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
214.2842 42.1443 0.0063 19.1540 95.4980 1.8104872 30.445 TRIG_00522656
Foreground time interval of the image:
-1.032 17.365 (delta_t = 18.397 [sec])
Background time interval of the image:
-180.435 -1.032 (delta_t = 179.403 [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 -1.032 sec. to 31.864 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.65555 ( -0.109984 0.111694 )
Norm@50keV : 3.93009E-03 ( -0.000253845 0.000251789 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 70.71 using 59 PHA bins.
# Reduced chi-squared = 1.241 for 57 degrees of freedom
# Null hypothesis probability = 1.047589e-01
Photon flux (15-150 keV) in 32.9 sec: 0.514115 ( -0.0308932 0.0309208 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.20188e-06 ( -8.28902e-08 8.3693e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -1.032 sec. to 31.864 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.36323 ( -0.457528 0.35144 )
Epeak [keV] : 103.018 ( -37.6375 -103.018 )
Norm@50keV : 5.59703E-03 ( -0.00183484 0.00404213 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 69.27 using 59 PHA bins.
# Reduced chi-squared = 1.237 for 56 degrees of freedom
# Null hypothesis probability = 1.095791e-01
Photon flux (15-150 keV) in 32.9 sec: 0.505861 ( -0.032945 0.032921 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.16793e-06 ( -9.63246e-08 9.64167e-08 ) ergs/cm2
Band function
Time interval is from -1.032 sec. to 31.864 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.36327 ( -0.267637 0.426549 )
beta : -10.0000 ( 10 1.06581e-14 )
Epeak [keV] : 103.000 ( -37.2083 -103 )
Norm@50keV : 5.59610E-03 ( -0.00183436 0.00404334 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 69.27 using 59 PHA bins.
# Reduced chi-squared = 1.260 for 55 degrees of freedom
# Null hypothesis probability = 9.331108e-02
Photon flux (15-150 keV) in 32.9 sec: 0.503441 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 1.17046e-06 ( 0 0 ) ergs/cm2
Single BB
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 12.6724 ( )
R^2/D10^2 : 0.100554 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 129.69 using 59 PHA bins.
# Reduced chi-squared = 2.2753 for 57 degrees of freedom
# Null hypothesis probability = 1.372105e-07
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.127e-07 1.328e-08
25- 50 3.774e-07 2.829e-08
50-150 3.773e-07 5.174e-08
15-150 8.674e-07 6.498e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 150.724 (-40.0979 -148.932)
Norm : 2.10488 (-0.141684 0.172896)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 69.40 using 59 PHA bins.
# Reduced chi-squared = 1.218 for 57 degrees of freedom
# Null hypothesis probability = 1.254709e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.778e-07 1.525e-08
25- 50 3.298e-07 3.815e-08
50-150 6.522e-07 2.350e-07
15-150 1.160e-06 2.757e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.33025 (-1.19279 1.23012)
R1^2/D10^2 : 0.505385 (-0.200073 0.409831)
kT2 [keV] : 27.0689 (-5.50257 9.49443)
R2^2/D10^2 : 4.91447E-03 (-0.00313336 0.00648997)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 68.36 using 59 PHA bins.
# Reduced chi-squared = 1.243 for 55 degrees of freedom
# Null hypothesis probability = 1.064251e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.699e-07 3.731e-08
25- 50 3.407e-07 7.185e-08
50-150 6.653e-07 3.005e-07
15-150 1.176e-06 3.415e-07
Peak spectrum fit
Power-law model
Time interval is from 0.184 sec. to 1.184 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.19519 ( -0.186182 0.18501 )
Norm@50keV : 1.63796E-02 ( -0.00161974 0.00161915 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 71.27 using 59 PHA bins.
# Reduced chi-squared = 1.250 for 57 degrees of freedom
# Null hypothesis probability = 9.683678e-02
Photon flux (15-150 keV) in 1 sec: 1.92134 ( -0.194156 0.194651 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.66405e-07 ( -1.88196e-08 1.8972e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.184 sec. to 1.184 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.30481 ( -0.194058 0.181171 )
Epeak [keV] : 103.691 ( -9999.36 -9999.36 )
Norm@50keV : 3.67551E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 66.41 using 59 PHA bins.
# Reduced chi-squared = 1.186 for 56 degrees of freedom
# Null hypothesis probability = 1.608540e-01
Photon flux (15-150 keV) in 1 sec: 1.92310 ( -0.19642 0.19226 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.66187e-07 ( -1.8515e-08 1.8904e-08 ) ergs/cm2
Band function
Time interval is from 0.184 sec. to 1.184 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.962528 ( 0.963068 0.963068 )
beta : -1.19517 ( -0.185213 0.186237 )
Epeak [keV] : 52.8840 ( -52.2399 -52.2399 )
Norm@50keV : 2.88884E-02 ( -0.0141318 2.41738 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 71.27 using 59 PHA bins.
# Reduced chi-squared = 1.296 for 55 degrees of freedom
# Null hypothesis probability = 6.915878e-02
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] : 20.5418 (-3.07811 3.75043)
R^2/D10^2 : 7.92932E-02 (-0.0324951 0.0544436)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 102.69 using 59 PHA bins.
# Reduced chi-squared = 1.8017 for 57 degrees of freedom
# Null hypothesis probability = 1.977173e-04
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.380e-09 1.403e-09
25- 50 3.234e-08 5.285e-09
50-150 1.015e-07 1.779e-08
15-150 1.402e-07 2.260e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 ( )
Norm : 7.86186 (-0.794417 0.794378)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 83.38 using 59 PHA bins.
# Reduced chi-squared = 1.463 for 57 degrees of freedom
# Null hypothesis probability = 1.293450e-02
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.958e-08 1.078e-08
25- 50 3.767e-08 2.058e-08
50-150 8.261e-08 4.470e-08
15-150 1.398e-07 7.580e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.46714 (-3.4674 2.9937)
R1^2/D10^2 : 2.26982 (-1.55936 10.8604)
kT2 [keV] : 33.3732 (-9.75861 18.8168)
R2^2/D10^2 : 1.54038E-02 (-0.0107097 0.0310537)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 71.76 using 59 PHA bins.
# Reduced chi-squared = 1.305 for 55 degrees of freedom
# Null hypothesis probability = 6.405594e-02
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.645e-08 8.295e-09
25- 50 3.242e-08 1.318e-08
50-150 1.228e-07 5.359e-08
15-150 1.716e-07 7.191e-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: 1.61516 ( -0.0997891 0.100906 )
Norm@50keV : 6.18901E-03 ( -0.00035492 0.00035272 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 74.55 using 59 PHA bins.
# Reduced chi-squared = 1.308 for 57 degrees of freedom
# Null hypothesis probability = 5.927526e-02
Photon flux (15-150 keV) in 18.4 sec: 0.799097 ( -0.0436574 0.0437021 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.06309e-06 ( -6.58293e-08 6.63607e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.43941 ( -0.392955 0.229221 )
Epeak [keV] : 152.988 ( )
Norm@50keV : 7.63946E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 73.87 using 59 PHA bins.
# Reduced chi-squared = 1.319 for 56 degrees of freedom
# Null hypothesis probability = 5.502646e-02
Photon flux (15-150 keV) in 18.4 sec: 0.791196 ( -0.046428 0.046405 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.04525e-06 ( -7.61797e-08 7.58522e-08 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.721257 ( 0.986379 0.986379 )
beta : -1.74396 ( 1.74106 0.17337 )
Epeak [keV] : 50.3732 ( -50.0194 203.174 )
Norm@50keV : 2.20811E-02 ( -0.0230031 713.599 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 72.11 using 59 PHA bins.
# Reduced chi-squared = 1.311 for 55 degrees of freedom
# Null hypothesis probability = 6.062199e-02
Photon flux (15-150 keV) in 18.4 sec: 0.788574 ( ) 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) = 3.19e-07
S(50-100 keV) = 4.05e-07
T90 vs. Hardness ratio plot
T90 = 27.067999958992 sec.
Hardness ratio (energy fluence ratio) = 1.26959
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.34964
Count Ratio (50-100 keV) / (15-25 keV) = 0.815127
Mask shadow pattern
IMX = -3.327848078866250E-02, IMY = -3.457392824339013E-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:
-180.435400 -1.032000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.5310 35.3828 4.3 40.8 44.6 1.1078 2.7 4.3 Her X-1
255.1457 31.6834 3.2 44.2 47.1 2.2271 3.6 ------ UNKNOWN
262.0384 40.0199 2.2 40.9 33.1 1.8389 5.3 ------ UNKNOWN
253.0335 46.7579 3.3 31.5 33.2 0.7756 3.5 ------ UNKNOWN
256.8369 47.5690 2.6 32.9 28.8 1.0896 4.5 ------ UNKNOWN
291.6799 41.8994 3.0 53.9 8.1 2.5165 3.8 ------ UNKNOWN
260.1969 65.7426 2.4 25.6 -6.1 0.8098 4.8 ------ UNKNOWN
136.7865 23.8453 3.7 57.8 -156.8 3.3612 3.1 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-1.032000 17.364600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.2424 35.2194 6.0 40.8 45.0 0.2559 1.9 12.9 Her X-1
214.2842 42.1443 0.4 19.2 95.5 1.8106 30.4 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
58.364580 962.155200
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.5710 35.2906 7.7 31.9 24.5 -1.1249 -1.5 6.4 Her X-1
231.2659 38.1436 2.8 13.6 37.2 2.1098 4.1 ------ UNKNOWN
179.9748 14.3254 4.0 40.6 172.7 2.4520 2.9 ------ UNKNOWN
297.9933 46.4136 3.5 57.2 -9.7 7.9817 3.3 ------ UNKNOWN
150.5318 19.2332 3.2 58.0 -156.8 12.4974 3.7 ------ UNKNOWN
Plot creation:
Sat May 30 19:27:14 EDT 2015