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
286.3798 -17.2401 0.0178 19.5454 -118.4072 1.2420216 10.836 TRIG_00684679
Foreground time interval of the image:
0.000 64.000 (delta_t = 64.000 [sec])
Background time interval of the image:
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 64.000000
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 64.000000
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 64.000000
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 0.000 sec. to 64.000 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.27825 ( -0.233464 0.252467 )
Norm@50keV : 1.00372E-03 ( -0.00017773 0.00017462 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 44.25 using 59 PHA bins.
# Reduced chi-squared = 0.7763 for 57 degrees of freedom
# Null hypothesis probability = 8.912930e-01
Photon flux (15-150 keV) in 64 sec: 0.173330 ( -0.021481 0.021487 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.11603e-07 ( -8.96038e-08 9.21331e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.000 sec. to 64.000 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.638093 ( -1.58083 1.21977 )
Epeak [keV] : 31.3174 ( )
Norm@50keV : 1.00556E-02 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 38.57 using 59 PHA bins.
# Reduced chi-squared = 0.6888 for 56 degrees of freedom
# Null hypothesis probability = 9.634552e-01
Photon flux (15-150 keV) in 64 sec: 0.165160 ( -0.021889 0.022021 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.37613e-07 ( -8.35149e-08 9.6023e-08 ) ergs/cm2
Band function
Time interval is from 0.000 sec. to 64.000 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.761631 ( -0.830172 2.20905 )
beta : -4.80799 ( 4.92906 14.3984 )
Epeak [keV] : 30.7473 ( -9.45638 7.46911 )
Norm@50keV : 8.50111E-03 ( -0.00924103 0.356147 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 38.59 using 59 PHA bins.
# Reduced chi-squared = 0.7016 for 55 degrees of freedom
# Null hypothesis probability = 9.544485e-01
Photon flux (15-150 keV) in 64 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] : 8.69273 (-1.06354 1.19933)
R^2/D10^2 : 0.139254 (-0.0567257 0.0965277)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 43.52 using 59 PHA bins.
# Reduced chi-squared = 0.7635 for 57 degrees of freedom
# Null hypothesis probability = 9.057420e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.286e-07 2.672e-08
25- 50 2.587e-07 4.486e-08
50-150 8.865e-08 3.188e-08
15-150 4.760e-07 8.112e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 41.7830 (-10.6572 16.5769)
Norm : 1.09903 (-0.229876 0.298434)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 39.40 using 59 PHA bins.
# Reduced chi-squared = 0.6912 for 57 degrees of freedom
# Null hypothesis probability = 9.635462e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.638e-07 2.640e-08
25- 50 2.196e-07 3.661e-08
50-150 1.780e-07 6.826e-08
15-150 5.614e-07 9.664e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 3.81754 (-3.32473 12.4374)
R1^2/D10^2 : 1.78004 (-1.58666 -1.78004)
kT2 [keV] : 10.8299 (-2.28833 8.17147)
R2^2/D10^2 : 4.75722E-02 (-0.0453201 0.0657631)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 38.18 using 59 PHA bins.
# Reduced chi-squared = 0.6942 for 55 degrees of freedom
# Null hypothesis probability = 9.589680e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.566e-07 8.026e-08
25- 50 2.320e-07 1.220e-07
50-150 1.351e-07 8.413e-08
15-150 5.238e-07 2.656e-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: 2.27825 ( -0.233464 0.252467 )
Norm@50keV : 1.00372E-03 ( -0.00017773 0.00017462 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 44.25 using 59 PHA bins.
# Reduced chi-squared = 0.7763 for 57 degrees of freedom
# Null hypothesis probability = 8.912930e-01
Photon flux (15-150 keV) in 64 sec: 0.173311 ( -0.021478 0.0214849 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.11478e-07 ( -8.95264e-08 9.2169e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.627731 ( -1.57728 1.22326 )
Epeak [keV] : 31.3584 ( )
Norm@50keV : 1.02033E-02 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 38.57 using 59 PHA bins.
# Reduced chi-squared = 0.6888 for 56 degrees of freedom
# Null hypothesis probability = 9.634554e-01
Photon flux (15-150 keV) in 64 sec: 0.165126 ( -0.021878 0.022008 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.37703e-07 ( -8.35168e-08 9.60826e-08 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.761631 ( -0.830172 2.20905 )
beta : -4.80799 ( 4.92906 14.3984 )
Epeak [keV] : 30.7473 ( -9.45639 7.46911 )
Norm@50keV : 8.50111E-03 ( -0.00924103 0.356147 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 38.59 using 59 PHA bins.
# Reduced chi-squared = 0.7016 for 55 degrees of freedom
# Null hypothesis probability = 9.544485e-01
Photon flux (15-150 keV) in 64 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) = 1.96e-07
S(50-100 keV) = 1.62e-07
T90 vs. Hardness ratio plot
T90 = N/A sec.
Hardness ratio (energy fluence ratio) = 0.826531
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) =
Count Ratio (50-100 keV) / (15-25 keV) =
Mask shadow pattern
IMX = -1.688906794539408E-01, IMY = 3.122635234765540E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 64.000000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 64.000000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 64.000000
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:
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
0.000000 64.000000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
244.9874 -15.6415 0.5 22.6 100.3 2.9108 21.8 0.5 Sco X-1
255.9718 -37.8727 0.7 16.1 23.7 1.7589 16.0 1.8 4U 1700-377
256.3333 -36.4365 5.1 14.8 26.4 0.2507 2.3 5.0 GX 349+2
262.9110 -24.5755 7.5 3.8 83.2 0.1579 1.5 11.5 GX 1+4
264.7400 -44.4497 15.9 19.7 -4.5 0.0761 0.7 0.1 4U 1735-44
268.2892 -1.5923 10.6 23.2 173.8 0.1176 1.1 9.6 SW J1753.5-0127
270.2365 -24.9218 38.1 2.9 -96.4 0.0315 0.3 9.8 GX 5-1
270.1723 -25.8019 5.5 3.0 -79.3 0.2158 2.1 7.9 GRS 1758-258
274.0578 -14.0833 2.7 12.6 -156.5 0.4637 4.3 4.1 GX 17+2
276.1142 -30.2322 0.0 9.7 -63.4 0.1405 1.3 12.7 H1820-303
285.1688 -24.7990 23.2 16.4 -95.6 -0.0574 -0.5 10.3 HT1900.1-2455
288.7228 10.9041 4.1 41.5 -156.2 0.4594 2.8 5.1 GRS 1915+105
263.1623 -33.8700 6.5 9.7 10.1 -0.1911 -1.8 8.9 GX 354-0
236.5413 -9.2356 2.7 32.9 103.5 0.9075 4.4 ------ UNKNOWN
259.7272 29.3054 2.2 54.6 162.8 3.2771 5.1 ------ UNKNOWN
286.3798 -17.2401 1.1 19.5 -118.4 1.2419 10.8 ------ UNKNOWN
310.6479 -62.1753 2.1 47.3 -35.4 1.3473 5.5 ------ UNKNOWN
316.1488 -41.7583 2.7 43.7 -64.1 2.2481 4.2 ------ UNKNOWN
312.4230 -25.9241 3.4 40.8 -87.8 1.5842 3.4 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
117.300600 963.070000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
245.0104 -15.6378 1.2 39.6 95.3 29.0860 9.6 1.8 Sco X-1
255.9932 -37.8510 0.7 33.6 55.3 21.6945 16.8 0.5 4U 1700-377
256.5742 -36.5708 6.0 32.6 56.9 2.4532 1.9 11.1 GX 349+2
262.9992 -24.6068 5.6 23.0 76.6 1.8206 2.1 8.3 GX 1+4
264.6337 -44.4538 4.8 32.8 38.4 2.5926 2.4 4.7 4U 1735-44
268.2278 -1.5005 11.7 23.8 138.7 0.7852 1.0 8.9 SW J1753.5-0127
270.1157 -25.0362 16.1 17.0 69.2 0.5048 0.7 9.5 GX 5-1
270.2003 -25.7492 3.9 17.2 66.9 2.1441 3.0 5.5 GRS 1758-258
274.0115 -14.0440 1.0 12.3 112.5 8.3600 11.7 0.6 GX 17+2
276.0247 -30.4737 5.7 16.2 42.8 1.4146 2.0 8.2 H1820-303
285.2237 -25.0464 0.0 7.9 16.8 0.9604 1.3 12.7 HT1900.1-2455
288.8201 10.9552 1.2 28.3 -165.7 6.7072 9.6 1.4 GRS 1915+105
299.5686 35.2125 1.0 53.9 -157.5 26.8991 12.0 1.2 Cyg X-1
262.8188 -33.9636 0.0 26.9 56.3 1.6368 1.9 11.5 GX 354-0
276.4323 3.4160 3.4 22.9 162.9 2.3703 3.4 ------ UNKNOWN
301.7173 38.8723 5.2 57.9 -156.8 11.5174 2.2 ------ UNKNOWN
Plot creation:
Fri Jun 3 15:34:01 EDT 2016