Click here for the BAT GCN circular template
Image
Pre-slew 15-350 keV image (Event data; bkg subtracted)
# RAcent DECcent POSerr Theta Phi Peak Cts SNR Name
318.2917 +62.4874 0.0626 23.4 -13.6 0.2767 3.1 TRIG_00356516
------------------------------------------
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) 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)
Flight mask-tagged light curves
Caution: Mask-weight map is always using the same on-axis map
Quad-rate summed light curves (from T0-300 to T0+1000)
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: 2.40252 ( -0.548539 0.6951 )
Norm@50keV : 2.32145E-04 ( -0.000232533 0.000128064 )
------------------------------------------------------------
# Chi-Squared = 81.30 using 59 PHA bins.
# Reduced chi-squared = 1.426 for 57 degrees of freedom
# Null hypothesis probability = 1.897067e-02
Photon flux (15-150 keV) in 64 sec: 4.30396E-02 ( -0.0150656 0.0151708 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.45448e-07 ( -5.99044e-08 6.84506e-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: -1.43755 ( 1.48094 2.81563 )
Epeak [keV] : 30.3521 ( -11.5085 10.1661 )
Norm@50keV : 7.80469E-02 ( -0.0933034 17.5282 )
------------------------------------------------------------
# Chi-Squared = 75.33 using 59 PHA bins.
# Reduced chi-squared = 1.345 for 56 degrees of freedom
# Null hypothesis probability = 4.344585e-02
Photon flux (15-150 keV) in 64 sec: 4.50638E-02 ( -0.0140374 0.014214 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.33004e-07 ( -4.64621e-08 5.28384e-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 : 1.37083 ( -2.74779 -1.37083 )
beta : -9.37167 ( 10 19.9993 )
Epeak [keV] : 30.5834 ( -11.7931 10.0016 )
Norm@50keV : 6.98668E-02 ( -0.069016 47.5261 )
------------------------------------------------------------
# Chi-Squared = 75.35 using 59 PHA bins.
# Reduced chi-squared = 1.370 for 55 degrees of freedom
# Null hypothesis probability = 3.559696e-02
Photon flux (15-150 keV) in 64 sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 0 ( 0 0 ) ergs/cm2
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: 2.40261 ( -0.541663 0.691051 )
Norm@50keV : 2.33583E-04 ( -0.000233738 0.000127519 )
------------------------------------------------------------
# Chi-Squared = 81.84 using 59 PHA bins.
# Reduced chi-squared = 1.436 for 57 degrees of freedom
# Null hypothesis probability = 1.719064e-02
Photon flux (15-150 keV) in 64 sec: 4.32946E-02 ( -0.0149422 0.0150627 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.46131e-07 ( -5.9572e-08 6.81466e-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: -1.46835 ( 1.50679 2.82543 )
Epeak [keV] : 30.2563 ( -11.3199 9.9976 )
Norm@50keV : 8.32847E-02 ( -0.0976733 17.9479 )
------------------------------------------------------------
# Chi-Squared = 75.79 using 59 PHA bins.
# Reduced chi-squared = 1.353 for 56 degrees of freedom
# Null hypothesis probability = 4.023629e-02
Photon flux (15-150 keV) in 64 sec: 4.53265E-02 ( -0.0139393 0.0140944 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.33004e-07 ( -4.64621e-08 5.28384e-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 : 1.51533 ( -2.50865 -1.34318 )
beta : -9.99980 ( 15771.9 15781.9 )
Epeak [keV] : 29.8319 ( -10.9799 10.3633 )
Norm@50keV : 9.40510E-02 ( -0.115352 11.0278 )
------------------------------------------------------------
# Chi-Squared = 75.80 using 59 PHA bins.
# Reduced chi-squared = 1.378 for 55 degrees of freedom
# Null hypothesis probability = 3.299314e-02
Photon flux (15-150 keV) in 64 sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 0 ( 0 0 ) ergs/cm2
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: 2.40252 ( -0.548539 0.6951 )
Norm@50keV : 2.32145E-04 ( -0.000232533 0.000128064 )
------------------------------------------------------------
# Chi-Squared = 81.30 using 59 PHA bins.
# Reduced chi-squared = 1.426 for 57 degrees of freedom
# Null hypothesis probability = 1.897067e-02
Photon flux (15-150 keV) in 64 sec: 4.30396E-02 ( -0.0150656 0.0151708 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.45448e-07 ( -5.99044e-08 6.84506e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -1.43755 ( 1.48094 2.81563 )
Epeak [keV] : 30.3521 ( -11.5085 10.1661 )
Norm@50keV : 7.80469E-02 ( -0.0933034 17.5282 )
------------------------------------------------------------
# Chi-Squared = 75.33 using 59 PHA bins.
# Reduced chi-squared = 1.345 for 56 degrees of freedom
# Null hypothesis probability = 4.344585e-02
Photon flux (15-150 keV) in 64 sec: 4.50638E-02 ( -0.0140374 0.014214 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.33004e-07 ( -4.64621e-08 5.28384e-08 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 1.37083 ( -2.74779 -1.37083 )
beta : -9.37167 ( 10 19.9993 )
Epeak [keV] : 30.5834 ( -11.7931 10.0016 )
Norm@50keV : 6.98668E-02 ( -0.069016 47.5261 )
------------------------------------------------------------
# Chi-Squared = 75.35 using 59 PHA bins.
# Reduced chi-squared = 1.370 for 55 degrees of freedom
# Null hypothesis probability = 3.559696e-02
Photon flux (15-150 keV) in 64 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) = 4.79267e-08
S(50-100 keV) = 3.6561e-08
T90 vs. Hardness ratio plot
T90 = 64 sec.
Hardness ratio (energy fluence ratio) = 0.762852
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 0.71506
Count Ratio (50-100 keV) / (15-25 keV) = -0.0678019
Mask shadow pattern
IMX = 0, IMY = 0
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] [']
254.6547 35.2525 8.8 28.5 118.7 0.1764 1.3 11.1 Her X-1
299.5992 35.1867 0.7 34.6 46.2 2.6053 16.5 1.0 Cyg X-1
308.0305 40.8338 7.0 33.1 30.8 0.1976 1.7 8.0 Cyg X-3
326.0968 38.2265 18.3 43.2 14.7 0.1008 0.6 6.7 Cyg X-2
254.9526 37.5865 2.1 26.2 119.1 0.5795 5.4 ------ UNKNOWN
288.0414 58.2206 2.4 11.8 22.4 0.3940 4.8 ------ UNKNOWN
207.1909 47.1407 2.3 35.6 -168.9 0.4965 5.0 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
338.700590 688.520000
690.000000 963.045800
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.4652 35.4650 5.1 47.2 145.3 3.9576 2.3 7.4 Her X-1
299.5902 35.1935 0.3 29.8 91.3 25.3944 34.2 0.5 Cyg X-1
308.1370 41.0858 5.4 22.4 80.0 1.1304 2.1 8.1 Cyg X-3
326.1275 38.4115 4.8 24.6 44.7 1.1534 2.4 5.8 Cyg X-2
308.0301 37.5212 2.0 25.9 78.4 3.3054 5.8 ------ UNKNOWN
232.7057 50.7229 2.8 44.9 175.7 3.3657 4.1 ------ UNKNOWN
225.8164 46.1035 2.9 51.3 176.6 4.8831 4.0 ------ UNKNOWN
306.7385 65.9367 2.4 6.1 -172.4 1.8721 4.9 ------ UNKNOWN
Plot creation:
Tue Feb 16 10:12:48 EST 2010