batgrbproduct analysis for trigger=230702

batgrbproduct Analysis for Trigger=230702

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): Wed Jan 22 13:23:17 EST 2014
             Host Name: batevent1
   Current Working Dir: /local/data/batevent/batevent_reproc/trigger230702
======================================================================

  Trigger: 00230702      Segment: 000

  BAT Trigger Time: 180704287.68   [s; MET]
      Trigger Stop: 180704291.776   [s; MET]
               UTC: 2006-09-23T11:38:06.217800    [includes UTCF correction] 
       Where From?: TDRSS position message

  BAT 
    RA: 238.201486511859   Dec: -30.9072142492461  [deg; J2000]

     Catalogged Source?: NO
     Point Source?:      YES
     GRB Indicated?:     YES    [ by BAT flight software ]
     Image S/N Ratio:    9.4
     Image Trigger?:     NO
     Rate S/N Ratio:     10.3923048454133  [ if not an image trigger ]
     Image S/N Ratio:    9.4

  Flight Position:   [ source = BAT ]
    RA: 238.201486511859   Dec: -30.9072142492461  [deg; J2000]

  Ground Position:   [ source = BAT pre-slew burst ]
    RA: 238.187882282817   Dec: -30.9054737709443  [deg; J2000]  
        { 15h 52m 45.1s , -30d 54' 19.7" }
         +/- 1.6711126016364 [arcmin] (estimated 90% radius based on SNR)
         +/- 0.76876867175969 [arcmin] (formal 1-sigma fit error)
    SNR: 14.6062519696874
 
  Angular difference between Flight and Ground position is 0.708095 arcmin
 
  Partial Coding Fraction: 0.3632812    [ including projection effects ]

  Duration
     T90: 8.94800001382828 +/- 1.29634099081825
        Measured from: 0.331999987363815
                   to: 9.28000000119209     [s; relative to TRIGTIME]
     T50: 4.30400002002716 +/- 1.05255496990518
        Measured from: 2.43599998950958
                   to: 6.74000000953674     [s; relative to TRIGTIME]



  Fluence
     Peak Flux  (peak 1 second)
        Measured from: 4.92800000309944     
                   to: 5.92800000309944     [s; relative to TRIGTIME]
     Total Fluence        
        Measured from: -0.0680000185966492     
                   to: 9.88799998164177     [s; relative to TRIGTIME]
     
             Band 1     Band 2     Band 3     Band 4
              15-25      25-50     50-100    100-350     keV
 Total     0.391487   0.368509   0.110670   0.029042
           0.036084   0.033707   0.029116   0.028135 [error]
 Peak      0.062140   0.059262   0.018138   0.005878
           0.011742   0.010860   0.009368   0.008608 [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 1.59e-07 1.62e-07 1.17e-07 1.35e-07 4.90e-07 5.72e-07   erg/cm2
              Error 2.32e-08 1.89e-08 2.70e-08 5.94e-08 6.25e-08 9.55e-08   erg/cm2
Peak flux Power-law 7.66e-01 4.46e-01 1.65e-01 8.06e-02 1.42e+00 1.46e+00   ph/cm2/s
              Error 2.17e-01 1.04e-01 6.91e-02 6.20e-02 3.18e-01 3.26e-01   ph/cm2/s
 
Fluence   Cutoff-PL 1.53e-07 1.73e-07 1.06e-07 4.04e-08 4.60e-07 4.72e-07   erg/cm2
              Error 2.56e-08 2.54e-08 3.52e-08 -------- 7.34e-08 1.26e-07   erg/cm2
Peak flux Cutoff-PL 7.03e-01 5.63e-01 6.48e-02 3.83e-04 1.33e+00 1.33e+00   ph/cm2/s
              Error 2.42e-01 1.52e-01 1.03e-01 3.05e-02 3.27e-01 3.27e-01   ph/cm2/s
 
Fluence        Band -------- -------- -------- -------- -------- --------   erg/cm2
              Error -------- -------- -------- -------- -------- --------   erg/cm2
Peak flux      Band -------- -------- 7.88e-02 -------- -------- 1.37e+00   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    2.474    0.237    -      -           4.96e-03 8.30e-04   58.540 57
CPL   1.815    0.745      10.4    0.0      1.26e-02 0.00e+00   57.280 56
 
 
=== 1-s peak spectral analysis ===
 
Model Ph_index Ph_90err Epeak  Epeak_90err Norm     Nomr_90err chi2   dof
PL    2.436    0.432    -      -           7.51e-03 2.44e-03   59.260 57
CPL  -0.033    1.067      26.9    0.0      3.26e-01 0.00e+00   55.850 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    9.956   -0.068    9.888
T90     8.948    0.332    9.280
T50     4.304    2.436    6.740
Peak    1.000    4.928    5.928

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
  238.1879   -30.9055   0.0131    46.0736  -156.8753         0.9609352     14.606 TRIG_00230702                 
 
Foreground time interval of the image:
 -0.068   9.888 (delta_t =   9.956 [sec])
Background time interval of the image:
-239.680  -0.068 (delta_t = 239.612 [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 4.096000

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 4.096000

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 4.096000

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   -0.068 sec. to    9.888 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 2.47374     ( -0.227504   0.246634 )
Norm@50keV  : 4.95785E-03    ( -0.000836987   0.000822281 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          58.54 using 59 PHA bins.
# Reduced chi-squared =          1.027 for     57 degrees of freedom 
# Null hypothesis probability =   4.185311e-01
 
Photon flux (15-150 keV)    in 9.956 sec: 0.958497 ( -0.105095  0.105189 ) ph/cm2/s
Energy fluence (15-150 keV)             : 4.90182e-07 ( -6.17177e-08  6.32222e-08 ) ergs/cm2

Cutoff power-law model

Time interval is from   -0.068 sec. to    9.888 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.81548     ( -1.30296   0.187877 )
Epeak [keV] : 10.4177      (   )
Norm@50keV  : 1.26142E-02    (     )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          57.28 using 59 PHA bins.
# Reduced chi-squared =          1.023 for     56 degrees of freedom 
# Null hypothesis probability =   4.275778e-01
 
Photon flux (15-150 keV)    in 9.956 sec: 0.934135 ( -0.110792  0.111025 ) ph/cm2/s
Energy fluence (15-150 keV)             : 4.59642e-07 ( -6.99339e-08  7.6924e-08 ) ergs/cm2

Band function

Time interval is from   -0.068 sec. to    9.888 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -1.51283   ( 0.966993   0.966993 )
beta        : -2.96495    ( 3.01225   0.688339 )
Epeak [keV] : 17.6929      ( -17.8169 10.2323 )
Norm@50keV   : 2.01816E-02    ( -0.0110805   2096.13 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          57.01 using 59 PHA bins.
# Reduced chi-squared =          1.037 for     55 degrees of freedom 
# Null hypothesis probability =   4.000745e-01
 
Photon flux (15-150 keV)    in 9.956 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]    : 7.68353  (-0.940209  1.0557)
R^2/D10^2   : 1.18447  (-0.492865   0.873732)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          69.94 using 59 PHA bins.
# Reduced chi-squared =          1.227 for     57 degrees of freedom 
# Null hypothesis probability =   1.165329e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.220e-07   2.564e-08
25- 50  1.988e-07   2.977e-08
50-150  4.562e-08   1.660e-08
15-150  3.664e-07   5.506e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 34.0932       (-8.06118      11.5697)
Norm        : 6.84259       (-1.488     2.02215)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          57.71 using 59 PHA bins.
# Reduced chi-squared =          1.012 for     57 degrees of freedom 
# Null hypothesis probability =   4.489819e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.472e-07   2.210e-08
25- 50  1.798e-07   2.628e-08
50-150  1.157e-07   4.202e-08
15-150  4.428e-07   6.850e-08

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 4.22043        (-1.72806      2.37997)
R1^2/D10^2  : 9.79693        (-7.75699      117.506)
kT2 [keV]   : 12.1014        (-3.31967      15.1449)
R2^2/D10^2  : 0.126649    (-0.122395   0.151605)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          58.17 using 59 PHA bins.
# Reduced chi-squared =          1.058 for     55 degrees of freedom 
# Null hypothesis probability =   3.594970e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.534e-07   7.975e-08
25- 50  1.722e-07   8.866e-08
50-150  1.108e-07   6.511e-08
15-150  4.364e-07   2.248e-07

Peak spectrum fit

Power-law model

Time interval is from    4.928 sec. to    5.928 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 2.43605     ( -0.401835   0.461428 )
Norm@50keV  : 7.50593E-03    ( -0.00244453   0.00243357 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          59.26 using 59 PHA bins.
# Reduced chi-squared =          1.040 for     57 degrees of freedom 
# Null hypothesis probability =   3.930457e-01
 
Photon flux (15-150 keV)    in 1 sec: 1.41866 ( -0.317943  0.318133 ) ph/cm2/s
Energy fluence (15-150 keV)             : 7.38295e-08 ( -1.88465e-08  1.97613e-08 ) ergs/cm2

Cutoff power-law model

Time interval is from    4.928 sec. to    5.928 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: -3.26131E-02     ( 0.0676691   2.20124 )
Epeak [keV] : 26.9055      (   )
Norm@50keV  : 0.325593    (     )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          55.85 using 59 PHA bins.
# Reduced chi-squared =         0.9973 for     56 degrees of freedom 
# Null hypothesis probability =   4.804951e-01
 
Photon flux (15-150 keV)    in 1 sec: 1.33149 ( -0.32466  0.33013 ) ph/cm2/s
Energy fluence (15-150 keV)             : 5.85036e-08 ( -1.6625e-08  2.34362e-08 ) ergs/cm2

Band function

Time interval is from    4.928 sec. to    5.928 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : 4.32671   ( -2.72792   -0.45476 )
beta        : -3.38975    ( 9.37167   19.3671 )
Epeak [keV] : 25.6906      ( -10.2329 9.00479 )
Norm@50keV   : 534.768    ( -533.853   187.906 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          53.54 using 59 PHA bins.
# Reduced chi-squared =         0.9734 for     55 degrees of freedom 
# Null hypothesis probability =   5.306166e-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]    : 7.02558  (-1.33749  1.77664)
R^2/D10^2   : 2.75622  (-1.70321   4.09279)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          55.85 using 59 PHA bins.
# Reduced chi-squared =         0.9798 for     57 degrees of freedom 
# Null hypothesis probability =   5.183120e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  2.194e-08   8.523e-09
25- 50  3.026e-08   1.560e-08
50-150  5.080e-09   3.421e-09
15-150  5.727e-08   2.525e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 32.5541       (-12.3819      24.4791)
Norm        : 10.8733       (-4.00758     6.82044)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          56.67 using 59 PHA bins.
# Reduced chi-squared =         0.9941 for     57 degrees of freedom 
# Null hypothesis probability =   4.875459e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  2.302e-08   7.570e-09
25- 50  2.748e-08   1.052e-08
50-150  1.671e-08   1.131e-08
15-150  6.720e-08   2.222e-08

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 6.15516        (-6.15543      2.05674)
R1^2/D10^2  : 4.20048        (-4.1859      -4.1859)
kT2 [keV]   : 18.8917        (-18.8297      -18.8297)
R2^2/D10^2  : 1.54973E-02    (-0.0165185   5.13852)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          54.42 using 59 PHA bins.
# Reduced chi-squared =         0.9895 for     55 degrees of freedom 
# Null hypothesis probability =   4.966444e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  2.300e-08   1.406e-08
25- 50  2.831e-08   1.701e-08
50-150  1.602e-08   9.800e-09
15-150  6.733e-08   3.819e-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: 2.47374     ( -0.227504   0.246634 )
Norm@50keV  : 4.95785E-03    ( -0.000836987   0.000822281 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          58.54 using 59 PHA bins.
# Reduced chi-squared =          1.027 for     57 degrees of freedom 
# Null hypothesis probability =   4.185311e-01
 
Photon flux (15-150 keV)    in 9.956 sec: 0.958497 ( -0.105095  0.105189 ) ph/cm2/s
Energy fluence (15-150 keV)             : 4.90182e-07 ( -6.17177e-08  6.32222e-08 ) ergs/cm2

Cutoff power-law model

Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.81548     ( -1.30296   0.187877 )
Epeak [keV] : 10.4177      (   )
Norm@50keV  : 1.26142E-02    (     )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          57.28 using 59 PHA bins.
# Reduced chi-squared =          1.023 for     56 degrees of freedom 
# Null hypothesis probability =   4.275778e-01
 
Photon flux (15-150 keV)    in 9.956 sec: 0.934135 ( -0.110792  0.111025 ) ph/cm2/s
Energy fluence (15-150 keV)             : 4.59642e-07 ( -6.99339e-08  7.6924e-08 ) ergs/cm2

Band function

 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -1.51283   ( 0.966993   0.966993 )
beta        : -2.96495    ( 3.01225   0.688339 )
Epeak [keV] : 17.6929      ( -17.8169 10.2339 )
Norm@50keV   : 2.01816E-02    ( -0.0110805   2096.13 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          57.01 using 59 PHA bins.
# Reduced chi-squared =          1.037 for     55 degrees of freedom 
# Null hypothesis probability =   4.000745e-01
 
Photon flux (15-150 keV)    in 9.956 sec:  (    ) ph/cm2/s
Energy fluence (15-150 keV)             : 0 ( 0  0 ) ergs/cm2

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

S(25-50 keV)  = 1.62e-07
S(50-100 keV) = 1.17e-07

T90 vs. Hardness ratio plot

T90                                   = 8.94800001382828 sec.
Hardness ratio (energy fluence ratio) = 0.722222

Color vs. Color plot

Count Ratio  (25-50 keV) / (15-25 keV) = 0.941306
Count Ratio (50-100 keV) / (15-25 keV) = 0.282691

Mask shadow pattern

IMX = -9.547791601715945E-01, IMY = 4.077347397311630E-01

TIME vs. PHA plot around the trigger time

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 4.096000

TIME vs. DetID plot around the trigger time

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 4.096000

100 us light curve (15-350 keV)

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 4.096000

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:
-239.680000 -0.068000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
244.9831 -15.6404    0.2  29.6 -157.5  12.5364  52.8    0.2	Sco X-1                       
254.4607  35.3451    1.8  23.0    3.1   1.5210   6.5    0.2	Her X-1                       
256.0200 -37.8621    1.9  50.3 -178.0   3.2547   6.2    1.9	4U 1700-377                   
256.4340 -36.4427    6.4  48.8 -178.5   0.7840   1.8    1.2	GX 349+2                      
263.0945 -24.7457    8.3  38.0  170.9   0.4604   1.4    4.7	GX 1+4                        
268.3932  -1.3044   11.0  19.3  137.5   0.2497   1.0    9.0	SW J1753.5-0127               
270.2347 -24.9761    5.3  40.3  161.3   0.9306   2.2    6.7	GX 5-1                        
270.3100 -25.8908    6.8  41.2  161.8   0.7556   1.7    8.9	GRS 1758-258                  
274.0133 -14.0253   27.0  32.6  146.8   0.1486   0.4    0.8	GX 17+2                       
276.0567 -30.2018   24.6  47.3  158.0   0.3302   0.5   12.0	H1820-303                     
284.9276 -25.0439   59.5  47.7  145.2   0.1719   0.2    9.5	HT1900.1-2455                 
288.7050  10.9054    3.3  33.4   92.3   1.8166   3.4    6.0	GRS 1915+105                  
262.9665 -33.8717    3.0  46.9  173.9   1.7874   3.8    2.5	GX 354-0                      
231.3413  -8.1506    2.8  30.9 -127.0   1.1591   4.1 ------	UNKNOWN                       
208.0506  32.7121    3.2  47.1  -53.1   3.8613   3.7 ------	UNKNOWN

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

Time interval of the image:
-0.068000 9.888000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
245.0958 -15.6468    4.4  29.6 -157.7  -0.1014  -2.6    6.7	Sco X-1                       
254.2785  35.4843    6.0  23.1    2.7   0.0735   1.9   12.2	Her X-1                       
255.8604 -37.8064    6.5  50.2 -177.8   0.1463   1.8    6.4	4U 1700-377                   
256.4607 -36.4347   30.2  48.8 -178.5   0.0295   0.4    1.4	GX 349+2                      
262.9227 -24.6741    7.3  37.9  171.1  -0.0818  -1.6    6.4	GX 1+4                        
268.2215  -1.3156    0.0  19.2  137.9  -0.0460  -1.2   12.0	SW J1753.5-0127               
270.2606 -25.0717    5.9  40.4  161.3  -0.1220  -2.0    1.4	GX 5-1                        
270.3601 -25.7063   12.4  41.0  161.6   0.0598   0.9    3.8	GRS 1758-258                  
274.1039 -14.0453   17.1  32.7  146.7   0.0342   0.7    5.7	GX 17+2                       
275.8462 -30.2350   10.4  47.3  158.2  -0.1091  -1.1    8.9	H1820-303                     
284.9069 -24.8840    3.7  47.5  145.1  -0.4239  -3.1    7.4	HT1900.1-2455                 
288.9293  11.0634    8.0  33.6   92.0   0.1178   1.5   10.5	GRS 1915+105                  
262.9827 -33.6846   11.0  46.7  173.9   0.0775   1.1    9.0	GX 354-0                      
286.9731  56.5503    2.8  50.7   25.8   0.6880   4.1 ------	UNKNOWN                       
239.3845  61.6710    2.2  50.5   -5.9   0.4358   5.2 ------	UNKNOWN                       
238.1879 -30.9055    0.8  46.1 -156.9   0.9613  14.6 ------	UNKNOWN                       
222.6574  49.9861    2.5  45.8  -24.9   0.3000   4.7 ------	UNKNOWN

Post-slew image of 15-350 keV band

Time interval of the image:
101.220590 388.920600
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
170.2972 -60.6233   78.3  52.7 -162.9   0.1051   0.1    0.5	Cen X-3                       
187.0181 -62.7662  113.3  45.4 -167.6   0.0485   0.1    9.9	GX 301-2                      
244.9781 -15.6388    0.2  16.5    6.0  13.2803  55.9    0.1	Sco X-1                       
255.9948 -37.8419    0.7  16.2  102.5   4.0199  15.9    0.4	4U 1700-377                   
256.4786 -36.4127    3.0  16.2   97.2   0.9802   3.9    2.2	GX 349+2                      
263.1171 -24.7487    2.2  22.8   62.9   1.8299   5.3    5.9	GX 1+4                        
264.6753 -44.3124    6.4  24.7  112.6  -0.6215  -1.8    8.8	4U 1735-44                    
268.4950  -1.3423    0.0  41.2   32.3   0.5796   1.0   10.1	SW J1753.5-0127               
270.2497 -25.1149    5.2  28.8   68.8   0.8618   2.2    2.8	GX 5-1                        
270.1383 -25.8432    5.1  28.5   70.2   0.9049   2.2   10.7	GRS 1758-258                  
273.9866 -13.8997    8.8  37.0   53.1   0.7369   1.3    8.3	GX 17+2                       
276.0304 -30.4718    5.6  32.4   81.5   1.1201   2.1    8.3	H1820-303                     
262.9567 -33.8641    1.9  21.1   87.0   1.8611   6.1    2.4	GX 354-0                      
156.8627 -59.1634    4.8  59.5 -161.7   6.2567   2.4 ------	UNKNOWN                       
195.5740 -16.9828    4.2  41.1  -98.0   5.1088   2.8 ------	UNKNOWN                       
183.7363 -31.8199    2.8  46.0 -123.8   6.2952   4.1 ------	UNKNOWN                       
218.1162  17.4035    4.7  52.0  -42.3   4.3281   2.5 ------	UNKNOWN

Plot creation:
Sun May 31 11:59:20 EDT 2015