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
245.0887 -15.7570 0.0918 44.8 -147.7 0.4378 2.1 TRIG_01212713
------------------------------------------
Foreground time interval of the image:
73.540 129.396 (delta_t = 55.856 [sec])
Background time interval of the image:
-13.699 23.220 (delta_t = 36.919 [sec])
24.000 73.540 (delta_t = 49.540 [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 64.000000
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 64.000000
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 64.000000
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 73.540 sec. to 129.396 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 5.15003 ( -0.602118 0.657053 )
Norm@50keV : 3.13377E-04 ( -0.00014768 0.000225417 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 42.62 using 59 PHA bins.
# Reduced chi-squared = 0.7477 for 57 degrees of freedom
# Null hypothesis probability = 9.216605e-01
Photon flux (15-150 keV) in 55.86 sec: 0.558360 ( -0.0665684 0.066733 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.86812e-07 ( -1.153e-07 1.15833e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from 73.540 sec. to 129.396 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.00000 ( )
Epeak [keV] : 50.0000 ( )
Norm@50keV : 5.07260E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 167.18 using 59 PHA bins.
# Reduced chi-squared = 2.9853 for 56 degrees of freedom
# Null hypothesis probability = 5.303859e-13
Photon flux (15-150 keV) in 55.86 sec: 0.557859 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 9.84343e-07 ( 0 0 ) ergs/cm2
Band function
Time interval is from 73.540 sec. to 129.396 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -7.06692 ( 7.06692 7.06692 )
beta : -5.16763 ( -0.642958 0.616102 )
Epeak [keV] : 6.28259 ( -6.28259 -6.28259 )
Norm@50keV : 4.18809E-02 ( -0.0195775 0.0311434 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 42.62 using 59 PHA bins.
# Reduced chi-squared = 0.7750 for 55 degrees of freedom
# Null hypothesis probability = 8.882948e-01
Photon flux (15-150 keV) in 55.86 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] : 2.82444 (-0.376905 0.469168)
R^2/D10^2 : 111.167 (-72.8478 211.381)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 53.44 using 59 PHA bins.
# Reduced chi-squared = 0.9375 for 57 degrees of freedom
# Null hypothesis probability = 6.095395e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.904e-07 2.925e-07
25- 50 9.287e-08 3.844e-08
50-150 9.026e-11 8.093e-11
15-150 8.833e-07 3.369e-07
Thermal bremsstrahlung (OTTB)
XSPEC12>exit
XSPEC: quit
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 5.67016 (-1.14568 1.63328)
Norm : 80.3597 (-44.396 107.295)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.852e-07 2.128e-07
25- 50 1.302e-07 4.681e-08
50-150 1.227e-09 1.011e-09
15-150 9.167e-07 2.420e-07
Double BB
XSPEC12>exit
XSPEC: quit
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 1.88189 (-0.459914 0.531255)
R1^2/D10^2 : 1949.19 (-1420.47 20898.1)
kT2 [keV] : 5.77499 (-1.71384 2.8841)
R2^2/D10^2 : 0.953473 (-0.755776 4.60612)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.525e-07 4.064e-07
25- 50 1.925e-07 1.168e-07
50-150 2.329e-08 2.033e-08
15-150 9.684e-07 5.022e-07
Peak spectrum fit
Power-law model
Time interval is from 112.120 sec. to 113.120 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 5.46585 ( -2.3248 2.93912 )
Norm@50keV : 3.71284E-04 ( -0.000369292 0.0029105 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 50.19 using 59 PHA bins.
# Reduced chi-squared = 0.8805 for 57 degrees of freedom
# Null hypothesis probability = 7.264591e-01
Photon flux (15-150 keV) in 1 sec: 0.898844 ( -0.348506 0.347092 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.78143e-08 ( -1.22536e-08 1.72506e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 112.120 sec. to 113.120 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.88422 ( )
Epeak [keV] : 0.588133 ( )
Norm@50keV : 0.532555 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 50.77 using 59 PHA bins.
# Reduced chi-squared = 0.9067 for 56 degrees of freedom
# Null hypothesis probability = 6.723858e-01
Photon flux (15-150 keV) in 1 sec: 0.900326 ( -0.350744 0.332844 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.66756e-08 ( -1.11717e-08 1.85095e-08 ) ergs/cm2
Band function
Time interval is from 112.120 sec. to 113.120 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -9.97614 ( 9.97614 9.97614 )
beta : -5.36806 ( -3.2573 2.05276 )
Epeak [keV] : 3.34559 ( -3.34559 -3.34559 )
Norm@50keV : 5.60901E-02 ( -0.0558636 0.390982 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 50.19 using 59 PHA bins.
# Reduced chi-squared = 0.9126 for 55 degrees of freedom
# Null hypothesis probability = 6.584510e-01
Photon flux (15-150 keV) in 1 sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 1.6359e-08 ( -1.6352e-08 -1.6359e-08 ) ergs/cm2
Single BB
XSPEC: quit
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 2.25120 (-0.733459 1.03527)
R^2/D10^2 : 943.270 (-957.969 27520.4)
(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 2.332e-08 1.319e-08
25- 50 1.100e-09 7.440e-10
50-150 1.175e-13 1.733e-13
15-150 2.442e-08 1.349e-08
Thermal bremsstrahlung (OTTB)
XSPEC12>exit
XSPEC: quit
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 4.05550 (-1.80735 4.27265)
Norm : 453.151 (-453.152 8835.42)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.316e-08 1.394e-08
25- 50 1.751e-09 1.254e-09
50-150 2.812e-12 4.022e-12
15-150 2.492e-08 1.447e-08
Double BB
XSPEC12>exit
XSPEC: quit
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 2.01077 (-0.713002 0.931217)
R1^2/D10^2 : 2012.70 (-1983.47 123701)
kT2 [keV] : 17.5108 (-8.07261 18.1596)
R2^2/D10^2 : 2.82295E-02 (-0.0263147 0.129655)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.114e-08 1.199e-08
25- 50 8.456e-09 5.765e-09
50-150 1.749e-08 1.583e-08
15-150 4.708e-08 2.526e-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: 5.15003 ( -0.602118 0.657053 )
Norm@50keV : 3.13377E-04 ( -0.00014768 0.000225417 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 42.62 using 59 PHA bins.
# Reduced chi-squared = 0.7477 for 57 degrees of freedom
# Null hypothesis probability = 9.216605e-01
Photon flux (15-150 keV) in 55.86 sec: 0.558360 ( -0.0665684 0.066733 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.86812e-07 ( -1.153e-07 1.15833e-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 : 5.07260E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 167.18 using 59 PHA bins.
# Reduced chi-squared = 2.9853 for 56 degrees of freedom
# Null hypothesis probability = 5.303859e-13
Photon flux (15-150 keV) in 55.86 sec: 0.557859 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 9.84343e-07 ( 0 0 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -7.06692 ( 7.06692 7.06692 )
beta : -5.16763 ( -0.642958 0.616102 )
Epeak [keV] : 6.28259 ( -6.28259 -6.28259 )
Norm@50keV : 4.18809E-02 ( -0.0195775 0.0311434 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 42.62 using 59 PHA bins.
# Reduced chi-squared = 0.7750 for 55 degrees of freedom
# Null hypothesis probability = 8.882948e-01
Photon flux (15-150 keV) in 55.86 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) = 1.75e-07
S(50-100 keV) = 1.97e-08
T90 vs. Hardness ratio plot
T90 = 49.444000005722 sec.
Hardness ratio (energy fluence ratio) = 0.112571
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 0.219425
Count Ratio (50-100 keV) / (15-25 keV) = 0.0352691
Mask shadow pattern
IMX = -8.383827386945458E-01, IMY = 5.301880142670414E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 64.000000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 64.000000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 64.000000
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:
-13.699390 23.220000
24.000000 73.540000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.4892 -40.5012 4.9 49.2 34.1 2.3798 2.4 3.7 Vela X-1
170.1847 -60.8143 0.0 26.9 1.7 0.7635 3.3 12.1 Cen X-3
186.2045 -62.7677 201.3 22.5 -13.9 -0.0122 -0.1 12.4 GX 301-2
245.0862 -15.8268 1.3 44.7 -147.6 3.9980 8.8 12.8 Sco X-1
256.1859 -37.9380 7.9 40.2 -112.1 0.9632 1.5 11.0 4U 1700-377
256.2706 -36.5320 0.0 40.8 -114.0 1.3474 1.9 10.3 GX 349+2
196.9818 0.9770 1.9 43.8 137.2 3.5552 6.0 ------ UNKNOWN
216.8884 8.4792 2.3 52.5 163.4 3.6042 5.0 ------ UNKNOWN
221.5030 6.4446 2.4 51.8 169.6 2.8343 4.7 ------ UNKNOWN
228.2373 -33.1231 2.2 21.9 -141.0 1.1099 5.3 ------ UNKNOWN
244.9170 -63.3515 2.5 31.8 -68.7 1.6921 4.6 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
73.540000 129.396000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.4447 -40.4536 3.1 49.3 34.1 -2.0635 -3.8 7.2 Vela X-1
170.3817 -60.4493 14.0 26.6 2.3 0.0935 0.8 10.6 Cen X-3
186.6379 -62.7590 62.9 22.4 -14.3 -0.0191 -0.2 0.8 GX 301-2
245.0886 -15.7572 5.5 44.8 -147.7 0.4376 2.1 9.4 Sco X-1
255.8896 -37.9093 4.3 40.0 -112.3 -0.7643 -2.7 6.0 4U 1700-377
256.4052 -36.4222 4.6 41.0 -114.1 -0.8635 -2.5 1.5 GX 349+2
216.6604 -37.7990 2.5 11.4 -143.8 0.4475 4.6 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
Plot creation:
Sun Feb 4 07:20:41 EST 2024