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Image
Pre-slew 15.0-350.0 keV image (Event data)
# RAcent DECcent POSerr Theta Phi Peak Cts SNR Name
13.0103 45.1025 0.0125 54.6259 -169.2392 3.6912900 15.364 TRIG_00603243
Foreground time interval of the image:
-2.524 30.621 (delta_t = 33.145 [sec])
Background time interval of the image:
-149.379 -2.524 (delta_t = 146.855 [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 2.048000
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 2.048000
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 2.048000
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 -2.524 sec. to 135.016 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.69945 ( -0.129646 0.131122 )
Norm@50keV : 3.04681E-03 ( -0.000230057 0.000228928 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 41.19 using 59 PHA bins.
# Reduced chi-squared = 0.7227 for 57 degrees of freedom
# Null hypothesis probability = 9.430642e-01
Photon flux (15-150 keV) in 137.5 sec: 0.404573 ( -0.0312872 0.0314067 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.87903e-06 ( -3.04069e-07 3.05613e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -2.524 sec. to 135.016 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.70038 ( -0.131922 0.130349 )
Epeak [keV] : 9999.36 ( -9999.35 -9999.36 )
Norm@50keV : 3.04959E-03 ( -0.00305112 0.0020742 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 41.19 using 59 PHA bins.
# Reduced chi-squared = 0.7356 for 56 degrees of freedom
# Null hypothesis probability = 9.307225e-01
Photon flux (15-150 keV) in 137.5 sec: 0.404618 ( -0.030965 0.031176 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.86928e-06 ( -3.09801e-07 3.17927e-07 ) ergs/cm2
Band function
Time interval is from -2.524 sec. to 135.016 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 4.94451 ( -4.94451 -4.94451 )
beta : -1.73456 ( -0.143936 0.137628 )
Epeak [keV] : 21.3191 ( -21.3191 5.11642 )
Norm@50keV : 939.829 ( -68.3975 2.13887e+06 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 40.33 using 59 PHA bins.
# Reduced chi-squared = 0.7334 for 55 degrees of freedom
# Null hypothesis probability = 9.307245e-01
Photon flux (15-150 keV) in 137.5 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] : 13.4327 (-1.3167 1.4651)
R^2/D10^2 : 6.36665E-02 (-0.020339 0.0296343)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 100.61 using 59 PHA bins.
# Reduced chi-squared = 1.7651 for 57 degrees of freedom
# Null hypothesis probability = 3.256038e-04
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.347e-07 4.957e-08
25- 50 1.193e-06 1.118e-07
50-150 1.387e-06 2.210e-07
15-150 2.915e-06 2.578e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 152.172 (-45.3111 -150.193)
Norm : 1.64285 (-0.141907 0.184178)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 43.50 using 59 PHA bins.
# Reduced chi-squared = 0.7631 for 57 degrees of freedom
# Null hypothesis probability = 9.061622e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.795e-07 5.981e-08
25- 50 1.076e-06 1.698e-07
50-150 2.137e-06 8.996e-07
15-150 3.793e-06 9.501e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.78396 (-1.43602 1.51464)
R1^2/D10^2 : 0.362689 (-0.164962 0.375935)
kT2 [keV] : 34.8828 (-9.77531 25.1928)
R2^2/D10^2 : 1.60017E-03 (-0.00125232 0.00341952)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 41.16 using 59 PHA bins.
# Reduced chi-squared = 0.7484 for 55 degrees of freedom
# Null hypothesis probability = 9.169840e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.730e-07 1.189e-07
25- 50 1.141e-06 1.893e-07
50-150 2.194e-06 1.005e-06
15-150 3.908e-06 1.119e-06
Peak spectrum fit
Power-law model
Time interval is from 0.360 sec. to 1.360 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.17099 ( -0.334503 0.316421 )
Norm@50keV : 2.36579E-02 ( -0.0048432 0.00477486 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 68.47 using 59 PHA bins.
# Reduced chi-squared = 1.201 for 57 degrees of freedom
# Null hypothesis probability = 1.420289e-01
Photon flux (15-150 keV) in 1 sec: 2.76612 ( -0.598712 0.606274 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.42031e-07 ( -4.78945e-08 4.79518e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.360 sec. to 1.360 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.518729 ( -1.76323 0.907334 )
Epeak [keV] : 137.850 ( -137.886 -137.886 )
Norm@50keV : 4.48485E-02 ( -0.0250289 0.183768 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 67.73 using 59 PHA bins.
# Reduced chi-squared = 1.210 for 56 degrees of freedom
# Null hypothesis probability = 1.352996e-01
Photon flux (15-150 keV) in 1 sec: 2.70242 ( -0.60533 0.6173 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.40271e-07 ( -4.936e-08 4.8722e-08 ) ergs/cm2
Band function
Time interval is from 0.360 sec. to 1.360 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 4.94789 ( -4.94789 -4.94789 )
beta : -1.29739 ( -0.400845 0.378603 )
Epeak [keV] : 32.1135 ( -32.1135 14.7475 )
Norm@50keV : 401.107 ( -77.407 7.65831e+06 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 67.23 using 59 PHA bins.
# Reduced chi-squared = 1.222 for 55 degrees of freedom
# Null hypothesis probability = 1.247068e-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] : 21.2330 (-4.41751 6.41564)
R^2/D10^2 : 0.109490 (-0.0645917 0.132617)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 70.95 using 59 PHA bins.
# Reduced chi-squared = 1.245 for 57 degrees of freedom
# Null hypothesis probability = 1.012414e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 9.281e-09 3.856e-09
25- 50 4.804e-08 1.767e-08
50-150 1.615e-07 6.127e-08
15-150 2.189e-07 6.185e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 ( )
Norm : 12.0905 (-2.42635 2.42559)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 72.55 using 59 PHA bins.
# Reduced chi-squared = 1.273 for 57 degrees of freedom
# Null hypothesis probability = 8.027963e-02
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.013e-08 1.791e-08
25- 50 5.796e-08 3.292e-08
50-150 1.271e-07 7.410e-08
15-150 2.152e-07 1.245e-07
Double BB
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 41.1331 ( )
R1^2/D10^2 : 9.03107E-03 (-0.00932983 0.10201)
kT2 [keV] : 12.0742 (-8.96329 -11.9136)
R2^2/D10^2 : 0.427844 (-0.389263 47.2696)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 67.89 using 59 PHA bins.
#Fit statistic : Chi-Squared = 67.78 using 59 PHA bins.
# Reduced chi-squared = 1.234 for 55 degrees of freedom
# Reduced chi-squared = 1.232 for 55 degrees of freedom
# Null hypothesis probability = 1.137972e-01
# Null hypothesis probability = 1.155599e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.704e-08 1.091e-08
25- 50 5.226e-08 2.978e-08
50-150 1.666e-07 9.615e-08
15-150 2.359e-07 1.246e-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: 1.52669 ( -0.149572 0.149152 )
Norm@50keV : 8.57097E-03 ( -0.000738568 0.000738461 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 42.19 using 59 PHA bins.
# Reduced chi-squared = 0.7401 for 57 degrees of freedom
# Null hypothesis probability = 9.286608e-01
Photon flux (15-150 keV) in 33.14 sec: 1.07786 ( -0.101737 0.102239 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.68322e-06 ( -2.40465e-07 2.4091e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.41295 ( -0.631504 1.3784 )
Epeak [keV] : 255.463 ( -298.952 -298.952 )
Norm@50keV : 9.70999E-03 ( -0.00961481 0.00911777 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 42.16 using 59 PHA bins.
# Reduced chi-squared = 0.7528 for 56 degrees of freedom
# Null hypothesis probability = 9.146971e-01
Photon flux (15-150 keV) in 33.14 sec: 1.07266 ( -0.10516 0.10535 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.67293e-06 ( -2.5089e-07 2.47963e-07 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.175987 ( 0.901442 5.53642 )
beta : -1.63150 ( 1.65755 0.252286 )
Epeak [keV] : 46.2132 ( -46.1849 232.874 )
Norm@50keV : 5.95147E-02 ( -0.0602661 1.02567e+06 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 41.11 using 59 PHA bins.
# Reduced chi-squared = 0.7475 for 55 degrees of freedom
# Null hypothesis probability = 9.178352e-01
Photon flux (15-150 keV) in 33.14 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) = 1.05e-06
S(50-100 keV) = 1.29e-06
T90 vs. Hardness ratio plot
T90 = 68.6439999341965 sec.
Hardness ratio (energy fluence ratio) = 1.22857
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.39573
Count Ratio (50-100 keV) / (15-25 keV) = 0.980338
Mask shadow pattern
IMX = -1.383715046351633E+00, IMY = 2.629757897240920E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 2.048000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 2.048000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 2.048000
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:
-149.379370 -2.524000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
355.5494 -15.7553 2.8 39.9 102.0 2.2986 4.1 ------ UNKNOWN
359.2587 -25.0649 2.7 39.2 86.4 2.6188 4.3 ------ UNKNOWN
70.0738 -44.7552 3.1 49.5 -2.9 1.0889 3.7 ------ UNKNOWN
40.7508 29.4266 2.8 35.7 -141.7 0.8128 4.1 ------ UNKNOWN
82.2878 -9.2573 2.2 47.0 -53.2 3.4033 5.3 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-2.524000 30.620600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
357.8692 21.5348 1.9 45.5 157.8 1.0152 6.0 ------ UNKNOWN
31.0893 -25.7085 2.3 20.2 39.8 0.3617 5.0 ------ UNKNOWN
13.0103 45.1025 0.7 54.6 -169.2 3.6905 15.4 ------ UNKNOWN
25.5362 49.1599 2.1 55.6 -157.8 1.6618 5.6 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
102.020580 239.820600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
326.2722 38.3582 5.2 35.0 112.0 0.7283 2.2 5.2 Cyg X-2
25.1117 11.6785 2.7 35.0 -4.8 0.7306 4.2 ------ UNKNOWN
199.4342 75.7083 2.3 59.1 -165.6 4.6733 5.0 ------ UNKNOWN
177.1140 75.7395 3.9 58.7 -159.3 2.7856 3.0 ------ UNKNOWN
58.5698 25.0716 2.0 41.6 -60.8 2.5092 5.9 ------ UNKNOWN
81.9087 55.9735 2.3 43.2 -114.1 2.7949 5.0 ------ UNKNOWN
57.0001 12.2591 2.6 49.7 -46.7 2.7451 4.5 ------ UNKNOWN
Plot creation:
Sat May 30 13:04:54 EDT 2015