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Image
Pre-slew 15-350 keV image (Event data; bkg subtracted)
# RAcent DECcent POSerr Theta Phi Peak Cts SNR Name
267.1415 -24.9429 0.1053 32.5 164.3 0.5160 1.8 TRIG_00526511
------------------------------------------
Foreground time interval of the image:
0.000 183.015 (delta_t = 183.015 [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 183.015 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.40604 ( -1.29463 2.33524 )
Norm@50keV : 1.25638E-04 ( -0.000125638 0.000123155 )
------------------------------------------------------------
# Chi-Squared = 55.16 using 59 PHA bins.
# Reduced chi-squared = 0.9677 for 57 degrees of freedom
# Null hypothesis probability = 5.445225e-01
Photon flux (15-150 keV) in 183 sec: 2.33287E-02 ( -0.0142163 0.0142335 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.24589e-07 ( -1.5751e-07 1.95444e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.000 sec. to 183.015 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.91139 ( )
Epeak [keV] : 6.42669 ( )
Norm@50keV : 2.58874E-04 ( )
------------------------------------------------------------
# Chi-Squared = 55.18 using 59 PHA bins.
# Reduced chi-squared = 0.9853 for 56 degrees of freedom
# Null hypothesis probability = 5.059463e-01
Photon flux (15-150 keV) in 183 sec: 2.33184E-02 ( -0.0141925 0.0141874 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.66086e-07 ( -2.66086e-07 5.00897e-07 ) ergs/cm2
Band function
Time interval is from 0.000 sec. to 183.015 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 2.20905 ( 1.75004 1.75004 )
beta : -2.53386 ( 2.94383 11.1939 )
Epeak [keV] : 19.0183 ( -12.8767 -12.8767 )
Norm@50keV : 0.776460 ( -0.81248 159.333 )
------------------------------------------------------------
# Chi-Squared = 55.11 using 59 PHA bins.
# Reduced chi-squared = 1.002 for 55 degrees of freedom
# Null hypothesis probability = 4.703437e-01
Photon flux (15-150 keV) in 183 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] : 7.49715 (-7.50877 9.75271)
R^2/D10^2 : 3.26947E-02 (-0.0323999 4.28297)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
# Chi-Squared = 55.77 using 59 PHA bins.
# Reduced chi-squared = 0.9784 for 57 degrees of freedom
# Null hypothesis probability = 5.212976e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.770e-08 4.010e-08
25- 50 8.993e-08 6.570e-08
50-150 1.898e-08 1.972e-08
15-150 1.666e-07 1.180e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 33.6626 (-33.6626 -33.6626)
Norm : 0.169976 (-0.169976 1.57417)
------------------------------------------------------------
# Chi-Squared = 55.23 using 59 PHA bins.
# Reduced chi-squared = 0.9689 for 57 degrees of freedom
# Null hypothesis probability = 5.418967e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.684e-08 4.742e-08
25- 50 8.116e-08 5.826e-08
50-150 5.142e-08 5.059e-08
15-150 1.994e-07 1.434e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 3.40930 (-3.4072 -3.4072)
R1^2/D10^2 : 0.650819 (-0.653175 -0.653175)
kT2 [keV] : 11.2126 (-11.2084 -11.2084)
R2^2/D10^2 : 4.76057E-03 (-0.00476972 1.78542)
------------------------------------------------------------
# Chi-Squared = 55.10 using 59 PHA bins.
# Reduced chi-squared = 1.002 for 55 degrees of freedom
# Null hypothesis probability = 4.709420e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.020e-08 3.492e-08
25- 50 7.708e-08 5.207e-08
50-150 4.799e-08 4.101e-08
15-150 1.953e-07 1.168e-07
Peak spectrum fit
Power-law model
Time interval is from 0.000 sec. to 183.015 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.40604 ( -1.29463 2.33524 )
Norm@50keV : 1.25638E-04 ( -0.000125638 0.000123155 )
------------------------------------------------------------
# Chi-Squared = 55.16 using 59 PHA bins.
# Reduced chi-squared = 0.9677 for 57 degrees of freedom
# Null hypothesis probability = 5.445225e-01
Photon flux (15-150 keV) in 183 sec: 2.33287E-02 ( -0.0142163 0.0142335 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.24589e-07 ( -1.5751e-07 1.95444e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.000 sec. to 183.015 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.91139 ( )
Epeak [keV] : 6.42669 ( )
Norm@50keV : 2.58874E-04 ( )
------------------------------------------------------------
# Chi-Squared = 55.18 using 59 PHA bins.
# Reduced chi-squared = 0.9853 for 56 degrees of freedom
# Null hypothesis probability = 5.059463e-01
Photon flux (15-150 keV) in 183 sec: 2.33184E-02 ( -0.0141925 0.0141874 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.66086e-07 ( -2.66086e-07 4.73884e-07 ) ergs/cm2
Band function
Time interval is from 0.000 sec. to 183.015 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 2.20905 ( 1.75004 1.75004 )
beta : -2.53386 ( 2.94383 11.1939 )
Epeak [keV] : 19.0183 ( -12.8767 -12.8767 )
Norm@50keV : 0.776460 ( -0.81248 159.333 )
------------------------------------------------------------
# Chi-Squared = 55.11 using 59 PHA bins.
# Reduced chi-squared = 1.002 for 55 degrees of freedom
# Null hypothesis probability = 4.703437e-01
Photon flux (15-150 keV) in 183 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] : 7.49715 (-7.50877 9.75271)
R^2/D10^2 : 3.26947E-02 (-0.0323999 4.28297)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
# Chi-Squared = 55.77 using 59 PHA bins.
# Reduced chi-squared = 0.9784 for 57 degrees of freedom
# Null hypothesis probability = 5.212976e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.770e-08 3.958e-08
25- 50 8.993e-08 6.421e-08
50-150 1.898e-08 1.769e-08
15-150 1.666e-07 1.174e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 33.6626 (-33.6626 -33.6626)
Norm : 0.169976 (-0.169976 1.57417)
------------------------------------------------------------
# Chi-Squared = 55.23 using 59 PHA bins.
# Reduced chi-squared = 0.9689 for 57 degrees of freedom
# Null hypothesis probability = 5.418967e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.684e-08 4.451e-08
25- 50 8.116e-08 5.930e-08
50-150 5.142e-08 5.176e-08
15-150 1.994e-07 1.451e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 3.40930 (-3.4072 -3.4072)
R1^2/D10^2 : 0.650819 (-0.653175 -0.653175)
kT2 [keV] : 11.2126 (-11.2084 -11.2084)
R2^2/D10^2 : 4.76057E-03 (-0.00476972 1.78542)
------------------------------------------------------------
# Chi-Squared = 55.10 using 59 PHA bins.
# Reduced chi-squared = 1.002 for 55 degrees of freedom
# Null hypothesis probability = 4.709420e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.020e-08 5.283e-08
25- 50 7.708e-08 5.356e-08
50-150 4.799e-08 4.789e-08
15-150 1.953e-07 1.240e-07
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: 2.40604 ( -1.29463 2.33524 )
Norm@50keV : 1.25638E-04 ( -0.000125638 0.000123155 )
------------------------------------------------------------
# Chi-Squared = 55.16 using 59 PHA bins.
# Reduced chi-squared = 0.9677 for 57 degrees of freedom
# Null hypothesis probability = 5.445225e-01
Photon flux (15-150 keV) in 183 sec: 2.33287E-02 ( -0.0142163 0.0142335 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.24589e-07 ( -1.5751e-07 1.95444e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.91139 ( )
Epeak [keV] : 6.42669 ( )
Norm@50keV : 2.58874E-04 ( )
------------------------------------------------------------
# Chi-Squared = 55.18 using 59 PHA bins.
# Reduced chi-squared = 0.9853 for 56 degrees of freedom
# Null hypothesis probability = 5.059463e-01
Photon flux (15-150 keV) in 183 sec: 2.33184E-02 ( -0.0141925 0.0141874 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.66086e-07 ( -2.66086e-07 4.79083e-07 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 2.20905 ( 1.75004 1.75004 )
beta : -2.53386 ( 2.94383 11.1939 )
Epeak [keV] : 19.0183 ( -12.8767 -12.8767 )
Norm@50keV : 0.776460 ( -0.81248 159.333 )
------------------------------------------------------------
# Chi-Squared = 55.11 using 59 PHA bins.
# Reduced chi-squared = 1.002 for 55 degrees of freedom
# Null hypothesis probability = 4.703437e-01
Photon flux (15-150 keV) in 183 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) = 7.37139e-08
S(50-100 keV) = 5.56313e-08
T90 vs. Hardness ratio plot
T90 = 1088 sec.
Hardness ratio (energy fluence ratio) = 0.754692
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 0.631745
Count Ratio (50-100 keV) / (15-25 keV) = 0.174746
Mask shadow pattern
IMX = -6.121162303725387E-01, IMY = -1.721164935028914E-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 183.014900
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
244.9739 -15.6369 0.8 45.3 -165.3 5.3562 15.1 0.4 Sco X-1
255.8699 -37.8008 4.4 48.4 161.6 -1.7137 -2.7 6.1 4U 1700-377
256.4348 -36.4240 86.2 47.1 162.5 0.0710 0.1 0.1 GX 349+2
263.0077 -24.7476 389.7 34.9 169.4 -0.0079 -0.0 0.1 GX 1+4
264.7018 -44.3403 19.7 49.4 149.3 0.5436 0.6 6.8 4U 1735-44
268.2638 -1.4489 7.3 19.7 -148.3 0.2991 1.6 6.3 SW J1753.5-0127
270.3040 -25.0942 2.3 30.8 159.8 1.2580 5.0 1.4 GX 5-1
270.2439 -25.6219 6.4 31.2 159.3 0.4745 1.8 7.9 GRS 1758-258
274.0060 -14.0363 30.9 20.0 170.3 -0.0684 -0.4 0.0 GX 17+2
275.8469 -30.2882 4.4 32.9 146.9 0.7838 2.6 6.2 H1820-303
284.9596 -25.0175 6.0 25.7 133.6 0.4806 1.9 7.2 HT1900.1-2455
288.7823 10.9449 0.7 10.4 -47.4 2.9155 16.5 0.9 GRS 1915+105
299.6279 35.1880 4.6 36.3 -36.1 0.7030 2.5 2.0 Cyg X-1
308.0994 40.9193 1.9 44.3 -30.4 2.0078 5.9 2.1 Cyg X-3
326.0501 38.2972 85.0 51.5 -14.1 -0.0697 -0.1 5.9 Cyg X-2
262.9790 -33.7347 6.6 41.5 159.5 0.6802 1.8 6.0 GX 354-0
334.1831 -5.7408 2.4 46.7 46.0 3.8256 4.8 ------ UNKNOWN
291.4426 -6.7683 2.6 8.2 101.7 0.8006 4.4 ------ UNKNOWN
239.2954 -30.4694 2.6 55.6 179.2 4.0236 4.4 ------ UNKNOWN
232.5653 -1.9168 3.0 55.3 -145.1 4.7377 3.9 ------ UNKNOWN
247.0161 18.3389 2.8 43.8 -116.1 3.7471 4.2 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
Plot creation:
Sat Jul 14 18:30:42 EDT 2012