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Image
Pre-slew 15.0-350.0 keV image (Event data)
# RAcent DECcent POSerr Theta Phi Peak Cts SNR Name
69.5267 -34.2366 0.0159 25.0445 -111.0085 0.9745536 12.082 TRIG_00589590
Foreground time interval of the image:
-19.220 21.580 (delta_t = 40.800 [sec])
Background time interval of the image:
-239.184 -19.220 (delta_t = 219.964 [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)
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 -19.220 sec. to 21.580 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.96338 ( -0.266457 0.28568 )
Norm@50keV : 1.21152E-03 ( -0.000225034 0.000216574 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 62.00 using 59 PHA bins.
# Reduced chi-squared = 1.088 for 57 degrees of freedom
# Null hypothesis probability = 3.023788e-01
Photon flux (15-150 keV) in 40.8 sec: 0.178736 ( -0.0247326 0.0247333 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.55091e-07 ( -7.85804e-08 8.11063e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -19.220 sec. to 21.580 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.96333 ( -0.793323 1.14978 )
Epeak [keV] : 598.003 ( )
Norm@50keV : 1.21273E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 62.00 using 59 PHA bins.
# Reduced chi-squared = 1.107 for 56 degrees of freedom
# Null hypothesis probability = 2.707079e-01
Photon flux (15-150 keV) in 40.8 sec: 0.178704 ( -0.02474 0.024723 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.52093e-07 ( -4.07633e-08 8.26649e-08 ) ergs/cm2
Band function
Time interval is from -19.220 sec. to 21.580 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 4.95842 ( -4.95842 -4.95842 )
beta : -2.03652 ( -0.347783 0.293219 )
Epeak [keV] : 19.4803 ( -19.4803 4.26113 )
Norm@50keV : 925.876 ( -127.65 1.65707e+06 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 61.07 using 59 PHA bins.
# Reduced chi-squared = 1.110 for 55 degrees of freedom
# Null hypothesis probability = 2.671375e-01
Photon flux (15-150 keV) in 40.8 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] : 9.00444 (-1.50047 1.83264)
R^2/D10^2 : 0.121202 (-0.0617391 0.124822)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 77.49 using 59 PHA bins.
# Reduced chi-squared = 1.360 for 57 degrees of freedom
# Null hypothesis probability = 3.681014e-02
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.808e-08 1.867e-08
25- 50 1.661e-07 3.315e-08
50-150 6.346e-08 2.658e-08
15-150 3.076e-07 6.648e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 69.7222 (-26.9796 61.8954)
Norm : 0.874499 (-0.186263 0.254004)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 64.09 using 59 PHA bins.
# Reduced chi-squared = 1.124 for 57 degrees of freedom
# Null hypothesis probability = 2.419336e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 9.150e-08 1.677e-08
25- 50 1.454e-07 2.456e-08
50-150 1.862e-07 9.233e-08
15-150 4.231e-07 1.003e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.66867 (-2.29461 1.94884)
R1^2/D10^2 : 0.334907 (-0.201425 1.21888)
kT2 [keV] : 41.2919 (-25.715 -42.3082)
R2^2/D10^2 : 3.96713E-04 (-0.000356135 0.00831223)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 62.29 using 59 PHA bins.
# Reduced chi-squared = 1.133 for 55 degrees of freedom
# Null hypothesis probability = 2.328752e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 9.605e-08 4.297e-08
25- 50 1.391e-07 5.392e-08
50-150 2.540e-07 1.429e-07
15-150 4.892e-07 2.174e-07
Peak spectrum fit
Power-law model
Time interval is from 0.108 sec. to 1.108 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.44393 ( -0.364911 0.367229 )
Norm@50keV : 6.59497E-03 ( -0.00134221 0.00132437 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 68.62 using 59 PHA bins.
# Reduced chi-squared = 1.204 for 57 degrees of freedom
# Null hypothesis probability = 1.393263e-01
Photon flux (15-150 keV) in 1 sec: 0.811521 ( -0.162877 0.16331 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.31806e-08 ( -1.41694e-08 1.43816e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.108 sec. to 1.108 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.45418 ( -0.922239 0.359903 )
Epeak [keV] : 9999.35 ( -9999.36 -9999.36 )
Norm@50keV : 6.57642E-03 ( -0.00133921 0.00921261 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 68.63 using 59 PHA bins.
# Reduced chi-squared = 1.225 for 56 degrees of freedom
# Null hypothesis probability = 1.198651e-01
Photon flux (15-150 keV) in 1 sec: 0.813468 ( -0.164885 0.161347 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.31846e-08 ( -1.41425e-08 1.41749e-08 ) ergs/cm2
Band function
Time interval is from 0.108 sec. to 1.108 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 4.97767 ( -4.97767 -4.97767 )
beta : -1.48766 ( -0.416926 0.382344 )
Epeak [keV] : 21.5082 ( -21.5082 7.88008 )
Norm@50keV : 1635.43 ( -320.498 4.15176e+06 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 68.22 using 59 PHA bins.
# Reduced chi-squared = 1.240 for 55 degrees of freedom
# Null hypothesis probability = 1.085909e-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] : 17.5968 (-4.98176 7.09115)
R^2/D10^2 : 5.19365E-02 (-0.0349668 0.110223)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 80.15 using 59 PHA bins.
# Reduced chi-squared = 1.406 for 57 degrees of freedom
# Null hypothesis probability = 2.332660e-02
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.243e-09 1.542e-09
25- 50 1.474e-08 6.123e-09
50-150 3.293e-08 1.447e-08
15-150 5.092e-08 2.281e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.362 (-42.8901 -199.363)
Norm : 3.32456 (-0.657508 0.658774)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 69.60 using 59 PHA bins.
# Reduced chi-squared = 1.221 for 57 degrees of freedom
# Null hypothesis probability = 1.221118e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.278e-09 4.819e-09
25- 50 1.592e-08 9.025e-09
50-150 3.493e-08 2.042e-08
15-150 5.913e-08 3.395e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.20505 (-1.86789 3.04451)
R1^2/D10^2 : 2.91256 (-2.4349 18.2796)
kT2 [keV] : 29.6447 (-10.0766 32.386)
R2^2/D10^2 : 8.09122E-03 (-0.0070185 0.0234891)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 67.02 using 59 PHA bins.
# Reduced chi-squared = 1.219 for 55 degrees of freedom
# Null hypothesis probability = 1.283367e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 9.417e-09 5.455e-09
25- 50 1.285e-08 6.875e-09
50-150 4.319e-08 2.571e-08
15-150 6.546e-08 3.530e-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: 1.96338 ( -0.266457 0.28568 )
Norm@50keV : 1.21152E-03 ( -0.000225034 0.000216574 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 62.00 using 59 PHA bins.
# Reduced chi-squared = 1.088 for 57 degrees of freedom
# Null hypothesis probability = 3.023788e-01
Photon flux (15-150 keV) in 40.8 sec: 0.178736 ( -0.0247326 0.0247333 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.55091e-07 ( -7.85804e-08 8.11063e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.96333 ( -0.793323 1.14978 )
Epeak [keV] : 598.003 ( )
Norm@50keV : 1.21273E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 62.00 using 59 PHA bins.
# Reduced chi-squared = 1.107 for 56 degrees of freedom
# Null hypothesis probability = 2.707079e-01
Photon flux (15-150 keV) in 40.8 sec: 0.178704 ( -0.02474 0.024723 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.52093e-07 ( -4.07633e-08 8.26649e-08 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 4.95842 ( -4.95842 -4.95842 )
beta : -2.03652 ( -0.347783 0.293219 )
Epeak [keV] : 19.4803 ( -19.4803 4.26113 )
Norm@50keV : 925.876 ( -127.65 1.65707e+06 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 61.07 using 59 PHA bins.
# Reduced chi-squared = 1.110 for 55 degrees of freedom
# Null hypothesis probability = 2.671375e-01
Photon flux (15-150 keV) in 40.8 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) = 1.35e-07
S(50-100 keV) = 1.39e-07
T90 vs. Hardness ratio plot
T90 = 27.8039999008179 sec.
Hardness ratio (energy fluence ratio) = 1.02963
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.06207
Count Ratio (50-100 keV) / (15-25 keV) = 0.527182
Mask shadow pattern
IMX = -1.675136405898341E-01, IMY = 4.361939605809910E-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:
-239.184000 -19.220000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6372 22.0162 0.5 45.0 0.2 8.6418 24.8 0.2 Crab
135.5754 -40.5428 1.8 39.5 142.2 2.4046 6.3 2.3 Vela X-1
100.0901 -24.4641 2.5 6.0 132.0 0.7327 4.6 ------ UNKNOWN
124.7709 -78.5532 2.8 58.5 -172.6 4.3775 4.1 ------ UNKNOWN
47.1385 -47.0177 2.2 45.4 -121.2 4.0206 5.1 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-19.220000 21.580000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6368 22.0211 8.7 45.0 0.2 0.1785 1.3 0.4 Crab
135.5171 -40.7534 11.6 39.6 142.5 0.1427 1.0 11.9 Vela X-1
115.0971 -34.9275 2.3 22.5 144.5 0.3641 5.0 ------ UNKNOWN
84.3850 30.2170 2.6 52.8 3.5 1.1409 4.4 ------ UNKNOWN
69.5267 -34.2365 1.0 25.0 -111.0 0.9747 12.1 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
75.516590 907.016600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
98.1158 -18.6702 3.3 29.8 70.5 2.7736 3.4 ------ UNKNOWN
67.5008 20.9457 2.7 55.2 2.4 11.1527 4.3 ------ UNKNOWN
141.7608 -89.5769 3.1 55.6 -175.7 6.6870 3.8 ------ UNKNOWN
43.0195 -52.4468 2.7 26.2 -137.1 2.2158 4.3 ------ UNKNOWN
318.6112 -81.7235 4.0 59.0 -166.2 9.6763 2.9 ------ UNKNOWN
10.5235 -47.8633 2.7 45.4 -121.2 9.8477 4.3 ------ UNKNOWN
Plot creation:
Sat May 30 14:22:06 EDT 2015