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
351.7377 26.5679 0.0045 32.6320 59.3781 2.7841195 42.847 TRIG_00431764
Foreground time interval of the image:
-0.708 4.520 (delta_t = 5.228 [sec])
Background time interval of the image:
-239.440 -0.708 (delta_t = 238.732 [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 -0.708 sec. to 4.520 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.16502 ( -0.0568583 0.0566231 )
Norm@50keV : 3.69589E-02 ( -0.00121655 0.00121589 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 61.05 using 59 PHA bins.
# Reduced chi-squared = 1.071 for 57 degrees of freedom
# Null hypothesis probability = 3.324200e-01
Photon flux (15-150 keV) in 5.228 sec: 4.31791 ( -0.148951 0.149401 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.98021e-06 ( -6.91738e-08 6.92454e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.708 sec. to 4.520 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.736292 ( -0.241284 0.229043 )
Epeak [keV] : 172.191 ( -41.4014 123.309 )
Norm@50keV : 5.69841E-02 ( -0.0114747 0.01513 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 50.40 using 59 PHA bins.
# Reduced chi-squared = 0.8999 for 56 degrees of freedom
# Null hypothesis probability = 6.860696e-01
Photon flux (15-150 keV) in 5.228 sec: 4.23447 ( -0.1547 0.15493 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.95088e-06 ( -7.21412e-08 7.19425e-08 ) ergs/cm2
Band function
Time interval is from -0.708 sec. to 4.520 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.736312 ( -0.184544 0.224419 )
beta : -10.0000 ( 10 5.32907e-15 )
Epeak [keV] : 172.176 ( -30.4708 123.152 )
Norm@50keV : 5.69800E-02 ( -0.0114704 0.0151402 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 50.40 using 59 PHA bins.
# Reduced chi-squared = 0.9163 for 55 degrees of freedom
# Null hypothesis probability = 6.509227e-01
Photon flux (15-150 keV) in 5.228 sec: 4.24038 ( ) 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] : 20.8245 ( )
R^2/D10^2 : 0.178282 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 190.18 using 59 PHA bins.
# Reduced chi-squared = 3.3366 for 57 degrees of freedom
# Null hypothesis probability = 3.076420e-16
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.664e-08 5.045e-09
25- 50 3.919e-07 1.981e-08
50-150 1.266e-06 6.274e-08
15-150 1.734e-06 7.006e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.363 ( )
Norm : 18.1746 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 190.22 using 59 PHA bins.
# Reduced chi-squared = 3.3372 for 57 degrees of freedom
# Null hypothesis probability = 3.036536e-16
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.366e-07 8.286e-09
25- 50 4.551e-07 1.702e-08
50-150 9.982e-07 3.555e-08
15-150 1.690e-06 5.646e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.65689 (-1.0267 1.18419)
R1^2/D10^2 : 2.34322 (-0.853245 1.45874)
kT2 [keV] : 29.7692 (-2.59594 3.4798)
R2^2/D10^2 : 4.76227E-02 (-0.0151237 0.0179311)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 45.68 using 59 PHA bins.
# Reduced chi-squared = 0.8306 for 55 degrees of freedom
# Null hypothesis probability = 8.104769e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.601e-07 2.692e-08
25- 50 4.165e-07 3.649e-08
50-150 1.385e-06 1.129e-07
15-150 1.962e-06 1.610e-07
Peak spectrum fit
Power-law model
Time interval is from 0.104 sec. to 1.104 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.06319 ( -0.0640873 0.0637516 )
Norm@50keV : 9.51735E-02 ( -0.00371251 0.00371072 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 67.92 using 59 PHA bins.
# Reduced chi-squared = 1.192 for 57 degrees of freedom
# Null hypothesis probability = 1.524917e-01
Photon flux (15-150 keV) in 1 sec: 11.0034 ( -0.439144 0.439481 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.00707e-06 ( -4.24572e-08 4.25044e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.104 sec. to 1.104 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.494233 ( -0.27703 0.260856 )
Epeak [keV] : 153.042 ( -32.0215 77.739 )
Norm@50keV : 0.171047 ( -0.0392471 0.0541616 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 53.07 using 59 PHA bins.
# Reduced chi-squared = 0.9477 for 56 degrees of freedom
# Null hypothesis probability = 5.864264e-01
Photon flux (15-150 keV) in 1 sec: 10.8258 ( -0.4456 0.4462 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.90778e-07 ( -4.4337e-08 4.4112e-08 ) ergs/cm2
Band function
Time interval is from 0.104 sec. to 1.104 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.494151 ( -0.24955 0.175906 )
beta : -10.0000 ( 10 20 )
Epeak [keV] : 153.012 ( -20.7189 77.7464 )
Norm@50keV : 0.171057 ( -0.0393265 0.0541687 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 53.07 using 59 PHA bins.
# Reduced chi-squared = 0.9649 for 55 degrees of freedom
# Null hypothesis probability = 5.486542e-01
Photon flux (15-150 keV) in 1 sec: 10.8546 ( ) 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] : 21.2632 ( )
R^2/D10^2 : 0.445178 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 140.81 using 59 PHA bins.
# Reduced chi-squared = 2.4704 for 57 degrees of freedom
# Null hypothesis probability = 4.814881e-09
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.782e-08 2.940e-09
25- 50 1.959e-07 1.065e-08
50-150 6.608e-07 4.045e-08
15-150 8.946e-07 4.280e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.363 ( )
Norm : 44.8237 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 215.14 using 59 PHA bins.
# Reduced chi-squared = 3.7744 for 57 degrees of freedom
# Null hypothesis probability = 3.327967e-20
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.116e-07 4.700e-09
25- 50 2.147e-07 9.350e-09
50-150 4.709e-07 2.200e-08
15-150 7.972e-07 3.475e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 8.89928 (-1.42447 1.65432)
R1^2/D10^2 : 3.48026 (-1.29342 2.32773)
kT2 [keV] : 32.2129 (-3.7786 5.77409)
R2^2/D10^2 : 9.76103E-02 (-0.0418523 0.0532118)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 48.53 using 59 PHA bins.
# Reduced chi-squared = 0.8824 for 55 degrees of freedom
# Null hypothesis probability = 7.185895e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.850e-08 1.255e-08
25- 50 2.075e-07 2.525e-08
50-150 7.240e-07 1.249e-07
15-150 1.000e-06 1.377e-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: 1.16502 ( -0.0568583 0.0566231 )
Norm@50keV : 3.69589E-02 ( -0.00121655 0.00121589 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 61.05 using 59 PHA bins.
# Reduced chi-squared = 1.071 for 57 degrees of freedom
# Null hypothesis probability = 3.324200e-01
Photon flux (15-150 keV) in 5.228 sec: 4.31791 ( -0.148951 0.149401 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.98021e-06 ( -6.91738e-08 6.92454e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.736292 ( -0.241284 0.229043 )
Epeak [keV] : 172.191 ( -41.4014 123.309 )
Norm@50keV : 5.69841E-02 ( -0.0114747 0.01513 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 50.40 using 59 PHA bins.
# Reduced chi-squared = 0.8999 for 56 degrees of freedom
# Null hypothesis probability = 6.860696e-01
Photon flux (15-150 keV) in 5.228 sec: 4.23447 ( -0.1547 0.15493 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.95088e-06 ( -7.21412e-08 7.19425e-08 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.736312 ( -0.184544 0.288977 )
beta : -10.0000 ( 10 1.77636e-15 )
Epeak [keV] : 172.176 ( -30.4709 123.152 )
Norm@50keV : 5.69800E-02 ( -0.0114704 0.0151402 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 50.40 using 59 PHA bins.
# Reduced chi-squared = 0.9163 for 55 degrees of freedom
# Null hypothesis probability = 6.509227e-01
Photon flux (15-150 keV) in 5.228 sec: 4.24038 ( ) 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) = 4.07e-07
S(50-100 keV) = 7.26e-07
T90 vs. Hardness ratio plot
T90 = 2.88399994373322 sec.
Hardness ratio (energy fluence ratio) = 1.78378
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.78637
Count Ratio (50-100 keV) / (15-25 keV) = 1.84793
Mask shadow pattern
IMX = 3.261569951733025E-01, IMY = -5.510208954698624E-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:
-239.440000 -0.708000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
299.5583 35.2204 1.3 38.0 142.1 3.1574 9.0 1.9 Cyg X-1
308.0023 41.0050 1.9 29.3 139.1 1.4112 6.0 5.8 Cyg X-3
326.3268 38.4021 3.9 23.8 109.2 0.6413 3.0 8.7 Cyg X-2
50.9140 22.1781 2.2 58.6 -11.0 4.4584 5.2 ------ UNKNOWN
227.5361 63.9743 3.2 48.4 -141.2 1.8345 3.6 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-0.708000 4.520000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
299.7080 35.3371 5.0 37.8 142.0 -0.1523 -2.3 10.0 Cyg X-1
308.2442 40.9077 6.0 29.3 138.7 0.0930 2.0 6.6 Cyg X-3
325.9888 38.2441 15.7 24.1 109.6 0.0348 0.7 9.8 Cyg X-2
351.7377 26.5679 0.3 32.6 59.4 2.7841 42.8 ------ UNKNOWN
242.4780 45.3912 2.4 58.1 -163.7 0.5976 4.9 ------ UNKNOWN
239.8627 54.4594 3.2 51.9 -155.3 0.2461 3.6 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
71.660600 612.560600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
299.6081 35.1669 2.2 45.1 168.9 3.7204 5.3 2.3 Cyg X-1
308.1191 40.9448 2.0 38.6 177.9 2.6861 5.7 0.6 Cyg X-3
326.2912 38.2432 2.9 24.3 179.6 1.1605 3.9 7.3 Cyg X-2
353.6561 -12.5856 2.6 39.2 51.7 3.1458 4.5 ------ UNKNOWN
320.3903 45.6802 2.4 31.4 -169.6 1.5469 4.9 ------ UNKNOWN
292.7825 56.6052 3.5 51.2 -162.6 2.4777 3.3 ------ UNKNOWN
314.6715 70.1629 2.6 48.5 -141.2 3.7674 4.4 ------ UNKNOWN
Plot creation:
Sun May 31 00:04:40 EDT 2015