Special notes of this burst
Image
Pre-slew 15.0-350.0 keV image (Event data)
# RAcent DECcent POSerr Theta Phi Peak Cts SNR Name
33.4936 -73.5482 0.0450 6.0638 91.9942 0.3034612 4.256 TRIG_00257741
Foreground time interval of the image:
0.000 64.000 (delta_t = 64.000 [sec])
Background time interval of the image:
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 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)
Quad-rate summed light curves (from T0-300s to T0+1000s)
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 0.000 sec. to 64.000 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.88105 ( -0.467696 0.537371 )
Norm@50keV : 2.74146E-04 ( -0.000106895 0.0001081 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 57.59 using 59 PHA bins.
# Reduced chi-squared = 1.010 for 57 degrees of freedom
# Null hypothesis probability = 4.530562e-01
Photon flux (15-150 keV) in 64 sec: 3.90383E-02 ( -0.0126674 0.0126817 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.61865e-07 ( -6.08434e-08 6.59955e-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: -7.01104 ( )
Epeak [keV] : 33.4600 ( -4.60292 5.9848 )
Norm@50keV : 170.039 ( -187.559 22949.8 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 46.27 using 59 PHA bins.
# Reduced chi-squared = 0.8263 for 56 degrees of freedom
# Null hypothesis probability = 8.197742e-01
Photon flux (15-150 keV) in 64 sec: 3.72834E-02 ( -0.0108452 0.0114898 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.17266e-07 ( -3.5369e-08 4.22502e-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 : 5.00000 ( -3.91092 -5 )
beta : -6.52331 ( 6.51029 15.7261 )
Epeak [keV] : 34.4303 ( -6.52214 6.13091 )
Norm@50keV : 7.83853 ( -2.12497 21.3929 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 46.52 using 59 PHA bins.
# Reduced chi-squared = 0.8458 for 55 degrees of freedom
# Null hypothesis probability = 7.852043e-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] : 9.35875 (-1.9317 2.57899)
R^2/D10^2 : 2.83900E-02 (-0.0175342 0.039736)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 48.81 using 59 PHA bins.
# Reduced chi-squared = 0.8563 for 57 degrees of freedom
# Null hypothesis probability = 7.715464e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.158e-08 1.888e-08
25- 50 7.126e-08 4.234e-08
50-150 3.060e-08 2.225e-08
15-150 1.334e-07 7.629e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 60.1548 (-31.041 127.209)
Norm : 0.213737 (-0.0811356 0.117621)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 55.01 using 59 PHA bins.
# Reduced chi-squared = 0.9650 for 57 degrees of freedom
# Null hypothesis probability = 5.501889e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.439e-08 2.119e-08
25- 50 5.239e-08 3.126e-08
50-150 5.974e-08 5.619e-08
15-150 1.465e-07 9.885e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 9.81690E-02 (-0.098169 -0.098169)
R1^2/D10^2 : 8.73608E-05 (-8.7361e-05 -8.7361e-05)
kT2 [keV] : 9.35900 (-1.93151 2.57918)
R2^2/D10^2 : 2.83872E-02 (-0.0175364 0.0397339)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 48.81 using 59 PHA bins.
# Reduced chi-squared = 0.8875 for 55 degrees of freedom
# Null hypothesis probability = 7.087276e-01
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: 1.88105 ( -0.467696 0.537371 )
Norm@50keV : 2.74146E-04 ( -0.000106895 0.0001081 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 57.59 using 59 PHA bins.
# Reduced chi-squared = 1.010 for 57 degrees of freedom
# Null hypothesis probability = 4.530562e-01
Photon flux (15-150 keV) in 64 sec: 3.90383E-02 ( -0.0126674 0.0126817 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.61865e-07 ( -6.08434e-08 6.59955e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -7.01104 ( )
Epeak [keV] : 33.4600 ( -4.60292 5.9848 )
Norm@50keV : 170.039 ( -187.559 22949.8 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 46.27 using 59 PHA bins.
# Reduced chi-squared = 0.8263 for 56 degrees of freedom
# Null hypothesis probability = 8.197742e-01
Photon flux (15-150 keV) in 64 sec: 3.72834E-02 ( -0.0108452 0.0114898 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.17266e-07 ( -3.5369e-08 4.22502e-08 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 5.00000 ( -3.91092 -5 )
beta : -6.52331 ( 6.51029 15.7261 )
Epeak [keV] : 34.4303 ( -6.52214 6.13091 )
Norm@50keV : 7.83853 ( -2.12497 21.3929 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 46.52 using 59 PHA bins.
# Reduced chi-squared = 0.8458 for 55 degrees of freedom
# Null hypothesis probability = 7.852043e-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) = 4.68e-08
S(50-100 keV) = 5.11e-08
T90 vs. Hardness ratio plot
T90 = 64 sec.
Hardness ratio (energy fluence ratio) = 1.09188
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 2.08272
Count Ratio (50-100 keV) / (15-25 keV) = 0.285186
Mask shadow pattern
IMX = -3.696553962752156E-03, IMY = -1.061658211320078E-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] [']
170.4266 -60.6116 3.5 45.4 153.4 0.6279 3.3 3.3 Cen X-3
186.6532 -62.7872 3.3 44.0 164.6 0.5122 3.5 1.0 GX 301-2
109.3823 -60.3717 2.2 35.5 110.6 0.8255 5.2 ------ UNKNOWN
29.6503 -24.0322 2.4 50.0 9.1 0.9718 4.7 ------ UNKNOWN
192.4051 -68.5243 2.9 38.3 168.4 0.4529 4.0 ------ UNKNOWN
303.8718 -45.1568 2.6 41.1 -97.9 1.5760 4.4 ------ UNKNOWN
299.4074 -46.0624 2.3 41.5 -102.8 1.7508 5.1 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
101.700600 433.400600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
170.7415 -60.6154 15.6 42.9 151.8 0.3443 0.7 12.5 Cen X-3
186.4108 -62.7337 4.8 42.6 163.2 1.0049 2.4 7.1 GX 301-2
60.5168 -31.0626 2.2 44.7 34.8 2.5561 5.2 ------ UNKNOWN
46.5644 -66.1244 2.4 8.6 38.9 0.8651 4.9 ------ UNKNOWN
325.6008 -62.0932 3.0 26.2 -99.5 1.1032 3.9 ------ UNKNOWN
Plot creation:
Sun May 31 10:59:29 EDT 2015