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
27.0307 -6.3472 0.0078 41.5243 -0.5153 2.8098263 24.758 TRIG_01061223
Foreground time interval of the image:
-4.404 13.861 (delta_t = 18.265 [sec])
Background time interval of the image:
-239.440 -4.404 (delta_t = 235.036 [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 1.024000
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 1.024000
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 1.024000
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 -4.404 sec. to 59.592 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.53653 ( -0.113846 0.114705 )
Norm@50keV : 4.05934E-03 ( -0.000273729 0.000273063 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 62.79 using 59 bins.
Reduced chi-squared = 1.10158
# Null hypothesis probability of 2.79e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 64 sec: 0.511922 ( -0.035126 0.035193 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.45087e-06 ( -1.77341e-07 1.78371e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -4.404 sec. to 59.592 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.986298 ( -0.5144 0.459836 )
Epeak [keV] : 94.8136 ( -23.9729 188.343 )
Norm@50keV : 7.57978E-03 ( -0.00302044 0.00578788 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 58.53 using 59 bins.
Reduced chi-squared = 1.04518
# Null hypothesis probability of 3.83e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 64 sec: 0.498875 ( -0.036779 0.03679 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.36876e-06 ( -1.91597e-07 1.91775e-07 ) ergs/cm2
Band function
Time interval is from -4.404 sec. to 59.592 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] : 15.3721 (-1.20421 1.32085)
R^2/D10^2 : 5.32437E-02 (-0.0135464 0.0179338)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 98.75 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.04e-04 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.679e-07 2.262e-08
25- 50 6.820e-07 5.443e-08
50-150 1.108e-06 1.424e-07
15-150 1.958e-06 1.510e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.326 (-50.6269 -199.338)
Norm : 2.09483 (-0.137847 0.138061)
------------------------------------------------------------
#Fit statistic : Chi-Squared 59.56 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.83e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.338e-07 2.691e-08
25- 50 6.422e-07 5.930e-08
50-150 1.408e-06 3.242e-07
15-150 2.384e-06 4.179e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.36897 (-1.75796 2.2487)
R1^2/D10^2 : 0.645836 (-0.399651 1.52453)
kT2 [keV] : 22.3846 (-3.60639 6.78622)
R2^2/D10^2 : 1.15306E-02 (-0.00743827 0.011547)
------------------------------------------------------------
#Fit statistic : Chi-Squared 59.71 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.09e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.094e-07 1.220e-07
25- 50 6.362e-07 1.551e-07
50-150 1.390e-06 4.093e-07
15-150 2.335e-06 6.707e-07
Peak spectrum fit
Power-law model
Time interval is from 1.000 sec. to 2.000 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.57217 ( -0.272666 0.284476 )
Norm@50keV : 1.74605E-02 ( -0.00294683 0.00290165 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 50.58 using 59 bins.
Reduced chi-squared = 0.887368
# Null hypothesis probability of 7.13e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 2.22492 ( -0.3607 0.36134 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.63897e-07 ( -2.95834e-08 2.98969e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 1.000 sec. to 2.000 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.40439 ( -1.13249 1.30672 )
Epeak [keV] : 182.340 ( -182.336 -182.336 )
Norm@50keV : 2.12046E-02 ( -0.00661531 0.0545299 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 50.49 using 59 bins.
Reduced chi-squared = 0.901607
# Null hypothesis probability of 6.83e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 2.21258 ( -0.3686 0.36754 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.62547e-07 ( -3.10154e-08 3.0241e-08 ) ergs/cm2
Band function
Time interval is from 1.000 sec. to 2.000 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] : 15.1701 (-3.23553 3.92788)
R^2/D10^2 : 0.239135 (-0.131468 0.311849)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 62.33 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.92e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.150e-08 3.617e-09
25- 50 4.617e-08 1.325e-08
50-150 7.267e-08 2.778e-08
15-150 1.303e-07 3.369e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.362 (-104.032 -199.363)
Norm : 9.06649 (-1.44348 1.6905)
------------------------------------------------------------
#Fit statistic : Chi-Squared 50.57 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.14e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.258e-08 1.280e-08
25- 50 4.343e-08 2.476e-08
50-150 9.525e-08 5.440e-08
15-150 1.612e-07 9.095e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.59734 (-2.4138 3.63697)
R1^2/D10^2 : 5.26064 (-4.31062 58.2475)
kT2 [keV] : 23.4858 (-6.49963 17.9657)
R2^2/D10^2 : 4.32696E-02 (-0.0374285 0.099913)
------------------------------------------------------------
#Fit statistic : Chi-Squared 50.22 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.57e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.396e-08 1.361e-08
25- 50 4.031e-08 2.173e-08
50-150 9.787e-08 5.790e-08
15-150 1.621e-07 8.585e-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: 1.51662 ( -0.106614 0.107183 )
Norm@50keV : 9.99519E-03 ( -0.000641319 0.000640253 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 59.88 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.72e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 18.26 sec: 1.25345 ( -0.0823742 0.0825143 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.7268e-06 ( -1.18843e-07 1.19307e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.908321 ( -0.479773 0.433277 )
Epeak [keV] : 92.7927 ( -20.9145 95.4329 )
Norm@50keV : 1.99181E-02 ( -0.00757303 0.0138406 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 53.91 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.54e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 18.26 sec: 1.22123 ( -0.08543 0.08549 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.66895e-06 ( -1.27267e-07 1.27201e-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) = 6.17e-07
S(50-100 keV) = 8.51e-07
T90 vs. Hardness ratio plot
T90 = 50.2039999961853 sec.
Hardness ratio (energy fluence ratio) = 1.37925
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.40665
Count Ratio (50-100 keV) / (15-25 keV) = 1.17249
Mask shadow pattern
IMX = 8.854468711545050E-01, IMY = 7.963226404710136E-03
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.024000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.024000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.024000
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:
-239.440000 -4.404000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
308.3168 40.9909 0.0 46.9 154.2 1.1688 1.2 9.6 Cyg X-3
326.1351 38.4693 5.9 33.2 150.3 0.8567 1.9 9.0 Cyg X-2
357.6059 0.2310 2.8 29.9 48.6 1.6618 4.1 144.3 UNKNOWN
324.1488 47.5409 3.4 36.2 165.6 1.4584 3.4 ------ UNKNOWN
341.9383 53.8753 2.2 29.7 -173.8 1.5844 5.3 ------ UNKNOWN
307.9870 80.7470 3.0 56.0 -155.5 5.3774 3.9 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-4.404000 13.860590
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
308.1181 40.8689 5.5 47.0 154.1 0.4502 2.1 5.0 Cyg X-3
325.9988 38.2608 7.8 33.3 149.9 -0.1525 -1.5 8.9 Cyg X-2
27.0307 -6.3472 0.5 41.5 -0.5 2.8101 24.8 ------ UNKNOWN
36.8104 19.5576 2.6 30.5 -44.8 0.3468 4.4 ------ UNKNOWN
44.7716 8.9320 1.9 42.5 -35.7 0.7414 6.2 ------ UNKNOWN
52.1616 1.3201 2.4 52.9 -33.1 1.5749 4.9 ------ UNKNOWN
55.1526 12.4193 2.4 49.5 -47.2 1.4207 4.8 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
73.860600 962.683800
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
346.1008 -3.2565 2.1 40.9 112.1 12.6709 5.5 ------ UNKNOWN
359.1017 -4.9481 2.3 27.8 111.1 5.1137 5.1 301.7 UNKNOWN
13.9578 -26.3812 3.9 23.6 50.1 2.3747 2.9 ------ UNKNOWN
359.6116 30.9422 4.1 45.6 166.1 5.5172 2.8 ------ UNKNOWN
29.0740 -41.1915 2.9 34.9 17.0 4.0116 4.0 ------ UNKNOWN
19.8460 6.3906 3.7 14.6 170.2 2.1465 3.2 ------ UNKNOWN
72.1505 -11.6355 3.1 44.8 -60.2 11.2279 3.7 ------ UNKNOWN
Plot creation:
Sat Jul 30 06:55:37 EDT 2022