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
320.8752 -53.0261 0.0055 44.1310 34.1709 7.4414648 35.163 TRIG_00214805
Foreground time interval of the image:
-1.496 14.941 (delta_t = 16.437 [sec])
Background time interval of the image:
-239.760 -1.496 (delta_t = 238.264 [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 -1.496 sec. to 179.080 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.03655 ( -0.0365574 0.0367046 )
Norm@50keV : 1.24314E-02 ( -0.000209102 0.000209085 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 48.38 using 59 PHA bins.
# Reduced chi-squared = 0.8488 for 57 degrees of freedom
# Null hypothesis probability = 7.848226e-01
Photon flux (15-150 keV) in 180.6 sec: 1.89674 ( -0.0445293 0.0449315 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.075e-05 ( -3.50564e-07 3.50666e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -1.496 sec. to 179.080 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.33949 ( )
Epeak [keV] : 136.389 ( )
Norm@50keV : 9.42767E-03 ( -0.0008223 0.00112772 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 34.01 using 59 PHA bins.
# Reduced chi-squared = 0.6073 for 56 degrees of freedom
# Null hypothesis probability = 9.911389e-01
Photon flux (15-150 keV) in 180.6 sec: 1.89497 ( -0.04445 0.04494 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.07462e-05 ( -3.48558e-07 3.50183e-07 ) ergs/cm2
Band function
Time interval is from -1.496 sec. to 179.080 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.64038 ( 1.64061 1.64061 )
beta : -2.03654 ( -0.0367111 0.0365708 )
Epeak [keV] : 13.7029 ( -13.5983 9979.93 )
Norm@50keV : 2.96907E-02 ( -0.0106689 0.767442 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 48.38 using 59 PHA bins.
# Reduced chi-squared = 0.8797 for 55 degrees of freedom
# Null hypothesis probability = 7.237279e-01
Photon flux (15-150 keV) in 180.6 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] : 14.0770 ( )
R^2/D10^2 : 0.202607 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 1143.74 using 59 PHA bins.
# Reduced chi-squared = 20.0656 for 57 degrees of freedom
# Null hypothesis probability = 5.347762e-202
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.531e-06 6.059e-08
25- 50 5.725e-06 1.535e-07
50-150 7.491e-06 2.185e-07
15-150 1.475e-05 2.628e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 89.3657 ( )
Norm : 7.82999 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 169.05 using 59 PHA bins.
# Reduced chi-squared = 2.9658 for 57 degrees of freedom
# Null hypothesis probability = 4.917095e-13
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.689e-06 1.219e-07
25- 50 6.230e-06 1.409e-07
50-150 9.445e-06 2.727e-07
15-150 1.936e-05 3.431e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.62376 (-0.321855 0.335666)
R1^2/D10^2 : 3.14213 (-0.585075 0.747854)
kT2 [keV] : 26.3142 (-1.46878 1.68556)
R2^2/D10^2 : 1.47963E-02 (-0.00305635 0.00361251)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 62.65 using 59 PHA bins.
# Reduced chi-squared = 1.139 for 55 degrees of freedom
# Null hypothesis probability = 2.233958e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.076e-06 2.456e-07
25- 50 6.438e-06 1.851e-07
50-150 9.880e-06 3.431e-07
15-150 2.039e-05 5.328e-07
Peak spectrum fit
Power-law model
Time interval is from -1.324 sec. to -0.324 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.59796 ( -0.10219 0.10353 )
Norm@50keV : 8.94811E-02 ( -0.00544234 0.00542329 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 52.44 using 59 PHA bins.
# Reduced chi-squared = 0.9201 for 57 degrees of freedom
# Null hypothesis probability = 6.464515e-01
Photon flux (15-150 keV) in 1 sec: 11.4915 ( -0.703693 0.704726 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.37046e-07 ( -5.42344e-08 5.44242e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -1.324 sec. to -0.324 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.38236 ( -0.429692 0.269352 )
Epeak [keV] : 147.865 ( -67.1244 -147.913 )
Norm@50keV : 0.114519 ( -0.0292837 0.0705795 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 51.60 using 59 PHA bins.
# Reduced chi-squared = 0.9214 for 56 degrees of freedom
# Null hypothesis probability = 6.420733e-01
Photon flux (15-150 keV) in 1 sec: 11.3863 ( -0.7279 0.7288 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.27797e-07 ( -5.7764e-08 5.7362e-08 ) ergs/cm2
Band function
Time interval is from -1.324 sec. to -0.324 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.03648 ( 1.03595 1.03595 )
beta : -1.72265 ( 1.72175 0.193762 )
Epeak [keV] : 69.9881 ( -68.5337 -68.5337 )
Norm@50keV : 0.186370 ( -0.103324 0 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 51.00 using 59 PHA bins.
# Reduced chi-squared = 0.9274 for 55 degrees of freedom
# Null hypothesis probability = 6.279939e-01
Photon flux (15-150 keV) in 1 sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 8.25095e-07 ( 0 0 ) ergs/cm2
Single BB
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 14.4986 ( )
R^2/D10^2 : 1.44452 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 121.34 using 59 PHA bins.
# Reduced chi-squared = 2.1288 for 57 degrees of freedom
# Null hypothesis probability = 1.501761e-06
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.389e-08 7.165e-09
25- 50 2.459e-07 1.785e-08
50-150 3.463e-07 3.780e-08
15-150 6.561e-07 4.340e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 187.749 (-49.1152 -187.749)
Norm : 46.7590 (-2.91556 3.20959)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 51.77 using 59 PHA bins.
# Reduced chi-squared = 0.9082 for 57 degrees of freedom
# Null hypothesis probability = 6.710107e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.173e-07 1.000e-08
25- 50 2.241e-07 3.900e-08
50-150 4.816e-07 1.807e-07
15-150 8.230e-07 2.351e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.90025 (-1.63144 1.6628)
R1^2/D10^2 : 8.47723 (-3.74979 9.5623)
kT2 [keV] : 29.4407 (-6.5473 13.6472)
R2^2/D10^2 : 8.56146E-02 (-0.0611723 0.135555)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 55.59 using 59 PHA bins.
# Reduced chi-squared = 1.011 for 55 degrees of freedom
# Null hypothesis probability = 4.524147e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.065e-07 1.992e-08
25- 50 2.342e-07 4.435e-08
50-150 4.841e-07 1.502e-07
15-150 8.248e-07 2.070e-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: 1.66688 ( -0.0628397 0.0632 )
Norm@50keV : 3.06336E-02 ( -0.00102476 0.00102364 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 36.77 using 59 PHA bins.
# Reduced chi-squared = 0.6450 for 57 degrees of freedom
# Null hypothesis probability = 9.828737e-01
Photon flux (15-150 keV) in 16.44 sec: 4.02254 ( -0.148959 0.14978 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.67618e-06 ( -1.62165e-07 1.6248e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.66796 ( -0.0653217 0.061706 )
Epeak [keV] : 9999.36 ( -9999.35 -9999.36 )
Norm@50keV : 3.06415E-02 ( -0.00102455 0.00596577 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 36.79 using 59 PHA bins.
# Reduced chi-squared = 0.6570 for 56 degrees of freedom
# Null hypothesis probability = 9.779170e-01
Photon flux (15-150 keV) in 16.44 sec: 4.02587 ( -0.15478 0.14439 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.67619e-06 ( -1.61622e-07 1.6948e-07 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.24383 ( 1.24147 1.24147 )
beta : -1.67041 ( -7.6222 0.0656165 )
Epeak [keV] : 42.3346 ( -41.8091 -41.8091 )
Norm@50keV : 6.43753E-02 ( -0.0361572 0 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 36.69 using 59 PHA bins.
# Reduced chi-squared = 0.6671 for 55 degrees of freedom
# Null hypothesis probability = 9.727781e-01
Photon flux (15-150 keV) in 16.44 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) = 6.31e-06
S(50-100 keV) = 6.15e-06
T90 vs. Hardness ratio plot
T90 = 109.104000002146 sec.
Hardness ratio (energy fluence ratio) = 0.974643
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 0.951798
Count Ratio (50-100 keV) / (15-25 keV) = 0.521164
Mask shadow pattern
IMX = 8.026413408118448E-01, IMY = -5.448789100544709E-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:
-239.760000 -1.496000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
326.2800 38.3693 9.4 50.3 -171.2 0.4745 1.2 5.8 Cyg X-2
300.0699 -29.6653 2.8 39.4 76.0 2.4648 4.2 ------ UNKNOWN
28.8172 -50.6670 2.8 57.8 -15.9 3.1134 4.1 ------ UNKNOWN
29.8613 -28.4624 3.4 52.1 -42.2 3.0662 3.4 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-1.496000 14.940590
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
326.2619 38.3674 8.9 50.3 -171.2 -0.1299 -1.3 5.1 Cyg X-2
297.0859 21.6184 3.6 51.1 149.6 0.7025 3.2 ------ UNKNOWN
320.8752 -53.0261 0.3 44.1 34.2 7.4416 35.2 ------ UNKNOWN
303.5568 4.8176 2.8 37.1 133.4 0.4816 4.1 ------ UNKNOWN
349.8328 32.6791 2.5 45.2 -145.0 0.3397 4.6 ------ UNKNOWN
6.8129 23.4731 2.2 44.9 -120.1 0.8123 5.2 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
80.340590 482.320000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
264.7984 -44.4279 13.8 36.9 69.3 1.9539 0.8 2.7 4U 1735-44
276.1027 -30.4229 15.0 39.4 96.1 -2.4561 -0.8 9.8 H1820-303
285.0043 -25.0440 10.3 38.7 111.2 -2.9865 -1.1 7.6 HT1900.1-2455
264.4403 -59.0110 2.6 31.1 45.3 5.4591 4.3 ------ UNKNOWN
217.8149 -71.2094 2.3 44.5 15.7 8.3265 5.0 ------ UNKNOWN
320.9232 -53.0304 1.6 0.1 -122.1 5.1790 7.2 ------ UNKNOWN
250.2160 -85.8225 4.1 35.7 -4.2 2.7881 2.9 ------ UNKNOWN
47.5577 -83.2779 2.3 37.1 -22.1 4.9517 5.1 ------ UNKNOWN
11.7357 -30.1810 2.2 43.2 -112.1 14.3766 5.2 ------ UNKNOWN
Plot creation:
Sun May 31 12:46:30 EDT 2015