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Image
Pre-slew 15-350 keV image (Event data; bkg subtracted)
# RAcent DECcent POSerr Theta Phi Peak Cts SNR Name
190.0127 +15.4540 0.0437 24.3 -153.2 0.4334 4.4 TRIG_00618402
------------------------------------------
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
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 64.000000
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 64.000000
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 64.000000
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 64.000 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.25955 ( -0.556537 0.691216 )
Norm@50keV : 3.32686E-04 ( -0.000158874 0.000161607 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 54.29 using 59 PHA bins.
# Reduced chi-squared = 0.9524 for 57 degrees of freedom
# Null hypothesis probability = 5.774336e-01
Photon flux (15-150 keV) in 64 sec: 5.68562E-02 ( -0.0178092 0.017891 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.01981e-07 ( -7.85056e-08 8.88704e-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: -0.113207 ( -6.68151 2.62208 )
Epeak [keV] : 28.2642 ( )
Norm@50keV : 1.35925E-02 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 52.43 using 59 PHA bins.
# Reduced chi-squared = 0.9363 for 56 degrees of freedom
# Null hypothesis probability = 6.106637e-01
Photon flux (15-150 keV) in 64 sec: 5.48030E-02 ( -0.0166813 0.017151 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.6017e-07 ( -5.77152e-08 9.27667e-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 : 0.581257 ( -2.89292 -0.0382335 )
beta : -10.0000 ( 10 3.55271e-15 )
Epeak [keV] : 28.4879 ( -8.86442 199.803 )
Norm@50keV : 2.87759E-02 ( -0.0293105 21.3389 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 52.40 using 59 PHA bins.
# Reduced chi-squared = 0.9528 for 55 degrees of freedom
# Null hypothesis probability = 5.744614e-01
Photon flux (15-150 keV) in 64 sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 1.69884e-07 ( 0 0 ) ergs/cm2
Single BB
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 7.36161 (-2.02821 2.69285)
R^2/D10^2 : 9.33164E-02 (-0.0933158 0.248164)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 52.57 using 59 PHA bins.
# Reduced chi-squared = 0.9223 for 57 degrees of freedom
# Null hypothesis probability = 6.418165e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.462e-08 3.370e-08
25- 50 8.232e-08 5.146e-08
50-150 1.631e-08 1.320e-08
15-150 1.532e-07 9.571e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 36.2334 (-18.4778 58.9902)
Norm : 0.402276 (-0.176851 0.360554)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 53.08 using 59 PHA bins.
# Reduced chi-squared = 0.9312 for 57 degrees of freedom
# Null hypothesis probability = 6.230110e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.703e-08 3.098e-08
25- 50 7.176e-08 4.378e-08
50-150 4.965e-08 4.112e-08
15-150 1.784e-07 1.146e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.10857 (-5.16558 -5.16558)
R1^2/D10^2 : 0.195720 (-0.191014 -0.191014)
kT2 [keV] : 9.67646 (-9.94609 -9.94609)
R2^2/D10^2 : 1.94986E-02 (-0.0157638 0.303469)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 52.32 using 59 PHA bins.
# Reduced chi-squared = 0.9513 for 55 degrees of freedom
# Null hypothesis probability = 5.776397e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.668e-08 6.496e-08
25- 50 7.859e-08 6.618e-08
50-150 2.747e-08 3.277e-08
15-150 1.627e-07 1.424e-07
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: 2.25955 ( -0.556537 0.691216 )
Norm@50keV : 3.32686E-04 ( -0.000158874 0.000161607 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 54.29 using 59 PHA bins.
# Reduced chi-squared = 0.9524 for 57 degrees of freedom
# Null hypothesis probability = 5.774336e-01
Photon flux (15-150 keV) in 64 sec: 5.68562E-02 ( -0.0178092 0.017891 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.01981e-07 ( -7.85056e-08 8.88704e-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: -0.113207 ( -6.68151 2.62208 )
Epeak [keV] : 28.2642 ( )
Norm@50keV : 1.35925E-02 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 52.43 using 59 PHA bins.
# Reduced chi-squared = 0.9363 for 56 degrees of freedom
# Null hypothesis probability = 6.106637e-01
Photon flux (15-150 keV) in 64 sec: 5.48030E-02 ( -0.0166813 0.017151 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.6017e-07 ( -5.77152e-08 9.27667e-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 : 0.581257 ( -2.89292 -0.0382335 )
beta : -10.0000 ( 10 1.77636e-15 )
Epeak [keV] : 28.4879 ( -8.86442 243.089 )
Norm@50keV : 2.87759E-02 ( -0.0293105 21.3389 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 52.40 using 59 PHA bins.
# Reduced chi-squared = 0.9528 for 55 degrees of freedom
# Null hypothesis probability = 5.744614e-01
Photon flux (15-150 keV) in 64 sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 1.69884e-07 ( 0 0 ) ergs/cm2
Single BB
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 7.36161 (-2.02821 2.69285)
R^2/D10^2 : 9.33164E-02 (-0.0933158 0.248164)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 52.57 using 59 PHA bins.
# Reduced chi-squared = 0.9223 for 57 degrees of freedom
# Null hypothesis probability = 6.418165e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.462e-08 3.360e-08
25- 50 8.232e-08 5.136e-08
50-150 1.631e-08 1.350e-08
15-150 1.532e-07 9.693e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 36.2334 (-18.4778 58.9902)
Norm : 0.402276 (-0.176851 0.360554)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 53.08 using 59 PHA bins.
# Reduced chi-squared = 0.9312 for 57 degrees of freedom
# Null hypothesis probability = 6.230110e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.703e-08 3.201e-08
25- 50 7.176e-08 4.416e-08
50-150 4.965e-08 4.083e-08
15-150 1.784e-07 1.147e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.10857 (-5.16558 -5.16558)
R1^2/D10^2 : 0.195720 (-0.191014 -0.191014)
kT2 [keV] : 9.67646 (-9.94609 -9.94609)
R2^2/D10^2 : 1.94986E-02 (-0.0157638 0.303469)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 52.32 using 59 PHA bins.
# Reduced chi-squared = 0.9513 for 55 degrees of freedom
# Null hypothesis probability = 5.776397e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.668e-08 7.216e-08
25- 50 7.859e-08 8.813e-08
50-150 2.747e-08 3.376e-08
15-150 1.627e-07 1.924e-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: 2.25955 ( -0.556537 0.691216 )
Norm@50keV : 3.32686E-04 ( -0.000158874 0.000161607 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 54.29 using 59 PHA bins.
# Reduced chi-squared = 0.9524 for 57 degrees of freedom
# Null hypothesis probability = 5.774336e-01
Photon flux (15-150 keV) in 64 sec: 5.68562E-02 ( -0.0178092 0.017891 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.01981e-07 ( -7.85056e-08 8.88704e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -0.113207 ( -6.68151 2.62208 )
Epeak [keV] : 28.2642 ( )
Norm@50keV : 1.35925E-02 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 52.43 using 59 PHA bins.
# Reduced chi-squared = 0.9363 for 56 degrees of freedom
# Null hypothesis probability = 6.106637e-01
Photon flux (15-150 keV) in 64 sec: 5.48030E-02 ( -0.0166813 0.017151 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.6017e-07 ( -5.77152e-08 9.27667e-08 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 0.581257 ( -2.89292 -0.0382335 )
beta : -10.0000 ( 10 1.77636e-15 )
Epeak [keV] : 28.4879 ( -8.86442 240.009 )
Norm@50keV : 2.87759E-02 ( -0.0293105 21.3389 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 52.40 using 59 PHA bins.
# Reduced chi-squared = 0.9528 for 55 degrees of freedom
# Null hypothesis probability = 5.744614e-01
Photon flux (15-150 keV) in 64 sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 1.69884e-07 ( 0 0 ) ergs/cm2
S(25-50 keV) vs. S(50-100 keV) plot
S(25-50 keV) = 6.48e-08
S(50-100 keV) = 5.41e-08
T90 vs. Hardness ratio plot
T90 = 64 sec.
Hardness ratio (energy fluence ratio) = 0.834877
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 0.740527
Count Ratio (50-100 keV) / (15-25 keV) = 0.110507
Mask shadow pattern
IMX = -4.025285114467173E-01, IMY = 2.030723226133307E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 64.000000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 64.000000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 64.000000
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] [']
135.5890 -40.5752 5.8 52.0 9.5 0.6270 2.0 3.0 Vela X-1
155.9361 -35.1688 2.3 38.2 -4.5 0.6924 5.0 ------ UNKNOWN
202.4115 -30.8044 2.8 43.4 -65.2 1.7732 4.1 ------ UNKNOWN
217.9011 11.6496 2.6 48.2 -129.4 1.9929 4.3 ------ UNKNOWN
208.4443 -16.1816 3.0 40.8 -88.3 1.6988 3.8 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
121.100600 764.200600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
149.2184 -15.2254 3.3 50.6 14.3 4.7136 3.5 ------ UNKNOWN
149.6709 -20.9737 4.0 53.8 8.2 4.9982 2.9 ------ UNKNOWN
184.4843 20.0416 3.0 6.9 91.7 1.3910 3.8 ------ UNKNOWN
225.8994 6.6943 2.7 36.3 -120.3 2.9025 4.4 ------ UNKNOWN
194.2035 -34.9680 3.6 50.6 -44.8 7.1762 3.2 ------ UNKNOWN
Plot creation:
Wed Nov 12 21:01:43 EST 2014