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Image
Pre-slew 15.0-350.0 keV image (Event data)
# RAcent DECcent POSerr Theta Phi Peak Cts SNR Name
299.7307 70.1169 0.0259 16.3481 -170.1111 0.9707006 7.391 TRIG_00296856
Foreground time interval of the image:
-31.480 72.501 (delta_t = 103.981 [sec])
Background time interval of the image:
-289.299 -31.480 (delta_t = 257.819 [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 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 -31.480 sec. to 87.496 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.52605 ( -0.277229 0.28592 )
Norm@50keV : 5.90498E-04 ( -0.000102117 9.9809e-05 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 51.93 using 59 PHA bins.
# Reduced chi-squared = 0.9110 for 57 degrees of freedom
# Null hypothesis probability = 6.652910e-01
Photon flux (15-150 keV) in 119 sec: 7.42458E-02 ( -0.0114351 0.0114357 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.63872e-07 ( -1.25535e-07 1.2999e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -31.480 sec. to 87.496 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.13557 ( -1.31251 0.652916 )
Epeak [keV] : 99.6987 ( -99.6986 -99.6986 )
Norm@50keV : 9.67601E-04 ( -0.000470428 0.00410959 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 51.54 using 59 PHA bins.
# Reduced chi-squared = 0.9203 for 56 degrees of freedom
# Null hypothesis probability = 6.443289e-01
Photon flux (15-150 keV) in 119 sec: 7.28776E-02 ( -0.0120114 0.0119258 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.32962e-07 ( -1.46579e-07 1.51266e-07 ) ergs/cm2
Band function
Time interval is from -31.480 sec. to 87.496 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 0.295215 ( -0.837357 4.01126 )
beta : -1.72797 ( 1.73175 0.449824 )
Epeak [keV] : 39.6439 ( -36.3687 153.718 )
Norm@50keV : 9.47891E-03 ( -0.00882544 81405.5 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 51.28 using 59 PHA bins.
# Reduced chi-squared = 0.9324 for 55 degrees of freedom
# Null hypothesis probability = 6.174054e-01
Photon flux (15-150 keV) in 119 sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 6.31994e-07 ( 0 0 ) ergs/cm2
Single BB
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 12.8139 (-2.44917 3.20151)
R^2/D10^2 : 1.43872E-02 (-0.00777148 0.0161339)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 59.73 using 59 PHA bins.
# Reduced chi-squared = 1.048 for 57 degrees of freedom
# Null hypothesis probability = 3.766403e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.963e-08 1.765e-08
25- 50 2.022e-07 5.889e-08
50-150 2.081e-07 7.649e-08
15-150 4.699e-07 1.153e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.004 (-110.032 -199.029)
Norm : 0.302443 (-0.046457 0.0531885)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 51.56 using 59 PHA bins.
# Reduced chi-squared = 0.9046 for 57 degrees of freedom
# Null hypothesis probability = 6.784662e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.964e-08 5.099e-08
25- 50 1.724e-07 9.556e-08
50-150 3.779e-07 2.094e-07
15-150 6.399e-07 3.560e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.97936 (-3.0201 3.58911)
R1^2/D10^2 : 8.00839E-02 (-0.0569442 0.484819)
kT2 [keV] : 25.2019 (-21.2454 83.5294)
R2^2/D10^2 : 1.01797E-03 (-0.000983918 0.00430284)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 51.13 using 59 PHA bins.
# Reduced chi-squared = 0.9297 for 55 degrees of freedom
# Null hypothesis probability = 6.231299e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.766e-08 5.062e-08
25- 50 1.770e-07 9.330e-08
50-150 3.732e-07 2.185e-07
15-150 6.379e-07 3.325e-07
Peak spectrum fit
Power-law model
Time interval is from 80.244 sec. to 81.244 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.09718 ( -0.839091 0.772616 )
Norm@50keV : 2.73322E-03 ( -0.00102393 0.00102322 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 81.55 using 59 PHA bins.
# Reduced chi-squared = 1.431 for 57 degrees of freedom
# Null hypothesis probability = 1.814085e-02
Photon flux (15-150 keV) in 1 sec: 0.316942 ( -0.120036 0.120453 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.86004e-08 ( -1.24028e-08 1.30977e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 80.244 sec. to 81.244 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.10502 ( -0.857812 0.765669 )
Epeak [keV] : 9999.36 ( -9999.36 -9999.36 )
Norm@50keV : 2.74648E-03 ( -0.00103218 0.0267653 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 81.55 using 59 PHA bins.
# Reduced chi-squared = 1.456 for 56 degrees of freedom
# Null hypothesis probability = 1.452580e-02
Photon flux (15-150 keV) in 1 sec: 0.317555 ( -0.120617 0.119721 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.86186e-08 ( -1.26165e-08 1.28676e-08 ) ergs/cm2
Band function
Time interval is from 80.244 sec. to 81.244 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 5.00000 ( -5 -5 )
beta : -1.18861 ( -1.0704 0.896305 )
Epeak [keV] : 26.0757 ( -26.0748 17.8511 )
Norm@50keV : 163.837 ( -61.1355 1.71051e+06 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 81.38 using 59 PHA bins.
# Reduced chi-squared = 1.480 for 55 degrees of freedom
# Null hypothesis probability = 1.192945e-02
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] : 24.5353 (-11.6256 30.9119)
R^2/D10^2 : 7.67180E-03 (-0.0075183 0.0465563)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 83.81 using 59 PHA bins.
# Reduced chi-squared = 1.470 for 57 degrees of freedom
# Null hypothesis probability = 1.193101e-02
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.102e-10 5.460e-10
25- 50 4.552e-09 2.906e-09
50-150 2.037e-08 1.358e-08
15-150 2.573e-08 1.676e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.363 (-199.363 -199.363)
Norm : 1.27126 (-0.491259 0.491259)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 82.73 using 59 PHA bins.
# Reduced chi-squared = 1.451 for 57 degrees of freedom
# Null hypothesis probability = 1.460359e-02
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.166e-09 2.074e-09
25- 50 6.089e-09 4.034e-09
50-150 1.335e-08 8.465e-09
15-150 2.261e-08 1.463e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.27623 (-2.3793 4.93399)
R1^2/D10^2 : 0.924320 (-0.927663 34.254)
kT2 [keV] : 35.7009 (-33.3198 -35.6156)
R2^2/D10^2 : 2.35134E-03 (-0.0023065 0.0110879)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 80.14 using 59 PHA bins.
# Reduced chi-squared = 1.457 for 55 degrees of freedom
# Null hypothesis probability = 1.509909e-02
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.193e-09 2.065e-09
25- 50 4.820e-09 2.367e-09
50-150 2.282e-08 1.425e-08
15-150 3.084e-08 1.648e-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: 1.55395 ( -0.286831 0.297618 )
Norm@50keV : 5.97660E-04 ( -0.00010975 0.000107142 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 58.99 using 59 PHA bins.
# Reduced chi-squared = 1.035 for 57 degrees of freedom
# Null hypothesis probability = 4.025360e-01
Photon flux (15-150 keV) in 104 sec: 7.57470E-02 ( -0.0122384 0.0122386 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.84819e-07 ( -1.16078e-07 1.20547e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.949248 ( -1.48107 1.22167 )
Epeak [keV] : 76.8379 ( -31.018 -76.8372 )
Norm@50keV : 1.29546E-03 ( -0.000788814 0.00737509 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 58.20 using 59 PHA bins.
# Reduced chi-squared = 1.039 for 56 degrees of freedom
# Null hypothesis probability = 3.942680e-01
Photon flux (15-150 keV) in 104 sec: 7.36847E-02 ( -0.0128053 0.0128258 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.43211e-07 ( -1.31896e-07 1.4315e-07 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 0.542093 ( -0.528287 4.30533 )
beta : -1.81596 ( 1.81182 0.485356 )
Epeak [keV] : 38.7807 ( -38.7945 199.709 )
Norm@50keV : 1.42586E-02 ( -0.013224 12.348 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 58.00 using 59 PHA bins.
# Reduced chi-squared = 1.055 for 55 degrees of freedom
# Null hypothesis probability = 3.652854e-01
Photon flux (15-150 keV) in 104 sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 5.43237e-07 ( 0 0 ) ergs/cm2
S(25-50 keV) vs. S(50-100 keV) plot
S(25-50 keV) = 1.66e-07
S(50-100 keV) = 2.31e-07
T90 vs. Hardness ratio plot
T90 = 105.59999999404 sec.
Hardness ratio (energy fluence ratio) = 1.39157
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.65598
Count Ratio (50-100 keV) / (15-25 keV) = 1.15718
Mask shadow pattern
IMX = -2.889730070590047E-01, IMY = 5.037623594092833E-02
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:
-289.299400 -31.480000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
299.6015 35.2028 0.7 51.0 -162.3 9.7052 17.7 0.6 Cyg X-1
308.1264 40.9559 3.2 45.8 -171.8 1.2533 3.6 0.8 Cyg X-3
326.0496 38.2613 5.2 49.8 169.9 1.3562 2.2 6.8 Cyg X-2
163.5384 59.3802 3.7 31.6 -16.1 0.7800 3.1 ------ UNKNOWN
298.2967 49.7487 3.4 36.5 -162.5 0.8635 3.4 ------ UNKNOWN
287.9850 28.4933 3.3 57.2 -149.7 4.2211 3.5 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-31.480000 72.500590
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
299.6607 35.2912 3.2 51.0 -162.3 -1.0923 -3.7 6.4 Cyg X-1
307.9734 40.9295 6.5 45.8 -171.6 0.4074 1.8 6.4 Cyg X-3
326.3010 38.3265 4.5 49.7 169.7 -0.8830 -2.5 6.1 Cyg X-2
299.7307 70.1169 1.6 16.3 -170.1 0.9707 7.4 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
111.900600 963.050000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
299.5878 35.1946 0.2 34.9 -151.2 36.8486 52.4 0.4 Cyg X-1
308.1257 40.9522 1.6 29.5 -164.4 4.0086 7.2 0.7 Cyg X-3
326.0835 38.3492 9.1 34.6 170.8 0.9742 1.3 4.5 Cyg X-2
321.6984 47.4263 4.2 25.0 171.9 1.6496 2.8 ------ UNKNOWN
325.2247 23.2753 2.8 49.2 177.1 5.7411 4.1 ------ UNKNOWN
308.0845 37.6223 1.5 32.8 -163.7 4.7791 7.8 ------ UNKNOWN
243.2569 55.9539 2.6 27.8 -62.5 3.0846 4.4 ------ UNKNOWN
Plot creation:
Sun May 31 08:38:22 EDT 2015