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Image
Pre-slew 15-350 keV image (Event data; bkg subtracted)
# RAcent DECcent POSerr Theta Phi Peak Cts SNR Name
16.7931 -50.1250 0.0499 34.0 -5.9 0.0123 3.8 TRIG_00345396
------------------------------------------
Foreground time interval of the image:
0.000 0.064 (delta_t = 0.064 [sec])
Background time interval of the image:
-60.000 -5.000 (delta_t = 55.000 [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
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.064000
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 0.064000
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 0.064000
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 0.064 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -0.413255 ( -1.51275 0.892983 )
Norm@50keV : 5.47607E-03 ( -0.00547645 0.00489232 )
------------------------------------------------------------
# Chi-Squared = 48.54 using 59 PHA bins.
# Reduced chi-squared = 0.8516 for 57 degrees of freedom
# Null hypothesis probability = 7.799014e-01
Photon flux (15-150 keV) in 0.064 sec: 0.879876 ( -0.879876 0.477278 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.21101e-09 ( -3.9008e-09 3.89976e-09 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.000 sec. to 0.064 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -4.98368 ( )
Epeak [keV] : 117.495 ( -31.8803 67.1007 )
Norm@50keV : 0.121539 ( -0.121539 0.126779 )
------------------------------------------------------------
# Chi-Squared = 45.45 using 59 PHA bins.
# Reduced chi-squared = 0.8116 for 56 degrees of freedom
# Null hypothesis probability = 8.421642e-01
Photon flux (15-150 keV) in 0.064 sec: 0.949911 ( 0.422299 -0.949911 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.72416e-09 ( 3.97638e-09 -8.72416e-09 ) ergs/cm2
Band function
Time interval is from 0.000 sec. to 0.064 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 4.38550 ( -5.47264 -0.614466 )
beta : -9.37166 ( 7.13344 9.45324 )
Epeak [keV] : 121.805 ( -31.101 549.06 )
Norm@50keV : 8.94573E-02 ( -0.0893594 0.0399509 )
------------------------------------------------------------
# Chi-Squared = 45.60 using 59 PHA bins.
# Reduced chi-squared = 0.8291 for 55 degrees of freedom
# Null hypothesis probability = 8.128059e-01
Photon flux (15-150 keV) in 0.064 sec: 0.925788 ( -0.394575 0.402972 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.63014e-09 ( -3.6772e-09 3.82272e-09 ) ergs/cm2
Peak spectrum fit
Power-law model
Time interval is from 0.000 sec. to 0.064 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -0.416816 ( -1.50211 0.890732 )
Norm@50keV : 5.46732E-03 ( -0.00546773 0.0048803 )
------------------------------------------------------------
# Chi-Squared = 48.81 using 59 PHA bins.
# Reduced chi-squared = 0.8563 for 57 degrees of freedom
# Null hypothesis probability = 7.715080e-01
Photon flux (15-150 keV) in 0.064 sec: 0.879999 ( -0.879999 0.476332 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.21818e-09 ( -3.89695e-09 3.89581e-09 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.000 sec. to 0.064 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -4.49705 ( )
Epeak [keV] : 126.775 ( -9999.47 -9999.47 )
Norm@50keV : 7.80759E-02 ( )
------------------------------------------------------------
# Chi-Squared = 45.88 using 59 PHA bins.
# Reduced chi-squared = 0.8192 for 56 degrees of freedom
# Null hypothesis probability = 8.307726e-01
Photon flux (15-150 keV) in 0.064 sec: 0.949911 ( 0.422299 -0.949911 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.72416e-09 ( 3.97638e-09 -8.72416e-09 ) ergs/cm2
Band function
Time interval is from 0.000 sec. to 0.064 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 4.38541 ( -2.31672 2.89587 )
beta : -10.00000 ( 2.87422e+10 2.87422e+10 )
Epeak [keV] : 128.245 ( -40.2078 1222.13 )
Norm@50keV : 7.06070E-02 ( -0.071076 0.115187 )
------------------------------------------------------------
# Chi-Squared = 45.89 using 59 PHA bins.
# Reduced chi-squared = 0.8344 for 55 degrees of freedom
# Null hypothesis probability = 8.043588e-01
Photon flux (15-150 keV) in 0.064 sec: 0.925788 ( -0.394575 0.402972 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.63014e-09 ( -3.6772e-09 3.82272e-09 ) 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: -0.413255 ( -1.51275 0.892983 )
Norm@50keV : 5.47607E-03 ( -0.00547645 0.00489232 )
------------------------------------------------------------
# Chi-Squared = 48.54 using 59 PHA bins.
# Reduced chi-squared = 0.8516 for 57 degrees of freedom
# Null hypothesis probability = 7.799014e-01
Photon flux (15-150 keV) in 0.064 sec: 0.879876 ( -0.879876 0.477278 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.21101e-09 ( -3.9008e-09 3.89976e-09 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -4.98368 ( )
Epeak [keV] : 117.495 ( -31.8803 67.1007 )
Norm@50keV : 0.121539 ( -0.121539 0.126779 )
------------------------------------------------------------
# Chi-Squared = 45.45 using 59 PHA bins.
# Reduced chi-squared = 0.8116 for 56 degrees of freedom
# Null hypothesis probability = 8.421642e-01
Photon flux (15-150 keV) in 0.064 sec: 0.949911 ( 0.422299 -0.949911 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.72416e-09 ( 3.97638e-09 -8.72416e-09 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 4.38550 ( -5.47221 -0.614466 )
beta : -9.37166 ( 7.13344 9.45324 )
Epeak [keV] : 121.805 ( -31.101 639.586 )
Norm@50keV : 8.94573E-02 ( -0.0893594 0.0399509 )
------------------------------------------------------------
# Chi-Squared = 45.60 using 59 PHA bins.
# Reduced chi-squared = 0.8291 for 55 degrees of freedom
# Null hypothesis probability = 8.128059e-01
Photon flux (15-150 keV) in 0.064 sec: 0.925788 ( -0.394575 0.402972 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.63014e-09 ( -3.6772e-09 3.82272e-09 ) ergs/cm2
S(25-50 keV) vs. S(50-100 keV) plot
S(25-50 keV) = 4.7256e-10
S(50-100 keV) = 2.51658e-09
T90 vs. Hardness ratio plot
T90 = 0.0640000104904175 sec.
Hardness ratio (energy fluence ratio) = 5.32542
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 0.0934579
Count Ratio (50-100 keV) / (15-25 keV) = -4.45594
Mask shadow pattern
IMX = 6.698492778619112E-01, IMY = 6.959880629369714E-02
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.064000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.064000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.064000
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:
-60.000000 -5.000000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
255.9031 -38.0132 3.8 46.2 147.5 0.6844 3.1 10.9 4U 1700-377
256.5754 -36.3852 14.0 46.9 149.6 -0.1904 -0.8 7.1 GX 349+2
262.8947 -24.7442 4.3 51.4 165.6 -0.6884 -2.7 6.2 GX 1+4
264.5841 -44.5227 30.4 37.1 145.7 0.0462 0.4 8.1 4U 1735-44
270.3636 -25.0159 7.8 46.8 172.2 -0.2202 -1.5 5.7 GX 5-1
270.4181 -25.7156 8.1 46.3 171.6 0.2024 1.4 6.5 GRS 1758-258
273.9756 -14.1406 7.7 53.6 -175.9 -0.3109 -1.5 6.5 GX 17+2
275.7235 -30.3088 0.0 39.7 172.4 0.1071 1.0 11.0 H1820-303
285.2393 -24.9571 5.3 38.7 -171.9 0.2039 2.2 11.3 HT1900.1-2455
29.7070 -66.1901 2.3 35.1 24.9 0.5009 5.0 ------ UNKNOWN
13.8206 -20.2259 2.6 51.9 -42.2 1.5642 4.4 ------ UNKNOWN
357.5553 -18.6206 2.9 44.5 -60.5 1.0865 4.0 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
0.000000 0.064000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
256.1173 -37.7059 5.7 46.3 147.9 -0.0148 -2.0 10.4 4U 1700-377
256.4240 -36.4255 21.9 47.0 149.5 0.0039 0.5 0.6 GX 349+2
263.0522 -24.5650 52.2 51.5 165.8 0.0018 0.2 11.1 GX 1+4
264.8111 -44.4211 9.9 37.0 145.9 -0.0052 -1.2 3.4 4U 1735-44
270.3532 -25.1894 6.4 46.7 172.0 -0.0092 -1.8 7.6 GX 5-1
270.1702 -25.7418 2.8 46.4 171.3 0.0208 4.2 7.1 GRS 1758-258
273.9280 -13.9746 4.7 53.8 -175.8 -0.0166 -2.5 5.9 GX 17+2
275.8700 -30.5058 306.2 39.5 172.3 0.0001 0.0 8.8 H1820-303
285.0955 -24.9295 3.2 38.8 -172.0 -0.0124 -3.6 3.3 HT1900.1-2455
Post-slew image of 15-350 keV band
Time interval of the image:
68.200590 238.780000
240.000000 243.044300
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
272.8705 -67.7608 2.5 49.4 158.3 1.8525 4.6 ------ UNKNOWN
22.5729 -28.8891 2.0 21.6 -36.7 0.7301 5.7 ------ UNKNOWN
294.7787 -38.8510 3.1 56.6 -163.2 2.0048 3.7 ------ UNKNOWN
341.7837 -28.8807 3.0 33.8 -115.1 0.8195 3.8 ------ UNKNOWN
23.3992 1.6073 3.4 52.0 -42.2 2.4157 3.4 ------ UNKNOWN
336.8288 -20.4517 2.9 43.2 -112.2 2.3385 4.0 ------ UNKNOWN
Plot creation:
Tue Feb 16 21:53:44 EST 2010