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
358.6351 29.4305 0.0035 41.6361 28.7309 8.3350036 54.116 TRIG_00568849
Foreground time interval of the image:
-1.856 9.781 (delta_t = 11.637 [sec])
Background time interval of the image:
-239.520 -1.856 (delta_t = 237.664 [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 0.512000
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 0.512000
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 0.512000
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)
The mask-weighted light curves based on cleaned DPHs
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 -1.856 sec. to 41.376 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.92840 ( -0.0486334 0.0488862 )
Norm@50keV : 1.63560E-02 ( -0.000410423 0.000409716 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 56.67 using 59 PHA bins.
# Reduced chi-squared = 0.9942 for 57 degrees of freedom
# Null hypothesis probability = 4.873431e-01
Photon flux (15-150 keV) in 43.23 sec: 2.37608 ( -0.0695295 0.0699112 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.50331e-06 ( -1.61733e-07 1.61831e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -1.856 sec. to 41.376 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.91415 ( -0.187294 0.222441 )
Epeak [keV] : 312.183 ( -321.723 -321.745 )
Norm@50keV : 1.66153E-02 ( -0.0034802 0.00367825 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 56.66 using 59 PHA bins.
# Reduced chi-squared = 1.012 for 56 degrees of freedom
# Null hypothesis probability = 4.503889e-01
Photon flux (15-150 keV) in 43.23 sec: 2.36475 ( -0.07403 0.08176 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.49756e-06 ( -1.66349e-07 1.66435e-07 ) ergs/cm2
Band function
Time interval is from -1.856 sec. to 41.376 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.936060 ( -1.23287 5.92787 )
beta : -1.96960 ( -0.0775359 0.0657976 )
Epeak [keV] : 33.4107 ( -13.5154 54.4255 )
Norm@50keV : 7.25532E-02 ( -0.0525013 3185.09 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 53.76 using 59 PHA bins.
# Reduced chi-squared = 0.9774 for 55 degrees of freedom
# Null hypothesis probability = 5.222653e-01
Photon flux (15-150 keV) in 43.23 sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 6.40154e-06 ( 0 0 ) ergs/cm2
Single BB
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 13.1403 ( )
R^2/D10^2 : 0.363995 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 509.94 using 59 PHA bins.
# Reduced chi-squared = 8.9463 for 57 degrees of freedom
# Null hypothesis probability = 5.456606e-74
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.761e-07 2.896e-08
25- 50 2.007e-06 6.441e-08
50-150 2.205e-06 1.063e-07
15-150 4.788e-06 1.297e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 95.9595 (-8.36757 9.73001)
Norm : 10.1145 (-0.432063 0.457673)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 82.46 using 59 PHA bins.
# Reduced chi-squared = 1.447 for 57 degrees of freedom
# Null hypothesis probability = 1.534870e-02
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.142e-06 6.506e-08
25- 50 1.959e-06 6.701e-08
50-150 3.100e-06 6.975e-07
15-150 6.201e-06 7.241e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.26123 (-0.493902 0.507408)
R1^2/D10^2 : 2.66401 (-0.588381 0.811318)
kT2 [keV] : 27.8435 (-2.61651 3.29319)
R2^2/D10^2 : 1.60551E-02 (-0.00533118 0.00722538)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 61.09 using 59 PHA bins.
# Reduced chi-squared = 1.111 for 55 degrees of freedom
# Null hypothesis probability = 2.665479e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.100e-06 8.841e-08
25- 50 2.012e-06 9.057e-08
50-150 3.234e-06 2.695e-07
15-150 6.346e-06 3.350e-07
Peak spectrum fit
Power-law model
Time interval is from 2.296 sec. to 3.296 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.70336 ( -0.0729188 0.0735909 )
Norm@50keV : 0.101943 ( -0.00427478 0.00425852 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 56.44 using 59 PHA bins.
# Reduced chi-squared = 0.9902 for 57 degrees of freedom
# Null hypothesis probability = 4.960543e-01
Photon flux (15-150 keV) in 1 sec: 13.5551 ( -0.589538 0.590873 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.43627e-07 ( -4.10211e-08 4.11038e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 2.296 sec. to 3.296 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.54476 ( -0.278735 0.196087 )
Epeak [keV] : 149.325 ( )
Norm@50keV : 0.121913 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 55.39 using 59 PHA bins.
# Reduced chi-squared = 0.9892 for 56 degrees of freedom
# Null hypothesis probability = 4.977414e-01
Photon flux (15-150 keV) in 1 sec: 13.4339 ( -0.6193 0.621 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.35577e-07 ( -4.3667e-08 4.347e-08 ) ergs/cm2
Band function
Time interval is from 2.296 sec. to 3.296 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.501600 ( -1.04234 5.41123 )
beta : -1.78357 ( -0.12751 0.107082 )
Epeak [keV] : 40.0589 ( -18.8907 55.3771 )
Norm@50keV : 0.609326 ( -0.602939 9018.6 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 53.34 using 59 PHA bins.
# Reduced chi-squared = 0.9697 for 55 degrees of freedom
# Null hypothesis probability = 5.384747e-01
Photon flux (15-150 keV) in 1 sec: 13.2497 ( ) 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] : 13.9268 ( )
R^2/D10^2 : 1.86294 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 228.80 using 59 PHA bins.
# Reduced chi-squared = 4.0140 for 57 degrees of freedom
# Null hypothesis probability = 1.919221e-22
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.636e-08 6.295e-09
25- 50 2.825e-07 1.455e-08
50-150 3.598e-07 2.935e-08
15-150 7.187e-07 3.630e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 143.693 ( )
Norm : 55.7717 (-2.98738 2.99602)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 57.79 using 59 PHA bins.
# Reduced chi-squared = 1.014 for 57 degrees of freedom
# Null hypothesis probability = 4.460452e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.407e-07 1.030e-08
25- 50 2.612e-07 1.865e-08
50-150 5.178e-07 1.475e-07
15-150 9.196e-07 1.510e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.21865 (-0.752813 0.796001)
R1^2/D10^2 : 14.5254 (-4.4501 7.05867)
kT2 [keV] : 28.0885 (-3.4452 4.70354)
R2^2/D10^2 : 0.112708 (-0.0476822 0.0704874)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 50.55 using 59 PHA bins.
# Reduced chi-squared = 0.9191 for 55 degrees of freedom
# Null hypothesis probability = 6.452120e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.399e-07 1.615e-08
25- 50 2.689e-07 2.310e-08
50-150 5.286e-07 9.105e-08
15-150 9.374e-07 1.180e-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: 1.87647 ( -0.0456979 0.0458889 )
Norm@50keV : 4.50561E-02 ( -0.00107201 0.00107121 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 45.10 using 59 PHA bins.
# Reduced chi-squared = 0.7912 for 57 degrees of freedom
# Null hypothesis probability = 8.728526e-01
Photon flux (15-150 keV) in 11.64 sec: 6.40240 ( -0.181082 0.182042 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.82128e-06 ( -1.14693e-07 1.14723e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.79415 ( -0.180425 0.120401 )
Epeak [keV] : 134.728 ( )
Norm@50keV : 4.92151E-02 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 44.46 using 59 PHA bins.
# Reduced chi-squared = 0.7938 for 56 degrees of freedom
# Null hypothesis probability = 8.669761e-01
Photon flux (15-150 keV) in 11.64 sec: 6.35272 ( -0.20592 0.20737 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.79631e-06 ( -1.28273e-07 1.2719e-07 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.21113 ( -0.711241 6.12201 )
beta : -1.92074 ( 1.92091 0.064519 )
Epeak [keV] : 41.0562 ( -16.8841 341.187 )
Norm@50keV : 0.115039 ( -0.0711327 10832.8 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 42.12 using 59 PHA bins.
# Reduced chi-squared = 0.7659 for 55 degrees of freedom
# Null hypothesis probability = 8.987049e-01
Photon flux (15-150 keV) in 11.64 sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 4.75046e-06 ( 0 0 ) ergs/cm2
S(25-50 keV) vs. S(50-100 keV) plot
S(25-50 keV) = 1.91e-06
S(50-100 keV) = 2.01e-06
T90 vs. Hardness ratio plot
T90 = 30.191999912262 sec.
Hardness ratio (energy fluence ratio) = 1.05236
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.20122
Count Ratio (50-100 keV) / (15-25 keV) = 0.703118
Mask shadow pattern
IMX = 7.795257443649564E-01, IMY = -4.273236697306579E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.512000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.512000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.512000
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:
-239.520000 -1.856000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
285.1341 -25.1333 0.0 48.6 -135.1 0.5448 0.7 13.8 HT1900.1-2455
299.5990 35.1945 2.0 45.5 -45.9 2.5643 5.7 0.6 Cyg X-1
308.1438 40.9982 1.7 46.1 -33.6 2.3322 6.7 3.1 Cyg X-3
326.3221 38.3048 5.0 39.5 -15.0 0.5112 2.3 7.2 Cyg X-2
337.0766 43.4778 3.5 45.1 -3.4 0.9242 3.3 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-1.856000 9.780590
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
285.1216 -25.1207 17.6 48.6 -135.0 -0.1052 -0.7 12.9 HT1900.1-2455
299.6558 35.2308 6.8 45.5 -45.8 -0.2245 -1.7 3.7 Cyg X-1
308.2612 40.9829 84.5 46.1 -33.5 0.0137 0.1 7.1 Cyg X-3
326.3466 38.3763 5.0 39.5 -15.0 -0.1851 -2.3 8.9 Cyg X-2
358.6351 29.4305 0.2 41.6 28.7 8.3349 54.2 ------ UNKNOWN
315.3471 -9.9365 3.0 16.2 -135.4 0.1932 3.8 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
113.180600 850.580610
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
299.4851 35.2952 9.5 49.6 174.9 1.2050 1.2 7.6 Cyg X-1
308.1191 40.9370 2.0 42.3 -178.2 3.1880 5.7 1.0 Cyg X-3
326.2021 38.4517 4.2 28.2 179.3 1.0150 2.7 7.9 Cyg X-2
296.2195 48.9517 3.6 50.6 -167.0 3.2605 3.2 ------ UNKNOWN
49.9397 20.5409 2.4 47.0 -29.5 3.2798 4.8 ------ UNKNOWN
Plot creation:
Sat May 30 15:45:34 EDT 2015