batgrbproduct analysis for trigger=238108

batgrbproduct Analysis for Trigger=238108

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 12:03:11 EST 2014
             Host Name: batevent1
   Current Working Dir: /local/data/batevent/batevent_reproc/trigger238108
======================================================================

  Trigger: 00238108      Segment: 000

  BAT Trigger Time: 184852042.88   [s; MET]
      Trigger Stop: 184852044.928   [s; MET]
               UTC: 2006-11-10T11:47:21.318140    [includes UTCF correction] 
       Where From?: TDRSS position message

  BAT 
    RA: 336.30368447156   Dec: -2.26672228601831  [deg; J2000]

     Catalogged Source?: NO
     Point Source?:      YES
     GRB Indicated?:     YES    [ by BAT flight software ]
     Image S/N Ratio:    7.33
     Image Trigger?:     NO
     Rate S/N Ratio:     8  [ if not an image trigger ]
     Image S/N Ratio:    7.33

  Flight Position:   [ source = BAT ]
    RA: 336.30368447156   Dec: -2.26672228601831  [deg; J2000]

  Ground Position:   [ source = BAT pre-slew burst ]
    RA: 336.285915402244   Dec: -2.25967051729736  [deg; J2000]  
        { 22h 25m 08.6s , -02d 15' 34.8" }
         +/- 1.14669362771445 [arcmin] (estimated 90% radius based on SNR)
         +/- 0.43026213724939 [arcmin] (formal 1-sigma fit error)
    SNR: 25.0145977831664
 
  Angular difference between Flight and Ground position is 1.146259 arcmin
 
  Partial Coding Fraction: 1.015625    [ including projection effects ]

  Duration
     T90: 44.5080000162125 +/- 5.90336208604624
        Measured from: -6.2039999961853
                   to: 38.3040000200272     [s; relative to TRIGTIME]
     T50: 22.1440000236034 +/- 3.23418241155829
        Measured from: 1.04399999976158
                   to: 23.188000023365     [s; relative to TRIGTIME]



  Fluence
     Peak Flux  (peak 1 second)
        Measured from: 2.11599999666214     
                   to: 3.11599999666214     [s; relative to TRIGTIME]
     Total Fluence        
        Measured from: -8.7960000038147     
                   to: 44.8840000033379     [s; relative to TRIGTIME]
     
             Band 1     Band 2     Band 3     Band 4
              15-25      25-50     50-100    100-350     keV
 Total     0.656172   0.736010   0.510980   0.088161
           0.036070   0.038080   0.035543   0.036373 [error]
 Peak      0.031733   0.016642   0.009808   0.015331
           0.005055   0.005286   0.005076   0.005195 [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 1.77e-07 2.98e-07 3.81e-07 9.81e-07 1.13e-06 1.84e-06   erg/cm2
              Error 1.78e-08 1.78e-08 3.51e-08 1.94e-07 8.05e-08 2.23e-07   erg/cm2
Peak flux Power-law 2.14e-01 1.56e-01 7.61e-02 5.25e-02 4.71e-01 4.99e-01   ph/cm2/s
              Error 6.98e-02 4.16e-02 3.95e-02 5.37e-02 1.18e-01 1.34e-01   ph/cm2/s
 
Fluence   Cutoff-PL 1.75e-07 3.01e-07 3.82e-07 8.38e-07 1.12e-06 1.68e-06   erg/cm2
              Error 2.05e-08 2.08e-08 3.56e-08 3.81e-07 9.28e-08 3.96e-07   erg/cm2
Peak flux Cutoff-PL 2.15e-01 1.56e-01 7.48e-02 5.03e-02 4.70e-01 4.96e-01   ph/cm2/s
              Error 6.95e-02 4.26e-02 5.90e-02 6.15e-02 1.16e-01 1.02e-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    1.643    0.117    -      -           2.26e-03 1.48e-04   59.030 57
CPL   1.556    0.322     240.3    0.0      2.51e-03 1.19e-03   58.900 56
 
 
=== 1-s peak spectral analysis ===
 
Model Ph_index Ph_90err Epeak  Epeak_90err Norm     Nomr_90err chi2   dof
PL    2.040    0.558    -      -           3.08e-03 1.19e-03   59.970 57
CPL   2.086    0.000      38.1    0.0      2.68e-03 0.00e+00   59.790 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: 42.944000 sec.
T50 in the 50-300 keV band: 19.520000 sec.

 
=== Table of the duration information ==
 
        Value   tstart    tstop
T100   53.680   -8.796   44.884
T90    44.508   -6.204   38.304
T50    22.144    1.044   23.188
Peak    1.000    2.116    3.116

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
  336.2859    -2.2597   0.0077     6.2687    43.7789         1.7067683     25.015 TRIG_00238108                 
 
Foreground time interval of the image:
 -8.796  30.021 (delta_t =  38.817 [sec])
Background time interval of the image:
-239.880  -8.796 (delta_t = 231.084 [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 2.048000

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 2.048000

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 2.048000

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   -8.796 sec. to   44.884 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.64326     ( -0.116363   0.118208 )
Norm@50keV  : 2.25567E-03    ( -0.000148295   0.000146779 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          59.03 using 59 PHA bins.
# Reduced chi-squared =          1.036 for     57 degrees of freedom 
# Null hypothesis probability =   4.012400e-01
 
Photon flux (15-150 keV)    in 53.68 sec: 0.293885 ( -0.0175294  0.0175503 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.1269e-06 ( -7.99875e-08  8.10632e-08 ) ergs/cm2

Cutoff power-law model

Time interval is from   -8.796 sec. to   44.884 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.55621     ( -0.448175   0.195893 )
Epeak [keV] : 240.328      ( -240.328 -240.328 )
Norm@50keV  : 2.50570E-03    ( -0.000645406   0.00173959 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          58.90 using 59 PHA bins.
# Reduced chi-squared =          1.052 for     56 degrees of freedom 
# Null hypothesis probability =   3.697646e-01
 
Photon flux (15-150 keV)    in 53.68 sec: 0.292203 ( -0.019143  0.009633 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.11625e-06 ( -9.5647e-08  8.99569e-08 ) ergs/cm2

Band function

Time interval is from   -8.796 sec. to   44.884 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -1.56181   ( 1.50463   1.50463 )
beta        : -2.72219    ( 8.42448   6.89486 )
Epeak [keV] : 252.022      ( -150.055 -252.078 )
Norm@50keV   : 2.48981E-03    ( -0.000375564   0.00212981 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          58.90 using 59 PHA bins.
# Reduced chi-squared =          1.071 for     55 degrees of freedom 
# Null hypothesis probability =   3.347063e-01
 
Photon flux (15-150 keV)    in 53.68 sec: 0.291637 (    ) 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]    : 13.1453  (  )
R^2/D10^2   : 4.94841E-02  (   )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =         128.34 using 59 PHA bins.
# Reduced chi-squared =         2.2515 for     57 degrees of freedom 
# Null hypothesis probability =   2.040942e-07
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  9.733e-08   1.055e-08
25- 50  3.392e-07   2.504e-08
50-150  3.730e-07   5.279e-08
15-150  8.096e-07   5.636e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 160.681       (-47.4788      -159.736)
Norm        : 1.19352       (-0.0766298     0.0964852)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          60.14 using 59 PHA bins.
# Reduced chi-squared =          1.055 for     57 degrees of freedom 
# Null hypothesis probability =   3.626383e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.635e-07   1.337e-08
25- 50  3.061e-07   5.556e-08
50-150  6.211e-07   2.561e-07
15-150  1.091e-06   2.738e-07

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 5.53364        (-1.03868      1.22548)
R1^2/D10^2  : 0.756205        (-0.393842      0.995228)
kT2 [keV]   : 22.1477        (-3.42562      5.18775)
R2^2/D10^2  : 6.47236E-03    (-0.00342704   0.005549)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          58.70 using 59 PHA bins.
# Reduced chi-squared =          1.067 for     55 degrees of freedom 
# Null hypothesis probability =   3.415618e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.771e-07   4.694e-08
25- 50  2.881e-07   5.604e-08
50-150  6.197e-07   1.430e-07
15-150  1.085e-06   2.300e-07

Peak spectrum fit

Power-law model

Time interval is from    2.116 sec. to    3.116 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 2.03985     ( -0.516577   0.59858 )
Norm@50keV  : 3.08211E-03    ( -0.00121727   0.00117054 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          59.97 using 59 PHA bins.
# Reduced chi-squared =          1.052 for     57 degrees of freedom 
# Null hypothesis probability =   3.686809e-01
 
Photon flux (15-150 keV)    in 1 sec: 0.470991 ( -0.117806  0.118058 ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.84917e-08 ( -9.65139e-09  1.08859e-08 ) ergs/cm2

Cutoff power-law model

Time interval is from    2.116 sec. to    3.116 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 2.08630     (     )
Epeak [keV] : 38.0733      (   )
Norm@50keV  : 2.68307E-03    (     )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          59.79 using 59 PHA bins.
# Reduced chi-squared =          1.068 for     56 degrees of freedom 
# Null hypothesis probability =   3.397716e-01
 
Photon flux (15-150 keV)    in 1 sec: 0.470024 ( -0.11678  0.115974 ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.83164e-08 ( -1.15668e-08  1.08852e-08 ) ergs/cm2

Band function

Time interval is from    2.116 sec. to    3.116 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : 4.97722   ( -4.97722   -4.97722 )
beta        : -2.37854    ( -1.29647   0.697384 )
Epeak [keV] : 21.3488      ( -21.3488 5.26383 )
Norm@50keV   : 1564.36    ( -377.687   5.74259e+06 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          58.47 using 59 PHA bins.
# Reduced chi-squared =          1.063 for     55 degrees of freedom 
# Null hypothesis probability =   3.492660e-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]    : 6.63947  (-1.68905  2.38138)
R^2/D10^2   : 1.06070  (-1.06018   2.50327)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          63.21 using 59 PHA bins.
# Reduced chi-squared =          1.109 for     57 degrees of freedom 
# Null hypothesis probability =   2.664022e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  7.087e-09   4.141e-09
25- 50  8.740e-09   5.400e-09
50-150  1.192e-09   9.931e-10
15-150  1.702e-08   1.009e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 48.7794       (-28.1467      -48.8766)
Norm        : 2.66083       (-1.02962     2.32857)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          61.12 using 59 PHA bins.
# Reduced chi-squared =          1.072 for     57 degrees of freedom 
# Null hypothesis probability =   3.303002e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  6.468e-09   2.897e-09
25- 50  9.208e-09   4.382e-09
50-150  8.732e-09   6.596e-09
15-150  2.441e-08   1.204e-08

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 5.68747        (-1.54937      1.99563)
R1^2/D10^2  : 1.82903        (-1.29905      5.17406)
kT2 [keV]   : 81.2615        (-60.1119      -81.2331)
R2^2/D10^2  : 3.24945E-04    (-0.000291193   0.00836358)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          55.97 using 59 PHA bins.
# Reduced chi-squared =          1.018 for     55 degrees of freedom 
# Null hypothesis probability =   4.381714e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  7.407e-09   4.425e-09
25- 50  7.655e-09   4.364e-09
50-150  2.225e-08   1.653e-08
15-150  3.731e-08   1.951e-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: 1.66135     ( -0.115499   0.117352 )
Norm@50keV  : 2.66636E-03    ( -0.000176123   0.00017429 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          57.45 using 59 PHA bins.
# Reduced chi-squared =          1.008 for     57 degrees of freedom 
# Null hypothesis probability =   4.584252e-01
 
Photon flux (15-150 keV)    in 38.82 sec: 0.349476 ( -0.0207604  0.0207829 ) ph/cm2/s
Energy fluence (15-150 keV)             : 9.61599e-07 ( -6.81376e-08  6.90651e-08 ) ergs/cm2

Cutoff power-law model

Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.53870     ( -0.453943   0.228506 )
Epeak [keV] : 174.649      ( -174.649 -174.649 )
Norm@50keV  : 3.09740E-03    (     )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          57.20 using 59 PHA bins.
# Reduced chi-squared =          1.021 for     56 degrees of freedom 
# Null hypothesis probability =   4.302716e-01
 
Photon flux (15-150 keV)    in 38.82 sec: 0.346726 ( -0.02265  0.022401 ) ph/cm2/s
Energy fluence (15-150 keV)             : 9.48155e-07 ( -8.24692e-08  7.92316e-08 ) ergs/cm2

Band function

 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -1.52057   ( -0.170893   0.239006 )
beta        : -9.37167    ( 9.37167   19.3717 )
Epeak [keV] : 161.326      ( -76.227 -161.492 )
Norm@50keV   : 3.15930E-03    ( -0.00065104   0.00107651 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          57.21 using 59 PHA bins.
# Reduced chi-squared =          1.040 for     55 degrees of freedom 
# Null hypothesis probability =   3.931582e-01
 
Photon flux (15-150 keV)    in 38.82 sec: 0.345092 (    ) 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)  = 2.98e-07
S(50-100 keV) = 3.81e-07

T90 vs. Hardness ratio plot

T90                                   = 44.5080000162125 sec.
Hardness ratio (energy fluence ratio) = 1.27852

Color vs. Color plot

Count Ratio  (25-50 keV) / (15-25 keV) = 1.12167
Count Ratio (50-100 keV) / (15-25 keV) = 0.778729

Mask shadow pattern

IMX = 7.931218979124242E-02, IMY = -7.600160850657510E-02

TIME vs. PHA plot around the trigger time

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 2.048000

TIME vs. DetID plot around the trigger time

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 2.048000

100 us light curve (15-350 keV)

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 2.048000

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:
-239.880000 -8.796000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
288.7924  10.9630    2.6  49.2  -41.9   3.1010   4.4    1.1	GRS 1915+105                  
299.5895  35.2113    0.9  54.4   -9.1   8.1955  13.2    0.6	Cyg X-1                       
308.1119  40.9785   39.7  54.8    1.7  -0.2217  -0.3    1.6	Cyg X-3                       
326.1511  38.1592    8.2  47.0   17.0   0.6723   1.4    9.8	Cyg X-2                       
348.4092  32.6354    3.1  43.0   43.3   2.2411   3.7 ------	UNKNOWN                       
331.5519  32.8448    2.2  41.2   22.2   1.8471   5.3 ------	UNKNOWN

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

Time interval of the image:
-8.796000 30.020610
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
288.9064  10.9148    4.6  49.1  -41.9   0.6534   2.5    6.6	GRS 1915+105                  
299.5875  35.2290    6.3  54.4   -9.1  -0.4077  -1.8    1.6	Cyg X-1                       
308.1993  40.8891    7.5  54.7    1.7   0.4604   1.5    5.5	Cyg X-3                       
326.1049  38.2106   87.6  47.1   17.0  -0.0230  -0.1    7.4	Cyg X-2                       
 23.2762 -25.4947    2.1  49.6  142.5   1.7504   5.4 ------	UNKNOWN                       
346.6464  38.5804    2.1  48.2   38.7   1.7002   5.6 ------	UNKNOWN                       
346.2906  19.8722    2.2  30.5   48.4   0.5496   5.4 ------	UNKNOWN                       
355.6217 -20.2886    2.1  23.8  148.5   0.4257   5.5 ------	UNKNOWN                       
336.2859  -2.2597    0.5   6.3   43.8   1.7067  25.0 ------	UNKNOWN                       
309.5150  17.1473    2.2  35.3  -18.2   0.4745   5.1 ------	UNKNOWN                       
288.3166   1.7399    2.2  47.0  -54.0   1.5226   5.2 ------	UNKNOWN

Post-slew image of 15-350 keV band

Time interval of the image:
57.620600 962.225600
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
299.5808  35.2021    0.5  50.8  -20.0  33.2653  25.7    0.5	Cyg X-1                       
308.1358  40.8499   30.1  50.2   -8.6   0.4581   0.4    6.3	Cyg X-3                       
326.2656  38.3990    6.3  41.7    7.2   1.4486   1.8    6.4	Cyg X-2                       
  9.2223  21.5859    3.2  40.1   70.8   7.3686   3.5 ------	UNKNOWN                       
  4.3493  32.6750    3.0  43.9   53.9   7.7660   3.9 ------	UNKNOWN                       
  0.1028   5.1857    3.0  24.9   91.7   2.3791   3.9  311.2	UNKNOWN                       
341.4074  41.6467    2.9  44.1   24.6   3.9731   4.0 ------	UNKNOWN                       
356.4099 -57.1507    4.2  57.2 -173.7   7.4126   2.8 ------	UNKNOWN                       
313.9136 -54.4170    5.1  55.3 -145.3   8.1456   2.3 ------	UNKNOWN

Plot creation:
Sun May 31 11:31:51 EDT 2015