Orbit Fit and Astrometric record for 14UD229

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: 14UD229   
# Created Sat Apr 20 01:16:36 2024
# Orbit generated by ELGB
# -->Covariance matrix from a Bernstein fit
# Fitting     49 observations of     49
# Arc:   9.30y
# First observation: 2013/08/09
#  Last observation: 2022/11/28
# Chi-squared of fit:    10.68 DOF:     92 RMS:  0.08
# Min/Max residuals:    -0.17    0.23
# Exact a, adot, b, bdot, g, gdot:
  1.714114E-05  3.147252E-02  2.036178E-06  3.221674E-03  2.911818E-02 -3.494227E-03
# Covariance matrix:
  1.7156E-13 -6.4972E-14  5.0718E-15 -7.4048E-15  6.6702E-14 -2.1140E-13
 -6.4972E-14  6.9486E-14 -6.7910E-15  7.8697E-15  5.3703E-15  2.3288E-13
  5.0718E-15 -6.7910E-15  4.6009E-14 -1.0568E-14 -1.3156E-15 -2.4726E-14
 -7.4048E-15  7.8697E-15 -1.0568E-14  6.7568E-15  1.3423E-16  2.8839E-14
  6.6702E-14  5.3703E-15 -1.3156E-15  1.3423E-16  6.5407E-14  1.1010E-14
 -2.1140E-13  2.3288E-13 -2.4726E-14  2.8839E-14  1.1010E-14  8.5248E-13
#      lat0       lon0       xBary       yBary       zBary        JD0
    3.415245   29.381133    0.968991    0.018150   -0.303550  2456514.027758
# Heliocentric elements and errors
Epoch:              2456514.5000  =  2013/08/10
Mean Anomaly:          298.18269 +/-     0.009
Argument of Peri:      107.64478 +/-     0.013
Long of Asc Node:      358.30219 +/-     0.001
Inclination:             6.85185 +/-     0.000
Eccentricity:         0.14812884 +/-    0.0000
Semi-Major Axis:     36.53092491 +/-    0.0014
Time of Perihelion: 2470362.8179 +/-       4.3
Perihelion:          31.11964140 +/-    0.0015
Aphelion:            41.94220843 +/-    0.0019
Period (y)              220.8001 +/-      0.01
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X           30.61232253 +/-    0.0003
Ecliptic Y           16.12708676 +/-    0.0001
Ecliptic Z            2.04597672 +/-    0.0000
Ecliptic XDOT        -0.00175957 +/-    0.0000
Ecliptic YDOT         0.00240795 +/-    0.0000
Ecliptic ZDOT         0.00028295 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   34.66105811 +/-    0.0002
Geocenter to KBO     34.34289559 +/-    0.0003
# Hcoef:  8.28

The following table shows the complete astrometric record for 14UD229. 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 (14UD229) followed by the observatory code and reference code for the source of the astrometry.

2013 08  09.52698  01 44 17.778  +14 26 45.25  23.7r 14UD229   568  C~2SDi      
2013 08  09.56967  01 44 17.735  +14 26 45.49  23.9r 14UD229   568  C~2SDi      
2013 09  02.44494  01 43 23.101  +14 24 43.46  23.7r 14UD229   568  C~2SDi      
2013 09  02.48778  01 43 22.947  +14 24 42.85  23.8r 14UD229   568  C~2SDi      
2013 10  08.52484  01 40 34.845  +14 12 15.32  23.5r 14UD229   568  C~2SDi      
2013 11  01.51045  01 38 19.950  +14 00 23.12  23.7r 14UD229   568  C~2SDi      
2013 11  29.25439  01 36 04.909  +13 47 08.18  23.7r 14UD229   568  C~2SDi      
2013 12  04.40215  01 35 45.514  +13 45 03.63  23.6r 14UD229   568  C~2SDi      
2013 12  29.26747  01 34 47.863  +13 37 59.89  23.7r 14UD229   568  C~2SDi      
2013 12  29.27201  01 34 47.870  +13 37 59.84  23.7r 14UD229   568  C~2SDi      
2013 12  29.27671  01 34 47.850  +13 37 59.70  23.9r 14UD229   568  C~2SDi      
2013 12  30.37416  01 34 46.820  +13 37 48.95  24.0r 14UD229   568  C~2SDi      
2014 01  02.24937  01 34 44.813  +13 37 24.19  24.1r 14UD229   568  C~2SDi      
2014 01  02.29641  01 34 44.785  +13 37 23.75  23.9r 14UD229   568  C~2SDi      
2014 01  02.30286  01 34 44.775  +13 37 23.81  24.2r 14UD229   568  C~2SDi      
2014 01  03.21937  01 34 44.338  +13 37 17.04  23.8r 14UD229   568  C~2SDi      
2014 01  03.26180  01 34 44.320  +13 37 16.81  23.5r 14UD229   568  C~2SDi      
2014 01  03.33071  01 34 44.296  +13 37 16.37  23.6r 14UD229   568  C~2SDi      
2014 08  24.48198  01 50 37.412  +15 15 28.61  23.6r 14UD229   568  C~2SDi      
2014 08  24.55192  01 50 37.232  +15 15 28.30  23.9r 14UD229   568  C~2SDj      
2014 08  27.56009  01 50 29.497  +15 15 09.75  25.3u 14UD229   568  C~2SDj      
2014 08  27.56435  01 50 29.488  +15 15 09.75  25.4u 14UD229   568  C~2SDj      
2014 08  27.57287  01 50 29.457  +15 15 09.79  25.2u 14UD229   568  C~2SDj      
2014 09  18.48241  01 49 08.717  +15 10 20.85  23.6r 14UD229   568  C~2SDj      
2014 09  18.52513  01 49 08.522  +15 10 19.95  23.9r 14UD229   568  C~2SDj      
2014 09  23.52346  01 48 44.980  +15 08 39.80  23.9r 14UD229   568  C~2SDj      
2014 10  22.30668  01 46 08.385  +14 56 07.98  23.4r 14UD229   568  C~2SDj      
2014 10  22.35220  01 46 08.126  +14 56 06.58  23.6r 14UD229   568  C~2SDj      
2014 10  22.40142  01 46 07.832  +14 56 05.19  23.7r 14UD229   568  C~2SDj      
2014 10  23.49660  01 46 01.552  +14 55 32.40  23.6r 14UD229   568  C~2SDj      
2014 11  21.28635  01 43 26.527  +14 41 13.02  23.6r 14UD229   568  C~2SDj      
2014 11  21.44138  01 43 25.781  +14 41 08.77  23.6r 14UD229   568  C~2SDj      
2015 01  28.28328  01 41 42.685  +14 26 48.19  23.7r 14UD229   568  C~2SDj      
2015 02  19.26046  01 42 58.091  +14 32 08.34  23.7r 14UD229   568  C~2SDj      
2015 02  19.26866  01 42 58.140  +14 32 08.49  24.0r 14UD229   568  C~2SDj      
2015 10  10.36050  01 54 14.275  +15 51 50.40  23.5r 14UD229   568  C~2SDj      
2015 10  10.42692  01 54 13.894  +15 51 48.65  23.5r 14UD229   568  C~2SDj      
2015 10  12.48210  01 54 02.343  +15 50 54.01        14UD229   568  C~2SDj      
2015 10  12.54868  01 54 01.963  +15 50 52.42        14UD229   568  C~2SDj      
2015 10  14.31603  01 53 51.976  +15 50 04.58  23.7r 14UD229   568  C~2SDj      
2015 10  14.38671  01 53 51.558  +15 50 02.56        14UD229   568  C~2SDj      
2015 10  14.39084  01 53 51.546  +15 50 02.47        14UD229   568  C~2SDj      
2015 12  06.27161  01 49 14.830  +15 24 50.64  23.5r 14UD229   568  C~2SDj      
2015 12  07.40375  01 49 10.570  +15 24 23.44  23.7w 14UD229   568  C~2SDj      
2015 12  31.32052  01 48 10.464  +15 17 07.81  24.1w 14UD229   568  C~2SDj      
2016 01  07.29206  01 48 04.690  +15 15 59.31  23.9w 14UD229   568  C~2SDj      
2022 11  28.268010 02 41 26.422  +21 04 51.81  23.6G 14UD229   G37  C~677W      
2022 11  28.317500 02 41 26.128  +21 04 50.31        14UD229   G37  C~677W      
2022 11  28.366910 02 41 25.860  +21 04 49.17        14UD229   G37  C~677W      

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     0.01       0.00    -0.06
     2   0.0001      0.00     0.12       0.00     0.08
     3   0.0655      0.00     0.05       0.00    -0.02
     4   0.0656      0.00    -0.01       0.00    -0.12
     5   0.1643      0.00    -0.13       0.00    -0.01
     6   0.2299      0.00    -0.09       0.00    -0.12
     7   0.3059      0.00     0.06       0.00     0.03
     8   0.3200      0.00     0.23       0.00    -0.05
     9   0.3881      0.00    -0.06       0.00     0.05
    10   0.3881      0.00     0.11       0.00     0.05
    11   0.3881      0.00    -0.11       0.00    -0.04
    12   0.3911      0.00    -0.10       0.00     0.01
    13   0.3990      0.00     0.03       0.00    -0.07
    14   0.3991      0.00     0.06       0.00    -0.14
    15   0.3991      0.00    -0.03       0.00    -0.03
    16   0.4016      0.00    -0.10       0.00    -0.06
    17   0.4017      0.00    -0.04       0.00     0.02
    18   0.4019      0.00     0.13       0.00     0.07
    19   1.0403      0.00    -0.06       0.00    -0.08
    20   1.0405      0.00    -0.12       0.00    -0.04
    21   1.0487      0.00     0.10       0.00     0.04
    22   1.0487      0.00     0.14       0.00     0.07
    23   1.0487      0.00     0.04       0.00     0.17
    24   1.1087      0.00     0.01       0.00     0.02
    25   1.1088      0.00     0.06       0.00    -0.08
    26   1.1225      0.00     0.02       0.00    -0.06
    27   1.2013      0.00    -0.11       0.00     0.14
    28   1.2014      0.00    -0.02       0.00     0.08
    29   1.2016      0.00    -0.12       0.00     0.14
    30   1.2046      0.00     0.05       0.00    -0.05
    31   1.2834      0.00    -0.02       0.00    -0.04
    32   1.2838      0.00     0.05       0.00     0.09
    33   1.4696      0.00     0.03       0.00     0.11
    34   1.5297      0.00    -0.17       0.00     0.07
    35   1.5298      0.00     0.01       0.00     0.04
    36   2.1679      0.00     0.03       0.00    -0.01
    37   2.1681      0.00    -0.02       0.00    -0.03
    38   2.1737      0.00    -0.09       0.00    -0.17
    39   2.1739      0.00    -0.06       0.00     0.03
    40   2.1788      0.00     0.03       0.00     0.05
    41   2.1789      0.00    -0.12       0.00    -0.05
    42   2.1790      0.00     0.06       0.00    -0.03
    43   2.3237      0.00     0.03       0.00     0.05
    44   2.3268      0.00     0.07       0.00    -0.02
    45   2.3923      0.00     0.11       0.00    -0.08
    46   2.4114      0.00     0.00       0.00     0.11
    47   9.3025      0.00     0.03       0.00     0.00
    48   9.3026      0.00    -0.12       0.00    -0.13
    49   9.3028      0.00     0.09       0.00     0.09

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.

14UD229    quality flag:3

Type:           4:3E      4:3E      4:3E

axisobj        36.675    36.675    36.675
ecceobj         0.146     0.146     0.146
incobj          6.832     6.832     6.832
qmin           30.322    30.323    30.320
qmax           43.017    43.020    43.012
amean          36.477    36.477    36.477
amin           36.132    36.132    36.136
amax           36.854    36.852    36.838
emean           0.145     0.145     0.145
emin            0.123     0.124     0.123
emax            0.169     0.169     0.169
imean           5.982     5.982     5.987
imin            4.057     4.058     4.068
imax            8.327     8.327     8.327
excite_mean     0.180     0.180     0.180
fracstop        1.000     1.000     1.000
cjmean          2.990     2.990     2.990

libcent 0       180.1     180.4     179.9
libamp  0        52.6      52.9      53.4
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       180.2     180.2     180.2
kozaiamp        180.0     180.0     180.0