Orbit Fit and Astrometric record for 01DS108

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: 01DS108   
# Created Thu Apr 18 01:10:25 2024
# Orbit generated from Bernstein formalism
# Fitting      6 observations of      6
# Arc:   3.07d
# First observation: 2001/02/22
#  Last observation: 2001/02/25
# WARNING Fitting with energy constraint
# WARNING and with gdot fixed = 0
# Chi-squared of fit:    13.22 DOF:      8 RMS:  0.26
# Min/Max residuals:    -0.57    0.54
# Exact a, adot, b, bdot, g, gdot:
  1.332122E-05  2.094693E-02  1.381382E-06  1.061854E-03  2.233071E-02  0.000000E+00
# Covariance matrix:
  2.7666E-11  3.8255E-08  1.2772E-14 -7.9846E-12  6.0359E-09  0.0000E+00
  3.8255E-08  5.3879E-05  1.7967E-11 -1.1230E-08  8.4873E-06  0.0000E+00
  1.2772E-14  1.7967E-11  4.2430E-13 -5.1330E-11  2.8309E-12  0.0000E+00
 -7.9846E-12 -1.1230E-08 -5.1330E-11  1.4682E-08 -1.7694E-09  0.0000E+00
  6.0359E-09  8.4873E-06  2.8309E-12 -1.7694E-09  1.3373E-06  0.0000E+00
  0.0000E+00  0.0000E+00  0.0000E+00  0.0000E+00  0.0000E+00  1.4653E-04
#      lat0       lon0       xBary       yBary       zBary        JD0
   -0.681159  153.642897   -0.007861   -0.011924   -0.990779  2451962.805583
# Heliocentric elements and errors
Epoch:              2451960.5000  =  2001/02/20
Mean Anomaly:            8.31259 +/-   278.569
Argument of Peri:      338.36160 +/-   344.675
Long of Asc Node:      166.54235 +/-     4.595
Inclination:             2.98295 +/-     1.046
Eccentricity:         0.02370351 +/-    0.5583
Semi-Major Axis:     46.86937905 +/-   24.3787
Time of Perihelion: 2449254.2610 +/-  442289.4
Perihelion:          45.75841018 +/-   35.3726
Aphelion:            47.98034791 +/-   36.1604
Period (y)              320.8795 +/-    250.35
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X          -41.01067424 +/-    2.0778
Ecliptic Y           20.31737607 +/-    1.0297
Ecliptic Z           -0.53230904 +/-    0.0276
Ecliptic XDOT        -0.00114988 +/-    0.0014
Ecliptic YDOT        -0.00229727 +/-    0.0010
Ecliptic ZDOT         0.00013037 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   45.77067320 +/-    1.9170
Geocenter to KBO     44.78138785 +/-    2.3191
# Hcoef:  8.01

The following table shows the complete astrometric record for 01DS108. 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 (01DS108) followed by the observatory code and reference code for the source of the astrometry.

2001 02  22.30484  10 21 12.96   +09 32 12.1         01DS108   568  Ce9335      
2001 02  22.34332  10 21 12.76   +09 32 13.4         01DS108   568  Ce9335      
2001 02  22.39974  10 21 12.53   +09 32 14.9         01DS108   568  Ce9335      
2001 02  25.29330  10 21 00.12   +09 33 27.2         01DS108   568  Ce9335      
2001 02  25.33179  10 20 59.97   +09 33 28.7         01DS108   568  Ce9335      
2001 02  25.37029  10 20 59.81   +09 33 30.2   24.2R 01DS108   568  Ce9335      

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     0.31       0.00    -0.13
     2   0.0001     -3.23    -0.26       0.14    -0.00
     3   0.0003     -6.94    -0.06       0.31     0.15
     4   0.0082   -204.24     0.00       1.39    -0.57
     5   0.0083   -206.85     0.05       1.99     0.01
     6   0.0084   -209.60    -0.04       2.53     0.54

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.

01DS108    quality flag:0

Type:      ERR2LARGE ERR2LARGE ERR2LARGE

axisobj         0.000     0.000     0.000
ecceobj        -1.000    -1.000    -1.000
incobj         -1.000    -1.000    -1.000
qmin            0.000     0.000     0.000
qmax            0.000     0.000     0.000
amean           0.000     0.000     0.000
amin            0.000     0.000     0.000
amax            0.000     0.000     0.000
emean           0.000     0.000     0.000
emin            0.000     0.000     0.000
emax            0.000     0.000     0.000
imean           0.000     0.000     0.000
imin            0.000     0.000     0.000
imax            0.000     0.000     0.000
excite_mean     0.000     0.000     0.000
fracstop        0.000     0.000     0.000
cjmean          0.000     0.000     0.000

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         0.0       0.0       0.0
kozaiamp          0.0       0.0       0.0