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Image
Pre-slew 15-350 keV image (Event data; bkg subtracted)
# RAcent DECcent POSerr Theta Phi Peak Cts SNR Name
170.2106 -61.8890 0.0272 25.9 -53.1 1.0047 7.0 TRIG_00340973
------------------------------------------
Foreground time interval of the image:
-7.899 117.772 (delta_t = 125.671 [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
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 64.000000
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 64.000000
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 64.000000
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 -40.496 sec. to 117.772 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.69609 ( -0.34861 0.402415 )
Norm@50keV : 3.44148E-04 ( -0.000107101 0.000112328 )
------------------------------------------------------------
# Chi-Squared = 54.08 using 59 PHA bins.
# Reduced chi-squared = 0.9487 for 57 degrees of freedom
# Null hypothesis probability = 5.854688e-01
Photon flux (15-150 keV) in 158.3 sec: 7.67358E-02 ( -0.0130513 0.013081 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.79547e-07 ( -1.23614e-07 1.3303e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -40.496 sec. to 117.772 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -2.61603 ( 1.52528 2.29833 )
Epeak [keV] : 25.6767 ( -5.44666 4.23866 )
Norm@50keV : 1.71845 ( )
------------------------------------------------------------
# Chi-Squared = 44.20 using 59 PHA bins.
# Reduced chi-squared = 0.7893 for 56 degrees of freedom
# Null hypothesis probability = 8.729393e-01
Photon flux (15-150 keV) in 158.3 sec: 7.44009E-02 ( -0.0121756 0.0124421 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.87007e-07 ( -8.57685e-08 9.40476e-08 ) ergs/cm2
Band function
Time interval is from -40.496 sec. to 117.772 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 2.66296 ( -17.2955 -7.44587 )
beta : -8.98988 ( 9.99999 19.9885 )
Epeak [keV] : 25.8504 ( -2.94598 3.06957 )
Norm@50keV : 1.80330 ( -1.80345 50.2776 )
------------------------------------------------------------
# Chi-Squared = 44.21 using 59 PHA bins.
# Reduced chi-squared = 0.8038 for 55 degrees of freedom
# Null hypothesis probability = 8.508663e-01
Photon flux (15-150 keV) in 158.3 sec: 7.310624E-02 ( -0.0117065 0.0117082 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.81286e-07 ( -8.07045e-08 1.00378e-07 ) ergs/cm2
Peak spectrum fit
Power-law model
Time interval is from -35.588 sec. to -34.588 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.17415 ( -1.60043 1.24219 )
Norm@50keV : 3.33373E-03 ( -0.002111 0.00183304 )
------------------------------------------------------------
# Chi-Squared = 55.88 using 59 PHA bins.
# Reduced chi-squared = 0.9803 for 57 degrees of freedom
# Null hypothesis probability = 5.172885e-01
Photon flux (15-150 keV) in 1 sec: 0.380292 ( -0.205581 0.226012 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.40749e-08 ( -2.03627e-08 2.11555e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -35.588 sec. to -34.588 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.20908 ( -1.6554 2.35996 )
Epeak [keV] : 9999.36 ( -9999.95 -9999.95 )
Norm@50keV : 3.35163E-03 ( -0.00335152 0.116746 )
------------------------------------------------------------
# Chi-Squared = 55.88 using 59 PHA bins.
# Reduced chi-squared = 0.9979 for 56 degrees of freedom
# Null hypothesis probability = 4.793003e-01
Photon flux (15-150 keV) in 1 sec: 0.389744 ( -0.389744 0.227789 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.40761e-08 ( -2.03707e-08 2.11692e-08 ) ergs/cm2
Band function
Time interval is from -35.588 sec. to -34.588 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 4.99133 ( -222.191 -222.191 )
beta : -1.16131 ( -1.87649 1.56733 )
Epeak [keV] : 21.7132 ( -21.6578 88.8732 )
Norm@50keV : 582.117 ( -606.389 29611.1 )
------------------------------------------------------------
# Chi-Squared = 55.82 using 59 PHA bins.
# Reduced chi-squared = 1.015 for 55 degrees of freedom
# Null hypothesis probability = 4.439535e-01
Photon flux (15-150 keV) in 1 sec: 0.390103 ( -0.390103 0.228852 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.05496e-07 ( -1.05496e-07 6.72949e-06 ) 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: 2.57281 ( -0.356628 0.411101 )
Norm@50keV : 3.75251E-04 ( -0.00011707 0.000120879 )
------------------------------------------------------------
# Chi-Squared = 59.89 using 59 PHA bins.
# Reduced chi-squared = 1.051 for 57 degrees of freedom
# Null hypothesis probability = 3.713186e-01
Photon flux (15-150 keV) in 125.7 sec: 7.71403E-02 ( -0.0138222 0.0138515 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.81567e-07 ( -1.08437e-07 1.16733e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -2.48543 ( 1.39724 2.47197 )
Epeak [keV] : 26.1197 ( -4.98511 4.54759 )
Norm@50keV : 1.26564 ( )
------------------------------------------------------------
# Chi-Squared = 52.25 using 59 PHA bins.
# Reduced chi-squared = 0.9331 for 56 degrees of freedom
# Null hypothesis probability = 6.174729e-01
Photon flux (15-150 keV) in 125.7 sec: 7.39709E-02 ( -0.0128652 0.0131954 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.89551e-07 ( -7.36665e-08 8.47381e-08 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 2.12324 ( -1.54054 -0.803825 )
beta : -9.99812 ( 1689.23 1698.89 )
Epeak [keV] : 25.9303 ( -7.44429 4.73761 )
Norm@50keV : 0.705485 ( -0.643183 31.4104 )
------------------------------------------------------------
# Chi-Squared = 52.21 using 59 PHA bins.
# Reduced chi-squared = 0.9493 for 55 degrees of freedom
# Null hypothesis probability = 5.818576e-01
Photon flux (15-150 keV) in 125.7 sec: 7.616794E-02 ( -0.0132211 0.0132215 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.28193e-07 ( -7.83802e-08 1.08084e-07 ) ergs/cm2
S(25-50 keV) vs. S(50-100 keV) plot
S(25-50 keV) = 1.94641e-07
S(50-100 keV) = 1.20063e-07
T90 vs. Hardness ratio plot
T90 = 152.247999995947 sec.
Hardness ratio (energy fluence ratio) = 0.616843
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 0.885107
Count Ratio (50-100 keV) / (15-25 keV) = -0.00972835
Mask shadow pattern
IMX = 2.915985051109055E-01, IMY = 3.888831795692195E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 64.000000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 64.000000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 64.000000
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:
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-7.899410 117.772000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.5106 -40.5139 1.9 28.3 15.5 0.8734 6.2 2.6 Vela X-1
170.2405 -60.6277 3.6 24.7 -53.1 0.4333 3.2 2.2 Cen X-3
186.6693 -62.7652 0.6 28.4 -69.1 3.3049 18.8 0.5 GX 301-2
142.2248 -37.2154 2.8 23.3 23.9 0.5107 4.2 ------ UNKNOWN
200.2710 -35.0680 2.3 23.5 -138.0 0.6742 5.1 ------ UNKNOWN
170.2104 -61.8889 1.6 25.9 -53.1 1.0047 7.1 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
355.400620 573.780000
575.000000 963.042900
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
170.2024 -60.4948 4.5 35.2 47.5 2.0063 2.6 8.4 Cen X-3
186.6508 -62.7655 0.4 27.1 46.7 15.4641 29.3 0.3 GX 301-2
244.9674 -15.6394 0.4 39.1 -173.5 17.0783 31.7 0.7 Sco X-1
255.9393 -37.8723 2.1 20.6 -140.1 2.4151 5.4 2.8 4U 1700-377
256.2655 -36.3391 3.7 22.1 -141.6 1.3879 3.1 9.6 GX 349+2
262.9884 -24.6794 2.6 35.1 -142.1 2.3505 4.4 4.1 GX 1+4
264.7458 -44.4413 70.6 20.0 -113.0 -0.0665 -0.2 0.5 4U 1735-44
270.3296 -25.1215 3.8 37.8 -131.9 2.5336 3.0 3.5 GX 5-1
270.2097 -25.8952 0.0 37.1 -131.4 -0.3678 -0.5 10.4 GRS 1758-258
274.0036 -13.9090 5.3 49.3 -135.4 4.6368 2.2 7.6 GX 17+2
276.0177 -30.3946 3.9 36.3 -120.1 2.1245 3.0 5.1 H1820-303
101.1566 -69.1632 2.9 52.5 13.4 6.0901 3.9 ------ UNKNOWN
243.4319 -11.6035 2.6 42.9 -176.4 2.8134 4.4 ------ UNKNOWN
269.6460 -35.9587 4.6 28.6 -121.3 1.2271 2.5 ------ UNKNOWN
327.4190 -56.6951 3.3 47.1 -53.1 8.0591 3.5 ------ UNKNOWN
Plot creation:
Tue Feb 16 23:52:38 EST 2010