batgrbproduct analysis for trigger=313299

batgrbproduct Analysis for Trigger=313299

Analysis Summary

Notes:

1) No attempt has been made to eliminate the non-significant decimal places.
2) This batgrbproduct analysis is done using the HEASARC data.
3) This batgrbproduct analysis is using the flight position for the mask-weighting calculation.

======================================================================
                  BAT GRB EVENT DATA PROCESSING REPORT
    Process Script Ver: batgrbproduct v2.46
    Process Start Time (local time): Mon Jan 20 01:18:58 EST 2014
             Host Name: batevent1
   Current Working Dir: /local/data/batevent/batevent_reproc/trigger313299
======================================================================

  Trigger: 00313299      Segment: 000

  BAT Trigger Time: 234402480.704   [s; MET]
      Trigger Stop: 234402481.728   [s; MET]
               UTC: 2008-06-05T23:47:57.859480    [includes UTCF correction] 
       Where From?: TDRSS position message

  BAT 
    RA: 262.127299384762   Dec: 4.00166807477933  [deg; J2000]

     Catalogged Source?: NO
     Point Source?:      YES
     GRB Indicated?:     YES    [ by BAT flight software ]
     Image S/N Ratio:    25.82
     Image Trigger?:     NO
     Rate S/N Ratio:     120.743529847359  [ if not an image trigger ]
     Image S/N Ratio:    25.82

  Flight Position:   [ source = BAT ]
    RA: 262.127299384762   Dec: 4.00166807477933  [deg; J2000]

  Ground Position:   [ source = BAT pre-slew burst ]
    RA: 262.129984962012   Dec: 4.00907888034348  [deg; J2000]  
        { 17h 28m 31.2s , +04d 00' 32.7" }
         +/- 0.558082704217376 [arcmin] (estimated 90% radius based on SNR)
         +/- 0.158187564979418 [arcmin] (formal 1-sigma fit error)
    SNR: 69.9805860664166
 
  Angular difference between Flight and Ground position is 0.472811 arcmin
 
  Partial Coding Fraction: 0.4140625    [ including projection effects ]

  Duration
     T90: 18.055999994278 +/- 0.888225208353073
        Measured from: -2.80399999022484
                   to: 15.2520000040531     [s; relative to TRIGTIME]
     T50: 7.06000000238419 +/- 0.116275537741645
        Measured from: 2.31600001454353
                   to: 9.37600001692772     [s; relative to TRIGTIME]



  Fluence
     Peak Flux  (peak 1 second)
        Measured from: 7.57199999690056     
                   to: 8.57199999690056     [s; relative to TRIGTIME]
     Total Fluence        
        Measured from: -5.53200000524521     
                   to: 22.5760000050068     [s; relative to TRIGTIME]
     
             Band 1     Band 2     Band 3     Band 4
              15-25      25-50     50-100    100-350     keV
 Total     4.289878   7.224310   6.262940   1.831162
           0.060148   0.069483   0.068050   0.057761 [error]
 Peak      0.395359   0.835084   0.926597   0.355922
           0.015363   0.020385   0.022146   0.017162 [error]

     [ fluence units of on-axis counts / fully illuminated detector ] 

======================================================================
 
=== Fluence/Peak Flux Summary ===
 
              Model    Band1    Band2    Band3    Band4    Band5    Total      
                       15-25    25-50   50-100  100-350   15-150   15-350   keV
Fluence   Power-law 1.49e-06 3.06e-06 4.88e-06 1.74e-05 1.35e-05 2.68e-05   erg/cm2
              Error 5.26e-08 6.26e-08 8.31e-08 7.10e-07 2.13e-07 7.32e-07   erg/cm2
Peak flux Power-law 4.17e+00 5.88e+00 6.14e+00 1.18e+01 1.99e+01 2.80e+01   ph/cm2/s
              Error 2.47e-01 2.10e-01 1.81e-01 7.68e-01 5.63e-01 8.68e-01   ph/cm2/s
 
Fluence   Cutoff-PL 1.41e-06 3.07e-06 4.98e-06 1.42e-05 1.34e-05 2.36e-05   erg/cm2
              Error 7.22e-08 6.42e-08 1.03e-07 1.93e-06 2.27e-07 1.92e-06   erg/cm2
Peak flux Cutoff-PL 3.91e+00 5.93e+00 6.31e+00 9.49e+00 1.97e+01 2.56e+01   ph/cm2/s
              Error 3.22e-01 2.19e-01 2.33e-01 1.74e+00 5.81e-01 1.84e+00   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    1.324    0.030    -      -           4.90e-02 7.82e-04   37.900 57
CPL   1.146    0.120     290.7  256.9      5.81e-02 6.53e-03   31.320 56
 
 
=== 1-s peak spectral analysis ===
 
Model Ph_index Ph_90err Epeak  Epeak_90err Norm     Nomr_90err chi2   dof
PL    0.938    0.049    -      -           1.73e-01 4.85e-03   42.370 57
CPL   0.714    0.189     344.1 1165.9      2.16e-01 3.92e-02   38.290 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: 16.320000 sec.
T50 in the 50-300 keV band: 6.656000 sec.

 
=== Table of the duration information ==
 
        Value   tstart    tstop
T100   28.108   -5.532   22.576
T90    18.056   -2.804   15.252
T50     7.060    2.316    9.376
Peak    1.000    7.572    8.572

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
  262.1300     4.0091   0.0027    29.5847    63.8919        17.4523451     69.981 TRIG_00313299                 
 
Foreground time interval of the image:
 -5.532  11.197 (delta_t =  16.729 [sec])
Background time interval of the image:
-219.803  -5.532 (delta_t = 214.271 [sec])

Lightcurves

Notes:

1) The mask-weighted light curves are using the flight position.
2) Multiple plots of different time binning/intervals are shown to cover all scenarios of short/long GRBs, rate/image triggers, and real/false positives.
3) For all the mask-weighted lightcurves, the y-axis units are counts/sec/det where a det is 0.4 x 0.4 = 0.16 sq cm.
4) The verticle lines correspond to following: green dotted lines are T50 interval, black dotted lines are T90 interval, blue solid line(s) is a spacecraft slew start time, and orange solid line(s) is a spacecraft slew end time.
5) Time of each bin is in the middle of the bin.

1 s binning

From T0-310 s to T0+310 s

From T100_start - 20 s to T100_end + 30 s

Full time interval

64 ms binning

Full time interval

From T100_start to T100_end

From T0-5 sec to T0+5 sec

16 ms binning

From T100_start-5 s to T100_start+5 s

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.024000

8 ms binning

From T100_start-3 s to T100_start+3 s

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.024000

2 ms binning

From T100_start-1 s to T100_start+1 s

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.024000

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

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

Quad-rate summed light curves (from T0-300s to T0+1000s)

Spectral Evolution

Spectra

Notes:

1) The fitting includes the systematic errors.
2) When the burst includes telescope slew time periods, the fitting uses an average response file made from multiple 5-s response files through out the slew time plus single time preiod for the non-slew times, and weighted by the total counts in the corresponding time period using addrmf. An average response file is needed becuase a spectral fit using the pre-slew DRM will introduce some errors in both a spectral shape and a normalization if the PHA file contains a lot of the slew/post-slew time interval.
3) For fits to more complicated models (e.g. a power-law over a cutoff power-law), the BAT team has decided to require a chi-square improvement of more than 6 for each extra dof.

Time averaged spectrum fit using the average DRM

Power-law model

Time interval is from   -5.532 sec. to   22.576 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.32397     ( -0.0297382   0.0296608 )
Norm@50keV  : 4.90480E-02    ( -0.000782837   0.000782077 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          37.90 using 59 PHA bins.
# Reduced chi-squared =         0.6649 for     57 degrees of freedom 
# Null hypothesis probability =   9.758903e-01
 
Photon flux (15-150 keV)    in 28.11 sec: 5.87817 ( -0.107208  0.107525 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.35465e-05 ( -2.13218e-07  2.13281e-07 ) ergs/cm2

Cutoff power-law model

Time interval is from   -5.532 sec. to   22.576 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.14604     ( -0.121858   0.118705 )
Epeak [keV] : 290.670      ( -92.5853 421.182 )
Norm@50keV  : 5.81274E-02    ( -0.00609048   0.00696947 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          31.32 using 59 PHA bins.
# Reduced chi-squared =         0.5592 for     56 degrees of freedom 
# Null hypothesis probability =   9.969155e-01
 
Photon flux (15-150 keV)    in 28.11 sec: 5.79265 ( -0.11943  0.12007 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.34394e-05 ( -2.27185e-07  2.2651e-07 ) ergs/cm2

Band function

Time interval is from   -5.532 sec. to   22.576 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -0.321657   ( -0.622011   3.73718 )
beta        : -1.37923    ( -0.0493393   0.0466874 )
Epeak [keV] : 61.9779      ( -30.4366 63.1859 )
Norm@50keV   : 0.187886    ( -0.112494   35.0233 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          25.95 using 59 PHA bins.
# Reduced chi-squared =         0.4718 for     55 degrees of freedom 
# Null hypothesis probability =   9.997039e-01
 
Photon flux (15-150 keV)    in 28.11 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]    : 20.2590  (  )
R^2/D10^2   : 0.242103  (   )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =         772.10 using 59 PHA bins.
# Reduced chi-squared =         13.546 for     57 degrees of freedom 
# Null hypothesis probability =  5.586625e-126
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  5.357e-07   1.841e-08
25- 50  2.691e-06   6.254e-08
50-150  8.202e-06   1.968e-07
15-150  1.143e-05   1.911e-07

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 199.363       (      )
Norm        : 25.3549       (     )
------------------------------------------------------------
#Fit statistic : Chi-Squared =         274.75 using 59 PHA bins.
# Reduced chi-squared =         4.8201 for     57 degrees of freedom 
# Null hypothesis probability =   2.946750e-30
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.775e-06   3.120e-08
25- 50  3.414e-06   6.325e-08
50-150  7.487e-06   1.377e-07
15-150  1.268e-05   2.193e-07

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 8.69030        (-0.536087      0.56263)
R1^2/D10^2  : 2.55562        (-0.465552      0.598008)
kT2 [keV]   : 33.5727        (-2.0355      2.45302)
R2^2/D10^2  : 3.69765E-02    (-0.00779913   0.00886596)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          24.98 using 59 PHA bins.
# Reduced chi-squared =         0.4541 for     55 degrees of freedom 
# Null hypothesis probability =   9.998363e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.207e-06   7.632e-08
25- 50  3.182e-06   9.276e-08
50-150  9.015e-06   2.881e-07
15-150  1.340e-05   3.584e-07

Peak spectrum fit

Power-law model

Time interval is from    7.572 sec. to    8.572 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 0.937964     ( -0.0492884   0.0490162 )
Norm@50keV  : 0.173330    ( -0.00485224   0.0048458 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          42.37 using 59 PHA bins.
# Reduced chi-squared =         0.7434 for     57 degrees of freedom 
# Null hypothesis probability =   9.257152e-01
 
Photon flux (15-150 keV)    in 1 sec: 19.9071 ( -0.562539  0.563046 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.91723e-06 ( -5.74613e-08  5.75418e-08 ) ergs/cm2

Cutoff power-law model

Time interval is from    7.572 sec. to    8.572 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 0.714137     ( -0.198396   0.179326 )
Epeak [keV] : 344.136      ( -132.467 2199.38 )
Norm@50keV  : 0.216077    ( -0.0333369   0.045077 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          38.29 using 59 PHA bins.
# Reduced chi-squared =         0.6838 for     56 degrees of freedom 
# Null hypothesis probability =   9.661218e-01
 
Photon flux (15-150 keV)    in 1 sec: 19.7274 ( -0.5807  0.5812 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.90293e-06 ( 0  0 ) ergs/cm2

Band function

Time interval is from    7.572 sec. to    8.572 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : 4.99996   ( -1.30699e-05   -4.99996 )
beta        : -0.976219    ( -0.0533926   0.0532348 )
Epeak [keV] : 28.5594      ( -5.96968 3.37697 )
Norm@50keV   : 5071.08    ( -138.418   14709.8 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          38.11 using 59 PHA bins.
# Reduced chi-squared =         0.6929 for     55 degrees of freedom 
# Null hypothesis probability =   9.597555e-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]    : 23.5054  (  )
R^2/D10^2   : 0.591209  (   )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =         234.27 using 59 PHA bins.
# Reduced chi-squared =         4.1100 for     57 degrees of freedom 
# Null hypothesis probability =   2.364655e-23
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  5.857e-08   3.450e-09
25- 50  3.216e-07   1.370e-08
50-150  1.326e-06   5.500e-08
15-150  1.706e-06   5.550e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 199.363       (      )
Norm        : 80.2168       (     )
------------------------------------------------------------
#Fit statistic : Chi-Squared =         455.76 using 59 PHA bins.
# Reduced chi-squared =         7.9957 for     57 degrees of freedom 
# Null hypothesis probability =   1.470179e-63
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.997e-07   5.600e-09
25- 50  3.842e-07   1.110e-08
50-150  8.427e-07   2.445e-08
15-150  1.427e-06   4.200e-08

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 9.56350        (-1.15866      1.28137)
R1^2/D10^2  : 5.02886        (-1.45631      2.26752)
kT2 [keV]   : 39.6221        (-4.48832      6.6466)
R2^2/D10^2  : 0.103160    (-0.0380182   0.0467967)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          34.15 using 59 PHA bins.
# Reduced chi-squared =         0.6209 for     55 degrees of freedom 
# Null hypothesis probability =   9.877631e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.132e-07   1.169e-08
25- 50  3.578e-07   2.705e-08
50-150  1.450e-06   1.485e-07
15-150  1.921e-06   1.425e-07

Pre-slew spectrum (Pre-slew PHA with pre-slew DRM)

Power-law model

 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.23209     ( -0.0289808   0.0288908 )
Norm@50keV  : 7.18336E-02    ( -0.00114662   0.00114516 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          44.60 using 59 PHA bins.
# Reduced chi-squared =         0.7825 for     57 degrees of freedom 
# Null hypothesis probability =   8.837655e-01
 
Photon flux (15-150 keV)    in 16.73 sec: 8.47186 ( -0.150361  0.150727 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.20849e-05 ( -1.88525e-07  1.88564e-07 ) ergs/cm2

Cutoff power-law model

Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.02120     ( -0.119402   0.11639 )
Epeak [keV] : 286.355      ( -80.2631 258.967 )
Norm@50keV  : 8.75656E-02    ( -0.0088697   0.0100952 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          34.91 using 59 PHA bins.
# Reduced chi-squared =         0.6233 for     56 degrees of freedom 
# Null hypothesis probability =   9.878805e-01
 
Photon flux (15-150 keV)    in 16.73 sec: 8.33906 ( -0.16456  0.16533 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.19912e-05 ( -1.97297e-07  1.96979e-07 ) ergs/cm2

Band function

 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -0.124846   ( -0.569282   2.43306 )
beta        : -1.29382    ( -0.0496794   0.04649 )
Epeak [keV] : 63.5461      ( -33.6703 65.5126 )
Norm@50keV   : 0.312413    ( -0.193566   14.1541 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          30.30 using 59 PHA bins.
# Reduced chi-squared =         0.5510 for     55 degrees of freedom 
# Null hypothesis probability =   9.972601e-01
 
Photon flux (15-150 keV)    in 16.73 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)  = 3.06e-06
S(50-100 keV) = 4.88e-06

T90 vs. Hardness ratio plot

T90                                   = 18.055999994278 sec.
Hardness ratio (energy fluence ratio) = 1.59477

Color vs. Color plot

Count Ratio  (25-50 keV) / (15-25 keV) = 1.68404
Count Ratio (50-100 keV) / (15-25 keV) = 1.45993

Mask shadow pattern

IMX = 2.498364785083470E-01, IMY = -5.097982982999856E-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:
-219.803410 -5.532000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
245.0034 -15.6498    0.8  37.1  110.3   7.5159  13.7    1.5	Sco X-1                       
254.4346  35.3262    1.5  21.3  -14.3   1.6594   7.5    1.5	Her X-1                       
268.4301  -1.3367    6.8  37.8   64.8   1.0499   1.7    7.9	SW J1753.5-0127               
299.6074  35.1990    2.0  56.4    3.9   6.8948   5.8    0.9	Cyg X-1                       
212.0848  24.8825    2.7  23.3 -131.5   0.8574   4.3 ------	UNKNOWN                       
293.5407  51.9597    2.4  53.5  -17.0   2.7587   4.9 ------	UNKNOWN                       
244.0644  67.4243    2.9  47.1  -53.1   4.2156   4.0 ------	UNKNOWN                       
197.6791  46.5417    4.2  41.1  -98.3   3.0053   2.8 ------	UNKNOWN

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

Time interval of the image:
-5.532000 11.196600
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
245.1713 -15.6784    9.6  37.2  110.0  -0.5457  -1.2   11.3	Sco X-1                       
254.3361  35.2046    4.8  21.1  -14.2   0.3220   2.4   10.2	Her X-1                       
268.3713  -1.4834   29.9  37.9   65.1  -0.1732  -0.4    1.9	SW J1753.5-0127               
299.5999  35.1838   11.1  56.4    3.9   1.0194   1.0    1.2	Cyg X-1                       
262.1300   4.0091    0.2  29.6   63.9  17.4519  70.0 ------	UNKNOWN                       
274.9777  23.8499    2.5  35.3   20.7   0.9198   4.5 ------	UNKNOWN                       
199.6916  31.9162    2.9  35.1 -120.2   0.5972   3.9 ------	UNKNOWN                       
191.0566  26.6415    2.9  42.3 -129.4   0.6583   4.0 ------	UNKNOWN                       
263.8307  68.5306    3.7  50.7  -44.5   1.5351   3.2 ------	UNKNOWN                       
189.7737  35.8379    3.8  43.8 -116.0   1.2331   3.1 ------	UNKNOWN                       
186.7048  30.5654    3.1  46.0 -123.7   1.6214   3.8 ------	UNKNOWN

Post-slew image of 15-350 keV band

Time interval of the image:
78.596600 962.359200
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
244.9900 -15.6342    0.3  25.9  115.2  31.3001  36.7    0.7	Sco X-1                       
254.4738  35.3300    1.6  32.1 -117.0   7.9137   7.0    1.1	Her X-1                       
262.9070 -24.5948    9.7  28.6   73.3   1.0890   1.2   10.6	GX 1+4                        
268.3213  -1.4360    3.5   8.2   25.9   2.1550   3.2    3.0	SW J1753.5-0127               
270.3055 -25.1157    2.2  30.2   59.9   5.0382   5.2    2.5	GX 5-1                        
270.3137 -25.7101    3.2  30.7   60.2   3.5951   3.6    2.1	GRS 1758-258                  
273.9251 -14.1494    4.0  21.6   42.2   1.8685   2.8    8.2	GX 17+2                       
275.9216 -30.2709    4.3  36.7   54.6   3.6367   2.7    5.8	H1820-303                     
285.0331 -25.0534   13.1  36.6   38.5   0.9276   0.9    8.0	HT1900.1-2455                 
288.7949  10.9387    0.6  27.3  -31.5  12.3296  20.2    0.5	GRS 1915+105                  
262.9474 -33.8358   10.6  37.8   73.7   2.4974   1.1    2.1	GX 354-0                      
266.8521 -27.3220    1.0  31.6   66.8  12.7145  11.4 ------	UNKNOWN                       
310.2729  24.9210    5.1  50.7  -44.5  10.1912   2.3 ------	UNKNOWN

Plot creation:
Sun May 31 07:18:00 EDT 2015