batgrbproduct analysis for trigger=509717

batgrbproduct Analysis for Trigger=509717

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 17:05:31 EST 2014
             Host Name: batevent1
   Current Working Dir: /local/data/batevent/batevent_reproc/trigger509717
======================================================================

  Trigger: 00509717      Segment: 000

  BAT Trigger Time: 345650656   [s; MET]
      Trigger Stop: 345650976   [s; MET]
               UTC: 2011-12-15T14:04:08.321280    [includes UTCF correction] 
       Where From?: TDRSS position message

  BAT 
    RA: 349.548231274995   Dec: 32.475567914634  [deg; J2000]

     Catalogged Source?: NO
     Point Source?:      YES
     GRB Indicated?:     NO    [ by BAT flight software ]
     Image S/N Ratio:    8.16
     Image Trigger?:     YES
     Rate S/N Ratio:     0  [ if not an image trigger ]
     Image S/N Ratio:    8.16

  Flight Position:   [ source = BAT ]
    RA: 349.548231274995   Dec: 32.475567914634  [deg; J2000]

  Ground Position:   [ source = BAT pre-slew burst ]
    RA: 349.548   Dec: 32.4756  [deg; J2000]
        { 23h 18m 11.5s , +32d 28' 32.2" }
        +/- 2.45235028722 [arcmin] (estimated 90% radius based on SNR)
    SNR: 8.44556606931
 
 
  Angular difference between Flight and Ground position is 0.011864 arcmin
 
  Partial Coding Fraction: 0.4648438    [ including projection effects ]

  Duration
     T90: 373.819999992847 +/- 93.2202465729463
        Measured from: 7.60399997234344
                   to: 381.423999965191     [s; relative to TRIGTIME]
     T50: 154.979999959469 +/- 110.461724542731
        Measured from: 129.431999981403
                   to: 284.411999940872     [s; relative to TRIGTIME]



  Fluence
     Peak Flux  (peak 1 second)
        Measured from: 216.347999989986     
                   to: 217.347999989986     [s; relative to TRIGTIME]
     Total Fluence        
        Measured from: 1.61599999666214     
                   to: 411.019999980927     [s; relative to TRIGTIME]
     
             Band 1     Band 2     Band 3     Band 4
              15-25      25-50     50-100    100-350     keV
 Total     1.302848   1.429054   1.185111   0.260853
           0.169394   0.175700   0.159015   0.146620 [error]
 Peak      0.016779   0.017615   0.024819   0.014824
           0.008662   0.008769   0.007763   0.007037 [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 4.09e-07 7.04e-07 9.26e-07 2.48e-06 2.71e-06 4.51e-06   erg/cm2
              Error 7.94e-08 8.76e-08 1.55e-07 8.63e-07 3.74e-07 9.98e-07   erg/cm2
Peak flux Power-law 1.51e-01 1.63e-01 1.25e-01 1.56e-01 4.98e-01 5.95e-01   ph/cm2/s
              Error 1.18e-01 1.21e-01 9.31e-02 1.90e-01 2.26e-01 2.58e-01   ph/cm2/s
 
Fluence   Cutoff-PL 3.87e-07 7.45e-07 9.41e-07 1.22e-06 2.61e-06 3.29e-06   erg/cm2
              Error 8.75e-08 1.10e-07 1.69e-07 1.74e-06 4.11e-07 1.30e-06   erg/cm2
Peak flux Cutoff-PL 1.30e-01 1.70e-01 1.34e-01 8.97e-02 4.84e-01 5.24e-01   ph/cm2/s
              Error 1.40e-01 1.32e-01 7.59e-02 1.66e-01 2.39e-01 2.65e-01   ph/cm2/s
 
Fluence        Band 3.89e-07 7.87e-07 8.77e-07 1.84e-06 2.62e-06 3.91e-06   erg/cm2
              Error -------- 1.14e-07 -------- -------- -------- --------   erg/cm2
Peak flux      Band 1.35e-01 1.67e-01 1.32e-01 1.07e-01 4.89e-01 5.42e-01   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    1.605    0.208    -      -           7.08e-04 9.09e-05   64.710 57
CPL   1.156    0.642      87.9  -24.0      1.23e-03 1.43e-03   63.570 56
 
 
=== 1-s peak spectral analysis ===
 
Model Ph_index Ph_90err Epeak  Epeak_90err Norm     Nomr_90err chi2   dof
PL    1.385    0.793    -      -           4.10e-03 1.77e-03   48.420 57
CPL   0.757    3.679     109.2    0.0      8.03e-03 4.07e+00   48.250 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  409.404    1.616  411.020
T90   373.820    7.604  381.424
T50   154.980  129.432  284.412
Peak    1.000  216.348  217.348

Click here for the BAT GCN circular template

Special notes of this burst

Image

Pre-slew 15.0-50.0 keV image (Event data)

#RAcent DECcent POSerr Theta  Phi  Peak_Cts  SNR Name
349.548 32.476 0.000 42.307 -26.439 2.447 8.446 TRIG_00509717
 
Image time interval: 0.000 to 320.000 [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)

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    1.616 sec. to  411.020 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.60499     ( -0.206021   0.209392 )
Norm@50keV  : 7.08415E-04    ( -9.14009e-05   9.04605e-05 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          64.71 using 59 PHA bins.
# Reduced chi-squared =          1.135 for     57 degrees of freedom 
# Null hypothesis probability =   2.256178e-01
 
Photon flux (15-150 keV)    in 409.4 sec: 9.11760E-02 ( -0.0112507  0.011265 ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.71072e-06 ( -3.71874e-07  3.76862e-07 ) ergs/cm2

Cutoff power-law model

Time interval is from    1.616 sec. to  411.020 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.15569     ( -0.852304   0.432269 )
Epeak [keV] : 87.8852      ( -39.8911 -87.8758 )
Norm@50keV  : 1.23495E-03    ( -0.000594941   0.0022604 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          63.57 using 59 PHA bins.
# Reduced chi-squared =          1.135 for     56 degrees of freedom 
# Null hypothesis probability =   2.273739e-01
 
Photon flux (15-150 keV)    in 409.4 sec: 8.97289E-02 ( -0.0114571  0.0114851 ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.60848e-06 ( -4.1019e-07  4.115e-07 ) ergs/cm2

Band function

Time interval is from    1.616 sec. to  411.020 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -1.15213   ( -0.577843   0.810551 )
beta        : -10.0000    ( 10   0 )
Epeak [keV] : 87.5936      ( -33.7295 -87.5938 )
Norm@50keV   : 1.23988E-03    ( -0.000599776   0.00225829 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          63.57 using 59 PHA bins.
# Reduced chi-squared =          1.156 for     55 degrees of freedom 
# Null hypothesis probability =   2.002427e-01
 
Photon flux (15-150 keV)    in 409.4 sec: 8.95788E-02 ( 6.91042  -0.01125 ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.61824e-06 ( 0  0 ) ergs/cm2

Single BB

 
Spectral model blackbody:
------------------------------------------------------------
Parameters  : value    Lower 90%  Upper 90%
kT [keV]    : 12.7094  (-2.10428  2.63155)
R^2/D10^2   : 1.81217E-02  (-0.00882783   0.016817)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          80.96 using 59 PHA bins.
# Reduced chi-squared =          1.420 for     57 degrees of freedom 
# Null hypothesis probability =   2.017554e-02
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  2.542e-07   5.818e-08
25- 50  8.540e-07   1.494e-07
50-150  8.604e-07   2.348e-07
15-150  1.969e-06   3.441e-07

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 161.295       (-67.0263      -160.156)
Norm        : 0.377662       (-0.0497957     0.0599827)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          63.57 using 59 PHA bins.
# Reduced chi-squared =          1.115 for     57 degrees of freedom 
# Null hypothesis probability =   2.561962e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  3.945e-07   2.186e-07
25- 50  7.388e-07   3.855e-07
50-150  1.501e-06   8.601e-07
15-150  2.635e-06   1.449e-06

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 6.95900        (-1.48385      1.01667)
R1^2/D10^2  : 0.115972        (-0.0646755      0.154324)
kT2 [keV]   : 27.9422        (-7.92701      17.8423)
R2^2/D10^2  : 8.27998E-04    (-0.000645281   0.00114866)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          58.54 using 59 PHA bins.
# Reduced chi-squared =          1.064 for     55 degrees of freedom 
# Null hypothesis probability =   3.468653e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  4.103e-07   1.950e-07
25- 50  7.556e-07   3.367e-07
50-150  1.542e-06   8.440e-07
15-150  2.708e-06   1.351e-06

Peak spectrum fit

Power-law model

Time interval is from  216.348 sec. to  217.348 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.38511     ( -0.805627   0.780848 )
Norm@50keV  : 4.10487E-03    ( -0.00176925   0.00176695 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          48.42 using 59 PHA bins.
# Reduced chi-squared =         0.8494 for     57 degrees of freedom 
# Null hypothesis probability =   7.837407e-01
 
Photon flux (15-150 keV)    in 1 sec: 0.498234 ( -0.223904  0.227777 ) ph/cm2/s
Energy fluence (15-150 keV)             : 3.97867e-08 ( -1.80748e-08  1.8476e-08 ) ergs/cm2

Cutoff power-law model

Time interval is from  216.348 sec. to  217.348 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 0.756873     ( -0.757972   6.60004 )
Epeak [keV] : 109.247      ( -109.347 -109.347 )
Norm@50keV  : 8.02976E-03    ( -0.00802124   8.13581 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          48.25 using 59 PHA bins.
# Reduced chi-squared =         0.8617 for     56 degrees of freedom 
# Null hypothesis probability =   7.595500e-01
 
Photon flux (15-150 keV)    in 1 sec: 0.484408 ( -0.244209  0.233883 ) ph/cm2/s
Energy fluence (15-150 keV)             : 3.87712e-08 ( -1.83727e-08  1.89731e-08 ) ergs/cm2

Band function

Time interval is from  216.348 sec. to  217.348 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -0.750569   ( -3.73886   0.845187 )
beta        : -10.0000    ( 10   10 )
Epeak [keV] : 108.339      ( -69.7784 -108.448 )
Norm@50keV   : 8.10377E-03    ( -0.00809561   0.911542 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          48.25 using 59 PHA bins.
# Reduced chi-squared =         0.8774 for     55 degrees of freedom 
# Null hypothesis probability =   7.281517e-01
 
Photon flux (15-150 keV)    in 1 sec: 0.488924 (    ) ph/cm2/s
Energy fluence (15-150 keV)             : 3.90568e-08 ( 0  0 ) ergs/cm2

Single BB

 
Spectral model blackbody:
------------------------------------------------------------
Parameters  : value    Lower 90%  Upper 90%
kT [keV]    : 18.9612  (-7.56327  15.4369)
R^2/D10^2   : 2.65199E-02  (-0.0265146   0.121883)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          49.02 using 59 PHA bins.
# Reduced chi-squared =         0.8600 for     57 degrees of freedom 
# Null hypothesis probability =   7.648851e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.875e-09   1.260e-09
25- 50  9.008e-09   5.720e-09
50-150  2.379e-08   1.712e-08
15-150  3.467e-08   2.309e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 199.363       (-199.363      -199.363)
Norm        : 2.08935       (-0.901833     1.10202)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          48.48 using 59 PHA bins.
# Reduced chi-squared =         0.8506 for     57 degrees of freedom 
# Null hypothesis probability =   7.816886e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  5.203e-09   3.284e-09
25- 50  1.001e-08   6.515e-09
50-150  2.195e-08   1.395e-08
15-150  3.716e-08   2.429e-08

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 5.02002        (-5.00549      21.2931)
R1^2/D10^2  : 1.74516        (-1.78461      -1.78461)
kT2 [keV]   : 23.8911        (-23.8881      -23.8881)
R2^2/D10^2  : 1.06299E-02    (-0.0106403   0.0689234)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          47.35 using 59 PHA bins.
# Reduced chi-squared =         0.8609 for     55 degrees of freedom 
# Null hypothesis probability =   7.586505e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  5.391e-09   3.832e-09
25- 50  8.822e-09   4.557e-09
50-150  2.555e-08   1.648e-08
15-150  3.976e-08   2.218e-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: 1.60522     ( -0.220725   0.22509 )
Norm@50keV  : 7.52164E-04    ( -0.000104269   0.000103216 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          61.43 using 59 PHA bins.
# Reduced chi-squared =          1.078 for     57 degrees of freedom 
# Null hypothesis probability =   3.202135e-01
 
Photon flux (15-150 keV)    in 343.3 sec: 9.68137E-02 ( -0.012929  0.0129507 ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.41335e-06 ( -3.54773e-07  3.59548e-07 ) ergs/cm2

Cutoff power-law model

Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.01816     ( -0.953228   0.724086 )
Epeak [keV] : 79.9328      ( -27.2634 -79.9306 )
Norm@50keV  : 1.53318E-03    ( -0.00087981   0.00324415 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          59.82 using 59 PHA bins.
# Reduced chi-squared =          1.068 for     56 degrees of freedom 
# Null hypothesis probability =   3.387897e-01
 
Photon flux (15-150 keV)    in 343.3 sec: 9.47593E-02 ( -0.0130704  0.0132267 ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.30871e-06 ( -3.82824e-07  3.87249e-07 ) ergs/cm2

Band function

 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -1.01662   ( -0.694336   0.91222 )
beta        : -10.0000    ( 10   8.52651e-14 )
Epeak [keV] : 79.8395      ( -27.1599 -79.8395 )
Norm@50keV   : 1.53582E-03    ( -0.000848713   0.00323705 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          59.82 using 59 PHA bins.
# Reduced chi-squared =          1.088 for     55 degrees of freedom 
# Null hypothesis probability =   3.050372e-01
 
Photon flux (15-150 keV)    in 343.3 sec: 9.47282E-02 ( 6.90527  -0.0125703 ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.31674e-06 ( 0  0 ) ergs/cm2

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

S(25-50 keV)  = 7.04e-07
S(50-100 keV) = 9.26e-07

T90 vs. Hardness ratio plot

T90                                   = 373.819999992847 sec.
Hardness ratio (energy fluence ratio) = 1.31534

Color vs. Color plot

Count Ratio  (25-50 keV) / (15-25 keV) = 1.09687
Count Ratio (50-100 keV) / (15-25 keV) = 0.909631

Mask shadow pattern

IMX = 0.814948701689, IMY = 0.405239122531

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:
-129.599400 1.616000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
 32.4519  58.3202    2.5  50.3   26.9   3.4297   4.7 ------	UNKNOWN                       
336.2419  22.2211    3.0  50.7  -44.7   2.8360   3.9 ------	UNKNOWN                       
352.2990 -14.4565    3.6  41.2 -100.0   2.3435   3.2 ------	UNKNOWN

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

Time interval of the image:
1.616000 344.900600
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
 53.3910  26.4740    2.0  31.0   73.8   4.2474   5.7 ------	UNKNOWN                       
 30.7926  32.4273    2.3  24.5   31.0   2.3147   5.1 ------	UNKNOWN                       
 15.8273  33.6318    2.1  27.4    2.7   2.2057   5.6 ------	UNKNOWN                       
 15.8043   8.1034    2.3  11.1  -66.5   1.8584   5.0 ------	UNKNOWN                       
 15.3421   0.0213    1.9  14.2 -101.4   2.2971   6.0 ------	UNKNOWN                       
  5.9883  15.4689    1.9  21.8  -45.4   2.4256   6.2 ------	UNKNOWN                       
 17.3493 -24.0253    2.4  33.6 -140.8   2.3669   4.8 ------	UNKNOWN                       
342.0557   9.8185    2.8  44.4  -61.1   6.4574   4.1 ------	UNKNOWN                       
351.2147 -11.8865    2.4  40.8  -95.8   6.7977   4.8 ------	UNKNOWN

Post-slew image of 15-350 keV band

Time interval of the image:
406.300600 963.080000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
299.5799  35.1906    0.5  41.2  -50.4  18.6224  22.5    0.8	Cyg X-1                       
308.1072  40.9485    1.9  34.0  -42.0   2.9671   5.9    0.3	Cyg X-3                       
326.1063  38.2336    5.7  19.9  -45.1   0.6911   2.0    6.1	Cyg X-2                       
 31.4296  43.7843    3.0  34.4   80.1   3.1908   3.9 ------	UNKNOWN                       
 28.6887  37.8487    3.1  32.2   90.9   2.6339   3.8 ------	UNKNOWN                       
 13.0254  -4.3043    2.6  43.0  166.0   3.3635   4.5 ------	UNKNOWN                       
349.5387  32.4866    1.5   0.0  -83.7   2.5633   7.6 ------	UNKNOWN                       
275.7203  60.9961    3.3  54.3  -13.4   3.6143   3.5 ------	UNKNOWN                       
328.5634 -11.6184    2.2  48.5 -130.4   9.1486   5.2 ------	UNKNOWN

Plot creation:
Thu Oct  8 20:23:32 EDT 2015