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Image
Pre-slew 15.0-350.0 keV image (Event data)
# RAcent DECcent POSerr Theta Phi Peak Cts SNR Name
356.4684 49.4880 0.0146 15.5643 -102.3370 1.2339771 13.134 TRIG_00412081
Foreground time interval of the image:
-44.116 10.149 (delta_t = 54.265 [sec])
Background time interval of the image:
-314.851 -44.116 (delta_t = 270.735 [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
8 ms binning
From T100_start-3 s to T100_start+3 s
2 ms binning
From T100_start-1 s to T100_start+1 s
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 -44.116 sec. to 134.052 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.24049 ( -0.186806 0.198631 )
Norm@50keV : 6.78370E-04 ( -9.42176e-05 9.32692e-05 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 58.28 using 59 PHA bins.
# Reduced chi-squared = 1.022 for 57 degrees of freedom
# Null hypothesis probability = 4.279677e-01
Photon flux (15-150 keV) in 178.2 sec: 0.114752 ( -0.0101716 0.0101722 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.14348e-06 ( -1.30777e-07 1.35716e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -44.116 sec. to 134.052 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.34888 ( -1.08179 0.603037 )
Epeak [keV] : 26.2853 ( -21.6675 9.12685 )
Norm@50keV : 2.46039E-03 ( -0.0015523 0.00973247 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 55.12 using 59 PHA bins.
# Reduced chi-squared = 0.9842 for 56 degrees of freedom
# Null hypothesis probability = 5.082428e-01
Photon flux (15-150 keV) in 178.2 sec: 0.110487 ( -0.0106608 0.010804 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.02052e-06 ( -1.44053e-07 1.71054e-07 ) ergs/cm2
Band function
Time interval is from -44.116 sec. to 134.052 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -2.53425E-03 ( -1.98839 0.736988 )
beta : -2.62874 ( 2.60056 0.387535 )
Epeak [keV] : 26.3382 ( -7.31698 8.69192 )
Norm@50keV : 2.37295E-02 ( -0.0228523 95.0185 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 54.57 using 59 PHA bins.
# Reduced chi-squared = 0.9922 for 55 degrees of freedom
# Null hypothesis probability = 4.908757e-01
Photon flux (15-150 keV) in 178.2 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] : 7.90229 (-0.777795 0.877292)
R^2/D10^2 : 0.129805 (-0.0447564 0.0677645)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 69.18 using 59 PHA bins.
# Reduced chi-squared = 1.214 for 57 degrees of freedom
# Null hypothesis probability = 1.293152e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.588e-07 3.715e-08
25- 50 4.433e-07 5.480e-08
50-150 1.118e-07 3.423e-08
15-150 8.139e-07 9.427e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 41.7387 (-9.18517 13.5737)
Norm : 0.717224 (-0.118448 0.148671)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 55.10 using 59 PHA bins.
# Reduced chi-squared = 0.9668 for 57 degrees of freedom
# Null hypothesis probability = 5.465011e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.976e-07 3.315e-08
25- 50 3.987e-07 4.402e-08
50-150 3.229e-07 1.092e-07
15-150 1.019e-06 1.374e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.43379 (-1.46044 1.33306)
R1^2/D10^2 : 0.420882 (-0.221927 0.865914)
kT2 [keV] : 15.6553 (-4.67669 10.6077)
R2^2/D10^2 : 5.09389E-03 (-0.0044776 0.00979483)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 54.31 using 59 PHA bins.
# Reduced chi-squared = 0.9875 for 55 degrees of freedom
# Null hypothesis probability = 5.009338e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.978e-07 1.335e-07
25- 50 3.914e-07 1.583e-07
50-150 3.361e-07 1.922e-07
15-150 1.025e-06 4.663e-07
Peak spectrum fit
Power-law model
Time interval is from -0.340 sec. to 0.660 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.28417 ( -0.139866 0.140579 )
Norm@50keV : 1.80901E-02 ( -0.00140991 0.00140607 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 77.38 using 59 PHA bins.
# Reduced chi-squared = 1.358 for 57 degrees of freedom
# Null hypothesis probability = 3.752043e-02
Photon flux (15-150 keV) in 1 sec: 2.15203 ( -0.166241 0.166366 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.79464e-07 ( -1.62246e-08 1.63958e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.340 sec. to 0.660 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.11412 ( -0.548157 0.292864 )
Epeak [keV] : 273.078 ( -273.358 -273.358 )
Norm@50keV : 2.18761E-02 ( -0.00502686 0.0176836 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 77.04 using 59 PHA bins.
# Reduced chi-squared = 1.376 for 56 degrees of freedom
# Null hypothesis probability = 3.258106e-02
Photon flux (15-150 keV) in 1 sec: 2.13368 ( -0.17451 0.17352 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.77203e-07 ( -1.7786e-08 1.7593e-08 ) ergs/cm2
Band function
Time interval is from -0.340 sec. to 0.660 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.11470 ( -0.214902 0.468628 )
beta : -10.00000 ( 10 6.03961e-14 )
Epeak [keV] : 266.593 ( -164.289 -266.593 )
Norm@50keV : 2.19614E-02 ( -0.00168003 0.0176108 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 77.05 using 59 PHA bins.
# Reduced chi-squared = 1.401 for 55 degrees of freedom
# Null hypothesis probability = 2.652267e-02
Photon flux (15-150 keV) in 1 sec: 2.12856 ( ) 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] : 17.4279 (-1.85614 2.12391)
R^2/D10^2 : 0.150794 (-0.047225 0.0679075)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 113.53 using 59 PHA bins.
# Reduced chi-squared = 1.9917 for 57 degrees of freedom
# Null hypothesis probability = 1.264048e-05
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 9.262e-09 1.372e-09
25- 50 4.179e-08 4.460e-09
50-150 9.132e-08 1.401e-08
15-150 1.424e-07 1.475e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 ( )
Norm : 8.70817 (-0.680724 0.680728)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 86.97 using 59 PHA bins.
# Reduced chi-squared = 1.526 for 57 degrees of freedom
# Null hypothesis probability = 6.457105e-03
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.183e-08 2.155e-09
25- 50 4.199e-08 8.195e-09
50-150 9.209e-08 4.055e-08
15-150 1.559e-07 4.625e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.60830 (-2.09573 2.37394)
R1^2/D10^2 : 2.23192 (-1.40068 7.10942)
kT2 [keV] : 27.6577 (-5.57722 10.2228)
R2^2/D10^2 : 2.82752E-02 (-0.0182442 0.0335781)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 77.38 using 59 PHA bins.
# Reduced chi-squared = 1.407 for 55 degrees of freedom
# Null hypothesis probability = 2.501397e-02
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.824e-08 7.707e-09
25- 50 3.910e-08 1.161e-08
50-150 1.199e-07 3.889e-08
15-150 1.772e-07 5.624e-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: 2.03626 ( -0.193809 0.20427 )
Norm@50keV : 1.28676E-03 ( -0.000179352 0.00017631 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 69.24 using 59 PHA bins.
# Reduced chi-squared = 1.215 for 57 degrees of freedom
# Null hypothesis probability = 1.282170e-01
Photon flux (15-150 keV) in 54.26 sec: 0.196303 ( -0.0190296 0.019032 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.45287e-07 ( -8.15446e-08 8.46364e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.66708 ( -1.09833 0.454552 )
Epeak [keV] : 33.2330 ( )
Norm@50keV : 2.18884E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 68.64 using 59 PHA bins.
# Reduced chi-squared = 1.226 for 56 degrees of freedom
# Null hypothesis probability = 1.195829e-01
Photon flux (15-150 keV) in 54.26 sec: 0.192797 ( -0.020441 0.020012 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.06741e-07 ( -1.10734e-07 1.13213e-07 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 0.792910 ( -1.54324 0.331876 )
beta : -2.33456 ( 2.35289 0.388221 )
Epeak [keV] : 26.8430 ( -11.2832 12.6576 )
Norm@50keV : 0.140341 ( -0.137253 169.671 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 65.97 using 59 PHA bins.
# Reduced chi-squared = 1.199 for 55 degrees of freedom
# Null hypothesis probability = 1.478290e-01
Photon flux (15-150 keV) in 54.26 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) = 3.65e-07
S(50-100 keV) = 3.09e-07
T90 vs. Hardness ratio plot
T90 = 163.763999938965 sec.
Hardness ratio (energy fluence ratio) = 0.846575
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 0.957797
Count Ratio (50-100 keV) / (15-25 keV) = 0.345183
Mask shadow pattern
IMX = -5.951191007813444E-02, IMY = 2.721016923148862E-01
TIME vs. PHA plot around the trigger time
TIME vs. DetID plot around the trigger time
100 us light curve (15-350 keV)
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:
-314.851400 -44.116000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
299.6120 35.1855 0.7 48.7 -39.8 13.9939 17.8 1.4 Cyg X-1
308.1725 40.9607 2.6 40.2 -43.2 1.8318 4.5 2.9 Cyg X-3
326.1173 38.2998 7.4 35.0 -64.8 0.6612 1.6 2.9 Cyg X-2
341.4732 65.4911 3.1 10.6 -18.3 0.7610 3.7 ------ UNKNOWN
28.4554 32.1514 2.3 34.8 -160.8 1.2442 5.0 ------ UNKNOWN
38.0285 18.3084 2.9 50.6 -167.0 2.2049 3.9 ------ UNKNOWN
358.6502 41.7394 2.5 22.8 -111.9 1.1537 4.6 ------ UNKNOWN
11.9618 31.2684 2.2 33.1 -135.7 1.5499 5.3 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-44.116000 10.148600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
299.5788 35.2976 6.3 48.7 -39.7 0.4804 1.8 5.8 Cyg X-1
308.1729 40.8431 7.2 40.3 -43.4 0.2475 1.6 7.2 Cyg X-3
326.0925 38.1837 5.6 35.1 -64.8 -0.3227 -2.1 9.1 Cyg X-2
220.6416 64.7796 2.0 48.7 34.6 2.2931 5.7 ------ UNKNOWN
356.4684 49.4880 0.9 15.6 -102.3 1.2340 13.1 ------ UNKNOWN
31.5200 18.2252 2.1 49.0 -159.2 1.0203 5.6 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
47.148600 842.504400
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
299.5893 35.2025 0.2 43.2 -28.8 41.9152 47.6 0.1 Cyg X-1
308.1356 40.9828 1.3 34.4 -27.2 5.8397 9.0 2.1 Cyg X-3
326.1286 38.4773 4.6 24.2 -47.2 1.4803 2.5 9.6 Cyg X-2
57.0597 34.4430 3.1 46.1 143.6 5.9197 3.7 ------ UNKNOWN
33.0249 27.6551 3.1 35.4 172.8 2.8736 3.8 ------ UNKNOWN
276.3664 49.0602 3.1 49.6 0.4 4.4372 3.8 ------ UNKNOWN
35.7106 14.9459 2.6 47.0 -178.4 4.2874 4.4 ------ UNKNOWN
348.7430 23.9179 3.2 26.3 -105.6 2.1896 3.6 ------ UNKNOWN
341.9980 26.3055 3.2 25.8 -90.7 2.4330 3.5 ------ UNKNOWN
Plot creation:
Sun May 31 02:14:14 EDT 2015