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Image
Pre-slew 15.0-350.0 keV image (Event data)
# RAcent DECcent POSerr Theta Phi Peak Cts SNR Name
289.9443 60.7279 0.0035 19.1104 -93.2045 6.5682266 54.547 TRIG_00356890
Foreground time interval of the image:
-49.787 16.613 (delta_t = 66.400 [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 1.024000
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 1.024000
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 1.024000
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 -67.296 sec. to 101.472 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.20946 ( -0.0246825 0.0245909 )
Norm@50keV : 1.48000E-02 ( -0.000206478 0.000206079 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 39.21 using 59 PHA bins.
# Reduced chi-squared = 0.6880 for 57 degrees of freedom
# Null hypothesis probability = 9.652633e-01
Photon flux (15-150 keV) in 168.8 sec: 1.73957 ( -0.0272976 0.027379 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.52785e-05 ( -3.24175e-07 3.24169e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -67.296 sec. to 101.472 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.07319 ( -0.102717 0.0927028 )
Epeak [keV] : 439.308 ( -158.591 938.165 )
Norm@50keV : 1.67094E-02 ( -0.000749629 0.00155954 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 33.87 using 59 PHA bins.
# Reduced chi-squared = 0.6049 for 56 degrees of freedom
# Null hypothesis probability = 9.915618e-01
Photon flux (15-150 keV) in 168.8 sec: 1.71968 ( -0.03048 0.03065 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.51792e-05 ( -3.35068e-07 3.34899e-07 ) ergs/cm2
Band function
Time interval is from -67.296 sec. to 101.472 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.07316 ( -0.612885 5.26071 )
beta : -10.00000 ( 10 20 )
Epeak [keV] : 439.211 ( -67.5264 946.425 )
Norm@50keV : 1.67080E-02 ( -0.00021319 0.0015582 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 33.87 using 59 PHA bins.
# Reduced chi-squared = 0.6159 for 55 degrees of freedom
# Null hypothesis probability = 9.888785e-01
Photon flux (15-150 keV) in 168.8 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] : 23.0431 ( )
R^2/D10^2 : 4.91693E-02 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 1017.61 using 59 PHA bins.
# Reduced chi-squared = 17.8528 for 57 degrees of freedom
# Null hypothesis probability = 5.304823e-176
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.980e-07 2.178e-08
25- 50 4.334e-06 9.959e-08
50-150 1.719e-05 2.954e-07
15-150 2.232e-05 2.954e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.363 ( )
Norm : 7.79165 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 791.03 using 59 PHA bins.
# Reduced chi-squared = 13.878 for 57 degrees of freedom
# Null hypothesis probability = 8.423006e-130
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.275e-06 5.148e-08
25- 50 6.300e-06 9.284e-08
50-150 1.382e-05 2.110e-07
15-150 2.339e-05 3.714e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 8.62837 (-0.504948 0.532769)
R1^2/D10^2 : 0.710194 (-0.127328 0.161569)
kT2 [keV] : 34.6678 (-1.60289 1.86999)
R2^2/D10^2 : 1.11000E-02 (-0.00178609 0.00193315)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 37.12 using 59 PHA bins.
# Reduced chi-squared = 0.6750 for 55 degrees of freedom
# Null hypothesis probability = 9.692062e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.018e-06 1.156e-07
25- 50 5.465e-06 1.283e-07
50-150 1.767e-05 3.882e-07
15-150 2.516e-05 4.558e-07
Peak spectrum fit
Power-law model
Time interval is from 21.828 sec. to 22.828 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.02473 ( -0.0636653 0.0633282 )
Norm@50keV : 6.75714E-02 ( -0.00242066 0.00241961 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 37.36 using 59 PHA bins.
# Reduced chi-squared = 0.6555 for 57 degrees of freedom
# Null hypothesis probability = 9.794314e-01
Photon flux (15-150 keV) in 1 sec: 7.79060 ( -0.283938 0.284234 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.24378e-07 ( -2.88784e-08 2.90139e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 21.828 sec. to 22.828 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.724292 ( -0.262407 0.247358 )
Epeak [keV] : 243.019 ( -86.649 730.726 )
Norm@50keV : 9.20583E-02 ( -0.0202272 0.0275232 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 33.01 using 59 PHA bins.
# Reduced chi-squared = 0.5895 for 56 degrees of freedom
# Null hypothesis probability = 9.938785e-01
Photon flux (15-150 keV) in 1 sec: 7.68940 ( -0.29542 0.29541 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.13715e-07 ( -3.0763e-08 3.0614e-08 ) ergs/cm2
Band function
Time interval is from 21.828 sec. to 22.828 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 4.99997 ( -4.99997 -4.99997 )
beta : -1.05256 ( -0.0677833 0.0673281 )
Epeak [keV] : 25.5174 ( -25.5174 3.80678 )
Norm@50keV : 4103.03 ( -146.021 1.03089e+07 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 35.31 using 59 PHA bins.
# Reduced chi-squared = 0.6420 for 55 degrees of freedom
# Null hypothesis probability = 9.820785e-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] : 21.4586 ( )
R^2/D10^2 : 0.299655 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 147.57 using 59 PHA bins.
# Reduced chi-squared = 2.5889 for 57 degrees of freedom
# Null hypothesis probability = 5.801889e-10
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.582e-08 1.860e-09
25- 50 1.345e-07 7.250e-09
50-150 4.624e-07 2.720e-08
15-150 6.227e-07 2.850e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.363 ( )
Norm : 31.4460 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 216.29 using 59 PHA bins.
# Reduced chi-squared = 3.7945 for 57 degrees of freedom
# Null hypothesis probability = 2.168452e-20
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.830e-08 2.860e-09
25- 50 1.506e-07 6.250e-09
50-150 3.303e-07 1.340e-08
15-150 5.593e-07 2.285e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 8.48161 (-1.4094 1.62557)
R1^2/D10^2 : 2.85807 (-1.10998 2.13115)
kT2 [keV] : 33.6116 (-4.17358 6.56744)
R2^2/D10^2 : 6.28632E-02 (-0.0272919 0.0346433)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 33.55 using 59 PHA bins.
# Reduced chi-squared = 0.6100 for 55 degrees of freedom
# Null hypothesis probability = 9.900725e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.903e-08 7.835e-09
25- 50 1.414e-07 1.495e-08
50-150 5.277e-07 6.545e-08
15-150 7.180e-07 8.245e-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: 1.34711 ( -0.0544441 0.0543581 )
Norm@50keV : 6.38295E-03 ( -0.000184409 0.000184409 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 43.98 using 59 PHA bins.
# Reduced chi-squared = 0.7716 for 57 degrees of freedom
# Null hypothesis probability = 8.967445e-01
Photon flux (15-150 keV) in 66.4 sec: 0.768505 ( -0.0237803 0.02383 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.14212e-06 ( -1.2976e-07 1.30044e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.10153 ( -0.226488 0.215017 )
Epeak [keV] : 200.159 ( -70.1039 780.654 )
Norm@50keV : 8.28048E-03 ( -0.00164854 0.00217812 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 40.16 using 59 PHA bins.
# Reduced chi-squared = 0.7172 for 56 degrees of freedom
# Null hypothesis probability = 9.454126e-01
Photon flux (15-150 keV) in 66.4 sec: 0.755956 ( -0.025987 0.026037 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.07217e-06 ( -1.45243e-07 1.445e-07 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.838229 ( -0.324218 5.56338 )
beta : -1.48867 ( 1.48894 0.128035 )
Epeak [keV] : 105.460 ( -70.6568 215.732 )
Norm@50keV : 1.16483E-02 ( -0.00398098 5.46468 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 38.63 using 59 PHA bins.
# Reduced chi-squared = 0.7023 for 55 degrees of freedom
# Null hypothesis probability = 9.539738e-01
Photon flux (15-150 keV) in 66.4 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) = 5.34e-06
S(50-100 keV) = 9.24e-06
T90 vs. Hardness ratio plot
T90 = 88.7439999580383 sec.
Hardness ratio (energy fluence ratio) = 1.73034
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.63308
Count Ratio (50-100 keV) / (15-25 keV) = 1.54529
Mask shadow pattern
IMX = -1.936842256253885E-02, IMY = 3.459417550868899E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.024000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.024000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.024000
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:
-49.787400 16.612600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.5853 35.4805 8.4 29.5 179.8 0.1677 1.4 10.4 Her X-1
288.6720 10.7955 7.5 31.0 95.3 0.3149 1.5 11.7 GRS 1915+105
299.6047 35.1908 0.4 8.9 43.3 2.7980 25.9 1.0 Cyg X-1
308.1638 41.0442 10.5 12.3 -3.2 0.1199 1.1 6.0 Cyg X-3
326.1726 38.3223 63.3 26.4 -4.8 0.0239 0.2 0.1 Cyg X-2
253.6014 53.3555 2.3 27.9 -142.6 0.6419 5.1 ------ UNKNOWN
289.9443 60.7279 0.2 19.1 -93.2 6.5685 54.5 ------ UNKNOWN
236.8091 48.3496 2.3 38.6 -151.3 0.8463 5.0 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
57.212600 538.412610
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.6971 35.2763 40.0 33.9 146.7 -0.5247 -0.3 12.4 Her X-1
299.6148 35.2125 0.9 26.2 71.0 19.4661 13.4 1.4 Cyg X-1
308.2396 40.7885 17.0 22.9 51.3 0.9294 0.7 11.5 Cyg X-3
326.0660 38.3572 6.9 31.7 27.3 2.5272 1.7 5.4 Cyg X-2
297.3541 27.6935 2.6 33.4 77.1 9.1162 4.5 ------ UNKNOWN
234.3248 45.8116 3.7 35.1 179.8 4.3803 3.2 ------ UNKNOWN
289.9643 60.7279 1.2 0.0 -61.6 10.3652 9.6 ------ UNKNOWN
8.2564 31.4627 2.3 57.3 -8.1 22.2508 5.0 ------ UNKNOWN
198.3789 37.3468 3.7 58.8 -159.3 23.5416 3.1 ------ UNKNOWN
180.7906 71.6683 3.4 39.0 -119.1 8.0788 3.4 ------ UNKNOWN
33.3278 54.2892 3.4 50.1 -43.2 16.7188 3.4 ------ UNKNOWN
Plot creation:
Sun May 31 03:37:45 EDT 2015