batgrbproduct analysis for trigger=543763

batgrbproduct Analysis for Trigger=543763

Analysis Summary

Notes:

1) No attempt has been made to eliminate the non-significant decimal places.
2) This batgrbproduct analysis is done of the amount of data for this trigger downloaded to date.
3) This batgrbproduct analysis is using the flight position for the mask-weighting calculation.
4) This page will be updated for up to 10 downlinks after the trigger.

======================================================================
                  BAT GRB EVENT DATA PROCESSING REPORT
    Process Script Ver: batgrbproduct v2.46
    Process Start Time (local time): Sat Jan  5 18:36:52 EST 2013
             Host Name: gcn5
   Current Working Dir: /local/data/raid16/prebascript_archive/trigger543763/SDC
======================================================================

  Trigger: 00543763      Segment: 000

  BAT Trigger Time: 377995485.192   [s; MET]
      Trigger Stop: 377995485.208   [s; MET]
               UTC: 2012-12-23T22:44:35.173140    [includes UTCF correction] 
       Where From?: (*SHORT BURST*) TDRSS scaled map message

  BAT 
    RA: 280.334340766917   Dec: -4.9025483923265  [deg; J2000]

     Catalogged Source?: YES
     Point Source?:      YES
     GRB Indicated?:     NO    [ by BAT flight software ]
     Image S/N Ratio:    7.98
     Image Trigger?:     NO
     Rate S/N Ratio:     24.6576560118759  [ if not an image trigger ]
     Image S/N Ratio:    7.98

  Flight Position:   [ source = BAT ]
    RA: 280.334340766917   Dec: -4.9025483923265  [deg; J2000]

  Ground Position:   [ source = BAT pre-slew burst ]
    RA: 280.302708895821   Dec: -4.91804909267376  [deg; J2000]  
        { 18h 41m 12.7s , -04d 55' 05.0" }
         +/- 2.35751214146969 [arcmin] (estimated 90% radius based on SNR)
         +/- 1.19188108211914 [arcmin] (formal 1-sigma fit error)
    SNR: 8.93390490857424
 
  Angular difference between Flight and Ground position is 2.107287 arcmin
 
  Partial Coding Fraction: 0.359375    [ including projection effects ]

  Duration
     T90: 0.0119999647140503 +/- 0.00894429003608426
        Measured from: 0
                   to: 0.0119999647140503     [s; relative to TRIGTIME]
     T50: 0.0079999566078186 +/- 0.00400000810623169
        Measured from: 0.00400000810623169
                   to: 0.0119999647140503     [s; relative to TRIGTIME]



  Fluence
     Peak Flux  (peak 1 second)
        Measured from: -0.489999949932098     
                   to: 0.510000050067902     [s; relative to TRIGTIME]
     Total Fluence        
        Measured from: 0     
                   to: 0.0160000324249268     [s; relative to TRIGTIME]
     
             Band 1     Band 2     Band 3     Band 4
              15-25      25-50     50-100    100-350     keV
 Total     0.010535   0.020164   0.007667  -0.000675
           0.002377   0.002995   0.001839   0.001146 [error]
 Peak      0.014143   0.011139   0.008338   0.002744
           0.008842   0.008761   0.007583   0.006243 [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 4.31e-09 3.35e-09 1.74e-09 1.31e-09 1.00e-08 1.07e-08   erg/cm2
              Error 1.19e-09 8.57e-10 7.17e-10 9.31e-10 2.50e-09 2.84e-09   erg/cm2
Peak flux Power-law 1.22e-01 8.31e-02 3.68e-02 2.26e-02 2.54e-01 2.66e-01   ph/cm2/s
              Error 1.33e-01 7.85e-02 4.54e-02 6.07e-02 2.23e-01 2.35e-01   ph/cm2/s
 
Fluence   Cutoff-PL 3.61e-09 6.93e-09 1.58e-09 1.18e-11 1.21e-08 0.00e+00   erg/cm2
              Error 1.54e-09 2.28e-09 1.32e-09 7.76e-11 2.70e-09 0.00e+00   erg/cm2
Peak flux Cutoff-PL 6.83e-02 1.16e-01 5.34e-02 3.78e-03 2.43e-01 2.45e-01   ph/cm2/s
              Error 1.21e-01 8.83e-02 7.37e-02 4.77e-02 2.15e-01 2.16e-01   ph/cm2/s
 
Fluence        Band 0.00e+00 0.00e+00 0.00e+00 0.00e+00 0.00e+00 0.00e+00   erg/cm2
              Error 0.00e+00 0.00e+00 0.00e+00 0.00e+00 0.00e+00 0.00e+00   erg/cm2
Peak flux      Band 2.37e-01 0.00e+00 0.00e+00 0.00e+00 0.00e+00 0.00e+00   ph/cm2/s
              Error 0.00e+00 0.00e+00 0.00e+00 0.00e+00 0.00e+00 0.00e+00   ph/cm2/s

 
=== Time-averaged spectral analysis ===
 
Model Ph_index Ph_90err Epeak  Epeak_90err Norm     Nomr_90err chi2   dof
PL    2.940    0.382    -      -           5.35e-02 1.76e-02    0.000 57
CPL  -1.937    5.137      31.3    3.9      5.46e+01 1.62e+06    0.000 56
 
 
=== 1-s peak spectral analysis ===
 
Model Ph_index Ph_90err Epeak  Epeak_90err Norm     Nomr_90err chi2   dof
PL    2.189    2.741    -      -           1.54e-03 1.63e-03    0.000 57
CPL  -0.066    0.000      45.6    0.0      2.35e-02 0.00e+00    0.000 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: 0.000000 sec.
T50 in the 50-300 keV band: 0.000000 sec.

 
=== Table of the duration information ==
 
        Value   tstart    tstop
T100    0.016    0.000    0.016
T90     0.012    0.000    0.012
T50     0.008    0.004    0.012
Peak    1.000   -0.490    0.510

Click here for the BAT GCN circular template

Image

Pre-slew 15-350 keV image (Event data; bkg subtracted)

#   RAcent  DECcent POSerr  Theta    Phi     Peak Cts     SNR  Name
  280.3027  -4.9180 0.0215   36.4 -124.7       0.0390     8.9  TRIG_00543763       
------------------------------------------
 
Foreground time interval of the image:
  0.000   0.016 (delta_t =   0.016 [sec])
Background time interval of the image:
-239.192   0.000 (delta_t = 239.192 [sec])

Lightcurves

Notes:

1) All plots contain as much data as has been downloaded to date.
2) The mask-weighted light curves are using the flight position.
3) Multiple plots of different time binning/intervals are shown to cover all scenarios of short/long GRBs, rate/image triggers, and real/false positives.
4) 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.
5) 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.
6) 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 0.016000

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 0.016000

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 0.016000

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

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

Spectra

Notes:

1) The fitting includes the systematic errors.
2) For long bursts, a spectral fit of 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.
4) For short bursts (T90<1sec), the specrtum is also fit with Blackbody, OTTB, and Double Blackbody.

Time averaged spectrum fit using the pre-slew DRM

Power-law model

Time interval is from    0.000 sec. to    0.016 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 2.94049     ( -0.345555   0.418603 )
Norm@50keV  : 5.34590E-02    ( -0.0179183   0.0172783 )
------------------------------------------------------------
#Test statistic : Chi-Squared =          56.91 using 59 PHA bins.
# Reduced chi-squared =         0.9984 for     57 degrees of freedom 
# Null hypothesis probability =   4.785739e-01
 
Photon flux (15-150 keV)    in 0.016 sec: 14.0844 ( -3.44814  3.44916 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.00049e-08 ( -2.49394e-09  2.49837e-09 ) ergs/cm2

Cutoff power-law model

Time interval is from    0.000 sec. to    0.016 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: -1.93686     ( -7.73145   2.54209 )
Epeak [keV] : 31.2996      ( -2.79253 4.93864 )
Norm@50keV  : 54.5849    ( -73.4326   3.23417e+06 )
------------------------------------------------------------
#Test statistic : Chi-Squared =          45.88 using 59 PHA bins.
# Reduced chi-squared =         0.8193 for     56 degrees of freedom 
# Null hypothesis probability =   8.306000e-01
 
Photon flux (15-150 keV)    in 0.016 sec: 16.0723 ( -3.6343  3.6299 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.21333e-08 ( -2.70638e-09  2.70173e-09 ) ergs/cm2

Band function

Time interval is from    0.000 sec. to    0.016 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : 4.24151   ( -4.42995   -4.24131 )
beta        : -5.66101    ( 5.69067   2.80392 )
Epeak [keV] : 32.2901      ( -4.86273 3.47958 )
Norm@50keV   : 1519.70    ( -1530.39   2590.58 )
------------------------------------------------------------
#Test statistic : Chi-Squared =          45.12 using 59 PHA bins.
# Reduced chi-squared =         0.8203 for     55 degrees of freedom 
# Null hypothesis probability =   8.266109e-01
 
Photon flux (15-150 keV)    in 0.016 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]    : 7.95981  (-1.16434  1.11634)
R^2/D10^2   : 20.8603  (-9.63702   18.9862)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Test statistic : Chi-Squared =          45.91 using 59 PHA bins.
# Reduced chi-squared =         0.8054 for     57 degrees of freedom 
# Null hypothesis probability =   8.535683e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  3.810e-09   1.366e-09
25- 50  6.609e-09   2.078e-09
50-150  1.707e-09   9.261e-10
15-150  1.213e-08   3.456e-09

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 25.2288       (-6.32898      7.91249)
Norm        : 151.554       (-50.4703     68.2163)
------------------------------------------------------------
#Test statistic : Chi-Squared =          50.66 using 59 PHA bins.
# Reduced chi-squared =         0.8887 for     57 degrees of freedom 
# Null hypothesis probability =   7.104498e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  4.467e-09   1.190e-09
25- 50  4.605e-09   1.332e-09
50-150  1.985e-09   1.029e-09
15-150  1.106e-08   2.828e-09

Double BB

kT1 [keV]   : 200.000        (      )
R1^2/D10^2  : 7.73975E-05        (-7.74029e-05      -7.74029e-05)
kT2 [keV]   : 7.84075        (-1.32738      1.19764)
R2^2/D10^2  : 22.0014    (-10.6629   19.214)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          45.91 using 59 PHA bins.
#Test statistic : Chi-Squared =          45.91 using 59 PHA bins.
#Fit statistic : Chi-Squared =          45.85 using 59 PHA bins.
#Test statistic : Chi-Squared =          45.85 using 59 PHA bins.
# Reduced chi-squared =         0.8346 for     55 degrees of freedom 
# Reduced chi-squared =         0.8336 for     55 degrees of freedom 
# Null hypothesis probability =   8.038888e-01
# Null hypothesis probability =   8.055256e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  3.801e-09   3.654e-09
25- 50  6.615e-09   1.857e-06
50-150  1.719e-09   1.987e-05
15-150  1.214e-08   1.380e-05

Peak spectrum fit

Power-law model

Time interval is from   -0.490 sec. to    0.510 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 2.18854     ( -1.45447   4.02713 )
Norm@50keV  : 1.54141E-03    ( -0.00154817   0.00171146 )
------------------------------------------------------------
#Test statistic : Chi-Squared =          68.04 using 59 PHA bins.
# Reduced chi-squared =          1.194 for     57 degrees of freedom 
# Null hypothesis probability =   1.501691e-01
 
Photon flux (15-150 keV)    in 1 sec: 0.253608 ( -0.223392  0.223413 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.45492e-08 ( -1.45492e-08  1.56012e-08 ) ergs/cm2

Cutoff power-law model

Time interval is from   -0.490 sec. to    0.510 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: -6.58544E-02     (     )
Epeak [keV] : 45.5565      (   )
Norm@50keV  : 2.34653E-02    (     )
------------------------------------------------------------
#Test statistic : Chi-Squared =          67.27 using 59 PHA bins.
# Reduced chi-squared =          1.201 for     56 degrees of freedom 
# Null hypothesis probability =   1.438612e-01
 
Photon flux (15-150 keV)    in 1 sec: 0.242673 ( -0.20559  0.223542 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.51547e-08 ( -1.51547e-08  3.03926e-08 ) ergs/cm2

Band function

Time interval is from   -0.490 sec. to    0.510 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : 0.913741   ( -7.22811   -0.913869 )
beta        : -9.37167    ( 9.37167   19.3714 )
Epeak [keV] : 47.9402      ( -35.5428 251.511 )
Norm@50keV   : 5.72628E-02    ( -0.0574058   65.1008 )
------------------------------------------------------------
#Test statistic : Chi-Squared =          67.21 using 59 PHA bins.
# Reduced chi-squared =          1.222 for     55 degrees of freedom 
# Null hypothesis probability =   1.250025e-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]    : 12.4257  (-8.80921  13.4007)
R^2/D10^2   : 6.23127E-02  (-0.0622851   7.03335)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Test statistic : Chi-Squared =          67.18 using 59 PHA bins.
# Reduced chi-squared =          1.179 for     57 degrees of freedom 
# Null hypothesis probability =   1.676987e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  2.039e-09   1.472e-09
25- 50  6.681e-09   4.789e-09
50-150  6.345e-09   5.290e-09
15-150  1.506e-08   1.137e-08

Thermal bremsstrahlung (OTTB)

***Warning: Zero alpha-matrix diagonal element for parameter 2
 Parameter 2 is pegged at 1.47427 due to zero or negative pivot element, likely
 caused by the fit being insensitive to the parameter.
***Warning: Zero alpha-matrix diagonal element for parameter 2
 Parameter 2 is pegged at 1.47427 due to zero or negative pivot element, likely
 caused by the fit being insensitive to the parameter.
***Warning: Zero alpha-matrix diagonal element for parameter 2
 Parameter 2 is pegged at 1.47427 due to zero or negative pivot element, likely
 caused by the fit being insensitive to the parameter.
***Warning: Zero alpha-matrix diagonal element for parameter 2
 Parameter 2 is pegged at 1.47427 due to zero or negative pivot element, likely
 caused by the fit being insensitive to the parameter.
***Warning: Zero alpha-matrix diagonal element for parameter 2
 Parameter 2 is pegged at 1.47427 due to zero or negative pivot element, likely
 caused by the fit being insensitive to the parameter.
***Warning: Zero alpha-matrix diagonal element for parameter 2
 Parameter 2 is pegged at 1.47427 due to zero or negative pivot element, likely
 caused by the fit being insensitive to the parameter.

Double BB

------------------------------------------------------------
#Fit statistic : Chi-Squared =          67.09 using 59 PHA bins.
#Test statistic : Chi-Squared =          67.09 using 59 PHA bins.
#Fit statistic : Chi-Squared =          67.07 using 59 PHA bins.
#Test statistic : Chi-Squared =          67.07 using 59 PHA bins.
#Fit statistic : Chi-Squared =          67.02 using 59 PHA bins.
#Test statistic : Chi-Squared =          67.02 using 59 PHA bins.
# Reduced chi-squared =          1.220 for     55 degrees of freedom 
# Reduced chi-squared =          1.219 for     55 degrees of freedom 
# Reduced chi-squared =          1.219 for     55 degrees of freedom 
# Null hypothesis probability =   1.270816e-01
# Null hypothesis probability =   1.274102e-01
# Null hypothesis probability =   1.282417e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  2.571e-09   1.531e-09
25- 50  6.364e-09   4.150e-09
50-150  6.558e-09   5.240e-09
15-150  1.549e-08   1.299e-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: 2.94049     ( -0.345555   0.418603 )
Norm@50keV  : 5.34590E-02    ( -0.0179183   0.0172783 )
------------------------------------------------------------
#Test statistic : Chi-Squared =          56.91 using 59 PHA bins.
# Reduced chi-squared =         0.9984 for     57 degrees of freedom 
# Null hypothesis probability =   4.785739e-01
 
Photon flux (15-150 keV)    in 0.016 sec: 14.0844 ( -3.44814  3.44916 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.00049e-08 ( -2.49394e-09  2.49837e-09 ) ergs/cm2

Cutoff power-law model

Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: -1.93686     ( -7.73145   2.54209 )
Epeak [keV] : 31.2996      ( -2.79253 4.93864 )
Norm@50keV  : 54.5849    ( -73.4326   3.23417e+06 )
------------------------------------------------------------
#Test statistic : Chi-Squared =          45.88 using 59 PHA bins.
# Reduced chi-squared =         0.8193 for     56 degrees of freedom 
# Null hypothesis probability =   8.306000e-01
 
Photon flux (15-150 keV)    in 0.016 sec: 16.0723 ( -3.6343  3.6299 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.21333e-08 ( -2.70638e-09  2.70173e-09 ) ergs/cm2

Band function

 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : 4.24151   ( -4.42995   -4.24131 )
beta        : -5.66101    ( 5.69067   2.80392 )
Epeak [keV] : 32.2901      ( -4.86273 3.47958 )
Norm@50keV   : 1519.70    ( -1530.39   2509.89 )
------------------------------------------------------------
#Test statistic : Chi-Squared =          45.12 using 59 PHA bins.
# Reduced chi-squared =         0.8203 for     55 degrees of freedom 
# Null hypothesis probability =   8.266109e-01
 
Photon flux (15-150 keV)    in 0.016 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)  = 3.34766e-09
S(50-100 keV) = 1.74386e-09

T90 vs. Hardness ratio plot

T90                                   = 0.0119999647140503 sec.
Hardness ratio (energy fluence ratio) = 0.520919

Color vs. Color plot

Count Ratio  (25-50 keV) / (15-25 keV) = 1.914
Count Ratio (50-100 keV) / (15-25 keV) = 0.727765

Mask shadow pattern

IMX = -4.192406304446508E-01, IMY = 6.052095270190621E-01

TIME vs. PHA plot around the trigger time

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.016000

TIME vs. DetID plot around the trigger time

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.016000

100 us light curve (15-350 keV)

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.016000

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:
-239.192000 0.000000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
244.9835 -15.6284    0.5  38.5  -63.2   8.2256  21.4    0.7	Sco X-1                       
254.2729  35.3661   70.1  13.7   98.9   0.0309   0.2    9.2	Her X-1                       
268.4039  -1.4288    3.4  26.6 -110.0   0.7875   3.4    2.6	SW J1753.5-0127               
274.1168 -13.9526    4.0  40.3 -108.2   1.6806   2.9    8.2	GX 17+2                       
288.7943  10.9365    2.5  34.1 -155.9   0.9558   4.6    0.6	GRS 1915+105                  
299.6118  35.2291    1.7  41.2  162.0   2.2611   7.0    2.0	Cyg X-1                       
308.1491  40.9917    4.7  48.5  155.0   1.4358   2.5    2.9	Cyg X-3                       
226.3867  54.9610    2.9  39.6   75.8   2.8800   4.0 ------	UNKNOWN                       
314.3594  40.5823    2.6  53.2  156.0   4.1321   4.4 ------	UNKNOWN                       
293.0990   8.6984    2.7  38.9 -155.2   1.0596   4.3 ------	UNKNOWN

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

Time interval of the image:
0.000000 0.016000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
245.1518 -15.7491   25.6  38.6  -63.5  -0.0025  -0.5   11.9	Sco X-1                       
254.6096  35.4627   38.0  13.8  100.1  -0.0005  -0.3   10.4	Her X-1                       
268.5194  -1.5746    0.0  26.7 -110.1   0.0019   0.6   11.7	SW J1753.5-0127               
274.1370 -14.1368   48.0  40.4 -108.1  -0.0022  -0.2    9.7	GX 17+2                       
288.7977  10.9454  929.4  34.1 -155.9   0.0000   0.0    0.0	GRS 1915+105                  
299.5370  35.0924    7.5  41.1  162.2  -0.0042  -1.5    7.1	Cyg X-1                       
308.0212  41.0319    3.0  48.4  155.0  -0.0151  -3.9    6.2	Cyg X-3                       
301.7815  46.7327    2.3  45.2  146.1   0.0171   5.0 ------	UNKNOWN                       
280.3027  -4.9181    1.3  36.4 -124.7   0.0390   8.9 ------	UNKNOWN

Post-slew image of 15-350 keV band

Time interval of the image:
299.508610 962.928000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
 61.4702 -39.9266    3.2  10.9 -160.8   1.2649   3.6 ------	UNKNOWN                       
 42.5708 -40.9373    5.0  13.1  -87.4   0.8093   2.3 ------	UNKNOWN                       
355.6505 -24.9492    3.9  50.8  -44.5   5.5541   3.0 ------	UNKNOWN

Plot creation:
Sun Jan  6 03:46:46 EST 2013