Estimated redshift from machine learning (Ukwatta et al. 2016) - may take a few minute to calcaulte
Image
Pre-slew 15.0-350.0 keV image (Event data)
# RAcent DECcent POSerr Theta Phi Peak Cts SNR Name
166.5437 -46.7859 0.0101 53.2460 -20.0970 2.0011949 19.099 TRIG_00737438
Foreground time interval of the image:
-0.036 8.060 (delta_t = 8.096 [sec])
Background time interval of the image:
-239.912 -0.036 (delta_t = 239.876 [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 0.512000
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 0.512000
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 0.512000
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 -0.036 sec. to 8.060 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.03939 ( -0.135775 0.130677 )
Norm@50keV : 1.78433E-02 ( -0.0014898 0.00147122 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 86.96 using 59 PHA bins.
# Reduced chi-squared = 1.526 for 57 degrees of freedom
# Null hypothesis probability = 6.459716e-03
Photon flux (15-150 keV) in 8.096 sec: 2.05926 ( -0.17903 0.18036 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.54103e-06 ( -1.16531e-07 1.16693e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.036 sec. to 8.060 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.686979 ( -0.591923 0.408507 )
Epeak [keV] : 233.046 ( -233.053 -233.053 )
Norm@50keV : 2.48953E-02 ( -0.00800007 0.017638 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 85.68 using 59 PHA bins.
# Reduced chi-squared = 1.530 for 56 degrees of freedom
# Null hypothesis probability = 6.518602e-03
Photon flux (15-150 keV) in 8.096 sec: 2.02963 ( -0.18316 0.18509 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.5332e-06 ( -1.18191e-07 1.17961e-07 ) ergs/cm2
Band function
Time interval is from -0.036 sec. to 8.060 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : ( )
beta : ( )
Epeak [keV] : ( )
Norm@50keV : ( )
------------------------------------------------------------
Photon flux (15-150 keV) in 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] : 23.6773 (-2.30422 2.73111)
R^2/D10^2 : 5.83094E-02 (-0.0176006 0.0237377)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 110.52 using 59 PHA bins.
# Reduced chi-squared = 1.9389 for 57 degrees of freedom
# Null hypothesis probability = 2.780222e-05
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.728e-08 7.550e-09
25- 50 2.607e-07 3.376e-08
50-150 1.090e-06 1.263e-07
15-150 1.398e-06 1.267e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.363 ( )
Norm : 9.19863 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 134.04 using 59 PHA bins.
# Reduced chi-squared = 2.3516 for 57 degrees of freedom
# Null hypothesis probability = 3.780026e-08
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.854e-07 1.814e-08
25- 50 3.567e-07 4.230e-08
50-150 7.824e-07 2.615e-07
15-150 1.325e-06 2.222e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 12.7305 (-2.90442 3.20641)
R1^2/D10^2 : 0.285328 (-0.131558 0.283899)
kT2 [keV] : 59.0362 (-24.9593 -59.0358)
R2^2/D10^2 : 2.93775E-03 (-0.00209112 0.00926674)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 81.36 using 59 PHA bins.
# Reduced chi-squared = 1.479 for 55 degrees of freedom
# Null hypothesis probability = 1.197017e-02
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.733e-08 3.610e-08
25- 50 3.266e-07 1.250e-07
50-150 1.111e-06 5.375e-07
15-150 1.525e-06 6.368e-07
Peak spectrum fit
Power-law model
Time interval is from -0.036 sec. to 0.964 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.02797 ( -0.172336 0.167279 )
Norm@50keV : 4.68991E-02 ( -0.00506723 0.00502054 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 71.66 using 59 PHA bins.
# Reduced chi-squared = 1.257 for 57 degrees of freedom
# Null hypothesis probability = 9.148741e-02
Photon flux (15-150 keV) in 1 sec: 0.141958 ( -0.001896 0.091529 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.02262e-07 ( -5.25029e-08 5.25425e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.036 sec. to 0.964 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.149450 ( -0.942 0.770484 )
Epeak [keV] : 133.467 ( -38.5922 413.316 )
Norm@50keV : 0.105972 ( -0.0534449 0.134718 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 67.83 using 59 PHA bins.
# Reduced chi-squared = 1.211 for 56 degrees of freedom
# Null hypothesis probability = 1.335846e-01
Photon flux (15-150 keV) in 1 sec: 5.23877 ( -0.61528 0.62044 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.98712e-07 ( -5.40603e-08 5.36833e-08 ) ergs/cm2
Band function
Time interval is from -0.036 sec. to 0.964 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : ( )
beta : ( )
Epeak [keV] : ( )
Norm@50keV : ( )
------------------------------------------------------------
Photon flux (15-150 keV) in 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] : 23.4630 (-2.67319 3.21439)
R^2/D10^2 : 0.164457 (-0.0561124 0.0796353)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 74.18 using 59 PHA bins.
# Reduced chi-squared = 1.301 for 57 degrees of freedom
# Null hypothesis probability = 6.274213e-02
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.625e-08 3.310e-09
25- 50 8.913e-08 1.449e-08
50-150 3.662e-07 5.240e-08
15-150 4.716e-07 6.425e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-17.9816 -200)
Norm : 23.1426 (-2.4906 2.4906)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 98.79 using 59 PHA bins.
# Reduced chi-squared = 1.733 for 57 degrees of freedom
# Null hypothesis probability = 4.991464e-04
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.765e-08 1.538e-08
25- 50 1.109e-07 5.495e-08
50-150 2.432e-07 1.325e-07
15-150 4.118e-07 2.255e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 2.16354 (-1.67474 10.1382)
R1^2/D10^2 : 1049.96 (-1049.69 -1052.54)
kT2 [keV] : 24.5640 (-2.97601 -24.5634)
R2^2/D10^2 : 0.139274 (-0.137536 0.0734655)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 67.79 using 59 PHA bins.
# Reduced chi-squared = 1.233 for 55 degrees of freedom
# Null hypothesis probability = 1.153258e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.356e-08 1.325e-08
25- 50 8.358e-08 1.494e-08
50-150 3.715e-07 5.970e-08
15-150 4.886e-07 7.140e-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: 1.03939 ( -0.135775 0.130677 )
Norm@50keV : 1.78433E-02 ( -0.0014898 0.00147122 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 86.96 using 59 PHA bins.
# Reduced chi-squared = 1.526 for 57 degrees of freedom
# Null hypothesis probability = 6.459716e-03
Photon flux (15-150 keV) in 8.096 sec: 2.05915 ( -0.178863 0.180427 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.54088e-06 ( -1.1665e-07 1.16665e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.686983 ( -0.591922 0.408508 )
Epeak [keV] : 233.046 ( -233.053 -233.053 )
Norm@50keV : 2.48953E-02 ( -0.00800007 0.017638 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 85.68 using 59 PHA bins.
# Reduced chi-squared = 1.530 for 56 degrees of freedom
# Null hypothesis probability = 6.518602e-03
Photon flux (15-150 keV) in 8.096 sec: 2.02955 ( -0.18311 0.18504 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.53394e-06 ( -1.18428e-07 1.18007e-07 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : ( )
beta : ( )
Epeak [keV] : ( )
Norm@50keV : ( )
------------------------------------------------------------
Photon flux (15-150 keV) in 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) = 2.93e-07
S(50-100 keV) = 5.70e-07
T90 vs. Hardness ratio plot
T90 = 7.44799995422363 sec.
Hardness ratio (energy fluence ratio) = 1.94539
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 2.40588
Count Ratio (50-100 keV) / (15-25 keV) = 2.91089
Mask shadow pattern
IMX = 1.257439648129232E+00, IMY = 4.600820549632218E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.512000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.512000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.512000
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:
-239.912000 -0.036000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.5138 -40.5555 1.3 48.1 9.2 3.6547 8.7 0.7 Vela X-1
148.9789 -50.8842 2.5 55.9 -5.4 3.2205 4.7 ------ UNKNOWN
163.6309 -13.7957 2.2 21.8 -38.5 1.0304 5.3 ------ UNKNOWN
191.0589 2.3858 4.7 38.6 -95.7 1.7359 2.5 ------ UNKNOWN
197.6880 25.9723 3.3 48.0 -129.0 3.3692 3.5 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-0.036000 8.060000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.6516 -40.6129 13.3 48.1 9.1 0.0674 0.9 6.6 Vela X-1
112.4244 11.4829 2.6 40.1 93.8 0.6498 4.5 ------ UNKNOWN
122.7581 49.2588 1.9 50.9 147.3 0.9399 6.2 ------ UNKNOWN
166.5437 -46.7859 0.6 53.2 -20.1 2.0007 19.1 ------ UNKNOWN
180.0453 7.8376 2.7 27.5 -105.5 0.2094 4.2 ------ UNKNOWN
185.3580 20.6360 3.1 35.6 -127.2 0.2114 3.8 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
103.388580 962.135100
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.5212 -40.5601 0.6 23.1 30.1 12.8837 20.7 0.5 Vela X-1
170.3839 -60.6347 2.5 14.1 -71.9 3.0103 4.6 2.1 Cen X-3
186.6444 -62.8012 2.5 19.6 -92.0 3.0997 4.7 1.9 GX 301-2
134.8277 -14.9467 2.8 41.3 65.6 9.5592 4.2 ------ UNKNOWN
145.7428 -32.7130 2.9 21.2 60.0 2.6537 4.0 ------ UNKNOWN
83.4537 -41.7329 4.0 56.9 -1.9 7.6503 2.9 ------ UNKNOWN
91.9563 -46.4346 2.9 49.2 -2.8 4.6846 4.0 ------ UNKNOWN
226.0253 -38.1774 3.8 43.6 -143.0 3.9950 3.1 ------ UNKNOWN
55.4516 -81.1270 3.1 47.0 -52.8 12.8836 3.7 ------ UNKNOWN
237.9731 -50.8593 3.1 45.4 -121.4 10.3165 3.8 ------ UNKNOWN
237.8291 -44.8617 3.8 48.0 -128.8 10.1519 3.1 ------ UNKNOWN
Plot creation:
Thu Apr 13 22:06:22 EDT 2017