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
245.0729 -15.8787 0.0252 42.1 -58.3 12.2146 7.6 TRIG_01204595
------------------------------------------
Foreground time interval of the image:
-147.699 23.840 (delta_t = 171.539 [sec])
25.000 105.450 (delta_t = 80.450 [sec])
107.000 130.630 (delta_t = 23.630 [sec])
132.000 244.901 (delta_t = 112.901 [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
-159.880000 23.840000
25.000000 105.450000
107.000000 130.630000
132.000000 327.464000
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 5.05544 ( -0.572929 0.589818 )
Norm@50keV : 1.92818E-04 ( -8.1148e-05 0.000122727 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 69.31 using 59 PHA bins.
# Reduced chi-squared = 1.216 for 57 degrees of freedom
# Null hypothesis probability = 1.270890e-01
Photon flux (15-150 keV) in 483.3 sec: 0.313724 ( -0.0338148 0.0339817 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.83208e-06 ( -4.71884e-07 4.71886e-07 ) ergs/cm2
Cutoff power-law model
Multiple GTIs in the spectrum
tstart tstop
-159.880000 23.840000
25.000000 105.450000
107.000000 130.630000
132.000000 327.464000
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.82156 ( )
Epeak [keV] : 1.08208 ( )
Norm@50keV : 0.106679 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 79.25 using 59 PHA bins.
# Reduced chi-squared = 1.415 for 56 degrees of freedom
# Null hypothesis probability = 2.213226e-02
Photon flux (15-150 keV) in 483.3 sec: 0.313639 ( -0.033966 0.033728 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.83011e-06 ( -4.71696e-07 4.71696e-07 ) ergs/cm2
Band function
Multiple GTIs in the spectrum
tstart tstop
-159.880000 23.840000
25.000000 105.450000
107.000000 130.630000
132.000000 327.464000
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -9.91875 ( 9.91875 9.91875 )
beta : -5.02792 ( -0.614412 0.550091 )
Epeak [keV] : 1.94310 ( -1.9431 -1.9431 )
Norm@50keV : 2.68725E-02 ( -0.0115166 0.0162145 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 69.31 using 59 PHA bins.
# Reduced chi-squared = 1.260 for 55 degrees of freedom
# Null hypothesis probability = 9.275635e-02
Photon flux (15-150 keV) in 483.3 sec: ( ) 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] : 2.73575 (-0.273584 0.329819)
R^2/D10^2 : 79.5550 (-44.5981 98.6256)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 85.06 using 59 PHA bins.
# Reduced chi-squared = 1.492 for 57 degrees of freedom
# Null hypothesis probability = 9.391409e-03
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.960e-06 1.069e-06
25- 50 4.135e-07 1.389e-07
50-150 3.036e-10 2.387e-10
15-150 4.374e-06 1.021e-06
Thermal bremsstrahlung (OTTB)
XSPEC12>exit
XSPEC: quit
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 5.34870 (-0.862619 1.22376)
Norm : 55.7233 (-28.4722 56.3461)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.910e-06 8.765e-07
25- 50 5.734e-07 1.618e-07
50-150 4.132e-09 3.037e-09
15-150 4.488e-06 8.533e-07
Double BB
XSPEC12>exit
XSPEC: quit
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 2.32862 (-0.274896 0.305922)
R1^2/D10^2 : 243.095 (-148.572 427.951)
kT2 [keV] : 12.6293 (-3.44389 5.8591)
R2^2/D10^2 : 1.51162E-02 (-0.0118092 0.0426346)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.033e-06 1.858e-06
25- 50 1.032e-06 4.832e-07
50-150 8.171e-07 5.550e-07
15-150 5.882e-06 2.257e-06
Peak spectrum fit
Power-law model
Time interval is from 159.724 sec. to 160.724 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.94477 ( -0.479399 0.958684 )
Norm@50keV : 4.35167E-03 ( -0.00258905 0.00200337 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 58.11 using 59 PHA bins.
# Reduced chi-squared = 1.019 for 57 degrees of freedom
# Null hypothesis probability = 4.342629e-01
Photon flux (15-150 keV) in 1 sec: 1.14994 ( -0.391006 0.390075 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.10013e-08 ( -1.84384e-08 1.7921e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 159.724 sec. to 160.724 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.97751 ( -0.216032 0.0185822 )
Epeak [keV] : 1.48099 ( -0.882991 39.492 )
Norm@50keV : 1.26628E-02 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 59.01 using 59 PHA bins.
# Reduced chi-squared = 1.054 for 56 degrees of freedom
# Null hypothesis probability = 3.662295e-01
Photon flux (15-150 keV) in 1 sec: 1.15067 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 5.08337e-08 ( -1.80701e-08 1.95727e-08 ) ergs/cm2
Band function
Time interval is from 159.724 sec. to 160.724 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 4.01352 ( 1.39502 1.39502 )
beta : -2.99300 ( 2.95577 0.487157 )
Epeak [keV] : 15.3836 ( -7.28801 538.195 )
Norm@50keV : 6333.12 ( -6319.64 1.25773e+07 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 57.96 using 59 PHA bins.
# Reduced chi-squared = 1.054 for 55 degrees of freedom
# Null hypothesis probability = 3.666175e-01
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] : 3.60697 (-1.21997 3.15649)
R^2/D10^2 : 46.3002 (-46.3243 496.137)
(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 2.493e-08 1.454e-08
25- 50 6.633e-09 4.676e-09
50-150 4.172e-11 4.288e-11
15-150 3.161e-08 1.873e-08
Thermal bremsstrahlung (OTTB)
XSPEC12>exit
XSPEC: quit
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 40.8279 (-40.8692 27.1127)
Norm : 7.04688 (-3.26196 60.9995)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.629e-08 6.823e-09
25- 50 2.162e-08 9.185e-09
50-150 1.710e-08 1.047e-08
15-150 5.502e-08 2.471e-08
Double BB
XSPEC12>exit
XSPEC: quit
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 2.91146 (-1.02448 1.53321)
R1^2/D10^2 : 132.280 (-120.435 2398.87)
kT2 [keV] : 16.9195 (-5.84067 6.44997)
R2^2/D10^2 : 4.47551E-02 (-0.0385087 0.138917)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.309e-08 1.353e-08
25- 50 1.420e-08 9.425e-09
50-150 2.351e-08 1.837e-08
15-150 6.080e-08 3.442e-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: 4.87450 ( -0.6009 0.630234 )
Norm@50keV : 2.34272E-04 ( -0.000103365 0.000157174 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 69.28 using 59 PHA bins.
# Reduced chi-squared = 1.216 for 57 degrees of freedom
# Null hypothesis probability = 1.274905e-01
Photon flux (15-150 keV) in 388.5 sec: 0.320881 ( -0.035473 0.0356797 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.03255e-06 ( -4.11981e-07 4.13209e-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 : 3.52692E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 181.80 using 59 PHA bins.
# Reduced chi-squared = 3.2465 for 56 degrees of freedom
# Null hypothesis probability = 3.286217e-15
Photon flux (15-150 keV) in 388.5 sec: 0.320720 ( -0.035519 0.035527 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.03065e-06 ( 0 0 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -9.78314 ( 9.78314 9.78314 )
beta : -4.87562 ( -0.630435 0.601549 )
Epeak [keV] : 2.27198 ( -2.27198 -2.27198 )
Norm@50keV : 3.18097E-02 ( -0.0140478 0.0213616 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 69.28 using 59 PHA bins.
# Reduced chi-squared = 1.260 for 55 degrees of freedom
# Null hypothesis probability = 9.316366e-02
Photon flux (15-150 keV) in 388.5 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) = 8.93e-07
S(50-100 keV) = 1.07e-07
T90 vs. Hardness ratio plot
T90 = 424.384000062943 sec.
Hardness ratio (energy fluence ratio) = 0.119821
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 0.236283
Count Ratio (50-100 keV) / (15-25 keV) = 0.0901535
Mask shadow pattern
IMX = 4.748293818933887E-01, IMY = 7.681279334864578E-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:
-147.699400 23.840000
25.000000 105.450000
107.000000 130.630000
132.000000 244.900600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
244.9777 -15.8062 2.6 42.0 -58.2 6.9737 4.4 10.0 Sco X-1
254.5691 35.2289 10.2 15.7 179.2 0.5929 1.1 8.7 Her X-1
268.3753 -1.4008 7.9 38.8 -100.4 -2.8504 -1.4 3.1 SW J1753.5-0127
288.7523 10.9654 15.0 48.4 -132.3 -1.7568 -0.8 3.0 GRS 1915+105
299.7379 35.3319 14.0 51.6 -166.6 1.1693 0.8 10.7 Cyg X-1
308.0967 40.9477 4.5 57.4 -174.5 6.4621 2.6 0.7 Cyg X-3
205.7313 41.8043 3.3 32.2 77.5 4.2240 3.5 ------ UNKNOWN
238.2078 55.1540 2.3 29.3 127.2 4.2087 5.0 ------ UNKNOWN
217.1646 30.8572 2.3 20.6 58.4 2.9665 4.9 ------ UNKNOWN
208.5568 -20.7351 2.1 55.7 -14.7 8.5875 5.3 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
347.100600 659.320000
661.000000 866.000000
867.000000 963.081100
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
170.4625 -60.6254 9.2 52.5 -8.9 -2.3486 -1.3 4.3 Cen X-3
186.7794 -62.8576 4.7 50.6 -18.8 -5.1756 -2.4 6.2 GX 301-2
245.0975 -15.8125 0.0 41.7 -108.9 7.1990 1.8 12.4 Sco X-1
170.9686 -3.4760 2.8 32.2 77.4 7.9419 4.1 ------ UNKNOWN
Plot creation:
Wed Dec 27 00:18:58 EST 2023