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
32.6044 69.9653 0.0095 57.6762 -18.1255 8.3681991 20.317 TRIG_00846088
Foreground time interval of the image:
-17.896 4.236 (delta_t = 22.132 [sec])
Background time interval of the image:
-239.064 -17.896 (delta_t = 221.168 [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 -17.896 sec. to 4.236 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.22440 ( -0.101665 0.100306 )
Norm@50keV : 2.75889E-02 ( -0.00166649 0.0016605 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 76.37 using 59 PHA bins.
# Reduced chi-squared = 1.340 for 57 degrees of freedom
# Null hypothesis probability = 4.431561e-02
Photon flux (15-150 keV) in 22.13 sec: 3.24996 ( -0.21322 0.21421 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.15307e-06 ( -3.6703e-07 3.67438e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -17.896 sec. to 4.236 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.868278 ( -0.459336 0.390702 )
Epeak [keV] : 194.054 ( -75.8682 -194.054 )
Norm@50keV : 3.89801E-02 ( -0.0120026 0.0208127 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 74.26 using 59 PHA bins.
# Reduced chi-squared = 1.326 for 56 degrees of freedom
# Null hypothesis probability = 5.166416e-02
Photon flux (15-150 keV) in 22.13 sec: 3.19388 ( -0.22201 0.22327 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.11226e-06 ( -3.73986e-07 3.73059e-07 ) ergs/cm2
Band function
Time interval is from -17.896 sec. to 4.236 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] : 21.3181 ( )
R^2/D10^2 : 0.122660 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 118.19 using 59 PHA bins.
# Reduced chi-squared = 2.0735 for 57 degrees of freedom
# Null hypothesis probability = 3.593947e-06
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.315e-07 3.034e-08
25- 50 1.201e-06 1.024e-07
50-150 4.074e-06 3.331e-07
15-150 5.507e-06 4.127e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-9.38164 -200)
Norm : 14.1241 (-0.843424 0.843424)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 110.79 using 59 PHA bins.
# Reduced chi-squared = 1.9436 for 57 degrees of freedom
# Null hypothesis probability = 2.594498e-05
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.787e-07 5.765e-08
25- 50 1.498e-06 1.095e-07
50-150 3.285e-06 2.512e-07
15-150 5.561e-06 4.802e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.86324 (-1.86684 3.48736)
R1^2/D10^2 : 2.63492 (-1.9119 6.29464)
kT2 [keV] : 28.1646 (-3.75239 9.14022)
R2^2/D10^2 : 4.25686E-02 (-0.0272931 0.0289525)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 77.14 using 59 PHA bins.
# Reduced chi-squared = 1.403 for 55 degrees of freedom
# Null hypothesis probability = 2.607160e-02
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.536e-07 2.096e-07
25- 50 1.299e-06 2.899e-07
50-150 4.264e-06 7.104e-07
15-150 6.116e-06 1.088e-06
Peak spectrum fit
Power-law model
Time interval is from 0.044 sec. to 1.044 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.10804 ( -0.182672 0.181505 )
Norm@50keV : 8.24408E-02 ( -0.00970206 0.00967261 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 68.97 using 59 PHA bins.
# Reduced chi-squared = 1.210 for 57 degrees of freedom
# Null hypothesis probability = 1.329337e-01
Photon flux (15-150 keV) in 1 sec: 3.36155E-02 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 8.59825e-07 ( -1.04089e-07 1.04248e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.044 sec. to 1.044 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -0.379232 ( -1.20003 0.935097 )
Epeak [keV] : 100.552 ( -19.7677 63.6515 )
Norm@50keV : 0.331316 ( -0.189886 0.612183 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 60.76 using 59 PHA bins.
# Reduced chi-squared = 1.085 for 56 degrees of freedom
# Null hypothesis probability = 3.083305e-01
Photon flux (15-150 keV) in 1 sec: 9.13872 ( -1.18103 1.19118 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.1749e-08 ( 0 0 ) ergs/cm2
Band function
Time interval is from 0.044 sec. to 1.044 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] : 22.0980 (-2.51093 2.95741)
R^2/D10^2 : 0.358683 (-0.121562 0.172837)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 62.62 using 59 PHA bins.
# Reduced chi-squared = 1.099 for 57 degrees of freedom
# Null hypothesis probability = 2.837350e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.235e-08 7.460e-09
25- 50 1.715e-07 3.050e-08
50-150 6.258e-07 1.115e-07
15-150 8.296e-07 1.359e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-24.8211 -200)
Norm : 40.1450 (-4.82556 4.82556)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 84.00 using 59 PHA bins.
# Reduced chi-squared = 1.474 for 57 degrees of freedom
# Null hypothesis probability = 1.149300e-02
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 9.993e-08 5.575e-08
25- 50 1.922e-07 1.062e-07
50-150 4.216e-07 2.340e-07
15-150 7.138e-07 3.935e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 3.70857 (-3.70737 10.1979)
R1^2/D10^2 : 56.1416 (-55.7275 -56.1891)
kT2 [keV] : 23.5914 (-3.05452 5.80454)
R2^2/D10^2 : 0.279393 (-0.176026 0.102227)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 58.70 using 59 PHA bins.
# Reduced chi-squared = 1.067 for 55 degrees of freedom
# Null hypothesis probability = 3.413675e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.280e-08 2.649e-08
25- 50 1.633e-07 3.710e-08
50-150 6.359e-07 1.346e-07
15-150 8.619e-07 1.618e-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: 1.22440 ( -0.101665 0.100306 )
Norm@50keV : 2.75889E-02 ( -0.00166649 0.0016605 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 76.37 using 59 PHA bins.
# Reduced chi-squared = 1.340 for 57 degrees of freedom
# Null hypothesis probability = 4.431561e-02
Photon flux (15-150 keV) in 22.13 sec: 3.24994 ( -0.213202 0.214194 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.15238e-06 ( -3.67281e-07 3.6748e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.868278 ( -0.459336 0.390702 )
Epeak [keV] : 194.054 ( -75.8683 -194.054 )
Norm@50keV : 3.89801E-02 ( -0.0120026 0.0208127 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 74.26 using 59 PHA bins.
# Reduced chi-squared = 1.326 for 56 degrees of freedom
# Null hypothesis probability = 5.166416e-02
Photon flux (15-150 keV) in 22.13 sec: 3.19367 ( -0.22195 0.2232 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.11494e-06 ( -3.74506e-07 3.73289e-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) = 1.31e-06
S(50-100 keV) = 2.24e-06
T90 vs. Hardness ratio plot
T90 = 19.6560000181198 sec.
Hardness ratio (energy fluence ratio) = 1.70992
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.88611
Count Ratio (50-100 keV) / (15-25 keV) = 2.29164
Mask shadow pattern
IMX = 1.501965875803406E+00, IMY = 4.916569183025535E-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:
-239.064000 -17.896000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
306.1083 74.7457 3.9 56.1 10.8 3.4748 3.0 ------ UNKNOWN
144.8029 80.7874 2.5 34.5 -4.8 1.0748 4.6 ------ UNKNOWN
102.7298 57.4891 2.1 36.8 -50.6 1.8265 5.4 ------ UNKNOWN
104.9119 39.9630 3.1 41.3 -77.8 3.8740 3.8 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-17.896000 4.236000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
229.3719 52.6456 2.3 42.2 56.4 1.1188 5.1 ------ UNKNOWN
209.2385 64.2171 2.4 30.8 38.5 0.3887 4.8 ------ UNKNOWN
164.2540 70.9584 2.3 24.2 1.7 0.3174 5.1 ------ UNKNOWN
32.6044 69.9653 0.6 57.7 -18.1 8.3681 20.3 ------ UNKNOWN
140.0597 6.0459 2.5 45.0 -147.8 0.5352 4.5 ------ UNKNOWN
111.5284 49.0135 3.0 33.5 -67.0 0.4016 3.8 ------ UNKNOWN
139.5487 -3.4382 2.4 54.0 -151.5 1.0663 4.7 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
581.236600 963.052300
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
244.9650 -15.6393 0.6 37.9 126.6 24.4954 18.3 0.8 Sco X-1
254.4794 35.3897 29.5 16.0 -19.2 -0.1512 -0.4 3.0 Her X-1
268.2910 -1.5672 8.8 33.6 80.1 -1.5107 -1.3 8.3 SW J1753.5-0127
288.8011 10.9521 6.1 44.2 45.4 2.7418 1.9 0.4 GRS 1915+105
299.5627 35.2195 10.4 49.8 10.1 1.1965 1.1 1.7 Cyg X-1
308.2775 40.9292 5.1 56.5 2.9 4.2591 2.3 7.7 Cyg X-3
275.0992 7.1849 0.4 33.6 60.0 26.1279 31.1 ------ UNKNOWN
253.5982 58.3089 3.2 36.7 -43.4 2.3134 3.6 ------ UNKNOWN
Plot creation:
Mon Aug 6 22:36:52 EDT 2018