Orbit Fit and Astrometric record for 14WM517

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: 14WM517   
# Created Sat Feb 22 02:10:16 2025
# Orbit generated by ELGB
# -->Covariance matrix from a Bernstein fit
# Fitting     49 observations of     49
# Arc:   5.03y
# First observation: 2014/11/23
#  Last observation: 2019/12/04
# Chi-squared of fit:    87.68 DOF:     92 RMS:  0.24
# Min/Max residuals:    -0.51    1.54
# Exact a, adot, b, bdot, g, gdot:
  1.392947E-05  1.938070E-02 -1.357159E-06 -3.260084E-03  2.147145E-02  1.072500E-03
# Covariance matrix:
  9.5673E-14 -5.5809E-14 -2.3793E-15  5.4336E-15 -2.1018E-14 -3.7597E-13
 -5.5809E-14  1.4789E-13  1.1171E-14 -2.1016E-14 -1.8787E-14  1.4698E-12
 -2.3793E-15  1.1171E-14  8.1050E-14 -2.4648E-14 -2.5368E-15  1.1899E-13
  5.4336E-15 -2.1016E-14 -2.4648E-14  1.4209E-14  1.5833E-15 -2.2678E-13
 -2.1018E-14 -1.8787E-14 -2.5368E-15  1.5833E-15  8.7632E-14 -1.2422E-13
 -3.7597E-13  1.4698E-12  1.1899E-13 -2.2678E-13 -1.2422E-13  1.5848E-11
#      lat0       lon0       xBary       yBary       zBary        JD0
  -17.462036   27.170108   -0.543666   -0.247401   -0.786998  2456984.818227
# Heliocentric elements and errors
Epoch:              2456984.5000  =  2014/11/23
Mean Anomaly:           80.83455 +/-     0.056
Argument of Peri:      154.05591 +/-     0.049
Long of Asc Node:      147.19376 +/-     0.001
Inclination:            19.50632 +/-     0.000
Eccentricity:         0.06301727 +/-    0.0002
Semi-Major Axis:     47.65392774 +/-    0.0042
Time of Perihelion: 2430004.5578 +/-      19.0
Perihelion:          44.65090746 +/-    0.0106
Aphelion:            50.65694803 +/-    0.0108
Period (y)              328.9700 +/-      0.04
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X           40.00752942 +/-    0.0005
Ecliptic Y           21.14895556 +/-    0.0003
Ecliptic Z          -13.97556062 +/-    0.0002
Ecliptic XDOT        -0.00112761 +/-    0.0000
Ecliptic YDOT         0.00219617 +/-    0.0000
Ecliptic ZDOT        -0.00043748 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   47.36235880 +/-    0.0005
Geocenter to KBO     46.57347348 +/-    0.0006
# Hcoef:  7.37

The following table shows the complete astrometric record for 14WM517. 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 (14WM517) followed by the observatory code and reference code for the source of the astrometry.

2014 11  23.317449 02 05 47.646  -05 51 24.88  23.9i 14WM517   568  C~2Tu9      
2014 11  23.436477 02 05 47.203  -05 51 25.84  23.7i 14WM517   568  C~2Tu9      
2014 11  23.459204 02 05 47.125  -05 51 25.98  23.7i 14WM517   568  C~2Tu9      
2014 11  23.474241 02 05 47.065  -05 51 26.21  23.7i 14WM517   568  C~2Tu9      
2014 11  25.31047  02 05 40.58   -05 51 40.5   23.5z 14WM517   T09  C~8eQP      
2014 11  25.33076  02 05 40.53   -05 51 40.4   23.6z 14WM517   T09  C~8eQP      
2014 11  25.34737  02 05 40.44   -05 51 40.5   23.9z 14WM517   T09  C~8eQP      
2014 11  25.47935  02 05 39.97   -05 51 39.9   23.7g 14WM517   T09  C~8eQP      
2014 11  28.363340 02 05 30.116  -05 51 59.60  24.1r 14WM517   568  C~2Tu9      
2014 11  28.382242 02 05 30.055  -05 51 59.73  24.2r 14WM517   568  C~2Tu9      
2014 11  28.403031 02 05 29.981  -05 51 59.75  24.3r 14WM517   568  C~2Tu9      
2014 11  28.419743 02 05 29.920  -05 51 59.90  24.3r 14WM517   568  C~2Tu9      
2014 11  28.457239 02 05 29.793  -05 52 00.07  23.8i 14WM517   568  C~2Tu9      
2014 11  28.463420 02 05 29.768  -05 52 00.07  24.0i 14WM517   568  C~2Tu9      
2014 11  28.474502 02 05 29.731  -05 52 00.22  23.4i 14WM517   568  C~2Tu9      
2014 11  28.479935 02 05 29.722  -05 52 00.17  23.9i 14WM517   568  C~2Tu9      
2016 08  15.413247 02 19 49.04   -04 42 32.1   23.9r 14WM517   W84  C~2b7x      
2016 08  25.389451 02 19 39.38   -04 47 14.2   23.7i 14WM517   W84  C~2b7x      
2016 08  25.393432 02 19 39.37   -04 47 14.5   23.7z 14WM517   W84  C~2b7x      
2016 09  22.172506 02 18 35.93   -05 01 35.7   24.0r 14WM517   W84  C~2b7x      
2016 11  02.061951 02 15 59.86   -05 19 54.0   24.1r 14WM517   W84  C~2b7x      
2016 11  02.064312 02 15 59.88   -05 19 54.0   23.5i 14WM517   W84  C~2b7x      
2016 11  09.059589 02 15 31.28   -05 22 01.3   23.2i 14WM517   W84  C~2b7x      
2017 08  17.374372 02 24 08.49   -04 29 59.3   23.8z 14WM517   W84  C~2b7x      
2017 08  17.405716 02 24 08.47   -04 30 00.2   24.5r 14WM517   W84  C~2b7x      
2017 08  18.283969 02 24 07.90   -04 30 24.3   23.9i 14WM517   W84  C~2b7x      
2017 08  24.386360 02 24 02.14   -04 33 16.9   24.1r 14WM517   W84  C~2b7x      
2017 08  24.415295 02 24 02.11   -04 33 17.5   24.0i 14WM517   W84  C~2b7x      
2017 08  25.363711 02 24 00.97   -04 33 45.1   24.0z 14WM517   W84  C~2b7x      
2017 09  13.333774 02 23 24.67   -04 43 24.3   23.8z 14WM517   W84  C~2b7x      
2017 09  14.217344 02 23 22.40   -04 43 52.4   24.6r 14WM517   W84  C~2b7x      
2017 09  19.271041 02 23 08.48   -04 46 31.1   24.1i 14WM517   W84  C~2b7x      
2017 09  19.307707 02 23 08.40   -04 46 31.7   23.6z 14WM517   W84  C~2b7x      
2017 09  23.249196 02 22 56.54   -04 48 35.2   24.3z 14WM517   W84  C~2b7x      
2017 09  23.298316 02 22 56.38   -04 48 37.2   24.9g 14WM517   W84  C~2b7x      
2017 09  23.310902 02 22 56.34   -04 48 37.1   24.3r 14WM517   W84  C~2b7x      
2017 09  25.179441 02 22 50.44   -04 49 35.4   24.1i 14WM517   W84  C~2b7x      
2017 10  02.287746 02 22 26.45   -04 53 11.7   24.1i 14WM517   W84  C~2b7x      
2017 10  10.131962 02 21 57.61   -04 57 00.5   23.3z 14WM517   W84  C~2b7x      
2017 12  22.048258 02 17 34.05   -05 11 49.9   23.6i 14WM517   W84  C~2b7x      
2018 01  04.092506 02 17 12.07   -05 09 15.1   23.4i 14WM517   W84  C~2b7x      
2018 01  04.099115 02 17 12.09   -05 09 14.9   23.6z 14WM517   W84  C~2b7x      
2019 10  27.43225  02 29 36.52   -04 37 00.2   24.4i 14WM517   T09  C~7bKK      
2019 10  27.45055  02 29 36.43   -04 37 00.7   24.2i 14WM517   T09  C~7bKK      
2019 10  27.46883  02 29 36.36   -04 37 00.9   24.4i 14WM517   T09  C~7bKK      
2019 12  04.33301  02 27 08.03   -04 45 40.3   25.4z 14WM517   T09  C~7bKK      
2019 12  04.35514  02 27 07.94   -04 45 40.5   24.8z 14WM517   T09  C~7bKK      
2019 12  04.40339  02 27 07.77   -04 45 40.5   24.9i 14WM517   T09  C~7bKK      
2019 12  04.44735  02 27 07.62   -04 45 40.8   24.2i 14WM517   T09  C~7bKK      

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     0.14       0.00    -0.18
     2   0.0003      0.00     0.01       0.00    -0.14
     3   0.0004      0.00     0.08       0.00    -0.10
     4   0.0004      0.00     0.00       0.00    -0.20
     5   0.0055      0.00    -0.07       0.00    -0.26
     6   0.0055      0.00     0.27       0.00    -0.01
     7   0.0056      0.00    -0.19       0.00     0.01
     8   0.0059      0.00    -0.20       0.00     1.54
     9   0.0138      0.00     0.04       0.00    -0.13
    10   0.0139      0.00     0.10       0.00    -0.16
    11   0.0139      0.00     0.06       0.00    -0.07
    12   0.0140      0.00    -0.00       0.00    -0.13
    13   0.0141      0.00     0.01       0.00    -0.10
    14   0.0141      0.00    -0.04       0.00    -0.07
    15   0.0141      0.00    -0.03       0.00    -0.16
    16   0.0141      0.00     0.11       0.00    -0.08
    17   1.7278      0.00    -0.15       0.00    -0.31
    18   1.7552      0.00    -0.05       0.00     0.19
    19   1.7552      0.00    -0.12       0.00     0.01
    20   1.8312      0.00     0.22       0.00     0.32
    21   1.9432      0.00    -0.51       0.00     0.19
    22   1.9432      0.00    -0.06       0.00     0.23
    23   1.9623      0.00    -0.31       0.00    -0.33
    24   2.7325      0.00    -0.03       0.00     0.03
    25   2.7326      0.00     0.00       0.00    -0.01
    26   2.7350      0.00     0.18       0.00    -0.07
    27   2.7517      0.00    -0.09       0.00    -0.20
    28   2.7518      0.00     0.00       0.00     0.04
    29   2.7544      0.00     0.06       0.00     0.02
    30   2.8063      0.00     0.32       0.00     0.45
    31   2.8088      0.00     0.24       0.00     0.07
    32   2.8226      0.00    -0.09       0.00    -0.03
    33   2.8227      0.00     0.34       0.00     0.52
    34   2.8335      0.00     0.10       0.00     0.09
    35   2.8336      0.00     0.04       0.00    -0.38
    36   2.8337      0.00     0.05       0.00     0.11
    37   2.8388      0.00     0.03       0.00    -0.26
    38   2.8582      0.00    -0.02       0.00    -0.01
    39   2.8797      0.00    -0.41       0.00    -0.22
    40   3.0793      0.00     0.16       0.00     0.03
    41   3.1151      0.00    -0.12       0.00     0.01
    42   3.1151      0.00     0.30       0.00     0.11
    43   4.9257      0.00    -0.03       0.00    -0.11
    44   4.9258      0.00    -0.23       0.00    -0.19
    45   4.9258      0.00    -0.13       0.00     0.03
    46   5.0295      0.00     0.26       0.00     0.06
    47   5.0295      0.00     0.05       0.00    -0.07
    48   5.0297      0.00    -0.01       0.00     0.09
    49   5.0298      0.00    -0.01       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.

14WM517    quality flag:2

Type:       SCATEXTD  SCATEXTD  SCATNEAR

axisobj        48.091    48.091    48.091
ecceobj         0.067     0.067     0.067
incobj         19.464    19.464    19.464
qmin           39.325    40.281    37.393
qmax           56.590    55.630    58.751
amean          47.798    47.798    47.798
amin           47.346    47.371    47.294
amax           48.266    48.294    48.364
emean           0.090     0.088     0.111
emin            0.002     0.013     0.001
emax            0.174     0.154     0.218
imean          18.030    17.910    17.715
imin           16.549    16.717    15.720
imax           19.348    19.025    18.992
excite_mean     0.325     0.322     0.328
fracstop        1.000     1.000     1.000
cjmean          3.014     3.016     3.012

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       220.0     220.2     235.9
kozaiamp        180.0     180.0     180.0