Orbit Fit and Astrometric record for 22GY3

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: 22GY3     
# Created Fri Nov 22 02:11:12 2024
# Orbit generated by ELGB
# -->Covariance matrix from a Bernstein fit
# Fitting     22 observations of     22
# Arc:  21.12y
# First observation: 2001/02/20
#  Last observation: 2022/04/05
# Chi-squared of fit:    35.58 DOF:     38 RMS:  0.22
# Min/Max residuals:    -0.51    0.75
# Exact a, adot, b, bdot, g, gdot:
  1.658463E-05  2.770391E-02 -8.195352E-08 -5.748391E-04  2.642448E-02 -1.454022E-03
# Covariance matrix:
  7.3413E-13 -3.0267E-12 -8.1157E-16  6.4881E-14  2.4987E-13 -5.9390E-12
 -3.0267E-12  8.8286E-09  1.0531E-12 -1.9423E-10  1.7620E-09  1.7482E-08
 -8.1157E-16  1.0531E-12  6.6231E-13 -2.5978E-13  2.0494E-13  2.0901E-12
  6.4881E-14 -1.9423E-10 -2.5978E-13  1.3066E-11 -3.8764E-11 -3.8502E-10
  2.4987E-13  1.7620E-09  2.0494E-13 -3.8764E-11  3.6117E-10  3.4879E-09
 -5.9390E-12  1.7482E-08  2.0901E-12 -3.8502E-10  3.4879E-09  3.4655E-08
#      lat0       lon0       xBary       yBary       zBary        JD0
   -1.326151  164.583663    0.214832   -0.022530   -0.966381  2451960.773018
# Heliocentric elements and errors
Epoch:              2451960.5000  =  2001/02/20
Mean Anomaly:          329.66937 +/-     0.019
Argument of Peri:      264.20711 +/-     0.001
Long of Asc Node:      296.82060 +/-     0.001
Inclination:             1.75549 +/-     0.000
Eccentricity:         0.09941243 +/-    0.0000
Semi-Major Axis:     42.31720630 +/-    0.0000
Time of Perihelion: 2460431.8549 +/-       5.4
Perihelion:          38.11035013 +/-    0.0014
Aphelion:            46.52406247 +/-    0.0014
Period (y)              275.2857 +/-      0.00
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X          -37.34298977 +/-    0.0000
Ecliptic Y           10.52589843 +/-    0.0000
Ecliptic Z           -0.87583162 +/-    0.0000
Ecliptic XDOT        -0.00062483 +/-    0.0000
Ecliptic YDOT        -0.00280425 +/-    0.0000
Ecliptic ZDOT        -0.00005587 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   38.80802980 +/-    0.0000
Geocenter to KBO     37.84375331 +/-    0.0000
# Hcoef:  7.38

The following table shows the complete astrometric record for 22GY3. 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 (22GY3) followed by the observatory code and reference code for the source of the astrometry.

2001 02  20.272275 11 01 09.36   +04 50 45.9   22.7r 22GY3     645  C~5fwS      
2001 02  20.273104 11 01 09.39   +04 50 45.9   23.0i 22GY3     645  C~5fwS      
2001 04  16.117057 10 57 05.22   +05 16 13.7         22GY3     645  C~5fwS      
2001 04  16.117886 10 57 05.20   +05 16 13.6         22GY3     645  C~5fwS      
2002 03  22.330104 11 04 36.23   +04 26 57.3   22.7R 22GY3     568  C~5fwS      
2002 03  22.388663 11 04 35.95   +04 26 59.1   23.0R 22GY3     568  C~5fwS      
2002 03  22.417914 11 04 35.80   +04 26 59.9   22.8R 22GY3     568  C~5fwS      
2015 04  14.074836 12 19 46.07   -03 58 52.4   23.4V 22GY3     W84  C~5fwS      
2019 05  05.005263 12 42 28.01   -06 27 57.5   23.4V 22GY3     W84  C~5fwS      
2019 05  05.223632 12 42 27.13   -06 27 51.6   23.5V 22GY3     W84  C~5fwS      
2021 04  16.10088  12 56 02.52   -07 54 59.6         22GY3     W93  C~5Y3z      
2021 04  16.13587  12 56 02.31   -07 54 58.8         22GY3     W93  C~5Y3z      
2021 04  16.17102  12 56 02.16   -07 54 57.5         22GY3     W93  C~5Y3z      
2021 04  18.10088  12 55 52.87   -07 53 59.0   23.1R 22GY3     W93  C~5Y3z      
2021 04  18.13546  12 55 52.73   -07 53 58.2   22.8R 22GY3     W93  C~5Y3z      
2021 04  18.17011  12 55 52.59   -07 53 57.2   23.1R 22GY3     W93  C~5Y3z      
2022 04  03.11592  13 03 16.00   -08 40 15.9         22GY3     W93  C~5Y3z      
2022 04  03.15089  13 03 15.81   -08 40 14.8         22GY3     W93  C~5Y3z      
2022 04  03.18623  13 03 15.67   -08 40 13.8         22GY3     W93  C~5Y3z      
2022 04  05.12689  13 03 06.08   -08 39 15.2   22.5R 22GY3     W93  C~5Y3z      
2022 04  05.15454  13 03 05.92   -08 39 14.2   22.6R 22GY3     W93  C~5Y3z      
2022 04  05.18230  13 03 05.80   -08 39 13.8   22.7R 22GY3     W93  C~5Y3z      

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    -0.02       0.00    -0.05
     2   0.0000      0.00     0.49       0.00    -0.07
     3   0.1502      0.00     0.00       0.00     0.16
     4   0.1502      0.00    -0.26       0.00     0.04
     5   1.0816      0.00     0.02       0.00    -0.07
     6   1.0818      0.00    -0.03       0.00     0.02
     7   1.0818      0.00    -0.20       0.00    -0.04
     8  14.1432      0.00    -0.24       0.00     0.07
     9  18.2005      0.00    -0.09       0.00    -0.05
    10  18.2011      0.00    -0.02       0.00     0.04
    11  20.1501      0.00     0.41       0.00     0.16
    12  20.1502      0.00    -0.16       0.00    -0.10
    13  20.1503      0.00     0.18       0.00     0.13
    14  20.1556      0.00    -0.10       0.00     0.04
    15  20.1557      0.00     0.32       0.00    -0.20
    16  20.1558      0.00     0.75       0.00    -0.25
    17  21.1139      0.00    -0.29       0.00    -0.13
    18  21.1140      0.00    -0.51       0.00    -0.07
    19  21.1141      0.00     0.05       0.00    -0.13
    20  21.1194      0.00     0.03       0.00     0.19
    21  21.1195      0.00    -0.29       0.00     0.36
    22  21.1195      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.

22GY3    quality flag:3

Type:          5:3EE     5:3EE     5:3EE

axisobj        42.155    42.155    42.155
ecceobj         0.097     0.097     0.097
incobj          1.759     1.759     1.759
qmin           37.183    37.182    37.184
qmax           48.083    48.079    48.086
amean          42.329    42.329    42.329
amin           41.913    41.912    41.914
amax           42.775    42.774    42.775
emean           0.099     0.099     0.099
emin            0.080     0.080     0.080
emax            0.124     0.124     0.124
imean           3.984     3.984     3.984
imin            2.681     2.682     2.681
imax            5.216     5.216     5.216
excite_mean     0.122     0.122     0.122
fracstop        1.000     1.000     1.000
cjmean          3.064     3.064     3.064

libcent 0       178.4     178.4     178.4
libamp  0       100.4     100.4     100.4
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       186.0     185.9     186.2
kozaiamp        179.9     180.0     180.0