batgrbproduct analysis for trigger=252593

batgrbproduct Analysis for Trigger=252593

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 Jan 20 12:15:18 EST 2014
             Host Name: batevent1
   Current Working Dir: /local/data/batevent/batevent_reproc/trigger252593
======================================================================

  Trigger: 00252593      Segment: 000

  BAT Trigger Time: 188453464   [s; MET]
      Trigger Stop: 188453528   [s; MET]
               UTC: 2006-12-22T04:11:02.350780    [includes UTCF correction] 
       Where From?: TDRSS position message

  BAT 
    RA: 105.357290328966   Dec: -25.8555478617164  [deg; J2000]

     Catalogged Source?: NO
     Point Source?:      YES
     GRB Indicated?:     YES    [ by BAT flight software ]
     Image S/N Ratio:    10.83
     Image Trigger?:     YES
     Rate S/N Ratio:     0  [ if not an image trigger ]
     Image S/N Ratio:    10.83

  Flight Position:   [ source = BAT ]
    RA: 105.357290328966   Dec: -25.8555478617164  [deg; J2000]

  Ground Position:   [ source = BAT pre-slew burst ]
    RA: 105.353903329546   Dec: -25.8678309517905  [deg; J2000]  
        { 07h 01m 24.9s , -25d 52' 04.2" }
         +/- 1.29600812761518 [arcmin] (estimated 90% radius based on SNR)
         +/- 0.447740856112547 [arcmin] (formal 1-sigma fit error)
    SNR: 21.001494515391
 
  Angular difference between Flight and Ground position is 0.759334 arcmin
 
  Partial Coding Fraction: 0.15625    [ including projection effects ]

  Duration
     T90: 37.2479999661446 +/- 6.05790721767193
        Measured from: 41.7039999961853
                   to: 78.9519999623299     [s; relative to TRIGTIME]
     T50: 19.311999976635 +/- 2.58750228941296
        Measured from: 47.0480000078678
                   to: 66.3599999845028     [s; relative to TRIGTIME]



  Fluence
     Peak Flux  (peak 1 second)
        Measured from: 59.2759999930859     
                   to: 60.2759999930859     [s; relative to TRIGTIME]
     Total Fluence        
        Measured from: 35.1119999885559     
                   to: 84.8880000114441     [s; relative to TRIGTIME]
     
             Band 1     Band 2     Band 3     Band 4
              15-25      25-50     50-100    100-350     keV
 Total     1.333452   1.667826   0.892326   0.147357
           0.092104   0.096250   0.081763   0.068577 [error]
 Peak      0.067076   0.066503   0.034062   0.022550
           0.013766   0.014334   0.011911   0.010016 [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 4.85e-07 6.75e-07 6.96e-07 1.31e-06 2.27e-06 3.17e-06   erg/cm2
              Error 5.11e-08 4.76e-08 7.86e-08 2.97e-07 1.83e-07 3.78e-07   erg/cm2
Peak flux Power-law 7.21e-01 4.92e-01 2.20e-01 1.36e-01 1.50e+00 1.57e+00   ph/cm2/s
              Error 2.07e-01 1.15e-01 8.41e-02 9.44e-02 3.43e-01 3.62e-01   ph/cm2/s
 
Fluence   Cutoff-PL 4.50e-07 7.27e-07 6.94e-07 4.94e-07 2.15e-06 2.37e-06   erg/cm2
              Error 5.81e-08 6.24e-08 8.76e-08 3.91e-07 2.02e-07 4.41e-07   erg/cm2
Peak flux Cutoff-PL 6.65e-01 6.34e-01 1.69e-01 8.13e-03 1.48e+00 1.48e+00   ph/cm2/s
              Error 2.27e-01 1.69e-01 1.44e-01 4.39e-02 3.34e-01 3.35e-01   ph/cm2/s
 
Fluence        Band 4.47e-07 7.23e-07 6.94e-07 5.26e-07 2.16e-06 2.41e-06   erg/cm2
              Error -------- -------- 8.45e-08 -------- -------- --------   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    1.956    0.129    -      -           4.96e-03 4.11e-04   51.930 57
CPL   1.306    0.536      47.3   16.0      1.14e-02 8.59e-03   46.870 56
 
 
=== 1-s peak spectral analysis ===
 
Model Ph_index Ph_90err Epeak  Epeak_90err Norm     Nomr_90err chi2   dof
PL    2.162    0.392    -      -           9.23e-03 2.78e-03   63.320 57
CPL  -0.067    2.512      33.4   16.0      2.38e-01 1.99e+01   59.200 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: 38.784000 sec.
T50 in the 50-300 keV band: 18.048000 sec.

 
=== Table of the duration information ==
 
        Value   tstart    tstop
T100   49.776   35.112   84.888
T90    37.248   41.704   78.952
T50    19.312   47.048   66.360
Peak    1.000   59.276   60.276

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
  105.3539   -25.8678   0.0092    37.1700   104.0873         3.9702804     21.001 TRIG_00252593                 
 
Foreground time interval of the image:
 35.112  76.701 (delta_t =  41.589 [sec])
Background time interval of the image:
-239.000  35.112 (delta_t = 274.112 [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 64.000000

8 ms binning

From T100_start-3 s to T100_start+3 s

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 64.000000

2 ms binning

From T100_start-1 s to T100_start+1 s

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 64.000000

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

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

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

Spectral Evolution

Spectra

Notes:

1) The fitting includes the systematic errors.
2) When the burst includes telescope slew time periods, the fitting uses an average response file made from multiple 5-s response files through out the slew time plus single time preiod for the non-slew times, and weighted by the total counts in the corresponding time period using addrmf. An average response file is needed becuase a spectral fit using the pre-slew DRM will introduce some errors in both a spectral shape and a normalization if the PHA file contains a lot of the slew/post-slew time interval.
3) For fits to more complicated models (e.g. a power-law over a cutoff power-law), the BAT team has decided to require a chi-square improvement of more than 6 for each extra dof.

Time averaged spectrum fit using the average DRM

Power-law model

Time interval is from   35.112 sec. to   84.888 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.95614     ( -0.127104   0.131039 )
Norm@50keV  : 4.96139E-03    ( -0.000413831   0.000408409 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          51.93 using 59 PHA bins.
# Reduced chi-squared =         0.9111 for     57 degrees of freedom 
# Null hypothesis probability =   6.650816e-01
 
Photon flux (15-150 keV)    in 49.78 sec: 0.729593 ( -0.052369  0.05242 ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.27331e-06 ( -1.82449e-07  1.84194e-07 ) ergs/cm2

Cutoff power-law model

Time interval is from   35.112 sec. to   84.888 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.30598     ( -0.56903   0.503173 )
Epeak [keV] : 47.2940      ( -11.3593 20.5878 )
Norm@50keV  : 1.13536E-02    ( -0.00527163   0.0119136 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          46.87 using 59 PHA bins.
# Reduced chi-squared =         0.8370 for     56 degrees of freedom 
# Null hypothesis probability =   8.024168e-01
 
Photon flux (15-150 keV)    in 49.78 sec: 0.709890 ( -0.054366  0.054402 ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.15417e-06 ( -1.99787e-07  2.03804e-07 ) ergs/cm2

Band function

Time interval is from   35.112 sec. to   84.888 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -1.30608   ( -0.269773   0.991163 )
beta        : -10.0000    ( 10   1.77636e-15 )
Epeak [keV] : 47.2854      ( -11.3463 20.5924 )
Norm@50keV   : 1.13508E-02    ( -0.00527007   0.0119206 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          46.87 using 59 PHA bins.
# Reduced chi-squared =         0.8522 for     55 degrees of freedom 
# Null hypothesis probability =   7.740375e-01
 
Photon flux (15-150 keV)    in 49.78 sec: 0.713365 (    ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.15719e-06 ( 0  0 ) ergs/cm2

Single BB

 
Spectral model blackbody:
------------------------------------------------------------
Parameters  : value    Lower 90%  Upper 90%
kT [keV]    : 10.7723  (-0.948199  1.04526)
R^2/D10^2   : 0.253681  (-0.0756414   0.107454)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          88.13 using 59 PHA bins.
# Reduced chi-squared =          1.546 for     57 degrees of freedom 
# Null hypothesis probability =   5.111131e-03
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  3.048e-07   4.199e-08
25- 50  8.388e-07   7.069e-08
50-150  5.409e-07   9.269e-08
15-150  1.685e-06   1.394e-07

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 74.4395       (-14.7978      21.0193)
Norm        : 3.50220       (-0.383006     0.439822)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          46.87 using 59 PHA bins.
# Reduced chi-squared =         0.8222 for     57 degrees of freedom 
# Null hypothesis probability =   8.285246e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  4.499e-07   4.615e-08
25- 50  7.275e-07   5.202e-08
50-150  9.771e-07   1.702e-07
15-150  2.155e-06   2.076e-07

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 5.91729        (-1.1109      1.19859)
R1^2/D10^2  : 1.67938        (-0.807135      1.99115)
kT2 [keV]   : 19.3643        (-3.3981      5.13452)
R2^2/D10^2  : 1.94814E-02    (-0.0120436   0.0244043)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          44.17 using 59 PHA bins.
# Reduced chi-squared =         0.8031 for     55 degrees of freedom 
# Null hypothesis probability =   8.519040e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  4.521e-07   1.241e-07
25- 50  7.147e-07   1.849e-07
50-150  9.886e-07   4.761e-07
15-150  2.155e-06   6.944e-07

Peak spectrum fit

Power-law model

Time interval is from   59.276 sec. to   60.276 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 2.16155     ( -0.367687   0.416047 )
Norm@50keV  : 9.23484E-03    ( -0.00280727   0.00274968 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          63.32 using 59 PHA bins.
# Reduced chi-squared =          1.111 for     57 degrees of freedom 
# Null hypothesis probability =   2.631481e-01
 
Photon flux (15-150 keV)    in 1 sec: 1.49862 ( -0.342526  0.342527 ) ph/cm2/s
Energy fluence (15-150 keV)             : 8.63678e-08 ( -2.30055e-08  2.40073e-08 ) ergs/cm2

Cutoff power-law model

Time interval is from   59.276 sec. to   60.276 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: -6.74355E-02     ( -3.10604   1.91846 )
Epeak [keV] : 33.3891      ( -19.3434 12.727 )
Norm@50keV  : 0.238095    ( -0.248155   39.5482 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          59.20 using 59 PHA bins.
# Reduced chi-squared =          1.057 for     56 degrees of freedom 
# Null hypothesis probability =   3.597389e-01
 
Photon flux (15-150 keV)    in 1 sec: 1.47595 ( -0.33302  0.3357 ) ph/cm2/s
Energy fluence (15-150 keV)             : 7.45704e-08 ( -1.99607e-08  2.32447e-08 ) ergs/cm2

Band function

Time interval is from   59.276 sec. to   60.276 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : 4.97963   ( -4.51519   -4.97963 )
beta        : -2.92247    ( -1.33669   0.68323 )
Epeak [keV] : 25.9667      ( -4.93924 4.47358 )
Norm@50keV   : 1561.93    ( -334.844   4823.04 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          56.24 using 59 PHA bins.
# Reduced chi-squared =          1.023 for     55 degrees of freedom 
# Null hypothesis probability =   4.281274e-01
 
Photon flux (15-150 keV)    in 1 sec:  (    ) ph/cm2/s
Energy fluence (15-150 keV)             : 8.02787e-08 ( 0  0 ) ergs/cm2

Single BB

 
Spectral model blackbody:
------------------------------------------------------------
Parameters  : value    Lower 90%  Upper 90%
kT [keV]    : 8.42771  (-1.90637  2.33736)
R^2/D10^2   : 1.46449  (-0.913343   2.5563)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          60.36 using 59 PHA bins.
# Reduced chi-squared =          1.059 for     57 degrees of freedom 
# Null hypothesis probability =   3.553750e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.950e-08   9.356e-09
25- 50  3.728e-08   1.491e-08
50-150  1.158e-08   7.147e-09
15-150  6.836e-08   2.678e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 45.0919       (-17.9405      39.082)
Norm        : 9.34974       (-3.0035     4.5355)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          60.51 using 59 PHA bins.
# Reduced chi-squared =          1.062 for     57 degrees of freedom 
# Null hypothesis probability =   3.503333e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  2.227e-08   6.320e-09
25- 50  3.078e-08   1.186e-08
50-150  2.701e-08   1.720e-08
15-150  8.006e-08   3.020e-08

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 5.66317        (-5.65302      79.8526)
R1^2/D10^2  : 4.41517        (-4.41618      -4.41618)
kT2 [keV]   : 13.5003        (-13.3922      -13.3922)
R2^2/D10^2  : 0.129368    (-0.134936   2.16826)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          58.22 using 59 PHA bins.
# Reduced chi-squared =          1.059 for     55 degrees of freedom 
# Null hypothesis probability =   3.577965e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  2.223e-08   1.381e-08
25- 50  3.302e-08   1.899e-08
50-150  2.216e-08   1.575e-08
15-150  7.740e-08   4.566e-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: 1.94687     ( -0.126209   0.130131 )
Norm@50keV  : 5.51967E-03    ( -0.000456849   0.000451029 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          51.58 using 59 PHA bins.
# Reduced chi-squared =         0.9049 for     57 degrees of freedom 
# Null hypothesis probability =   6.779669e-01
 
Photon flux (15-150 keV)    in 41.59 sec: 0.808367 ( -0.0579424  0.0580009 ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.11241e-06 ( -1.6889e-07  1.70442e-07 ) ergs/cm2

Cutoff power-law model

Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.20478     ( -0.593629   0.524016 )
Epeak [keV] : 47.7011      ( -9.61148 16.5618 )
Norm@50keV  : 1.41396E-02    ( -0.00674837   0.0156579 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          45.44 using 59 PHA bins.
# Reduced chi-squared =         0.8115 for     56 degrees of freedom 
# Null hypothesis probability =   8.423702e-01
 
Photon flux (15-150 keV)    in 41.59 sec: 0.783388 ( -0.060346  0.060394 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.9899e-06 ( -1.84227e-07  1.88498e-07 ) ergs/cm2

Band function

 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -1.21077   ( -0.517939   0.586609 )
beta        : -9.36561    ( 9.3656   19.3656 )
Epeak [keV] : 47.7962      ( -8.70077 16.4366 )
Norm@50keV   : 1.40176E-02    ( -0.00533964   0.00291279 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          45.44 using 59 PHA bins.
# Reduced chi-squared =         0.8262 for     55 degrees of freedom 
# Null hypothesis probability =   8.174286e-01
 
Photon flux (15-150 keV)    in 41.59 sec:  (    ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.98702e-06 ( 0  0 ) ergs/cm2

S(25-50 keV) vs. S(50-100 keV) plot

S(25-50 keV)  = 6.75e-07
S(50-100 keV) = 6.96e-07

T90 vs. Hardness ratio plot

T90                                   = 37.2479999661446 sec.
Hardness ratio (energy fluence ratio) = 1.03111

Color vs. Color plot

Count Ratio  (25-50 keV) / (15-25 keV) = 1.25076
Count Ratio (50-100 keV) / (15-25 keV) = 0.669185

Mask shadow pattern

IMX = -1.845495917877787E-01, IMY = -7.354137459376950E-01

TIME vs. PHA plot around the trigger time

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 64.000000

TIME vs. DetID plot around the trigger time

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 64.000000

100 us light curve (15-350 keV)

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 64.000000

Spacecraft aspect plot

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

Pre-burst image of 15-350 keV band

Time interval of the image:
-239.000000 35.112000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
135.5216 -40.5193    1.7  32.4  155.5   1.8294   6.9    2.1	Vela X-1                      
170.3025 -60.6752    3.8  33.8 -149.4   0.7206   3.1    3.2	Cen X-3                       
186.7515 -62.6763    4.7  38.5 -138.4   0.9454   2.4    6.2	GX 301-2                      
 90.9357 -59.5056    2.0   3.6   51.2   1.1220   5.9 ------	UNKNOWN                       
 74.4079 -64.3738    2.8   9.5  -22.0   0.7575   4.1 ------	UNKNOWN                       
162.2172 -85.8515    3.1  26.2  -99.7   1.0431   3.8 ------	UNKNOWN                       
205.2858 -54.5121    2.3  51.0 -135.6   5.1594   5.0 ------	UNKNOWN

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

Time interval of the image:
35.112000 76.700600
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
135.5125 -40.7092    3.7  32.2  155.7   0.2478   3.1    9.3	Vela X-1                      
170.3158 -60.6185   27.3  33.8 -149.4   0.0310   0.4    0.3	Cen X-3                       
186.5464 -62.6817    8.5  38.5 -138.5  -0.1360  -1.4    6.1	GX 301-2                      
105.3539 -25.8678    0.6  37.2  104.1   3.9706  21.0 ------	UNKNOWN                       
 38.0890 -45.4418    2.4  36.1   -0.3   0.4239   4.9 ------	UNKNOWN                       
 93.4180 -68.3165    2.6   5.9  -84.3   0.2717   4.5 ------	UNKNOWN                       
335.9878 -65.8560    2.5  44.3  -60.3   1.1685   4.7 ------	UNKNOWN

Post-slew image of 15-350 keV band

Time interval of the image:
134.300620 483.070600
661.000000 723.068900
841.000000 887.100590
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
135.5318 -40.5858    1.4  29.0 -124.0   3.0748   8.4    1.9	Vela X-1                      
 86.1990   5.5592    3.8  36.5   74.7   2.1427   3.1 ------	UNKNOWN                       
 52.5797 -11.7003    2.5  51.6   23.5   6.5050   4.5 ------	UNKNOWN                       
 71.1410  -8.9346    2.3  36.6   39.3   2.2685   4.9 ------	UNKNOWN                       
101.9274 -30.5979    2.7   5.6  -40.2   1.1167   4.3 ------	UNKNOWN                       
105.9975 -64.2773    3.6  38.4  -72.5   2.5844   3.2 ------	UNKNOWN                       
123.1769 -65.2857    3.4  41.0  -83.3   4.6800   3.4 ------	UNKNOWN

Plot creation:
Sun May 31 11:08:41 EDT 2015