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
333.7056 83.5774 0.0047 39.3291 -31.5989 5.8252301 41.010 TRIG_01262165
Foreground time interval of the image:
-28.428 23.509 (delta_t = 51.937 [sec])
Background time interval of the image:
-239.992 -28.428 (delta_t = 211.564 [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 2.048000
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 2.048000
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 2.048000
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 -28.428 sec. to 132.908 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.36508 ( -0.0573832 0.0571837 )
Norm@50keV : 3.93244E-03 ( -0.00012515 0.000125125 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 53.98 using 59 bins.
Reduced chi-squared = 0.947018
# Null hypothesis probability of 5.89e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 161.3 sec: 0.475246 ( -0.016571 0.016618 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.17524e-06 ( -2.05378e-07 2.05548e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -28.428 sec. to 132.908 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.996533 ( -0.244649 0.231829 )
Epeak [keV] : 153.989 ( -39.5389 153.616 )
Norm@50keV : 5.75368E-03 ( -0.00119612 0.00159829 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 46.41 using 59 bins.
Reduced chi-squared = 0.82875
# Null hypothesis probability of 8.16e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 161.3 sec: 0.464475 ( -0.017755 0.01783 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.05793e-06 ( -2.20058e-07 2.19249e-07 ) ergs/cm2
Band function
Time interval is from -28.428 sec. to 132.908 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] : 18.5080 ( )
R^2/D10^2 : 2.66996E-02 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 212.73 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.19e-20 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.927e-07 1.863e-08
25- 50 1.382e-06 6.000e-08
50-150 3.458e-06 1.863e-07
15-150 5.133e-06 1.815e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-5.58704 -200)
Norm : 2.00587 (-0.0640327 0.0640327)
------------------------------------------------------------
#Fit statistic : Chi-Squared 85.85 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.05e-03 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.056e-07 2.879e-08
25- 50 1.550e-06 5.162e-08
50-150 3.399e-06 1.169e-07
15-150 5.754e-06 1.960e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.33046 (-1.00794 1.15308)
R1^2/D10^2 : 0.346500 (-0.130772 0.234372)
kT2 [keV] : 27.2445 (-2.53283 3.50961)
R2^2/D10^2 : 5.99175E-03 (-0.00213876 0.00260139)
------------------------------------------------------------
#Fit statistic : Chi-Squared 49.43 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.87e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.237e-07 8.517e-08
25- 50 1.458e-06 1.219e-07
50-150 3.950e-06 3.202e-07
15-150 6.032e-06 4.218e-07
Peak spectrum fit
Power-law model
Time interval is from 22.164 sec. to 23.164 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.24081 ( -0.20738 0.202513 )
Norm@50keV : 1.60327E-02 ( -0.00200176 0.00199595 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 57.47 using 59 bins.
Reduced chi-squared = 1.00825
# Null hypothesis probability of 4.58e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 1.89345 ( -0.24904 0.24995 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.60864e-07 ( -2.09923e-08 2.10432e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 22.164 sec. to 23.164 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.833911 ( -0.921428 0.510934 )
Epeak [keV] : 161.386 ( -161.406 -161.406 )
Norm@50keV : 2.47114E-02 ( -0.0104078 0.0380597 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 56.69 using 59 bins.
Reduced chi-squared = 1.01232
# Null hypothesis probability of 4.49e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 1.87049 ( -0.25344 0.25396 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.58921e-07 ( -2.17507e-08 2.15469e-08 ) ergs/cm2
Band function
Time interval is from 22.164 sec. to 23.164 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] : 19.4077 (-2.93883 3.60588)
R^2/D10^2 : 9.70698E-02 (-0.0424417 0.072226)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 68.63 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.39e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.131e-09 1.740e-09
25- 50 3.481e-08 8.015e-09
50-150 9.673e-08 2.097e-08
15-150 1.387e-07 2.480e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-36.4964 -200)
Norm : 8.02514 (-1.01289 1.01289)
------------------------------------------------------------
#Fit statistic : Chi-Squared 63.77 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.51e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.999e-08 1.114e-08
25- 50 3.845e-08 2.147e-08
50-150 8.433e-08 4.601e-08
15-150 1.428e-07 7.975e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 9.61238 (-5.00955 5.62219)
R1^2/D10^2 : 0.608597 (-0.423097 5.93899)
kT2 [keV] : 35.2003 (-13.5853 -35.4016)
R2^2/D10^2 : 1.03649E-02 (-0.00997141 0.0497433)
------------------------------------------------------------
#Fit statistic : Chi-Squared 57.05 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.99e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.310e-08 7.555e-09
25- 50 3.837e-08 2.071e-08
50-150 1.082e-07 5.755e-08
15-150 1.597e-07 8.120e-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: 1.08393 ( -0.065494 0.0646652 )
Norm@50keV : 7.39398E-03 ( -0.000282782 0.000281785 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 50.92 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.01e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 51.94 sec: 0.856369 ( -0.0345383 0.0346399 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.03609e-06 ( -1.50644e-07 1.50785e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.686050 ( -0.285013 0.266981 )
Epeak [keV] : 202.502 ( -58.957 263.226 )
Norm@50keV : 1.08091E-02 ( -0.00237735 0.00323855 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 44.27 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.71e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 51.94 sec: 0.838763 ( -0.03626 0.036436 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.99075e-06 ( -1.55898e-07 1.55212e-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) = 1.42e-06
S(50-100 keV) = 2.21e-06
T90 vs. Hardness ratio plot
T90 = 130.088000059128 sec.
Hardness ratio (energy fluence ratio) = 1.55634
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.5677
Count Ratio (50-100 keV) / (15-25 keV) = 1.43491
Mask shadow pattern
IMX = 6.978609709133737E-01, IMY = 4.293089372563206E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 2.048000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 2.048000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 2.048000
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:
-239.992000 -28.428000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
299.6046 35.1847 0.6 33.2 -121.4 7.2168 18.9 1.2 Cyg X-1
308.0945 40.9482 2.8 24.8 -116.2 1.2018 4.1 0.8 Cyg X-3
326.2281 38.2897 4.5 13.1 -142.3 0.6450 2.6 3.3 Cyg X-2
297.1034 38.1839 2.5 33.7 -114.9 1.9266 4.6 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-28.428000 23.508600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
299.5948 35.3348 22.4 33.2 -121.1 0.0746 0.5 8.0 Cyg X-1
308.2211 41.0595 5.2 24.7 -116.0 -0.2498 -2.2 8.1 Cyg X-3
326.3926 38.3702 8.0 12.9 -142.3 0.1240 1.5 10.8 Cyg X-2
317.2065 -7.9406 2.9 56.8 179.2 2.0679 3.9 ------ UNKNOWN
71.1316 80.6249 2.6 46.3 -17.2 0.7515 4.4 ------ UNKNOWN
333.7056 83.5774 0.3 39.3 -31.6 5.8250 41.0 ------ UNKNOWN
300.3467 33.1929 2.2 33.7 -125.1 0.7372 5.2 ------ UNKNOWN
284.1933 40.7653 2.8 41.6 -104.2 1.6573 4.1 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
103.308600 962.081100
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
299.5550 35.1983 1.5 49.6 -175.2 19.0638 7.8 1.7 Cyg X-1
308.2393 41.0638 4.6 43.2 176.0 4.3275 2.5 8.9 Cyg X-3
326.3158 38.2859 7.5 45.3 155.9 4.4412 1.5 7.1 Cyg X-2
91.8100 49.3245 3.5 44.0 23.7 4.5449 3.3 ------ UNKNOWN
303.3406 32.8347 2.5 51.7 -179.5 12.7485 4.7 ------ UNKNOWN
256.2283 40.7697 3.5 48.1 -129.2 17.5390 3.3 ------ UNKNOWN
Plot creation:
Wed Dec 18 17:44:07 EST 2024