batgrbproduct analysis for trigger=866993

batgrbproduct Analysis for Trigger=866993

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): Mon Oct 15 08:18:15 EDT 2018
             Host Name: bat1
   Current Working Dir: /local/data/bat1/prebascript/trigger866993/GCN5_download_cron
======================================================================

  Trigger: 00866993      Segment: 000

  BAT Trigger Time: 561197756.668   [s; MET]
      Trigger Stop: 561197756.732   [s; MET]
               UTC: 2018-10-14T08:15:34.916700    [includes UTCF correction] 
       Where From?: (*SHORT BURST*) TDRSS scaled map message

  BAT 
    RA: 272.166007718439   Dec: -20.380370164253  [deg; J2000]

     Catalogged Source?: YES
     Point Source?:      YES
     GRB Indicated?:     NO    [ by BAT flight software ]
     Image S/N Ratio:    6.92
     Image Trigger?:     NO
     Rate S/N Ratio:     18.3847763108502  [ if not an image trigger ]
     Image S/N Ratio:    6.92

  Flight Position:   [ source = BAT ]
    RA: 272.166007718439   Dec: -20.380370164253  [deg; J2000]

  Ground Position:   [ source = BAT pre-slew burst ]
    RA: 272.153116847413   Dec: -20.4069110844602  [deg; J2000]  
        { 18h 08m 36.7s , -20d 24' 24.9" }
         +/- 1.5533874228864 [arcmin] (estimated 90% radius based on SNR)
         +/- 0.569575055151348 [arcmin] (formal 1-sigma fit error)
    SNR: 16.2129313929944
 
  Angular difference between Flight and Ground position is 1.749714 arcmin
 
  Partial Coding Fraction: 0.3125    [ including projection effects ]

  Duration
     T90: 1.90400004386902 +/- 0.365557208133314
        Measured from: -0.0679998397827148
                   to: 1.8360002040863     [s; relative to TRIGTIME]
     T50: 0.927999973297119 +/- 0.192665487917238
        Measured from: 0.124000191688538
                   to: 1.05200016498566     [s; relative to TRIGTIME]



  Fluence
     Peak Flux  (peak 1 second)
        Measured from: -0.175999999046326     
                   to: 0.824000000953674     [s; relative to TRIGTIME]
     Total Fluence        
        Measured from: -0.195999979972839     
                   to: 2.0440000295639     [s; relative to TRIGTIME]
     
             Band 1     Band 2     Band 3     Band 4
              15-25      25-50     50-100    100-350     keV
 Total     0.316368   0.329771   0.078690   0.016439
           0.025073   0.024657   0.017661   0.013318 [error]
 Peak      0.232020   0.210452   0.043677   0.003027
           0.018905   0.018104   0.012434   0.009066 [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 1.13e-07 1.22e-07 9.36e-08 1.17e-07 3.73e-07 4.46e-07   erg/cm2
              Error 1.34e-08 1.19e-08 1.56e-08 3.59e-08 3.94e-08 5.94e-08   erg/cm2
Peak flux Power-law 2.65e+00 1.45e+00 4.96e-01 2.21e-01 4.71e+00 4.82e+00   ph/cm2/s
              Error 3.43e-01 1.58e-01 9.48e-02 7.43e-02 4.95e-01 5.03e-01   ph/cm2/s
 
Fluence   Cutoff-PL 1.00e-07 1.62e-07 6.37e-08 3.27e-09 3.29e-07 3.29e-07   erg/cm2
              Error 1.53e-08 1.82e-08 2.14e-08 5.73e-09 3.54e-08 3.56e-08   erg/cm2
Peak flux Cutoff-PL 2.33e+00 1.86e+00 3.90e-01 1.36e-02 4.60e+00 4.60e+00   ph/cm2/s
              Error 3.95e-01 2.37e-01 1.29e-01 2.37e-02 4.96e-01 4.96e-01   ph/cm2/s
 
Fluence        Band 9.93e-08 1.61e-07 6.42e-08 8.76e-09 3.32e-07 3.34e-07   erg/cm2
              Error 1.51e-08 -------- -------- 3.37e-08 -------- --------   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    2.382    0.163    -      -           1.71e-02 2.16e-03   86.170 57
CPL  -0.387    1.162      31.3    3.8      9.29e-01 3.00e+00   60.250 56
 
The chi2 of BB fit is 63.19 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    2.546    0.188    -      -           2.33e-02 3.49e-03   54.280 57
CPL   0.133    1.210      28.2    5.9      7.59e-01 2.68e+00   36.550 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    2.240   -0.196    2.044
T90     1.904   -0.068    1.836
T50     0.928    0.124    1.052
Peak    1.000   -0.176    0.824

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
  272.1531 -20.4069 0.0119   36.6  -60.8       0.7659    16.2  TRIG_00866993       
------------------------------------------
 
Foreground time interval of the image:
 -0.196   2.044 (delta_t =   2.240 [sec])
Background time interval of the image:
-239.668  -0.196 (delta_t = 239.472 [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 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)

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   -0.196 sec. to    2.044 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 2.38209     ( -0.158589   0.167244 )
Norm@50keV  : 1.71310E-02    ( -0.00216982   0.00214851 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          86.17 using 59 PHA bins.
# Reduced chi-squared =          1.512 for     57 degrees of freedom 
# Null hypothesis probability =   7.567251e-03
 
Photon flux (15-150 keV)    in 2.24 sec: 3.13678 ( -0.297336  0.297455 ) ph/cm2/s
Energy fluence (15-150 keV)             : 3.7281e-07 ( -3.92152e-08  3.96646e-08 ) ergs/cm2

Cutoff power-law model

Time interval is from   -0.196 sec. to    2.044 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: -0.387176     ( -1.26664   1.05666 )
Epeak [keV] : 31.2631      ( -4.10263 3.4319 )
Norm@50keV  : 0.928690    ( -0.930257   5.07134 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          60.25 using 59 PHA bins.
# Reduced chi-squared =          1.076 for     56 degrees of freedom 
# Null hypothesis probability =   3.246521e-01
 
Photon flux (15-150 keV)    in 2.24 sec: 3.03461 ( -0.29635  0.29702 ) ph/cm2/s
Energy fluence (15-150 keV)             : 3.28646e-07 ( -3.45856e-08  3.62477e-08 ) ergs/cm2

Band function

Time interval is from   -0.196 sec. to    2.044 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : 0.411705   ( -1.30104   -0.624053 )
beta        : -5.12406    ( 4.5413   1.63186 )
Epeak [keV] : 31.2037      ( -5.18993 3.53577 )
Norm@50keV   : 0.969199    ( -0.9692   1075.07 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          60.08 using 59 PHA bins.
# Reduced chi-squared =          1.092 for     55 degrees of freedom 
# Null hypothesis probability =   2.969954e-01
 
Photon flux (15-150 keV)    in 2.24 sec:  (    ) ph/cm2/s
Energy fluence (15-150 keV)             : 3.32297e-07 ( 0  0 ) ergs/cm2

Single BB

 
Spectral model blackbody:
------------------------------------------------------------
Parameters  : value    Lower 90%  Upper 90%
kT [keV]    : 8.27677  (-0.697291  0.745539)
R^2/D10^2   : 3.23368  (-0.974959   1.41311)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          63.19 using 59 PHA bins.
# Reduced chi-squared =          1.109 for     57 degrees of freedom 
# Null hypothesis probability =   2.670307e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  9.192e-08   1.401e-08
25- 50  1.705e-07   1.876e-08
50-150  5.001e-08   1.308e-08
15-150  3.124e-07   3.282e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 36.4599       (-6.21855      7.98716)
Norm        : 22.4463       (-3.56994     4.23234)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          68.19 using 59 PHA bins.
# Reduced chi-squared =          1.196 for     57 degrees of freedom 
# Null hypothesis probability =   1.473000e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.117e-07   1.267e-08
25- 50  1.409e-07   1.427e-08
50-150  9.819e-08   2.788e-08
15-150  3.507e-07   3.707e-08

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 5.54381        (-2.78768      -5.54381)
R1^2/D10^2  : 7.62755        (-6.26656      54.7558)
kT2 [keV]   : 10.5837        (-5.14042      -10.5837)
R2^2/D10^2  : 0.771287    (-0.767796   1.36789)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          59.70 using 59 PHA bins.
# Reduced chi-squared =          1.085 for     55 degrees of freedom 
# Null hypothesis probability =   3.089436e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.018e-07   5.570e-08
25- 50  1.593e-07   8.396e-08
50-150  6.950e-08   3.931e-08
15-150  3.306e-07   1.717e-07

Peak spectrum fit

Power-law model

Time interval is from   -0.176 sec. to    0.824 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 2.54630     ( -0.18133   0.195131 )
Norm@50keV  : 2.33215E-02    ( -0.00350575   0.00346993 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          54.28 using 59 PHA bins.
# Reduced chi-squared =         0.9522 for     57 degrees of freedom 
# Null hypothesis probability =   5.778820e-01
 
Photon flux (15-150 keV)    in 1 sec: 4.71450 ( -0.494591  0.49474 ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.36232e-07 ( -2.75116e-08  2.78662e-08 ) ergs/cm2

Cutoff power-law model

Time interval is from   -0.176 sec. to    0.824 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 0.132582     ( -1.3316   1.08921 )
Epeak [keV] : 28.1658      ( -7.36923 4.41173 )
Norm@50keV  : 0.759023    ( -0.758722   4.61059 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          36.55 using 59 PHA bins.
# Reduced chi-squared =         0.6528 for     56 degrees of freedom 
# Null hypothesis probability =   9.794379e-01
 
Photon flux (15-150 keV)    in 1 sec: 4.59946 ( -0.49575  0.4961 ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.15886e-07 ( -2.4967e-08  2.6082e-08 ) ergs/cm2

Band function

Time interval is from   -0.176 sec. to    0.824 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -0.151426   ( -1.06583   1.42493 )
beta        : -6.10128    ( 6.04445   2.73595 )
Epeak [keV] : 28.1034      ( -7.21397 3.83726 )
Norm@50keV   : 0.739694    ( -0.236454   5.71524 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          36.53 using 59 PHA bins.
# Reduced chi-squared =         0.6642 for     55 degrees of freedom 
# Null hypothesis probability =   9.740203e-01
 
Photon flux (15-150 keV)    in 1 sec:  (    ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.27936e-07 ( -2.27929e-07  -2.8371e-08 ) ergs/cm2

Single BB

 
Spectral model blackbody:
------------------------------------------------------------
Parameters  : value    Lower 90%  Upper 90%
kT [keV]    : 7.92086  (-0.773755  0.821536)
R^2/D10^2   : 5.67390  (-1.92574   3.03135)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          41.18 using 59 PHA bins.
# Reduced chi-squared =         0.7224 for     57 degrees of freedom 
# Null hypothesis probability =   9.432492e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  6.389e-08   1.027e-08
25- 50  1.099e-07   1.457e-08
50-150  2.793e-08   8.910e-09
15-150  2.017e-07   2.700e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 31.6605       (-5.72114      7.27042)
Norm        : 37.4811       (-6.80224     8.43822)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          39.95 using 59 PHA bins.
# Reduced chi-squared =         0.7009 for     57 degrees of freedom 
# Null hypothesis probability =   9.579152e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  7.833e-08   1.002e-08
25- 50  9.215e-08   1.207e-08
50-150  5.410e-08   1.763e-08
15-150  2.246e-07   2.765e-08

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 4.12414        (-1.82479      2.22055)
R1^2/D10^2  : 35.1612        (-28.2929      468.549)
kT2 [keV]   : 9.63616        (-1.59868      4.8472)
R2^2/D10^2  : 1.96491    (-1.81828   3.08748)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          35.80 using 59 PHA bins.
# Reduced chi-squared =         0.6509 for     55 degrees of freedom 
# Null hypothesis probability =   9.791021e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  7.366e-08   3.805e-08
25- 50  1.010e-07   5.280e-08
50-150  4.067e-08   2.428e-08
15-150  2.153e-07   1.088e-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: 2.38209     ( -0.158589   0.167244 )
Norm@50keV  : 1.71310E-02    ( -0.00216982   0.00214851 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          86.17 using 59 PHA bins.
# Reduced chi-squared =          1.512 for     57 degrees of freedom 
# Null hypothesis probability =   7.567251e-03
 
Photon flux (15-150 keV)    in 2.24 sec: 3.13678 ( -0.297336  0.297455 ) ph/cm2/s
Energy fluence (15-150 keV)             : 3.7281e-07 ( -3.92152e-08  3.96646e-08 ) ergs/cm2

Cutoff power-law model

Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: -0.387176     ( -1.26664   1.05666 )
Epeak [keV] : 31.2631      ( -4.10263 3.4319 )
Norm@50keV  : 0.928690    ( -0.930257   5.07134 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          60.25 using 59 PHA bins.
# Reduced chi-squared =          1.076 for     56 degrees of freedom 
# Null hypothesis probability =   3.246521e-01
 
Photon flux (15-150 keV)    in 2.24 sec: 3.03461 ( -0.29635  0.29702 ) ph/cm2/s
Energy fluence (15-150 keV)             : 3.28646e-07 ( -3.45856e-08  3.62477e-08 ) ergs/cm2

Band function

 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : 0.411705   ( -1.30104   -0.624053 )
beta        : -5.12406    ( 4.5413   1.63186 )
Epeak [keV] : 31.2037      ( -5.18993 3.53577 )
Norm@50keV   : 0.969199    ( -0.9692   1075.33 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          60.08 using 59 PHA bins.
# Reduced chi-squared =          1.092 for     55 degrees of freedom 
# Null hypothesis probability =   2.969954e-01
 
Photon flux (15-150 keV)    in 2.24 sec:  (    ) ph/cm2/s
Energy fluence (15-150 keV)             : 3.32297e-07 ( 0  0 ) ergs/cm2

S(25-50 keV) vs. S(50-100 keV) plot

S(25-50 keV)  = 1.22e-07
S(50-100 keV) = 9.36e-08

T90 vs. Hardness ratio plot

T90                                   = 1.90400004386902 sec.
Hardness ratio (energy fluence ratio) = 0.767213

Color vs. Color plot

Count Ratio  (25-50 keV) / (15-25 keV) = 1.04237
Count Ratio (50-100 keV) / (15-25 keV) = 0.248729

Mask shadow pattern

IMX = 3.629490446022527E-01, IMY = 6.481876366556062E-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:
-239.668000 -0.196000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
264.7270 -44.5694    5.9  38.4 -102.2   1.3567   2.0    7.2	4U 1735-44                    
268.2515  -1.5174    6.2  50.3  -40.8  -1.6774  -1.9    8.0	SW J1753.5-0127               
270.1154 -25.2201    0.0  36.5  -69.4   0.7951   1.7   12.5	GX 5-1                        
270.3060 -25.7940    6.8  36.2  -70.3   0.7993   1.7    3.1	GRS 1758-258                  
274.0808 -14.0113    7.1  38.2  -50.1   0.6352   1.6    4.6	GX 17+2                       
275.9180 -30.2361    7.0  30.2  -75.8   0.5335   1.7    7.9	H1820-303                     
285.0851 -24.7714    9.0  23.9  -59.1  -0.3596  -1.3    9.3	HT1900.1-2455                 
288.8215  11.0085    3.0  47.5   -9.0   1.5526   3.8    4.0	GRS 1915+105                  
262.8651 -33.7913    3.8  40.5  -85.3   2.9651   3.0    6.7	GX 354-0                      
 20.9122 -51.4994    2.2  53.7  155.1   6.9168   5.2 ------	UNKNOWN                       
  4.4204 -44.9577    2.8  43.1  145.5   2.6226   4.1 ------	UNKNOWN                       
  8.9478 -50.2501    3.1  46.2  153.0   2.3445   3.8 ------	UNKNOWN

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

Time interval of the image:
-0.196000 2.044000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
264.6873 -44.3265    6.0  38.4 -101.8  -0.1560  -1.9    7.8	4U 1735-44                    
268.3692  -1.3159    8.6  50.4  -40.5   0.1399   1.3    8.2	SW J1753.5-0127               
270.4321 -25.1909   12.2  36.3  -69.2  -0.0480  -0.9   10.5	GX 5-1                        
270.4672 -25.7124   13.1  36.1  -70.0   0.0454   0.9    9.1	GRS 1758-258                  
274.1478 -14.1394    0.0  38.0  -50.2   0.0928   2.3   10.3	GX 17+2                       
275.7967 -30.5079    3.8  30.3  -76.3   0.1110   3.0   10.7	H1820-303                     
284.8725 -24.9164    5.5  24.1  -59.7  -0.0500  -2.1    8.9	HT1900.1-2455                 
288.9177  10.8957    5.3  47.3   -9.0   0.0773   2.2    7.6	GRS 1915+105                  
263.0342 -33.9524   94.9  40.3  -85.6  -0.0122  -0.1    7.4	GX 354-0                      
319.4872  -0.4713    2.3  31.8   37.3   0.1336   4.9 ------	UNKNOWN                       
298.8516  -8.2922    2.6  25.8   -7.7   0.0845   4.3 ------	UNKNOWN                       
272.1531 -20.4069    0.7  36.6  -60.8   0.7658  16.2 ------	UNKNOWN

Post-slew image of 15-350 keV band

Time interval of the image:
210.832600 783.532570
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
330.8829 -28.1535    2.7  45.8   30.8   4.5410   4.4 ------	UNKNOWN                       
304.5087 -37.1638    2.4  52.1    0.1   4.9366   4.9 ------	UNKNOWN                       
287.1591 -38.7019    2.9  59.4  -14.0  10.7718   4.0 ------	UNKNOWN                       
 91.7340 -64.5039    3.1  32.3 -128.3   2.2087   3.8 ------	UNKNOWN                       
256.5494 -67.6521    3.2  47.2  -53.4   7.3562   3.6 ------	UNKNOWN

Plot creation:
Mon Oct 15 08:22:12 EDT 2018