batgrbproduct analysis for trigger=500100

batgrbproduct Analysis for Trigger=500100

Analysis Summary

Notes:

1) No attempt has been made to eliminate the non-significant decimal places.
2) This batgrbproduct analysis is done of the amount of data for this trigger downloaded to date.
3) This batgrbproduct analysis is using the flight position for the mask-weighting calculation.
4) This page will be updated for up to 10 downlinks after the trigger.

======================================================================
                  BAT GRB EVENT DATA PROCESSING REPORT
    Process Script Ver: batgrbproduct v2.46
    Process Start Time (local time): Fri Aug 12 13:17:40 EDT 2011
             Host Name: gcn5
   Current Working Dir: /local/data/raid16/prebascript_archive/trigger500100/GCN5_download_cron
======================================================================

  Trigger: 00500100      Segment: 000

  BAT Trigger Time: 334823891.136   [s; MET]
      Trigger Stop: 334823918.016   [s; MET]
               UTC: 2011-08-12T06:38:03.884040    [includes UTCF correction] 
       Where From?: TDRSS position message

  BAT 
    RA: 135.531579592115   Dec: -40.558481890169  [deg; J2000]

     Catalogged Source?: YES
     Point Source?:      YES
     GRB Indicated?:     NO    [ by BAT flight software ]
     Image S/N Ratio:    16.84
     Image Trigger?:     NO
     Rate S/N Ratio:     31.6701752442262  [ if not an image trigger ]
     Image S/N Ratio:    16.84

  Flight Position:   [ source = BAT ]
    RA: 135.531579592115   Dec: -40.558481890169  [deg; J2000]

  Ground Position:   [ source = BAT pre-slew burst ]
    RA: 135.29803252226   Dec: -40.5245979701403  [deg; J2000]  
        { 09h 01m 11.5s , -40d 31' 28.6" }
         +/- 10.7588915732078 [arcmin] (estimated 90% radius based on SNR)
         +/- 9.25520109534102 [arcmin] (formal 1-sigma fit error)
    SNR: 1.02132688582196
 
  Angular difference between Flight and Ground position is 10.841164 arcmin
 
  Partial Coding Fraction: 0.9609375    [ including projection effects ]

  Duration
     T90: 451.199999988079 +/- 111.338388671289
        Measured from: -170.079999864101
                   to: 281.120000123978     [s; relative to TRIGTIME]
     T50: 92.9919999837875 +/- 176.688833857157
        Measured from: -61.5359998345375
                   to: 31.45600014925     [s; relative to TRIGTIME]



  Fluence
     Peak Flux  (peak 1 second)
        Measured from: 25.3560000061989     
                   to: 26.3560000061989     [s; relative to TRIGTIME]
     Total Fluence        
        Measured from: -181.215999960899     
                   to: 380.896000027657     [s; relative to TRIGTIME]
     
             Band 1     Band 2     Band 3     Band 4
              15-25      25-50     50-100    100-350     keV
 Total     8.326549   5.079895   0.245744   0.095615
           0.113921   0.113603   0.099069   0.090643 [error]
 Peak      0.042638   0.029608   0.003523   0.008060
           0.005101   0.005149   0.004208   0.003715 [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 0.00e+00 0.00e+00 0.00e+00 0.00e+00 0.00e+00 0.00e+00   erg/cm2
              Error 0.00e+00 0.00e+00 0.00e+00 0.00e+00 0.00e+00 0.00e+00   erg/cm2
Peak flux Power-law 3.76e-01 1.96e-01 6.35e-02 2.65e-02 6.50e-01 6.62e-01   ph/cm2/s
              Error 7.58e-02 4.21e-02 2.74e-02 2.04e-02 1.15e-01 1.19e-01   ph/cm2/s
 
Fluence   Cutoff-PL 2.36e-06 2.07e-06 1.16e-07 5.33e-11 4.55e-06 4.55e-06   erg/cm2
              Error 1.95e-07 8.96e-08 3.64e-08 1.04e-10 2.25e-07 2.25e-07   erg/cm2
Peak flux Cutoff-PL 3.61e-01 2.42e-01 2.58e-02 1.83e-04 6.28e-01 6.28e-01   ph/cm2/s
              Error 8.47e-02 6.05e-02 3.25e-02 5.30e-03 1.10e-01 1.10e-01   ph/cm2/s
 
Fluence        Band 0.00e+00 0.00e+00 0.00e+00 0.00e+00 0.00e+00 0.00e+00   erg/cm2
              Error 0.00e+00 0.00e+00 0.00e+00 0.00e+00 0.00e+00 0.00e+00   erg/cm2
Peak flux      Band 0.00e+00 0.00e+00 0.00e+00 0.00e+00 0.00e+00 0.00e+00   ph/cm2/s
              Error 0.00e+00 0.00e+00 0.00e+00 0.00e+00 0.00e+00 0.00e+00   ph/cm2/s

 
=== Time-averaged spectral analysis ===
 
Model Ph_index Ph_90err Epeak  Epeak_90err Norm     Nomr_90err chi2   dof
PL    3.426    0.000    -      -           6.72e-04 0.00e+00  216.110 57
CPL   1.000    0.000      50.0    0.0      2.74e-03 0.00e+00  973.630 56
 
The chi2 of BB fit is 39.55 which shows a significant improvement in the fit over a PL.
Check the BB fit.
 
=== 1-s peak spectral analysis ===
 
Model Ph_index Ph_90err Epeak  Epeak_90err Norm     Nomr_90err chi2   dof
PL    2.626    0.403    -      -           3.06e-03 1.02e-03   78.270 57
CPL  -0.045    3.444      23.3    0.0      2.13e-01 0.00e+00   74.370 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  562.112 -181.216  380.896
T90   451.200 -170.080  281.120
T50    92.992  -61.536   31.456
Peak    1.000   25.356   26.356

Click here for the BAT GCN circular template

Image

Pre-slew 15-350 keV image (Event data; bkg subtracted)

#   RAcent  DECcent POSerr  Theta    Phi     Peak Cts     SNR  Name
  135.2980 -40.5246 0.1887    8.2   94.2       0.3686     1.0  TRIG_00500100       
------------------------------------------
 
Foreground time interval of the image:
-181.216 -56.261 (delta_t = 124.955 [sec])
-55.136  85.565 (delta_t = 140.701 [sec])
Background time interval of the image:
-239.136 -181.216 (delta_t =  57.920 [sec])

Lightcurves

Notes:

1) All plots contain as much data as has been downloaded to date.
2) The mask-weighted light curves are using the flight position.
3) Multiple plots of different time binning/intervals are shown to cover all scenarios of short/long GRBs, rate/image triggers, and real/false positives.
4) 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.
5) 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.
6) 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 26.880000

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 26.880000

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 26.880000

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

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

The mask-weighted light curves based on cleaned DPHs

Spectra

Notes:

1) The fitting includes the systematic errors.
2) For long bursts, a spectral fit of 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.
4) For short bursts (T90<1sec), the specrtum is also fit with Blackbody, OTTB, and Double Blackbody.

Time averaged spectrum fit using the pre-slew DRM

Power-law model

Multiple GTIs in the spectrum
tstart tstop
-181.216000 -56.261500
-55.136000 380.896000
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 3.42589     (     )
Norm@50keV  : 6.72111E-04    (     )
------------------------------------------------------------
# Chi-Squared =         216.11 using 59 PHA bins.
# Reduced chi-squared =         3.7915 for     57 degrees of freedom 
# Null hypothesis probability =   2.313291e-20
 
Photon flux (15-150 keV)    in 561 sec:  (    ) ph/cm2/s
Energy fluence (15-150 keV)             : 0 ( 0  0 ) ergs/cm2

Cutoff power-law model

Multiple GTIs in the spectrum
tstart tstop
-181.216000 -56.261500
-55.136000 380.896000
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.00000     (     )
Epeak [keV] : 50.0000      (   )
Norm@50keV  : 2.73874E-03    (     )
------------------------------------------------------------
# Chi-Squared =         973.63 using 59 PHA bins.
# Reduced chi-squared =         17.386 for     56 degrees of freedom 
# Null hypothesis probability =  1.332707e-167
 
Photon flux (15-150 keV)    in 561 sec: 0.209796 ( -0.012325  0.012418 ) ph/cm2/s
Energy fluence (15-150 keV)             : 4.54864e-06 ( -2.24641e-07  2.26133e-07 ) ergs/cm2

Band function

Multiple GTIs in the spectrum
tstart tstop
-181.216000 -56.261500
-55.136000 380.896000
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : 2.41602   ( -0.709345   1.46024 )
beta        : -7.04217    ( 5.75928   0.0893744 )
Epeak [keV] : 22.5976      ( -1.54679 0.706498 )
Norm@50keV   : 6.22791    ( -7.2628   39.6495 )
------------------------------------------------------------
# Chi-Squared =          37.88 using 59 PHA bins.
# Reduced chi-squared =         0.6887 for     55 degrees of freedom 
# Null hypothesis probability =   9.621416e-01
 
Photon flux (15-150 keV)    in 561 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]    : 5.55764  (-0.166509  0.172453)
R^2/D10^2   : 1.19975  (-0.179111   0.210778)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
# Chi-Squared =          39.55 using 59 PHA bins.
# Reduced chi-squared =         0.6938 for     57 degrees of freedom 
# Null hypothesis probability =   9.620621e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  2.454e-06   1.456e-07
25- 50  2.061e-06   8.920e-08
50-150  1.364e-07   2.121e-08
15-150  4.651e-06   1.753e-07

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 14.8752       (-0.822895      0.892144)
Norm        : 4.46776       (-0.467567     0.524182)
------------------------------------------------------------
# Chi-Squared =          93.87 using 59 PHA bins.
# Reduced chi-squared =          1.647 for     57 degrees of freedom 
# Null hypothesis probability =   1.518474e-03
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  2.884e-06   1.534e-07
25- 50  1.950e-06   8.527e-08
50-150  3.377e-07   5.167e-08
15-150  5.171e-06   1.905e-07

Double BB

------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 199.984        (      )
R1^2/D10^2  : 3.56305E-07        (-3.56305e-07      1.66143e-06)
kT2 [keV]   : 5.55009        (-0.169515      0.175942)
R2^2/D10^2  : 1.20709    (-0.182746   0.215501)
------------------------------------------------------------
# Chi-Squared =          39.55 using 59 PHA bins.
# Chi-Squared =          39.42 using 59 PHA bins.
# Reduced chi-squared =         0.7191 for     55 degrees of freedom 
# Reduced chi-squared =         0.7168 for     55 degrees of freedom 
# Null hypothesis probability =   9.422793e-01
# Null hypothesis probability =   9.439711e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  2.454e-06   8.224e+02
25- 50  2.061e-06   7.635e+03
50-150  1.364e-07   1.856e+05
15-150  4.651e-06   1.783e+05

Peak spectrum fit

Power-law model

Time interval is from   25.356 sec. to   26.356 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 2.62646     ( -0.370715   0.436147 )
Norm@50keV  : 3.05535E-03    ( -0.00100119   0.00103154 )
------------------------------------------------------------
# Chi-Squared =          78.27 using 59 PHA bins.
# Reduced chi-squared =          1.373 for     57 degrees of freedom 
# Null hypothesis probability =   3.227554e-02
 
Photon flux (15-150 keV)    in 1 sec: 0.649890 ( -0.114835  0.115068 ) ph/cm2/s
Energy fluence (15-150 keV)             : 3.17123e-08 ( -7.20353e-09  7.76502e-09 ) ergs/cm2

Cutoff power-law model

Time interval is from   25.356 sec. to   26.356 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: -4.46030E-02     ( -4.63133   2.25596 )
Epeak [keV] : 23.3133      (   )
Norm@50keV  : 0.213145    (     )
------------------------------------------------------------
# Chi-Squared =          74.37 using 59 PHA bins.
# Reduced chi-squared =          1.328 for     56 degrees of freedom 
# Null hypothesis probability =   5.080681e-02
 
Photon flux (15-150 keV)    in 1 sec: 0.628285 ( -0.110118  0.110794 ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.65718e-08 ( -5.3326e-09  6.3252e-09 ) ergs/cm2

Band function

Time interval is from   25.356 sec. to   26.356 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : 0.944749   ( -2.23374   -0.965868 )
beta        : -8.30421    ( 6.56136   16.5578 )
Epeak [keV] : 24.8353      ( -6.43435 4.96248 )
Norm@50keV   : 0.900808    ( -0.900822   570.555 )
------------------------------------------------------------
# Chi-Squared =          74.31 using 59 PHA bins.
# Reduced chi-squared =          1.351 for     55 degrees of freedom 
# Null hypothesis probability =   4.241588e-02
 
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]    : 6.56755  (-1.0214  1.15442)
R^2/D10^2   : 1.69365  (-0.840326   1.76422)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
# Chi-Squared =          74.51 using 59 PHA bins.
# Reduced chi-squared =          1.307 for     57 degrees of freedom 
# Null hypothesis probability =   5.959895e-02
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.093e-08   3.413e-09
25- 50  1.319e-08   4.320e-09
50-150  1.725e-09   1.071e-09
15-150  2.584e-08   7.545e-09

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 24.6816       (-7.62946      12.4347)
Norm        : 6.34906       (-2.03494     3.25504)
------------------------------------------------------------
# Chi-Squared =          75.57 using 59 PHA bins.
# Reduced chi-squared =          1.326 for     57 degrees of freedom 
# Null hypothesis probability =   5.041119e-02
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.153e-08   2.745e-09
25- 50  1.172e-08   3.193e-09
50-150  4.891e-09   3.372e-09
15-150  2.814e-08   8.400e-09

Double BB

R1^2/D10^2  : 1.88797        (      )
kT2 [keV]   : 185.156        (      )
R2^2/D10^2  : 3.18275E-05    (-3.13761e-05   2.76627)
------------------------------------------------------------
# Chi-Squared =          73.31 using 59 PHA bins.
# Chi-Squared =          73.20 using 59 PHA bins.
# Chi-Squared =          73.12 using 59 PHA bins.
# Reduced chi-squared =          1.333 for     55 degrees of freedom 
# Reduced chi-squared =          1.331 for     55 degrees of freedom 
# Reduced chi-squared =          1.329 for     55 degrees of freedom 
# Null hypothesis probability =   5.003242e-02
# Null hypothesis probability =   5.095351e-02
# Null hypothesis probability =   5.156734e-02
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.087e-08   5.855e-09
25- 50  1.320e-08   7.715e-09
50-150  2.226e-09   1.581e-09
15-150  2.630e-08   1.484e-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: 3.30014     (     )
Norm@50keV  : 7.40685E-04    (     )
------------------------------------------------------------
# Chi-Squared =         183.00 using 59 PHA bins.
# Reduced chi-squared =         3.2105 for     57 degrees of freedom 
# Null hypothesis probability =   3.940365e-15
 
Photon flux (15-150 keV)    in 265.7 sec:  (    ) ph/cm2/s
Energy fluence (15-150 keV)             : 0 ( 0  0 ) ergs/cm2

Cutoff power-law model

Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.00000     (     )
Epeak [keV] : 50.0000      (   )
Norm@50keV  : 3.18268E-03    (     )
------------------------------------------------------------
# Chi-Squared =         659.20 using 59 PHA bins.
# Reduced chi-squared =         11.771 for     56 degrees of freedom 
# Null hypothesis probability =  6.957564e-104
 
Photon flux (15-150 keV)    in 265.7 sec: 0.217249 ( -0.013647  0.013705 ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.22597e-06 ( -1.22488e-07  1.23519e-07 ) ergs/cm2

Band function

 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : 3.01437   ( -0.982145   1.64638 )
beta        : -7.44036    ( 5.73984   0.201329 )
Epeak [keV] : 23.0432      ( -1.59673 0.901766 )
Norm@50keV   : 17.3819    ( -17.3842   119.726 )
------------------------------------------------------------
# Chi-Squared =          54.90 using 59 PHA bins.
# Reduced chi-squared =         0.9982 for     55 degrees of freedom 
# Null hypothesis probability =   4.783557e-01
 
Photon flux (15-150 keV)    in 265.7 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)  = 
S(50-100 keV) =

T90 vs. Hardness ratio plot

T90                                   = 451.199999988079 sec.
Hardness ratio (energy fluence ratio) =

Color vs. Color plot

Count Ratio  (25-50 keV) / (15-25 keV) = 0.610084
Count Ratio (50-100 keV) / (15-25 keV) = 0.0295133

Mask shadow pattern

IMX = -1.062384972716201E-02, IMY = -1.437822354218976E-01

TIME vs. PHA plot around the trigger time

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 26.880000

TIME vs. DetID plot around the trigger time

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 26.880000

100 us light curve (15-350 keV)

Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 26.880000

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:
-239.136000 -181.216000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
135.5508 -40.5370    1.1   8.2   92.9   0.7602  10.3    1.5	Vela X-1                      
170.3024 -60.6408    7.2  35.9   61.3   0.2768   1.6    1.1	Cen X-3                       
 80.2046 -14.8589    2.3  53.6 -175.6   1.1266   5.0 ------	UNKNOWN                       
 97.7864 -14.8656    2.2  39.0 -163.4   0.5594   5.2 ------	UNKNOWN                       
108.6435   7.7593    2.2  48.0 -129.0   1.7078   5.2 ------	UNKNOWN

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

Time interval of the image:
-181.216000 -56.261500
-55.136000 85.564600
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
135.3339 -40.5314    9.5   8.2   94.0   0.4275   1.2    9.0	Vela X-1                      
170.5694 -60.5893   19.0  36.0   61.1  -0.5024  -0.6    7.7	Cen X-3                       
136.7503 -40.5380    1.8   8.2   86.5   2.2363   6.3 ------	UNKNOWN                       
 74.7175 -16.8541    2.7  57.3  179.1   8.7450   4.3 ------	UNKNOWN

Post-slew image of 15-350 keV band

Time interval of the image:
113.764600 422.917900
540.864000 602.967300
780.864000 842.975200
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
135.5261 -40.5599    0.3   0.0  122.4  11.0134  42.7    0.3	Vela X-1                      
170.5311 -60.6257    8.0  29.3   48.0   0.5068   1.4    6.3	Cen X-3                       
186.6195 -62.8008    2.9  37.2   47.0   2.0748   4.0    2.1	GX 301-2                      
148.8314 -37.5011    2.3  10.7  -19.1   1.2934   4.9 ------	UNKNOWN                       
103.7570 -24.2947    2.3  31.1 -165.3   1.3807   5.1 ------	UNKNOWN                       
176.8598 -14.1910    2.7  44.5  -31.1   2.1653   4.3 ------	UNKNOWN

Plot creation:
Fri Aug 12 13:35:25 EDT 2011