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
266.9022 -68.2297 0.0049 34.2185 -38.6316 9.6602545 38.864 TRIG_01142847
Foreground time interval of the image:
-13.299 22.920 (delta_t = 36.219 [sec])
Background time interval of the image:
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 -20.884 sec. to 22.920 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.63299 ( -0.0476073 0.0476358 )
Norm@50keV : 2.09075E-02 ( -0.000529787 0.000529753 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 79.99 using 59 bins.
Reduced chi-squared = 1.40333
# Null hypothesis probability of 2.40e-02 with 57 degrees of freedom
Photon flux (15-150 keV) in 43.8 sec: 2.71500 ( -0.07862 0.07891 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.53303e-06 ( -2.22395e-07 2.22737e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -20.884 sec. to 22.920 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.38947 ( -0.19547 0.187071 )
Epeak [keV] : 135.829 ( -37.3972 238.167 )
Norm@50keV : 2.71193E-02 ( -0.00479441 0.00612133 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 74.99 using 59 bins.
Reduced chi-squared = 1.33911
# Null hypothesis probability of 4.59e-02 with 56 degrees of freedom
Photon flux (15-150 keV) in 43.8 sec: 2.66422 ( -0.08673 0.08715 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.39585e-06 ( -2.46663e-07 2.45752e-07 ) ergs/cm2
Band function
Time interval is from -20.884 sec. to 22.920 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] : 15.5476 ( )
R^2/D10^2 : 0.251672 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 404.67 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.05e-54 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.543e-07 2.869e-08
25- 50 2.275e-06 8.212e-08
50-150 3.800e-06 1.653e-07
15-150 6.629e-06 1.949e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 179.203 (-23.1678 -178.938)
Norm : 10.9052 (-0.334244 0.362202)
------------------------------------------------------------
#Fit statistic : Chi-Squared 75.70 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.94e-02 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.205e-06 5.957e-08
25- 50 2.288e-06 1.314e-07
50-150 4.838e-06 1.100e-06
15-150 8.331e-06 1.194e-06
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 8.13365 (-0.697628 0.720807)
R1^2/D10^2 : 1.77143 (-0.429805 0.623494)
kT2 [keV] : 29.7536 (-3.09995 4.1556)
R2^2/D10^2 : 1.87543E-02 (-0.00692671 0.00942515)
------------------------------------------------------------
#Fit statistic : Chi-Squared 77.81 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.32e-02 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.054e-06 7.227e-08
25- 50 2.395e-06 1.303e-07
50-150 4.879e-06 4.187e-07
15-150 8.327e-06 4.687e-07
Peak spectrum fit
Power-law model
Time interval is from -13.508 sec. to -12.508 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.01451 ( -0.0860821 0.0851776 )
Norm@50keV : 9.65000E-02 ( -0.00496326 0.004957 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 58.17 using 59 bins.
Reduced chi-squared = 1.02053
# Null hypothesis probability of 4.32e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.456917 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 1.03829e-06 ( -5.72652e-08 5.74058e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -13.508 sec. to -12.508 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.628913 ( -0.373398 0.343528 )
Epeak [keV] : 205.840 ( -73.6344 793.272 )
Norm@50keV : 0.143608 ( -0.041917 0.0647199 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 54.48 using 59 bins.
Reduced chi-squared = 0.972857
# Null hypothesis probability of 5.33e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 10.9978 ( -0.5928 0.593 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.02542e-06 ( -5.96583e-08 5.93309e-08 ) ergs/cm2
Band function
Time interval is from -13.508 sec. to -12.508 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] : 21.6565 (-1.44083 1.58702)
R^2/D10^2 : 0.425332 (-0.0854543 0.104394)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 108.60 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.56e-05 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.718e-08 3.780e-09
25- 50 1.948e-07 1.465e-08
50-150 6.822e-07 5.030e-08
15-150 9.141e-07 5.890e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.363 ( )
Norm : 45.0096 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared 160.59 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.46e-12 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.121e-07 5.850e-09
25- 50 2.156e-07 1.330e-08
50-150 4.728e-07 7.735e-08
15-150 8.005e-07 8.745e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 11.1244 (-2.87345 3.18892)
R1^2/D10^2 : 2.03291 (-0.885411 2.30005)
kT2 [keV] : 42.4862 (-11.6435 81.2611)
R2^2/D10^2 : 4.06712E-02 (-0.0336264 0.0756879)
------------------------------------------------------------
#Fit statistic : Chi-Squared 55.80 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.44e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.174e-08 1.214e-08
25- 50 2.140e-07 4.565e-08
50-150 7.528e-07 2.987e-07
15-150 1.029e-06 3.280e-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: 1.75478 ( -0.0547709 0.0549511 )
Norm@50keV : 1.84237E-02 ( -0.000550068 0.000549575 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 75.55 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.06e-02 with 57 degrees of freedom
Photon flux (15-150 keV) in 36.22 sec: 2.49559 ( -0.082262 0.0825604 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.15581e-06 ( -1.87749e-07 1.8797e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.37399 ( -0.235367 0.223009 )
Epeak [keV] : 84.5512 ( -14.7019 45.9655 )
Norm@50keV : 2.82021E-02 ( -0.00608095 0.00828675 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 66.75 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.54e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 36.22 sec: 2.42697 ( -0.0903 0.09068 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.988e-06 ( -2.13118e-07 2.12141e-07 ) 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) = 2.25e-06
S(50-100 keV) = 2.90e-06
T90 vs. Hardness ratio plot
T90 = 33.7199999094009 sec.
Hardness ratio (energy fluence ratio) = 1.28889
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.39637
Count Ratio (50-100 keV) / (15-25 keV) = 0.988423
Mask shadow pattern
IMX = 5.312556052117654E-01, IMY = 4.245756649878484E-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:
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-13.299410 22.920000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.5291 -40.5548 56.2 33.2 114.3 -0.0546 -0.2 0.0 Vela X-1
170.4636 -60.4776 4.5 4.0 122.2 0.4228 2.6 9.8 Cen X-3
186.6666 -62.8088 2.0 4.2 -81.2 0.8384 5.8 2.3 GX 301-2
95.6286 -53.5340 2.8 41.2 66.0 1.9002 4.2 ------ UNKNOWN
63.4220 -58.3858 2.3 48.9 42.1 2.9700 5.0 ------ UNKNOWN
152.9869 -23.4125 3.1 42.6 148.3 1.3727 3.8 ------ UNKNOWN
69.2969 -74.8706 2.5 34.9 28.3 0.9191 4.7 ------ UNKNOWN
122.0019 -70.2876 2.5 22.5 49.2 0.8350 4.7 ------ UNKNOWN
266.9022 -68.2297 0.3 34.2 -38.6 9.6580 38.8 ------ UNKNOWN
191.8339 -6.0270 2.0 57.6 -160.5 5.3874 5.6 ------ UNKNOWN
195.1307 -11.8913 3.0 52.3 -155.5 1.8157 3.9 ------ UNKNOWN
214.1379 -29.7618 2.0 40.4 -124.5 2.3881 5.9 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
158.300590 830.239400
831.000000 833.909500
835.000000 940.958000
942.000000 963.045400
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
170.4508 -60.5959 5.3 38.0 167.1 2.2767 2.2 4.3 Cen X-3
186.5595 -62.7622 1.4 31.3 174.8 6.4980 8.1 2.7 GX 301-2
255.9366 -37.8641 2.2 31.0 -82.4 5.6044 5.2 2.7 4U 1700-377
256.3407 -36.3650 6.2 32.4 -81.4 2.2974 1.9 5.8 GX 349+2
264.6472 -44.6356 0.0 23.6 -69.4 -0.1243 -0.1 11.9 4U 1735-44
270.3211 -24.9375 2.1 43.3 -60.9 12.2037 5.4 8.7 GX 5-1
270.2047 -25.6247 5.2 42.6 -61.0 4.7406 2.2 8.9 GRS 1758-258
275.7564 -30.2820 5.5 38.3 -53.0 2.8224 2.1 10.1 H1820-303
284.8530 -24.8665 11.4 44.7 -42.0 -1.5452 -1.0 10.5 HT1900.1-2455
262.7680 -33.7399 0.0 34.6 -71.5 -2.1311 -1.5 12.4 GX 354-0
327.7949 -70.9172 3.0 20.5 60.0 3.0256 3.8 ------ UNKNOWN
310.4203 -30.9769 2.5 44.9 -8.6 4.2297 4.6 ------ UNKNOWN
188.7730 -35.5829 3.0 53.0 -159.7 7.4803 3.8 ------ UNKNOWN
Plot creation:
Fri Oct 13 22:56:46 EDT 2023