batgrbproduct analysis for trigger=518792

batgrbproduct Analysis for Trigger=518792

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 05:03:21 EST 2014
             Host Name: batevent1
   Current Working Dir: /local/data/batevent/batevent_reproc/trigger518792
======================================================================

  Trigger: 00518792      Segment: 000

  BAT Trigger Time: 354596787.072   [s; MET]
      Trigger Stop: 354596788.48   [s; MET]
               UTC: 2012-03-28T03:06:19.032840    [includes UTCF correction] 
       Where From?: TDRSS position message

  BAT 
    RA: 241.549796791991   Dec: -39.3402511024914  [deg; J2000]

     Catalogged Source?: NO
     Point Source?:      YES
     GRB Indicated?:     YES    [ by BAT flight software ]
     Image S/N Ratio:    6.57
     Image Trigger?:     NO
     Rate S/N Ratio:     13.1909059582729  [ if not an image trigger ]
     Image S/N Ratio:    6.57

  Flight Position:   [ source = BAT ]
    RA: 241.549796791991   Dec: -39.3402511024914  [deg; J2000]

  Ground Position:   [ source = BAT pre-slew burst ]
    RA: 241.606988592298   Dec: -39.3221541575653  [deg; J2000]  
        { 16h 06m 25.7s , -39d 19' 19.8" }
         +/- 1.7695533704008 [arcmin] (estimated 90% radius based on SNR)
         +/- 0.724701411119114 [arcmin] (formal 1-sigma fit error)
    SNR: 13.4594535820635
 
  Angular difference between Flight and Ground position is 2.867763 arcmin
 
  Partial Coding Fraction: 1.015625    [ including projection effects ]

  Duration
     T90: 29.9279999732971 +/- 6.66506352223562
        Measured from: -15.9000000357628
                   to: 14.0279999375343     [s; relative to TRIGTIME]
     T50: 12.3359999656677 +/- 2.93431559074022
        Measured from: -10.8440000414848
                   to: 1.49199992418289     [s; relative to TRIGTIME]



  Fluence
     Peak Flux  (peak 1 second)
        Measured from: 0.107999980449677     
                   to: 1.10799998044968     [s; relative to TRIGTIME]
     Total Fluence        
        Measured from: -17.2600000500679     
                   to: 20.5479999780655     [s; relative to TRIGTIME]
     
             Band 1     Band 2     Band 3     Band 4
              15-25      25-50     50-100    100-350     keV
 Total     0.302021   0.385292   0.187890   0.065593
           0.038000   0.033065   0.027693   0.023895 [error]
 Peak      0.028965   0.031687   0.031992   0.006983
           0.006374   0.005850   0.004904   0.004075 [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 9.34e-08 1.37e-07 1.50e-07 3.10e-07 4.76e-07 6.91e-07   erg/cm2
              Error 1.51e-08 1.49e-08 2.58e-08 1.07e-07 6.02e-08 1.33e-07   erg/cm2
Peak flux Power-law 2.27e-01 2.42e-01 1.83e-01 2.25e-01 7.38e-01 8.78e-01   ph/cm2/s
              Error 7.53e-02 4.81e-02 4.00e-02 1.06e-01 1.35e-01 1.58e-01   ph/cm2/s
 
Fluence   Cutoff-PL 8.58e-08 1.53e-07 1.41e-07 6.55e-08 4.25e-07 4.45e-07   erg/cm2
              Error 1.70e-08 2.12e-08 3.33e-08 1.32e-07 7.15e-08 1.47e-07   erg/cm2
Peak flux Cutoff-PL 2.22e-01 2.44e-01 1.85e-01 2.01e-01 7.34e-01 8.52e-01   ph/cm2/s
              Error 6.41e-02 5.14e-02 4.41e-02 1.59e-01 1.40e-01 2.00e-01   ph/cm2/s
 
Fluence        Band 8.00e-08 1.60e-07 1.33e-07 1.78e-07 4.39e-07 5.53e-07   erg/cm2
              Error 1.81e-08 2.14e-08 2.99e-08 9.17e-08 6.33e-08 1.34e-07   erg/cm2
Peak flux      Band 2.15e-01 2.45e-01 1.86e-01 1.78e-01 7.29e-01 8.27e-01   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    1.867    0.197    -      -           1.37e-03 1.72e-04   77.140 57
CPL   0.882    1.037      46.6   35.5      5.10e-03 1.24e-02   73.700 56
 
 
=== 1-s peak spectral analysis ===
 
Model Ph_index Ph_90err Epeak  Epeak_90err Norm     Nomr_90err chi2   dof
PL    1.402    0.326    -      -           6.06e-03 1.07e-03   63.130 57
CPL   1.287    1.423     330.4    0.0      6.86e-03 0.00e+00   63.100 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: 18.624000 sec.
T50 in the 50-300 keV band: 13.696000 sec.

 
=== Table of the duration information ==
 
        Value   tstart    tstop
T100   37.808  -17.260   20.548
T90    29.928  -15.900   14.028
T50    12.336  -10.844    1.492
Peak    1.000    0.108    1.108

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
  241.6070   -39.3222   0.0143    10.8068     2.0572         0.9263590     13.459 TRIG_00518792                 
 
Foreground time interval of the image:
-17.260  20.548 (delta_t =  37.808 [sec])
Background time interval of the image:
-239.072 -17.260 (delta_t = 221.812 [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 1.408000

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 1.408000

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 1.408000

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  -17.260 sec. to   20.548 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.86726     ( -0.193913   0.200155 )
Norm@50keV  : 1.36853E-03    ( -0.000173906   0.000171089 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          77.14 using 59 PHA bins.
# Reduced chi-squared =          1.353 for     57 degrees of freedom 
# Null hypothesis probability =   3.902349e-02
 
Photon flux (15-150 keV)    in 37.81 sec: 0.193725 ( -0.0212205  0.0212424 ) ph/cm2/s
Energy fluence (15-150 keV)             : 4.75699e-07 ( -5.95647e-08  6.07622e-08 ) ergs/cm2

Cutoff power-law model

Time interval is from  -17.260 sec. to   20.548 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 0.882136     ( -1.16598   0.90846 )
Epeak [keV] : 46.5847      ( -10.3295 60.6847 )
Norm@50keV  : 5.09807E-03    ( -0.00509991   0.0197133 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          73.70 using 59 PHA bins.
# Reduced chi-squared =          1.316 for     56 degrees of freedom 
# Null hypothesis probability =   5.657957e-02
 
Photon flux (15-150 keV)    in 37.81 sec: 0.185561 ( -0.022359  0.022457 ) ph/cm2/s
Energy fluence (15-150 keV)             : 4.24852e-07 ( -6.81185e-08  7.49394e-08 ) ergs/cm2

Band function

Time interval is from  -17.260 sec. to   20.548 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : 2.43038   ( -2.34218   -1.12305 )
beta        : -2.31902    ( -0.501709   0.371971 )
Epeak [keV] : 31.4253      ( -7.81334 9.04143 )
Norm@50keV   : 1.06284    ( -1.0618   30.8048 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          70.16 using 59 PHA bins.
# Reduced chi-squared =          1.276 for     55 degrees of freedom 
# Null hypothesis probability =   8.183136e-02
 
Photon flux (15-150 keV)    in 37.81 sec:  (    ) ph/cm2/s
Energy fluence (15-150 keV)             : 4.39288e-07 ( -4.39023e-07  -6.28395e-08 ) ergs/cm2

Single BB

 
Spectral model blackbody:
------------------------------------------------------------
Parameters  : value    Lower 90%  Upper 90%
kT [keV]    : 10.2976  (-1.23248  1.44092)
R^2/D10^2   : 8.15991E-02  (-0.0323705   0.0519733)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          83.28 using 59 PHA bins.
# Reduced chi-squared =          1.461 for     57 degrees of freedom 
# Null hypothesis probability =   1.316855e-02
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  6.726e-08   1.208e-08
25- 50  1.742e-07   2.486e-08
50-150  9.891e-08   2.781e-08
15-150  3.404e-07   4.722e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 78.8546       (-23.5226      43.9085)
Norm        : 0.916843       (-0.145834     0.181444)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          74.14 using 59 PHA bins.
# Reduced chi-squared =          1.301 for     57 degrees of freedom 
# Null hypothesis probability =   6.318798e-02
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  8.987e-08   1.512e-08
25- 50  1.474e-07   1.849e-08
50-150  2.061e-07   8.785e-08
15-150  4.434e-07   9.161e-08

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 7.22600        (-1.89389      2.27523)
R1^2/D10^2  : 0.233754        (-0.131598      0.223205)
kT2 [keV]   : 23.1230        (-8.97846      -23.5215)
R2^2/D10^2  : 2.22660E-03    (-0.00208367   0.013781)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          71.06 using 59 PHA bins.
# Reduced chi-squared =          1.292 for     55 degrees of freedom 
# Null hypothesis probability =   7.141485e-02
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  8.467e-08   3.962e-08
25- 50  1.557e-07   7.719e-08
50-150  1.975e-07   1.153e-07
15-150  4.378e-07   2.070e-07

Peak spectrum fit

Power-law model

Time interval is from    0.108 sec. to    1.108 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.40239     ( -0.326036   0.325935 )
Norm@50keV  : 6.05572E-03    ( -0.00107514   0.001071 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          63.13 using 59 PHA bins.
# Reduced chi-squared =          1.107 for     57 degrees of freedom 
# Null hypothesis probability =   2.688608e-01
 
Photon flux (15-150 keV)    in 1 sec: 0.737878 ( -0.134173  0.134996 ) ph/cm2/s
Energy fluence (15-150 keV)             : 5.8486e-08 ( -1.14103e-08  1.15863e-08 ) ergs/cm2

Cutoff power-law model

Time interval is from    0.108 sec. to    1.108 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.28739     ( -1.22095   1.62487 )
Epeak [keV] : 330.440      ( -260.35 -260.35 )
Norm@50keV  : 6.86137E-03    (     )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          63.10 using 59 PHA bins.
# Reduced chi-squared =          1.127 for     56 degrees of freedom 
# Null hypothesis probability =   2.398023e-01
 
Photon flux (15-150 keV)    in 1 sec: 0.733717 ( -0.141613  0.137531 ) ph/cm2/s
Energy fluence (15-150 keV)             : 5.81513e-08 ( -1.21544e-08  1.18382e-08 ) ergs/cm2

Band function

Time interval is from    0.108 sec. to    1.108 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -1.22380   ( -0.435344   0.9267 )
beta        : -9.37167    ( 9.37167   19.3717 )
Epeak [keV] : 240.093      ( -162.4 -240.409 )
Norm@50keV   : 7.32118E-03    ( -0.00229512   0.00917735 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          63.11 using 59 PHA bins.
# Reduced chi-squared =          1.147 for     55 degrees of freedom 
# Null hypothesis probability =   2.114787e-01
 
Photon flux (15-150 keV)    in 1 sec: 0.729463 (    ) 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]    : 18.6629  (-4.05243  5.3027)
R^2/D10^2   : 3.96581E-02  (-0.0224148   0.0512557)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          71.36 using 59 PHA bins.
# Reduced chi-squared =          1.252 for     57 degrees of freedom 
# Null hypothesis probability =   9.559108e-02
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  2.732e-09   9.980e-10
25- 50  1.298e-08   4.473e-09
50-150  3.309e-08   1.281e-08
15-150  4.880e-08   1.572e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 199.363       (-84.6671      -199.363)
Norm        : 3.04617       (-0.537093     0.537093)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          63.95 using 59 PHA bins.
# Reduced chi-squared =          1.122 for     57 degrees of freedom 
# Null hypothesis probability =   2.455971e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  7.585e-09   4.458e-09
25- 50  1.459e-08   8.405e-09
50-150  3.200e-08   1.847e-08
15-150  5.418e-08   3.107e-08

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 5.54232        (-2.30893      2.93509)
R1^2/D10^2  : 1.72174        (-1.42337      6.3707)
kT2 [keV]   : 26.0210        (-6.90589      14.2843)
R2^2/D10^2  : 1.14468E-02    (-0.0086822   0.0157869)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          61.02 using 59 PHA bins.
# Reduced chi-squared =          1.109 for     55 degrees of freedom 
# Null hypothesis probability =   2.685596e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  7.531e-09   4.292e-09
25- 50  1.281e-08   6.920e-09
50-150  3.837e-08   2.311e-08
15-150  5.871e-08   3.179e-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: 1.86726     ( -0.193913   0.200155 )
Norm@50keV  : 1.36853E-03    ( -0.000173906   0.000171089 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          77.14 using 59 PHA bins.
# Reduced chi-squared =          1.353 for     57 degrees of freedom 
# Null hypothesis probability =   3.902349e-02
 
Photon flux (15-150 keV)    in 37.81 sec: 0.193725 ( -0.0212205  0.0212424 ) ph/cm2/s
Energy fluence (15-150 keV)             : 4.75699e-07 ( -5.95647e-08  6.07622e-08 ) ergs/cm2

Cutoff power-law model

Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 0.882136     ( -1.16598   0.90846 )
Epeak [keV] : 46.5847      ( -10.3295 60.6847 )
Norm@50keV  : 5.09807E-03    ( -0.00509991   0.0197133 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          73.70 using 59 PHA bins.
# Reduced chi-squared =          1.316 for     56 degrees of freedom 
# Null hypothesis probability =   5.657957e-02
 
Photon flux (15-150 keV)    in 37.81 sec: 0.185561 ( -0.022359  0.022457 ) ph/cm2/s
Energy fluence (15-150 keV)             : 4.24852e-07 ( -6.81185e-08  7.49394e-08 ) ergs/cm2

Band function

 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : 2.43038   ( -2.34218   -1.12305 )
beta        : -2.31902    ( -0.501709   0.371971 )
Epeak [keV] : 31.4253      ( -7.81334 9.04143 )
Norm@50keV   : 1.06284    ( -1.0618   30.8044 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          70.16 using 59 PHA bins.
# Reduced chi-squared =          1.276 for     55 degrees of freedom 
# Null hypothesis probability =   8.183136e-02
 
Photon flux (15-150 keV)    in 37.81 sec:  (    ) ph/cm2/s
Energy fluence (15-150 keV)             : 4.39288e-07 ( -4.39023e-07  -6.28395e-08 ) ergs/cm2

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

S(25-50 keV)  = 1.37e-07
S(50-100 keV) = 1.50e-07

T90 vs. Hardness ratio plot

T90                                   = 29.9279999732971 sec.
Hardness ratio (energy fluence ratio) = 1.09489

Color vs. Color plot

Count Ratio  (25-50 keV) / (15-25 keV) = 1.27571
Count Ratio (50-100 keV) / (15-25 keV) = 0.622109

Mask shadow pattern

IMX = 1.907596990060531E-01, IMY = -6.852290622875360E-03

TIME vs. PHA plot around the trigger time

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.408000

TIME vs. DetID plot around the trigger time

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.408000

100 us light curve (15-350 keV)

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.408000

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:
-239.072000 -17.260000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
186.6123 -62.8088    3.1  50.6   10.6   2.4332   3.7    2.6	GX 301-2                      
244.9791 -15.6426    0.2  13.9  152.0  13.4082  65.0    0.1	Sco X-1                       
255.8547 -37.6637    0.0  11.1  -60.1   0.2268   1.0   12.5	4U 1700-377                   
256.4814 -36.4595    5.3  10.7  -66.6   0.4684   2.2    3.1	GX 349+2                      
263.0177 -24.7609  340.5  15.1 -124.5  -0.0069  -0.0    1.0	GX 1+4                        
264.6434 -44.5041    3.0  20.6  -58.4   0.8754   3.8    5.4	4U 1735-44                    
268.3856  -1.4906    2.4  34.6 -160.1   1.1704   4.8    2.5	SW J1753.5-0127               
270.1019 -25.1906    8.2  21.0 -116.3   0.3255   1.4   11.9	GX 5-1                        
270.1187 -25.8558    0.0  20.8 -114.5   0.0693   0.3   12.0	GRS 1758-258                  
273.9530 -14.0540    2.9  29.3 -136.0   1.0422   4.0    3.3	GX 17+2                       
275.8410 -30.4037    5.4  25.0 -100.8   0.5791   2.2    4.9	H1820-303                     
285.0306 -24.9214    9.8  34.1 -108.6   0.4828   1.2    0.3	HT1900.1-2455                 
262.8322 -33.7262  102.1  14.2  -88.6   0.0255   0.1   10.2	GX 354-0                      
195.2890 -32.9440    3.7  43.8   51.4   2.6047   3.1 ------	UNKNOWN                       
258.1284  22.6319    2.3  53.2  172.7   3.9677   4.9 ------	UNKNOWN                       
262.6453  25.7272    2.9  57.2  176.6   5.5396   4.0 ------	UNKNOWN                       
228.1285 -61.9010    2.8  34.7   -4.9   1.0474   4.1 ------	UNKNOWN                       
293.6411 -23.4427    3.1  42.0 -107.1   3.6061   3.8 ------	UNKNOWN

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

Time interval of the image:
-17.260000 20.548000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
186.7284 -62.7622    4.3  50.6   10.7  -0.5537  -2.7    2.0	GX 301-2                      
244.7792 -15.7276    0.0  13.8  151.2   0.1741   2.6   12.7	Sco X-1                       
256.1239 -37.9478    4.2  11.5  -59.8   0.2004   2.7    9.0	4U 1700-377                   
256.5666 -36.6034    0.0  10.8  -66.2  -0.1159  -1.6   12.5	GX 349+2                      
263.2010 -24.6376    0.0  15.3 -124.7   0.1080   1.5   12.3	GX 1+4                        
264.8601 -44.4827    5.6  20.7  -58.8   0.1604   2.0    5.4	4U 1735-44                    
268.3918  -1.6146   61.2  34.5 -160.0  -0.0164  -0.2    9.8	SW J1753.5-0127               
270.3213 -25.2171   12.6  21.2 -116.1   0.0733   0.9    8.5	GX 5-1                        
270.4661 -25.7601    7.3  21.2 -114.6  -0.1369  -1.7    8.9	GRS 1758-258                  
273.9199 -13.8703   18.7  29.4 -136.4  -0.0548  -0.6   11.2	GX 17+2                       
276.1096 -30.2484    0.0  25.3 -101.1   0.2762   3.1   11.9	H1820-303                     
285.1979 -24.8589    2.8  34.2 -108.6   0.5215   4.1    9.6	HT1900.1-2455                 
263.1396 -33.7123    6.0  14.5  -88.9   0.1386   1.9   10.5	GX 354-0                      
241.6070 -39.3221    0.9  10.8    2.1   0.9263  13.5 ------	UNKNOWN                       
291.1137  -1.1605    2.2  50.7 -135.9   1.8831   5.4 ------	UNKNOWN

Post-slew image of 15-350 keV band

Time interval of the image:
57.428640 864.128600
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
170.2728 -60.5814   13.0  47.6   17.3   1.5232   0.9    2.8	Cen X-3                       
186.6179 -62.8101    1.6  39.9   13.9   7.4277   7.3    2.6	GX 301-2                      
244.9708 -15.6427    0.2  23.9  166.4  45.6315  66.8    0.5	Sco X-1                       
255.9722 -37.9818    8.1  11.3 -114.1   0.9262   1.4    8.3	4U 1700-377                   
256.2761 -36.3756    3.5  12.0 -121.5   2.0790   3.3    8.2	GX 349+2                      
262.8836 -24.8637    5.1  23.1 -144.3   1.4832   2.3    9.8	GX 1+4                        
264.6019 -44.4694    3.5  17.8  -87.6   2.2654   3.3    6.1	4U 1735-44                    
268.3771  -1.4245    7.3  45.1 -162.2   1.8305   1.6    1.8	SW J1753.5-0127               
270.3133 -24.9405    4.3  28.1 -133.9   2.2518   2.7    8.5	GX 5-1                        
270.4010 -25.6148    2.7  27.8 -132.7   3.5808   4.2    9.4	GRS 1758-258                  
273.9967 -13.9959    2.4  38.1 -144.3   4.5723   4.7    2.5	GX 17+2                       
275.8937 -30.2285    9.6  29.4 -119.1   1.0702   1.2    8.5	H1820-303                     
285.0360 -24.9213   72.1  39.1 -120.1   0.2115   0.2    0.0	HT1900.1-2455                 
262.9892 -33.9819   14.3  18.0 -122.4   0.4906   0.8    8.8	GX 354-0                      
187.6470 -52.1394    2.9  38.7   30.7   4.0904   4.0 ------	UNKNOWN                       
248.3487  13.4197    3.3  53.1  166.5  10.2023   3.5 ------	UNKNOWN                       
238.5809 -53.0299    2.8  13.8  -14.3   2.4100   4.2 ------	UNKNOWN                       
283.6358 -39.6233    3.0  32.2  -97.6   3.8331   3.9 ------	UNKNOWN

Plot creation:
Sat May 30 19:51:36 EDT 2015