batgrbproduct analysis for trigger=132247

batgrbproduct Analysis for Trigger=132247

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): Wed Jan 22 21:50:38 EST 2014
             Host Name: batevent1
   Current Working Dir: /local/data/batevent/batevent_reproc/trigger132247
======================================================================

  Trigger: 00132247      Segment: 000

  BAT Trigger Time: 139828282.368   [s; MET]
      Trigger Stop: 139828283.392   [s; MET]
               UTC: 2005-06-07T09:11:22.807560    [includes UTCF correction] 
       Where From?: TDRSS position message

  BAT 
    RA: 300.166992902482   Dec: 9.13699352299647  [deg; J2000]

     Catalogged Source?: NO
     Point Source?:      YES
     GRB Indicated?:     YES    [ by BAT flight software ]
     Image S/N Ratio:    9
     Image Trigger?:     NO
     Rate S/N Ratio:     18.1383571472171  [ if not an image trigger ]
     Image S/N Ratio:    9

  Flight Position:   [ source = BAT ]
    RA: 300.166992902482   Dec: 9.13699352299647  [deg; J2000]

  Ground Position:   [ source = BAT pre-slew burst ]
    RA: 300.180869821667   Dec: 9.13111981264177  [deg; J2000]  
        { 20h 00m 43.4s , +09d 07' 52.0" }
         +/- 1.51118549977616 [arcmin] (estimated 90% radius based on SNR)
         +/- 0.543115261093875 [arcmin] (formal 1-sigma fit error)
    SNR: 16.8635935437948
 
  Angular difference between Flight and Ground position is 0.894416 arcmin
 
  Partial Coding Fraction: 0.8359375    [ including projection effects ]

  Duration
     T90: 48 +/- 22.6274169979695
        Measured from: -11.3680000007153
                   to: 36.6319999992847     [s; relative to TRIGTIME]
     T50: 16 +/- 16
        Measured from: -11.3680000007153
                   to: 4.63199999928474     [s; relative to TRIGTIME]



  Fluence
     Peak Flux  (peak 1 second)
        Measured from: 12.1319999992847     
                   to: 13.1319999992847     [s; relative to TRIGTIME]
     Total Fluence        
        Measured from: -11.3680000007153     
                   to: 36.6319999992847     [s; relative to TRIGTIME]
     
             Band 1     Band 2     Band 3     Band 4
              15-25      25-50     50-100    100-350     keV
 Total     0.387469   0.457089   0.218004   0.061574
           0.035640   0.036169   0.030520   0.024851 [error]
 Peak      0.018113   0.005771   0.005803   0.000973
           0.005439   0.005379   0.004450   0.003626 [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 1.26e-07 1.79e-07 1.90e-07 3.72e-07 6.11e-07 8.67e-07   erg/cm2
              Error 1.76e-08 1.68e-08 2.97e-08 1.17e-07 6.82e-08 1.47e-07   erg/cm2
Peak flux Power-law 1.24e-01 8.71e-02 4.04e-02 2.62e-02 2.64e-01 2.78e-01   ph/cm2/s
              Error 7.79e-02 4.42e-02 3.41e-02 4.73e-02 1.27e-01 1.36e-01   ph/cm2/s
 
Fluence   Cutoff-PL 1.24e-07 1.82e-07 1.90e-07 2.96e-07 6.03e-07 7.91e-07   erg/cm2
              Error 1.92e-08 2.15e-08 3.06e-08 1.96e-07 7.87e-08 2.26e-07   erg/cm2
Peak flux Cutoff-PL 1.20e-01 9.31e-02 3.97e-02 1.25e-02 2.61e-01 2.65e-01   ph/cm2/s
              Error 1.02e-01 5.63e-02 3.98e-02 3.57e-02 1.28e-01 1.39e-01   ph/cm2/s
 
Fluence        Band -------- -------- -------- -------- -------- --------   erg/cm2
              Error -------- -------- -------- -------- -------- --------   erg/cm2
Peak flux      Band -------- -------- -------- -------- -------- --------   ph/cm2/s
              Error -------- -------- -------- -------- -------- --------   ph/cm2/s

 
=== Time-averaged spectral analysis ===
 
Model Ph_index Ph_90err Epeak  Epeak_90err Norm     Nomr_90err chi2   dof
PL    1.916    0.178    -      -           1.38e-03 1.57e-04   66.170 57
CPL   1.797    0.655      73.4   -1.2      1.62e-03 2.06e-03   66.090 56
 
 
=== 1-s peak spectral analysis ===
 
Model Ph_index Ph_90err Epeak  Epeak_90err Norm     Nomr_90err chi2   dof
PL    2.110    1.083    -      -           1.67e-03 1.37e-03   55.990 57
CPL   1.595    0.000      31.5    0.0      3.40e-03 0.00e+00   55.950 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: 2.624000 sec.
T50 in the 50-300 keV band: 1.600000 sec.

 
=== Table of the duration information ==
 
        Value   tstart    tstop
T100   48.000  -11.368   36.632
T90    48.000  -11.368   36.632
T50    16.000  -11.368    4.632
Peak    1.000   12.132   13.132

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
  300.1809     9.1311   0.0114    27.0509     3.0420         0.9011650     16.864 TRIG_00132247                 
 
Foreground time interval of the image:
-11.368  16.533 (delta_t =  27.901 [sec])
Background time interval of the image:
-101.867 -11.368 (delta_t =  90.499 [sec])

Lightcurves

Notes:

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

1 s binning

From T0-310 s to T0+310 s

From T100_start - 20 s to T100_end + 30 s

Full time interval

64 ms binning

Full time interval

From T100_start to T100_end

From T0-5 sec to T0+5 sec

16 ms binning

From T100_start-5 s to T100_start+5 s

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

8 ms binning

From T100_start-3 s to T100_start+3 s

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

2 ms binning

From T100_start-1 s to T100_start+1 s

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

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

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

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

Spectral Evolution

Spectra

Notes:

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

Time averaged spectrum fit using the average DRM

Power-law model

Time interval is from  -11.368 sec. to   36.632 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.91624     ( -0.174385   0.181448 )
Norm@50keV  : 1.38378E-03    ( -0.000158554   0.000155186 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          66.17 using 59 PHA bins.
# Reduced chi-squared =          1.161 for     57 degrees of freedom 
# Null hypothesis probability =   1.898920e-01
 
Photon flux (15-150 keV)    in 48 sec: 0.199969 ( -0.0189675  0.0189776 ) ph/cm2/s
Energy fluence (15-150 keV)             : 6.10776e-07 ( -6.76886e-08  6.87254e-08 ) ergs/cm2

Cutoff power-law model

Time interval is from  -11.368 sec. to   36.632 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.79684     ( -0.836389   0.474352 )
Epeak [keV] : 73.3808      ( -71.2407 -73.5825 )
Norm@50keV  : 1.61792E-03    ( -0.000917926   0.00320143 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          66.09 using 59 PHA bins.
# Reduced chi-squared =          1.180 for     56 degrees of freedom 
# Null hypothesis probability =   1.675848e-01
 
Photon flux (15-150 keV)    in 48 sec: 0.198981 ( -0.019873  0.019585 ) ph/cm2/s
Energy fluence (15-150 keV)             : 6.03288e-07 ( -8.25888e-08  7.48512e-08 ) ergs/cm2

Band function

Time interval is from  -11.368 sec. to   36.632 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -1.31080   ( 1.32136   5.86321 )
beta        : -2.11865    ( 2.11254   0.344538 )
Epeak [keV] : 42.4545      ( -42.7524 94.583 )
Norm@50keV   : 3.23656E-03    ( -0.00191024   334.159 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          65.41 using 59 PHA bins.
# Reduced chi-squared =          1.189 for     55 degrees of freedom 
# Null hypothesis probability =   1.589377e-01
 
Photon flux (15-150 keV)    in 48 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]    : 10.3688  (-1.087  1.22737)
R^2/D10^2   : 8.08055E-02  (-0.0281651   0.0426241)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          88.82 using 59 PHA bins.
# Reduced chi-squared =          1.558 for     57 degrees of freedom 
# Null hypothesis probability =   4.441037e-03
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  8.590e-08   1.526e-08
25- 50  2.246e-07   2.791e-08
50-150  1.300e-07   3.079e-08
15-150  4.405e-07   5.016e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 78.2990       (-21.5567      37.0318)
Norm        : 0.941100       (-0.133279     0.164264)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          67.09 using 59 PHA bins.
# Reduced chi-squared =          1.177 for     57 degrees of freedom 
# Null hypothesis probability =   1.695766e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.170e-07   1.642e-08
25- 50  1.917e-07   1.901e-08
50-150  2.667e-07   1.084e-07
15-150  5.754e-07   1.042e-07

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 8.30102        (-1.94206      1.45844)
R1^2/D10^2  : 0.164742        (-0.069905      0.0835894)
kT2 [keV]   : 53.8096        (-35.5748      -57.5656)
R2^2/D10^2  : 1.76696E-04    (-0.000135296   0.00289701)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          67.80 using 59 PHA bins.
# Reduced chi-squared =          1.233 for     55 degrees of freedom 
# Null hypothesis probability =   1.151861e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.037e-07   2.198e-08
25- 50  2.071e-07   4.793e-08
50-150  2.992e-07   1.544e-07
15-150  6.099e-07   2.095e-07

Peak spectrum fit

Power-law model

Time interval is from   12.132 sec. to   13.132 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 2.11048     ( -0.885201   1.28118 )
Norm@50keV  : 1.66970E-03    ( -0.0016697   0.00107546 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          55.99 using 59 PHA bins.
# Reduced chi-squared =         0.9823 for     57 degrees of freedom 
# Null hypothesis probability =   5.128489e-01
 
Photon flux (15-150 keV)    in 1 sec: 0.264053 ( -0.127087  0.127104 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.55293e-08 ( -8.86162e-09  9.88093e-09 ) ergs/cm2

Cutoff power-law model

Time interval is from   12.132 sec. to   13.132 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.59478     (     )
Epeak [keV] : 31.5476      (   )
Norm@50keV  : 3.40076E-03    (     )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          55.95 using 59 PHA bins.
# Reduced chi-squared =         0.9990 for     56 degrees of freedom 
# Null hypothesis probability =   4.769273e-01
 
Photon flux (15-150 keV)    in 1 sec: 0.261065 ( -0.127829  0.128491 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.48213e-08 ( -8.50709e-09  1.04274e-08 ) ergs/cm2

Band function

Time interval is from   12.132 sec. to   13.132 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -8.29251   ( 9.39159   8.29251 )
beta        : -2.11049    ( -1.28101   0.885305 )
Epeak [keV] : 67.8306      ( -67.8306 -67.8306 )
Norm@50keV   : 0.226934    ( -0.226934   0.146171 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          55.99 using 59 PHA bins.
# Reduced chi-squared =          1.018 for     55 degrees of freedom 
# Null hypothesis probability =   4.373395e-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]    : 10.8753  (-6.87018  7.81105)
R^2/D10^2   : 9.08874E-02  (-0.0907784   4.91034)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          57.09 using 59 PHA bins.
# Reduced chi-squared =          1.002 for     57 degrees of freedom 
# Null hypothesis probability =   4.718930e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  2.241e-09   1.523e-09
25- 50  6.243e-09   4.091e-09
50-150  4.134e-09   3.520e-09
15-150  1.262e-08   8.645e-09

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 55.1927       (-55.1927      -55.1927)
Norm        : 1.45141       (-0.839302     2.84378)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          55.96 using 59 PHA bins.
# Reduced chi-squared =         0.9818 for     57 degrees of freedom 
# Null hypothesis probability =   5.140493e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  3.594e-09   2.316e-09
25- 50  5.326e-09   3.486e-09
50-150  5.643e-09   4.961e-09
15-150  1.456e-08   1.101e-08

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 3.58764        (-3.56365      10.8887)
R1^2/D10^2  : 5.32759        (-5.42146      -5.42146)
kT2 [keV]   : 14.3089        (-6.475      -14.275)
R2^2/D10^2  : 2.55481E-02    (-0.0257818   0.369608)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          55.20 using 59 PHA bins.
# Reduced chi-squared =          1.004 for     55 degrees of freedom 
# Null hypothesis probability =   4.671400e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  3.891e-09   2.448e-09
25- 50  4.919e-09   3.072e-09
50-150  5.714e-09   5.265e-09
15-150  1.452e-08   8.345e-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: 1.82800     ( -0.178746   0.185223 )
Norm@50keV  : 1.83008E-03    ( -0.000208311   0.000204123 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          68.22 using 59 PHA bins.
# Reduced chi-squared =          1.197 for     57 degrees of freedom 
# Null hypothesis probability =   1.467873e-01
 
Photon flux (15-150 keV)    in 27.9 sec: 0.254971 ( -0.0251477  0.0251732 ) ph/cm2/s
Energy fluence (15-150 keV)             : 4.69669e-07 ( -5.34793e-08  5.42189e-08 ) ergs/cm2

Cutoff power-law model

Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.76258     ( -0.79306   0.777889 )
Epeak [keV] : 162.818      (   )
Norm@50keV  : 1.98883E-03    (     )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          68.20 using 59 PHA bins.
# Reduced chi-squared =          1.218 for     56 degrees of freedom 
# Null hypothesis probability =   1.271636e-01
 
Photon flux (15-150 keV)    in 27.9 sec: 0.254263 ( -0.026208  0.025608 ) ph/cm2/s
Energy fluence (15-150 keV)             : 4.66979e-07 ( -6.24569e-08  5.63301e-08 ) ergs/cm2

Band function

 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -1.40193   ( 1.41499   1.41499 )
beta        : -1.97897    ( 1.97156   0.312153 )
Epeak [keV] : 55.0762      ( -57.1918 -57.1918 )
Norm@50keV   : 3.26598E-03    ( -0.00155626   0 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          67.92 using 59 PHA bins.
# Reduced chi-squared =          1.235 for     55 degrees of freedom 
# Null hypothesis probability =   1.132719e-01
 
Photon flux (15-150 keV)    in 27.9 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)  = 1.79e-07
S(50-100 keV) = 1.90e-07

T90 vs. Hardness ratio plot

T90                                   = 48 sec.
Hardness ratio (energy fluence ratio) = 1.06145

Color vs. Color plot

Count Ratio  (25-50 keV) / (15-25 keV) = 1.17968
Count Ratio (50-100 keV) / (15-25 keV) = 0.562636

Mask shadow pattern

IMX = 5.099258376762459E-01, IMY = -2.709861638310307E-02

TIME vs. PHA plot around the trigger time

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

TIME vs. DetID plot around the trigger time

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

100 us light curve (15-350 keV)

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

Spacecraft aspect plot

Bright source in the pre-burst/pre-slew/post-slew images

Pre-burst image of 15-350 keV band

Time interval of the image:
-101.867410 -11.368000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
254.3745  35.3822    4.7  22.2  177.4   0.2167   2.4    4.7	Her X-1                       
268.1795  -1.5187   14.1  29.4   78.2   0.1279   0.8   12.0	SW J1753.5-0127               
273.8709 -14.1304   36.7  40.7   64.0  -0.1089  -0.3    9.7	GX 17+2                       
288.6952  10.8412    3.4  18.4   22.9   0.3043   3.3    8.7	GRS 1915+105                  
299.5895  35.1941    0.4  20.4  -63.3   3.0103  30.7    0.5	Cyg X-1                       
308.0900  40.9411    2.1  28.7  -70.6   0.6806   5.6    1.1	Cyg X-3                       
326.2431  38.4584    5.6  41.9  -61.6  -0.5794  -2.1    8.9	Cyg X-2                       
298.0005   6.6955    1.8  27.3   10.2   0.6183   6.3 ------	UNKNOWN                       
232.5064  37.2358    2.1  39.9  175.1   0.6850   5.5 ------	UNKNOWN                       
335.9641  21.0621    2.3  52.8  -39.7   2.1708   5.0 ------	UNKNOWN

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

Time interval of the image:
-11.368000 16.532600
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
254.2555  35.3275    9.1  22.3  177.2  -0.0638  -1.3    9.9	Her X-1                       
268.4070  -1.5447    6.5  29.4   77.7  -0.1573  -1.8    6.0	SW J1753.5-0127               
274.0983 -13.9375   15.5  40.4   63.7   0.1548   0.7    8.0	GX 17+2                       
288.5981  10.9071    5.1  18.3   23.0  -0.1139  -2.2   12.0	GRS 1915+105                  
299.7356  35.1206    4.9  20.5  -63.0   0.1302   2.3    8.6	Cyg X-1                       
307.9088  40.9060    5.8  28.6  -70.6  -0.1465  -2.0    9.5	Cyg X-3                       
326.1398  38.1467    7.6  41.8  -61.1   0.2249   1.5   10.6	Cyg X-2                       
300.1802   9.1309    0.7  27.1    3.0   0.9000  16.8 ------	UNKNOWN                       
209.1542  40.1198    2.5  57.9 -179.8   1.4591   4.6 ------	UNKNOWN

Post-slew image of 15-350 keV band

Time interval of the image:
66.132590 302.714300
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
254.4103  35.2776    5.0  49.2  166.3   1.0990   2.3    4.5	Her X-1                       
268.3893  -1.6074   21.9  33.4  109.8  -0.1729  -0.5    9.4	SW J1753.5-0127               
274.0025 -13.9993    3.5  34.8   85.6   1.2454   3.3    2.2	GX 17+2                       
285.0072 -24.8838    6.4  37.1   60.1  -0.7245  -1.8    2.7	HT1900.1-2455                 
288.8742  11.0267    3.9  11.3  137.7   0.4316   2.9    6.6	GRS 1915+105                  
299.5915  35.2045    0.2  26.1 -144.1   8.1105  49.1    0.2	Cyg X-1                       
308.1168  40.9738    1.4  32.6 -131.9   1.7669   8.5    1.3	Cyg X-3                       
326.1576  38.4492   15.6  37.5 -108.7   0.3040   0.7    7.7	Cyg X-2

Plot creation:
Sun May 31 16:41:44 EDT 2015