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Image
Pre-slew 15-350 keV image (Event data; bkg subtracted)
# RAcent DECcent POSerr Theta Phi Peak Cts SNR Name
42.6259 -2.2966 0.0574 25.2 -159.2 0.2549 3.3 TRIG_00433953
------------------------------------------
Foreground time interval of the image:
0.000 64.000 (delta_t = 64.000 [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)
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)
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 64.000 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.50647 ( -0.517568 0.620293 )
Norm@50keV : 2.20182E-04 ( -0.000106672 0.000118787 )
------------------------------------------------------------
# Chi-Squared = 80.21 using 59 PHA bins.
# Reduced chi-squared = 1.407 for 57 degrees of freedom
# Null hypothesis probability = 2.304575e-02
Photon flux (15-150 keV) in 64 sec: 4.34896E-02 ( -0.0146079 0.0146943 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.41938e-07 ( -2.61215e-08 6.21673e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.000 sec. to 64.000 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -7.89641 ( )
Epeak [keV] : 28.0816 ( -3.60344 4.47046 )
Norm@50keV : 3971.65 ( -3882.67 169997 )
------------------------------------------------------------
# Chi-Squared = 64.80 using 59 PHA bins.
# Reduced chi-squared = 1.157 for 56 degrees of freedom
# Null hypothesis probability = 1.965256e-01
Photon flux (15-150 keV) in 64 sec: 4.77877E-02 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 1.30298e-07 ( -3.69037e-08 4.06381e-08 ) ergs/cm2
Band function
Time interval is from 0.000 sec. to 64.000 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 4.99204 ( -252.062 -242.062 )
beta : -9.99795 ( 1547.13 1557.12 )
Epeak [keV] : 28.4236 ( -4.07972 4.64228 )
Norm@50keV : 34.0600 ( -34.0601 50.509 )
------------------------------------------------------------
# Chi-Squared = 65.31 using 59 PHA bins.
# Reduced chi-squared = 1.187 for 55 degrees of freedom
# Null hypothesis probability = 1.610358e-01
Photon flux (15-150 keV) in 64 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] : ( )
R^2/D10^2 : ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25
25- 50
50-150
15-150
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : ( )
Norm : ( )
------------------------------------------------------------
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25
25- 50
50-150
15-150
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : ( )
R1^2/D10^2 : ( )
kT2 [keV] : ( )
R2^2/D10^2 : ( )
------------------------------------------------------------
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25
25- 50
50-150
15-150
Peak spectrum fit
Power-law model
Time interval is from 0.000 sec. to 64.000 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.48049 ( -0.496995 0.626281 )
Norm@50keV : 2.25105E-04 ( -0.000107978 0.000116807 )
------------------------------------------------------------
# Chi-Squared = 80.90 using 59 PHA bins.
# Reduced chi-squared = 1.419 for 57 degrees of freedom
# Null hypothesis probability = 2.038597e-02
Photon flux (15-150 keV) in 64 sec: 4.36483E-02 ( -0.0144253 0.0145241 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.42695e-07 ( -5.39585e-08 6.19371e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.000 sec. to 64.000 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -7.78967 ( )
Epeak [keV] : 28.0631 ( -3.57143 4.41863 )
Norm@50keV : 3384.56 ( -3343.07 174622 )
------------------------------------------------------------
# Chi-Squared = 65.27 using 59 PHA bins.
# Reduced chi-squared = 1.166 for 56 degrees of freedom
# Null hypothesis probability = 1.856263e-01
Photon flux (15-150 keV) in 64 sec: 4.80916E-02 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 1.31044e-07 ( -3.69722e-08 4.03898e-08 ) ergs/cm2
Band function
Time interval is from 0.000 sec. to 64.000 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 4.99960 ( -4758.02 -4743.03 )
beta : -9.99791 ( 1519.12 1529.12 )
Epeak [keV] : 28.3915 ( -4.01757 4.5809 )
Norm@50keV : 34.8949 ( -34.8949 60.7277 )
------------------------------------------------------------
# Chi-Squared = 65.76 using 59 PHA bins.
# Reduced chi-squared = 1.196 for 55 degrees of freedom
# Null hypothesis probability = 1.517873e-01
Photon flux (15-150 keV) in 64 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] : ( )
R^2/D10^2 : ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25
25- 50
50-150
15-150
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : ( )
Norm : ( )
------------------------------------------------------------
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25
25- 50
50-150
15-150
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : ( )
R1^2/D10^2 : ( )
kT2 [keV] : ( )
R2^2/D10^2 : ( )
------------------------------------------------------------
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25
25- 50
50-150
15-150
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: 2.50647 ( -0.517568 0.620293 )
Norm@50keV : 2.20182E-04 ( -0.000106672 0.000118787 )
------------------------------------------------------------
# Chi-Squared = 80.21 using 59 PHA bins.
# Reduced chi-squared = 1.407 for 57 degrees of freedom
# Null hypothesis probability = 2.304575e-02
Photon flux (15-150 keV) in 64 sec: 4.34896E-02 ( -0.0146079 0.0146943 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.41938e-07 ( -2.61215e-08 6.21673e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -7.89641 ( )
Epeak [keV] : 28.0816 ( -3.60344 4.47046 )
Norm@50keV : 3971.65 ( -3882.67 170008 )
------------------------------------------------------------
# Chi-Squared = 64.80 using 59 PHA bins.
# Reduced chi-squared = 1.157 for 56 degrees of freedom
# Null hypothesis probability = 1.965256e-01
Photon flux (15-150 keV) in 64 sec: 4.77877E-02 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 1.30298e-07 ( -3.69037e-08 4.06381e-08 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 4.99204 ( -252.062 -242.062 )
beta : -9.99795 ( 1547.13 1557.12 )
Epeak [keV] : 28.4236 ( -4.07972 4.64228 )
Norm@50keV : 34.0600 ( -34.0601 50.509 )
------------------------------------------------------------
# Chi-Squared = 65.31 using 59 PHA bins.
# Reduced chi-squared = 1.187 for 55 degrees of freedom
# Null hypothesis probability = 1.610358e-01
Photon flux (15-150 keV) in 64 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) = 4.70741e-08
S(50-100 keV) = 3.34024e-08
T90 vs. Hardness ratio plot
T90 = 64 sec.
Hardness ratio (energy fluence ratio) = 0.709571
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.14613
Count Ratio (50-100 keV) / (15-25 keV) = -0.29708
Mask shadow pattern
IMX = -4.395981835793915E-01, IMY = 1.665709130221912E-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 64.000000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
333.7025 -19.1820 2.7 46.2 47.6 1.5329 4.3 ------ UNKNOWN
43.0236 -26.1400 3.0 20.6 -96.0 0.3333 3.9 ------ UNKNOWN
52.6661 -46.4564 2.5 37.7 -67.2 0.8025 4.5 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
131.700590 210.120000
211.000000 916.300000
917.000000 963.048500
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
12.5754 -21.3299 2.7 35.0 58.4 3.2587 4.3 ------ UNKNOWN
62.3478 -51.4291 2.4 51.9 -11.6 4.9528 4.9 ------ UNKNOWN
68.1871 3.7915 3.2 26.2 -99.3 1.8268 3.6 ------ UNKNOWN
85.2913 -25.1188 3.6 47.0 -53.1 6.8858 3.3 ------ UNKNOWN
Plot creation:
Sun Sep 12 19:45:41 EDT 2010