Orbit Fit and Astrometric record for 13CG269

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: 13CG269   
# Created Mon Jul  7 01:09:26 2025
# Orbit generated by ELGB
# -->Covariance matrix from a Bernstein fit
# Fitting     21 observations of     21
# Arc:   9.26y
# First observation: 2013/02/04
#  Last observation: 2022/05/10
# Chi-squared of fit:     7.58 DOF:     36 RMS:  0.11
# Min/Max residuals:    -0.31    0.21
# Exact a, adot, b, bdot, g, gdot:
  1.598101E-05  2.517881E-02 -3.378111E-08  5.640436E-04  2.478314E-02 -1.843659E-04
# Covariance matrix:
  3.9709E-13 -1.1552E-13  2.3732E-15 -1.7890E-15  5.0783E-14 -3.7612E-13
 -1.1552E-13  7.6717E-14 -2.0051E-15  1.4674E-15  5.0370E-14  3.3938E-13
  2.3732E-15 -2.0051E-15  2.8410E-13 -5.9761E-14 -8.6255E-16 -1.1825E-14
 -1.7890E-15  1.4674E-15 -5.9761E-14  1.6599E-14  5.4830E-16  8.7063E-15
  5.0783E-14  5.0370E-14 -8.6255E-16  5.4830E-16  1.9733E-13  1.8670E-13
 -3.7612E-13  3.3938E-13 -1.1825E-14  8.7063E-15  1.8670E-13  1.9759E-12
#      lat0       lon0       xBary       yBary       zBary        JD0
    1.634196 -164.075635    0.855484    0.014004   -0.487844  2456327.828402
# Heliocentric elements and errors
Epoch:              2456328.5000  =  2013/02/05
Mean Anomaly:          339.99317 +/-     0.041
Argument of Peri:       73.84241 +/-     0.048
Long of Asc Node:      143.96319 +/-     0.007
Inclination:             2.08401 +/-     0.000
Eccentricity:         0.07146141 +/-    0.0001
Semi-Major Axis:     43.75408644 +/-    0.0032
Time of Perihelion: 2462203.4217 +/-      16.3
Perihelion:          40.62735752 +/-    0.0037
Aphelion:            46.88081537 +/-    0.0041
Period (y)              289.4251 +/-      0.03
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X          -39.48856823 +/-    0.0007
Ecliptic Y          -10.37563013 +/-    0.0002
Ecliptic Z            1.15067020 +/-    0.0000
Ecliptic XDOT         0.00077826 +/-    0.0000
Ecliptic YDOT        -0.00266775 +/-    0.0000
Ecliptic ZDOT         0.00006184 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   40.84514841 +/-    0.0007
Geocenter to KBO     40.35003793 +/-    0.0007
# Hcoef:  6.86

The following table shows the complete astrometric record for 13CG269. 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 (13CG269) followed by the observatory code and reference code for the source of the astrometry.

2013 02  04.327624 13 01 12.075  -04 45 24.80  22.6z 13CG269   W84  C~8vD4      
2013 02  06.392143 13 01 08.32   -04 44 55.8   22.7z 13CG269   W84  C~8vD4      
2013 02  08.393616 13 01 04.326  -04 44 25.60  22.6z 13CG269   W84  C~8vD4      
2013 06  16.088846 12 53 40.06   -03 57 58.9   22.7i 13CG269   W84  C~8vD4      
2016 07  22.048426 13 10 00.79   -05 34 36.4   22.7z 13CG269   W84  C~8vD4      
2016 08  12.002386 13 10 58.15   -05 41 14.0   22.6z 13CG269   W84  C~8vD4      
2017 02  24.561983 13 22 12.84   -06 44 53.8   23.3r 13CG269   T09  C~8vD4      
2017 02  24.622738 13 22 12.66   -06 44 52.6   23.3r 13CG269   T09  C~8vD4      
2017 03  23.248598 13 20 34.301  -06 34 12.04  23.0w 13CG269   W84  C~8vD4      
2017 03  23.271319 13 20 34.20   -06 34 11.4   23.0w 13CG269   W84  C~8vD4      
2017 03  24.266573 13 20 29.88   -06 33 44.1   23.1w 13CG269   W84  C~8vD4      
2017 03  24.319946 13 20 29.66   -06 33 42.9   23.1w 13CG269   W84  C~8vD4      
2017 03  25.226454 13 20 25.70   -06 33 18.0   23.0w 13CG269   W84  C~8vD4      
2017 03  25.237477 13 20 25.653  -06 33 17.66  23.1w 13CG269   W84  C~8vD4      
2017 03  26.230919 13 20 21.287  -06 32 50.25  23.2w 13CG269   W84  C~8vD4      
2017 03  26.276502 13 20 21.09   -06 32 49.1   23.2w 13CG269   W84  C~8vD4      
2017 03  26.324599 13 20 20.861  -06 32 47.66  23.2w 13CG269   W84  C~8vD4      
2017 05  21.110962 13 16 21.09   -06 08 56.9   23.1r 13CG269   W84  C~8vD4      
2017 07  18.081017 13 15 15.84   -06 04 31.1   24.0g 13CG269   W84  C~8vD4      
2017 07  19.067649 13 15 17.23   -06 04 41.9   23.0r 13CG269   W84  C~8vD4      
2022 05  10.156415 13 44 48.34   -08 47 01.5   22.8i 13CG269   W84  C~8vD4      

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     0.05       0.00     0.07
     2   0.0057      0.00     0.12       0.00     0.10
     3   0.0111      0.00    -0.04       0.00     0.18
     4   0.3607      0.00    -0.05       0.00    -0.09
     5   3.4599      0.00     0.15       0.00     0.05
     6   3.5172      0.00    -0.02       0.00    -0.12
     7   4.0554      0.00    -0.06       0.00    -0.08
     8   4.0556      0.00    -0.05       0.00    -0.09
     9   4.1285      0.00    -0.04       0.00     0.05
    10   4.1285      0.00    -0.05       0.00     0.07
    11   4.1312      0.00    -0.13       0.00     0.20
    12   4.1314      0.00     0.11       0.00    -0.06
    13   4.1339      0.00    -0.01       0.00    -0.03
    14   4.1339      0.00     0.02       0.00     0.00
    15   4.1366      0.00     0.03       0.00     0.02
    16   4.1368      0.00     0.14       0.00    -0.09
    17   4.1369      0.00    -0.06       0.00     0.02
    18   4.2896      0.00    -0.00       0.00    -0.31
    19   4.4483      0.00    -0.13       0.00    -0.08
    20   4.4510      0.00    -0.18       0.00     0.02
    21   9.2589      0.00     0.10       0.00     0.21

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.

13CG269    quality flag:3

Type:      CLASSICAL CLASSICAL CLASSICAL

axisobj        43.579    43.579    43.579
ecceobj         0.068     0.068     0.068
incobj          2.087     2.087     2.087
qmin           40.097    40.095    40.100
qmax           47.843    47.820    47.849
amean          43.848    43.848    43.848
amin           43.496    43.504    43.501
amax           44.230    44.214    44.227
emean           0.065     0.065     0.065
emin            0.048     0.048     0.048
emax            0.082     0.082     0.082
imean           1.939     1.939     1.939
imin            1.179     1.179     1.180
imax            2.626     2.626     2.626
excite_mean     0.074     0.074     0.074
fracstop        1.000     1.000     1.000
cjmean          3.093     3.093     3.093

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       166.3     166.2     166.3
kozaiamp        180.0     180.0     180.0