batgrbproduct analysis for trigger=426405

batgrbproduct Analysis for Trigger=426405

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 8 downlinks after the trigger.

======================================================================
                  BAT GRB EVENT DATA PROCESSING REPORT
    Process Script Ver: batgrbproduct v2.46
    Process Start Time (local time): Fri Jul  2 11:22:17 EDT 2010
             Host Name: gcn5
   Current Working Dir: /local/data/raid16/prebascript_archive/trigger426405/GCN5_download_cron
======================================================================

  Trigger: 00426405      Segment: 000

  BAT Trigger Time: 299688946.688   [s; MET]
      Trigger Stop: 299688950.784   [s; MET]
               UTC: 2010-07-01T14:55:40.743940    [includes UTCF correction] 
       Where From?: TDRSS position message

  BAT 
    RA: 258.12423007392   Dec: -37.638555572182  [deg; J2000]

     Catalogged Source?: YES
     Point Source?:      YES
     GRB Indicated?:     NO    [ by BAT flight software ]
     Image S/N Ratio:    8.26
     Image Trigger?:     NO
     Rate S/N Ratio:     6.78232998312527  [ if not an image trigger ]
     Image S/N Ratio:    8.26

  Flight Position:   [ source = BAT ]
    RA: 258.12423007392   Dec: -37.638555572182  [deg; J2000]

  Ground Position:   [ source = BAT pre-slew burst ]
    RA: 258.133428449551   Dec: -37.6632187614317  [deg; J2000]  
        { 17h 12m 32.0s , -37d 39' 47.6" }
         +/- 2.15947132265272 [arcmin] (estimated 90% radius based on SNR)
         +/- 1.01674826448374 [arcmin] (formal 1-sigma fit error)
    SNR: 10.1269619555371
 
  Angular difference between Flight and Ground position is 1.542959 arcmin
 
  Partial Coding Fraction: 0.9140625    [ including projection effects ]

  Duration
     T90: 15.1279999017715 +/- 2.27599030015451
        Measured from: -9.70399987697601
                   to: 5.42400002479553     [s; relative to TRIGTIME]
     T50: 7.72399997711182 +/- 2.99826682363402
        Measured from: -5.84399992227554
                   to: 1.88000005483627     [s; relative to TRIGTIME]



  Fluence
     Peak Flux  (peak 1 second)
        Measured from: 1.30799996852875     
                   to: 2.30799996852875     [s; relative to TRIGTIME]
     Total Fluence        
        Measured from: -10.4000000357628     
                   to: 6.32400000095367     [s; relative to TRIGTIME]
     
             Band 1     Band 2     Band 3     Band 4
              15-25      25-50     50-100    100-350     keV
 Total     0.414489   0.079495   0.001437   0.000679
           0.030075   0.025339   0.022091   0.021374 [error]
 Peak      0.041198   0.008434   0.005609  -0.001191
           0.007618   0.006250   0.005315   0.005262 [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 1.20e-07 3.95e-08 7.29e-09 1.57e-09 1.68e-07 1.68e-07   erg/cm2
              Error 1.81e-08 1.34e-08 5.62e-09 2.24e-09 2.86e-08 2.91e-08   erg/cm2
Peak flux Power-law 3.32e-01 1.12e-01 2.12e-02 4.71e-03 4.68e-01 4.69e-01   ph/cm2/s
              Error 1.09e-01 5.69e-02 2.33e-02 1.10e-02 1.53e-01 1.54e-01   ph/cm2/s
 
Fluence   Cutoff-PL 1.20e-07 3.95e-08 7.27e-09 1.56e-09 1.68e-07 1.68e-07   erg/cm2
              Error 1.81e-08 1.34e-08 5.62e-09 2.22e-09 2.86e-08 2.91e-08   erg/cm2
Peak flux Cutoff-PL 4.08e-01 7.71e-02 1.52e-05 1.77e-15 4.85e-01 4.85e-01   ph/cm2/s
              Error 1.24e-01 5.37e-02 1.04e-03 1.40e-01 0.00e+00 0.00e+00   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 0.00e+00 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    4.436    0.623    -      -           3.26e-04 1.95e-04   46.600 57
CPL   1.000    0.000      50.0    0.0      3.59e-03 0.00e+00  121.360 56
 
 
=== 1-s peak spectral analysis ===
 
Model Ph_index Ph_90err Epeak  Epeak_90err Norm     Nomr_90err chi2   dof
PL    3.397    0.956    -      -           1.26e-03 1.26e-03   52.060 57
CPL   1.000    0.000      50.0    0.0      7.79e-03 0.00e+00   63.910 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   16.724  -10.400    6.324
T90    15.128   -9.704    5.424
T50     7.724   -5.844    1.880
Peak    1.000    1.308    2.308

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
  258.1334 -37.6632 0.0189   19.0  153.8       0.5624    10.1  TRIG_00426405       
------------------------------------------
 
Foreground time interval of the image:
-10.400   6.324 (delta_t =  16.724 [sec])
Background time interval of the image:
-119.688 -89.648 (delta_t =  30.040 [sec])
-88.688 -10.400 (delta_t =  78.288 [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 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)

The mask-weighted light curves based on cleaned DPHs

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  -10.400 sec. to    6.324 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 4.43601     ( -0.574255   0.67102 )
Norm@50keV  : 3.26005E-04    ( -0.00016124   0.000229568 )
------------------------------------------------------------
# Chi-Squared =          46.60 using 59 PHA bins.
# Reduced chi-squared =         0.8175 for     57 degrees of freedom 
# Null hypothesis probability =   8.357785e-01
 
Photon flux (15-150 keV)    in 16.72 sec: 0.296872 ( -0.0438845  0.0439117 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.67646e-07 ( -2.80119e-08  2.92515e-08 ) ergs/cm2

Cutoff power-law model

Time interval is from  -10.400 sec. to    6.324 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.00000     (     )
Epeak [keV] : 50.0000      (   )
Norm@50keV  : 3.58960E-03    (     )
------------------------------------------------------------
# Chi-Squared =         121.36 using 59 PHA bins.
# Reduced chi-squared =         2.1671 for     56 degrees of freedom 
# Null hypothesis probability =   9.980399e-07
 
Photon flux (15-150 keV)    in 16.72 sec: 0.296652 (    ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.67608e-07 ( -2.8015e-08  2.92533e-08 ) ergs/cm2

Band function

Time interval is from  -10.400 sec. to    6.324 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -2.18999   ( 2.18999   2.18999 )
beta        : -4.43814    ( -0.66899   0.576319 )
Epeak [keV] : 5.63551      ( -5.63551 -5.63551 )
Norm@50keV   : 3.29074    ( -3.29073   16.8355 )
------------------------------------------------------------
# Chi-Squared =          46.60 using 59 PHA bins.
# Reduced chi-squared =         0.8472 for     55 degrees of freedom 
# Null hypothesis probability =   7.827496e-01
 
Photon flux (15-150 keV)    in 16.72 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]    : 3.18798  (-0.439977  0.528486)
R^2/D10^2   : 28.1891  (-17.0218   45.0321)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
# Chi-Squared =          47.54 using 59 PHA bins.
# Reduced chi-squared =         0.8341 for     57 degrees of freedom 
# Null hypothesis probability =   8.096262e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.273e-07   4.836e-08
25- 50  2.282e-08   1.026e-08
50-150  5.932e-11   5.497e-11
15-150  1.502e-07   6.378e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 7.02042       (-1.60337      2.31445)
Norm        : 23.3481       (-11.8946     27.0164)
------------------------------------------------------------
# Chi-Squared =          46.73 using 59 PHA bins.
# Reduced chi-squared =         0.8199 for     57 degrees of freedom 
# Null hypothesis probability =   8.321603e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.242e-07   3.841e-08
25- 50  3.098e-08   1.457e-08
50-150  6.937e-10   6.284e-10
15-150  1.558e-07   5.241e-08

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 2.82233        (-1.42262      0.62227)
R1^2/D10^2  : 53.6315        (-37.2155      295.897)
kT2 [keV]   : 8.85614        (-9.087      -9.087)
R2^2/D10^2  : 4.21702E-02    (-0.0402388   32.9403)
------------------------------------------------------------
# Chi-Squared =          44.93 using 59 PHA bins.
# Reduced chi-squared =         0.8168 for     55 degrees of freedom 
# Null hypothesis probability =   8.318884e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.243e-07   6.629e-08
25- 50  3.543e-08   1.929e-08
50-150  8.043e-09   6.084e-09
15-150  1.677e-07   8.485e-08

Peak spectrum fit

Power-law model

Time interval is from    1.308 sec. to    2.308 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 3.39738     ( -0.826747   1.08492 )
Norm@50keV  : 1.25521E-03    ( -0.00125469   0.00125792 )
------------------------------------------------------------
# Chi-Squared =          52.06 using 59 PHA bins.
# Reduced chi-squared =         0.9133 for     57 degrees of freedom 
# Null hypothesis probability =   6.605310e-01
 
Photon flux (15-150 keV)    in 1 sec: 0.467705 ( -0.152135  0.153651 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.85786e-08 ( -7.19537e-09  8.58122e-09 ) ergs/cm2

Cutoff power-law model

Time interval is from    1.308 sec. to    2.308 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.00000     (     )
Epeak [keV] : 50.0000      (   )
Norm@50keV  : 7.79153E-03    (     )
------------------------------------------------------------
# Chi-Squared =          63.91 using 59 PHA bins.
# Reduced chi-squared =          1.141 for     56 degrees of freedom 
# Null hypothesis probability =   2.185964e-01
 
Photon flux (15-150 keV)    in 1 sec: 0.484839 (    ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.61228e-08 ( -4.7648e-09  4.8573e-09 ) ergs/cm2

Band function

Time interval is from    1.308 sec. to    2.308 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : 3.15636   ( 0.0251181   0.0251181 )
beta        : -7.40703    ( 181.293   191.293 )
Epeak [keV] : 16.5208      ( -7.89837 8.97975 )
Norm@50keV   : 346.471    ( -346.448   13235.5 )
------------------------------------------------------------
# Chi-Squared =          48.38 using 59 PHA bins.
# Reduced chi-squared =         0.8796 for     55 degrees of freedom 
# Null hypothesis probability =   7.237791e-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]    : 4.11919  (-0.907334  1.13696)
R^2/D10^2   : 11.0699  (-7.86751   29.7958)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
# Chi-Squared =          48.81 using 59 PHA bins.
# Reduced chi-squared =         0.8563 for     57 degrees of freedom 
# Null hypothesis probability =   7.715899e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.159e-08   7.140e-09
25- 50  4.545e-09   2.970e-09
50-150  6.579e-11   7.055e-11
15-150  1.620e-08   9.780e-09

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 10.7007       (-4.17229      9.03817)
Norm        : 14.2598       (-8.71691     26.1138)
------------------------------------------------------------
# Chi-Squared =          50.72 using 59 PHA bins.
# Reduced chi-squared =         0.8897 for     57 degrees of freedom 
# Null hypothesis probability =   7.083911e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.076e-08   6.700e-09
25- 50  5.060e-09   3.555e-09
50-150  4.153e-10   4.494e-10
15-150  1.623e-08   9.985e-09

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 3.99962        (-0.901452      1.13294)
R1^2/D10^2  : 12.4868        (-8.96314      35.5221)
kT2 [keV]   : 36.8570        (-37.6454      -37.6454)
R2^2/D10^2  : 6.70810E-04    (-0.000626498   30.7068)
------------------------------------------------------------
# Chi-Squared =          47.83 using 59 PHA bins.
# Reduced chi-squared =         0.8696 for     55 degrees of freedom 
# Null hypothesis probability =   7.427871e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.148e-08   6.700e-09
25- 50  4.926e-09   2.910e-09
50-150  7.180e-09   5.940e-09
15-150  2.358e-08   1.444e-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: 4.43601     ( -0.574255   0.67102 )
Norm@50keV  : 3.26005E-04    ( -0.00016124   0.000229568 )
------------------------------------------------------------
# Chi-Squared =          46.60 using 59 PHA bins.
# Reduced chi-squared =         0.8175 for     57 degrees of freedom 
# Null hypothesis probability =   8.357785e-01
 
Photon flux (15-150 keV)    in 16.72 sec: 0.296872 ( -0.0438845  0.0439117 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.67646e-07 ( -2.80119e-08  2.92515e-08 ) ergs/cm2

Cutoff power-law model

Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.00000     (     )
Epeak [keV] : 50.0000      (   )
Norm@50keV  : 3.58960E-03    (     )
------------------------------------------------------------
# Chi-Squared =         121.36 using 59 PHA bins.
# Reduced chi-squared =         2.1671 for     56 degrees of freedom 
# Null hypothesis probability =   9.980399e-07
 
Photon flux (15-150 keV)    in 16.72 sec: 0.296652 (    ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.67608e-07 ( -2.8015e-08  2.92533e-08 ) ergs/cm2

Band function

 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -2.18999   ( 2.18999   2.18999 )
beta        : -4.43814    ( -0.66899   0.576319 )
Epeak [keV] : 5.63551      ( -5.63551 -5.63551 )
Norm@50keV   : 3.29074    ( -3.29073   16.8355 )
------------------------------------------------------------
# Chi-Squared =          46.60 using 59 PHA bins.
# Reduced chi-squared =         0.8472 for     55 degrees of freedom 
# Null hypothesis probability =   7.827496e-01
 
Photon flux (15-150 keV)    in 16.72 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)  = 3.9491e-08
S(50-100 keV) = 7.28704e-09

T90 vs. Hardness ratio plot

T90                                   = 15.1279999017715 sec.
Hardness ratio (energy fluence ratio) = 0.184524

Color vs. Color plot

Count Ratio  (25-50 keV) / (15-25 keV) = 0.19179
Count Ratio (50-100 keV) / (15-25 keV) = 0.00346692

Mask shadow pattern

IMX = -3.081075677882813E-01, IMY = -1.518419168542080E-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:
-119.688000 -89.648000
-88.688000 -10.400000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
244.9852 -15.6422    0.2   7.4   15.7   7.6661  52.7    0.4	Sco X-1                       
256.0750 -37.8212    1.7  18.0  158.0   0.9856   6.9    4.4	4U 1700-377                   
256.2539 -36.4365    3.9  17.0  154.7   0.4234   3.0    8.8	GX 349+2                      
262.8838 -24.7496    7.2  17.2  109.5   0.2547   1.6    6.8	GX 1+4                        
264.7671 -44.3765    7.3  27.3  156.5   0.3076   1.6    4.5	4U 1735-44                    
268.5183  -1.4737    3.2  31.9   60.9   0.9792   3.7    9.1	SW J1753.5-0127               
270.3688 -25.1976    6.2  24.0  110.4   0.3734   1.9    8.5	GX 5-1                        
270.2526 -25.6847    4.3  23.9  111.6   0.5958   3.0    4.4	GRS 1758-258                  
274.0826 -14.1486    3.2  29.6   87.7   0.9974   3.6    8.1	GX 17+2                       
276.1212 -30.4031    6.7  29.4  121.3   0.4106   1.7   10.4	H1820-303                     
285.2286 -24.9579    0.0  37.4  111.3   0.3571   0.8   10.7	HT1900.1-2455                 
230.6081  19.9211    2.5  44.9   -8.5   1.2937   4.6 ------	UNKNOWN                       
198.4997 -40.4950    2.3  42.1 -115.9   2.6430   4.9 ------	UNKNOWN

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

Time interval of the image:
-10.400000 6.324000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
244.8208 -15.6312    8.7   7.4   14.5   0.0657   1.3    9.2	Sco X-1                       
255.8049 -37.7316    4.3  17.8  158.4   0.1397   2.7   10.9	4U 1700-377                   
256.2161 -36.3209    0.0  16.9  154.5  -0.0320  -0.6   12.2	GX 349+2                      
262.8980 -24.9304    0.0  17.2  110.1  -0.0636  -1.0   12.6	GX 1+4                        
264.5187 -44.4021   16.9  27.2  156.8   0.0424   0.7   10.0	4U 1735-44                    
268.5464  -1.5264    3.4  31.9   61.0  -0.3242  -3.4   11.6	SW J1753.5-0127               
270.1460 -25.1722    9.0  23.8  110.3  -0.0917  -1.3    9.4	GX 5-1                        
270.2597 -25.7647    5.4  23.9  111.8  -0.1631  -2.3    2.7	GRS 1758-258                  
274.1639 -14.0198   19.2  29.7   87.5  -0.0572  -0.6    9.3	GX 17+2                       
276.0792 -30.3088    5.0  29.3  121.1  -0.1946  -2.3    8.7	H1820-303                     
285.1476 -25.0034   50.2  37.3  111.4  -0.0336  -0.2    7.9	HT1900.1-2455                 
258.7837  11.8247    2.3  37.6   33.6   0.4836   5.0 ------	UNKNOWN                       
258.1334 -37.6632    1.1  19.0  153.8   0.5624  10.1 ------	UNKNOWN

Post-slew image of 15-350 keV band

Time interval of the image:
79.412600 195.352500
300.312000 732.712600
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
244.9738 -15.6439    0.2  24.9   -0.4  38.1971  73.0    0.4	Sco X-1                       
256.0106 -37.8804    1.9   1.7  -68.3   3.4930   6.1    2.5	4U 1700-377                   
256.4116 -36.2963    5.9   1.9  -15.0   1.0587   1.9    7.7	GX 349+2                      
263.0881 -24.8748    4.4  13.4   50.8   1.2802   2.6    8.9	GX 1+4                        
264.8077 -44.2588    9.3   8.3  175.8  -0.6240  -1.2   11.8	4U 1735-44                    
268.2600  -1.3585   13.9  37.5   47.8   0.8949   0.8    8.6	SW J1753.5-0127               
270.2936 -25.2117    3.7  16.2   74.3   1.7565   3.1    8.0	GX 5-1                        
270.3024 -25.8669    2.5  15.7   75.8   2.5318   4.6    7.4	GRS 1758-258                  
273.9509 -14.1994    4.9  27.3   66.2   1.7354   2.4   10.3	GX 17+2                       
275.9391 -30.3332    3.1  16.5  100.0   1.9433   3.7    2.2	H1820-303                     
285.0195 -24.7408    4.3  26.2   99.4   2.0304   2.7   10.8	HT1900.1-2455

Plot creation:
Fri Jul  2 11:36:00 EDT 2010