batgrbproduct analysis for trigger=550906

batgrbproduct Analysis for Trigger=550906

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): Sun Jan 12 05:06:49 EST 2014
             Host Name: batevent1
   Current Working Dir: /local/data/batevent/batevent_reproc/trigger550906
======================================================================

  Trigger: 00550906      Segment: 000

  BAT Trigger Time: 384883701.376   [s; MET]
      Trigger Stop: 384883701.504   [s; MET]
               UTC: 2013-03-13T16:08:11.057240    [includes UTCF correction] 
       Where From?: TDRSS position message

  BAT 
    RA: 236.42303778442   Dec: -0.361783296507332  [deg; J2000]

     Catalogged Source?: NO
     Point Source?:      YES
     GRB Indicated?:     YES    [ by BAT flight software ]
     Image S/N Ratio:    7.95
     Image Trigger?:     NO
     Rate S/N Ratio:     12.9228479833201  [ if not an image trigger ]
     Image S/N Ratio:    7.95

  Flight Position:   [ source = BAT ]
    RA: 236.42303778442   Dec: -0.361783296507332  [deg; J2000]

  Ground Position:   [ source = BAT pre-slew burst ]
    RA: 236.437591682223   Dec: -0.360699108529194  [deg; J2000]  
        { 15h 45m 45.0s , -00d 21' 38.5" }
         +/- 2.39180430748566 [arcmin] (estimated 90% radius based on SNR)
         +/- 1.09537422327281 [arcmin] (formal 1-sigma fit error)
    SNR: 8.75148486701875
 
  Angular difference between Flight and Ground position is 0.875636 arcmin
 
  Partial Coding Fraction: 0.828125    [ including projection effects ]

  Duration
     T90: 0.171999931335449 +/- 0.0357770801763245
        Measured from: 0.0200000405311584
                   to: 0.191999971866608     [s; relative to TRIGTIME]
     T50: 0.0839999318122864 +/- 0.0393954323691675
        Measured from: 0.0440000295639038
                   to: 0.12799996137619     [s; relative to TRIGTIME]



  Fluence
     Peak Flux  (peak 1 second)
        Measured from: -0.38400000333786     
                   to: 0.61599999666214     [s; relative to TRIGTIME]
     Total Fluence        
        Measured from: 0.0120000243186951     
                   to: 0.216000020503998     [s; relative to TRIGTIME]
     
             Band 1     Band 2     Band 3     Band 4
              15-25      25-50     50-100    100-350     keV
 Total     0.015219   0.015743   0.015893   0.004812
           0.003270   0.003082   0.002879   0.002173 [error]
 Peak      0.015763   0.019607   0.018934   0.005267
           0.006515   0.005975   0.005202   0.004325 [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 4.00e-09 7.32e-09 1.03e-08 3.03e-08 2.95e-08 5.20e-08   erg/cm2
              Error 1.28e-09 1.43e-09 2.69e-09 1.73e-08 6.44e-09 1.94e-08   erg/cm2
Peak flux Power-law 1.31e-01 1.50e-01 1.24e-01 1.70e-01 4.67e-01 5.75e-01   ph/cm2/s
              Error 7.10e-02 5.07e-02 4.16e-02 1.23e-01 1.41e-01 1.72e-01   ph/cm2/s
 
Fluence   Cutoff-PL 3.90e-09 7.45e-09 1.04e-08 2.38e-08 2.92e-08 4.54e-08   erg/cm2
              Error 1.44e-09 1.66e-09 2.87e-09 1.87e-08 6.86e-09 2.47e-08   erg/cm2
Peak flux Cutoff-PL 8.83e-02 1.59e-01 1.41e-01 5.63e-02 4.29e-01 4.45e-01   ph/cm2/s
              Error 8.68e-02 6.24e-02 5.31e-02 1.27e-01 1.52e-01 2.05e-01   ph/cm2/s
 
Fluence        Band -------- -------- -------- -------- -------- --------   erg/cm2
              Error -------- -------- -------- -------- -------- --------   erg/cm2
Peak flux      Band 9.07e-02 1.59e-01 1.40e-01 6.01e-02 4.33e-01 4.50e-01   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    1.508    0.345    -      -           1.53e-02 3.00e-03   68.200 57
CPL   1.354    1.511     210.1    0.0      1.83e-02 5.07e-02   68.160 56
 
 
=== 1-s peak spectral analysis ===
 
Model Ph_index Ph_90err Epeak  Epeak_90err Norm     Nomr_90err chi2   dof
PL    1.282    0.512    -      -           3.92e-03 1.14e-03   49.150 57
CPL  -0.210    3.131      81.9  -25.4      1.85e-02 4.94e-01   47.930 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    0.204    0.012    0.216
T90     0.172    0.020    0.192
T50     0.084    0.044    0.128
Peak    1.000   -0.384    0.616

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
  236.4376    -0.3607   0.0219    20.8065   -50.5674         0.0474488      8.751 TRIG_00550906                 
 
Foreground time interval of the image:
  0.012   0.216 (delta_t =   0.204 [sec])
Background time interval of the image:
-239.376   0.012 (delta_t = 239.388 [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 0.128000

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 0.128000

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 0.128000

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    0.012 sec. to    0.216 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.50836     ( -0.338699   0.350597 )
Norm@50keV  : 1.52537E-02    ( -0.0030302   0.00297764 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          68.20 using 59 PHA bins.
# Reduced chi-squared =          1.197 for     57 degrees of freedom 
# Null hypothesis probability =   1.470537e-01
 
Photon flux (15-150 keV)    in 0.204 sec: 1.90858 ( -0.363446  0.364374 ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.94798e-08 ( -6.36517e-09  6.50727e-09 ) ergs/cm2

Cutoff power-law model

Time interval is from    0.012 sec. to    0.216 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.35363     ( -1.51762   1.50512 )
Epeak [keV] : 210.124      ( -210.021 -210.021 )
Norm@50keV  : 1.82648E-02    ( -0.018267   0.0832145 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          68.16 using 59 PHA bins.
# Reduced chi-squared =          1.217 for     56 degrees of freedom 
# Null hypothesis probability =   1.277779e-01
 
Photon flux (15-150 keV)    in 0.204 sec: 1.89505 ( -0.37941  0.37333 ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.9152e-08 ( -6.94661e-09  6.76505e-09 ) ergs/cm2

Band function

Time interval is from    0.012 sec. to    0.216 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -1.34086   ( -0.475301   0.803797 )
beta        : -8.90684    ( 9.33545   19.2673 )
Epeak [keV] : 202.004      ( -142.94 -201.927 )
Norm@50keV   : 1.82501E-02    ( -0.0062019   0.0251662 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          68.17 using 59 PHA bins.
# Reduced chi-squared =          1.239 for     55 degrees of freedom 
# Null hypothesis probability =   1.093416e-01
 
Photon flux (15-150 keV)    in 0.204 sec: 1.89062 (    ) 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]    : 15.3639  (-3.48498  4.55008)
R^2/D10^2   : 0.197595  (-0.117158   0.284568)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          75.10 using 59 PHA bins.
# Reduced chi-squared =          1.318 for     57 degrees of freedom 
# Null hypothesis probability =   5.435722e-02
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.984e-09   7.191e-10
25- 50  8.056e-09   2.647e-09
50-150  1.308e-08   5.434e-09
15-150  2.312e-08   7.926e-09

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 199.360       (-108.785      -199.362)
Norm        : 7.79155       (-1.46182     1.46335)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          68.27 using 59 PHA bins.
# Reduced chi-squared =          1.198 for     57 degrees of freedom 
# Null hypothesis probability =   1.458535e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  3.958e-09   2.326e-09
25- 50  7.614e-09   4.401e-09
50-150  1.670e-08   9.583e-09
15-150  2.827e-08   1.647e-08

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 5.02776        (-2.46327      5.34726)
R1^2/D10^2  : 6.41094        (-5.84885      154.937)
kT2 [keV]   : 22.0426        (-6.69239      31.7975)
R2^2/D10^2  : 4.87038E-02    (-0.0461678   0.0777359)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          67.92 using 59 PHA bins.
# Reduced chi-squared =          1.235 for     55 degrees of freedom 
# Null hypothesis probability =   1.133250e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  4.144e-09   2.348e-09
25- 50  6.878e-09   3.721e-09
50-150  1.724e-08   1.003e-08
15-150  2.827e-08   1.515e-08

Peak spectrum fit

Power-law model

Time interval is from   -0.384 sec. to    0.616 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.28194     ( -0.516997   0.506561 )
Norm@50keV  : 3.92435E-03    ( -0.00113948   0.00113917 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          49.15 using 59 PHA bins.
# Reduced chi-squared =         0.8623 for     57 degrees of freedom 
# Null hypothesis probability =   7.606453e-01
 
Photon flux (15-150 keV)    in 1 sec: 0.466667 ( -0.139834  0.141327 ) ph/cm2/s
Energy fluence (15-150 keV)             : 3.8953e-08 ( -1.21902e-08  1.24917e-08 ) ergs/cm2

Cutoff power-law model

Time interval is from   -0.384 sec. to    0.616 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: -0.209759     ( -4.38636   1.87551 )
Epeak [keV] : 81.9378      ( -30.9551 -81.6843 )
Norm@50keV  : 1.84846E-02    ( -0.0188137   0.96883 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          47.93 using 59 PHA bins.
# Reduced chi-squared =         0.8559 for     56 degrees of freedom 
# Null hypothesis probability =   7.698955e-01
 
Photon flux (15-150 keV)    in 1 sec: 0.429418 ( -0.151368  0.153074 ) ph/cm2/s
Energy fluence (15-150 keV)             : 3.57965e-08 ( -1.25539e-08  1.34621e-08 ) ergs/cm2

Band function

Time interval is from   -0.384 sec. to    0.616 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : 0.211561   ( -1.40748   4.40653 )
beta        : -10.0000    ( 10   1.77636e-14 )
Epeak [keV] : 81.6465      ( -28.4185 155.197 )
Norm@50keV   : 1.86138E-02    ( -0.0185951   0.966491 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          47.93 using 59 PHA bins.
# Reduced chi-squared =         0.8715 for     55 degrees of freedom 
# Null hypothesis probability =   7.391597e-01
 
Photon flux (15-150 keV)    in 1 sec: 0.432565 (    ) ph/cm2/s
Energy fluence (15-150 keV)             : 3.64427e-08 ( 0  0 ) ergs/cm2

Single BB

 
Spectral model blackbody:
------------------------------------------------------------
Parameters  : value    Lower 90%  Upper 90%
kT [keV]    : 18.4460  (-5.08261  7.77521)
R^2/D10^2   : 2.82860E-02  (-0.028286   0.0559881)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          48.25 using 59 PHA bins.
# Reduced chi-squared =         0.8465 for     57 degrees of freedom 
# Null hypothesis probability =   7.887384e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.911e-09   1.221e-09
25- 50  9.001e-09   5.310e-09
50-150  2.237e-08   1.419e-08
15-150  3.328e-08   1.947e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 199.363       (-112.791      -199.363)
Norm        : 1.95467       (-0.571218     0.571235)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          49.59 using 59 PHA bins.
# Reduced chi-squared =         0.8700 for     57 degrees of freedom 
# Null hypothesis probability =   7.465110e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  4.867e-09   2.953e-09
25- 50  9.363e-09   5.740e-09
50-150  2.054e-08   1.221e-08
15-150  3.477e-08   2.112e-08

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 2.71432        (-2.71165      21.8654)
R1^2/D10^2  : 17.1801        (-17.3377      2.77557e+06)
kT2 [keV]   : 19.5255        (-5.68842      -19.5235)
R2^2/D10^2  : 2.27374E-02    (-0.0227464   0.04726)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          47.43 using 59 PHA bins.
# Reduced chi-squared =         0.8623 for     55 degrees of freedom 
# Null hypothesis probability =   7.561320e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  3.365e-09   1.469e-09
25- 50  8.438e-09   4.990e-09
50-150  2.328e-08   1.515e-08
15-150  3.508e-08   2.093e-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: 1.50836     ( -0.338699   0.350597 )
Norm@50keV  : 1.52537E-02    ( -0.0030302   0.00297764 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          68.20 using 59 PHA bins.
# Reduced chi-squared =          1.197 for     57 degrees of freedom 
# Null hypothesis probability =   1.470537e-01
 
Photon flux (15-150 keV)    in 0.204 sec: 1.90858 ( -0.363446  0.364374 ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.94798e-08 ( -6.36517e-09  6.50727e-09 ) ergs/cm2

Cutoff power-law model

Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.35363     ( -1.51762   1.50512 )
Epeak [keV] : 210.124      ( -210.021 -210.021 )
Norm@50keV  : 1.82648E-02    ( -0.018267   0.0832145 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          68.16 using 59 PHA bins.
# Reduced chi-squared =          1.217 for     56 degrees of freedom 
# Null hypothesis probability =   1.277779e-01
 
Photon flux (15-150 keV)    in 0.204 sec: 1.89505 ( -0.37941  0.37333 ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.9152e-08 ( -6.9464e-09  6.76525e-09 ) ergs/cm2

Band function

 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -1.34086   ( -0.475301   0.803797 )
beta        : -8.90684    ( 9.33545   19.2673 )
Epeak [keV] : 202.004      ( -142.94 -201.927 )
Norm@50keV   : 1.82501E-02    ( -0.0062019   0.0251662 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          68.17 using 59 PHA bins.
# Reduced chi-squared =          1.239 for     55 degrees of freedom 
# Null hypothesis probability =   1.093416e-01
 
Photon flux (15-150 keV)    in 0.204 sec: 1.89062 (    ) 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)  = 7.32e-09
S(50-100 keV) = 1.03e-08

T90 vs. Hardness ratio plot

T90                                   = 0.171999931335449 sec.
Hardness ratio (energy fluence ratio) = 1.4071

Color vs. Color plot

Count Ratio  (25-50 keV) / (15-25 keV) = 1.03443
Count Ratio (50-100 keV) / (15-25 keV) = 1.04429

Mask shadow pattern

IMX = 2.413613012851211E-01, IMY = 2.934972487999810E-01

TIME vs. PHA plot around the trigger time

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.128000

TIME vs. DetID plot around the trigger time

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.128000

100 us light curve (15-350 keV)

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.128000

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:
-239.376000 0.012000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
244.9914 -15.6290    0.3  36.8  -35.4  11.0677  38.5    1.0	Sco X-1                       
254.4862  35.3010    2.1  41.7 -122.3   3.0056   5.6    2.9	Her X-1                       
256.4363 -36.4226   28.2  58.6  -24.6  -0.5161  -0.4    0.1	GX 349+2                      
217.9715 -12.7768    2.3  22.6   11.7   1.0604   5.1 ------	UNKNOWN                       
194.6483  64.3165    5.0  56.9  179.2   3.0634   2.3 ------	UNKNOWN                       
235.2787 -31.0277    3.1  44.0  -10.1   1.2410   3.7 ------	UNKNOWN                       
237.6448  20.0085    2.9  21.3 -109.6   0.8942   3.9 ------	UNKNOWN                       
249.2227 -23.5676    2.9  45.1  -30.7   1.4218   4.0 ------	UNKNOWN

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

Time interval of the image:
0.012000 0.216000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
245.1278 -15.7412    0.0  36.9  -35.4  -0.0056  -0.7   10.5	Sco X-1                       
254.3811  35.3833    3.9  41.6 -122.5  -0.0420  -3.0    4.5	Her X-1                       
256.3819 -36.4673    4.6  58.6  -24.5   0.0865   2.5    3.7	GX 349+2                      
177.0559  52.3907    2.8  54.0  161.3   0.1164   4.2 ------	UNKNOWN                       
226.3771 -46.3851    2.3  56.7    4.4   0.1388   5.0 ------	UNKNOWN                       
192.8818  63.6299    2.4  56.7  177.9   0.1321   4.8 ------	UNKNOWN                       
225.9512   2.2044    2.3  10.8  -34.6   0.0249   5.0 ------	UNKNOWN                       
236.4376  -0.3607    1.3  20.8  -50.6   0.0475   8.8 ------	UNKNOWN

Post-slew image of 15-350 keV band

Time interval of the image:
62.124600 962.701900
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
244.9760 -15.6333    0.2  17.5  -31.7  45.2120  77.1    0.5	Sco X-1                       
254.4550  35.3534    1.6  39.5 -159.6   7.1087   7.4    0.7	Her X-1                       
255.8338 -37.9453   67.8  41.6  -26.3   0.1745   0.2    9.4	4U 1700-377                   
256.3859 -36.3945    5.4  40.5  -28.1   2.0797   2.1    2.9	GX 349+2                      
263.1583 -24.7722   81.9  35.6  -47.7   0.1298   0.1    8.3	GX 1+4                        
264.6692 -44.4777    4.4  50.7  -28.9   4.0693   2.6    3.6	4U 1735-44                    
268.2504  -1.4948    3.4  31.9  -90.8   3.5107   3.4    7.5	SW J1753.5-0127               
270.4358 -24.9733    7.8  41.1  -53.6   2.2056   1.5   10.4	GX 5-1                        
270.4246 -25.5863    5.9  41.4  -52.8   3.1063   2.0   11.5	GRS 1758-258                  
274.0094 -13.9156    4.3  39.6  -71.4   4.7146   2.7    7.3	GX 17+2                       
275.8374 -30.2636    5.8  47.9  -50.7   5.8541   2.0    7.7	H1820-303                     
263.0014 -33.8951    2.5  41.8  -36.9   5.1748   4.7    3.7	GX 354-0                      
269.7316  51.1748    3.8  58.8 -159.3  14.8451   3.1 ------	UNKNOWN                       
272.5304 -33.9715    2.7  47.7  -44.4   8.6622   4.2 ------	UNKNOWN                       
275.6183 -37.8963    2.4  52.0  -42.3  15.7233   4.8 ------	UNKNOWN

Plot creation:
Sat May 30 17:15:45 EDT 2015