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
317.9449 25.3523 0.0107 30.3162 -22.4353 0.4002490 17.954 TRIG_01038247
Foreground time interval of the image:
-0.092 1.256 (delta_t = 1.348 [sec])
Background time interval of the image:
-19.083 -0.092 (delta_t = 18.991 [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 0.064000
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 0.064000
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 0.064000
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 -0.092 sec. to 1.256 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.45562 ( -0.165649 0.166856 )
Norm@50keV : 1.89549E-02 ( -0.00179892 0.00178719 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 53.63 using 59 bins.
Reduced chi-squared = 0.940877
# Null hypothesis probability of 6.02e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1.348 sec: 2.33926 ( -0.21723 0.2175 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.44287e-07 ( -2.5793e-08 2.61085e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.092 sec. to 1.256 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.45289 ( -0.574258 0.868206 )
Epeak [keV] : 9998.38 ( -9998.49 -9998.49 )
Norm@50keV : 1.90168E-02 ( -0.00558584 0.0193319 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 53.63 using 59 bins.
Reduced chi-squared = 0.957679
# Null hypothesis probability of 5.65e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1.348 sec: 1.51509 ( -0.37074 0.31911 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.44647e-07 ( -2.88976e-08 2.14498e-08 ) ergs/cm2
Band function
Time interval is from -0.092 sec. to 1.256 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] : 15.3465 (-1.89803 2.22318)
R^2/D10^2 : 0.242023 (-0.0898997 0.140834)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 86.67 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.85e-03 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.602e-08 2.627e-09
25- 50 6.500e-08 8.695e-09
50-150 1.052e-07 2.025e-08
15-150 1.863e-07 2.386e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-50.8925 -200)
Norm : 9.53581 (-0.876541 0.876541)
------------------------------------------------------------
#Fit statistic : Chi-Squared 55.28 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.40e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.213e-08 7.549e-09
25- 50 6.181e-08 1.794e-08
50-150 1.356e-07 7.174e-08
15-150 2.295e-07 8.680e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.14391 (-1.8282 2.5421)
R1^2/D10^2 : 3.77926 (-2.57894 6.82577)
kT2 [keV] : 26.0667 (-6.04711 15.0953)
R2^2/D10^2 : 3.30498E-02 (-0.0256391 0.051664)
------------------------------------------------------------
#Fit statistic : Chi-Squared 55.07 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.72e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.156e-08 1.555e-08
25- 50 5.751e-08 1.854e-08
50-150 1.518e-07 6.766e-08
15-150 2.408e-07 9.355e-08
Peak spectrum fit
Power-law model
Time interval is from -0.096 sec. to 0.904 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.39327 ( -0.163945 0.164686 )
Norm@50keV : 2.41883E-02 ( -0.00220385 0.00219379 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 55.52 using 59 bins.
Reduced chi-squared = 0.974035
# Null hypothesis probability of 5.31e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 2.94127 ( -0.26605 0.26642 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.34078e-07 ( -2.40535e-08 2.43324e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.096 sec. to 0.904 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.39025 ( -0.449063 0.200291 )
Epeak [keV] : 1.00000E+04 ( -10000 -10000 )
Norm@50keV : 2.42752E-02 ( -0.00221766 0.00215589 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 55.53 using 59 bins.
Reduced chi-squared = 0.991607
# Null hypothesis probability of 4.93e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 1.42409 ( -0.40211 0.44632 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.36331e-07 ( -2.68764e-08 2.17702e-08 ) ergs/cm2
Band function
Time interval is from -0.096 sec. to 0.904 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] : 16.1426 (-2.04649 2.41004)
R^2/D10^2 : 0.256677 (-0.0960363 0.15125)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 92.77 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.93e-03 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.380e-08 2.365e-09
25- 50 5.852e-08 7.245e-09
50-150 1.069e-07 1.876e-08
15-150 1.793e-07 2.220e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-39.3555 -200)
Norm : 12.0553 (-1.07686 1.07686)
------------------------------------------------------------
#Fit statistic : Chi-Squared 59.45 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.87e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.002e-08 4.635e-09
25- 50 5.774e-08 1.096e-08
50-150 1.266e-07 6.657e-08
15-150 2.144e-07 7.544e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.36847 (-1.96137 2.71772)
R1^2/D10^2 : 4.12874 (-2.82564 12.8653)
kT2 [keV] : 28.4161 (-6.94063 19.9183)
R2^2/D10^2 : 3.27748E-02 (-0.0262833 0.0533242)
------------------------------------------------------------
#Fit statistic : Chi-Squared 57.72 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.75e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.840e-08 1.229e-08
25- 50 5.310e-08 2.060e-08
50-150 1.531e-07 6.815e-08
15-150 2.346e-07 8.739e-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: 1.45562 ( -0.165649 0.166856 )
Norm@50keV : 1.89549E-02 ( -0.00179892 0.00178719 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 53.63 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.02e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1.348 sec: 2.33921 ( -0.217213 0.217491 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.44256e-07 ( -2.58373e-08 2.61144e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.45289 ( -0.574867 0.867274 )
Epeak [keV] : 9998.43 ( -9998.54 -9998.54 )
Norm@50keV : 1.90168E-02 ( -0.00558544 0.0193282 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 53.63 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.65e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1.348 sec: 2.33875 ( -0.21383 0.21664 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.442e-07 ( -2.74992e-08 2.60245e-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) = 5.90e-08
S(50-100 keV) = 8.61e-08
T90 vs. Hardness ratio plot
T90 = 1.12000000476837 sec.
Hardness ratio (energy fluence ratio) = 1.45932
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.33717
Count Ratio (50-100 keV) / (15-25 keV) = 1.04977
Mask shadow pattern
IMX = 5.404735181931878E-01, IMY = 2.231571670947622E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.064000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.064000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.064000
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:
-19.083400 -0.092000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
288.7594 10.9292 31.4 53.7 9.6 0.0798 0.4 2.5 GRS 1915+105
299.5880 35.3590 3.2 27.7 16.3 0.2406 3.6 9.4 Cyg X-1
307.8575 40.8811 0.0 19.4 11.7 0.2149 3.8 12.2 Cyg X-3
326.2987 38.4315 5.4 16.3 -35.6 0.1248 2.1 8.9 Cyg X-2
283.0477 13.5075 2.4 54.1 17.2 1.3120 4.8 ------ UNKNOWN
306.2217 -1.8534 2.2 59.4 -15.4 1.9746 5.2 ------ UNKNOWN
62.9687 41.4907 2.6 59.6 -161.4 1.7531 4.5 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-0.092000 1.256000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
288.7847 11.0568 8.5 53.6 9.7 0.1004 1.3 6.7 GRS 1915+105
299.5374 35.3408 4.6 27.7 16.4 -0.0558 -2.5 8.7 Cyg X-1
308.1924 40.7536 0.0 19.3 10.9 0.0081 0.4 12.5 Cyg X-3
325.9519 38.2698 4.6 16.5 -34.7 0.0458 2.5 10.8 Cyg X-2
317.9450 25.3524 0.6 30.3 -22.4 0.4002 18.0 ------ UNKNOWN
57.2925 38.0522 1.8 59.2 -154.9 0.7243 6.5 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
69.316600 962.859600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
288.9129 11.0574 6.6 31.0 46.5 2.4087 1.7 9.5 GRS 1915+105
299.6121 35.1663 2.4 18.6 104.8 5.0177 4.9 2.4 Cyg X-1
308.1315 40.9070 3.2 17.6 133.4 3.2739 3.6 2.9 Cyg X-3
326.1594 38.2187 5.9 14.6 -174.9 1.7566 2.0 6.2 Cyg X-2
280.7769 22.2548 3.0 34.0 71.4 7.3121 3.9 ------ UNKNOWN
310.6977 23.0244 2.7 7.0 50.7 3.2004 4.4 ------ UNKNOWN
302.4285 -3.6034 2.5 32.7 8.4 4.7651 4.7 ------ UNKNOWN
19.1401 43.7174 3.4 52.3 -148.2 8.9097 3.4 ------ UNKNOWN
Plot creation:
Sat Jul 30 07:08:48 EDT 2022