batgrbproduct analysis for trigger=355942

batgrbproduct Analysis for Trigger=355942

Analysis Summary

Notes:

1) No attempt has been made to eliminate the non-significant decimal places.
2) This batgrbproduct analysis is done using the HEASARC data.
3) This batgrbproduct analysis is using the flight position for the mask-weighting calculation.

======================================================================
                  BAT GRB EVENT DATA PROCESSING REPORT
    Process Script Ver: batgrbproduct v2.46
    Process Start Time (local time): Sun Jan 19 15:43:58 EST 2014
             Host Name: batevent1
   Current Working Dir: /local/data/batevent/batevent_reproc/trigger355942
======================================================================

  Trigger: 00355942      Segment: 000

  BAT Trigger Time: 267916816.896   [s; MET]
      Trigger Stop: 267916817.92   [s; MET]
               UTC: 2009-06-28T21:20:12.029720    [includes UTCF correction] 
       Where From?: TDRSS position message

  BAT 
    RA: 237.049710631592   Dec: -15.9769445036211  [deg; J2000]

     Catalogged Source?: NO
     Point Source?:      YES
     GRB Indicated?:     YES    [ by BAT flight software ]
     Image S/N Ratio:    10.03
     Image Trigger?:     NO
     Rate S/N Ratio:     15.3622914957372  [ if not an image trigger ]
     Image S/N Ratio:    10.03

  Flight Position:   [ source = BAT ]
    RA: 237.049710631592   Dec: -15.9769445036211  [deg; J2000]

  Ground Position:   [ source = BAT pre-slew burst ]
    RA: 237.036860994085   Dec: -15.9707594216292  [deg; J2000]  
        { 15h 48m 08.8s , -15d 58' 14.7" }
         +/- 1.69410512838328 [arcmin] (estimated 90% radius based on SNR)
         +/- 0.739441961279157 [arcmin] (formal 1-sigma fit error)
    SNR: 14.3238817451087
 
  Angular difference between Flight and Ground position is 0.828921 arcmin
 
  Partial Coding Fraction: 0.6328125    [ including projection effects ]

  Duration
     T90: 24.944000005722 +/- 4.05342179186581
        Measured from: -21.5239999890327
                   to: 3.4200000166893     [s; relative to TRIGTIME]
     T50: 11.1960000097752 +/- 4.42866889265547
        Measured from: -9.72799998521805
                   to: 1.46800002455711     [s; relative to TRIGTIME]



  Fluence
     Peak Flux  (peak 1 second)
        Measured from: 0.0520000159740448     
                   to: 1.05200001597404     [s; relative to TRIGTIME]
     Total Fluence        
        Measured from: -25.0920000076294     
                   to: 3.99200001358986     [s; relative to TRIGTIME]
     
             Band 1     Band 2     Band 3     Band 4
              15-25      25-50     50-100    100-350     keV
 Total     0.272927   0.341130   0.338619   0.113458
           0.040571   0.037911   0.032530   0.028177 [error]
 Peak      0.039763   0.069436   0.052994   0.009039
           0.007970   0.007906   0.007005   0.005711 [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 8.25e-08 1.63e-07 2.51e-07 8.43e-07 7.02e-07 1.34e-06   erg/cm2
              Error 1.70e-08 1.95e-08 3.27e-08 2.54e-07 8.02e-08 2.72e-07   erg/cm2
Peak flux Power-law 4.68e-01 4.86e-01 3.57e-01 4.22e-01 1.47e+00 1.73e+00   ph/cm2/s
              Error 1.06e-01 6.89e-02 5.75e-02 1.39e-01 1.97e-01 2.29e-01   ph/cm2/s
 
Fluence   Cutoff-PL 8.19e-08 1.64e-07 2.49e-07 8.32e-07 6.98e-07 1.27e-06   erg/cm2
              Error 1.71e-08 1.93e-08 3.26e-08 2.85e-07 7.97e-08 3.58e-07   erg/cm2
Peak flux Cutoff-PL 4.12e-01 5.20e-01 3.76e-01 1.94e-01 1.43e+00 1.50e+00   ph/cm2/s
              Error 1.25e-01 8.36e-02 6.56e-02 2.05e-01 2.04e-01 2.97e-01   ph/cm2/s
 
Fluence        Band -------- -------- -------- -------- -------- --------   erg/cm2
              Error -------- -------- -------- -------- -------- --------   erg/cm2
Peak flux      Band 4.11e-01 5.21e-01 3.75e-01 2.22e-01 1.43e+00 1.53e+00   ph/cm2/s
              Error -------- -------- -------- -------- -------- --------   ph/cm2/s

 
=== Time-averaged spectral analysis ===
 
Model Ph_index Ph_90err Epeak  Epeak_90err Norm     Nomr_90err chi2   dof
PL    1.379    0.197    -      -           2.49e-03 2.60e-04   44.950 57
CPL   1.376    0.199    9999.3    0.0      2.50e-03 2.01e-03   44.970 56
 
 
=== 1-s peak spectral analysis ===
 
Model Ph_index Ph_90err Epeak  Epeak_90err Norm     Nomr_90err chi2   dof
PL    1.446    0.221    -      -           1.20e-02 1.58e-03   49.160 57
CPL   0.716    0.962      86.9  -29.9      2.82e-02 4.49e-02   47.170 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: 25.728000 sec.
T50 in the 50-300 keV band: 11.968000 sec.

 
=== Table of the duration information ==
 
        Value   tstart    tstop
T100   29.084  -25.092    3.992
T90    24.944  -21.524    3.420
T50    11.196   -9.728    1.468
Peak    1.000    0.052    1.052

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
  237.0369   -15.9708   0.0134    31.2844   -40.4363         1.0985708     14.324 TRIG_00355942                 
 
Foreground time interval of the image:
-25.092   3.992 (delta_t =  29.084 [sec])
Background time interval of the image:
-239.896 -25.092 (delta_t = 214.804 [sec])

Lightcurves

Notes:

1) The mask-weighted light curves are using the flight position.
2) Multiple plots of different time binning/intervals are shown to cover all scenarios of short/long GRBs, rate/image triggers, and real/false positives.
3) For all the mask-weighted lightcurves, the y-axis units are counts/sec/det where a det is 0.4 x 0.4 = 0.16 sq cm.
4) The verticle lines correspond to following: green dotted lines are T50 interval, black dotted lines are T90 interval, blue solid line(s) is a spacecraft slew start time, and orange solid line(s) is a spacecraft slew end time.
5) Time of each bin is in the middle of the bin.

1 s binning

From T0-310 s to T0+310 s

From T100_start - 20 s to T100_end + 30 s

Full time interval

64 ms binning

Full time interval

From T100_start to T100_end

From T0-5 sec to T0+5 sec

16 ms binning

From T100_start-5 s to T100_start+5 s

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

Quad-rate summed light curves (from T0-300s to T0+1000s)

Spectral Evolution

Spectra

Notes:

1) The fitting includes the systematic errors.
2) When the burst includes telescope slew time periods, the fitting uses an average response file made from multiple 5-s response files through out the slew time plus single time preiod for the non-slew times, and weighted by the total counts in the corresponding time period using addrmf. An average response file is needed becuase a spectral fit using the pre-slew DRM will introduce some errors in both a spectral shape and a normalization if the PHA file contains a lot of the slew/post-slew time interval.
3) For fits to more complicated models (e.g. a power-law over a cutoff power-law), the BAT team has decided to require a chi-square improvement of more than 6 for each extra dof.

Time averaged spectrum fit using the average DRM

Power-law model

Time interval is from  -25.092 sec. to    3.992 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.37950     ( -0.198477   0.19625 )
Norm@50keV  : 2.48626E-03    ( -0.0002598   0.000259618 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          44.95 using 59 PHA bins.
# Reduced chi-squared =         0.7886 for     57 degrees of freedom 
# Null hypothesis probability =   8.761089e-01
 
Photon flux (15-150 keV)    in 29.08 sec: 0.301401 ( -0.0333446  0.0334797 ) ph/cm2/s
Energy fluence (15-150 keV)             : 7.01604e-07 ( -7.9947e-08  8.05077e-08 ) ergs/cm2

Cutoff power-law model

Time interval is from  -25.092 sec. to    3.992 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.37587     ( -0.199845   0.197827 )
Epeak [keV] : 9999.29      ( -9999.36 -9999.36 )
Norm@50keV  : 2.49537E-03    ( -0.00249535   0.00151991 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          44.97 using 59 PHA bins.
# Reduced chi-squared =         0.8029 for     56 degrees of freedom 
# Null hypothesis probability =   8.545572e-01
 
Photon flux (15-150 keV)    in 29.08 sec: 0.302093 ( -0.034061  0.032738 ) ph/cm2/s
Energy fluence (15-150 keV)             : 6.98129e-07 ( -7.68003e-08  8.26715e-08 ) ergs/cm2

Band function

Time interval is from  -25.092 sec. to    3.992 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : 4.91021   ( -4.91021   -4.91021 )
beta        : -1.41265    ( -0.216063   0.209745 )
Epeak [keV] : 22.4941      ( -22.4941 6.77159 )
Norm@50keV   : 382.149    ( -39.8283   1.06832e+06 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          44.56 using 59 PHA bins.
# Reduced chi-squared =         0.8102 for     55 degrees of freedom 
# Null hypothesis probability =   8.417945e-01
 
Photon flux (15-150 keV)    in 29.08 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]    : 18.6660  (-2.81585  3.42426)
R^2/D10^2   : 1.58579E-02  (-0.00680306   0.011812)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          76.16 using 59 PHA bins.
# Reduced chi-squared =          1.336 for     57 degrees of freedom 
# Null hypothesis probability =   4.588787e-02
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  3.178e-08   7.299e-09
25- 50  1.509e-07   2.822e-08
50-150  3.851e-07   7.808e-08
15-150  5.678e-07   8.506e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 200.000       (      )
Norm        : 1.25084       (-0.13162     0.131594)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          49.05 using 59 PHA bins.
# Reduced chi-squared =         0.8605 for     57 degrees of freedom 
# Null hypothesis probability =   7.639283e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  9.058e-08   2.162e-08
25- 50  1.743e-07   8.763e-08
50-150  3.822e-07   2.089e-07
15-150  6.470e-07   3.263e-07

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 6.07050        (-1.36562      1.84397)
R1^2/D10^2  : 0.559131        (-0.353669      1.01155)
kT2 [keV]   : 30.7953        (-6.85771      13.4985)
R2^2/D10^2  : 2.67099E-03    (-0.0017601   0.00340852)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          42.04 using 59 PHA bins.
# Reduced chi-squared =         0.7644 for     55 degrees of freedom 
# Null hypothesis probability =   9.004069e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  9.229e-08   4.724e-08
25- 50  1.535e-07   5.563e-08
50-150  4.764e-07   2.288e-07
15-150  7.222e-07   2.759e-07

Peak spectrum fit

Power-law model

Time interval is from    0.052 sec. to    1.052 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.44642     ( -0.221175   0.221478 )
Norm@50keV  : 1.19734E-02    ( -0.00158239   0.00157672 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          49.16 using 59 PHA bins.
# Reduced chi-squared =         0.8625 for     57 degrees of freedom 
# Null hypothesis probability =   7.604187e-01
 
Photon flux (15-150 keV)    in 1 sec: 1.47425 ( -0.196336  0.196836 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.14653e-07 ( -1.64849e-08  1.6688e-08 ) ergs/cm2

Cutoff power-law model

Time interval is from    0.052 sec. to    1.052 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 0.716491     ( -1.10591   0.818785 )
Epeak [keV] : 86.8606      ( -27.0991 -86.8607 )
Norm@50keV  : 2.81887E-02    ( -0.0169891   0.0728312 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          47.17 using 59 PHA bins.
# Reduced chi-squared =         0.8423 for     56 degrees of freedom 
# Null hypothesis probability =   7.935652e-01
 
Photon flux (15-150 keV)    in 1 sec: 1.42882 ( -0.20431  0.20436 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.08251e-07 ( -1.83653e-08  1.8519e-08 ) ergs/cm2

Band function

Time interval is from    0.052 sec. to    1.052 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : 4.51245   ( -6.11636   -4.51245 )
beta        : -1.64649    ( -0.317919   0.283889 )
Epeak [keV] : 30.1794      ( -8.95351 7.6381 )
Norm@50keV   : 188.043    ( -24.2059   4.37067e+06 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          46.51 using 59 PHA bins.
# Reduced chi-squared =         0.8456 for     55 degrees of freedom 
# Null hypothesis probability =   7.855061e-01
 
Photon flux (15-150 keV)    in 1 sec: 1.42768 (    ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.10565e-07 ( -1.10558e-07  -1.71984e-08 ) ergs/cm2

Single BB

 
Spectral model blackbody:
------------------------------------------------------------
Parameters  : value    Lower 90%  Upper 90%
kT [keV]    : 14.9560  (-2.25138  2.77659)
R^2/D10^2   : 0.172315  (-0.0777626   0.134624)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          55.70 using 59 PHA bins.
# Reduced chi-squared =         0.9772 for     57 degrees of freedom 
# Null hypothesis probability =   5.238541e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  8.073e-09   1.926e-09
25- 50  3.199e-08   6.460e-09
50-150  4.864e-08   1.300e-08
15-150  8.870e-08   1.756e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 199.362       (-74.3223      -199.363)
Norm        : 6.09264       (-0.788327     0.789817)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          48.45 using 59 PHA bins.
# Reduced chi-squared =         0.8499 for     57 degrees of freedom 
# Null hypothesis probability =   7.828469e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.517e-08   8.500e-09
25- 50  2.918e-08   1.617e-08
50-150  6.401e-08   3.581e-08
15-150  1.084e-07   6.015e-08

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 8.38487        (-3.33789      3.96029)
R1^2/D10^2  : 0.809654        (-0.517001      3.1181)
kT2 [keV]   : 27.7469        (-22.7004      95.6577)
R2^2/D10^2  : 1.44191E-02    (-0.0138636   0.062876)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          46.25 using 59 PHA bins.
# Reduced chi-squared =         0.8409 for     55 degrees of freedom 
# Null hypothesis probability =   7.935222e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.245e-08   7.100e-09
25- 50  3.102e-08   1.631e-08
50-150  6.677e-08   3.748e-08
15-150  1.102e-07   5.700e-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: 1.37950     ( -0.198477   0.19625 )
Norm@50keV  : 2.48626E-03    ( -0.0002598   0.000259618 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          44.95 using 59 PHA bins.
# Reduced chi-squared =         0.7886 for     57 degrees of freedom 
# Null hypothesis probability =   8.761089e-01
 
Photon flux (15-150 keV)    in 29.08 sec: 0.301401 ( -0.0333446  0.0334797 ) ph/cm2/s
Energy fluence (15-150 keV)             : 7.01604e-07 ( -7.9947e-08  8.05077e-08 ) ergs/cm2

Cutoff power-law model

Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.37587     ( -0.199845   0.197827 )
Epeak [keV] : 9999.29      ( -9999.36 -9999.36 )
Norm@50keV  : 2.49537E-03    ( -0.00249535   0.00151991 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          44.97 using 59 PHA bins.
# Reduced chi-squared =         0.8029 for     56 degrees of freedom 
# Null hypothesis probability =   8.545572e-01
 
Photon flux (15-150 keV)    in 29.08 sec: 0.302093 ( -0.03406  0.032738 ) ph/cm2/s
Energy fluence (15-150 keV)             : 6.98129e-07 ( -7.68003e-08  8.26715e-08 ) ergs/cm2

Band function

 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : 4.91021   ( -4.91021   -4.91021 )
beta        : -1.41265    ( -0.216063   0.209745 )
Epeak [keV] : 22.4941      ( -22.4941 6.77159 )
Norm@50keV   : 382.149    ( -39.8283   1.06832e+06 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          44.56 using 59 PHA bins.
# Reduced chi-squared =         0.8102 for     55 degrees of freedom 
# Null hypothesis probability =   8.417945e-01
 
Photon flux (15-150 keV)    in 29.08 sec:  (    ) ph/cm2/s
Energy fluence (15-150 keV)             : 0 ( 0  0 ) ergs/cm2

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

S(25-50 keV)  = 1.63e-07
S(50-100 keV) = 2.51e-07

T90 vs. Hardness ratio plot

T90                                   = 24.944000005722 sec.
Hardness ratio (energy fluence ratio) = 1.53988

Color vs. Color plot

Count Ratio  (25-50 keV) / (15-25 keV) = 1.24989
Count Ratio (50-100 keV) / (15-25 keV) = 1.24069

Mask shadow pattern

IMX = 4.624901037000976E-01, IMY = 3.941150020758289E-01

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:
-239.896000 -25.092000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
244.9828 -15.6480    0.3  25.6  -29.5   6.2874  34.2    0.5	Sco X-1                       
255.9961 -37.8480    3.7  10.3 -100.8   0.5867   3.1    0.5	4U 1700-377                   
256.4227 -36.4094    4.2   9.4  -94.2   0.5291   2.7    1.0	GX 349+2                      
263.1038 -24.7919    3.6   8.0    2.3   0.5755   3.3    5.9	GX 1+4                        
264.7357 -44.2895    4.7  12.2 -148.5   0.4140   2.4    9.6	4U 1735-44                    
268.3092  -1.4786    3.1  30.8   28.8   0.9363   3.7    3.9	SW J1753.5-0127               
270.2738 -25.0657    2.0   7.8   50.9   1.0220   5.8    1.0	GX 5-1                        
270.2148 -25.7557    2.6   7.2   52.7   0.8128   4.5    4.8	GRS 1758-258                  
274.1050 -13.9109    6.0  19.5   47.8   0.3563   1.9    9.5	GX 17+2                       
275.9228 -30.3050    2.5   8.2  104.5   0.7858   4.6    3.7	H1820-303                     
285.0466 -24.7857  125.3  17.8   95.5  -0.0195  -0.1    8.1	HT1900.1-2455                 
263.0095 -33.7945    2.7   3.4  -93.9   0.7831   4.3    2.6	GX 354-0                      
314.7781 -26.7394    2.4  42.0  120.8   3.4014   4.8 ------	UNKNOWN                       
277.5703 -23.8230    2.4  12.8   77.4   0.8729   4.7 ------	UNKNOWN                       
249.6566  19.6266    2.7  54.3    5.7   2.9084   4.3 ------	UNKNOWN                       
255.1453 -41.7102    2.0  13.2 -114.2   1.1641   5.8 ------	UNKNOWN                       
354.5567 -75.6645    2.6  58.4 -171.5   4.7639   4.4 ------	UNKNOWN

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

Time interval of the image:
-25.092000 3.992000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
244.9683 -15.4890    5.2  25.8  -29.3   0.1425   2.2    9.1	Sco X-1                       
255.8690 -38.0323    0.0  10.5 -101.4   0.0575   1.0   12.6	4U 1700-377                   
256.3510 -36.6041    5.0   9.5  -95.1   0.1332   2.3   11.6	GX 349+2                      
262.8451 -24.7758    8.8   8.1    0.7   0.0732   1.3    9.1	GX 1+4                        
264.8061 -44.2675    5.5  12.1 -148.7  -0.1207  -2.1   11.3	4U 1735-44                    
268.2219  -1.4669    5.8  30.8   28.6  -0.1511  -2.0    8.8	SW J1753.5-0127               
270.3302 -25.0987    5.9   7.8   51.3  -0.1077  -1.9    2.8	GX 5-1                        
270.2703 -25.8046    3.5   7.2   53.3  -0.1871  -3.3    4.1	GRS 1758-258                  
273.9427 -14.2229    4.8  19.2   47.6   0.1592   2.4   11.8	GX 17+2                       
275.9957 -30.5034   10.0   8.2  106.0  -0.0628  -1.1    9.0	H1820-303                     
285.0619 -25.0221    6.6  17.7   96.2   0.1131   1.7    6.3	HT1900.1-2455                 
262.7917 -33.7425    3.8   3.5  -91.8  -0.1777  -3.1   11.3	GX 354-0                      
237.0369 -15.9708    0.8  31.3  -40.4   1.0988  14.3 ------	UNKNOWN

Post-slew image of 15-350 keV band

Time interval of the image:
194.604600 882.804600
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
170.3121 -60.6244    4.1  42.8  -25.1   1.8090   2.8    0.1	Cen X-3                       
186.6338 -62.8007    2.2  38.9  -14.4   2.8956   5.4    1.9	GX 301-2                      
264.7477 -44.5013   11.4  39.2   62.9   1.2507   1.0    3.1	4U 1735-44                    
296.1963 -36.8415    3.0  40.4  102.2   6.0122   3.9 ------	UNKNOWN                       
353.6936 -53.3783    3.3  25.2 -178.0   1.4112   3.5 ------	UNKNOWN                       
 27.8627 -38.5963    3.0  46.8 -147.3   3.6466   3.8 ------	UNKNOWN

Plot creation:
Sun May 31 03:41:56 EDT 2015