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Image
Pre-slew 15.0-350.0 keV image (Event data)
# RAcent DECcent POSerr Theta Phi Peak Cts SNR Name
120.1278 45.8081 0.0197 13.8173 -144.1414 0.7262714 9.754 TRIG_00453788
Foreground time interval of the image:
0.568 49.869 (delta_t = 49.301 [sec])
Background time interval of the image:
-239.432 0.568 (delta_t = 240.000 [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 8.192000
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 8.192000
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 8.192000
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)
The mask-weighted light curves based on cleaned DPHs
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 0.568 sec. to 108.568 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.764703 ( -0.374755 0.335202 )
Norm@50keV : 5.23647E-04 ( -0.000103856 9.96412e-05 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 52.26 using 59 PHA bins.
# Reduced chi-squared = 0.9168 for 57 degrees of freedom
# Null hypothesis probability = 6.533286e-01
Photon flux (15-150 keV) in 108 sec: 6.02751E-02 ( -0.0111787 0.0112598 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.70895e-07 ( -1.25528e-07 1.26513e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.568 sec. to 108.568 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.766495 ( -0.386358 0.329709 )
Epeak [keV] : 9999.36 ( -9999.36 -9999.36 )
Norm@50keV : 5.27483E-04 ( -0.000104854 0.000945194 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 52.27 using 59 PHA bins.
# Reduced chi-squared = 0.9334 for 56 degrees of freedom
# Null hypothesis probability = 6.168603e-01
Photon flux (15-150 keV) in 108 sec: 6.04696E-02 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 6.69655e-07 ( -1.2426e-07 1.26821e-07 ) ergs/cm2
Band function
Time interval is from 0.568 sec. to 108.568 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.807335 ( 0.807521 0.807521 )
beta : -0.764704 ( -0.335001 0.374756 )
Epeak [keV] : 16.9577 ( -16.9572 -16.9572 )
Norm@50keV : 7.39732E-04 ( -0.000316504 0 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 52.26 using 59 PHA bins.
# Reduced chi-squared = 0.9501 for 55 degrees of freedom
# Null hypothesis probability = 5.801216e-01
Photon flux (15-150 keV) in 108 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] : 26.3948 (-6.553 11.5938)
R^2/D10^2 : 1.27323E-03 (-0.000812827 0.0017573)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 58.31 using 59 PHA bins.
# Reduced chi-squared = 1.023 for 57 degrees of freedom
# Null hypothesis probability = 4.268193e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.616e-08 6.759e-09
25- 50 9.416e-08 3.833e-08
50-150 4.817e-07 2.027e-07
15-150 5.920e-07 1.979e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 ( )
Norm : 0.243419 (-0.0468092 0.0468046)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 67.38 using 59 PHA bins.
# Reduced chi-squared = 1.182 for 57 degrees of freedom
# Null hypothesis probability = 1.635626e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.546e-08 3.830e-08
25- 50 1.259e-07 7.355e-08
50-150 2.761e-07 1.575e-07
15-150 4.675e-07 2.706e-07
Double BB
R1^2/D10^2 : 6.64208E-03 ( )
kT2 [keV] : 200.000 ( )
R2^2/D10^2 : 1.40611E-05 (-6.9484e-06 8.32347e-05)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 51.46 using 59 PHA bins.
#Fit statistic : Chi-Squared = 51.08 using 59 PHA bins.
#Fit statistic : Chi-Squared = 51.04 using 59 PHA bins.
# Reduced chi-squared = 0.9357 for 55 degrees of freedom
# Reduced chi-squared = 0.9288 for 55 degrees of freedom
# Reduced chi-squared = 0.9279 for 55 degrees of freedom
# Null hypothesis probability = 6.104929e-01
# Null hypothesis probability = 6.250560e-01
# Null hypothesis probability = 6.268246e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.106e-08 1.886e-08
25- 50 1.167e-07 6.491e-08
50-150 5.306e-07 3.560e-07
15-150 6.784e-07 4.520e-07
Peak spectrum fit
Power-law model
Time interval is from 7.568 sec. to 8.568 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.737404 ( -0.673377 0.529493 )
Norm@50keV : 3.75007E-03 ( -0.00122614 0.00109897 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 65.57 using 59 PHA bins.
# Reduced chi-squared = 1.150 for 57 degrees of freedom
# Null hypothesis probability = 2.040907e-01
Photon flux (15-150 keV) in 1 sec: 0.432319 ( -0.123465 0.124209 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.50183e-08 ( -1.3043e-08 1.32135e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 7.568 sec. to 8.568 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.756260 ( -1.00449 0.509823 )
Epeak [keV] : 9999.36 ( -9999.36 -9999.36 )
Norm@50keV : 3.79992E-03 ( -0.00107537 0.00897402 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 65.59 using 59 PHA bins.
# Reduced chi-squared = 1.171 for 56 degrees of freedom
# Null hypothesis probability = 1.784844e-01
Photon flux (15-150 keV) in 1 sec: 0.435038 ( -0.126457 0.121712 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.47605e-08 ( -1.27922e-08 1.29931e-08 ) ergs/cm2
Band function
Time interval is from 7.568 sec. to 8.568 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.769431 ( 0.768729 0.768729 )
beta : -0.737426 ( -0.528766 0.674051 )
Epeak [keV] : 17.3819 ( -17.3819 -17.3819 )
Norm@50keV : 5.30968E-03 ( -0.00264437 92913.3 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 65.57 using 59 PHA bins.
# Reduced chi-squared = 1.192 for 55 degrees of freedom
# Null hypothesis probability = 1.557613e-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] : 23.5084 (-9.64685 77.2831)
R^2/D10^2 : 1.24974E-02 (-0.012164 0.0531586)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 70.46 using 59 PHA bins.
# Reduced chi-squared = 1.236 for 57 degrees of freedom
# Null hypothesis probability = 1.084546e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.238e-09 7.700e-10
25- 50 6.800e-09 4.189e-09
50-150 2.804e-08 1.784e-08
15-150 3.608e-08 2.256e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 ( )
Norm : 1.72962 (-0.512076 0.512057)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 72.06 using 59 PHA bins.
# Reduced chi-squared = 1.264 for 57 degrees of freedom
# Null hypothesis probability = 8.631014e-02
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.306e-09 2.667e-09
25- 50 8.284e-09 4.884e-09
50-150 1.817e-08 1.110e-08
15-150 3.076e-08 1.940e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 11.7224 (-4.07345 4.40616)
R1^2/D10^2 : 7.89115E-02 (-0.0616795 0.127904)
kT2 [keV] : 199.085 (-146.719 -199.19)
R2^2/D10^2 : 1.15053E-04 (-5.06104e-05 0.00107949)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 62.16 using 59 PHA bins.
# Reduced chi-squared = 1.130 for 55 degrees of freedom
# Null hypothesis probability = 2.363740e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.435e-09 1.510e-09
25- 50 8.253e-09 5.165e-09
50-150 3.610e-08 8.340e-09
15-150 4.679e-08 1.492e-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: 0.759667 ( -0.29397 0.270666 )
Norm@50keV : 9.51354E-04 ( -0.00015243 0.000148313 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 47.85 using 59 PHA bins.
# Reduced chi-squared = 0.8394 for 57 degrees of freedom
# Null hypothesis probability = 8.008327e-01
Photon flux (15-150 keV) in 49.3 sec: 0.109537 ( -0.0166045 0.016704 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.57598e-07 ( -8.56681e-08 8.62503e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.754408 ( -0.298231 0.271634 )
Epeak [keV] : 9999.36 ( -9999.36 -9999.36 )
Norm@50keV : 9.58738E-04 ( -0.000143104 0.00196641 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 47.85 using 59 PHA bins.
# Reduced chi-squared = 0.8544 for 56 degrees of freedom
# Null hypothesis probability = 7.725517e-01
Photon flux (15-150 keV) in 49.3 sec: 0.109552 ( -0.0167489 0.016636 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.57608e-07 ( -8.97768e-08 8.58609e-08 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.899096 ( 0.899096 0.899096 )
beta : -0.759666 ( -0.27038 0.29397 )
Epeak [keV] : 14.9054 ( -14.9054 -14.9054 )
Norm@50keV : 1.36743E-03 ( -0.000560115 0 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 47.85 using 59 PHA bins.
# Reduced chi-squared = 0.8699 for 55 degrees of freedom
# Null hypothesis probability = 7.420542e-01
Photon flux (15-150 keV) in 49.3 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-07
S(50-100 keV) = 2.48e-07
T90 vs. Hardness ratio plot
T90 = 96 sec.
Hardness ratio (energy fluence ratio) = 2.3619
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 2.42037
Count Ratio (50-100 keV) / (15-25 keV) = 2.58885
Mask shadow pattern
IMX = -1.993289069839686E-01, IMY = 1.440704497886629E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 8.192000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 8.192000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 8.192000
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:
-239.432000 0.568000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
181.4505 58.9865 3.0 24.8 54.4 0.9758 3.8 ------ UNKNOWN
140.4938 44.8723 2.3 12.2 149.0 0.9095 5.1 ------ UNKNOWN
355.3487 83.5961 2.1 38.6 -16.6 1.3707 5.4 ------ UNKNOWN
117.3398 11.0190 2.2 47.3 -166.9 1.9142 5.3 ------ UNKNOWN
93.2845 15.9832 2.1 50.9 -135.5 4.8742 5.4 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
0.568000 49.868590
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
246.8004 80.7881 2.2 37.9 4.0 0.5830 5.1 ------ UNKNOWN
126.7086 19.3764 2.3 37.5 -178.0 0.5302 5.0 ------ UNKNOWN
124.7346 12.7020 2.3 44.4 -176.4 0.6993 5.0 ------ UNKNOWN
120.1282 45.8082 1.2 13.8 -144.1 0.7223 9.7 ------ UNKNOWN
115.0129 19.1274 2.6 40.0 -160.8 0.5259 4.5 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
84.668630 962.601200
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6352 22.0096 0.4 38.0 -111.0 35.7939 31.0 0.3 Crab
166.2062 33.8733 3.1 36.7 97.7 4.9511 3.7 ------ UNKNOWN
107.6355 -6.0997 2.6 53.1 -159.1 5.8764 4.5 ------ UNKNOWN
6.9135 67.3928 3.1 56.2 -19.9 7.0864 3.7 ------ UNKNOWN
Plot creation:
Sat May 30 22:14:58 EDT 2015