Estimated redshift from machine learning (Ukwatta et al. 2016) - may take a few minute to calcaulte
Image
Pre-slew 15.0-350.0 keV image (Event data)
# RAcent DECcent POSerr Theta Phi Peak Cts SNR Name
173.7597 -49.1655 0.0188 12.9739 129.1905 0.2421616 10.246 TRIG_01059460
Foreground time interval of the image:
-0.688 2.440 (delta_t = 3.128 [sec])
Background time interval of the image:
-239.416 -0.688 (delta_t = 238.728 [sec])
Lightcurves
Notes:
- 1) The mask-weighted light curves are using the flight position.
- 2) Multiple plots of different time binning/intervals are shown to cover all scenarios of short/long GRBs, rate/image triggers, and real/false positives.
- 3) 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.
- 4) 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.
- 5) 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)
Quad-rate summed light curves (from T0-300s to T0+1000s)
Spectral Evolution
Spectra
Notes:
- 1) The fitting includes the systematic errors.
- 2) When the burst includes telescope slew time periods, the fitting uses an average response file made from multiple 5-s response files through out the slew time plus single time preiod for the non-slew times, and weighted by the total counts in the corresponding time period using addrmf. An average response file is needed becuase a spectral fit using 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.
Time averaged spectrum fit using the average DRM
Power-law model
Time interval is from -0.688 sec. to 2.440 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.05009 ( -0.276571 0.301953 )
Norm@50keV : 3.62410E-03 ( -0.000811058 0.000798302 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 60.53 using 59 bins.
Reduced chi-squared = 1.06193
# Null hypothesis probability of 3.50e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 3.128 sec: 0.556551 ( -0.093715 0.093749 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.04859e-07 ( -2.14189e-08 2.22879e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.688 sec. to 2.440 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -2.87834 ( -5.24446 2.25735 )
Epeak [keV] : 34.1068 ( -4.32279 5.63623 )
Norm@50keV : 5.12786 ( -4.84372 4453.52 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 47.62 using 59 bins.
Reduced chi-squared = 0.850357
# Null hypothesis probability of 7.80e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 3.128 sec: 0.524800 ( -0.091281 0.091813 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.14118e-08 ( -1.58038e-08 1.84333e-08 ) ergs/cm2
Band function
Time interval is from -0.688 sec. to 2.440 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : ( )
beta : ( )
Epeak [keV] : ( )
Norm@50keV : ( )
------------------------------------------------------------
Photon flux (15-150 keV) in 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] : 8.92530 (-1.19438 1.40144)
R^2/D10^2 : 0.449364 (-0.19727 0.334623)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 48.03 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.96e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.171e-08 5.817e-09
25- 50 4.553e-08 1.051e-08
50-150 1.693e-08 7.471e-09
15-150 8.417e-08 1.885e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 51.3232 (-16.7525 31.9109)
Norm : 3.21710 (-0.745782 0.993182)
------------------------------------------------------------
#Fit statistic : Chi-Squared 55.06 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.48e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.475e-08 5.160e-09
25- 50 3.588e-08 7.665e-09
50-150 3.569e-08 1.839e-08
15-150 9.632e-08 2.638e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 9.02752 (-25.6037 -25.6037)
R1^2/D10^2 : 0.426060 (-0.000704095 0.77508)
kT2 [keV] : 0.458953 (-8.66426 1.46362)
R2^2/D10^2 : 2.50286E+11 (-2.71665e+11 6.17899e+18)
------------------------------------------------------------
#Fit statistic : Chi-Squared 47.74 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.46e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.198e-08 1.288e-08
25- 50 4.478e-08 3.034e-08
50-150 2.064e-08 2.285e-08
15-150 8.740e-08 6.347e-08
Peak spectrum fit
Power-law model
Time interval is from -0.144 sec. to 0.856 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.85172 ( -0.313894 0.341741 )
Norm@50keV : 5.91102E-03 ( -0.00142713 0.00139335 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 81.53 using 59 bins.
Reduced chi-squared = 1.43035
# Null hypothesis probability of 1.82e-02 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.831487 ( -0.166777 0.166781 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.43526e-08 ( -1.28161e-08 1.32464e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.144 sec. to 0.856 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -1.66898 ( -5.48049 2.28661 )
Epeak [keV] : 40.8684 ( -6.5207 11.007 )
Norm@50keV : 0.731618 ( -0.836631 1772.26 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 73.06 using 59 bins.
Reduced chi-squared = 1.30464
# Null hypothesis probability of 6.25e-02 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.778478 ( -0.166525 0.167851 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.3443e-08 ( -1.03246e-08 1.25843e-08 ) ergs/cm2
Band function
Time interval is from -0.144 sec. to 0.856 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : ( )
beta : ( )
Epeak [keV] : ( )
Norm@50keV : ( )
------------------------------------------------------------
Photon flux (15-150 keV) in 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] : 10.5005 (-1.66947 2.05178)
R^2/D10^2 : 0.369386 (-0.18404 0.336642)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 73.14 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.36e-02 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.419e-09 2.854e-09
25- 50 2.239e-08 6.400e-09
50-150 1.344e-08 6.394e-09
15-150 4.425e-08 1.376e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 75.2542 (-31.0961 81.5245)
Norm : 4.11142 (-1.12686 1.31369)
------------------------------------------------------------
#Fit statistic : Chi-Squared 78.30 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.22e-02 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.062e-08 2.874e-09
25- 50 1.722e-08 5.666e-09
50-150 2.331e-08 1.711e-08
15-150 5.115e-08 2.171e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 1.00008E-04 (1.92006e-08 -0.000100008)
R1^2/D10^2 : 1.14181E+04 (-11418.1 -11418.1)
kT2 [keV] : 10.5005 (-1.66945 2.05179)
R2^2/D10^2 : 0.369388 (-0.184042 0.33664)
------------------------------------------------------------
#Fit statistic : Chi-Squared 73.14 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.14e-02 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 9.426e-09 3.985e-09
25- 50 2.214e-08 8.813e-09
50-150 1.029e-08 5.301e-09
15-150 4.185e-08 1.343e-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: 2.05009 ( -0.276571 0.301953 )
Norm@50keV : 3.62410E-03 ( -0.000811058 0.000798302 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 60.53 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.50e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 3.128 sec: 0.556507 ( -0.0937089 0.0937422 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.04835e-07 ( -2.14112e-08 2.23164e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -2.88138 ( -5.23859 2.26193 )
Epeak [keV] : 34.1049 ( -4.3194 5.63691 )
Norm@50keV : 5.15097 ( -4.86003 4454.8 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 47.62 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.80e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 3.128 sec: 0.524770 ( -0.091281 0.091784 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.14315e-08 ( -1.58058e-08 1.84152e-08 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : ( )
beta : ( )
Epeak [keV] : ( )
Norm@50keV : ( )
------------------------------------------------------------
Photon flux (15-150 keV) in 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) = 3.19e-08
S(50-100 keV) = 3.09e-08
T90 vs. Hardness ratio plot
T90 = 2.77199995517731 sec.
Hardness ratio (energy fluence ratio) = 0.968652
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.56051
Count Ratio (50-100 keV) / (15-25 keV) = 0.381382
Mask shadow pattern
IMX = -1.455828367530893E-01, IMY = -1.785626666599883E-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:
-239.416000 -0.688000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.5046 -40.5633 3.1 25.9 -144.1 1.0765 3.7 1.2 Vela X-1
170.5635 -60.5271 5.1 23.8 142.1 0.7493 2.3 9.3 Cen X-3
186.6492 -62.7317 3.7 28.3 127.1 1.2770 3.1 2.3 GX 301-2
217.2284 -16.9220 2.6 47.1 43.2 4.1814 4.5 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-0.688000 2.440000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.7447 -40.6075 25.1 25.7 -144.2 0.0119 0.5 10.3 Vela X-1
170.2932 -60.6642 4.0 23.9 142.4 0.0821 2.9 2.6 Cen X-3
186.5495 -62.7730 10.6 28.3 127.2 -0.0369 -1.1 2.9 GX 301-2
218.2175 -65.8442 1.9 40.7 116.0 0.5468 6.2 ------ UNKNOWN
173.7597 -49.1656 1.1 13.0 129.2 0.2422 10.2 ------ UNKNOWN
192.3580 9.1146 2.3 51.0 -4.6 0.2740 5.1 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
44.284590 705.184630
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.5529 -40.5676 1.4 28.0 -118.8 6.5643 8.6 1.4 Vela X-1
170.3476 -60.5912 3.0 11.6 156.1 2.3901 3.8 2.1 Cen X-3
186.6957 -62.6488 3.0 15.3 124.8 2.5296 3.9 7.4 GX 301-2
218.9898 -23.7180 3.6 43.5 38.9 4.2847 3.2 ------ UNKNOWN
152.4072 -58.3189 2.4 15.5 -166.4 3.1822 4.8 ------ UNKNOWN
170.7001 -9.4388 2.7 39.8 -36.7 4.5365 4.2 ------ UNKNOWN
154.0943 -7.4968 3.9 44.8 -60.2 8.6267 3.0 ------ UNKNOWN
Plot creation:
Sat Jul 30 06:56:42 EDT 2022