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
245.2550 -15.7533 0.0626 0.0 -30.1 -0.0575 -3.1 TRIG_01216909
------------------------------------------
Foreground time interval of the image:
134.480 136.212 (delta_t = 1.732 [sec])
164.000 164.876 (delta_t = 0.876 [sec])
Background time interval of the image:
-119.000 -23.150 (delta_t = 95.850 [sec])
-20.000 134.480 (delta_t = 154.480 [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
Multiple GTIs in the spectrum
tstart tstop
134.480000 136.212200
164.000000 164.876000
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 5.94387 ( -1.54523 2.20711 )
Norm@50keV : 7.21599E-05 ( -7.21459e-05 0.000293303 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 40.89 using 59 PHA bins.
# Reduced chi-squared = 0.7173 for 57 degrees of freedom
# Null hypothesis probability = 9.470362e-01
Photon flux (15-150 keV) in 2.608 sec: 0.280694 ( -0.091461 0.0911029 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.20491e-08 ( -8.05095e-09 9.0387e-09 ) ergs/cm2
Cutoff power-law model
Multiple GTIs in the spectrum
tstart tstop
134.480000 136.212200
164.000000 164.876000
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.00000 ( )
Epeak [keV] : 50.0000 ( )
Norm@50keV : 3.58153E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 70.07 using 59 PHA bins.
# Reduced chi-squared = 1.251 for 56 degrees of freedom
# Null hypothesis probability = 9.786145e-02
Photon flux (15-150 keV) in 2.608 sec: 0.279286 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 2.18357e-08 ( -7.87566e-09 9.24773e-09 ) ergs/cm2
Band function
Multiple GTIs in the spectrum
tstart tstop
134.480000 136.212200
164.000000 164.876000
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -3.58842 ( 1.27707 3.58739 )
beta : -5.94654 ( 1.4608 -1.74731 )
Epeak [keV] : 31.7487 ( -31.7487 -31.7487 )
Norm@50keV : 1.02221 ( 842.236 -1.01975 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 40.89 using 59 PHA bins.
# Reduced chi-squared = 0.7434 for 55 degrees of freedom
# Null hypothesis probability = 9.217413e-01
Photon flux (15-150 keV) in 2.608 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] : 2.27277 (-0.622651 0.774048)
R^2/D10^2 : 289.658 (-289.658 3796.14)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 41.14 using 59 PHA bins.
# Reduced chi-squared = 0.7218 for 57 degrees of freedom
# Null hypothesis probability = 9.437219e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.014e-08 1.138e-08
25- 50 9.910e-10 6.683e-10
50-150 1.174e-13 1.614e-13
15-150 2.113e-08 1.152e-08
Thermal bremsstrahlung (OTTB)
XSPEC12>exit
XSPEC: quit
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 3.99970 (-1.50184 2.59607)
Norm : 157.632 (-157.633 1428.89)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.979e-08 1.132e-08
25- 50 1.441e-09 8.996e-10
50-150 2.123e-12 2.658e-12
15-150 2.124e-08 1.202e-08
Double BB
XSPEC12>exit
XSPEC: quit
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 2.10719 (-0.622643 0.774057)
R1^2/D10^2 : 490.015 (-251.497 3796.36)
kT2 [keV] : 9.89986 (-3.65024 -3.65024)
R2^2/D10^2 : 2.26311E-02 (-0.0198541 16830.7)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 0.000e+00 0.000e+00
25- 50 0.000e+00 0.000e+00
50-150 0.000e+00 0.000e+00
15-150 0.000e+00 0.000e+00
Peak spectrum fit
Power-law model
Time interval is from 135.448 sec. to 136.212 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 5.93850 ( -2.94969 -5.94761 )
Norm@50keV : 8.70644E-05 ( -8.57223e-05 0.00152842 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 36.60 using 59 PHA bins.
# Reduced chi-squared = 0.6420 for 57 degrees of freedom
# Null hypothesis probability = 9.837632e-01
Photon flux (15-150 keV) in 0.7642 sec: 0.336255 ( -0.178747 0.190735 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.73745e-09 ( -7.73523e-09 7.88502e-09 ) ergs/cm2
Cutoff power-law model
Time interval is from 135.448 sec. to 136.212 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.86896 ( )
Epeak [keV] : 0.641871 ( )
Norm@50keV : 0.257985 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 37.46 using 59 PHA bins.
# Reduced chi-squared = 0.6689 for 56 degrees of freedom
# Null hypothesis probability = 9.731350e-01
Photon flux (15-150 keV) in 0.7642 sec: 0.338270 ( -0.181272 0.183091 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.31613e-09 ( -4.06323e-09 8.33673e-09 ) ergs/cm2
Band function
Time interval is from 135.448 sec. to 136.212 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 5.00000 ( -5 -5 )
beta : -6.20047 ( )
Epeak [keV] : 0.663774 ( )
Norm@50keV : 9.09460E+07 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 36.61 using 59 PHA bins.
# Reduced chi-squared = 0.6657 for 55 degrees of freedom
# Null hypothesis probability = 9.733865e-01
Photon flux (15-150 keV) in 0.7642 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] : 2.00509 (-0.825884 1.24816)
R^2/D10^2 : 873.877 (-991.077 189002)
(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 6.275e-09 3.844e-09
25- 50 1.723e-10 1.408e-10
50-150 4.816e-15 1.294e-14
15-150 6.448e-09 3.901e-09
Thermal bremsstrahlung (OTTB)
XSPEC12>exit
XSPEC: quit
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 3.43046 (-1.80109 5.6052)
Norm : 359.230 (-375.124 42115.7)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.445e-09 3.589e-09
25- 50 3.022e-10 2.284e-10
50-150 1.572e-13 2.522e-13
15-150 6.748e-09 3.924e-09
Double BB
XSPEC12>exit
XSPEC: quit
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 1.87687 (-0.86153 1.09968)
R1^2/D10^2 : 1293.00 (-3216.3 6623.31)
kT2 [keV] : 14.2396 (-7.90869 22.3293)
R2^2/D10^2 : 2.63019E-02 (-0.0304724 0.791273)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.972e-09 3.615e-09
25- 50 3.351e-09 2.259e-09
50-150 4.377e-09 3.667e-09
15-150 1.370e-08 8.227e-09
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: 5.94387 ( -1.54523 2.20711 )
Norm@50keV : 7.21599E-05 ( -7.21459e-05 0.000293303 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 40.89 using 59 PHA bins.
# Reduced chi-squared = 0.7173 for 57 degrees of freedom
# Null hypothesis probability = 9.470362e-01
Photon flux (15-150 keV) in 2.608 sec: 0.280694 ( -0.091461 0.0911029 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.20491e-08 ( -8.05095e-09 9.0387e-09 ) 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 : 3.58153E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 70.07 using 59 PHA bins.
# Reduced chi-squared = 1.251 for 56 degrees of freedom
# Null hypothesis probability = 9.786145e-02
Photon flux (15-150 keV) in 2.608 sec: 0.279286 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 2.18357e-08 ( -7.87566e-09 9.24773e-09 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -3.58842 ( 1.27707 3.58739 )
beta : -5.94654 ( 1.4608 -1.74731 )
Epeak [keV] : 31.7487 ( -31.7487 -31.7487 )
Norm@50keV : 1.02221 ( 842.236 -1.01975 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 40.89 using 59 PHA bins.
# Reduced chi-squared = 0.7434 for 55 degrees of freedom
# Null hypothesis probability = 9.217413e-01
Photon flux (15-150 keV) in 2.608 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) = 2.75e-09
S(50-100 keV) = 1.79e-10
T90 vs. Hardness ratio plot
T90 = 1.1360000371933 sec.
Hardness ratio (energy fluence ratio) = 0.0650909
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 0.139151
Count Ratio (50-100 keV) / (15-25 keV) = -0.0809559
Mask shadow pattern
IMX = 1.833684830662600E-04, IMY = 1.064235333154780E-04
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:
-119.000000 -23.150000
-20.000000 134.480000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
244.9941 -15.6441 313.3 0.3 101.9 0.0141 0.0 0.9 Sco X-1
254.3820 35.5037 9.8 52.0 179.8 1.3320 1.2 10.4 Her X-1
256.1804 -37.7508 7.3 24.0 -31.3 -0.7026 -1.6 10.8 4U 1700-377
256.5381 -36.5732 11.0 23.1 -33.3 -0.4571 -1.0 10.3 GX 349+2
262.9581 -24.6866 5.5 18.8 -68.5 -0.9205 -2.1 4.5 GX 1+4
264.8804 -44.2984 7.9 33.0 -35.8 -0.7608 -1.5 10.8 4U 1735-44
268.5035 -1.6173 0.0 26.9 -129.0 0.7447 1.5 12.8 SW J1753.5-0127
270.1178 -25.1189 7.6 25.1 -73.7 -0.7654 -1.5 9.3 GX 5-1
270.1416 -25.6859 10.2 25.3 -72.4 0.6036 1.2 9.3 GRS 1758-258
273.8522 -14.0064 4.2 27.7 -99.4 -1.5267 -2.7 9.1 GX 17+2
276.0963 -30.2188 8.4 31.7 -67.1 -0.8057 -1.4 12.6 H1820-303
284.9004 -24.8287 20.6 38.1 -79.3 0.5964 0.6 9.2 HT1900.1-2455
263.1583 -33.8872 9.1 24.3 -48.0 0.5929 1.3 9.0 GX 354-0
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
134.480000 136.212200
164.000000 164.876000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
245.1189 -15.7449 5.5 0.1 78.9 -0.0393 -2.1 10.2 Sco X-1
254.3397 35.3353 6.2 51.8 179.8 0.0978 1.8 5.8 Her X-1
255.7936 -37.9301 78.2 24.1 -30.4 0.0028 0.1 10.5 4U 1700-377
256.3290 -36.3696 13.3 22.9 -33.1 0.0163 0.9 6.1 GX 349+2
263.1678 -24.8125 5.7 19.1 -68.4 -0.0423 -2.0 9.5 GX 1+4
264.6172 -44.5238 6.7 33.1 -35.3 -0.0437 -1.7 7.0 4U 1735-44
268.3360 -1.5898 5.3 26.8 -129.3 0.0514 2.2 8.5 SW J1753.5-0127
270.3227 -24.9585 6.6 25.2 -74.1 0.0440 1.7 7.5 GX 5-1
270.4621 -25.8769 0.0 25.6 -72.2 0.0347 1.4 11.8 GRS 1758-258
273.8491 -14.1611 0.0 27.7 -99.1 -0.0444 -1.5 11.8 GX 17+2
275.8572 -30.4353 5.8 31.6 -66.6 0.0599 2.0 5.4 H1820-303
284.9714 -25.0432 223.9 38.2 -79.0 0.0034 0.1 8.2 HT1900.1-2455
263.1604 -33.8656 7.7 24.3 -48.1 -0.0322 -1.5 8.7 GX 354-0
Post-slew image of 15-350 keV band
Time interval of the image:
Plot creation:
Fri Feb 23 20:18:29 EST 2024