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Image
Pre-slew 15-350 keV image (Event data; bkg subtracted)
# RAcent DECcent POSerr Theta Phi Peak Cts SNR Name
268.6275 -26.3382 0.0313 24.6 -161.2 1.8638 6.1 TRIG_00414875
------------------------------------------
Foreground time interval of the image:
0.000 320.000 (delta_t = 320.000 [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)
The mask-weighted light curves based on cleaned DPHs
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 320.000 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 3.20232 ( -0.50598 0.604348 )
Norm@50keV : 1.47118E-04 ( -6.43391e-05 7.6007e-05 )
------------------------------------------------------------
# Chi-Squared = 70.08 using 59 PHA bins.
# Reduced chi-squared = 1.230 for 57 degrees of freedom
# Null hypothesis probability = 1.143308e-01
Photon flux (15-150 keV) in 320 sec: 4.70508E-02 ( -0.00814731 0.00817854 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.25053e-07 ( -1.40387e-07 1.57564e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.000 sec. to 320.000 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.00000 ( )
Epeak [keV] : 50.0000 ( )
Norm@50keV : 8.54540E-04 ( )
------------------------------------------------------------
# Chi-Squared = 98.96 using 59 PHA bins.
# Reduced chi-squared = 1.767 for 56 degrees of freedom
# Null hypothesis probability = 3.522297e-04
Photon flux (15-150 keV) in 320 sec: 4.70264E-02 ( -0.008144 0.0081752 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.24874e-07 ( -1.4033e-07 1.57472e-07 ) ergs/cm2
Band function
Time interval is from 0.000 sec. to 320.000 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.55789 ( 1.5579 1.5579 )
beta : -3.46679 ( 3.47145 0.738306 )
Epeak [keV] : 6.09362 ( -6.08437 12.7932 )
Norm@50keV : 2.96533E-03 ( -0.00298295 16.6824 )
------------------------------------------------------------
# Chi-Squared = 69.70 using 59 PHA bins.
# Reduced chi-squared = 1.267 for 55 degrees of freedom
# Null hypothesis probability = 8.762281e-02
Photon flux (15-150 keV) in 320 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 320.000 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 3.17261 ( -0.453232 0.543484 )
Norm@50keV : 1.50374E-04 ( -6.26422e-05 7.37378e-05 )
------------------------------------------------------------
# Chi-Squared = 70.83 using 59 PHA bins.
# Reduced chi-squared = 1.243 for 57 degrees of freedom
# Null hypothesis probability = 1.030647e-01
Photon flux (15-150 keV) in 320 sec: 4.70249E-02 ( -0.00761408 0.00766057 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.29411e-07 ( -1.39164e-07 1.56854e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.000 sec. to 320.000 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.00000 ( )
Epeak [keV] : 50.0000 ( )
Norm@50keV : 9.29292E-04 ( )
------------------------------------------------------------
# Chi-Squared = 108.20 using 59 PHA bins.
# Reduced chi-squared = 1.9321 for 56 degrees of freedom
# Null hypothesis probability = 3.554630e-05
Photon flux (15-150 keV) in 320 sec: 4.70009E-02 ( -0.0076115 0.0076579 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.29226e-07 ( -1.39104e-07 1.56762e-07 ) ergs/cm2
Band function
Time interval is from 0.000 sec. to 320.000 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.400072 ( 1.70554 1.70554 )
beta : -3.54085 ( 3.47161 11.6132 )
Epeak [keV] : 12.8471 ( -12.8156 6.83391 )
Norm@50keV : 2.47786E-02 ( -0.0252596 710.594 )
------------------------------------------------------------
# Chi-Squared = 70.29 using 59 PHA bins.
# Reduced chi-squared = 1.278 for 55 degrees of freedom
# Null hypothesis probability = 8.024766e-02
Photon flux (15-150 keV) in 320 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: 3.20232 ( -0.50598 0.604348 )
Norm@50keV : 1.47118E-04 ( -6.43391e-05 7.6007e-05 )
------------------------------------------------------------
# Chi-Squared = 70.08 using 59 PHA bins.
# Reduced chi-squared = 1.230 for 57 degrees of freedom
# Null hypothesis probability = 1.143308e-01
Photon flux (15-150 keV) in 320 sec: 4.70508E-02 ( -0.00814731 0.00817854 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.25053e-07 ( -1.40387e-07 1.57564e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.00000 ( )
Epeak [keV] : 50.0000 ( )
Norm@50keV : 8.54540E-04 ( )
------------------------------------------------------------
# Chi-Squared = 98.96 using 59 PHA bins.
# Reduced chi-squared = 1.767 for 56 degrees of freedom
# Null hypothesis probability = 3.522297e-04
Photon flux (15-150 keV) in 320 sec: 4.70264E-02 ( -0.008144 0.0081752 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.24874e-07 ( -1.4033e-07 1.57472e-07 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.55789 ( 1.5579 1.5579 )
beta : -3.46679 ( 3.47145 0.738306 )
Epeak [keV] : 6.09362 ( -6.08437 12.7932 )
Norm@50keV : 2.96533E-03 ( -0.00298295 16.6824 )
------------------------------------------------------------
# Chi-Squared = 69.70 using 59 PHA bins.
# Reduced chi-squared = 1.267 for 55 degrees of freedom
# Null hypothesis probability = 8.762281e-02
Photon flux (15-150 keV) in 320 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) = 2.04035e-07
S(50-100 keV) = 8.86682e-08
T90 vs. Hardness ratio plot
T90 = 320 sec.
Hardness ratio (energy fluence ratio) = 0.434573
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 0.387915
Count Ratio (50-100 keV) / (15-25 keV) = 0.144314
Mask shadow pattern
IMX = -4.331646531596388E-01, IMY = 1.478716112025306E-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 320.000000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
170.4707 -60.6339 6.8 47.0 32.1 1.4513 1.7 4.6 Cen X-3
186.6404 -62.8035 2.4 39.0 32.8 2.6277 4.8 2.0 GX 301-2
244.9926 -15.6469 0.4 34.3 151.6 12.0624 26.4 0.9 Sco X-1
255.9925 -37.8428 137.2 11.0 171.2 -0.0235 -0.1 0.3 4U 1700-377
256.4354 -36.4230 3.0 12.4 172.8 1.1229 3.9 0.0 GX 349+2
262.9391 -24.8066 2.8 24.6 -174.0 1.1499 4.2 5.3 GX 1+4
264.7079 -44.5980 4.4 7.4 -130.8 0.6857 2.6 9.0 4U 1735-44
268.4644 -1.3718 97.8 48.7 -172.8 0.0673 0.1 7.5 SW J1753.5-0127
270.3630 -25.0668 4.2 26.3 -158.8 0.8450 2.8 4.3 GX 5-1
270.3964 -25.7495 4.5 25.7 -158.2 0.7914 2.6 5.1 GRS 1758-258
274.0190 -14.0144 5.5 37.9 -160.2 0.9677 2.1 1.5 GX 17+2
275.9879 -30.3013 4.1 24.0 -142.7 0.8499 2.8 5.1 H1820-303
284.8964 -24.9861 6.9 32.9 -135.6 0.6193 1.7 8.6 HT1900.1-2455
205.9044 -54.3647 2.9 30.8 50.6 1.6764 4.0 ------ UNKNOWN
225.9216 -52.9702 3.1 19.1 56.2 1.0891 3.7 ------ UNKNOWN
255.1832 -41.6256 1.8 7.2 166.8 1.7553 6.5 ------ UNKNOWN
259.9092 -20.5587 2.7 28.4 178.4 1.2522 4.2 ------ UNKNOWN
255.6940 -48.7763 0.8 0.0 115.7 3.9330 14.1 ------ UNKNOWN
268.6273 -26.3382 1.9 24.6 -161.2 1.8643 6.1 ------ UNKNOWN
55.4905 -73.9784 3.7 56.5 -16.4 3.7669 3.1 ------ UNKNOWN
291.8709 -4.4122 3.3 54.0 -143.2 6.6260 3.6 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
383.900600 821.920000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
244.9854 -15.6460 0.3 24.5 111.6 15.9470 37.3 0.5 Sco X-1
255.9930 -37.9937 6.0 15.8 39.7 -0.6614 -1.9 9.0 4U 1700-377
256.4701 -36.5753 3.1 14.5 42.7 1.2448 3.7 9.3 GX 349+2
262.9520 -24.7194 3.4 5.4 106.8 1.1087 3.4 3.5 GX 1+4
264.7934 -44.5656 26.0 18.5 9.0 -0.1446 -0.4 7.3 4U 1735-44
268.3695 -1.3356 3.1 25.0 179.8 1.3034 3.8 7.0 SW J1753.5-0127
270.1681 -25.1377 4.9 1.9 -129.9 0.8442 2.3 7.2 GX 5-1
270.4683 -25.7619 6.9 1.8 -108.4 0.6212 1.7 9.0 GRS 1758-258
274.0272 -14.1055 2.5 13.2 -156.1 1.6673 4.6 4.3 GX 17+2
275.7414 -30.2287 0.0 7.4 -56.2 1.1948 3.5 12.6 H1820-303
285.1118 -24.8196 112.4 15.0 -91.8 0.0365 0.1 7.3 HT1900.1-2455
288.7826 10.9446 1.2 42.1 -149.3 6.4479 10.1 0.9 GRS 1915+105
250.3232 0.6234 2.9 32.2 144.3 1.8935 3.9 ------ UNKNOWN
255.1773 -41.6253 1.6 18.9 32.9 2.6062 7.3 ------ UNKNOWN
261.5917 25.0288 2.9 51.8 172.3 4.4050 4.1 ------ UNKNOWN
255.7206 -48.8056 1.0 24.6 21.0 4.0302 11.8 ------ UNKNOWN
268.5966 -26.2866 1.8 0.1 170.1 2.3116 6.4 ------ UNKNOWN
340.4276 -67.8317 3.2 58.9 -24.4 10.2170 3.6 ------ UNKNOWN
323.1803 -43.8397 4.4 47.0 -53.1 5.7796 2.7 ------ UNKNOWN
Plot creation:
Fri Mar 5 13:22:11 EST 2010