batgrbproduct analysis for trigger=566545

batgrbproduct Analysis for Trigger=566545

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): Sat Jan 11 23:49:49 EST 2014
             Host Name: batevent1
   Current Working Dir: /local/data/batevent/batevent_reproc/trigger566545
======================================================================

  Trigger: 00566545      Segment: 000

  BAT Trigger Time: 398310426.624   [s; MET]
      Trigger Stop: 398310427.648   [s; MET]
               UTC: 2013-08-16T01:46:55.708120    [includes UTCF correction] 
       Where From?: TDRSS position message

  BAT 
    RA: 197.167012694417   Dec: -58.9479813527746  [deg; J2000]

     Catalogged Source?: NO
     Point Source?:      YES
     GRB Indicated?:     YES    [ by BAT flight software ]
     Image S/N Ratio:    9.35
     Image Trigger?:     NO
     Rate S/N Ratio:     12.8452325786651  [ if not an image trigger ]
     Image S/N Ratio:    9.35

  Flight Position:   [ source = BAT ]
    RA: 197.167012694417   Dec: -58.9479813527746  [deg; J2000]

  Ground Position:   [ source = BAT pre-slew burst ]
    RA: 197.092507986141   Dec: -58.9959761092675  [deg; J2000]  
        { 13h 08m 22.2s , -58d 59' 45.5" }
         +/- 2.59470454607613 [arcmin] (estimated 90% radius based on SNR)
         +/- 1.25458471540651 [arcmin] (formal 1-sigma fit error)
    SNR: 7.79048003519999
 
  Angular difference between Flight and Ground position is 3.688103 arcmin
 
  Partial Coding Fraction: 0.3554688    [ including projection effects ]

  Duration
     T90: 29.9759999513626 +/- 1.35699668952184
        Measured from: -27.772000014782
                   to: 2.20399993658066     [s; relative to TRIGTIME]
     T50: 17.027999997139 +/- 14.6264964686467
        Measured from: -16.3120000362396
                   to: 0.715999960899353     [s; relative to TRIGTIME]



  Fluence
     Peak Flux  (peak 1 second)
        Measured from: -0.0360000133514404     
                   to: 0.96399998664856     [s; relative to TRIGTIME]
     Total Fluence        
        Measured from: -28.055999994278     
                   to: 2.58399999141693     [s; relative to TRIGTIME]
     
             Band 1     Band 2     Band 3     Band 4
              15-25      25-50     50-100    100-350     keV
 Total     0.230650   0.317410   0.147434   0.012580
           0.047181   0.048327   0.041770   0.036674 [error]
 Peak      0.058786   0.080067   0.027130   0.006479
           0.009435   0.010099   0.008414   0.006598 [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 8.33e-08 1.23e-07 1.35e-07 2.80e-07 4.27e-07 6.22e-07   erg/cm2
              Error 2.20e-08 2.27e-08 4.09e-08 1.71e-07 9.54e-08 2.14e-07   erg/cm2
Peak flux Power-law 7.02e-01 5.15e-01 2.51e-01 1.73e-01 1.55e+00 1.64e+00   ph/cm2/s
              Error 1.49e-01 8.26e-02 6.54e-02 8.31e-02 2.47e-01 2.65e-01   ph/cm2/s
 
Fluence   Cutoff-PL 8.12e-08 1.29e-07 1.34e-07 1.48e-07 4.11e-07 4.92e-07   erg/cm2
              Error 2.36e-08 3.04e-08 4.72e-08 1.85e-07 1.10e-07 2.68e-07   erg/cm2
Peak flux Cutoff-PL 5.89e-01 6.45e-01 2.38e-01 2.16e-02 1.49e+00 1.49e+00   ph/cm2/s
              Error 1.76e-01 1.25e-01 8.42e-02 4.64e-02 2.48e-01 2.50e-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    1.861    0.339    -      -           1.52e-03 3.38e-04   42.280 57
CPL   1.516    1.251      58.9    0.0      2.40e-03 0.00e+00   42.080 56
 
 
=== 1-s peak spectral analysis ===
 
Model Ph_index Ph_90err Epeak  Epeak_90err Norm     Nomr_90err chi2   dof
PL    2.038    0.278    -      -           1.02e-02 2.05e-03   53.290 57
CPL   0.024    1.709      40.0   10.3      1.53e-01 1.07e+00   47.410 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: 1.664000 sec.
T50 in the 50-300 keV band: 1.152000 sec.

 
=== Table of the duration information ==
 
        Value   tstart    tstop
T100   30.640  -28.056    2.584
T90    29.976  -27.772    2.204
T50    17.028  -16.312    0.716
Peak    1.000   -0.036    0.964

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
  197.0925   -58.9960   0.0247    31.9036    56.9179         0.7316770      7.790 TRIG_00566545                 
 
Foreground time interval of the image:
-28.056   2.584 (delta_t =  30.640 [sec])
Background time interval of the image:
-173.123 -28.056 (delta_t = 145.067 [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)

The mask-weighted light curves based on cleaned DPHs

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  -28.056 sec. to    2.584 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.86083     ( -0.326303   0.352225 )
Norm@50keV  : 1.51609E-03    ( -0.000344144   0.000331347 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          42.28 using 59 PHA bins.
# Reduced chi-squared =         0.7418 for     57 degrees of freedom 
# Null hypothesis probability =   9.271984e-01
 
Photon flux (15-150 keV)    in 30.64 sec: 0.214047 ( -0.0394332  0.0394411 ) ph/cm2/s
Energy fluence (15-150 keV)             : 4.27076e-07 ( -9.37857e-08  9.6948e-08 ) ergs/cm2

Cutoff power-law model

Time interval is from  -28.056 sec. to    2.584 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.51606     ( -1.8106   0.69066 )
Epeak [keV] : 58.8958      (   )
Norm@50keV  : 2.40479E-03    (     )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          42.08 using 59 PHA bins.
# Reduced chi-squared =         0.7515 for     56 degrees of freedom 
# Null hypothesis probability =   9.160276e-01
 
Photon flux (15-150 keV)    in 30.64 sec: 0.211625 ( -0.04059  0.020208 ) ph/cm2/s
Energy fluence (15-150 keV)             : 4.11219e-07 ( -1.09822e-07  1.09342e-07 ) ergs/cm2

Band function

Time interval is from  -28.056 sec. to    2.584 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : 1.70457   ( -4.05271   -4.05271 )
beta        : -2.09043    ( -0.720883   0.485399 )
Epeak [keV] : 28.0435      ( -25.6999 43.8638 )
Norm@50keV   : 0.559719    ( -0.542147   94.059 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          41.34 using 59 PHA bins.
# Reduced chi-squared =         0.7516 for     55 degrees of freedom 
# Null hypothesis probability =   9.137868e-01
 
Photon flux (15-150 keV)    in 30.64 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]    : 9.98600  (-2.02022  2.62826)
R^2/D10^2   : 0.101617  (-0.0597107   0.138133)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          47.83 using 59 PHA bins.
# Reduced chi-squared =         0.8392 for     57 degrees of freedom 
# Null hypothesis probability =   8.012923e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  6.320e-08   2.306e-08
25- 50  1.568e-07   5.057e-08
50-150  8.152e-08   3.788e-08
15-150  3.016e-07   8.837e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 83.2868       (-38.2304      -83.2868)
Norm        : 0.996375       (-0.242795     0.342459)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          42.12 using 59 PHA bins.
# Reduced chi-squared =         0.7390 for     57 degrees of freedom 
# Null hypothesis probability =   9.296615e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  7.940e-08   2.016e-08
25- 50  1.320e-07   3.387e-08
50-150  1.913e-07   1.434e-07
15-150  4.027e-07   1.582e-07

Double BB

------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 7.18985        (-3.38768      3.20189)
R1^2/D10^2  : 0.284006        (      )
kT2 [keV]   : 30.8536        (-18.0641      -30.9184)
R2^2/D10^2  : 1.03985E-03    (-0.00100746   0.00352197)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          41.75 using 59 PHA bins.
#Fit statistic : Chi-Squared =          41.40 using 59 PHA bins.
# Reduced chi-squared =         0.7591 for     55 degrees of freedom 
# Reduced chi-squared =         0.7527 for     55 degrees of freedom 
# Null hypothesis probability =   9.061138e-01
# Null hypothesis probability =   9.126569e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  7.997e-08   4.777e-08
25- 50  1.281e-07   7.079e-08
50-150  1.816e-07   1.181e-07
15-150  3.897e-07   2.107e-07

Peak spectrum fit

Power-law model

Time interval is from   -0.036 sec. to    0.964 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 2.03768     ( -0.264669   0.290397 )
Norm@50keV  : 1.01512E-02    ( -0.00208255   0.00202655 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          53.29 using 59 PHA bins.
# Reduced chi-squared =         0.9349 for     57 degrees of freedom 
# Null hypothesis probability =   6.151634e-01
 
Photon flux (15-150 keV)    in 1 sec: 1.54966 ( -0.247024  0.247042 ) ph/cm2/s
Energy fluence (15-150 keV)             : 9.38261e-08 ( -1.76553e-08  1.8144e-08 ) ergs/cm2

Cutoff power-law model

Time interval is from   -0.036 sec. to    0.964 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 2.40199E-02     ( -1.94661   1.47051 )
Epeak [keV] : 39.9878      ( -9.69258 10.963 )
Norm@50keV  : 0.153083    ( -0.153942   1.98102 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          47.41 using 59 PHA bins.
# Reduced chi-squared =         0.8467 for     56 degrees of freedom 
# Null hypothesis probability =   7.861517e-01
 
Photon flux (15-150 keV)    in 1 sec: 1.49126 ( -0.24722  0.24851 ) ph/cm2/s
Energy fluence (15-150 keV)             : 8.32941e-08 ( -1.59547e-08  1.79789e-08 ) ergs/cm2

Band function

Time interval is from   -0.036 sec. to    0.964 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -6.85010E-02   ( 1.17714   1.24674 )
beta        : -10.00000    ( 10   4.38316e-11 )
Epeak [keV] : 39.9373      ( -7.58367 8.77264 )
Norm@50keV   : 0.144641    ( -0.0224373   2.0001 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          47.42 using 59 PHA bins.
# Reduced chi-squared =         0.8621 for     55 degrees of freedom 
# Null hypothesis probability =   7.564631e-01
 
Photon flux (15-150 keV)    in 1 sec:  (    ) ph/cm2/s
Energy fluence (15-150 keV)             : 8.41046e-08 ( 0  0 ) ergs/cm2

Single BB

 
Spectral model blackbody:
------------------------------------------------------------
Parameters  : value    Lower 90%  Upper 90%
kT [keV]    : 10.2253  (-1.49944  1.69239)
R^2/D10^2   : 0.718102  (-0.321337   0.589599)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          49.28 using 59 PHA bins.
# Reduced chi-squared =         0.8646 for     57 degrees of freedom 
# Null hypothesis probability =   7.564122e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.540e-08   3.905e-09
25- 50  3.951e-08   9.470e-09
50-150  2.199e-08   8.985e-09
15-150  7.689e-08   1.851e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 59.1316       (-19.698      36.3658)
Norm        : 8.37731       (-1.88068     2.34773)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          49.46 using 59 PHA bins.
# Reduced chi-squared =         0.8678 for     57 degrees of freedom 
# Null hypothesis probability =   7.506098e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  2.100e-08   4.165e-09
25- 50  3.182e-08   6.340e-09
50-150  3.577e-08   1.521e-08
15-150  8.860e-08   2.173e-08

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 3.57241        (-3.57238      -3.57238)
R1^2/D10^2  : 14.8409        (-14.8414      -14.8414)
kT2 [keV]   : 11.6237        (-2.19214      -11.6237)
R2^2/D10^2  : 0.392483    (-0.392485   0.6032)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          46.91 using 59 PHA bins.
# Reduced chi-squared =         0.8530 for     55 degrees of freedom 
# Null hypothesis probability =   7.727685e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.877e-08   9.520e-09
25- 50  3.583e-08   2.014e-08
50-150  2.693e-08   1.648e-08
15-150  8.153e-08   4.351e-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: 1.86083     ( -0.326303   0.352225 )
Norm@50keV  : 1.51609E-03    ( -0.000344144   0.000331347 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          42.28 using 59 PHA bins.
# Reduced chi-squared =         0.7418 for     57 degrees of freedom 
# Null hypothesis probability =   9.271984e-01
 
Photon flux (15-150 keV)    in 30.64 sec: 0.214047 ( -0.0394332  0.0394411 ) ph/cm2/s
Energy fluence (15-150 keV)             : 4.27076e-07 ( -9.37857e-08  9.6948e-08 ) ergs/cm2

Cutoff power-law model

Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.51606     ( -1.8106   0.690717 )
Epeak [keV] : 58.8958      (   )
Norm@50keV  : 2.40479E-03    (     )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          42.08 using 59 PHA bins.
# Reduced chi-squared =         0.7515 for     56 degrees of freedom 
# Null hypothesis probability =   9.160276e-01
 
Photon flux (15-150 keV)    in 30.64 sec: 0.211625 ( -0.04059  0.020208 ) ph/cm2/s
Energy fluence (15-150 keV)             : 4.11219e-07 ( -1.09822e-07  1.09342e-07 ) ergs/cm2

Band function

 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : 1.70457   ( -4.05271   -4.05271 )
beta        : -2.09043    ( -0.720883   0.485399 )
Epeak [keV] : 28.0435      ( -25.6999 43.8638 )
Norm@50keV   : 0.559719    ( -0.542147   94.0766 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          41.34 using 59 PHA bins.
# Reduced chi-squared =         0.7516 for     55 degrees of freedom 
# Null hypothesis probability =   9.137868e-01
 
Photon flux (15-150 keV)    in 30.64 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)  = 1.23e-07
S(50-100 keV) = 1.35e-07

T90 vs. Hardness ratio plot

T90                                   = 29.9759999513626 sec.
Hardness ratio (energy fluence ratio) = 1.09756

Color vs. Color plot

Count Ratio  (25-50 keV) / (15-25 keV) = 1.37615
Count Ratio (50-100 keV) / (15-25 keV) = 0.639211

Mask shadow pattern

IMX = 3.398025988801988E-01, IMY = -5.216129614581994E-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:
-173.123400 -28.056000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
135.3921 -40.6430    4.1  16.0  176.7   0.3614   2.8    8.2	Vela X-1                      
170.2382 -60.7338    3.8  22.6   78.6   0.4728   3.1    7.0	Cen X-3                       
186.6366 -62.8398   14.5  29.2   68.3   0.1728   0.8    4.2	GX 301-2                      
218.9505 -46.1651    2.7  45.0   36.0   1.5587   4.2 ------	UNKNOWN                       
201.4108 -42.9886    2.2  33.5   26.8   0.9031   5.2 ------	UNKNOWN                       
217.0647 -21.3700    2.4  54.3    5.5   2.4602   4.8 ------	UNKNOWN                       
103.9059 -37.1720    2.3  40.6  172.8   1.0130   5.0 ------	UNKNOWN                       
170.1121 -19.7567    2.5  23.3  -49.2   0.6094   4.6 ------	UNKNOWN

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

Time interval of the image:
-28.056000 2.584000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
135.7474 -40.4302    0.0  15.8  177.6   0.0724   1.3   12.5	Vela X-1                      
170.5005 -60.7506   15.9  22.7   78.4  -0.0542  -0.7    9.4	Cen X-3                       
186.4147 -62.6665    6.4  29.0   68.1   0.1759   1.8    9.1	GX 301-2                      
197.0925 -58.9960    1.5  31.9   56.9   0.7315   7.8 ------	UNKNOWN                       
120.0820 -49.9102    2.0  27.3  152.6   0.4003   5.8 ------	UNKNOWN                       
126.2284 -46.8593    2.1  22.9  158.5   0.3234   5.4 ------	UNKNOWN                       
168.4530 -42.7892    2.1   9.5   28.4   0.2934   5.5 ------	UNKNOWN                       
130.3905 -35.5095    2.1  20.9 -170.0   0.3108   5.6 ------	UNKNOWN                       
108.9797 -19.7803    2.3  45.1 -161.5   0.4556   5.0 ------	UNKNOWN                       
181.3620   2.8403    2.3  48.4  -49.3   1.2053   5.1 ------	UNKNOWN

Post-slew image of 15-350 keV band

Time interval of the image:
71.676590 962.391500
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
135.6399 -40.5476    4.3  41.9 -132.1   2.7684   2.7    5.1	Vela X-1                      
170.3036 -60.6061    1.4  13.5 -148.6   3.7007   8.4    1.1	Cen X-3                       
186.7711 -62.7819    1.5   6.3 -171.9   3.5075   7.7    3.2	GX 301-2                      
255.7849 -37.7071   24.8  42.6   46.9   0.6127   0.5   12.6	4U 1700-377                   
256.5922 -36.4384    5.6  44.0   46.4   2.8799   2.1    7.6	GX 349+2                      
214.4944 -35.4575    3.1  26.1   -6.4   1.7838   3.7 ------	UNKNOWN                       
219.0863 -27.3205    2.8  35.1   -4.7   2.3962   4.1 ------	UNKNOWN                       
201.4250 -42.9310    2.3  16.2  -28.7   2.2406   5.1 ------	UNKNOWN                       
193.6641  -8.2507    3.9  50.7  -44.4   8.0538   3.0 ------	UNKNOWN                       
169.2766 -22.9333    2.9  41.1  -80.9   8.9605   4.0 ------	UNKNOWN

Plot creation:
Sat May 30 15:53:20 EDT 2015