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
111.8954 -29.8447 0.0030 34.2671 -118.4470 7.3591946 64.203 TRIG_00224364
Foreground time interval of the image:
-0.488 9.237 (delta_t = 9.725 [sec])
Background time interval of the image:
-239.064 -0.488 (delta_t = 238.576 [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 0.256000
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 0.256000
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 0.256000
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 -0.488 sec. to 35.956 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.33367 ( -0.0416391 0.0415473 )
Norm@50keV : 1.57149E-02 ( -0.000354465 0.000354309 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 46.26 using 59 PHA bins.
# Reduced chi-squared = 0.8116 for 57 degrees of freedom
# Null hypothesis probability = 8.446379e-01
Photon flux (15-150 keV) in 36.44 sec: 1.88695 ( -0.0472203 0.0473467 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.6138e-06 ( -1.30545e-07 1.3062e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.488 sec. to 35.956 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.07296 ( -0.173275 0.166899 )
Epeak [keV] : 207.517 ( -59.5368 245.679 )
Norm@50keV : 2.03812E-02 ( -0.00305354 0.00372892 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 39.03 using 59 PHA bins.
# Reduced chi-squared = 0.6970 for 56 degrees of freedom
# Null hypothesis probability = 9.588205e-01
Photon flux (15-150 keV) in 36.44 sec: 1.85259 ( -0.05139 0.05161 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.54435e-06 ( -1.39638e-07 1.38982e-07 ) ergs/cm2
Band function
Time interval is from -0.488 sec. to 35.956 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.07242 ( -0.611824 1.47644 )
beta : -6.69204 ( 6.22972 16.1966 )
Epeak [keV] : 207.582 ( -30.0069 230.899 )
Norm@50keV : 2.03856E-02 ( -0.000454964 0.00119815 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 39.03 using 59 PHA bins.
# Reduced chi-squared = 0.7097 for 55 degrees of freedom
# Null hypothesis probability = 9.490879e-01
Photon flux (15-150 keV) in 36.44 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] : 19.2579 ( )
R^2/D10^2 : 9.29398E-02 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 387.38 using 59 PHA bins.
# Reduced chi-squared = 6.7962 for 57 degrees of freedom
# Null hypothesis probability = 1.212099e-50
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.457e-07 1.168e-08
25- 50 1.193e-06 3.808e-08
50-150 3.259e-06 1.192e-07
15-150 4.698e-06 1.257e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.363 ( )
Norm : 8.02320 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 142.75 using 59 PHA bins.
# Reduced chi-squared = 2.5044 for 57 degrees of freedom
# Null hypothesis probability = 2.641845e-09
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.280e-07 1.986e-08
25- 50 1.400e-06 3.553e-08
50-150 3.071e-06 7.616e-08
15-150 5.200e-06 1.330e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 8.29806 (-0.782051 0.839742)
R1^2/D10^2 : 0.936546 (-0.244294 0.360198)
kT2 [keV] : 31.1818 (-2.57143 3.35544)
R2^2/D10^2 : 1.50701E-02 (-0.00448281 0.00539188)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 42.97 using 59 PHA bins.
# Reduced chi-squared = 0.7813 for 55 degrees of freedom
# Null hypothesis probability = 8.806031e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.176e-07 4.701e-08
25- 50 1.323e-06 6.905e-08
50-150 3.693e-06 2.008e-07
15-150 5.534e-06 2.423e-07
Peak spectrum fit
Power-law model
Time interval is from 3.592 sec. to 4.592 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.12314 ( -0.0710838 0.0707937 )
Norm@50keV : 7.64427E-02 ( -0.00307536 0.00307305 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 42.06 using 59 PHA bins.
# Reduced chi-squared = 0.7379 for 57 degrees of freedom
# Null hypothesis probability = 9.306539e-01
Photon flux (15-150 keV) in 1 sec: 8.88777 ( -0.37017 0.37056 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.93422e-07 ( -3.47355e-08 3.48093e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 3.592 sec. to 4.592 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.963891 ( -0.284602 0.208867 )
Epeak [keV] : 378.814 ( -378.814 -378.814 )
Norm@50keV : 8.99115E-02 ( -0.0171549 0.0291723 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 41.05 using 59 PHA bins.
# Reduced chi-squared = 0.7330 for 56 degrees of freedom
# Null hypothesis probability = 9.329168e-01
Photon flux (15-150 keV) in 1 sec: 8.82723 ( -0.38282 0.38331 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.89177e-07 ( -3.5952e-08 3.5819e-08 ) ergs/cm2
Band function
Time interval is from 3.592 sec. to 4.592 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.964016 ( 0.789795 0.789795 )
beta : -10.0000 ( 10 3.55271e-15 )
Epeak [keV] : 379.019 ( -119.18 -379.019 )
Norm@50keV : 8.98922E-02 ( -0.00359449 0.0291998 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 41.05 using 59 PHA bins.
# Reduced chi-squared = 0.7464 for 55 degrees of freedom
# Null hypothesis probability = 9.188945e-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] : 21.0797 ( )
R^2/D10^2 : 0.354330 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 157.17 using 59 PHA bins.
# Reduced chi-squared = 2.7574 for 57 degrees of freedom
# Null hypothesis probability = 2.610195e-11
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.970e-08 2.460e-09
25- 50 1.530e-07 9.750e-09
50-150 5.069e-07 3.400e-08
15-150 6.896e-07 3.690e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.363 ( )
Norm : 36.8093 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 145.64 using 59 PHA bins.
# Reduced chi-squared = 2.5551 for 57 degrees of freedom
# Null hypothesis probability = 1.068335e-09
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 9.166e-08 4.095e-09
25- 50 1.763e-07 7.900e-09
50-150 3.867e-07 1.650e-08
15-150 6.547e-07 2.760e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.47064 (-1.33407 1.56313)
R1^2/D10^2 : 5.41334 (-2.44021 5.29351)
kT2 [keV] : 31.8439 (-3.72572 5.54024)
R2^2/D10^2 : 8.21314E-02 (-0.0335684 0.0426563)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 43.53 using 59 PHA bins.
# Reduced chi-squared = 0.7915 for 55 degrees of freedom
# Null hypothesis probability = 8.676974e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.422e-08 1.112e-08
25- 50 1.593e-07 1.975e-08
50-150 5.701e-07 6.525e-08
15-150 7.937e-07 7.825e-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: 1.19618 ( -0.036159 0.0360538 )
Norm@50keV : 5.17880E-02 ( -0.001047 0.00104584 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 47.85 using 59 PHA bins.
# Reduced chi-squared = 0.8394 for 57 degrees of freedom
# Null hypothesis probability = 8.008129e-01
Photon flux (15-150 keV) in 9.725 sec: 6.07561 ( -0.13317 0.133431 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.11515e-06 ( -1.04227e-07 1.04272e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.899460 ( -0.153862 0.149013 )
Epeak [keV] : 226.775 ( -56.2782 158.235 )
Norm@50keV : 6.87248E-02 ( -0.00890294 0.0105351 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 36.01 using 59 PHA bins.
# Reduced chi-squared = 0.6431 for 56 degrees of freedom
# Null hypothesis probability = 9.826170e-01
Photon flux (15-150 keV) in 9.725 sec: 5.96090 ( -0.14289 0.14349 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.06501e-06 ( -1.08502e-07 1.08288e-07 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.899862 ( -0.107849 0.150175 )
beta : -9.36834 ( 9.37131 19.3713 )
Epeak [keV] : 227.725 ( -27.7144 79.3338 )
Norm@50keV : 6.86555E-02 ( -0.00604318 0.00148119 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 36.02 using 59 PHA bins.
# Reduced chi-squared = 0.6548 for 55 degrees of freedom
# Null hypothesis probability = 9.776961e-01
Photon flux (15-150 keV) in 9.725 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) = 1.27e-06
S(50-100 keV) = 2.02e-06
T90 vs. Hardness ratio plot
T90 = 15.9679999947548 sec.
Hardness ratio (energy fluence ratio) = 1.59055
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.59796
Count Ratio (50-100 keV) / (15-25 keV) = 1.45713
Mask shadow pattern
IMX = -3.245400832142962E-01, IMY = 5.990500984735029E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.256000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.256000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.256000
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:
-239.064000 -0.488000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.6911 -40.4968 16.9 32.4 -77.8 0.1760 0.7 8.2 Vela X-1
170.5204 -60.4755 6.0 33.9 -23.0 0.3478 1.9 10.7 Cen X-3
186.6602 -62.7623 1.0 38.4 -11.8 2.4793 11.8 0.5 GX 301-2
55.8746 -28.2749 2.5 42.7 159.9 1.5427 4.7 ------ UNKNOWN
218.5468 -66.6956 2.4 44.5 7.4 1.2899 4.8 ------ UNKNOWN
188.6361 -67.8765 3.2 35.8 -4.4 0.7051 3.6 ------ UNKNOWN
107.2018 -63.3447 2.9 5.5 -39.1 0.6282 4.1 ------ UNKNOWN
198.2402 -45.2448 2.9 56.2 -20.1 2.2596 4.0 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-0.488000 9.236590
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.4414 -40.3625 0.0 32.4 -78.2 0.1978 1.7 12.2 Vela X-1
169.9773 -60.5799 7.7 33.7 -23.1 0.0998 1.5 10.3 Cen X-3
186.3610 -62.7052 6.1 38.4 -12.0 -0.1496 -1.9 9.0 GX 301-2
69.8529 -9.5089 2.6 56.0 -175.2 0.8722 4.4 ------ UNKNOWN
111.8954 -29.8447 0.2 34.3 -118.4 7.3585 64.2 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
62.836600 669.636600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6384 22.0279 1.3 58.6 -159.8 20.2927 9.2 0.9 Crab
135.5433 -40.5757 12.5 22.0 -3.4 -0.2719 -0.9 1.4 Vela X-1
170.3795 -60.5792 7.5 49.0 17.4 -1.2068 -1.5 3.2 Cen X-3
59.8615 -11.8600 2.9 51.3 150.1 5.7949 4.0 ------ UNKNOWN
Plot creation:
Sun May 31 12:20:36 EDT 2015