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
64.7279 13.3505 0.0133 50.5685 15.9005 5.0384774 14.562 TRIG_01125809
Foreground time interval of the image:
-3.416 15.421 (delta_t = 18.837 [sec])
Background time interval of the image:
-68.379 -3.416 (delta_t = 64.963 [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 -3.416 sec. to 224.200 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.48018 ( -0.12138 0.121448 )
Norm@50keV : 2.69768E-03 ( -0.000192386 0.00019209 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 54.18 using 59 bins.
Reduced chi-squared = 0.950526
# Null hypothesis probability of 5.82e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 227.6 sec: 0.335021 ( -0.024981 0.025039 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.8447e-06 ( -4.45092e-07 4.47061e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -3.416 sec. to 224.200 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.17107 ( -0.527404 0.368061 )
Epeak [keV] : 139.202 ( -58.1872 -139.205 )
Norm@50keV : 3.83306E-03 ( -0.00126577 0.00304799 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 52.95 using 59 bins.
Reduced chi-squared = 0.945536
# Null hypothesis probability of 5.91e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 227.6 sec: 0.330833 ( -0.025795 0.025823 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.74107e-06 ( -4.80509e-07 4.76089e-07 ) ergs/cm2
Band function
Time interval is from -3.416 sec. to 224.200 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] : 15.3792 (-1.34843 1.51948)
R^2/D10^2 : 3.50950E-02 (-0.00999515 0.0136042)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 94.78 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.24e-03 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.938e-07 5.303e-08
25- 50 1.601e-06 1.537e-07
50-150 2.605e-06 3.368e-07
15-150 4.599e-06 4.120e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-37.5192 -200)
Norm : 1.37863 (-0.0980205 0.0980205)
------------------------------------------------------------
#Fit statistic : Chi-Squared 54.21 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.80e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.848e-07 6.771e-08
25- 50 1.510e-06 1.312e-07
50-150 3.311e-06 9.822e-07
15-150 5.606e-06 9.480e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 9.40481 (-1.80678 1.88991)
R1^2/D10^2 : 0.145177 (-0.0616789 0.131602)
kT2 [keV] : 40.1394 (-12.9901 53.3505)
R2^2/D10^2 : 9.58899E-04 (-0.000838451 0.00261329)
------------------------------------------------------------
#Fit statistic : Chi-Squared 50.08 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.63e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.264e-07 1.466e-07
25- 50 1.630e-06 3.729e-07
50-150 3.542e-06 1.500e-06
15-150 5.799e-06 1.817e-06
Peak spectrum fit
Power-law model
Time interval is from -0.484 sec. to 0.516 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.28990 ( -0.261477 0.257337 )
Norm@50keV : 5.05418E-02 ( -0.00788832 0.00787258 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 73.83 using 59 bins.
Reduced chi-squared = 1.29526
# Null hypothesis probability of 6.63e-02 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 6.01876 ( -0.9924 0.99734 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.00749e-07 ( -8.21193e-08 8.23603e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.484 sec. to 0.516 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.836460 ( -1.32504 0.589216 )
Epeak [keV] : 143.030 ( -143.064 -143.064 )
Norm@50keV : 8.22138E-02 ( -0.038411 0.24284 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 73.34 using 59 bins.
Reduced chi-squared = 1.30964
# Null hypothesis probability of 5.99e-02 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 5.93543 ( -1.01063 1.01645 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.93696e-07 ( -8.64095e-08 8.47729e-08 ) ergs/cm2
Band function
Time interval is from -0.484 sec. to 0.516 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] : 18.1621 (-3.21675 4.0876)
R^2/D10^2 : 0.385255 (-0.193629 0.364785)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 80.18 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.32e-02 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.537e-08 8.415e-09
25- 50 1.181e-07 3.093e-08
50-150 2.835e-07 6.935e-08
15-150 4.269e-07 9.285e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-55.4227 -200)
Norm : 25.4630 (-4.01161 4.01161)
------------------------------------------------------------
#Fit statistic : Chi-Squared 76.65 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.23e-02 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.341e-08 3.691e-08
25- 50 1.220e-07 6.785e-08
50-150 2.675e-07 1.499e-07
15-150 4.529e-07 2.598e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 11.8055 (-5.0281 4.96728)
R1^2/D10^2 : 1.26047 (-0.781337 1.05708)
kT2 [keV] : 65.6927 (-60.4482 -67.2925)
R2^2/D10^2 : 5.09572E-03 (-0.00376921 0.137533)
------------------------------------------------------------
#Fit statistic : Chi-Squared 72.17 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.01e-02 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.065e-08 2.446e-08
25- 50 1.248e-07 7.280e-08
50-150 3.082e-07 1.662e-07
15-150 4.737e-07 2.470e-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: 1.32051 ( -0.12786 0.126544 )
Norm@50keV : 1.99897E-02 ( -0.00151112 0.00151016 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 48.15 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.92e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 18.84 sec: 2.39407 ( -0.193541 0.19411 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.70328e-06 ( -2.93678e-07 2.94217e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.06002 ( -0.539531 0.325342 )
Epeak [keV] : 199.498 ( -199.512 -199.512 )
Norm@50keV : 2.64904E-02 ( -0.00765859 0.0201807 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 47.33 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.89e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 18.84 sec: 2.37226 ( -0.1973 0.19798 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.66966e-06 ( -3.06037e-07 3.03343e-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) = 1.43e-06
S(50-100 keV) = 2.05e-06
T90 vs. Hardness ratio plot
T90 = 182.095999956131 sec.
Hardness ratio (energy fluence ratio) = 1.43357
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.705
Count Ratio (50-100 keV) / (15-25 keV) = 1.30828
Mask shadow pattern
IMX = 1.169526350298008E+00, IMY = -3.331601940831920E-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:
-68.379400 -3.416000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
326.1675 38.3219 56.1 39.2 -145.5 0.0418 0.2 0.2 Cyg X-2
16.3491 -4.9384 2.6 34.6 92.5 1.3949 4.4 ------ UNKNOWN
43.5715 39.7558 2.4 27.2 -21.5 0.6487 4.8 ------ UNKNOWN
338.1355 47.3097 3.4 32.0 -127.7 0.6256 3.4 ------ UNKNOWN
308.8763 41.6273 2.0 52.1 -139.3 3.5199 5.7 ------ UNKNOWN
57.4781 66.3005 2.2 45.6 -57.8 3.1464 5.1 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-3.416000 15.420600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
326.1782 38.3260 65.8 39.2 -145.5 0.0180 0.2 0.4 Cyg X-2
340.3496 -9.0510 2.3 49.6 142.9 1.5723 5.0 ------ UNKNOWN
64.7279 13.3506 0.8 50.6 15.9 5.0373 14.6 ------ UNKNOWN
319.9749 22.8146 2.6 47.4 -166.3 0.5719 4.5 ------ UNKNOWN
313.0898 26.8842 2.6 52.0 -158.6 0.8428 4.4 ------ UNKNOWN
346.7231 67.4966 3.1 41.0 -95.9 1.0655 3.7 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
156.820600 717.858300
720.920000 963.110800
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6218 22.0320 0.5 20.0 -113.2 31.3247 23.4 1.2 Crab
104.8092 -8.8654 2.8 45.6 -57.8 25.3233 4.1 ------ UNKNOWN
Plot creation:
Wed Jun 14 13:59:53 EDT 2023