Orbit Fit and Astrometric record for 18FL73

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: 18FL73    
# Created Tue Apr  1 01:11:09 2025
# Orbit generated by ELGB
# -->Covariance matrix from a Bernstein fit
# Fitting     21 observations of     21
# Arc:   5.01y
# First observation: 2014/02/28
#  Last observation: 2019/03/02
# Chi-squared of fit:     7.07 DOF:     36 RMS:  0.10
# Min/Max residuals:    -0.25    0.21
# Exact a, adot, b, bdot, g, gdot:
  1.526279E-05  2.246285E-02 -1.938259E-07 -9.141406E-04  2.343934E-02 -2.676911E-03
# Covariance matrix:
  3.6694E-13 -1.6422E-13 -5.4227E-16  3.4395E-15 -8.3582E-14 -7.9249E-13
 -1.6422E-13  1.2232E-12  8.2199E-15 -4.6219E-14  1.7147E-12  1.0859E-11
 -5.4227E-16  8.2199E-15  3.5441E-13 -7.9391E-14  1.1966E-14  7.4156E-14
  3.4395E-15 -4.6219E-14 -7.9391E-14  2.3666E-14 -6.5020E-14 -4.1834E-13
 -8.3582E-14  1.7147E-12  1.1966E-14 -6.5020E-14  2.6674E-12  1.5366E-11
 -7.9249E-13  1.0859E-11  7.4156E-14 -4.1834E-13  1.5366E-11  9.8228E-11
#      lat0       lon0       xBary       yBary       zBary        JD0
    2.611665  172.439668    0.218041    0.044042   -0.963364  2456716.991570
# Heliocentric elements and errors
Epoch:              2456716.5000  =  2014/02/28
Mean Anomaly:          292.40158 +/-     0.050
Argument of Peri:      213.88234 +/-     0.031
Long of Asc Node:       39.81365 +/-     0.004
Inclination:             3.45300 +/-     0.000
Eccentricity:         0.12551863 +/-    0.0005
Semi-Major Axis:     45.14036135 +/-    0.0133
Time of Perihelion: 2477517.3001 +/-      42.7
Perihelion:          39.47440489 +/-    0.0244
Aphelion:            50.80631780 +/-    0.0262
Period (y)              303.2884 +/-      0.13
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X          -43.17722887 +/-    0.0029
Ecliptic Y            5.95189206 +/-    0.0004
Ecliptic Z            1.94400668 +/-    0.0001
Ecliptic XDOT        -0.00004616 +/-    0.0000
Ecliptic YDOT        -0.00264441 +/-    0.0000
Ecliptic ZDOT        -0.00012078 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   43.62893698 +/-    0.0029
Geocenter to KBO     42.66343096 +/-    0.0030
# Hcoef:  6.89

The following table shows the complete astrometric record for 18FL73. 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 (18FL73) followed by the observatory code and reference code for the source of the astrometry.

2014 02  28.490792 11 36 22.25   +05 23 55.7         18FL73    T09  C~89VM      
2014 02  28.505033 11 36 22.19   +05 23 56.2         18FL73    T09  C~89VM      
2014 02  28.524138 11 36 22.11   +05 23 56.7         18FL73    T09  C~89VM      
2014 02  28.566397 11 36 21.93   +05 23 57.8         18FL73    T09  C~89VM      
2018 03  18.46645  11 53 55.90   +03 15 44.4   22.9i 18FL73    T09  C~86yU      
2018 03  18.46982  11 53 55.87   +03 15 44.5   22.8i 18FL73    T09  C~86yU      
2018 03  18.51105  11 53 55.71   +03 15 45.7   23.0i 18FL73    T09  C~86yU      
2018 03  18.56803  11 53 55.45   +03 15 47.1   23.6i 18FL73    T09  C~86yU      
2018 04  24.40415  11 51 25.82   +03 30 53.7   22.9z 18FL73    T09  C~86yU      
2018 04  24.40683  11 51 25.79   +03 30 53.7   23.2z 18FL73    T09  C~86yU      
2018 04  24.45059  11 51 25.65   +03 30 54.6   22.7z 18FL73    T09  C~86yU      
2018 04  24.49071  11 51 25.50   +03 30 55.4   22.6z 18FL73    T09  C~86yU      
2018 06  09.043981 11 50 01.335  +03 37 14.20        18FL73    X11  C~86yU      
2018 06  09.049178 11 50 01.333  +03 37 14.20        18FL73    X11  C~86yU      
2018 06  09.051771 11 50 01.330  +03 37 14.20        18FL73    X11  C~86yU      
2019 02  02.644951 12 01 29.23   +02 22 07.3         18FL73    T09  C~89VM      
2019 02  04.590836 12 01 23.80   +02 22 46.6         18FL73    T09  C~89VM      
2019 03  02.42071  11 59 51.58   +02 33 20.1   22.7y 18FL73    T09  C~8CPH      
2019 03  02.52415  11 59 51.15   +02 33 22.9   23.2y 18FL73    T09  C~8CPH      
2019 03  02.56456  11 59 50.97   +02 33 23.8   23.1y 18FL73    T09  C~8CPH      
2019 03  02.60552  11 59 50.80   +02 33 25.1   23.0y 18FL73    T09  C~8CPH      

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    -0.06       0.00    -0.07
     2   0.0000      0.00    -0.04       0.00     0.04
     3   0.0001      0.00    -0.00       0.00     0.01
     4   0.0002      0.00     0.03       0.00    -0.06
     5   4.0492      0.00    -0.00       0.00     0.05
     6   4.0492      0.00    -0.23       0.00     0.06
     7   4.0493      0.00     0.14       0.00     0.10
     8   4.0495      0.00     0.06       0.00    -0.09
     9   4.1503      0.00     0.21       0.00     0.01
    10   4.1504      0.00    -0.10       0.00    -0.04
    11   4.1505      0.00     0.07       0.00     0.02
    12   4.1506      0.00    -0.11       0.00     0.06
    13   4.2753      0.00     0.09       0.00     0.14
    14   4.2753      0.00     0.08       0.00     0.16
    15   4.2753      0.00     0.04       0.00     0.17
    16   4.9286      0.00     0.06       0.00    -0.07
    17   4.9339      0.00     0.10       0.00    -0.08
    18   5.0046      0.00    -0.10       0.00    -0.01
    19   5.0049      0.00    -0.02       0.00    -0.04
    20   5.0050      0.00    -0.17       0.00    -0.25
    21   5.0051      0.00    -0.14       0.00    -0.07

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.

18FL73    quality flag:3

Type:      CLASSICAL CLASSICAL CLASSICAL

axisobj        44.824    44.823    44.824
ecceobj         0.124     0.124     0.124
incobj          3.458     3.458     3.458
qmin           38.824    38.826    38.825
qmax           51.619    51.621    51.616
amean          45.039    45.039    45.039
amin           44.667    44.654    44.665
amax           45.460    45.453    45.451
emean           0.120     0.120     0.120
emin            0.104     0.104     0.104
emax            0.136     0.136     0.136
imean           2.705     2.705     2.704
imin            2.022     2.021     2.023
imax            3.287     3.287     3.288
excite_mean     0.129     0.129     0.129
fracstop        1.000     1.000     1.000
cjmean          3.094     3.094     3.094

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       186.9     186.9     186.9
kozaiamp        180.0     179.9     180.0