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
65.5427 2.1955 0.0130 23.1849 34.3301 1.4600142 14.794 TRIG_00883600
Foreground time interval of the image:
126.400 185.101 (delta_t = 58.701 [sec])
Background time interval of the image:
-239.000 126.400 (delta_t = 365.400 [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
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 126.400 sec. to 199.580 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.05550 ( -0.210763 0.225798 )
Norm@50keV : 1.18608E-03 ( -0.000185557 0.000181408 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 48.29 using 59 PHA bins.
# Reduced chi-squared = 0.8472 for 57 degrees of freedom
# Null hypothesis probability = 7.875519e-01
Photon flux (15-150 keV) in 73.18 sec: 0.182622 ( -0.020737 0.020738 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.03472e-07 ( -1.13785e-07 1.1713e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from 126.400 sec. to 199.580 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.38802 ( -0.963758 0.722075 )
Epeak [keV] : 36.5311 ( -30.0131 -36.5311 )
Norm@50keV : 2.97046E-03 ( -0.00297044 0.00832533 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 46.23 using 59 PHA bins.
# Reduced chi-squared = 0.8255 for 56 degrees of freedom
# Null hypothesis probability = 8.209707e-01
Photon flux (15-150 keV) in 73.18 sec: 0.178868 ( -0.021039 0.021116 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.49173e-07 ( -1.20967e-07 1.3103e-07 ) ergs/cm2
Band function
Time interval is from 126.400 sec. to 199.580 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] : 9.18172 (-1.3373 1.5625)
R^2/D10^2 : 0.116913 (-0.0526449 0.0980127)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 63.06 using 59 PHA bins.
# Reduced chi-squared = 1.106 for 57 degrees of freedom
# Null hypothesis probability = 2.707423e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.418e-07 2.715e-08
25- 50 3.110e-07 4.749e-08
50-150 1.261e-07 4.076e-08
15-150 5.789e-07 1.001e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 58.1761 (-16.7879 27.7269)
Norm : 0.974618 (-0.173538 0.211412)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 46.25 using 59 PHA bins.
# Reduced chi-squared = 0.8114 for 57 degrees of freedom
# Null hypothesis probability = 8.448159e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.783e-07 2.671e-08
25- 50 2.688e-07 3.304e-08
50-150 2.980e-07 1.032e-07
15-150 7.452e-07 1.131e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 4.85274 (-1.1728 1.41718)
R1^2/D10^2 : 0.961150 (-0.596875 1.73131)
kT2 [keV] : 16.4401 (-3.78983 6.24325)
R2^2/D10^2 : 9.13591E-03 (-0.00662102 0.017648)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 43.44 using 59 PHA bins.
# Reduced chi-squared = 0.7897 for 55 degrees of freedom
# Null hypothesis probability = 8.699628e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.887e-07 1.019e-07
25- 50 2.517e-07 1.220e-07
50-150 3.082e-07 1.841e-07
15-150 7.486e-07 3.750e-07
Peak spectrum fit
Power-law model
Time interval is from 151.076 sec. to 152.076 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.50802 ( -0.647681 0.671833 )
Norm@50keV : 4.34450E-03 ( -0.00155799 0.00146642 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 39.61 using 59 PHA bins.
# Reduced chi-squared = 0.6950 for 57 degrees of freedom
# Null hypothesis probability = 9.614146e-01
Photon flux (15-150 keV) in 1 sec: 0.543557 ( -0.179698 0.179947 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.11652e-08 ( -1.55227e-08 1.59353e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 151.076 sec. to 152.076 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.20719 ( -0.677248 0.651457 )
Epeak [keV] : 76.3959 ( -9999.36 -9999.36 )
Norm@50keV : 1.85165E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 39.17 using 59 PHA bins.
# Reduced chi-squared = 0.6994 for 56 degrees of freedom
# Null hypothesis probability = 9.573356e-01
Photon flux (15-150 keV) in 1 sec: 0.545585 ( -0.184032 0.179953 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.30877e-08 ( -1.82104e-08 1.21218e-08 ) ergs/cm2
Band function
Time interval is from 151.076 sec. to 152.076 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] : 12.2448 (-5.81166 21.071)
R^2/D10^2 : 0.115653 (-0.110707 1.07228)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 45.34 using 59 PHA bins.
# Reduced chi-squared = 0.7955 for 57 degrees of freedom
# Null hypothesis probability = 8.671657e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.673e-09 2.425e-09
25- 50 1.183e-08 7.355e-09
50-150 1.081e-08 7.745e-09
15-150 2.632e-08 1.661e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.355 (-199.363 -199.363)
Norm : 2.20603 (-0.724037 0.724834)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 40.11 using 59 PHA bins.
# Reduced chi-squared = 0.7037 for 57 degrees of freedom
# Null hypothesis probability = 9.561755e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.493e-09 3.338e-09
25- 50 1.057e-08 6.705e-09
50-150 2.318e-08 1.403e-08
15-150 3.924e-08 2.395e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.37522 (-3.23126 5.798)
R1^2/D10^2 : 1.04449 (-0.94556 20.5406)
kT2 [keV] : 49.0754 (-45.9167 -49.0608)
R2^2/D10^2 : 1.23448E-03 (-0.00111795 0.0241905)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 38.62 using 59 PHA bins.
# Reduced chi-squared = 0.7022 for 55 degrees of freedom
# Null hypothesis probability = 9.540431e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.453e-09 3.923e-09
25- 50 9.318e-09 5.950e-09
50-150 2.924e-08 1.759e-08
15-150 4.501e-08 2.648e-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: 2.00873 ( -0.215293 0.230258 )
Norm@50keV : 1.31885E-03 ( -0.000207873 0.000202817 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 45.61 using 59 PHA bins.
# Reduced chi-squared = 0.8001 for 57 degrees of freedom
# Null hypothesis probability = 8.608726e-01
Photon flux (15-150 keV) in 58.7 sec: 0.198626 ( -0.0232653 0.0232653 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.14267e-07 ( -1.03854e-07 1.06917e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.38046 ( -0.985726 0.807268 )
Epeak [keV] : 40.1120 ( -32.4259 -40.112 )
Norm@50keV : 3.09588E-03 ( -0.00309588 0.00871675 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 43.88 using 59 PHA bins.
# Reduced chi-squared = 0.7835 for 56 degrees of freedom
# Null hypothesis probability = 8.802578e-01
Photon flux (15-150 keV) in 58.7 sec: 0.194676 ( -0.023661 0.023728 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.69867e-07 ( -1.10912e-07 1.19672e-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) = 2.46e-07
S(50-100 keV) = 2.36e-07
T90 vs. Hardness ratio plot
T90 = 67.095999956131 sec.
Hardness ratio (energy fluence ratio) = 0.95935
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 0.869759
Count Ratio (50-100 keV) / (15-25 keV) = 0.501162
Mask shadow pattern
IMX = 3.536813571934281E-01, IMY = -2.415373204495026E-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:
-239.000000 126.400000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
133.0720 -43.2197 3.0 56.8 173.8 6.6132 3.8 ------ UNKNOWN
27.8846 1.1571 3.9 46.4 -22.2 1.7659 3.0 ------ UNKNOWN
30.0919 -45.5934 4.2 40.9 -92.1 4.0189 2.8 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
126.400000 185.100590
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
65.5428 2.1955 0.8 23.2 34.3 1.4600 14.8 ------ UNKNOWN
118.6291 -41.6408 2.5 46.1 173.5 1.0018 4.6 ------ UNKNOWN
34.3262 -11.8391 2.4 35.0 -36.1 0.6544 4.9 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
235.500600 963.123700
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6329 22.0204 0.3 26.5 65.9 30.7920 35.9 0.4 Crab
82.0057 -37.6819 3.2 42.7 -173.6 4.5376 3.6 ------ UNKNOWN
28.1613 -1.1086 4.2 37.5 -68.9 5.0106 2.7 ------ UNKNOWN
62.1261 -54.4953 3.2 56.7 -151.9 15.4541 3.6 ------ UNKNOWN
Plot creation:
Thu Mar 21 14:27:49 EDT 2019