2.2 34.2 -14.5 1.2248 5.1 ------ UNKNOWN
26.8857 -33.0217 3.0 14.9 -43.4 0.8079 3.8 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-4.516000 76.876600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
53.4129 -62.3261 2.1 25.9 66.5 0.8459 5.4 ------ UNKNOWN
324.9880 -61.4612 0.5 33.5 148.4 4.1718 23.7 ------ UNKNOWN
64.7397 -9.6743 2.8 54.1 -12.0 1.3212 4.1 ------ UNKNOWN
348.3716 -25.2190 2.3 31.3 -133.4 0.6833 4.9 ------ UNKNOWN
330.2965 -11.7879 2.5 52.6 -140.1 2.2841 4.7 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
130.076590 962.483800
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
255.9843 -37.8428 56.3 47.6 140.4 -0.4969 -0.2 0.1 4U 1700-377
256.5747 -36.4194 8.4 48.5 142.0 3.3804 1.4 6.7 GX 349+2
264.8665 -44.3246 9.8 38.4 141.9 1.4224 1.2 9.2 4U 1735-44
270.3241 -24.9245 38.5 51.6 163.1 0.6765 0.3 9.5 GX 5-1
270.1979 -25.8508 9.6 50.9 162.4 2.5057 1.2 8.6 GRS 1758-258
275.9629 -30.4594 6.6 44.3 165.2 2.4525 1.7 5.9 H1820-303
284.8636 -24.8274 0.0 45.6 178.8 2.8108 2.6 10.9 HT1900.1-2455
263.0350 -33.8221 153.3 47.5 149.8 -0.1551 -0.1 2.4 GX 354-0
266.5057 -46.2752 3.0 36.2 141.1 4.0561 3.9 ------ UNKNOWN
282.4383 -23.9208 3.6 47.3 176.6 3.8309 3.2 ------ UNKNOWN
14.8352 -48.7031 2.7 30.3 -37.9 2.6261 4.3 ------ UNKNOWN
301.6589 -12.3524 2.9 52.0 -155.6 6.4610 4.0 ------ UNKNOWN
9.2449 -28.7310 3.2 43.8 -64.0 12.6770 3.7 ------ UNKNOWN
322.7828 -13.5236 2.6 48.0 -129.1 12.1028 4.5 ------ UNKNOWN
Plot creation:
Mon Jun 8 13:42:46 EDT 2015