batgrbproduct analysis for trigger=650617

batgrbproduct Analysis for Trigger=650617

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): Sun Aug 30 18:14:51 EDT 2015
             Host Name: bat1
   Current Working Dir: /local/data/bat1/alien/Swift_3rdBATcatalog/event/batevent_reproc/trigger650617
======================================================================

  Trigger: 00650617      Segment: 000

  BAT Trigger Time: 459780685.952   [s; MET]
      Trigger Stop: 459780686.976   [s; MET]
               UTC: 2015-07-28T12:51:11.036780    [includes UTCF correction] 
       Where From?: TDRSS position message

  BAT 
    RA: 292.287805747232   Dec: 33.9039039617548  [deg; J2000]

     Catalogged Source?: NO
     Point Source?:      YES
     GRB Indicated?:     YES    [ by BAT flight software ]
     Image S/N Ratio:    6.74
     Image Trigger?:     NO
     Rate S/N Ratio:     7.93725393319377  [ if not an image trigger ]
     Image S/N Ratio:    6.74

  Flight Position:   [ source = BAT ]
    RA: 292.287805747232   Dec: 33.9039039617548  [deg; J2000]

  Ground Position:   [ source = BAT pre-slew burst ]
    RA: 292.271249895788   Dec: 33.9058805610823  [deg; J2000]  
        { 19h 29m 05.1s , +33d 54' 21.2" }
         +/- 2.59616397126304 [arcmin] (estimated 90% radius based on SNR)
         +/- 1.14634336460646 [arcmin] (formal 1-sigma fit error)
    SNR: 7.78422451294506
 
  Angular difference between Flight and Ground position is 0.832933 arcmin
 
  Partial Coding Fraction: 1.015625    [ including projection effects ]

  Duration
     T90: 0.832000017166138 +/- 0.230755269859374
        Measured from: 0.303999960422516
                   to: 1.13599997758865     [s; relative to TRIGTIME]
     T50: 0.448000013828278 +/- 0.181019365655138
        Measured from: 0.431999981403351
                   to: 0.879999995231628     [s; relative to TRIGTIME]



  Fluence
     Peak Flux  (peak 1 second)
        Measured from: 0.219999969005585     
                   to: 1.21999996900558     [s; relative to TRIGTIME]
     Total Fluence        
        Measured from: 0.239999949932098     
                   to: 1.19999998807907     [s; relative to TRIGTIME]
     
             Band 1     Band 2     Band 3     Band 4
              15-25      25-50     50-100    100-350     keV
 Total     0.025261   0.022351   0.015465   0.007699
           0.005317   0.005404   0.004486   0.003591 [error]
 Peak      0.026412   0.020252   0.017060   0.007577
           0.005417   0.005507   0.004585   0.003664 [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 7.35e-09 9.87e-09 9.75e-09 1.73e-08 3.26e-08 4.43e-08   erg/cm2
              Error 2.30e-09 2.32e-09 4.28e-09 1.55e-08 9.67e-09 2.03e-08   erg/cm2
Peak flux Power-law 2.37e-01 1.81e-01 9.31e-02 6.88e-02 5.43e-01 5.80e-01   ph/cm2/s
              Error 7.83e-02 4.15e-02 3.87e-02 5.64e-02 1.23e-01 1.36e-01   ph/cm2/s
 
Fluence   Cutoff-PL 7.38e-09 9.87e-09 9.69e-09 1.69e-08 3.25e-08 4.39e-08   erg/cm2
              Error 2.27e-09 2.39e-09 4.29e-09 1.84e-08 9.57e-09 2.00e-08   erg/cm2
Peak flux Cutoff-PL 2.38e-01 1.81e-01 9.24e-02 6.72e-02 5.43e-01 5.79e-01   ph/cm2/s
              Error 7.76e-02 3.15e-02 3.87e-02 6.92e-02 1.23e-01 1.36e-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    2.018    0.481    -      -           3.68e-03 1.17e-03   54.460 57
CPL   2.399    0.803     147.4    0.0      2.33e-03 0.00e+00   54.070 56
 
 
=== 1-s peak spectral analysis ===
 
Model Ph_index Ph_90err Epeak  Epeak_90err Norm     Nomr_90err chi2   dof
PL    1.962    0.485    -      -           3.68e-03 1.14e-03   58.130 57
CPL   1.955    0.565    9999.1    0.0      3.69e-03 0.00e+00   58.140 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: 0.000000 sec.
T50 in the 50-300 keV band: 0.000000 sec.

 
=== Table of the duration information ==
 
        Value   tstart    tstop
T100    0.960    0.240    1.200
T90     0.832    0.304    1.136
T50     0.448    0.432    0.880
Peak    1.000    0.220    1.220

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
  292.2712    33.9059   0.0248    11.3888  -173.9397         0.0753820      7.784 TRIG_00650617                 
 
Foreground time interval of the image:
  0.240   1.200 (delta_t =   0.960 [sec])
Background time interval of the image:
-239.952   0.240 (delta_t = 240.192 [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 1.024000

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 1.024000

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 1.024000

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    0.240 sec. to    1.200 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 2.01826     ( -0.445039   0.517055 )
Norm@50keV  : 3.68008E-03    ( -0.00121558   0.00112565 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          54.46 using 59 PHA bins.
# Reduced chi-squared =         0.9554 for     57 degrees of freedom 
# Null hypothesis probability =   5.709601e-01
 
Photon flux (15-150 keV)    in 0.96 sec: 0.556700 ( -0.125593  0.125596 ) ph/cm2/s
Energy fluence (15-150 keV)             : 3.26132e-08 ( -9.42129e-09  9.92352e-09 ) ergs/cm2

Cutoff power-law model

Time interval is from    0.240 sec. to    1.200 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 2.39905     ( -1.43163   0.17423 )
Epeak [keV] : 147.394      (   )
Norm@50keV  : 2.33391E-03    (     )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          54.07 using 59 PHA bins.
# Reduced chi-squared =         0.9655 for     56 degrees of freedom 
# Null hypothesis probability =   5.483001e-01
 
Photon flux (15-150 keV)    in 0.96 sec: 0.556489 ( -0.125521  0.125512 ) ph/cm2/s
Energy fluence (15-150 keV)             : 3.25192e-08 ( -9.44957e-09  9.69821e-09 ) ergs/cm2

Band function

Time interval is from    0.240 sec. to    1.200 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : 4.98492   ( -4.98492   -4.98492 )
beta        : -2.06150    ( -0.686443   0.470125 )
Epeak [keV] : 18.2273      ( -18.2273 71.8904 )
Norm@50keV   : 4851.13    ( -1092.48   7.78597e+06 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          54.31 using 59 PHA bins.
# Reduced chi-squared =         0.9874 for     55 degrees of freedom 
# Null hypothesis probability =   5.010653e-01
 
Photon flux (15-150 keV)    in 0.96 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]    : 8.64549  (-2.99332  4.23152)
R^2/D10^2   : 0.430129  (-0.327201   1.83965)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          63.61 using 59 PHA bins.
# Reduced chi-squared =          1.116 for     57 degrees of freedom 
# Null hypothesis probability =   2.550859e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  5.877e-09   3.438e-09
25- 50  1.172e-08   5.745e-09
50-150  3.947e-09   2.756e-09
15-150  2.154e-08   1.312e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 66.9150       (-36.4574      -66.9492)
Norm        : 2.76068       (-0.894733     1.60493)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          55.92 using 59 PHA bins.
# Reduced chi-squared =         0.9810 for     57 degrees of freedom 
# Null hypothesis probability =   5.157405e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  6.765e-09   2.622e-09
25- 50  1.063e-08   4.696e-09
50-150  1.320e-08   9.946e-09
15-150  3.059e-08   1.645e-08

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 4.35472        (-1.76669      2.90564)
R1^2/D10^2  : 5.46046        (-4.6815      66.007)
kT2 [keV]   : 21.0382        (-9.29108      -21.0393)
R2^2/D10^2  : 1.20186E-02    (-0.0119698   0.0857681)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          54.08 using 59 PHA bins.
# Reduced chi-squared =         0.9833 for     55 degrees of freedom 
# Null hypothesis probability =   5.096159e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  8.054e-09   4.540e-09
25- 50  8.202e-09   4.342e-09
50-150  1.643e-08   1.116e-08
15-150  3.269e-08   1.735e-08

Peak spectrum fit

Power-law model

Time interval is from    0.220 sec. to    1.220 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.96165     ( -0.449209   0.52015 )
Norm@50keV  : 3.68241E-03    ( -0.00119289   0.0010936 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          58.13 using 59 PHA bins.
# Reduced chi-squared =          1.020 for     57 degrees of freedom 
# Null hypothesis probability =   4.333085e-01
 
Photon flux (15-150 keV)    in 1 sec: 0.542846 ( -0.122912  0.122911 ) ph/cm2/s
Energy fluence (15-150 keV)             : 3.39009e-08 ( -9.81423e-09  1.02668e-08 ) ergs/cm2

Cutoff power-law model

Time interval is from    0.220 sec. to    1.220 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.95468     ( -0.600287   0.52901 )
Epeak [keV] : 9999.09      (   )
Norm@50keV  : 3.69481E-03    (     )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          58.14 using 59 PHA bins.
# Reduced chi-squared =          1.038 for     56 degrees of freedom 
# Null hypothesis probability =   3.966102e-01
 
Photon flux (15-150 keV)    in 1 sec: 0.542615 ( -0.122872  0.122873 ) ph/cm2/s
Energy fluence (15-150 keV)             : 3.37654e-08 ( -9.6699e-09  1.01945e-08 ) ergs/cm2

Band function

Time interval is from    0.220 sec. to    1.220 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : 4.99490   ( -4.9949   -4.9949 )
beta        : -1.99311    ( -0.599365   0.468716 )
Epeak [keV] : 17.6798      ( -17.6798 7.19237 )
Norm@50keV   : 5722.82    ( -1294.57   7.1606e+06 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          58.04 using 59 PHA bins.
# Reduced chi-squared =          1.055 for     55 degrees of freedom 
# Null hypothesis probability =   3.640161e-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]    : 9.82970  (-4.22486  5.44585)
R^2/D10^2   : 0.253552  (-0.196311   1.93996)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          68.99 using 59 PHA bins.
# Reduced chi-squared =          1.210 for     57 degrees of freedom 
# Null hypothesis probability =   1.325505e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  4.959e-09   2.778e-09
25- 50  1.203e-08   6.222e-09
50-150  5.974e-09   3.803e-09
15-150  2.297e-08   1.270e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 79.8853       (-45.4332      -79.9546)
Norm        : 2.51994       (-0.747934     1.37093)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          59.73 using 59 PHA bins.
# Reduced chi-squared =          1.048 for     57 degrees of freedom 
# Null hypothesis probability =   3.767711e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  6.538e-09   3.205e-09
25- 50  1.076e-08   4.026e-09
50-150  1.517e-08   1.229e-08
15-150  3.247e-08   1.994e-08

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 4.02220        (-1.45218      2.03178)
R1^2/D10^2  : 7.57406        (-6.36249      70.3781)
kT2 [keV]   : 21.2194        (-8.1196      31.5797)
R2^2/D10^2  : 1.23456E-02    (-0.0115346   0.0583413)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          56.74 using 59 PHA bins.
# Reduced chi-squared =          1.032 for     55 degrees of freedom 
# Null hypothesis probability =   4.101302e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  8.121e-09   4.576e-09
25- 50  8.004e-09   4.316e-09
50-150  1.820e-08   1.147e-08
15-150  3.432e-08   1.847e-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: 2.01826     ( -0.445039   0.517055 )
Norm@50keV  : 3.68008E-03    ( -0.00121558   0.00112565 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          54.46 using 59 PHA bins.
# Reduced chi-squared =         0.9554 for     57 degrees of freedom 
# Null hypothesis probability =   5.709601e-01
 
Photon flux (15-150 keV)    in 0.96 sec: 0.556700 ( -0.125593  0.125596 ) ph/cm2/s
Energy fluence (15-150 keV)             : 3.26132e-08 ( -9.42129e-09  9.92352e-09 ) ergs/cm2

Cutoff power-law model

Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 2.39905     ( -1.43163   0.174232 )
Epeak [keV] : 147.394      (   )
Norm@50keV  : 2.33391E-03    (     )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          54.07 using 59 PHA bins.
# Reduced chi-squared =         0.9655 for     56 degrees of freedom 
# Null hypothesis probability =   5.483001e-01
 
Photon flux (15-150 keV)    in 0.96 sec: 0.556489 ( -0.125521  0.125512 ) ph/cm2/s
Energy fluence (15-150 keV)             : 3.25192e-08 ( -9.44957e-09  9.69821e-09 ) ergs/cm2

Band function

 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : 4.98492   ( -4.98492   -4.98492 )
beta        : -2.06150    ( -0.686443   0.470125 )
Epeak [keV] : 18.2273      ( -18.2273 95.3662 )
Norm@50keV   : 4851.13    ( -1092.48   7.78597e+06 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          54.31 using 59 PHA bins.
# Reduced chi-squared =         0.9874 for     55 degrees of freedom 
# Null hypothesis probability =   5.010653e-01
 
Photon flux (15-150 keV)    in 0.96 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)  = 9.87e-09
S(50-100 keV) = 9.75e-09

T90 vs. Hardness ratio plot

T90                                   = 0.832000017166138 sec.
Hardness ratio (energy fluence ratio) = 0.987842

Color vs. Color plot

Count Ratio  (25-50 keV) / (15-25 keV) = 0.884803
Count Ratio (50-100 keV) / (15-25 keV) = 0.612209

Mask shadow pattern

IMX = -2.003064599409896E-01, IMY = 2.126625601115743E-02

TIME vs. PHA plot around the trigger time

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.024000

TIME vs. DetID plot around the trigger time

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.024000

100 us light curve (15-350 keV)

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.024000

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:
-239.952000 0.240000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
254.3794  35.3516    7.3  42.0 -160.8   0.4858   1.6    3.9	Her X-1                       
268.5665  -1.5668    0.0  49.9  144.5   0.7346   0.7   13.7	SW J1753.5-0127               
288.9254  11.0331   10.6  27.6  130.3   0.2533   1.1    9.1	GRS 1915+105                  
299.5951  35.1990    0.4   5.4 -161.9   5.0082  26.0    0.3	Cyg X-1                       
308.1174  40.9593    0.8   7.3  -75.4   2.3934  14.0    0.5	Cyg X-3                       
326.1711  38.3207   22.4  16.9  -19.3   0.0976   0.5    0.1	Cyg X-2                       
350.9669  20.4716    2.7  41.8    8.7   1.2571   4.2 ------	UNKNOWN                       
286.7703  25.5346    2.9  18.6  160.5   0.7340   4.0 ------	UNKNOWN                       
 13.0748  50.9553    2.7  50.5  -39.3   3.4248   4.2 ------	UNKNOWN

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

Time interval of the image:
0.240000 1.200000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
254.3808  35.2409    4.1  42.1 -161.0  -0.0438  -2.8    7.2	Her X-1                       
268.4225  -1.4427   35.9  49.9  144.8  -0.0181  -0.3    3.3	SW J1753.5-0127               
288.7835  10.8360    4.7  27.9  130.3  -0.0326  -2.4    6.6	GRS 1915+105                  
299.5878  35.3413  667.5   5.5 -160.5   0.0002   0.0    8.4	Cyg X-1                       
307.9153  40.8459    6.9   7.2  -76.4   0.0154   1.7   10.9	Cyg X-3                       
326.3286  38.1511    0.0  17.0  -18.6   0.0093   1.0   12.6	Cyg X-2                       
292.2713  33.9059    1.5  11.4 -173.9   0.0754   7.8 ------	UNKNOWN                       
  2.9587  29.4664    2.6  48.1   -9.3   0.0811   4.4 ------	UNKNOWN

Post-slew image of 15-350 keV band

Time interval of the image:
53.948590 962.101700
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
254.4879  35.5537    0.0  30.9 -148.2   0.1678   0.3   12.8	Her X-1                       
268.2710  -1.3509    4.5  41.9  145.4   3.7626   2.5    8.4	SW J1753.5-0127               
288.9653  10.9108    5.2  23.2  116.2   1.4399   2.2   10.1	GRS 1915+105                  
299.5989  35.1961    0.3   6.1    3.7  19.1278  38.7    0.5	Cyg X-1                       
308.1252  40.9347    0.7  14.4  -16.0   9.7508  17.2    1.3	Cyg X-3                       
326.1144  38.4246    4.8  27.5   -1.4   1.3434   2.4    6.7	Cyg X-2                       
323.5758  13.2799    2.7  35.1   46.3   3.8765   4.2 ------	UNKNOWN                       
252.2547  -1.4847    2.8  51.6  163.0   9.0978   4.2 ------	UNKNOWN                       
289.3801  23.2356    3.3  11.0  122.1   1.7998   3.5 ------	UNKNOWN                       
260.3519  25.5745    2.7  28.8 -170.3   2.3398   4.2 ------	UNKNOWN                       
338.1437  50.0677    3.1  37.0  -22.2   2.6185   3.7 ------	UNKNOWN                       
313.6700  54.6779    2.8  25.6  -42.9   2.3484   4.1 ------	UNKNOWN                       
231.5749  15.0234    4.7  57.6 -165.4   6.8582   2.4 ------	UNKNOWN                       
256.9583  48.4477    2.8  29.9 -122.4   2.9166   4.1 ------	UNKNOWN

Plot creation:
Sun Aug 30 19:05:12 EDT 2015