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
284.0114 +32.3269 0.0131 39.2 138.8 2.5386 14.7 TRIG_01330958
------------------------------------------
Foreground time interval of the image:
-0.096 27.400 (delta_t = 27.496 [sec])
28.120 40.088 (delta_t = 11.968 [sec])
Background time interval of the image:
-239.880 -0.096 (delta_t = 239.784 [sec])
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
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 8.192000
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 8.192000
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 8.192000
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
-0.096000 27.400000
28.120000 40.088000
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.34438 ( -0.169755 0.167442 )
Norm@50keV : 4.15214E-03 ( -0.000428818 0.000428811 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 59.12 using 59 PHA bins.
# Reduced chi-squared = 1.037 for 57 degrees of freedom
# Null hypothesis probability = 3.978653e-01
Photon flux (15-150 keV) in 39.46 sec: 0.499641 ( -0.0544128 0.0546141 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.60225e-06 ( -1.75256e-07 1.75978e-07 ) ergs/cm2
Cutoff power-law model
Multiple GTIs in the spectrum
tstart tstop
-0.096000 27.400000
28.120000 40.088000
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.345899 ( -0.908775 0.75015 )
Epeak [keV] : 88.6200 ( -20.1431 99.6311 )
Norm@50keV : 1.23976E-02 ( -0.0068358 0.0195706 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 53.71 using 59 PHA bins.
# Reduced chi-squared = 0.9591 for 56 degrees of freedom
# Null hypothesis probability = 5.620006e-01
Photon flux (15-150 keV) in 39.46 sec: 0.480514 ( -0.056594 0.056626 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.52523e-06 ( -1.87344e-07 1.8779e-07 ) ergs/cm2
Band function
Multiple GTIs in the spectrum
tstart tstop
-0.096000 27.400000
28.120000 40.088000
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 4.84571 ( -13.5884 -4.84571 )
beta : -1.54826 ( -0.231441 0.21713 )
Epeak [keV] : 32.0389 ( -8.10456 5.90322 )
Norm@50keV : 71.1775 ( -7.27757 440.493 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 54.02 using 59 PHA bins.
# Reduced chi-squared = 0.9822 for 55 degrees of freedom
# Null hypothesis probability = 5.121075e-01
Photon flux (15-150 keV) in 39.46 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] : 17.4702 (-1.92335 2.23748)
R^2/D10^2 : 3.59824E-02 (-0.0124272 0.0181817)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 62.35 using 59 PHA bins.
# Reduced chi-squared = 1.094 for 57 degrees of freedom
# Null hypothesis probability = 2.917466e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.757e-08 1.805e-08
25- 50 3.959e-07 6.442e-08
50-150 8.699e-07 1.687e-07
15-150 1.353e-06 1.784e-07
Thermal bremsstrahlung (OTTB)
XSPEC12>exit
XSPEC: quit
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-37.88 -200)
Norm : 2.11009 (-0.218706 0.218706)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.074e-07 3.113e-08
25- 50 3.989e-07 1.254e-07
50-150 8.750e-07 4.258e-07
15-150 1.481e-06 6.950e-07
Double BB
XSPEC12>exit
XSPEC: quit
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.63009 (-2.38846 5.08033)
R1^2/D10^2 : 0.403157 (-0.318754 1.59558)
kT2 [keV] : 22.1220 (-3.91676 12.8018)
R2^2/D10^2 : 1.37081E-02 (-0.011617 0.0153364)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.547e-07 8.446e-08
25- 50 3.894e-07 1.902e-07
50-150 9.656e-07 5.028e-07
15-150 1.510e-06 6.461e-07
Peak spectrum fit
Power-law model
Time interval is from 1.932 sec. to 2.932 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.859894 ( -0.419824 0.374506 )
Norm@50keV : 1.09999E-02 ( -0.00293989 0.00284905 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 51.32 using 59 PHA bins.
# Reduced chi-squared = 0.9003 for 57 degrees of freedom
# Null hypothesis probability = 6.872776e-01
Photon flux (15-150 keV) in 1 sec: 1.26247 ( -0.325229 0.331591 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.25419e-07 ( -3.00077e-08 3.00704e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 1.932 sec. to 2.932 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -0.791245 ( -3.92414 1.78684 )
Epeak [keV] : 103.359 ( -35.1728 -103.36 )
Norm@50keV : 5.27797E-02 ( -0.0527771 1.50389 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 49.24 using 59 PHA bins.
# Reduced chi-squared = 0.8794 for 56 degrees of freedom
# Null hypothesis probability = 7.264971e-01
Photon flux (15-150 keV) in 1 sec: 1.20323 ( -0.336308 0.33866 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.20506e-07 ( -3.46803e-08 3.2332e-08 ) ergs/cm2
Band function
Time interval is from 1.932 sec. to 2.932 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 1.65492 ( -3.25888 -1.37336 )
beta : -1.82063 ( 1.76968 1.04712 )
Epeak [keV] : 83.1689 ( -57.0995 82.992 )
Norm@50keV : 0.130716 ( -0.133657 11.4759 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 48.40 using 59 PHA bins.
# Reduced chi-squared = 0.8800 for 55 degrees of freedom
# Null hypothesis probability = 7.230540e-01
Photon flux (15-150 keV) in 1 sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 1.19643e-07 ( 0 0 ) ergs/cm2
Single BB
XSPEC: quit
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 23.5994 (-5.62735 9.0652)
R^2/D10^2 : 3.98432E-02 (-0.0254967 0.0562008)
(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 3.971e-09 2.059e-09
25- 50 2.185e-08 9.191e-09
50-150 9.079e-08 4.027e-08
15-150 1.166e-07 5.808e-08
Thermal bremsstrahlung (OTTB)
XSPEC12>exit
XSPEC: quit
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-59.2395 -200)
Norm : 5.35234 (-1.39454 1.39454)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.334e-08 8.125e-09
25- 50 2.566e-08 1.518e-08
50-150 5.629e-08 3.456e-08
15-150 9.529e-08 5.710e-08
Double BB
XSPEC12>exit
XSPEC: quit
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 18.4911 (-18.4915 10.9258)
R1^2/D10^2 : 6.99408E-02 (-0.0700005 -0.0700005)
kT2 [keV] : 195.452 (-196.126 -196.126)
R2^2/D10^2 : 1.37631E-04 (-0.000135515 0.0752406)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 0.000e+00 0.000e+00
25- 50 0.000e+00 0.000e+00
50-150 0.000e+00 0.000e+00
15-150 0.000e+00 0.000e+00
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: 1.34438 ( -0.169755 0.167442 )
Norm@50keV : 4.15214E-03 ( -0.000428818 0.000428811 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 59.12 using 59 PHA bins.
# Reduced chi-squared = 1.037 for 57 degrees of freedom
# Null hypothesis probability = 3.978653e-01
Photon flux (15-150 keV) in 39.46 sec: 0.499641 ( -0.0544128 0.0546141 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.60225e-06 ( -1.75256e-07 1.75978e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.345899 ( -0.908775 0.75015 )
Epeak [keV] : 88.6200 ( -20.1431 99.6311 )
Norm@50keV : 1.23976E-02 ( -0.0068358 0.0195706 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 53.71 using 59 PHA bins.
# Reduced chi-squared = 0.9591 for 56 degrees of freedom
# Null hypothesis probability = 5.620006e-01
Photon flux (15-150 keV) in 39.46 sec: 0.480514 ( -0.056594 0.056626 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.52523e-06 ( -1.87344e-07 1.8779e-07 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 4.84571 ( -13.7767 -4.84571 )
beta : -1.54826 ( -0.231441 0.21713 )
Epeak [keV] : 32.0389 ( -8.10456 5.90322 )
Norm@50keV : 71.1775 ( -7.27757 440.493 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 54.02 using 59 PHA bins.
# Reduced chi-squared = 0.9822 for 55 degrees of freedom
# Null hypothesis probability = 5.121075e-01
Photon flux (15-150 keV) in 39.46 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) = 3.66e-07
S(50-100 keV) = 5.76e-07
T90 vs. Hardness ratio plot
T90 = 31.8919999599457 sec.
Hardness ratio (energy fluence ratio) = 1.57377
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.61622
Count Ratio (50-100 keV) / (15-25 keV) = 1.64678
Mask shadow pattern
IMX = -6.140125512282825E-01, IMY = -5.380918370859334E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 8.192000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 8.192000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 8.192000
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:
-239.880000 -0.096000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
299.5661 35.1879 0.6 27.5 127.3 8.9674 18.0 1.4 Cyg X-1
307.9842 40.9194 3.6 18.8 128.3 1.1878 3.2 6.1 Cyg X-3
326.3968 38.3803 34.1 11.8 78.0 0.1182 0.3 11.2 Cyg X-2
285.7679 23.0760 2.7 44.6 127.2 7.2347 4.3 ------ UNKNOWN
342.2183 33.1584 3.3 18.0 27.4 1.1582 3.5 ------ UNKNOWN
240.5340 60.6845 2.6 49.1 -164.0 4.1145 4.4 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-0.096000 27.400000
28.120000 40.088000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
299.5853 35.2332 9.6 27.5 127.4 0.1243 1.2 1.9 Cyg X-1
308.1918 40.9745 5.0 18.6 128.2 0.1977 2.3 3.9 Cyg X-3
326.0141 38.2193 122.5 12.0 79.1 0.0076 0.1 9.6 Cyg X-2
284.0114 32.3269 0.8 39.2 138.8 2.5387 14.7 ------ UNKNOWN
339.9481 45.8920 2.6 6.5 -3.1 0.3151 4.5 ------ UNKNOWN
33.0049 46.7857 2.3 39.7 -54.0 0.7788 5.0 ------ UNKNOWN
39.6253 42.3874 2.1 46.0 -51.9 1.5351 5.3 ------ UNKNOWN
38.2700 27.5402 1.8 54.4 -35.8 2.5078 6.3 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
129.720600 508.120590
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.4402 35.3892 3.7 24.7 -162.0 1.6921 3.1 2.9 Her X-1
268.2701 -1.5991 0.0 37.0 119.3 0.5893 0.4 10.6 SW J1753.5-0127
288.8033 10.9479 49.1 21.8 79.8 0.1603 0.2 0.3 GRS 1915+105
299.5818 35.1884 0.5 13.3 -14.3 13.0376 23.9 0.9 Cyg X-1
308.1318 40.9818 2.3 21.1 -28.6 2.5980 4.9 2.0 Cyg X-3
326.3337 38.3998 12.7 34.7 -19.7 0.6319 0.9 9.0 Cyg X-2
283.9980 49.6364 3.3 17.3 -87.5 2.0255 3.5 ------ UNKNOWN
220.7158 31.4129 2.6 52.9 -160.3 7.1195 4.4 ------ UNKNOWN
298.4934 65.6147 2.3 34.5 -76.9 5.0348 5.0 ------ UNKNOWN
Plot creation:
Mon Jul 7 11:10:01 EDT 2025