batgrbproduct analysis for trigger=294120

batgrbproduct Analysis for Trigger=294120

Analysis Summary

Notes:

1) No attempt has been made to eliminate the non-significant decimal places.
2) This batgrbproduct analysis is done using the HEASARC data.
3) This batgrbproduct analysis is using the flight position for the mask-weighting calculation.

======================================================================
                  BAT GRB EVENT DATA PROCESSING REPORT
    Process Script Ver: batgrbproduct v2.46
    Process Start Time (local time): Mon Sep 15 19:50:19 EDT 2014
             Host Name: batevent1
   Current Working Dir: /local/data/batevent/batevent_reproc/trigger294120
======================================================================

  Trigger: 00294120      Segment: 000

  BAT Trigger Time: 213970161.344   [s; MET]
      Trigger Stop: 213970177.728   [s; MET]
               UTC: 2007-10-13T12:09:19.055540    [includes UTCF correction] 
       Where From?: TDRSS position message

  BAT 
    RA: 279.524890921608   Dec: 33.8574571315757  [deg; J2000]

     Catalogged Source?: NO
     Point Source?:      YES
     GRB Indicated?:     YES    [ by BAT flight software ]
     Image S/N Ratio:    7.84
     Image Trigger?:     NO
     Rate S/N Ratio:     10.9087121146357  [ if not an image trigger ]
     Image S/N Ratio:    7.84

  Flight Position:   [ source = BAT ]
    RA: 279.524890921608   Dec: 33.8574571315757  [deg; J2000]

  Ground Position:   [ source = BAT pre-slew burst ]
    RA: 279.525   Dec: 33.8575  [deg; J2000]
        { 18h 38m 06.0s , +33d 51' 27.0" }
        +/- 2.66158841925 [arcmin] (estimated 90% radius based on SNR)
    SNR: 7.51330565953
 
 
  Angular difference between Flight and Ground position is 0.006013 arcmin
 
  Partial Coding Fraction: 0.703125    [ including projection effects ]

  Duration
     T90: 75.5840000212193 +/- 25.7891412844253
        Measured from: 4.11199998855591
                   to: 79.6960000097752     [s; relative to TRIGTIME]
     T50: 49.216000020504 +/- 35.7333842698928
        Measured from: 9.16799998283386
                   to: 58.3840000033379     [s; relative to TRIGTIME]



  Fluence
     Peak Flux  (peak 1 second)
        Measured from: 3.64399999380112     
                   to: 4.64399999380112     [s; relative to TRIGTIME]
     Total Fluence        
        Measured from: 3.59999999403954     
                   to: 81.5519999861717     [s; relative to TRIGTIME]
     
             Band 1     Band 2     Band 3     Band 4
              15-25      25-50     50-100    100-350     keV
 Total     0.232546   0.211041   0.098366   0.135400
           0.053378   0.054153   0.046876   0.040838 [error]
 Peak      0.019051   0.012944   0.007794   0.008489
           0.006024   0.006091   0.005293   0.004623 [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 5.96e-08 1.03e-07 1.35e-07 3.60e-07 3.95e-07 6.57e-07   erg/cm2
              Error 2.53e-08 2.57e-08 5.00e-08 3.08e-07 1.15e-07 3.44e-07   erg/cm2
Peak flux Power-law 1.55e-01 1.21e-01 6.38e-02 4.87e-02 3.62e-01 3.88e-01   ph/cm2/s
              Error 1.28e-01 5.15e-02 5.70e-02 9.24e-02 1.49e-01 1.66e-01   ph/cm2/s
 
Fluence   Cutoff-PL 6.08e-08 1.03e-07 1.33e-07 3.41e-07 3.91e-07 6.37e-07   erg/cm2
              Error 1.92e-08 2.56e-08 5.01e-08 3.75e-07 1.15e-07 3.64e-07   erg/cm2
Peak flux Cutoff-PL 1.65e-01 1.20e-01 5.72e-02 3.88e-02 3.61e-01 3.80e-01   ph/cm2/s
              Error 1.29e-01 5.20e-02 5.05e-02 9.28e-02 1.49e-01 1.67e-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    1.607    0.509    -      -           5.42e-04 1.46e-04   45.280 57
CPL   2.289    0.000     104.7    0.0      2.29e-04 0.00e+00   43.810 56
 
 
=== 1-s peak spectral analysis ===
 
Model Ph_index Ph_90err Epeak  Epeak_90err Norm     Nomr_90err chi2   dof
PL    1.924    1.083    -      -           2.50e-03 1.91e-03   54.900 57
CPL   3.300    0.000     360.1    0.0      5.37e-04 0.00e+00   54.010 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: 0.000000 sec.
T50 in the 50-300 keV band: 0.000000 sec.

 
=== Table of the duration information ==
 
        Value   tstart    tstop
T100   77.952    3.600   81.552
T90    75.584    4.112   79.696
T50    49.216    9.168   58.384
Peak    1.000    3.644    4.644

Click here for the BAT GCN circular template

Special notes of this burst

Image

Pre-slew 15.0-50.0 keV image (Event data)

#RAcent DECcent POSerr Theta  Phi  Peak_Cts  SNR Name
279.525 33.858 0.000 30.683 -35.567 0.277 7.513 TRIG_00294120
 
Image time interval: 0.000 to 16.384 [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 16.384000

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 16.384000

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 16.384000

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    3.600 sec. to   81.552 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.60675     ( -0.500654   0.516572 )
Norm@50keV  : 5.42055E-04    ( -0.000150132   0.000141117 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          45.28 using 59 PHA bins.
# Reduced chi-squared =         0.7943 for     57 degrees of freedom 
# Null hypothesis probability =   8.686642e-01
 
Photon flux (15-150 keV)    in 77.95 sec: 6.98030E-02 ( -0.0172344  0.0172519 ) ph/cm2/s
Energy fluence (15-150 keV)             : 3.94835e-07 ( -1.13694e-07  1.171e-07 ) ergs/cm2

Cutoff power-law model

Time interval is from    3.600 sec. to   81.552 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 2.28870     (     )
Epeak [keV] : 104.674      (   )
Norm@50keV  : 2.29241E-04    (     )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          43.81 using 59 PHA bins.
# Reduced chi-squared =         0.7823 for     56 degrees of freedom 
# Null hypothesis probability =   8.817694e-01
 
Photon flux (15-150 keV)    in 77.95 sec: 6.99008E-02 ( -0.0170019  0.0171348 ) ph/cm2/s
Energy fluence (15-150 keV)             : 3.91173e-07 ( -1.10052e-07  1.2094e-07 ) ergs/cm2

Band function

Time interval is from    3.600 sec. to   81.552 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -1.28552   ( 1.2864   1.2864 )
beta        : -1.60673    ( 1.60685   0.500634 )
Epeak [keV] : 26.4335      ( -26.0802 -26.0802 )
Norm@50keV   : 1.18572E-03    ( -0.00118719   0.0205921 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          45.28 using 59 PHA bins.
# Reduced chi-squared =         0.8232 for     55 degrees of freedom 
# Null hypothesis probability =   8.221121e-01
 
Photon flux (15-150 keV)    in 77.95 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]    : 10.8663  (-3.2663  6.11397)
R^2/D10^2   : 2.29439E-02  (-0.018319   0.0643206)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          54.09 using 59 PHA bins.
# Reduced chi-squared =         0.9489 for     57 degrees of freedom 
# Null hypothesis probability =   5.849806e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  4.401e-08   2.731e-08
25- 50  1.225e-07   7.129e-08
50-150  8.093e-08   5.874e-08
15-150  2.474e-07   1.516e-07

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 199.363       (-199.363      -199.363)
Norm        : 0.279310       (-0.068612     0.102572)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          46.34 using 59 PHA bins.
# Reduced chi-squared =         0.8130 for     57 degrees of freedom 
# Null hypothesis probability =   8.425291e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  5.422e-08   3.253e-08
25- 50  1.043e-07   6.236e-08
50-150  2.287e-07   1.354e-07
15-150  3.872e-07   2.343e-07

Double BB

------------------------------------------------------------
#Fit statistic : Chi-Squared =          42.42 using 59 PHA bins.
#Fit statistic : Chi-Squared =          42.33 using 59 PHA bins.
#Fit statistic : Chi-Squared =          42.30 using 59 PHA bins.
#Fit statistic : Chi-Squared =          42.28 using 59 PHA bins.
# Reduced chi-squared =         0.7713 for     55 degrees of freedom 
# Reduced chi-squared =         0.7697 for     55 degrees of freedom 
# Reduced chi-squared =         0.7691 for     55 degrees of freedom 
# Reduced chi-squared =         0.7688 for     55 degrees of freedom 
# Null hypothesis probability =   8.925246e-01
# Null hypothesis probability =   8.944702e-01
# Null hypothesis probability =   8.951034e-01
# Null hypothesis probability =   8.954230e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  6.135e-08   3.657e-08
25- 50  1.020e-07   5.901e-08
50-150  2.931e-07   1.631e-07
15-150  4.564e-07   2.192e-07

Peak spectrum fit

Power-law model

Time interval is from    3.644 sec. to    4.644 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.92433     ( -0.990105   1.1767 )
Norm@50keV  : 2.49549E-03    ( -0.00249375   0.00131916 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          54.90 using 59 PHA bins.
# Reduced chi-squared =         0.9632 for     57 degrees of freedom 
# Null hypothesis probability =   5.541346e-01
 
Photon flux (15-150 keV)    in 1 sec: 0.361891 ( -0.149365  0.149374 ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.29347e-08 ( -2.2934e-08  1.32922e-08 ) ergs/cm2

Cutoff power-law model

Time interval is from    3.644 sec. to    4.644 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 3.30027     (     )
Epeak [keV] : 360.103      (   )
Norm@50keV  : 5.37392E-04    (     )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          54.01 using 59 PHA bins.
# Reduced chi-squared =         0.9645 for     56 degrees of freedom 
# Null hypothesis probability =   5.505371e-01
 
Photon flux (15-150 keV)    in 1 sec: 0.361034 ( -0.14924  0.149468 ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.225e-08 ( -1.13367e-08  1.39992e-08 ) ergs/cm2

Band function

Time interval is from    3.644 sec. to    4.644 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : 4.99493   ( -4.99493   -4.99493 )
beta        : -2.03332    ( -5.19188   1.06584 )
Epeak [keV] : 19.6625      ( -19.6625 71.3653 )
Norm@50keV   : 1889.48    ( -776.345   8.71987e+06 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          54.77 using 59 PHA bins.
# Reduced chi-squared =         0.9958 for     55 degrees of freedom 
# Null hypothesis probability =   4.834862e-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]    : 5.81007  (-2.23807  5.48884)
R^2/D10^2   : 1.37039  (-1.37008   10.9082)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          57.49 using 59 PHA bins.
# Reduced chi-squared =          1.009 for     57 degrees of freedom 
# Null hypothesis probability =   4.567788e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  5.860e-09   3.792e-09
25- 50  5.445e-09   3.803e-09
50-150  4.362e-10   4.030e-10
15-150  1.174e-08   7.865e-09

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 99.9709       (-99.9913      -99.9913)
Norm        : 1.54605       (-0.740543     5.21121)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          55.92 using 59 PHA bins.
# Reduced chi-squared =         0.9810 for     57 degrees of freedom 
# Null hypothesis probability =   5.157548e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  4.041e-09   2.685e-09
25- 50  6.987e-09   4.567e-09
50-150  1.132e-08   9.200e-09
15-150  2.235e-08   1.566e-08

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 5.19154        (-2.03817      3.07069)
R1^2/D10^2  : 2.08648        (-1.83538      19.4251)
kT2 [keV]   : 198.276        (-198.25      -198.25)
R2^2/D10^2  : 7.13224E-05    (-4.72909e-05   0.00734963)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          51.50 using 59 PHA bins.
# Reduced chi-squared =         0.9364 for     55 degrees of freedom 
# Null hypothesis probability =   6.091021e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  5.975e-09   3.775e-09
25- 50  4.982e-09   2.852e-09
50-150  1.895e-08   2.454e-09
15-150  2.991e-08   8.940e-09

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: 1.60675     ( -0.500654   0.516572 )
Norm@50keV  : 5.42055E-04    ( -0.000150132   0.000141117 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          45.28 using 59 PHA bins.
# Reduced chi-squared =         0.7943 for     57 degrees of freedom 
# Null hypothesis probability =   8.686642e-01
 
Photon flux (15-150 keV)    in 77.95 sec: 6.98030E-02 ( -0.0172344  0.0172519 ) ph/cm2/s
Energy fluence (15-150 keV)             : 3.94835e-07 ( -1.13694e-07  1.171e-07 ) ergs/cm2

Cutoff power-law model

Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 2.92805     ( -1.63489   0.269239 )
Epeak [keV] : 277.485      (   )
Norm@50keV  : 1.20707E-04    (     )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          43.42 using 59 PHA bins.
# Reduced chi-squared =         0.7754 for     56 degrees of freedom 
# Null hypothesis probability =   8.901156e-01
 
Photon flux (15-150 keV)    in 77.95 sec: 6.99008E-02 ( -0.0170019  0.0171348 ) ph/cm2/s
Energy fluence (15-150 keV)             : 3.91173e-07 ( -1.10052e-07  1.2094e-07 ) ergs/cm2

Band function

 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -1.28552   ( 1.2864   1.2864 )
beta        : -1.60673    ( 1.60685   0.500634 )
Epeak [keV] : 26.4335      ( -26.0802 -26.0802 )
Norm@50keV   : 1.18572E-03    ( -0.00118719   0.0232208 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          45.28 using 59 PHA bins.
# Reduced chi-squared =         0.8232 for     55 degrees of freedom 
# Null hypothesis probability =   8.221121e-01
 
Photon flux (15-150 keV)    in 77.95 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)  = 1.03e-07
S(50-100 keV) = 1.35e-07

T90 vs. Hardness ratio plot

T90                                   = 75.5840000212193 sec.
Hardness ratio (energy fluence ratio) = 1.31068

Color vs. Color plot

Count Ratio  (25-50 keV) / (15-25 keV) = 0.907524
Count Ratio (50-100 keV) / (15-25 keV) = 0.422996

Mask shadow pattern

IMX = 0.482663359722, IMY = 0.345128921831

TIME vs. PHA plot around the trigger time

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 16.384000

TIME vs. DetID plot around the trigger time

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 16.384000

100 us light curve (15-350 keV)

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 16.384000

Spacecraft aspect plot

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

Pre-burst image of 15-350 keV band

Time interval of the image:
-239.344000 -96.030100
-95.344000 3.600000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
268.4657  -1.3245    6.5  35.3 -105.7   0.7148   1.8    9.7	SW J1753.5-0127               
270.4310 -25.1110   43.0  47.2 -137.6  -0.1607  -0.3    8.2	GX 5-1                        
270.4299 -25.6691   10.6  47.6 -138.1  -0.6837  -1.1    8.2	GRS 1758-258                  
273.9092 -14.0722    6.1  37.2 -129.0   0.6223   1.9    6.0	GX 17+2                       
276.0511 -30.3061    9.0  48.1 -147.3  -0.5879  -1.3    7.5	H1820-303                     
285.0240 -24.9182    6.3  39.4 -153.2   0.5611   1.8    0.7	HT1900.1-2455                 
288.7747  10.9527    0.8  12.8  -86.0   2.6277  14.6    1.5	GRS 1915+105                  
299.5914  35.2070    0.3  24.4   -1.9   8.7636  45.4    0.3	Cyg X-1                       
308.1467  40.9538    1.3  30.6   12.0   1.7861   8.7    1.7	Cyg X-3                       
326.2398  38.3951    3.1  35.1   36.8   1.0844   3.8    5.4	Cyg X-2                       
308.0571  37.6600    1.2  27.4   13.3   1.9402   9.8 ------	UNKNOWN                       
293.4093 -47.2584    2.8  58.6 -170.9   4.6168   4.1 ------	UNKNOWN                       
284.2330  34.1155    2.6  28.2  -29.4   0.8684   4.5 ------	UNKNOWN                       
265.4020 -22.1502    2.1  48.6 -130.5   4.4814   5.6 ------	UNKNOWN

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

Time interval of the image:
3.600000 81.552000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
268.4966  -1.3234    9.0  35.3 -105.7  -0.2358  -1.3   10.9	SW J1753.5-0127               
270.4323 -25.1182   10.6  47.2 -137.6   0.2966   1.1    8.4	GX 5-1                        
270.4413 -25.7319   13.2  47.7 -138.2   0.2377   0.9    7.5	GRS 1758-258                  
274.0057 -14.0377  926.5  37.2 -129.0  -0.0020  -0.0    0.1	GX 17+2                       
275.7784 -30.3160    4.8  48.2 -147.0   0.5831   2.4    8.2	H1820-303                     
285.1127 -24.9051    8.7  39.3 -153.3  -0.1883  -1.3    4.3	HT1900.1-2455                 
288.7048  11.0025    2.8  12.8  -85.8  -0.3979  -4.1    6.5	GRS 1915+105                  
299.4199  35.2446    5.5  24.4   -2.2   0.2067   2.1    8.7	Cyg X-1                       
307.9645  41.0738    3.5  30.7   11.6   0.3573   3.3    9.8	Cyg X-3                       
326.0389  38.2319    6.6  34.9   36.8   0.2741   1.7    8.3	Cyg X-2                       
322.6710  52.4923    2.0  44.9   20.4   1.2244   5.7 ------	UNKNOWN                       
311.6680 -28.4887    2.4  40.5  169.1   0.7401   4.9 ------	UNKNOWN                       
311.0242 -21.7267    2.9  33.9  166.9   0.5059   3.9 ------	UNKNOWN                       
294.2004  67.6614    2.5  57.0   -0.9   2.5605   4.6 ------	UNKNOWN                       
279.4873  33.8050    1.8  30.7  -35.7   0.6973   6.3 ------	UNKNOWN

Post-slew image of 15-350 keV band

Time interval of the image:
791.556610 962.664100
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
326.2040  38.4322   54.3  35.5  -89.7   0.0652   0.2    6.8	Cyg X-2                       
 37.0729  11.6921    2.3  35.2   59.9   1.3140   5.0 ------	UNKNOWN                       
319.6173 -15.2878    2.5  54.3 -166.1   1.8712   4.6 ------	UNKNOWN

Plot creation:
Thu Oct  8 20:36:10 EDT 2015