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
244.8298 -15.6230 0.0170 18.3 119.1 2.0815 11.2 TRIG_01212373
------------------------------------------
Foreground time interval of the image:
0.000 19.530 (delta_t = 19.530 [sec])
21.000 64.000 (delta_t = 43.000 [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 19.530000
21.000000 64.000000
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 5.32435 ( -0.527853 0.567889 )
Norm@50keV : 1.47971E-04 ( -6.4393e-05 9.51488e-05 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 46.03 using 59 PHA bins.
# Reduced chi-squared = 0.8076 for 57 degrees of freedom
# Null hypothesis probability = 8.503322e-01
Photon flux (15-150 keV) in 62.53 sec: 0.312117 ( -0.0359973 0.0360097 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.09797e-07 ( -7.14937e-08 7.18376e-08 ) ergs/cm2
Cutoff power-law model
Multiple GTIs in the spectrum
tstart tstop
0.000000 19.530000
21.000000 64.000000
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.00000 ( )
Epeak [keV] : 50.0000 ( )
Norm@50keV : 2.56383E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 192.71 using 59 PHA bins.
# Reduced chi-squared = 3.4413 for 56 degrees of freedom
# Null hypothesis probability = 6.626208e-17
Photon flux (15-150 keV) in 62.53 sec: 0.308820 ( -0.03636 0.036355 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.88702e-07 ( -7.03888e-08 7.27524e-08 ) ergs/cm2
Band function
Multiple GTIs in the spectrum
tstart tstop
0.000000 19.530000
21.000000 64.000000
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -6.89127 ( 4.34321 6.89127 )
beta : -5.39615 ( -0.514724 0.58968 )
Epeak [keV] : 384.200 ( -384.2 -384.2 )
Norm@50keV : 1.87123E-02 ( -0.00786437 0.0139385 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 46.08 using 59 PHA bins.
# Reduced chi-squared = 0.8379 for 55 degrees of freedom
# Null hypothesis probability = 7.985627e-01
Photon flux (15-150 keV) in 62.53 sec: 0.212759 ( ) 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] : 2.77362 (-0.294894 0.344323)
R^2/D10^2 : 72.9756 (-40.6804 93.6721)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 46.21 using 59 PHA bins.
# Reduced chi-squared = 0.8106 for 57 degrees of freedom
# Null hypothesis probability = 8.459961e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.153e-07 1.785e-07
25- 50 5.663e-08 2.114e-08
50-150 4.698e-11 4.284e-11
15-150 5.719e-07 1.726e-07
Thermal bremsstrahlung (OTTB)
XSPEC12>exit
XSPEC: quit
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 5.28817 (-0.84715 1.09919)
Norm : 58.4376 (-27.7858 56.0878)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.109e-07 1.564e-07
25- 50 7.311e-08 2.583e-08
50-150 4.991e-10 4.090e-10
15-150 5.845e-07 1.523e-07
Double BB
XSPEC12>exit
XSPEC: quit
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 4.37163 (-4.39792 195.596)
R1^2/D10^2 : 1.57493 (-1.47469 126.268)
kT2 [keV] : 2.28284 (-2.28259 13.7247)
R2^2/D10^2 : 218.767 (-215.251 -215.251)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.746e-07 2.782e-07
25- 50 8.465e-08 4.734e-08
50-150 2.172e-10 1.545e-10
15-150 5.595e-07 3.173e-07
Peak spectrum fit
Power-law model
Time interval is from 21.000 sec. to 64.000 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 5.32435 ( -0.527853 0.567889 )
Norm@50keV : 1.47971E-04 ( -6.4393e-05 9.51488e-05 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 46.03 using 59 PHA bins.
# Reduced chi-squared = 0.8076 for 57 degrees of freedom
# Null hypothesis probability = 8.503322e-01
Photon flux (15-150 keV) in 62.53 sec: 0.312117 ( -0.0359973 0.0360097 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.09797e-07 ( -7.14937e-08 7.18376e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 21.000 sec. to 64.000 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.00000 ( )
Epeak [keV] : 50.0000 ( )
Norm@50keV : 2.56383E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 192.71 using 59 PHA bins.
# Reduced chi-squared = 3.4413 for 56 degrees of freedom
# Null hypothesis probability = 6.626208e-17
Photon flux (15-150 keV) in 62.53 sec: 0.308820 ( -0.03636 0.036355 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.88702e-07 ( -7.03888e-08 7.27524e-08 ) ergs/cm2
Band function
Time interval is from 21.000 sec. to 64.000 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -6.89127 ( 4.34321 6.89127 )
beta : -5.39615 ( -0.514724 0.58968 )
Epeak [keV] : 384.200 ( -384.2 -384.2 )
Norm@50keV : 1.87123E-02 ( -0.00786437 0.0139385 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 46.08 using 59 PHA bins.
# Reduced chi-squared = 0.8379 for 55 degrees of freedom
# Null hypothesis probability = 7.985627e-01
Photon flux (15-150 keV) in 62.53 sec: 0.212759 ( ) 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] : 2.77362 (-0.294894 0.344323)
R^2/D10^2 : 72.9756 (-40.6804 93.6721)
(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 5.153e-07 1.656e-07
25- 50 5.663e-08 2.174e-08
50-150 4.698e-11 4.248e-11
15-150 5.719e-07 1.889e-07
Thermal bremsstrahlung (OTTB)
XSPEC12>exit
XSPEC: quit
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 5.28817 (-0.84715 1.09919)
Norm : 58.4376 (-27.7858 56.0878)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.109e-07 1.450e-07
25- 50 7.311e-08 2.630e-08
50-150 4.991e-10 4.133e-10
15-150 5.845e-07 1.519e-07
Double BB
XSPEC12>exit
XSPEC: quit
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 4.37163 (-4.39792 195.596)
R1^2/D10^2 : 1.57493 (-1.47469 126.268)
kT2 [keV] : 2.28284 (-2.28259 14.933)
R2^2/D10^2 : 218.767 (-215.251 -215.251)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.746e-07 2.795e-07
25- 50 8.465e-08 5.093e-08
50-150 2.172e-10 1.403e-10
15-150 5.595e-07 3.227e-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: 5.32435 ( -0.527853 0.567889 )
Norm@50keV : 1.47971E-04 ( -6.4393e-05 9.51488e-05 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 46.03 using 59 PHA bins.
# Reduced chi-squared = 0.8076 for 57 degrees of freedom
# Null hypothesis probability = 8.503322e-01
Photon flux (15-150 keV) in 62.53 sec: 0.312117 ( -0.0359973 0.0360097 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.09797e-07 ( -7.14937e-08 7.18376e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.00000 ( )
Epeak [keV] : 50.0000 ( )
Norm@50keV : 2.56383E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 192.71 using 59 PHA bins.
# Reduced chi-squared = 3.4413 for 56 degrees of freedom
# Null hypothesis probability = 6.626208e-17
Photon flux (15-150 keV) in 62.53 sec: 0.308820 ( -0.03636 0.036355 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.88702e-07 ( -7.03888e-08 7.27524e-08 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -6.89127 ( 4.34321 6.89127 )
beta : -5.39615 ( -0.514724 0.58968 )
Epeak [keV] : 384.200 ( -384.2 -384.2 )
Norm@50keV : 1.87123E-02 ( -0.00786437 0.0139385 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 46.08 using 59 PHA bins.
# Reduced chi-squared = 0.8379 for 55 degrees of freedom
# Null hypothesis probability = 7.985627e-01
Photon flux (15-150 keV) in 62.53 sec: 0.212759 ( ) 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) = 1.01e-07
S(50-100 keV) = 1.00e-08
T90 vs. Hardness ratio plot
T90 = 64 sec.
Hardness ratio (energy fluence ratio) = 0.0990099
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 0.144022
Count Ratio (50-100 keV) / (15-25 keV) = 0.00655829
Mask shadow pattern
IMX = -1.602825588680999E-01, IMY = -2.882197296406623E-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:
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
0.000000 19.530000
21.000000 64.000000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
244.8299 -15.6230 1.0 18.3 119.1 2.0816 11.2 8.7 Sco X-1
255.9303 -37.7883 0.7 10.0 3.7 2.2286 15.4 4.3 4U 1700-377
256.3765 -36.5158 6.3 8.7 3.8 0.2756 1.8 6.2 GX 349+2
263.0213 -24.7569 322.6 4.8 -145.0 -0.0055 -0.0 1.0 GX 1+4
264.5743 -44.2851 0.0 16.7 -24.8 0.2526 1.8 12.3 4U 1735-44
268.2575 -1.2815 0.0 28.2 -171.8 0.1694 1.0 12.2 SW J1753.5-0127
270.1352 -24.9321 5.4 10.3 -116.9 0.3049 2.1 12.0 GX 5-1
270.2473 -25.6289 2.8 10.2 -113.0 0.6078 4.2 7.5 GRS 1758-258
273.9661 -13.8830 4.8 19.8 -144.3 0.3643 2.4 9.5 GX 17+2
276.1057 -30.2299 37.2 14.9 -89.1 -0.0452 -0.3 12.5 H1820-303
285.1970 -24.7940 5.3 23.5 -103.4 0.3505 2.2 11.6 HT1900.1-2455
288.6817 10.9545 9.0 48.4 -151.0 0.4164 1.3 6.9 GRS 1915+105
262.7889 -33.9386 17.2 6.6 -38.4 0.0980 0.7 11.8 GX 354-0
201.8117 -51.1460 3.2 48.3 33.8 2.2291 3.7 ------ UNKNOWN
242.9116 -29.5207 2.9 14.3 69.3 0.6703 4.0 ------ UNKNOWN
227.6144 -71.6343 2.5 46.8 1.8 1.4567 4.7 ------ UNKNOWN
290.5902 1.4738 2.2 42.3 -140.5 1.3589 5.3 ------ UNKNOWN
300.1460 -50.5842 2.7 38.1 -53.7 1.0822 4.3 ------ UNKNOWN
310.4081 -45.1524 2.7 43.6 -64.1 2.3846 4.3 ------ UNKNOWN
301.3101 -6.5737 3.2 45.3 -121.6 2.2095 3.6 ------ UNKNOWN
300.2755 -0.3983 2.4 48.1 -129.3 3.0336 4.8 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
126.200600 243.036200
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
244.8294 -15.5988 0.7 0.1 -131.5 3.8547 15.4 9.0 Sco X-1
254.5361 35.3482 7.0 51.8 178.1 1.1430 1.6 3.9 Her X-1
255.8805 -37.7714 0.6 24.2 -33.9 4.8727 18.5 6.7 4U 1700-377
256.2935 -36.3532 3.6 23.1 -36.3 0.8194 3.2 8.0 GX 349+2
262.8267 -24.8749 0.0 19.3 -70.5 0.2182 0.8 12.6 GX 1+4
264.7562 -44.5619 7.4 33.5 -38.3 0.4880 1.6 6.7 4U 1735-44
268.5102 -1.4692 5.5 27.4 -131.0 0.6265 2.1 8.6 SW J1753.5-0127
270.4397 -25.1871 5.3 25.8 -76.2 -0.6987 -2.2 10.6 GX 5-1
270.1872 -25.7578 4.6 25.8 -74.8 0.8221 2.6 6.3 GRS 1758-258
273.8601 -13.8878 0.0 28.2 -101.8 0.6896 2.2 12.3 GX 17+2
275.7530 -30.3870 8.8 32.0 -69.1 0.4982 1.3 9.0 H1820-303
285.0645 -24.9297 9.9 38.8 -81.6 0.8009 1.2 1.6 HT1900.1-2455
262.8128 -33.8397 4.6 24.4 -50.6 0.6754 2.5 8.8 GX 354-0
287.8543 -37.1807 3.0 43.7 -64.1 3.3460 3.8 ------ UNKNOWN
Plot creation:
Fri Feb 2 19:43:50 EST 2024