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
348.5833 5.9862 0.0104 10.0018 -119.7654 2.0383631 18.591 TRIG_00442978
Foreground time interval of the image:
-86.260 11.141 (delta_t = 97.401 [sec])
Background time interval of the image:
-239.960 -86.260 (delta_t = 153.700 [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 -86.260 sec. to 239.708 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.47710 ( -0.0525543 0.052583 )
Norm@50keV : 2.34078E-03 ( -6.27817e-05 6.27612e-05 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 50.72 using 59 PHA bins.
# Reduced chi-squared = 0.8899 for 57 degrees of freedom
# Null hypothesis probability = 7.080570e-01
Photon flux (15-150 keV) in 326 sec: 0.290459 ( -0.00842416 0.0084468 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.26703e-06 ( -2.10657e-07 2.1119e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -86.260 sec. to 239.708 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.38243 ( -0.209354 0.124614 )
Epeak [keV] : 347.451 ( -347.458 -347.458 )
Norm@50keV : 2.59294E-03 ( -0.000299739 0.000638449 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 50.09 using 59 PHA bins.
# Reduced chi-squared = 0.8944 for 56 degrees of freedom
# Null hypothesis probability = 6.970847e-01
Photon flux (15-150 keV) in 326 sec: 0.288316 ( -0.009474 0.009498 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.21246e-06 ( -2.44044e-07 2.42577e-07 ) ergs/cm2
Band function
Time interval is from -86.260 sec. to 239.708 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 0.757372 ( -2.01806 -0.755176 )
beta : -1.51490 ( -0.0681511 0.0632757 )
Epeak [keV] : 32.9410 ( -8.77297 112.815 )
Norm@50keV : 9.18280E-02 ( -0.090436 84.9994 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 47.32 using 59 PHA bins.
# Reduced chi-squared = 0.8604 for 55 degrees of freedom
# Null hypothesis probability = 7.595505e-01
Photon flux (15-150 keV) in 326 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] : 16.3070 ( )
R^2/D10^2 : 2.35768E-02 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 333.28 using 59 PHA bins.
# Reduced chi-squared = 5.8469 for 57 degrees of freedom
# Null hypothesis probability = 1.116945e-40
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.207e-07 2.412e-08
25- 50 1.799e-06 7.139e-08
50-150 3.368e-06 1.710e-07
15-150 5.588e-06 1.842e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 ( )
Norm : 1.19016 (-0.0318495 0.0318489)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 62.01 using 59 PHA bins.
# Reduced chi-squared = 1.088 for 57 degrees of freedom
# Null hypothesis probability = 3.022842e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 9.663e-07 2.690e-08
25- 50 1.859e-06 5.444e-08
50-150 4.077e-06 1.157e-07
15-150 6.902e-06 1.956e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.54239 (-0.767577 0.837966)
R1^2/D10^2 : 0.226219 (-0.0659641 0.100885)
kT2 [keV] : 29.1737 (-3.12427 4.37046)
R2^2/D10^2 : 2.58437E-03 (-0.000977432 0.0012742)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 56.55 using 59 PHA bins.
# Reduced chi-squared = 1.028 for 55 degrees of freedom
# Null hypothesis probability = 4.168427e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.377e-07 7.563e-08
25- 50 1.836e-06 1.058e-07
50-150 4.472e-06 3.668e-07
15-150 7.146e-06 4.906e-07
Peak spectrum fit
Power-law model
Time interval is from 33.160 sec. to 34.160 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.895547 ( -0.117749 0.115654 )
Norm@50keV : 1.93111E-02 ( -0.00127135 0.00126788 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 63.87 using 59 PHA bins.
# Reduced chi-squared = 1.121 for 57 degrees of freedom
# Null hypothesis probability = 2.479031e-01
Photon flux (15-150 keV) in 1 sec: 2.21640 ( -0.145957 0.146131 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.171e-07 ( -1.56688e-08 1.57588e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 33.160 sec. to 34.160 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.889002 ( -0.482455 0.151718 )
Epeak [keV] : 9999.96 ( )
Norm@50keV : 1.94396E-02 ( -0.00127591 0.00125391 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 63.86 using 59 PHA bins.
# Reduced chi-squared = 1.140 for 56 degrees of freedom
# Null hypothesis probability = 2.198620e-01
Photon flux (15-150 keV) in 1 sec: 2.21153 ( -0.14943 0.14889 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.16665e-07 ( -1.6188e-08 8.13e-09 ) ergs/cm2
Band function
Time interval is from 33.160 sec. to 34.160 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 5.00000 ( -5 -5 )
beta : -0.896456 ( -0.115861 0.118252 )
Epeak [keV] : 17.2588 ( -17.2598 9981.45 )
Norm@50keV : 1.02325E+04 ( -569.688 2.69576e+06 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 63.83 using 59 PHA bins.
# Reduced chi-squared = 1.161 for 55 degrees of freedom
# Null hypothesis probability = 1.938624e-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] : 24.2087 (-2.26032 2.59898)
R^2/D10^2 : 6.03424E-02 (-0.0158264 0.0208053)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 105.05 using 59 PHA bins.
# Reduced chi-squared = 1.8430 for 57 degrees of freedom
# Null hypothesis probability = 1.110356e-04
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.247e-09 8.735e-10
25- 50 3.485e-08 3.450e-09
50-150 1.521e-07 1.630e-08
15-150 1.932e-07 1.585e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.363 ( )
Norm : 8.66214 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 147.14 using 59 PHA bins.
# Reduced chi-squared = 2.5815 for 57 degrees of freedom
# Null hypothesis probability = 6.638558e-10
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.157e-08 1.800e-09
25- 50 4.149e-08 5.670e-09
50-150 9.100e-08 3.365e-08
15-150 1.541e-07 2.745e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.94479 (-2.17714 2.97747)
R1^2/D10^2 : 0.963709 (-0.578898 1.83655)
kT2 [keV] : 37.1373 (-7.10351 16.0728)
R2^2/D10^2 : 1.49954E-02 (-0.00956334 0.0137632)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 63.99 using 59 PHA bins.
# Reduced chi-squared = 1.163 for 55 degrees of freedom
# Null hypothesis probability = 1.901849e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.375e-08 5.258e-09
25- 50 3.767e-08 1.067e-08
50-150 1.679e-07 5.378e-08
15-150 2.193e-07 4.995e-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: 1.34400 ( -0.131787 0.13199 )
Norm@50keV : 1.25708E-03 ( -9.82411e-05 9.80185e-05 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 65.00 using 59 PHA bins.
# Reduced chi-squared = 1.140 for 57 degrees of freedom
# Null hypothesis probability = 2.180615e-01
Photon flux (15-150 keV) in 97.4 sec: 0.151257 ( -0.0117348 0.0117438 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.19746e-06 ( -1.05521e-07 1.06648e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.269632 ( -0.719853 0.618009 )
Epeak [keV] : 79.4104 ( -14.8749 42.0545 )
Norm@50keV : 4.38819E-03 ( -0.00221512 0.0055412 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 55.32 using 59 PHA bins.
# Reduced chi-squared = 0.9879 for 56 degrees of freedom
# Null hypothesis probability = 5.004651e-01
Photon flux (15-150 keV) in 97.4 sec: 0.143624 ( -0.012486 0.012482 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.08861e-06 ( -1.18838e-07 1.22023e-07 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.272449 ( -0.594775 3.05436 )
beta : -2.42372 ( 2.39006 0.854479 )
Epeak [keV] : 78.7415 ( -38.1641 41.542 )
Norm@50keV : 4.40558E-03 ( -0.00259499 0.484001 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 55.13 using 59 PHA bins.
# Reduced chi-squared = 1.002 for 55 degrees of freedom
# Null hypothesis probability = 4.695755e-01
Photon flux (15-150 keV) in 97.4 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) = 1.78e-06
S(50-100 keV) = 2.55e-06
T90 vs. Hardness ratio plot
T90 = 213.927999973297 sec.
Hardness ratio (energy fluence ratio) = 1.43258
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.38479
Count Ratio (50-100 keV) / (15-25 keV) = 1.04707
Mask shadow pattern
IMX = -8.755345310674198E-02, IMY = 1.530911219523165E-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:
-239.960000 -86.260000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
299.6151 35.1837 2.9 50.5 -15.6 1.2204 4.0 1.6 Cyg X-1
308.0714 40.9569 2.5 45.5 -5.8 1.1753 4.5 1.8 Cyg X-3
325.9567 38.2886 3.3 32.2 1.3 0.5810 3.5 10.3 Cyg X-2
348.9831 52.7371 2.7 37.3 38.4 1.2027 4.2 ------ UNKNOWN
328.6939 42.2884 3.3 33.4 9.3 0.5694 3.5 ------ UNKNOWN
335.1062 -10.7007 2.2 31.0 -105.4 1.0631 5.4 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-86.260000 11.140600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
299.7099 35.2580 12.1 50.4 -15.5 -0.2715 -1.0 6.8 Cyg X-1
308.1128 41.0725 9.3 45.6 -5.7 -0.2933 -1.2 7.2 Cyg X-3
326.2206 38.4512 8.3 32.2 1.7 0.2031 1.4 8.1 Cyg X-2
348.5832 5.9862 0.6 10.0 -119.8 2.0387 18.6 ------ UNKNOWN
303.2187 33.3498 2.8 47.3 -17.4 1.0317 4.1 ------ UNKNOWN
359.2273 -32.1079 2.4 48.1 -147.2 1.3332 4.8 ------ UNKNOWN
325.4373 -15.7449 1.8 40.7 -97.7 3.1098 6.6 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
45.740610 722.076800
780.040000 842.200000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
299.5482 35.1798 3.1 53.6 -18.8 3.4177 3.7 2.4 Cyg X-1
308.1667 40.9602 3.2 50.2 -8.4 3.0321 3.6 2.6 Cyg X-3
326.3099 38.3358 3.8 38.1 2.4 1.6044 3.1 6.6 Cyg X-2
348.5803 5.9845 0.5 0.0 156.3 6.8794 21.5 ------ UNKNOWN
335.4330 -0.8778 3.1 14.8 -86.0 1.1469 3.7 ------ UNKNOWN
14.8857 -47.9707 3.4 58.7 -169.1 6.8478 3.4 ------ UNKNOWN
341.2761 -47.0038 2.8 53.4 -142.6 8.7452 4.1 ------ UNKNOWN
311.0722 -11.0903 3.0 41.0 -83.3 6.2568 3.8 ------ UNKNOWN
Plot creation:
Sat May 30 23:08:45 EDT 2015