batgrbproduct analysis for trigger=519256

batgrbproduct Analysis for Trigger=519256

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): Fri Jun 12 01:54:47 EDT 2015
             Host Name: bat1
   Current Working Dir: /local/data/bat1/alien/Swift_3rdBATcatalog/event/batevent_reproc/trigger519256
======================================================================

  Trigger: 00519256      Segment: 000

  BAT Trigger Time: 355178044.544   [s; MET]
      Trigger Stop: 355178046.592   [s; MET]
               UTC: 2012-04-03T20:33:56.481060    [includes UTCF correction] 
       Where From?: TDRSS position message

  BAT 
    RA: 54.8088242661129   Dec: -89.0369268415211  [deg; J2000]

     Catalogged Source?: NO
     Point Source?:      YES
     GRB Indicated?:     YES    [ by BAT flight software ]
     Image S/N Ratio:    7.17
     Image Trigger?:     NO
     Rate S/N Ratio:     13  [ if not an image trigger ]
     Image S/N Ratio:    7.17

  Flight Position:   [ source = BAT ]
    RA: 54.8088242661129   Dec: -89.0369268415211  [deg; J2000]

  Ground Position:   [ source = BAT pre-slew burst ]
    RA: 54.3070003273007   Dec: -89.0291744260173  [deg; J2000]  
        { 03h 37m 13.7s , -89d 01' 45.0" }
         +/- 2.44072116868332 [arcmin] (estimated 90% radius based on SNR)
         +/- 1.33412987402905 [arcmin] (formal 1-sigma fit error)
    SNR: 8.50199797779882
 
  Angular difference between Flight and Ground position is 0.688866 arcmin
 
  Partial Coding Fraction: 0.4765625    [ including projection effects ]

  Duration
     T90: 7.28399991989136 +/- 1.919334249261
        Measured from: -2.60000002384186
                   to: 4.6839998960495     [s; relative to TRIGTIME]
     T50: 2.27199995517731 +/- 2.14724098740904
        Measured from: -0.636000037193298
                   to: 1.63599991798401     [s; relative to TRIGTIME]



  Fluence
     Peak Flux  (peak 1 second)
        Measured from: 0.915999948978424     
                   to: 1.91599994897842     [s; relative to TRIGTIME]
     Total Fluence        
        Measured from: -2.96000003814697     
                   to: 5.32799994945526     [s; relative to TRIGTIME]
     
             Band 1     Band 2     Band 3     Band 4
              15-25      25-50     50-100    100-350     keV
 Total     0.142074   0.114404   0.104750  -0.030197
           0.022381   0.022587   0.019270   0.016285 [error]
 Peak      0.029840   0.032613   0.045793   0.002905
           0.008140   0.008556   0.007579   0.005806 [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 3.77e-08 5.82e-08 6.76e-08 1.51e-07 2.08e-07 3.14e-07   erg/cm2
              Error 9.81e-09 1.04e-08 1.85e-08 8.36e-08 4.38e-08 1.02e-07   erg/cm2
Peak flux Power-law 2.70e-01 3.06e-01 2.48e-01 3.36e-01 9.47e-01 1.16e+00   ph/cm2/s
              Error 1.01e-01 7.25e-02 5.94e-02 1.65e-01 2.03e-01 2.47e-01   ph/cm2/s
 
Fluence   Cutoff-PL 3.58e-08 6.20e-08 6.84e-08 7.03e-08 2.00e-07 2.37e-07   erg/cm2
              Error 1.08e-08 1.30e-08 2.03e-08 8.89e-08 4.61e-08 1.24e-07   erg/cm2
Peak flux Cutoff-PL 2.25e-01 3.22e-01 2.72e-01 1.74e-01 9.20e-01 9.93e-01   ph/cm2/s
              Error 1.26e-01 8.33e-02 7.52e-02 2.41e-01 2.10e-01 3.08e-01   ph/cm2/s
 
Fluence        Band 3.51e-08 6.22e-08 6.83e-08 6.49e-08 1.99e-07 2.31e-07   erg/cm2
              Error -------- -------- -------- -------- 4.51e-08 9.43e-08   erg/cm2
Peak flux      Band 2.52e-01 3.15e-01 2.59e-01 2.46e-01 9.40e-01 1.07e+00   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    1.785    0.314    -      -           2.72e-03 5.59e-04   47.170 57
CPL   1.303    1.001      65.6   -7.6      5.02e-03 1.15e-02   46.470 56
 
 
=== 1-s peak spectral analysis ===
 
Model Ph_index Ph_90err Epeak  Epeak_90err Norm     Nomr_90err chi2   dof
PL    1.302    0.345    -      -           7.93e-03 1.64e-03   53.370 57
CPL   0.526    1.445     105.6    0.0      1.81e-02 0.00e+00   52.430 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    8.288   -2.960    5.328
T90     7.284   -2.600    4.684
T50     2.272   -0.636    1.636
Peak    1.000    0.916    1.916

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
   54.3070   -89.0292   0.0227    30.6493  -115.8824         0.3581574      8.502 TRIG_00519256                 
 
Foreground time interval of the image:
 -2.960   5.328 (delta_t =   8.288 [sec])
Background time interval of the image:
-239.544  -2.960 (delta_t = 236.584 [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)

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   -2.960 sec. to    5.328 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.78539     ( -0.3044   0.323164 )
Norm@50keV  : 2.72359E-03    ( -0.000566875   0.000550322 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          47.17 using 59 PHA bins.
# Reduced chi-squared =         0.8275 for     57 degrees of freedom 
# Null hypothesis probability =   8.203205e-01
 
Photon flux (15-150 keV)    in 8.288 sec: 0.373201 ( -0.0667689  0.0667985 ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.07927e-07 ( -4.32647e-08  4.44146e-08 ) ergs/cm2

Cutoff power-law model

Time interval is from   -2.960 sec. to    5.328 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.30320     ( -1.21354   0.788509 )
Epeak [keV] : 65.6204      ( -50.2363 -65.5337 )
Norm@50keV  : 5.01920E-03    ( -0.00503311   0.0179079 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          46.47 using 59 PHA bins.
# Reduced chi-squared =         0.8299 for     56 degrees of freedom 
# Null hypothesis probability =   8.140274e-01
 
Photon flux (15-150 keV)    in 8.288 sec: 0.367883 ( -0.067484  0.067573 ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.00303e-07 ( -4.51812e-08  4.69399e-08 ) ergs/cm2

Band function

Time interval is from   -2.960 sec. to    5.328 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -1.31872   ( -1.68667   1.18358 )
beta        : -9.37167    ( 9.37167   19.3717 )
Epeak [keV] : 67.3169      ( -38.5211 -67.3146 )
Norm@50keV   : 4.88981E-03    ( -0.00206653   0.0179859 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          46.48 using 59 PHA bins.
# Reduced chi-squared =         0.8450 for     55 degrees of freedom 
# Null hypothesis probability =   7.865043e-01
 
Photon flux (15-150 keV)    in 8.288 sec: 0.368743 ( 6.63126  -0.065511 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.99249e-07 ( -1.99191e-07  -4.34697e-08 ) ergs/cm2

Single BB

 
Spectral model blackbody:
------------------------------------------------------------
Parameters  : value    Lower 90%  Upper 90%
kT [keV]    : 12.0592  (-3.13422  4.01919)
R^2/D10^2   : 8.74363E-02  (-0.0557879   0.176046)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          56.74 using 59 PHA bins.
# Reduced chi-squared =         0.9954 for     57 degrees of freedom 
# Null hypothesis probability =   4.848245e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  2.230e-08   8.429e-09
25- 50  7.058e-08   2.148e-08
50-150  6.192e-08   2.423e-08
15-150  1.548e-07   5.002e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 105.899       (-48.9606      -104.814)
Norm        : 1.63145       (-0.328571     0.498016)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          46.49 using 59 PHA bins.
# Reduced chi-squared =         0.8156 for     57 degrees of freedom 
# Null hypothesis probability =   8.385935e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  3.533e-08   1.002e-08
25- 50  6.179e-08   2.655e-08
50-150  1.034e-07   7.201e-08
15-150  2.005e-07   1.135e-07

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 5.29804        (-1.55265      2.15584)
R1^2/D10^2  : 1.32545        (-0.976315      4.23391)
kT2 [keV]   : 21.4390        (-5.93462      11.2706)
R2^2/D10^2  : 8.54415E-03    (-0.0066552   0.0207933)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          43.62 using 59 PHA bins.
# Reduced chi-squared =         0.7931 for     55 degrees of freedom 
# Null hypothesis probability =   8.655840e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  3.959e-08   2.209e-08
25- 50  5.689e-08   3.051e-08
50-150  1.102e-07   6.734e-08
15-150  2.067e-07   1.089e-07

Peak spectrum fit

Power-law model

Time interval is from    0.916 sec. to    1.916 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.30185     ( -0.347462   0.343366 )
Norm@50keV  : 7.93181E-03    ( -0.0016454   0.00164409 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          53.37 using 59 PHA bins.
# Reduced chi-squared =         0.9364 for     57 degrees of freedom 
# Null hypothesis probability =   6.119647e-01
 
Photon flux (15-150 keV)    in 1 sec: 0.946604 ( -0.20267  0.203494 ) ph/cm2/s
Energy fluence (15-150 keV)             : 7.83457e-08 ( -1.7553e-08  1.7729e-08 ) ergs/cm2

Cutoff power-law model

Time interval is from    0.916 sec. to    1.916 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 0.525822     ( -1.91716   0.972528 )
Epeak [keV] : 105.622      (   )
Norm@50keV  : 1.81233E-02    (     )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          52.43 using 59 PHA bins.
# Reduced chi-squared =         0.9363 for     56 degrees of freedom 
# Null hypothesis probability =   6.107376e-01
 
Photon flux (15-150 keV)    in 1 sec: 0.920366 ( -0.210931  0.209424 ) ph/cm2/s
Energy fluence (15-150 keV)             : 7.6219e-08 ( -1.80505e-08  1.8262e-08 ) ergs/cm2

Band function

Time interval is from    0.916 sec. to    1.916 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -0.606376   ( -0.77245   2.16199 )
beta        : -10.0000    ( 10   0 )
Epeak [keV] : 110.994      ( -45.6669 606.347 )
Norm@50keV   : 1.68348E-02    ( -0.01007   0.0993662 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          52.44 using 59 PHA bins.
# Reduced chi-squared =         0.9535 for     55 degrees of freedom 
# Null hypothesis probability =   5.729223e-01
 
Photon flux (15-150 keV)    in 1 sec: 0.940273 (    ) ph/cm2/s
Energy fluence (15-150 keV)             : 7.63279e-08 ( 0  0 ) ergs/cm2

Single BB

 
Spectral model blackbody:
------------------------------------------------------------
Parameters  : value    Lower 90%  Upper 90%
kT [keV]    : 18.9824  (-4.00848  5.42462)
R^2/D10^2   : 5.24565E-02  (-0.0301878   0.0644236)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          55.08 using 59 PHA bins.
# Reduced chi-squared =         0.9664 for     57 degrees of freedom 
# Null hypothesis probability =   5.473111e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  3.717e-09   1.779e-09
25- 50  1.786e-08   6.087e-09
50-150  4.730e-08   1.920e-08
15-150  6.888e-08   2.473e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 200.000       (      )
Norm        : 3.95838       (-0.827773     0.827708)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          54.47 using 59 PHA bins.
# Reduced chi-squared =         0.9556 for     57 degrees of freedom 
# Null hypothesis probability =   5.705421e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  9.857e-09   5.745e-09
25- 50  1.896e-08   1.102e-08
50-150  4.159e-08   2.419e-08
15-150  7.041e-08   4.147e-08

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 4.75573        (-2.17006      8.09549)
R1^2/D10^2  : 2.88201        (-2.80099      18.4756)
kT2 [keV]   : 22.5424        (-5.6461      14.3598)
R2^2/D10^2  : 2.68374E-02    (-0.0229835   0.0453728)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          51.26 using 59 PHA bins.
# Reduced chi-squared =         0.9320 for     55 degrees of freedom 
# Null hypothesis probability =   6.182343e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  8.207e-09   4.577e-09
25- 50  1.667e-08   9.060e-09
50-150  5.093e-08   2.978e-08
15-150  7.581e-08   4.033e-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: 1.78539     ( -0.3044   0.323164 )
Norm@50keV  : 2.72359E-03    ( -0.000566875   0.000550322 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          47.17 using 59 PHA bins.
# Reduced chi-squared =         0.8275 for     57 degrees of freedom 
# Null hypothesis probability =   8.203205e-01
 
Photon flux (15-150 keV)    in 8.288 sec: 0.373201 ( -0.0667689  0.0667985 ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.07927e-07 ( -4.32647e-08  4.44146e-08 ) ergs/cm2

Cutoff power-law model

Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.30320     ( -1.21354   0.788509 )
Epeak [keV] : 65.6204      ( -50.2363 -65.5337 )
Norm@50keV  : 5.01920E-03    ( -0.00503311   0.0179079 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          46.47 using 59 PHA bins.
# Reduced chi-squared =         0.8299 for     56 degrees of freedom 
# Null hypothesis probability =   8.140274e-01
 
Photon flux (15-150 keV)    in 8.288 sec: 0.367883 ( -0.067484  0.067573 ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.00303e-07 ( -4.51812e-08  4.69399e-08 ) ergs/cm2

Band function

 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -1.31872   ( -1.68667   1.18358 )
beta        : -9.37167    ( 9.37167   19.3717 )
Epeak [keV] : 67.3169      ( -38.5211 -67.3146 )
Norm@50keV   : 4.88981E-03    ( -0.00206653   0.0179859 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          46.48 using 59 PHA bins.
# Reduced chi-squared =         0.8450 for     55 degrees of freedom 
# Null hypothesis probability =   7.865043e-01
 
Photon flux (15-150 keV)    in 8.288 sec: 0.368743 ( 6.63126  -0.065511 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.99249e-07 ( -1.99191e-07  -4.34697e-08 ) ergs/cm2

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

S(25-50 keV)  = 5.82e-08
S(50-100 keV) = 6.76e-08

T90 vs. Hardness ratio plot

T90                                   = 7.28399991989136 sec.
Hardness ratio (energy fluence ratio) = 1.16151

Color vs. Color plot

Count Ratio  (25-50 keV) / (15-25 keV) = 0.805242
Count Ratio (50-100 keV) / (15-25 keV) = 0.737292

Mask shadow pattern

IMX = -2.586676173132431E-01, IMY = 5.331216493044129E-01

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:
-239.544000 -2.960000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
135.5427 -40.5474    1.0  24.9   10.9   2.2412  11.7    0.8	Vela X-1                      
170.2062 -60.6001   26.2   4.6  168.2  -0.0773  -0.4    3.5	Cen X-3                       
186.6561 -62.7860    0.8  12.6  177.6   2.7218  15.2    0.9	GX 301-2                      
156.7784 -18.6250    3.0  41.1   55.9   2.0402   3.8 ------	UNKNOWN                       
179.6549 -68.7470    2.4  12.0 -151.1   0.7711   4.9 ------	UNKNOWN                       
 80.9007 -41.4260    4.3  50.6  -44.7   2.4650   2.7 ------	UNKNOWN                       
 81.6671 -39.1189    3.1  52.0  -42.2   3.3412   3.8 ------	UNKNOWN

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

Time interval of the image:
-2.960000 5.328000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
135.3861 -40.4508   11.6  25.0   10.7  -0.0291  -1.0    9.0	Vela X-1                      
169.9757 -60.7215    6.6   4.5  169.9   0.0460   1.7   11.6	Cen X-3                       
186.2994 -62.9017    0.0  12.4  178.2  -0.0332  -1.2   12.6	GX 301-2                      
210.9721 -33.3879    2.9  41.6  135.9   0.2961   4.0 ------	UNKNOWN                       
204.3173 -61.4376    2.3  20.9  175.9   0.1409   5.1 ------	UNKNOWN                       
 54.3051 -89.0291    1.4  30.6 -115.9   0.3582   8.5 ------	UNKNOWN                       
286.4167 -68.8699    2.5  45.6 -142.1   0.2853   4.6 ------	UNKNOWN

Post-slew image of 15-350 keV band

Time interval of the image:

Plot creation:
Fri Jun 12 02:02:38 EDT 2015