batgrbproduct analysis for trigger=312047

batgrbproduct Analysis for Trigger=312047

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): Mon Jan 20 01:50:00 EST 2014
             Host Name: batevent1
   Current Working Dir: /local/data/batevent/batevent_reproc/trigger312047
======================================================================

  Trigger: 00312047      Segment: 000

  BAT Trigger Time: 233014827.584   [s; MET]
      Trigger Stop: 233014829.632   [s; MET]
               UTC: 2008-05-20T22:20:24.778640    [includes UTCF correction] 
       Where From?: TDRSS position message

  BAT 
    RA: 280.191885316142   Dec: -55.003825646117  [deg; J2000]

     Catalogged Source?: NO
     Point Source?:      YES
     GRB Indicated?:     YES    [ by BAT flight software ]
     Image S/N Ratio:    8.7
     Image Trigger?:     NO
     Rate S/N Ratio:     10.6301458127346  [ if not an image trigger ]
     Image S/N Ratio:    8.7

  Flight Position:   [ source = BAT ]
    RA: 280.191885316142   Dec: -55.003825646117  [deg; J2000]

  Ground Position:   [ source = BAT pre-slew burst ]
    RA: 280.193945024291   Dec: -54.9655922327671  [deg; J2000]  
        { 18h 40m 46.5s , -54d 57' 56.1" }
         +/- 2.29903343420742 [arcmin] (estimated 90% radius based on SNR)
         +/- 1.02204662051792 [arcmin] (formal 1-sigma fit error)
    SNR: 9.26030119778863
 
  Angular difference between Flight and Ground position is 2.295101 arcmin
 
  Partial Coding Fraction: 1    [ including projection effects ]

  Duration
     T90: 3.324000030756 +/- 0.861895610176173
        Measured from: -0.131999999284744
                   to: 3.19200003147125     [s; relative to TRIGTIME]
     T50: 1.74399998784065 +/- 0.776672417691704
        Measured from: 0.276000022888184
                   to: 2.02000001072884     [s; relative to TRIGTIME]



  Fluence
     Peak Flux  (peak 1 second)
        Measured from: 0.0200000107288361     
                   to: 1.02000001072884     [s; relative to TRIGTIME]
     Total Fluence        
        Measured from: -0.311999976634979     
                   to: 3.32400000095367     [s; relative to TRIGTIME]
     
             Band 1     Band 2     Band 3     Band 4
              15-25      25-50     50-100    100-350     keV
 Total     0.089738   0.055799   0.003052   0.010998
           0.010875   0.010333   0.008713   0.007576 [error]
 Peak      0.029001   0.022705   0.003692   0.003752
           0.005837   0.005519   0.004556   0.003973 [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 2.72e-08 1.95e-08 9.22e-09 6.13e-09 5.89e-08 6.21e-08   erg/cm2
              Error 5.33e-09 5.44e-09 5.42e-09 7.63e-09 1.43e-08 1.77e-08   erg/cm2
Peak flux Power-law 2.78e-01 1.49e-01 4.96e-02 2.14e-02 4.88e-01 4.98e-01   ph/cm2/s
              Error 8.69e-02 4.76e-02 3.15e-02 2.80e-02 1.30e-01 1.34e-01   ph/cm2/s
 
Fluence   Cutoff-PL 2.71e-08 2.07e-08 7.08e-09 1.13e-09 5.59e-08 5.60e-08   erg/cm2
              Error 5.52e-09 6.40e-09 7.30e-09 6.94e-09 1.45e-08 1.79e-08   erg/cm2
Peak flux Cutoff-PL 2.68e-01 1.66e-01 4.29e-02 4.89e-03 4.81e-01 4.83e-01   ph/cm2/s
              Error 9.60e-02 6.36e-02 4.08e-02 2.58e-02 1.28e-01 1.30e-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    3.080    0.520    -      -           1.30e-03 5.75e-04   55.790 57
CPL   1.898    0.000       2.7    0.0      8.42e-03 0.00e+00   55.340 56
 
 
=== 1-s peak spectral analysis ===
 
Model Ph_index Ph_90err Epeak  Epeak_90err Norm     Nomr_90err chi2   dof
PL    2.586    0.637    -      -           2.36e-03 1.15e-03   44.940 57
CPL   1.583    0.000      14.6    0.0      1.04e-02 0.00e+00   44.480 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    3.636   -0.312    3.324
T90     3.324   -0.132    3.192
T50     1.744    0.276    2.020
Peak    1.000    0.020    1.020

Click here for the BAT GCN circular template

Special notes of this burst

Image

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

#   RAcent    DECcent   POSerr    Theta     Phi              Peak Cts       SNR   Name
  280.1939   -54.9656   0.0209    17.3684  -157.9874         0.1762445      9.260 TRIG_00312047                 
 
Foreground time interval of the image:
 -0.312   3.324 (delta_t =   3.636 [sec])
Background time interval of the image:
-137.283  -0.312 (delta_t = 136.971 [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)

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   -0.312 sec. to    3.324 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 3.08025     ( -0.462925   0.576709 )
Norm@50keV  : 1.29706E-03    ( -0.000546091   0.000603509 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          55.79 using 59 PHA bins.
# Reduced chi-squared =         0.9787 for     57 degrees of freedom 
# Null hypothesis probability =   5.206201e-01
 
Photon flux (15-150 keV)    in 3.636 sec: 0.378363 ( -0.0688647  0.0690302 ) ph/cm2/s
Energy fluence (15-150 keV)             : 5.88588e-08 ( -1.37038e-08  1.49732e-08 ) ergs/cm2

Cutoff power-law model

Time interval is from   -0.312 sec. to    3.324 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.89773     (     )
Epeak [keV] : 2.66527      (   )
Norm@50keV  : 8.42231E-03    (     )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          55.34 using 59 PHA bins.
# Reduced chi-squared =         0.9883 for     56 degrees of freedom 
# Null hypothesis probability =   4.996999e-01
 
Photon flux (15-150 keV)    in 3.636 sec: 0.374687 ( -0.067764  0.068812 ) ph/cm2/s
Energy fluence (15-150 keV)             : 5.59322e-08 ( -1.2778e-08  1.62449e-08 ) ergs/cm2

Band function

Time interval is from   -0.312 sec. to    3.324 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -1.94143   ( -4.16157   1.91072 )
beta        : -9.37167    ( 9.37167   19.3716 )
Epeak [keV] : 1.59157      ( -1.59154 19.0538 )
Norm@50keV   : 7.83205E-03    ( -0.00324598   0.00761842 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          55.32 using 59 PHA bins.
# Reduced chi-squared =          1.006 for     55 degrees of freedom 
# Null hypothesis probability =   4.624301e-01
 
Photon flux (15-150 keV)    in 3.636 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]    : 5.32419  (-1.24209  1.50642)
R^2/D10^2   : 2.31979  (-1.54245   5.81706)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          60.84 using 59 PHA bins.
# Reduced chi-squared =          1.067 for     57 degrees of freedom 
# Null hypothesis probability =   3.395073e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  2.620e-08   1.040e-08
25- 50  1.992e-08   8.819e-09
50-150  1.088e-09   8.109e-10
15-150  4.721e-08   1.821e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 18.1797       (-6.36723      9.81793)
Norm        : 5.16312       (-2.04412     4.11706)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          55.75 using 59 PHA bins.
# Reduced chi-squared =         0.9781 for     57 degrees of freedom 
# Null hypothesis probability =   5.220847e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  2.673e-08   7.468e-09
25- 50  2.168e-08   7.414e-09
50-150  5.505e-09   4.117e-09
15-150  5.392e-08   1.533e-08

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 2.73584        (-1.22522      1.57537)
R1^2/D10^2  : 44.9997        (-42.9126      3854.03)
kT2 [keV]   : 8.77731        (-2.68764      4.92842)
R2^2/D10^2  : 0.184049    (-0.169562   0.905869)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          53.82 using 59 PHA bins.
# Reduced chi-squared =         0.9785 for     55 degrees of freedom 
# Null hypothesis probability =   5.198369e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  2.676e-08   1.366e-08
25- 50  2.199e-08   1.240e-08
50-150  7.145e-09   4.549e-09
15-150  5.590e-08   2.843e-08

Peak spectrum fit

Power-law model

Time interval is from    0.020 sec. to    1.020 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 2.58555     ( -0.549233   0.724471 )
Norm@50keV  : 2.35728E-03    ( -0.00114645   0.00116333 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          44.94 using 59 PHA bins.
# Reduced chi-squared =         0.7885 for     57 degrees of freedom 
# Null hypothesis probability =   8.763171e-01
 
Photon flux (15-150 keV)    in 1 sec: 0.488453 ( -0.129506  0.12972 ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.41564e-08 ( -8.12353e-09  8.97275e-09 ) ergs/cm2

Cutoff power-law model

Time interval is from    0.020 sec. to    1.020 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.58268     (     )
Epeak [keV] : 14.6289      (   )
Norm@50keV  : 1.04210E-02    (     )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          44.48 using 59 PHA bins.
# Reduced chi-squared =         0.7942 for     56 degrees of freedom 
# Null hypothesis probability =   8.664363e-01
 
Photon flux (15-150 keV)    in 1 sec: 0.481366 ( -0.125686  0.129327 ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.25019e-08 ( -7.2535e-09  9.7918e-09 ) ergs/cm2

Band function

Time interval is from    0.020 sec. to    1.020 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : 4.73507   ( -4.73507   -4.73507 )
beta        : -2.65610    ( -0.947952   0.597053 )
Epeak [keV] : 16.9474      ( -16.9474 6.95503 )
Norm@50keV   : 5614.79    ( -1471.58   1.58522e+07 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          44.83 using 59 PHA bins.
# Reduced chi-squared =         0.8152 for     55 degrees of freedom 
# Null hypothesis probability =   8.344338e-01
 
Photon flux (15-150 keV)    in 1 sec:  (    ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.39807e-08 ( 0  0 ) ergs/cm2

Single BB

 
Spectral model blackbody:
------------------------------------------------------------
Parameters  : value    Lower 90%  Upper 90%
kT [keV]    : 7.83341  (-2.43934  2.59377)
R^2/D10^2   : 0.591759  (-0.590678   2.12753)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          47.21 using 59 PHA bins.
# Reduced chi-squared =         0.8283 for     57 degrees of freedom 
# Null hypothesis probability =   8.189851e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  6.461e-09   3.886e-09
25- 50  1.090e-08   6.445e-09
50-150  2.669e-09   2.069e-09
15-150  2.003e-08   1.080e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 29.6096       (-13.6659      30.1785)
Norm        : 4.01575       (-1.71712     3.692)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          44.52 using 59 PHA bins.
# Reduced chi-squared =         0.7810 for     57 degrees of freedom 
# Null hypothesis probability =   8.855963e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  8.118e-09   3.465e-09
25- 50  9.209e-09   4.463e-09
50-150  4.957e-09   4.124e-09
15-150  2.228e-08   1.157e-08

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 2.73196        (-1.63703      2.41023)
R1^2/D10^2  : 45.3646        (-49.1995      127911)
kT2 [keV]   : 10.2994        (-3.05648      5.11433)
R2^2/D10^2  : 0.155911    (-0.137694   0.482413)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          42.66 using 59 PHA bins.
# Reduced chi-squared =         0.7757 for     55 degrees of freedom 
# Null hypothesis probability =   8.874211e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  8.029e-09   4.006e-09
25- 50  9.289e-09   5.595e-09
50-150  5.004e-09   3.447e-09
15-150  2.232e-08   1.148e-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: 3.08025     ( -0.462925   0.576709 )
Norm@50keV  : 1.29706E-03    ( -0.000546091   0.000603509 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          55.79 using 59 PHA bins.
# Reduced chi-squared =         0.9787 for     57 degrees of freedom 
# Null hypothesis probability =   5.206201e-01
 
Photon flux (15-150 keV)    in 3.636 sec: 0.378363 ( -0.0688647  0.0690302 ) ph/cm2/s
Energy fluence (15-150 keV)             : 5.88588e-08 ( -1.37038e-08  1.49732e-08 ) ergs/cm2

Cutoff power-law model

Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.89773     (     )
Epeak [keV] : 2.66527      (   )
Norm@50keV  : 8.42231E-03    (     )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          55.34 using 59 PHA bins.
# Reduced chi-squared =         0.9883 for     56 degrees of freedom 
# Null hypothesis probability =   4.996999e-01
 
Photon flux (15-150 keV)    in 3.636 sec: 0.374687 ( -0.067764  0.068812 ) ph/cm2/s
Energy fluence (15-150 keV)             : 5.59322e-08 ( -1.2778e-08  1.62449e-08 ) ergs/cm2

Band function

 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -1.94143   ( -2.76944   1.91072 )
beta        : -9.37167    ( 9.37167   19.3716 )
Epeak [keV] : 1.59157      ( -1.59154 19.0538 )
Norm@50keV   : 7.83205E-03    ( -0.00324598   0.00761982 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          55.32 using 59 PHA bins.
# Reduced chi-squared =          1.006 for     55 degrees of freedom 
# Null hypothesis probability =   4.624301e-01
 
Photon flux (15-150 keV)    in 3.636 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)  = 1.95e-08
S(50-100 keV) = 9.22e-09

T90 vs. Hardness ratio plot

T90                                   = 3.324000030756 sec.
Hardness ratio (energy fluence ratio) = 0.472821

Color vs. Color plot

Count Ratio  (25-50 keV) / (15-25 keV) = 0.621799
Count Ratio (50-100 keV) / (15-25 keV) = 0.0340101

Mask shadow pattern

IMX = -2.899739492053793E-01, IMY = 1.172313939840287E-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:
-137.283380 -0.312000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
170.0594 -60.6004    7.1  41.2  -36.7   0.3821   1.6    7.7	Cen X-3                       
186.6473 -62.7730    1.0  33.1  -35.4   2.0772  11.7    0.3	GX 301-2                      
244.9642 -15.6390    1.0  38.4   87.9   6.4644  11.6    0.9	Sco X-1                       
255.9613 -37.8288    0.9  16.5  112.2   1.8060  12.5    1.5	4U 1700-377                   
256.5744 -36.2533    0.0  18.1  112.7   0.3256   2.1   12.2	GX 349+2                      
263.0089 -24.8160   10.8  30.5  119.3  -0.2255  -1.1    4.2	GX 1+4                        
264.7005 -44.3055    4.6  13.4  146.7   0.3465   2.5    8.9	4U 1735-44                    
270.2276 -25.2374    6.3  32.2  131.5  -0.4133  -1.8   10.0	GX 5-1                        
270.4276 -25.7773    7.1  31.8  132.2   0.3641   1.6    7.1	GRS 1758-258                  
274.0165 -14.0467    7.9  43.9  130.4   0.9572   1.5    0.9	GX 17+2                       
275.9846 -30.4229  150.0  29.9  144.9  -0.0158  -0.1    4.6	H1820-303                     
284.9517 -25.0294    8.1  38.6  151.8  -0.3726  -1.4    8.0	HT1900.1-2455                 
263.0445 -33.8607    4.1  21.9  125.6   0.4668   2.8    3.2	GX 354-0                      
266.7964 -27.3604    1.3  29.1  127.4   1.7664   9.1 ------	UNKNOWN                       
251.5722 -45.6524    3.1   8.2  102.7   0.4900   3.7 ------	UNKNOWN                       
243.3505 -52.3279    2.3   4.4   22.9   0.6647   5.0 ------	UNKNOWN                       
341.8266 -52.6094    3.5  50.9 -135.5   3.0309   3.4 ------	UNKNOWN

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

Time interval of the image:
-0.312000 3.324000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
170.3308 -60.7754   14.8  41.0  -36.9  -0.0241  -0.8    9.2	Cen X-3                       
186.2639 -62.7482    0.0  33.3  -35.4  -0.0157  -0.6   10.9	GX 301-2                      
245.1041 -15.6964    7.5  38.3   88.1   0.1153   1.5    8.0	Sco X-1                       
255.9539 -37.6973    4.1  16.6  112.1  -0.0567  -2.8    8.9	4U 1700-377                   
256.6117 -36.3990    4.9  18.0  112.9   0.0499   2.4    8.6	GX 349+2                      
262.8124 -24.6318    0.0  30.7  118.9  -0.0088  -0.3   12.7	GX 1+4                        
264.6576 -44.5943    5.6  13.1  147.4  -0.0411  -2.1    9.4	4U 1735-44                    
270.2769 -25.1608    3.2  32.3  131.5   0.1122   3.6    4.9	GX 5-1                        
270.5152 -25.8331    2.9  31.8  132.4  -0.1171  -4.0   12.7	GRS 1758-258                  
273.9602 -14.0591  113.2  43.9  130.3   0.0078   0.1    3.0	GX 17+2                       
275.9827 -30.4947    8.3  29.8  144.9  -0.0380  -1.4    8.2	H1820-303                     
284.9502 -24.9249    5.2  38.7  151.7   0.0832   2.2    4.7	HT1900.1-2455                 
262.8503 -33.9465   10.2  21.8  125.3   0.0260   1.1    9.6	GX 354-0                      
280.1939 -54.9656    1.3  17.4 -158.0   0.1763   9.3 ------	UNKNOWN

Post-slew image of 15-350 keV band

Time interval of the image:
82.116590 962.486400
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
170.4328 -60.5498   12.2  51.8    5.6   1.5020   0.9    5.6	Cen X-3                       
186.6871 -62.7556    1.3  44.6   10.2   8.6469   9.1    1.2	GX 301-2                      
255.9918 -37.8298    1.0  23.7   96.0   8.6267  12.1    0.9	4U 1700-377                   
256.3870 -36.2578    6.6  24.8   98.8   1.3195   1.8   10.2	GX 349+2                      
263.0802 -24.7497   16.3  32.8  120.0   0.6986   0.7    3.9	GX 1+4                        
264.8270 -44.3086    6.0  14.6  100.6   0.8990   1.9    9.2	4U 1735-44                    
270.2873 -25.0989    3.6  30.8  131.9   2.8435   3.2    1.2	GX 5-1                        
270.3414 -25.7095    3.7  30.2  131.7   2.7124   3.1    2.9	GRS 1758-258                  
274.1148 -14.1121    3.9  41.2  140.6   4.7550   3.0    7.8	GX 17+2                       
275.9306 -30.3142    3.4  24.9  140.8   2.3664   3.4    3.2	H1820-303                     
284.9678 -24.8675    4.6  30.4  158.2   2.0271   2.5    4.9	HT1900.1-2455                 
262.9393 -33.9133    4.4  24.3  112.8   1.8746   2.6    5.3	GX 354-0                      
266.8442 -27.3440    0.7  29.3  124.8  12.5741  15.9 ------	UNKNOWN                       
243.1221 -52.4431    1.7  21.8   50.9   3.8602   6.6 ------	UNKNOWN                       
104.8595 -68.6684    5.5  56.3  -28.4   8.2311   2.1 ------	UNKNOWN                       
335.1282 -23.6205    4.1  50.9 -135.5  14.0825   2.8 ------	UNKNOWN

Plot creation:
Sun May 31 07:32:50 EDT 2015