batgrbproduct analysis for trigger=173904

batgrbproduct Analysis for Trigger=173904

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 19:20:02 EST 2014
             Host Name: batevent1
   Current Working Dir: /local/data/batevent/batevent_reproc/trigger173904
======================================================================

  Trigger: 00173904      Segment: 000

  BAT Trigger Time: 156888200   [s; MET]
      Trigger Stop: 156888392   [s; MET]
               UTC: 2005-12-21T20:03:20.090560    [includes UTCF correction] 
       Where From?: TDRSS position message

  BAT 
    RA: 312.395437708596   Dec: 53.0538094719893  [deg; J2000]

     Catalogged Source?: NO
     Point Source?:      YES
     GRB Indicated?:     YES    [ by BAT flight software ]
     Image S/N Ratio:    7.45
     Image Trigger?:     YES
     Rate S/N Ratio:     0  [ if not an image trigger ]
     Image S/N Ratio:    7.45

  Flight Position:   [ source = BAT ]
    RA: 312.395437708596   Dec: 53.0538094719893  [deg; J2000]

  Ground Position:   [ source = BAT pre-slew burst ]
    RA: 312.384013273902   Dec: 53.0424027507575  [deg; J2000]  
        { 20h 49m 32.2s , +53d 02' 32.6" }
         +/- 1.64171136435465 [arcmin] (estimated 90% radius based on SNR)
         +/- 0.669486708358259 [arcmin] (formal 1-sigma fit error)
    SNR: 14.9813695291972
 
  Angular difference between Flight and Ground position is 0.798877 arcmin
 
  Partial Coding Fraction: 0.4492188    [ including projection effects ]

  Duration
     T90: 42.5720000267029 +/- 5.87969658803675
        Measured from: 51.6999999880791
                   to: 94.272000014782     [s; relative to TRIGTIME]
     T50: 24.0160000026226 +/- 4.88270417274367
        Measured from: 61.2360000014305
                   to: 85.2520000040531     [s; relative to TRIGTIME]



  Fluence
     Peak Flux  (peak 1 second)
        Measured from: 58.891999989748     
                   to: 59.891999989748     [s; relative to TRIGTIME]
     Total Fluence        
        Measured from: 48.527999997139     
                   to: 98.1040000021458     [s; relative to TRIGTIME]
     
             Band 1     Band 2     Band 3     Band 4
              15-25      25-50     50-100    100-350     keV
 Total     0.323248   0.517578   0.455272   0.102745
           0.051697   0.053580   0.046351   0.037965 [error]
 Peak      0.014431   0.016365   0.032531   0.010467
           0.007575   0.007935   0.007002   0.005789 [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 1.07e-07 2.20e-07 3.53e-07 1.27e-06 9.79e-07 1.95e-06   erg/cm2
              Error 2.19e-08 2.71e-08 4.41e-08 3.54e-07 1.11e-07 3.79e-07   erg/cm2
Peak flux Power-law 1.09e-01 1.62e-01 1.79e-01 3.72e-01 5.63e-01 8.21e-01   ph/cm2/s
              Error 8.78e-02 7.87e-02 5.35e-02 2.84e-01 1.93e-01 2.70e-01   ph/cm2/s
 
Fluence   Cutoff-PL 9.92e-08 2.26e-07 3.66e-07 8.24e-07 9.64e-07 1.52e-06   erg/cm2
              Error 2.69e-08 3.08e-08 5.22e-08 6.04e-07 1.18e-07 5.30e-07   erg/cm2
Peak flux Cutoff-PL 1.15e-01 1.66e-01 1.78e-01 3.56e-01 5.68e-01 8.18e-01   ph/cm2/s
              Error 1.06e-01 7.89e-02 5.72e-02 3.66e-01 1.93e-01 3.01e-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    1.314    0.185    -      -           2.01e-03 2.13e-04   53.170 57
CPL   0.983    0.639     169.2    0.0      2.86e-03 2.56e-03   52.580 56
 
 
=== 1-s peak spectral analysis ===
 
Model Ph_index Ph_90err Epeak  Epeak_90err Norm     Nomr_90err chi2   dof
PL    0.856    0.659    -      -           4.90e-03 1.76e-03   56.160 57
CPL   0.863    0.665    9999.3    0.0      4.95e-03 1.43e-02   56.170 56
 
Model      : spectral model: simple power-law (PL) and cutoff power-law (CPL)
Ph_index   : photon index: E^-{Ph_index} (minus sign is not included in the index)
Ph_90err   : 90% error of the photon index
Epeak      : Epeak in keV
Epeak_90err: 90% error of Epeak
Norm       : normalization at 50 keV in PL model and at 1 keV in CPL model
Nomr_90err : 90% error of the normalization
chi2       : Chi-Squared
dof        : degree of freedom

 
=== T90/T50 calculation in the 50-300 keV band (BATSE band) using 64 ms lc ===
 
T90 in the 50-300 keV band: 43.520000 sec.
T50 in the 50-300 keV band: 28.096000 sec.

 
=== Table of the duration information ==
 
        Value   tstart    tstop
T100   49.576   48.528   98.104
T90    42.572   51.700   94.272
T50    24.016   61.236   85.252
Peak    1.000   58.892   59.892

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
  312.3840    53.0424   0.0129    38.3252    17.3836         1.5005010     14.981 TRIG_00173904                 
 
Foreground time interval of the image:
 48.528  98.104 (delta_t =  49.576 [sec])
Background time interval of the image:
-299.000  48.528 (delta_t = 347.528 [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 192.000000

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 192.000000

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 192.000000

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   48.528 sec. to   98.104 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.31404     ( -0.186771   0.18388 )
Norm@50keV  : 2.00578E-03    ( -0.00021341   0.00021334 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          53.17 using 59 PHA bins.
# Reduced chi-squared =         0.9327 for     57 degrees of freedom 
# Null hypothesis probability =   6.196839e-01
 
Photon flux (15-150 keV)    in 49.58 sec: 0.239926 ( -0.0271013  0.0272102 ) ph/cm2/s
Energy fluence (15-150 keV)             : 9.79398e-07 ( -1.10999e-07  1.1146e-07 ) ergs/cm2

Cutoff power-law model

Time interval is from   48.528 sec. to   98.104 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 0.982518     ( -0.853837   0.424687 )
Epeak [keV] : 169.240      ( -169.239 -169.239 )
Norm@50keV  : 2.86122E-03    ( -0.00110658   0.00400845 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          52.58 using 59 PHA bins.
# Reduced chi-squared =         0.9390 for     56 degrees of freedom 
# Null hypothesis probability =   6.049967e-01
 
Photon flux (15-150 keV)    in 49.58 sec: 0.236339 ( -0.028361  0.028312 ) ph/cm2/s
Energy fluence (15-150 keV)             : 9.64207e-07 ( -1.18184e-07  1.17034e-07 ) ergs/cm2

Band function

Time interval is from   48.528 sec. to   98.104 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -0.919305   ( 0.921495   1.41244 )
beta        : -1.60193    ( 1.61321   0.461671 )
Epeak [keV] : 147.771      ( -148.908 613.52 )
Norm@50keV   : 3.07474E-03    ( -0.00120791   0.00645792 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          52.52 using 59 PHA bins.
# Reduced chi-squared =         0.9549 for     55 degrees of freedom 
# Null hypothesis probability =   5.699944e-01
 
Photon flux (15-150 keV)    in 49.58 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]    : 18.4671  (-2.31486  2.77801)
R^2/D10^2   : 1.39924E-02  (-0.00533838   0.00821388)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          67.57 using 59 PHA bins.
# Reduced chi-squared =          1.185 for     57 degrees of freedom 
# Null hypothesis probability =   1.595691e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  4.697e-08   9.941e-09
25- 50  2.214e-07   3.850e-08
50-150  5.514e-07   9.936e-08
15-150  8.198e-07   1.197e-07

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 200.000       (      )
Norm        : 1.01085       (-0.108554     0.10854)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          57.85 using 59 PHA bins.
# Reduced chi-squared =          1.015 for     57 degrees of freedom 
# Null hypothesis probability =   4.435324e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.248e-07   6.912e-08
25- 50  2.401e-07   9.170e-08
50-150  5.267e-07   2.885e-07
15-150  8.916e-07   4.849e-07

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 5.94803        (-2.68108      6.00557)
R1^2/D10^2  : 0.334350        (-0.26878      4.14597)
kT2 [keV]   : 24.4392        (-5.03045      28.2724)
R2^2/D10^2  : 4.77763E-03    (-0.00443224   0.00630337)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          53.69 using 59 PHA bins.
# Reduced chi-squared =         0.9762 for     55 degrees of freedom 
# Null hypothesis probability =   5.247021e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.018e-07   5.280e-08
25- 50  2.148e-07   7.611e-08
50-150  6.261e-07   2.578e-07
15-150  9.427e-07   3.576e-07

Peak spectrum fit

Power-law model

Time interval is from   58.892 sec. to   59.892 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 0.856312     ( -0.731692   0.586516 )
Norm@50keV  : 4.90138E-03    ( -0.00186363   0.00164763 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          56.16 using 59 PHA bins.
# Reduced chi-squared =         0.9854 for     57 degrees of freedom 
# Null hypothesis probability =   5.063922e-01
 
Photon flux (15-150 keV)    in 1 sec: 0.562598 ( -0.19117  0.195474 ) ph/cm2/s
Energy fluence (15-150 keV)             : 5.59654e-08 ( -1.6993e-08  1.70169e-08 ) ergs/cm2

Cutoff power-law model

Time interval is from   58.892 sec. to   59.892 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 0.862780     ( -0.751509   0.578106 )
Epeak [keV] : 9999.33      ( -9999.36 -9999.36 )
Norm@50keV  : 4.95353E-03    ( -0.00100564   0.0276754 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          56.17 using 59 PHA bins.
# Reduced chi-squared =          1.003 for     56 degrees of freedom 
# Null hypothesis probability =   4.683143e-01
 
Photon flux (15-150 keV)    in 1 sec: 0.568324 ( -0.197143  0.189808 ) ph/cm2/s
Energy fluence (15-150 keV)             : 5.59693e-08 ( -1.69516e-08  1.68184e-08 ) ergs/cm2

Band function

Time interval is from   58.892 sec. to   59.892 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -0.822498   ( 0.821698   0.821698 )
beta        : -0.857227    ( -0.586798   0.73239 )
Epeak [keV] : 13.4004      ( -13.3924 -13.3924 )
Norm@50keV   : 7.54901E-03    ( -0.00429586   0 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          56.17 using 59 PHA bins.
# Reduced chi-squared =          1.021 for     55 degrees of freedom 
# Null hypothesis probability =   4.310069e-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]    : 27.5248  (-9.94633  34.3557)
R^2/D10^2   : 1.02153E-02  (-0.0101673   0.0320707)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          58.78 using 59 PHA bins.
# Reduced chi-squared =          1.031 for     57 degrees of freedom 
# Null hypothesis probability =   4.100402e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.275e-09   8.290e-10
25- 50  7.575e-09   4.619e-09
50-150  4.171e-08   2.557e-08
15-150  5.056e-08   2.996e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 200.000       (      )
Norm        : 2.45944       (-0.790088     0.789934)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          60.61 using 59 PHA bins.
# Reduced chi-squared =          1.063 for     57 degrees of freedom 
# Null hypothesis probability =   3.468612e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  6.124e-09   3.813e-09
25- 50  1.178e-08   7.450e-09
50-150  2.584e-08   1.610e-08
15-150  4.374e-08   2.714e-08

Double BB

------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 1.40031        (-1.76167      2.62622)
R1^2/D10^2  : 1.06067E+04        (      )
kT2 [keV]   : 30.1036        (-11.3079      49.6982)
R2^2/D10^2  : 7.67828E-03    (-0.00689192   0.0241359)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          55.32 using 59 PHA bins.
#Fit statistic : Chi-Squared =          55.22 using 59 PHA bins.
# Reduced chi-squared =          1.006 for     55 degrees of freedom 
# Reduced chi-squared =          1.004 for     55 degrees of freedom 
# Null hypothesis probability =   4.625347e-01
# Null hypothesis probability =   4.661401e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  4.332e-09   2.014e-09
25- 50  6.704e-09   4.161e-09
50-150  4.282e-08   2.648e-08
15-150  5.385e-08   3.188e-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: 1.31404     ( -0.186771   0.18388 )
Norm@50keV  : 2.00578E-03    ( -0.00021341   0.00021334 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          53.17 using 59 PHA bins.
# Reduced chi-squared =         0.9327 for     57 degrees of freedom 
# Null hypothesis probability =   6.196839e-01
 
Photon flux (15-150 keV)    in 49.58 sec: 0.239926 ( -0.0271013  0.0272102 ) ph/cm2/s
Energy fluence (15-150 keV)             : 9.79398e-07 ( -1.10999e-07  1.1146e-07 ) ergs/cm2

Cutoff power-law model

Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 0.982518     ( -0.853837   0.424687 )
Epeak [keV] : 169.240      ( -169.239 -169.239 )
Norm@50keV  : 2.86122E-03    ( -0.00110658   0.00400845 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          52.58 using 59 PHA bins.
# Reduced chi-squared =         0.9390 for     56 degrees of freedom 
# Null hypothesis probability =   6.049967e-01
 
Photon flux (15-150 keV)    in 49.58 sec: 0.236339 ( -0.028361  0.028312 ) ph/cm2/s
Energy fluence (15-150 keV)             : 9.64207e-07 ( -1.18184e-07  1.17034e-07 ) ergs/cm2

Band function

 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -0.919305   ( 0.921495   1.41244 )
beta        : -1.60193    ( 1.61321   0.461671 )
Epeak [keV] : 147.771      ( -148.908 613.516 )
Norm@50keV   : 3.07474E-03    ( -0.00120791   0.00645792 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          52.52 using 59 PHA bins.
# Reduced chi-squared =         0.9549 for     55 degrees of freedom 
# Null hypothesis probability =   5.699944e-01
 
Photon flux (15-150 keV)    in 49.58 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)  = 2.20e-07
S(50-100 keV) = 3.53e-07

T90 vs. Hardness ratio plot

T90                                   = 42.5720000267029 sec.
Hardness ratio (energy fluence ratio) = 1.60455

Color vs. Color plot

Count Ratio  (25-50 keV) / (15-25 keV) = 1.60118
Count Ratio (50-100 keV) / (15-25 keV) = 1.40843

Mask shadow pattern

IMX = 7.543637651388493E-01, IMY = -2.361660840860857E-01

TIME vs. PHA plot around the trigger time

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 192.000000

TIME vs. DetID plot around the trigger time

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 192.000000

100 us light curve (15-350 keV)

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 192.000000

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:
-299.000000 48.528000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
288.7781  10.9292    1.5  39.1  -60.2   4.3364   7.8    1.5	GRS 1915+105                  
299.5853  35.2029    0.2  31.7  -16.0  12.0926  52.9    0.3	Cyg X-1                       
308.1349  40.9341    1.9  29.8    1.0   1.4375   6.2    1.6	Cyg X-3                       
326.1258  38.3846    4.3  21.6   27.7   0.5627   2.7    4.3	Cyg X-2                       
305.4647  58.7415    3.4  45.2   16.4   1.5559   3.4 ------	UNKNOWN                       
308.0655  37.6562    1.7  27.6   -3.9   1.6338   6.9 ------	UNKNOWN                       
343.1975 -25.4403    2.7  44.6 -165.6   1.5582   4.3 ------	UNKNOWN                       
350.0530 -38.5854    3.5  59.0 -166.2   5.6272   3.3 ------	UNKNOWN                       
275.0447  20.0557    2.6  50.8  -44.4   4.8002   4.5 ------	UNKNOWN                       
292.3019  -2.9067    2.7  41.0  -82.3   4.2985   4.3 ------	UNKNOWN

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

Time interval of the image:
48.528000 98.104000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
288.7192  10.8606   10.5  39.2  -60.3   0.1575   1.1    6.9	GRS 1915+105                  
299.6897  35.0694    4.3  31.6  -16.1   0.1977   2.7    9.3	Cyg X-1                       
307.9042  41.0120    5.6  30.0    0.8   0.1578   2.1   10.0	Cyg X-3                       
325.9293  38.3751    6.7  21.6   27.3  -0.1147  -1.7   11.8	Cyg X-2                       
312.3840  53.0424    0.8  38.3   17.4   1.5006  15.0 ------	UNKNOWN                       
294.9230  47.6007    1.8  41.3   -1.4   0.5788   6.4 ------	UNKNOWN                       
338.3740 -29.4951    2.4  47.3 -158.3   0.6179   4.8 ------	UNKNOWN                       
335.2208 -31.4162    2.0  48.7 -154.2   0.7987   5.7 ------	UNKNOWN                       
269.8112  27.5848    1.8  55.0  -34.6   2.3306   6.3 ------	UNKNOWN                       
276.7105  18.0097    2.5  49.4  -47.3   1.4238   4.7 ------	UNKNOWN

Post-slew image of 15-350 keV band

Time interval of the image:
259.700600 303.058700
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
254.3876  35.4736    8.3  43.7  -38.0  -0.1573  -1.4    8.6	Her X-1                       
299.5944  35.2007    0.5  20.0  -96.4   1.6065  25.1    0.2	Cyg X-1                       
308.0301  40.8958    4.1  12.5 -112.9   0.1697   2.8    5.0	Cyg X-3                       
326.2622  38.4568    4.3  17.5 -167.0   0.1513   2.7    9.2	Cyg X-2                       
346.3521   5.3702    2.6  55.2 -170.9   0.8012   4.4 ------	UNKNOWN

Plot creation:
Sun May 31 14:52:21 EDT 2015