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
50.7835 34.4373 0.0136 38.6948 70.7101 1.7676041 14.197 TRIG_01263840
Foreground time interval of the image:
-1.184 7.104 (delta_t = 8.288 [sec])
Background time interval of the image:
-103.659 -1.184 (delta_t = 102.475 [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 -1.184 sec. to 7.104 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.39076 ( -0.159035 0.159372 )
Norm@50keV : 1.45045E-02 ( -0.00142504 0.00142379 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 61.45 using 59 bins.
Reduced chi-squared = 1.07807
# Null hypothesis probability of 3.20e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 8.288 sec: 1.76275 ( -0.17785 0.17818 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.16394e-06 ( -1.23783e-07 1.24396e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -1.184 sec. to 7.104 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.592813 ( -0.77393 0.654861 )
Epeak [keV] : 92.7070 ( -23.8957 161.833 )
Norm@50keV : 3.55077E-02 ( -0.0181621 0.0475297 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 56.99 using 59 bins.
Reduced chi-squared = 1.01768
# Null hypothesis probability of 4.38e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 8.288 sec: 1.71660 ( -0.18195 0.1822 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.11975e-06 ( -1.32039e-07 1.31487e-07 ) ergs/cm2
Band function
Time interval is from -1.184 sec. to 7.104 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] : 16.2183 (-1.84505 2.15579)
R^2/D10^2 : 0.161924 (-0.0572811 0.0849298)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 71.67 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.14e-02 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.276e-08 1.375e-08
25- 50 3.097e-07 4.625e-08
50-150 5.723e-07 1.051e-07
15-150 9.549e-07 1.193e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-40.8342 -200)
Norm : 7.35450 (-0.71922 0.71922)
------------------------------------------------------------
#Fit statistic : Chi-Squared 61.88 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.06e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.518e-07 3.294e-08
25- 50 2.920e-07 1.231e-07
50-150 6.403e-07 3.272e-07
15-150 1.084e-06 3.480e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 9.44685 (-2.70431 2.88726)
R1^2/D10^2 : 0.639366 (-0.336857 0.655966)
kT2 [keV] : 30.1728 (-8.52541 26.221)
R2^2/D10^2 : 1.31633E-02 (-0.0117318 0.0358466)
------------------------------------------------------------
#Fit statistic : Chi-Squared 55.56 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.54e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.097e-07 5.738e-08
25- 50 3.114e-07 1.616e-07
50-150 7.095e-07 3.859e-07
15-150 1.131e-06 5.559e-07
Peak spectrum fit
Power-law model
Time interval is from 0.676 sec. to 1.676 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.22075 ( -0.279129 0.269253 )
Norm@50keV : 2.69956E-02 ( -0.00473818 0.00471965 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 61.16 using 59 bins.
Reduced chi-squared = 1.07298
# Null hypothesis probability of 3.29e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 3.17831 ( -0.5879 0.59057 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.72333e-07 ( -4.88523e-08 4.88999e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.676 sec. to 1.676 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.539131 ( -1.54241 0.883301 )
Epeak [keV] : 121.661 ( -50.3756 -121.659 )
Norm@50keV : 5.57994E-02 ( -0.0324293 0.211027 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 60.26 using 59 bins.
Reduced chi-squared = 1.07607
# Null hypothesis probability of 3.24e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 3.14581 ( -0.58878 0.59275 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.69967e-07 ( -5.03732e-08 4.97679e-08 ) ergs/cm2
Band function
Time interval is from 0.676 sec. to 1.676 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] : 19.1908 (-3.3689 4.37532)
R^2/D10^2 : 0.179444 (-0.092076 0.167026)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 64.52 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.31e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.294e-08 4.291e-09
25- 50 6.269e-08 1.872e-08
50-150 1.700e-07 5.090e-08
15-150 2.456e-07 5.445e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-53.0308 -200)
Norm : 13.5701 (-2.40394 2.40394)
------------------------------------------------------------
#Fit statistic : Chi-Squared 65.15 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.14e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.381e-08 1.969e-08
25- 50 6.504e-08 3.776e-08
50-150 1.426e-07 8.020e-08
15-150 2.415e-07 1.374e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 13.3327 (-6.03331 5.64622)
R1^2/D10^2 : 0.474967 (-0.289481 0.544852)
kT2 [keV] : 94.6570 (-90.998 -98.014)
R2^2/D10^2 : 1.21129E-03 (-0.000932602 0.0856321)
------------------------------------------------------------
#Fit statistic : Chi-Squared 58.92 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.34e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.941e-08 1.198e-08
25- 50 6.825e-08 3.984e-08
50-150 1.822e-07 8.875e-08
15-150 2.699e-07 1.319e-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: 1.39076 ( -0.159035 0.159372 )
Norm@50keV : 1.45045E-02 ( -0.00142504 0.00142379 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 61.45 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.20e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 8.288 sec: 1.76272 ( -0.17784 0.178178 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.16379e-06 ( -1.23756e-07 1.24409e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.592812 ( -0.77393 0.654861 )
Epeak [keV] : 92.7070 ( -23.8956 161.832 )
Norm@50keV : 3.55077E-02 ( -0.0181622 0.0475297 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 56.99 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.38e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 8.288 sec: 1.71647 ( -0.18192 0.18216 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.12019e-06 ( -1.31928e-07 1.31589e-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) = 2.72e-07
S(50-100 keV) = 4.15e-07
T90 vs. Hardness ratio plot
T90 = 6.62399995326996 sec.
Hardness ratio (energy fluence ratio) = 1.52574
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 2.06645
Count Ratio (50-100 keV) / (15-25 keV) = 1.62959
Mask shadow pattern
IMX = 2.646090096228398E-01, IMY = -7.560338609049904E-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:
-103.659400 -1.184000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
308.2082 41.0839 5.7 39.2 -130.2 0.5200 2.0 9.0 Cyg X-3
326.3480 38.3960 6.4 32.2 -151.5 0.3362 1.8 9.4 Cyg X-2
48.8472 31.8319 2.6 39.9 75.2 2.6794 4.5 ------ UNKNOWN
334.6646 12.9015 3.1 51.6 -179.5 1.5681 3.8 ------ UNKNOWN
345.8353 57.4136 2.7 10.2 -130.6 0.5697 4.2 ------ UNKNOWN
317.2918 75.2638 3.4 23.3 -67.0 0.5640 3.4 ------ UNKNOWN
307.2162 35.2583 2.2 44.1 -135.0 1.7807 5.3 ------ UNKNOWN
304.2786 27.8861 2.5 51.5 -138.2 2.9903 4.6 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-1.184000 7.104000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
307.9116 40.9868 41.1 39.4 -130.0 -0.0151 -0.3 9.2 Cyg X-3
326.1719 38.3209 32.7 32.3 -151.4 0.0134 0.4 0.0 Cyg X-2
50.7835 34.4373 0.8 38.7 70.7 1.7672 14.1 ------ UNKNOWN
316.2656 34.8379 2.1 39.9 -144.2 0.2707 5.4 ------ UNKNOWN
307.5956 49.8217 2.4 33.5 -118.9 0.2328 4.9 ------ UNKNOWN
297.6281 43.3978 2.5 42.9 -119.1 0.5431 4.6 ------ UNKNOWN
306.7147 23.4925 2.2 54.0 -143.6 0.8750 5.2 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
139.140600 917.040600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6328 22.0055 0.4 31.3 -23.2 31.2467 30.7 0.5 Crab
85.0053 -5.8547 3.0 51.6 6.6 6.0627 3.8 ------ UNKNOWN
92.7214 9.9839 2.9 45.4 -15.5 6.3507 4.1 ------ UNKNOWN
331.9538 58.1429 2.5 55.6 -166.7 14.6716 4.7 ------ UNKNOWN
102.1422 55.6162 2.7 40.8 -85.4 16.9473 4.3 ------ UNKNOWN
Plot creation:
Wed Dec 18 17:42:13 EST 2024