batgrbproduct analysis for trigger=540255

batgrbproduct Analysis for Trigger=540255

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 22:56:07 EST 2014
             Host Name: batevent1
   Current Working Dir: /local/data/batevent/batevent_reproc/trigger540255
======================================================================

  Trigger: 00540255      Segment: 000

  BAT Trigger Time: 376114814.976   [s; MET]
      Trigger Stop: 376114816   [s; MET]
               UTC: 2012-12-02T04:20:05.038260    [includes UTCF correction] 
       Where From?: TDRSS position message

  BAT 
    RA: 256.81487469703   Dec: 23.9520792363031  [deg; J2000]

     Catalogged Source?: NO
     Point Source?:      YES
     GRB Indicated?:     YES    [ by BAT flight software ]
     Image S/N Ratio:    7.49
     Image Trigger?:     NO
     Rate S/N Ratio:     13.7840487520902  [ if not an image trigger ]
     Image S/N Ratio:    7.49

  Flight Position:   [ source = BAT ]
    RA: 256.81487469703   Dec: 23.9520792363031  [deg; J2000]

  Ground Position:   [ source = BAT pre-slew burst ]
    RA: 256.795738457097   Dec: 23.9449641866872  [deg; J2000]  
        { 17h 07m 11.0s , +23d 56' 41.9" }
         +/- 1.09715379311727 [arcmin] (estimated 90% radius based on SNR)
         +/- 0.40248048221767 [arcmin] (formal 1-sigma fit error)
    SNR: 26.643628360915
 
  Angular difference between Flight and Ground position is 1.132845 arcmin
 
  Partial Coding Fraction: 0.703125    [ including projection effects ]

  Duration
     T90: 19.5359999537468 +/- 1.49226541307976
        Measured from: -1.33600002527237
                   to: 18.1999999284744     [s; relative to TRIGTIME]
     T50: 10.1599999666214 +/- 1.31444893960463
        Measured from: 2.96399998664856
                   to: 13.12399995327     [s; relative to TRIGTIME]



  Fluence
     Peak Flux  (peak 1 second)
        Measured from: -0.0160000324249268     
                   to: 0.983999967575073     [s; relative to TRIGTIME]
     Total Fluence        
        Measured from: -2.18400001525879     
                   to: 19.0080000162125     [s; relative to TRIGTIME]
     
             Band 1     Band 2     Band 3     Band 4
              15-25      25-50     50-100    100-350     keV
 Total     0.493030   0.696439   0.476748   0.089506
           0.035695   0.036567   0.032498   0.028303 [error]
 Peak      0.042170   0.056458   0.035999   0.007827
           0.008103   0.008258   0.007567   0.006145 [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 1.68e-07 2.92e-07 3.86e-07 1.04e-06 1.13e-06 1.89e-06   erg/cm2
              Error 1.72e-08 1.85e-08 3.20e-08 1.82e-07 7.69e-08 2.08e-07   erg/cm2
Peak flux Power-law 4.64e-01 4.10e-01 2.49e-01 2.28e-01 1.22e+00 1.35e+00   ph/cm2/s
              Error 1.19e-01 6.99e-02 6.02e-02 1.07e-01 2.07e-01 2.32e-01   ph/cm2/s
 
Fluence   Cutoff-PL 1.52e-07 3.14e-07 3.96e-07 3.93e-07 1.06e-06 1.25e-06   erg/cm2
              Error 2.03e-08 2.37e-08 3.54e-08 2.51e-07 8.77e-08 2.63e-07   erg/cm2
Peak flux Cutoff-PL 4.11e-01 4.54e-01 2.56e-01 8.04e-02 1.18e+00 1.20e+00   ph/cm2/s
              Error 1.37e-01 9.21e-02 7.10e-02 1.45e-01 1.60e-01 2.53e-01   ph/cm2/s
 
Fluence        Band 1.45e-07 3.22e-07 3.79e-07 6.94e-07 1.07e-06 1.54e-06   erg/cm2
              Error 2.17e-08 2.70e-08 -------- -------- 8.44e-08 --------   erg/cm2
Peak flux      Band 4.12e-01 4.53e-01 2.57e-01 8.36e-02 1.18e+00 1.21e+00   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    1.596    0.106    -      -           5.69e-03 3.60e-04   48.920 57
CPL   0.904    0.489      76.0   34.9      1.30e-02 8.19e-03   41.930 56
 
 
=== 1-s peak spectral analysis ===
 
Model Ph_index Ph_90err Epeak  Epeak_90err Norm     Nomr_90err chi2   dof
PL    1.721    0.292    -      -           9.11e-03 1.72e-03   51.060 57
CPL   0.780    1.346      58.5  -22.1      2.98e-02 1.13e-01   49.200 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: 21.056000 sec.
T50 in the 50-300 keV band: 9.536000 sec.

 
=== Table of the duration information ==
 
        Value   tstart    tstop
T100   21.192   -2.184   19.008
T90    19.536   -1.336   18.200
T50    10.160    2.964   13.124
Peak    1.000   -0.016    0.984

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
  256.7957    23.9450   0.0073    33.4596   -26.3777         1.9366919     26.644 TRIG_00540255                 
 
Foreground time interval of the image:
 -2.184  19.008 (delta_t =  21.192 [sec])
Background time interval of the image:
-239.976  -2.184 (delta_t = 237.792 [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

8 ms binning

From T100_start-3 s to T100_start+3 s

2 ms binning

From T100_start-1 s to T100_start+1 s

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   -2.184 sec. to   19.008 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.59637     ( -0.105843   0.106687 )
Norm@50keV  : 5.68865E-03    ( -0.000361193   0.000359741 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          48.92 using 59 PHA bins.
# Reduced chi-squared =         0.8583 for     57 degrees of freedom 
# Null hypothesis probability =   7.679357e-01
 
Photon flux (15-150 keV)    in 21.19 sec: 0.730196 ( -0.0457047  0.0457704 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.12783e-06 ( -7.66315e-08  7.71187e-08 ) ergs/cm2

Cutoff power-law model

Time interval is from   -2.184 sec. to   19.008 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 0.903736     ( -0.519037   0.459164 )
Epeak [keV] : 75.9935      ( -15.0018 54.7253 )
Norm@50keV  : 1.30250E-02    ( -0.00541015   0.0109672 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          41.93 using 59 PHA bins.
# Reduced chi-squared =         0.7488 for     56 degrees of freedom 
# Null hypothesis probability =   9.186046e-01
 
Photon flux (15-150 keV)    in 21.19 sec: 0.706600 ( -0.04833  0.048268 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.06406e-06 ( -8.74596e-08  8.78749e-08 ) ergs/cm2

Band function

Time interval is from   -2.184 sec. to   19.008 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -0.507585   ( -0.763219   4.8546 )
beta        : -1.99753    ( 1.99231   0.30426 )
Epeak [keV] : 58.4232      ( -28.7839 42.4976 )
Norm@50keV   : 2.28644E-02    ( -0.0258144   104.179 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          40.38 using 59 PHA bins.
# Reduced chi-squared =         0.7341 for     55 degrees of freedom 
# Null hypothesis probability =   9.300507e-01
 
Photon flux (15-150 keV)    in 21.19 sec:  (    ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.07288e-06 ( -1.07273e-06  -8.47219e-08 ) ergs/cm2

Single BB

 
Spectral model blackbody:
------------------------------------------------------------
Parameters  : value    Lower 90%  Upper 90%
kT [keV]    : 13.6482  (-0.969634  1.05783)
R^2/D10^2   : 0.113892  (-0.0270749   0.0350054)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          79.92 using 59 PHA bins.
# Reduced chi-squared =          1.402 for     57 degrees of freedom 
# Null hypothesis probability =   2.429099e-02
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  9.516e-08   1.124e-08
25- 50  3.449e-07   2.649e-08
50-150  4.175e-07   5.255e-08
15-150  8.576e-07   6.304e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 165.511       (-42.7881      -165.624)
Norm        : 3.00600       (-0.203879     0.225703)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          43.49 using 59 PHA bins.
# Reduced chi-squared =         0.7631 for     57 degrees of freedom 
# Null hypothesis probability =   9.061757e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.621e-07   1.418e-08
25- 50  3.046e-07   4.577e-08
50-150  6.253e-07   2.671e-07
15-150  1.092e-06   2.613e-07

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 8.37516        (-2.14658      2.01545)
R1^2/D10^2  : 0.436576        (-0.196262      0.59328)
kT2 [keV]   : 27.0008        (-7.53508      21.9793)
R2^2/D10^2  : 6.63439E-03    (-0.00565694   0.0180714)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          42.57 using 59 PHA bins.
# Reduced chi-squared =         0.7741 for     55 degrees of freedom 
# Null hypothesis probability =   8.893635e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.382e-07   3.034e-08
25- 50  3.298e-07   7.064e-08
50-150  6.052e-07   2.675e-07
15-150  1.073e-06   3.160e-07

Peak spectrum fit

Power-law model

Time interval is from   -0.016 sec. to    0.984 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.72098     ( -0.283661   0.299794 )
Norm@50keV  : 9.11056E-03    ( -0.00173943   0.00169979 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          51.06 using 59 PHA bins.
# Reduced chi-squared =         0.8958 for     57 degrees of freedom 
# Null hypothesis probability =   6.963907e-01
 
Photon flux (15-150 keV)    in 1 sec: 1.21899 ( -0.207208  0.207366 ) ph/cm2/s
Energy fluence (15-150 keV)             : 8.42216e-08 ( -1.64495e-08  1.68548e-08 ) ergs/cm2

Cutoff power-law model

Time interval is from   -0.016 sec. to    0.984 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 0.780148     ( -1.59207   1.10045 )
Epeak [keV] : 58.5394      ( -14.3728 -58.5396 )
Norm@50keV  : 2.98130E-02    ( -0.0298125   0.195314 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          49.20 using 59 PHA bins.
# Reduced chi-squared =         0.8786 for     56 degrees of freedom 
# Null hypothesis probability =   7.278901e-01
 
Photon flux (15-150 keV)    in 1 sec: 1.17957 ( -0.10714  0.2133 ) ph/cm2/s
Energy fluence (15-150 keV)             : 7.79025e-08 ( -1.76108e-08  1.86422e-08 ) ergs/cm2

Band function

Time interval is from   -0.016 sec. to    0.984 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : 3.81208   ( -0.959213   1.17496 )
beta        : -1.96325    ( 9.37016   19.3702 )
Epeak [keV] : 28.0712      ( -18.953 577.612 )
Norm@50keV   : 88.3631    ( -88.4213   202.108 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          49.00 using 59 PHA bins.
# Reduced chi-squared =         0.8909 for     55 degrees of freedom 
# Null hypothesis probability =   7.019627e-01
 
Photon flux (15-150 keV)    in 1 sec: 1.18150 (    ) ph/cm2/s
Energy fluence (15-150 keV)             : 7.79251e-08 ( 0  0 ) ergs/cm2

Single BB

 
Spectral model blackbody:
------------------------------------------------------------
Parameters  : value    Lower 90%  Upper 90%
kT [keV]    : 12.2075  (-2.28676  2.83735)
R^2/D10^2   : 0.284124  (-0.151926   0.322582)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          54.14 using 59 PHA bins.
# Reduced chi-squared =         0.9498 for     57 degrees of freedom 
# Null hypothesis probability =   5.830195e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  8.966e-09   2.922e-09
25- 50  2.879e-08   7.960e-09
50-150  2.609e-08   1.071e-08
15-150  6.384e-08   1.652e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 116.381       (-53.0595      -114.993)
Norm        : 5.25033       (-0.989941     1.41992)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          49.65 using 59 PHA bins.
# Reduced chi-squared =         0.8711 for     57 degrees of freedom 
# Null hypothesis probability =   7.443688e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.369e-08   5.403e-09
25- 50  2.436e-08   1.357e-08
50-150  4.282e-08   2.956e-08
15-150  8.087e-08   4.776e-08

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 5.87103        (-2.98808      67.512)
R1^2/D10^2  : 2.22233        (-1.8628      35.273)
kT2 [keV]   : 18.1898        (-5.72597      55.1905)
R2^2/D10^2  : 5.10720E-02    (-0.0504688   0.188289)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          48.88 using 59 PHA bins.
# Reduced chi-squared =         0.8888 for     55 degrees of freedom 
# Null hypothesis probability =   7.060822e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.323e-08   7.885e-09
25- 50  2.509e-08   1.286e-08
50-150  3.863e-08   2.262e-08
15-150  7.695e-08   4.035e-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: 1.59637     ( -0.105843   0.106687 )
Norm@50keV  : 5.68865E-03    ( -0.000361193   0.000359741 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          48.92 using 59 PHA bins.
# Reduced chi-squared =         0.8583 for     57 degrees of freedom 
# Null hypothesis probability =   7.679357e-01
 
Photon flux (15-150 keV)    in 21.19 sec: 0.730196 ( -0.0457047  0.0457704 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.12783e-06 ( -7.66315e-08  7.71187e-08 ) ergs/cm2

Cutoff power-law model

Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 0.903736     ( -0.519037   0.459164 )
Epeak [keV] : 75.9935      ( -15.0018 54.7253 )
Norm@50keV  : 1.30250E-02    ( -0.00541015   0.0109672 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          41.93 using 59 PHA bins.
# Reduced chi-squared =         0.7488 for     56 degrees of freedom 
# Null hypothesis probability =   9.186046e-01
 
Photon flux (15-150 keV)    in 21.19 sec: 0.706600 ( -0.04833  0.048268 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.06406e-06 ( -8.74596e-08  8.78749e-08 ) ergs/cm2

Band function

 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -0.507585   ( -0.763219   4.8546 )
beta        : -1.99753    ( 1.99231   0.30426 )
Epeak [keV] : 58.4232      ( -28.7839 42.4976 )
Norm@50keV   : 2.28644E-02    ( -0.0258144   105.418 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          40.38 using 59 PHA bins.
# Reduced chi-squared =         0.7341 for     55 degrees of freedom 
# Null hypothesis probability =   9.300507e-01
 
Photon flux (15-150 keV)    in 21.19 sec:  (    ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.07288e-06 ( -1.07273e-06  -8.47219e-08 ) ergs/cm2

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

S(25-50 keV)  = 2.92e-07
S(50-100 keV) = 3.86e-07

T90 vs. Hardness ratio plot

T90                                   = 19.5359999537468 sec.
Hardness ratio (energy fluence ratio) = 1.32192

Color vs. Color plot

Count Ratio  (25-50 keV) / (15-25 keV) = 1.41257
Count Ratio (50-100 keV) / (15-25 keV) = 0.966976

Mask shadow pattern

IMX = 5.920643393936137E-01, IMY = 2.936165033805292E-01

TIME vs. PHA plot around the trigger time

TIME vs. DetID plot around the trigger time

100 us light curve (15-350 keV)

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:
-239.976000 -2.184000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
254.4080  35.3244    2.3  40.7  -11.3   1.4325   4.9    2.7	Her X-1                       
263.0475 -24.7270    4.8  41.0 -112.3   1.7881   2.5    2.4	GX 1+4                        
268.4151  -1.3110    2.8  21.6  -83.6   1.0060   4.2    9.0	SW J1753.5-0127               
270.3478 -25.1413    3.9  37.6 -121.3   1.0884   3.0    5.1	GX 5-1                        
270.1528 -25.6617    9.5  38.2 -121.5  -0.4704  -1.2    9.5	GRS 1758-258                  
274.0789 -14.0757    3.5  26.3 -116.4   0.9047   3.3    4.9	GX 17+2                       
276.0487 -30.2940   52.2  40.3 -132.0  -0.0921  -0.2    7.8	H1820-303                     
285.1846 -24.8758    4.2  33.4 -143.4  -0.7281  -2.8    8.5	HT1900.1-2455                 
288.8083  10.9563    1.0   2.7   53.5   2.2776  11.1    0.9	GRS 1915+105                  
299.6169  35.0596   10.9  28.8   52.6  -0.3275  -1.0    8.6	Cyg X-1                       
308.2068  40.9625    3.5  37.2   58.0   1.7899   3.3    4.4	Cyg X-3                       
259.6815  55.6429    2.3  52.2   12.6   3.8313   5.0 ------	UNKNOWN                       
265.5120  31.3636    2.5  30.9   -6.8   1.1180   4.6 ------	UNKNOWN

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

Time interval of the image:
-2.184000 19.008000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
254.3988  35.3151    2.4  40.7  -11.3  -0.4059  -4.8    3.3	Her X-1                       
262.8466 -24.6774   10.3  41.1 -112.0  -0.2119  -1.1    9.8	GX 1+4                        
268.1676  -1.4194    0.0  21.9  -83.5   0.0727   1.1   12.2	SW J1753.5-0127               
270.2808 -25.0838   76.7  37.6 -121.2   0.0163   0.2    0.3	GX 5-1                        
270.3016 -25.7431   22.9  38.2 -121.7  -0.0573  -0.5    0.0	GRS 1758-258                  
273.7932 -13.9934    0.0  26.4 -115.8   0.1839   2.6   12.6	GX 17+2                       
275.9953 -30.2248    3.4  40.3 -131.9  -0.3558  -3.4    9.3	H1820-303                     
285.1251 -25.0383   25.2  33.6 -143.3  -0.0360  -0.5    8.6	HT1900.1-2455                 
288.7321  11.0085   35.1   2.8   51.6  -0.0184  -0.3    5.4	GRS 1915+105                  
299.6338  35.3689    5.1  29.1   52.4   0.1840   2.3   10.3	Cyg X-1                       
308.2159  41.0736    7.4  37.3   58.0  -0.2256  -1.6    8.7	Cyg X-3                       
256.7965  23.9454    0.4  33.5  -26.4   1.9431  26.7 ------	UNKNOWN

Post-slew image of 15-350 keV band

Time interval of the image:
274.724600 706.124660
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
135.5270 -40.5599    1.1  39.3 -175.9   5.0375  10.3    0.3	Vela X-1                      
170.2584 -60.6234    3.1  34.5 -126.9   2.0408   3.7    1.7	Cen X-3                       
186.6576 -62.7596    2.4  37.4 -114.1   3.8598   4.7    0.6	GX 301-2                      
 93.4448 -47.9333    2.8  21.9  131.2   1.7461   4.2 ------	UNKNOWN                       
 11.9277 -50.6704    2.7  37.4   14.9   1.9882   4.2 ------	UNKNOWN                       
152.4143 -58.2977    0.4  30.4 -142.6  11.8023  30.2 ------	UNKNOWN                       
327.2431 -44.5140    3.0  57.1  -17.3   5.4795   3.8 ------	UNKNOWN

Plot creation:
Sat May 30 17:46:28 EDT 2015