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Image
Pre-slew 15.0-350.0 keV image (Event data)
# RAcent DECcent POSerr Theta Phi Peak Cts SNR Name
134.1643 47.0096 0.0086 33.9982 41.1004 3.6740091 22.637 TRIG_00441676
Foreground time interval of the image:
-30.448 23.504 (delta_t = 53.952 [sec])
Background time interval of the image:
-239.552 -30.448 (delta_t = 209.104 [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 1.024000
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 1.024000
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 1.024000
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 -30.448 sec. to 23.504 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.81923 ( -0.121751 0.12416 )
Norm@50keV : 4.12901E-03 ( -0.00030681 0.000303348 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 36.48 using 59 PHA bins.
# Reduced chi-squared = 0.6399 for 57 degrees of freedom
# Null hypothesis probability = 9.843703e-01
Photon flux (15-150 keV) in 53.95 sec: 0.573265 ( -0.0385872 0.0386316 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.04951e-06 ( -1.53863e-07 1.5522e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -30.448 sec. to 23.504 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.67389 ( -0.494908 0.458669 )
Epeak [keV] : 101.992 ( )
Norm@50keV : 4.95494E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 36.18 using 59 PHA bins.
# Reduced chi-squared = 0.6460 for 56 degrees of freedom
# Null hypothesis probability = 9.816938e-01
Photon flux (15-150 keV) in 53.95 sec: 0.569192 ( -0.040496 0.040019 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.02105e-06 ( -1.79287e-07 1.75186e-07 ) ergs/cm2
Band function
Time interval is from -30.448 sec. to 23.504 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 4.90832 ( -4.90832 -4.90832 )
beta : -1.87816 ( -0.164485 0.134747 )
Epeak [keV] : 21.4529 ( -21.4529 3.80718 )
Norm@50keV : 1292.24 ( -84.7912 3.37044e+06 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 34.53 using 59 PHA bins.
# Reduced chi-squared = 0.6278 for 55 degrees of freedom
# Null hypothesis probability = 9.860904e-01
Photon flux (15-150 keV) in 53.95 sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 2.00671e-06 ( -2.00634e-06 -1.66889e-07 ) ergs/cm2
Single BB
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 11.2551 (-0.962491 1.07518)
R^2/D10^2 : 0.168514 (-0.0489362 0.0678616)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 94.57 using 59 PHA bins.
# Reduced chi-squared = 1.659 for 57 degrees of freedom
# Null hypothesis probability = 1.301034e-03
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.416e-07 2.986e-08
25- 50 7.035e-07 5.719e-08
50-150 5.122e-07 8.395e-08
15-150 1.457e-06 1.122e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 99.1095 (-22.3852 34.7628)
Norm : 2.51725 (-0.239122 0.276448)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 37.72 using 59 PHA bins.
# Reduced chi-squared = 0.6618 for 57 degrees of freedom
# Null hypothesis probability = 9.771292e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.549e-07 4.262e-08
25- 50 6.127e-07 4.478e-08
50-150 9.878e-07 3.143e-07
15-150 1.955e-06 3.377e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.93160 (-1.12243 1.17499)
R1^2/D10^2 : 0.788500 (-0.328063 0.678824)
kT2 [keV] : 27.4850 (-6.57231 13.2404)
R2^2/D10^2 : 4.52483E-03 (-0.00324913 0.0079081)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 34.75 using 59 PHA bins.
# Reduced chi-squared = 0.6317 for 55 degrees of freedom
# Null hypothesis probability = 9.850580e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.554e-07 6.881e-08
25- 50 6.171e-07 1.033e-07
50-150 1.061e-06 5.256e-07
15-150 2.034e-06 6.150e-07
Peak spectrum fit
Power-law model
Time interval is from 4.884 sec. to 5.884 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.54452 ( -0.224066 0.229837 )
Norm@50keV : 1.62806E-02 ( -0.00228795 0.00226987 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 43.06 using 59 PHA bins.
# Reduced chi-squared = 0.7554 for 57 degrees of freedom
# Null hypothesis probability = 9.141939e-01
Photon flux (15-150 keV) in 1 sec: 2.05777 ( -0.283768 0.284295 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.53388e-07 ( -2.31108e-08 2.3367e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 4.884 sec. to 5.884 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.515736 ( -1.30697 1.01959 )
Epeak [keV] : 72.9581 ( -18.1849 593.213 )
Norm@50keV : 5.31937E-02 ( -0.0531939 0.175117 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 40.12 using 59 PHA bins.
# Reduced chi-squared = 0.7164 for 56 degrees of freedom
# Null hypothesis probability = 9.460144e-01
Photon flux (15-150 keV) in 1 sec: 1.97664 ( -0.298 0.29684 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.44751e-07 ( -2.4447e-08 2.5038e-08 ) ergs/cm2
Band function
Time interval is from 4.884 sec. to 5.884 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.663766 ( -0.628066 2.40445 )
beta : -2.96808 ( 2.89578 12.7804 )
Epeak [keV] : 77.1770 ( -25.071 481.935 )
Norm@50keV : 4.47678E-02 ( -0.0326159 0.0960821 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 40.17 using 59 PHA bins.
# Reduced chi-squared = 0.7303 for 55 degrees of freedom
# Null hypothesis probability = 9.333142e-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] : 15.0578 (-2.12226 2.48693)
R^2/D10^2 : 0.238290 (-0.100364 0.169498)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 45.55 using 59 PHA bins.
# Reduced chi-squared = 0.7992 for 57 degrees of freedom
# Null hypothesis probability = 8.621839e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.130e-08 3.063e-09
25- 50 4.508e-08 8.280e-09
50-150 6.968e-08 1.835e-08
15-150 1.261e-07 2.318e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 198.753 (-93.6125 -198.705)
Norm : 8.44815 (-1.13806 1.32437)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 41.51 using 59 PHA bins.
# Reduced chi-squared = 0.7283 for 57 degrees of freedom
# Null hypothesis probability = 9.386503e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.105e-08 1.194e-08
25- 50 4.047e-08 2.248e-08
50-150 8.866e-08 4.827e-08
15-150 1.502e-07 8.200e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 2.42699 (-1.48142 5.95953)
R1^2/D10^2 : 218.364 (-218.826 1.48261e+06)
kT2 [keV] : 16.5548 (-2.58301 5.797)
R2^2/D10^2 : 0.162554 (-0.113916 0.141768)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 38.52 using 59 PHA bins.
# Reduced chi-squared = 0.7004 for 55 degrees of freedom
# Null hypothesis probability = 9.551997e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.877e-08 8.047e-09
25- 50 4.019e-08 1.172e-08
50-150 7.674e-08 2.493e-08
15-150 1.357e-07 3.520e-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: 1.81923 ( -0.121751 0.12416 )
Norm@50keV : 4.12901E-03 ( -0.00030681 0.000303348 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 36.48 using 59 PHA bins.
# Reduced chi-squared = 0.6399 for 57 degrees of freedom
# Null hypothesis probability = 9.843703e-01
Photon flux (15-150 keV) in 53.95 sec: 0.573265 ( -0.0385872 0.0386316 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.04951e-06 ( -1.53863e-07 1.5522e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.67389 ( -0.494908 0.458669 )
Epeak [keV] : 101.992 ( )
Norm@50keV : 4.95494E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 36.18 using 59 PHA bins.
# Reduced chi-squared = 0.6460 for 56 degrees of freedom
# Null hypothesis probability = 9.816938e-01
Photon flux (15-150 keV) in 53.95 sec: 0.569192 ( -0.040496 0.040019 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.02105e-06 ( -1.79287e-07 1.75186e-07 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 4.90832 ( -4.90832 -4.90832 )
beta : -1.87816 ( -0.164485 0.134747 )
Epeak [keV] : 21.4529 ( -21.4529 3.80718 )
Norm@50keV : 1292.24 ( -84.7912 3.36807e+06 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 34.53 using 59 PHA bins.
# Reduced chi-squared = 0.6278 for 55 degrees of freedom
# Null hypothesis probability = 9.860904e-01
Photon flux (15-150 keV) in 53.95 sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 2.00671e-06 ( -2.00634e-06 -1.66889e-07 ) ergs/cm2
S(25-50 keV) vs. S(50-100 keV) plot
S(25-50 keV) = 5.81e-07
S(50-100 keV) = 6.59e-07
T90 vs. Hardness ratio plot
T90 = 43.4240000247955 sec.
Hardness ratio (energy fluence ratio) = 1.13425
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.122
Count Ratio (50-100 keV) / (15-25 keV) = 0.670305
Mask shadow pattern
IMX = 5.082475128329527E-01, IMY = -4.433787700491502E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.024000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.024000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.024000
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:
-239.552000 -30.448000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6171 22.0250 1.3 42.3 121.5 7.3969 8.8 1.1 Crab
175.9834 57.2168 3.0 43.2 -0.6 1.1909 3.8 ------ UNKNOWN
1.7665 64.9856 3.0 31.2 -105.3 1.1238 3.9 ------ UNKNOWN
14.9817 33.0182 2.3 49.5 -149.2 2.2151 4.9 ------ UNKNOWN
5.4808 55.4289 2.7 35.9 -120.8 1.4283 4.2 ------ UNKNOWN
297.4949 74.5261 2.5 39.1 -67.6 2.3857 4.6 ------ UNKNOWN
260.3759 68.8553 3.3 47.0 -53.0 3.1610 3.5 ------ UNKNOWN
334.2954 63.6296 2.3 40.8 -93.4 4.3307 5.1 ------ UNKNOWN
353.2903 50.7439 2.2 44.2 -117.2 4.1705 5.3 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-30.448000 23.504000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.8526 21.9739 7.2 42.3 121.2 -0.6408 -1.6 12.4 Crab
134.1641 47.0094 0.5 34.0 41.1 3.6728 22.6 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
310.548600 962.535200
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
65.1235 38.1312 2.4 50.0 146.3 10.5450 4.9 ------ UNKNOWN
146.7446 -4.0500 2.6 52.2 24.0 8.2959 4.4 ------ UNKNOWN
180.4881 2.8160 3.2 59.6 -17.0 10.4237 3.6 ------ UNKNOWN
0.7692 70.3030 5.1 58.0 -156.9 6.4668 2.3 ------ UNKNOWN
193.3434 31.5342 4.2 47.1 -53.0 6.7308 2.7 ------ UNKNOWN
191.6284 21.9902 3.8 52.1 -42.1 8.2307 3.1 ------ UNKNOWN
Plot creation:
Sat May 30 23:12:04 EDT 2015