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
274.1396 +74.6943 0.0085 30.0 69.2 1.2608 22.7 TRIG_01277428
------------------------------------------
Foreground time interval of the image:
-2.616 3.380 (delta_t = 5.996 [sec])
Background time interval of the image:
-239.752 -2.616 (delta_t = 237.136 [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 1.024000
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 1.024000
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 1.024000
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 -2.616 sec. to 3.380 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.69867 ( -0.113979 0.11584 )
Norm@50keV : 1.31473E-02 ( -0.000950409 0.000944974 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 55.86 using 59 PHA bins.
# Reduced chi-squared = 0.9800 for 57 degrees of freedom
# Null hypothesis probability = 5.179617e-01
Photon flux (15-150 keV) in 5.996 sec: 1.74530 ( -0.122739 0.122893 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.29959e-07 ( -5.49386e-08 5.52124e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -2.616 sec. to 3.380 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.928936 ( -0.532837 0.476878 )
Epeak [keV] : 68.2569 ( -11.6996 33.4418 )
Norm@50keV : 3.27563E-02 ( -0.0138832 0.027953 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 47.78 using 59 PHA bins.
# Reduced chi-squared = 0.8533 for 56 degrees of freedom
# Null hypothesis probability = 7.746115e-01
Photon flux (15-150 keV) in 5.996 sec: 1.69534 ( -0.12655 0.12658 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.9839e-07 ( -5.81672e-08 5.85929e-08 ) ergs/cm2
Band function
Time interval is from -2.616 sec. to 3.380 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.929199 ( -0.449474 0.545646 )
beta : -10.0000 ( 10 1.77636e-15 )
Epeak [keV] : 68.2539 ( -11.7013 33.3041 )
Norm@50keV : 3.27436E-02 ( -0.0138679 0.0279839 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 47.78 using 59 PHA bins.
# Reduced chi-squared = 0.8688 for 55 degrees of freedom
# Null hypothesis probability = 7.441950e-01
Photon flux (15-150 keV) in 5.996 sec: 1.70204 ( 5.29796 -0.13194 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.98864e-07 ( -6.98822e-07 -5.90846e-08 ) ergs/cm2
Single BB
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 13.7065 (-1.07557 1.16918)
R^2/D10^2 : 0.268826 (-0.0699359 0.0939123)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 85.52 using 59 PHA bins.
# Reduced chi-squared = 1.500 for 57 degrees of freedom
# Null hypothesis probability = 8.588702e-03
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.408e-08 8.676e-09
25- 50 2.333e-07 1.919e-08
50-150 2.854e-07 4.158e-08
15-150 5.828e-07 4.890e-08
Thermal bremsstrahlung (OTTB)
XSPEC12>exit
XSPEC: quit
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 134.635 (-33.575 47.279)
Norm : 7.28242 (-0.594519 0.729269)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.131e-07 1.091e-08
25- 50 2.061e-07 2.219e-08
50-150 3.884e-07 1.328e-07
15-150 7.076e-07 1.587e-07
Double BB
XSPEC12>exit
XSPEC: quit
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.03606 (-1.44638 1.72145)
R1^2/D10^2 : 2.89227 (-1.6377 5.31722)
kT2 [keV] : 19.9983 (-2.9392 4.63504)
R2^2/D10^2 : 5.34578E-02 (-0.0309958 0.0497977)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.094e-07 4.142e-08
25- 50 2.086e-07 4.722e-08
50-150 3.730e-07 1.074e-07
15-150 6.910e-07 1.886e-07
Peak spectrum fit
Power-law model
Time interval is from -0.056 sec. to 0.944 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.59516 ( -0.12505 0.127357 )
Norm@50keV : 3.15245E-02 ( -0.00268839 0.00267801 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 63.52 using 59 PHA bins.
# Reduced chi-squared = 1.114 for 57 degrees of freedom
# Null hypothesis probability = 2.576229e-01
Photon flux (15-150 keV) in 1 sec: 4.04499 ( -0.341158 0.341471 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.94998e-07 ( -2.65478e-08 2.6651e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.056 sec. to 0.944 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.232562 ( -0.720353 0.619587 )
Epeak [keV] : 65.6594 ( -8.59534 15.7125 )
Norm@50keV : 0.153985 ( -0.0777631 0.193792 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 47.29 using 59 PHA bins.
# Reduced chi-squared = 0.8445 for 56 degrees of freedom
# Null hypothesis probability = 7.899202e-01
Photon flux (15-150 keV) in 1 sec: 3.93233 ( -0.34675 0.34666 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.8242e-07 ( -2.7333e-08 2.755e-08 ) ergs/cm2
Band function
Time interval is from -0.056 sec. to 0.944 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.232421 ( -0.42699 1.34061 )
beta : -10.0000 ( 10 1.77636e-15 )
Epeak [keV] : 65.6459 ( -8.60234 15.7147 )
Norm@50keV : 0.154024 ( -0.0778386 0.194491 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 47.29 using 59 PHA bins.
# Reduced chi-squared = 0.8598 for 55 degrees of freedom
# Null hypothesis probability = 7.605855e-01
Photon flux (15-150 keV) in 1 sec: 3.96444 ( 3.03556 -0.39033 ) ph/cm2/s
Energy fluence (15-150 keV) : 0 ( 0 0 ) ergs/cm2
Single BB
XSPEC: quit
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 14.6590 (-1.18639 1.29563)
R^2/D10^2 : 0.536504 (-0.142857 0.190803)
(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 2.422e-08 3.515e-09
25- 50 9.420e-08 9.335e-09
50-150 1.363e-07 2.095e-08
15-150 2.547e-07 2.575e-08
Thermal bremsstrahlung (OTTB)
XSPEC12>exit
XSPEC: quit
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 165.151 (-45.3147 -162.422)
Norm : 17.0347 (-1.53493 1.64399)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.336e-08 4.805e-09
25- 50 8.146e-08 1.462e-08
50-150 1.671e-07 6.519e-08
15-150 2.919e-07 8.780e-08
Double BB
XSPEC12>exit
XSPEC: quit
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.03145 (-2.45281 5.67619)
R1^2/D10^2 : 8.41452 (-7.34079 195.927)
kT2 [keV] : 17.3181 (-2.28678 9.63953)
R2^2/D10^2 : 0.260488 (-0.229405 0.20571)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.681e-08 1.571e-08
25- 50 8.498e-08 2.283e-08
50-150 1.536e-07 4.183e-08
15-150 2.754e-07 6.670e-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: 1.69867 ( -0.113979 0.11584 )
Norm@50keV : 1.31473E-02 ( -0.000950409 0.000944974 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 55.86 using 59 PHA bins.
# Reduced chi-squared = 0.9800 for 57 degrees of freedom
# Null hypothesis probability = 5.179617e-01
Photon flux (15-150 keV) in 5.996 sec: 1.74530 ( -0.122739 0.122893 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.29959e-07 ( -5.49386e-08 5.52124e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.928936 ( -0.532837 0.476878 )
Epeak [keV] : 68.2569 ( -11.6996 33.4418 )
Norm@50keV : 3.27563E-02 ( -0.0138832 0.027953 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 47.78 using 59 PHA bins.
# Reduced chi-squared = 0.8533 for 56 degrees of freedom
# Null hypothesis probability = 7.746115e-01
Photon flux (15-150 keV) in 5.996 sec: 1.69534 ( -0.12655 0.12658 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.9839e-07 ( -5.81672e-08 5.85929e-08 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.929217 ( -0.426962 0.561427 )
beta : -10.0000 ( 10 20 )
Epeak [keV] : 68.2536 ( -11.701 33.3043 )
Norm@50keV : 3.27432E-02 ( -0.0138675 0.0279844 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 47.78 using 59 PHA bins.
# Reduced chi-squared = 0.8688 for 55 degrees of freedom
# Null hypothesis probability = 7.441950e-01
Photon flux (15-150 keV) in 5.996 sec: 1.70204 ( 5.29796 -0.13194 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.98864e-07 ( -6.98822e-07 -5.90846e-08 ) ergs/cm2
S(25-50 keV) vs. S(50-100 keV) plot
S(25-50 keV) = 1.97e-07
S(50-100 keV) = 2.43e-07
T90 vs. Hardness ratio plot
T90 = 5.0479998588562 sec.
Hardness ratio (energy fluence ratio) = 1.2335
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.46257
Count Ratio (50-100 keV) / (15-25 keV) = 0.988905
Mask shadow pattern
IMX = 2.049574936706344E-01, IMY = -5.395893732863686E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.024000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.024000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.024000
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:
-239.752000 -2.616000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.4555 35.3537 3.8 34.1 -11.9 1.2220 3.0 0.7 Her X-1
288.9228 10.9640 6.9 36.3 -83.8 -1.3200 -1.7 7.4 GRS 1915+105
299.6252 35.2326 2.2 11.3 -106.3 1.6965 5.3 2.5 Cyg X-1
308.1204 41.0329 2.3 9.2 -156.1 1.5295 4.9 4.8 Cyg X-3
325.9190 38.2689 0.0 22.2 -177.0 -0.7000 -2.1 12.3 Cyg X-2
224.1432 31.4854 3.4 57.0 4.2 4.3869 3.4 ------ UNKNOWN
329.2456 37.3338 3.0 24.9 -178.4 1.2384 3.8 ------ UNKNOWN
271.5645 7.6600 2.8 44.9 -60.2 5.9673 4.1 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-2.616000 3.380000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.2458 35.3690 25.5 34.2 -11.7 0.0178 0.5 10.5 Her X-1
288.6729 10.9011 5.6 36.4 -83.4 0.1417 2.1 7.9 GRS 1915+105
299.4442 35.3733 0.0 11.2 -105.6 0.0471 1.4 12.5 Cyg X-1
308.2237 40.7749 5.1 9.5 -155.2 -0.0687 -2.2 11.8 Cyg X-3
326.1671 38.4805 4.8 22.3 -177.8 0.0774 2.4 9.5 Cyg X-2
274.1397 74.6943 0.5 30.0 69.2 1.2608 22.7 ------ UNKNOWN
271.6762 7.5986 2.8 44.9 -60.4 0.4510 4.2 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
Plot creation:
Sun Dec 29 22:27:56 EST 2024