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
44.8327 13.7620 0.0076 32.3021 -45.9966 2.7447121 25.421 TRIG_00529486
Foreground time interval of the image:
-35.680 15.981 (delta_t = 51.661 [sec])
Background time interval of the image:
-239.120 -35.680 (delta_t = 203.440 [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)
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 -35.680 sec. to 27.952 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.84527 ( -0.100588 0.102385 )
Norm@50keV : 2.96943E-03 ( -0.000181775 0.000180288 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 58.68 using 59 PHA bins.
# Reduced chi-squared = 1.030 for 57 degrees of freedom
# Null hypothesis probability = 4.135033e-01
Photon flux (15-150 keV) in 63.63 sec: 0.416585 ( -0.0235833 0.0236209 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.73742e-06 ( -1.06739e-07 1.07469e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -35.680 sec. to 27.952 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.21810 ( -0.497494 0.441783 )
Epeak [keV] : 57.2574 ( -9.44075 29.9469 )
Norm@50keV : 6.42760E-03 ( -0.00265521 0.00534249 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 52.57 using 59 PHA bins.
# Reduced chi-squared = 0.9388 for 56 degrees of freedom
# Null hypothesis probability = 6.054401e-01
Photon flux (15-150 keV) in 63.63 sec: 0.402845 ( -0.025452 0.025398 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.64277e-06 ( -1.24002e-07 1.2537e-07 ) ergs/cm2
Band function
Time interval is from -35.680 sec. to 27.952 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.04201 ( -0.533932 0.764739 )
beta : -2.28341 ( 2.29121 0.331257 )
Epeak [keV] : 51.7047 ( -11.3707 22.8276 )
Norm@50keV : 8.22800E-03 ( -0.00469064 0.0154216 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 51.56 using 59 PHA bins.
# Reduced chi-squared = 0.9374 for 55 degrees of freedom
# Null hypothesis probability = 6.069394e-01
Photon flux (15-150 keV) in 63.63 sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 1.64956e-06 ( -1.64912e-06 -1.19701e-07 ) ergs/cm2
Single BB
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 11.9450 (-0.739757 0.793129)
R^2/D10^2 : 9.95643E-02 (-0.0214671 0.0271884)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 102.35 using 59 PHA bins.
# Reduced chi-squared = 1.7956 for 57 degrees of freedom
# Null hypothesis probability = 2.148199e-04
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.911e-07 1.982e-08
25- 50 5.982e-07 4.193e-08
50-150 5.116e-07 6.576e-08
15-150 1.301e-06 8.749e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 92.5818 (-16.618 23.1532)
Norm : 1.86437 (-0.151812 0.169694)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 52.63 using 59 PHA bins.
# Reduced chi-squared = 0.9233 for 57 degrees of freedom
# Null hypothesis probability = 6.397010e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.098e-07 3.169e-08
25- 50 5.271e-07 3.315e-08
50-150 8.166e-07 2.491e-07
15-150 1.654e-06 2.558e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 4.72202 (-1.14284 2.16975)
R1^2/D10^2 : 1.78429 (-1.29584 4.26242)
kT2 [keV] : 16.0464 (-2.00105 4.78602)
R2^2/D10^2 : 2.75210E-02 (-0.0187497 0.0237836)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 57.75 using 59 PHA bins.
# Reduced chi-squared = 1.050 for 55 degrees of freedom
# Null hypothesis probability = 3.739888e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.116e-07 1.134e-07
25- 50 5.166e-07 9.614e-08
50-150 7.119e-07 1.230e-07
15-150 1.540e-06 2.669e-07
Peak spectrum fit
Power-law model
Time interval is from 7.940 sec. to 8.940 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.65906 ( -0.122207 0.124378 )
Norm@50keV : 2.31435E-02 ( -0.00175725 0.00174509 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 60.78 using 59 PHA bins.
# Reduced chi-squared = 1.066 for 57 degrees of freedom
# Null hypothesis probability = 3.412683e-01
Photon flux (15-150 keV) in 1 sec: 3.03106 ( -0.221184 0.221416 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.15047e-07 ( -1.72213e-08 1.73419e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 7.940 sec. to 8.940 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.19407 ( -0.531044 0.469511 )
Epeak [keV] : 84.0566 ( -23.3221 915.148 )
Norm@50keV : 4.04226E-02 ( -0.0170437 0.0353324 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 57.91 using 59 PHA bins.
# Reduced chi-squared = 1.034 for 56 degrees of freedom
# Null hypothesis probability = 4.045862e-01
Photon flux (15-150 keV) in 1 sec: 2.97621 ( -0.22798 0.22796 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.08238e-07 ( -1.8867e-08 1.8795e-08 ) ergs/cm2
Band function
Time interval is from 7.940 sec. to 8.940 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.19384 ( -0.3426 0.525644 )
beta : -10.0000 ( 10 3.55271e-15 )
Epeak [keV] : 84.0299 ( -19.9379 1290.38 )
Norm@50keV : 4.04280E-02 ( -0.0170579 0.035335 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 57.91 using 59 PHA bins.
# Reduced chi-squared = 1.053 for 55 degrees of freedom
# Null hypothesis probability = 3.683524e-01
Photon flux (15-150 keV) in 1 sec: 2.97216 ( 4.02784 -0.22383 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.08174e-07 ( -2.08167e-07 -1.8312e-08 ) ergs/cm2
Single BB
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 12.8072 (-1.12911 1.27791)
R^2/D10^2 : 0.588000 (-0.1725 0.236174)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 98.63 using 59 PHA bins.
# Reduced chi-squared = 1.730 for 57 degrees of freedom
# Null hypothesis probability = 5.179914e-04
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.046e-08 2.645e-09
25- 50 6.932e-08 6.220e-09
50-150 7.125e-08 1.162e-08
15-150 1.610e-07 1.350e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 150.192 (-43.3008 -149.063)
Norm : 12.4963 (-1.00646 1.24118)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 57.97 using 59 PHA bins.
# Reduced chi-squared = 1.017 for 57 degrees of freedom
# Null hypothesis probability = 4.392643e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.209e-08 3.140e-09
25- 50 5.949e-08 1.144e-08
50-150 1.175e-07 4.711e-08
15-150 2.091e-07 6.095e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 8.07061 (-1.36324 1.39239)
R1^2/D10^2 : 2.23775 (-0.89067 1.81447)
kT2 [keV] : 29.2936 (-6.82042 13.2901)
R2^2/D10^2 : 2.05994E-02 (-0.0146498 0.0351688)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 55.22 using 59 PHA bins.
# Reduced chi-squared = 1.004 for 55 degrees of freedom
# Null hypothesis probability = 4.663484e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.933e-08 6.785e-09
25- 50 6.428e-08 1.333e-08
50-150 1.176e-07 5.383e-08
15-150 2.112e-07 6.977e-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: 1.77534 ( -0.0961446 0.0975465 )
Norm@50keV : 3.41589E-03 ( -0.000200817 0.000199546 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 71.93 using 59 PHA bins.
# Reduced chi-squared = 1.262 for 57 degrees of freedom
# Null hypothesis probability = 8.791885e-02
Photon flux (15-150 keV) in 51.66 sec: 0.466276 ( -0.0259598 0.0260005 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.62618e-06 ( -9.80156e-08 9.86153e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.954961 ( -0.500322 0.44503 )
Epeak [keV] : 59.1546 ( -8.15411 18.1345 )
Norm@50keV : 9.30103E-03 ( -0.00384499 0.00770242 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 61.16 using 59 PHA bins.
# Reduced chi-squared = 1.092 for 56 degrees of freedom
# Null hypothesis probability = 2.960565e-01
Photon flux (15-150 keV) in 51.66 sec: 0.447301 ( -0.02784 0.027805 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.51643e-06 ( -1.12014e-07 1.13575e-07 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.725416 ( -0.572315 0.763318 )
beta : -2.33762 ( 2.3481 0.356536 )
Epeak [keV] : 53.0792 ( -10.0181 17.1194 )
Norm@50keV : 1.28360E-02 ( -0.00647253 0.0238926 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 59.93 using 59 PHA bins.
# Reduced chi-squared = 1.090 for 55 degrees of freedom
# Null hypothesis probability = 3.014343e-01
Photon flux (15-150 keV) in 51.66 sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 1.52813e-06 ( -1.52777e-06 -1.09152e-07 ) ergs/cm2
S(25-50 keV) vs. S(50-100 keV) plot
S(25-50 keV) = 4.97e-07
S(50-100 keV) = 5.54e-07
T90 vs. Hardness ratio plot
T90 = 50.2880000472069 sec.
Hardness ratio (energy fluence ratio) = 1.11469
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.24243
Count Ratio (50-100 keV) / (15-25 keV) = 0.704864
Mask shadow pattern
IMX = 4.392073192457991E-01, IMY = 4.547580763038182E-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:
-239.120000 -35.680000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
326.3360 38.3329 27.1 42.0 157.3 0.1313 0.4 7.8 Cyg X-2
331.1518 50.3189 2.7 42.3 175.9 0.9857 4.3 ------ UNKNOWN
45.8008 -17.2387 2.9 51.6 -8.4 1.3067 4.1 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-35.680000 15.980590
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
326.2827 38.1698 9.9 42.0 157.1 0.1642 1.2 10.5 Cyg X-2
350.0969 10.1989 1.8 24.2 97.7 0.6013 6.4 ------ UNKNOWN
49.3809 -21.2437 2.6 56.8 -8.3 1.3935 4.4 ------ UNKNOWN
44.8327 13.7620 0.5 32.3 -46.0 2.7446 25.4 ------ UNKNOWN
35.7111 39.7690 2.2 26.6 -102.1 0.5136 5.3 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
68.580590 879.380600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6279 22.0115 0.5 37.7 -91.4 33.1795 24.7 0.3 Crab
14.3382 12.9831 2.7 29.7 109.1 2.8728 4.3 ------ UNKNOWN
39.9335 0.8464 3.0 13.8 37.9 1.3505 3.8 ------ UNKNOWN
57.5995 -40.2271 2.5 55.3 5.1 7.2840 4.6 ------ UNKNOWN
58.4875 -41.5812 3.1 56.7 4.7 7.1237 3.7 ------ UNKNOWN
36.3700 41.1525 2.3 28.4 -176.6 2.0023 4.9 ------ UNKNOWN
77.5823 -14.2171 2.7 42.8 -33.6 2.7597 4.2 ------ UNKNOWN
Plot creation:
Sat May 30 18:59:04 EDT 2015