Orbit Fit and Astrometric record for 01XW254

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: 01XW254   
# Created Fri Nov  1 01:08:09 2024
# Orbit generated from Bernstein formalism
# Fitting      4 observations of      4
# Arc:  29.04d
# First observation: 2001/12/10
#  Last observation: 2002/01/08
# WARNING Fitting with energy constraint
# WARNING and with gdot fixed = 0
# Chi-squared of fit:     0.57 DOF:      4 RMS:  0.07
# Min/Max residuals:    -0.11    0.11
# Exact a, adot, b, bdot, g, gdot:
  1.504366E-05  2.354066E-02  1.648659E-06  2.371592E-03  2.420841E-02  0.000000E+00
# Covariance matrix:
  3.1549E-11  4.7391E-08 -6.9709E-14 -1.0943E-10  7.5701E-09  0.0000E+00
  4.7391E-08  7.2888E-05 -1.0719E-10 -1.6827E-07  1.1641E-05  0.0000E+00
 -6.9709E-14 -1.0719E-10  7.2384E-13 -8.8655E-12 -1.7119E-11  0.0000E+00
 -1.0943E-10 -1.6827E-07 -8.8655E-12  6.2104E-10 -2.6873E-08  0.0000E+00
  7.5701E-09  1.1641E-05 -1.7119E-11 -2.6873E-08  1.8591E-06  0.0000E+00
  0.0000E+00  0.0000E+00  0.0000E+00  0.0000E+00  0.0000E+00  1.8669E-04
#      lat0       lon0       xBary       yBary       zBary        JD0
    0.922419  101.563009    0.382283    0.014430   -0.901135  2452254.065433
# Heliocentric elements and errors
Epoch:              2452250.5000  =  2001/12/07
Mean Anomaly:          343.58758 +/-    14.148
Argument of Peri:       26.31876 +/-    80.504
Long of Asc Node:       92.14487 +/-     3.252
Inclination:             5.81736 +/-     2.084
Eccentricity:         0.02914623 +/-    0.5645
Semi-Major Axis:     43.42714261 +/-   22.7818
Time of Perihelion: 2457016.0203 +/-  317675.5
Perihelion:          42.16140529 +/-   33.0177
Aphelion:            44.69287994 +/-   33.9217
Period (y)              286.1871 +/-    225.20
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X           -8.08393027 +/-    0.4661
Ecliptic Y           41.42941141 +/-    2.2791
Ecliptic Z            0.66505918 +/-    0.0375
Ecliptic XDOT        -0.00261602 +/-    0.0009
Ecliptic YDOT        -0.00053793 +/-    0.0015
Ecliptic ZDOT         0.00026839 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   42.21597283 +/-    2.2384
Geocenter to KBO     41.30795089 +/-    2.3266
# Hcoef:  7.75

The following table shows the complete astrometric record for 01XW254. 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 (01XW254) followed by the observatory code and reference code for the source of the astrometry.

2001 12  10.56469  06 50 38.05   +23 51 18.1         01XW254   568  Ce7056      
2001 12  10.61127  06 50 37.81   +23 51 18.5         01XW254   568  Ce7056      
2002 01  08.58150  06 48 05.91   +23 55 00.9   23.6R 01XW254   568  Ce7056      
2002 01  08.59976  06 48 05.81   +23 55 00.8   23.6R 01XW254   568  Ce7056      

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     0.07       0.00    -0.02
     2   0.0001     -3.31    -0.07       0.11     0.02
     3   0.0794  -2098.10     0.00      44.74     0.11
     4   0.0795  -2099.46    -0.00      44.52    -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.

01XW254    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