batgrbproduct analysis for trigger=419015

batgrbproduct Analysis for Trigger=419015

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 page will be updated for up to 8 downlinks after the trigger.

======================================================================
                  BAT GRB EVENT DATA PROCESSING REPORT
    Process Script Ver: batgrbproduct v2.45
    Process Start Time (local time): Sun Apr 11 14:16:28 EDT 2010
             Host Name: gcn5
   Current Working Dir: /local/data/raid16/prebascript_archive/trigger419015/GCN5_download_cron
======================================================================

  Trigger: 00419015      Segment: 000

  BAT Trigger Time: 292577266.24   [s; MET]
      Trigger Stop: 292577267.264   [s; MET]
               UTC: 2010-04-10T07:27:40.546740    [includes UTCF correction] 
       Where From?: TDRSS position message

  BAT 
    RA: 293.31015696162   Dec: -34.3087131523313  [deg; J2000]

     Catalogged Source?: NO
     Point Source?:      YES
     GRB Indicated?:     YES    [ by BAT flight software ]
     Image S/N Ratio:    7.29
     Image Trigger?:     NO
     Rate S/N Ratio:     17.6635217326557  [ if not an image trigger ]
     Image S/N Ratio:    7.29

  Flight Position:   [ source = BAT ]
    RA: 293.31015696162   Dec: -34.3087131523313  [deg; J2000]

  Ground Position:   [ source = BAT pre-slew burst ]
    RA: 293.325081692273   Dec: -34.3196326539268  [deg; J2000]  
        { 19h 33m 18.0s , -34d 19' 10.7" }
         +/- 3.53858532522285 [arcmin] (estimated 90% radius based on SNR)
         +/- 1.51954763560159 [arcmin] (formal 1-sigma fit error)
    SNR: 5.00122036817166
 
  Angular difference between Flight and Ground position is 0.988081 arcmin
 
  Partial Coding Fraction: 1    [ including projection effects ]

  Duration
     T90: 1.02399998903275 +/- 35.7770876399966
        Measured from: 0
                   to: 1.02399998903275     [s; relative to TRIGTIME]
     T50: 1.02399998903275 +/- 16
        Measured from: 0
                   to: 1.02399998903275     [s; relative to TRIGTIME]

    WARNING: battblocks failed.  Used TDRSS fore/background intervals

  Fluence
     Peak Flux  (peak 1.02399998903275 second)
        Measured from: -2.98023223876953e-08     
                   to: 1.02399995923042     [s; relative to TRIGTIME]
     Total Fluence        
        Measured from: 0     
                   to: 1.02399998903275     [s; relative to TRIGTIME]
     
             Band 1     Band 2     Band 3     Band 4
              15-25      25-50     50-100    100-350     keV
 Total     0.003422  -0.000661   0.024055   0.023526
           0.006270   0.006418   0.005887   0.006583 [error]
 Peak      0.003422  -0.000661   0.024055   0.023526
           0.006270   0.006418   0.005887   0.006583 [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 3.64e-10 2.22e-09 1.18e-08 2.84e-07 3.85e-08 3.00e-07   erg/cm2
              Error 6.50e-10 2.39e-09 7.72e-09 3.94e-07 1.58e-08 3.98e-07   erg/cm2
Peak flux Power-law 1.10e-02 3.57e-02 9.47e-02 7.36e-01 2.59e-01 8.83e-01   ph/cm2/s
              Error 2.00e-02 3.94e-02 6.99e-02 7.87e-01 1.60e-01 7.48e-01   ph/cm2/s
 
Fluence   Cutoff-PL 1.51e-10 1.48e-10 1.99e-09 1.48e-08 6.22e-08 3.94e-08   erg/cm2
              Error 2.04e-09 6.68e-09 2.98e-07 1.62e-08 2.81e-07 0.00e+00   erg/cm2
Peak flux Cutoff-PL 1.10e-02 3.56e-02 9.49e-02 7.33e-01 2.59e-01 8.75e-01   ph/cm2/s
              Error 2.00e-02 3.94e-02 7.00e-02 8.18e-01 1.59e-01 7.70e-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 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   -0.411    1.356    -      -           1.61e-03 1.44e-03   46.190 57
CPL  -4.982    0.000     124.5   51.3      2.49e-02 2.48e-02   43.530 56
 
 
=== 1-s peak spectral analysis ===
 
Model Ph_index Ph_90err Epeak  Epeak_90err Norm     Nomr_90err chi2   dof
PL   -0.409    1.353    -      -           1.61e-03 1.44e-03   46.370 57
CPL  -4.982    0.000     124.4   51.1      2.50e-02 2.48e-02   43.690 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: 0.896000 sec.
T50 in the 50-300 keV band: 0.448000 sec.

 
=== Table of the duration information ==
 
        Value   tstart    tstop
T100    1.024    0.000    1.024
T90     1.024    0.000    1.024
T50     1.024    0.000    1.024
Peak    1.024   -0.000    1.024

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
  293.3251 -34.3196 0.0384   10.1   33.3       0.0665     5.0  TRIG_00419015       
------------------------------------------
 
Foreground time interval of the image:
  0.000   1.024 (delta_t =   1.024 [sec])
Background time interval of the image:
-54.139 -54.105 (delta_t =   0.035 [sec])
-17.240 -10.240 (delta_t =   7.000 [sec])

Lightcurves

Notes:

1) All plots contain as much data as has been downloaded to date.
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)

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    0.000 sec. to    1.024 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: -0.411068     ( -1.81168   0.899519 )
Norm@50keV  : 1.60680E-03    ( -0.00160725   0.00127694 )
------------------------------------------------------------
# Chi-Squared =          46.19 using 59 PHA bins.
# Reduced chi-squared =         0.8103 for     57 degrees of freedom 
# Null hypothesis probability =   8.464231e-01
 
Photon flux (15-150 keV)    in 1.024 sec: 0.257963 ( -0.202031  0.118508 ) ph/cm2/s
Energy fluence (15-150 keV)             : 3.85001e-08 ( -1.57861e-08  1.58038e-08 ) ergs/cm2

Cutoff power-law model

Time interval is from    0.000 sec. to    1.024 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: -4.98200     (     )
Epeak [keV] : 124.451      ( -30.9442 71.7006 )
Norm@50keV  : 2.49210E-02    ( -0.024921   0.0245996 )
------------------------------------------------------------
# Chi-Squared =          43.53 using 59 PHA bins.
# Reduced chi-squared =         0.7772 for     56 degrees of freedom 
# Null hypothesis probability =   8.879024e-01
 
Photon flux (15-150 keV)    in 1.024 sec: 0.258123 ( -0.199098  0.118353 ) ph/cm2/s
Energy fluence (15-150 keV)             : 3.94332e-08 ( -1.59299e-08  1.64712e-08 ) ergs/cm2

Band function

Time interval is from    0.000 sec. to    1.024 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -0.398661   ( 0.398273   0.398273 )
beta        : 0.410487    ( -0.897841   1.81607 )
Epeak [keV] : 13.6464      ( -13.641 -13.641 )
Norm@50keV   : 2.86184E-03    ( 1684.47   -0.00286034 )
------------------------------------------------------------
# Chi-Squared =          46.19 using 59 PHA bins.
# Reduced chi-squared =         0.8398 for     55 degrees of freedom 
# Null hypothesis probability =   7.953676e-01
 
Photon flux (15-150 keV)    in 1.024 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]    : 66.7389  (-66.736  -66.736)
R^2/D10^2   : 7.77248E-04  (-0.000777282   0.00359949)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
# Chi-Squared =          45.53 using 59 PHA bins.
# Reduced chi-squared =         0.7987 for     57 degrees of freedom 
# Null hypothesis probability =   8.628067e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  3.064e-10   2.340e-10
25- 50  2.343e-09   1.762e-09
50-150  3.646e-08   2.490e-08
15-150  3.911e-08   2.439e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 199.363       (-199.999      -199.999)
Norm        : 0.747149       (-0.563056     0.563055)
------------------------------------------------------------
# Chi-Squared =          57.53 using 59 PHA bins.
# Reduced chi-squared =          1.009 for     57 degrees of freedom 
# Null hypothesis probability =   4.553923e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.905e-09   1.348e-09
25- 50  3.665e-09   2.760e-09
50-150  8.037e-09   6.216e-09
15-150  1.361e-08   1.047e-08

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 0.102252        (-0.102252      -0.102252)
R1^2/D10^2  : 6.85532E-03        (-0.00685268      -0.00685268)
kT2 [keV]   : 63.0019        (-63.444      -63.444)
R2^2/D10^2  : 8.69280E-04    (-0.000853872   0.00352415)
------------------------------------------------------------
# Chi-Squared =          45.53 using 59 PHA bins.
# Reduced chi-squared =         0.8279 for     55 degrees of freedom 
# Null hypothesis probability =   8.148149e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  0.000e+00   0.000e+00
25- 50  0.000e+00   0.000e+00
50-150  0.000e+00   0.000e+00
15-150  0.000e+00   0.000e+00

Peak spectrum fit

Power-law model

Time interval is from    0.000 sec. to    1.024 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: -0.409180     ( -1.80995   0.896546 )
Norm@50keV  : 1.61217E-03    ( -0.00161259   0.00127598 )
------------------------------------------------------------
# Chi-Squared =          46.37 using 59 PHA bins.
# Reduced chi-squared =         0.8136 for     57 degrees of freedom 
# Null hypothesis probability =   8.416919e-01
 
Photon flux (15-150 keV)    in 1.024 sec: 0.258589 ( -0.201874  0.118412 ) ph/cm2/s
Energy fluence (15-150 keV)             : 3.85783e-08 ( -1.57684e-08  1.57864e-08 ) ergs/cm2

Cutoff power-law model

Time interval is from    0.000 sec. to    1.024 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: -4.98166     (     )
Epeak [keV] : 124.379      ( -30.8385 71.3663 )
Norm@50keV  : 2.50448E-02    ( -0.0250448   0.024555 )
------------------------------------------------------------
# Chi-Squared =          43.69 using 59 PHA bins.
# Reduced chi-squared =         0.7802 for     56 degrees of freedom 
# Null hypothesis probability =   8.843592e-01
 
Photon flux (15-150 keV)    in 1.024 sec: 0.258746 ( -0.198907  0.118282 ) ph/cm2/s
Energy fluence (15-150 keV)             : 3.95035e-08 ( -1.59084e-08  1.64469e-08 ) ergs/cm2

Band function

Time interval is from    0.000 sec. to    1.024 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -0.383453   ( 0.382711   0.382711 )
beta        : 0.408793    ( -0.895981   1.81234 )
Epeak [keV] : 13.7740      ( -13.7761 -13.7761 )
Norm@50keV   : 2.87119E-03    ( -0.00287137   44282.3 )
------------------------------------------------------------
# Chi-Squared =          46.37 using 59 PHA bins.
# Reduced chi-squared =         0.8431 for     55 degrees of freedom 
# Null hypothesis probability =   7.897450e-01
 
Photon flux (15-150 keV)    in 1.024 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]    : 62.2931  (-62.384  -62.384)
R^2/D10^2   : 8.90737E-04  (-0.000885687   0.003499)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
# Chi-Squared =          45.71 using 59 PHA bins.
# Reduced chi-squared =         0.8020 for     57 degrees of freedom 
# Null hypothesis probability =   8.582930e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  3.239e-10   2.541e-10
25- 50  2.447e-09   1.740e-09
50-150  3.620e-08   2.410e-08
15-150  3.897e-08   2.518e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 199.363       (-199.954      -199.954)
Norm        : 0.749293       (-0.562521     0.56225)
------------------------------------------------------------
# Chi-Squared =          57.78 using 59 PHA bins.
# Reduced chi-squared =          1.014 for     57 degrees of freedom 
# Null hypothesis probability =   4.463246e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.911e-09   1.461e-09
25- 50  3.675e-09   2.715e-09
50-150  8.061e-09   5.806e-09
15-150  1.365e-08   9.815e-09

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 0.122913        (-0.122913      -0.122913)
R1^2/D10^2  : 1.67501E-02        (-0.0167435      -0.0167435)
kT2 [keV]   : 62.8591        (-63.3011      -63.3011)
R2^2/D10^2  : 8.75025E-04    (-0.000859475   0.00352215)
------------------------------------------------------------
# Chi-Squared =          45.71 using 59 PHA bins.
# Reduced chi-squared =         0.8311 for     55 degrees of freedom 
# Null hypothesis probability =   8.096477e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  0.000e+00   0.000e+00
25- 50  0.000e+00   0.000e+00
50-150  0.000e+00   0.000e+00
15-150  0.000e+00   0.000e+00

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: -0.411068     ( -1.81168   0.899519 )
Norm@50keV  : 1.60680E-03    ( -0.00160725   0.00127694 )
------------------------------------------------------------
# Chi-Squared =          46.19 using 59 PHA bins.
# Reduced chi-squared =         0.8103 for     57 degrees of freedom 
# Null hypothesis probability =   8.464231e-01
 
Photon flux (15-150 keV)    in 1.024 sec: 0.257963 ( -0.202031  0.118508 ) ph/cm2/s
Energy fluence (15-150 keV)             : 3.85001e-08 ( -1.57861e-08  1.58038e-08 ) ergs/cm2

Cutoff power-law model

Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: -4.98200     (     )
Epeak [keV] : 124.451      ( -30.9442 71.7006 )
Norm@50keV  : 2.49210E-02    ( -0.024921   0.0245996 )
------------------------------------------------------------
# Chi-Squared =          43.53 using 59 PHA bins.
# Reduced chi-squared =         0.7772 for     56 degrees of freedom 
# Null hypothesis probability =   8.879024e-01
 
Photon flux (15-150 keV)    in 1.024 sec: 0.258123 ( -0.199059  0.118376 ) ph/cm2/s
Energy fluence (15-150 keV)             : 3.94332e-08 ( -1.59299e-08  1.64712e-08 ) ergs/cm2

Band function

 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -0.398661   ( 0.398273   0.398273 )
beta        : 0.410487    ( -0.897841   1.81607 )
Epeak [keV] : 13.6464      ( -13.641 -13.641 )
Norm@50keV   : 2.86184E-03    ( 1684.47   -0.00286034 )
------------------------------------------------------------
# Chi-Squared =          46.19 using 59 PHA bins.
# Reduced chi-squared =         0.8398 for     55 degrees of freedom 
# Null hypothesis probability =   7.953676e-01
 
Photon flux (15-150 keV)    in 1.024 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)  = 2.21935e-09
S(50-100 keV) = 1.18065e-08

T90 vs. Hardness ratio plot

T90                                   = 1.02399998903275 sec.
Hardness ratio (energy fluence ratio) = 5.3198

Color vs. Color plot

Count Ratio  (25-50 keV) / (15-25 keV) = -0.193162
Count Ratio (50-100 keV) / (15-25 keV) = 7.02951

Mask shadow pattern

IMX = 1.492324766306893E-01, IMY = -9.792494225213652E-02

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:
-54.139410 -54.104800
-17.240000 -10.240000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
255.9477 -37.8176  221.3  37.7   71.1  -0.0054  -0.1    2.4	4U 1700-377                   
256.4279 -36.4220  282.1  37.1   73.3  -0.0041  -0.0    0.4	GX 349+2                      
262.9756 -24.7751   22.5  31.6   94.1   0.0329   0.5    2.5	GX 1+4                        
264.9298 -44.6059   17.7  33.1   56.5   0.0394   0.6   12.3	4U 1735-44                    
268.2355  -1.3892    7.6  37.1  136.2   0.1032   1.5    8.8	SW J1753.5-0127               
270.4174 -25.2001    3.2  24.8   94.9   0.1916   3.6   10.2	GX 5-1                        
270.4663 -25.8801    0.0  24.7   93.3  -0.0415  -0.8   12.1	GRS 1758-258                  
274.0134 -14.1766    8.8  24.9  122.5   0.0561   1.3    8.4	GX 17+2                       
276.0670 -30.2250   16.5  20.0   81.2  -0.0291  -0.7   11.3	H1820-303                     
285.1049 -24.9573    3.1  11.6   98.8   0.1315   3.7    4.3	HT1900.1-2455                 
288.8013  10.9315    3.1  37.0  176.3   0.1772   3.7    0.9	GRS 1915+105                  
300.0648  29.8896    2.8  54.9 -166.4   0.4746   4.1 ------	UNKNOWN

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

Time interval of the image:
0.000000 1.024000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
256.1700 -37.7579    6.2  37.5   71.1  -0.0775  -1.8   10.1	4U 1700-377                   
256.4262 -36.4493    8.9  37.1   73.2   0.0535   1.3    1.6	GX 349+2                      
262.8551 -24.6101    0.0  31.7   94.4   0.0326   1.2   11.7	GX 1+4                        
264.8129 -44.4866    6.0  33.1   56.8   0.0511   1.9    3.7	4U 1735-44                    
268.4194  -1.3041   97.5  37.0  136.5  -0.0031  -0.1    9.4	SW J1753.5-0127               
270.1982 -24.9431   21.3  25.1   95.5   0.0108   0.5    9.4	GX 5-1                        
270.3753 -25.7778   26.2  24.8   93.5   0.0089   0.4    4.5	GRS 1758-258                  
274.0052 -14.0391  587.5  25.0  122.8  -0.0004  -0.0    0.2	GX 17+2                       
275.8686 -30.2263    4.7  20.2   81.3   0.0398   2.4    8.9	H1820-303                     
285.1265 -25.0021   12.8  11.6   98.6  -0.0129  -0.9    6.9	HT1900.1-2455                 
288.7536  10.8913    7.2  37.0  176.2  -0.0302  -1.6    4.2	GRS 1915+105                  
285.0854  19.8253    2.4  46.5  174.6   0.1464   4.9 ------	UNKNOWN                       
310.0289   2.1573    2.5  29.6 -143.6   0.0695   4.6 ------	UNKNOWN

Post-slew image of 15-350 keV band

Time interval of the image:
45.560600 101.460000
102.760000 122.760000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
255.9338 -37.7801    8.6  30.2   81.7   1.9300   1.3    4.6	4U 1700-377                   
256.5119 -36.3039   10.2  29.9   84.8  -1.6094  -1.1    8.0	GX 349+2                      
263.1509 -24.8886    0.0  27.7  111.0   1.3906   1.0   11.5	GX 1+4                        
264.6766 -44.3710   10.7  24.2   66.1  -1.2261  -1.1    5.5	4U 1735-44                    
268.3112  -1.4511    5.7  40.3  148.5   3.4124   2.0    3.4	SW J1753.5-0127               
270.2725 -24.9375   32.8  22.0  118.3   0.3367   0.4    8.5	GX 5-1                        
270.3325 -25.6692    4.9  21.6  116.7  -2.2425  -2.3    4.7	GRS 1758-258                  
274.1003 -14.1747    7.8  26.6  143.8  -1.5330  -1.5   10.0	GX 17+2                       
275.9847 -30.2902    3.4  15.2  109.9  -3.3464  -3.4    5.5	H1820-303                     
285.0232 -24.9170   30.1  11.8  149.7  -0.3398  -0.4    0.7	HT1900.1-2455                 
288.6965  10.9068  365.1  45.4 -177.1   0.0524   0.0    6.4	GRS 1915+105                  
282.3631   6.5085    2.3  42.1  172.9   7.6967   5.0 ------	UNKNOWN                       
283.0107  18.8773    3.6  54.1  177.2  14.1198   3.2 ------	UNKNOWN

Plot creation:
Sun Apr 11 14:27:34 EDT 2010