batgrbproduct analysis for trigger=668543

batgrbproduct Analysis for Trigger=668543

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): Sat Mar 19 20:54:19 EDT 2016
             Host Name: bat1
   Current Working Dir: /local/data/bat1/alien/Swift_3rdBATcatalog/event/batevent_reproc/trigger668543
======================================================================

  Trigger: 00668543      Segment: 000

  BAT Trigger Time: 472964728   [s; MET]
      Trigger Stop: 472964728.256   [s; MET]
               UTC: 2015-12-28T03:05:12.384680    [includes UTCF correction] 
       Where From?: TDRSS position message

  BAT 
    RA: 214.003951052387   Dec: -17.6890004436844  [deg; J2000]

     Catalogged Source?: NO
     Point Source?:      YES
     GRB Indicated?:     YES    [ by BAT flight software ]
     Image S/N Ratio:    6.53
     Image Trigger?:     NO
     Rate S/N Ratio:     36.8510515453766  [ if not an image trigger ]
     Image S/N Ratio:    6.53

  Flight Position:   [ source = BAT ]
    RA: 214.003951052387   Dec: -17.6890004436844  [deg; J2000]

  Ground Position:   [ source = BAT pre-slew burst ]
    RA: 214.019846236906   Dec: -17.6664070977249  [deg; J2000]  
        { 14h 16m 04.8s , -17d 39' 59.1" }
         +/- 1.7825050825542 [arcmin] (estimated 90% radius based on SNR)
         +/- 0.670078010584032 [arcmin] (formal 1-sigma fit error)
    SNR: 13.3199619579118
 
  Angular difference between Flight and Ground position is 1.631976 arcmin
 
  Partial Coding Fraction: 1    [ including projection effects ]

  Duration
     T90: 0.275999963283539 +/- 0.039999997615816
        Measured from: -0.0279999971389771
                   to: 0.247999966144562     [s; relative to TRIGTIME]
     T50: 0.167999982833862 +/- 0.0432666533938203
        Measured from: 0.0199999809265137
                   to: 0.187999963760376     [s; relative to TRIGTIME]



  Fluence
     Peak Flux  (peak 1 second)
        Measured from: -0.378000020980835     
                   to: 0.621999979019165     [s; relative to TRIGTIME]
     Total Fluence        
        Measured from: -0.0360000133514404     
                   to: 0.276000022888184     [s; relative to TRIGTIME]
     
             Band 1     Band 2     Band 3     Band 4
              15-25      25-50     50-100    100-350     keV
 Total     0.012773   0.042010   0.045040   0.009667
           0.003802   0.004469   0.004718   0.004119 [error]
 Peak      0.016989   0.041701   0.041932   0.013461
           0.006355   0.006844   0.006473   0.005673 [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 4.90e-09 1.37e-08 3.09e-08 1.87e-07 8.33e-08 2.36e-07   erg/cm2
              Error 1.17e-09 2.00e-09 4.12e-09 5.55e-08 1.12e-08 5.78e-08   erg/cm2
Peak flux Power-law 1.74e-01 2.47e-01 2.60e-01 5.04e-01 8.39e-01 1.19e+00   ph/cm2/s
              Error 6.49e-02 5.62e-02 4.92e-02 2.10e-01 1.52e-01 2.38e-01   ph/cm2/s
 
Fluence   Cutoff-PL 3.56e-09 1.52e-08 3.49e-08 4.12e-08 7.64e-08 9.48e-08   erg/cm2
              Error 1.37e-09 2.49e-09 5.17e-09 4.39e-08 1.26e-08 4.44e-08   erg/cm2
Peak flux Cutoff-PL 1.48e-01 2.54e-01 2.78e-01 2.85e-01 8.19e-01 9.66e-01   ph/cm2/s
              Error 7.85e-02 6.24e-02 6.14e-02 2.88e-01 1.57e-01 3.03e-01   ph/cm2/s
 
Fluence        Band -------- -------- -------- -------- -------- --------   erg/cm2
              Error -------- -------- -------- -------- -------- --------   erg/cm2
Peak flux      Band -------- -------- -------- -------- -------- --------   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    0.824    0.200    -      -           2.31e-02 2.84e-03   54.960 57
CPL  -0.584    1.101     102.0   62.2      1.01e-01 1.57e-01   48.270 56
 
 
=== 1-s peak spectral analysis ===
 
Model Ph_index Ph_90err Epeak  Epeak_90err Norm     Nomr_90err chi2   dof
PL    0.927    0.313    -      -           7.31e-03 1.32e-03   58.090 57
CPL   0.323    1.179     159.6    0.0      1.35e-02 2.52e-02   57.340 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: 0.192000 sec.
T50 in the 50-300 keV band: 0.128000 sec.

 
=== Table of the duration information ==
 
        Value   tstart    tstop
T100    0.312   -0.036    0.276
T90     0.276   -0.028    0.248
T50     0.168    0.020    0.188
Peak    1.000   -0.378    0.622

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
  214.0198   -17.6664   0.0145    14.2243  -167.1569         0.1175101     13.320 TRIG_00668543                 
 
Foreground time interval of the image:
 -0.036   0.276 (delta_t =   0.312 [sec])
Background time interval of the image:
-67.499  -0.036 (delta_t =  67.463 [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 0.256000

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 0.256000

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 0.256000

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   -0.036 sec. to    0.276 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 0.824371     ( -0.203026   0.196566 )
Norm@50keV  : 2.31150E-02    ( -0.00284636   0.00283681 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          54.96 using 59 PHA bins.
# Reduced chi-squared =         0.9642 for     57 degrees of freedom 
# Null hypothesis probability =   5.519268e-01
 
Photon flux (15-150 keV)    in 0.312 sec: 2.65468 ( -0.32399  0.3243 ) ph/cm2/s
Energy fluence (15-150 keV)             : 8.34363e-08 ( -1.11935e-08  1.12931e-08 ) ergs/cm2

Cutoff power-law model

Time interval is from   -0.036 sec. to    0.276 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: -0.583979     ( -1.23273   0.968552 )
Epeak [keV] : 101.966      ( -25.0876 99.3817 )
Norm@50keV  : 0.101308    ( -0.0637016   0.250547 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          48.27 using 59 PHA bins.
# Reduced chi-squared =         0.8619 for     56 degrees of freedom 
# Null hypothesis probability =   7.591867e-01
 
Photon flux (15-150 keV)    in 0.312 sec: 2.53317 ( -0.33594  0.33578 ) ph/cm2/s
Energy fluence (15-150 keV)             : 7.65729e-08 ( -1.26091e-08  1.26085e-08 ) ergs/cm2

Band function

Time interval is from   -0.036 sec. to    0.276 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : 4.99999   ( -5.0229e-05   -4.99999 )
beta        : -1.33626    ( -0.518707   0.339035 )
Epeak [keV] : 46.9547      ( -10.4656 7.98883 )
Norm@50keV   : 45.7123    ( -5.4008   132.179 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          46.28 using 59 PHA bins.
# Reduced chi-squared =         0.8414 for     55 degrees of freedom 
# Null hypothesis probability =   7.926765e-01
 
Photon flux (15-150 keV)    in 0.312 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]    : 21.9507  (-3.03941  3.80623)
R^2/D10^2   : 0.102607  (-0.0395901   0.0599057)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          49.79 using 59 PHA bins.
# Reduced chi-squared =         0.8736 for     57 degrees of freedom 
# Null hypothesis probability =   7.397560e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  2.858e-09   6.831e-10
25- 50  1.509e-08   2.613e-09
50-150  5.432e-08   1.225e-08
15-150  7.227e-08   1.285e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 200.000       (-23.7947      -200)
Norm        : 9.89150       (-1.3107     1.3107)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          85.91 using 59 PHA bins.
# Reduced chi-squared =          1.507 for     57 degrees of freedom 
# Null hypothesis probability =   7.960060e-03
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  7.685e-09   4.343e-09
25- 50  1.478e-08   8.318e-09
50-150  3.242e-08   1.810e-08
15-150  5.489e-08   3.083e-08

Double BB

------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 44.7857        (-45.3042      -45.3042)
R1^2/D10^2  : 6.83720E-03        (-0.00637631      0.113829)
kT2 [keV]   : 15.3733        (-15.5008      -15.5008)
R2^2/D10^2  : 0.195159    (-0.193487   -0.193487)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          47.41 using 59 PHA bins.
#Fit statistic : Chi-Squared =          47.39 using 59 PHA bins.
# Reduced chi-squared =         0.8620 for     55 degrees of freedom 
# Reduced chi-squared =         0.8617 for     55 degrees of freedom 
# Null hypothesis probability =   7.565557e-01
# Null hypothesis probability =   7.572784e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  3.526e-09   2.206e-09
25- 50  1.573e-08   1.066e-08
50-150  5.875e-08   3.677e-08
15-150  7.801e-08   6.572e-08

Peak spectrum fit

Power-law model

Time interval is from   -0.378 sec. to    0.622 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 0.927100     ( -0.322195   0.303625 )
Norm@50keV  : 7.30736E-03    ( -0.00132434   0.0013133 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          58.09 using 59 PHA bins.
# Reduced chi-squared =          1.019 for     57 degrees of freedom 
# Null hypothesis probability =   4.348806e-01
 
Photon flux (15-150 keV)    in 1 sec: 0.839045 ( -0.152114  0.152736 ) ph/cm2/s
Energy fluence (15-150 keV)             : 8.1169e-08 ( -1.55409e-08  1.57012e-08 ) ergs/cm2

Cutoff power-law model

Time interval is from   -0.378 sec. to    0.622 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 0.322614     ( -1.50958   0.848305 )
Epeak [keV] : 159.557      ( -159.558 -159.558 )
Norm@50keV  : 1.35369E-02    ( -0.00727411   0.0430815 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          57.34 using 59 PHA bins.
# Reduced chi-squared =          1.024 for     56 degrees of freedom 
# Null hypothesis probability =   4.251674e-01
 
Photon flux (15-150 keV)    in 1 sec: 0.818779 ( -0.157238  0.1577 ) ph/cm2/s
Energy fluence (15-150 keV)             : 7.86466e-08 ( -1.67182e-08  1.65848e-08 ) ergs/cm2

Band function

Time interval is from   -0.378 sec. to    0.622 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -0.319568   ( 0.571831   1.59004 )
beta        : -10.0000    ( 10   10 )
Epeak [keV] : 159.724      ( -61.9125 194.491 )
Norm@50keV   : 1.35514E-02    ( -0.00727438   0.0431835 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          57.34 using 59 PHA bins.
# Reduced chi-squared =          1.043 for     55 degrees of freedom 
# Null hypothesis probability =   3.883635e-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]    : 23.0472  (-4.96033  7.05738)
R^2/D10^2   : 2.65581E-02  (-0.0147598   0.0301615)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          60.62 using 59 PHA bins.
# Reduced chi-squared =          1.064 for     57 degrees of freedom 
# Null hypothesis probability =   3.465991e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  2.554e-09   1.093e-09
25- 50  1.387e-08   4.612e-09
50-150  5.504e-08   1.820e-08
15-150  7.146e-08   2.562e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 200.000       (-47.5863      -200)
Norm        : 3.36055       (-0.631339     0.631339)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          68.62 using 59 PHA bins.
# Reduced chi-squared =          1.204 for     57 degrees of freedom 
# Null hypothesis probability =   1.393679e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  8.367e-09   4.848e-09
25- 50  1.610e-08   9.380e-09
50-150  3.530e-08   2.032e-08
15-150  5.976e-08   3.491e-08

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 9.09915        (-4.94668      -9.12233)
R1^2/D10^2  : 0.229498        (-0.196721      2.17741)
kT2 [keV]   : 34.2602        (-32.3434      -34.3304)
R2^2/D10^2  : 6.65912E-03    (-0.00599473   0.0135683)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          56.52 using 59 PHA bins.
# Reduced chi-squared =          1.028 for     55 degrees of freedom 
# Null hypothesis probability =   4.178253e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  4.843e-09   2.880e-09
25- 50  1.533e-08   8.255e-09
50-150  5.985e-08   3.185e-08
15-150  8.003e-08   3.941e-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: 0.824371     ( -0.203026   0.196566 )
Norm@50keV  : 2.31150E-02    ( -0.00284636   0.00283681 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          54.96 using 59 PHA bins.
# Reduced chi-squared =         0.9642 for     57 degrees of freedom 
# Null hypothesis probability =   5.519268e-01
 
Photon flux (15-150 keV)    in 0.312 sec: 2.65471 ( -0.32399  0.324301 ) ph/cm2/s
Energy fluence (15-150 keV)             : 8.34254e-08 ( -1.11876e-08  1.12996e-08 ) ergs/cm2

Cutoff power-law model

Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: -0.584016     ( -1.23273   0.968556 )
Epeak [keV] : 101.965      ( -25.0874 99.3819 )
Norm@50keV  : 0.101312    ( -0.0637021   0.250547 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          48.27 using 59 PHA bins.
# Reduced chi-squared =         0.8619 for     56 degrees of freedom 
# Null hypothesis probability =   7.591867e-01
 
Photon flux (15-150 keV)    in 0.312 sec: 2.53317 ( -0.33594  0.33578 ) ph/cm2/s
Energy fluence (15-150 keV)             : 7.66094e-08 ( -1.26132e-08  1.26238e-08 ) ergs/cm2

Band function

 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : 4.99999   ( -14.9998   -4.99999 )
beta        : -1.33626    ( -0.518707   0.339035 )
Epeak [keV] : 46.9547      ( -10.4656 7.98883 )
Norm@50keV   : 45.7123    ( -5.4008   132.179 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          46.28 using 59 PHA bins.
# Reduced chi-squared =         0.8414 for     55 degrees of freedom 
# Null hypothesis probability =   7.926765e-01
 
Photon flux (15-150 keV)    in 0.312 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)  = 1.37e-08
S(50-100 keV) = 3.09e-08

T90 vs. Hardness ratio plot

T90                                   = 0.275999963283539 sec.
Hardness ratio (energy fluence ratio) = 2.25547

Color vs. Color plot

Count Ratio  (25-50 keV) / (15-25 keV) = 3.28897
Count Ratio (50-100 keV) / (15-25 keV) = 3.52619

Mask shadow pattern

IMX = -2.471490745748556E-01, IMY = 5.634636703088051E-02

TIME vs. PHA plot around the trigger time

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.256000

TIME vs. DetID plot around the trigger time

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.256000

100 us light curve (15-350 keV)

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.256000

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:
-67.499400 -0.036000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
170.3029 -60.6036    2.7  38.8   17.4   0.7207   4.3    1.2	Cen X-3                       
186.6402 -62.7296    3.6  34.8    5.8   0.4339   3.2    2.5	GX 301-2                      
244.9837 -15.6536    1.1  37.0 -116.8   2.1989  11.0    0.8	Sco X-1                       
255.9403 -37.8528    2.8  39.8  -77.6   1.6206   4.1    2.3	4U 1700-377                   
256.4871 -36.4958   64.3  40.4  -79.7   0.0728   0.2    5.0	GX 349+2                      
127.5362 -84.6796    2.7  58.5   -5.1   2.8525   4.3 ------	UNKNOWN                       
245.4680  -7.6297    2.5  42.0 -126.8   1.1349   4.6 ------	UNKNOWN

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

Time interval of the image:
-0.036000 0.276000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
170.3492 -60.8083    6.5  38.9   17.1   0.0253   1.8   11.2	Cen X-3                       
186.3370 -62.7874   13.1  34.9    5.9   0.0103   0.9    8.8	GX 301-2                      
245.0687 -15.5783    9.5  37.1 -116.9   0.0222   1.2    6.4	Sco X-1                       
255.9342 -37.7347    7.6  39.8  -77.8   0.0525   1.5    7.0	4U 1700-377                   
256.4194 -36.5033    7.5  40.3  -79.7  -0.0586  -1.5    4.9	GX 349+2                      
213.0662  11.1716    2.3  42.2  176.2   0.0752   4.9 ------	UNKNOWN                       
214.0198 -17.6664    0.9  14.2 -167.2   0.1175  13.3 ------	UNKNOWN                       
232.9542   7.5313    2.2  45.2 -155.1   0.0828   5.3 ------	UNKNOWN

Post-slew image of 15-350 keV band

Time interval of the image:
71.700600 201.100600
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
170.4564 -60.6016    3.6  39.1   16.8   0.7298   3.2    4.3	Cen X-3                       
186.5787 -62.7509    1.9  35.2    5.3   1.1885   6.0    2.4	GX 301-2                      
244.9642 -15.6200    0.7  37.2 -115.8   4.5009  15.8    1.5	Sco X-1                       
255.9791 -37.8289    1.5  40.4  -76.9   4.5343   7.8    1.0	4U 1700-377                   
256.4380 -36.3765    4.1  40.9  -79.1   1.8266   2.9    2.8	GX 349+2                      
201.5287  12.8337    2.7  43.4  160.2   1.4430   4.3 ------	UNKNOWN                       
155.2941 -82.7835    2.7  55.6   -4.3   2.3078   4.3 ------	UNKNOWN                       
241.9469 -56.8839    2.5  35.8  -43.0   1.0169   4.6 ------	UNKNOWN

Plot creation:
Sat Mar 19 22:25:28 EDT 2016