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Image
Pre-slew 15-350 keV image (Event data; bkg subtracted)
# RAcent DECcent POSerr Theta Phi Peak Cts SNR Name
242.6849 +3.5857 0.0364 20.3 14.3 0.0278 5.3 TRIG_00355981
------------------------------------------
Foreground time interval of the image:
0.000 0.256 (delta_t = 0.256 [sec])
Background time interval of the image:
-24.283 -3.584 (delta_t = 20.699 [sec])
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 0.256 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.15525 ( -0.544493 0.704391 )
Norm@50keV : 4.02304E-03 ( -0.00195456 0.00188021 )
------------------------------------------------------------
# Chi-Squared = 89.48 using 59 PHA bins.
# Reduced chi-squared = 1.570 for 57 degrees of freedom
# Null hypothesis probability = 3.874813e-03
Photon flux (15-150 keV) in 0.256 sec: 0.650063 ( -0.251093 0.251221 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.61047e-09 ( -4.11098e-09 4.27827e-09 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.000 sec. to 0.256 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -4.82131 ( )
Epeak [keV] : 35.9648 ( -6.49735 7.41734 )
Norm@50keV : 73.5476 ( -73.5554 27.0153 )
------------------------------------------------------------
# Chi-Squared = 83.27 using 59 PHA bins.
# Reduced chi-squared = 1.487 for 56 degrees of freedom
# Null hypothesis probability = 1.049078e-02
Photon flux (15-150 keV) in 0.256 sec: 0.650737 ( -0.220857 0.223514 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.19967e-09 ( -3.02228e-09 3.15548e-09 ) ergs/cm2
Band function
Time interval is from 0.000 sec. to 0.256 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 4.97340 ( -83.8058 -73.806 )
beta : -7.20790 ( 5.8498 15.0399 )
Epeak [keV] : 35.8824 ( -6.31835 7.34999 )
Norm@50keV : 91.9855 ( -50.0544 153.594 )
------------------------------------------------------------
# Chi-Squared = 83.21 using 59 PHA bins.
# Reduced chi-squared = 1.513 for 55 degrees of freedom
# Null hypothesis probability = 8.356770e-03
Photon flux (15-150 keV) in 0.256 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 0.256 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.16230 ( -0.536213 0.695392 )
Norm@50keV : 4.05716E-03 ( -0.00195288 0.00187791 )
------------------------------------------------------------
# Chi-Squared = 90.31 using 59 PHA bins.
# Reduced chi-squared = 1.584 for 57 degrees of freedom
# Null hypothesis probability = 3.256426e-03
Photon flux (15-150 keV) in 0.256 sec: 0.657996 ( -0.24936 0.249422 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.70171e-09 ( -4.09577e-09 4.26447e-09 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.000 sec. to 0.256 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -4.80148 ( )
Epeak [keV] : 35.8612 ( -6.45321 7.31844 )
Norm@50keV : 73.6545 ( -73.6643 27.3739 )
------------------------------------------------------------
# Chi-Squared = 84.14 using 59 PHA bins.
# Reduced chi-squared = 1.502 for 56 degrees of freedom
# Null hypothesis probability = 8.854697e-03
Photon flux (15-150 keV) in 0.256 sec: 0.658183 ( -0.220722 0.222579 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.19967e-09 ( -3.02228e-09 3.15548e-09 ) ergs/cm2
Band function
Time interval is from 0.000 sec. to 0.256 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 4.99994 ( -31286.6 -31283.5 )
beta : -7.45901 ( 5.80408 15.4489 )
Epeak [keV] : 36.3144 ( -6.69989 6.84415 )
Norm@50keV : 88.9159 ( -71.6678 245.599 )
------------------------------------------------------------
# Chi-Squared = 84.09 using 59 PHA bins.
# Reduced chi-squared = 1.529 for 55 degrees of freedom
# Null hypothesis probability = 7.005235e-03
Photon flux (15-150 keV) in 0.256 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: 2.15525 ( -0.544493 0.704391 )
Norm@50keV : 4.02304E-03 ( -0.00195456 0.00188021 )
------------------------------------------------------------
# Chi-Squared = 89.48 using 59 PHA bins.
# Reduced chi-squared = 1.570 for 57 degrees of freedom
# Null hypothesis probability = 3.874813e-03
Photon flux (15-150 keV) in 0.256 sec: 0.650063 ( -0.251093 0.251221 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.61047e-09 ( -4.11098e-09 4.27827e-09 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -4.82131 ( )
Epeak [keV] : 35.9648 ( -6.49735 7.41734 )
Norm@50keV : 73.5476 ( -73.5554 27.0153 )
------------------------------------------------------------
# Chi-Squared = 83.27 using 59 PHA bins.
# Reduced chi-squared = 1.487 for 56 degrees of freedom
# Null hypothesis probability = 1.049078e-02
Photon flux (15-150 keV) in 0.256 sec: 0.650737 ( -0.220857 0.223514 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.19967e-09 ( -3.02228e-09 3.15548e-09 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 4.97340 ( -83.8057 -73.806 )
beta : -7.20790 ( 5.8498 15.0399 )
Epeak [keV] : 35.8824 ( -6.31835 7.34999 )
Norm@50keV : 91.9855 ( -50.0544 118.425 )
------------------------------------------------------------
# Chi-Squared = 83.21 using 59 PHA bins.
# Reduced chi-squared = 1.513 for 55 degrees of freedom
# Null hypothesis probability = 8.356770e-03
Photon flux (15-150 keV) in 0.256 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) = 3.0146e-09
S(50-100 keV) = 2.70405e-09
T90 vs. Hardness ratio plot
T90 = 0.256000012159348 sec.
Hardness ratio (energy fluence ratio) = 0.896985
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 2.03311
Count Ratio (50-100 keV) / (15-25 keV) = -0.0222524
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:
-24.283400 -3.584000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
186.6737 -62.8066 6.0 58.3 -157.6 -0.5323 -1.9 2.2 GX 301-2
244.9597 -15.6170 0.6 7.6 86.4 0.8707 19.0 1.8 Sco X-1
254.5763 35.3120 14.4 53.9 15.7 0.2150 0.8 6.1 Her X-1
255.8849 -37.7648 5.4 27.4 144.3 0.1438 2.1 6.8 4U 1700-377
256.2675 -36.5133 8.8 26.7 142.0 0.0874 1.3 9.7 GX 349+2
263.1645 -24.6644 3.1 25.9 111.8 0.2673 3.7 9.8 GX 1+4
264.7151 -44.6048 14.6 36.9 144.6 0.0703 0.8 9.4 4U 1735-44
268.5307 -1.5852 0.0 34.2 66.3 -0.3399 -3.2 12.6 SW J1753.5-0127
270.2835 -25.2125 37.9 32.3 110.1 -0.0279 -0.3 8.0 GX 5-1
270.3006 -25.8771 33.1 32.5 111.3 0.0316 0.4 8.0 GRS 1758-258
274.1149 -14.1446 4.2 35.8 90.2 0.3276 2.7 9.1 GX 17+2
276.0396 -30.4642 10.7 38.4 117.2 0.1638 1.1 8.3 H1820-303
241.9658 0.4762 2.2 17.1 14.8 0.2509 5.4 ------ UNKNOWN
197.3168 -68.0418 2.4 57.9 -165.6 1.1553 4.8 ------ UNKNOWN
205.0465 -4.9658 2.4 33.3 -76.2 0.3859 4.7 ------ UNKNOWN
193.7897 -22.3308 3.1 41.2 -107.9 0.7291 3.8 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
0.000000 0.256000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
186.6430 -62.7560 5.9 58.3 -157.5 0.0616 2.0 0.9 GX 301-2
245.0202 -15.7888 5.2 7.6 87.7 -0.0111 -2.2 9.2 Sco X-1
254.4617 35.3563 8.8 53.9 15.5 0.0377 1.3 0.9 Her X-1
256.0604 -37.9302 5.2 27.6 144.4 0.0146 2.2 6.2 4U 1700-377
256.3561 -36.3128 5.2 26.6 141.5 -0.0146 -2.2 7.6 GX 349+2
262.8343 -24.6324 0.0 25.6 111.9 0.0175 2.5 11.7 GX 1+4
264.7954 -44.3285 6.0 36.8 144.2 -0.0185 -1.9 7.6 4U 1735-44
268.3808 -1.5818 10.0 34.0 66.1 0.0128 1.2 7.8 SW J1753.5-0127
270.3214 -25.2044 6.6 32.4 110.1 -0.0167 -1.7 7.8 GX 5-1
270.1605 -25.9078 0.0 32.4 111.4 -0.0098 -1.0 12.5 GRS 1758-258
273.9932 -14.1341 7.5 35.7 90.1 0.0203 1.5 5.9 GX 17+2
275.8199 -30.4881 5.5 38.2 117.3 0.0328 2.1 9.1 H1820-303
278.2907 -57.1545 2.4 51.4 150.8 0.1208 4.8 ------ UNKNOWN
257.8705 -69.6791 2.3 55.2 169.4 0.1454 5.0 ------ UNKNOWN
249.2629 9.7108 1.9 28.4 24.0 0.0385 6.2 ------ UNKNOWN
237.9885 30.2905 2.1 46.3 -0.9 0.0536 5.6 ------ UNKNOWN
212.6923 29.7920 2.5 51.4 -29.3 0.0688 4.7 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
70.416600 113.916600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
244.9735 -15.6397 0.5 19.4 134.5 1.7334 23.6 0.3 Sco X-1
254.3507 35.2661 3.5 33.4 -21.5 -0.2650 -3.3 7.0 Her X-1
255.7697 -37.8268 7.2 43.2 126.0 0.4997 1.6 10.3 4U 1700-377
256.4331 -36.2822 9.4 41.9 124.5 0.3458 1.2 8.5 GX 349+2
263.0697 -24.8138 5.9 34.6 107.4 0.3131 2.0 5.3 GX 1+4
268.4146 -1.4190 21.2 26.2 61.8 -0.0517 -0.5 3.4 SW J1753.5-0127
270.4502 -25.0325 13.3 39.3 99.4 0.2497 0.9 9.4 GX 5-1
270.2747 -25.8635 31.0 39.8 100.5 -0.1110 -0.4 7.4 GRS 1758-258
274.0320 -13.9008 10.1 35.7 81.2 -0.2122 -1.1 8.3 GX 17+2
288.8032 11.1710 0.0 46.3 39.1 0.6523 2.7 13.5 GRS 1915+105
243.9361 -24.6590 2.5 28.3 138.8 0.4209 4.6 ------ UNKNOWN
205.4509 -38.2727 3.0 54.3 176.9 1.0669 3.8 ------ UNKNOWN
193.0928 -14.9426 2.5 52.5 -150.9 1.0763 4.6 ------ UNKNOWN
189.6937 -10.6229 3.4 54.7 -144.7 1.4972 3.4 ------ UNKNOWN
Plot creation:
Tue Feb 16 10:43:43 EST 2010