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
207.5151 7.4922 0.0077 10.0972 -1.6013 2.4510182 24.927 TRIG_00302728
Foreground time interval of the image:
5.160 73.901 (delta_t = 68.741 [sec])
Background time interval of the image:
-132.499 5.160 (delta_t = 137.659 [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 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 5.160 sec. to 332.892 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.56063 ( -0.0580422 0.0581782 )
Norm@50keV : 2.07582E-03 ( -6.40214e-05 6.39756e-05 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 63.51 using 59 PHA bins.
# Reduced chi-squared = 1.114 for 57 degrees of freedom
# Null hypothesis probability = 2.579988e-01
Photon flux (15-150 keV) in 327.7 sec: 0.263602 ( -0.00865568 0.00867797 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.39434e-06 ( -2.1087e-07 2.11436e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from 5.160 sec. to 332.892 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.24559 ( -0.243782 0.230913 )
Epeak [keV] : 124.610 ( -32.9227 180.416 )
Norm@50keV : 2.93960E-03 ( -0.000645791 0.000883942 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 57.99 using 59 PHA bins.
# Reduced chi-squared = 1.035 for 56 degrees of freedom
# Null hypothesis probability = 4.019365e-01
Photon flux (15-150 keV) in 327.7 sec: 0.257646 ( -0.009587 0.009614 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.23338e-06 ( -2.43186e-07 2.42203e-07 ) ergs/cm2
Band function
Time interval is from 5.160 sec. to 332.892 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.14532 ( -0.319112 3.40896 )
beta : -1.77411 ( 1.77261 0.202818 )
Epeak [keV] : 99.4381 ( -71.2399 175.15 )
Norm@50keV : 3.35658E-03 ( -0.00102316 0.00714598 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 57.76 using 59 PHA bins.
# Reduced chi-squared = 1.050 for 55 degrees of freedom
# Null hypothesis probability = 3.737917e-01
Photon flux (15-150 keV) in 327.7 sec: 0.256978 ( 6.74302 -0.009748 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.2537e-06 ( 0 0 ) ergs/cm2
Single BB
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 15.3509 ( )
R^2/D10^2 : 2.61594E-02 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 256.70 using 59 PHA bins.
# Reduced chi-squared = 4.5036 for 57 degrees of freedom
# Null hypothesis probability = 3.831207e-27
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.212e-07 2.409e-08
25- 50 1.709e-06 7.046e-08
50-150 2.769e-06 1.742e-07
15-150 4.899e-06 1.819e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 ( )
Norm : 1.06468 (-0.0324351 0.0324351)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 58.05 using 59 PHA bins.
# Reduced chi-squared = 1.019 for 57 degrees of freedom
# Null hypothesis probability = 4.362211e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.696e-07 2.966e-08
25- 50 1.673e-06 5.882e-08
50-150 3.668e-06 1.180e-07
15-150 6.210e-06 2.081e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.20254 (-0.856785 0.936096)
R1^2/D10^2 : 0.238153 (-0.0781087 0.131177)
kT2 [keV] : 25.6346 (-2.73191 3.81611)
R2^2/D10^2 : 3.40113E-03 (-0.00136005 0.00181373)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 62.22 using 59 PHA bins.
# Reduced chi-squared = 1.131 for 55 degrees of freedom
# Null hypothesis probability = 2.347913e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.948e-07 8.274e-08
25- 50 1.689e-06 1.080e-07
50-150 3.678e-06 3.887e-07
15-150 6.162e-06 5.145e-07
Peak spectrum fit
Power-law model
Time interval is from 330.336 sec. to 331.336 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.41749 ( -0.485512 0.480682 )
Norm@50keV : 8.99247E-03 ( -0.0025251 0.00252489 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 42.66 using 59 PHA bins.
# Reduced chi-squared = 0.7484 for 57 degrees of freedom
# Null hypothesis probability = 9.210333e-01
Photon flux (15-150 keV) in 1 sec: 1.09967 ( -0.326164 0.329109 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.65869e-08 ( -2.56351e-08 2.58598e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 330.336 sec. to 331.336 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.988934 ( -2.66714 1.45598 )
Epeak [keV] : 127.383 ( -127.396 -127.396 )
Norm@50keV : 1.44246E-02 ( -0.00782789 0.231688 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 42.50 using 59 PHA bins.
# Reduced chi-squared = 0.7590 for 56 degrees of freedom
# Null hypothesis probability = 9.083438e-01
Photon flux (15-150 keV) in 1 sec: 1.08315 ( -0.334334 0.3362 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.51769e-08 ( -2.74174e-08 2.66461e-08 ) ergs/cm2
Band function
Time interval is from 330.336 sec. to 331.336 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 4.10891 ( 0.775158 0.775158 )
beta : -1.55509 ( 1.70651 0.751225 )
Epeak [keV] : 29.4786 ( -89.2371 -89.2371 )
Norm@50keV : 83.1287 ( -83.2386 94.776 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 42.12 using 59 PHA bins.
# Reduced chi-squared = 0.7658 for 55 degrees of freedom
# Null hypothesis probability = 8.988564e-01
Photon flux (15-150 keV) in 1 sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 8.48713e-08 ( 0 0 ) ergs/cm2
Single BB
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 16.9785 (-5.20796 7.96643)
R^2/D10^2 : 8.42341E-02 (-0.0839803 0.216585)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 44.94 using 59 PHA bins.
# Reduced chi-squared = 0.7884 for 57 degrees of freedom
# Null hypothesis probability = 8.763585e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.947e-09 3.131e-09
25- 50 2.187e-08 1.310e-08
50-150 4.499e-08 3.021e-08
15-150 7.180e-08 4.047e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.363 (-118.242 -199.363)
Norm : 4.60589 (-1.2962 1.2964)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 42.81 using 59 PHA bins.
# Reduced chi-squared = 0.7511 for 57 degrees of freedom
# Null hypothesis probability = 9.184288e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.147e-08 7.000e-09
25- 50 2.206e-08 1.358e-08
50-150 4.839e-08 2.843e-08
15-150 8.192e-08 4.928e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.28324 (-7.44613 -7.44613)
R1^2/D10^2 : 0.860394 (-0.807151 -0.807151)
kT2 [keV] : 25.8820 (-27.1877 -27.1877)
R2^2/D10^2 : 1.50458E-02 (-0.0128239 0.115821)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 42.59 using 59 PHA bins.
# Reduced chi-squared = 0.7743 for 55 degrees of freedom
# Null hypothesis probability = 8.890731e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 9.344e-09 5.895e-09
25- 50 2.119e-08 1.167e-08
50-150 5.114e-08 3.295e-08
15-150 8.167e-08 4.570e-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: 1.33326 ( -0.0907183 0.0904045 )
Norm@50keV : 2.32853E-03 ( -0.000118606 0.000118557 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 53.08 using 59 PHA bins.
# Reduced chi-squared = 0.9312 for 57 degrees of freedom
# Null hypothesis probability = 6.229082e-01
Photon flux (15-150 keV) in 68.74 sec: 0.279574 ( -0.0146478 0.0146666 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.56927e-06 ( -8.88698e-08 8.93104e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.955745 ( -0.380002 0.34841 )
Epeak [keV] : 144.319 ( -47.7329 751.907 )
Norm@50keV : 3.54954E-03 ( -0.00111733 0.0018029 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 49.62 using 59 PHA bins.
# Reduced chi-squared = 0.8861 for 56 degrees of freedom
# Null hypothesis probability = 7.134071e-01
Photon flux (15-150 keV) in 68.74 sec: 0.274111 ( -0.015491 0.015474 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.52505e-06 ( -9.88275e-08 9.85732e-08 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.958875 ( -0.345114 0.233569 )
beta : -7.01254 ( 4.59903 14.599 )
Epeak [keV] : 145.052 ( -108.887 700.9 )
Norm@50keV : 3.53720E-03 ( -0.000385067 0.000641114 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 49.62 using 59 PHA bins.
# Reduced chi-squared = 0.9023 for 55 degrees of freedom
# Null hypothesis probability = 6.794535e-01
Photon flux (15-150 keV) in 68.74 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) = 1.63e-06
S(50-100 keV) = 2.21e-06
T90 vs. Hardness ratio plot
T90 = 292.460000008345 sec.
Hardness ratio (energy fluence ratio) = 1.35583
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.31717
Count Ratio (50-100 keV) / (15-25 keV) = 0.951998
Mask shadow pattern
IMX = 1.780072672979531E-01, IMY = 4.976312632555476E-03
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:
-132.499410 5.160000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
195.1665 -18.7174 2.3 38.1 20.0 0.9055 5.0 ------ UNKNOWN
230.1360 48.8030 2.5 36.5 -152.4 0.7072 4.7 ------ UNKNOWN
230.0218 27.7371 2.2 23.6 -117.9 0.6990 5.2 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
5.160000 73.900590
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
173.9871 14.1515 2.2 31.8 90.4 0.9860 5.3 ------ UNKNOWN
207.5151 7.4923 0.5 10.1 -1.6 2.4510 24.9 ------ UNKNOWN
242.9278 3.0138 2.1 38.2 -70.0 1.2185 5.5 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
112.100600 194.900590
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.4207 35.2741 5.1 51.1 -143.2 -0.7884 -2.2 4.5 Her X-1
174.0160 34.5251 3.5 41.0 122.9 1.1335 3.3 ------ UNKNOWN
171.3349 -3.9961 2.0 37.9 60.3 1.5004 5.8 ------ UNKNOWN
207.5084 7.4818 0.3 0.0 -28.9 3.3205 34.7 ------ UNKNOWN
208.5433 -45.3028 2.0 52.8 -14.1 1.5424 5.8 ------ UNKNOWN
227.6220 -39.2160 2.3 50.3 -33.5 1.4511 5.1 ------ UNKNOWN
248.2060 2.2147 2.4 40.9 -97.9 2.0214 4.9 ------ UNKNOWN
Plot creation:
Sun May 31 08:25:04 EDT 2015