batgrbproduct analysis for trigger=781740

batgrbproduct Analysis for Trigger=781740

Analysis Summary

Notes:

1) No attempt has been made to eliminate the non-significant decimal places.
2) This batgrbproduct analysis is done of the amount of data for this trigger downloaded to date.
3) This batgrbproduct analysis is using the flight position for the mask-weighting calculation.
4) This page will be updated for up to 15 downlinks after the trigger.

======================================================================
                  BAT GRB EVENT DATA PROCESSING REPORT
    Process Script Ver: batgrbproduct v2.46
    Process Start Time (local time): Tue Oct 24 11:12:41 EDT 2017
             Host Name: bat1
   Current Working Dir: /local/data/bat1/prebascript/trigger781740/GCN5_download_cron
======================================================================

  Trigger: 00781740      Segment: 000

  BAT Trigger Time: 530440458.56   [s; MET]
      Trigger Stop: 530440459.584   [s; MET]
               UTC: 2017-10-23T08:33:58.675420    [includes UTCF correction] 
       Where From?: TDRSS position message

  BAT 
    RA: 10.6330848310285   Dec: 41.1650551179965  [deg; J2000]

     Catalogged Source?: YES
     Point Source?:      YES
     GRB Indicated?:     NO    [ by BAT flight software ]
     Image S/N Ratio:    5.93
     Image Trigger?:     NO
     Rate S/N Ratio:     26.5706605111728  [ if not an image trigger ]
     Image S/N Ratio:    5.93

  Flight Position:   [ source = BAT ]
    RA: 10.6330848310285   Dec: 41.1650551179965  [deg; J2000]

  Ground Position:   [ source = BAT pre-slew burst ]
    RA: 10.6593153962933   Dec: 41.1434831765995  [deg; J2000]  
        { 00h 42m 38.2s , +41d 08' 36.5" }
         +/- 3.0739140686614 [arcmin] (estimated 90% radius based on SNR)
         +/- 1.42961372425083 [arcmin] (formal 1-sigma fit error)
    SNR: 6.11527397692301
 
  Angular difference between Flight and Ground position is 1.754847 arcmin
 
  Partial Coding Fraction: 0.6328125    [ including projection effects ]

  Duration
     T90: 0.915999948978424 +/- 0.260376657598808
        Measured from: 0.0160000920295715
                   to: 0.932000041007996     [s; relative to TRIGTIME]
     T50: 0.539999961853027 +/- 0.277243547135739
        Measured from: 0.232000112533569
                   to: 0.772000074386597     [s; relative to TRIGTIME]



  Fluence
     Peak Flux  (peak 1 second)
        Measured from: -0.0300000309944153     
                   to: 0.969999969005585     [s; relative to TRIGTIME]
     Total Fluence        
        Measured from: -0.0239999890327454     
                   to: 0.995999991893768     [s; relative to TRIGTIME]
     
             Band 1     Band 2     Band 3     Band 4
              15-25      25-50     50-100    100-350     keV
 Total     0.034136   0.053683   0.004685   0.010349
           0.009490   0.009635   0.006731   0.005445 [error]
 Peak      0.031647   0.050196   0.005794   0.011071
           0.009380   0.009517   0.006674   0.005393 [error]

     [ fluence units of on-axis counts / fully illuminated detector ] 

======================================================================
 
=== Fluence/Peak Flux Summary ===
 
              Model    Band1    Band2    Band3    Band4    Band5    Total      
                       15-25    25-50   50-100  100-350   15-150   15-350   keV
Fluence   Power-law 1.16e-08 1.41e-08 1.23e-08 1.84e-08 4.44e-08 5.64e-08   erg/cm2
              Error 3.90e-09 4.00e-09 5.78e-09 1.65e-08 1.44e-08 2.46e-08   erg/cm2
Peak flux Power-law 3.51e-01 2.46e-01 1.13e-01 7.30e-02 7.45e-01 7.83e-01   ph/cm2/s
              Error 1.28e-01 7.03e-02 5.18e-02 6.17e-02 2.11e-01 2.23e-01   ph/cm2/s
 
Fluence   Cutoff-PL 9.34e-09 2.25e-08 5.72e-09 3.80e-11 3.76e-08 3.76e-08   erg/cm2
              Error 7.10e-09 7.04e-09 6.75e-09 1.12e-09 1.09e-08 1.09e-08   erg/cm2
Peak flux Cutoff-PL 2.78e-01 3.74e-01 6.25e-02 3.74e-04 7.15e-01 7.15e-01   ph/cm2/s
              Error 2.17e-01 1.26e-01 6.98e-02 1.33e-02 2.12e-01 2.12e-01   ph/cm2/s
 
Fluence        Band -------- -------- -------- -------- -------- --------   erg/cm2
              Error -------- -------- -------- -------- -------- --------   erg/cm2
Peak flux      Band -------- -------- -------- -------- -------- --------   ph/cm2/s
              Error -------- -------- -------- -------- -------- --------   ph/cm2/s

 
=== Time-averaged spectral analysis ===
 
Model Ph_index Ph_90err Epeak  Epeak_90err Norm     Nomr_90err chi2   dof
PL    2.193    0.472    -      -           4.64e-03 1.67e-03   62.950 57
CPL  -3.290    0.354      34.2    7.0      1.31e+01 1.57e+05   56.490 56
 
The chi2 of BB fit is 56.77 which shows a significant improvement in the fit over a PL.
Check the BB fit.
 
=== 1-s peak spectral analysis ===
 
Model Ph_index Ph_90err Epeak  Epeak_90err Norm     Nomr_90err chi2   dof
PL    2.118    0.491    -      -           4.70e-03 1.69e-03   64.630 57
CPL  -2.849    0.698      34.5    8.3      6.36e+00 1.08e+05   60.430 56
 
Model      : spectral model: simple power-law (PL) and cutoff power-law (CPL)
Ph_index   : photon index: E^-{Ph_index} (minus sign is not included in the index)
Ph_90err   : 90% error of the photon index
Epeak      : Epeak in keV
Epeak_90err: 90% error of Epeak
Norm       : normalization at 50 keV in PL model and at 1 keV in CPL model
Nomr_90err : 90% error of the normalization
chi2       : Chi-Squared
dof        : degree of freedom

 
=== T90/T50 calculation in the 50-300 keV band (BATSE band) using 64 ms lc ===
 
T90 in the 50-300 keV band: 0.000000 sec.
T50 in the 50-300 keV band: 0.000000 sec.

 
=== Table of the duration information ==
 
        Value   tstart    tstop
T100    1.020   -0.024    0.996
T90     0.916    0.016    0.932
T50     0.540    0.232    0.772
Peak    1.000   -0.030    0.970

Click here for the BAT GCN circular template

Estimated redshift from machine learning (Ukwatta et al. 2016) - may take a few minutes to calcaulte

Image

Pre-slew 15-350 keV image (Event data; bkg subtracted)

#   RAcent  DECcent POSerr  Theta    Phi     Peak Cts     SNR  Name
   10.6593 +41.1435 0.0313   23.2  110.0       0.0997     6.1  TRIG_00781740       
------------------------------------------
 
Foreground time interval of the image:
 -0.024   0.996 (delta_t =   1.020 [sec])
Background time interval of the image:
-128.459  -0.024 (delta_t = 128.435 [sec])

Lightcurves

Notes:

1) All plots contain as much data as has been downloaded to date.
2) The mask-weighted light curves are using the flight position.
3) Multiple plots of different time binning/intervals are shown to cover all scenarios of short/long GRBs, rate/image triggers, and real/false positives.
4) 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.
5) 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.
6) 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)

Spectra

Notes:

1) The fitting includes the systematic errors.
2) For long bursts, a spectral fit of 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.
4) For short bursts (T90<1sec), the specrtum is also fit with Blackbody, OTTB, and Double Blackbody.

Time averaged spectrum fit using the pre-slew DRM

Power-law model

Time interval is from   -0.024 sec. to    0.996 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 2.19350     ( -0.436969   0.50628 )
Norm@50keV  : 4.63833E-03    ( -0.00169476   0.00165232 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          62.95 using 59 PHA bins.
# Reduced chi-squared =          1.104 for     57 degrees of freedom 
# Null hypothesis probability =   2.739396e-01
 
Photon flux (15-150 keV)    in 1.02 sec: 0.765280 ( -0.2094  0.209401 ) ph/cm2/s
Energy fluence (15-150 keV)             : 4.44349e-08 ( -1.40244e-08  1.46805e-08 ) ergs/cm2

Cutoff power-law model

Time interval is from   -0.024 sec. to    0.996 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: -3.29044     ( 2.48868   3.196 )
Epeak [keV] : 34.1918      ( -6.80157 7.15223 )
Norm@50keV  : 13.1253    ( -12.6002   313294 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          56.49 using 59 PHA bins.
# Reduced chi-squared =          1.009 for     56 degrees of freedom 
# Null hypothesis probability =   4.564425e-01
 
Photon flux (15-150 keV)    in 1.02 sec: 0.743817 ( -0.210046  0.208251 ) ph/cm2/s
Energy fluence (15-150 keV)             : 3.76219e-08 ( -1.04806e-08  1.13868e-08 ) ergs/cm2

Band function

Time interval is from   -0.024 sec. to    0.996 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : 4.51390   ( -5.18378   -4.5139 )
beta        : -4.89608    ( 4.89608   2.06645 )
Epeak [keV] : 33.8101      ( -5.39441 5.70462 )
Norm@50keV   : 79.9776    ( -20.1731   602.865 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          56.56 using 59 PHA bins.
# Reduced chi-squared =          1.028 for     55 degrees of freedom 
# Null hypothesis probability =   4.165022e-01
 
Photon flux (15-150 keV)    in 1.02 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]    : 8.74622  (-1.66207  2.01244)
R^2/D10^2   : 0.693454  (-0.401085   0.895457)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          56.77 using 59 PHA bins.
# Reduced chi-squared =         0.9959 for     57 degrees of freedom 
# Null hypothesis probability =   4.837441e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.037e-08   4.979e-09
25- 50  2.107e-08   9.551e-09
50-150  7.358e-09   4.735e-09
15-150  3.880e-08   1.777e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 42.2059       (-17.5407      42.4701)
Norm        : 5.02735       (-1.87075     2.8393)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          60.51 using 59 PHA bins.
# Reduced chi-squared =          1.062 for     57 degrees of freedom 
# Null hypothesis probability =   3.502003e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.198e-08   4.952e-09
25- 50  1.612e-08   6.918e-09
50-150  1.322e-08   9.997e-09
15-150  4.132e-08   1.745e-08

Double BB

#Fit statistic : Chi-Squared =          56.73 using 59 PHA bins.
#Fit statistic : Chi-Squared =          56.29 using 59 PHA bins.
#Fit statistic : Chi-Squared =          56.27 using 59 PHA bins.
# Reduced chi-squared =          1.032 for     55 degrees of freedom 
# Reduced chi-squared =          1.032 for     55 degrees of freedom 
# Reduced chi-squared =          1.031 for     55 degrees of freedom 
# Reduced chi-squared =          1.023 for     55 degrees of freedom 
# Reduced chi-squared =          1.023 for     55 degrees of freedom 
# Null hypothesis probability =   4.089468e-01
# Null hypothesis probability =   4.096536e-01
# Null hypothesis probability =   4.104672e-01
# Null hypothesis probability =   4.263768e-01
# Null hypothesis probability =   4.272285e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  0.000e+00   0.000e+00
25- 50  0.000e+00   0.000e+00
50-150  0.000e+00   0.000e+00
15-150  0.000e+00   0.000e+00

Peak spectrum fit

Power-law model

Time interval is from   -0.030 sec. to    0.970 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 2.11796     ( -0.457281   0.524301 )
Norm@50keV  : 4.69612E-03    ( -0.00172517   0.00166454 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          64.63 using 59 PHA bins.
# Reduced chi-squared =          1.134 for     57 degrees of freedom 
# Null hypothesis probability =   2.276755e-01
 
Photon flux (15-150 keV)    in 1 sec: 0.745433 ( -0.21095  0.210984 ) ph/cm2/s
Energy fluence (15-150 keV)             : 4.37158e-08 ( -1.41773e-08  1.47845e-08 ) ergs/cm2

Cutoff power-law model

Time interval is from   -0.030 sec. to    0.970 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: -2.84855     ( 1.96169   3.35762 )
Epeak [keV] : 34.4628      ( -6.90025 9.70268 )
Norm@50keV  : 6.35537    ( -5.88218   215026 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          60.43 using 59 PHA bins.
# Reduced chi-squared =          1.079 for     56 degrees of freedom 
# Null hypothesis probability =   3.187987e-01
 
Photon flux (15-150 keV)    in 1 sec: 0.714728 ( -0.212748  0.21065 ) ph/cm2/s
Energy fluence (15-150 keV)             : 3.56825e-08 ( -1.07253e-08  7.0504e-09 ) ergs/cm2

Band function

Time interval is from   -0.030 sec. to    0.970 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : 3.88369   ( -5.60635   -4.40437 )
beta        : -4.22606    ( 4.25402   1.79967 )
Epeak [keV] : 33.5533      ( -5.83094 7.73277 )
Norm@50keV   : 31.9471    ( -31.8824   54.7787 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          60.16 using 59 PHA bins.
# Reduced chi-squared =          1.094 for     55 degrees of freedom 
# Null hypothesis probability =   2.943188e-01
 
Photon flux (15-150 keV)    in 1 sec:  (    ) ph/cm2/s
Energy fluence (15-150 keV)             : 3.80684e-08 ( 0  0 ) ergs/cm2

Single BB

 
Spectral model blackbody:
------------------------------------------------------------
Parameters  : value    Lower 90%  Upper 90%
kT [keV]    : 8.87732  (-1.82331  2.28258)
R^2/D10^2   : 0.624416  (-0.382507   0.911353)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          60.53 using 59 PHA bins.
# Reduced chi-squared =          1.062 for     57 degrees of freedom 
# Null hypothesis probability =   3.495578e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  9.511e-09   5.176e-09
25- 50  1.978e-08   1.010e-08
50-150  7.236e-09   5.040e-09
15-150  3.653e-08   2.013e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 46.8988       (-21.1822      61.707)
Norm        : 4.55416       (-1.76291     2.74753)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          63.06 using 59 PHA bins.
# Reduced chi-squared =          1.106 for     57 degrees of freedom 
# Null hypothesis probability =   2.707745e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.096e-08   4.711e-09
25- 50  1.538e-08   7.526e-09
50-150  1.404e-08   1.017e-08
15-150  4.038e-08   2.086e-08

Double BB

------------------------------------------------------------
#Fit statistic : Chi-Squared =          60.53 using 59 PHA bins.
#Fit statistic : Chi-Squared =          60.50 using 59 PHA bins.
#Fit statistic : Chi-Squared =          59.28 using 59 PHA bins.
#Fit statistic : Chi-Squared =          59.26 using 59 PHA bins.
# Reduced chi-squared =          1.101 for     55 degrees of freedom 
# Reduced chi-squared =          1.100 for     55 degrees of freedom 
# Reduced chi-squared =          1.078 for     55 degrees of freedom 
# Reduced chi-squared =          1.077 for     55 degrees of freedom 
# Null hypothesis probability =   2.829916e-01
# Null hypothesis probability =   2.841177e-01
# Null hypothesis probability =   3.221889e-01
# Null hypothesis probability =   3.230234e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  0.000e+00   0.000e+00
25- 50  0.000e+00   0.000e+00
50-150  0.000e+00   0.000e+00
15-150  0.000e+00   0.000e+00

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: 2.19350     ( -0.436969   0.50628 )
Norm@50keV  : 4.63833E-03    ( -0.00169476   0.00165232 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          62.95 using 59 PHA bins.
# Reduced chi-squared =          1.104 for     57 degrees of freedom 
# Null hypothesis probability =   2.739396e-01
 
Photon flux (15-150 keV)    in 1.02 sec: 0.765280 ( -0.2094  0.209401 ) ph/cm2/s
Energy fluence (15-150 keV)             : 4.44349e-08 ( -1.40244e-08  1.46805e-08 ) ergs/cm2

Cutoff power-law model

Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: -3.29044     ( 2.48868   3.196 )
Epeak [keV] : 34.1918      ( -6.80157 7.15223 )
Norm@50keV  : 13.1253    ( -12.6002   322774 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          56.49 using 59 PHA bins.
# Reduced chi-squared =          1.009 for     56 degrees of freedom 
# Null hypothesis probability =   4.564425e-01
 
Photon flux (15-150 keV)    in 1.02 sec: 0.743817 ( -0.210046  0.208251 ) ph/cm2/s
Energy fluence (15-150 keV)             : 3.76219e-08 ( -1.04806e-08  1.13868e-08 ) ergs/cm2

Band function

 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : 4.51390   ( -5.18378   -4.5139 )
beta        : -4.89608    ( 4.89608   2.06645 )
Epeak [keV] : 33.8101      ( -5.39441 5.70462 )
Norm@50keV   : 79.9776    ( -20.1731   602.865 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          56.56 using 59 PHA bins.
# Reduced chi-squared =          1.028 for     55 degrees of freedom 
# Null hypothesis probability =   4.165022e-01
 
Photon flux (15-150 keV)    in 1.02 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)  = 1.41e-08
S(50-100 keV) = 1.23e-08

T90 vs. Hardness ratio plot

T90                                   = 0.915999948978424 sec.
Hardness ratio (energy fluence ratio) = 0.87234

Color vs. Color plot

Count Ratio  (25-50 keV) / (15-25 keV) = 1.57262
Count Ratio (50-100 keV) / (15-25 keV) = 0.137245

Mask shadow pattern

IMX = -1.465336033624136E-01, IMY = -4.028140344914817E-01

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:
-128.459400 -0.024000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
299.4432  35.3610   10.7  48.7 -154.5  -0.5530  -1.1   12.0	Cyg X-1                       
308.1705  40.9494    2.6  40.2 -158.3   1.3744   4.4    2.7	Cyg X-3                       
326.1103  38.3134   13.6  35.0 -179.8   0.2131   0.9    2.9	Cyg X-2                       
 71.6737  34.1051    2.9  49.0   33.3   3.0729   4.0 ------	UNKNOWN                       
 55.4063  49.5897    2.3  29.5   34.2   1.2391   5.0 ------	UNKNOWN                       
 40.9250  61.4277    0.1  15.8   22.4  14.8531  80.5 ------	UNKNOWN                       
293.9307  28.1812    2.8  57.3 -154.1   5.1423   4.1 ------	UNKNOWN                       
133.1924  49.5772    2.7  58.9  -24.5   5.6123   4.3 ------	UNKNOWN

Pre-slew background subtracted image of 15-350 keV band

Time interval of the image:
-0.024000 0.996000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
299.6258  35.1993    5.3  48.8 -154.8   0.0698   2.2    1.7	Cyg X-1                       
308.0718  41.0349   22.1  40.2 -158.1   0.0102   0.5    5.2	Cyg X-3                       
325.9939  38.3235    7.1  35.1 -179.6   0.0257   1.6    8.4	Cyg X-2                       
 10.6593  41.1435    1.9  23.2  110.0   0.0997   6.1 ------	UNKNOWN                       
 40.9359  61.4332    0.8  15.8   22.4   0.1898  15.0 ------	UNKNOWN                       
348.8151  61.2334    2.2   8.5 -164.1   0.0637   5.2 ------	UNKNOWN                       
123.9115  47.7723    2.7  57.9  -17.1   0.2830   4.3 ------	UNKNOWN                       
129.9796  49.2353    2.3  58.3  -22.1   0.3666   5.2 ------	UNKNOWN

Post-slew image of 15-350 keV band

Time interval of the image:
58.340650 962.480000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
308.0954  40.8236   11.7  46.1 -126.3  -5.0089  -1.0    7.8	Cyg X-3                       
326.0138  38.2370   13.6  34.1 -137.6   1.4182   0.8    9.0	Cyg X-2                       
359.7337  18.2876    2.1  24.7  147.8   6.6385   5.5 ------	UNKNOWN                       
 14.2574  46.7668    3.5   6.2  -33.7   3.1893   3.3 ------	UNKNOWN                       
 40.9167  61.4300    0.1  27.2  -25.8 100.1398  92.7 ------	UNKNOWN                       
334.7613  41.1463    3.1  26.8 -135.7   4.5614   3.8 ------	UNKNOWN                       
 35.0312  68.0927    3.3  29.9  -39.6   4.4642   3.5 ------	UNKNOWN

Plot creation:
Tue Oct 24 11:18:13 EDT 2017