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
20.4669 -12.9538 0.0111 27.7905 20.7818 0.8745436 17.229 TRIG_00154112
Foreground time interval of the image:
-6.816 15.840 (delta_t = 22.656 [sec])
Background time interval of the image:
-299.104 -6.816 (delta_t = 292.288 [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 2.048000
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 2.048000
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 2.048000
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 -6.816 sec. to 15.840 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.83264 ( -0.154318 0.159634 )
Norm@50keV : 2.31804E-03 ( -0.000241785 0.000238221 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 54.75 using 59 PHA bins.
# Reduced chi-squared = 0.9606 for 57 degrees of freedom
# Null hypothesis probability = 5.598560e-01
Photon flux (15-150 keV) in 22.66 sec: 0.323553 ( -0.0287835 0.0287918 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.8312e-07 ( -5.04244e-08 5.1198e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -6.816 sec. to 15.840 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.936602 ( -0.82513 0.688289 )
Epeak [keV] : 50.4617 ( -9.61363 31.3107 )
Norm@50keV : 7.51652E-03 ( -0.00441821 0.0148383 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 49.60 using 59 PHA bins.
# Reduced chi-squared = 0.8856 for 56 degrees of freedom
# Null hypothesis probability = 7.143657e-01
Photon flux (15-150 keV) in 22.66 sec: 0.313256 ( -0.02973 0.029767 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.42212e-07 ( -5.59906e-08 5.88571e-08 ) ergs/cm2
Band function
Time interval is from -6.816 sec. to 15.840 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 1.37443 ( -1.68003 -0.297156 )
beta : -2.16770 ( 2.18091 0.311966 )
Epeak [keV] : 32.0040 ( -11.0929 25.021 )
Norm@50keV : 0.339251 ( -0.336208 81.9854 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 47.82 using 59 PHA bins.
# Reduced chi-squared = 0.8695 for 55 degrees of freedom
# Null hypothesis probability = 7.429662e-01
Photon flux (15-150 keV) in 22.66 sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 4.58337e-07 ( -4.58178e-07 -5.26482e-08 ) ergs/cm2
Single BB
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 10.7940 (-1.08769 1.22315)
R^2/D10^2 : 0.116452 (-0.0387701 0.0573302)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 67.18 using 59 PHA bins.
# Reduced chi-squared = 1.179 for 57 degrees of freedom
# Null hypothesis probability = 1.677101e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.398e-08 1.019e-08
25- 50 1.765e-07 1.852e-08
50-150 1.145e-07 2.734e-08
15-150 3.550e-07 3.932e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 86.5525 (-22.4799 37.478)
Norm : 1.49475 (-0.18467 0.217593)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 50.23 using 59 PHA bins.
# Reduced chi-squared = 0.8811 for 57 degrees of freedom
# Null hypothesis probability = 7.252200e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.825e-08 1.185e-08
25- 50 1.480e-07 1.468e-08
50-150 2.199e-07 9.285e-08
15-150 4.561e-07 9.755e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.77424 (-1.68808 1.83056)
R1^2/D10^2 : 0.445786 (-0.231082 0.367342)
kT2 [keV] : 20.5441 (-5.55701 14.7196)
R2^2/D10^2 : 6.74617E-03 (-0.00586969 0.0191182)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 47.75 using 59 PHA bins.
# Reduced chi-squared = 0.8682 for 55 degrees of freedom
# Null hypothesis probability = 7.453341e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.419e-08 2.973e-08
25- 50 1.547e-07 6.492e-08
50-150 2.093e-07 1.104e-07
15-150 4.482e-07 1.860e-07
Peak spectrum fit
Power-law model
Time interval is from 1.656 sec. to 2.656 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.48468 ( -0.310829 0.316317 )
Norm@50keV : 5.60849E-03 ( -0.0011051 0.00109457 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 54.36 using 59 PHA bins.
# Reduced chi-squared = 0.9537 for 57 degrees of freedom
# Null hypothesis probability = 5.746558e-01
Photon flux (15-150 keV) in 1 sec: 0.697319 ( -0.133933 0.134166 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.33408e-08 ( -1.13431e-08 1.15645e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 1.656 sec. to 2.656 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.228703 ( -2.0766 1.36428 )
Epeak [keV] : 67.9212 ( -16.2523 -67.9211 )
Norm@50keV : 2.51794E-02 ( -0.0251796 0.26041 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 52.11 using 59 PHA bins.
# Reduced chi-squared = 0.9305 for 56 degrees of freedom
# Null hypothesis probability = 6.229793e-01
Photon flux (15-150 keV) in 1 sec: 0.667169 ( -0.139527 0.1392 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.86884e-08 ( -1.19018e-08 1.27492e-08 ) ergs/cm2
Band function
Time interval is from 1.656 sec. to 2.656 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.228642 ( -0.738484 0.686258 )
beta : -10.0000 ( 10 5.32907e-15 )
Epeak [keV] : 67.9089 ( -18.3155 225.672 )
Norm@50keV : 2.51831E-02 ( -0.0251831 0.261382 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 52.11 using 59 PHA bins.
# Reduced chi-squared = 0.9474 for 55 degrees of freedom
# Null hypothesis probability = 5.858644e-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] : 14.4945 (-2.69764 3.50126)
R^2/D10^2 : 9.38351E-02 (-0.0506644 0.101029)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 54.10 using 59 PHA bins.
# Reduced chi-squared = 0.9491 for 57 degrees of freedom
# Null hypothesis probability = 5.845930e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.148e-09 1.573e-09
25- 50 1.596e-08 4.926e-09
50-150 2.246e-08 8.860e-09
15-150 4.257e-08 1.214e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.361 (-107.899 -199.362)
Norm : 2.87926 (-0.542603 0.543373)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 53.46 using 59 PHA bins.
# Reduced chi-squared = 0.9380 for 57 degrees of freedom
# Null hypothesis probability = 6.085450e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.170e-09 4.134e-09
25- 50 1.379e-08 7.960e-09
50-150 3.025e-08 1.752e-08
15-150 5.121e-08 2.894e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.36344 (-6.36344 -6.36344)
R1^2/D10^2 : 0.614042 (-0.614042 -0.614042)
kT2 [keV] : 18.3040 (-18.304 -18.304)
R2^2/D10^2 : 3.44188E-02 (-0.0344188 0.106481)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 52.22 using 59 PHA bins.
# Reduced chi-squared = 0.9495 for 55 degrees of freedom
# Null hypothesis probability = 5.814539e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.874e-09 3.373e-09
25- 50 1.480e-08 7.755e-09
50-150 2.673e-08 1.543e-08
15-150 4.740e-08 2.459e-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: 1.83264 ( -0.154318 0.159634 )
Norm@50keV : 2.31804E-03 ( -0.000241785 0.000238221 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 54.75 using 59 PHA bins.
# Reduced chi-squared = 0.9606 for 57 degrees of freedom
# Null hypothesis probability = 5.598560e-01
Photon flux (15-150 keV) in 22.66 sec: 0.323553 ( -0.0287835 0.0287918 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.8312e-07 ( -5.04244e-08 5.1198e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.936602 ( -0.82513 0.688289 )
Epeak [keV] : 50.4617 ( -9.61363 31.3107 )
Norm@50keV : 7.51652E-03 ( -0.00441821 0.0148383 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 49.60 using 59 PHA bins.
# Reduced chi-squared = 0.8856 for 56 degrees of freedom
# Null hypothesis probability = 7.143657e-01
Photon flux (15-150 keV) in 22.66 sec: 0.313256 ( -0.02973 0.029767 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.42212e-07 ( -5.59906e-08 5.88571e-08 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 1.37443 ( -1.68003 -0.297156 )
beta : -2.16770 ( 2.18091 0.311966 )
Epeak [keV] : 32.0040 ( -11.0929 25.0215 )
Norm@50keV : 0.339251 ( -0.336208 81.9824 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 47.82 using 59 PHA bins.
# Reduced chi-squared = 0.8695 for 55 degrees of freedom
# Null hypothesis probability = 7.429662e-01
Photon flux (15-150 keV) in 22.66 sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 4.58337e-07 ( -4.58178e-07 -5.26482e-08 ) ergs/cm2
S(25-50 keV) vs. S(50-100 keV) plot
S(25-50 keV) = 1.38e-07
S(50-100 keV) = 1.55e-07
T90 vs. Hardness ratio plot
T90 = 18.2840000092983 sec.
Hardness ratio (energy fluence ratio) = 1.12319
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.24906
Count Ratio (50-100 keV) / (15-25 keV) = 0.695385
Mask shadow pattern
IMX = 4.927397904715308E-01, IMY = -1.869951146872751E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 2.048000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 2.048000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 2.048000
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:
-299.104000 -6.816000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
326.0351 38.2796 66.1 48.5 164.2 0.0837 0.2 6.9 Cyg X-2
345.5004 -6.6037 2.7 34.8 90.4 1.7864 4.3 ------ UNKNOWN
14.7479 -32.7721 2.3 46.8 33.8 2.8199 5.2 ------ UNKNOWN
36.2750 -34.2349 2.9 52.8 11.5 2.6042 4.0 ------ UNKNOWN
324.3529 50.9774 3.4 54.1 178.9 2.1064 3.4 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-6.816000 15.840000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
326.2186 38.4265 6.7 48.4 164.4 0.2029 1.7 6.7 Cyg X-2
346.9470 -14.9725 2.4 39.3 78.4 0.7820 4.7 ------ UNKNOWN
25.0290 -36.2399 2.9 51.4 23.3 0.7993 4.0 ------ UNKNOWN
340.2874 27.9765 2.5 34.0 154.6 0.2820 4.7 ------ UNKNOWN
20.4669 -12.9538 0.7 27.8 20.8 0.8745 17.2 ------ UNKNOWN
60.7091 -20.0012 3.1 57.4 -19.7 0.7463 3.7 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
88.996600 127.091700
127.896000 302.966000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
359.7649 8.0873 2.5 29.5 125.4 0.9363 4.7 485.4 UNKNOWN
52.8823 37.1839 3.5 58.7 -159.3 3.5145 3.3 ------ UNKNOWN
62.3643 -7.1556 2.6 41.6 -103.1 2.9247 4.5 ------ UNKNOWN
Plot creation:
Sun May 31 15:43:10 EDT 2015