Orbit Fit and Astrometric record for 13RG157

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: 13RG157   
# Created Sun Dec 22 02:09:35 2024
# Orbit generated by ELGB
# -->Covariance matrix from a Bernstein fit
# Fitting     20 observations of     20
# Arc:   6.22y
# First observation: 2013/09/10
#  Last observation: 2019/11/28
# Chi-squared of fit:    10.21 DOF:     34 RMS:  0.13
# Min/Max residuals:    -0.33    0.29
# Exact a, adot, b, bdot, g, gdot:
  1.344819E-05  2.032471E-02 -4.698218E-06 -4.898028E-03  2.309568E-02  3.005456E-03
# Covariance matrix:
  3.5741E-13 -1.7120E-13 -3.3762E-14  3.9403E-14  6.5777E-14 -1.2769E-12
 -1.7120E-13  2.0189E-13  4.5837E-14 -5.3359E-14  8.6366E-14  1.7127E-12
 -3.3762E-14  4.5837E-14  2.2391E-13 -5.9340E-14  1.5118E-14  4.2719E-13
  3.9403E-14 -5.3359E-14 -5.9340E-14  3.0841E-14 -1.7396E-14 -4.9750E-13
  6.5777E-14  8.6366E-14  1.5118E-14 -1.7396E-14  2.9122E-13  5.3374E-13
 -1.2769E-12  1.7127E-12  4.2719E-13 -4.9750E-13  5.3374E-13  1.5995E-11
#      lat0       lon0       xBary       yBary       zBary        JD0
   -4.906270   20.807568    0.553742   -0.071912   -0.838926  2456545.850228
# Heliocentric elements and errors
Epoch:              2456546.5000  =  2013/09/11
Mean Anomaly:          109.65947 +/-     0.063
Argument of Peri:       75.67215 +/-     0.053
Long of Asc Node:      180.96741 +/-     0.001
Inclination:            14.41362 +/-     0.000
Eccentricity:         0.14262471 +/-    0.0001
Semi-Major Axis:     41.46182638 +/-    0.0041
Time of Perihelion: 2426842.5148 +/-      17.6
Perihelion:          35.54834541 +/-    0.0065
Aphelion:            47.37530734 +/-    0.0073
Period (y)              266.9813 +/-      0.04
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X           41.30915385 +/-    0.0009
Ecliptic Y           15.10894665 +/-    0.0004
Ecliptic Z           -3.70334165 +/-    0.0001
Ecliptic XDOT        -0.00057666 +/-    0.0000
Ecliptic YDOT         0.00235952 +/-    0.0000
Ecliptic ZDOT        -0.00060884 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   44.14107133 +/-    0.0009
Geocenter to KBO     43.29807421 +/-    0.0010
# Hcoef:  7.48

The following table shows the complete astrometric record for 13RG157. 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 (13RG157) followed by the observatory code and reference code for the source of the astrometry.

2013 09  10.34945  01 24 15.827  +03 34 21.99  24.5g 13RG157   W84  C~52RO      
2013 09  10.36825  01 24 15.763  +03 34 21.25  23.8r 13RG157   W84  C~52RO      
2013 09  10.36963  01 24 15.751  +03 34 21.13  23.4i 13RG157   W84  C~52RO      
2013 11  22.15611  01 19 26.438  +03 02 14.95  23.7i 13RG157   W84  C~52RO      
2014 11  14.13577  01 24 39.338  +03 15 21.32  23.4i 13RG157   W84  C~52RO      
2014 11  18.15976  01 24 24.861  +03 14 00.15  23.1z 13RG157   W84  C~52RO      
2015 11  06.18503  01 29 54.222  +03 28 41.90  23.2r 13RG157   W84  C~52RO      
2015 11  06.18639  01 29 54.221  +03 28 42.35  23.5i 13RG157   W84  C~52RO      
2015 11  18.16315  01 29 08.410  +03 24 22.34  23.8r 13RG157   W84  C~52RO      
2016 08  16.38008  01 39 22.696  +04 14 19.12  23.5z 13RG157   W84  C~52RO      
2016 10  21.23668  01 35 40.228  +03 45 21.01  23.8i 13RG157   W84  C~52RO      
2016 10  28.24390  01 35 10.149  +03 42 14.00  23.6r 13RG157   W84  C~52RO      
2016 11  05.15343  01 34 37.087  +03 38 56.31  23.8r 13RG157   W84  C~52RO      
2017 08  22.38370  01 43 50.281  +04 22 05.73  23.2i 13RG157   W84  C~52RO      
2017 08  22.38506  01 43 50.284  +04 22 05.58  24.2r 13RG157   W84  C~52RO      
2019 11  28.26426  01 47 09.65   +04 01 07.1   25.0g 13RG157   T09  C~7gpV      
2019 11  28.32974  01 47 09.43   +04 01 06.3   25.1g 13RG157   T09  C~7gpV      
2019 11  28.34265  01 47 09.39   +04 01 06.1   25.3g 13RG157   T09  C~7gpV      
2019 11  28.40299  01 47 09.18   +04 01 04.9   24.8g 13RG157   T09  C~7gpV      
2019 11  28.41562  01 47 09.14   +04 01 04.9   25.0g 13RG157   T09  C~7gpV      

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     0.29
     2   0.0001      0.00     0.00       0.00     0.07
     3   0.0001      0.00    -0.11       0.00    -0.01
     4   0.1993      0.00     0.21       0.00    -0.09
     5   1.1767      0.00    -0.06       0.00     0.03
     6   1.1877      0.00    -0.11       0.00    -0.23
     7   2.1542      0.00    -0.02       0.00    -0.33
     8   2.1542      0.00     0.05       0.00     0.16
     9   2.1870      0.00    -0.03       0.00     0.02
    10   2.9323      0.00    -0.10       0.00    -0.02
    11   3.1126      0.00    -0.06       0.00    -0.20
    12   3.1318      0.00     0.24       0.00     0.26
    13   3.1535      0.00     0.04       0.00    -0.04
    14   3.9481      0.00    -0.00       0.00     0.08
    15   3.9481      0.00     0.08       0.00    -0.04
    16   6.2147      0.00    -0.03       0.00    -0.07
    17   6.2149      0.00    -0.01       0.00     0.13
    18   6.2149      0.00     0.05       0.00     0.13
    19   6.2151      0.00    -0.05       0.00    -0.15
    20   6.2151      0.00    -0.01       0.00     0.04

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.

13RG157    quality flag:3

Type:       SCATEXTD  SCATEXTD  SCATEXTD

axisobj        41.678    41.678    41.677
ecceobj         0.142     0.142     0.142
incobj         14.368    14.368    14.368
qmin           34.959    34.961    34.957
qmax           48.194    48.197    48.191
amean          41.462    41.455    41.438
amin           41.104    41.098    41.095
amax           41.872    41.847    41.851
emean           0.132     0.132     0.131
emin            0.113     0.113     0.111
emax            0.154     0.154     0.154
imean          15.076    15.073    15.090
imin           13.892    13.892    13.891
imax           16.266    16.257    16.268
excite_mean     0.292     0.292     0.292
fracstop        1.000     1.000     1.000
cjmean          2.972     2.972     2.972

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       179.7     179.5     179.5
kozaiamp        179.9     179.9     180.0