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
246.0007 -15.4534 0.0269 55.0 -11.3 9.8046 7.2 TRIG_01218414
------------------------------------------
Foreground time interval of the image:
0.000 233.050 (delta_t = 233.050 [sec])
234.000 287.500 (delta_t = 53.500 [sec])
291.000 363.050 (delta_t = 72.050 [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
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 472.000000
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 472.000000
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 472.000000
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
0.000000 233.050000
234.000000 287.500000
291.000000 363.050000
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 5.37117 ( -0.597265 0.66267 )
Norm@50keV : 1.82757E-04 ( -8.84196e-05 0.000135867 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 69.83 using 59 PHA bins.
# Reduced chi-squared = 1.225 for 57 degrees of freedom
# Null hypothesis probability = 1.183161e-01
Photon flux (15-150 keV) in 358.6 sec: 0.403481 ( -0.0502623 0.0503253 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.50645e-06 ( -5.6288e-07 5.65139e-07 ) ergs/cm2
Cutoff power-law model
Multiple GTIs in the spectrum
tstart tstop
0.000000 233.050000
234.000000 287.500000
291.000000 363.050000
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.81622 ( )
Epeak [keV] : 1.12184 ( )
Norm@50keV : 0.135316 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 69.41 using 59 PHA bins.
# Reduced chi-squared = 1.240 for 56 degrees of freedom
# Null hypothesis probability = 1.074501e-01
Photon flux (15-150 keV) in 358.6 sec: 0.397178 ( -0.051614 0.051685 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.37105e-06 ( -5.68883e-07 6.25255e-07 ) ergs/cm2
Band function
Multiple GTIs in the spectrum
tstart tstop
0.000000 233.050000
234.000000 287.500000
291.000000 363.050000
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -8.59753 ( 5.81563 8.59753 )
beta : -5.44919 ( -0.602738 0.66636 )
Epeak [keV] : 373.883 ( -373.883 -373.883 )
Norm@50keV : 2.29900E-02 ( -0.0107789 0.0198396 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 69.88 using 59 PHA bins.
# Reduced chi-squared = 1.270 for 55 degrees of freedom
# Null hypothesis probability = 8.535732e-02
Photon flux (15-150 keV) in 358.6 sec: 0.309972 ( ) 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] : 2.89561 (-0.354591 0.40608)
R^2/D10^2 : 68.6962 (-40.3923 107.326)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 71.34 using 59 PHA bins.
# Reduced chi-squared = 1.252 for 57 degrees of freedom
# Null hypothesis probability = 9.585309e-02
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.684e-06 1.418e-06
25- 50 4.736e-07 2.038e-07
50-150 5.692e-10 4.968e-10
15-150 4.158e-06 1.365e-06
Thermal bremsstrahlung (OTTB)
XSPEC12>exit
XSPEC: quit
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 5.48877 (-0.991198 1.28964)
Norm : 65.5607 (-32.8949 73.9568)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.712e-06 1.148e-06
25- 50 5.753e-07 2.239e-07
50-150 4.677e-09 4.048e-09
15-150 4.292e-06 1.335e-06
Double BB
XSPEC12>exit
XSPEC: quit
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 0.983576 (-0.956191 1.53743)
R1^2/D10^2 : 8.30697E+05 (-813486 -813592)
kT2 [keV] : 3.29543 (-0.544178 2.42284)
R2^2/D10^2 : 26.1479 (-24.6223 35.0731)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.685e-06 1.484e-06
25- 50 5.056e-07 2.057e-07
50-150 3.399e-07 2.176e-07
15-150 4.531e-06 1.677e-06
Peak spectrum fit
Power-law model
Time interval is from 291.000 sec. to 363.050 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 5.37117 ( -0.597265 0.66267 )
Norm@50keV : 1.82757E-04 ( -8.84196e-05 0.000135867 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 69.83 using 59 PHA bins.
# Reduced chi-squared = 1.225 for 57 degrees of freedom
# Null hypothesis probability = 1.183161e-01
Photon flux (15-150 keV) in 358.6 sec: 0.403481 ( -0.0502623 0.0503253 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.50645e-06 ( -5.6288e-07 5.65139e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from 291.000 sec. to 363.050 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.81622 ( )
Epeak [keV] : 1.12184 ( )
Norm@50keV : 0.135316 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 69.41 using 59 PHA bins.
# Reduced chi-squared = 1.240 for 56 degrees of freedom
# Null hypothesis probability = 1.074501e-01
Photon flux (15-150 keV) in 358.6 sec: 0.397178 ( -0.051614 0.051685 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.37105e-06 ( -5.68883e-07 6.25255e-07 ) ergs/cm2
Band function
Time interval is from 291.000 sec. to 363.050 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -8.59753 ( 5.81563 8.59753 )
beta : -5.44919 ( -0.602738 0.66636 )
Epeak [keV] : 373.883 ( -373.883 -373.883 )
Norm@50keV : 2.29900E-02 ( -0.0107789 0.0198396 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 69.88 using 59 PHA bins.
# Reduced chi-squared = 1.270 for 55 degrees of freedom
# Null hypothesis probability = 8.535732e-02
Photon flux (15-150 keV) in 358.6 sec: 0.309972 ( ) 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] : 2.89561 (-0.354591 0.40608)
R^2/D10^2 : 68.6962 (-40.3923 107.326)
(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 3.684e-06 1.165e-06
25- 50 4.736e-07 2.564e-07
50-150 5.692e-10 4.767e-10
15-150 4.158e-06 1.455e-06
Thermal bremsstrahlung (OTTB)
XSPEC12>exit
XSPEC: quit
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 5.48877 (-0.991198 1.28964)
Norm : 65.5607 (-32.8949 73.9568)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.712e-06 1.014e-06
25- 50 5.753e-07 2.315e-07
50-150 4.677e-09 3.890e-09
15-150 4.292e-06 1.148e-06
Double BB
XSPEC12>exit
XSPEC: quit
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 0.983576 (-1.14103 1.53728)
R1^2/D10^2 : 8.30697E+05 (-813486 -813592)
kT2 [keV] : 3.29543 (-0.544178 2.42284)
R2^2/D10^2 : 26.1479 (-24.6223 35.0731)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.685e-06 1.544e-06
25- 50 5.056e-07 2.150e-07
50-150 3.399e-07 3.758e-07
15-150 4.531e-06 1.660e-06
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: 5.37117 ( -0.597265 0.66267 )
Norm@50keV : 1.82757E-04 ( -8.84196e-05 0.000135867 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 69.83 using 59 PHA bins.
# Reduced chi-squared = 1.225 for 57 degrees of freedom
# Null hypothesis probability = 1.183161e-01
Photon flux (15-150 keV) in 358.6 sec: 0.403481 ( -0.0502623 0.0503253 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.50645e-06 ( -5.6288e-07 5.65139e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.81622 ( )
Epeak [keV] : 1.12184 ( )
Norm@50keV : 0.135316 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 69.41 using 59 PHA bins.
# Reduced chi-squared = 1.240 for 56 degrees of freedom
# Null hypothesis probability = 1.074501e-01
Photon flux (15-150 keV) in 358.6 sec: 0.397178 ( -0.051614 0.051685 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.37105e-06 ( -5.68883e-07 6.25255e-07 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -8.59753 ( 5.81563 8.59753 )
beta : -5.44919 ( -0.602738 0.66636 )
Epeak [keV] : 373.883 ( -373.883 -373.883 )
Norm@50keV : 2.29900E-02 ( -0.0107789 0.0198396 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 69.88 using 59 PHA bins.
# Reduced chi-squared = 1.270 for 55 degrees of freedom
# Null hypothesis probability = 8.535732e-02
Photon flux (15-150 keV) in 358.6 sec: 0.309972 ( ) 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) = 7.28e-07
S(50-100 keV) = 7.03e-08
T90 vs. Hardness ratio plot
T90 = 472 sec.
Hardness ratio (energy fluence ratio) = 0.0965659
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 0.214998
Count Ratio (50-100 keV) / (15-25 keV) = 0.00430183
Mask shadow pattern
IMX = 1.398502806912078E+00, IMY = 2.791186164796267E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 472.000000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 472.000000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 472.000000
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:
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
0.000000 233.050000
234.000000 287.500000
291.000000 363.050000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
244.9929 -15.6749 5.0 54.7 -10.1 -3.1945 -2.3 2.2 Sco X-1
254.3526 35.2090 7.6 27.7 -83.4 -1.0335 -1.5 9.5 Her X-1
214.4819 -18.5710 4.0 52.8 26.3 5.0120 2.9 ------ UNKNOWN
170.6757 47.5666 2.5 39.5 144.7 5.0602 4.7 ------ UNKNOWN
184.5513 54.1660 2.6 32.3 158.9 3.0322 4.5 ------ UNKNOWN
212.7272 75.5917 2.8 41.9 -163.9 3.0458 4.2 ------ UNKNOWN
246.0007 -15.4534 1.6 55.0 -11.3 9.8092 7.1 ------ UNKNOWN
252.1296 -14.2903 2.2 56.8 -18.2 9.1941 5.2 ------ UNKNOWN
265.2957 60.1137 2.6 39.0 -127.1 4.0021 4.4 ------ UNKNOWN
268.7136 35.9399 2.6 39.1 -88.1 8.2819 4.5 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
Plot creation:
Sun Mar 3 20:42:50 EST 2024