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
10.3246 8.5342 0.0194 33.5211 -145.2458 0.6807146 9.838 TRIG_01205708
Foreground time interval of the image:
-5.024 13.552 (delta_t = 18.576 [sec])
Background time interval of the image:
-239.984 -5.024 (delta_t = 234.960 [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 4.096000
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 4.096000
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 4.096000
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 -5.024 sec. to 13.552 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.10022 ( -0.256778 0.280556 )
Norm@50keV : 2.15387E-03 ( -0.000424825 0.000414255 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 53.76 using 59 bins.
Reduced chi-squared = 0.943158
# Null hypothesis probability of 5.97e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 18.58 sec: 0.338924 ( -0.04931 0.04931 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.71908e-07 ( -6.53271e-08 6.73557e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -5.024 sec. to 13.552 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.392967 ( -2.01188 1.41015 )
Epeak [keV] : 36.3138 ( -15.5492 11.1418 )
Norm@50keV : 2.31846E-02 ( -0.0237078 0.388397 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 49.19 using 59 bins.
Reduced chi-squared = 0.878393
# Null hypothesis probability of 7.28e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 18.58 sec: 0.324691 ( -0.049982 0.050276 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.23725e-07 ( -6.12573e-08 7.25675e-08 ) ergs/cm2
Band function
Time interval is from -5.024 sec. to 13.552 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] : 9.30278 (-1.2867 1.48288)
R^2/D10^2 : 0.217138 (-0.0955652 0.169935)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 51.80 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.70e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.908e-08 1.790e-08
25- 50 1.545e-07 3.405e-08
50-150 6.516e-08 2.398e-08
15-150 2.888e-07 5.425e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 52.4751 (-16.3871 29.4745)
Norm : 1.90380 (-0.408411 0.54945)
------------------------------------------------------------
#Fit statistic : Chi-Squared 50.26 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.24e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.741e-08 1.593e-08
25- 50 1.277e-07 2.270e-08
50-150 1.296e-07 5.825e-08
15-150 3.447e-07 7.674e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 3.69714 (-3.69701 -3.69701)
R1^2/D10^2 : 2.98433 (-2.98473 -2.98473)
kT2 [keV] : 10.8974 (-1.8812 188.75)
R2^2/D10^2 : 0.102094 (-0.102101 0.187551)
------------------------------------------------------------
#Fit statistic : Chi-Squared 49.21 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.95e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.096e-08 4.008e-08
25- 50 1.410e-07 7.811e-08
50-150 8.747e-08 5.437e-08
15-150 3.094e-07 1.577e-07
Peak spectrum fit
Power-law model
Time interval is from 2.100 sec. to 3.100 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.11461 ( -0.394339 0.458132 )
Norm@50keV : 5.96207E-03 ( -0.00189705 0.00183537 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 40.74 using 59 bins.
Reduced chi-squared = 0.714737
# Null hypothesis probability of 9.49e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.944888 ( -0.218372 0.218382 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.54843e-08 ( -1.54115e-08 1.62274e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 2.100 sec. to 3.100 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.491260 ( -2.74402 1.64062 )
Epeak [keV] : 37.2049 ( -37.2078 -37.2078 )
Norm@50keV : 5.49764E-02 ( -0.0549967 2.55923 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 38.29 using 59 bins.
Reduced chi-squared = 0.68375
# Null hypothesis probability of 9.66e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.918089 ( -0.216553 0.218011 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.00587e-08 ( -1.38269e-08 1.62942e-08 ) ergs/cm2
Band function
Time interval is from 2.100 sec. to 3.100 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] : 9.62491 (-2.12411 2.66647)
R^2/D10^2 : 0.537350 (-0.331074 0.863176)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 40.05 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.57e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 9.995e-09 4.449e-09
25- 50 2.352e-08 9.245e-09
50-150 1.098e-08 6.297e-09
15-150 4.449e-08 1.863e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 52.2615 (-22.5481 55.2204)
Norm : 5.35524 (-1.67789 2.55946)
------------------------------------------------------------
#Fit statistic : Chi-Squared 38.81 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.69e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.322e-08 5.300e-09
25- 50 1.929e-08 7.701e-09
50-150 1.951e-08 1.402e-08
15-150 5.202e-08 2.317e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 4.02788 (-4.02684 195.279)
R1^2/D10^2 : 7.47058 (-7.47841 -7.47841)
kT2 [keV] : 12.2726 (-3.86214 -12.2715)
R2^2/D10^2 : 0.172313 (-0.172387 0.664441)
------------------------------------------------------------
#Fit statistic : Chi-Squared 37.94 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.61e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.252e-08 6.410e-09
25- 50 2.035e-08 1.149e-08
50-150 1.636e-08 1.005e-08
15-150 4.923e-08 2.552e-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: 2.10022 ( -0.256778 0.280556 )
Norm@50keV : 2.15387E-03 ( -0.000424825 0.000414255 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 53.76 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.97e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 18.58 sec: 0.338895 ( -0.0493052 0.0493056 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.71849e-07 ( -6.52669e-08 6.73943e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.376707 ( -2.0054 1.41662 )
Epeak [keV] : 36.3181 ( -15.545 11.1409 )
Norm@50keV : 2.37336E-02 ( -0.0237431 0.388807 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 49.19 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.28e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 18.58 sec: 0.324634 ( -0.049962 0.050256 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.23803e-07 ( -6.13419e-08 7.25846e-08 ) 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) = 1.15e-07
S(50-100 keV) = 1.07e-07
T90 vs. Hardness ratio plot
T90 = 16.4160000085831 sec.
Hardness ratio (energy fluence ratio) = 0.930435
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.21759
Count Ratio (50-100 keV) / (15-25 keV) = 0.404033
Mask shadow pattern
IMX = -5.442445568205163E-01, IMY = 3.776147829377905E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 4.096000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 4.096000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 4.096000
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:
-239.984000 -5.024000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
309.2285 88.3690 2.4 50.6 4.1 3.1761 4.9 ------ UNKNOWN
30.6880 51.2084 2.7 12.6 20.3 1.4245 4.2 ------ UNKNOWN
21.6844 1.8683 2.0 37.4 -167.0 2.5904 5.8 ------ UNKNOWN
326.6360 41.2354 3.1 44.4 -61.2 5.2549 3.7 ------ UNKNOWN
354.3110 0.4382 2.3 48.2 -129.3 7.9109 4.9 342.3 UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-5.024000 13.552000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
17.7486 10.4032 2.0 29.5 -157.6 0.3182 5.7 ------ UNKNOWN
10.3246 8.5342 1.2 33.5 -145.2 0.6804 9.8 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
112.116600 962.040400
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
326.2573 38.4158 2.9 49.6 -22.6 -9.5056 -4.0 6.9 Cyg X-2
11.5637 -17.5508 2.9 26.1 -159.5 4.6536 4.0 ------ UNKNOWN
Plot creation:
Sat Mar 9 15:19:09 EST 2024