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
37.0572 +19.1807 0.0156 31.5 140.9 1.2254 12.4 TRIG_01278305
------------------------------------------
Foreground time interval of the image:
-0.220 35.637 (delta_t = 35.857 [sec])
Background time interval of the image:
-239.864 -0.220 (delta_t = 239.644 [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 4.096000
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 4.096000
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 4.096000
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
Time interval is from -0.220 sec. to 36.496 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.12065 ( -0.233549 0.252545 )
Norm@50keV : 1.84415E-03 ( -0.000320961 0.000312356 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 58.48 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.21e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 36.72 sec: 0.293124 ( -0.0370378 0.0370395 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.30479e-07 ( -9.66037e-08 9.92619e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.220 sec. to 36.496 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.54776 ( -1.21799 0.533844 )
Epeak [keV] : 31.0751 ( -27.6109 -31.0755 )
Norm@50keV : 4.08422E-03 ( -0.00408441 0.0189259 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 57.43 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.22e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 36.72 sec: 0.288179 ( -0.037814 0.03786 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.94166e-07 ( -1.07288e-07 1.15069e-07 ) ergs/cm2
Band function
Time interval is from -0.220 sec. to 36.496 sec.
XSPEC12>exit
XSPEC: quit
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 2.15924E-02 ( -0.0700144 -0.0700144 )
beta : -2.37008 ( 2.37214 0.396979 )
Epeak [keV] : 26.8825 ( -26.739 294.763 )
Norm@50keV : 5.93533E-02 ( -0.0778718 308.272 )
------------------------------------------------------------
Photon flux (15-150 keV) in 36.72 sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 6.06005e-07 ( -6.05748e-07 -1.00143e-07 ) ergs/cm2
Single BB
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 8.68486 (-1.26842 1.48798)
R^2/D10^2 : 0.233669 (-0.10795 0.202073)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 69.12 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.30e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.236e-07 2.805e-08
25- 50 2.482e-07 4.520e-08
50-150 8.479e-08 3.154e-08
15-150 4.565e-07 7.430e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 52.5862 (-15.7772 27.2794)
Norm : 1.62532 (-0.325015 0.439887)
------------------------------------------------------------
#Fit statistic : Chi-Squared 57.53 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.55e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.475e-07 2.464e-08
25- 50 2.157e-07 3.323e-08
50-150 2.194e-07 8.133e-08
15-150 5.826e-07 1.021e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.60414 (-1.69035 1.86199)
R1^2/D10^2 : 0.971179 (-0.617481 1.06068)
kT2 [keV] : 18.5460 (-6.43905 18.9849)
R2^2/D10^2 : 7.69467E-03 (-0.00664254 0.0317982)
------------------------------------------------------------
#Fit statistic : Chi-Squared 56.53 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.18e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.533e-07 8.109e-08
25- 50 2.058e-07 1.017e-07
50-150 2.369e-07 1.411e-07
15-150 5.960e-07 2.748e-07
Peak spectrum fit
Power-law model
Time interval is from 0.952 sec. to 1.952 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.29483 ( -0.362859 0.350473 )
Norm@50keV : 7.08324E-03 ( -0.00173125 0.0017312 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 59.29 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.92e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.844152 ( -0.212704 0.214112 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.00899e-08 ( -1.79765e-08 1.81793e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.952 sec. to 1.952 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -1.85466 ( -4.47303 2.25156 )
Epeak [keV] : 61.1504 ( -12.1643 33.1228 )
Norm@50keV : 0.262640 ( -0.264831 31.8513 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 52.47 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.09e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.792407 ( -0.214928 0.218183 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.10729e-08 ( -1.72748e-08 1.90009e-08 ) ergs/cm2
Band function
Time interval is from 0.952 sec. to 1.952 sec.
XSPEC12>exit
XSPEC: quit
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 1.79055 ( -1.32498 2.85709 )
beta : -9.99999 ( 9.99999 2.86685e-05 )
Epeak [keV] : 61.4682 ( -11.5111 32.9145 )
Norm@50keV : 0.244041 ( -0.0556069 4.96277 )
------------------------------------------------------------
Photon flux (15-150 keV) in 1 sec: 0.796797 ( 6.2032 -0.209213 ) 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] : 16.0430 (-3.08824 4.12245)
R^2/D10^2 : 9.09806E-02 (-0.0513022 0.101526)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 52.60 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.41e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.839e-09 2.016e-09
25- 50 2.041e-08 8.200e-09
50-150 3.675e-08 1.669e-08
15-150 6.200e-08 2.696e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.359 (-92.7836 -199.363)
Norm : 3.59285 (-0.877968 0.877935)
------------------------------------------------------------
#Fit statistic : Chi-Squared 59.24 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.94e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.947e-09 5.470e-09
25- 50 1.721e-08 9.965e-09
50-150 3.774e-08 2.220e-08
15-150 6.390e-08 3.879e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 200.000 (-200 -200)
R1^2/D10^2 : 2.36181E-05 (-2.36191e-05 -2.36191e-05)
kT2 [keV] : 15.2524 (-3.69102 4.7605)
R2^2/D10^2 : 0.103640 (-0.0628988 0.0849217)
------------------------------------------------------------
#Fit statistic : Chi-Squared 52.44 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.73e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.873e-09 1.791e-05
25- 50 2.038e-08 1.574e-04
50-150 3.686e-08 3.788e-03
15-150 6.212e-08 3.636e-03
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: 2.15998 ( -0.239117 0.259477 )
Norm@50keV : 1.81471E-03 ( -0.000327109 0.000318436 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 61.72 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.11e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 35.86 sec: 0.294252 ( -0.0375934 0.0375942 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.08645e-07 ( -9.48056e-08 9.75349e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.55189 ( -1.29081 0.770856 )
Epeak [keV] : 28.5742 ( -25.6928 -28.5754 )
Norm@50keV : 4.25147E-03 ( -0.00425201 0.022863 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 60.65 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.12e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 35.86 sec: 0.289072 ( -0.038316 0.038458 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.71296e-07 ( -1.04987e-07 1.14063e-07 ) ergs/cm2
Band function
XSPEC12>exit
XSPEC: quit
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 0.176092 ( 0.622011 0.622011 )
beta : -2.43007 ( 2.412 0.40886 )
Epeak [keV] : 26.3413 ( -26.4111 16.1007 )
Norm@50keV : 8.10756E-02 ( -0.0798278 360.619 )
------------------------------------------------------------
Photon flux (15-150 keV) in 35.86 sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 5.85207e-07 ( -5.84955e-07 -1.00236e-07 ) ergs/cm2
S(25-50 keV) vs. S(50-100 keV) plot
S(25-50 keV) = 1.96e-07
S(50-100 keV) = 1.80e-07
T90 vs. Hardness ratio plot
T90 = 34.1920000314713 sec.
Hardness ratio (energy fluence ratio) = 0.918367
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.03391
Count Ratio (50-100 keV) / (15-25 keV) = 0.492309
Mask shadow pattern
IMX = -4.762319146990416E-01, IMY = -3.867192714437972E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 4.096000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 4.096000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 4.096000
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:
-239.864000 -0.220000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
326.1769 38.3214 188.4 34.3 -68.0 0.0309 0.1 0.2 Cyg X-2
267.1219 64.9890 3.4 58.1 -16.2 3.8276 3.3 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-0.220000 35.636600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
326.0260 38.3857 39.4 34.4 -67.8 -0.0345 -0.3 7.9 Cyg X-2
50.7751 11.3303 2.3 46.0 132.6 1.5168 5.1 ------ UNKNOWN
37.0572 19.1807 0.9 31.5 140.9 1.2250 12.4 ------ UNKNOWN
352.5245 30.8172 2.5 18.7 -107.7 0.3512 4.6 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
110.036600 931.997200
939.136000 939.576000
941.136000 942.836600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
76.4163 45.9411 2.5 41.9 57.7 13.6794 4.6 ------ UNKNOWN
70.0965 31.5032 3.2 32.1 77.3 6.0642 3.6 ------ UNKNOWN
65.8006 34.4831 3.0 29.7 69.5 5.8667 3.8 ------ UNKNOWN
60.8456 19.1458 3.3 22.4 102.6 4.0064 3.5 ------ UNKNOWN
47.1083 11.6282 3.4 12.3 143.0 2.7992 3.4 ------ UNKNOWN
10.0484 14.8729 2.8 26.2 -78.9 4.0680 4.1 ------ UNKNOWN
1.5284 13.9017 2.8 34.4 -76.9 6.6492 4.2 ------ UNKNOWN
10.2777 -21.0416 2.1 48.0 -129.1 20.4384 5.4 ------ UNKNOWN
Plot creation:
Thu Jan 2 16:28:38 EST 2025