batgrbproduct analysis for trigger=332399

batgrbproduct Analysis for Trigger=332399

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): Thu Sep 11 13:01:22 EDT 2014
             Host Name: batevent1
   Current Working Dir: /local/data/batevent/batevent_reproc/trigger332399
======================================================================

  Trigger: 00332399      Segment: 000

  BAT Trigger Time: 246378232   [s; MET]
      Trigger Stop: 246378296   [s; MET]
               UTC: 2008-10-22T14:23:48.804900    [includes UTCF correction] 
       Where From?: TDRSS position message

  BAT 
    RA: 226.618689631337   Dec: 12.4160839741371  [deg; J2000]

     Catalogged Source?: NO
     Point Source?:      YES
     GRB Indicated?:     YES    [ by BAT flight software ]
     Image S/N Ratio:    14.84
     Image Trigger?:     YES
     Rate S/N Ratio:     0  [ if not an image trigger ]
     Image S/N Ratio:    14.84

  Flight Position:   [ source = BAT ]
    RA: 226.618689631337   Dec: 12.4160839741371  [deg; J2000]

  Ground Position:   [ source = BAT pre-slew burst ]
    RA: 226.581519842759   Dec: 12.4092449267054  [deg; J2000]  
        { 15h 06m 19.6s , +12d 24' 33.3" }
         +/- 1.40617389679695 [arcmin] (estimated 90% radius based on SNR)
         +/- 0.543495283891171 [arcmin] (formal 1-sigma fit error)
    SNR: 18.6910650488041
 
  Angular difference between Flight and Ground position is 2.216373 arcmin
 
  Partial Coding Fraction: 0.6484375    [ including projection effects ]

  Duration
     T90: 157.580000013113 +/- 41.8824727554893
        Measured from: 11.4880000054836
                   to: 169.068000018597     [s; relative to TRIGTIME]
     T50: 59.5679999887943 +/- 8.23259083705847
        Measured from: 39.4040000140667
                   to: 98.972000002861     [s; relative to TRIGTIME]



  Fluence
     Peak Flux  (peak 1 second)
        Measured from: 57.1759999990463     
                   to: 58.1759999990463     [s; relative to TRIGTIME]
     Total Fluence        
        Measured from: -4.92800000309944     
                   to: 213.819999992847     [s; relative to TRIGTIME]
     
             Band 1     Band 2     Band 3     Band 4
              15-25      25-50     50-100    100-350     keV
 Total     1.288665   1.634069   1.128120   0.318785
           0.085315   0.087420   0.077443   0.068146 [error]
 Peak      0.027263   0.024102   0.020305   0.007837
           0.005889   0.006391   0.005577   0.004784 [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 3.94e-07 6.75e-07 8.81e-07 2.33e-06 2.59e-06 4.28e-06   erg/cm2
              Error 4.10e-08 4.25e-08 7.63e-08 4.32e-07 1.80e-07 4.93e-07   erg/cm2
Peak flux Power-law 2.21e-01 2.04e-01 1.30e-01 1.28e-01 6.09e-01 6.83e-01   ph/cm2/s
              Error 8.54e-02 4.96e-02 4.78e-02 9.66e-02 1.46e-01 1.72e-01   ph/cm2/s
 
Fluence   Cutoff-PL 3.76e-07 6.97e-07 8.91e-07 1.43e-06 2.51e-06 3.39e-06   erg/cm2
              Error 4.88e-08 5.28e-08 8.05e-08 7.63e-07 2.09e-07 6.93e-07   erg/cm2
Peak flux Cutoff-PL 2.23e-01 2.04e-01 1.29e-01 1.24e-01 6.09e-01 6.81e-01   ph/cm2/s
              Error 8.55e-02 4.94e-02 4.78e-02 1.23e-01 1.46e-01 1.75e-01   ph/cm2/s
 
Fluence        Band 3.67e-07 7.01e-07 8.78e-07 1.82e-06 2.51e-06 3.78e-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    1.615    0.112    -      -           1.27e-03 8.16e-05   47.090 57
CPL   1.306    0.428     108.3  -34.1      1.83e-03 1.02e-03   45.700 56
 
 
=== 1-s peak spectral analysis ===
 
Model Ph_index Ph_90err Epeak  Epeak_90err Norm     Nomr_90err chi2   dof
PL    1.649    0.474    -      -           4.66e-03 1.30e-03   48.390 57
CPL   2.306    0.000     111.1    0.0      2.11e-03 0.00e+00   48.030 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: 102.976000 sec.
T50 in the 50-300 keV band: 44.864000 sec.

 
=== Table of the duration information ==
 
        Value   tstart    tstop
T100  218.748   -4.928  213.820
T90   157.580   11.488  169.068
T50    59.568   39.404   98.972
Peak    1.000   57.176   58.176

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
  226.5815    12.4092   0.0103    23.1248   -85.8716         4.0107209     18.691 TRIG_00332399                 
 
Foreground time interval of the image:
 -4.928 213.820 (delta_t = 218.748 [sec])
Background time interval of the image:
-239.000  -4.928 (delta_t = 234.072 [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 64.000000

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 64.000000

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 64.000000

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   -4.928 sec. to  213.820 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.61526     ( -0.1118   0.11299 )
Norm@50keV  : 1.26644E-03    ( -8.18131e-05   8.13239e-05 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          47.09 using 59 PHA bins.
# Reduced chi-squared =         0.8262 for     57 degrees of freedom 
# Null hypothesis probability =   8.224058e-01
 
Photon flux (15-150 keV)    in 218.7 sec: 0.163522 ( -0.0102136  0.0102271 ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.58558e-06 ( -1.79448e-07  1.80908e-07 ) ergs/cm2

Cutoff power-law model

Time interval is from   -4.928 sec. to  213.820 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.30649     ( -0.494013   0.361636 )
Epeak [keV] : 108.297      ( -40.1691 -108.298 )
Norm@50keV  : 1.82965E-03    ( -0.00061789   0.00142592 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          45.70 using 59 PHA bins.
# Reduced chi-squared =         0.8161 for     56 degrees of freedom 
# Null hypothesis probability =   8.354259e-01
 
Photon flux (15-150 keV)    in 218.7 sec: 0.160760 ( -0.010978  0.010924 ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.51295e-06 ( -2.09077e-07  2.08858e-07 ) ergs/cm2

Band function

Time interval is from   -4.928 sec. to  213.820 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -1.13761   ( 1.14203   6.02342 )
beta        : -1.89985    ( 1.89757   0.346544 )
Epeak [keV] : 82.1152      ( -82.1399 -82.1399 )
Norm@50keV   : 2.27669E-03    ( -0.00106801   0.0578829 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          45.27 using 59 PHA bins.
# Reduced chi-squared =         0.8231 for     55 degrees of freedom 
# Null hypothesis probability =   8.222793e-01
 
Photon flux (15-150 keV)    in 218.7 sec:  (    ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.5096e-06 ( 0  0 ) ergs/cm2

Single BB

 
Spectral model blackbody:
------------------------------------------------------------
Parameters  : value    Lower 90%  Upper 90%
kT [keV]    : 13.6712  (-1.02006  1.12464)
R^2/D10^2   : 2.46738E-02  (-0.00609172   0.0079768)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          96.70 using 59 PHA bins.
# Reduced chi-squared =          1.696 for     57 degrees of freedom 
# Null hypothesis probability =   8.070619e-04
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  2.135e-07   2.416e-08
25- 50  7.751e-07   6.277e-08
50-150  9.421e-07   1.198e-07
15-150  1.931e-06   1.410e-07

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 164.860       (-44.6227      -165.129)
Norm        : 0.666700       (-0.0453043     0.0510536)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          45.71 using 59 PHA bins.
# Reduced chi-squared =         0.8019 for     57 degrees of freedom 
# Null hypothesis probability =   8.583395e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  3.712e-07   3.095e-08
25- 50  6.972e-07   1.590e-07
50-150  1.429e-06   5.687e-07
15-150  2.498e-06   6.996e-07

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 5.83320        (-1.68031      2.61874)
R1^2/D10^2  : 0.304935        (-0.206481      0.544247)
kT2 [keV]   : 20.7474        (-3.71357      10.4867)
R2^2/D10^2  : 4.52981E-03    (-0.00352447   0.00527746)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          51.09 using 59 PHA bins.
# Reduced chi-squared =         0.9288 for     55 degrees of freedom 
# Null hypothesis probability =   6.249474e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  3.702e-07   1.544e-07
25- 50  6.842e-07   1.651e-07
50-150  1.346e-06   3.493e-07
15-150  2.400e-06   5.104e-07

Peak spectrum fit

Power-law model

Time interval is from   57.176 sec. to   58.176 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.64854     ( -0.456172   0.492075 )
Norm@50keV  : 4.66442E-03    ( -0.00134078   0.00125408 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          48.39 using 59 PHA bins.
# Reduced chi-squared =         0.8490 for     57 degrees of freedom 
# Null hypothesis probability =   7.844843e-01
 
Photon flux (15-150 keV)    in 1 sec: 0.608763 ( -0.146441  0.146471 ) ph/cm2/s
Energy fluence (15-150 keV)             : 4.33866e-08 ( -1.27389e-08  1.32042e-08 ) ergs/cm2

Cutoff power-law model

Time interval is from   57.176 sec. to   58.176 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 2.30647     (     )
Epeak [keV] : 111.119      (   )
Norm@50keV  : 2.11222E-03    (     )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          48.03 using 59 PHA bins.
# Reduced chi-squared =         0.8576 for     56 degrees of freedom 
# Null hypothesis probability =   7.668424e-01
 
Photon flux (15-150 keV)    in 1 sec: 0.608810 ( -0.146241  0.146176 ) ph/cm2/s
Energy fluence (15-150 keV)             : 4.33024e-08 ( -6.3375e-09  1.29454e-08 ) ergs/cm2

Band function

Time interval is from   57.176 sec. to   58.176 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : 3.89221   ( 0.461612   0.461612 )
beta        : -1.69349    ( 1.66811   0.471579 )
Epeak [keV] : 20.4725      ( -26.454 447.335 )
Norm@50keV   : 246.075    ( -245.847   934733 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          48.25 using 59 PHA bins.
# Reduced chi-squared =         0.8773 for     55 degrees of freedom 
# Null hypothesis probability =   7.282345e-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]    : 11.2170  (-4.55052  9.15111)
R^2/D10^2   : 0.176804  (-0.148779   1.00728)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          58.27 using 59 PHA bins.
# Reduced chi-squared =          1.022 for     57 degrees of freedom 
# Null hypothesis probability =   4.284424e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  4.665e-09   2.900e-09
25- 50  1.352e-08   6.784e-09
50-150  9.754e-09   6.791e-09
15-150  2.794e-08   1.666e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 176.677       (-122.141      -178.752)
Norm        : 2.45932       (-0.606985     0.923804)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          49.18 using 59 PHA bins.
# Reduced chi-squared =         0.8628 for     57 degrees of freedom 
# Null hypothesis probability =   7.597928e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  6.215e-09   3.791e-09
25- 50  1.178e-08   6.735e-09
50-150  2.478e-08   1.482e-08
15-150  4.277e-08   2.559e-08

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 5.31514        (-1.85218      3.19558)
R1^2/D10^2  : 2.38194        (-1.95977      13.1953)
kT2 [keV]   : 33.2917        (-15.1025      111.332)
R2^2/D10^2  : 3.80263E-03    (-0.0036416   0.0225634)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          46.57 using 59 PHA bins.
# Reduced chi-squared =         0.8468 for     55 degrees of freedom 
# Null hypothesis probability =   7.835777e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  7.969e-09   4.868e-09
25- 50  9.529e-09   5.155e-09
50-150  2.988e-08   1.817e-08
15-150  4.737e-08   2.568e-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: 1.61526     ( -0.1118   0.11299 )
Norm@50keV  : 1.26644E-03    ( -8.18131e-05   8.13239e-05 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          47.09 using 59 PHA bins.
# Reduced chi-squared =         0.8262 for     57 degrees of freedom 
# Null hypothesis probability =   8.224058e-01
 
Photon flux (15-150 keV)    in 218.7 sec: 0.163522 ( -0.0102136  0.0102271 ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.58558e-06 ( -1.79448e-07  1.80908e-07 ) ergs/cm2

Cutoff power-law model

Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.30649     ( -0.494013   0.361636 )
Epeak [keV] : 108.297      ( -40.1691 -108.298 )
Norm@50keV  : 1.82965E-03    ( -0.00061789   0.00142592 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          45.70 using 59 PHA bins.
# Reduced chi-squared =         0.8161 for     56 degrees of freedom 
# Null hypothesis probability =   8.354259e-01
 
Photon flux (15-150 keV)    in 218.7 sec: 0.160760 ( -0.010978  0.010924 ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.51295e-06 ( -2.09077e-07  2.08858e-07 ) ergs/cm2

Band function

 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -1.13761   ( 1.14203   6.02342 )
beta        : -1.89985    ( 1.89757   0.346544 )
Epeak [keV] : 82.1152      ( -82.1399 -82.1399 )
Norm@50keV   : 2.27669E-03    ( -0.00106564   0.0512229 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          45.27 using 59 PHA bins.
# Reduced chi-squared =         0.8231 for     55 degrees of freedom 
# Null hypothesis probability =   8.222793e-01
 
Photon flux (15-150 keV)    in 218.7 sec:  (    ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.5096e-06 ( 0  0 ) ergs/cm2

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

S(25-50 keV)  = 6.75e-07
S(50-100 keV) = 8.81e-07

T90 vs. Hardness ratio plot

T90                                   = 157.580000013113 sec.
Hardness ratio (energy fluence ratio) = 1.30519

Color vs. Color plot

Count Ratio  (25-50 keV) / (15-25 keV) = 1.26803
Count Ratio (50-100 keV) / (15-25 keV) = 0.875418

Mask shadow pattern

IMX = 3.074378814217653E-02, IMY = 4.259403152872967E-01

TIME vs. PHA plot around the trigger time

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 64.000000

TIME vs. DetID plot around the trigger time

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 64.000000

100 us light curve (15-350 keV)

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 64.000000

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:
-239.000000 -4.928000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
254.4365  35.3311    0.8  13.3  137.0   2.4235  14.4    1.2	Her X-1                       
268.3318  -1.5032    2.7  44.2 -162.5   1.3661   4.3    3.7	SW J1753.5-0127               
274.1685 -13.9936    8.1  57.7 -159.1  -1.6262  -1.4    9.8	GX 17+2                       
288.7442  10.8634   70.3  50.8  166.3  -0.0989  -0.2    5.9	GRS 1915+105                  
284.7051  21.8525    2.1  42.0  155.7   1.9466   5.4 ------	UNKNOWN                       
270.6245  11.5894    2.2  36.1 -178.9   1.1152   5.2 ------	UNKNOWN                       
189.8893  20.0957    3.3  45.1  -30.9   1.0917   3.5 ------	UNKNOWN

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

Time interval of the image:
-4.928000 213.820000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
254.2635  35.3752    9.6  13.2  136.7  -0.2186  -1.2    9.7	Her X-1                       
268.3361  -1.4648    7.4  44.2 -162.5  -0.5018  -1.5    2.0	SW J1753.5-0127               
274.0313 -14.0164    7.7  57.7 -158.9   1.2994   1.5    1.9	GX 17+2                       
288.9270  10.9295   76.7  50.9  166.1   0.0910   0.1    7.6	GRS 1915+105                  
175.3205  64.6947    2.5  49.5   32.5   4.0203   4.6 ------	UNKNOWN                       
171.5065  63.3478    2.1  51.0   30.6   4.9131   5.4 ------	UNKNOWN                       
278.2835  -7.0579    1.7  54.8 -168.0   3.9482   6.9 ------	UNKNOWN                       
226.5815  12.4093    0.6  23.1  -85.9   4.0104  18.7 ------	UNKNOWN                       
191.9718  12.2390    2.4  47.3  -41.8   2.5460   4.8 ------	UNKNOWN

Post-slew image of 15-350 keV band

Time interval of the image:
387.200600 663.150000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
244.9598 -15.6413    1.6  15.2 -124.5   6.6373   7.2    1.1	Sco X-1                       
254.3117  35.3435    5.9  40.3    8.7   2.5369   1.9    7.1	Her X-1                       
256.1691 -37.9051    7.8  32.9 -169.4  -1.4952  -1.5    9.4	4U 1700-377                   
256.5696 -36.3170    3.9  31.4 -170.0   2.8727   3.0    9.1	GX 349+2                      
263.1728 -24.8599   76.6  21.1  172.5   0.1356   0.2   11.3	GX 1+4                        
264.5339 -44.3370    7.0  40.1 -178.6   2.3245   1.7   11.2	4U 1735-44                    
268.2153  -1.4550    3.7  12.7   85.2   2.9489   3.1    9.2	SW J1753.5-0127               
270.4344 -25.0524    4.6  24.4  157.8  -2.5066  -2.5    8.3	GX 5-1                        
270.2513 -25.7073   11.4  24.8  159.0   1.0471   1.0    3.5	GRS 1758-258                  
274.1200 -13.8552    0.0  19.9  128.6  -0.5582  -0.5   12.7	GX 17+2                       
275.8169 -30.5404    9.4  31.7  157.1   1.6433   1.2   11.8	H1820-303                     
285.0896 -24.9747  236.5  34.3  139.5   0.0824   0.0    4.4	HT1900.1-2455                 
288.7296  10.9669    5.8  36.3   74.7   5.4057   2.0    4.2	GRS 1915+105                  
262.9912 -33.8735    5.5  29.6  179.1   2.2347   2.1    2.3	GX 354-0                      
276.6422 -35.4850    2.8  36.0  161.6   5.8438   4.1 ------	UNKNOWN                       
245.9007  29.4777    3.3  35.8   -4.3   3.9302   3.5 ------	UNKNOWN                       
236.0319  47.4988    3.0  55.3   -5.4  11.6016   3.9 ------	UNKNOWN                       
215.7814 -16.8579    2.9  41.1  -99.2  14.6637   3.9 ------	UNKNOWN

Plot creation:
Sun May 31 05:47:45 EDT 2015