batgrbproduct analysis for trigger=605612

batgrbproduct Analysis for Trigger=605612

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): Thu Jul 31 01:56:03 EDT 2014
             Host Name: bat1
   Current Working Dir: /local/data/bat1/prebascript/trigger605612
======================================================================

  Trigger: 00605612      Segment: 000

  BAT Trigger Time: 427442047.488   [s; MET]
      Trigger Stop: 427442048.512   [s; MET]
               UTC: 2014-07-19T05:53:55.204500    [includes UTCF correction] 
       Where From?: TDRSS position message

  BAT 
    RA: 171.592074083928   Dec: -50.1345189156071  [deg; J2000]

     Catalogged Source?: NO
     Point Source?:      YES
     GRB Indicated?:     YES    [ by BAT flight software ]
     Image S/N Ratio:    6.92
     Image Trigger?:     NO
     Rate S/N Ratio:     7.14142842854285  [ if not an image trigger ]
     Image S/N Ratio:    6.92

  Flight Position:   [ source = BAT ]
    RA: 171.592074083928   Dec: -50.1345189156071  [deg; J2000]

  Ground Position:   [ source = BAT pre-slew burst ]
    RA: 171.57124258296   Dec: -50.1153193404698  [deg; J2000]  
        { 11h 26m 17.1s , -50d 06' 55.1" }
         +/- 2.42349151941687 [arcmin] (estimated 90% radius based on SNR)
         +/- 1.53918923445099 [arcmin] (formal 1-sigma fit error)
    SNR: 8.5884784635106
 
  Angular difference between Flight and Ground position is 1.403270 arcmin
 
  Partial Coding Fraction: 0.7578125    [ including projection effects ]

  Duration
     T90: 48 +/- 22.6274169979695
        Measured from: -31.4879999756813
                   to: 16.5120000243187     [s; relative to TRIGTIME]
     T50: 16 +/- 16
        Measured from: -15.4879999756813
                   to: 0.512000024318695     [s; relative to TRIGTIME]



  Fluence
     Peak Flux  (peak 1 second)
        Measured from: 8.0120000243187     
                   to: 9.0120000243187     [s; relative to TRIGTIME]
     Total Fluence        
        Measured from: -31.4879999756813     
                   to: 16.5120000243187     [s; relative to TRIGTIME]
     
             Band 1     Band 2     Band 3     Band 4
              15-25      25-50     50-100    100-350     keV
 Total     0.238728   0.314772   0.196743   0.036398
           0.043527   0.043318   0.038236   0.034547 [error]
 Peak      0.017079   0.002540   0.004581   0.001430
           0.006216   0.006279   0.005524   0.005292 [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 8.64e-08 1.25e-07 1.34e-07 2.69e-07 4.29e-07 6.15e-07   erg/cm2
              Error 1.96e-08 2.02e-08 3.55e-08 1.41e-07 8.33e-08 1.80e-07   erg/cm2
Peak flux Power-law 1.23e-01 5.21e-02 1.31e-02 4.03e-03 1.91e-01 1.94e-01   ph/cm2/s
              Error 9.40e-02 5.30e-02 2.58e-02 2.53e-02 1.45e-01 1.48e-01   ph/cm2/s
 
Fluence   Cutoff-PL 7.79e-08 1.42e-07 1.32e-07 6.20e-08 3.94e-07 4.14e-07   erg/cm2
              Error 2.26e-08 2.79e-08 4.21e-08 1.54e-07 8.72e-08 1.84e-07   erg/cm2
Peak flux Cutoff-PL 1.78e-01 3.68e-02 9.04e-06 1.66e-15 2.15e-01 2.15e-01   ph/cm2/s
              Error 1.08e-01 3.70e-02 5.57e-03 0.00e+00 1.27e-01 1.27e-01   ph/cm2/s
 
Fluence        Band 7.74e-08 1.41e-07 1.32e-07 6.40e-08 3.95e-07 4.15e-07   erg/cm2
              Error -------- -------- 4.05e-08 -------- 8.68e-08 --------   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    1.895    0.291    -      -           9.72e-04 1.90e-04   51.100 57
CPL   0.843    1.356      47.6  -14.7      3.80e-03 1.44e-02   48.750 56
 
 
=== 1-s peak spectral analysis ===
 
Model Ph_index Ph_90err Epeak  Epeak_90err Norm     Nomr_90err chi2   dof
PL    2.985    2.211    -      -           7.03e-04 1.00e-03   56.840 57
CPL  -9.984    0.990      20.2    4.9      2.49e+07 2.83e+08   54.010 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   48.000  -31.488   16.512
T90    48.000  -31.488   16.512
T50    16.000  -15.488    0.512
Peak    1.000    8.012    9.012

Click here for the BAT GCN circular template

Special notes of this burst

Image

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

#   RAcent  DECcent POSerr  Theta    Phi     Peak Cts     SNR  Name
  171.5712 -50.1153 0.0224   32.5  -12.9       0.7241     8.6  TRIG_00605612       
------------------------------------------
 
Foreground time interval of the image:
-31.488  11.213 (delta_t =  42.701 [sec])
Background time interval of the image:
-239.488 -31.488 (delta_t = 208.000 [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

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)

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

Time interval is from  -31.488 sec. to   16.512 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.89505     ( -0.27924   0.301785 )
Norm@50keV  : 9.71748E-04    ( -0.00019316   0.000187543 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          51.10 using 59 PHA bins.
# Reduced chi-squared =         0.8965 for     57 degrees of freedom 
# Null hypothesis probability =   6.949758e-01
 
Photon flux (15-150 keV)    in 48 sec: 0.139164 ( -0.0225179  0.0225238 ) ph/cm2/s
Energy fluence (15-150 keV)             : 4.28812e-07 ( -8.20171e-08  8.45314e-08 ) ergs/cm2

Cutoff power-law model

Time interval is from  -31.488 sec. to   16.512 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 0.843370     ( -1.55527   1.15726 )
Epeak [keV] : 47.6396      ( -18.1728 -47.6396 )
Norm@50keV  : 3.79885E-03    ( -0.00379886   0.0250415 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          48.75 using 59 PHA bins.
# Reduced chi-squared =         0.8706 for     56 degrees of freedom 
# Null hypothesis probability =   7.431854e-01
 
Photon flux (15-150 keV)    in 48 sec: 0.134509 ( -0.022997  0.023053 ) ph/cm2/s
Energy fluence (15-150 keV)             : 3.94278e-07 ( -8.32363e-08  9.11314e-08 ) ergs/cm2

Band function

Time interval is from  -31.488 sec. to   16.512 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -0.842582   ( -2.10744   5.84078 )
beta        : -10.0000    ( 10   3.55271e-15 )
Epeak [keV] : 47.6208      ( -22.9074 -47.6208 )
Norm@50keV   : 3.80302E-03    ( -0.00380302   0.0251151 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          48.75 using 59 PHA bins.
# Reduced chi-squared =         0.8864 for     55 degrees of freedom 
# Null hypothesis probability =   7.108056e-01
 
Photon flux (15-150 keV)    in 48 sec: 0.136126 ( 6.86387  -0.024996 ) ph/cm2/s
Energy fluence (15-150 keV)             : 3.94917e-07 ( -3.94581e-07  -8.41934e-08 ) ergs/cm2

Single BB

 
Spectral model blackbody:
------------------------------------------------------------
Parameters  : value    Lower 90%  Upper 90%
kT [keV]    : 11.0971  (-1.98388  2.36679)
R^2/D10^2   : 4.53384E-02  (-0.0233502   0.0491099)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          54.21 using 59 PHA bins.
# Reduced chi-squared =         0.9511 for     57 degrees of freedom 
# Null hypothesis probability =   5.803208e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  5.609e-08   1.767e-08
25- 50  1.604e-07   3.679e-08
50-150  1.123e-07   4.452e-08
15-150  3.288e-07   8.789e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 78.1853       (-30.3484      71.0017)
Norm        : 0.664973       (-0.142896     0.184538)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          49.13 using 59 PHA bins.
# Reduced chi-squared =         0.8620 for     57 degrees of freedom 
# Null hypothesis probability =   7.612772e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  8.269e-08   1.920e-08
25- 50  1.354e-07   2.846e-08
50-150  1.881e-07   1.126e-07
15-150  4.062e-07   1.269e-07

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 5.27475        (-3.45793      3.9511)
R1^2/D10^2  : 0.393233        (-0.325703      94.935)
kT2 [keV]   : 16.0388        (-4.88868      15.3334)
R2^2/D10^2  : 8.73331E-03    (-0.0079467   0.0324146)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          48.47 using 59 PHA bins.
# Reduced chi-squared =         0.8813 for     55 degrees of freedom 
# Null hypothesis probability =   7.206978e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  7.887e-08   4.356e-08
25- 50  1.360e-07   7.015e-08
50-150  1.713e-07   1.087e-07
15-150  3.862e-07   2.070e-07

Peak spectrum fit

Power-law model

Time interval is from    8.012 sec. to    9.012 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 2.98467     ( -1.58447   2.83764 )
Norm@50keV  : 7.03170E-04    ( -0.000701459   0.00129849 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          56.84 using 59 PHA bins.
# Reduced chi-squared =         0.9973 for     57 degrees of freedom 
# Null hypothesis probability =   4.808983e-01
 
Photon flux (15-150 keV)    in 1 sec: 0.190933 ( -0.142236  0.14778 ) ph/cm2/s
Energy fluence (15-150 keV)             : 8.36208e-09 ( -8.38231e-09  1.00643e-08 ) ergs/cm2

Cutoff power-law model

Time interval is from    8.012 sec. to    9.012 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: -9.98365     ( 9.99531   11.9758 )
Epeak [keV] : 20.2223      ( -4.51697 5.25747 )
Norm@50keV  : 2.48571E+07    ( -2.60466e+07   5.39846e+08 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          54.01 using 59 PHA bins.
# Reduced chi-squared =         0.9644 for     56 degrees of freedom 
# Null hypothesis probability =   5.506177e-01
 
Photon flux (15-150 keV)    in 1 sec: 0.214767 ( -0.126419  0.126747 ) ph/cm2/s
Energy fluence (15-150 keV)             : 7.20881e-09 ( -4.31852e-09  4.50029e-09 ) ergs/cm2

Band function

Time interval is from    8.012 sec. to    9.012 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : 2.12287   ( 0.881336   0.881336 )
beta        : -10.0000    ( 10   10 )
Epeak [keV] : 17.7871      (   )
Norm@50keV   : 10.5655    (     )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          55.54 using 59 PHA bins.
# Reduced chi-squared =          1.010 for     55 degrees of freedom 
# Null hypothesis probability =   4.542261e-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]    : 4.37836  (-1.85528  3.90866)
R^2/D10^2   : 3.33135  (-3.28364   45.0813)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          55.62 using 59 PHA bins.
# Reduced chi-squared =         0.9758 for     57 degrees of freedom 
# Null hypothesis probability =   5.269732e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  4.617e-09   3.150e-09
25- 50  2.141e-09   1.622e-09
50-150  4.385e-11   6.750e-11
15-150  6.802e-09   4.773e-09

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 13.3847       (-13.4661      157.569)
Norm        : 3.93746       (-3.89884     2.72867)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          56.40 using 59 PHA bins.
# Reduced chi-squared =         0.9894 for     57 degrees of freedom 
# Null hypothesis probability =   4.977274e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  4.121e-09   2.652e-09
25- 50  2.516e-09   1.927e-09
50-150  3.517e-10   4.839e-10
15-150  6.989e-09   5.080e-09

Double BB

------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 4.34668        (-1.83155      3.92962)
R1^2/D10^2  : 3.41021        (-3.04707      45.1661)
kT2 [keV]   : 27.6999        (      )
R2^2/D10^2  : 2.89593E-04    (-0.000309393   0.0252846)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          55.62 using 59 PHA bins.
#Fit statistic : Chi-Squared =          55.59 using 59 PHA bins.
# Reduced chi-squared =          1.011 for     55 degrees of freedom 
# Reduced chi-squared =          1.011 for     55 degrees of freedom 
# Null hypothesis probability =   4.512980e-01
# Null hypothesis probability =   4.525769e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  0.000e+00   0.000e+00
25- 50  0.000e+00   0.000e+00
50-150  0.000e+00   0.000e+00
15-150  0.000e+00   0.000e+00

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: 1.83240     ( -0.292809   0.315264 )
Norm@50keV  : 1.01655E-03    ( -0.000204298   0.000197971 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          57.16 using 59 PHA bins.
# Reduced chi-squared =          1.003 for     57 degrees of freedom 
# Null hypothesis probability =   4.691759e-01
 
Photon flux (15-150 keV)    in 42.7 sec: 0.141876 ( -0.0238738  0.0238848 ) ph/cm2/s
Energy fluence (15-150 keV)             : 3.99238e-07 ( -7.89139e-08  8.11496e-08 ) ergs/cm2

Cutoff power-law model

Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.09766     ( -1.44458   1.09767 )
Epeak [keV] : 55.6350      (   )
Norm@50keV  : 2.56458E-03    (     )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          55.93 using 59 PHA bins.
# Reduced chi-squared =         0.9988 for     56 degrees of freedom 
# Null hypothesis probability =   4.774081e-01
 
Photon flux (15-150 keV)    in 42.7 sec: 0.138229 ( -0.02449  0.0245 ) ph/cm2/s
Energy fluence (15-150 keV)             : 3.77488e-07 ( -8.20284e-08  8.72036e-08 ) ergs/cm2

Band function

 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -1.09686   ( -1.46963   1.91328 )
beta        : -10.0000    ( 10   3.55271e-15 )
Epeak [keV] : 55.6017      ( -39.5889 -55.6019 )
Norm@50keV   : 2.56730E-03    ( -0.00256726   0.013084 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          55.93 using 59 PHA bins.
# Reduced chi-squared =          1.017 for     55 degrees of freedom 
# Null hypothesis probability =   4.396204e-01
 
Photon flux (15-150 keV)    in 42.7 sec:  (    ) ph/cm2/s
Energy fluence (15-150 keV)             : 3.77138e-07 ( -3.76839e-07  -8.18499e-08 ) ergs/cm2

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

S(25-50 keV)  = 1.25e-07
S(50-100 keV) = 1.34e-07

T90 vs. Hardness ratio plot

T90                                   = 48 sec.
Hardness ratio (energy fluence ratio) = 1.072

Color vs. Color plot

Count Ratio  (25-50 keV) / (15-25 keV) = 1.31854
Count Ratio (50-100 keV) / (15-25 keV) = 0.82413

Mask shadow pattern

IMX = 6.199372693605700E-01, IMY = 1.418463931609550E-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:
-239.488000 -31.488000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
135.5250 -40.5506    0.6  32.4  -64.1   4.2951  18.1    0.3	Vela X-1                      
170.3157 -60.6233  505.6  23.4   -1.3   0.0039   0.0    0.0	Cen X-3                       
186.7818 -62.7210    3.9  27.0   15.8   0.5349   2.9    4.5	GX 301-2                      
 42.0487 -37.4872    2.4  49.8  178.9   1.9705   4.9 ------	UNKNOWN                       
 71.0947 -22.4718    3.3  55.3 -144.8   4.0377   3.6 ------	UNKNOWN                       
157.8546 -24.7971    3.2  52.1  -42.2   3.1876   3.6 ------	UNKNOWN                       
152.4067 -26.2340    2.9  49.5  -47.9   3.2318   4.0 ------	UNKNOWN

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

Time interval of the image:
-31.488000 11.212600
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
135.3889 -40.6232    7.6  32.3  -64.2   0.1506   1.5    7.6	Vela X-1                      
170.6961 -60.6205    5.6  23.5   -1.0  -0.1420  -2.1   11.2	Cen X-3                       
186.5364 -62.5738 2700.0  27.0   15.4  -0.0002  -0.0   12.2	GX 301-2                      
171.5713 -50.1153    1.3  32.5  -12.9   0.7241   8.6 ------	UNKNOWN

Post-slew image of 15-350 keV band

Time interval of the image:
63.212590 962.584300
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
135.5419 -40.5583    0.3  26.8 -124.3  21.1480  37.6    0.6	Vela X-1                      
170.3400 -60.8286    9.1  10.7  142.1  -0.6629  -1.3   12.4	Cen X-3                       
186.7844 -62.6930    2.3  15.0  111.2   2.6149   5.0    5.8	GX 301-2                      
 76.7217 -58.3154    3.0  51.4 -179.2   5.9648   3.8 ------	UNKNOWN                       
131.9478 -45.6872    2.7  26.6 -137.1   2.3040   4.2 ------	UNKNOWN

Plot creation:
Thu Jul 31 02:13:01 EDT 2014