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
202.3958 47.0654 0.0081 37.1088 146.9556 2.0030748 23.624 TRIG_01101675
Foreground time interval of the image:
-0.548 10.149 (delta_t = 10.697 [sec])
Background time interval of the image:
-51.051 -0.548 (delta_t = 50.503 [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
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.512000
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 0.512000
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 0.512000
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 -0.548 sec. to 18.256 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.13695 ( -0.12535 0.130455 )
Norm@50keV : 7.12773E-03 ( -0.000625011 0.000616886 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 68.28 using 59 bins.
Reduced chi-squared = 1.19789
# Null hypothesis probability of 1.46e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 18.8 sec: 1.14237 ( -0.07859 0.07865 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.25008e-06 ( -9.79328e-08 9.91561e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.548 sec. to 18.256 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.15898 ( -0.613502 0.533713 )
Epeak [keV] : 35.6756 ( -10.0503 6.8226 )
Norm@50keV : 2.61070E-02 ( -0.0130798 0.0330975 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 57.37 using 59 bins.
Reduced chi-squared = 1.02446
# Null hypothesis probability of 4.24e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 18.8 sec: 1.10117 ( -0.08097 0.08115 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.15361e-06 ( -1.04239e-07 1.07952e-07 ) ergs/cm2
Band function
Time interval is from -0.548 sec. to 18.256 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] : 9.43685 (-0.759009 0.822712)
R^2/D10^2 : 0.651993 (-0.182884 0.255426)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 91.19 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.71e-03 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.174e-07 2.776e-08
25- 50 4.968e-07 3.854e-08
50-150 2.187e-07 4.158e-08
15-150 9.328e-07 7.623e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 53.9705 (-9.10579 12.1698)
Norm : 6.22858 (-0.677546 0.823881)
------------------------------------------------------------
#Fit statistic : Chi-Squared 57.58 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.53e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.910e-07 2.181e-08
25- 50 4.291e-07 6.383e-08
50-150 4.470e-07 1.465e-07
15-150 1.167e-06 2.421e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.74920 (-0.991767 1.04933)
R1^2/D10^2 : 3.13242 (-1.40803 3.16851)
kT2 [keV] : 17.1773 (-3.10235 4.50405)
R2^2/D10^2 : 4.08483E-02 (-0.0261449 0.0586568)
------------------------------------------------------------
#Fit statistic : Chi-Squared 53.44 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.34e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.886e-07 7.901e-08
25- 50 4.254e-07 1.280e-07
50-150 4.507e-07 2.303e-07
15-150 1.165e-06 3.920e-07
Peak spectrum fit
Power-law model
Time interval is from 2.476 sec. to 3.476 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.09386 ( -0.136789 0.142883 )
Norm@50keV : 3.08836E-02 ( -0.00323091 0.00319175 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 78.40 using 59 bins.
Reduced chi-squared = 1.37544
# Null hypothesis probability of 3.16e-02 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 4.84461 ( -0.41566 0.4158 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.86807e-07 ( -2.76458e-08 2.79533e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 2.476 sec. to 3.476 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -4.12222E-02 ( -0.942641 0.785074 )
Epeak [keV] : 39.4036 ( -4.13515 4.4791 )
Norm@50keV : 0.538059 ( -0.539948 1.40583 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 50.45 using 59 bins.
Reduced chi-squared = 0.900893
# Null hypothesis probability of 6.84e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 4.67404 ( -0.41718 0.41801 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.58607e-07 ( -2.63601e-08 2.75537e-08 ) ergs/cm2
Band function
Time interval is from 2.476 sec. to 3.476 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] : 10.0254 (-0.807478 0.869314)
R^2/D10^2 : 2.41271 (-0.671509 0.929671)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 57.21 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.67e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.943e-08 5.935e-09
25- 50 1.233e-07 1.190e-08
50-150 6.484e-08 1.520e-08
15-150 2.376e-07 2.365e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 55.8308 (-10.3941 13.4533)
Norm : 27.1140 (-3.46324 3.73934)
------------------------------------------------------------
#Fit statistic : Chi-Squared 59.63 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.80e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.729e-08 6.785e-09
25- 50 1.001e-07 8.740e-09
50-150 1.071e-07 2.416e-08
15-150 2.745e-07 2.850e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.14896 (-2.58565 2.66412)
R1^2/D10^2 : 7.40527 (-4.42455 34.3718)
kT2 [keV] : 13.4050 (-2.73245 8.51641)
R2^2/D10^2 : 0.533355 (-0.499796 0.708847)
------------------------------------------------------------
#Fit statistic : Chi-Squared 49.87 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.70e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.881e-08 3.111e-08
25- 50 1.127e-07 5.740e-08
50-150 8.764e-08 5.065e-08
15-150 2.592e-07 1.341e-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: 2.07289 ( -0.114532 0.118317 )
Norm@50keV : 1.09228E-02 ( -0.000860326 0.000850399 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 66.91 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.73e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 10.7 sec: 1.69581 ( -0.109742 0.109821 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.08321e-06 ( -7.87087e-08 7.94533e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.11985 ( -0.560002 0.491376 )
Epeak [keV] : 38.8575 ( -7.73913 6.8363 )
Norm@50keV : 3.83162E-02 ( -0.0180064 0.0420274 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 54.60 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.28e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 10.7 sec: 1.63678 ( -0.11295 0.11315 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.00171e-06 ( -8.47643e-08 8.71226e-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) = 3.91e-07
S(50-100 keV) = 3.55e-07
T90 vs. Hardness ratio plot
T90 = 17.2439999580383 sec.
Hardness ratio (energy fluence ratio) = 0.907928
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.03999
Count Ratio (50-100 keV) / (15-25 keV) = 0.527769
Mask shadow pattern
IMX = -6.341652372335767E-01, IMY = -4.125302674174665E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.512000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.512000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.512000
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:
-51.051400 -0.548000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.4086 35.1845 30.8 4.7 18.6 0.0358 0.4 9.8 Her X-1
268.4880 -1.5663 4.9 43.6 6.3 0.3910 2.4 9.9 SW J1753.5-0127
274.0149 -14.1197 5.9 57.2 4.4 1.0207 1.9 5.0 GX 17+2
288.6804 10.8765 5.8 42.5 -28.6 -0.3400 -2.0 8.1 GRS 1915+105
299.5804 35.2010 1.3 36.5 -69.5 1.8255 8.9 0.5 Cyg X-1
308.1922 41.0338 3.7 41.0 -81.8 1.1991 3.1 6.1 Cyg X-3
277.8208 17.6796 2.5 30.5 -22.3 0.5127 4.7 ------ UNKNOWN
286.4542 50.1673 2.5 25.3 -96.9 0.5653 4.6 ------ UNKNOWN
304.8104 38.5920 2.5 39.3 -77.0 1.2933 4.6 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-0.548000 10.148580
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.4578 35.3322 243.7 4.5 17.8 0.0020 0.0 0.6 Her X-1
268.2799 -1.5222 5.1 43.5 6.5 -0.1808 -2.3 6.7 SW J1753.5-0127
273.9900 -13.9963 5.9 57.1 4.4 0.5320 2.0 2.6 GX 17+2
288.8522 11.0604 7.9 42.5 -29.0 -0.1115 -1.5 7.6 GRS 1915+105
299.4210 35.2621 37.0 36.3 -69.5 0.0273 0.3 9.1 Cyg X-1
308.2433 40.9986 6.5 41.1 -81.8 -0.3260 -1.8 6.6 Cyg X-3
229.5167 4.1897 2.2 41.6 65.9 1.1268 5.3 ------ UNKNOWN
202.3958 47.0654 0.5 37.1 147.0 2.0030 23.6 ------ UNKNOWN
286.6969 45.6739 2.2 24.9 -86.3 0.2907 5.2 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
91.948590 183.111400
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.4526 35.4093 3.6 40.0 -8.9 -0.6173 -3.2 4.0 Her X-1
151.5640 24.8951 2.9 45.7 162.9 1.4388 4.0 ------ UNKNOWN
162.2029 48.7793 2.4 26.7 -167.8 0.6492 4.8 ------ UNKNOWN
128.0964 61.7596 2.0 43.0 -138.4 1.5248 5.7 ------ UNKNOWN
275.7708 58.8901 2.4 43.3 -50.3 1.6498 4.9 ------ UNKNOWN
Plot creation:
Mon Oct 24 05:02:57 EDT 2022