batgrbproduct analysis for trigger=448229

batgrbproduct Analysis for Trigger=448229

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): Mon Jan 13 23:53:46 EST 2014
             Host Name: batevent1
   Current Working Dir: /local/data/batevent/batevent_reproc/trigger448229
======================================================================

  Trigger: 00448229      Segment: 000

  BAT Trigger Time: 320999887.936   [s; MET]
      Trigger Stop: 320999892.032   [s; MET]
               UTC: 2011-03-05T06:38:01.212340    [includes UTCF correction] 
       Where From?: TDRSS position message

  BAT 
    RA: 260.877330338745   Dec: -15.7900383779732  [deg; J2000]

     Catalogged Source?: NO
     Point Source?:      YES
     GRB Indicated?:     YES    [ by BAT flight software ]
     Image S/N Ratio:    7.2
     Image Trigger?:     NO
     Rate S/N Ratio:     13.9283882771841  [ if not an image trigger ]
     Image S/N Ratio:    7.2

  Flight Position:   [ source = BAT ]
    RA: 260.877330338745   Dec: -15.7900383779732  [deg; J2000]

  Ground Position:   [ source = BAT pre-slew burst ]
    RA: 260.875140191826   Dec: -15.799752811987  [deg; J2000]  
        { 17h 23m 30.0s , -15d 47' 59.1" }
         +/- 1.84881494100128 [arcmin] (estimated 90% radius based on SNR)
         +/- 0.943587676916032 [arcmin] (formal 1-sigma fit error)
    SNR: 12.642764083763
 
  Angular difference between Flight and Ground position is 0.596424 arcmin
 
  Partial Coding Fraction: 0.2226562    [ including projection effects ]

  Duration
     T90: 12 +/- 2.23606797749979
        Measured from: -0.935999989509583
                   to: 11.0640000104904     [s; relative to TRIGTIME]
     T50: 6 +/- 1
        Measured from: 1.06400001049042
                   to: 7.06400001049042     [s; relative to TRIGTIME]



  Fluence
     Peak Flux  (peak 1 second)
        Measured from: 6.06400001049042     
                   to: 7.06400001049042     [s; relative to TRIGTIME]
     Total Fluence        
        Measured from: -0.935999989509583     
                   to: 12.0640000104904     [s; relative to TRIGTIME]
     
             Band 1     Band 2     Band 3     Band 4
              15-25      25-50     50-100    100-350     keV
 Total     0.365885   0.445813   0.384308   0.013428
           0.046604   0.046825   0.041321   0.037057 [error]
 Peak      0.052180   0.047498   0.050391   0.004253
           0.012654   0.013238   0.011904   0.010519 [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 1.18e-07 2.06e-07 2.73e-07 7.43e-07 7.97e-07 1.34e-06   erg/cm2
              Error 2.16e-08 2.32e-08 4.10e-08 2.37e-07 9.82e-08 2.70e-07   erg/cm2
Peak flux Power-law 4.69e-01 4.19e-01 2.57e-01 2.40e-01 1.25e+00 1.39e+00   ph/cm2/s
              Error 1.89e-01 1.12e-01 9.51e-02 1.75e-01 3.30e-01 3.69e-01   ph/cm2/s
 
Fluence   Cutoff-PL 1.13e-07 2.12e-07 2.78e-07 4.79e-07 7.81e-07 1.08e-06   erg/cm2
              Error 2.49e-08 2.77e-08 4.39e-08 3.96e-07 1.06e-07 4.12e-07   erg/cm2
Peak flux Cutoff-PL 4.25e-01 4.50e-01 2.70e-01 1.19e-01 1.22e+00 1.26e+00   ph/cm2/s
              Error 2.20e-01 1.36e-01 1.10e-01 2.13e-01 3.36e-01 4.07e-01   ph/cm2/s
 
Fluence        Band 1.10e-07 2.13e-07 2.79e-07 4.40e-07 7.79e-07 1.05e-06   erg/cm2
              Error -------- -------- -------- -------- -------- --------   erg/cm2
Peak flux      Band 4.25e-01 4.50e-01 2.70e-01 1.20e-01 1.22e+00 1.27e+00   ph/cm2/s
              Error 2.20e-01 -------- -------- -------- -------- --------   ph/cm2/s

 
=== Time-averaged spectral analysis ===
 
Model Ph_index Ph_90err Epeak  Epeak_90err Norm     Nomr_90err chi2   dof
PL    1.589    0.194    -      -           6.55e-03 7.46e-04   64.760 57
CPL   1.301    0.569     120.3    0.0      9.19e-03 7.95e-03   64.220 56
 
 
=== 1-s peak spectral analysis ===
 
Model Ph_index Ph_90err Epeak  Epeak_90err Norm     Nomr_90err chi2   dof
PL    1.704    0.463    -      -           9.38e-03 2.73e-03   56.560 57
CPL   1.040    1.856      69.5    0.0      2.10e-02 0.00e+00   56.080 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: 7.872000 sec.
T50 in the 50-300 keV band: 4.416000 sec.

 
=== Table of the duration information ==
 
        Value   tstart    tstop
T100   13.000   -0.936   12.064
T90    12.000   -0.936   11.064
T50     6.000    1.064    7.064
Peak    1.000    6.064    7.064

Click here for the BAT GCN circular template

Special notes of this burst

Image

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

#   RAcent    DECcent   POSerr    Theta     Phi              Peak Cts       SNR   Name
  260.8751   -15.7998   0.0153    35.6026    62.8952         1.2229148     12.643 TRIG_00448229                 
 
Foreground time interval of the image:
 -0.936  12.064 (delta_t =  13.000 [sec])
Background time interval of the image:
-151.835  -0.936 (delta_t = 150.899 [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 4.096000

8 ms binning

From T100_start-3 s to T100_start+3 s

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 4.096000

2 ms binning

From T100_start-1 s to T100_start+1 s

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 4.096000

SN=5 or 10 sec. binning (whichever binning is satisfied first)

SN=5 or 10 sec. binning (T < 200 sec)

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

The mask-weighted light curves based on cleaned DPHs

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   -0.936 sec. to   12.064 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.58938     ( -0.192205   0.195119 )
Norm@50keV  : 6.55026E-03    ( -0.000748981   0.000742182 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          64.76 using 59 PHA bins.
# Reduced chi-squared =          1.136 for     57 degrees of freedom 
# Null hypothesis probability =   2.242971e-01
 
Photon flux (15-150 keV)    in 13 sec: 0.838991 ( -0.0933977  0.0935639 ) ph/cm2/s
Energy fluence (15-150 keV)             : 7.97415e-07 ( -9.76151e-08  9.87034e-08 ) ergs/cm2

Cutoff power-law model

Time interval is from   -0.936 sec. to   12.064 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.30141     ( -0.761347   0.376133 )
Epeak [keV] : 120.284      ( -120.288 -120.288 )
Norm@50keV  : 9.18919E-03    ( -0.00329784   0.0126015 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          64.22 using 59 PHA bins.
# Reduced chi-squared =          1.147 for     56 degrees of freedom 
# Null hypothesis probability =   2.106426e-01
 
Photon flux (15-150 keV)    in 13 sec: 0.828012 ( -0.096869  0.096773 ) ph/cm2/s
Energy fluence (15-150 keV)             : 7.80894e-07 ( -1.05294e-07  1.05907e-07 ) ergs/cm2

Band function

Time interval is from   -0.936 sec. to   12.064 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -1.26518   ( -0.398198   0.72331 )
beta        : -9.37167    ( 9.37167   19.3717 )
Epeak [keV] : 114.352      ( -50.5288 -114.315 )
Norm@50keV   : 9.55197E-03    ( -0.00363702   0.00599919 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          64.23 using 59 PHA bins.
# Reduced chi-squared =          1.168 for     55 degrees of freedom 
# Null hypothesis probability =   1.845812e-01
 
Photon flux (15-150 keV)    in 13 sec: 0.826837 (    ) ph/cm2/s
Energy fluence (15-150 keV)             : 7.78791e-07 ( 0  0 ) ergs/cm2

Single BB

 
Spectral model blackbody:
------------------------------------------------------------
Parameters  : value    Lower 90%  Upper 90%
kT [keV]    : 15.0255  (-2.18718  2.52561)
R^2/D10^2   : 9.12663E-02  (-0.0384113   0.0682818)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          87.35 using 59 PHA bins.
# Reduced chi-squared =          1.532 for     57 degrees of freedom 
# Null hypothesis probability =   5.985613e-03
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  5.607e-08   1.188e-08
25- 50  2.231e-07   3.549e-08
50-150  3.431e-07   8.125e-08
15-150  6.222e-07   9.262e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 183.433       (-75.8917      -183.378)
Norm        : 3.41946       (-0.386205     0.456301)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          64.26 using 59 PHA bins.
# Reduced chi-squared =          1.127 for     57 degrees of freedom 
# Null hypothesis probability =   2.373522e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.119e-07   6.221e-08
25- 50  2.130e-07   1.132e-07
50-150  4.541e-07   2.452e-07
15-150  7.789e-07   4.146e-07

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 5.74372        (-1.43226      1.80006)
R1^2/D10^2  : 1.87017        (-1.19309      4.05659)
kT2 [keV]   : 23.4788        (-4.72302      7.88929)
R2^2/D10^2  : 1.57324E-02    (-0.0100502   0.0118039)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          61.08 using 59 PHA bins.
# Reduced chi-squared =          1.111 for     55 degrees of freedom 
# Null hypothesis probability =   2.667113e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.200e-07   6.137e-08
25- 50  2.014e-07   7.502e-08
50-150  4.635e-07   2.502e-07
15-150  7.850e-07   3.177e-07

Peak spectrum fit

Power-law model

Time interval is from    6.064 sec. to    7.064 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.70375     ( -0.442972   0.48233 )
Norm@50keV  : 9.37719E-03    ( -0.00277693   0.00267588 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          56.56 using 59 PHA bins.
# Reduced chi-squared =         0.9923 for     57 degrees of freedom 
# Null hypothesis probability =   4.915585e-01
 
Photon flux (15-150 keV)    in 1 sec: 1.24705 ( -0.329583  0.33 ) ph/cm2/s
Energy fluence (15-150 keV)             : 8.67959e-08 ( -2.59838e-08  2.68191e-08 ) ergs/cm2

Cutoff power-law model

Time interval is from    6.064 sec. to    7.064 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.04019     ( -2.17062   1.54181 )
Epeak [keV] : 69.4655      (   )
Norm@50keV  : 2.09641E-02    (     )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          56.08 using 59 PHA bins.
# Reduced chi-squared =          1.001 for     56 degrees of freedom 
# Null hypothesis probability =   4.718627e-01
 
Photon flux (15-150 keV)    in 1 sec: 1.22110 ( -0.335789  0.33582 ) ph/cm2/s
Energy fluence (15-150 keV)             : 8.33993e-08 ( -2.64241e-08  2.80377e-08 ) ergs/cm2

Band function

Time interval is from    6.064 sec. to    7.064 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -1.11987   ( -1.31922   2.35155 )
beta        : -10.0000    ( 10   20 )
Epeak [keV] : 71.7509      ( -37.4538 -71.8195 )
Norm@50keV   : 1.92458E-02    ( -0.0191607   0.22882 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          56.09 using 59 PHA bins.
# Reduced chi-squared =          1.020 for     55 degrees of freedom 
# Null hypothesis probability =   4.339105e-01
 
Photon flux (15-150 keV)    in 1 sec: 1.22162 (    ) ph/cm2/s
Energy fluence (15-150 keV)             : 8.32869e-08 ( 0  0 ) ergs/cm2

Single BB

 
Spectral model blackbody:
------------------------------------------------------------
Parameters  : value    Lower 90%  Upper 90%
kT [keV]    : 14.4741  (-4.38034  5.25814)
R^2/D10^2   : 0.158923  (-0.106733   0.403312)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          59.42 using 59 PHA bins.
# Reduced chi-squared =          1.043 for     57 degrees of freedom 
# Null hypothesis probability =   3.874050e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  7.007e-09   4.324e-09
25- 50  2.692e-08   1.469e-08
50-150  3.776e-08   2.306e-08
15-150  7.169e-08   4.038e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 133.434       (-79.9511      -130.645)
Norm        : 5.21287       (-1.49416     2.3023)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          56.15 using 59 PHA bins.
# Reduced chi-squared =         0.9852 for     57 degrees of freedom 
# Null hypothesis probability =   5.067831e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.350e-08   7.960e-09
25- 50  2.459e-08   1.416e-08
50-150  4.614e-08   3.043e-08
15-150  8.423e-08   5.230e-08

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 4.72522        (-2.14714      4.23356)
R1^2/D10^2  : 5.96408        (-5.51995      94.0525)
kT2 [keV]   : 19.3398        (-6.09424      14.6045)
R2^2/D10^2  : 4.68129E-02    (-0.0411431   0.0876525)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          54.63 using 59 PHA bins.
# Reduced chi-squared =         0.9933 for     55 degrees of freedom 
# Null hypothesis probability =   4.887596e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.492e-08   8.870e-09
25- 50  2.317e-08   1.250e-08
50-150  4.612e-08   2.914e-08
15-150  8.422e-08   4.573e-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: 1.58938     ( -0.192205   0.195119 )
Norm@50keV  : 6.55026E-03    ( -0.000748981   0.000742182 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          64.76 using 59 PHA bins.
# Reduced chi-squared =          1.136 for     57 degrees of freedom 
# Null hypothesis probability =   2.242971e-01
 
Photon flux (15-150 keV)    in 13 sec: 0.838991 ( -0.0933977  0.0935639 ) ph/cm2/s
Energy fluence (15-150 keV)             : 7.97415e-07 ( -9.76151e-08  9.87034e-08 ) ergs/cm2

Cutoff power-law model

Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.30141     ( -0.761347   0.376133 )
Epeak [keV] : 120.284      ( -120.288 -120.288 )
Norm@50keV  : 9.18919E-03    ( -0.00329784   0.0126015 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          64.22 using 59 PHA bins.
# Reduced chi-squared =          1.147 for     56 degrees of freedom 
# Null hypothesis probability =   2.106426e-01
 
Photon flux (15-150 keV)    in 13 sec: 0.828012 ( -0.096869  0.096773 ) ph/cm2/s
Energy fluence (15-150 keV)             : 7.80894e-07 ( -1.05294e-07  1.05907e-07 ) ergs/cm2

Band function

 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -1.26518   ( -0.39819   0.723324 )
beta        : -9.37167    ( 9.37167   19.3717 )
Epeak [keV] : 114.352      ( -50.5288 -114.315 )
Norm@50keV   : 9.55197E-03    ( -0.00363702   0.00632839 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          64.23 using 59 PHA bins.
# Reduced chi-squared =          1.168 for     55 degrees of freedom 
# Null hypothesis probability =   1.845812e-01
 
Photon flux (15-150 keV)    in 13 sec: 0.826837 (    ) ph/cm2/s
Energy fluence (15-150 keV)             : 7.78791e-07 ( 0  0 ) ergs/cm2

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

S(25-50 keV)  = 2.06e-07
S(50-100 keV) = 2.73e-07

T90 vs. Hardness ratio plot

T90                                   = 12 sec.
Hardness ratio (energy fluence ratio) = 1.32524

Color vs. Color plot

Count Ratio  (25-50 keV) / (15-25 keV) = 1.21845
Count Ratio (50-100 keV) / (15-25 keV) = 1.05035

Mask shadow pattern

IMX = 3.262225522227327E-01, IMY = -6.373634552866851E-01

TIME vs. PHA plot around the trigger time

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 4.096000

TIME vs. DetID plot around the trigger time

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 4.096000

100 us light curve (15-350 keV)

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 4.096000

Spacecraft aspect plot

Bright source in the pre-burst/pre-slew/post-slew images

Pre-burst image of 15-350 keV band

Time interval of the image:
-151.835400 -0.936000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
255.9731 -37.7834    4.7  47.4   33.7   1.3892   2.5    3.7	4U 1700-377                   
256.4128 -36.5258    6.2  46.5   35.0   0.9540   1.9    6.3	GX 349+2                      
263.1519 -24.7934   12.1  36.1   47.1   0.2759   1.0    8.3	GX 1+4                        
264.7008 -44.5478    5.5  46.2   20.9  -0.7886  -2.1    6.1	4U 1735-44                    
268.3858  -1.5916    3.7  28.4   90.2   0.7956   3.1    8.4	SW J1753.5-0127               
270.3030 -25.1158    2.3  30.4   41.2   1.1275   5.2    2.4	GX 5-1                        
270.1961 -25.5514    0.0  30.8   40.6   0.1424   0.6   12.9	GRS 1758-258                  
273.8386 -14.0877    8.2  23.0   61.0   0.2751   1.4   10.2	GX 17+2                       
276.0702 -30.4203    7.1  29.8   26.6   0.3429   1.6    8.2	H1820-303                     
285.0277 -24.9104   19.3  20.5   20.0   0.0935   0.6    0.8	HT1900.1-2455                 
288.7853  10.9427    1.0  19.8  147.6   2.0472  11.6    0.8	GRS 1915+105                  
299.4471  35.1884    4.1  42.7  173.6   0.7849   2.8    7.1	Cyg X-1                       
308.0752  40.9580  127.1  49.6 -178.5  -0.0341  -0.1    1.6	Cyg X-3                       
326.3125  38.4074   11.6  53.7 -161.1  -0.5093  -1.0    8.4	Cyg X-2                       
263.1460 -33.8376    6.3  40.4   34.2   0.5760   1.8    7.8	GX 354-0                      
329.9779  26.8726    2.9  47.4 -147.9   1.4478   4.0 ------	UNKNOWN                       
338.2525   3.8806    2.9  43.4 -114.0   3.3492   4.0 ------	UNKNOWN

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

Time interval of the image:
-0.936000 12.064000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
255.8484 -37.7947    5.2  47.5   33.8   0.3449   2.2    7.2	4U 1700-377                   
256.4641 -36.4534    6.9  46.4   35.0   0.2359   1.7    2.3	GX 349+2                      
263.1129 -24.6411   19.8  36.1   47.4   0.0465   0.6    8.4	GX 1+4                        
264.7083 -44.2657    7.6  46.0   21.2   0.1531   1.5   11.2	4U 1735-44                    
268.2431  -1.3229    6.9  28.6   90.7  -0.1132  -1.7   10.8	SW J1753.5-0127               
270.3202 -25.1807    5.4  30.5   41.1  -0.1272  -2.1    6.4	GX 5-1                        
270.1217 -25.8296    0.0  31.0   40.2   0.0494   0.8   11.1	GRS 1758-258                  
273.9234 -14.1482   10.7  22.9   60.8  -0.0553  -1.1    8.2	GX 17+2                       
275.7821 -30.3052   18.3  29.9   27.1  -0.0338  -0.6    8.3	H1820-303                     
285.0731 -25.0831   11.9  20.6   19.6   0.0375   1.0   10.0	HT1900.1-2455                 
288.9598  11.0032    7.3  19.8  148.1   0.0686   1.6   10.1	GRS 1915+105                  
299.5035  35.2388    4.8  42.8  173.7  -0.1652  -2.4    4.8	Cyg X-1                       
308.0399  40.8451    5.5  49.5 -178.5  -0.1919  -2.1    7.2	Cyg X-3                       
326.0749  38.3616    5.7  53.5 -161.2   0.2317   2.0    5.1	Cyg X-2                       
262.8868 -33.6626    6.9  40.5   34.6   0.1535   1.7   11.5	GX 354-0                      
260.8751 -15.7997    0.9  35.6   62.9   1.2228  12.6 ------	UNKNOWN

Post-slew image of 15-350 keV band

Time interval of the image:
93.164590 962.121800
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
244.9764 -15.6409    0.2  15.3   84.1  43.9858  74.5    0.2	Sco X-1                       
254.5739  35.3274   92.5  51.5  169.1   0.2781   0.1    5.8	Her X-1                       
256.0032 -37.8416    0.8  22.5    5.8   8.8918  13.9    0.8	4U 1700-377                   
256.4409 -36.4112    2.4  21.0    5.7   3.1051   4.9    0.8	GX 349+2                      
263.0459 -24.7103    1.8   9.1  -16.7   3.8616   6.4    2.9	GX 1+4                        
264.7412 -44.3005    4.9  28.7  -10.1   1.6642   2.4    9.0	4U 1735-44                    
268.2169  -1.5914    0.0  15.9 -156.7   0.7825   1.2   12.3	SW J1753.5-0127               
270.2649 -25.0666    1.6  12.8  -46.2   4.7807   7.4    1.3	GX 5-1                        
270.1938 -25.7676    4.1  13.2  -43.9   1.8197   2.8    6.1	GRS 1758-258                  
273.9519 -14.0155    3.6  12.7 -100.7   2.1030   3.2    3.4	GX 17+2                       
275.8383 -30.3728    2.4  20.0  -44.9   3.1763   4.9    4.5	H1820-303                     
285.1241 -24.7728    7.4  24.4  -68.8   1.4471   1.5   10.1	HT1900.1-2455                 
288.8067  10.9401    1.5  38.4 -136.7   9.3430   7.9    0.6	GRS 1915+105                  
262.9767 -33.7750    4.8  18.1   -9.9   1.4856   2.4    3.6	GX 354-0                      
222.6842 -22.4776    2.4  36.6   69.1   7.8125   4.7 ------	UNKNOWN                       
246.2664 -67.0554    3.4  52.1    2.8   5.7477   3.4 ------	UNKNOWN                       
283.4214 -64.1239    5.0  50.7  -16.8   3.3309   2.3 ------	UNKNOWN                       
299.2049  11.4660    3.0  46.7 -127.8  10.8033   3.9 ------	UNKNOWN                       
308.4892 -48.0925    4.8  50.5  -44.1   8.3747   2.4 ------	UNKNOWN

Plot creation:
Sat May 30 22:50:05 EDT 2015