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
229.7604 -57.3863 0.0340 29.3 -156.8 0.9603 5.7 TRIG_01218645
------------------------------------------
Foreground time interval of the image:
0.000 64.000 (delta_t = 64.000 [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
Time interval is from 0.000 sec. to 64.000 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.65636 ( -0.2961 0.334611 )
Norm@50keV : 7.57036E-04 ( -0.000195187 0.000198762 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 72.25 using 59 PHA bins.
# Reduced chi-squared = 1.268 for 57 degrees of freedom
# Null hypothesis probability = 8.391097e-02
Photon flux (15-150 keV) in 64 sec: 0.164180 ( -0.024535 0.0245454 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.07784e-07 ( -9.21197e-08 9.65171e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.000 sec. to 64.000 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -0.340946 ( -4.22262 1.7206 )
Epeak [keV] : 24.0115 ( -20.1634 5.98579 )
Norm@50keV : 8.57976E-02 ( -0.0840624 32.8176 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 65.51 using 59 PHA bins.
# Reduced chi-squared = 1.170 for 56 degrees of freedom
# Null hypothesis probability = 1.802460e-01
Photon flux (15-150 keV) in 64 sec: 0.159274 ( -0.024212 0.02432 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.33467e-07 ( -7.77062e-08 9.34752e-08 ) ergs/cm2
Band function
Time interval is from 0.000 sec. to 64.000 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 1.80712 ( -3.3995 -1.7413 )
beta : -3.98967 ( 3.96381 1.12884 )
Epeak [keV] : 24.4874 ( -4.89228 4.03635 )
Norm@50keV : 1.07016 ( -0.796657 152.946 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 64.84 using 59 PHA bins.
# Reduced chi-squared = 1.179 for 55 degrees of freedom
# Null hypothesis probability = 1.710600e-01
Photon flux (15-150 keV) in 64 sec: 0.161010 ( 6.83899 -0.025419 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.46147e-07 ( 0 0 ) ergs/cm2
Single BB
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 6.47717 (-0.86039 0.990415)
R^2/D10^2 : 0.451271 (-0.207528 0.386067)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 66.07 using 59 PHA bins.
# Reduced chi-squared = 1.159 for 57 degrees of freedom
# Null hypothesis probability = 1.921504e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.783e-07 4.445e-08
25- 50 2.091e-07 5.341e-08
50-150 2.594e-08 1.379e-08
15-150 4.133e-07 9.824e-08
Thermal bremsstrahlung (OTTB)
XSPEC12>exit
XSPEC: quit
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 25.6110 (-6.78367 10.0187)
Norm : 1.55899 (-0.433992 0.640874)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.856e-07 3.354e-08
25- 50 1.932e-07 4.432e-08
50-150 8.507e-08 4.880e-08
15-150 4.638e-07 9.651e-08
Double BB
XSPEC12>exit
XSPEC: quit
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.72742 (-5.56226 1.59241)
R1^2/D10^2 : 0.663487 (-0.371266 -0.654527)
kT2 [keV] : 14.7934 (-14.8504 -14.8504)
R2^2/D10^2 : 3.87234E-03 (-0.00373835 0.683329)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.847e-07 1.093e-07
25- 50 1.995e-07 1.214e-07
50-150 7.334e-08 3.917e-08
15-150 4.575e-07 2.518e-07
Peak spectrum fit
Power-law model
Time interval is from 0.000 sec. to 64.000 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.65636 ( -0.2961 0.334611 )
Norm@50keV : 7.57036E-04 ( -0.000195187 0.000198762 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 72.25 using 59 PHA bins.
# Reduced chi-squared = 1.268 for 57 degrees of freedom
# Null hypothesis probability = 8.391097e-02
Photon flux (15-150 keV) in 64 sec: 0.164180 ( -0.024535 0.0245454 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.07784e-07 ( -9.21197e-08 9.65171e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.000 sec. to 64.000 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -0.340946 ( -4.22262 1.7206 )
Epeak [keV] : 24.0115 ( -20.1634 5.98579 )
Norm@50keV : 8.57976E-02 ( -0.0840624 32.8176 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 65.51 using 59 PHA bins.
# Reduced chi-squared = 1.170 for 56 degrees of freedom
# Null hypothesis probability = 1.802460e-01
Photon flux (15-150 keV) in 64 sec: 0.159274 ( -0.024212 0.02432 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.33467e-07 ( -7.77062e-08 9.34752e-08 ) ergs/cm2
Band function
Time interval is from 0.000 sec. to 64.000 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 1.80712 ( -3.3995 -1.7413 )
beta : -3.98967 ( 3.96381 1.12884 )
Epeak [keV] : 24.4874 ( -4.89228 4.03635 )
Norm@50keV : 1.07016 ( -0.796657 152.946 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 64.84 using 59 PHA bins.
# Reduced chi-squared = 1.179 for 55 degrees of freedom
# Null hypothesis probability = 1.710600e-01
Photon flux (15-150 keV) in 64 sec: 0.161010 ( 6.83899 -0.025419 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.46147e-07 ( 0 0 ) ergs/cm2
Single BB
XSPEC: quit
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 6.47717 (-0.86039 0.990415)
R^2/D10^2 : 0.451271 (-0.207528 0.386067)
(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 1.783e-07 3.930e-08
25- 50 2.091e-07 5.379e-08
50-150 2.594e-08 1.476e-08
15-150 4.133e-07 9.994e-08
Thermal bremsstrahlung (OTTB)
XSPEC12>exit
XSPEC: quit
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 25.6110 (-6.78367 10.0187)
Norm : 1.55899 (-0.433992 0.640874)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.856e-07 3.402e-08
25- 50 1.932e-07 4.954e-08
50-150 8.507e-08 4.395e-08
15-150 4.638e-07 1.040e-07
Double BB
XSPEC12>exit
XSPEC: quit
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.72742 (-5.56226 1.59101)
R1^2/D10^2 : 0.663487 (-0.371266 -0.654527)
kT2 [keV] : 14.7934 (-14.8504 -14.8504)
R2^2/D10^2 : 3.87234E-03 (-0.00373835 0.683329)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.847e-07 1.073e-07
25- 50 1.995e-07 1.258e-07
50-150 7.334e-08 4.330e-08
15-150 4.575e-07 2.664e-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: 2.65636 ( -0.2961 0.334611 )
Norm@50keV : 7.57036E-04 ( -0.000195187 0.000198762 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 72.25 using 59 PHA bins.
# Reduced chi-squared = 1.268 for 57 degrees of freedom
# Null hypothesis probability = 8.391097e-02
Photon flux (15-150 keV) in 64 sec: 0.164180 ( -0.024535 0.0245454 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.07784e-07 ( -9.21197e-08 9.65171e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -0.340946 ( -4.22262 1.7206 )
Epeak [keV] : 24.0115 ( -20.1634 5.98579 )
Norm@50keV : 8.57976E-02 ( -0.0840624 32.8176 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 65.51 using 59 PHA bins.
# Reduced chi-squared = 1.170 for 56 degrees of freedom
# Null hypothesis probability = 1.802460e-01
Photon flux (15-150 keV) in 64 sec: 0.159274 ( -0.024212 0.02432 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.33467e-07 ( -7.77062e-08 9.34752e-08 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 1.80712 ( -3.3995 -1.7413 )
beta : -3.98967 ( 3.96381 1.12884 )
Epeak [keV] : 24.4874 ( -4.89228 4.03635 )
Norm@50keV : 1.07016 ( -0.796657 152.946 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 64.84 using 59 PHA bins.
# Reduced chi-squared = 1.179 for 55 degrees of freedom
# Null hypothesis probability = 1.710600e-01
Photon flux (15-150 keV) in 64 sec: 0.161010 ( 6.83899 -0.025419 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.46147e-07 ( 0 0 ) ergs/cm2
S(25-50 keV) vs. S(50-100 keV) plot
S(25-50 keV) = 1.70e-07
S(50-100 keV) = 1.08e-07
T90 vs. Hardness ratio plot
T90 = 64 sec.
Hardness ratio (energy fluence ratio) = 0.635294
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 0.810045
Count Ratio (50-100 keV) / (15-25 keV) = 0.141993
Mask shadow pattern
IMX = -5.160221169952246E-01, IMY = 2.212746356637942E-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 64.000000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.4988 -40.4022 6.9 30.0 34.7 0.3267 1.7 9.3 Vela X-1
170.4511 -60.5972 9.7 1.4 99.7 0.1706 1.2 4.3 Cen X-3
186.6376 -62.7642 0.5 7.6 -162.2 3.1437 23.0 0.6 GX 301-2
255.9779 -37.7959 7.1 55.4 -158.5 0.9941 1.6 2.9 4U 1700-377
256.5154 -36.4888 8.4 56.7 -158.9 -0.8736 -1.4 5.5 GX 349+2
264.5327 -44.2711 0.0 53.8 -147.4 -1.9851 -3.1 14.0 4U 1735-44
182.1868 -21.3906 2.9 41.4 111.8 2.6328 4.0 ------ UNKNOWN
97.0572 -36.6083 2.0 50.5 -0.7 1.6902 5.7 ------ UNKNOWN
173.9620 -66.8954 2.4 5.1 -101.8 0.6829 4.8 ------ UNKNOWN
229.7604 -57.3863 2.0 29.3 -156.8 0.9594 5.7 ------ UNKNOWN
65.7059 -47.4585 1.9 55.2 -32.3 4.8416 6.1 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
140.100600 503.990000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
170.3666 -60.6002 4.0 29.7 33.2 2.7146 2.9 2.0 Cen X-3
186.6523 -62.7605 0.5 21.7 32.4 18.7849 23.8 0.6 GX 301-2
244.9932 -15.6583 1.5 43.3 176.4 10.5247 7.6 1.3 Sco X-1
255.9577 -37.8048 62.4 26.0 -152.7 -0.1374 -0.2 2.7 4U 1700-377
256.4142 -36.2723 5.5 27.5 -153.8 1.6774 2.1 9.1 GX 349+2
263.0680 -24.7750 6.0 40.4 -154.9 2.2534 1.9 3.7 GX 1+4
264.9559 -44.5284 8.8 25.2 -130.6 1.0538 1.3 10.3 4U 1735-44
270.2086 -24.9772 3.2 43.3 -146.3 4.8741 3.6 7.4 GX 5-1
270.2455 -25.8088 8.4 42.6 -145.6 -1.7649 -1.4 5.0 GRS 1758-258
274.0201 -14.0401 75.2 54.6 -149.2 0.5178 0.2 0.9 GX 17+2
276.0760 -30.3457 12.7 41.7 -135.5 -1.4063 -0.9 7.9 H1820-303
262.9896 -33.8345 118.6 32.5 -147.3 -0.0936 -0.1 0.0 GX 354-0
150.5278 -46.1912 2.5 47.3 42.3 9.5404 4.6 ------ UNKNOWN
229.7719 -57.3473 1.3 0.0 167.6 6.3808 9.2 ------ UNKNOWN
34.9916 -66.9413 2.1 55.2 -32.3 21.0399 5.4 ------ UNKNOWN
Plot creation:
Tue Mar 5 12:19:47 EST 2024