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Image
Pre-slew 15.0-350.0 keV image (Event data)
# RAcent DECcent POSerr Theta Phi Peak Cts SNR Name
198.2827 8.1976 0.0067 26.1407 16.5987 3.5298217 28.714 TRIG_00622006
Foreground time interval of the image:
-24.112 16.397 (delta_t = 40.509 [sec])
Background time interval of the image:
-66.603 -24.112 (delta_t = 42.491 [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 -24.112 sec. to 20.332 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.73620 ( -0.0833918 0.0842692 )
Norm@50keV : 5.14748E-03 ( -0.000250348 0.000249051 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 73.00 using 59 PHA bins.
# Reduced chi-squared = 1.281 for 57 degrees of freedom
# Null hypothesis probability = 7.509017e-02
Photon flux (15-150 keV) in 44.44 sec: 0.692519 ( -0.0324121 0.0324645 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.11256e-06 ( -1.06762e-07 1.07359e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -24.112 sec. to 20.332 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.25567 ( -0.384986 0.351711 )
Epeak [keV] : 72.8343 ( -14.4238 67.5774 )
Norm@50keV : 9.20439E-03 ( -0.0031285 0.00536025 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 67.42 using 59 PHA bins.
# Reduced chi-squared = 1.204 for 56 degrees of freedom
# Null hypothesis probability = 1.411597e-01
Photon flux (15-150 keV) in 44.44 sec: 0.673819 ( -0.035046 0.035025 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.01951e-06 ( -1.26121e-07 1.26538e-07 ) ergs/cm2
Band function
Time interval is from -24.112 sec. to 20.332 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.984335 ( -0.488504 0.990272 )
beta : -2.06697 ( 2.06879 0.290726 )
Epeak [keV] : 57.9241 ( -32.9402 34.828 )
Norm@50keV : 1.33946E-02 ( -0.00623435 126.004 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 65.44 using 59 PHA bins.
# Reduced chi-squared = 1.190 for 55 degrees of freedom
# Null hypothesis probability = 1.583116e-01
Photon flux (15-150 keV) in 44.44 sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 2.02252e-06 ( -2.02221e-06 -1.21255e-07 ) ergs/cm2
Single BB
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 12.6513 ( )
R^2/D10^2 : 0.135351 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 149.49 using 59 PHA bins.
# Reduced chi-squared = 2.6226 for 57 degrees of freedom
# Null hypothesis probability = 3.146027e-10
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.042e-07 1.720e-08
25- 50 6.826e-07 3.555e-08
50-150 6.795e-07 7.377e-08
15-150 1.566e-06 7.777e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 111.814 (-18.2097 34.6354)
Norm : 3.00881 (-0.204604 0.182689)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 67.61 using 59 PHA bins.
# Reduced chi-squared = 1.186 for 57 degrees of freedom
# Null hypothesis probability = 1.588031e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.491e-07 2.869e-08
25- 50 6.166e-07 3.666e-08
50-150 1.062e-06 2.971e-07
15-150 2.028e-06 3.140e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.85896 (-1.41165 1.70516)
R1^2/D10^2 : 0.821503 (-0.396632 0.954585)
kT2 [keV] : 22.3845 (-4.28759 9.82093)
R2^2/D10^2 : 1.21073E-02 (-0.00889039 0.0163065)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 72.33 using 59 PHA bins.
# Reduced chi-squared = 1.315 for 55 degrees of freedom
# Null hypothesis probability = 5.850651e-02
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.195e-07 5.211e-08
25- 50 6.198e-07 8.021e-08
50-150 1.045e-06 2.693e-07
15-150 1.984e-06 3.946e-07
Peak spectrum fit
Power-law model
Time interval is from -0.096 sec. to 0.904 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.13067 ( -0.135538 0.133737 )
Norm@50keV : 2.62627E-02 ( -0.00199174 0.00199132 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 63.12 using 59 PHA bins.
# Reduced chi-squared = 1.107 for 57 degrees of freedom
# Null hypothesis probability = 2.689130e-01
Photon flux (15-150 keV) in 1 sec: 3.05599 ( -0.237548 0.237804 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.71958e-07 ( -2.30655e-08 2.31901e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.096 sec. to 0.904 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.08495 ( -0.532616 0.169177 )
Epeak [keV] : 997.895 ( -999.871 -999.871 )
Norm@50keV : 2.77374E-02 ( -0.00317706 0.0210481 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 63.13 using 59 PHA bins.
# Reduced chi-squared = 1.127 for 56 degrees of freedom
# Null hypothesis probability = 2.390757e-01
Photon flux (15-150 keV) in 1 sec: 3.05041 ( -0.2426 0.24233 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.71162e-07 ( -2.4508e-08 2.4e-08 ) ergs/cm2
Band function
Time interval is from -0.096 sec. to 0.904 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 0.180039 ( 0.428155 5.14478 )
beta : -1.20960 ( 1.19653 0.178925 )
Epeak [keV] : 53.0998 ( -53.1323 222.376 )
Norm@50keV : 0.186305 ( -0.195066 2437.01 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 62.14 using 59 PHA bins.
# Reduced chi-squared = 1.130 for 55 degrees of freedom
# Null hypothesis probability = 2.368260e-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] : 18.8938 (-1.94186 2.26771)
R^2/D10^2 : 0.170398 (-0.0526368 0.0729369)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 98.05 using 59 PHA bins.
# Reduced chi-squared = 1.720 for 57 degrees of freedom
# Null hypothesis probability = 5.926883e-04
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.198e-08 2.020e-09
25- 50 5.740e-08 7.000e-09
50-150 1.504e-07 1.940e-08
15-150 2.198e-07 2.160e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 ( )
Norm : 12.5119 (-0.975992 0.975927)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 89.39 using 59 PHA bins.
# Reduced chi-squared = 1.568 for 57 degrees of freedom
# Null hypothesis probability = 3.944244e-03
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.116e-08 3.155e-09
25- 50 5.994e-08 8.810e-09
50-150 1.315e-07 4.819e-08
15-150 2.226e-07 5.365e-08
Double BB
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 12.3667 (-3.12678 2.30592)
R1^2/D10^2 : 0.544046 (-0.232512 0.689315)
kT2 [keV] : 199.509 ( )
R2^2/D10^2 : 4.94222E-04 (-0.00011776 0.0173245)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 62.03 using 59 PHA bins.
#Fit statistic : Chi-Squared = 61.96 using 59 PHA bins.
# Reduced chi-squared = 1.128 for 55 degrees of freedom
# Reduced chi-squared = 1.126 for 55 degrees of freedom
# Null hypothesis probability = 2.398643e-01
# Null hypothesis probability = 2.419047e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.891e-08 4.815e-09
25- 50 6.238e-08 1.736e-08
50-150 1.886e-07 1.327e-07
15-150 2.698e-07 1.657e-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: 1.69969 ( -0.0831124 0.0838737 )
Norm@50keV : 5.45460E-03 ( -0.000261729 0.000260523 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 68.47 using 59 PHA bins.
# Reduced chi-squared = 1.201 for 57 degrees of freedom
# Null hypothesis probability = 1.420378e-01
Photon flux (15-150 keV) in 40.51 sec: 0.724356 ( -0.0338817 0.033929 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.04593e-06 ( -1.03009e-07 1.03557e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.29582 ( -0.375632 0.343823 )
Epeak [keV] : 82.9623 ( -19.7805 170.896 )
Norm@50keV : 8.85636E-03 ( -0.00293504 0.00494126 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 64.41 using 59 PHA bins.
# Reduced chi-squared = 1.150 for 56 degrees of freedom
# Null hypothesis probability = 2.059807e-01
Photon flux (15-150 keV) in 40.51 sec: 0.707862 ( -0.036578 0.036537 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.97093e-06 ( -1.21485e-07 1.21465e-07 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.999512 ( -0.508023 0.996602 )
beta : -1.97670 ( 1.97627 0.267639 )
Epeak [keV] : 60.9496 ( -37.6517 55.6235 )
Norm@50keV : 1.33165E-02 ( -0.00641721 251.254 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 62.35 using 59 PHA bins.
# Reduced chi-squared = 1.134 for 55 degrees of freedom
# Null hypothesis probability = 2.313134e-01
Photon flux (15-150 keV) in 40.51 sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 1.9707e-06 ( -1.97042e-06 -1.16786e-07 ) ergs/cm2
S(25-50 keV) vs. S(50-100 keV) plot
S(25-50 keV) = 5.80e-07
S(50-100 keV) = 6.97e-07
T90 vs. Hardness ratio plot
T90 = 36.8159999847412 sec.
Hardness ratio (energy fluence ratio) = 1.20172
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.28981
Count Ratio (50-100 keV) / (15-25 keV) = 0.777686
Mask shadow pattern
IMX = 4.703254137966747E-01, IMY = -1.401982135373573E-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:
-66.603390 -24.112000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.3701 35.2671 6.6 31.8 -154.8 0.1631 1.8 6.2 Her X-1
185.8414 -15.0699 2.5 51.6 5.5 1.0511 4.5 ------ UNKNOWN
234.5494 -18.3945 2.3 45.7 -57.7 1.8838 5.0 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-24.112000 16.396600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.5156 35.5474 0.0 32.0 -155.2 0.2154 1.7 12.6 Her X-1
192.0431 46.0526 2.0 30.4 103.6 1.1430 5.6 ------ UNKNOWN
200.8048 52.9555 2.3 31.4 121.0 0.9856 5.0 ------ UNKNOWN
198.2827 8.1976 0.4 26.1 16.6 3.5299 28.7 ------ UNKNOWN
230.4463 -18.4867 2.2 44.7 -52.4 1.8756 5.2 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
63.596600 645.396610
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.4906 35.3580 8.3 57.9 -153.4 4.2442 1.4 1.9 Her X-1
232.6970 55.0447 4.1 54.2 177.0 5.3318 2.8 ------ UNKNOWN
196.0271 0.3009 3.4 8.2 -10.5 1.6334 3.5 ------ UNKNOWN
220.9423 20.5538 2.8 25.1 -148.4 2.0201 4.1 ------ UNKNOWN
251.3387 46.0373 2.7 59.0 -166.1 13.1148 4.3 ------ UNKNOWN
253.6401 38.2412 3.7 58.0 -156.8 9.9217 3.2 ------ UNKNOWN
197.4255 -50.5353 5.2 58.7 -25.9 7.2810 2.2 ------ UNKNOWN
209.2816 -45.2009 2.6 54.3 -36.0 12.7612 4.5 ------ UNKNOWN
244.1125 9.2356 3.7 45.3 -121.4 5.8572 3.1 ------ UNKNOWN
246.8965 14.8077 3.5 48.0 -129.1 8.1050 3.3 ------ UNKNOWN
Plot creation:
Thu May 28 13:49:41 EDT 2015