batgrbproduct analysis for trigger=345777

batgrbproduct Analysis for Trigger=345777

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 19 18:27:20 EST 2014
             Host Name: batevent1
   Current Working Dir: /local/data/batevent/batevent_reproc/trigger345777
======================================================================

  Trigger: 00345777      Segment: 000

  BAT Trigger Time: 258228088   [s; MET]
      Trigger Stop: 258228152   [s; MET]
               UTC: 2009-03-08T18:01:23.441660    [includes UTCF correction] 
       Where From?: TDRSS position message

  BAT 
    RA: 183.526014699304   Dec: -48.8329591097236  [deg; J2000]

     Catalogged Source?: NO
     Point Source?:      YES
     GRB Indicated?:     YES    [ by BAT flight software ]
     Image S/N Ratio:    8.92
     Image Trigger?:     YES
     Rate S/N Ratio:     0  [ if not an image trigger ]
     Image S/N Ratio:    8.92

  Flight Position:   [ source = BAT ]
    RA: 183.526014699304   Dec: -48.8329591097236  [deg; J2000]

  Ground Position:   [ source = BAT pre-slew burst ]
    RA: 183.504494783963   Dec: -48.7285990877751  [deg; J2000]  
        { 12h 14m 01.1s , -48d 43' 43.0" }
         +/- 2.39511017607746 [arcmin] (estimated 90% radius based on SNR)
         +/- 1.48454993146122 [arcmin] (formal 1-sigma fit error)
    SNR: 8.73423382659895
 
  Angular difference between Flight and Ground position is 6.319141 arcmin
 
  Partial Coding Fraction: 0.890625    [ including projection effects ]

  Duration
     T90: 25.0959999859333 +/- 5.86202596421854
        Measured from: 17.1240000128746
                   to: 42.2199999988079     [s; relative to TRIGTIME]
     T50: 12.5160000026226 +/- 6.54216722789276
        Measured from: 25.2680000066757
                   to: 37.7840000092983     [s; relative to TRIGTIME]



  Fluence
     Peak Flux  (peak 1 second)
        Measured from: 16.5920000076294     
                   to: 17.5920000076294     [s; relative to TRIGTIME]
     Total Fluence        
        Measured from: 16.5959999859333     
                   to: 45.3560000061989     [s; relative to TRIGTIME]
     
             Band 1     Band 2     Band 3     Band 4
              15-25      25-50     50-100    100-350     keV
 Total     0.257635   0.163587   0.057186   0.004593
           0.029542   0.029078   0.024654   0.021992 [error]
 Peak      0.021188   0.016567   0.005745   0.001051
           0.005395   0.005457   0.004561   0.003942 [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 6.45e-08 7.16e-08 5.68e-08 7.44e-08 2.20e-07 2.67e-07   erg/cm2
              Error 1.29e-08 1.33e-08 2.01e-08 4.96e-08 4.73e-08 7.81e-08   erg/cm2
Peak flux Power-law 1.63e-01 1.09e-01 4.81e-02 2.91e-02 3.34e-01 3.49e-01   ph/cm2/s
              Error 7.16e-02 4.19e-02 3.18e-02 3.95e-02 1.21e-01 1.30e-01   ph/cm2/s
 
Fluence   Cutoff-PL 6.16e-08 8.24e-08 4.72e-08 9.89e-09 1.99e-07 2.01e-07   erg/cm2
              Error 1.41e-08 1.82e-08 2.39e-08 4.40e-08 4.64e-08 5.85e-08   erg/cm2
Peak flux Cutoff-PL 1.40e-01 1.41e-01 4.32e-02 2.72e-03 3.27e-01 3.27e-01   ph/cm2/s
              Error 1.12e-01 6.14e-02 4.17e-02 2.87e-02 1.19e-01 1.19e-01   ph/cm2/s
 
Fluence        Band 6.10e-08 8.20e-08 4.73e-08 9.94e-09 1.99e-07 2.01e-07   erg/cm2
              Error 1.38e-08 1.80e-08 2.46e-08 -------- 4.63e-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    2.335    0.340    -      -           7.97e-04 2.09e-04   58.460 57
CPL   1.089    1.396      26.7    0.0      4.84e-03 0.00e+00   56.010 56
 
 
=== 1-s peak spectral analysis ===
 
Model Ph_index Ph_90err Epeak  Epeak_90err Norm     Nomr_90err chi2   dof
PL    2.186    0.709    -      -           2.03e-03 1.08e-03   38.870 57
CPL   0.124    3.862      35.5    0.0      3.59e-02 0.00e+00   37.300 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   28.760   16.596   45.356
T90    25.096   17.124   42.220
T50    12.516   25.268   37.784
Peak    1.000   16.592   17.592

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
  183.5045   -48.7286   0.0222    15.1478   133.3729         0.4699268      8.734 TRIG_00345777                 
 
Foreground time interval of the image:
 16.596  45.356 (delta_t =  28.760 [sec])
Background time interval of the image:
-239.000  16.596 (delta_t = 255.596 [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 64.000000

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 64.000000

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 64.000000

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   16.596 sec. to   45.356 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 2.33531     ( -0.317951   0.362588 )
Norm@50keV  : 7.96745E-04    ( -0.000210218   0.000207722 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          58.46 using 59 PHA bins.
# Reduced chi-squared =          1.026 for     57 degrees of freedom 
# Null hypothesis probability =   4.216588e-01
 
Photon flux (15-150 keV)    in 28.76 sec: 0.142026 ( -0.0234121  0.0234258 ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.20459e-07 ( -4.60399e-08  4.86309e-08 ) ergs/cm2

Cutoff power-law model

Time interval is from   16.596 sec. to   45.356 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.08930     ( -1.87871   0.913703 )
Epeak [keV] : 26.6689      (   )
Norm@50keV  : 4.83965E-03    (     )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          56.01 using 59 PHA bins.
# Reduced chi-squared =          1.000 for     56 degrees of freedom 
# Null hypothesis probability =   4.746051e-01
 
Photon flux (15-150 keV)    in 28.76 sec: 0.138710 ( -0.023135  0.023342 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.9939e-07 ( -4.23281e-08  5.05149e-08 ) ergs/cm2

Band function

Time interval is from   16.596 sec. to   45.356 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -1.09545   ( -3.61221   1.67808 )
beta        : -10.0000    ( 10   20 )
Epeak [keV] : 26.6387      ( -16.1608 12.3134 )
Norm@50keV   : 4.79271E-03    ( -0.00479272   0.0753192 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          56.01 using 59 PHA bins.
# Reduced chi-squared =          1.018 for     55 degrees of freedom 
# Null hypothesis probability =   4.368453e-01
 
Photon flux (15-150 keV)    in 28.76 sec:  (    ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.99258e-07 ( -1.99057e-07  -4.24138e-08 ) ergs/cm2

Single BB

 
Spectral model blackbody:
------------------------------------------------------------
Parameters  : value    Lower 90%  Upper 90%
kT [keV]    : 8.04943  (-1.42818  1.67115)
R^2/D10^2   : 0.155933  (-0.0826285   0.185422)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          60.93 using 59 PHA bins.
# Reduced chi-squared =          1.069 for     57 degrees of freedom 
# Null hypothesis probability =   3.365840e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  5.278e-08   1.462e-08
25- 50  9.337e-08   2.389e-08
50-150  2.502e-08   1.223e-08
15-150  1.712e-07   4.661e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 38.2314       (-12.6128      22.182)
Norm        : 0.961007       (-0.258989     0.380972)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          56.09 using 59 PHA bins.
# Reduced chi-squared =         0.9841 for     57 degrees of freedom 
# Null hypothesis probability =   5.090690e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  6.248e-08   1.441e-08
25- 50  8.057e-08   2.069e-08
50-150  5.928e-08   3.539e-08
15-150  2.023e-07   5.474e-08

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 3.75173        (-2.0257      2.72255)
R1^2/D10^2  : 2.05396        (-1.79146      189.152)
kT2 [keV]   : 11.3976        (-3.12487      7.18816)
R2^2/D10^2  : 2.98314E-02    (-0.0270653   0.0960757)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          55.17 using 59 PHA bins.
# Reduced chi-squared =          1.003 for     55 degrees of freedom 
# Null hypothesis probability =   4.681897e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  6.248e-08   3.220e-08
25- 50  8.099e-08   4.272e-08
50-150  5.231e-08   3.329e-08
15-150  1.958e-07   1.008e-07

Peak spectrum fit

Power-law model

Time interval is from   16.592 sec. to   17.592 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 2.18589     ( -0.612254   0.806212 )
Norm@50keV  : 2.03427E-03    ( -0.00110723   0.001044 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          38.87 using 59 PHA bins.
# Reduced chi-squared =         0.6819 for     57 degrees of freedom 
# Null hypothesis probability =   9.683385e-01
 
Photon flux (15-150 keV)    in 1 sec: 0.334298 ( -0.120862  0.12108 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.90867e-08 ( -8.32032e-09  9.21806e-09 ) ergs/cm2

Cutoff power-law model

Time interval is from   16.592 sec. to   17.592 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 0.123736     ( -5.66856   2.056 )
Epeak [keV] : 35.4978      (   )
Norm@50keV  : 3.59039E-02    (     )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          37.30 using 59 PHA bins.
# Reduced chi-squared =         0.6661 for     56 degrees of freedom 
# Null hypothesis probability =   9.743326e-01
 
Photon flux (15-150 keV)    in 1 sec: 0.327002 ( -0.118349  0.118829 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.7164e-08 ( -6.8103e-09  8.7003e-09 ) ergs/cm2

Band function

Time interval is from   16.592 sec. to   17.592 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -0.195973   ( -1.80512   0.153564 )
beta        : -9.37167    ( 9.37167   19.3716 )
Epeak [keV] : 35.5137      ( -17.2082 133.289 )
Norm@50keV   : 3.23264E-02    ( -0.0428934   1.12738e+06 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          37.31 using 59 PHA bins.
# Reduced chi-squared =         0.6784 for     55 degrees of freedom 
# Null hypothesis probability =   9.675450e-01
 
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]    : 9.49435  (-2.99814  3.91487)
R^2/D10^2   : 0.206973  (-0.206973   0.669728)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          37.65 using 59 PHA bins.
# Reduced chi-squared =         0.6605 for     57 degrees of freedom 
# Null hypothesis probability =   9.776157e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  3.725e-09   2.343e-09
25- 50  8.590e-09   5.540e-09
50-150  3.850e-09   3.256e-09
15-150  1.617e-08   1.060e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 46.2071       (-25.7152      100.988)
Norm        : 2.04543       (-0.930779     1.82974)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          37.79 using 59 PHA bins.
# Reduced chi-squared =         0.6631 for     57 degrees of freedom 
# Null hypothesis probability =   9.766320e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  4.905e-09   3.126e-09
25- 50  6.842e-09   4.317e-09
50-150  6.154e-09   4.905e-09
15-150  1.790e-08   1.208e-08

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 2.94161        (-2.9486      -2.9486)
R1^2/D10^2  : 10.6352        (-10.5712      -10.5712)
kT2 [keV]   : 10.8647        (-3.89752      -10.8681)
R2^2/D10^2  : 0.109359    (-0.1092   0.561371)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          36.83 using 59 PHA bins.
# Reduced chi-squared =         0.6696 for     55 degrees of freedom 
# Null hypothesis probability =   9.716638e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  4.448e-09   2.128e-09
25- 50  7.725e-09   4.697e-09
50-150  4.944e-09   3.517e-09
15-150  1.712e-08   9.900e-09

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: 2.33531     ( -0.317951   0.362588 )
Norm@50keV  : 7.96745E-04    ( -0.000210218   0.000207722 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          58.46 using 59 PHA bins.
# Reduced chi-squared =          1.026 for     57 degrees of freedom 
# Null hypothesis probability =   4.216588e-01
 
Photon flux (15-150 keV)    in 28.76 sec: 0.142026 ( -0.0234121  0.0234258 ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.20459e-07 ( -4.60399e-08  4.86309e-08 ) ergs/cm2

Cutoff power-law model

Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.08930     ( -1.87871   0.913703 )
Epeak [keV] : 26.6689      (   )
Norm@50keV  : 4.83965E-03    (     )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          56.01 using 59 PHA bins.
# Reduced chi-squared =          1.000 for     56 degrees of freedom 
# Null hypothesis probability =   4.746051e-01
 
Photon flux (15-150 keV)    in 28.76 sec: 0.138710 ( -0.023135  0.023342 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.9939e-07 ( -4.23281e-08  5.05149e-08 ) ergs/cm2

Band function

 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -1.09545   ( -3.61221   1.67807 )
beta        : -10.0000    ( 10   20 )
Epeak [keV] : 26.6387      ( -16.1609 12.3133 )
Norm@50keV   : 4.79271E-03    ( -0.00479272   0.0753192 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          56.01 using 59 PHA bins.
# Reduced chi-squared =          1.018 for     55 degrees of freedom 
# Null hypothesis probability =   4.368453e-01
 
Photon flux (15-150 keV)    in 28.76 sec:  (    ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.99258e-07 ( -1.99057e-07  -4.24138e-08 ) ergs/cm2

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

S(25-50 keV)  = 7.16e-08
S(50-100 keV) = 5.68e-08

T90 vs. Hardness ratio plot

T90                                   = 25.0959999859333 sec.
Hardness ratio (energy fluence ratio) = 0.793296

Color vs. Color plot

Count Ratio  (25-50 keV) / (15-25 keV) = 0.634956
Count Ratio (50-100 keV) / (15-25 keV) = 0.221965

Mask shadow pattern

IMX = -1.859131598750296E-01, IMY = -1.967837481636095E-01

TIME vs. PHA plot around the trigger time

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 64.000000

TIME vs. DetID plot around the trigger time

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 64.000000

100 us light curve (15-350 keV)

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 64.000000

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:
-239.000000 16.596000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
135.5197 -40.5701    1.1  29.8   37.4   2.8002  10.9    1.0	Vela X-1                      
170.3605 -60.6176    1.3   1.3  101.0   1.6112   9.1    1.4	Cen X-3                       
186.6272 -62.7696    0.5   7.6 -158.6   4.4806  21.9    0.8	GX 301-2                      
255.9050 -37.7924    3.7  55.3 -155.4   2.2036   3.1    5.0	4U 1700-377                   
256.5776 -36.6159    0.0  56.6 -155.7   0.8626   0.9   13.4	GX 349+2                      
264.5853 -44.4697   27.5  53.7 -144.1   0.5616   0.4    6.9	4U 1735-44                    
 54.4749 -55.7975    3.9  52.1  -42.1   3.4913   3.0 ------	UNKNOWN                       
346.3524 -77.0459    3.7  41.0  -83.4   2.6201   3.1 ------	UNKNOWN                       
299.2591 -72.0516    4.0  41.6 -103.2   2.6089   2.9 ------	UNKNOWN

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

Time interval of the image:
16.596000 45.356000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
135.4966 -40.4914    3.2  29.9   37.5  -0.2918  -3.6    4.1	Vela X-1                      
170.0103 -60.6340    4.1   1.3   93.5  -0.1468  -2.8    9.0	Cen X-3                       
186.4065 -62.6872    4.6   7.5 -159.2   0.1243   2.5    8.5	GX 301-2                      
256.0025 -37.8259    4.4  55.4 -155.3   0.5478   2.6    1.3	4U 1700-377                   
256.3326 -36.4883    6.8  56.6 -156.0   0.4039   1.7    6.3	GX 349+2                      
264.7404 -44.4489   39.6  53.7 -144.0  -0.0770  -0.3    0.1	4U 1735-44                    
183.5044 -48.7287    1.3  15.1  133.4   0.4693   8.7 ------	UNKNOWN                       
129.8112 -48.8497    2.4  25.8   19.5   0.3043   4.9 ------	UNKNOWN                       
251.2813 -43.3674    2.9  48.8 -154.8   0.4789   3.9 ------	UNKNOWN                       
259.2209 -35.1773    2.1  59.0 -154.5   1.9919   5.5 ------	UNKNOWN

Post-slew image of 15-350 keV band

Time interval of the image:
110.900600 673.000610
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
135.5532 -40.5407    1.0  34.5   13.2   4.8082  11.2    1.4	Vela X-1                      
170.3621 -60.6217    1.1  14.0  -44.8   3.4424  10.9    1.4	Cen X-3                       
186.6437 -62.7663    0.4  14.0  -78.2   9.9555  30.6    0.4	GX 301-2                      
255.9606 -37.8494    1.4  51.8 -145.7   8.2832   8.5    1.3	4U 1700-377                   
256.5325 -36.4322    8.0  53.0 -146.8   1.6898   1.4    4.7	GX 349+2                      
132.6568 -32.2269    3.5  41.2   22.1   1.9105   3.3 ------	UNKNOWN                       
126.7688 -42.5779    3.0  39.2    4.8   1.9368   3.9 ------	UNKNOWN                       
149.3371 -53.5896    3.6  21.7   -7.9   0.9935   3.2 ------	UNKNOWN                       
242.8682 -17.2189    3.2  57.1 -174.1   5.0713   3.6 ------	UNKNOWN                       
170.0914 -61.9205    2.0  15.1  -47.5   1.7968   5.7 ------	UNKNOWN                       
239.4215 -25.4241    2.2  49.0 -169.8   3.2107   5.2 ------	UNKNOWN                       
242.7998 -30.5108    2.8  47.8 -162.1   2.7449   4.1 ------	UNKNOWN                       
 94.6153 -59.0313    3.3  49.3  -29.6   2.4970   3.5 ------	UNKNOWN                       
 84.1172 -51.2082    3.7  58.7  -26.0   7.2855   3.1 ------	UNKNOWN                       
 78.3012 -65.7411    4.8  52.0  -42.1   4.9210   2.4 ------	UNKNOWN                       
261.7299 -57.9087    3.0  44.8 -119.9   5.3653   3.9 ------	UNKNOWN                       
268.6422 -82.6462    3.9  41.1  -83.5   4.5555   3.0 ------	UNKNOWN

Plot creation:
Sun May 31 04:44:35 EDT 2015