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
245.1685 -15.7310 0.0209 34.2 159.0 2.7555 9.2 TRIG_01213829
------------------------------------------
Foreground time interval of the image:
-19.099 72.701 (delta_t = 91.800 [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
-61.520000 201.360000
202.000000 218.370000
219.000000 249.790000
251.000000 600.028000
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 6.61042 ( -0.309415 0.312903 )
Norm@50keV : 4.89268E-05 ( -1.22313e-05 1.54181e-05 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 86.62 using 59 PHA bins.
# Reduced chi-squared = 1.520 for 57 degrees of freedom
# Null hypothesis probability = 6.914752e-03
Photon flux (15-150 keV) in 659.1 sec: 0.374197 ( -0.030884 0.0312121 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.21194e-06 ( -5.52226e-07 5.56722e-07 ) ergs/cm2
Cutoff power-law model
Multiple GTIs in the spectrum
tstart tstop
-61.520000 201.360000
202.000000 218.370000
219.000000 249.790000
251.000000 600.028000
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.00000 ( )
Epeak [keV] : 50.0000 ( )
Norm@50keV : 8.75763E-04 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 599.74 using 59 PHA bins.
# Reduced chi-squared = 10.710 for 56 degrees of freedom
# Null hypothesis probability = 4.461138e-92
Photon flux (15-150 keV) in 659.1 sec: 0.343237 ( -0.037563 0.037 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.64887e-06 ( -6.68809e-07 6.52311e-07 ) ergs/cm2
Band function
Multiple GTIs in the spectrum
tstart tstop
-61.520000 201.360000
202.000000 218.370000
219.000000 249.790000
251.000000 600.028000
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 0.192300 ( -0.582974 0.582967 )
beta : -10.0000 ( 10 10 )
Epeak [keV] : 7.06724 ( -1.30909 5.30422 )
Norm@50keV : 13.7032 ( -13.7032 20871 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 65.90 using 59 PHA bins.
# Reduced chi-squared = 1.198 for 55 degrees of freedom
# Null hypothesis probability = 1.491585e-01
Photon flux (15-150 keV) in 659.1 sec: 0.400197 ( ) 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] : 2.53907 (-0.138347 0.151521)
R^2/D10^2 : 150.732 (-58.342 94.2702)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 65.06 using 59 PHA bins.
# Reduced chi-squared = 1.141 for 57 degrees of freedom
# Null hypothesis probability = 2.164705e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.095e-06 8.552e-07
25- 50 4.768e-07 8.282e-08
50-150 1.752e-10 1.018e-10
15-150 6.572e-06 9.148e-07
Thermal bremsstrahlung (OTTB)
XSPEC12>exit
XSPEC: quit
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 4.21908 (-0.317882 0.361688)
Norm : 159.409 (-52.7884 78.8116)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.345e-06 9.138e-07
25- 50 5.319e-07 9.185e-08
50-150 1.086e-09 6.136e-10
15-150 6.878e-06 9.227e-07
Double BB
XSPEC12>exit
XSPEC: quit
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 0.940360 (-1.02065 1.59278)
R1^2/D10^2 : 7.31492E+05 (-724683 -724683)
kT2 [keV] : 2.62166 (-0.176396 0.312435)
R2^2/D10^2 : 112.416 (-112.373 97.7729)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.092e-06 3.039e-06
25- 50 5.097e-07 2.688e-07
50-150 2.668e-10 1.987e-10
15-150 6.602e-06 3.277e-06
Peak spectrum fit
Power-law model
Time interval is from 38.232 sec. to 39.232 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.78826 ( -0.785606 0.950415 )
Norm@50keV : 4.55964E-03 ( -0.00207765 0.00176717 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 74.25 using 59 PHA bins.
# Reduced chi-squared = 1.303 for 57 degrees of freedom
# Null hypothesis probability = 6.205599e-02
Photon flux (15-150 keV) in 1 sec: 0.625498 ( -0.239105 0.240793 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.19945e-08 ( -1.71821e-08 1.74265e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 38.232 sec. to 39.232 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.61631 ( -2.66049 1.38851 )
Epeak [keV] : 207.880 ( )
Norm@50keV : 1.90650E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 73.51 using 59 PHA bins.
# Reduced chi-squared = 1.313 for 56 degrees of freedom
# Null hypothesis probability = 5.821284e-02
Photon flux (15-150 keV) in 1 sec: 0.628488 ( -0.240803 0.237369 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.19245e-08 ( -1.69642e-08 1.2661e-08 ) ergs/cm2
Band function
Time interval is from 38.232 sec. to 39.232 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.51159 ( 1.51165 1.51165 )
beta : -1.78753 ( 1.78839 0.785641 )
Epeak [keV] : 18.2618 ( -18.2981 -18.2981 )
Norm@50keV : 9.28905E-03 ( -0.00929201 0.175632 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 74.25 using 59 PHA bins.
# Reduced chi-squared = 1.350 for 55 degrees of freedom
# Null hypothesis probability = 4.283096e-02
Photon flux (15-150 keV) in 1 sec: ( ) 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] : 16.0570 (-5.86813 10.8331)
R^2/D10^2 : 4.96962E-02 (-0.0496151 0.203714)
(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 2.647e-09 1.788e-09
25- 50 1.117e-08 7.105e-09
50-150 2.016e-08 1.403e-08
15-150 3.398e-08 2.094e-08
Thermal bremsstrahlung (OTTB)
XSPEC12>exit
XSPEC: quit
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 173.818 (-155.676 -155.676)
Norm : 2.41334 (-0.948586 2.00646)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.076e-09 3.924e-09
25- 50 1.166e-08 7.220e-09
50-150 2.536e-08 1.527e-08
15-150 4.310e-08 2.564e-08
Double BB
XSPEC12>exit
XSPEC: quit
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 1.94547 (-0.934672 1.71603)
R1^2/D10^2 : 1039.71 (-1003.16 722797)
kT2 [keV] : 18.9592 (-6.71482 19.0629)
R2^2/D10^2 : 2.53398E-02 (-0.0225481 0.0808861)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 9.262e-09 5.145e-09
25- 50 8.781e-09 5.350e-09
50-150 2.272e-08 1.542e-08
15-150 4.077e-08 2.316e-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: 5.52652 ( -0.554998 0.591153 )
Norm@50keV : 1.33585E-04 ( -5.94159e-05 9.0619e-05 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 45.95 using 59 PHA bins.
# Reduced chi-squared = 0.8062 for 57 degrees of freedom
# Null hypothesis probability = 8.523964e-01
Photon flux (15-150 keV) in 91.8 sec: 0.343378 ( -0.0388139 0.0388666 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.72006e-07 ( -1.08381e-07 1.08598e-07 ) 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 : 2.76993E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 196.66 using 59 PHA bins.
# Reduced chi-squared = 3.5118 for 56 degrees of freedom
# Null hypothesis probability = 1.579851e-17
Photon flux (15-150 keV) in 91.8 sec: 0.340646 ( -0.040743 0.03933 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.55106e-07 ( -1.20046e-07 1.20304e-07 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -9.99994 ( 9.99994 9.99994 )
beta : -5.48628 ( -0.626798 0.523726 )
Epeak [keV] : 3.33680 ( -3.3368 -3.3368 )
Norm@50keV : 1.88896E-02 ( -0.0085816 0.0118418 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 45.97 using 59 PHA bins.
# Reduced chi-squared = 0.8358 for 55 degrees of freedom
# Null hypothesis probability = 8.020761e-01
Photon flux (15-150 keV) in 91.8 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) = 6.56e-07
S(50-100 keV) = 2.69e-08
T90 vs. Hardness ratio plot
T90 = 567.503999948502 sec.
Hardness ratio (energy fluence ratio) = 0.0410061
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 0.0496245
Count Ratio (50-100 keV) / (15-25 keV) = -0.00555198
Mask shadow pattern
IMX = -6.341929006961363E-01, IMY = -2.432227251517549E-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:
-19.099400 72.700630
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
170.3169 -60.6223 52.9 47.0 39.2 -0.1515 -0.2 0.1 Cen X-3
186.4475 -62.6887 14.1 39.1 40.1 -0.3795 -0.8 7.5 GX 301-2
245.0948 -15.7290 1.4 34.2 158.9 2.4220 8.1 8.5 Sco X-1
256.1715 -37.8754 1.7 10.9 179.2 1.2925 6.9 9.0 4U 1700-377
256.5310 -36.5761 13.8 12.2 -179.6 0.1595 0.8 10.3 GX 349+2
263.1394 -24.7697 56.1 24.7 -166.4 0.0396 0.2 7.3 GX 1+4
264.9366 -44.2917 0.0 7.8 -124.8 0.2258 1.1 12.6 4U 1735-44
268.2472 -1.3591 16.4 48.7 -165.9 -0.3162 -0.7 9.2 SW J1753.5-0127
270.1548 -25.2246 7.7 26.1 -151.9 0.3359 1.5 11.2 GX 5-1
270.4597 -25.8803 8.0 25.6 -150.8 0.3174 1.4 11.8 GRS 1758-258
273.9878 -14.0344 2668.7 37.9 -153.0 -0.0009 -0.0 1.1 GX 17+2
275.9193 -30.4555 9.3 23.9 -135.4 0.2695 1.2 5.3 H1820-303
284.9851 -24.8536 64.2 33.1 -128.4 -0.0490 -0.2 4.9 HT1900.1-2455
263.1474 -33.8730 4.8 15.9 -159.7 0.4778 2.4 8.2 GX 354-0
217.6009 -19.4137 2.7 42.4 117.5 4.6129 4.4 ------ UNKNOWN
237.9659 -42.3267 2.4 14.0 108.3 0.9251 4.8 ------ UNKNOWN
157.8332 -80.9805 3.4 43.2 10.4 1.3289 3.4 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
145.300600 201.360000
202.000000 218.370000
219.000000 249.790000
251.000000 620.970000
639.000000 645.680000
647.000000 652.940000
655.000000 659.820000
661.000000 661.330000
662.000000 665.200000
667.000000 671.620000
674.000000 732.120000
733.000000 734.670000
736.000000 738.070000
739.000000 769.980000
781.000000 817.750000
819.000000 820.310000
821.000000 870.570000
872.000000 872.250000
873.000000 873.280000
874.000000 876.140000
878.000000 878.790000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
245.1329 -15.6661 3.7 0.1 151.9 8.8830 3.1 9.0 Sco X-1
254.3325 35.2823 195.7 51.8 178.4 -0.4622 -0.1 7.1 Her X-1
256.1628 -37.7069 21.9 24.0 -33.0 -1.5683 -0.5 11.7 4U 1700-377
256.5766 -36.5772 4.5 23.1 -35.0 7.4882 2.5 11.5 GX 349+2
262.9579 -24.7838 20.0 18.9 -69.9 2.0196 0.6 3.6 GX 1+4
264.9261 -44.3684 8.2 33.1 -37.4 5.3614 1.4 9.3 4U 1735-44
268.4989 -1.6212 0.0 27.0 -130.5 -2.2342 -0.6 12.8 SW J1753.5-0127
270.3626 -25.1674 6.2 25.3 -75.3 -7.6509 -1.9 6.8 GX 5-1
270.3990 -25.7045 5.2 25.5 -74.2 -9.9476 -2.5 5.7 GRS 1758-258
274.1590 -14.0615 6.1 28.0 -100.8 7.9463 1.9 9.0 GX 17+2
276.0921 -30.4713 6.7 31.8 -68.2 -9.1298 -1.7 10.7 H1820-303
285.1113 -24.8820 5.7 38.4 -80.8 -21.6627 -2.0 4.7 HT1900.1-2455
262.9465 -33.9767 10.3 24.2 -49.3 3.6277 1.1 8.8 GX 354-0
210.9989 8.1627 2.9 41.5 111.7 50.4482 4.0 ------ UNKNOWN
206.1243 -60.5587 2.7 52.8 11.7 53.1377 4.3 ------ UNKNOWN
237.7952 1.7014 2.6 18.9 145.6 13.4977 4.4 ------ UNKNOWN
268.1579 22.8756 2.4 44.7 -160.4 25.4678 4.7 ------ UNKNOWN
270.9321 23.8958 2.4 47.0 -158.2 29.7591 4.8 ------ UNKNOWN
273.3614 -13.7067 2.5 27.3 -101.8 19.0398 4.7 ------ UNKNOWN
Plot creation:
Fri Feb 9 10:14:48 EST 2024