batgrbproduct analysis for trigger=744791

batgrbproduct Analysis for Trigger=744791

Analysis Summary

Notes:

1) No attempt has been made to eliminate the non-significant decimal places.
2) This batgrbproduct analysis is done using the HEASARC data.
3) This batgrbproduct analysis is using the flight position for the mask-weighting calculation.

======================================================================
                  BAT GRB EVENT DATA PROCESSING REPORT
    Process Script Ver: batgrbproduct v2.46
    Process Start Time (local time): Tue Apr 25 16:26:13 EDT 2017
             Host Name: bat1
   Current Working Dir: /local/data/bat1/alien/Swift_3rdBATcatalog/event/batevent_reproc/trigger744791
======================================================================

  Trigger: 00744791      Segment: 000

  BAT Trigger Time: 512617265.28   [s; MET]
      Trigger Stop: 512617273.472   [s; MET]
               UTC: 2017-03-31T01:40:46.444640    [includes UTCF correction] 
       Where From?: TDRSS position message

  BAT 
    RA: 323.782196657932   Dec: -24.413770984427  [deg; J2000]

     Catalogged Source?: NO
     Point Source?:      YES
     GRB Indicated?:     YES    [ by BAT flight software ]
     Image S/N Ratio:    7.93
     Image Trigger?:     NO
     Rate S/N Ratio:     9.4339811320566  [ if not an image trigger ]
     Image S/N Ratio:    7.93

  Flight Position:   [ source = BAT ]
    RA: 323.782196657932   Dec: -24.413770984427  [deg; J2000]

  Ground Position:   [ source = BAT pre-slew burst ]
    RA: 323.77794176101   Dec: -24.4054251923295  [deg; J2000]  
        { 21h 35m 06.7s , -24d 24' 19.5" }
         +/- 2.01901709458333 [arcmin] (estimated 90% radius based on SNR)
         +/- 0.868021849924879 [arcmin] (formal 1-sigma fit error)
    SNR: 11.1481832769637
 
  Angular difference between Flight and Ground position is 0.552080 arcmin
 
  Partial Coding Fraction: 0.1855469    [ including projection effects ]

  Duration
     T90: 17.6160000562668 +/- 2.47690129067317
        Measured from: -1.72799998521805
                   to: 15.8880000710487     [s; relative to TRIGTIME]
     T50: 9.60000002384186 +/- 2.44361699787484
        Measured from: 1.44000005722046
                   to: 11.0400000810623     [s; relative to TRIGTIME]



  Fluence
     Peak Flux  (peak 1 second)
        Measured from: 0.420000016689301     
                   to: 1.4200000166893     [s; relative to TRIGTIME]
     Total Fluence        
        Measured from: -2.783999979496     
                   to: 17.1520000100136     [s; relative to TRIGTIME]
     
             Band 1     Band 2     Band 3     Band 4
              15-25      25-50     50-100    100-350     keV
 Total     0.520557   0.814011   0.374668   0.060832
           0.075245   0.077393   0.064755   0.053952 [error]
 Peak      0.038653   0.063699   0.044627   0.023698
           0.016554   0.017425   0.014898   0.013122 [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 2.11e-07 3.09e-07 3.39e-07 6.98e-07 1.07e-06 1.56e-06   erg/cm2
              Error 3.74e-08 3.77e-08 6.19e-08 2.52e-07 1.48e-07 3.17e-07   erg/cm2
Peak flux Power-law 4.76e-01 4.20e-01 2.54e-01 2.32e-01 1.25e+00 1.38e+00   ph/cm2/s
              Error 2.37e-01 1.43e-01 1.01e-01 1.77e-01 4.21e-01 4.48e-01   ph/cm2/s
 
Fluence   Cutoff-PL 1.78e-07 3.67e-07 3.35e-07 1.11e-07 9.67e-07 9.91e-07   erg/cm2
              Error 4.43e-08 5.51e-08 7.72e-08 1.61e-07 1.55e-07 2.20e-07   erg/cm2
Peak flux Cutoff-PL 2.94e-01 5.56e-01 2.83e-01 2.17e-02 1.15e+00 1.15e+00   ph/cm2/s
              Error 2.78e-01 2.00e-01 1.40e-01 9.59e-02 4.36e-01 4.39e-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    1.869    0.206    -      -           5.85e-03 8.07e-04   68.890 57
CPL   0.356    1.199      48.0   12.4      4.02e-02 1.13e-01   62.200 56
 
 
=== 1-s peak spectral analysis ===
 
Model Ph_index Ph_90err Epeak  Epeak_90err Norm     Nomr_90err chi2   dof
PL    1.725    0.508    -      -           9.32e-03 3.12e-03   68.910 57
CPL  -1.244    4.572      50.3   36.2      3.54e-01 1.13e+02   65.640 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   19.936   -2.784   17.152
T90    17.616   -1.728   15.888
T50     9.600    1.440   11.040
Peak    1.000    0.420    1.420

Click here for the BAT GCN circular template

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
  323.7779   -24.4054   0.0174    39.6492   -62.7566         1.7659817     11.148 TRIG_00744791                 
 
Foreground time interval of the image:
 -2.784  17.152 (delta_t =  19.936 [sec])
Background time interval of the image:
-239.280  -2.784 (delta_t = 236.496 [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 8.192000

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 8.192000

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 8.192000

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   -2.784 sec. to   17.152 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.86877     ( -0.201759   0.210921 )
Norm@50keV  : 5.85021E-03    ( -0.000813261   0.000799855 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          68.89 using 59 PHA bins.
# Reduced chi-squared =          1.209 for     57 degrees of freedom 
# Null hypothesis probability =   1.344039e-01
 
Photon flux (15-150 keV)    in 19.94 sec: 0.828698 ( -0.102284  0.102405 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.07262e-06 ( -1.47164e-07  1.49111e-07 ) ergs/cm2

Cutoff power-law model

Time interval is from   -2.784 sec. to   17.152 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 0.355513     ( -1.35509   1.04264 )
Epeak [keV] : 47.9571      ( -8.32925 16.3744 )
Norm@50keV  : 4.01682E-02    ( -0.0401692   0.186362 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          62.20 using 59 PHA bins.
# Reduced chi-squared =          1.111 for     56 degrees of freedom 
# Null hypothesis probability =   2.649671e-01
 
Photon flux (15-150 keV)    in 19.94 sec: 0.789239 ( -0.105778  0.105911 ) ph/cm2/s
Energy fluence (15-150 keV)             : 9.66619e-07 ( -1.49764e-07  1.60384e-07 ) ergs/cm2

Band function

Time interval is from   -2.784 sec. to   17.152 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]    : 11.4898  (-1.35961  1.55095)
R^2/D10^2   : 0.243733  (-0.0935965   0.148677)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          67.06 using 59 PHA bins.
# Reduced chi-squared =          1.177 for     57 degrees of freedom 
# Null hypothesis probability =   1.701044e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.350e-07   2.927e-08
25- 50  4.034e-07   6.620e-08
50-150  3.107e-07   8.385e-08
15-150  8.491e-07   1.287e-07

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 82.5182       (-24.8433      46.0694)
Norm        : 3.91371       (-0.65006     0.790861)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          64.38 using 59 PHA bins.
# Reduced chi-squared =          1.129 for     57 degrees of freedom 
# Null hypothesis probability =   2.341587e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  2.029e-07   3.563e-08
25- 50  3.364e-07   4.427e-08
50-150  4.848e-07   2.349e-07
15-150  1.024e-06   2.167e-07

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 5.97818        (-5.2329      -6.05198)
R1^2/D10^2  : 1.18264        (-0.896221      -1.11391)
kT2 [keV]   : 15.0353        (-3.83425      -15.2689)
R2^2/D10^2  : 6.79028E-02    (-0.0615111   0.214411)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          62.70 using 59 PHA bins.
# Reduced chi-squared =          1.140 for     55 degrees of freedom 
# Null hypothesis probability =   2.221041e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.755e-07   9.383e-08
25- 50  3.653e-07   1.853e-07
50-150  4.028e-07   2.338e-07
15-150  9.435e-07   4.790e-07

Peak spectrum fit

Power-law model

Time interval is from    0.420 sec. to    1.420 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.72458     ( -0.50131   0.514016 )
Norm@50keV  : 9.32168E-03    ( -0.00313968   0.00310209 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          68.91 using 59 PHA bins.
# Reduced chi-squared =          1.209 for     57 degrees of freedom 
# Null hypothesis probability =   1.339954e-01
 
Photon flux (15-150 keV)    in 1 sec: 1.24879 ( -0.418702  0.42231 ) ph/cm2/s
Energy fluence (15-150 keV)             : 8.61747e-08 ( -2.93339e-08  2.97698e-08 ) ergs/cm2

Cutoff power-law model

Time interval is from    0.420 sec. to    1.420 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: -1.24437     ( -6.20315   2.94186 )
Epeak [keV] : 50.2748      ( -12.5389 59.8914 )
Norm@50keV  : 0.354045    ( -0.466591   225.446 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          65.64 using 59 PHA bins.
# Reduced chi-squared =          1.172 for     56 degrees of freedom 
# Null hypothesis probability =   1.773120e-01
 
Photon flux (15-150 keV)    in 1 sec: 1.15371 ( -0.435607  0.43604 ) ph/cm2/s
Energy fluence (15-150 keV)             : 7.51623e-08 ( -2.57085e-08  2.93097e-08 ) ergs/cm2

Band function

Time interval is from    0.420 sec. to    1.420 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]    : 12.8729  (-3.095  4.04822)
R^2/D10^2   : 0.267530  (-0.26753   0.477773)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          65.59 using 59 PHA bins.
# Reduced chi-squared =          1.151 for     57 degrees of freedom 
# Null hypothesis probability =   2.036418e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  9.403e-09   5.950e-09
25- 50  3.204e-08   2.007e-08
50-150  3.337e-08   2.306e-08
15-150  7.482e-08   4.011e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 107.379       (-61.5446      -106.087)
Norm        : 5.60732       (-2.07847     3.09771)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          67.87 using 59 PHA bins.
# Reduced chi-squared =          1.191 for     57 degrees of freedom 
# Null hypothesis probability =   1.535813e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.465e-08   9.210e-09
25- 50  2.569e-08   1.569e-08
50-150  4.329e-08   3.242e-08
15-150  8.363e-08   5.765e-08

Double BB

------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 196.992        (-197.553      -197.553)
R1^2/D10^2  : 4.76676E-05        (-4.72287e-05      0.693314)
kT2 [keV]   : 12.0096        (-12.0088      4.50318)
R2^2/D10^2  : 0.327498    (-0.328021   1.70148)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          65.57 using 59 PHA bins.
#Fit statistic : Chi-Squared =          65.22 using 59 PHA bins.
# Reduced chi-squared =          1.192 for     55 degrees of freedom 
# Reduced chi-squared =          1.186 for     55 degrees of freedom 
# Null hypothesis probability =   1.557874e-01
# Null hypothesis probability =   1.628299e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.024e-08   7.695e-09
25- 50  3.187e-08   2.377e-08
50-150  3.366e-08   2.471e-08
15-150  7.577e-08   5.115e-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: 1.86877     ( -0.201759   0.210921 )
Norm@50keV  : 5.85021E-03    ( -0.000813261   0.000799855 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          68.89 using 59 PHA bins.
# Reduced chi-squared =          1.209 for     57 degrees of freedom 
# Null hypothesis probability =   1.344039e-01
 
Photon flux (15-150 keV)    in 19.94 sec: 0.828648 ( -0.102274  0.102396 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.07244e-06 ( -1.47114e-07  1.49174e-07 ) ergs/cm2

Cutoff power-law model

Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 0.359644     ( -1.35617   1.04163 )
Epeak [keV] : 47.9715      ( -8.33153 16.3384 )
Norm@50keV  : 3.99541E-02    ( -0.0401654   0.186362 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          62.20 using 59 PHA bins.
# Reduced chi-squared =          1.111 for     56 degrees of freedom 
# Null hypothesis probability =   2.649660e-01
 
Photon flux (15-150 keV)    in 19.94 sec: 0.789132 ( -0.105745  0.105876 ) ph/cm2/s
Energy fluence (15-150 keV)             : 9.66879e-07 ( -1.49845e-07  1.60467e-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)  = 3.09e-07
S(50-100 keV) = 3.39e-07

T90 vs. Hardness ratio plot

T90                                   = 17.6160000562668 sec.
Hardness ratio (energy fluence ratio) = 1.09709

Color vs. Color plot

Count Ratio  (25-50 keV) / (15-25 keV) = 1.56373
Count Ratio (50-100 keV) / (15-25 keV) = 0.719744

Mask shadow pattern

IMX = 3.793650527095629E-01, IMY = 7.367904562794484E-01

TIME vs. PHA plot around the trigger time

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 8.192000

TIME vs. DetID plot around the trigger time

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 8.192000

100 us light curve (15-350 keV)

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 8.192000

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:
-239.280000 -2.784000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
244.9453 -15.5901    1.4  37.2   86.9   7.2556   8.5    3.6	Sco X-1                       
255.9994 -37.8163    2.6  34.4   45.0   2.0584   4.4    1.8	4U 1700-377                   
256.3684 -36.4808    5.6  33.4   46.6   0.9202   2.1    4.7	GX 349+2                      
262.9789 -24.7072    4.2  22.2   61.6   0.8574   2.8    2.8	GX 1+4                        
264.8119 -44.6037    7.3  34.9   28.3   0.6256   1.6    9.7	4U 1735-44                    
268.2183  -1.3215    6.7  19.2  132.9  -0.5134  -1.7   11.9	SW J1753.5-0127               
270.3586 -25.0275    2.7  16.8   49.7   1.2083   4.2    5.1	GX 5-1                        
270.1337 -25.5950    0.0  17.4   48.7   0.7499   2.6   12.7	GRS 1758-258                  
273.9995 -14.0743    3.3   9.1   90.0   0.9031   3.5    2.3	GX 17+2                       
275.9186 -30.2912   23.8  18.2   26.0  -0.1360  -0.5    4.6	H1820-303                     
285.0794 -24.8352   74.2  11.5   -2.9   0.0464   0.2    5.6	HT1900.1-2455                 
288.7600  10.8935    1.6  24.9 -162.2   2.1128   7.2    3.9	GRS 1915+105                  
299.5922  35.1936    1.3  51.0 -157.8   7.3841   8.8    0.5	Cyg X-1                       
263.0886 -33.9159    5.6  27.5   43.5   0.7024   2.1    7.0	GX 354-0                      
259.9017 -25.0173    0.8  24.9   63.9   4.9948  15.1 ------	UNKNOWN                       
290.7376  39.9920    2.6  53.9 -167.9   4.3290   4.4 ------	UNKNOWN                       
325.4784 -46.5195    3.1  48.3  -33.1   2.3326   3.7 ------	UNKNOWN                       
329.3296 -38.6308    4.8  47.7  -44.4   2.9189   2.4 ------	UNKNOWN                       
324.7343 -15.5586    3.1  40.1  -76.6   4.6211   3.8 ------	UNKNOWN

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

Time interval of the image:
-2.784000 17.152000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
244.8201 -15.6816    8.6  37.3   86.7  -0.2580  -1.4    9.5	Sco X-1                       
255.8404 -37.9589    5.6  34.6   44.9   0.2170   2.1    9.8	4U 1700-377                   
256.5183 -36.4292    7.1  33.2   46.5   0.1632   1.6    4.0	GX 349+2                      
263.1719 -24.8843    7.5  22.2   61.0   0.1103   1.5   12.2	GX 1+4                        
264.8229 -44.5278    5.4  34.9   28.4  -0.1784  -2.1    5.8	4U 1735-44                    
268.5161  -1.5169    8.7  18.9  133.0  -0.0835  -1.3    9.7	SW J1753.5-0127               
270.2094 -25.2138   10.8  17.1   49.5  -0.0647  -1.1    9.0	GX 5-1                        
270.4676 -25.7919    6.0  17.3   47.5   0.1221   2.0    9.4	GRS 1758-258                  
274.1567 -13.9611    8.4   8.9   90.6   0.0822   1.4    9.9	GX 17+2                       
275.7684 -30.5181    0.0  18.4   26.0   0.0631   1.0   12.2	H1820-303                     
284.9563 -25.0300    5.9  11.7   -2.3   0.1108   1.9    7.9	HT1900.1-2455                 
288.9250  10.8502    5.4  24.9 -161.8  -0.1286  -2.2    9.4	GRS 1915+105                  
299.5694  35.2017    4.1  51.0 -157.8   0.4749   2.8    1.0	Cyg X-1                       
263.1595 -33.8853    3.7  27.4   43.5  -0.2290  -3.1    9.0	GX 354-0                      
294.5601 -28.1171    1.9  18.0  -28.7   0.3375   6.0 ------	UNKNOWN                       
323.7779 -24.4054    1.0  39.6  -62.8   1.7657  11.1 ------	UNKNOWN

Post-slew image of 15-350 keV band

Time interval of the image:
108.220600 962.854800
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
285.1984 -24.9076    5.6  34.9  107.4  -2.6856  -2.1    8.9	HT1900.1-2455                 
288.7431  10.9437    4.3  49.2  158.3   5.4093   2.7    3.3	GRS 1915+105                  
 26.3386 -58.6555    3.5  55.2   -7.8   5.8767   3.3 ------	UNKNOWN                       
 11.9362 -19.3067    3.7  44.8  -60.2  10.6092   3.1 ------	UNKNOWN

Plot creation:
Tue Apr 25 19:02:02 EDT 2017