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
341.2076 46.5483 0.0061 22.1745 136.0874 4.5474478 31.925 TRIG_01352124
Foreground time interval of the image:
-21.768 64.424 (delta_t = 86.192 [sec])
Background time interval of the image:
-239.912 -209.316 (delta_t = 30.596 [sec])
-207.912 -21.768 (delta_t = 186.144 [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 -21.768 sec. to 64.424 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.86367 ( -0.0872953 0.0884553 )
Norm@50keV : 3.31688E-03 ( -0.000162018 0.000160836 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 48.06 using 59 bins.
Reduced chi-squared = 0.843158
# Null hypothesis probability of 7.94e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 86.19 sec: 0.468861 ( -0.021958 0.022045 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.62867e-06 ( -1.28232e-07 1.28961e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -21.768 sec. to 64.424 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.85386 ( -0.328804 0.29389 )
Epeak [keV] : 704.360 ( -753.418 -814.698 )
Norm@50keV : 3.35630E-03 ( -0.00102255 0.00156767 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 48.06 using 59 bins.
Reduced chi-squared = 0.858214
# Null hypothesis probability of 7.66e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 86.19 sec: 0.468597 ( -0.023948 0.022092 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.62655e-06 ( -1.49549e-07 1.29558e-07 ) ergs/cm2
Band function
Time interval is from -21.768 sec. to 64.424 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] : 12.0920 ( )
R^2/D10^2 : 0.101843 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 189.24 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.31e-16 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.716e-07 2.349e-08
25- 50 8.625e-07 4.581e-08
50-150 7.622e-07 8.098e-08
15-150 1.896e-06 9.438e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 97.4842 (-15.7834 21.2378)
Norm : 2.03494 (-0.140744 0.156537)
------------------------------------------------------------
#Fit statistic : Chi-Squared 55.40 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.35e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.584e-07 4.103e-08
25- 50 7.885e-07 4.314e-08
50-150 1.259e-06 3.383e-07
15-150 2.506e-06 3.689e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.89305 (-0.772178 0.859563)
R1^2/D10^2 : 1.11842 (-0.448548 0.83931)
kT2 [keV] : 22.7990 (-3.06957 4.35501)
R2^2/D10^2 : 7.55833E-03 (-0.00360161 0.00562114)
------------------------------------------------------------
#Fit statistic : Chi-Squared 51.31 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.16e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.949e-07 6.813e-08
25- 50 7.481e-07 7.895e-08
50-150 1.327e-06 2.215e-07
15-150 2.570e-06 2.900e-07
Peak spectrum fit
Power-law model
Time interval is from 0.192 sec. to 1.192 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.53730 ( -0.26201 0.270388 )
Norm@50keV : 9.08775E-03 ( -0.00145667 0.00143584 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 46.36 using 59 bins.
Reduced chi-squared = 0.813333
# Null hypothesis probability of 8.42e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 1.14630 ( -0.176331 0.17657 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.57215e-08 ( -1.48568e-08 1.5032e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.192 sec. to 1.192 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.01533 ( -1.7265 -2.01533 )
Epeak [keV] : 6.13630 ( )
Norm@50keV : 4.98884E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared 46.26 using 59 bins.
Reduced chi-squared = 0.826071
# Null hypothesis probability of 8.20e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 1.14155 ( -0.180549 0.17958 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.14588e-08 ( -1.60501e-08 1.24028e-08 ) ergs/cm2
Band function
Time interval is from 0.192 sec. to 1.192 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] : 14.2329 (-2.68284 3.54908)
R^2/D10^2 : 0.155797 (-0.084479 0.170835)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 58.09 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.35e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.656e-09 1.841e-09
25- 50 2.516e-08 6.130e-09
50-150 3.384e-08 1.041e-08
15-150 6.566e-08 1.527e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.363 (-96.2785 -199.363)
Norm : 4.68547 (-0.710206 0.710622)
------------------------------------------------------------
#Fit statistic : Chi-Squared 46.44 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.40e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.167e-08 6.625e-09
25- 50 2.244e-08 1.249e-08
50-150 4.922e-08 2.812e-08
15-150 8.333e-08 4.625e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 8.04568 (-6.98012 3.62708)
R1^2/D10^2 : 0.786328 (-0.523502 148971)
kT2 [keV] : 30.9024 (-15.5975 150.237)
R2^2/D10^2 : 7.62448E-03 (-0.00724784 0.128602)
------------------------------------------------------------
#Fit statistic : Chi-Squared 47.42 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.56e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.120e-08 5.049e-09
25- 50 2.023e-08 7.686e-09
50-150 4.356e-08 1.813e-08
15-150 7.499e-08 2.332e-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: 1.86367 ( -0.0872953 0.0884553 )
Norm@50keV : 3.31688E-03 ( -0.000162018 0.000160836 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 48.06 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.94e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 86.19 sec: 0.468834 ( -0.021956 0.022042 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.62825e-06 ( -1.2827e-07 1.28939e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.85267 ( -0.327366 0.295336 )
Epeak [keV] : 623.947 ( -768.371 -785.656 )
Norm@50keV : 3.36109E-03 ( -0.000994354 0.00156786 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 48.06 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.66e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 86.19 sec: 0.468614 ( -0.024058 0.02193 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.63079e-06 ( -1.53375e-07 1.25518e-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) = 7.58e-07
S(50-100 keV) = 8.33e-07
T90 vs. Hardness ratio plot
T90 = 62.6879999637604 sec.
Hardness ratio (energy fluence ratio) = 1.09894
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.06564
Count Ratio (50-100 keV) / (15-25 keV) = 0.633227
Mask shadow pattern
IMX = -2.936154824808744E-01, IMY = -2.826765472614852E-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:
-239.912000 -209.315600
-207.912000 -21.768000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
299.5898 35.1942 56.5 48.6 173.0 0.1608 0.2 0.4 Cyg X-1
308.0929 40.9423 5.4 40.1 169.6 1.1210 2.1 1.0 Cyg X-3
326.3424 38.3782 40.3 34.7 147.8 0.1385 0.3 8.7 Cyg X-2
307.9584 30.3771 2.0 49.1 161.7 5.3281 5.7 ------ UNKNOWN
282.1551 64.0652 2.2 34.0 -144.8 2.1113 5.2 ------ UNKNOWN
245.6203 59.9726 3.2 48.1 -129.2 5.6360 3.7 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-21.768000 64.424000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
299.6788 35.1510 2.4 48.6 172.9 -1.5290 -4.8 5.3 Cyg X-1
308.1926 41.0545 3.0 40.0 169.6 0.7895 3.9 7.2 Cyg X-3
326.3579 38.2847 3.2 34.8 147.7 0.6952 3.6 9.0 Cyg X-2
341.2076 46.5483 0.4 22.2 136.1 4.5475 31.9 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
502.588590 962.142000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.3944 -40.5257 7.2 55.2 -26.0 -3.9347 -1.6 6.4 Vela X-1
90.8806 -8.5798 2.8 44.4 40.9 5.2326 4.1 ------ UNKNOWN
171.2565 63.1265 3.0 56.8 -179.1 10.0289 3.8 ------ UNKNOWN
118.8562 -21.9874 2.4 37.8 -4.4 3.8415 4.8 ------ UNKNOWN
Plot creation:
Sun Mar 1 23:22:27 EST 2026