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
332.3503 -31.7616 0.0137 16.4117 48.8996 0.4802669 14.031 TRIG_00577968
Foreground time interval of the image:
-0.472 10.701 (delta_t = 11.173 [sec])
Background time interval of the image:
-239.000 -0.472 (delta_t = 238.528 [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 -0.472 sec. to 11.944 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.80568 ( -0.175531 0.182261 )
Norm@50keV : 2.60469E-03 ( -0.000323883 0.000319202 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 52.53 using 59 PHA bins.
# Reduced chi-squared = 0.9215 for 57 degrees of freedom
# Null hypothesis probability = 6.434044e-01
Photon flux (15-150 keV) in 12.42 sec: 0.359715 ( -0.0378566 0.0378615 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.97766e-07 ( -3.72698e-08 3.8034e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.472 sec. to 11.944 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -0.179941 ( -1.59258 1.11293 )
Epeak [keV] : 44.3046 ( -5.88966 10.5033 )
Norm@50keV : 3.78826E-02 ( -0.0383174 0.301742 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 40.70 using 59 PHA bins.
# Reduced chi-squared = 0.7268 for 56 degrees of freedom
# Null hypothesis probability = 9.380711e-01
Photon flux (15-150 keV) in 12.42 sec: 0.338416 ( -0.039327 0.039321 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.48152e-07 ( -3.71271e-08 4.2341e-08 ) ergs/cm2
Band function
Time interval is from -0.472 sec. to 11.944 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 0.186874 ( -0.750746 1.45926 )
beta : -9.99999 ( 9.99999 1.43765e-05 )
Epeak [keV] : 44.2718 ( -5.73435 10.4955 )
Norm@50keV : 3.82564E-02 ( -0.0039286 0.302623 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 40.70 using 59 PHA bins.
# Reduced chi-squared = 0.7400 for 55 degrees of freedom
# Null hypothesis probability = 9.248575e-01
Photon flux (15-150 keV) in 12.42 sec: 0.341404 ( 6.6586 -0.039348 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.6233e-07 ( -2.62243e-07 -3.90336e-08 ) ergs/cm2
Single BB
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 10.6571 (-1.04686 1.19219)
R^2/D10^2 : 0.142034 (-0.0470657 0.0676846)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 42.87 using 59 PHA bins.
# Reduced chi-squared = 0.7521 for 57 degrees of freedom
# Null hypothesis probability = 9.174840e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.157e-08 7.415e-09
25- 50 1.128e-07 1.602e-08
50-150 7.057e-08 1.915e-08
15-150 2.249e-07 2.962e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 84.7651 (-24.2147 43.5184)
Norm : 1.68667 (-0.236593 0.281234)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 46.00 using 59 PHA bins.
# Reduced chi-squared = 0.8070 for 57 degrees of freedom
# Null hypothesis probability = 8.512075e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.453e-08 7.967e-09
25- 50 9.100e-08 1.080e-08
50-150 1.334e-07 6.145e-08
15-150 2.790e-07 6.253e-08
Double BB
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 9.16397 ( )
R1^2/D10^2 : 0.211382 (-0.186682 0.216805)
kT2 [keV] : 27.9695 (-29.3335 -31.6562)
R2^2/D10^2 : 1.29958E-03 (-0.00092018 0.0625629)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 41.35 using 59 PHA bins.
#Fit statistic : Chi-Squared = 38.94 using 59 PHA bins.
# Reduced chi-squared = 0.7518 for 55 degrees of freedom
# Reduced chi-squared = 0.7080 for 55 degrees of freedom
# Null hypothesis probability = 9.135702e-01
# Null hypothesis probability = 9.502219e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.591e-08 1.610e-08
25- 50 1.077e-07 3.327e-08
50-150 7.845e-08 2.928e-08
15-150 2.321e-07 6.227e-08
Peak spectrum fit
Power-law model
Time interval is from -0.236 sec. to 0.764 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.57859 ( -0.298384 0.312324 )
Norm@50keV : 5.20681E-03 ( -0.00112725 0.00111371 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 60.31 using 59 PHA bins.
# Reduced chi-squared = 1.058 for 57 degrees of freedom
# Null hypothesis probability = 3.569044e-01
Photon flux (15-150 keV) in 1 sec: 0.664717 ( -0.134316 0.134401 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.88358e-08 ( -1.11345e-08 1.14345e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.236 sec. to 0.764 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -0.953679 ( -2.57552 1.63426 )
Epeak [keV] : 53.7239 ( -10.15 20.8399 )
Norm@50keV : 0.118081 ( -0.11829 2.57792 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 51.98 using 59 PHA bins.
# Reduced chi-squared = 0.9283 for 56 degrees of freedom
# Null hypothesis probability = 6.276191e-01
Photon flux (15-150 keV) in 1 sec: 0.631556 ( -0.068173 0.134949 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.27642e-08 ( -1.0133e-08 1.13238e-08 ) ergs/cm2
Band function
Time interval is from -0.236 sec. to 0.764 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 0.944385 ( -1.31891 2.93147 )
beta : -10.0000 ( 10 0 )
Epeak [keV] : 53.7075 ( -10.2131 20.8357 )
Norm@50keV : 0.117058 ( -0.117002 2.59766 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 51.98 using 59 PHA bins.
# Reduced chi-squared = 0.9452 for 55 degrees of freedom
# Null hypothesis probability = 5.906017e-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] : 13.4442 (-2.30987 2.85724)
R^2/D10^2 : 0.123409 (-0.0625144 0.11829)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 52.17 using 59 PHA bins.
# Reduced chi-squared = 0.9153 for 57 degrees of freedom
# Null hypothesis probability = 6.564761e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.726e-09 1.732e-09
25- 50 1.687e-08 4.555e-09
50-150 1.964e-08 8.673e-09
15-150 4.124e-08 1.114e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 145.207 (-72.4394 -143.413)
Norm : 2.82448 (-0.594061 0.735695)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 57.69 using 59 PHA bins.
# Reduced chi-squared = 1.012 for 57 degrees of freedom
# Null hypothesis probability = 4.495299e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.274e-09 4.190e-09
25- 50 1.342e-08 7.610e-09
50-150 2.613e-08 1.623e-08
15-150 4.682e-08 2.789e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.65144 (-6.65145 -6.65145)
R1^2/D10^2 : 0.242578 (-0.242499 -0.242499)
kT2 [keV] : 14.6665 (-14.6667 -14.6667)
R2^2/D10^2 : 8.14109E-02 (-0.0814048 0.153322)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 51.93 using 59 PHA bins.
# Reduced chi-squared = 0.9442 for 55 degrees of freedom
# Null hypothesis probability = 5.926259e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.309e-09 3.922e-09
25- 50 1.633e-08 1.003e-08
50-150 2.102e-08 1.441e-08
15-150 4.266e-08 2.806e-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: 1.84956 ( -0.174393 0.181616 )
Norm@50keV : 2.73010E-03 ( -0.000344049 0.000339258 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 56.90 using 59 PHA bins.
# Reduced chi-squared = 0.9982 for 57 degrees of freedom
# Null hypothesis probability = 4.789755e-01
Photon flux (15-150 keV) in 11.17 sec: 0.383677 ( -0.040208 0.0402107 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.8039e-07 ( -3.50386e-08 3.58087e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -0.534118 ( -1.71574 1.21033 )
Epeak [keV] : 42.2472 ( -4.87929 7.56866 )
Norm@50keV : 6.93040E-02 ( -0.0712188 0.672151 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 41.50 using 59 PHA bins.
# Reduced chi-squared = 0.7411 for 56 degrees of freedom
# Null hypothesis probability = 9.258593e-01
Photon flux (15-150 keV) in 11.17 sec: 0.358333 ( -0.041543 0.041486 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.29642e-07 ( -3.24835e-08 3.73893e-08 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 1.39454 ( -1.94301 1.97869 )
beta : -3.15400 ( 3.14787 0.747417 )
Epeak [keV] : 39.3630 ( -4.44133 7.87218 )
Norm@50keV : 0.247362 ( -0.246902 5.3276 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 40.05 using 59 PHA bins.
# Reduced chi-squared = 0.7282 for 55 degrees of freedom
# Null hypothesis probability = 9.351017e-01
Photon flux (15-150 keV) in 11.17 sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 2.43612e-07 ( -2.43534e-07 -3.67571e-08 ) ergs/cm2
S(25-50 keV) vs. S(50-100 keV) plot
S(25-50 keV) = 8.40e-08
S(50-100 keV) = 9.61e-08
T90 vs. Hardness ratio plot
T90 = 10.8799999952316 sec.
Hardness ratio (energy fluence ratio) = 1.14405
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.41909
Count Ratio (50-100 keV) / (15-25 keV) = 0.529389
Mask shadow pattern
IMX = 1.936229680931073E-01, IMY = -2.219509725843758E-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:
-239.000000 -0.472000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
265.0006 -44.3917 0.0 40.5 -84.7 -1.8837 -2.1 11.6 4U 1735-44
276.0622 -30.2429 20.8 40.5 -59.0 0.2989 0.6 10.3 H1820-303
285.0116 -24.9561 80.2 38.1 -44.4 -0.0433 -0.1 2.5 HT1900.1-2455
341.5814 -4.2270 2.6 45.3 48.7 3.4616 4.5 ------ UNKNOWN
315.9188 -0.9278 3.0 46.6 12.5 1.5347 3.9 ------ UNKNOWN
73.2076 -63.7450 2.5 56.1 173.9 5.4577 4.6 ------ UNKNOWN
304.3507 -1.0840 2.9 49.1 -2.7 1.5861 4.1 ------ UNKNOWN
259.1652 -52.1655 3.3 41.1 -98.0 3.5003 3.5 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-0.472000 10.700600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
264.6562 -44.5494 26.0 40.7 -85.1 0.0612 0.4 7.0 4U 1735-44
276.0834 -30.4038 5.0 40.4 -59.2 0.1858 2.3 8.5 H1820-303
285.0179 -24.7862 12.0 38.2 -44.3 0.0533 1.0 8.1 HT1900.1-2455
332.3503 -31.7616 0.8 16.4 48.9 0.4802 14.0 ------ UNKNOWN
20.5372 -84.8007 2.1 40.3 -162.5 0.2641 5.5 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
49.900610 685.900600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
285.1016 -24.8487 4.9 41.8 -71.5 -4.4126 -2.4 5.6 HT1900.1-2455
38.8105 -78.4109 3.2 54.3 -171.7 4.7951 3.6 ------ UNKNOWN
290.9302 -25.8021 3.3 36.5 -70.0 3.0620 3.6 ------ UNKNOWN
281.8027 -42.2154 4.2 41.1 -98.1 6.3447 2.7 ------ UNKNOWN
Plot creation:
Sat May 30 15:06:53 EDT 2015