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
142.0319 14.5707 0.0094 38.1020 -60.1641 2.5010720 20.699 TRIG_00610953
Foreground time interval of the image:
-6.708 18.316 (delta_t = 25.024 [sec])
Background time interval of the image:
-239.496 -6.708 (delta_t = 232.788 [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)
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 -6.708 sec. to 18.316 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.72921 ( -0.123863 0.126522 )
Norm@50keV : 6.38423E-03 ( -0.000502301 0.000497927 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 65.25 using 59 PHA bins.
# Reduced chi-squared = 1.145 for 57 degrees of freedom
# Null hypothesis probability = 2.119278e-01
Photon flux (15-150 keV) in 25.02 sec: 0.856733 ( -0.0624457 0.0625025 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.47582e-06 ( -1.20433e-07 1.21503e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -6.708 sec. to 18.316 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.795101 ( -0.653584 0.570356 )
Epeak [keV] : 59.7894 ( -9.44257 24.3325 )
Norm@50keV : 2.01132E-02 ( -0.00998719 0.0241893 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 56.84 using 59 PHA bins.
# Reduced chi-squared = 1.015 for 56 degrees of freedom
# Null hypothesis probability = 4.435145e-01
Photon flux (15-150 keV) in 25.02 sec: 0.823137 ( -0.065606 0.065582 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.36932e-06 ( -1.32233e-07 1.35723e-07 ) ergs/cm2
Band function
Time interval is from -6.708 sec. to 18.316 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.821096 ( -0.591341 0.871479 )
beta : -2.57163 ( 2.65073 0.698199 )
Epeak [keV] : 59.6982 ( -14.6774 23.5146 )
Norm@50keV : 1.95654E-02 ( -0.0110669 0.0494816 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 56.65 using 59 PHA bins.
# Reduced chi-squared = 1.030 for 55 degrees of freedom
# Null hypothesis probability = 4.132374e-01
Photon flux (15-150 keV) in 25.02 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] : 12.7672 (-1.00474 1.09089)
R^2/D10^2 : 0.168799 (-0.0440658 0.0592687)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 81.03 using 59 PHA bins.
# Reduced chi-squared = 1.422 for 57 degrees of freedom
# Null hypothesis probability = 1.992856e-02
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.460e-07 2.033e-08
25- 50 4.931e-07 3.853e-08
50-150 5.027e-07 8.269e-08
15-150 1.142e-06 1.036e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 111.716 (-25.9488 46.5638)
Norm : 3.73674 (-0.352273 0.37464)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 58.83 using 59 PHA bins.
# Reduced chi-squared = 1.032 for 57 degrees of freedom
# Null hypothesis probability = 4.083972e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.441e-07 2.651e-08
25- 50 4.311e-07 3.978e-08
50-150 7.420e-07 2.595e-07
15-150 1.417e-06 2.798e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.27272 (-1.50945 2.15462)
R1^2/D10^2 : 2.08582 (-1.40948 5.2023)
kT2 [keV] : 16.9395 (-2.40492 4.47456)
R2^2/D10^2 : 4.93152E-02 (-0.0316567 0.0351866)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 56.70 using 59 PHA bins.
# Reduced chi-squared = 1.031 for 55 degrees of freedom
# Null hypothesis probability = 4.114747e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.284e-07 9.999e-08
25- 50 4.345e-07 1.416e-07
50-150 6.577e-07 1.948e-07
15-150 1.321e-06 3.301e-07
Peak spectrum fit
Power-law model
Time interval is from 0.496 sec. to 1.496 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.71495 ( -0.228024 0.239993 )
Norm@50keV : 1.67282E-02 ( -0.002673 0.00262152 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 56.09 using 59 PHA bins.
# Reduced chi-squared = 0.9840 for 57 degrees of freedom
# Null hypothesis probability = 5.092634e-01
Photon flux (15-150 keV) in 1 sec: 2.23343 ( -0.314539 0.314598 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.5471e-07 ( -2.54585e-08 2.5961e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.496 sec. to 1.496 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.800227 ( -1.07628 0.863975 )
Epeak [keV] : 60.2027 ( -16.1183 154.543 )
Norm@50keV : 5.27532E-02 ( -0.0527259 0.151758 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 52.73 using 59 PHA bins.
# Reduced chi-squared = 0.9417 for 56 degrees of freedom
# Null hypothesis probability = 5.992406e-01
Photon flux (15-150 keV) in 1 sec: 2.18315 ( -0.3173 0.31766 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.45468e-07 ( -2.6487e-08 2.7425e-08 ) ergs/cm2
Band function
Time interval is from 0.496 sec. to 1.496 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.798387 ( -0.54871 1.42034 )
beta : -10.0000 ( 10 7.10543e-15 )
Epeak [keV] : 60.1533 ( -16.019 153.39 )
Norm@50keV : 5.28787E-02 ( -0.0335034 0.151704 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 52.73 using 59 PHA bins.
# Reduced chi-squared = 0.9588 for 55 degrees of freedom
# Null hypothesis probability = 5.616566e-01
Photon flux (15-150 keV) in 1 sec: 2.19695 ( 4.80305 -0.30569 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.47693e-07 ( -1.47686e-07 -2.8787e-08 ) ergs/cm2
Single BB
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 12.1983 (-2.11214 2.5927)
R^2/D10^2 : 0.527113 (-0.264068 0.523722)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 62.33 using 59 PHA bins.
# Reduced chi-squared = 1.093 for 57 degrees of freedom
# Null hypothesis probability = 2.925073e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.661e-08 4.265e-09
25- 50 5.328e-08 1.115e-08
50-150 4.819e-08 1.595e-08
15-150 1.181e-07 2.417e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 117.026 (-46.4167 -115.988)
Norm : 9.65095 (-1.53038 1.99072)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 53.54 using 59 PHA bins.
# Reduced chi-squared = 0.9393 for 57 degrees of freedom
# Null hypothesis probability = 6.057627e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.516e-08 5.530e-09
25- 50 4.482e-08 1.342e-08
50-150 7.899e-08 4.754e-08
15-150 1.490e-07 7.024e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.27919 (-2.01884 2.58306)
R1^2/D10^2 : 3.56163 (-2.44657 11.7559)
kT2 [keV] : 20.5334 (-5.33122 10.3789)
R2^2/D10^2 : 5.91880E-02 (-0.0487578 0.144625)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 50.93 using 59 PHA bins.
# Reduced chi-squared = 0.9260 for 55 degrees of freedom
# Null hypothesis probability = 6.307686e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.462e-08 1.352e-08
25- 50 4.595e-08 2.378e-08
50-150 7.803e-08 4.416e-08
15-150 1.486e-07 7.770e-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: 1.72921 ( -0.123863 0.126522 )
Norm@50keV : 6.38423E-03 ( -0.000502301 0.000497927 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 65.25 using 59 PHA bins.
# Reduced chi-squared = 1.145 for 57 degrees of freedom
# Null hypothesis probability = 2.119278e-01
Photon flux (15-150 keV) in 25.02 sec: 0.856733 ( -0.0624457 0.0625025 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.47582e-06 ( -1.20433e-07 1.21503e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.795101 ( -0.653584 0.570356 )
Epeak [keV] : 59.7894 ( -9.44257 24.3325 )
Norm@50keV : 2.01132E-02 ( -0.00998719 0.0241893 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 56.84 using 59 PHA bins.
# Reduced chi-squared = 1.015 for 56 degrees of freedom
# Null hypothesis probability = 4.435145e-01
Photon flux (15-150 keV) in 25.02 sec: 0.823137 ( -0.065606 0.065582 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.36932e-06 ( -1.32233e-07 1.35723e-07 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.821096 ( -0.591341 0.871479 )
beta : -2.57163 ( 2.65073 0.698199 )
Epeak [keV] : 59.6982 ( -14.6774 23.5146 )
Norm@50keV : 1.95654E-02 ( -0.0110669 0.0494816 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 56.65 using 59 PHA bins.
# Reduced chi-squared = 1.030 for 55 degrees of freedom
# Null hypothesis probability = 4.132374e-01
Photon flux (15-150 keV) in 25.02 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) = 4.04e-07
S(50-100 keV) = 4.88e-07
T90 vs. Hardness ratio plot
T90 = 19.1480000019073 sec.
Hardness ratio (energy fluence ratio) = 1.20792
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.40452
Count Ratio (50-100 keV) / (15-25 keV) = 0.920302
Mask shadow pattern
IMX = 3.901322941736836E-01, IMY = 6.802207809030785E-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:
-239.496000 -6.708000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6299 22.0084 0.5 42.7 31.8 9.9746 23.9 0.4 Crab
92.9809 3.2604 3.1 53.9 8.1 2.9080 3.7 ------ UNKNOWN
223.7665 48.7589 3.1 59.3 -163.3 5.2775 3.7 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-6.708000 18.316000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.4978 22.1172 21.6 42.6 32.0 -0.0649 -0.5 9.7 Crab
72.2379 26.8873 2.0 46.0 47.5 1.3455 5.7 ------ UNKNOWN
253.1212 74.9958 2.2 50.4 162.8 0.9108 5.2 ------ UNKNOWN
243.8160 80.3096 1.9 45.4 159.4 0.7854 6.1 ------ UNKNOWN
124.7541 29.3537 2.8 20.7 -32.3 0.2211 4.1 ------ UNKNOWN
151.4314 40.8115 2.5 20.7 -106.3 0.3021 4.7 ------ UNKNOWN
114.0465 -8.3612 2.2 59.1 -20.1 1.7338 5.4 ------ UNKNOWN
142.0319 14.5706 0.6 38.1 -60.2 2.5007 20.7 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
274.204600 815.404610
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.3645 35.5112 8.6 44.8 50.6 -2.0026 -1.3 11.1 Her X-1
249.5644 29.3340 3.2 40.1 59.0 3.8592 3.6 ------ UNKNOWN
257.9235 50.6884 4.0 50.9 31.4 5.2275 2.9 ------ UNKNOWN
239.2438 51.9061 2.4 41.2 22.1 2.8450 4.8 ------ UNKNOWN
202.5725 -27.7441 3.0 47.3 176.7 2.4944 3.9 ------ UNKNOWN
206.2435 -5.8254 2.9 25.3 172.8 1.3923 3.9 ------ UNKNOWN
183.4243 -35.2964 2.2 59.0 -166.1 10.5755 5.3 ------ UNKNOWN
175.6977 -29.8293 3.3 57.6 -156.3 8.0730 3.5 ------ UNKNOWN
Plot creation:
Sat May 30 12:43:25 EDT 2015