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
1.3621 31.7583 0.0194 33.4785 -148.7279 2.8689191 9.877 TRIG_01091527
Foreground time interval of the image:
-58.076 15.429 (delta_t = 73.505 [sec])
Background time interval of the image:
-77.971 -58.076 (delta_t = 19.895 [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 -58.076 sec. to 259.104 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.26493 ( -0.0310811 0.0309777 )
Norm@50keV : 7.49179E-03 ( -0.000124648 0.000124408 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 42.09 using 59 bins.
Reduced chi-squared = 0.738421
# Null hypothesis probability of 9.30e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 317.2 sec: 0.888279 ( -0.016628 0.016677 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.36932e-05 ( -3.86867e-07 3.87212e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -58.076 sec. to 259.104 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.15911 ( -0.12707 0.0825308 )
Epeak [keV] : 483.172 ( -251.53 -483.209 )
Norm@50keV : 8.28414E-03 ( -0.000809783 0.001034 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 39.98 using 59 bins.
Reduced chi-squared = 0.713929
# Null hypothesis probability of 9.48e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 317.2 sec: 0.880734 ( -0.018617 0.018713 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.35718e-05 ( -4.12116e-07 4.11703e-07 ) ergs/cm2
Band function
Time interval is from -58.076 sec. to 259.104 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] : 20.8962 ( )
R^2/D10^2 : 3.36546E-02 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 718.89 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.82e-115 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.825e-07 3.061e-08
25- 50 4.522e-06 1.190e-07
50-150 1.471e-05 3.473e-07
15-150 2.012e-05 3.775e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.363 ( )
Norm : 3.86226 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared 365.32 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.51e-46 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.051e-06 5.535e-08
25- 50 5.868e-06 1.094e-07
50-150 1.287e-05 2.316e-07
15-150 2.179e-05 3.917e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 8.69722 (-0.615293 0.652512)
R1^2/D10^2 : 0.372300 (-0.0761232 0.101597)
kT2 [keV] : 34.3878 (-2.30425 2.85891)
R2^2/D10^2 : 5.47437E-03 (-0.00126158 0.00144077)
------------------------------------------------------------
#Fit statistic : Chi-Squared 51.72 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.01e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.001e-06 1.285e-07
25- 50 5.348e-06 1.713e-07
50-150 1.613e-05 5.789e-07
15-150 2.348e-05 6.550e-07
Peak spectrum fit
Power-law model
Time interval is from 89.072 sec. to 90.072 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.01129 ( -0.0700457 0.0696308 )
Norm@50keV : 5.78728E-02 ( -0.00234945 0.00234852 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 61.57 using 59 bins.
Reduced chi-squared = 1.08018
# Null hypothesis probability of 3.16e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.451564 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 6.2339e-07 ( -2.81803e-08 2.82534e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 89.072 sec. to 90.072 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.723284 ( -0.28937 0.256981 )
Epeak [keV] : 252.874 ( -98.1726 1939.59 )
Norm@50keV : 7.81066E-02 ( -0.017721 0.0264016 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 58.27 using 59 bins.
Reduced chi-squared = 1.04054
# Null hypothesis probability of 3.92e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 6.60039 ( -0.28159 0.28148 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.15375e-07 ( -2.96281e-08 2.94918e-08 ) ergs/cm2
Band function
Time interval is from 89.072 sec. to 90.072 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] : 21.5986 ( )
R^2/D10^2 : 0.254534 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 151.62 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.59e-10 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.216e-08 1.750e-09
25- 50 1.159e-07 6.700e-09
50-150 4.037e-07 2.895e-08
15-150 5.417e-07 2.720e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.363 ( )
Norm : 26.5810 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared 214.37 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.44e-20 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.619e-08 2.715e-09
25- 50 1.273e-07 5.750e-09
50-150 2.792e-07 1.525e-08
15-150 4.728e-07 2.120e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.95492 (-1.57443 2.06428)
R1^2/D10^2 : 2.90416 (-1.38069 2.95125)
kT2 [keV] : 32.2700 (-4.18256 7.52597)
R2^2/D10^2 : 6.25911E-02 (-0.0309904 0.036962)
------------------------------------------------------------
#Fit statistic : Chi-Squared 61.27 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.61e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.283e-08 7.760e-09
25- 50 1.192e-07 1.528e-08
50-150 4.552e-07 5.635e-08
15-150 6.172e-07 7.835e-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: 1.80279 ( -0.126539 0.129401 )
Norm@50keV : 2.69405E-03 ( -0.000221651 0.000219283 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 67.91 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.53e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 73.5 sec: 0.371637 ( -0.0272558 0.0272734 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.82275e-06 ( -1.52123e-07 1.53709e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.11448 ( -0.583281 0.509952 )
Epeak [keV] : 56.9653 ( -10.9479 38.6308 )
Norm@50keV : 6.48815E-03 ( -0.00304943 0.0070897 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 62.34 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.61e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 73.5 sec: 0.361683 ( -0.028167 0.028177 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.71023e-06 ( -1.69381e-07 1.73012e-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) = 5.17e-06
S(50-100 keV) = 8.60e-06
T90 vs. Hardness ratio plot
T90 = 161.888000011444 sec.
Hardness ratio (energy fluence ratio) = 1.66344
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.55518
Count Ratio (50-100 keV) / (15-25 keV) = 1.43107
Mask shadow pattern
IMX = -5.652594020079352E-01, IMY = 3.433067346143954E-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:
-77.971400 -58.076000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
326.1673 38.4735 5.7 40.5 -100.1 -0.4560 -2.0 9.1 Cyg X-2
74.9262 37.1519 2.4 41.4 102.8 1.1095 4.8 ------ UNKNOWN
177.6184 63.0993 2.1 52.8 13.5 1.0946 5.5 ------ UNKNOWN
61.7865 69.0604 3.2 17.4 52.3 0.2216 3.6 ------ UNKNOWN
182.7380 69.5401 2.9 47.0 9.1 0.4529 4.0 ------ UNKNOWN
352.8880 36.4851 2.1 31.4 -133.4 0.3986 5.6 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-58.076000 15.428600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
326.2370 38.3789 12.2 40.5 -100.3 0.8713 0.9 4.6 Cyg X-2
1.3621 31.7583 1.2 33.5 -148.7 2.8687 9.9 ------ UNKNOWN
358.0745 34.4678 2.1 31.7 -142.3 1.5142 5.5 ------ UNKNOWN
235.3905 57.6654 2.3 56.5 -20.8 5.1316 5.1 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
69.428590 240.428600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
299.4166 35.1663 9.8 51.0 -43.3 -2.3989 -1.2 8.8 Cyg X-1
308.2142 40.9555 5.4 43.1 -37.2 1.5807 2.1 4.7 Cyg X-3
325.9490 38.3346 9.7 29.6 -42.2 -0.5642 -1.2 10.5 Cyg X-2
1.3601 31.7760 0.1 0.0 -76.8 28.3873 89.1 ------ UNKNOWN
350.1429 -0.3540 2.7 33.9 -134.5 2.3129 4.3 591.8 UNKNOWN
Plot creation:
Mon Oct 24 05:10:25 EDT 2022