batgrbproduct analysis for trigger=824063

batgrbproduct Analysis for Trigger=824063

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): Fri May 11 18:13:07 EDT 2018
             Host Name: bat1
   Current Working Dir: /local/data/bat1/alien/Swift_3rdBATcatalog/event/batevent_reproc/trigger824063
======================================================================

  Trigger: 00824063      Segment: 000

  BAT Trigger Time: 545040200   [s; MET]
      Trigger Stop: 545040296   [s; MET]
               UTC: 2018-04-10T08:02:59.237600    [includes UTCF correction] 
       Where From?: TDRSS position message

  BAT 
    RA: 95.981565817236   Dec: 12.8078803516501  [deg; J2000]

     Catalogged Source?: NO
     Point Source?:      YES
     GRB Indicated?:     YES    [ by BAT flight software ]
     Image S/N Ratio:    10.52
     Image Trigger?:     YES
     Rate S/N Ratio:     0  [ if not an image trigger ]
     Image S/N Ratio:    10.52

  Flight Position:   [ source = BAT ]
    RA: 95.981565817236   Dec: 12.8078803516501  [deg; J2000]

  Ground Position:   [ source = BAT pre-slew burst ]
    RA: 95.9714996106793   Dec: 12.8062630733419  [deg; J2000]  
        { 06h 23m 53.2s , +12d 48' 22.5" }
         +/- 1.83821515799834 [arcmin] (estimated 90% radius based on SNR)
         +/- 0.735250936209581 [arcmin] (formal 1-sigma fit error)
    SNR: 12.7470391179459
 
  Angular difference between Flight and Ground position is 0.596887 arcmin
 
  Partial Coding Fraction: 0.53125    [ including projection effects ]

  Duration
     T90: 114.799999952316 +/- 14.4293076043345
        Measured from: 25.6879999637604
                   to: 140.487999916077     [s; relative to TRIGTIME]
     T50: 50.2719999551773 +/- 10.1099760924878
        Measured from: 37.9119999408722
                   to: 88.1839998960495     [s; relative to TRIGTIME]



  Fluence
     Peak Flux  (peak 1 second)
        Measured from: 25.7039999961853     
                   to: 26.7039999961853     [s; relative to TRIGTIME]
     Total Fluence        
        Measured from: 20.7120000123978     
                   to: 154.751999974251     [s; relative to TRIGTIME]
     
             Band 1     Band 2     Band 3     Band 4
              15-25      25-50     50-100    100-350     keV
 Total     0.849995   1.226270   1.203924   0.191441
           0.087169   0.090106   0.076698   0.063939 [error]
 Peak      0.008085   0.030000   0.039674   0.013972
           0.007899   0.008594   0.007933   0.006422 [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 2.87e-07 5.61e-07 8.52e-07 2.81e-06 2.39e-06 4.50e-06   erg/cm2
              Error 3.79e-08 4.46e-08 7.48e-08 5.43e-07 1.86e-07 5.92e-07   erg/cm2
Peak flux Power-law 1.32e-01 2.03e-01 2.34e-01 5.18e-01 7.23e-01 1.09e+00   ph/cm2/s
              Error 7.79e-02 7.50e-02 5.98e-02 2.85e-01 1.98e-01 3.05e-01   ph/cm2/s
 
Fluence   Cutoff-PL 2.61e-07 5.84e-07 8.84e-07 1.53e-06 2.32e-06 3.26e-06   erg/cm2
              Error 4.70e-08 5.24e-08 8.55e-08 1.01e-06 2.02e-07 1.33e-06   erg/cm2
Peak flux Cutoff-PL 9.66e-02 2.11e-01 2.66e-01 2.21e-01 6.98e-01 7.94e-01   ph/cm2/s
              Error 1.01e-01 8.70e-02 8.21e-02 2.53e-01 2.02e-01 3.70e-01   ph/cm2/s
 
Fluence        Band 4.03e-07 5.91e-07 9.09e-07 1.96e-06 2.36e-06 3.59e-06   erg/cm2
              Error -------- 5.28e-08 9.16e-08 2.39e-07 1.74e-07 3.87e-07   erg/cm2
Peak flux      Band 6.89e-02 2.24e-01 2.58e-01 3.47e-01 6.82e-01 9.02e-01   ph/cm2/s
              Error 9.40e-02 1.04e-01 8.09e-02 2.89e-01 1.56e-01 3.08e-01   ph/cm2/s

 
=== Time-averaged spectral analysis ===
 
Model Ph_index Ph_90err Epeak  Epeak_90err Norm     Nomr_90err chi2   dof
PL    1.399    0.125    -      -           1.85e-03 1.32e-04   50.110 57
CPL   0.942    0.539     122.8  -40.6      3.06e-03 1.93e-03   47.810 56
 
 
=== 1-s peak spectral analysis ===
 
Model Ph_index Ph_90err Epeak  Epeak_90err Norm     Nomr_90err chi2   dof
PL    0.795    0.455    -      -           6.29e-03 1.78e-03   69.710 57
CPL  -0.289    2.288     126.2  -35.0      1.81e-02 1.71e-01   68.790 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: 108.800000 sec.
T50 in the 50-300 keV band: 35.968000 sec.

 
=== Table of the duration information ==
 
        Value   tstart    tstop
T100  134.040   20.712  154.752
T90   114.800   25.688  140.488
T50    50.272   37.912   88.184
Peak    1.000   25.704   26.704

Click here for the BAT GCN circular template

Estimated redshift from machine learning (Ukwatta et al. 2016) - may take a few minute to calcaulte

Image

Pre-slew 15.0-350.0 keV image (Event data)

#   RAcent    DECcent   POSerr    Theta     Phi              Peak Cts       SNR   Name
   95.9715    12.8063   0.0151    33.5944   155.9414         3.1846240     12.747 TRIG_00824063                 
 
Foreground time interval of the image:
 20.712 105.301 (delta_t =  84.589 [sec])
Background time interval of the image:
-15.899  20.712 (delta_t =  36.611 [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   20.712 sec. to  154.752 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.39874     ( -0.125062   0.124602 )
Norm@50keV  : 1.84512E-03    ( -0.000132125   0.000132033 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          50.11 using 59 PHA bins.
# Reduced chi-squared =         0.8791 for     57 degrees of freedom 
# Null hypothesis probability =   7.292438e-01
 
Photon flux (15-150 keV)    in 134 sec: 0.224641 ( -0.016822  0.016862 ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.38998e-06 ( -1.85105e-07  1.8607e-07 ) ergs/cm2

Cutoff power-law model

Time interval is from   20.712 sec. to  154.752 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 0.942267     ( -0.580261   0.497272 )
Epeak [keV] : 122.827      ( -41.5261 -122.826 )
Norm@50keV  : 3.05502E-03    ( -0.00125559   0.00261085 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          47.81 using 59 PHA bins.
# Reduced chi-squared =         0.8537 for     56 degrees of freedom 
# Null hypothesis probability =   7.738346e-01
 
Photon flux (15-150 keV)    in 134 sec: 0.219688 ( -0.017819  0.017746 ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.32308e-06 ( -2.01911e-07  2.0136e-07 ) ergs/cm2

Band function

Time interval is from   20.712 sec. to  154.752 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -0.875982   ( 0.875731   0.740963 )
beta        : -1.81394    ( 1.8156   0.452709 )
Epeak [keV] : 110.533      ( -110.323 -110.323 )
Norm@50keV   : 3.32008E-03    ( -0.00137829   0 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          47.59 using 59 PHA bins.
# Reduced chi-squared =         0.8654 for     55 degrees of freedom 
# Null hypothesis probability =   7.505204e-01
 
Photon flux (15-150 keV)    in 134 sec: 0.219366 ( -0.018042  0.017635 ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.35899e-06 ( -1.80955e-07  1.67891e-07 ) ergs/cm2

Single BB

 
Spectral model blackbody:
------------------------------------------------------------
Parameters  : value    Lower 90%  Upper 90%
kT [keV]    : 17.0094  (-1.42087  1.59337)
R^2/D10^2   : 1.69256E-02  (-0.00454729   0.00604559)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          77.74 using 59 PHA bins.
# Reduced chi-squared =          1.364 for     57 degrees of freedom 
# Null hypothesis probability =   3.533214e-02
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.336e-07   2.013e-08
25- 50  5.915e-07   5.702e-08
50-150  1.222e-06   1.560e-07
15-150  1.947e-06   1.762e-07

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 200.000       (-27.1367      -200)
Norm        : 0.935018       (-0.0669293     0.0669293)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          53.01 using 59 PHA bins.
# Reduced chi-squared =         0.9300 for     57 degrees of freedom 
# Null hypothesis probability =   6.254676e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  3.120e-07   2.646e-08
25- 50  6.001e-07   5.735e-08
50-150  1.316e-06   3.295e-07
15-150  2.228e-06   4.187e-07

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 5.09543        (-1.41268      2.14734)
R1^2/D10^2  : 0.568504        (-0.412231      1.79496)
kT2 [keV]   : 21.4876        (-2.70912      4.34733)
R2^2/D10^2  : 6.76465E-03    (-0.00338873   0.00435609)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          48.01 using 59 PHA bins.
# Reduced chi-squared =         0.8729 for     55 degrees of freedom 
# Null hypothesis probability =   7.366360e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  2.780e-07   1.197e-07
25- 50  5.448e-07   1.369e-07
50-150  1.413e-06   2.403e-07
15-150  2.236e-06   3.873e-07

Peak spectrum fit

Power-law model

Time interval is from   25.704 sec. to   26.704 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 0.795291     ( -0.487892   0.422012 )
Norm@50keV  : 6.29325E-03    ( -0.00181609   0.00174449 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          69.71 using 59 PHA bins.
# Reduced chi-squared =          1.223 for     57 degrees of freedom 
# Null hypothesis probability =   1.204065e-01
 
Photon flux (15-150 keV)    in 1 sec: 0.723419 ( -0.196311  0.199705 ) ph/cm2/s
Energy fluence (15-150 keV)             : 7.36953e-08 ( -1.91358e-08  1.92313e-08 ) ergs/cm2

Cutoff power-law model

Time interval is from   25.704 sec. to   26.704 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: -0.288678     ( -3.29278   1.28263 )
Epeak [keV] : 126.197      ( -56.1118 -126.207 )
Norm@50keV  : 1.81383E-02    ( -0.0181351   0.324032 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          68.79 using 59 PHA bins.
# Reduced chi-squared =          1.228 for     56 degrees of freedom 
# Null hypothesis probability =   1.171652e-01
 
Photon flux (15-150 keV)    in 1 sec: 0.698419 ( -0.20041  0.204387 ) ph/cm2/s
Energy fluence (15-150 keV)             : 7.07115e-08 ( -2.14248e-08  2.04098e-08 ) ergs/cm2

Band function

Time interval is from   25.704 sec. to   26.704 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : 1.69570   ( -1.72888   -1.72888 )
beta        : -1.29145    ( 1.29754   0.828756 )
Epeak [keV] : 72.4947      ( -71.6454 196.152 )
Norm@50keV   : 0.101575    ( -0.114319   9.43913 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          68.17 using 59 PHA bins.
# Reduced chi-squared =          1.240 for     55 degrees of freedom 
# Null hypothesis probability =   1.093187e-01
 
Photon flux (15-150 keV)    in 1 sec: 0.682399 ( -0.1983  0.114574 ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.20755e-09 ( -2.20755e-09  5.71199e-09 ) ergs/cm2

Single BB

 
Spectral model blackbody:
------------------------------------------------------------
Parameters  : value    Lower 90%  Upper 90%
kT [keV]    : 24.3185  (-6.65526  12.0594)
R^2/D10^2   : 2.04599E-02  (-0.0143454   0.0359657)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          69.38 using 59 PHA bins.
# Reduced chi-squared =          1.217 for     57 degrees of freedom 
# Null hypothesis probability =   1.259254e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  2.132e-09   1.236e-09
25- 50  1.193e-08   5.543e-09
50-150  5.248e-08   2.780e-08
15-150  6.654e-08   3.859e-08

Thermal bremsstrahlung (OTTB)

 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 200.000       (-66.8853      -200)
Norm        : 2.99000       (-0.841361     0.841361)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          77.82 using 59 PHA bins.
# Reduced chi-squared =          1.365 for     57 degrees of freedom 
# Null hypothesis probability =   3.483243e-02
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  7.452e-09   4.549e-09
25- 50  1.434e-08   8.980e-09
50-150  3.144e-08   1.899e-08
15-150  5.323e-08   3.224e-08

Double BB

 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 17.2024        (-6.25339      14.2423)
R1^2/D10^2  : 4.61932E-02        (-0.0359221      -0.0461581)
kT2 [keV]   : 198.468        (-198.564      -198.564)
R2^2/D10^2  : 1.03247E-04    (-0.000104554   0.0422774)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          68.03 using 59 PHA bins.
# Reduced chi-squared =          1.237 for     55 degrees of freedom 
# Null hypothesis probability =   1.114805e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  2.906e-09   1.880e-09
25- 50  1.351e-08   9.330e-09
50-150  5.346e-08   2.957e-08
15-150  6.987e-08   4.239e-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: 1.28133     ( -0.127914   0.126313 )
Norm@50keV  : 2.44301E-03    ( -0.00017924   0.00017916 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          59.92 using 59 PHA bins.
# Reduced chi-squared =          1.051 for     57 degrees of freedom 
# Null hypothesis probability =   3.703203e-01
 
Photon flux (15-150 keV)    in 84.59 sec: 0.290479 ( -0.0225786  0.0226484 ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.0516e-06 ( -1.60372e-07  1.60883e-07 ) ergs/cm2

Cutoff power-law model

Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 0.724676     ( -0.610384   0.530598 )
Epeak [keV] : 126.220      ( -39.3231 873.101 )
Norm@50keV  : 4.41823E-03    ( -0.00187419   0.00382439 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          56.71 using 59 PHA bins.
# Reduced chi-squared =          1.013 for     56 degrees of freedom 
# Null hypothesis probability =   4.483155e-01
 
Photon flux (15-150 keV)    in 84.59 sec: 0.282770 ( -0.023857  0.023811 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.99227e-06 ( -1.73519e-07  1.72301e-07 ) ergs/cm2

Band function

 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -0.629053   ( -0.611684   3.4261 )
beta        : -1.72623    ( 1.73015   0.446335 )
Epeak [keV] : 111.235      ( -85.1777 630.3 )
Norm@50keV   : 4.97962E-03    ( -0.00227733   0.025859 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          56.57 using 59 PHA bins.
# Reduced chi-squared =          1.028 for     55 degrees of freedom 
# Null hypothesis probability =   4.162745e-01
 
Photon flux (15-150 keV)    in 84.59 sec: 0.282007 ( -0.024021  0.02395 ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.02624e-06 ( -1.63852e-07  1.40865e-07 ) ergs/cm2

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

S(25-50 keV)  = 5.61e-07
S(50-100 keV) = 8.52e-07

T90 vs. Hardness ratio plot

T90                                   = 114.799999952316 sec.
Hardness ratio (energy fluence ratio) = 1.51872

Color vs. Color plot

Count Ratio  (25-50 keV) / (15-25 keV) = 1.44268
Count Ratio (50-100 keV) / (15-25 keV) = 1.41639

Mask shadow pattern

IMX = -6.065525978282925E-01, IMY = -2.707984011356575E-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:
-15.899400 20.712000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
 83.6444  22.0098    0.5  20.4  171.7   1.5136  22.0    0.7	Crab                          
 75.6678  -7.2280    2.3  48.4 -166.1   0.7624   5.1 ------	UNKNOWN

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

Time interval of the image:
20.712000 105.300590
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
 83.6520  22.1700    5.6  20.2  171.6   0.3545   2.1    9.4	Crab                          
158.6722  70.3595    2.0  49.5   40.4   4.6475   5.7 ------	UNKNOWN                       
 95.9715  12.8063    0.9  33.6  155.9   3.1843  12.7 ------	UNKNOWN

Post-slew image of 15-350 keV band

Time interval of the image:
159.500610 963.090000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
 83.6314  22.0156    0.2  14.9  -55.2  34.0387  50.5    0.1	Crab                          
110.3803 -39.6390    2.5  54.2  161.4  16.1500   4.5 ------	UNKNOWN                       
 79.3575 -42.9600    2.8  57.8 -170.6  14.2879   4.1 ------	UNKNOWN                       
 82.3868  64.0425    4.5  52.1  -12.4   3.9923   2.6 ------	UNKNOWN                       
 67.2071  50.9094    3.1  44.7  -30.5   4.2165   3.8 ------	UNKNOWN                       
 69.8407 -39.0271    2.3  57.3 -160.9  16.8344   5.1 ------	UNKNOWN                       
 54.8982  21.3705    2.8  40.1  -76.9   9.6317   4.1 ------	UNKNOWN                       
 55.6091  -5.0222    2.2  43.9 -116.4  13.6272   5.3 ------	UNKNOWN

Plot creation:
Sun May 13 07:52:04 EDT 2018