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
244.9646 -15.6410 0.0081 0.1 10.8 2.4458 23.7 TRIG_01042032
------------------------------------------
Foreground time interval of the image:
0.000 63.107 (delta_t = 63.107 [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 63.107 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 5.62977 ( -0.447195 0.468155 )
Norm@50keV : 1.22159E-04 ( -4.48208e-05 6.27001e-05 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 63.27 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.65e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 63.11 sec: 0.347649 ( -0.0342937 0.0343856 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.72317e-07 ( -6.38396e-08 6.38396e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.000 sec. to 63.107 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.703631 ( )
Epeak [keV] : 5.54018 ( )
Norm@50keV : 1.32426 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared 59.10 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.63e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 63.11 sec: 0.337972 ( -0.037068 0.036422 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.40939e-07 ( -6.66113e-08 6.61456e-08 ) ergs/cm2
Band function
Time interval is from 0.000 sec. to 63.107 sec.
XSPEC12>exit
XSPEC: quit
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -6.28765 ( 4.02368 6.28765 )
beta : -5.68718 ( -0.425005 0.496569 )
Epeak [keV] : 358.028 ( -358.028 -358.028 )
Norm@50keV : 1.56932E-02 ( -0.00552334 0.00915515 )
------------------------------------------------------------
Photon flux (15-150 keV) in 63.11 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] : 2.75807 (-0.234992 0.26365)
R^2/D10^2 : 82.5805 (-40.0616 79.8932)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 59.82 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.74e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.669e-07 1.291e-07
25- 50 6.101e-08 1.839e-08
50-150 4.816e-11 3.650e-11
15-150 6.279e-07 1.445e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 5.00616 (-0.624972 0.758304)
Norm : 78.3011 (-32.3646 57.4943)
------------------------------------------------------------
#Fit statistic : Chi-Squared 59.22 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.95e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.730e-07 1.212e-07
25- 50 7.262e-08 2.025e-08
50-150 3.788e-10 2.778e-10
15-150 6.460e-07 1.162e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 2.72151 (-0.245452 0.265493)
R1^2/D10^2 : 90.1332 (-44.9111 94.9149)
kT2 [keV] : 22.6566 (-22.3079 -22.3079)
R2^2/D10^2 : 3.93321E-04 (-0.000447693 0.0220684)
------------------------------------------------------------
#Fit statistic : Chi-Squared 58.45 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.50e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.680e-07 1.494e-07
25- 50 7.042e-08 2.182e-08
50-150 4.803e-08 4.294e-08
15-150 6.864e-07 1.857e-07
Peak spectrum fit
Power-law model
Time interval is from 0.000 sec. to 63.107 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 5.62977 ( -0.447195 0.468155 )
Norm@50keV : 1.22159E-04 ( -4.48208e-05 6.27001e-05 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 63.27 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.65e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 63.11 sec: 0.347649 ( -0.0342937 0.0343856 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.72317e-07 ( -6.38396e-08 6.38396e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.000 sec. to 63.107 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.703631 ( )
Epeak [keV] : 5.54018 ( )
Norm@50keV : 1.32426 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared 59.10 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.63e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 63.11 sec: 0.337972 ( -0.037068 0.036422 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.40939e-07 ( -6.66113e-08 6.61456e-08 ) ergs/cm2
Band function
Time interval is from 0.000 sec. to 63.107 sec.
XSPEC12>exit
XSPEC: quit
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -6.28765 ( 4.02368 6.28765 )
beta : -5.68718 ( -0.425005 0.496569 )
Epeak [keV] : 358.028 ( -358.028 -358.028 )
Norm@50keV : 1.56932E-02 ( -0.00552334 0.00915515 )
------------------------------------------------------------
Photon flux (15-150 keV) in 63.11 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] : 2.75807 (-0.234992 0.26365)
R^2/D10^2 : 82.5805 (-40.0616 79.8932)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 59.82 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.74e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.669e-07 1.500e-07
25- 50 6.101e-08 1.799e-08
50-150 4.816e-11 3.712e-11
15-150 6.279e-07 1.446e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 5.00616 (-0.624972 0.758304)
Norm : 78.3011 (-32.3646 57.4943)
------------------------------------------------------------
#Fit statistic : Chi-Squared 59.22 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.95e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.730e-07 1.263e-07
25- 50 7.262e-08 1.943e-08
50-150 3.788e-10 2.659e-10
15-150 6.460e-07 1.416e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 2.72151 (-0.245452 0.265493)
R1^2/D10^2 : 90.1332 (-44.9111 94.9149)
kT2 [keV] : 22.6566 (-22.3079 -22.3079)
R2^2/D10^2 : 3.93321E-04 (-0.000447693 0.0214728)
------------------------------------------------------------
#Fit statistic : Chi-Squared 58.45 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.50e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.680e-07 1.323e-07
25- 50 7.042e-08 2.167e-08
50-150 4.803e-08 4.332e-08
15-150 6.864e-07 1.695e-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: 5.62977 ( -0.447195 0.468155 )
Norm@50keV : 1.22159E-04 ( -4.48208e-05 6.27001e-05 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 63.27 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.65e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 63.11 sec: 0.347649 ( -0.0342937 0.0343856 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.72317e-07 ( -6.38396e-08 6.38396e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.703631 ( )
Epeak [keV] : 5.54018 ( )
Norm@50keV : 1.32426 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared 59.10 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.63e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 63.11 sec: 0.337972 ( -0.037068 0.036422 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.40939e-07 ( -6.66113e-08 6.61456e-08 ) ergs/cm2
Band function
XSPEC12>exit
XSPEC: quit
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -6.28765 ( 4.02368 6.28765 )
beta : -5.68718 ( -0.425005 0.496569 )
Epeak [keV] : 358.028 ( -358.028 -358.028 )
Norm@50keV : 1.56932E-02 ( -0.00552334 0.00915515 )
------------------------------------------------------------
Photon flux (15-150 keV) in 63.11 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) = 9.68e-08
S(50-100 keV) = 7.82e-09
T90 vs. Hardness ratio plot
T90 = 64 sec.
Hardness ratio (energy fluence ratio) = 0.0807851
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 0.0897917
Count Ratio (50-100 keV) / (15-25 keV) = 0.0428745
Mask shadow pattern
IMX = 9.735366519373632E-04, IMY = -1.864894132743255E-04
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 63.106600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
244.9646 -15.6410 0.5 0.1 10.8 2.4457 23.7 0.9 Sco X-1
254.5200 35.3101 177.6 51.7 -174.0 0.0200 0.1 3.6 Her X-1
255.9695 -37.9014 1.9 24.3 -25.3 0.6797 5.9 3.5 4U 1700-377
256.3949 -36.4760 4.0 23.2 -27.7 0.3213 2.9 3.7 GX 349+2
262.9971 -24.8581 6.8 19.3 -62.2 0.2158 1.7 6.8 GX 1+4
264.6554 -44.4847 8.7 33.3 -29.8 0.1911 1.3 4.3 4U 1735-44
268.3888 -1.3149 5.7 27.1 -123.4 0.2918 2.0 8.4 SW J1753.5-0127
270.1142 -24.9675 7.1 25.3 -68.1 -0.2251 -1.6 11.4 GX 5-1
270.1758 -25.6191 8.8 25.6 -66.7 0.1843 1.3 10.1 GRS 1758-258
273.9644 -14.0119 5.7 28.0 -93.3 0.3477 2.0 2.8 GX 17+2
275.7721 -30.5331 0.0 31.9 -60.5 0.1961 1.2 12.7 H1820-303
284.8933 -25.0778 6.6 38.5 -73.0 0.4884 1.8 12.2 HT1900.1-2455
262.9833 -33.8416 443.1 24.4 -42.3 0.0032 0.0 0.5 GX 354-0
235.0850 -1.1700 3.0 17.4 141.1 0.4263 3.8 ------ UNKNOWN
240.1795 14.5555 2.3 30.5 166.9 0.6744 5.0 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
Plot creation:
Fri Apr 9 18:14:53 EDT 2021