batgrbproduct analysis for trigger=556753

batgrbproduct Analysis for Trigger=556753

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 03:01:18 EST 2014
             Host Name: batevent1
   Current Working Dir: /local/data/batevent/batevent_reproc/trigger556753
======================================================================

  Trigger: 00556753      Segment: 000

  BAT Trigger Time: 391357300.8   [s; MET]
      Trigger Stop: 391357301.824   [s; MET]
               UTC: 2013-05-27T14:21:30.195820    [includes UTCF correction] 
       Where From?: TDRSS position message

  BAT 
    RA: 309.278622826908   Dec: -24.7278211819239  [deg; J2000]

     Catalogged Source?: NO
     Point Source?:      YES
     GRB Indicated?:     YES    [ by BAT flight software ]
     Image S/N Ratio:    13.89
     Image Trigger?:     NO
     Rate S/N Ratio:     255.998046867549  [ if not an image trigger ]
     Image S/N Ratio:    13.89

  Flight Position:   [ source = BAT ]
    RA: 309.278622826908   Dec: -24.7278211819239  [deg; J2000]

  Ground Position:   [ source = BAT pre-slew burst ]
    RA: 309.28367215012   Dec: -24.7256766136192  [deg; J2000]  
        { 20h 37m 08.1s , -24d 43' 32.4" }
         +/- 1.09781641137707 [arcmin] (estimated 90% radius based on SNR)
         +/- 0.452517545266986 [arcmin] (formal 1-sigma fit error)
    SNR: 26.6206577351153
 
  Angular difference between Flight and Ground position is 0.303780 arcmin
 
  Partial Coding Fraction: 0.1005859    [ including projection effects ]

  Duration
     T90: 64 +/- 16
        Measured from: -11.8000000119209
                   to: 52.1999999880791     [s; relative to TRIGTIME]
     T50: 32 +/- 16
        Measured from: -11.8000000119209
                   to: 20.1999999880791     [s; relative to TRIGTIME]



  Fluence
     Peak Flux  (peak 1 second)
        Measured from: -4.30000001192093     
                   to: -3.30000001192093     [s; relative to TRIGTIME]
     Total Fluence        
        Measured from: -11.8000000119209     
                   to: 164.199999988079     [s; relative to TRIGTIME]
     
             Band 1     Band 2     Band 3     Band 4
              15-25      25-50     50-100    100-350     keV
 Total     3.274903   5.901808   6.010891   2.751821
           0.181348   0.198521   0.188777   0.165669 [error]
 Peak      0.018947   0.010782   0.010736  -0.026477
           0.021768   0.022964   0.018371   0.017685 [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 1.21e-06 2.73e-06 4.86e-06 2.04e-05 1.33e-05 2.92e-05   erg/cm2
              Error 9.42e-08 1.24e-07 1.86e-07 1.86e-06 4.83e-07 1.92e-06   erg/cm2
Peak flux Power-law 1.45e-01 1.34e-01 8.60e-02 8.50e-02 4.00e-01 4.47e-01   ph/cm2/s
              Error 3.95e-01 1.73e-01 9.91e-02 7.14e-01 5.43e-01 5.56e-01   ph/cm2/s
 
Fluence   Cutoff-PL 1.21e-06 2.73e-06 4.87e-06 2.03e-05 1.33e-05 2.92e-05   erg/cm2
              Error 9.68e-08 1.24e-07 1.83e-07 2.39e-06 4.78e-07 2.86e-06   erg/cm2
Peak flux Cutoff-PL 2.02e-01 1.51e-01 7.52e-02 5.43e-02 2.72e-01 4.82e-01   ph/cm2/s
              Error 3.95e-01 1.74e-01 1.46e-01 -------- -------- 5.58e-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    1.167    0.065    -      -           7.35e-03 2.65e-04   49.710 57
CPL   1.164    0.094    9999.4    0.0      7.39e-03 7.61e-04   49.760 56
 
 
=== 1-s peak spectral analysis ===
 
Model Ph_index Ph_90err Epeak  Epeak_90err Norm     Nomr_90err chi2   dof
PL    9.430    0.000    -      -           1.81e-06 3.32e-03   69.430 57
CPL   9.349    0.000    9999.4    0.0      2.04e-06 0.00e+00   69.450 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: 42.112000 sec.
T50 in the 50-300 keV band: 5.696000 sec.

 
=== Table of the duration information ==
 
        Value   tstart    tstop
T100  176.000  -11.800  164.200
T90    64.000  -11.800   52.200
T50    32.000  -11.800   20.200
Peak    1.000   -4.300   -3.300

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
  309.2837   -24.7257   0.0072    48.7603   155.8505        13.4439160     26.621 TRIG_00556753                 
 
Foreground time interval of the image:
-11.800  17.701 (delta_t =  29.501 [sec])
Background time interval of the image:
-644.699 -630.292 (delta_t =  14.408 [sec])
-239.800 -11.800 (delta_t = 228.000 [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 1.024000

8 ms binning

From T100_start-3 s to T100_start+3 s

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.024000

2 ms binning

From T100_start-1 s to T100_start+1 s

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.024000

SN=5 or 10 sec. binning (whichever binning is satisfied first)

SN=5 or 10 sec. binning (T < 200 sec)

Quad-rate summed light curves (from T0-300s to T0+1000s)

Spectral Evolution

Spectra

Notes:

1) The fitting includes the systematic errors.
2) When the burst includes telescope slew time periods, the fitting uses an average response file made from multiple 5-s response files through out the slew time plus single time preiod for the non-slew times, and weighted by the total counts in the corresponding time period using addrmf. An average response file is needed becuase a spectral fit using the pre-slew DRM will introduce some errors in both a spectral shape and a normalization if the PHA file contains a lot of the slew/post-slew time interval.
3) For fits to more complicated models (e.g. a power-law over a cutoff power-law), the BAT team has decided to require a chi-square improvement of more than 6 for each extra dof.

Time averaged spectrum fit using the average DRM

Power-law model

Time interval is from  -11.800 sec. to  164.200 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.16667     ( -0.0655488   0.0649779 )
Norm@50keV  : 7.35439E-03    ( -0.000265596   0.000264573 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          49.71 using 59 PHA bins.
# Reduced chi-squared =         0.8720 for     57 degrees of freedom 
# Null hypothesis probability =   7.426208e-01
 
Photon flux (15-150 keV)    in 176 sec: 0.859424 ( -0.0333574  0.0335074 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.32588e-05 ( -4.82298e-07  4.82877e-07 ) ergs/cm2

Cutoff power-law model

Time interval is from  -11.800 sec. to  164.200 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.16371     ( -0.123837   0.0636399 )
Epeak [keV] : 9999.35      ( -9999.36 -9999.36 )
Norm@50keV  : 7.39297E-03    ( -0.00026386   0.00125913 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          49.76 using 59 PHA bins.
# Reduced chi-squared =         0.8886 for     56 degrees of freedom 
# Null hypothesis probability =   7.086324e-01
 
Photon flux (15-150 keV)    in 176 sec: 0.859910 (    ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.3262e-05 ( -4.80357e-07  4.7615e-07 ) ergs/cm2

Band function

Time interval is from  -11.800 sec. to  164.200 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -0.997153   ( 0.919508   0.919508 )
beta        : -1.18579    ( -0.0649467   0.0656058 )
Epeak [keV] : 243.206      ( -242.15 -242.15 )
Norm@50keV   : 9.11391E-03    ( -0.00202894   0 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          49.50 using 59 PHA bins.
# Reduced chi-squared =         0.9001 for     55 degrees of freedom 
# Null hypothesis probability =   6.838623e-01
 
Photon flux (15-150 keV)    in 176 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]    : 21.3272  (  )
R^2/D10^2   : 3.17569E-02  (   )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =         228.19 using 59 PHA bins.
# Reduced chi-squared =         4.0034 for     57 degrees of freedom 
# Null hypothesis probability =   2.415114e-22
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  4.771e-07   3.546e-08
25- 50  2.476e-06   1.487e-07
50-150  8.403e-06   4.690e-07
15-150  1.136e-05   4.356e-07

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 199.363       (      )
Norm        : 3.70714       (     )
------------------------------------------------------------
#Fit statistic : Chi-Squared =         167.13 using 59 PHA bins.
# Reduced chi-squared =         2.9320 for     57 degrees of freedom 
# Null hypothesis probability =   9.451476e-13
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.625e-06   6.266e-08
25- 50  3.125e-06   1.126e-07
50-150  6.854e-06   2.658e-07
15-150  1.160e-05   4.215e-07

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 10.5266        (-1.37071      1.46823)
R1^2/D10^2  : 0.216894        (-0.0668447      0.109488)
kT2 [keV]   : 51.9315        (-11.8172      28.1579)
R2^2/D10^2  : 1.70895E-03    (-0.00109088   0.00183536)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          52.35 using 59 PHA bins.
# Reduced chi-squared =         0.9518 for     55 degrees of freedom 
# Null hypothesis probability =   5.764668e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  9.609e-07   1.136e-07
25- 50  2.961e-06   2.772e-07
50-150  9.351e-06   1.940e-06
15-150  1.327e-05   2.296e-06

Peak spectrum fit

Power-law model

Time interval is from   -4.300 sec. to   -3.300 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 9.43048     (     )
Norm@50keV  : 1.80930E-06    ( -1.79502e-06   0.00663907 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          69.43 using 59 PHA bins.
# Reduced chi-squared =          1.218 for     57 degrees of freedom 
# Null hypothesis probability =   1.249623e-01
 
Photon flux (15-150 keV)    in 1 sec: 0.399975 ( -0.400483  0.686101 ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.86134e-08 ( -2.86146e-08  3.57782e-08 ) ergs/cm2

Cutoff power-law model

Time interval is from   -4.300 sec. to   -3.300 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 9.34936     (     )
Epeak [keV] : 9999.36      (   )
Norm@50keV  : 2.04466E-06    (     )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          69.45 using 59 PHA bins.
# Reduced chi-squared =          1.240 for     56 degrees of freedom 
# Null hypothesis probability =   1.068814e-01
 
Photon flux (15-150 keV)    in 1 sec: 0.451551 0.271744 (    ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.80439e-16 ( 0  0 ) ergs/cm2

Band function

Time interval is from   -4.300 sec. to   -3.300 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -1.41453   ( 1.29181   1.29181 )
beta        : -9.35630    ( 1.60521   1.60521 )
Epeak [keV] : 0.781225      ( -26.8244 -26.8244 )
Norm@50keV   : 1251.25    ( -1251.14   1.0195e+10 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          69.44 using 59 PHA bins.
# Reduced chi-squared =          1.263 for     55 degrees of freedom 
# Null hypothesis probability =   9.099188e-02
 
Photon flux (15-150 keV)    in 1 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]    : 36.8205  (  )
R^2/D10^2   : 1.70901E-03  (   )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          70.29 using 59 PHA bins.
# Reduced chi-squared =          1.233 for     57 degrees of freedom 
# Null hypothesis probability =   1.110534e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  9.511e-09   7.185e-09
25- 50  3.510e-09   2.773e-09
50-150  4.470e-11   8.250e-11
15-150  1.307e-08   1.146e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 1.30048       (      )
Norm        : 5.08858E+05       (     )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          68.96 using 59 PHA bins.
# Reduced chi-squared =          1.210 for     57 degrees of freedom 
# Null hypothesis probability =   1.331165e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  8.507e-09   5.495e-09
25- 50  1.012e-09   1.059e-09
50-150  4.583e-12   1.306e-11
15-150  9.523e-09   6.640e-09

Double BB

R1^2/D10^2  : 1.36793E+08        (      )
kT2 [keV]   : 77.6806        (-199.291      -199.291)
R2^2/D10^2  : 2.12977E-04    (   )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          69.16 using 59 PHA bins.
#Fit statistic : Chi-Squared =          69.09 using 59 PHA bins.
#Fit statistic : Chi-Squared =          67.45 using 59 PHA bins.
# Reduced chi-squared =          1.257 for     55 degrees of freedom 
# Reduced chi-squared =          1.256 for     55 degrees of freedom 
# Reduced chi-squared =          1.226 for     55 degrees of freedom 
# Null hypothesis probability =   9.490156e-02
# Null hypothesis probability =   9.581908e-02
# Null hypothesis probability =   1.209179e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  9.376e-09   6.515e-09
25- 50  3.954e-09   2.154e-09
50-150  1.650e-08   9.890e-09
15-150  2.983e-08   1.447e-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: 1.00685     ( -0.0713175   0.0703319 )
Norm@50keV  : 3.14900E-02    ( -0.00128829   0.00128235 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          54.65 using 59 PHA bins.
# Reduced chi-squared =         0.9587 for     57 degrees of freedom 
# Null hypothesis probability =   5.638312e-01
 
Photon flux (15-150 keV)    in 29.5 sec: 3.62663 ( -0.152936  0.153814 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.00205e-05 ( -4.00049e-07  4.01415e-07 ) ergs/cm2

Cutoff power-law model

Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.00073     ( -0.0718193   0.0708465 )
Epeak [keV] : 9999.35      ( -9999.35 -9999.35 )
Norm@50keV  : 3.16777E-02    ( -0.00122305   0.00955572 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          54.65 using 59 PHA bins.
# Reduced chi-squared =         0.9758 for     56 degrees of freedom 
# Null hypothesis probability =   5.262010e-01
 
Photon flux (15-150 keV)    in 29.5 sec: 3.62560 ( -0.15886  0.15335 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.00248e-05 ( -3.88338e-07  4.00758e-07 ) ergs/cm2

Band function

 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -0.251107   ( 0.783779   0.783779 )
beta        : -1.06891    ( -0.0703478   0.0713446 )
Epeak [keV] : 90.4744      ( -90.4744 306.952 )
Norm@50keV   : 8.43923E-02    ( -0.0467227   897115 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          52.91 using 59 PHA bins.
# Reduced chi-squared =         0.9621 for     55 degrees of freedom 
# Null hypothesis probability =   5.547289e-01
 
Photon flux (15-150 keV)    in 29.5 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)  = 2.73e-06
S(50-100 keV) = 4.86e-06

T90 vs. Hardness ratio plot

T90                                   = 64 sec.
Hardness ratio (energy fluence ratio) = 1.78022

Color vs. Color plot

Count Ratio  (25-50 keV) / (15-25 keV) = 1.80213
Count Ratio (50-100 keV) / (15-25 keV) = 1.83544

Mask shadow pattern

IMX = -1.040862663714176E+00, IMY = -4.666803415466253E-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:
-644.699410 -630.291900
-239.800000 -11.800000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
170.4168 -60.6356    5.7  41.1   -5.2   0.6448   2.0    3.1	Cen X-3                       
186.6606 -62.7652    9.0  35.8    4.4   0.3817   1.3    0.3	GX 301-2                      
255.8959 -38.0172    6.5  39.1   87.2   1.7562   1.8   11.2	4U 1700-377                   
264.5889 -44.5218    7.1  31.0   95.0   0.7091   1.6    7.9	4U 1735-44                    
275.1702 -54.4532    2.8  19.6  104.2   1.0321   4.2 ------	UNKNOWN                       
319.8802 -19.9909    3.4  54.8  167.4   4.7239   3.5 ------	UNKNOWN                       
146.9880 -45.4890    3.5  59.5  -17.0   4.8279   3.3 ------	UNKNOWN                       
125.4661 -51.9410    3.7  55.1  -34.7   4.4437   3.1 ------	UNKNOWN                       
 48.8672 -59.6168    3.0  40.8  -88.3   4.5069   3.9 ------	UNKNOWN                       
  7.9572 -36.5153    3.0  51.0 -135.6   4.8801   3.9 ------	UNKNOWN

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

Time interval of the image:
-11.800000 17.700600
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
170.2168 -60.7162    5.3  41.1   -5.4  -0.2796  -2.2    6.3	Cen X-3                       
186.4347 -62.8376    5.9  35.8    4.2   0.2270   1.9    7.3	GX 301-2                      
256.0329 -37.9079    3.8  39.2   87.4   1.5289   3.0    4.4	4U 1700-377                   
264.9616 -44.4928   20.1  31.0   95.5   0.1295   0.6    9.7	4U 1735-44                    
220.9103 -41.3379    3.8  45.6   47.8   1.2618   3.1 ------	UNKNOWN                       
281.6635 -33.0668    2.5  40.0  121.2   1.9644   4.5 ------	UNKNOWN                       
309.2837 -24.7257    0.4  48.8  155.9  13.4432  26.6 ------	UNKNOWN                       
183.6073 -43.2733    2.0  54.3   13.6   2.5694   5.9 ------	UNKNOWN                       
338.8132 -34.3329    2.9  44.8 -166.7   0.6553   4.0 ------	UNKNOWN                       
154.4253 -45.2580    2.5  58.6  -11.0   2.2642   4.7 ------	UNKNOWN                       
357.2890 -38.6386    2.8  45.9 -145.0   0.7045   4.2 ------	UNKNOWN                       
 50.2827 -59.9312    3.0  40.8  -87.1   1.1849   3.9 ------	UNKNOWN

Post-slew image of 15-350 keV band

Time interval of the image:
93.700590 962.270000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
264.8693 -44.5221    8.1  40.9   61.0  -3.4330  -1.4    6.9	4U 1735-44                    
270.3737 -25.0841    3.6  35.2   92.3   4.6216   3.2    4.9	GX 5-1                        
270.1514 -25.6066    0.0  35.3   91.3  -1.0166  -0.7   11.6	GRS 1758-258                  
273.8939 -14.1417    4.3  34.9  112.3   4.2515   2.7    9.1	GX 17+2                       
275.7582 -30.3096    5.1  30.1   83.0   2.5478   2.3    9.3	H1820-303                     
284.8712 -24.9661    4.8  22.1   95.5  -1.8147  -2.4    9.4	HT1900.1-2455                 
288.8033  10.9470    1.1  40.9  159.6  12.8436  10.3    0.3	GRS 1915+105                  
280.7428 -16.8086    2.7  27.8  112.3   3.9393   4.3 ------	UNKNOWN                       
285.3544  -5.8314    2.4  29.7  136.8   4.2901   4.9 ------	UNKNOWN                       
299.5766 -13.3391    2.7  14.6  150.7   2.2832   4.3 ------	UNKNOWN                       
 12.2688 -60.9592    3.9  55.5  -20.4   6.7084   3.0 ------	UNKNOWN                       
  7.6744 -41.2726    4.1  50.7  -44.6  11.0308   2.8 ------	UNKNOWN

Plot creation:
Sat May 30 16:47:49 EDT 2015