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Image
Pre-slew 15.0-350.0 keV image (Event data)
# RAcent DECcent POSerr Theta Phi Peak Cts SNR Name
184.0500 20.2252 0.0184 28.4810 125.5736 0.4459840 10.437 TRIG_00592204
Foreground time interval of the image:
2.244 11.676 (delta_t = 9.432 [sec])
Background time interval of the image:
-239.744 2.244 (delta_t = 241.988 [sec])
Lightcurves
Notes:
- 1) The mask-weighted light curves are using the flight position.
- 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 12.160000
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 12.160000
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 12.160000
SN=5 or 10 sec. binning (whichever binning is satisfied first)
SN=5 or 10 sec. binning (T < 200 sec)
Quad-rate summed light curves (from T0-300s to T0+1000s)
The mask-weighted light curves based on cleaned DPHs
Spectral Evolution
Spectra
Notes:
- 1) The fitting includes the systematic errors.
- 2) When the burst includes telescope slew time periods, the fitting uses an average response file made from multiple 5-s response files through out the slew time plus single time preiod for the non-slew times, and weighted by the total counts in the corresponding time period using addrmf. An average response file is needed becuase a spectral fit using 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.
Time averaged spectrum fit using the average DRM
Power-law model
Time interval is from 2.244 sec. to 11.676 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.34592 ( -0.279583 0.275889 )
Norm@50keV : 3.09471E-03 ( -0.00048326 0.000482605 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 54.96 using 59 PHA bins.
# Reduced chi-squared = 0.9642 for 57 degrees of freedom
# Null hypothesis probability = 5.519712e-01
Photon flux (15-150 keV) in 9.432 sec: 0.372512 ( -0.0598418 0.060068 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.85347e-07 ( -4.89791e-08 4.96445e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 2.244 sec. to 11.676 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.08584 ( -1.23954 1.57593 )
Epeak [keV] : 180.841 ( -180.868 -180.868 )
Norm@50keV : 4.16066E-03 ( -0.00151764 0.0122224 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 54.78 using 59 PHA bins.
# Reduced chi-squared = 0.9782 for 56 degrees of freedom
# Null hypothesis probability = 5.211698e-01
Photon flux (15-150 keV) in 9.432 sec: 0.367990 ( -0.062592 0.062479 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.7977e-07 ( -5.4948e-08 5.34898e-08 ) ergs/cm2
Band function
Time interval is from 2.244 sec. to 11.676 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 1.15580 ( -4.48025 -4.48025 )
beta : -1.52488 ( -0.401036 0.352094 )
Epeak [keV] : 40.7365 ( -46.2755 57.7162 )
Norm@50keV : 0.127710 ( -0.129551 38.5598 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 54.07 using 59 PHA bins.
# Reduced chi-squared = 0.9831 for 55 degrees of freedom
# Null hypothesis probability = 5.100968e-01
Photon flux (15-150 keV) in 9.432 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] : 16.6738 (-3.31681 4.32439)
R^2/D10^2 : 2.98190E-02 (-0.0161774 0.0342882)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 63.45 using 59 PHA bins.
# Reduced chi-squared = 1.113 for 57 degrees of freedom
# Null hypothesis probability = 2.596931e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.601e-08 5.340e-09
25- 50 6.973e-08 1.992e-08
50-150 1.375e-07 4.243e-08
15-150 2.233e-07 5.810e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 ( )
Norm : 1.54597 (-0.241777 0.241754)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 56.30 using 59 PHA bins.
# Reduced chi-squared = 0.9877 for 57 degrees of freedom
# Null hypothesis probability = 5.014124e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.631e-08 2.092e-08
25- 50 6.985e-08 3.923e-08
50-150 1.532e-07 8.531e-08
15-150 2.594e-07 1.472e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 8.01170 (-3.05423 4.88153)
R1^2/D10^2 : 0.235453 (-0.175818 0.374159)
kT2 [keV] : 31.4851 (-11.986 -31.6715)
R2^2/D10^2 : 2.75382E-03 (-0.00270183 0.00746913)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 54.01 using 59 PHA bins.
# Reduced chi-squared = 0.9820 for 55 degrees of freedom
# Null hypothesis probability = 5.124188e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.971e-08 1.758e-08
25- 50 6.986e-08 3.857e-08
50-150 1.806e-07 1.019e-07
15-150 2.801e-07 1.448e-07
Peak spectrum fit
Power-law model
Time interval is from 5.480 sec. to 6.480 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.00886 ( -0.604807 0.514144 )
Norm@50keV : 4.65914E-03 ( -0.0015134 0.00146615 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 87.56 using 59 PHA bins.
# Reduced chi-squared = 1.536 for 57 degrees of freedom
# Null hypothesis probability = 5.733856e-03
Photon flux (15-150 keV) in 1 sec: 0.535533 ( -0.172249 0.177499 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.02238e-08 ( -1.58007e-08 1.59888e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 5.480 sec. to 6.480 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.619272 ( -2.666 -0.634507 )
Epeak [keV] : 187.722 ( -192.874 -192.874 )
Norm@50keV : 7.20588E-03 ( -0.00384588 0.159319 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 87.44 using 59 PHA bins.
# Reduced chi-squared = 1.561 for 56 degrees of freedom
# Null hypothesis probability = 4.564631e-03
Photon flux (15-150 keV) in 1 sec: 0.530709 ( -0.174074 0.17864 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.89721e-08 ( -1.8294e-08 1.69038e-08 ) ergs/cm2
Band function
Time interval is from 5.480 sec. to 6.480 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 4.95747 ( -4.95747 -4.95747 )
beta : -1.48445 ( -1.21353 0.773161 )
Epeak [keV] : 38.0813 ( -38.0813 38.4237 )
Norm@50keV : 32.7530 ( -9.51484 833511 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 84.98 using 59 PHA bins.
# Reduced chi-squared = 1.545 for 55 degrees of freedom
# Null hypothesis probability = 5.853914e-03
Photon flux (15-150 keV) in 1 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] : 19.4271 (-7.58471 16.9033)
R^2/D10^2 : 2.79783E-02 (-0.027665 0.120033)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 89.52 using 59 PHA bins.
# Reduced chi-squared = 1.571 for 57 degrees of freedom
# Null hypothesis probability = 3.841080e-03
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.059e-09 1.326e-09
25- 50 1.005e-08 6.285e-09
50-150 2.801e-08 1.820e-08
15-150 4.012e-08 2.421e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.363 (-99.6773 -199.363)
Norm : 2.29245 (-0.728923 0.728922)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 90.28 using 59 PHA bins.
# Reduced chi-squared = 1.584 for 57 degrees of freedom
# Null hypothesis probability = 3.280977e-03
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.708e-09 3.622e-09
25- 50 1.098e-08 6.605e-09
50-150 2.408e-08 1.479e-08
15-150 4.077e-08 2.571e-08
Double BB
------------------------------------------------------------
#Fit statistic : Chi-Squared = 89.52 using 59 PHA bins.
#Fit statistic : Chi-Squared = 85.27 using 59 PHA bins.
#Fit statistic : Chi-Squared = 85.25 using 59 PHA bins.
#Fit statistic : Chi-Squared = 85.21 using 59 PHA bins.
# Reduced chi-squared = 1.628 for 55 degrees of freedom
# Reduced chi-squared = 1.550 for 55 degrees of freedom
# Reduced chi-squared = 1.550 for 55 degrees of freedom
# Reduced chi-squared = 1.549 for 55 degrees of freedom
# Null hypothesis probability = 2.249944e-03
# Null hypothesis probability = 5.518267e-03
# Null hypothesis probability = 5.540766e-03
# Null hypothesis probability = 5.583155e-03
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 0.000e+00 0.000e+00
25- 50 0.000e+00 0.000e+00
50-150 0.000e+00 0.000e+00
15-150 0.000e+00 0.000e+00
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: 1.34592 ( -0.279583 0.275889 )
Norm@50keV : 3.09471E-03 ( -0.00048326 0.000482605 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 54.96 using 59 PHA bins.
# Reduced chi-squared = 0.9642 for 57 degrees of freedom
# Null hypothesis probability = 5.519712e-01
Photon flux (15-150 keV) in 9.432 sec: 0.372512 ( -0.0598418 0.060068 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.85347e-07 ( -4.89791e-08 4.96445e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.08584 ( -1.23954 1.57593 )
Epeak [keV] : 180.841 ( -180.868 -180.868 )
Norm@50keV : 4.16066E-03 ( -0.00151764 0.0122224 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 54.78 using 59 PHA bins.
# Reduced chi-squared = 0.9782 for 56 degrees of freedom
# Null hypothesis probability = 5.211698e-01
Photon flux (15-150 keV) in 9.432 sec: 0.367990 ( -0.062592 0.062479 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.7977e-07 ( -5.4948e-08 5.34898e-08 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 1.15580 ( -4.48025 -4.48025 )
beta : -1.52488 ( -0.401036 0.352094 )
Epeak [keV] : 40.7365 ( -46.2755 57.7162 )
Norm@50keV : 0.127710 ( -0.129551 38.5532 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 54.07 using 59 PHA bins.
# Reduced chi-squared = 0.9831 for 55 degrees of freedom
# Null hypothesis probability = 5.100968e-01
Photon flux (15-150 keV) in 9.432 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) = 6.52e-08
S(50-100 keV) = 1.03e-07
T90 vs. Hardness ratio plot
T90 = 7.6039999127388 sec.
Hardness ratio (energy fluence ratio) = 1.57975
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.73417
Count Ratio (50-100 keV) / (15-25 keV) = 1.3373
Mask shadow pattern
IMX = -3.156132590397236E-01, IMY = -4.412741659074138E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 12.160000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 12.160000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 12.160000
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:
-239.744000 2.244000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
244.9761 -15.6424 0.3 50.4 -0.1 19.1982 38.7 0.2 Sco X-1
254.6136 35.4387 21.7 35.9 -77.2 0.3152 0.5 9.6 Her X-1
168.5806 15.7407 2.5 43.9 126.0 3.5909 4.5 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
2.244000 11.676000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
245.0505 -15.5720 7.4 50.4 -0.2 -0.1150 -1.6 5.8 Sco X-1
254.3658 35.2148 6.8 35.6 -76.8 0.1058 1.7 8.9 Her X-1
214.5084 -15.0494 2.1 40.2 39.3 0.3433 5.5 ------ UNKNOWN
184.0500 20.2252 1.1 28.5 125.6 0.4460 10.4 ------ UNKNOWN
148.8855 65.8535 2.3 57.3 -167.1 0.6685 5.1 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
113.356600 303.756630
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
149.1948 -7.0848 2.7 43.8 126.0 2.7197 4.3 ------ UNKNOWN
177.0434 17.8846 2.6 7.0 142.8 0.5963 4.4 ------ UNKNOWN
203.7684 10.1449 2.8 21.5 6.1 0.5617 4.2 ------ UNKNOWN
122.0316 25.7163 3.7 56.9 179.2 3.0381 3.2 ------ UNKNOWN
119.7489 30.1534 4.1 58.3 -175.3 2.7915 2.8 ------ UNKNOWN
119.2978 32.6269 2.7 58.5 -172.4 4.1924 4.3 ------ UNKNOWN
Plot creation:
Sat May 30 14:01:43 EDT 2015