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
325.8913 4.2324 0.0108 39.9619 11.8350 4.1081163 17.776 TRIG_01223072
Foreground time interval of the image:
-24.620 49.869 (delta_t = 74.489 [sec])
Background time interval of the image:
-79.931 -24.620 (delta_t = 55.311 [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 4.096000
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 4.096000
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 4.096000
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 -24.620 sec. to 161.080 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.79909 ( -0.0857981 0.0867423 )
Norm@50keV : 2.57317E-03 ( -0.000126587 0.00012584 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 44.27 using 59 bins.
Reduced chi-squared = 0.776667
# Null hypothesis probability of 8.91e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 185.7 sec: 0.354469 ( -0.01688 0.016915 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.39979e-06 ( -2.20602e-07 2.21806e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -24.620 sec. to 161.080 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.63334 ( -0.343946 0.235639 )
Epeak [keV] : 104.956 ( -42.6992 -104.957 )
Norm@50keV : 3.14206E-03 ( -0.000673442 0.00157133 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 43.50 using 59 bins.
Reduced chi-squared = 0.776786
# Null hypothesis probability of 8.89e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 185.7 sec: 0.351013 ( -0.018115 0.01812 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.33283e-06 ( -2.55909e-07 2.49772e-07 ) ergs/cm2
Band function
Time interval is from -24.620 sec. to 161.080 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] : 12.3197 ( )
R^2/D10^2 : 7.39754E-02 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 161.90 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.46e-12 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.418e-07 3.965e-08
25- 50 1.433e-06 7.075e-08
50-150 1.331e-06 1.406e-07
15-150 3.206e-06 1.727e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 104.439 (-16.4568 27.9315)
Norm : 1.53931 (-0.109947 0.104311)
------------------------------------------------------------
#Fit statistic : Chi-Squared 46.13 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.48e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.471e-07 6.249e-08
25- 50 1.303e-06 7.242e-08
50-150 2.163e-06 5.841e-07
15-150 4.213e-06 6.342e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.63232 (-0.902133 0.979157)
R1^2/D10^2 : 0.533069 (-0.202521 0.373737)
kT2 [keV] : 24.7936 (-3.97647 6.24439)
R2^2/D10^2 : 4.20120E-03 (-0.0023279 0.00400063)
------------------------------------------------------------
#Fit statistic : Chi-Squared 44.47 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.44e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.428e-07 1.040e-07
25- 50 1.284e-06 1.494e-07
50-150 2.267e-06 5.109e-07
15-150 4.294e-06 6.091e-07
Peak spectrum fit
Power-law model
Time interval is from 116.284 sec. to 117.284 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.58624 ( -0.138439 0.14122 )
Norm@50keV : 1.62217E-02 ( -0.00139728 0.00138554 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 56.03 using 59 bins.
Reduced chi-squared = 0.982982
# Null hypothesis probability of 5.11e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 2.07584 ( -0.16821 0.16832 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.51988e-07 ( -1.41148e-08 1.42805e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 116.284 sec. to 117.284 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.825574 ( -0.727336 0.617601 )
Epeak [keV] : 73.5289 ( -16.4939 103.308 )
Norm@50keV : 4.06429E-02 ( -0.0210435 0.0559821 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 51.50 using 59 bins.
Reduced chi-squared = 0.919643
# Null hypothesis probability of 6.46e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 2.01023 ( -0.17756 0.17654 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.42702e-07 ( -1.58784e-08 1.61234e-08 ) ergs/cm2
Band function
Time interval is from 116.284 sec. to 117.284 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] : 13.5833 (-1.22796 1.36828)
R^2/D10^2 : 0.335309 (-0.0975973 0.135045)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 70.76 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.04e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.310e-08 1.825e-09
25- 50 4.725e-08 4.670e-09
50-150 5.650e-08 9.200e-09
15-150 1.169e-07 1.280e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 168.457 (-54.4216 -168.456)
Norm : 8.55261 (-0.732192 0.816806)
------------------------------------------------------------
#Fit statistic : Chi-Squared 52.82 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.33e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.173e-08 3.085e-09
25- 50 4.092e-08 1.257e-08
50-150 8.457e-08 4.175e-08
15-150 1.472e-07 5.146e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 4.71385 (-2.33692 6.54349)
R1^2/D10^2 : 6.70863 (-5.86997 194.433)
kT2 [keV] : 17.1735 (-2.96622 51.6196)
R2^2/D10^2 : 0.127153 (-0.122871 0.140098)
------------------------------------------------------------
#Fit statistic : Chi-Squared 54.17 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.06e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.043e-08 9.130e-09
25- 50 4.118e-08 1.114e-08
50-150 7.198e-08 2.140e-08
15-150 1.336e-07 3.293e-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: 1.73537 ( -0.118168 0.119843 )
Norm@50keV : 3.21587E-03 ( -0.000236018 0.000234313 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 45.39 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.66e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 74.49 sec: 0.432518 ( -0.0303678 0.0304074 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.21238e-06 ( -1.67881e-07 1.68952e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.24351 ( -0.540779 0.474914 )
Epeak [keV] : 71.3529 ( -17.4694 359.702 )
Norm@50keV : 5.91273E-03 ( -0.00257817 0.00553052 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 42.25 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.13e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 74.49 sec: 0.424069 ( -0.031482 0.031467 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.12445e-06 ( -1.89644e-07 1.89689e-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) = 1.24e-06
S(50-100 keV) = 1.42e-06
T90 vs. Hardness ratio plot
T90 = 144.551999926567 sec.
Hardness ratio (energy fluence ratio) = 1.14516
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.15606
Count Ratio (50-100 keV) / (15-25 keV) = 0.700622
Mask shadow pattern
IMX = 8.201534568808309E-01, IMY = -1.718620511270201E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 4.096000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 4.096000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 4.096000
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:
-79.931400 -24.620000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
299.5286 35.1882 1.7 35.5 78.3 1.8217 6.7 3.1 Cyg X-1
308.0528 40.8775 5.0 27.4 85.0 0.4017 2.3 5.2 Cyg X-3
326.1010 38.2495 6.0 14.3 69.0 -0.2039 -1.9 5.5 Cyg X-2
73.5927 66.3009 2.2 53.2 -167.6 1.4418 5.2 ------ UNKNOWN
354.3809 15.1999 2.4 26.8 -39.5 0.5435 4.9 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-24.620000 49.868600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
299.8047 35.1015 0.0 35.3 78.0 0.4089 1.2 12.1 Cyg X-1
307.9345 40.8052 0.0 27.5 84.9 -0.3010 -1.3 11.9 Cyg X-3
326.1204 38.2628 4.1 14.3 69.0 0.4388 2.9 4.3 Cyg X-2
325.8914 4.2324 0.6 40.0 11.8 4.1082 17.8 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
136.068600 789.368600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
288.6883 11.0373 6.8 37.4 113.6 -4.0901 -1.7 8.5 GRS 1915+105
299.5946 35.2141 0.7 39.4 156.2 21.7101 15.5 0.8 Cyg X-1
308.1266 40.9169 5.6 40.0 169.9 2.8280 2.0 2.3 Cyg X-3
326.1665 38.4720 8.7 34.3 -168.7 -1.2450 -1.3 9.0 Cyg X-2
307.5750 -38.1965 3.0 45.7 31.1 7.4645 3.8 ------ UNKNOWN
340.1664 62.5746 3.1 59.3 -161.5 22.6625 3.7 ------ UNKNOWN
3.2929 38.1649 3.1 48.1 -129.1 14.4155 3.7 ------ UNKNOWN
Plot creation:
Sat Oct 19 18:28:40 EDT 2024