batgrbproduct analysis for trigger=564028

batgrbproduct Analysis for Trigger=564028

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): Sun Jan 12 00:21:39 EST 2014
             Host Name: batevent1
   Current Working Dir: /local/data/batevent/batevent_reproc/trigger564028
======================================================================

  Trigger: 00564028      Segment: 000

  BAT Trigger Time: 396466778.432   [s; MET]
      Trigger Stop: 396466778.944   [s; MET]
               UTC: 2013-07-25T17:39:27.599040    [includes UTCF correction] 
       Where From?: TDRSS position message

  BAT 
    RA: 214.232041308035   Dec: -11.1402286245125  [deg; J2000]

     Catalogged Source?: NO
     Point Source?:      YES
     GRB Indicated?:     YES    [ by BAT flight software ]
     Image S/N Ratio:    10.17
     Image Trigger?:     NO
     Rate S/N Ratio:     20.2237484161567  [ if not an image trigger ]
     Image S/N Ratio:    10.17

  Flight Position:   [ source = BAT ]
    RA: 214.232041308035   Dec: -11.1402286245125  [deg; J2000]

  Ground Position:   [ source = BAT pre-slew burst ]
    RA: 214.236639943365   Dec: -11.1198350527407  [deg; J2000]  
        { 14h 16m 56.8s , -11d 07' 11.4" }
         +/- 1.02718546279786 [arcmin] (estimated 90% radius based on SNR)
         +/- 0.387976456956507 [arcmin] (formal 1-sigma fit error)
    SNR: 29.273668134919
 
  Angular difference between Flight and Ground position is 1.253206 arcmin
 
  Partial Coding Fraction: 0.96875    [ including projection effects ]

  Duration
     T90: 4.77599990367889 +/- 0.855083658147749
        Measured from: 0.0480000376701355
                   to: 4.82399994134903     [s; relative to TRIGTIME]
     T50: 1.93999993801117 +/- 0.286216694722533
        Measured from: 0.776000022888184
                   to: 2.71599996089935     [s; relative to TRIGTIME]



  Fluence
     Peak Flux  (peak 1 second)
        Measured from: 0.276000022888184     
                   to: 1.27600002288818     [s; relative to TRIGTIME]
     Total Fluence        
        Measured from: -0.38400000333786     
                   to: 5.89600002765656     [s; relative to TRIGTIME]
     
             Band 1     Band 2     Band 3     Band 4
              15-25      25-50     50-100    100-350     keV
 Total     0.348350   0.282604   0.125882   0.016226
           0.014444   0.013992   0.012302   0.010984 [error]
 Peak      0.108023   0.101938   0.050608   0.008612
           0.006371   0.006345   0.005435   0.004601 [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 1.05e-07 1.21e-07 9.95e-08 1.38e-07 3.75e-07 4.63e-07   erg/cm2
              Error 9.40e-09 7.19e-09 1.18e-08 3.26e-08 2.56e-08 4.51e-08   erg/cm2
Peak flux Power-law 1.05e+00 7.60e-01 3.63e-01 2.45e-01 2.29e+00 2.42e+00   ph/cm2/s
              Error 1.15e-01 5.45e-02 4.60e-02 6.00e-02 1.66e-01 1.74e-01   ph/cm2/s
 
Fluence   Cutoff-PL 1.04e-07 1.22e-07 9.88e-08 1.16e-07 3.71e-07 4.40e-07   erg/cm2
              Error 1.04e-08 8.67e-09 1.28e-08 5.47e-08 3.14e-08 7.51e-08   erg/cm2
Peak flux Cutoff-PL 1.03e+00 7.77e-01 3.61e-01 1.77e-01 2.27e+00 2.34e+00   ph/cm2/s
              Error 1.31e-01 6.92e-02 4.83e-02 1.18e-01 1.78e-01 2.25e-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    2.276    0.133    -      -           6.27e-03 5.18e-04   67.710 57
CPL   1.995    0.000       0.8    0.5      9.04e-03 1.26e-03   68.000 56
 
 
=== 1-s peak spectral analysis ===
 
Model Ph_index Ph_90err Epeak  Epeak_90err Norm     Nomr_90err chi2   dof
PL    2.066    0.147    -      -           1.48e-02 1.38e-03   69.450 57
CPL   1.851    0.444      29.0   -2.5      1.97e-02 0.00e+00   69.030 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: 10.304000 sec.
T50 in the 50-300 keV band: 3.712000 sec.

 
=== Table of the duration information ==
 
        Value   tstart    tstop
T100    6.280   -0.384    5.896
T90     4.776    0.048    4.824
T50     1.940    0.776    2.716
Peak    1.000    0.276    1.276

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
  214.2366   -11.1198   0.0066    19.6024  -147.5253         0.7839156     29.274 TRIG_00564028                 
 
Foreground time interval of the image:
 -0.384   5.896 (delta_t =   6.280 [sec])
Background time interval of the image:
-239.432  -0.384 (delta_t = 239.048 [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   -0.384 sec. to    5.896 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 2.27610     ( -0.13023   0.134947 )
Norm@50keV  : 6.27231E-03    ( -0.000522278   0.000514689 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          67.71 using 59 PHA bins.
# Reduced chi-squared =          1.188 for     57 degrees of freedom 
# Null hypothesis probability =   1.568031e-01
 
Photon flux (15-150 keV)    in 6.28 sec: 1.08175 ( -0.0651574  0.0653578 ) ph/cm2/s
Energy fluence (15-150 keV)             : 3.7481e-07 ( -2.5438e-08  2.58193e-08 ) ergs/cm2

Cutoff power-law model

Time interval is from   -0.384 sec. to    5.896 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.99488     (     )
Epeak [keV] : 0.762979      ( -0.270533 0.728382 )
Norm@50keV  : 9.04191E-03    ( -0.00115845   0.00135191 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          68.00 using 59 PHA bins.
# Reduced chi-squared =          1.214 for     56 degrees of freedom 
# Null hypothesis probability =   1.305682e-01
 
Photon flux (15-150 keV)    in 6.28 sec: 1.07575 ( -0.07316  0.06975 ) ph/cm2/s
Energy fluence (15-150 keV)             : 3.70965e-07 ( -3.37795e-08  2.90381e-08 ) ergs/cm2

Band function

Time interval is from   -0.384 sec. to    5.896 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -1.15422   (     )
beta        : -9.00270    (     )
Epeak [keV] : 61.9522      (   )
Norm@50keV   : 1.53076E-02    (     )
------------------------------------------------------------
#Fit statistic : Chi-Squared =         113.89 using 59 PHA bins.
# Reduced chi-squared =         2.0707 for     55 degrees of freedom 
# Null hypothesis probability =   5.379013e-06
 
Photon flux (15-150 keV)    in 6.28 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]    : 8.70489  (  )
R^2/D10^2   : 0.783063  (   )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =         128.20 using 59 PHA bins.
# Reduced chi-squared =         2.2491 for     57 degrees of freedom 
# Null hypothesis probability =   2.123932e-07
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  7.124e-08   7.501e-09
25- 50  1.436e-07   1.017e-08
50-150  4.942e-08   9.674e-09
15-150  2.643e-07   1.934e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 45.3067       (-7.30483      9.79262)
Norm        : 6.26417       (-0.76411     0.902451)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          73.65 using 59 PHA bins.
# Reduced chi-squared =          1.292 for     57 degrees of freedom 
# Null hypothesis probability =   6.807074e-02
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  9.384e-08   8.070e-09
25- 50  1.299e-07   8.133e-09
50-150  1.146e-07   1.893e-08
15-150  3.383e-07   2.368e-08

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 4.67306        (-0.973867      1.18064)
R1^2/D10^2  : 7.37220        (-4.29333      13.3021)
kT2 [keV]   : 15.6759        (-3.0637      5.79374)
R2^2/D10^2  : 5.45099E-02    (-0.0394579   0.0852158)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          72.54 using 59 PHA bins.
# Reduced chi-squared =          1.319 for     55 degrees of freedom 
# Null hypothesis probability =   5.660313e-02
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.027e-07   2.229e-08
25- 50  1.191e-07   2.926e-08
50-150  1.244e-07   4.297e-08
15-150  3.463e-07   9.313e-08

Peak spectrum fit

Power-law model

Time interval is from    0.276 sec. to    1.276 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 2.06577     ( -0.144621   0.150295 )
Norm@50keV  : 1.48119E-02    ( -0.00139548   0.00137035 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          69.45 using 59 PHA bins.
# Reduced chi-squared =          1.218 for     57 degrees of freedom 
# Null hypothesis probability =   1.246878e-01
 
Photon flux (15-150 keV)    in 1 sec: 2.29170 ( -0.166126  0.166254 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.37198e-07 ( -1.17152e-08  1.19085e-08 ) ergs/cm2

Cutoff power-law model

Time interval is from    0.276 sec. to    1.276 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.85118     ( -0.636181   0.251886 )
Epeak [keV] : 29.0321      ( -24.0065 -29.0322 )
Norm@50keV  : 1.96578E-02    (     )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          69.03 using 59 PHA bins.
# Reduced chi-squared =          1.233 for     56 degrees of freedom 
# Null hypothesis probability =   1.133859e-01
 
Photon flux (15-150 keV)    in 1 sec: 2.26572 ( -0.17882  0.17812 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.33863e-07 ( -1.4387e-08  1.4281e-08 ) ergs/cm2

Band function

Time interval is from    0.276 sec. to    1.276 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -1.62471   ( 0.83315   0.83315 )
beta        : -2.23224    ( 2.23957   0.301299 )
Epeak [keV] : 31.6943      ( -31.1495 -31.1495 )
Norm@50keV   : 2.74469E-02    ( -0.00955968   12327.2 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          68.84 using 59 PHA bins.
# Reduced chi-squared =          1.252 for     55 degrees of freedom 
# Null hypothesis probability =   9.933088e-02
 
Photon flux (15-150 keV)    in 1 sec:  (    ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.34008e-07 ( 0  0 ) ergs/cm2

Single BB

 
Spectral model blackbody:
------------------------------------------------------------
Parameters  : value    Lower 90%  Upper 90%
kT [keV]    : 9.61797  (-0.830499  0.912681)
R^2/D10^2   : 1.18311  (-0.352515   0.501925)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =         109.53 using 59 PHA bins.
# Reduced chi-squared =         1.9216 for     57 degrees of freedom 
# Null hypothesis probability =   3.586078e-05
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  2.197e-08   2.945e-09
25- 50  5.164e-08   4.580e-09
50-150  2.405e-08   4.895e-09
15-150  9.766e-08   8.130e-09

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 60.9492       (-12.7592      17.9978)
Norm        : 11.7368       (-1.47311     1.63759)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          70.98 using 59 PHA bins.
# Reduced chi-squared =          1.245 for     57 degrees of freedom 
# Null hypothesis probability =   1.009016e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  2.957e-08   3.050e-09
25- 50  4.522e-08   3.250e-09
50-150  5.213e-08   1.010e-08
15-150  1.269e-07   1.165e-08

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 5.39704        (-1.48017      1.60116)
R1^2/D10^2  : 8.02600        (-4.76324      20.803)
kT2 [keV]   : 18.3759        (-4.73994      10.0185)
R2^2/D10^2  : 6.93443E-02    (-0.0571753   0.172771)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          72.44 using 59 PHA bins.
# Reduced chi-squared =          1.317 for     55 degrees of freedom 
# Null hypothesis probability =   5.748749e-02
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  3.090e-08   9.985e-09
25- 50  4.247e-08   1.164e-08
50-150  5.507e-08   2.998e-08
15-150  1.284e-07   4.257e-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: 2.27610     ( -0.13023   0.134947 )
Norm@50keV  : 6.27231E-03    ( -0.000522278   0.000514689 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          67.71 using 59 PHA bins.
# Reduced chi-squared =          1.188 for     57 degrees of freedom 
# Null hypothesis probability =   1.568031e-01
 
Photon flux (15-150 keV)    in 6.28 sec: 1.08175 ( -0.0651574  0.0653578 ) ph/cm2/s
Energy fluence (15-150 keV)             : 3.7481e-07 ( -2.5438e-08  2.58193e-08 ) ergs/cm2

Cutoff power-law model

Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.99488     (     )
Epeak [keV] : 0.762979      ( -0.270533 0.728382 )
Norm@50keV  : 9.04191E-03    ( -0.00115845   0.00135191 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          68.00 using 59 PHA bins.
# Reduced chi-squared =          1.214 for     56 degrees of freedom 
# Null hypothesis probability =   1.305682e-01
 
Photon flux (15-150 keV)    in 6.28 sec: 1.07575 ( -0.07316  0.06975 ) ph/cm2/s
Energy fluence (15-150 keV)             : 3.70965e-07 ( -3.37795e-08  2.90381e-08 ) ergs/cm2

Band function

 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -1.15422   (     )
beta        : -9.00270    (     )
Epeak [keV] : 61.9522      (   )
Norm@50keV   : 1.53076E-02    (     )
------------------------------------------------------------
#Fit statistic : Chi-Squared =         113.89 using 59 PHA bins.
# Reduced chi-squared =         2.0707 for     55 degrees of freedom 
# Null hypothesis probability =   5.379013e-06
 
Photon flux (15-150 keV)    in 6.28 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)  = 1.21e-07
S(50-100 keV) = 9.95e-08

T90 vs. Hardness ratio plot

T90                                   = 4.77599990367889 sec.
Hardness ratio (energy fluence ratio) = 0.822314

Color vs. Color plot

Count Ratio  (25-50 keV) / (15-25 keV) = 0.811265
Count Ratio (50-100 keV) / (15-25 keV) = 0.361366

Mask shadow pattern

IMX = -3.004419539939238E-01, IMY = 1.912158196150189E-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:
-239.432000 -0.384000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
244.9831 -15.6390    0.4  22.0  118.2   7.2207  30.9    0.2	Sco X-1                       
254.3773  35.4716    5.5  41.6   10.3   0.6766   2.1    8.7	Her X-1                       
255.9545 -37.9673    2.6  45.4  130.9  -4.1943  -4.4    7.5	4U 1700-377                   
256.6170 -36.4165    5.3  44.5  128.9  -1.7821  -2.2    8.8	GX 349+2                      
268.3976  -1.3710    6.2  38.4   72.8   1.4078   1.8    5.2	SW J1753.5-0127               
203.0348  45.4840    3.4  50.7  -44.4   4.0695   3.4 ------	UNKNOWN

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

Time interval of the image:
-0.384000 5.896000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
244.8700 -15.4979    5.9  21.8  118.2  -0.0629  -2.0   10.6	Sco X-1                       
254.4854  35.2477   14.2  41.4   10.6   0.0360   0.8    5.8	Her X-1                       
255.8421 -37.7705    7.7  45.2  130.8  -0.1748  -1.5    8.2	4U 1700-377                   
256.5542 -36.5519    0.0  44.6  129.1   0.1125   0.9    9.6	GX 349+2                      
268.3368  -1.5708    5.1  38.4   73.2  -0.2212  -2.3    7.3	SW J1753.5-0127               
257.2546 -35.5677    2.3  44.2  127.6   0.6056   5.0 ------	UNKNOWN                       
245.5618 -48.2567    2.2  50.7  146.5   0.7824   5.4 ------	UNKNOWN                       
219.3631 -44.7038    2.2  46.3  170.3   0.3116   5.2 ------	UNKNOWN                       
214.0937 -33.3361    2.6  37.1 -177.9   0.1657   4.4 ------	UNKNOWN                       
214.2366 -11.1198    0.4  19.6 -147.5   0.7838  29.3 ------	UNKNOWN                       
195.7320 -14.0264    2.4  37.0 -134.9   0.2038   4.8 ------	UNKNOWN

Post-slew image of 15-350 keV band

Time interval of the image:
52.068580 962.655900
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
186.4962 -62.7907    5.8  55.3  175.9   4.9012   2.0    4.6	GX 301-2                      
244.9912 -15.6343    0.4  30.2   82.9  30.1499  32.4    0.8	Sco X-1                       
207.6280  47.4892    3.7  58.9  -24.3  12.1356   3.2 ------	UNKNOWN                       
186.7748  27.6056    4.5  47.0  -53.1   7.8035   2.6 ------	UNKNOWN

Plot creation:
Sat May 30 16:03:49 EDT 2015