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
96.7213 30.2983 0.0271 26.1626 -73.5963 2.0876672 7.066 TRIG_01243868
Foreground time interval of the image:
-0.116 193.892 (delta_t = 194.008 [sec])
Background time interval of the image:
-239.120 -0.116 (delta_t = 239.004 [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 -0.116 sec. to 193.892 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.48959 ( -0.213604 0.216105 )
Norm@50keV : 9.74235E-04 ( -0.000116863 0.000116016 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 52.75 using 59 bins.
Reduced chi-squared = 0.925439
# Null hypothesis probability of 6.35e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 194 sec: 0.121288 ( -0.014493 0.014534 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.79627e-06 ( -2.36426e-07 2.38998e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.116 sec. to 193.892 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.48700 ( -0.705327 1.61558 )
Epeak [keV] : 1.00000E+04 ( -10000 -10000 )
Norm@50keV : 9.77208E-04 ( -0.000117573 0.0001135 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 52.76 using 59 bins.
Reduced chi-squared = 0.942143
# Null hypothesis probability of 5.98e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 194 sec: 0.121913 ( -0.017444 0.016209 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.80058e-06 ( -2.55246e-07 2.40182e-07 ) ergs/cm2
Band function
Time interval is from -0.116 sec. to 193.892 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] : 15.9840 (-2.56801 3.10436)
R^2/D10^2 : 1.07600E-02 (-0.00492072 0.00906749)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 75.82 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.84e-02 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.103e-07 2.637e-08
25- 50 4.637e-07 8.187e-08
50-150 8.278e-07 1.938e-07
15-150 1.402e-06 2.513e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-69.5121 -200)
Norm : 0.495741 (-0.0577365 0.0577365)
------------------------------------------------------------
#Fit statistic : Chi-Squared 53.80 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.96e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.395e-07 1.354e-07
25- 50 4.608e-07 2.514e-07
50-150 1.010e-06 5.577e-07
15-150 1.711e-06 9.479e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.22670 (-2.15281 2.48805)
R1^2/D10^2 : 0.194247 (-0.134087 0.46829)
kT2 [keV] : 27.0796 (-6.94467 15.9079)
R2^2/D10^2 : 1.48439E-03 (-0.00114359 0.00167492)
------------------------------------------------------------
#Fit statistic : Chi-Squared 52.94 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.54e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.395e-07 1.268e-07
25- 50 4.278e-07 1.752e-07
50-150 1.132e-06 6.081e-07
15-150 1.799e-06 8.236e-07
Peak spectrum fit
Power-law model
Time interval is from 0.440 sec. to 1.440 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.942988 ( -0.18415 0.18019 )
Norm@50keV : 2.22031E-02 ( -0.00226355 0.00225733 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 42.08 using 59 bins.
Reduced chi-squared = 0.738246
# Null hypothesis probability of 9.30e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 2.55038 ( -0.26165 0.26205 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.45155e-07 ( -2.77047e-08 2.78811e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.440 sec. to 1.440 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.936757 ( -0.666441 0.289798 )
Epeak [keV] : 9996.30 ( -9995.79 -9995.79 )
Norm@50keV : 2.23449E-02 ( -0.00225083 0.025535 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 42.07 using 59 bins.
Reduced chi-squared = 0.75125
# Null hypothesis probability of 9.16e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 2.54688 ( -0.27273 0.26708 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.4481e-07 ( -2.92888e-08 2.75228e-08 ) ergs/cm2
Band function
Time interval is from 0.440 sec. to 1.440 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] : 23.2481 (-3.24708 4.02195)
R^2/D10^2 : 7.77927E-02 (-0.0296829 0.0456688)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 59.79 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.75e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.580e-09 1.748e-09
25- 50 4.137e-08 7.660e-09
50-150 1.669e-07 3.025e-08
15-150 2.159e-07 2.975e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-20.4054 -200)
Norm : 10.0561 (-1.07311 1.07311)
------------------------------------------------------------
#Fit statistic : Chi-Squared 71.73 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.06e-02 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.504e-08 1.390e-08
25- 50 4.817e-08 2.648e-08
50-150 1.056e-07 5.760e-08
15-150 1.789e-07 9.870e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 8.35828 (-3.59129 4.70244)
R1^2/D10^2 : 0.985267 (-0.696326 5.73738)
kT2 [keV] : 37.5832 (-10.6033 45.7408)
R2^2/D10^2 : 1.59737E-02 (-0.0123509 0.0195088)
------------------------------------------------------------
#Fit statistic : Chi-Squared 42.46 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.92e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.588e-08 8.538e-09
25- 50 4.457e-08 1.985e-08
50-150 1.872e-07 1.015e-07
15-150 2.476e-07 1.147e-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: 1.48959 ( -0.213604 0.216105 )
Norm@50keV : 9.74235E-04 ( -0.000116863 0.000116016 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 52.75 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.35e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 194 sec: 0.121285 ( -0.0144925 0.0145323 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.79605e-06 ( -2.36416e-07 2.39002e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.48700 ( -0.702631 1.6194 )
Epeak [keV] : 1.00000E+04 ( -10000 -10000 )
Norm@50keV : 9.77209E-04 ( -0.000117573 0.0001135 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 52.76 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.98e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 194 sec: 0.121251 ( -0.007398 0.014345 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.79645e-06 ( -2.45237e-07 2.36362e-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) = 4.42e-07
S(50-100 keV) = 6.31e-07
T90 vs. Hardness ratio plot
T90 = 183.475999951363 sec.
Hardness ratio (energy fluence ratio) = 1.4276
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.27724
Count Ratio (50-100 keV) / (15-25 keV) = 1.03124
Mask shadow pattern
IMX = 1.387310552712313E-01, IMY = 4.712554378230551E-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:
-239.120000 -0.116000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6226 22.0146 0.4 22.4 -39.4 9.8636 27.1 0.6 Crab
4.9384 46.7010 2.0 44.7 127.2 11.2072 5.8 ------ UNKNOWN
107.4801 37.9651 2.3 31.8 -95.0 2.8542 5.1 ------ UNKNOWN
116.2988 31.5204 2.4 40.8 -89.0 7.3680 4.7 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-0.116000 193.892000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.7919 22.0526 10.6 22.4 -39.8 -0.2556 -1.1 9.1 Crab
348.2227 60.9309 2.8 51.2 148.7 5.1242 4.1 ------ UNKNOWN
96.7213 30.2983 1.6 26.2 -73.6 2.0882 7.1 ------ UNKNOWN
101.0081 7.5046 2.3 44.1 -47.4 2.7090 5.0 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
-239.120000 963.015400
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6209 22.0172 0.4 22.4 -39.4 48.8470 30.9 0.7 Crab
4.9337 46.6900 2.2 44.7 127.2 48.2188 5.4 ------ UNKNOWN
33.3277 23.4512 3.7 32.1 77.3 10.8705 3.1 ------ UNKNOWN
31.4100 26.9747 2.9 31.6 84.7 13.3715 3.9 ------ UNKNOWN
48.7452 24.9014 2.9 20.6 58.4 7.1615 3.9 ------ UNKNOWN
97.7173 -8.0105 2.3 55.2 -32.3 48.4941 5.0 ------ UNKNOWN
116.2923 31.4980 2.1 40.8 -88.9 38.0165 5.5 ------ UNKNOWN
Plot creation:
Sat Oct 19 18:23:06 EDT 2024