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Image
Pre-slew 15-350 keV image (Event data; bkg subtracted)
# RAcent DECcent POSerr Theta Phi Peak Cts SNR Name
188.7783 +12.6401 0.0392 12.9 -121.4 0.3848 4.9 TRIG_00648422
------------------------------------------
Foreground time interval of the image:
0.000 64.000 (delta_t = 64.000 [sec])
Background time interval of the image:
Lightcurves
Notes:
- 1) All plots contain as much data as has been downloaded to date.
- 2) The mask-weighted light curves are using the flight position.
- 3) Multiple plots of different time binning/intervals are shown to cover all scenarios of short/long GRBs, rate/image triggers, and real/false positives.
- 4) 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.
- 5) 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.
- 6) 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)
Spectra
Notes:
- 1) The fitting includes the systematic errors.
- 2) For long bursts, a spectral fit of 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.
- 4) For short bursts (T90<1sec), the specrtum is also fit with Blackbody, OTTB, and Double Blackbody.
Time averaged spectrum fit using the pre-slew DRM
Power-law model
Time interval is from 0.000 sec. to 64.000 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.00096 ( -0.652913 0.809682 )
Norm@50keV : 2.26335E-04 ( -0.000124419 0.00012478 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 40.49 using 59 PHA bins.
# Reduced chi-squared = 0.7104 for 57 degrees of freedom
# Null hypothesis probability = 9.518517e-01
Photon flux (15-150 keV) in 64 sec: 3.39487E-02 ( -0.0144146 0.0145429 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.32836e-07 ( -6.59878e-08 7.48832e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.000 sec. to 64.000 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -5.56685 ( )
Epeak [keV] : 32.2489 ( -6.72848 21.7065 )
Norm@50keV : 23.0188 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 36.48 using 59 PHA bins.
# Reduced chi-squared = 0.6514 for 56 degrees of freedom
# Null hypothesis probability = 9.798990e-01
Photon flux (15-150 keV) in 64 sec: 3.25505E-02 ( -0.0129075 0.0138081 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.98637e-08 ( -4.27866e-08 6.37133e-08 ) ergs/cm2
Band function
Time interval is from 0.000 sec. to 64.000 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 4.89593 ( -7.06661 -4.89593 )
beta : -4.22165 ( 4.22165 2.15445 )
Epeak [keV] : 31.9245 ( -10.0017 9.59078 )
Norm@50keV : 8.98282 ( -3.3717 95.7594 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 36.28 using 59 PHA bins.
# Reduced chi-squared = 0.6596 for 55 degrees of freedom
# Null hypothesis probability = 9.758738e-01
Photon flux (15-150 keV) in 64 sec: 3.34267E-02 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 1.09231e-07 ( 0 0 ) ergs/cm2
Single BB
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 8.94363 (-2.66076 4.03267)
R^2/D10^2 : 2.84106E-02 (-0.0284106 0.0793784)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 36.87 using 59 PHA bins.
# Reduced chi-squared = 0.6468 for 57 degrees of freedom
# Null hypothesis probability = 9.823334e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.822e-08 1.748e-08
25- 50 5.940e-08 3.699e-08
50-150 2.223e-08 1.837e-08
15-150 1.099e-07 7.350e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 52.4354 (-30.0587 -51.1949)
Norm : 0.196665 (-0.0942849 0.180458)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 39.04 using 59 PHA bins.
# Reduced chi-squared = 0.6848 for 57 degrees of freedom
# Null hypothesis probability = 9.668874e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.110e-08 1.983e-08
25- 50 4.541e-08 2.886e-08
50-150 4.608e-08 3.878e-08
15-150 1.226e-07 8.320e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 8.48179 (-8.55436 -8.55436)
R1^2/D10^2 : 3.28766E-03 (-0.0037788 -0.0037788)
kT2 [keV] : 9.11331 (-9.00839 188.364)
R2^2/D10^2 : 2.40144E-02 (-0.0243069 -0.0243069)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 36.87 using 59 PHA bins.
# Reduced chi-squared = 0.6703 for 55 degrees of freedom
# Null hypothesis probability = 9.713409e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.786e-08 1.250e-03
25- 50 5.971e-08 1.142e-02
50-150 2.323e-08 2.590e-01
15-150 1.108e-07 3.000e-01
Peak spectrum fit
Power-law model
Time interval is from 0.000 sec. to 64.000 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.00096 ( -0.652913 0.809682 )
Norm@50keV : 2.26335E-04 ( -0.000124419 0.00012478 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 40.49 using 59 PHA bins.
# Reduced chi-squared = 0.7104 for 57 degrees of freedom
# Null hypothesis probability = 9.518517e-01
Photon flux (15-150 keV) in 64 sec: 3.39487E-02 ( -0.0144146 0.0145429 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.32836e-07 ( -6.59878e-08 7.48832e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.000 sec. to 64.000 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -5.56685 ( )
Epeak [keV] : 32.2489 ( -6.72848 21.7065 )
Norm@50keV : 23.0188 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 36.48 using 59 PHA bins.
# Reduced chi-squared = 0.6514 for 56 degrees of freedom
# Null hypothesis probability = 9.798990e-01
Photon flux (15-150 keV) in 64 sec: 3.25505E-02 ( -0.0129075 0.0138081 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.98637e-08 ( -4.27866e-08 6.36358e-08 ) ergs/cm2
Band function
Time interval is from 0.000 sec. to 64.000 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 4.89593 ( -7.06661 -4.89593 )
beta : -4.22165 ( 4.22165 2.15445 )
Epeak [keV] : 31.9245 ( -10.0017 9.59078 )
Norm@50keV : 8.98282 ( -3.3717 95.7594 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 36.28 using 59 PHA bins.
# Reduced chi-squared = 0.6596 for 55 degrees of freedom
# Null hypothesis probability = 9.758738e-01
Photon flux (15-150 keV) in 64 sec: 3.34267E-02 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 1.09231e-07 ( 0 0 ) ergs/cm2
Single BB
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 8.94363 (-2.66076 4.03267)
R^2/D10^2 : 2.84106E-02 (-0.0284106 0.0793784)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 36.87 using 59 PHA bins.
# Reduced chi-squared = 0.6468 for 57 degrees of freedom
# Null hypothesis probability = 9.823334e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.822e-08 1.759e-08
25- 50 5.940e-08 3.808e-08
50-150 2.223e-08 1.821e-08
15-150 1.099e-07 7.510e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 52.4354 (-30.0587 -51.1949)
Norm : 0.196665 (-0.0942849 0.180458)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 39.04 using 59 PHA bins.
# Reduced chi-squared = 0.6848 for 57 degrees of freedom
# Null hypothesis probability = 9.668874e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.110e-08 2.020e-08
25- 50 4.541e-08 2.820e-08
50-150 4.608e-08 3.818e-08
15-150 1.226e-07 8.438e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 8.48179 (-8.55436 -8.55436)
R1^2/D10^2 : 3.28766E-03 (-0.0037788 -0.0037788)
kT2 [keV] : 9.11331 (-9.00839 188.364)
R2^2/D10^2 : 2.40144E-02 (-0.0243069 -0.0243069)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 36.87 using 59 PHA bins.
# Reduced chi-squared = 0.6703 for 55 degrees of freedom
# Null hypothesis probability = 9.713409e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.786e-08 1.348e-03
25- 50 5.971e-08 1.038e-02
50-150 2.323e-08 2.625e-01
15-150 1.108e-07 2.778e-01
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: 2.00096 ( -0.652913 0.809682 )
Norm@50keV : 2.26335E-04 ( -0.000124419 0.00012478 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 40.49 using 59 PHA bins.
# Reduced chi-squared = 0.7104 for 57 degrees of freedom
# Null hypothesis probability = 9.518517e-01
Photon flux (15-150 keV) in 64 sec: 3.39487E-02 ( -0.0144146 0.0145429 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.32836e-07 ( -6.59878e-08 7.48832e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -5.56685 ( )
Epeak [keV] : 32.2489 ( -6.72848 21.7065 )
Norm@50keV : 23.0188 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 36.48 using 59 PHA bins.
# Reduced chi-squared = 0.6514 for 56 degrees of freedom
# Null hypothesis probability = 9.798990e-01
Photon flux (15-150 keV) in 64 sec: 3.25505E-02 ( -0.0129075 0.0138081 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.98637e-08 ( -4.27866e-08 6.37139e-08 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 4.89593 ( -7.06661 -4.89593 )
beta : -4.22165 ( 4.22165 2.15445 )
Epeak [keV] : 31.9245 ( -10.0017 9.59078 )
Norm@50keV : 8.98282 ( -3.3717 95.7594 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 36.28 using 59 PHA bins.
# Reduced chi-squared = 0.6596 for 55 degrees of freedom
# Null hypothesis probability = 9.758738e-01
Photon flux (15-150 keV) in 64 sec: 3.34267E-02 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 1.09231e-07 ( 0 0 ) ergs/cm2
S(25-50 keV) vs. S(50-100 keV) plot
S(25-50 keV) = 4.01e-08
S(50-100 keV) = 3.98e-08
T90 vs. Hardness ratio plot
T90 = 64 sec.
Hardness ratio (energy fluence ratio) = 0.992519
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.30145
Count Ratio (50-100 keV) / (15-25 keV) = 0.344742
Mask shadow pattern
IMX = -1.195951765288605E-01, IMY = 1.957714828374364E-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:
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
0.000000 64.000000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
210.2944 -4.0322 2.2 20.8 133.2 0.4751 5.1 ------ UNKNOWN
183.2834 -35.0075 2.6 53.0 176.6 1.3844 4.5 ------ UNKNOWN
159.0520 20.3407 4.5 41.0 -98.6 0.9968 2.6 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
208.100590 619.460000
621.000000 963.032300
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
186.7418 -62.7125 4.2 39.0 -110.3 4.4796 2.8 4.2 GX 301-2
244.9871 -15.6359 0.3 34.2 8.5 23.9863 34.0 0.5 Sco X-1
255.9796 -37.8703 0.7 10.9 28.3 8.3365 15.9 1.6 4U 1700-377
256.3156 -36.4381 3.6 12.3 29.5 1.6821 3.2 5.9 GX 349+2
262.9931 -24.7100 10.0 24.7 43.0 0.7133 1.1 2.3 GX 1+4
264.9762 -44.4295 12.1 7.7 86.5 0.4823 1.0 10.1 4U 1735-44
270.4486 -25.1479 7.5 26.3 58.4 1.1340 1.5 9.8 GX 5-1
270.3097 -25.6717 2.3 25.8 58.6 3.5559 5.2 4.3 GRS 1758-258
274.0865 -13.9743 4.9 37.9 56.9 3.2206 2.4 6.0 GX 17+2
275.8424 -30.4272 4.4 23.9 74.3 1.6930 2.6 5.6 H1820-303
285.1397 -24.8788 9.1 33.2 81.6 1.5443 1.3 6.2 HT1900.1-2455
262.8861 -33.7994 5.4 15.9 49.4 1.1426 2.2 5.6 GX 354-0
251.9718 3.8166 2.5 52.7 22.3 11.3949 4.6 ------ UNKNOWN
247.7811 -1.1353 2.7 48.1 16.3 5.6352 4.3 ------ UNKNOWN
248.7189 -5.1216 1.8 44.0 17.0 6.0392 6.6 ------ UNKNOWN
4.9359 -64.6426 4.0 54.1 177.0 7.4789 2.9 ------ UNKNOWN
248.0972 -67.4078 2.6 19.1 -144.2 2.3583 4.4 ------ UNKNOWN
30.4862 -69.3409 4.2 57.4 -170.4 8.1652 2.8 ------ UNKNOWN
209.5053 -64.7364 1.3 29.0 -113.7 7.2560 8.6 ------ UNKNOWN
107.6098 -83.1168 3.3 47.2 -148.1 4.7211 3.5 ------ UNKNOWN
Plot creation:
Fri Jul 10 16:59:37 EDT 2015