Orbit Fit and Astrometric record for 11UR412

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: 11UR412   
# Created Sat Dec  4 02:11:23 2021
# Orbit generated by ELGB
# -->Covariance matrix from a Bernstein fit
# Fitting     22 observations of     22
# Arc:   8.16y
# First observation: 2011/08/30
#  Last observation: 2019/10/26
# Chi-squared of fit:     8.77 DOF:     38 RMS:  0.11
# Min/Max residuals:    -0.22    0.30
# Exact a, adot, b, bdot, g, gdot:
  1.712591E-05  3.148927E-02  5.530660E-06  9.641527E-03  2.810132E-02 -4.351429E-03
# Covariance matrix:
  2.4402E-13 -1.1840E-13  1.0784E-14 -3.6523E-14  1.5349E-13 -4.0638E-13
 -1.1840E-13  4.0906E-13 -4.7727E-14  1.3520E-13  5.8223E-14  1.5540E-12
  1.0784E-14 -4.7727E-14  8.7477E-14 -2.9923E-14 -9.2131E-15 -1.8649E-13
 -3.6523E-14  1.3520E-13 -2.9923E-14  5.7270E-14  1.8616E-14  5.2820E-13
  1.5349E-13  5.8223E-14 -9.2131E-15  1.8616E-14  2.2004E-13  2.3074E-13
 -4.0638E-13  1.5540E-12 -1.8649E-13  5.2820E-13  2.3074E-13  6.0711E-12
#      lat0       lon0       xBary       yBary       zBary        JD0
    5.064481   32.295108    0.832509    0.049933   -0.563792  2455804.003996
# Heliocentric elements and errors
Epoch:              2455804.5000  =  2011/08/31
Mean Anomaly:          341.15915 +/-     0.009
Argument of Peri:       53.78896 +/-     0.018
Long of Asc Node:       15.24923 +/-     0.000
Inclination:            17.84089 +/-     0.000
Eccentricity:         0.32022417 +/-    0.0001
Semi-Major Axis:     50.55629970 +/-    0.0053
Time of Perihelion: 2462676.1241 +/-      20.0
Perihelion:          34.36695074 +/-    0.0047
Aphelion:            66.74564865 +/-    0.0077
Period (y)              359.4770 +/-      0.06
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X           30.88986095 +/-    0.0005
Ecliptic Y           18.53829886 +/-    0.0003
Ecliptic Z            3.14159554 +/-    0.0001
Ecliptic XDOT        -0.00206936 +/-    0.0000
Ecliptic YDOT         0.00232881 +/-    0.0000
Ecliptic ZDOT         0.00089832 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   36.16253584 +/-    0.0005
Geocenter to KBO     35.58562932 +/-    0.0006
# Hcoef:  8.73

The following table shows the complete astrometric record for 11UR412. 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 (11UR412) followed by the observatory code and reference code for the source of the astrometry.

2011 08  30.50323  01 53 09.341  +17 01 08.04  24.2r 11UR412   568  C~1CKy      
2011 08  30.54972  01 53 09.190  +17 01 08.09  24.6r 11UR412   568  C~1CKy      
2011 08  30.59613  01 53 09.063  +17 01 07.93  24.2r 11UR412   568  C~1CKy      
2011 10  25.34656  01 48 48.940  +16 46 57.35  24.1r 11UR412   568  C~1CKy      
2011 10  25.39635  01 48 48.666  +16 46 55.96  24.0r 11UR412   568  C~1CKy      
2011 10  25.40523  01 48 48.626  +16 46 55.73  24.0r 11UR412   568  C~1CKy      
2011 10  26.29551  01 48 43.666  +16 46 33.78  24.3r 11UR412   568  C~1CKy      
2011 10  26.30517  01 48 43.615  +16 46 33.48  23.9r 11UR412   568  C~1CKy      
2011 10  26.34841  01 48 43.365  +16 46 32.51  24.4r 11UR412   568  C~1CKy      
2011 10  26.39151  01 48 43.121  +16 46 31.28  24.3r 11UR412   568  C~1CKy      
2011 10  31.39702  01 48 15.390  +16 44 25.77  23.9r 11UR412   568  C~1CKy      
2011 11  24.25792  01 46 13.820  +16 34 23.00  24.6r 11UR412   568  C~1CKy      
2011 11  26.47841  01 46 03.966  +16 33 30.10  24.4r 11UR412   568  C~1CKy      
2012 01  26.30218  01 44 33.141  +16 22 32.81  23.9r 11UR412   568  C~1CKy      
2012 01  27.23615  01 44 34.862  +16 22 38.87  24.5r 11UR412   568  C~1CKy      
2012 08  17.57715  01 59 55.442  +18 09 30.67  24.8r 11UR412   568  C~1CKy      
2012 08  24.53489  01 59 42.372  +18 10 06.59        11UR412   568  C~1CKy      
2012 10  17.38245  01 55 51.230  +18 00 13.10  24.2r 11UR412   568  C~1CKy      
2012 10  20.47747  01 55 33.856  +17 59 02.60  24.1r 11UR412   568  C~1CKy      
2013 02  06.26716  01 51 06.930  +17 32 53.62        11UR412   568  C~1CKy      
2019 10  26.410840 02 43 56.780  +25 59 52.53  23.7G 11UR412   G37  C~3chz      
2019 10  26.496010 02 43 56.243  +25 59 51.23        11UR412   G37  C~3chz      

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     0.13       0.00     0.02
     2   0.0001      0.00    -0.08       0.00     0.16
     3   0.0003      0.00     0.08       0.00     0.09
     4   0.1529      0.00    -0.13       0.00     0.01
     5   0.1530      0.00    -0.00       0.00    -0.16
     6   0.1531      0.00     0.15       0.00    -0.17
     7   0.1555      0.00    -0.02       0.00    -0.09
     8   0.1555      0.00     0.03       0.00    -0.15
     9   0.1556      0.00    -0.05       0.00    -0.06
    10   0.1558      0.00    -0.05       0.00    -0.22
    11   0.1695      0.00    -0.06       0.00     0.02
    12   0.2348      0.00     0.02       0.00     0.01
    13   0.2409      0.00     0.02       0.00    -0.07
    14   0.4074      0.00     0.11       0.00     0.03
    15   0.4099      0.00     0.05       0.00     0.13
    16   0.9667      0.00    -0.06       0.00     0.30
    17   0.9857      0.00    -0.07       0.00     0.18
    18   1.1331      0.00    -0.22       0.00    -0.04
    19   1.1416      0.00     0.08       0.00    -0.08
    20   1.4395      0.00    -0.10       0.00     0.08
    21   8.1558      0.00     0.13       0.00    -0.09
    22   8.1560      0.00    -0.08       0.00     0.05

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.

11UR412    quality flag:3

Type:       SCATNEAR  SCATNEAR  SCATNEAR

axisobj        50.683    50.682    50.683
ecceobj         0.321     0.321     0.321
incobj         17.823    17.823    17.823
qmin           33.485    33.179    33.335
qmax           67.627    67.758    67.385
amean          49.918    50.063    49.810
amin           49.189    49.450    49.058
amax           50.862    50.770    50.734
emean           0.308     0.312     0.308
emin            0.285     0.289     0.284
emax            0.331     0.337     0.330
imean          17.948    17.845    17.906
imin           16.918    16.834    16.884
imax           18.812    18.895    18.817
excite_mean     0.436     0.438     0.435
fracstop        1.000     1.000     1.000
cjmean          2.933     2.933     2.933

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       172.1     170.8     174.1
kozaiamp        180.0     180.0     180.0