batgrbproduct analysis for trigger=522578

batgrbproduct Analysis for Trigger=522578

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 13 04:24:10 EST 2014
             Host Name: batevent1
   Current Working Dir: /local/data/batevent/batevent_reproc/trigger522578
======================================================================

  Trigger: 00522578      Segment: 000

  BAT Trigger Time: 359272791.168   [s; MET]
      Trigger Stop: 359272791.68   [s; MET]
               UTC: 2012-05-21T05:59:42.937680    [includes UTCF correction] 
       Where From?: TDRSS position message

  BAT 
    RA: 148.69332117108   Dec: -49.4193802244313  [deg; J2000]

     Catalogged Source?: NO
     Point Source?:      YES
     GRB Indicated?:     YES    [ by BAT flight software ]
     Image S/N Ratio:    11.48
     Image Trigger?:     NO
     Rate S/N Ratio:     24.6981780704569  [ if not an image trigger ]
     Image S/N Ratio:    11.48

  Flight Position:   [ source = BAT ]
    RA: 148.69332117108   Dec: -49.4193802244313  [deg; J2000]

  Ground Position:   [ source = BAT pre-slew burst ]
    RA: 148.686940886453   Dec: -49.4244012807195  [deg; J2000]  
        { 09h 54m 44.9s , -49d 25' 27.8" }
         +/- 1.75349438379915 [arcmin] (estimated 90% radius based on SNR)
         +/- 0.740366609476014 [arcmin] (formal 1-sigma fit error)
    SNR: 13.6358919896314
 
  Angular difference between Flight and Ground position is 0.390856 arcmin
 
  Partial Coding Fraction: 1    [ including projection effects ]

  Duration
     T90: 0.51199996471405 +/- 0.143108374017273
        Measured from: -0.0079999566078186
                   to: 0.504000008106232     [s; relative to TRIGTIME]
     T50: 0.25600004196167 +/- 0.0640000104904175
        Measured from: 0.0559999942779541
                   to: 0.312000036239624     [s; relative to TRIGTIME]



  Fluence
     Peak Flux  (peak 1 second)
        Measured from: -0.187999963760376     
                   to: 0.812000036239624     [s; relative to TRIGTIME]
     Total Fluence        
        Measured from: -0.0079999566078186     
                   to: 0.568000018596649     [s; relative to TRIGTIME]
     
             Band 1     Band 2     Band 3     Band 4
              15-25      25-50     50-100    100-350     keV
 Total     0.018330   0.042938   0.041515   0.015896
           0.004411   0.004847   0.004633   0.004105 [error]
 Peak      0.012586   0.046076   0.046788   0.018408
           0.005605   0.005971   0.005565   0.004875 [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 5.90e-09 1.46e-08 2.91e-08 1.44e-07 7.85e-08 1.93e-07   erg/cm2
              Error 1.45e-09 2.15e-09 4.26e-09 4.85e-08 1.12e-08 5.10e-08   erg/cm2
Peak flux Power-law 1.74e-01 2.56e-01 2.82e-01 5.82e-01 8.89e-01 1.29e+00   ph/cm2/s
              Error 5.31e-02 4.79e-02 4.23e-02 1.92e-01 1.30e-01 2.13e-01   ph/cm2/s
 
Fluence   Cutoff-PL 5.13e-09 1.53e-08 3.07e-08 6.41e-08 7.52e-08 1.15e-07   erg/cm2
              Error 1.75e-09 2.47e-09 4.92e-09 7.30e-08 1.23e-08 8.16e-08   erg/cm2
Peak flux Cutoff-PL 1.32e-01 2.64e-01 3.11e-01 2.59e-01 8.52e-01 9.66e-01   ph/cm2/s
              Error 6.40e-02 5.48e-02 5.33e-02 2.43e-01 1.35e-01 2.79e-01   ph/cm2/s
 
Fluence        Band -------- -------- -------- -------- -------- --------   erg/cm2
              Error -------- -------- -------- -------- -------- --------   erg/cm2
Peak flux      Band 1.45e-01 2.61e-01 3.03e-01 3.37e-01 8.69e-01 1.05e+00   ph/cm2/s
              Error 6.31e-02 -------- -------- -------- -------- --------   ph/cm2/s

 
=== Time-averaged spectral analysis ===
 
Model Ph_index Ph_90err Epeak  Epeak_90err Norm     Nomr_90err chi2   dof
PL    1.009    0.222    -      -           1.27e-02 1.59e-03   47.100 57
CPL   0.391    0.864     142.9    0.0      2.44e-02 0.00e+00   45.470 56
 
 
=== 1-s peak spectral analysis ===
 
Model Ph_index Ph_90err Epeak  Epeak_90err Norm     Nomr_90err chi2   dof
PL    0.864    0.250    -      -           7.75e-03 1.14e-03   42.380 57
CPL  -0.098    1.128     127.9 2698.1      2.00e-02 2.83e-02   39.570 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: 0.320000 sec.
T50 in the 50-300 keV band: 0.128000 sec.

 
=== Table of the duration information ==
 
        Value   tstart    tstop
T100    0.576   -0.008    0.568
T90     0.512   -0.008    0.504
T50     0.256    0.056    0.312
Peak    1.000   -0.188    0.812

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
  148.6869   -49.4244   0.0140    13.1385   -32.7837         0.1131131     13.636 TRIG_00522578                 
 
Foreground time interval of the image:
 -0.008   0.568 (delta_t =   0.576 [sec])
Background time interval of the image:
-597.067 -578.595 (delta_t =  18.472 [sec])
-239.168  -0.008 (delta_t = 239.160 [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 0.512000

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 0.512000

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 0.512000

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)

The mask-weighted light curves based on cleaned DPHs

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   -0.008 sec. to    0.568 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.00943     ( -0.224853   0.218693 )
Norm@50keV  : 1.26532E-02    ( -0.0015916   0.00158927 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          47.10 using 59 PHA bins.
# Reduced chi-squared =         0.8264 for     57 degrees of freedom 
# Null hypothesis probability =   8.220801e-01
 
Photon flux (15-150 keV)    in 0.576 sec: 1.45733 ( -0.184996  0.185613 ) ph/cm2/s
Energy fluence (15-150 keV)             : 7.85111e-08 ( -1.11058e-08  1.12894e-08 ) ergs/cm2

Cutoff power-law model

Time interval is from   -0.008 sec. to    0.568 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 0.391049     ( -1.01425   0.713982 )
Epeak [keV] : 142.865      (   )
Norm@50keV  : 2.44153E-02    (     )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          45.47 using 59 PHA bins.
# Reduced chi-squared =         0.8120 for     56 degrees of freedom 
# Null hypothesis probability =   8.415114e-01
 
Photon flux (15-150 keV)    in 0.576 sec: 1.41598 ( -0.19052  0.19352 ) ph/cm2/s
Energy fluence (15-150 keV)             : 7.52187e-08 ( -1.23016e-08  1.22498e-08 ) ergs/cm2

Band function

Time interval is from   -0.008 sec. to    0.568 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -0.391047   ( -0.575859   1.00363 )
beta        : -10.0000    ( 10   0 )
Epeak [keV] : 142.849      ( -58.56 202.733 )
Norm@50keV   : 2.44152E-02    ( -0.0127103   0.0437672 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          45.47 using 59 PHA bins.
# Reduced chi-squared =         0.8268 for     55 degrees of freedom 
# Null hypothesis probability =   8.165054e-01
 
Photon flux (15-150 keV)    in 0.576 sec: 1.43354 (    ) 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]    : 20.9234  (-3.43921  4.34867)
R^2/D10^2   : 6.05653E-02  (-0.0267199   0.0461882)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          52.47 using 59 PHA bins.
# Reduced chi-squared =         0.9206 for     57 degrees of freedom 
# Null hypothesis probability =   6.453399e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  2.890e-09   7.468e-10
25- 50  1.482e-08   2.863e-09
50-150  4.834e-08   1.175e-08
15-150  6.606e-08   1.208e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 200.000       (      )
Norm        : 5.81069       (-0.761057     0.761043)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          61.64 using 59 PHA bins.
# Reduced chi-squared =          1.081 for     57 degrees of freedom 
# Null hypothesis probability =   3.138190e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  8.335e-09   4.674e-09
25- 50  1.603e-08   8.893e-09
50-150  3.517e-08   1.962e-08
15-150  5.954e-08   3.318e-08

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 0.102194        (0.822496      -0.102194)
R1^2/D10^2  : 1.25365E+18        (-1.25366e+18      -1.25366e+18)
kT2 [keV]   : 20.9342        (-3.44228      4.3456)
R2^2/D10^2  : 6.04704E-02    (-0.0266958   0.0462154)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          52.47 using 59 PHA bins.
# Reduced chi-squared =         0.9541 for     55 degrees of freedom 
# Null hypothesis probability =   5.717304e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  0.000e+00   0.000e+00
25- 50  0.000e+00   0.000e+00
50-150  0.000e+00   0.000e+00
15-150  0.000e+00   0.000e+00

Peak spectrum fit

Power-law model

Time interval is from   -0.188 sec. to    0.812 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 0.863632     ( -0.256454   0.244189 )
Norm@50keV  : 7.74876E-03    ( -0.0011408   0.00113154 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          42.38 using 59 PHA bins.
# Reduced chi-squared =         0.7435 for     57 degrees of freedom 
# Null hypothesis probability =   9.255783e-01
 
Photon flux (15-150 keV)    in 1 sec: 0.889374 ( -0.129586  0.130094 ) ph/cm2/s
Energy fluence (15-150 keV)             : 8.8216e-08 ( -1.35646e-08  1.37085e-08 ) ergs/cm2

Cutoff power-law model

Time interval is from   -0.188 sec. to    0.812 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: -9.77873E-02     ( -1.28316   0.972507 )
Epeak [keV] : 127.854      ( -43.0824 5353.09 )
Norm@50keV  : 2.00406E-02    ( -0.0121298   0.0445453 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          39.57 using 59 PHA bins.
# Reduced chi-squared =         0.7065 for     56 degrees of freedom 
# Null hypothesis probability =   9.528179e-01
 
Photon flux (15-150 keV)    in 1 sec: 0.851636 ( -0.134801  0.135475 ) ph/cm2/s
Energy fluence (15-150 keV)             : 8.38431e-08 ( -1.47512e-08  1.4711e-08 ) ergs/cm2

Band function

Time interval is from   -0.188 sec. to    0.812 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : 9.51423E-02   ( -0.780444   1.39256 )
beta        : -10.0000    ( 10   8.88178e-15 )
Epeak [keV] : 128.022      ( -41.8345 284.339 )
Norm@50keV   : 1.99930E-02    ( -0.0120479   0.044522 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          39.57 using 59 PHA bins.
# Reduced chi-squared =         0.7194 for     55 degrees of freedom 
# Null hypothesis probability =   9.420289e-01
 
Photon flux (15-150 keV)    in 1 sec: 0.868777 (    ) 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]    : 23.7830  (-4.17814  5.51039)
R^2/D10^2   : 2.60165E-02  (-0.0120559   0.0211234)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          42.19 using 59 PHA bins.
# Reduced chi-squared =         0.7402 for     57 degrees of freedom 
# Null hypothesis probability =   9.286308e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  2.623e-09   8.215e-10
25- 50  1.450e-08   3.676e-09
50-150  6.114e-08   1.667e-08
15-150  7.826e-08   1.869e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 200.000       (      )
Norm        : 3.53029       (-0.540367     0.540347)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          61.62 using 59 PHA bins.
# Reduced chi-squared =          1.081 for     57 degrees of freedom 
# Null hypothesis probability =   3.144132e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  8.792e-09   5.085e-09
25- 50  1.691e-08   9.490e-09
50-150  3.709e-08   2.092e-08
15-150  6.280e-08   3.563e-08

Double BB

R1^2/D10^2  : 9.87372E+08        (      )
kT2 [keV]   : 24.2154        (-4.35174      5.80095)
R2^2/D10^2  : 2.44968E-02    (-0.00707847   0.0105493)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          42.19 using 59 PHA bins.
#Fit statistic : Chi-Squared =          40.42 using 59 PHA bins.
#Fit statistic : Chi-Squared =          40.16 using 59 PHA bins.
# Reduced chi-squared =         0.7671 for     55 degrees of freedom 
# Reduced chi-squared =         0.7349 for     55 degrees of freedom 
# Reduced chi-squared =         0.7302 for     55 degrees of freedom 
# Null hypothesis probability =   8.973831e-01
# Null hypothesis probability =   9.294318e-01
# Null hypothesis probability =   9.334416e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  0.000e+00   0.000e+00
25- 50  0.000e+00   0.000e+00
50-150  0.000e+00   0.000e+00
15-150  0.000e+00   0.000e+00

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: 1.00943     ( -0.224853   0.218693 )
Norm@50keV  : 1.26532E-02    ( -0.0015916   0.00158927 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          47.10 using 59 PHA bins.
# Reduced chi-squared =         0.8264 for     57 degrees of freedom 
# Null hypothesis probability =   8.220801e-01
 
Photon flux (15-150 keV)    in 0.576 sec: 1.45733 ( -0.184996  0.185613 ) ph/cm2/s
Energy fluence (15-150 keV)             : 7.85111e-08 ( -1.11058e-08  1.12894e-08 ) ergs/cm2

Cutoff power-law model

Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 0.391049     ( -1.01425   0.713982 )
Epeak [keV] : 142.865      (   )
Norm@50keV  : 2.44153E-02    (     )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          45.47 using 59 PHA bins.
# Reduced chi-squared =         0.8120 for     56 degrees of freedom 
# Null hypothesis probability =   8.415114e-01
 
Photon flux (15-150 keV)    in 0.576 sec: 1.41598 ( -0.19051  0.19352 ) ph/cm2/s
Energy fluence (15-150 keV)             : 7.52187e-08 ( -1.23016e-08  1.22498e-08 ) ergs/cm2

Band function

 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -0.391086   ( -0.575399   1.00655 )
beta        : -10.0000    ( 10   2.91323e-13 )
Epeak [keV] : 142.855      ( -58.5663 202.765 )
Norm@50keV   : 2.44142E-02    ( -0.0127092   0.0437682 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          45.47 using 59 PHA bins.
# Reduced chi-squared =         0.8268 for     55 degrees of freedom 
# Null hypothesis probability =   8.165054e-01
 
Photon flux (15-150 keV)    in 0.576 sec: 1.43354 (    ) 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)  = 1.46e-08
S(50-100 keV) = 2.91e-08

T90 vs. Hardness ratio plot

T90                                   = 0.51199996471405 sec.
Hardness ratio (energy fluence ratio) = 1.99315

Color vs. Color plot

Count Ratio  (25-50 keV) / (15-25 keV) = 2.3425
Count Ratio (50-100 keV) / (15-25 keV) = 2.26487

Mask shadow pattern

IMX = 1.962374582997249E-01, IMY = 1.263874497532329E-01

TIME vs. PHA plot around the trigger time

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.512000

TIME vs. DetID plot around the trigger time

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.512000

100 us light curve (15-350 keV)

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.512000

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:
-597.067410 -578.595400
-239.168000 -0.008000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
135.5277 -40.5514    1.0  25.6  -42.5   2.5028  11.3    0.2	Vela X-1                      
170.4156 -60.6790    1.4   4.0  115.7   1.4754   8.3    4.5	Cen X-3                       
186.7592 -62.6451    6.8  11.9  124.5   0.3270   1.7    8.0	GX 301-2                      
167.4864 -34.4646    2.5  25.6   20.0   0.9599   4.6 ------	UNKNOWN                       
147.5821  -5.8994    2.3  55.2   -7.6   3.2874   5.0 ------	UNKNOWN                       
140.2208  -4.7615    3.0  57.7  -16.0   3.5497   3.9 ------	UNKNOWN                       
  4.9577 -61.0240    3.7  57.9 -156.7   4.4599   3.1 ------	UNKNOWN

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

Time interval of the image:
-0.008000 0.568000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
135.5011 -40.5285 1689.7  25.6  -42.5  -0.0001  -0.0    2.0	Vela X-1                      
170.1877 -60.5702    6.3   3.8  114.4   0.0174   1.8    4.9	Cen X-3                       
186.6296 -62.9368  189.5  11.8  126.0   0.0006   0.1   10.0	GX 301-2                      
148.6869 -49.4244    0.8  13.1  -32.8   0.1131  13.6 ------	UNKNOWN                       
134.4507  -5.0158    2.4  58.9  -22.6   0.2787   4.8 ------	UNKNOWN                       
 82.0477 -61.8363    2.2  36.7 -118.2   0.0897   5.2 ------	UNKNOWN                       
124.1715 -15.2011    2.2  52.7  -38.3   0.2162   5.2 ------	UNKNOWN

Post-slew image of 15-350 keV band

Time interval of the image:
56.732610 594.832600
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
135.5129 -40.5572    0.5  12.8  -64.5   8.1953  23.6    0.7	Vela X-1                      
170.2281 -60.6152    1.8  16.5  127.7   2.2579   6.3    2.6	Cen X-3                       
186.5374 -62.6991    4.6  24.4  124.0   1.0219   2.5    5.4	GX 301-2                      
 39.2723 -61.6824    2.7  55.5 -160.3   5.7018   4.3 ------	UNKNOWN                       
132.4172   3.0568    4.1  54.3  -33.3   6.0986   2.8 ------	UNKNOWN                       
 86.2622 -40.5752    3.6  43.7 -116.2   5.5674   3.2 ------	UNKNOWN

Plot creation:
Sat May 30 19:31:26 EDT 2015