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
248.3249 19.5782 0.0169 40.1231 -25.5672 2.0245601 11.344 TRIG_00868427
Foreground time interval of the image:
-16.299 36.940 (delta_t = 53.239 [sec])
Background time interval of the image:
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
8 ms binning
From T100_start-3 s to T100_start+3 s
2 ms binning
From T100_start-1 s to T100_start+1 s
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 -29.016 sec. to 36.940 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.72205 ( -0.236162 0.240581 )
Norm@50keV : 2.14004E-03 ( -0.000290052 0.00028677 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 71.77 using 59 PHA bins.
# Reduced chi-squared = 1.259 for 57 degrees of freedom
# Null hypothesis probability = 9.011103e-02
Photon flux (15-150 keV) in 65.96 sec: 0.286459 ( -0.038827 0.039046 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.305e-06 ( -1.82152e-07 1.84022e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -29.016 sec. to 36.940 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.55058 ( -0.980561 0.833897 )
Epeak [keV] : 129.856 ( -129.854 -129.854 )
Norm@50keV : 2.61513E-03 ( -0.000756533 0.00533001 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 71.65 using 59 PHA bins.
# Reduced chi-squared = 1.279 for 56 degrees of freedom
# Null hypothesis probability = 7.760368e-02
Photon flux (15-150 keV) in 65.96 sec: 0.283707 ( -0.04118 0.038446 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.28793e-06 ( -2.01076e-07 1.96163e-07 ) ergs/cm2
Band function
Time interval is from -29.016 sec. to 36.940 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] : 14.2861 (-2.28417 2.70416)
R^2/D10^2 : 3.54843E-02 (-0.016582 0.0317686)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 88.16 using 59 PHA bins.
# Reduced chi-squared = 1.547 for 57 degrees of freedom
# Null hypothesis probability = 5.074943e-03
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.007e-07 2.918e-08
25- 50 3.820e-07 7.826e-08
50-150 5.186e-07 1.413e-07
15-150 1.001e-06 1.870e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 141.775 (-59.8674 -138.522)
Norm : 1.16395 (-0.177092 0.254637)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 71.94 using 59 PHA bins.
# Reduced chi-squared = 1.262 for 57 degrees of freedom
# Null hypothesis probability = 8.784305e-02
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.981e-07 4.393e-08
25- 50 3.641e-07 1.711e-07
50-150 7.017e-07 4.205e-07
15-150 1.264e-06 6.765e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.18734 (-1.43407 2.07553)
R1^2/D10^2 : 1.03422 (-0.759392 3.05203)
kT2 [keV] : 21.2452 (-4.67616 8.81984)
R2^2/D10^2 : 7.04306E-03 (-0.00505245 0.00800693)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 69.95 using 59 PHA bins.
# Reduced chi-squared = 1.272 for 55 degrees of freedom
# Null hypothesis probability = 8.439479e-02
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.312e-07 1.229e-07
25- 50 3.411e-07 1.515e-07
50-150 6.938e-07 3.982e-07
15-150 1.266e-06 6.160e-07
Peak spectrum fit
Power-law model
Time interval is from 32.184 sec. to 33.184 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.94931 ( -0.605855 0.681477 )
Norm@50keV : 6.74221E-03 ( -0.00255052 0.00234089 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 50.38 using 59 PHA bins.
# Reduced chi-squared = 0.8838 for 57 degrees of freedom
# Null hypothesis probability = 7.199909e-01
Photon flux (15-150 keV) in 1 sec: 0.988544 ( -0.309954 0.312156 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.20555e-08 ( -2.11379e-08 2.19176e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 32.184 sec. to 33.184 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.94072 ( -1.88835 1.66945 )
Epeak [keV] : 350.793 ( )
Norm@50keV : 6.81968E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 50.38 using 59 PHA bins.
# Reduced chi-squared = 0.8997 for 56 degrees of freedom
# Null hypothesis probability = 6.865754e-01
Photon flux (15-150 keV) in 1 sec: 0.969311 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 6.28507e-08 ( -5.96119e-08 1.83594e-08 ) ergs/cm2
Band function
Time interval is from 32.184 sec. to 33.184 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] : 11.2233 (-5.91827 9.31477)
R^2/D10^2 : 0.272164 (-0.257472 4.98075)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 56.13 using 59 PHA bins.
# Reduced chi-squared = 0.9848 for 57 degrees of freedom
# Null hypothesis probability = 5.075264e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.190e-09 4.640e-09
25- 50 2.086e-08 1.280e-08
50-150 1.507e-08 1.065e-08
15-150 4.311e-08 2.693e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 87.0418 (-87.0555 -87.0555)
Norm : 4.39582 (-1.71408 3.69903)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 51.05 using 59 PHA bins.
# Reduced chi-squared = 0.8955 for 57 degrees of freedom
# Null hypothesis probability = 6.968222e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.146e-08 7.295e-09
25- 50 1.923e-08 1.177e-08
50-150 2.868e-08 2.332e-08
15-150 5.937e-08 4.102e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.00579 (-2.05115 3.26286)
R1^2/D10^2 : 5.58608 (-4.91181 62.2054)
kT2 [keV] : 24.8614 (-11.61 -24.8567)
R2^2/D10^2 : 1.19679E-02 (-0.0115285 0.106063)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 49.22 using 59 PHA bins.
# Reduced chi-squared = 0.8950 for 55 degrees of freedom
# Null hypothesis probability = 6.939525e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.494e-08 9.340e-09
25- 50 1.623e-08 8.150e-09
50-150 3.381e-08 2.192e-08
15-150 6.497e-08 3.417e-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: 1.68076 ( -0.221831 0.225512 )
Norm@50keV : 2.42757E-03 ( -0.000314791 0.000312509 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 66.84 using 59 PHA bins.
# Reduced chi-squared = 1.173 for 57 degrees of freedom
# Null hypothesis probability = 1.748710e-01
Photon flux (15-150 keV) in 53.24 sec: 0.320272 ( -0.0421643 0.0424172 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.19856e-06 ( -1.61364e-07 1.62898e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.02299 ( -1.0837 0.875687 )
Epeak [keV] : 74.6905 ( -22.1184 -74.6904 )
Norm@50keV : 5.16034E-03 ( -0.00293084 0.011839 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 65.25 using 59 PHA bins.
# Reduced chi-squared = 1.165 for 56 degrees of freedom
# Null hypothesis probability = 1.860027e-01
Photon flux (15-150 keV) in 53.24 sec: 0.308447 ( -0.04518 0.045225 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.14506e-06 ( -1.75122e-07 1.78152e-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) = 3.56e-07
S(50-100 keV) = 4.32e-07
T90 vs. Hardness ratio plot
T90 = 56.9839998483658 sec.
Hardness ratio (energy fluence ratio) = 1.21348
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.1624
Count Ratio (50-100 keV) / (15-25 keV) = 0.882101
Mask shadow pattern
IMX = 7.602424147215958E-01, IMY = 3.637123024316146E-01
TIME vs. PHA plot around the trigger time
TIME vs. DetID plot around the trigger time
100 us light curve (15-350 keV)
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:
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-16.299400 36.940000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
244.9754 -15.6418 0.3 13.8 -87.3 4.3709 35.0 0.3 Sco X-1
254.3446 35.3516 1393.0 54.7 -14.5 0.0030 0.0 5.6 Her X-1
256.0151 -37.8110 2.3 18.8 177.5 0.6217 5.2 2.4 4U 1700-377
256.2243 -36.5429 0.0 17.6 177.5 0.2658 2.1 12.5 GX 349+2
263.1946 -24.6284 11.8 6.7 135.4 0.1154 1.0 12.3 GX 1+4
264.5437 -44.4747 7.0 25.7 161.0 0.2372 1.7 8.7 4U 1735-44
268.4845 -1.5218 6.7 19.9 19.0 -0.2020 -1.7 8.1 SW J1753.5-0127
270.3208 -25.1110 2.8 12.1 111.8 0.5202 4.1 2.8 GX 5-1
270.3173 -25.8919 4.2 12.4 115.0 0.3541 2.7 9.0 GRS 1758-258
274.0601 -14.0918 8.1 15.3 63.1 0.1804 1.4 4.6 GX 17+2
275.7613 -30.2671 18.7 18.8 119.6 0.0880 0.6 10.4 H1820-303
285.1554 -24.7973 62.6 24.9 98.0 0.0321 0.2 9.8 HT1900.1-2455
288.8379 10.8842 127.3 42.0 37.0 0.0264 0.1 4.4 GRS 1915+105
263.0994 -33.9026 5.6 15.2 157.0 0.2443 2.1 6.8 GX 354-0
292.1084 -64.1034 2.4 50.2 152.0 2.4310 4.8 ------ UNKNOWN
248.3249 19.5781 1.0 40.1 -25.6 2.0240 11.3 ------ UNKNOWN
241.6229 26.0463 2.1 48.2 -30.9 1.6227 5.4 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
179.100600 963.088300
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
244.9897 -15.6371 0.2 35.4 -140.2 53.7091 46.8 0.6 Sco X-1
254.3610 35.4516 3.7 16.8 51.7 2.6197 3.1 8.1 Her X-1
256.3854 -36.3199 47.2 56.4 -153.5 -0.9692 -0.2 6.6 GX 349+2
263.0069 -24.7461 99.1 46.6 -164.2 0.1941 0.1 0.1 GX 1+4
268.3862 -1.4433 12.3 28.8 168.9 0.9461 0.9 1.2 SW J1753.5-0127
270.3366 -24.9817 5.9 49.4 -172.3 3.7497 2.0 6.5 GX 5-1
270.4286 -25.7392 8.2 50.2 -171.9 2.8961 1.4 6.8 GRS 1758-258
274.0061 -14.2173 11.7 42.2 175.6 1.6382 1.0 10.9 GX 17+2
275.9196 -30.3699 1210.4 56.6 -174.3 -0.0336 -0.0 0.3 H1820-303
288.8420 11.0147 4.2 39.9 130.5 5.8880 2.7 4.9 GRS 1915+105
263.0158 -33.7822 4.7 55.2 -160.6 7.3314 2.4 3.4 GX 354-0
285.9008 26.9382 5.0 35.2 105.0 4.4236 2.3 ------ UNKNOWN
282.7712 30.1914 3.0 32.9 98.6 6.0851 3.9 ------ UNKNOWN
275.9674 27.7110 3.8 26.6 101.2 3.8724 3.1 ------ UNKNOWN
190.8864 58.9659 3.3 56.7 3.0 13.4386 3.4 ------ UNKNOWN
Plot creation:
Mon Dec 17 21:14:43 EST 2018