batgrbproduct analysis for trigger=303631

batgrbproduct Analysis for Trigger=303631

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 04:15:28 EST 2014
             Host Name: batevent1
   Current Working Dir: /local/data/batevent/batevent_reproc/trigger303631
======================================================================

  Trigger: 00303631      Segment: 000

  BAT Trigger Time: 225071869.76   [s; MET]
      Trigger Stop: 225071873.856   [s; MET]
               UTC: 2008-02-18T23:57:47.175420    [includes UTCF correction] 
       Where From?: TDRSS position message

  BAT 
    RA: 177.951347600546   Dec: -53.1004105987458  [deg; J2000]

     Catalogged Source?: NO
     Point Source?:      YES
     GRB Indicated?:     YES    [ by BAT flight software ]
     Image S/N Ratio:    7.25
     Image Trigger?:     NO
     Rate S/N Ratio:     11.7898261225516  [ if not an image trigger ]
     Image S/N Ratio:    7.25

  Flight Position:   [ source = BAT ]
    RA: 177.951347600546   Dec: -53.1004105987458  [deg; J2000]

  Ground Position:   [ source = BAT pre-slew burst ]
    RA: 177.927442200414   Dec: -53.0870378471626  [deg; J2000]  
        { 11h 51m 42.6s , -53d 05' 13.3" }
         +/- 2.01258624932174 [arcmin] (estimated 90% radius based on SNR)
         +/- 1.39361482228635 [arcmin] (formal 1-sigma fit error)
    SNR: 11.1991065960042
 
  Angular difference between Flight and Ground position is 1.177143 arcmin
 
  Partial Coding Fraction: 0.1015625    [ including projection effects ]

  Duration
     T90: 6.5280000269413 +/- 1.42857693147711
        Measured from: -0.527999997138977
                   to: 6.00000002980232     [s; relative to TRIGTIME]
     T50: 2.94400000572205 +/- 1.20245082782922
        Measured from: 0.432000011205673
                   to: 3.37600001692772     [s; relative to TRIGTIME]



  Fluence
     Peak Flux  (peak 1 second)
        Measured from: 0.412000000476837     
                   to: 1.41200000047684     [s; relative to TRIGTIME]
     Total Fluence        
        Measured from: -0.84799998998642     
                   to: 6.57600000500679     [s; relative to TRIGTIME]
     
             Band 1     Band 2     Band 3     Band 4
              15-25      25-50     50-100    100-350     keV
 Total     0.482757   0.531959   0.097956   0.055327
           0.055665   0.059159   0.048200   0.041815 [error]
 Peak      0.123463   0.108841   0.054071   0.011913
           0.021487   0.023340   0.019477   0.015681 [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 2.08e-07 2.05e-07 1.42e-07 1.55e-07 6.17e-07 7.10e-07   erg/cm2
              Error 3.36e-08 3.12e-08 4.08e-08 8.18e-08 1.01e-07 1.46e-07   erg/cm2
Peak flux Power-law 1.71e+00 6.23e-01 1.30e-01 3.21e-02 2.49e+00 2.50e+00   ph/cm2/s
              Error 4.26e-01 1.53e-01 5.18e-02 2.06e-02 5.68e-01 5.69e-01   ph/cm2/s
 
Fluence   Cutoff-PL 1.93e-07 2.64e-07 3.92e-08 1.55e-10 4.96e-07 4.96e-07   erg/cm2
              Error 3.83e-08 4.68e-08 4.82e-08 4.73e-09 8.52e-08 8.52e-08   erg/cm2
Peak flux Cutoff-PL 1.52e+00 1.06e+00 1.94e-01 6.04e-03 2.79e+00 2.79e+00   ph/cm2/s
              Error 4.74e-01 3.12e-01 1.47e-01 9.66e-03 5.96e-01 5.96e-01   ph/cm2/s
 
Fluence        Band -------- -------- -------- -------- -------- --------   erg/cm2
              Error -------- -------- -------- -------- -------- --------   erg/cm2
Peak flux      Band -------- -------- -------- -------- -------- --------   ph/cm2/s
              Error -------- -------- -------- -------- -------- --------   ph/cm2/s

 
=== Time-averaged spectral analysis ===
 
Model Ph_index Ph_90err Epeak  Epeak_90err Norm     Nomr_90err chi2   dof
PL    2.531    0.271    -      -           8.24e-03 1.77e-03   61.840 57
CPL  -2.238    3.499      27.4    4.6      1.43e+01 0.00e+00   50.890 56
 
 
=== 1-s peak spectral analysis ===
 
Model Ph_index Ph_90err Epeak  Epeak_90err Norm     Nomr_90err chi2   dof
PL    3.264    0.363    -      -           7.42e-03 2.47e-03   54.630 57
CPL   0.409    1.883      24.4    0.0      3.72e-01 0.00e+00   46.740 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    7.424   -0.848    6.576
T90     6.528   -0.528    6.000
T50     2.944    0.432    3.376
Peak    1.000    0.412    1.412

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
  177.9274   -53.0870   0.0172    45.6740   140.4691         1.1752033     11.199 TRIG_00303631                 
 
Foreground time interval of the image:
 -0.848   6.576 (delta_t =   7.424 [sec])
Background time interval of the image:
-239.760  -0.848 (delta_t = 238.912 [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

8 ms binning

From T100_start-3 s to T100_start+3 s

2 ms binning

From T100_start-1 s to T100_start+1 s

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

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

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

Spectral Evolution

Spectra

Notes:

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

Time averaged spectrum fit using the average DRM

Power-law model

Time interval is from   -0.848 sec. to    6.576 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 2.53099     ( -0.256229   0.285377 )
Norm@50keV  : 8.23885E-03    ( -0.0017745   0.00176813 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          61.84 using 59 PHA bins.
# Reduced chi-squared =          1.085 for     57 degrees of freedom 
# Null hypothesis probability =   3.074100e-01
 
Photon flux (15-150 keV)    in 7.424 sec: 1.64970 ( -0.222778  0.222781 ) ph/cm2/s
Energy fluence (15-150 keV)             : 6.1685e-07 ( -9.91446e-08  1.02553e-07 ) ergs/cm2

Cutoff power-law model

Time interval is from   -0.848 sec. to    6.576 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: -2.23768     ( -4.83104   2.16725 )
Epeak [keV] : 27.3693      ( -5.439 3.66893 )
Norm@50keV  : 14.3078    (     )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          50.89 using 59 PHA bins.
# Reduced chi-squared =         0.9088 for     56 degrees of freedom 
# Null hypothesis probability =   6.680701e-01
 
Photon flux (15-150 keV)    in 7.424 sec: 1.55004 ( -0.22194  0.22365 ) ph/cm2/s
Energy fluence (15-150 keV)             : 4.96435e-07 ( -7.85244e-08  9.1777e-08 ) ergs/cm2

Band function

Time interval is from   -0.848 sec. to    6.576 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : 2.28903   ( -0.517742   0.225335 )
beta        : -10.0000    ( 10   3.78314e-07 )
Epeak [keV] : 27.2252      ( -3.32352 3.67695 )
Norm@50keV   : 15.9633    ( -2.08023   501.939 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          50.90 using 59 PHA bins.
# Reduced chi-squared =         0.9254 for     55 degrees of freedom 
# Null hypothesis probability =   6.320852e-01
 
Photon flux (15-150 keV)    in 7.424 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]    : 6.96524  (-0.804352  0.907082)
R^2/D10^2   : 3.37218  (-1.36728   2.29418)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          50.98 using 59 PHA bins.
# Reduced chi-squared =         0.8943 for     57 degrees of freedom 
# Null hypothesis probability =   6.992421e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.941e-07   4.198e-08
25- 50  2.633e-07   5.241e-08
50-150  4.285e-08   1.961e-08
15-150  5.002e-07   9.351e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 29.1218       (-7.20753      10.3861)
Norm        : 13.9097       (-3.39561     4.71509)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          55.16 using 59 PHA bins.
# Reduced chi-squared =         0.9677 for     57 degrees of freedom 
# Null hypothesis probability =   5.444778e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  2.069e-07   3.560e-08
25- 50  2.326e-07   4.391e-08
50-150  1.224e-07   5.485e-08
15-150  5.619e-07   1.076e-07

Double BB

------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 6.61955        (-6.68898      0.491005)
R1^2/D10^2  : 3.98310        (-1.6343      4.25207)
kT2 [keV]   : 27.6812        (-27.8459      -27.8459)
R2^2/D10^2  : 2.69221E-03    (   )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          49.51 using 59 PHA bins.
#Fit statistic : Chi-Squared =          49.48 using 59 PHA bins.
# Reduced chi-squared =         0.9002 for     55 degrees of freedom 
# Reduced chi-squared =         0.8997 for     55 degrees of freedom 
# Null hypothesis probability =   6.835916e-01
# Null hypothesis probability =   6.845525e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.970e-07   4.907e-08
25- 50  2.565e-07   8.044e-08
50-150  1.163e-07   5.247e-08
15-150  5.698e-07   1.507e-07

Peak spectrum fit

Power-law model

Time interval is from    0.412 sec. to    1.412 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 3.26400     ( -0.313263   0.413049 )
Norm@50keV  : 7.41514E-03    ( -0.00253738   0.00240295 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          54.63 using 59 PHA bins.
# Reduced chi-squared =         0.9584 for     57 degrees of freedom 
# Null hypothesis probability =   5.646130e-01
 
Photon flux (15-150 keV)    in 1 sec: 2.48684 ( -0.56755  0.56757 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.01754e-07 ( -2.37053e-08  2.36959e-08 ) ergs/cm2

Cutoff power-law model

Time interval is from    0.412 sec. to    1.412 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 0.408938     ( -2.17274   1.59348 )
Epeak [keV] : 24.4286      (   )
Norm@50keV  : 0.372416    (     )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          46.74 using 59 PHA bins.
# Reduced chi-squared =         0.8346 for     56 degrees of freedom 
# Null hypothesis probability =   8.063577e-01
 
Photon flux (15-150 keV)    in 1 sec: 2.78811 ( -0.59544  0.59576 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.25151e-07 ( -2.79905e-08  2.8151e-08 ) ergs/cm2

Band function

Time interval is from    0.412 sec. to    1.412 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -0.156119   ( -1.17446   4.82973 )
beta        : -9.23415    ( 9.08822   18.2578 )
Epeak [keV] : 25.9128      ( -6.71283 8.49435 )
Norm@50keV   : 0.518747    ( -0.436625   1253.18 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          46.79 using 59 PHA bins.
# Reduced chi-squared =         0.8508 for     55 degrees of freedom 
# Null hypothesis probability =   7.765881e-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]    : 7.56837  (-1.85568  1.90813)
R^2/D10^2   : 4.12306  (-2.51016   8.94074)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          49.37 using 59 PHA bins.
# Reduced chi-squared =         0.8662 for     57 degrees of freedom 
# Null hypothesis probability =   7.535211e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  4.085e-08   1.824e-08
25- 50  6.479e-08   2.514e-08
50-150  1.413e-08   8.938e-09
15-150  1.198e-07   4.732e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 23.6195       (-6.11409      6.1509)
Norm        : 28.7728       (-8.82038     13.1754)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          47.60 using 59 PHA bins.
# Reduced chi-squared =         0.8350 for     57 degrees of freedom 
# Null hypothesis probability =   8.081232e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  5.072e-08   1.299e-08
25- 50  5.008e-08   1.150e-08
50-150  1.957e-08   9.931e-09
15-150  1.204e-07   3.161e-08

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 3.97150        (-3.97076      -3.9715)
R1^2/D10^2  : 32.2479        (-31.0416      -32.2479)
kT2 [keV]   : 9.82065        (-2.81357      -9.82062)
R2^2/D10^2  : 0.988717    (-0.988733   3.76161)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          46.43 using 59 PHA bins.
# Reduced chi-squared =         0.8442 for     55 degrees of freedom 
# Null hypothesis probability =   7.879662e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  4.762e-08   2.803e-08
25- 50  5.677e-08   3.442e-08
50-150  2.327e-08   1.595e-08
15-150  1.277e-07   7.015e-08

Pre-slew spectrum (Pre-slew PHA with pre-slew DRM)

Power-law model

 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 2.53099     ( -0.256229   0.285377 )
Norm@50keV  : 8.23885E-03    ( -0.0017745   0.00176813 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          61.84 using 59 PHA bins.
# Reduced chi-squared =          1.085 for     57 degrees of freedom 
# Null hypothesis probability =   3.074100e-01
 
Photon flux (15-150 keV)    in 7.424 sec: 1.64970 ( -0.222778  0.222781 ) ph/cm2/s
Energy fluence (15-150 keV)             : 6.1685e-07 ( -9.91446e-08  1.02553e-07 ) ergs/cm2

Cutoff power-law model

Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: -2.23768     ( -4.83104   2.16725 )
Epeak [keV] : 27.3693      ( -5.439 3.66893 )
Norm@50keV  : 14.3078    (     )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          50.89 using 59 PHA bins.
# Reduced chi-squared =         0.9088 for     56 degrees of freedom 
# Null hypothesis probability =   6.680701e-01
 
Photon flux (15-150 keV)    in 7.424 sec: 1.55004 ( -0.22194  0.22365 ) ph/cm2/s
Energy fluence (15-150 keV)             : 4.96435e-07 ( -7.85244e-08  9.1777e-08 ) ergs/cm2

Band function

 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : 2.28903   ( -0.517742   0.225335 )
beta        : -10.0000    ( 10   3.78314e-07 )
Epeak [keV] : 27.2252      ( -3.32352 3.67695 )
Norm@50keV   : 15.9633    ( -2.08023   501.907 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          50.90 using 59 PHA bins.
# Reduced chi-squared =         0.9254 for     55 degrees of freedom 
# Null hypothesis probability =   6.320852e-01
 
Photon flux (15-150 keV)    in 7.424 sec:  (    ) ph/cm2/s
Energy fluence (15-150 keV)             : 0 ( 0  0 ) ergs/cm2

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

S(25-50 keV)  = 2.05e-07
S(50-100 keV) = 1.42e-07

T90 vs. Hardness ratio plot

T90                                   = 6.5280000269413 sec.
Hardness ratio (energy fluence ratio) = 0.692683

Color vs. Color plot

Count Ratio  (25-50 keV) / (15-25 keV) = 1.10192
Count Ratio (50-100 keV) / (15-25 keV) = 0.20291

Mask shadow pattern

IMX = -7.896449343651111E-01, IMY = -6.516477441098890E-01

TIME vs. PHA plot around the trigger time

TIME vs. DetID plot around the trigger time

100 us light curve (15-350 keV)

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:
-239.760000 -0.848000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
170.0455 -60.6471    5.8  37.0  140.8   1.1276   2.0    8.1	Cen X-3                       
186.1975 -62.7389    0.0  39.3  153.0  -0.9960  -1.9   12.8	GX 301-2                      
109.6942 -36.0917    4.0  39.1   64.4   2.7340   2.9 ------	UNKNOWN                       
184.7981 -50.2344    2.7  50.1  143.9   6.0223   4.3 ------	UNKNOWN                       
 73.3186 -21.1485    2.8  48.8   15.0   2.9833   4.1 ------	UNKNOWN                       
206.3529 -63.4004    2.4  42.7  166.0   2.5363   4.8 ------	UNKNOWN                       
 58.9000 -23.9173    2.6  46.8   -3.2   2.5423   4.5 ------	UNKNOWN                       
245.9646 -53.6892    2.7  56.2 -170.4   4.6671   4.3 ------	UNKNOWN                       
280.9373 -53.1322    3.0  55.2 -145.3   6.4991   3.8 ------	UNKNOWN                       
 21.2231 -30.9782    4.0  48.3  -49.8   3.8985   2.9 ------	UNKNOWN

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

Time interval of the image:
-0.848000 6.576000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
170.1368 -60.7734    0.0  36.9  140.9   0.1052   1.8   10.4	Cen X-3                       
186.6124 -62.6592    4.4  39.5  153.2  -0.1351  -2.6    6.8	GX 301-2                      
177.9275 -53.0871    1.0  45.7  140.5   1.1741  11.2 ------	UNKNOWN                       
 65.4434 -15.5860    2.3  54.6    5.6   0.6821   5.1 ------	UNKNOWN                       
280.0246 -53.0497    2.5  55.4 -146.0   0.6800   4.6 ------	UNKNOWN                       
 31.3597 -20.5842    2.1  55.3  -34.6   0.8333   5.4 ------	UNKNOWN                       
  0.0620 -46.8166    2.5  41.1  -80.7   0.4832   4.6 ------	UNKNOWN

Post-slew image of 15-350 keV band

Time interval of the image:
98.940600 962.340000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
135.5099 -40.5754    0.8  31.0   34.3   8.9700  13.7    1.5	Vela X-1                      
170.5279 -60.6649    2.6   8.6  -37.0   2.5080   4.5    6.7	Cen X-3                       
186.8501 -62.6407   16.8  10.6  -84.9   0.3516   0.7    9.4	GX 301-2                      
100.0829 -41.3354    3.2  51.5    7.6   5.7162   3.6 ------	UNKNOWN                       
226.4943 -11.2543    4.7  56.9  179.2   8.9368   2.5 ------	UNKNOWN                       
236.8705 -65.6079    3.3  31.1 -105.4   3.0644   3.6 ------	UNKNOWN

Plot creation:
Sun May 31 08:17:32 EDT 2015