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Image
Pre-slew 15-350 keV image (Event data; bkg subtracted)
# RAcent DECcent POSerr Theta Phi Peak Cts SNR Name
54.3787 +53.1972 0.0221 41.0 -119.5 1.8906 8.7 TRIG_00650411
------------------------------------------
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: 4.47239 ( -0.818128 0.984438 )
Norm@50keV : 3.30643E-04 ( -0.000209814 0.000365674 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 80.31 using 59 PHA bins.
# Reduced chi-squared = 1.409 for 57 degrees of freedom
# Null hypothesis probability = 2.265005e-02
Photon flux (15-150 keV) in 64 sec: 0.311309 ( -0.0514846 0.0515026 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.70374e-07 ( -1.33058e-07 1.46586e-07 ) 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: 1.83025 ( )
Epeak [keV] : 1.21077 ( )
Norm@50keV : 6.34753E-02 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 84.23 using 59 PHA bins.
# Reduced chi-squared = 1.504 for 56 degrees of freedom
# Null hypothesis probability = 8.705066e-03
Photon flux (15-150 keV) in 64 sec: 0.310905 ( -0.051315 0.051619 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.54835e-07 ( 0 0 ) 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 : -6.53481 ( 6.53481 6.53481 )
beta : -4.47304 ( -0.985017 0.818585 )
Epeak [keV] : 12.2738 ( -12.2738 -12.2738 )
Norm@50keV : 4.49113E-02 ( -0.0284918 0.0497203 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 80.31 using 59 PHA bins.
# Reduced chi-squared = 1.460 for 55 degrees of freedom
# Null hypothesis probability = 1.461483e-02
Photon flux (15-150 keV) in 64 sec: 0.176920 ( ) 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] : 2.70772 (-0.452343 0.610869)
R^2/D10^2 : 81.8591 (-81.8592 222.962)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 86.35 using 59 PHA bins.
# Reduced chi-squared = 1.515 for 57 degrees of freedom
# Null hypothesis probability = 7.298855e-03
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.034e-07 2.741e-07
25- 50 5.055e-08 3.105e-08
50-150 3.385e-11 3.530e-11
15-150 5.540e-07 3.058e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 5.93120 (-1.71457 3.46838)
Norm : 38.6006 (-27.1504 89.2443)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 84.63 using 59 PHA bins.
# Reduced chi-squared = 1.485 for 57 degrees of freedom
# Null hypothesis probability = 1.020714e-02
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.953e-07 2.345e-07
25- 50 9.004e-08 4.867e-08
50-150 1.033e-09 1.021e-09
15-150 5.864e-07 2.436e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 2.19760 (-0.488515 0.555373)
R1^2/D10^2 : 303.838 (-240.808 1889.63)
kT2 [keV] : 9.93483 (-3.58089 7.9542)
R2^2/D10^2 : 5.68633E-02 (-0.0523514 0.181087)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 74.92 using 59 PHA bins.
# Reduced chi-squared = 1.362 for 55 degrees of freedom
# Null hypothesis probability = 3.829371e-02
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.692e-07 2.540e-07
25- 50 1.966e-07 1.196e-07
50-150 9.208e-08 7.485e-08
15-150 7.578e-07 3.894e-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: 4.47239 ( -0.818128 0.984438 )
Norm@50keV : 3.30643E-04 ( -0.000209814 0.000365674 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 80.31 using 59 PHA bins.
# Reduced chi-squared = 1.409 for 57 degrees of freedom
# Null hypothesis probability = 2.265005e-02
Photon flux (15-150 keV) in 64 sec: 0.311309 ( -0.0514846 0.0515026 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.70374e-07 ( -1.33058e-07 1.46586e-07 ) 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: 1.83025 ( )
Epeak [keV] : 1.21077 ( )
Norm@50keV : 6.34753E-02 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 84.23 using 59 PHA bins.
# Reduced chi-squared = 1.504 for 56 degrees of freedom
# Null hypothesis probability = 8.705066e-03
Photon flux (15-150 keV) in 64 sec: 0.310905 ( -0.051315 0.051619 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.54835e-07 ( 0 0 ) 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 : -6.53481 ( 6.53481 6.53481 )
beta : -4.47304 ( -0.985017 0.818585 )
Epeak [keV] : 12.2738 ( -12.2738 -12.2738 )
Norm@50keV : 4.49113E-02 ( -0.0284918 0.0497203 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 80.31 using 59 PHA bins.
# Reduced chi-squared = 1.460 for 55 degrees of freedom
# Null hypothesis probability = 1.461483e-02
Photon flux (15-150 keV) in 64 sec: 0.176920 ( ) 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] : 2.70772 (-0.452343 0.610869)
R^2/D10^2 : 81.8591 (-81.8592 222.962)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 86.35 using 59 PHA bins.
# Reduced chi-squared = 1.515 for 57 degrees of freedom
# Null hypothesis probability = 7.298855e-03
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.034e-07 2.785e-07
25- 50 5.055e-08 3.029e-08
50-150 3.385e-11 3.773e-11
15-150 5.540e-07 3.015e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 5.93120 (-1.71457 3.46838)
Norm : 38.6006 (-27.1504 89.2443)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 84.63 using 59 PHA bins.
# Reduced chi-squared = 1.485 for 57 degrees of freedom
# Null hypothesis probability = 1.020714e-02
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.953e-07 1.988e-07
25- 50 9.004e-08 5.207e-08
50-150 1.033e-09 1.067e-09
15-150 5.864e-07 2.679e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 2.19760 (-0.488515 0.555373)
R1^2/D10^2 : 303.838 (-240.808 1889.63)
kT2 [keV] : 9.93483 (-3.58089 7.9542)
R2^2/D10^2 : 5.68633E-02 (-0.0523514 0.181087)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 74.92 using 59 PHA bins.
# Reduced chi-squared = 1.362 for 55 degrees of freedom
# Null hypothesis probability = 3.829371e-02
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.692e-07 2.516e-07
25- 50 1.966e-07 1.233e-07
50-150 9.208e-08 7.014e-08
15-150 7.578e-07 4.038e-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: 4.47239 ( -0.818128 0.984438 )
Norm@50keV : 3.30643E-04 ( -0.000209814 0.000365674 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 80.31 using 59 PHA bins.
# Reduced chi-squared = 1.409 for 57 degrees of freedom
# Null hypothesis probability = 2.265005e-02
Photon flux (15-150 keV) in 64 sec: 0.311309 ( -0.0514846 0.0515026 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.70374e-07 ( -1.33058e-07 1.46586e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.83025 ( )
Epeak [keV] : 1.21077 ( )
Norm@50keV : 6.34753E-02 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 84.23 using 59 PHA bins.
# Reduced chi-squared = 1.504 for 56 degrees of freedom
# Null hypothesis probability = 8.705066e-03
Photon flux (15-150 keV) in 64 sec: 0.310905 ( -0.051315 0.051619 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.54835e-07 ( 0 0 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -6.53481 ( 6.53481 6.53481 )
beta : -4.47304 ( -0.985017 0.818585 )
Epeak [keV] : 12.2738 ( -12.2738 -12.2738 )
Norm@50keV : 4.49113E-02 ( -0.0284918 0.0497203 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 80.31 using 59 PHA bins.
# Reduced chi-squared = 1.460 for 55 degrees of freedom
# Null hypothesis probability = 1.461483e-02
Photon flux (15-150 keV) in 64 sec: 0.176920 ( ) 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) = 1.56e-07
S(50-100 keV) = 2.81e-08
T90 vs. Hardness ratio plot
T90 = 64 sec.
Hardness ratio (energy fluence ratio) = 0.180128
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 0.319103
Count Ratio (50-100 keV) / (15-25 keV) = 0.0599676
Mask shadow pattern
IMX = -4.285954717880360E-01, IMY = 7.576954428551287E-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] [']
326.0850 38.2249 7.2 46.7 149.6 0.4302 1.6 7.1 Cyg X-2
53.0046 -17.8506 3.1 53.0 -15.3 0.8342 3.7 ------ UNKNOWN
349.1283 74.2806 2.3 53.8 -161.6 1.1647 4.9 ------ UNKNOWN
54.3788 53.1972 1.3 41.0 -119.5 1.8903 8.7 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
130.700680 363.100000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.8496 22.1000 0.0 38.4 -49.6 0.9475 2.6 13.1 Crab
54.4233 53.2418 0.3 0.1 -127.4 7.9833 39.7 ------ UNKNOWN
208.6184 75.1673 2.1 50.5 -174.0 2.5078 5.4 ------ UNKNOWN
84.0521 21.9334 0.5 38.6 -49.8 9.5100 26.2 ------ UNKNOWN
Plot creation:
Mon Jul 27 22:00:19 EDT 2015