batgrbproduct analysis for trigger=558399

batgrbproduct Analysis for Trigger=558399

Analysis Summary

Notes:

1) No attempt has been made to eliminate the non-significant decimal places.
2) This batgrbproduct analysis is done of the amount of data for this trigger downloaded to date.
3) This batgrbproduct analysis is using the flight position for the mask-weighting calculation.
4) This page will be updated for up to 10 downlinks after the trigger.

======================================================================
                  BAT GRB EVENT DATA PROCESSING REPORT
    Process Script Ver: batgrbproduct v2.46
    Process Start Time (local time): Tue Jun 18 03:39:23 EDT 2013
             Host Name: gcn5
   Current Working Dir: /local/data/raid16/prebascript_archive/trigger558399/GCN5_download_cron
======================================================================

  Trigger: 00558399      Segment: 000

  BAT Trigger Time: 393155560.944   [s; MET]
      Trigger Stop: 393155560.96   [s; MET]
               UTC: 2013-06-17T09:52:30.259560    [includes UTCF correction] 
       Where From?: (*SHORT BURST*) TDRSS scaled map message

  BAT 
    RA: 237.714151615488   Dec: -54.2768302799622  [deg; J2000]

     Catalogged Source?: YES
     Point Source?:      YES
     GRB Indicated?:     NO    [ by BAT flight software ]
     Image S/N Ratio:    8.57
     Image Trigger?:     NO
     Rate S/N Ratio:     27.6405499221705  [ if not an image trigger ]
     Image S/N Ratio:    8.57

  Flight Position:   [ source = BAT ]
    RA: 237.714151615488   Dec: -54.2768302799622  [deg; J2000]

  Ground Position:   [ source = BAT pre-slew burst ]
    RA: 237.721174163164   Dec: -54.3007219105831  [deg; J2000]  
        { 15h 50m 53.1s , -54d 18' 02.6" }
         +/- 1.27546247579649 [arcmin] (estimated 90% radius based on SNR)
         +/- 0.492034253928338 [arcmin] (formal 1-sigma fit error)
    SNR: 21.4864438410339
 
  Angular difference between Flight and Ground position is 1.454443 arcmin
 
  Partial Coding Fraction: 0.875    [ including projection effects ]

  Duration
     T90: 0.13999992609024 +/- 0.0126491362748289
        Measured from: 1.19209289550781e-07
                   to: 0.14000004529953     [s; relative to TRIGTIME]
     T50: 0.0799999833106995 +/- 0.0144221847352656
        Measured from: 0.0160000920295715
                   to: 0.096000075340271     [s; relative to TRIGTIME]



  Fluence
     Peak Flux  (peak 1 second)
        Measured from: -0.424000024795532     
                   to: 0.575999975204468     [s; relative to TRIGTIME]
     Total Fluence        
        Measured from: -0.00400000810623169     
                   to: 0.15200001001358     [s; relative to TRIGTIME]
     
             Band 1     Band 2     Band 3     Band 4
              15-25      25-50     50-100    100-350     keV
 Total     0.044827   0.082896   0.036666   0.003145
           0.004188   0.005199   0.003856   0.001833 [error]
 Peak      0.044146   0.078716   0.044068   0.006661
           0.007181   0.007853   0.006253   0.004693 [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 0.00e+00 0.00e+00 0.00e+00 0.00e+00 0.00e+00 0.00e+00   erg/cm2
              Error 0.00e+00 0.00e+00 0.00e+00 0.00e+00 0.00e+00 0.00e+00   erg/cm2
Peak flux Power-law 5.01e-01 4.67e-01 3.02e-01 3.01e-01 1.39e+00 1.57e+00   ph/cm2/s
              Error 9.27e-02 5.94e-02 4.88e-02 9.14e-02 1.75e-01 1.98e-01   ph/cm2/s
 
Fluence   Cutoff-PL 1.13e-08 3.56e-08 2.77e-08 2.74e-09 7.72e-08 7.73e-08   erg/cm2
              Error 2.24e-09 3.39e-09 4.14e-09 1.66e-09 6.85e-09 6.93e-09   erg/cm2
Peak flux Cutoff-PL 3.61e-01 5.97e-01 3.31e-01 1.33e+00 1.33e+00 0.00e+00   ph/cm2/s
              Error 1.12e-01 8.82e-02 6.53e-02 1.78e-01 1.82e-01 0.00e+00   ph/cm2/s
 
Fluence        Band 0.00e+00 0.00e+00 0.00e+00 0.00e+00 0.00e+00 0.00e+00   erg/cm2
              Error 0.00e+00 0.00e+00 0.00e+00 0.00e+00 0.00e+00 0.00e+00   erg/cm2
Peak flux      Band 0.00e+00 0.00e+00 0.00e+00 0.00e+00 0.00e+00 0.00e+00   ph/cm2/s
              Error 0.00e+00 0.00e+00 0.00e+00 0.00e+00 0.00e+00 0.00e+00   ph/cm2/s

 
=== Time-averaged spectral analysis ===
 
Model Ph_index Ph_90err Epeak  Epeak_90err Norm     Nomr_90err chi2   dof
PL    2.160    0.000    -      -           4.58e-02 0.00e+00  138.220 57
CPL  -1.544    0.897      46.2    2.9      4.39e+00 6.38e+00   50.040 56
 
The chi2 of BB fit is 49.46 which shows a significant improvement in the fit over a PL.
Check the BB fit.
 
=== 1-s peak spectral analysis ===
 
Model Ph_index Ph_90err Epeak  Epeak_90err Norm     Nomr_90err chi2   dof
PL    1.630    0.189    -      -           1.07e-02 1.42e-03   69.760 57
CPL  -0.755    1.371      52.9    9.0      2.06e-01 7.24e-01   54.160 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: 0.128000 sec.
T50 in the 50-300 keV band: 0.064000 sec.

 
=== Table of the duration information ==
 
        Value   tstart    tstop
T100    0.156   -0.004    0.152
T90     0.140    0.000    0.140
T50     0.080    0.016    0.096
Peak    1.000   -0.424    0.576

Click here for the BAT GCN circular template

Image

Pre-slew 15-350 keV image (Event data; bkg subtracted)

#   RAcent  DECcent POSerr  Theta    Phi     Peak Cts     SNR  Name
  237.7212 -54.3007 0.0090   22.0   19.5       0.1707    21.5  TRIG_00558399       
------------------------------------------
 
Foreground time interval of the image:
 -0.004   0.152 (delta_t =   0.156 [sec])
Background time interval of the image:
-239.944  -0.004 (delta_t = 239.940 [sec])

Lightcurves

Notes:

1) All plots contain as much data as has been downloaded to date.
2) The mask-weighted light curves are using the flight position.
3) Multiple plots of different time binning/intervals are shown to cover all scenarios of short/long GRBs, rate/image triggers, and real/false positives.
4) For all the mask-weighted lightcurves, the y-axis units are counts/sec/det where a det is 0.4 x 0.4 = 0.16 sq cm.
5) The verticle lines correspond to following: green dotted lines are T50 interval, black dotted lines are T90 interval, blue solid line(s) is a spacecraft slew start time, and orange solid line(s) is a spacecraft slew end time.
6) Time of each bin is in the middle of the bin.

1 s binning

From T0-310 s to T0+310 s

From T100_start - 20 s to T100_end + 30 s

Full time interval

64 ms binning

Full time interval

From T100_start to T100_end

From T0-5 sec to T0+5 sec

16 ms binning

From T100_start-5 s to T100_start+5 s

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.016000

8 ms binning

From T100_start-3 s to T100_start+3 s

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.016000

2 ms binning

From T100_start-1 s to T100_start+1 s

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.016000

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

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

The mask-weighted light curves based on cleaned DPHs

Spectra

Notes:

1) The fitting includes the systematic errors.
2) For long bursts, a spectral fit of the pre-slew DRM will introduce some errors in both a spectral shape and a normalization if the PHA file contains a lot of the slew/post-slew time interval.
3) For fits to more complicated models (e.g. a power-law over a cutoff power-law), the BAT team has decided to require a chi-square improvement of more than 6 for each extra dof.
4) For short bursts (T90<1sec), the specrtum is also fit with Blackbody, OTTB, and Double Blackbody.

Time averaged spectrum fit using the pre-slew DRM

Power-law model

Time interval is from   -0.004 sec. to    0.152 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 2.15976     (     )
Norm@50keV  : 4.58098E-02    (     )
------------------------------------------------------------
#Fit statistic : Chi-Squared =         138.22 using 59 PHA bins.
# Reduced chi-squared =         2.4249 for     57 degrees of freedom 
# Null hypothesis probability =   1.068270e-08
 
Photon flux (15-150 keV)    in 0.156 sec:  (    ) ph/cm2/s
Energy fluence (15-150 keV)             : 0 ( 0  0 ) ergs/cm2

Cutoff power-law model

Time interval is from   -0.004 sec. to    0.152 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: -1.54426     ( -0.981564   0.812405 )
Epeak [keV] : 46.2282      ( -2.8731 2.92657 )
Norm@50keV  : 4.39127    ( -2.7292   10.037 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          50.04 using 59 PHA bins.
# Reduced chi-squared =         0.8936 for     56 degrees of freedom 
# Null hypothesis probability =   6.987513e-01
 
Photon flux (15-150 keV)    in 0.156 sec: 8.03826 ( -0.69191  0.69308 ) ph/cm2/s
Energy fluence (15-150 keV)             : 7.71716e-08 ( -6.83951e-09  6.85854e-09 ) ergs/cm2

Band function

Time interval is from   -0.004 sec. to    0.152 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : 1.54658   ( -1.0688   0.810117 )
beta        : -9.98140    ( 9.9814   19.9768 )
Epeak [keV] : 46.2170      ( -2.86912 2.91866 )
Norm@50keV   : 4.40599    ( -2.74073   10.7683 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          50.04 using 59 PHA bins.
# Reduced chi-squared =         0.9099 for     55 degrees of freedom 
# Null hypothesis probability =   6.640720e-01
 
Photon flux (15-150 keV)    in 0.156 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]    : 11.9322  (-0.742377  0.754825)
R^2/D10^2   : 2.41820  (-0.514823   0.659663)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          49.46 using 59 PHA bins.
# Reduced chi-squared =         0.8677 for     57 degrees of freedom 
# Null hypothesis probability =   7.507043e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.135e-08   1.396e-09
25- 50  3.550e-08   3.159e-09
50-150  3.027e-08   5.257e-09
15-150  7.712e-08   7.348e-09

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 58.3149       (-8.53166      9.77768)
Norm        : 43.9462       (-4.99719     5.11679)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          97.19 using 59 PHA bins.
# Reduced chi-squared =          1.705 for     57 degrees of freedom 
# Null hypothesis probability =   7.213484e-04
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.715e-08   1.942e-09
25- 50  2.587e-08   2.348e-09
50-150  2.874e-08   4.532e-09
15-150  7.176e-08   6.739e-09

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 1.99910        (-1.99649      11.0042)
R1^2/D10^2  : 980.298        (-993.436      -993.436)
kT2 [keV]   : 12.1324        (-0.802067      0.870255)
R2^2/D10^2  : 2.23089    (-0.578476   0.596903)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          47.91 using 59 PHA bins.
# Reduced chi-squared =         0.8711 for     55 degrees of freedom 
# Null hypothesis probability =   7.399502e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.224e-08   2.102e-09
25- 50  3.461e-08   4.173e-09
50-150  3.082e-08   5.148e-09
15-150  7.767e-08   7.511e-09

Peak spectrum fit

Power-law model

Time interval is from   -0.424 sec. to    0.576 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.62953     ( -0.186893   0.191834 )
Norm@50keV  : 1.07475E-02    ( -0.00142108   0.00140972 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          69.76 using 59 PHA bins.
# Reduced chi-squared =          1.224 for     57 degrees of freedom 
# Null hypothesis probability =   1.194419e-01
 
Photon flux (15-150 keV)    in 1 sec: 1.39402 ( -0.174797  0.174927 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.00178e-07 ( -1.39082e-08  1.40677e-08 ) ergs/cm2

Cutoff power-law model

Time interval is from   -0.424 sec. to    0.576 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: -0.754973     ( -1.57543   1.16659 )
Epeak [keV] : 52.8943      ( -6.82019 11.1721 )
Norm@50keV  : 0.206173    ( -0.212003   1.23665 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          54.16 using 59 PHA bins.
# Reduced chi-squared =         0.9672 for     56 degrees of freedom 
# Null hypothesis probability =   5.447122e-01
 
Photon flux (15-150 keV)    in 1 sec: 1.32542 ( -0.17825  0.17848 ) ph/cm2/s
Energy fluence (15-150 keV)             : 0 ( 0  0 ) ergs/cm2

Band function

Time interval is from   -0.424 sec. to    0.576 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : 0.772421   ( -1.04858   1.32718 )
beta        : -9.99994    ( 9.99994   19.9998 )
Epeak [keV] : 52.8169      ( -6.41645 11.1552 )
Norm@50keV   : 0.211082    ( -0.211082   1.22139 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          54.16 using 59 PHA bins.
# Reduced chi-squared =         0.9848 for     55 degrees of freedom 
# Null hypothesis probability =   5.066529e-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]    : 13.0737  (-1.41493  1.61215)
R^2/D10^2   : 0.282359  (-0.0991131   0.14668)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          54.90 using 59 PHA bins.
# Reduced chi-squared =         0.9631 for     57 degrees of freedom 
# Null hypothesis probability =   5.544350e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.024e-08   2.335e-09
25- 50  3.547e-08   5.505e-09
50-150  3.845e-08   9.505e-09
15-150  8.415e-08   1.343e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 135.146       (-48.7434      -133.49)
Norm        : 5.94728       (-0.758258     0.989945)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          64.20 using 59 PHA bins.
# Reduced chi-squared =          1.126 for     57 degrees of freedom 
# Null hypothesis probability =   2.389046e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.539e-08   3.796e-09
25- 50  2.809e-08   9.960e-09
50-150  5.301e-08   3.121e-08
15-150  9.649e-08   4.364e-08

Double BB

------------------------------------------------------------
#Fit statistic : Chi-Squared =          54.20 using 59 PHA bins.
#Fit statistic : Chi-Squared =          54.16 using 59 PHA bins.
#Fit statistic : Chi-Squared =          54.14 using 59 PHA bins.
#Fit statistic : Chi-Squared =          54.03 using 59 PHA bins.
# Reduced chi-squared =         0.9854 for     55 degrees of freedom 
# Reduced chi-squared =         0.9847 for     55 degrees of freedom 
# Reduced chi-squared =         0.9843 for     55 degrees of freedom 
# Reduced chi-squared =         0.9824 for     55 degrees of freedom 
# Null hypothesis probability =   5.052746e-01
# Null hypothesis probability =   5.068615e-01
# Null hypothesis probability =   5.075518e-01
# Null hypothesis probability =   5.116534e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.150e-08   3.410e-09
25- 50  3.418e-08   9.160e-09
50-150  4.001e-08   1.144e-08
15-150  8.570e-08   1.947e-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: 2.15976     (     )
Norm@50keV  : 4.58098E-02    (     )
------------------------------------------------------------
#Fit statistic : Chi-Squared =         138.22 using 59 PHA bins.
# Reduced chi-squared =         2.4249 for     57 degrees of freedom 
# Null hypothesis probability =   1.068270e-08
 
Photon flux (15-150 keV)    in 0.156 sec:  (    ) ph/cm2/s
Energy fluence (15-150 keV)             : 0 ( 0  0 ) ergs/cm2

Cutoff power-law model

Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: -1.54426     ( -0.981564   0.812405 )
Epeak [keV] : 46.2282      ( -2.8731 2.92657 )
Norm@50keV  : 4.39127    ( -2.7292   10.037 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          50.04 using 59 PHA bins.
# Reduced chi-squared =         0.8936 for     56 degrees of freedom 
# Null hypothesis probability =   6.987513e-01
 
Photon flux (15-150 keV)    in 0.156 sec: 8.03826 ( -0.69191  0.69308 ) ph/cm2/s
Energy fluence (15-150 keV)             : 7.71716e-08 ( -6.83951e-09  6.85854e-09 ) ergs/cm2

Band function

 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : 1.54658   ( -1.0688   0.810117 )
beta        : -9.98140    ( 9.9814   19.9768 )
Epeak [keV] : 46.2170      ( -2.86912 2.91866 )
Norm@50keV   : 4.40599    ( -2.74073   10.7683 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          50.04 using 59 PHA bins.
# Reduced chi-squared =         0.9099 for     55 degrees of freedom 
# Null hypothesis probability =   6.640720e-01
 
Photon flux (15-150 keV)    in 0.156 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)  = 
S(50-100 keV) =

T90 vs. Hardness ratio plot

T90                                   = 0.13999992609024 sec.
Hardness ratio (energy fluence ratio) =

Color vs. Color plot

Count Ratio  (25-50 keV) / (15-25 keV) = 1.84924
Count Ratio (50-100 keV) / (15-25 keV) = 0.817945

Mask shadow pattern

IMX = 0, IMY = 0

TIME vs. PHA plot around the trigger time

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.016000

TIME vs. DetID plot around the trigger time

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.016000

100 us light curve (15-350 keV)

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.016000

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:
-239.944000 -0.004000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
170.3921 -60.5022    6.3  40.3  -43.4   0.6977   1.8    7.6	Cen X-3                       
186.6412 -62.8219    3.5  33.7  -35.7   0.9125   3.3    3.1	GX 301-2                      
256.2174 -37.7362    0.0  32.1   61.0  -0.2014  -0.5   12.7	4U 1700-377                   
256.4350 -36.4175    3.2  33.4   61.8   1.5671   3.6    0.3	GX 349+2                      
264.7631 -44.3019    9.4  24.4   71.7   0.3548   1.2    8.9	4U 1735-44                    
275.7880 -30.5167    0.0  37.7   90.6   0.5268   0.6   11.4	H1820-303                     
263.1832 -33.7065    0.0  35.1   72.3   0.6739   1.2   12.4	GX 354-0                      
186.7418 -50.5032    2.9  43.5  -23.6   1.4237   3.9 ------	UNKNOWN                       
  9.9797 -35.2149    3.2  59.5 -161.7   7.1259   3.6 ------	UNKNOWN                       
 16.8809 -38.4862    2.4  58.9 -154.2   8.4455   4.8 ------	UNKNOWN                       
145.2156 -62.1078    3.4  44.8  -60.1   3.6468   3.4 ------	UNKNOWN

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

Time interval of the image:
-0.004000 0.152000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
170.1463 -60.6845    8.7  40.2  -43.7  -0.0181  -1.3    6.2	Cen X-3                       
186.3668 -62.8488    3.8  33.8  -35.9  -0.0294  -3.0    9.2	GX 301-2                      
256.0045 -37.8556    4.9  32.0   60.6   0.0307   2.4    1.1	4U 1700-377                   
256.6599 -36.3129    0.0  33.4   62.2  -0.0223  -1.5   12.7	GX 349+2                      
264.9051 -44.3158    5.8  24.4   72.0   0.0205   2.0   10.6	4U 1735-44                    
276.0085 -30.3490   21.6  37.8   90.9   0.0151   0.5    4.5	H1820-303                     
263.1474 -33.8268    5.6  35.0   72.2  -0.0365  -2.1    7.9	GX 354-0                      
310.7837 -46.6428    1.9  28.2  147.9   0.0558   6.0 ------	UNKNOWN                       
237.7212 -54.3007    0.5  22.0   19.5   0.1706  21.5 ------	UNKNOWN                       
 91.9407 -70.9805    1.9  40.8  -92.3   0.1618   6.1 ------	UNKNOWN

Post-slew image of 15-350 keV band

Time interval of the image:
55.156590 133.366000
134.056000 325.336000
326.056000 962.195600
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
170.5733 -60.5256    8.5  35.1  -83.5   2.2764   1.4    9.6	Cen X-3                       
186.7406 -62.8111    7.6  27.1  -84.4   1.4988   1.5    3.4	GX 301-2                      
244.9978 -15.6266    0.9  39.1   55.6  23.7132  12.6    1.3	Sco X-1                       
255.8482 -37.7545    9.2  20.6   88.7   0.9610   1.3    8.5	4U 1700-377                   
256.3954 -36.4049    1.9  22.0   87.8   5.2216   6.1    2.2	GX 349+2                      
262.8509 -24.7496    6.5  34.9   86.8   3.0028   1.8    8.6	GX 1+4                        
264.8749 -44.3311    9.2  20.1  116.0  -0.7825  -1.3    9.1	4U 1735-44                    
270.4176 -25.0973   15.3  37.9   97.2  -1.6736  -0.7    7.3	GX 5-1                        
270.4417 -25.7521    7.1  37.3   97.8  -3.3289  -1.6    7.5	GRS 1758-258                  
275.8353 -30.3472    7.9  36.2  108.7   2.5415   1.5    4.8	H1820-303                     
262.7652 -33.9049    0.0  26.9   95.4   1.7550   1.7   11.9	GX 354-0                      
229.3950 -33.0101    2.9  22.1   25.6   2.7087   4.0 ------	UNKNOWN                       
299.2214 -60.1665    3.4  32.6  170.1   2.7520   3.4 ------	UNKNOWN                       
187.4042 -42.5398    3.3  34.5  -46.9   2.8540   3.5 ------	UNKNOWN                       
  8.9575 -59.7544    5.2  59.5 -161.7  15.3707   2.2 ------	UNKNOWN                       
173.9673 -30.4563    3.8  50.6  -44.6  13.4459   3.1 ------	UNKNOWN

Plot creation:
Mon Jul  8 00:26:51 EDT 2013