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
179.8706 11.4429 0.0097 11.6521 -49.6522 0.7918514 19.858 TRIG_01429020
Foreground time interval of the image:
-1.604 9.725 (delta_t = 11.329 [sec])
Background time interval of the image:
-121.275 -1.604 (delta_t = 119.671 [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 -1.604 sec. to 73.216 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.12301 ( -0.042023 0.0417871 )
Norm@50keV : 7.63572E-03 ( -0.000172656 0.000172161 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 43.40 using 59 bins.
Reduced chi-squared = 0.761404
# Null hypothesis probability of 9.08e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 74.82 sec: 0.887772 ( -0.02146 0.021536 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.93058e-06 ( -1.34461e-07 1.34651e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -1.604 sec. to 73.216 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.12767 ( -0.049547 0.0472271 )
Epeak [keV] : 9999.36 ( -9999.36 -9999.36 )
Norm@50keV : 7.60174E-03 ( -0.000170452 0.00111705 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 44.26 using 59 bins.
Reduced chi-squared = 0.790357
# Null hypothesis probability of 8.71e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 74.82 sec: 0.888331 ( -0.022156 0.022097 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.93318e-06 ( -1.47857e-07 1.18105e-07 ) ergs/cm2
Band function
Time interval is from -1.604 sec. to 73.216 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] : 22.2852 ( )
R^2/D10^2 : 2.86915E-02 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 435.41 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.10e-59 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.961e-07 9.465e-09
25- 50 1.045e-06 3.853e-08
50-150 3.878e-06 1.205e-07
15-150 5.119e-06 1.414e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.363 ( )
Norm : 3.84294 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared 383.15 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.46e-50 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.160e-07 1.942e-08
25- 50 1.377e-06 3.292e-08
50-150 3.021e-06 6.734e-08
15-150 5.114e-06 1.257e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 9.12355 (-0.819528 0.886394)
R1^2/D10^2 : 0.311910 (-0.0761776 0.107446)
kT2 [keV] : 39.5257 (-3.94384 5.4687)
R2^2/D10^2 : 4.04521E-03 (-0.00128845 0.00156211)
------------------------------------------------------------
#Fit statistic : Chi-Squared 46.24 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.94e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.424e-07 3.240e-08
25- 50 1.245e-06 5.948e-08
50-150 4.268e-06 2.469e-07
15-150 5.955e-06 3.098e-07
Peak spectrum fit
Power-law model
Time interval is from 28.680 sec. to 29.680 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.954560 ( -0.0950887 0.0938135 )
Norm@50keV : 3.10062E-02 ( -0.00172911 0.00172734 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 57.86 using 59 bins.
Reduced chi-squared = 1.01509
# Null hypothesis probability of 4.43e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 3.56279 ( -0.20028 0.20039 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.40887e-07 ( -2.0968e-08 2.10475e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 28.680 sec. to 29.680 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.537760 ( -0.416878 0.377996 )
Epeak [keV] : 196.695 ( -71.4474 4316.79 )
Norm@50keV : 4.82189E-02 ( -0.0155015 0.0256946 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 54.30 using 59 bins.
Reduced chi-squared = 0.969643
# Null hypothesis probability of 5.40e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 3.51687 ( -0.20505 0.20485 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.33664e-07 ( -2.25425e-08 2.23524e-08 ) ergs/cm2
Band function
Time interval is from 28.680 sec. to 29.680 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] : 21.3196 (-1.58343 1.77401)
R^2/D10^2 : 0.143650 (-0.031769 0.0395723)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 95.25 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.12e-03 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.225e-08 1.250e-09
25- 50 6.358e-08 5.235e-09
50-150 2.156e-07 2.090e-08
15-150 2.915e-07 2.190e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.363 ( )
Norm : 13.9989 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared 157.41 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.41e-11 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.486e-08 2.295e-09
25- 50 6.706e-08 5.890e-09
50-150 1.471e-07 3.504e-08
15-150 2.490e-07 3.685e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 12.0515 (-2.61369 2.78276)
R1^2/D10^2 : 0.548521 (-0.212977 0.431009)
kT2 [keV] : 52.3602 (-18.3551 -52.8671)
R2^2/D10^2 : 7.46563E-03 (-0.00670202 0.0118829)
------------------------------------------------------------
#Fit statistic : Chi-Squared 50.83 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.35e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.901e-08 4.350e-09
25- 50 6.905e-08 1.557e-08
50-150 2.476e-07 1.031e-07
15-150 3.357e-07 1.221e-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: 1.36305 ( -0.138019 0.137574 )
Norm@50keV : 4.21501E-03 ( -0.000342839 0.000341683 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 39.43 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.63e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 11.33 sec: 0.509171 ( -0.0416381 0.0416771 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.65075e-07 ( -4.20557e-08 4.23791e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.00009 ( -0.587747 0.442086 )
Epeak [keV] : 137.807 ( -57.4551 -137.808 )
Norm@50keV : 6.44870E-03 ( -0.00245166 0.00615014 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 38.02 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.69e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 11.33 sec: 0.501999 ( -0.042974 0.042912 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.51975e-07 ( -4.6751e-08 4.65357e-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) = 1.19e-06
S(50-100 keV) = 2.18e-06
T90 vs. Hardness ratio plot
T90 = 68.7400000095367 sec.
Hardness ratio (energy fluence ratio) = 1.83193
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.67326
Count Ratio (50-100 keV) / (15-25 keV) = 1.58947
Mask shadow pattern
IMX = 1.335109340589435E-01, IMY = 1.571649603194333E-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:
-121.275410 -1.604000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
160.6878 -18.5458 3.2 40.8 6.9 0.9996 3.7 ------ UNKNOWN
206.7200 -7.2689 4.5 43.8 -64.2 2.2139 2.6 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-1.604000 9.724600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
134.0561 -3.7092 2.6 44.7 51.3 0.7003 4.5 ------ UNKNOWN
137.3273 -3.1383 2.0 41.7 49.2 0.6413 5.7 ------ UNKNOWN
179.8706 11.4429 0.6 11.7 -49.7 0.7916 19.9 ------ UNKNOWN
220.2830 44.6301 2.1 46.1 -143.0 0.4635 5.4 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
55.724600 962.954700
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
145.7742 14.0983 2.7 33.4 77.2 9.3036 4.3 ------ UNKNOWN
212.9266 -7.5142 3.6 37.9 -82.8 10.1459 3.2 ------ UNKNOWN
209.9753 -20.5934 4.0 43.6 -64.1 18.5059 3.3 ------ UNKNOWN
210.2061 -20.7322 5.1 43.8 -64.2 17.1186 2.9 ------ UNKNOWN
Plot creation:
Sun Mar 1 23:09:32 EST 2026