Orbit Fit and Astrometric record for 13WG114

The following information shows the result of the orbit fit based on Gary Bernstein's method. Most of the information should be self-explanatory. Take special note that while the original Bernstein software works with barycentric coordinates, we convert these results into a heliocentric coordinate system.

# Object: 13WG114   
# Created Tue Apr  1 01:09:55 2025
# Orbit generated by ELGB
# -->Covariance matrix from a Bernstein fit
# Fitting     35 observations of     35
# Arc:   5.17y
# First observation: 2013/09/08
#  Last observation: 2018/11/09
# Chi-squared of fit:     8.31 DOF:     64 RMS:  0.09
# Min/Max residuals:    -0.20    0.26
# Exact a, adot, b, bdot, g, gdot:
  1.544345E-05  2.485120E-02  3.703294E-07  2.389762E-04  2.470672E-02  6.325245E-04
# Covariance matrix:
  2.5857E-13 -2.4026E-14 -1.0842E-15  2.6422E-16  1.7710E-13  1.4564E-13
 -2.4026E-14  1.6301E-13 -1.5889E-15  1.8039E-15  1.5022E-13  1.3998E-12
 -1.0842E-15 -1.5889E-15  1.3336E-13 -3.3470E-14 -2.9088E-15 -1.5216E-14
  2.6422E-16  1.8039E-15 -3.3470E-14  1.2304E-14  2.0016E-15  1.6824E-14
  1.7710E-13  1.5022E-13 -2.9088E-15  2.0016E-15  3.7538E-13  1.4734E-12
  1.4564E-13  1.3998E-12 -1.5216E-14  1.6824E-14  1.4734E-12  1.3028E-11
#      lat0       lon0       xBary       yBary       zBary        JD0
   -1.400466    1.993067    0.288343   -0.023532   -0.966035  2456543.690868
# Heliocentric elements and errors
Epoch:              2456544.5000  =  2013/09/09
Mean Anomaly:           13.78052 +/-     0.119
Argument of Peri:      275.88717 +/-     0.137
Long of Asc Node:       70.02986 +/-     0.009
Inclination:             1.47072 +/-     0.000
Eccentricity:         0.06413914 +/-    0.0001
Semi-Major Axis:     44.18258181 +/-    0.0039
Time of Perihelion: 2452438.3191 +/-      35.5
Perihelion:          41.34874888 +/-    0.0046
Aphelion:            47.01641474 +/-    0.0050
Period (y)              293.6871 +/-      0.04
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X           41.41371263 +/-    0.0010
Ecliptic Y            1.15577179 +/-    0.0000
Ecliptic Z           -0.98920996 +/-    0.0000
Ecliptic XDOT        -0.00003128 +/-    0.0000
Ecliptic YDOT         0.00275351 +/-    0.0000
Ecliptic ZDOT         0.00002490 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   41.44163451 +/-    0.0010
Geocenter to KBO     40.47483417 +/-    0.0010
# Hcoef:  6.52

The following table shows the complete astrometric record for 13WG114. The first three columns show the date of observation. The next six columns are RA and DEC. The next column (when provided) is the observed magnitude and filter. The next column is the object name (13WG114) followed by the observatory code and reference code for the source of the astrometry.

2013 09  08.19009  00 09 32.516  -00 29 32.57  23.6g 13WG114   W84  C~4yRf      
2013 09  11.30866  00 09 19.100  -00 31 01.06  23.6g 13WG114   W84  C~4yRf      
2013 09  24.26905  00 08 21.589  -00 37 15.99  22.1Y 13WG114   W84  C~4yRf      
2013 10  13.09753  00 06 58.489  -00 46 05.93  21.9z 13WG114   W84  C~4yRf      
2013 11  22.06844  00 04 48.704  -00 59 06.20  24.1g 13WG114   W84  C~4yRf      
2013 11  22.06982  00 04 48.705  -00 59 06.21  22.9r 13WG114   W84  C~4yRf      
2013 11  22.07119  00 04 48.694  -00 59 06.18  22.6i 13WG114   W84  C~4yRf      
2013 11  23.09553  00 04 46.790  -00 59 16.51  22.4i 13WG114   W84  C~4yRf      
2014 10  02.25127  00 12 58.964  -00 06 17.10  23.7g 13WG114   W84  C~4yRf      
2014 10  02.25263  00 12 58.959  -00 06 17.10  22.5i 13WG114   W84  C~4yRf      
2014 10  28.19540  00 11 10.644  -00 17 36.47  22.8r 13WG114   W84  C~4yRf      
2014 11  15.101019 00 10 13.85   -00 23 15.4   21.9z 13WG114   W84  C~352E      
2014 11  15.10154  00 10 13.853  -00 23 15.43  21.8z 13WG114   W84  C~4yRf      
2015 11  02.096007 00 16 04.09   +00 15 11.3   23.1r 13WG114   W84  C~352E      
2015 11  02.09653  00 16 04.101  +00 15 11.28  22.8r 13WG114   W84  C~4yRf      
2016 11  30.10650  00 19 57.067  +00 42 13.40  22.4i 13WG114   W84  C~4yRf      
2016 11  30.10788  00 19 57.071  +00 42 13.40  23.2r 13WG114   W84  C~4yRf      
2016 12  04.08842  00 19 51.464  +00 41 45.76  22.9z 13WG114   W84  C~4yRf      
2016 12  05.09585  00 19 50.256  +00 41 40.14  22.4z 13WG114   W84  C~4yRf      
2017 08  27.36996  00 31 01.90   +01 53 41.5   23.0r 13WG114   T09  C~7bIM      
2017 08  27.39162  00 31 01.83   +01 53 40.8   23.0r 13WG114   T09  C~7bIM      
2017 08  27.43568  00 31 01.66   +01 53 39.8   23.1r 13WG114   T09  C~7bIM      
2017 10  22.18159  00 27 04.164  +01 28 10.15  22.0r 13WG114   W84  C~4yRf      
2017 10  22.182431 00 27 04.15   +01 28 10.1   21.5i 13WG114   W84  C~352E      
2017 10  22.18295  00 27 04.176  +01 28 09.85  21.1i 13WG114   W84  C~4yRf      
2017 10  27.173773 00 26 44.01   +01 26 05.8   22.2z 13WG114   W84  C~352E      
2017 10  27.17431  00 26 44.018  +01 26 05.73  22.1z 13WG114   W84  C~4yRf      
2017 10  29.146169 00 26 36.35   +01 25 18.9   22.3z 13WG114   W84  C~352E      
2017 10  29.14670  00 26 36.353  +01 25 18.76  22.2z 13WG114   W84  C~4yRf      
2018 09  09.32306  00 35 23.269  +02 22 37.05  22.5i 13WG114   W84  C~4yRf      
2018 09  09.32445  00 35 23.268  +02 22 37.02  22.8r 13WG114   W84  C~4yRf      
2018 09  09.32583  00 35 23.263  +02 22 37.01  23.9g 13WG114   W84  C~4yRf      
2018 10  18.15348  00 32 32.650  +02 04 26.35  21.8z 13WG114   W84  C~4yRf      
2018 10  18.19053  00 32 32.493  +02 04 25.18  22.3i 13WG114   W84  C~4yRf      
2018 11  09.14493  00 31 07.077  +01 55 43.14  23.1r 13WG114   W84  C~4yRf      

The following table shows the residuals to the orbit fit. The first coumn is the point number. The second column is the time, in years, measured from the first observation. The third and fifth columns are the regularized positions used in the orbit fit. The fourth and sixth columns are the residuals, in arc seconds, for RA and Dec respectively.

     1   0.0000      0.00     0.11       0.00    -0.00
     2   0.0085      0.00     0.10       0.00    -0.09
     3   0.0440      0.00    -0.03       0.00    -0.04
     4   0.0956      0.00    -0.08       0.00    -0.04
     5   0.2050      0.00    -0.06       0.00     0.02
     6   0.2050      0.00    -0.01       0.00     0.02
     7   0.2050      0.00    -0.13       0.00     0.06
     8   0.2078      0.00     0.14       0.00     0.03
     9   1.0652      0.00     0.02       0.00     0.03
    10   1.0652      0.00     0.04       0.00     0.07
    11   1.1362      0.00     0.02       0.00     0.01
    12   1.1852      0.00    -0.13       0.00    -0.06
    13   1.1852      0.00    -0.06       0.00    -0.09
    14   2.1490      0.00     0.05       0.00     0.13
    15   2.1490      0.00     0.24       0.00     0.13
    16   3.2277      0.00    -0.11       0.00    -0.00
    17   3.2277      0.00    -0.01       0.00     0.01
    18   3.2386      0.00     0.04       0.00    -0.00
    19   3.2414      0.00    -0.03       0.00    -0.08
    20   3.9676      0.00    -0.11       0.00     0.09
    21   3.9677      0.00     0.02       0.00    -0.10
    22   3.9678      0.00    -0.13       0.00    -0.04
    23   4.1204      0.00    -0.00       0.00     0.07
    24   4.1204      0.00    -0.16       0.00     0.04
    25   4.1204      0.00     0.26       0.00    -0.20
    26   4.1341      0.00    -0.14       0.00     0.00
    27   4.1341      0.00     0.01       0.00    -0.05
    28   4.1395      0.00    -0.00       0.00     0.12
    29   4.1395      0.00     0.07       0.00    -0.01
    30   5.0024      0.00    -0.03       0.00    -0.01
    31   5.0024      0.00     0.04       0.00    -0.01
    32   5.0024      0.00     0.05       0.00     0.02
    33   5.1087      0.00     0.02       0.00     0.08
    34   5.1088      0.00     0.10       0.00    -0.09
    35   5.1689      0.00     0.04       0.00     0.06

The following table comes from a 10My integration of the orbit of the object. Three columns are shown. The first column is the result of integrating the nominal orbit. The other two columns are based on clones of the nominal orbit that are +/- 3 sigma from the nominal orbit. If all three types agree then the classificiation is deemed secure. The basis for these calculations is described in more detail in AJ, 129, 1117 (2005). Any use made of these calculations should refer to and credit this publication and the Deep Ecliptic Survey Team.

13WG114    quality flag:3

Type:      CLASSICAL CLASSICAL CLASSICAL

axisobj        44.441    44.441    44.441
ecceobj         0.070     0.070     0.070
incobj          1.471     1.471     1.471
qmin           40.474    40.475    40.473
qmax           48.171    48.170    48.179
amean          44.213    44.213    44.213
amin           43.860    43.860    43.860
amax           44.589    44.589    44.590
emean           0.065     0.065     0.065
emin            0.049     0.049     0.049
emax            0.080     0.080     0.080
imean           0.747     0.747     0.747
imin            0.101     0.099     0.101
imax            1.191     1.191     1.191
excite_mean     0.066     0.066     0.066
fracstop        1.000     1.000     1.000
cjmean          3.099     3.099     3.099

libcent 0      -180.0    -180.0    -180.0
libamp  0      -180.0    -180.0    -180.0
libcent 1      -180.0    -180.0    -180.0
libamp  1      -180.0    -180.0    -180.0
libcent 2      -180.0    -180.0    -180.0
libamp  2      -180.0    -180.0    -180.0
libcent 3      -180.0    -180.0    -180.0
libamp  3      -180.0    -180.0    -180.0
libcent 4      -180.0    -180.0    -180.0
libamp  4      -180.0    -180.0    -180.0

kozaimean       200.8     200.8     201.0
kozaiamp        180.0     180.0     179.9