batgrbproduct analysis for trigger=455904

batgrbproduct Analysis for Trigger=455904

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): Tue Jul  5 10:12:47 EDT 2011
             Host Name: gcn5
   Current Working Dir: /local/data/raid16/prebascript_archive/trigger455904/batgroup_hand_proc
======================================================================

  Trigger: 00455904      Segment: 000

  BAT Trigger Time: 330532909.812   [s; MET]
      Trigger Stop: 330532909.844   [s; MET]
               UTC: 2011-06-23T14:41:42.726200    [includes UTCF correction] 
       Where From?: (*SHORT BURST*) TDRSS scaled map message

  BAT 
    RA: 280.316536827048   Dec: -4.93719335603939  [deg; J2000]

     Catalogged Source?: YES
     Point Source?:      YES
     GRB Indicated?:     NO    [ by BAT flight software ]
     Image S/N Ratio:    13.67
     Image Trigger?:     NO
     Rate S/N Ratio:     102.186104730536  [ if not an image trigger ]
     Image S/N Ratio:    13.67

  Flight Position:   [ source = BAT ]
    RA: 280.316536827048   Dec: -4.93719335603939  [deg; J2000]

  Ground Position:   [ source = BAT pre-slew burst ]
    RA: 280.32663448628   Dec: -4.94109856404019  [deg; J2000]  
        { 18h 41m 18.4s , -04d 56' 28.0" }
         +/- 1.52912061566178 [arcmin] (estimated 90% radius based on SNR)
         +/- 0.632816782839611 [arcmin] (formal 1-sigma fit error)
    SNR: 16.5817428172014
 
  Angular difference between Flight and Ground position is 0.647493 arcmin
 
  Partial Coding Fraction: 0.1855469    [ including projection effects ]

  Duration
     T90: 0.0199999809265137 +/- 0.00894426338023564
        Measured from: 0
                   to: 0.0199999809265137     [s; relative to TRIGTIME]
     T50: 0.0119999647140503 +/- 0.004
        Measured from: 0.00400000810623169
                   to: 0.015999972820282     [s; relative to TRIGTIME]



  Fluence
     Peak Flux  (peak 1 second)
        Measured from: -0.486000001430511     
                   to: 0.513999998569489     [s; relative to TRIGTIME]
     Total Fluence        
        Measured from: 0     
                   to: 0.0240000486373901     [s; relative to TRIGTIME]
     
             Band 1     Band 2     Band 3     Band 4
              15-25      25-50     50-100    100-350     keV
 Total     0.135082   0.135671   0.037572  -0.001407
           0.011848   0.012067   0.006624   0.002373 [error]
 Peak      0.176246   0.153967   0.055989   0.005190
           0.018752   0.018403   0.014559   0.011400 [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 4.88e-08 3.92e-08 2.12e-08 1.68e-08 1.17e-07 1.26e-07   erg/cm2
              Error 6.34e-09 4.65e-09 4.14e-09 5.67e-09 1.36e-08 1.58e-08   erg/cm2
Peak flux Power-law 1.96e+00 1.13e+00 4.16e-01 2.02e-01 3.62e+00 3.71e+00   ph/cm2/s
              Error 3.36e-01 1.59e-01 1.07e-01 9.35e-02 4.85e-01 4.97e-01   ph/cm2/s
 
Fluence   Cutoff-PL 4.37e-08 6.12e-08 2.01e-08 8.09e-10 1.26e-07 1.26e-07   erg/cm2
              Error 7.22e-09 8.59e-09 5.58e-09 1.09e-09 1.36e-08 1.36e-08   erg/cm2
Peak flux Cutoff-PL 1.83e+00 1.30e+00 3.71e-01 4.13e-02 3.54e+00 3.54e+00   ph/cm2/s
              Error 3.77e-01 2.30e-01 1.42e-01 1.10e-01 4.93e-01 4.99e-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    2.883    0.177    -      -           4.26e-01 6.55e-02   66.830 57
CPL  -0.214    1.125      28.0    5.0      3.40e+01 9.42e+01   37.000 56
 
The chi2 of BB fit is 40.81 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    2.447    0.262    -      -           1.90e-02 3.77e-03   60.170 57
CPL   1.251    1.197      23.2    0.0      1.06e-01 0.00e+00   57.610 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    0.024    0.000    0.024
T90     0.020    0.000    0.020
T50     0.012    0.004    0.016
Peak    1.000   -0.486    0.514

Click here for the BAT GCN circular template

Image

Pre-slew 15.0-350.0 keV image (Event data)

#   RAcent    DECcent   POSerr    Theta     Phi              Peak Cts       SNR   Name
  280.3266    -4.9411   0.0116    35.6880   117.2420         0.3294945     16.582 TRIG_00455904                 
 
Foreground time interval of the image:
  0.000   0.024 (delta_t =   0.024 [sec])
Background time interval of the image:
-239.812   0.000 (delta_t = 239.812 [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 0.032000

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 0.032000

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 0.032000

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    0.000 sec. to    0.024 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 2.88305     ( -0.169442   0.184746 )
Norm@50keV  : 0.426071    ( -0.0660715   0.0650251 )
------------------------------------------------------------
# Chi-Squared =          66.83 using 59 PHA bins.
# Reduced chi-squared =          1.173 for     57 degrees of freedom 
# Null hypothesis probability =   1.750289e-01
 
Photon flux (15-150 keV)    in 0.024 sec: 107.763 ( -12.3  12.3043 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.16713e-07 ( -1.36285e-08  1.36503e-08 ) ergs/cm2

Cutoff power-law model

Time interval is from    0.000 sec. to    0.024 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: -0.213684     ( -1.2135   1.03731 )
Epeak [keV] : 27.9678      ( -5.99351 3.9565 )
Norm@50keV  : 34.0470    ( -34.047   154.39 )
------------------------------------------------------------
# Chi-Squared =          37.00 using 59 PHA bins.
# Reduced chi-squared =         0.6607 for     56 degrees of freedom 
# Null hypothesis probability =   9.765200e-01
 
Photon flux (15-150 keV)    in 0.024 sec: 113.976 ( -12.571  12.573 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.25729e-07 ( 0  0 ) ergs/cm2

Band function

Time interval is from    0.000 sec. to    0.024 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : 0.214392   ( -0.914598   1.4215 )
beta        : -9.99983    ( 19042.2   19052.2 )
Epeak [keV] : 27.9613      ( -5.99135 3.9553 )
Norm@50keV   : 34.0967    ( -34.0971   155.049 )
------------------------------------------------------------
# Chi-Squared =          37.00 using 59 PHA bins.
# Reduced chi-squared =         0.6727 for     55 degrees of freedom 
# Null hypothesis probability =   9.702661e-01
 
Photon flux (15-150 keV)    in 0.024 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]    : 7.96838  (-0.711508  0.697611)
R^2/D10^2   : 140.201  (-43.2819   67.6577)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
# Chi-Squared =          40.81 using 59 PHA bins.
# Reduced chi-squared =         0.7159 for     57 degrees of freedom 
# Null hypothesis probability =   9.479951e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  3.852e-08   6.264e-09
25- 50  6.696e-08   8.172e-09
50-150  1.735e-08   4.966e-09
15-150  1.228e-07   1.486e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 26.3119       (-3.63484      4.10845)
Norm        : 1071.78       (-188.031     222.593)
------------------------------------------------------------
# Chi-Squared =          43.57 using 59 PHA bins.
# Reduced chi-squared =         0.7643 for     57 degrees of freedom 
# Null hypothesis probability =   9.048330e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  4.865e-08   6.312e-09
25- 50  5.149e-08   6.324e-09
50-150  2.357e-08   6.326e-09
15-150  1.237e-07   1.535e-08

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 3.85619        (-2.85645      12.0539)
R1^2/D10^2  : 982.302        (-875.848      866577)
kT2 [keV]   : 8.97850        (-1.16927      6.92741)
R2^2/D10^2  : 69.3842    (-68.4385   76.8961)
------------------------------------------------------------
# Chi-Squared =          36.52 using 59 PHA bins.
# Reduced chi-squared =         0.6640 for     55 degrees of freedom 
# Null hypothesis probability =   9.740948e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  4.401e-08   2.308e-08
25- 50  6.109e-08   3.392e-08
50-150  2.099e-08   1.200e-08
15-150  1.261e-07   6.536e-08

Peak spectrum fit

Power-law model

Time interval is from   -0.486 sec. to    0.514 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 2.44720     ( -0.247438   0.276197 )
Norm@50keV  : 1.90136E-02    ( -0.00382332   0.00372441 )
------------------------------------------------------------
# Chi-Squared =          60.17 using 59 PHA bins.
# Reduced chi-squared =          1.056 for     57 degrees of freedom 
# Null hypothesis probability =   3.616954e-01
 
Photon flux (15-150 keV)    in 1 sec: 3.61762 ( -0.485122  0.485218 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.87559e-07 ( -2.92037e-08  2.97817e-08 ) ergs/cm2

Cutoff power-law model

Time interval is from   -0.486 sec. to    0.514 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.25064     ( -1.63674   0.757293 )
Epeak [keV] : 23.2226      (   )
Norm@50keV  : 0.105668    (     )
------------------------------------------------------------
# Chi-Squared =          57.61 using 59 PHA bins.
# Reduced chi-squared =          1.029 for     56 degrees of freedom 
# Null hypothesis probability =   4.153107e-01
 
Photon flux (15-150 keV)    in 1 sec: 3.53775 ( -0.49191  0.49342 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.73024e-07 ( -2.9061e-08  3.3148e-08 ) ergs/cm2

Band function

Time interval is from   -0.486 sec. to    0.514 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -1.19595   ( -0.936985   1.20326 )
beta        : -3.67032    ( 3.65127   1.27776 )
Epeak [keV] : 23.7093      ( -12.3086 8.23914 )
Norm@50keV   : 0.114588    ( -0.0363196   5956.51 )
------------------------------------------------------------
# Chi-Squared =          57.35 using 59 PHA bins.
# Reduced chi-squared =          1.043 for     55 degrees of freedom 
# Null hypothesis probability =   3.880320e-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]    : 8.04612  (-1.13058  1.24488)
R^2/D10^2   : 3.92915  (-1.76089   3.3897)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
# Chi-Squared =          64.75 using 59 PHA bins.
# Reduced chi-squared =          1.136 for     57 degrees of freedom 
# Null hypothesis probability =   2.243890e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  4.619e-08   1.195e-08
25- 50  8.166e-08   1.673e-08
50-150  2.185e-08   8.110e-09
15-150  1.497e-07   2.785e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 35.0994       (-9.18751      13.6559)
Norm        : 25.9578       (-6.17322     8.44895)
------------------------------------------------------------
# Chi-Squared =          57.63 using 59 PHA bins.
# Reduced chi-squared =          1.011 for     57 degrees of freedom 
# Null hypothesis probability =   4.517132e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  5.678e-08   9.825e-09
25- 50  7.036e-08   1.127e-08
50-150  4.689e-08   1.960e-08
15-150  1.740e-07   3.405e-08

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 3.49744        (-1.57546      2.2462)
R1^2/D10^2  : 72.1873        (-62.0028      2241.43)
kT2 [keV]   : 10.5073        (-2.14105      4.62804)
R2^2/D10^2  : 1.04594    (-0.883539   1.96116)
------------------------------------------------------------
# Chi-Squared =          56.77 using 59 PHA bins.
# Reduced chi-squared =          1.032 for     55 degrees of freedom 
# Null hypothesis probability =   4.088413e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  5.682e-08   3.006e-08
25- 50  7.152e-08   3.799e-08
50-150  3.825e-08   2.295e-08
15-150  1.666e-07   8.540e-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: 2.88305     ( -0.169442   0.184746 )
Norm@50keV  : 0.426071    ( -0.0660715   0.0650251 )
------------------------------------------------------------
# Chi-Squared =          66.83 using 59 PHA bins.
# Reduced chi-squared =          1.173 for     57 degrees of freedom 
# Null hypothesis probability =   1.750289e-01
 
Photon flux (15-150 keV)    in 0.024 sec: 107.763 ( -12.3  12.3043 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.16713e-07 ( -1.36285e-08  1.36503e-08 ) ergs/cm2

Cutoff power-law model

Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: -0.213684     ( -1.2135   1.03731 )
Epeak [keV] : 27.9678      ( -5.99351 3.9565 )
Norm@50keV  : 34.0470    ( -34.047   154.39 )
------------------------------------------------------------
# Chi-Squared =          37.00 using 59 PHA bins.
# Reduced chi-squared =         0.6607 for     56 degrees of freedom 
# Null hypothesis probability =   9.765200e-01
 
Photon flux (15-150 keV)    in 0.024 sec: 113.976 ( -12.571  12.573 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.25729e-07 ( 0  0 ) ergs/cm2

Band function

 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : 0.214392   ( -0.914598   1.4215 )
beta        : -9.99983    ( 19042.2   19052.2 )
Epeak [keV] : 27.9613      ( -5.99135 3.9553 )
Norm@50keV   : 34.0967    ( -34.0971   155.049 )
------------------------------------------------------------
# Chi-Squared =          37.00 using 59 PHA bins.
# Reduced chi-squared =         0.6727 for     55 degrees of freedom 
# Null hypothesis probability =   9.702661e-01
 
Photon flux (15-150 keV)    in 0.024 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)  = 3.91558e-08
S(50-100 keV) = 2.12356e-08

T90 vs. Hardness ratio plot

T90                                   = 0.0199999809265137 sec.
Hardness ratio (energy fluence ratio) = 0.542336

Color vs. Color plot

Count Ratio  (25-50 keV) / (15-25 keV) = 1.00436
Count Ratio (50-100 keV) / (15-25 keV) = 0.278142

Mask shadow pattern

IMX = -3.287815392335487E-01, IMY = -6.385882527558204E-01

TIME vs. PHA plot around the trigger time

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.032000

TIME vs. DetID plot around the trigger time

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.032000

100 us light curve (15-350 keV)

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.032000

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:
-239.812000 0.000000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
288.7892  10.9491    1.1  26.2  147.5   2.7224  10.1    0.6	GRS 1915+105                  
299.5783  35.1981    0.5  33.1 -159.7   5.5233  21.2    0.6	Cyg X-1                       
308.1905  40.9121    2.5  36.2 -145.1   1.3594   4.6    4.4	Cyg X-3                       
326.0378  38.3615    4.0  34.8 -121.1   1.0753   2.9    6.7	Cyg X-2                       
271.9237  44.3825    2.7  54.1 -173.6   3.2030   4.3 ------	UNKNOWN                       
314.3548  31.3833    3.2  26.2 -137.4   0.8859   3.7 ------	UNKNOWN                       
300.9771  59.4027    4.6  55.3 -145.3   3.6081   2.5 ------	UNKNOWN                       
  5.1619   1.6389    2.8  50.6  -44.8   4.9128   4.2  324.9	UNKNOWN                       
350.7722  27.3298    2.6  40.9  -83.7   4.7269   4.5 ------	UNKNOWN                       
322.6712  53.2962    3.3  48.6 -130.5   3.4845   3.4 ------	UNKNOWN

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

Time interval of the image:
0.000000 0.024000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
288.7984  10.7550    5.2  26.2  147.1  -0.0152  -2.2   11.4	GRS 1915+105                  
299.5370  35.1244    3.8  33.0 -159.8   0.0161   3.0    5.3	Cyg X-1                       
308.2158  40.8951   10.1  36.2 -145.1  -0.0048  -1.1    5.9	Cyg X-3                       
326.0476  38.4103    4.6  34.9 -121.1  -0.0093  -2.5    7.9	Cyg X-2                       
280.3266  -4.9411    0.7  35.7  117.2   0.3295  16.6 ------	UNKNOWN                       
344.5984  35.6919    2.4  41.2  -98.8   0.0458   4.7 ------	UNKNOWN

Post-slew image of 15-350 keV band

Time interval of the image:
69.888590 731.588600
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
244.9730 -15.6423    0.6  36.3  137.6  18.9399  20.0    0.4	Sco X-1                       
254.3513  35.4720    0.0  47.2 -141.6  -0.9436  -0.8    9.3	Her X-1                       
256.1209 -37.8760    7.5  39.7   97.9   3.2008   1.5    6.6	4U 1700-377                   
256.4409 -36.4257   35.9  38.4   99.1   0.6114   0.3    0.3	GX 349+2                      
263.0112 -24.7131    1.1  25.9  105.8   7.3903  10.2    1.9	GX 1+4                        
268.2937  -1.4763    4.7  12.5  173.0   1.2327   2.5    4.7	SW J1753.5-0127               
270.3147 -25.0769    1.7  22.3   92.0   4.1935   6.8    1.7	GX 5-1                        
270.1050 -25.8247    4.9  23.1   91.5   1.5411   2.4   11.7	GRS 1758-258                  
274.1348 -14.0805   12.8  11.0  100.7   0.4413   0.9    8.0	GX 17+2                       
275.9332 -30.3647    3.1  25.8   76.2   3.0332   3.7    0.4	H1820-303                     
285.2491 -24.8332    0.0  20.5   54.6   1.0406   1.7   12.7	HT1900.1-2455                 
288.7886  10.9575    0.8  18.0  -84.7   7.9588  15.0    0.9	GRS 1915+105                  
313.8379 -22.8434    2.9  37.0    9.7   2.8481   4.0 ------	UNKNOWN                       
248.5178  10.3698    2.8  35.2 -176.7   2.5093   4.1 ------	UNKNOWN                       
313.9842 -14.1894    3.0  34.4   -4.5   2.3487   3.8 ------	UNKNOWN                       
309.2465 -12.3436    3.3  29.5   -6.1   1.8356   3.5 ------	UNKNOWN                       
324.8962 -16.4008    2.2  45.2   -4.2   4.8530   5.2 ------	UNKNOWN                       
329.7898  -1.1850    2.8  49.5  -25.2   4.1536   4.2 ------	UNKNOWN                       
245.0099  39.7563    5.0  55.2 -145.3  10.7919   2.4 ------	UNKNOWN                       
262.7636  40.8758    3.5  48.5 -130.3   9.5346   3.3 ------	UNKNOWN                       
256.7945  41.1873    2.8  50.9 -135.3  14.2329   4.1 ------	UNKNOWN

Plot creation:
Tue Jul  5 10:42:22 EDT 2011