Estimated redshift from machine learning (Ukwatta et al. 2016) - may take a few minutes to calcaulte
Image
Pre-slew 15-350 keV image (Event data; bkg subtracted)
# RAcent DECcent POSerr Theta Phi Peak Cts SNR Name
300.1204 +35.1489 0.0186 16.6 6.7 1.9922 10.4 TRIG_01212791
------------------------------------------
Foreground time interval of the image:
0.000 56.320 (delta_t = 56.320 [sec])
57.000 100.820 (delta_t = 43.820 [sec])
114.000 128.000 (delta_t = 14.000 [sec])
Background time interval of the image:
Lightcurves
Notes:
- 1) All plots contain as much data as has been downloaded to date.
- 2) The mask-weighted light curves are using the flight position.
- 3) Multiple plots of different time binning/intervals are shown to cover all scenarios of short/long GRBs, rate/image triggers, and real/false positives.
- 4) 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.
- 5) 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.
- 6) 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)
Spectra
Notes:
- 1) The fitting includes the systematic errors.
- 2) For long bursts, a spectral fit of 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.
- 4) For short bursts (T90<1sec), the specrtum is also fit with Blackbody, OTTB, and Double Blackbody.
Time averaged spectrum fit using the pre-slew DRM
Power-law model
Multiple GTIs in the spectrum
tstart tstop
0.000000 56.320000
57.000000 100.820000
114.000000 128.000000
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.22004 ( -0.196467 0.210537 )
Norm@50keV : 9.38458E-04 ( -0.000136407 0.000133804 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 41.64 using 59 PHA bins.
# Reduced chi-squared = 0.7304 for 57 degrees of freedom
# Null hypothesis probability = 9.369195e-01
Photon flux (15-150 keV) in 114.1 sec: 0.157021 ( -0.0153337 0.015334 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.00969e-06 ( -1.22786e-07 1.26378e-07 ) ergs/cm2
Cutoff power-law model
Multiple GTIs in the spectrum
tstart tstop
0.000000 56.320000
57.000000 100.820000
114.000000 128.000000
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.65153 ( -1.04635 0.351362 )
Epeak [keV] : 23.2843 ( -22.4065 14.8217 )
Norm@50keV : 2.08967E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 40.30 using 59 PHA bins.
# Reduced chi-squared = 0.7196 for 56 degrees of freedom
# Null hypothesis probability = 9.436387e-01
Photon flux (15-150 keV) in 114.1 sec: 0.153630 ( -0.016003 0.016065 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.45041e-07 ( -1.41574e-07 1.55954e-07 ) ergs/cm2
Band function
Multiple GTIs in the spectrum
tstart tstop
0.000000 56.320000
57.000000 100.820000
114.000000 128.000000
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.33895 ( 1.33476 1.33476 )
beta : -2.56994 ( 2.57848 0.487389 )
Epeak [keV] : 25.7107 ( -25.9126 11.7966 )
Norm@50keV : 3.45102E-03 ( -0.00353569 258.69 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 40.08 using 59 PHA bins.
# Reduced chi-squared = 0.7287 for 55 degrees of freedom
# Null hypothesis probability = 9.346744e-01
Photon flux (15-150 keV) in 114.1 sec: 0.156238 ( 6.84376 -0.020327 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.59195e-07 ( 0 0 ) ergs/cm2
Single BB
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 8.30478 (-0.913862 1.026)
R^2/D10^2 : 0.146443 (-0.0544175 0.0872268)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 56.61 using 59 PHA bins.
# Reduced chi-squared = 0.9931 for 57 degrees of freedom
# Null hypothesis probability = 4.898496e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.140e-07 3.543e-08
25- 50 3.992e-07 4.952e-08
50-150 1.184e-07 3.620e-08
15-150 7.315e-07 9.853e-08
Thermal bremsstrahlung (OTTB)
XSPEC12>exit
XSPEC: quit
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 45.0472 (-10.7847 16.3743)
Norm : 0.939219 (-0.159269 0.20934)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.552e-07 3.104e-08
25- 50 3.525e-07 3.891e-08
50-150 3.091e-07 8.963e-08
15-150 9.169e-07 1.245e-07
Double BB
XSPEC12>exit
XSPEC: quit
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.19527 (-2.05312 1.87821)
R1^2/D10^2 : 0.673416 (-0.424917 4.30844)
kT2 [keV] : 15.7891 (-5.45889 16.1116)
R2^2/D10^2 : 7.37825E-03 (-0.00657632 0.0125607)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.608e-07 1.302e-07
25- 50 3.368e-07 1.722e-07
50-150 3.214e-07 1.782e-07
15-150 9.191e-07 4.748e-07
Peak spectrum fit
Power-law model
Time interval is from 114.000 sec. to 128.000 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.22004 ( -0.196467 0.210537 )
Norm@50keV : 9.38458E-04 ( -0.000136407 0.000133804 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 41.64 using 59 PHA bins.
# Reduced chi-squared = 0.7304 for 57 degrees of freedom
# Null hypothesis probability = 9.369195e-01
Photon flux (15-150 keV) in 114.1 sec: 0.157021 ( -0.0153337 0.015334 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.00969e-06 ( -1.22786e-07 1.26378e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from 114.000 sec. to 128.000 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.65153 ( -1.04635 0.351362 )
Epeak [keV] : 23.2843 ( -21.0644 14.776 )
Norm@50keV : 2.08967E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 40.30 using 59 PHA bins.
# Reduced chi-squared = 0.7196 for 56 degrees of freedom
# Null hypothesis probability = 9.436387e-01
Photon flux (15-150 keV) in 114.1 sec: 0.153630 ( -0.016003 0.016065 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.45041e-07 ( -1.41574e-07 1.55954e-07 ) ergs/cm2
Band function
Time interval is from 114.000 sec. to 128.000 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.33895 ( 1.33476 1.33476 )
beta : -2.56994 ( 2.57848 0.487389 )
Epeak [keV] : 25.7107 ( -25.9126 11.7966 )
Norm@50keV : 3.45102E-03 ( -0.00353569 258.732 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 40.08 using 59 PHA bins.
# Reduced chi-squared = 0.7287 for 55 degrees of freedom
# Null hypothesis probability = 9.346744e-01
Photon flux (15-150 keV) in 114.1 sec: 0.156238 ( 6.84376 -0.020327 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.59195e-07 ( 0 0 ) ergs/cm2
Single BB
XSPEC: quit
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 8.30478 (-0.913862 1.026)
R^2/D10^2 : 0.146443 (-0.0544175 0.0872268)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.140e-07 3.731e-08
25- 50 3.992e-07 5.351e-08
50-150 1.184e-07 3.750e-08
15-150 7.315e-07 9.408e-08
Thermal bremsstrahlung (OTTB)
XSPEC12>exit
XSPEC: quit
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 45.0472 (-10.7847 16.3743)
Norm : 0.939219 (-0.159269 0.20934)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.552e-07 3.400e-08
25- 50 3.525e-07 4.028e-08
50-150 3.091e-07 9.259e-08
15-150 9.169e-07 1.383e-07
Double BB
XSPEC12>exit
XSPEC: quit
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.19527 (-2.05312 1.87821)
R1^2/D10^2 : 0.673416 (-0.424917 4.30844)
kT2 [keV] : 15.7891 (-5.45889 16.1116)
R2^2/D10^2 : 7.37825E-03 (-0.00657632 0.0125607)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.608e-07 1.329e-07
25- 50 3.368e-07 1.729e-07
50-150 3.214e-07 1.823e-07
15-150 9.191e-07 4.273e-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: 2.22004 ( -0.196467 0.210537 )
Norm@50keV : 9.38458E-04 ( -0.000136407 0.000133804 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 41.64 using 59 PHA bins.
# Reduced chi-squared = 0.7304 for 57 degrees of freedom
# Null hypothesis probability = 9.369195e-01
Photon flux (15-150 keV) in 114.1 sec: 0.157021 ( -0.0153337 0.015334 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.00969e-06 ( -1.22786e-07 1.26378e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.65153 ( -1.04635 0.351362 )
Epeak [keV] : 23.2843 ( -22.8862 14.7515 )
Norm@50keV : 2.08967E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 40.30 using 59 PHA bins.
# Reduced chi-squared = 0.7196 for 56 degrees of freedom
# Null hypothesis probability = 9.436387e-01
Photon flux (15-150 keV) in 114.1 sec: 0.153630 ( -0.016003 0.016065 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.45041e-07 ( -1.41574e-07 1.55954e-07 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.33895 ( 1.33476 1.33476 )
beta : -2.56994 ( 2.57848 0.487389 )
Epeak [keV] : 25.7107 ( -25.9126 11.7966 )
Norm@50keV : 3.45102E-03 ( -0.00353569 258.724 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 40.08 using 59 PHA bins.
# Reduced chi-squared = 0.7287 for 55 degrees of freedom
# Null hypothesis probability = 9.346744e-01
Photon flux (15-150 keV) in 114.1 sec: 0.156238 ( 6.84376 -0.020327 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.59195e-07 ( 0 0 ) ergs/cm2
S(25-50 keV) vs. S(50-100 keV) plot
S(25-50 keV) = 3.21e-07
S(50-100 keV) = 2.76e-07
T90 vs. Hardness ratio plot
T90 = 128 sec.
Hardness ratio (energy fluence ratio) = 0.859813
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 0.843539
Count Ratio (50-100 keV) / (15-25 keV) = 0.350789
Mask shadow pattern
IMX = 2.952284551577634E-01, IMY = -3.459098250329486E-02
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:
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
0.000000 56.320000
57.000000 100.820000
114.000000 128.000000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
288.9315 11.0028 11.9 37.7 -30.5 -0.2942 -1.0 8.6 GRS 1915+105
299.4050 35.2244 3.8 17.1 7.2 -0.5936 -3.0 9.2 Cyg X-1
308.2717 41.1262 0.0 11.0 36.0 -0.2748 -1.4 12.7 Cyg X-3
326.0590 38.4728 4.9 5.3 148.6 -0.4310 -2.3 10.5 Cyg X-2
301.4213 51.3374 2.7 20.8 57.4 1.0015 4.2 ------ UNKNOWN
359.5793 31.7249 2.3 32.6 177.9 1.1638 5.0 ------ UNKNOWN
284.9953 -5.0918 2.3 52.6 -40.8 5.0082 4.9 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
188.100600 243.132800
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.2444 35.3250 0.0 37.1 34.1 0.2107 0.9 10.5 Her X-1
268.5120 -1.4184 36.1 47.0 -24.1 0.0743 0.3 8.9 SW J1753.5-0127
288.8663 11.1250 0.0 26.1 -44.0 -0.0667 -0.5 11.5 GRS 1915+105
299.5912 35.1334 11.6 0.4 15.4 -0.1116 -1.0 4.1 Cyg X-1
308.3294 40.9153 9.4 8.6 156.1 0.1445 1.2 10.2 Cyg X-3
325.9867 38.2507 31.6 20.9 -175.9 -0.0452 -0.4 9.7 Cyg X-2
245.1724 39.6139 2.3 43.2 43.1 1.7242 4.9 ------ UNKNOWN
248.9274 29.0120 2.4 43.3 26.9 1.2878 4.8 ------ UNKNOWN
Plot creation:
Sun Feb 4 20:37:16 EST 2024