batgrbproduct analysis for trigger=173780

batgrbproduct Analysis for Trigger=173780

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): Wed Jan 22 19:22:29 EST 2014
             Host Name: batevent1
   Current Working Dir: /local/data/batevent/batevent_reproc/trigger173780
======================================================================

  Trigger: 00173780      Segment: 000

  BAT Trigger Time: 156822675.776   [s; MET]
      Trigger Stop: 156822675.84   [s; MET]
               UTC: 2005-12-21T01:51:15.868000    [includes UTCF correction] 
       Where From?: (*SHORT BURST*) TDRSS scaled map message

  BAT 
    RA: 328.710912255944   Dec: 16.8957209657683  [deg; J2000]

     Catalogged Source?: NO
     Point Source?:      YES
     GRB Indicated?:     YES    [ by BAT flight software ]
     Image S/N Ratio:    16.39
     Image Trigger?:     NO
     Rate S/N Ratio:     56.0267793113258  [ if not an image trigger ]
     Image S/N Ratio:    16.39

  Flight Position:   [ source = BAT ]
    RA: 328.710912255944   Dec: 16.8957209657683  [deg; J2000]

  Ground Position:   [ source = BAT pre-slew burst ]
    RA: 328.712488221718   Dec: 16.8911945453272  [deg; J2000]  
        { 21h 54m 51.0s , +16d 53' 28.3" }
         +/- 0.616931500733245 [arcmin] (estimated 90% radius based on SNR)
         +/- 0.191656142438593 [arcmin] (formal 1-sigma fit error)
    SNR: 60.6428894105721
 
  Angular difference between Flight and Ground position is 0.286260 arcmin
 
  Partial Coding Fraction: 0.6328125    [ including projection effects ]

  Duration
     T90: 1.39200001955032 +/- 0.1974638995435
        Measured from: 0.0320000052452087
                   to: 1.42400002479553     [s; relative to TRIGTIME]
     T50: 0.548000007867813 +/- 0.0800999213143316
        Measured from: 0.112000018358231
                   to: 0.660000026226044     [s; relative to TRIGTIME]



  Fluence
     Peak Flux  (peak 1 second)
        Measured from: -0.0279999971389771     
                   to: 0.972000002861023     [s; relative to TRIGTIME]
     Total Fluence        
        Measured from: -0.0320000052452087     
                   to: 2.09200000762939     [s; relative to TRIGTIME]
     
             Band 1     Band 2     Band 3     Band 4
              15-25      25-50     50-100    100-350     keV
 Total     0.453369   0.589756   0.545039   0.166671
           0.013733   0.015021   0.014121   0.010538 [error]
 Peak      0.333818   0.493821   0.491908   0.150075
           0.010863   0.012541   0.012510   0.009073 [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 1.38e-07 2.71e-07 4.13e-07 1.37e-06 1.16e-06 2.19e-06   erg/cm2
              Error 8.26e-09 9.32e-09 1.41e-08 1.09e-07 3.50e-08 1.15e-07   erg/cm2
Peak flux Power-law 3.37e+00 3.89e+00 3.23e+00 4.50e+00 1.21e+01 1.50e+01   ph/cm2/s
              Error 2.02e-01 1.39e-01 1.03e-01 3.15e-01 3.72e-01 4.32e-01   ph/cm2/s
 
Fluence   Cutoff-PL 1.38e-07 2.72e-07 4.13e-07 1.36e-06 1.16e-06 2.18e-06   erg/cm2
              Error 8.62e-09 9.27e-09 1.38e-08 1.15e-07 3.47e-08 1.75e-07   erg/cm2
Peak flux Cutoff-PL 3.31e+00 3.90e+00 3.25e+00 4.19e+00 1.21e+01 1.47e+01   ph/cm2/s
              Error 2.01e-01 1.38e-01 1.26e-01 6.14e-01 3.97e-01 7.93e-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    1.395    0.054    -      -           5.63e-02 1.61e-03   61.000 57
CPL   1.392    0.055    9998.4    0.0      5.65e-02 4.08e-03   61.040 56
 
 
=== 1-s peak spectral analysis ===
 
Model Ph_index Ph_90err Epeak  Epeak_90err Norm     Nomr_90err chi2   dof
PL    1.270    0.052    -      -           1.02e-01 2.91e-03   66.640 57
CPL   1.196    0.156     579.6    0.0      1.10e-01 1.72e-02   66.480 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: 1.280000 sec.
T50 in the 50-300 keV band: 0.128000 sec.

 
=== Table of the duration information ==
 
        Value   tstart    tstop
T100    2.124   -0.032    2.092
T90     1.392    0.032    1.424
T50     0.548    0.112    0.660
Peak    1.000   -0.028    0.972

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
  328.7125    16.8912   0.0032    36.6224  -178.5787         1.8182488     60.643 TRIG_00173780                 
 
Foreground time interval of the image:
 -0.032   2.092 (delta_t =   2.124 [sec])
Background time interval of the image:
-223.875  -0.032 (delta_t = 223.843 [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 0.064000

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 0.064000

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 0.064000

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   -0.032 sec. to    2.092 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.39466     ( -0.0544858   0.0544723 )
Norm@50keV  : 5.63380E-02    ( -0.00161317   0.00161293 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          61.00 using 59 PHA bins.
# Reduced chi-squared =          1.070 for     57 degrees of freedom 
# Null hypothesis probability =   3.342475e-01
 
Photon flux (15-150 keV)    in 2.124 sec: 6.85263 ( -0.21709  0.218065 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.15752e-06 ( -3.49203e-08  3.4981e-08 ) ergs/cm2

Cutoff power-law model

Time interval is from   -0.032 sec. to    2.092 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.39177     ( -0.0553948   0.0542987 )
Epeak [keV] : 9998.40      ( -9998.81 -9998.81 )
Norm@50keV  : 5.64594E-02    ( -0.00161641   0.00654324 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          61.04 using 59 PHA bins.
# Reduced chi-squared =          1.090 for     56 degrees of freedom 
# Null hypothesis probability =   2.996771e-01
 
Photon flux (15-150 keV)    in 2.124 sec: 6.85580 ( -0.11262  0.21132 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.15756e-06 ( -3.47253e-08  3.46085e-08 ) ergs/cm2

Band function

Time interval is from   -0.032 sec. to    2.092 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -1.12032   ( 1.12033   1.12033 )
beta        : -1.39466    ( -0.0544125   0.054413 )
Epeak [keV] : 37.1401      ( -37.1376 -37.1376 )
Norm@50keV   : 0.110711    ( -0.0522048   7.76563 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          61.00 using 59 PHA bins.
# Reduced chi-squared =          1.109 for     55 degrees of freedom 
# Null hypothesis probability =   2.691337e-01
 
Photon flux (15-150 keV)    in 2.124 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]    : 18.4007  (  )
R^2/D10^2   : 0.381752  (   )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =         355.61 using 59 PHA bins.
# Reduced chi-squared =         6.2388 for     57 degrees of freedom 
# Null hypothesis probability =   9.278110e-45
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  5.457e-08   3.207e-09
25- 50  2.565e-07   9.983e-09
50-150  6.339e-07   2.952e-08
15-150  9.450e-07   3.250e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 200.000       (      )
Norm        : 28.6635       (-0.825393     0.825041)
------------------------------------------------------------
#Fit statistic : Chi-Squared =         104.78 using 59 PHA bins.
# Reduced chi-squared =         1.8382 for     57 degrees of freedom 
# Null hypothesis probability =   1.189227e-04
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.516e-07   4.864e-09
25- 50  2.917e-07   8.496e-09
50-150  6.398e-07   1.965e-08
15-150  1.083e-06   3.547e-08

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 7.61307        (-0.923827      1.01702)
R1^2/D10^2  : 5.00603        (-1.7004      2.92099)
kT2 [keV]   : 31.6718        (-3.37896      4.7493)
R2^2/D10^2  : 5.11655E-02    (-0.0190029   0.0244012)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          78.74 using 59 PHA bins.
# Reduced chi-squared =          1.432 for     55 degrees of freedom 
# Null hypothesis probability =   1.956578e-02
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.236e-07   1.288e-08
25- 50  2.756e-07   1.827e-08
50-150  7.576e-07   6.011e-08
15-150  1.157e-06   7.753e-08

Peak spectrum fit

Power-law model

Time interval is from   -0.028 sec. to    0.972 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.27041     ( -0.0522041   0.0521367 )
Norm@50keV  : 0.102082    ( -0.00291305   0.00291161 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          66.64 using 59 PHA bins.
# Reduced chi-squared =          1.169 for     57 degrees of freedom 
# Null hypothesis probability =   1.793145e-01
 
Photon flux (15-150 keV)    in 1 sec: 12.1148 ( -0.371958  0.373034 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.01624e-06 ( -3.07279e-08  3.07608e-08 ) ergs/cm2

Cutoff power-law model

Time interval is from   -0.028 sec. to    0.972 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.19558     ( -0.216378   0.0952368 )
Epeak [keV] : 579.572      ( -657.598 -657.598 )
Norm@50keV  : 0.110055    ( -0.00954338   0.0249324 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          66.48 using 59 PHA bins.
# Reduced chi-squared =          1.187 for     56 degrees of freedom 
# Null hypothesis probability =   1.595198e-01
 
Photon flux (15-150 keV)    in 1 sec: 12.0629 ( -0.3968  0.3975 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.01369e-06 ( -3.2073e-08  2.887e-08 ) ergs/cm2

Band function

Time interval is from   -0.028 sec. to    0.972 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -1.08171   ( 0.90993   0.90993 )
beta        : -1.31428    ( 1.31674   0.0919492 )
Epeak [keV] : 228.786      ( -237.923 -237.923 )
Norm@50keV   : 0.127156    ( -0.0250153   0 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          66.01 using 59 PHA bins.
# Reduced chi-squared =          1.200 for     55 degrees of freedom 
# Null hypothesis probability =   1.469583e-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]    : 19.5969  (  )
R^2/D10^2   : 0.578085  (   )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =         321.84 using 59 PHA bins.
# Reduced chi-squared =         5.6463 for     57 degrees of freedom 
# Null hypothesis probability =   1.309602e-38
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  4.314e-08   2.565e-09
25- 50  2.120e-07   8.250e-09
50-150  6.016e-07   2.895e-08
15-150  8.567e-07   2.985e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 199.363       (      )
Norm        : 51.2234       (     )
------------------------------------------------------------
#Fit statistic : Chi-Squared =         166.35 using 59 PHA bins.
# Reduced chi-squared =         2.9184 for     57 degrees of freedom 
# Null hypothesis probability =   1.228363e-12
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.276e-07   3.800e-09
25- 50  2.454e-07   7.850e-09
50-150  5.381e-07   1.555e-08
15-150  9.110e-07   2.725e-08

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 8.33697        (-1.05992      1.16563)
R1^2/D10^2  : 5.92832        (-1.94585      3.3252)
kT2 [keV]   : 33.5573        (-3.78479      5.57413)
R2^2/D10^2  : 8.14354E-02    (-0.0321184   0.0410393)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          79.34 using 59 PHA bins.
# Reduced chi-squared =          1.442 for     55 degrees of freedom 
# Null hypothesis probability =   1.753100e-02
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  9.005e-08   9.045e-09
25- 50  2.301e-07   1.500e-08
50-150  6.927e-07   6.555e-08
15-150  1.013e-06   6.820e-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: 1.39466     ( -0.0544858   0.0544723 )
Norm@50keV  : 5.63380E-02    ( -0.00161317   0.00161293 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          61.00 using 59 PHA bins.
# Reduced chi-squared =          1.070 for     57 degrees of freedom 
# Null hypothesis probability =   3.342475e-01
 
Photon flux (15-150 keV)    in 2.124 sec: 6.85263 ( -0.21709  0.218065 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.15752e-06 ( -3.49203e-08  3.4981e-08 ) ergs/cm2

Cutoff power-law model

Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.39177     ( -0.0553948   0.0542987 )
Epeak [keV] : 9998.40      ( -9998.81 -9998.81 )
Norm@50keV  : 5.64594E-02    ( -0.00161641   0.00654324 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          61.04 using 59 PHA bins.
# Reduced chi-squared =          1.090 for     56 degrees of freedom 
# Null hypothesis probability =   2.996771e-01
 
Photon flux (15-150 keV)    in 2.124 sec: 6.85580 ( -0.11262  0.21132 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.15756e-06 ( -3.47253e-08  3.46085e-08 ) ergs/cm2

Band function

 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -1.12032   ( 1.12033   1.12033 )
beta        : -1.39466    ( -0.0544125   0.054413 )
Epeak [keV] : 37.1401      ( -37.1376 -37.1376 )
Norm@50keV   : 0.110711    ( -0.0559859   7.76563 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          61.00 using 59 PHA bins.
# Reduced chi-squared =          1.109 for     55 degrees of freedom 
# Null hypothesis probability =   2.691337e-01
 
Photon flux (15-150 keV)    in 2.124 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)  = 2.71e-07
S(50-100 keV) = 4.13e-07

T90 vs. Hardness ratio plot

T90                                   = 1.39200001955032 sec.
Hardness ratio (energy fluence ratio) = 1.52399

Color vs. Color plot

Count Ratio  (25-50 keV) / (15-25 keV) = 1.30083
Count Ratio (50-100 keV) / (15-25 keV) = 1.2022

Mask shadow pattern

IMX = -7.430423029095083E-01, IMY = 1.843573853546018E-02

TIME vs. PHA plot around the trigger time

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.064000

TIME vs. DetID plot around the trigger time

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.064000

100 us light curve (15-350 keV)

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.064000

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:
-223.875410 -0.032000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
254.2593  35.4597    0.0  31.3   -4.1  -0.1827  -1.0   12.0	Her X-1                       
268.3728  -1.4794   27.3  42.3  -70.0  -0.3276  -0.4    1.6	SW J1753.5-0127               
288.8034  10.9475    1.0  23.5  -98.2   2.2623  12.1    0.3	GRS 1915+105                  
299.5954  35.2068    0.2   5.8  150.6   8.4280  57.0    0.4	Cyg X-1                       
308.1176  40.9471    1.2  14.0  129.1   1.6485   9.9    0.5	Cyg X-3                       
325.9302  38.3016    0.0  27.0  144.0   0.2889   1.4   11.4	Cyg X-2                       
308.0334  37.6509    2.3  13.0  142.6   0.7942   5.0 ------	UNKNOWN                       
253.5291  34.6955    2.4  32.0   -5.4   0.9066   4.7 ------	UNKNOWN                       
261.5087  13.7542    2.3  34.8  -46.0   1.1761   5.0 ------	UNKNOWN                       
319.2934 -11.9825    2.9  52.7 -141.1   3.4436   4.0 ------	UNKNOWN

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

Time interval of the image:
-0.032000 2.092000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
254.4546  35.3423  125.4  31.2   -4.4  -0.0023  -0.1    0.1	Her X-1                       
268.3713  -1.6049    4.5  42.4  -70.1   0.2224   2.5    9.1	SW J1753.5-0127               
288.9672  11.0551    7.5  23.4  -98.6  -0.0425  -1.5   11.9	GRS 1915+105                  
299.6674  35.0157   25.9   5.9  152.5  -0.0092  -0.4   11.8	Cyg X-1                       
308.0246  41.1546    0.0  14.0  128.2   0.0455   2.0   12.7	Cyg X-3                       
326.2491  38.1556    7.6  27.3  144.3  -0.0427  -1.5   10.6	Cyg X-2                       
311.9930  33.7512    2.5  16.1  158.6   0.0992   4.5 ------	UNKNOWN                       
341.8897   9.1392    2.4  51.6  179.5   0.3077   4.8 ------	UNKNOWN                       
328.7125  16.8912    0.2  36.6 -178.6   1.8183  60.6 ------	UNKNOWN                       
335.5700   5.0871    2.0  49.3 -171.2   0.2788   5.7 ------	UNKNOWN                       
260.3820  23.9530    2.0  29.8  -29.1   0.1423   5.9 ------	UNKNOWN                       
279.7984  19.8688    2.3  18.3  -66.0   0.1215   4.9 ------	UNKNOWN                       
227.4760  20.6360    2.7  58.4  -12.9   0.4406   4.3 ------	UNKNOWN

Post-slew image of 15-350 keV band

Time interval of the image:
71.524590 290.682800
292.224000 302.318300
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
288.8013  10.9748    2.0  39.1  -60.2   2.4122   5.9    1.8	GRS 1915+105                  
299.5908  35.2037    0.2  31.7  -15.9   8.7165  48.3    0.1	Cyg X-1                       
308.1094  40.9643    1.4  29.9    1.0   1.3731   8.0    0.7	Cyg X-3                       
326.3159  38.2764    3.8  21.5   28.1   0.4481   3.0    7.3	Cyg X-2                       
308.0424  20.2956    2.6  19.8  -43.8   0.7076   4.5 ------	UNKNOWN                       
347.0517 -39.9776    3.5  59.4 -163.1   4.8915   3.3 ------	UNKNOWN                       
311.0822  -3.7825    2.3  27.0 -105.2   1.0067   4.9 ------	UNKNOWN                       
265.3358  36.0675    2.3  58.8  -24.5   5.4058   5.0 ------	UNKNOWN                       
278.0306  16.0245    2.4  48.4  -50.2   3.5392   4.8 ------	UNKNOWN

Plot creation:
Sun May 31 14:54:08 EDT 2015