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Image
Pre-slew 15.0-350.0 keV image (Event data)
# RAcent DECcent POSerr Theta Phi Peak Cts SNR Name
32.6397 64.1301 0.0044 20.2392 -64.6463 2.7711897 44.235 TRIG_00318170
Foreground time interval of the image:
-3.300 18.533 (delta_t = 21.833 [sec])
Background time interval of the image:
-239.368 -3.300 (delta_t = 236.068 [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 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 -3.300 sec. to 110.248 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.22108 ( -0.0473229 0.0471193 )
Norm@50keV : 4.74126E-03 ( -0.000120603 0.000120567 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 68.62 using 59 PHA bins.
# Reduced chi-squared = 1.204 for 57 degrees of freedom
# Null hypothesis probability = 1.392519e-01
Photon flux (15-150 keV) in 113.5 sec: 0.558234 ( -0.0151255 0.0151522 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.42763e-06 ( -1.47903e-07 1.48171e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -3.300 sec. to 110.248 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.864335 ( -0.197145 0.188406 )
Epeak [keV] : 178.906 ( -43.8743 129.495 )
Norm@50keV : 6.85075E-03 ( -0.00117953 0.00149286 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 57.75 using 59 PHA bins.
# Reduced chi-squared = 1.031 for 56 degrees of freedom
# Null hypothesis probability = 4.104455e-01
Photon flux (15-150 keV) in 113.5 sec: 0.545664 ( -0.016358 0.016387 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.30465e-06 ( -1.6369e-07 1.62793e-07 ) ergs/cm2
Band function
Time interval is from -3.300 sec. to 110.248 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 1.36234 ( -1.87319 -1.36309 )
beta : -1.31152 ( -0.0926621 0.0669797 )
Epeak [keV] : 40.2881 ( -8.18006 49.2611 )
Norm@50keV : 0.233168 ( -0.234328 56.6652 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 52.82 using 59 PHA bins.
# Reduced chi-squared = 0.9604 for 55 degrees of freedom
# Null hypothesis probability = 5.582491e-01
Photon flux (15-150 keV) in 113.5 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] : 19.4562 ( )
R^2/D10^2 : 2.73638E-02 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 287.10 using 59 PHA bins.
# Reduced chi-squared = 5.0368 for 57 degrees of freedom
# Null hypothesis probability = 2.032451e-32
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.291e-07 1.266e-08
25- 50 1.120e-06 4.495e-08
50-150 3.130e-06 1.356e-07
15-150 4.479e-06 1.300e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.363 ( )
Norm : 2.36061 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 205.50 using 59 PHA bins.
# Reduced chi-squared = 3.6052 for 57 degrees of freedom
# Null hypothesis probability = 1.189941e-18
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.672e-07 1.856e-08
25- 50 1.283e-06 3.689e-08
50-150 2.815e-06 7.548e-08
15-150 4.765e-06 1.379e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 8.51092 (-0.873063 0.959507)
R1^2/D10^2 : 0.240004 (-0.0655194 0.0966244)
kT2 [keV] : 31.8162 (-3.06687 4.2261)
R2^2/D10^2 : 4.49903E-03 (-0.00153031 0.00188145)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 50.92 using 59 PHA bins.
# Reduced chi-squared = 0.9259 for 55 degrees of freedom
# Null hypothesis probability = 6.310303e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.501e-07 4.444e-08
25- 50 1.215e-06 8.104e-08
50-150 3.663e-06 3.047e-07
15-150 5.329e-06 3.604e-07
Peak spectrum fit
Power-law model
Time interval is from 15.232 sec. to 16.232 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.04968 ( -0.121956 0.120358 )
Norm@50keV : 1.98789E-02 ( -0.00144378 0.00144335 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 77.44 using 59 PHA bins.
# Reduced chi-squared = 1.359 for 57 degrees of freedom
# Null hypothesis probability = 3.717234e-02
Photon flux (15-150 keV) in 1 sec: 2.29589 ( -0.169255 0.169425 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.11296e-07 ( -1.70347e-08 1.71941e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 15.232 sec. to 16.232 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.251374 ( -0.587278 0.513448 )
Epeak [keV] : 121.347 ( -29.7206 112.134 )
Norm@50keV : 4.64149E-02 ( -0.0190896 0.0376419 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 69.91 using 59 PHA bins.
# Reduced chi-squared = 1.248 for 56 degrees of freedom
# Null hypothesis probability = 1.001374e-01
Photon flux (15-150 keV) in 1 sec: 2.23139 ( -0.17492 0.17467 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.02601e-07 ( -1.8344e-08 1.8317e-08 ) ergs/cm2
Band function
Time interval is from 15.232 sec. to 16.232 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.251410 ( -0.457963 0.503122 )
beta : -10.0000 ( 10 20 )
Epeak [keV] : 121.336 ( -22.0377 112.077 )
Norm@50keV : 4.64140E-02 ( -0.0190708 0.0376897 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 69.91 using 59 PHA bins.
# Reduced chi-squared = 1.271 for 55 degrees of freedom
# Null hypothesis probability = 8.495413e-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] : 20.4455 (-1.79213 2.02688)
R^2/D10^2 : 0.104890 (-0.0273815 0.035967)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 86.33 using 59 PHA bins.
# Reduced chi-squared = 1.515 for 57 degrees of freedom
# Null hypothesis probability = 7.325413e-03
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.377e-09 1.255e-09
25- 50 4.234e-08 4.360e-09
50-150 1.316e-07 1.590e-08
15-150 1.823e-07 1.765e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.363 ( )
Norm : 9.22161 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 118.24 using 59 PHA bins.
# Reduced chi-squared = 2.0744 for 57 degrees of freedom
# Null hypothesis probability = 3.546734e-06
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.296e-08 1.860e-09
25- 50 4.417e-08 1.019e-08
50-150 9.688e-08 3.358e-08
15-150 1.640e-07 4.379e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.40889 (-2.54818 4.16223)
R1^2/D10^2 : 1.04939 (-0.726044 3.25699)
kT2 [keV] : 26.6522 (-4.28608 10.117)
R2^2/D10^2 : 3.92365E-02 (-0.0270321 0.033807)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 69.03 using 59 PHA bins.
# Reduced chi-squared = 1.255 for 55 degrees of freedom
# Null hypothesis probability = 9.672467e-02
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.445e-08 6.661e-09
25- 50 4.228e-08 1.651e-08
50-150 1.455e-07 5.060e-08
15-150 2.022e-07 6.736e-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: 1.26889 ( -0.0597858 0.059601 )
Norm@50keV : 8.77444E-03 ( -0.000297209 0.000297208 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 70.15 using 59 PHA bins.
# Reduced chi-squared = 1.231 for 57 degrees of freedom
# Null hypothesis probability = 1.133030e-01
Photon flux (15-150 keV) in 21.83 sec: 1.04105 ( -0.0367133 0.0367585 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.9076e-06 ( -7.10032e-08 7.11996e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.594978 ( -0.27164 0.255263 )
Epeak [keV] : 111.904 ( -17.8179 35.4033 )
Norm@50keV : 1.81957E-02 ( -0.00427944 0.00600486 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 47.74 using 59 PHA bins.
# Reduced chi-squared = 0.8524 for 56 degrees of freedom
# Null hypothesis probability = 7.760968e-01
Photon flux (15-150 keV) in 21.83 sec: 1.00449 ( -0.038957 0.03898 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.8218e-06 ( -7.89853e-08 7.88041e-08 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.594953 ( -0.179838 0.346606 )
beta : -10.0000 ( 10 5.32907e-15 )
Epeak [keV] : 111.886 ( -10.6497 35.406 )
Norm@50keV : 1.81959E-02 ( -0.00428678 0.00600774 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 47.74 using 59 PHA bins.
# Reduced chi-squared = 0.8679 for 55 degrees of freedom
# Null hypothesis probability = 7.457933e-01
Photon flux (15-150 keV) in 21.83 sec: 1.00826 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 1.83343e-06 ( 0 0 ) ergs/cm2
S(25-50 keV) vs. S(50-100 keV) plot
S(25-50 keV) = 1.15e-06
S(50-100 keV) = 1.98e-06
T90 vs. Hardness ratio plot
T90 = 77.363999992609 sec.
Hardness ratio (energy fluence ratio) = 1.72174
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.79225
Count Ratio (50-100 keV) / (15-25 keV) = 1.58187
Mask shadow pattern
IMX = 1.578814225197023E-01, IMY = 3.331922850841051E-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:
-239.368000 -3.300000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
299.5857 35.1879 0.7 40.7 135.9 8.7618 17.4 0.9 Cyg X-1
308.1612 40.9372 4.2 32.0 133.4 0.8160 2.8 2.5 Cyg X-3
326.0996 38.2689 3.9 26.0 106.9 0.8061 2.9 4.6 Cyg X-2
285.6341 33.0528 2.3 49.6 146.9 4.3002 4.9 ------ UNKNOWN
323.3445 31.6332 2.4 32.9 104.6 1.7250 4.9 ------ UNKNOWN
106.4056 73.0572 4.3 41.1 -98.2 3.1772 2.7 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-3.300000 18.532610
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
299.4654 35.0703 4.4 40.9 135.9 0.3782 2.6 10.0 Cyg X-1
308.3157 40.8133 11.3 32.0 133.1 -0.0909 -1.0 12.5 Cyg X-3
326.3772 38.4336 0.0 25.7 106.6 -0.1144 -1.5 11.8 Cyg X-2
37.4393 41.9851 3.0 33.2 -22.3 0.2569 3.8 ------ UNKNOWN
32.6397 64.1301 0.3 20.2 -64.6 2.7713 44.2 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
61.532600 362.774100
420.632000 482.693600
600.632000 662.724100
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
270.1649 59.0226 3.4 49.4 158.2 2.8548 3.4 ------ UNKNOWN
32.7203 64.1684 1.9 0.0 -105.4 1.5542 6.0 ------ UNKNOWN
39.2630 44.4543 1.9 20.0 -0.8 1.3837 6.0 ------ UNKNOWN
74.7641 19.5421 3.1 52.7 -39.5 4.3553 3.7 ------ UNKNOWN
Plot creation:
Sun May 31 06:48:32 EDT 2015