batgrbproduct analysis for trigger=547918

batgrbproduct Analysis for Trigger=547918

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): Sun Jan 12 05:36:56 EST 2014
             Host Name: batevent1
   Current Working Dir: /local/data/batevent/batevent_reproc/trigger547918
======================================================================

  Trigger: 00547918      Segment: 000

  BAT Trigger Time: 381872198.784   [s; MET]
      Trigger Stop: 381872200.832   [s; MET]
               UTC: 2013-02-06T19:36:28.596780    [includes UTCF correction] 
       Where From?: TDRSS position message

  BAT 
    RA: 140.374791824771   Dec: -58.1604827693569  [deg; J2000]

     Catalogged Source?: NO
     Point Source?:      YES
     GRB Indicated?:     YES    [ by BAT flight software ]
     Image S/N Ratio:    8.15
     Image Trigger?:     NO
     Rate S/N Ratio:     14.3527000944073  [ if not an image trigger ]
     Image S/N Ratio:    8.15

  Flight Position:   [ source = BAT ]
    RA: 140.374791824771   Dec: -58.1604827693569  [deg; J2000]

  Ground Position:   [ source = BAT pre-slew burst ]
    RA: 140.377028982237   Dec: -58.1994806823637  [deg; J2000]  
        { 09h 21m 30.5s , -58d 11' 58.1" }
         +/- 1.54546431335891 [arcmin] (estimated 90% radius based on SNR)
         +/- 0.516519850310467 [arcmin] (formal 1-sigma fit error)
    SNR: 16.3318025698332
 
  Angular difference between Flight and Ground position is 2.340945 arcmin
 
  Partial Coding Fraction: 0.5234375    [ including projection effects ]

  Duration
     T90: 121 +/- 32.3882694814033
        Measured from: -4.783999979496
                   to: 116.216000020504     [s; relative to TRIGTIME]
     T50: 45 +/- 7.21110255092798
        Measured from: 7.216000020504
                   to: 52.216000020504     [s; relative to TRIGTIME]



  Fluence
     Peak Flux  (peak 1 second)
        Measured from: 1.216000020504     
                   to: 2.216000020504     [s; relative to TRIGTIME]
     Total Fluence        
        Measured from: -8.783999979496     
                   to: 147.216000020504     [s; relative to TRIGTIME]
     
             Band 1     Band 2     Band 3     Band 4
              15-25      25-50     50-100    100-350     keV
 Total     1.015228   1.074623   0.948257   0.146027
           0.094701   0.095118   0.083836   0.075957 [error]
 Peak      0.034062   0.042924   0.024420   0.012197
           0.007978   0.008372   0.007583   0.006586 [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 2.92e-07 5.08e-07 6.76e-07 1.84e-06 1.97e-06 3.31e-06   erg/cm2
              Error 4.48e-08 4.69e-08 8.54e-08 5.01e-07 2.02e-07 5.68e-07   erg/cm2
Peak flux Power-law 3.20e-01 2.94e-01 1.87e-01 1.82e-01 8.77e-01 9.83e-01   ph/cm2/s
              Error 1.12e-01 6.89e-02 6.05e-02 1.17e-01 2.03e-01 2.33e-01   ph/cm2/s
 
Fluence   Cutoff-PL 2.94e-07 5.09e-07 6.78e-07 1.69e-06 1.96e-06 3.17e-06   erg/cm2
              Error 4.47e-08 4.99e-08 8.73e-08 -------- 2.09e-07 8.25e-07   erg/cm2
Peak flux Cutoff-PL 3.06e-01 3.19e-01 1.85e-01 7.55e-02 8.59e-01 8.84e-01   ph/cm2/s
              Error 1.19e-01 9.22e-02 -------- 1.10e-01 1.55e-01 2.62e-01   ph/cm2/s
 
Fluence        Band -------- -------- -------- -------- -------- --------   erg/cm2
              Error -------- -------- -------- -------- -------- --------   erg/cm2
Peak flux      Band 3.06e-01 3.18e-01 1.85e-01 7.85e-02 8.60e-01 8.88e-01   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    1.589    0.166    -      -           1.35e-03 1.27e-04   59.270 57
CPL   1.588    0.205    9999.3    0.0      1.35e-03 8.14e-04   59.270 56
 
 
=== 1-s peak spectral analysis ===
 
Model Ph_index Ph_90err Epeak  Epeak_90err Norm     Nomr_90err chi2   dof
PL    1.655    0.397    -      -           6.70e-03 1.71e-03   55.980 57
CPL   1.046    1.925      64.9   -5.6      1.53e-02 3.69e-01   55.400 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: 59.776000 sec.
T50 in the 50-300 keV band: 37.504000 sec.

 
=== Table of the duration information ==
 
        Value   tstart    tstop
T100  156.000   -8.784  147.216
T90   121.000   -4.784  116.216
T50    45.000    7.216   52.216
Peak    1.000    1.216    2.216

Click here for the BAT GCN circular template

Image

Pre-slew 15.0-350.0 keV image (Event data)

#   RAcent    DECcent   POSerr    Theta     Phi              Peak Cts       SNR   Name
  140.3770   -58.1995   0.0118    30.6001    36.7810         3.8008661     16.332 TRIG_00547918                 
 
Foreground time interval of the image:
 -8.784 147.216 (delta_t = 156.000 [sec])
Background time interval of the image:
-239.784  -8.784 (delta_t = 231.000 [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 2.048000

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 2.048000

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 2.048000

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)

The mask-weighted light curves based on cleaned DPHs

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   -8.784 sec. to  147.216 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.58852     ( -0.164687   0.166595 )
Norm@50keV  : 1.34933E-03    ( -0.000127225   0.000126037 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          59.27 using 59 PHA bins.
# Reduced chi-squared =          1.040 for     57 degrees of freedom 
# Null hypothesis probability =   3.928505e-01
 
Photon flux (15-150 keV)    in 156 sec: 0.172785 ( -0.0157467  0.0157782 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.97139e-06 ( -2.00661e-07  2.02805e-07 ) ergs/cm2

Cutoff power-law model

Time interval is from   -8.784 sec. to  147.216 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.58849     ( -0.244517   0.166278 )
Epeak [keV] : 9999.33      ( -9999.36 -9999.36 )
Norm@50keV  : 1.34876E-03    ( -0.000454029   0.00117324 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          59.27 using 59 PHA bins.
# Reduced chi-squared =          1.058 for     56 degrees of freedom 
# Null hypothesis probability =   3.571666e-01
 
Photon flux (15-150 keV)    in 156 sec: 0.172780 ( -0.015806  0.015708 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.96401e-06 ( -2.08853e-07  2.10085e-07 ) ergs/cm2

Band function

Time interval is from   -8.784 sec. to  147.216 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : 4.85521   ( -4.85521   -4.85521 )
beta        : -1.62851    ( -0.184861   0.175997 )
Epeak [keV] : 21.1519      ( -21.1519 4.82411 )
Norm@50keV   : 336.891    ( -29.9102   799550 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          58.47 using 59 PHA bins.
# Reduced chi-squared =          1.063 for     55 degrees of freedom 
# Null hypothesis probability =   3.491584e-01
 
Photon flux (15-150 keV)    in 156 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]    : 14.9510  (-1.92994  2.23146)
R^2/D10^2   : 1.86997E-02  (-0.00716759   0.0118069)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =         101.71 using 59 PHA bins.
# Reduced chi-squared =         1.7843 for     57 degrees of freedom 
# Null hypothesis probability =   2.507742e-04
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.366e-07   2.421e-08
25- 50  5.411e-07   7.511e-08
50-150  8.220e-07   1.679e-07
15-150  1.500e-06   1.752e-07

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 197.832       (-77.771      -197.667)
Norm        : 0.698090       (-0.0627795     0.0731879)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          60.40 using 59 PHA bins.
# Reduced chi-squared =          1.060 for     57 degrees of freedom 
# Null hypothesis probability =   3.539679e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  2.715e-07   6.755e-08
25- 50  5.217e-07   2.291e-07
50-150  1.141e-06   5.692e-07
15-150  1.934e-06   9.248e-07

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 5.37302        (-1.05942      1.32874)
R1^2/D10^2  : 0.533983        (-0.309495      0.811904)
kT2 [keV]   : 24.5368        (-4.34996      6.68641)
R2^2/D10^2  : 2.83949E-03    (-0.00157983   0.00279801)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          55.12 using 59 PHA bins.
# Reduced chi-squared =          1.002 for     55 degrees of freedom 
# Null hypothesis probability =   4.701830e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  3.147e-07   1.231e-07
25- 50  4.709e-07   1.376e-07
50-150  1.188e-06   3.789e-07
15-150  1.974e-06   5.838e-07

Peak spectrum fit

Power-law model

Time interval is from    1.216 sec. to    2.216 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.65540     ( -0.390416   0.403484 )
Norm@50keV  : 6.70068E-03    ( -0.00172869   0.00168683 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          55.98 using 59 PHA bins.
# Reduced chi-squared =         0.9821 for     57 degrees of freedom 
# Null hypothesis probability =   5.133478e-01
 
Photon flux (15-150 keV)    in 1 sec: 0.876505 ( -0.203291  0.203448 ) ph/cm2/s
Energy fluence (15-150 keV)             : 6.22859e-08 ( -1.65624e-08  1.72462e-08 ) ergs/cm2

Cutoff power-law model

Time interval is from    1.216 sec. to    2.216 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.04579     ( -2.50797   1.34116 )
Epeak [keV] : 64.9177      ( -53.7035 -64.9797 )
Norm@50keV  : 1.52708E-02    ( -0.0152862   0.722311 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          55.40 using 59 PHA bins.
# Reduced chi-squared =         0.9893 for     56 degrees of freedom 
# Null hypothesis probability =   4.974256e-01
 
Photon flux (15-150 keV)    in 1 sec: 0.858739 ( -0.20548  0.105002 ) ph/cm2/s
Energy fluence (15-150 keV)             : 5.75708e-08 ( -2.00041e-08  2.0014e-08 ) ergs/cm2

Band function

Time interval is from    1.216 sec. to    2.216 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : 4.24625   ( -6.61627   1.24557 )
beta        : -2.24306    ( 9.37167   19.3717 )
Epeak [keV] : 29.3002      ( -33.7629 -67.3623 )
Norm@50keV   : 113.372    ( -112.901   62.6494 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          50.78 using 59 PHA bins.
# Reduced chi-squared =         0.9232 for     55 degrees of freedom 
# Null hypothesis probability =   6.365530e-01
 
Photon flux (15-150 keV)    in 1 sec: 0.859830 (    ) ph/cm2/s
Energy fluence (15-150 keV)             : 5.65703e-08 ( -5.65633e-08  -1.65544e-08 ) ergs/cm2

Single BB

 
Spectral model blackbody:
------------------------------------------------------------
Parameters  : value    Lower 90%  Upper 90%
kT [keV]    : 9.45887  (-2.26988  4.06451)
R^2/D10^2   : 0.517637  (-0.379961   0.958418)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          58.55 using 59 PHA bins.
# Reduced chi-squared =          1.027 for     57 degrees of freedom 
# Null hypothesis probability =   4.183050e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  9.232e-09   4.233e-09
25- 50  2.117e-08   9.277e-09
50-150  9.385e-09   5.666e-09
15-150  3.979e-08   1.701e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 132.366       (-77.7594      -129.416)
Norm        : 3.67472       (-0.932594     1.48851)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          55.44 using 59 PHA bins.
# Reduced chi-squared =         0.9727 for     57 degrees of freedom 
# Null hypothesis probability =   5.336464e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  9.524e-09   5.600e-09
25- 50  1.732e-08   9.845e-09
50-150  3.238e-08   2.136e-08
15-150  5.922e-08   3.606e-08

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 6.95527        (-1.83557      2.5657)
R1^2/D10^2  : 1.31658        (-0.901737      2.66466)
kT2 [keV]   : 31.7069        (-15.4235      -31.6944)
R2^2/D10^2  : 4.80083E-03    (-0.0045572   0.0146142)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          51.64 using 59 PHA bins.
# Reduced chi-squared =         0.9389 for     55 degrees of freedom 
# Null hypothesis probability =   6.037822e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.089e-08   6.630e-09
25- 50  1.835e-08   1.046e-08
50-150  3.412e-08   2.100e-08
15-150  6.336e-08   3.466e-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: 1.58852     ( -0.164687   0.166595 )
Norm@50keV  : 1.34933E-03    ( -0.000127225   0.000126037 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          59.27 using 59 PHA bins.
# Reduced chi-squared =          1.040 for     57 degrees of freedom 
# Null hypothesis probability =   3.928505e-01
 
Photon flux (15-150 keV)    in 156 sec: 0.172785 ( -0.0157467  0.0157782 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.97139e-06 ( -2.00661e-07  2.02805e-07 ) ergs/cm2

Cutoff power-law model

Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.58849     ( -0.244517   0.166278 )
Epeak [keV] : 9999.33      ( -9999.36 -9999.36 )
Norm@50keV  : 1.34876E-03    ( -0.000454029   0.00117324 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          59.27 using 59 PHA bins.
# Reduced chi-squared =          1.058 for     56 degrees of freedom 
# Null hypothesis probability =   3.571666e-01
 
Photon flux (15-150 keV)    in 156 sec: 0.172780 ( -0.015806  0.015708 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.96401e-06 ( -2.08853e-07  2.10085e-07 ) ergs/cm2

Band function

 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : 4.85521   ( -4.85521   -4.85521 )
beta        : -1.62851    ( -0.184861   0.175997 )
Epeak [keV] : 21.1519      ( -21.1519 4.82411 )
Norm@50keV   : 336.891    ( -29.9102   799550 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          58.47 using 59 PHA bins.
# Reduced chi-squared =          1.063 for     55 degrees of freedom 
# Null hypothesis probability =   3.491584e-01
 
Photon flux (15-150 keV)    in 156 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)  = 5.08e-07
S(50-100 keV) = 6.76e-07

T90 vs. Hardness ratio plot

T90                                   = 121 sec.
Hardness ratio (energy fluence ratio) = 1.33071

Color vs. Color plot

Count Ratio  (25-50 keV) / (15-25 keV) = 1.0585
Count Ratio (50-100 keV) / (15-25 keV) = 0.934034

Mask shadow pattern

IMX = 4.736715253089596E-01, IMY = -3.541063402407680E-01

TIME vs. PHA plot around the trigger time

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 2.048000

TIME vs. DetID plot around the trigger time

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 2.048000

100 us light curve (15-350 keV)

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 2.048000

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:
-239.784000 -8.784000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
170.3020 -60.5941    1.9  16.4   51.9   1.2528   6.0    1.8	Cen X-3                       
186.5448 -62.7814    2.5   8.5   54.9   0.8013   4.6    3.1	GX 301-2                      
244.9453 -15.6425    1.1  55.2 -164.6   7.3948  10.9    2.0	Sco X-1                       
255.9605 -37.8568    2.3  39.5 -139.2   1.6267   5.0    1.4	4U 1700-377                   
256.4265 -36.4576    3.5  40.8 -139.8   1.0891   3.3    2.1	GX 349+2                      
264.5199 -44.3536  119.4  37.9 -124.7   0.0309   0.1   11.2	4U 1735-44                    
262.9347 -33.9669    8.4  45.7 -135.1  -0.6903  -1.4    8.4	GX 354-0                      
121.1635 -43.7172    2.0  49.3   38.6   5.3844   5.9 ------	UNKNOWN                       
118.1265 -59.9082    3.0  38.1   21.2   1.1040   3.9 ------	UNKNOWN                       
  4.0902 -64.5759    4.2  50.8  -44.5   2.5921   2.8 ------	UNKNOWN                       
  8.8072 -63.6135    2.9  52.1  -42.2   3.7976   3.9 ------	UNKNOWN

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

Time interval of the image:
-8.784000 147.216000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
170.2759 -60.7232    7.5  16.4   51.5   0.2572   1.5    6.1	Cen X-3                       
186.5646 -62.9519    4.4   8.4   53.8  -0.4187  -2.6   11.2	GX 301-2                      
244.8971 -15.7739    0.0  55.1 -164.6  -0.6370  -1.2    9.3	Sco X-1                       
255.9606 -37.8399    5.8  39.5 -139.2  -0.5062  -2.0    1.3	4U 1700-377                   
256.6465 -36.5459   46.7  40.9 -139.5  -0.0695  -0.2   12.6	GX 349+2                      
264.6347 -44.5570    4.9  37.8 -124.4   0.6953   2.3    7.9	4U 1735-44                    
263.0879 -33.7005    0.0  46.0 -135.2  -0.8633  -1.9    9.4	GX 354-0                      
140.3770 -58.1995    0.7  30.6   36.8   3.8012  16.3 ------	UNKNOWN                       
231.5410 -11.3717    1.9  55.5  178.7   4.4420   6.1 ------	UNKNOWN                       
 31.8628 -58.5220    1.9  57.7  -28.9   5.8498   5.9 ------	UNKNOWN

Post-slew image of 15-350 keV band

Time interval of the image:
741.516600 962.280800
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
254.3276  35.2399    3.3  29.5   37.1   0.8099   3.5    8.9	Her X-1                       
268.2597  -1.4059    4.7  48.7  -19.5   0.9121   2.5    7.1	SW J1753.5-0127               
288.7713  10.9437    0.9  31.7  -46.2   3.1371  12.8    1.6	GRS 1915+105                  
299.5922  35.1936    0.6   9.8  -94.6   3.5052  20.0    0.5	Cyg X-1                       
308.0982  40.9481    1.9  12.6 -139.1   1.0120   5.9    0.6	Cyg X-3                       
326.0399  38.2839    3.8  26.6 -143.4   0.5934   3.1    6.6	Cyg X-2                       
  8.5090  82.5186    2.5  46.2  139.1   3.3067   4.6 ------	UNKNOWN                       
290.4565  37.7391    3.0   4.9  -42.7   0.6083   3.8 ------	UNKNOWN                       
  3.1001  42.6941    3.1  51.1 -167.2   1.7961   3.7 ------	UNKNOWN                       
332.2138  16.0059    2.6  43.8 -116.3   3.4440   4.4 ------	UNKNOWN

Plot creation:
Sat May 30 17:27:19 EDT 2015