batgrbproduct analysis for trigger=434360

batgrbproduct Analysis for Trigger=434360

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): Fri Jan 17 15:56:59 EST 2014
             Host Name: batevent1
   Current Working Dir: /local/data/batevent/batevent_reproc/trigger434360
======================================================================

  Trigger: 00434360      Segment: 000

  BAT Trigger Time: 306392611.968   [s; MET]
      Trigger Stop: 306392616.064   [s; MET]
               UTC: 2010-09-17T05:03:25.783360    [includes UTCF correction] 
       Where From?: TDRSS position message

  BAT 
    RA: 289.264654463964   Dec: -17.1044750247871  [deg; J2000]

     Catalogged Source?: NO
     Point Source?:      YES
     GRB Indicated?:     YES    [ by BAT flight software ]
     Image S/N Ratio:    7.15
     Image Trigger?:     NO
     Rate S/N Ratio:     7.87400787401181  [ if not an image trigger ]
     Image S/N Ratio:    7.15

  Flight Position:   [ source = BAT ]
    RA: 289.264654463964   Dec: -17.1044750247871  [deg; J2000]

  Ground Position:   [ source = BAT pre-slew burst ]
    RA: 289.245015480821   Dec: -17.1145190496547  [deg; J2000]  
        { 19h 16m 58.8s , -17d 06' 52.3" }
         +/- 2.02941237603008 [arcmin] (estimated 90% radius based on SNR)
         +/- 0.85007181876365 [arcmin] (formal 1-sigma fit error)
    SNR: 11.066695103936
 
  Angular difference between Flight and Ground position is 1.277295 arcmin
 
  Partial Coding Fraction: 0.625    [ including projection effects ]

  Duration
     T90: 63.8159999251366 +/- 21.5559585471355
        Measured from: -0.755999982357025
                   to: 63.0599999427795     [s; relative to TRIGTIME]
     T50: 19.095999956131 +/- 8.08033788468745
        Measured from: 4.66000002622604
                   to: 23.755999982357     [s; relative to TRIGTIME]



  Fluence
     Peak Flux  (peak 1 second)
        Measured from: 3.22000002861023     
                   to: 4.22000002861023     [s; relative to TRIGTIME]
     Total Fluence        
        Measured from: -2.21200001239777     
                   to: 66.2239999771118     [s; relative to TRIGTIME]
     
             Band 1     Band 2     Band 3     Band 4
              15-25      25-50     50-100    100-350     keV
 Total     0.492077   0.472441   0.381378   0.085281
           0.055022   0.055659   0.048648   0.042845 [error]
 Peak      0.014026   0.031949   0.018047   0.016462
           0.006982   0.007115   0.006355   0.005415 [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 1.30e-07 2.22e-07 2.90e-07 7.69e-07 8.52e-07 1.41e-06   erg/cm2
              Error 2.50e-08 2.57e-08 4.95e-08 2.85e-07 1.15e-07 3.24e-07   erg/cm2
Peak flux Power-law 2.24e-01 2.05e-01 1.29e-01 1.25e-01 6.10e-01 6.83e-01   ph/cm2/s
              Error 1.02e-01 5.70e-02 5.49e-02 1.14e-01 1.67e-01 1.94e-01   ph/cm2/s
 
Fluence   Cutoff-PL 1.29e-07 2.22e-07 2.92e-07 7.72e-07 8.54e-07 1.42e-06   erg/cm2
              Error 2.50e-08 2.55e-08 4.90e-08 2.80e-07 1.12e-07 3.63e-07   erg/cm2
Peak flux Cutoff-PL 2.26e-01 2.05e-01 1.28e-01 1.21e-01 6.10e-01 6.80e-01   ph/cm2/s
              Error 1.03e-01 5.62e-02 5.47e-02 1.42e-01 1.67e-01 1.96e-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    1.614    0.221    -      -           1.33e-03 1.64e-04   69.190 57
CPL   1.626    0.223    9999.4    0.0      1.33e-03 1.02e-03   69.220 56
 
 
=== 1-s peak spectral analysis ===
 
Model Ph_index Ph_90err Epeak  Epeak_90err Norm     Nomr_90err chi2   dof
PL    1.661    0.576    -      -           4.65e-03 1.49e-03   67.170 57
CPL   2.194    0.000      72.8    0.0      2.32e-03 0.00e+00   66.140 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: 42.688000 sec.
T50 in the 50-300 keV band: 24.960000 sec.

 
=== Table of the duration information ==
 
        Value   tstart    tstop
T100   68.436   -2.212   66.224
T90    63.816   -0.756   63.060
T50    19.096    4.660   23.756
Peak    1.000    3.220    4.220

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
  289.2450   -17.1145   0.0174    24.5648  -106.0921         1.3105564     11.067 TRIG_00434360                 
 
Foreground time interval of the image:
 -2.212  66.224 (delta_t =  68.436 [sec])
Background time interval of the image:
-235.867  -2.212 (delta_t = 233.655 [sec])

Lightcurves

Notes:

1) The mask-weighted light curves are using the flight position.
2) Multiple plots of different time binning/intervals are shown to cover all scenarios of short/long GRBs, rate/image triggers, and real/false positives.
3) For all the mask-weighted lightcurves, the y-axis units are counts/sec/det where a det is 0.4 x 0.4 = 0.16 sq cm.
4) The verticle lines correspond to following: green dotted lines are T50 interval, black dotted lines are T90 interval, blue solid line(s) is a spacecraft slew start time, and orange solid line(s) is a spacecraft slew end time.
5) Time of each bin is in the middle of the bin.

1 s binning

From T0-310 s to T0+310 s

From T100_start - 20 s to T100_end + 30 s

Full time interval

64 ms binning

Full time interval

From T100_start to T100_end

From T0-5 sec to T0+5 sec

16 ms binning

From T100_start-5 s to T100_start+5 s

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

8 ms binning

From T100_start-3 s to T100_start+3 s

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

2 ms binning

From T100_start-1 s to T100_start+1 s

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

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

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

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

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   -2.212 sec. to   66.224 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.61438     ( -0.218264   0.223454 )
Norm@50keV  : 1.33349E-03    ( -0.000166006   0.000162573 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          69.19 using 59 PHA bins.
# Reduced chi-squared =          1.214 for     57 degrees of freedom 
# Null hypothesis probability =   1.290772e-01
 
Photon flux (15-150 keV)    in 68.44 sec: 0.172132 ( -0.019717  0.0197492 ) ph/cm2/s
Energy fluence (15-150 keV)             : 8.52051e-07 ( -1.14092e-07  1.15881e-07 ) ergs/cm2

Cutoff power-law model

Time interval is from   -2.212 sec. to   66.224 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.62612     ( -0.232881   0.212921 )
Epeak [keV] : 9999.36      ( -9999.36 -9999.36 )
Norm@50keV  : 1.32549E-03    ( -0.00133272   0.000703662 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          69.22 using 59 PHA bins.
# Reduced chi-squared =          1.236 for     56 degrees of freedom 
# Null hypothesis probability =   1.104083e-01
 
Photon flux (15-150 keV)    in 68.44 sec: 0.172471 ( -0.019951  0.019455 ) ph/cm2/s
Energy fluence (15-150 keV)             : 8.53885e-07 ( -1.15588e-07  1.08635e-07 ) ergs/cm2

Band function

Time interval is from   -2.212 sec. to   66.224 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -1.29404   ( 1.29427   1.29427 )
beta        : -1.61390    ( -0.920768   0.218285 )
Epeak [keV] : 25.6242      ( -25.6112 -25.6112 )
Norm@50keV   : 2.92681E-03    ( -0.00175535   4.66443 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          69.19 using 59 PHA bins.
# Reduced chi-squared =          1.258 for     55 degrees of freedom 
# Null hypothesis probability =   9.442130e-02
 
Photon flux (15-150 keV)    in 68.44 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]    : 13.3934  (-2.47198  3.19283)
R^2/D10^2   : 2.68269E-02  (-0.0139784   0.028922)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =         104.57 using 59 PHA bins.
# Reduced chi-squared =         1.8345 for     57 degrees of freedom 
# Null hypothesis probability =   1.252375e-04
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  6.979e-08   1.609e-08
25- 50  2.481e-07   4.692e-08
50-150  2.862e-07   7.850e-08
15-150  6.041e-07   9.996e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 199.165       (-94.9034      -199.165)
Norm        : 0.691168       (-0.0784815     0.0958262)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          71.70 using 59 PHA bins.
# Reduced chi-squared =          1.258 for     57 degrees of freedom 
# Null hypothesis probability =   9.101318e-02
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.178e-07   6.550e-08
25- 50  2.266e-07   1.228e-07
50-150  4.968e-07   2.697e-07
15-150  8.412e-07   4.596e-07

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 5.77535        (-1.4372      1.77611)
R1^2/D10^2  : 0.448338        (-0.286608      0.674041)
kT2 [keV]   : 30.5821        (-8.73032      22.2522)
R2^2/D10^2  : 1.35506E-03    (-0.00106217   0.00275517)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          67.76 using 59 PHA bins.
# Reduced chi-squared =          1.232 for     55 degrees of freedom 
# Null hypothesis probability =   1.159136e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.419e-07   6.484e-08
25- 50  2.011e-07   7.509e-08
50-150  5.557e-07   3.074e-07
15-150  8.987e-07   3.503e-07

Peak spectrum fit

Power-law model

Time interval is from    3.220 sec. to    4.220 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.66119     ( -0.556308   0.595394 )
Norm@50keV  : 4.65190E-03    ( -0.00154892   0.00142265 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          67.17 using 59 PHA bins.
# Reduced chi-squared =          1.178 for     57 degrees of freedom 
# Null hypothesis probability =   1.678871e-01
 
Photon flux (15-150 keV)    in 1 sec: 0.609686 ( -0.167266  0.16734 ) ph/cm2/s
Energy fluence (15-150 keV)             : 4.32147e-08 ( -1.44278e-08  1.51027e-08 ) ergs/cm2

Cutoff power-law model

Time interval is from    3.220 sec. to    4.220 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 2.19374     (     )
Epeak [keV] : 72.8264      (   )
Norm@50keV  : 2.31534E-03    (     )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          66.14 using 59 PHA bins.
# Reduced chi-squared =          1.181 for     56 degrees of freedom 
# Null hypothesis probability =   1.664983e-01
 
Photon flux (15-150 keV)    in 1 sec: 0.609853 ( -0.166733  0.166836 ) ph/cm2/s
Energy fluence (15-150 keV)             : 4.28192e-08 ( -1.404e-08  1.47173e-08 ) ergs/cm2

Band function

Time interval is from    3.220 sec. to    4.220 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -1.41735   ( 1.41736   1.41736 )
beta        : -1.66119    ( 1.66124   0.556298 )
Epeak [keV] : 9.53519      ( -9.53748 -9.53748 )
Norm@50keV   : 1.09963E-02    ( -0.0109966   0.139124 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          67.17 using 59 PHA bins.
# Reduced chi-squared =          1.221 for     55 degrees of freedom 
# Null hypothesis probability =   1.257489e-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]    : 9.93089  (-2.96183  4.85321)
R^2/D10^2   : 0.284268  (-0.283386   0.792253)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          72.34 using 59 PHA bins.
# Reduced chi-squared =          1.269 for     57 degrees of freedom 
# Null hypothesis probability =   8.281127e-02
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  5.696e-09   3.377e-09
25- 50  1.402e-08   8.545e-09
50-150  7.173e-09   5.495e-09
15-150  2.689e-08   1.621e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 174.979       (-176.146      -176.146)
Norm        : 2.45834       (-0.691019     1.3216)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          68.04 using 59 PHA bins.
# Reduced chi-squared =          1.194 for     57 degrees of freedom 
# Null hypothesis probability =   1.501644e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  6.219e-09   3.754e-09
25- 50  1.177e-08   6.895e-09
50-150  2.468e-08   1.519e-08
15-150  4.267e-08   2.555e-08

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 7.67682        (-2.25176      2.53533)
R1^2/D10^2  : 0.657519        (-0.488491      0.565901)
kT2 [keV]   : 198.127        (-198.453      -198.453)
R2^2/D10^2  : 1.09620E-04    (-5.59103e-05   0.00193482)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          63.39 using 59 PHA bins.
# Reduced chi-squared =          1.152 for     55 degrees of freedom 
# Null hypothesis probability =   2.046673e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  6.923e-09   4.346e-09
25- 50  1.222e-08   7.760e-09
50-150  3.131e-08   5.820e-09
15-150  5.046e-08   1.632e-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: 1.61438     ( -0.218264   0.223454 )
Norm@50keV  : 1.33349E-03    ( -0.000166006   0.000162573 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          69.19 using 59 PHA bins.
# Reduced chi-squared =          1.214 for     57 degrees of freedom 
# Null hypothesis probability =   1.290772e-01
 
Photon flux (15-150 keV)    in 68.44 sec: 0.172132 ( -0.019717  0.0197492 ) ph/cm2/s
Energy fluence (15-150 keV)             : 8.52051e-07 ( -1.14092e-07  1.15881e-07 ) ergs/cm2

Cutoff power-law model

Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.62612     ( -0.232881   0.212921 )
Epeak [keV] : 9999.36      ( -9999.36 -9999.36 )
Norm@50keV  : 1.32549E-03    ( -0.00133272   0.000703662 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          69.22 using 59 PHA bins.
# Reduced chi-squared =          1.236 for     56 degrees of freedom 
# Null hypothesis probability =   1.104083e-01
 
Photon flux (15-150 keV)    in 68.44 sec: 0.172471 ( -0.019951  0.019455 ) ph/cm2/s
Energy fluence (15-150 keV)             : 8.53885e-07 ( -1.15588e-07  1.08635e-07 ) ergs/cm2

Band function

 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -1.29404   ( 1.29427   1.29427 )
beta        : -1.61390    ( -0.920768   0.218285 )
Epeak [keV] : 25.6242      ( -25.6112 -25.6112 )
Norm@50keV   : 2.92681E-03    ( -0.00175535   4.66443 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          69.19 using 59 PHA bins.
# Reduced chi-squared =          1.258 for     55 degrees of freedom 
# Null hypothesis probability =   9.442130e-02
 
Photon flux (15-150 keV)    in 68.44 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)  = 2.22e-07
S(50-100 keV) = 2.90e-07

T90 vs. Hardness ratio plot

T90                                   = 63.8159999251366 sec.
Hardness ratio (energy fluence ratio) = 1.30631

Color vs. Color plot

Count Ratio  (25-50 keV) / (15-25 keV) = 0.960096
Count Ratio (50-100 keV) / (15-25 keV) = 0.775037

Mask shadow pattern

IMX = -1.266979308608149E-01, IMY = 4.391831519623013E-01

TIME vs. PHA plot around the trigger time

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

TIME vs. DetID plot around the trigger time

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

100 us light curve (15-350 keV)

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

Spacecraft aspect plot

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

Pre-burst image of 15-350 keV band

Time interval of the image:
-235.867400 -2.212000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
274.0272 -14.0136    4.3  37.7  -92.0   1.7341   2.7    1.9	GX 17+2                       
276.0136 -30.3329   19.8  41.5 -117.2   0.3574   0.6    5.0	H1820-303                     
285.2240 -25.0449    0.0  31.8 -116.8   0.2127   0.8   12.7	HT1900.1-2455                 
288.7660  10.9472    0.7  27.9  -40.0   3.4055  16.6    1.9	GRS 1915+105                  
299.5792  35.2159    1.1  42.3   -0.7   3.4038  10.9    1.0	Cyg X-1                       
308.1339  40.9763    2.4  46.6   10.4   1.8993   4.8    1.8	Cyg X-3                       
326.2122  38.3019    6.8  46.0   30.0  -0.8405  -1.7    2.2	Cyg X-2                       
336.5629 -12.4908    2.8  25.8  121.1   1.0725   4.2 ------	UNKNOWN                       
324.4043  -8.7494    2.6  13.3  118.4   0.8089   4.5 ------	UNKNOWN                       
290.9330 -14.5350    2.2  22.0 -101.8   1.0128   5.3 ------	UNKNOWN                       
284.3918 -58.4227    3.1  56.8 -149.7   4.6069   3.8 ------	UNKNOWN                       
279.6944 -52.0846    2.7  53.4 -142.5   4.7737   4.3 ------	UNKNOWN                       
267.8220  12.6174    2.6  47.0  -53.2   3.5916   4.4 ------	UNKNOWN

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

Time interval of the image:
-2.212000 66.224000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
273.9195 -14.1654    9.3  37.9  -92.2  -0.3408  -1.2    9.2	GX 17+2                       
275.8492 -30.4828    6.1  41.7 -117.3   0.5206   1.9    8.0	H1820-303                     
285.0344 -24.9185  284.8  31.8 -116.4   0.0059   0.0    0.1	HT1900.1-2455                 
288.9059  11.1312    0.0  27.9  -39.5   0.2790   2.6   12.8	GRS 1915+105                  
299.4669  35.3274    5.3  42.4   -0.7  -0.3202  -2.2    9.7	Cyg X-1                       
308.2100  41.0543   15.5  46.7   10.4   0.1643   0.7    7.6	Cyg X-3                       
326.1773  38.2934   22.6  46.0   29.9   0.1293   0.5    1.7	Cyg X-2                       
289.2450 -17.1145    1.0  24.6 -106.1   1.3100  11.0 ------	UNKNOWN

Post-slew image of 15-350 keV band

Time interval of the image:
406.132600 962.118400
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
326.1441  38.3176    3.1  53.9  170.9   4.7857   3.7    1.3	Cyg X-2                       
  5.3317  10.4421    2.2  24.3  112.4   1.8464   5.2 ------	UNKNOWN                       
335.1627  42.4695    2.9  47.3  176.7   2.5543   3.9 ------	UNKNOWN                       
 47.7265  -0.5283    3.1  30.6    5.8   1.2874   3.7 ------	UNKNOWN                       
  1.6085  65.9790    2.9  46.3 -145.0   2.8900   4.0 ------	UNKNOWN                       
 78.7970  24.0798    5.7  47.0  -53.3   3.2475   2.1 ------	UNKNOWN                       
 70.9249  42.3792    2.7  41.1  -80.0   6.1181   4.3 ------	UNKNOWN                       
 30.6569  70.8547    2.7  48.2 -129.4   6.1898   4.3 ------	UNKNOWN

Plot creation:
Sat May 30 23:50:01 EDT 2015