Orbit Fit and Astrometric record for 14UC225

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: 14UC225   
# Created Sun Dec 22 02:10:06 2024
# Orbit generated by ELGB
# -->Covariance matrix from a Bernstein fit
# Fitting     20 observations of     20
# Arc:  10.86y
# First observation: 2013/11/22
#  Last observation: 2024/10/01
# Chi-squared of fit:     5.86 DOF:     34 RMS:  0.10
# Min/Max residuals:    -0.19    0.22
# Exact a, adot, b, bdot, g, gdot:
  1.858036E-05  3.823752E-02 -1.189858E-06 -1.697624E-03  3.257714E-02 -2.712456E-03
# Covariance matrix:
  3.0155E-13 -2.0032E-13 -8.1444E-15  7.9764E-15  3.7457E-14 -3.5128E-13
 -2.0032E-13  2.3767E-13  8.2944E-15 -9.6156E-15 -2.6971E-13  4.0672E-13
 -8.1444E-15  8.2944E-15  1.1680E-13 -1.5500E-14 -2.3638E-15  1.5627E-14
  7.9764E-15 -9.6156E-15 -1.5500E-14  5.2923E-15  9.6087E-15 -1.7041E-14
  3.7457E-14 -2.6971E-13 -2.3638E-15  9.6087E-15  1.1426E-12 -3.4130E-13
 -3.5128E-13  4.0672E-13  1.5627E-14 -1.7041E-14 -3.4130E-13  7.3098E-13
#      lat0       lon0       xBary       yBary       zBary        JD0
   -4.396986   18.710709   -0.646754   -0.056921   -0.742114  2456618.656888
# Heliocentric elements and errors
Epoch:              2456618.5000  =  2013/11/22
Mean Anomaly:          336.80879 +/-     0.027
Argument of Peri:      269.65989 +/-     0.034
Long of Asc Node:      139.63830 +/-     0.001
Inclination:             4.94034 +/-     0.000
Eccentricity:         0.11760102 +/-    0.0001
Semi-Major Axis:     35.15615371 +/-    0.0059
Time of Perihelion: 2461523.2997 +/-      18.9
Perihelion:          31.02175402 +/-    0.0064
Aphelion:            39.29055340 +/-    0.0076
Period (y)              208.4540 +/-      0.05
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X           29.48506187 +/-    0.0010
Ecliptic Y           10.67234253 +/-    0.0003
Ecliptic Z           -2.35347605 +/-    0.0001
Ecliptic XDOT        -0.00126267 +/-    0.0000
Ecliptic YDOT         0.00296544 +/-    0.0000
Ecliptic ZDOT        -0.00012463 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   31.44532532 +/-    0.0009
Geocenter to KBO     30.69644964 +/-    0.0010
# Hcoef:  7.41

The following table shows the complete astrometric record for 14UC225. 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 (14UC225) followed by the observatory code and reference code for the source of the astrometry.

2013 11  22.15611  01 15 44.098  +03 15 40.16  22.1i 14UC225   W84  C~4yUy      
2013 11  22.15893  01 15 44.093  +03 15 40.02  21.6z 14UC225   W84  C~4yUy      
2014 10  21.22515  01 26 53.312  +04 15 20.16  22.9g 14UC225   W84  C~4yUy      
2014 10  21.22651  01 26 53.286  +04 15 20.20  22.6r 14UC225   W84  C~4yUy      
2014 10  28.21303  01 26 12.591  +04 11 22.82  22.2r 14UC225   W84  C~4yUy      
2014 10  28.23025  01 26 12.486  +04 11 22.16  23.3g 14UC225   W84  C~4yUy      
2014 11  14.071181 01 24 41.22   +04 03 03.2   22.6r 14UC225   W84  C~352R      
2014 11  14.07171  01 24 41.223  +04 03 03.25  22.8r 14UC225   W84  C~4yUy      
2014 11  14.13577  01 24 40.896  +04 03 01.56  22.2i 14UC225   W84  C~4yUy      
2014 11  15.17294  01 24 35.754  +04 02 35.08  22.0i 14UC225   W84  C~4yUy      
2014 11  17.15109  01 24 26.148  +04 01 46.32  21.8z 14UC225   W84  C~4yUy      
2014 11  28.10420  01 23 38.333  +03 57 57.84  21.8z 14UC225   W84  C~4yUy      
2015 11  06.18503  01 33 47.028  +04 50 56.36  22.1r 14UC225   W84  C~4yUy      
2015 11  18.16042  01 32 43.99   +04 45 28.8   22.3z 14UC225   W84  C~3coL      
2015 12  18.07433  01 30 55.282  +04 38 00.00  22.3z 14UC225   W84  C~4yUy      
2017 09  23.37758  01 54 50.69   +06 42 49.5   22.2R 14UC225   G37  C~2LT9      
2017 09  23.46046  01 54 50.25   +06 42 46.7         14UC225   G37  C~2LT9      
2024 10  01.479802 02 54 57.369  +11 25 17.67  22.5w 14UC225   F52  C~8H4Q      
2024 10  01.491737 02 54 57.312  +11 25 16.97  22.4w 14UC225   F52  C~8H4Q      
2024 10  01.503681 02 54 57.248  +11 25 16.72  22.5w 14UC225   F52  C~8H4Q      

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    -0.03       0.00     0.07
     2   0.0000      0.00     0.07       0.00    -0.01
     3   0.9119      0.00     0.22       0.00    -0.07
     4   0.9119      0.00    -0.05       0.00     0.02
     5   0.9310      0.00    -0.00       0.00    -0.05
     6   0.9311      0.00    -0.07       0.00    -0.14
     7   0.9772      0.00    -0.04       0.00    -0.02
     8   0.9772      0.00     0.05       0.00     0.04
     9   0.9774      0.00     0.03       0.00     0.00
    10   0.9802      0.00     0.02       0.00    -0.06
    11   0.9856      0.00    -0.08       0.00    -0.05
    12   1.0156      0.00     0.01       0.00     0.03
    13   1.9549      0.00    -0.06       0.00    -0.05
    14   1.9877      0.00    -0.07       0.00    -0.07
    15   2.0696      0.00     0.09       0.00     0.14
    16   3.8363      0.00     0.12       0.00     0.20
    17   3.8366      0.00    -0.17       0.00     0.15
    18  10.8592      0.00     0.03       0.00     0.19
    19  10.8592      0.00     0.03       0.00    -0.19
    20  10.8593      0.00    -0.07       0.00    -0.11

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.

14UC225    quality flag:3

Type:           5:4E      5:4E      5:4E

axisobj        35.339    35.339    35.339
ecceobj         0.121     0.120     0.121
incobj          4.933     4.933     4.933
qmin           30.629    30.593    30.597
qmax           39.827    39.835    39.854
amean          34.944    34.944    34.944
amin           34.524    34.519    34.508
amax           35.392    35.407    35.410
emean           0.104     0.104     0.104
emin            0.083     0.083     0.083
emax            0.126     0.125     0.126
imean           3.094     3.104     3.063
imin            1.913     1.973     1.928
imax            4.190     4.187     4.194
excite_mean     0.118     0.118     0.118
fracstop        1.000     1.000     1.000
cjmean          3.002     3.001     3.002

libcent 0       179.6     178.4     180.4
libamp  0       116.0     117.3     118.2
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       177.2     183.7     181.9
kozaiamp        180.0     180.0     180.0