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
144.9980 -65.8270 0.0129 16.2015 86.8548 1.3689639 14.817 TRIG_00595608
Foreground time interval of the image:
-31.632 16.368 (delta_t = 48.000 [sec])
Background time interval of the image:
-239.632 -31.632 (delta_t = 208.000 [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 1.024000
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 1.024000
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 1.024000
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 -31.632 sec. to 16.368 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.02873 ( -0.183636 0.192586 )
Norm@50keV : 1.59922E-03 ( -0.000198339 0.000193558 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 36.25 using 59 PHA bins.
# Reduced chi-squared = 0.6359 for 57 degrees of freedom
# Null hypothesis probability = 9.854623e-01
Photon flux (15-150 keV) in 48 sec: 0.243108 ( -0.0223996 0.0224053 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.09094e-07 ( -8.0375e-08 8.22504e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -31.632 sec. to 16.368 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.99884 ( )
Epeak [keV] : 5.18608 ( )
Norm@50keV : 1.63517E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 36.31 using 59 PHA bins.
# Reduced chi-squared = 0.6484 for 56 degrees of freedom
# Null hypothesis probability = 9.809344e-01
Photon flux (15-150 keV) in 48 sec: 0.243105 ( -0.022513 0.022335 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.07371e-07 ( -8.80368e-08 8.24544e-08 ) ergs/cm2
Band function
Time interval is from -31.632 sec. to 16.368 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.39206 ( 1.39289 1.39289 )
beta : -2.12948 ( 2.13061 0.272991 )
Epeak [keV] : 29.3464 ( -29.4121 33.1641 )
Norm@50keV : 4.30533E-03 ( -0.00431348 1105.55 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 35.88 using 59 PHA bins.
# Reduced chi-squared = 0.6524 for 55 degrees of freedom
# Null hypothesis probability = 9.785846e-01
Photon flux (15-150 keV) in 48 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] : 8.86777 (-0.932803 1.06144)
R^2/D10^2 : 0.173857 (-0.062297 0.0957885)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 61.89 using 59 PHA bins.
# Reduced chi-squared = 1.086 for 57 degrees of freedom
# Null hypothesis probability = 3.059746e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.268e-07 1.939e-08
25- 50 2.632e-07 3.394e-08
50-150 9.595e-08 2.602e-08
15-150 4.860e-07 5.791e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 61.2434 (-16.516 26.9365)
Norm : 1.24760 (-0.197907 0.236576)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 39.58 using 59 PHA bins.
# Reduced chi-squared = 0.6944 for 57 degrees of freedom
# Null hypothesis probability = 9.617542e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.510e-07 2.016e-08
25- 50 2.312e-07 2.362e-08
50-150 2.676e-07 6.427e-08
15-150 6.499e-07 8.880e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.37503 (-1.20046 1.11052)
R1^2/D10^2 : 0.324696 (-0.0795166 0.150664)
kT2 [keV] : 72.1857 (-45.9192 -73.2094)
R2^2/D10^2 : 1.29818E-04 (-0.000108042 0.00152563)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 33.90 using 59 PHA bins.
# Reduced chi-squared = 0.6163 for 55 degrees of freedom
# Null hypothesis probability = 9.887892e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.459e-07 3.029e-08
25- 50 2.370e-07 4.812e-08
50-150 3.770e-07 1.999e-07
15-150 7.600e-07 2.419e-07
Peak spectrum fit
Power-law model
Time interval is from 7.868 sec. to 8.868 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.12821 ( -0.436474 0.509962 )
Norm@50keV : 3.85864E-03 ( -0.00134956 0.00130482 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 47.97 using 59 PHA bins.
# Reduced chi-squared = 0.8416 for 57 degrees of freedom
# Null hypothesis probability = 7.972031e-01
Photon flux (15-150 keV) in 1 sec: 0.615654 ( -0.149379 0.149444 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.59556e-08 ( -1.07715e-08 1.15255e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 7.868 sec. to 8.868 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.432136 ( -4.2298 1.66972 )
Epeak [keV] : 33.6255 ( -33.6259 -33.6259 )
Norm@50keV : 4.46847E-02 ( -0.044732 22.432 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 46.65 using 59 PHA bins.
# Reduced chi-squared = 0.8331 for 56 degrees of freedom
# Null hypothesis probability = 8.089062e-01
Photon flux (15-150 keV) in 1 sec: 0.590946 ( -0.14992 0.15225 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.06608e-08 ( -9.3177e-09 1.35527e-08 ) ergs/cm2
Band function
Time interval is from 7.868 sec. to 8.868 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 8.18682E-02 ( -0.298218 -0.298218 )
beta : -3.28975 ( 3.34299 1.51934 )
Epeak [keV] : 32.9897 ( -33.0149 14.0852 )
Norm@50keV : 9.85293E-02 ( -0.0950553 559.03 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 46.53 using 59 PHA bins.
# Reduced chi-squared = 0.8461 for 55 degrees of freedom
# Null hypothesis probability = 7.847203e-01
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] : 8.72394 (-1.89403 2.4508)
R^2/D10^2 : 0.504584 (-0.315752 0.811748)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 47.46 using 59 PHA bins.
# Reduced chi-squared = 0.8326 for 57 degrees of freedom
# Null hypothesis probability = 8.121532e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.351e-09 3.955e-09
25- 50 1.487e-08 7.127e-09
50-150 5.153e-09 3.676e-09
15-150 2.737e-08 1.252e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 48.1398 (-22.0031 62.3938)
Norm : 3.61294 (-1.24904 2.06182)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 46.93 using 59 PHA bins.
# Reduced chi-squared = 0.8234 for 57 degrees of freedom
# Null hypothesis probability = 8.267753e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.755e-09 3.135e-09
25- 50 1.240e-08 4.948e-09
50-150 1.161e-08 8.285e-09
15-150 3.277e-08 1.260e-08
Double BB
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 1.23478 (-1.63679 8.86188)
R1^2/D10^2 : 1.74596E+04 ( )
kT2 [keV] : 9.29226 (-2.16796 -9.28486)
R2^2/D10^2 : 0.377944 (-0.38074 0.709405)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 46.30 using 59 PHA bins.
#Fit statistic : Chi-Squared = 46.27 using 59 PHA bins.
# Reduced chi-squared = 0.8418 for 55 degrees of freedom
# Reduced chi-squared = 0.8413 for 55 degrees of freedom
# Null hypothesis probability = 7.919620e-01
# Null hypothesis probability = 7.929185e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.608e-09 3.954e-09
25- 50 1.424e-08 8.505e-09
50-150 6.274e-09 4.234e-09
15-150 2.813e-08 1.620e-08
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: 2.02873 ( -0.183636 0.192586 )
Norm@50keV : 1.59922E-03 ( -0.000198339 0.000193558 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 36.25 using 59 PHA bins.
# Reduced chi-squared = 0.6359 for 57 degrees of freedom
# Null hypothesis probability = 9.854623e-01
Photon flux (15-150 keV) in 48 sec: 0.243108 ( -0.0223996 0.0224053 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.09094e-07 ( -8.0375e-08 8.22504e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.99884 ( )
Epeak [keV] : 5.18608 ( )
Norm@50keV : 1.63517E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 36.31 using 59 PHA bins.
# Reduced chi-squared = 0.6484 for 56 degrees of freedom
# Null hypothesis probability = 9.809344e-01
Photon flux (15-150 keV) in 48 sec: 0.243105 ( -0.022513 0.022335 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.07371e-07 ( -8.80368e-08 8.24544e-08 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.39206 ( 1.39289 1.39289 )
beta : -2.12948 ( 2.13061 0.272991 )
Epeak [keV] : 29.3464 ( -29.4121 33.1641 )
Norm@50keV : 4.30533E-03 ( -0.00431348 1105.55 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 35.88 using 59 PHA bins.
# Reduced chi-squared = 0.6524 for 55 degrees of freedom
# Null hypothesis probability = 9.785846e-01
Photon flux (15-150 keV) in 48 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) = 2.15e-07
S(50-100 keV) = 2.11e-07
T90 vs. Hardness ratio plot
T90 = 48 sec.
Hardness ratio (energy fluence ratio) = 0.981395
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.0335
Count Ratio (50-100 keV) / (15-25 keV) = 0.403458
Mask shadow pattern
IMX = 1.594155435631204E-02, IMY = -2.901177717198384E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.024000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.024000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.024000
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:
-239.632000 -31.632000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.5219 -40.5362 1.3 34.0 38.7 2.5973 8.8 1.1 Vela X-1
170.1627 -60.5802 3.5 28.1 96.0 0.9224 3.3 5.2 Cen X-3
186.5854 -62.7191 2.6 31.7 110.5 1.5031 4.4 3.6 GX 301-2
105.5157 -34.9459 2.4 35.0 -4.8 1.1201 4.8 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-31.632000 16.368000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.4719 -40.5221 9.5 34.0 38.6 0.1557 1.2 3.2 Vela X-1
170.6468 -60.5964 6.6 28.3 96.4 0.2216 1.7 9.9 Cen X-3
186.4859 -62.5774 0.0 31.8 110.3 0.2103 1.6 12.5 GX 301-2
123.1404 -23.7744 2.9 47.8 16.7 0.8250 4.0 ------ UNKNOWN
144.9974 -65.8257 0.8 16.2 86.9 1.3748 14.9 ------ UNKNOWN
104.2638 -13.6826 2.2 56.3 -7.0 1.6499 5.2 ------ UNKNOWN
78.9190 -27.9706 2.2 44.1 -39.6 0.8276 5.3 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
55.268590 962.438000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.5287 -40.5436 0.6 25.8 11.6 11.4972 20.2 0.7 Vela X-1
170.3329 -60.6772 2.0 12.4 105.7 3.1724 5.8 3.3 Cen X-3
186.6532 -62.7756 0.8 18.0 128.0 8.8767 14.1 0.3 GX 301-2
168.5307 -44.0429 2.3 25.3 70.5 3.7134 5.0 ------ UNKNOWN
120.3506 -73.2452 2.3 11.2 -113.6 2.7219 4.9 ------ UNKNOWN
Plot creation:
Sat May 30 13:53:25 EDT 2015