batgrbproduct analysis for trigger=451757

batgrbproduct Analysis for Trigger=451757

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 13 22:54:14 EST 2014
             Host Name: batevent1
   Current Working Dir: /local/data/batevent/batevent_reproc/trigger451757
======================================================================

  Trigger: 00451757      Segment: 000

  BAT Trigger Time: 324990150.912   [s; MET]
      Trigger Stop: 324990151.936   [s; MET]
               UTC: 2011-04-20T11:02:24.037860    [includes UTCF correction] 
       Where From?: TDRSS position message

  BAT 
    RA: 2.16510709260475   Dec: -37.8550292612526  [deg; J2000]

     Catalogged Source?: NO
     Point Source?:      YES
     GRB Indicated?:     YES    [ by BAT flight software ]
     Image S/N Ratio:    7.93
     Image Trigger?:     NO
     Rate S/N Ratio:     12.6491106406735  [ if not an image trigger ]
     Image S/N Ratio:    7.93

  Flight Position:   [ source = BAT ]
    RA: 2.16510709260475   Dec: -37.8550292612526  [deg; J2000]

  Ground Position:   [ source = BAT pre-slew burst ]
    RA: 2.16392106610135   Dec: -37.8770094287737  [deg; J2000]  
        { 00h 08m 39.3s , -37d 52' 37.2" }
         +/- 0.84520773199824 [arcmin] (estimated 90% radius based on SNR)
         +/- 0.317731189257129 [arcmin] (formal 1-sigma fit error)
    SNR: 38.6773127603391
 
  Angular difference between Flight and Ground position is 1.320006 arcmin
 
  Partial Coding Fraction: 0.1503906    [ including projection effects ]

  Duration
     T90: 13.8679999709129 +/- 1.30256362054126
        Measured from: 1.42799997329712
                   to: 15.2959999442101     [s; relative to TRIGTIME]
     T50: 4.72799998521805 +/- 0.404850582176752
        Measured from: 5.92799997329712
                   to: 10.6559999585152     [s; relative to TRIGTIME]



  Fluence
     Peak Flux  (peak 1 second)
        Measured from: 8.04399996995926     
                   to: 9.04399996995926     [s; relative to TRIGTIME]
     Total Fluence        
        Measured from: -0.103999972343445     
                   to: 21.8159999847412     [s; relative to TRIGTIME]
     
             Band 1     Band 2     Band 3     Band 4
              15-25      25-50     50-100    100-350     keV
 Total     4.135931   4.135400   2.100571   0.341742
           0.095461   0.096117   0.078715   0.057984 [error]
 Peak      0.441170   0.519792   0.393224   0.091834
           0.026448   0.029003   0.024733   0.015954 [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 1.79e-06 2.07e-06 1.71e-06 2.39e-06 6.43e-06 7.96e-06   erg/cm2
              Error 1.01e-07 6.75e-08 8.40e-08 2.49e-07 2.06e-07 3.23e-07   erg/cm2
Peak flux Power-law 5.65e+00 4.78e+00 2.75e+00 2.35e+00 1.42e+01 1.55e+01   ph/cm2/s
              Error 5.95e-01 3.05e-01 2.08e-01 3.65e-01 9.13e-01 9.23e-01   ph/cm2/s
 
Fluence   Cutoff-PL 1.74e-06 2.09e-06 1.72e-06 1.91e-06 6.35e-06 7.46e-06   erg/cm2
              Error 1.29e-07 5.79e-08 8.70e-08 5.42e-07 2.40e-07 6.72e-07   erg/cm2
Peak flux Cutoff-PL 5.70e+00 4.78e+00 2.74e+00 2.31e+00 1.42e+01 1.55e+01   ph/cm2/s
              Error 6.07e-01 3.02e-01 1.78e-01 3.86e-01 9.16e-01 9.93e-01   ph/cm2/s
 
Fluence        Band -------- 2.08e-06 1.72e-06 1.92e-06 6.34e-06 7.46e-06   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    2.270    0.065    -      -           3.09e-02 1.09e-03   42.920 57
CPL   1.991    0.000       1.7    9.5      4.24e-02 2.59e-03   42.370 56
 
 
=== 1-s peak spectral analysis ===
 
Model Ph_index Ph_90err Epeak  Epeak_90err Norm     Nomr_90err chi2   dof
PL    1.797    0.106    -      -           1.03e-01 6.25e-03   37.250 57
CPL   2.015    0.000       6.7    0.0      7.95e-02 0.00e+00   36.570 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: 9.600000 sec.
T50 in the 50-300 keV band: 3.200000 sec.

 
=== Table of the duration information ==
 
        Value   tstart    tstop
T100   21.920   -0.104   21.816
T90    13.868    1.428   15.296
T50     4.728    5.928   10.656
Peak    1.000    8.044    9.044

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
    2.1639   -37.8770   0.0050    50.1980   -34.0831         8.9135016     38.677 TRIG_00451757                 
 
Foreground time interval of the image:
 -0.104  10.989 (delta_t =  11.093 [sec])
Background time interval of the image:
-239.912  -0.104 (delta_t = 239.808 [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   -0.104 sec. to   21.816 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 2.27024     ( -0.0648655   0.0658492 )
Norm@50keV  : 3.08648E-02    ( -0.00109266   0.0010864 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          42.92 using 59 PHA bins.
# Reduced chi-squared =         0.7530 for     57 degrees of freedom 
# Null hypothesis probability =   9.165109e-01
 
Photon flux (15-150 keV)    in 21.92 sec: 5.30605 ( -0.198921  0.200372 ) ph/cm2/s
Energy fluence (15-150 keV)             : 6.43115e-06 ( -2.05763e-07  2.05852e-07 ) ergs/cm2

Cutoff power-law model

Time interval is from   -0.104 sec. to   21.816 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.99058     (     )
Epeak [keV] : 1.69146      ( -0.346674 18.577 )
Norm@50keV  : 4.23606E-02    ( -0.0020974   0.00307436 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          42.37 using 59 PHA bins.
# Reduced chi-squared =         0.7566 for     56 degrees of freedom 
# Null hypothesis probability =   9.108694e-01
 
Photon flux (15-150 keV)    in 21.92 sec: 5.22884 ( -0.22879  0.22698 ) ph/cm2/s
Energy fluence (15-150 keV)             : 6.35371e-06 ( -2.40419e-07  2.38621e-07 ) ergs/cm2

Band function

Time interval is from   -0.104 sec. to   21.816 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -1.94605   ( 1.87629   1.87629 )
beta        : -2.32775    ( 2.32633   0.109033 )
Epeak [keV] : 6.37338      ( -6.15095 11.9366 )
Norm@50keV   : 4.76110E-02    ( -0.00743948   0.217902 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          41.97 using 59 PHA bins.
# Reduced chi-squared =         0.7631 for     55 degrees of freedom 
# Null hypothesis probability =   9.017809e-01
 
Photon flux (15-150 keV)    in 21.92 sec:  (    ) ph/cm2/s
Energy fluence (15-150 keV)             : 6.34209e-06 ( 0  0 ) ergs/cm2

Single BB

 
Spectral model blackbody:
------------------------------------------------------------
Parameters  : value    Lower 90%  Upper 90%
kT [keV]    : 10.8411  (  )
R^2/D10^2   : 1.54451  (   )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =         305.60 using 59 PHA bins.
# Reduced chi-squared =         5.3614 for     57 degrees of freedom 
# Null hypothesis probability =   1.070517e-35
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  8.289e-07   5.096e-08
25- 50  2.300e-06   8.878e-08
50-150  1.510e-06   1.111e-07
15-150  4.638e-06   1.611e-07

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 56.3757       (-4.79525      5.40501)
Norm        : 26.6483       (-1.73191     1.56051)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          63.63 using 59 PHA bins.
# Reduced chi-squared =          1.116 for     57 degrees of freedom 
# Null hypothesis probability =   2.545214e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.452e-06   8.023e-08
25- 50  2.167e-06   8.209e-08
50-150  2.339e-06   1.502e-07
15-150  5.959e-06   1.995e-07

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 5.67147        (-0.546365      0.58079)
R1^2/D10^2  : 16.2697        (-5.3436      8.89263)
kT2 [keV]   : 19.5185        (-1.81778      2.27121)
R2^2/D10^2  : 0.106507    (-0.0397694   0.0561718)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          52.13 using 59 PHA bins.
# Reduced chi-squared =         0.9479 for     55 degrees of freedom 
# Null hypothesis probability =   5.849009e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.572e-06   1.580e-07
25- 50  2.080e-06   1.345e-07
50-150  2.476e-06   2.327e-07
15-150  6.128e-06   4.099e-07

Peak spectrum fit

Power-law model

Time interval is from    8.044 sec. to    9.044 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.79720     ( -0.105164   0.106893 )
Norm@50keV  : 0.103216    ( -0.00625877   0.00623383 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          37.25 using 59 PHA bins.
# Reduced chi-squared =         0.6534 for     57 degrees of freedom 
# Null hypothesis probability =   9.801441e-01
 
Photon flux (15-150 keV)    in 1 sec: 14.2075 ( -0.911349  0.914459 ) ph/cm2/s
Energy fluence (15-150 keV)             : 9.50303e-07 ( -5.84112e-08  5.85737e-08 ) ergs/cm2

Cutoff power-law model

Time interval is from    8.044 sec. to    9.044 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 2.01456     ( -2.01456   -2.01456 )
Epeak [keV] : 6.66160      (   )
Norm@50keV  : 7.95025E-02    (     )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          36.57 using 59 PHA bins.
# Reduced chi-squared =         0.6530 for     56 degrees of freedom 
# Null hypothesis probability =   9.793684e-01
 
Photon flux (15-150 keV)    in 1 sec: 14.2373 ( -0.9496  0.8819 ) ph/cm2/s
Energy fluence (15-150 keV)             : 9.49887e-07 ( -5.7815e-08  5.8163e-08 ) ergs/cm2

Band function

Time interval is from    8.044 sec. to    9.044 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -1.46602   ( 1.48086   1.48086 )
beta        : -1.79684    ( -0.106874   0.10512 )
Epeak [keV] : 23.4027      ( -20.3728 -20.3728 )
Norm@50keV   : 0.216416    ( -0.0969442   14.6559 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          37.25 using 59 PHA bins.
# Reduced chi-squared =         0.6772 for     55 degrees of freedom 
# Null hypothesis probability =   9.681106e-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]    : 14.5301  (  )
R^2/D10^2   : 1.64124  (   )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =         144.29 using 59 PHA bins.
# Reduced chi-squared =         2.5314 for     57 degrees of freedom 
# Null hypothesis probability =   1.633006e-09
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  7.289e-08   9.050e-09
25- 50  2.811e-07   2.315e-08
50-150  3.980e-07   4.245e-08
15-150  7.520e-07   5.430e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 132.476       (-30.4104      36.8281)
Norm        : 57.5202       (-4.35678     5.60425)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          44.38 using 59 PHA bins.
# Reduced chi-squared =         0.7785 for     57 degrees of freedom 
# Null hypothesis probability =   8.886033e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.491e-07   1.385e-08
25- 50  2.711e-07   2.145e-08
50-150  5.071e-07   1.524e-07
15-150  9.273e-07   1.760e-07

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 5.54157        (-1.05442      1.30184)
R1^2/D10^2  : 42.8270        (-23.8612      63.711)
kT2 [keV]   : 23.6014        (-3.35812      5.26245)
R2^2/D10^2  : 0.221571    (-0.117646   0.182126)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          44.63 using 59 PHA bins.
# Reduced chi-squared =         0.8114 for     55 degrees of freedom 
# Null hypothesis probability =   8.399722e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.766e-07   4.115e-08
25- 50  2.505e-07   3.720e-08
50-150  5.135e-07   7.860e-08
15-150  9.405e-07   1.320e-07

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: 2.23055     ( -0.0656687   0.0666144 )
Norm@50keV  : 4.76618E-02    ( -0.00169332   0.00168429 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          41.45 using 59 PHA bins.
# Reduced chi-squared =         0.7273 for     57 degrees of freedom 
# Null hypothesis probability =   9.394789e-01
 
Photon flux (15-150 keV)    in 11.09 sec: 8.01949 ( -0.308466  0.310698 ) ph/cm2/s
Energy fluence (15-150 keV)             : 4.9921e-06 ( -1.62978e-07  1.63064e-07 ) ergs/cm2

Cutoff power-law model

Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.98875     (     )
Epeak [keV] : 2.47458      ( -0.585118 16.0062 )
Norm@50keV  : 6.19016E-02    ( -0.00441797   0.00455387 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          44.17 using 59 PHA bins.
# Reduced chi-squared =         0.7887 for     56 degrees of freedom 
# Null hypothesis probability =   8.737133e-01
 
Photon flux (15-150 keV)    in 11.09 sec: 8.02303 ( -0.17815  0.30107 ) ph/cm2/s
Energy fluence (15-150 keV)             : 4.99204e-06 ( -1.62036e-07  1.61659e-07 ) ergs/cm2

Band function

 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -1.15970   (     )
beta        : -9.37167    (     )
Epeak [keV] : 65.0901      (   )
Norm@50keV   : 0.101634    (     )
------------------------------------------------------------
#Fit statistic : Chi-Squared =         154.02 using 59 PHA bins.
# Reduced chi-squared =         2.8003 for     55 degrees of freedom 
# Null hypothesis probability =   2.561870e-11
 
Photon flux (15-150 keV)    in 11.09 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)  = 2.07e-06
S(50-100 keV) = 1.71e-06

T90 vs. Hardness ratio plot

T90                                   = 13.8679999709129 sec.
Hardness ratio (energy fluence ratio) = 0.826087

Color vs. Color plot

Count Ratio  (25-50 keV) / (15-25 keV) = 0.999872
Count Ratio (50-100 keV) / (15-25 keV) = 0.507883

Mask shadow pattern

IMX = 9.939953859145266E-01, IMY = 6.725578022923394E-01

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:
-239.912000 -0.104000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
268.3554  -1.4339    3.5  43.2  129.1   2.7231   3.3    1.4	SW J1753.5-0127               
270.2372 -25.0575    8.8  36.6   93.2   0.7962   1.3    2.9	GX 5-1                        
270.3738 -25.8568   12.0  36.6   91.9   0.5926   1.0    7.8	GRS 1758-258                  
274.0373 -13.9885    2.0  33.8  112.8   2.2181   5.8    3.4	GX 17+2                       
276.1194 -30.4774    0.0  32.3   82.3   0.6564   1.6   12.0	H1820-303                     
285.0231 -24.8921    3.5  23.3   89.9   0.8799   3.3    1.8	HT1900.1-2455                 
288.8054  10.9494    1.3  35.2  165.1   2.5155   8.9    0.5	GRS 1915+105                  
299.6070  35.1648    2.1  53.9 -168.3   3.2537   5.6    2.4	Cyg X-1                       
308.2266  40.8413   13.3  58.9 -159.5   1.4504   0.9    8.5	Cyg X-3                       
316.6725   5.7813    3.2  25.0 -140.5   0.7255   3.6 ------	UNKNOWN                       
339.5783  12.6187    3.3  43.0 -112.1   3.5345   3.5 ------	UNKNOWN

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

Time interval of the image:
-0.104000 10.988590
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
268.2247  -1.3754    0.0  43.4  129.1  -0.3188  -2.1    9.8	SW J1753.5-0127               
270.1594 -25.2147    6.0  36.7   92.9  -0.2157  -1.9   10.6	GX 5-1                        
270.4015 -25.8395   18.2  36.5   91.9   0.0709   0.6    7.9	GRS 1758-258                  
273.9532 -14.1836   13.4  33.9  112.5   0.0732   0.9    9.3	GX 17+2                       
275.9504 -30.3519   59.8  32.4   82.6  -0.0148  -0.2    1.6	H1820-303                     
285.1589 -25.0372    6.0  23.2   89.5  -0.1096  -1.9    9.7	HT1900.1-2455                 
288.8043  10.7873    4.3  35.0  165.0   0.1598   2.7    9.5	GRS 1915+105                  
299.6196  35.3416    3.3  54.1 -168.3   0.3940   3.5    8.5	Cyg X-1                       
308.0616  40.9435   12.7  59.0 -159.6  -0.2166  -0.9    2.3	Cyg X-3                       
292.6422 -36.1985    2.7  23.2   56.4   0.2168   4.3 ------	UNKNOWN                       
306.7288  -0.1912    2.1  18.0 -166.3   0.2779   5.6 ------	UNKNOWN                       
314.4515   5.8463    2.7  24.5 -145.7   0.2386   4.3 ------	UNKNOWN                       
352.4674 -34.4243    2.7  41.9  -36.9   0.4733   4.3 ------	UNKNOWN                       
324.9207  14.9785    2.6  36.5 -132.4   0.4296   4.5 ------	UNKNOWN                       
  2.1639 -37.8770    0.3  50.2  -34.1   8.9136  38.7 ------	UNKNOWN

Post-slew image of 15-350 keV band

Time interval of the image:
76.788600 962.158300
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
306.4456 -49.4310    2.2  40.9  113.9   9.8157   5.3 ------	UNKNOWN                       
 68.4914 -43.3005    3.9  49.3   -2.7   2.9751   3.0 ------	UNKNOWN                       
 50.1896 -13.2184    4.1  49.1  -48.0   7.1081   2.8 ------	UNKNOWN

Plot creation:
Sat May 30 22:27:26 EDT 2015