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
350.9207 29.7631 0.0036 36.3844 -124.7862 18.0223877 53.209 TRIG_00348128
Foreground time interval of the image:
-4.899 165.008 (delta_t = 169.907 [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
8 ms binning
From T100_start-3 s to T100_start+3 s
2 ms binning
From T100_start-1 s to T100_start+1 s
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 -11.948 sec. to 165.008 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.62833 ( -0.0473648 0.0474909 )
Norm@50keV : 6.76467E-03 ( -0.000164195 0.000164175 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 45.63 using 59 PHA bins.
# Reduced chi-squared = 0.8006 for 57 degrees of freedom
# Null hypothesis probability = 8.602492e-01
Photon flux (15-150 keV) in 177 sec: 0.877088 ( -0.0245258 0.0246484 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.11611e-05 ( -2.79568e-07 2.7981e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -11.948 sec. to 165.008 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.51801 ( -0.186229 0.135973 )
Epeak [keV] : 242.678 ( -117.719 -242.678 )
Norm@50keV : 7.58682E-03 ( -0.000933805 0.00157001 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 44.54 using 59 PHA bins.
# Reduced chi-squared = 0.7954 for 56 degrees of freedom
# Null hypothesis probability = 8.649266e-01
Photon flux (15-150 keV) in 177 sec: 0.868507 ( -0.027835 0.024951 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.10835e-05 ( -3.10387e-07 3.05874e-07 ) ergs/cm2
Band function
Time interval is from -11.948 sec. to 165.008 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.794239 ( 1.12958 1.12958 )
beta : -1.64181 ( -0.0615684 0.0546789 )
Epeak [keV] : 39.2982 ( -39.2596 419.59 )
Norm@50keV : 2.62006E-02 ( -0.0263636 834779 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 44.86 using 59 PHA bins.
# Reduced chi-squared = 0.8157 for 55 degrees of freedom
# Null hypothesis probability = 8.336801e-01
Photon flux (15-150 keV) in 177 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] : 16.3999 ( )
R^2/D10^2 : 6.65138E-02 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 435.20 using 59 PHA bins.
# Reduced chi-squared = 7.6351 for 57 degrees of freedom
# Null hypothesis probability = 1.209654e-59
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.509e-07 3.363e-08
25- 50 2.797e-06 9.204e-08
50-150 5.306e-06 2.177e-07
15-150 8.754e-06 2.248e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 189.748 (-24.3051 -189.169)
Norm : 3.49491 (-0.0983246 0.106561)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 49.62 using 59 PHA bins.
# Reduced chi-squared = 0.8706 for 57 degrees of freedom
# Null hypothesis probability = 7.453735e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.550e-06 7.806e-08
25- 50 2.964e-06 1.735e-07
50-150 6.394e-06 1.389e-06
15-150 1.091e-05 1.597e-06
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.45953 (-0.531974 0.576568)
R1^2/D10^2 : 1.26765 (-0.354005 0.518955)
kT2 [keV] : 25.4123 (-1.66555 1.99442)
R2^2/D10^2 : 1.16570E-02 (-0.00283709 0.00336786)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 41.58 using 59 PHA bins.
# Reduced chi-squared = 0.7561 for 55 degrees of freedom
# Null hypothesis probability = 9.092251e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.602e-06 1.380e-07
25- 50 2.913e-06 1.416e-07
50-150 6.466e-06 3.443e-07
15-150 1.098e-05 4.859e-07
Peak spectrum fit
Power-law model
Time interval is from 122.048 sec. to 123.048 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.30308 ( -0.0709804 0.0708966 )
Norm@50keV : 9.17034E-02 ( -0.00354666 0.00354663 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 61.24 using 59 PHA bins.
# Reduced chi-squared = 1.074 for 57 degrees of freedom
# Null hypothesis probability = 3.264042e-01
Photon flux (15-150 keV) in 1 sec: 10.9467 ( -0.448116 0.449197 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.05514e-07 ( -3.81074e-08 3.82625e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 122.048 sec. to 123.048 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.29933 ( )
Epeak [keV] : 1.00000E+04 ( )
Norm@50keV : 9.20874E-02 ( -0.00356137 0.00356138 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 61.29 using 59 PHA bins.
# Reduced chi-squared = 1.095 for 56 degrees of freedom
# Null hypothesis probability = 2.919059e-01
Photon flux (15-150 keV) in 1 sec: 10.9447 ( -0.4478 0.4463 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.04845e-07 ( -3.7248e-08 3.8251e-08 ) ergs/cm2
Band function
Time interval is from 122.048 sec. to 123.048 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.928491 ( 0.93978 0.93978 )
beta : -1.31431 ( 1.31414 0.0810858 )
Epeak [keV] : 83.0217 ( -87.4745 625.711 )
Norm@50keV : 0.165003 ( -0.0664356 0 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 61.19 using 59 PHA bins.
# Reduced chi-squared = 1.113 for 55 degrees of freedom
# Null hypothesis probability = 2.635460e-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] : 18.3232 ( )
R^2/D10^2 : 0.641557 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 242.67 using 59 PHA bins.
# Reduced chi-squared = 4.2574 for 57 degrees of freedom
# Null hypothesis probability = 9.234765e-25
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.288e-08 3.655e-09
25- 50 2.009e-07 1.170e-08
50-150 4.918e-07 3.350e-08
15-150 7.356e-07 3.645e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 ( )
Norm : 45.7387 (-1.79216 1.79166)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 106.34 using 59 PHA bins.
# Reduced chi-squared = 1.8656 for 57 degrees of freedom
# Null hypothesis probability = 8.059140e-05
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.139e-07 4.650e-09
25- 50 2.192e-07 9.250e-09
50-150 4.806e-07 2.010e-08
15-150 8.137e-07 3.350e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 8.94373 (-1.15953 1.23558)
R1^2/D10^2 : 4.95780 (-1.61325 2.72214)
kT2 [keV] : 42.5991 (-8.35309 16.0261)
R2^2/D10^2 : 3.46403E-02 (-0.019857 0.032876)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 64.90 using 59 PHA bins.
# Reduced chi-squared = 1.180 for 55 degrees of freedom
# Null hypothesis probability = 1.698173e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.471e-08 1.100e-08
25- 50 2.158e-07 2.095e-08
50-150 6.150e-07 1.140e-07
15-150 9.155e-07 1.303e-07
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: 1.63547 ( -0.0474176 0.0475087 )
Norm@50keV : 6.90137E-03 ( -0.000167619 0.000167599 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 44.79 using 59 PHA bins.
# Reduced chi-squared = 0.7857 for 57 degrees of freedom
# Null hypothesis probability = 8.797736e-01
Photon flux (15-150 keV) in 169.9 sec: 0.896880 ( -0.0251038 0.0252117 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.09215e-05 ( -2.73614e-07 2.73974e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.53270 ( -0.186031 0.129164 )
Epeak [keV] : 251.918 ( )
Norm@50keV : 7.68177E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 43.84 using 59 PHA bins.
# Reduced chi-squared = 0.7829 for 56 degrees of freedom
# Null hypothesis probability = 8.810677e-01
Photon flux (15-150 keV) in 169.9 sec: 0.888697 ( -0.02847 0.014324 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.08505e-05 ( -3.04121e-07 2.98073e-07 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.966789 ( 1.12538 1.12538 )
beta : -1.65023 ( -0.0624419 0.0552755 )
Epeak [keV] : 44.1679 ( -44.0443 -44.0443 )
Norm@50keV : 1.98127E-02 ( -0.0201493 918767 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 43.97 using 59 PHA bins.
# Reduced chi-squared = 0.7994 for 55 degrees of freedom
# Null hypothesis probability = 8.570446e-01
Photon flux (15-150 keV) in 169.9 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) = 2.93e-06
S(50-100 keV) = 3.79e-06
T90 vs. Hardness ratio plot
T90 = 117.004000008106 sec.
Hardness ratio (energy fluence ratio) = 1.29352
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.30637
Count Ratio (50-100 keV) / (15-25 keV) = 1.01445
Mask shadow pattern
IMX = -4.203805169982753E-01, IMY = 6.051591383681547E-01
TIME vs. PHA plot around the trigger time
TIME vs. DetID plot around the trigger time
100 us light curve (15-350 keV)
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:
-4.899400 165.008000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
288.8042 10.9288 1.7 34.0 113.5 2.0943 6.8 1.1 GRS 1915+105
299.5729 35.1965 0.4 36.9 159.1 7.8576 28.3 0.9 Cyg X-1
308.0669 40.9091 2.6 38.2 173.4 1.1338 4.5 3.3 Cyg X-3
326.2396 38.1791 11.1 33.3 -163.5 0.2368 1.0 9.1 Cyg X-2
291.2683 -2.4922 2.8 32.2 88.6 1.3365 4.1 ------ UNKNOWN
350.9207 29.7631 0.2 36.4 -124.8 18.0209 53.2 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
730.300600 963.182300
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6299 22.0007 0.6 52.7 -177.8 8.8541 19.3 0.8 Crab
308.0120 40.8491 34.3 56.9 -26.2 -0.3210 -0.3 7.6 Cyg X-3
68.7119 36.8851 3.3 36.4 -161.9 0.7355 3.5 ------ UNKNOWN
19.4086 36.8103 3.2 41.1 -97.8 2.8772 3.6 ------ UNKNOWN
Plot creation:
Sun May 31 04:38:03 EDT 2015