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
334.6116 -9.1200 0.0070 38.1231 -159.7447 2.5247048 27.470 TRIG_01314210
Foreground time interval of the image:
-19.960 9.957 (delta_t = 29.917 [sec])
Background time interval of the image:
-239.544 -19.960 (delta_t = 219.584 [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 -19.960 sec. to 22.696 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.68959 ( -0.0843909 0.0849784 )
Norm@50keV : 5.88547E-03 ( -0.000277459 0.000276597 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 63.09 using 59 bins.
Reduced chi-squared = 1.10684
# Null hypothesis probability of 2.70e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 42.66 sec: 0.778867 ( -0.037843 0.037975 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.32697e-06 ( -1.14585e-07 1.14946e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -19.960 sec. to 22.696 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.69063 ( -0.0866392 0.083845 )
Epeak [keV] : 9999.32 ( -9999.35 -9999.36 )
Norm@50keV : 5.88058E-03 ( -0.000271165 0.00216102 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 63.10 using 59 bins.
Reduced chi-squared = 1.12679
# Null hypothesis probability of 2.40e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 42.66 sec: 0.779532 ( -0.039266 0.037916 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.32912e-06 ( -1.22124e-07 1.14769e-07 ) ergs/cm2
Band function
Time interval is from -19.960 sec. to 22.696 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] : 13.4400 ( )
R^2/D10^2 : 0.120959 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 204.95 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.45e-18 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.975e-07 1.766e-08
25- 50 7.046e-07 4.053e-08
50-150 8.200e-07 7.785e-08
15-150 1.722e-06 9.833e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 144.991 (-26.6719 47.1275)
Norm : 3.20401 (-0.194572 0.192948)
------------------------------------------------------------
#Fit statistic : Chi-Squared 68.27 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.46e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.436e-07 2.532e-08
25- 50 6.398e-07 5.460e-08
50-150 1.279e-06 3.827e-07
15-150 2.263e-06 4.279e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.62479 (-0.874278 0.916035)
R1^2/D10^2 : 0.727460 (-0.234856 0.386793)
kT2 [keV] : 33.0973 (-6.0417 10.0528)
R2^2/D10^2 : 3.74451E-03 (-0.00208746 0.00371745)
------------------------------------------------------------
#Fit statistic : Chi-Squared 60.91 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.72e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.398e-07 4.855e-08
25- 50 6.696e-07 7.018e-08
50-150 1.332e-06 3.086e-07
15-150 2.342e-06 3.739e-07
Peak spectrum fit
Power-law model
Time interval is from 19.388 sec. to 20.388 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.57597 ( -0.129558 0.130919 )
Norm@50keV : 2.95216E-02 ( -0.00228531 0.00227318 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 40.28 using 59 bins.
Reduced chi-squared = 0.706667
# Null hypothesis probability of 9.54e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 3.76609 ( -0.28963 0.29001 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.76968e-07 ( -2.2976e-08 2.31071e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 19.388 sec. to 20.388 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.57703 ( -0.132748 0.129311 )
Epeak [keV] : 9999.36 ( -9999.36 -9999.36 )
Norm@50keV : 2.95470E-02 ( -0.0295865 0.0147512 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 40.29 using 59 bins.
Reduced chi-squared = 0.719464
# Null hypothesis probability of 9.44e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 3.77747 ( -0.38201 0.35731 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.78356e-07 ( -3.24948e-08 2.98137e-08 ) ergs/cm2
Band function
Time interval is from 19.388 sec. to 20.388 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] : 13.6015 (-1.41746 1.63587)
R^2/D10^2 : 0.585900 (-0.196138 0.285003)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 104.45 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.29e-04 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.295e-08 3.450e-09
25- 50 8.289e-08 8.960e-09
50-150 9.945e-08 1.601e-08
15-150 2.053e-07 1.935e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 198.730 (-61.5205 -198.831)
Norm : 15.2897 (-1.13734 1.25181)
------------------------------------------------------------
#Fit statistic : Chi-Squared 42.47 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.24e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.809e-08 3.630e-09
25- 50 7.324e-08 1.468e-08
50-150 1.605e-07 6.370e-08
15-150 2.718e-07 6.530e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.61979 (-1.22542 1.36847)
R1^2/D10^2 : 3.57739 (-1.54427 3.05041)
kT2 [keV] : 37.7471 (-9.74634 22.1416)
R2^2/D10^2 : 1.37097E-02 (-0.00979084 0.0222179)
------------------------------------------------------------
#Fit statistic : Chi-Squared 36.40 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.75e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.876e-08 8.305e-09
25- 50 7.562e-08 1.704e-08
50-150 1.693e-07 7.949e-08
15-150 2.836e-07 8.725e-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: 1.56724 ( -0.105958 0.106414 )
Norm@50keV : 5.30832E-03 ( -0.000319186 0.000317875 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 61.21 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.27e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 29.92 sec: 0.675405 ( -0.0418404 0.0419624 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.49162e-06 ( -9.57335e-08 9.62547e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.56783 ( -0.108296 0.105195 )
Epeak [keV] : 9999.36 ( -9999.36 -9999.36 )
Norm@50keV : 5.31772E-03 ( -0.00227039 0.00271749 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 61.21 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.94e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 29.92 sec: 0.675436 ( -0.042873 0.041398 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.49036e-06 ( -5.31349e-08 9.69199e-08 ) 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) = 6.27e-07
S(50-100 keV) = 7.76e-07
T90 vs. Hardness ratio plot
T90 = 30.0360000133514 sec.
Hardness ratio (energy fluence ratio) = 1.23764
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.35544
Count Ratio (50-100 keV) / (15-25 keV) = 0.880469
Mask shadow pattern
IMX = -7.362225741987247E-01, IMY = 2.716847853550358E-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:
-239.544000 -19.960000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
330.0989 -9.8006 2.1 37.4 -167.0 2.0749 5.6 ------ UNKNOWN
342.1997 1.4864 3.5 49.4 -150.4 2.5856 3.3 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-19.960000 9.956590
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
334.4593 -23.7461 2.3 23.5 -158.5 0.3159 4.9 ------ UNKNOWN
334.6116 -9.1200 0.4 38.1 -159.7 2.5247 27.5 ------ UNKNOWN
27.8595 -61.5366 2.4 34.1 -27.9 0.3957 4.7 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
87.356600 962.576000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
308.2254 40.9366 87.9 55.6 177.1 0.5923 0.1 5.3 Cyg X-3
326.2050 38.4804 8.3 48.2 -167.7 -3.7555 -1.4 9.7 Cyg X-2
297.7690 1.0692 2.6 38.1 124.7 12.8553 4.5 ------ UNKNOWN
313.7547 39.0437 3.1 51.9 -179.4 12.3636 3.7 ------ UNKNOWN
329.0223 27.9014 2.3 37.4 -167.0 6.7773 5.0 ------ UNKNOWN
351.3335 -3.0333 2.7 17.7 -88.0 5.1085 4.2 550.7 UNKNOWN
1.5182 26.5604 2.5 44.2 -123.4 22.5754 4.6 ------ UNKNOWN
16.9086 -5.1677 2.0 42.2 -71.3 26.1389 5.8 ------ UNKNOWN
Plot creation:
Fri Jun 20 01:39:28 EDT 2025