batgrbproduct analysis for trigger=505516

batgrbproduct Analysis for Trigger=505516

Analysis Summary

Notes:

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

======================================================================
                  BAT GRB EVENT DATA PROCESSING REPORT
    Process Script Ver: batgrbproduct v2.46
    Process Start Time (local time): Sat Oct 15 14:51:54 EDT 2011
             Host Name: gcn5
   Current Working Dir: /local/data/raid16/prebascript_archive/trigger505516/GCN5_download_cron
======================================================================

  Trigger: 00505516      Segment: 000

  BAT Trigger Time: 340333968   [s; MET]
      Trigger Stop: 340334032   [s; MET]
               UTC: 2011-10-15T01:12:40.532120    [includes UTCF correction] 
       Where From?: TDRSS position message

  BAT 
    RA: 265.215496981894   Dec: -28.0913859568875  [deg; J2000]

     Catalogged Source?: YES
     Point Source?:      YES
     GRB Indicated?:     NO    [ by BAT flight software ]
     Image S/N Ratio:    8
     Image Trigger?:     YES
     Rate S/N Ratio:     0  [ if not an image trigger ]
     Image S/N Ratio:    8

  Flight Position:   [ source = BAT ]
    RA: 265.215496981894   Dec: -28.0913859568875  [deg; J2000]

  Ground Position:   [ source = BAT pre-slew burst ]
    RA: 265.208760041102   Dec: -28.0904924263295  [deg; J2000]  
        { 17h 40m 50.1s , -28d 05' 25.8" }
         +/- 3.24819606002415 [arcmin] (estimated 90% radius based on SNR)
         +/- 1.59700325059743 [arcmin] (formal 1-sigma fit error)
    SNR: 5.65198370507143
 
  Angular difference between Flight and Ground position is 0.360608 arcmin
 
  Partial Coding Fraction: 0.921875    [ including projection effects ]

  Duration
     T90: 890.432000041008 +/- 53.2668908660368
        Measured from: 34.4080001115799
                   to: 924.840000152588     [s; relative to TRIGTIME]
     T50: 861.37600004673 +/- 661.777730508391
        Measured from: 38.3120000958443
                   to: 899.688000142574     [s; relative to TRIGTIME]



  Fluence
     Peak Flux  (peak 1 second)
        Measured from: -29.8040000200272     
                   to: -28.8040000200272     [s; relative to TRIGTIME]
     Total Fluence        
        Measured from: -29.783999979496     
                   to: 933.480000019073     [s; relative to TRIGTIME]
     
             Band 1     Band 2     Band 3     Band 4
              15-25      25-50     50-100    100-350     keV
 Total     0.167881   1.101908   0.558923   0.123978
           0.192682   0.172888   0.147708   0.131507 [error]
 Peak      0.012763   0.023200   0.003621   0.008773
           0.006524   0.005725   0.004835   0.004453 [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 1.58e-07 3.10e-07 4.72e-07 1.57e-06 1.32e-06 2.49e-06   erg/cm2
              Error 6.09e-08 7.93e-08 1.34e-07 9.10e-07 3.41e-07 1.02e-06   erg/cm2
Peak flux Power-law 2.05e-01 1.12e-01 3.85e-02 1.72e-02 3.65e-01 3.72e-01   ph/cm2/s
              Error 9.85e-02 5.10e-02 3.35e-02 3.15e-02 1.41e-01 1.46e-01   ph/cm2/s
 
Fluence   Cutoff-PL 1.01e-07 4.79e-07 3.44e-07 1.42e-08 9.37e-07 9.36e-07   erg/cm2
              Error 6.34e-08 1.34e-07 2.94e-07 1.05e-07 3.06e-07 3.18e-07   erg/cm2
Peak flux Cutoff-PL 1.81e-01 1.38e-01 2.25e-02 4.20e-04 3.43e-01 3.45e-01   ph/cm2/s
              Error 1.50e-01 1.15e-01 3.71e-02 2.89e-02 1.57e-01 1.66e-01   ph/cm2/s
 
Fluence        Band 0.00e+00 0.00e+00 0.00e+00 0.00e+00 0.00e+00 0.00e+00   erg/cm2
              Error 0.00e+00 0.00e+00 0.00e+00 0.00e+00 0.00e+00 0.00e+00   erg/cm2
Peak flux      Band 3.73e-01 0.00e+00 0.00e+00 0.00e+00 0.00e+00 0.00e+00   ph/cm2/s
              Error 0.00e+00 0.00e+00 0.00e+00 0.00e+00 0.00e+00 0.00e+00   ph/cm2/s

 
=== Time-averaged spectral analysis ===
 
Model Ph_index Ph_90err Epeak  Epeak_90err Norm     Nomr_90err chi2   dof
PL    1.398    0.358    -      -           1.42e-04 3.42e-05   95.810 57
CPL  -2.845    2.799      47.7   12.7      3.55e-02 5.92e+01   84.610 56
 
The chi2 of BB fit is 85.65 which shows a significant improvement in the fit over a PL.
Check the BB fit.
 
=== 1-s peak spectral analysis ===
 
Model Ph_index Ph_90err Epeak  Epeak_90err Norm     Nomr_90err chi2   dof
PL    2.543    0.999    -      -           1.81e-03 1.22e-03   46.740 57
CPL   0.672    0.000      24.1    0.0      2.91e-02 0.00e+00   46.450 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  963.264  -29.784  933.480
T90   890.432   34.408  924.840
T50   861.376   38.312  899.688
Peak    1.000  -29.804  -28.804

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
  265.2088 -28.0905 0.0340   20.7   19.9       0.7676     5.7  TRIG_00505516       
------------------------------------------
 
Foreground time interval of the image:
-29.784  72.901 (delta_t = 102.685 [sec])
Background time interval of the image:
-239.000 -29.784 (delta_t = 209.216 [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

8 ms binning

From T100_start-3 s to T100_start+3 s

2 ms binning

From T100_start-1 s to T100_start+1 s

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

Multiple GTIs in the spectrum
tstart tstop
-29.784000 501.980000
503.000000 933.480000
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.39841     ( -0.359493   0.35678 )
Norm@50keV  : 1.42163E-04    ( -3.42493e-05   3.42411e-05 )
------------------------------------------------------------
# Chi-Squared =          95.81 using 59 PHA bins.
# Reduced chi-squared =          1.681 for     57 degrees of freedom 
# Null hypothesis probability =   9.865871e-04
 
Photon flux (15-150 keV)    in 962.2 sec: 1.72911E-02 ( -0.00422141  0.00426556 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.32405e-06 ( -3.36946e-07  3.45799e-07 ) ergs/cm2

Cutoff power-law model

Multiple GTIs in the spectrum
tstart tstop
-29.784000 501.980000
503.000000 933.480000
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: -2.84498     ( -3.03688   2.5617 )
Epeak [keV] : 47.6627      ( -9.47324 15.9221 )
Norm@50keV  : 3.54867E-02    ( -0.0418639   118.419 )
------------------------------------------------------------
# Chi-Squared =          84.61 using 59 PHA bins.
# Reduced chi-squared =          1.511 for     56 degrees of freedom 
# Null hypothesis probability =   8.068343e-03
 
Photon flux (15-150 keV)    in 962.2 sec: 1.53483E-02 ( -0.003886  0.0041563 ) ph/cm2/s
Energy fluence (15-150 keV)             : 9.37354e-07 ( -2.61538e-07  3.50454e-07 ) ergs/cm2

Band function

Multiple GTIs in the spectrum
tstart tstop
-29.784000 501.980000
503.000000 933.480000
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : 4.99975   ( -7714.38   -7699.39 )
beta        : -2.72612    ( 2.72562   0.970395 )
Epeak [keV] : 40.1589      ( -8.58969 8.93898 )
Norm@50keV   : 1.07994    ( -1.08045   3.55156 )
------------------------------------------------------------
# Chi-Squared =          82.32 using 59 PHA bins.
# Reduced chi-squared =          1.497 for     55 degrees of freedom 
# Null hypothesis probability =   9.941048e-03
 
Photon flux (15-150 keV)    in 962.2 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]    : 13.2036  (-2.50758  3.44358)
R^2/D10^2   : 3.49277E-03  (-0.0020076   0.0040648)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
# Chi-Squared =          85.65 using 59 PHA bins.
# Reduced chi-squared =          1.503 for     57 degrees of freedom 
# Null hypothesis probability =   8.379581e-03
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.242e-07   6.021e-08
25- 50  4.350e-07   1.734e-07
50-150  4.838e-07   2.501e-07
15-150  1.043e-06   4.088e-07

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 199.363       (-117.845      -199.993)
Norm        : 7.29851E-02       (-0.0172061     0.019516)
------------------------------------------------------------
# Chi-Squared =          94.20 using 59 PHA bins.
# Reduced chi-squared =          1.653 for     57 degrees of freedom 
# Null hypothesis probability =   1.412322e-03
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.749e-07   1.005e-07
25- 50  3.364e-07   1.891e-07
50-150  7.378e-07   4.282e-07
15-150  1.249e-06   7.231e-07

Double BB

------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 1.00000E-04        (      )
R1^2/D10^2  : 3.47526E-07        (-3.47526e-07      -3.47526e-07)
kT2 [keV]   : 13.2033        (-2.50729      3.44387)
R2^2/D10^2  : 3.49304E-03    (-0.00200787   0.00406453)
------------------------------------------------------------
# Chi-Squared =          85.77 using 59 PHA bins.
# Chi-Squared =          85.65 using 59 PHA bins.
# Reduced chi-squared =          1.559 for     55 degrees of freedom 
# Reduced chi-squared =          1.557 for     55 degrees of freedom 
# Null hypothesis probability =   4.980631e-03
# Null hypothesis probability =   5.107929e-03
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.339e-07   8.453e-08
25- 50  4.459e-07   2.611e-07
50-150  4.403e-07   3.051e-07
15-150  1.020e-06   5.999e-07

Peak spectrum fit

Power-law model

Time interval is from  -29.804 sec. to  -28.804 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 2.54326     ( -0.795053   1.20223 )
Norm@50keV  : 1.80712E-03    ( -0.00121713   0.00121593 )
------------------------------------------------------------
# Chi-Squared =          46.74 using 59 PHA bins.
# Reduced chi-squared =         0.8200 for     57 degrees of freedom 
# Null hypothesis probability =   8.320626e-01
 
Photon flux (15-150 keV)    in 1 sec: 0.364621 ( -0.141277  0.141366 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.82892e-08 ( -8.54216e-09  9.69947e-09 ) ergs/cm2

Cutoff power-law model

Time interval is from  -29.804 sec. to  -28.804 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 0.672377     (     )
Epeak [keV] : 24.0934      (   )
Norm@50keV  : 2.90785E-02    (     )
------------------------------------------------------------
# Chi-Squared =          46.45 using 59 PHA bins.
# Reduced chi-squared =         0.8294 for     56 degrees of freedom 
# Null hypothesis probability =   8.148124e-01
 
Photon flux (15-150 keV)    in 1 sec: 0.342957 ( -0.162926  0.151117 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.54333e-08 ( -7.44944e-09  1.1866e-08 ) ergs/cm2

Band function

Time interval is from  -29.804 sec. to  -28.804 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : 1.59949   ( -1.59171   -1.59171 )
beta        : -3.73962    ( 3.73899   1.94015 )
Epeak [keV] : 27.6119      ( -27.6009 16.3254 )
Norm@50keV   : 1.01493    ( -0.968807   120.948 )
------------------------------------------------------------
# Chi-Squared =          46.39 using 59 PHA bins.
# Reduced chi-squared =         0.8435 for     55 degrees of freedom 
# Null hypothesis probability =   7.890599e-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]    : 7.31317  (-2.26147  3.32483)
R^2/D10^2   : 0.589484  (-0.589484   2.19966)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
# Chi-Squared =          46.42 using 59 PHA bins.
# Reduced chi-squared =         0.8144 for     57 degrees of freedom 
# Null hypothesis probability =   8.405071e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  5.288e-09   3.430e-09
25- 50  7.872e-09   4.937e-09
50-150  1.524e-09   1.299e-09
15-150  1.468e-08   9.390e-09

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 29.9389       (-17.4461      71.2729)
Norm        : 2.94325       (-1.68377     4.83119)
------------------------------------------------------------
# Chi-Squared =          46.50 using 59 PHA bins.
# Reduced chi-squared =         0.8157 for     57 degrees of freedom 
# Null hypothesis probability =   8.384543e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  5.984e-09   3.807e-09
25- 50  6.830e-09   4.476e-09
50-150  3.730e-09   3.362e-09
15-150  1.654e-08   1.100e-08

Double BB

------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 0.884511        (-1.09282      1.2796)
R1^2/D10^2  : 3.11315E+06        (      )
kT2 [keV]   : 8.22715        (-2.56845      4.47881)
R2^2/D10^2  : 0.327804    (-0.274347   0.473235)
------------------------------------------------------------
# Chi-Squared =          42.97 using 59 PHA bins.
# Chi-Squared =          42.79 using 59 PHA bins.
# Reduced chi-squared =         0.7813 for     55 degrees of freedom 
# Reduced chi-squared =         0.7780 for     55 degrees of freedom 
# Null hypothesis probability =   8.806146e-01
# Null hypothesis probability =   8.846277e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  5.297e-09   2.661e-09
25- 50  7.438e-09   4.749e-09
50-150  2.239e-09   1.695e-09
15-150  1.498e-08   9.025e-09

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: 1.88314     ( -0.396205   0.420202 )
Norm@50keV  : 4.02337E-04    ( -0.000113983   0.000111659 )
------------------------------------------------------------
# Chi-Squared =          61.98 using 59 PHA bins.
# Reduced chi-squared =          1.087 for     57 degrees of freedom 
# Null hypothesis probability =   3.031741e-01
 
Photon flux (15-150 keV)    in 102.7 sec: 5.73316E-02 ( -0.0136864  0.0136981 ) ph/cm2/s
Energy fluence (15-150 keV)             : 3.79802e-07 ( -1.03523e-07  1.08745e-07 ) ergs/cm2

Cutoff power-law model

Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: -1.65234     ( -3.57189   2.79669 )
Epeak [keV] : 35.9487      ( -6.88309 14.3718 )
Norm@50keV  : 7.24601E-02    ( -0.0858656   1562.05 )
------------------------------------------------------------
# Chi-Squared =          56.94 using 59 PHA bins.
# Reduced chi-squared =          1.017 for     56 degrees of freedom 
# Null hypothesis probability =   4.398984e-01
 
Photon flux (15-150 keV)    in 102.7 sec: 5.22667E-02 ( -0.0129549  0.0134114 ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.72763e-07 ( -7.50326e-08  1.05634e-07 ) ergs/cm2

Band function

 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : 4.99993   ( -25631.3   -25616.3 )
beta        : -2.81808    ( -2.30101   0.809961 )
Epeak [keV] : 29.7187      ( -5.5717 6.13207 )
Norm@50keV   : 24.1857    ( -24.8398   68.0024 )
------------------------------------------------------------
# Chi-Squared =          54.41 using 59 PHA bins.
# Reduced chi-squared =         0.9893 for     55 degrees of freedom 
# Null hypothesis probability =   4.970734e-01
 
Photon flux (15-150 keV)    in 102.7 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)  = 3.10057e-07
S(50-100 keV) = 4.72272e-07

T90 vs. Hardness ratio plot

T90                                   = 890.432000041008 sec.
Hardness ratio (energy fluence ratio) = 1.52318

Color vs. Color plot

Count Ratio  (25-50 keV) / (15-25 keV) = 6.56363
Count Ratio (50-100 keV) / (15-25 keV) = 3.32928

Mask shadow pattern

IMX = 3.543051582569957E-01, IMY = -1.285547450117715E-01

TIME vs. PHA plot around the trigger time

TIME vs. DetID plot around the trigger time

100 us light curve (15-350 keV)

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:
-239.000000 -29.784000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
170.4615 -60.7202   12.1  47.4 -154.4  -0.4330  -1.0    7.2	Cen X-3                       
186.6565 -62.7701   42.4  39.5 -154.7   0.0879   0.3    0.0	GX 301-2                      
244.9832 -15.6415    0.3  30.7  -28.4   9.1785  42.2    0.2	Sco X-1                       
256.0889 -37.8251    7.7   8.6    7.7   0.2818   1.5    5.0	4U 1700-377                   
256.3423 -36.3997    3.8  10.0    6.0   0.5686   3.0    4.7	GX 349+2                      
263.1789 -24.6410   42.0  23.1   11.7  -0.0552  -0.3   11.2	GX 1+4                        
264.6535 -44.5919   72.3   9.1   71.4   0.0291   0.2    9.3	4U 1735-44                    
268.4219  -1.4665    6.8  46.7    7.6   0.7181   1.7    3.3	SW J1753.5-0127               
270.3759 -24.9408    6.4  25.7   26.3   0.3837   1.8    9.7	GX 5-1                        
270.1423 -25.8743    0.0  24.7   27.0  -0.3890  -1.9   11.7	GRS 1758-258                  
274.1086 -14.0034    5.6  37.0   22.3   0.6399   2.0    6.3	GX 17+2                       
275.9451 -30.3850    3.3  24.3   43.5   0.8566   3.5    1.5	H1820-303                     
285.0303 -24.9673   29.0  33.8   47.8   0.1392   0.4    2.8	HT1900.1-2455                 
263.1404 -33.7035    6.8  14.9   24.0   0.3367   1.7   10.9	GX 354-0                      
306.9652 -40.3231    3.3  39.9   87.0   3.0349   3.5 ------	UNKNOWN                       
277.1758 -33.5118    3.0  22.9   51.0   0.9676   3.8 ------	UNKNOWN                       
272.7057 -28.7706    2.3  23.7   35.7   1.1248   4.9 ------	UNKNOWN                       
218.8746 -88.3723    2.7  42.8  165.8   1.6744   4.3 ------	UNKNOWN                       
107.9587 -79.1694    2.7  53.2  172.5   3.3056   4.2 ------	UNKNOWN                       
165.7779 -70.2648    3.1  46.3 -167.7   1.3502   3.7 ------	UNKNOWN

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

Time interval of the image:
-29.784000 72.900590
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
170.5455 -60.6889  246.1  47.4 -154.4  -0.0125  -0.0    7.8	Cen X-3                       
186.6605 -62.9052    5.5  39.5 -155.0   0.3851   2.1    8.1	GX 301-2                      
244.8085 -15.6849   11.3  30.7  -28.8   0.1481   1.0   10.2	Sco X-1                       
255.7614 -37.9574    0.0   8.4    6.4  -0.2511  -1.9   12.6	4U 1700-377                   
256.6077 -36.4809    8.3  10.0    7.3  -0.1815  -1.4    9.0	GX 349+2                      
263.0672 -24.6809    5.6  23.0   11.5   0.2958   2.1    5.0	GX 1+4                        
264.9299 -44.6143    0.0   9.3   71.8  -0.2552  -2.0   12.7	4U 1735-44                    
268.3662  -1.4741   95.7  46.7    7.6   0.0351   0.1    1.3	SW J1753.5-0127               
270.2749 -24.9969    9.2  25.6   26.2  -0.1833  -1.3    5.0	GX 5-1                        
270.4202 -25.6073   15.4  25.1   27.2  -0.1077  -0.7   10.3	GRS 1758-258                  
274.1349 -14.0654    8.2  36.9   22.4   0.2995   1.4    7.7	GX 17+2                       
276.0090 -30.4396    7.5  24.3   43.7  -0.2446  -1.5    6.2	H1820-303                     
285.0143 -24.7835    7.9  33.9   47.6  -0.3383  -1.5    8.3	HT1900.1-2455                 
262.9893 -33.7470    3.9  14.8   23.7  -0.3913  -3.0    5.3	GX 354-0                      
  5.4816 -76.0416    2.4  51.1  148.0   3.1905   4.8 ------	UNKNOWN                       
265.2087 -28.0905    2.0  20.7   19.9   0.7677   5.7 ------	UNKNOWN                       
176.6592 -68.2427    2.4  42.9 -163.8   0.9210   4.8 ------	UNKNOWN

Post-slew image of 15-350 keV band

Time interval of the image:
114.900640 501.980000
503.000000 912.300600
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
244.9774 -15.6434    0.2  22.5  -64.6  37.9353  52.7    0.2	Sco X-1                       
256.1947 -37.7392    5.1  12.3 -148.3   1.4102   2.2   11.7	4U 1700-377                   
256.6136 -36.4103    4.9  11.0 -145.1   1.4903   2.3    8.6	GX 349+2                      
262.8323 -24.8586    3.8   3.9  -37.9   1.8376   3.0   11.8	GX 1+4                        
264.5489 -44.3753    8.6  16.3  177.7   0.7542   1.3    9.4	4U 1735-44                    
268.4359  -1.4229    3.5  26.8    3.2   1.8776   3.2    4.4	SW J1753.5-0127               
270.4156 -25.2325    5.1   5.5   55.7   1.2870   2.3   11.6	GX 5-1                        
270.2339 -25.7685    3.4   5.0   59.9   2.1964   3.9    4.0	GRS 1758-258                  
273.9523 -14.0550    2.0  16.2   27.9   3.0504   5.7    3.3	GX 17+2                       
275.7487 -30.2456    3.9   9.5  101.8   1.6633   2.9   11.7	H1820-303                     
285.1292 -24.8080    4.3  18.1   80.2   1.6512   2.7    8.4	HT1900.1-2455                 
288.8192  11.0845    6.8  45.3   29.6   2.5379   1.7    8.4	GRS 1915+105                  
262.9866 -33.8012    3.9   6.0 -166.1   1.6628   3.0    2.0	GX 354-0                      
308.7036 -21.5037    3.4  39.8   86.5   9.4143   3.4 ------	UNKNOWN                       
281.8495  -9.4053    2.3  24.4   39.2   3.2868   5.0 ------	UNKNOWN                       
231.4923 -68.0995    2.8  44.7 -166.9   4.2637   4.0 ------	UNKNOWN                       
253.3652  -1.9256    2.6  28.5  -29.4   2.7289   4.4 ------	UNKNOWN                       
189.5409 -68.3011    4.2  58.8 -159.2  13.0003   2.8 ------	UNKNOWN                       
235.1146   7.3449    3.7  45.8  -47.9   6.4491   3.2 ------	UNKNOWN                       
200.0165 -53.9033    3.4  53.2 -142.1  12.3990   3.4 ------	UNKNOWN                       
228.2853  -2.0642    4.3  43.8  -64.1   7.7130   2.7 ------	UNKNOWN

Plot creation:
Sat Oct 15 15:08:48 EDT 2011