Orbit Fit and Astrometric record for 13TY187

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: 13TY187   
# Created Sun Nov 24 02:09:40 2024
# Orbit generated by ELGB
# -->Covariance matrix from a Bernstein fit
# Fitting     50 observations of     50
# Arc:   6.95y
# First observation: 2013/10/03
#  Last observation: 2020/09/14
# Chi-squared of fit:    18.85 DOF:     94 RMS:  0.11
# Min/Max residuals:    -0.26    0.33
# Exact a, adot, b, bdot, g, gdot:
  1.638912E-05  2.339624E-02  8.633958E-07  8.873135E-04  2.406510E-02 -1.382228E-03
# Covariance matrix:
  2.3791E-13 -1.3079E-13  3.2688E-15 -3.7322E-15  1.5562E-14 -5.9700E-13
 -1.3079E-13  9.2333E-14 -2.9770E-15  3.0621E-15 -2.9468E-15  4.8849E-13
  3.2688E-15 -2.9770E-15  1.1268E-13 -3.0254E-14 -4.5601E-15 -2.0560E-14
 -3.7322E-15  3.0621E-15 -3.0254E-14  1.1023E-14  4.9355E-16  1.8719E-14
  1.5562E-14 -2.9468E-15 -4.5601E-15  4.9355E-16  1.3531E-13  6.0554E-14
 -5.9700E-13  4.8849E-13 -2.0560E-14  1.8719E-14  6.0554E-14  2.9757E-12
#      lat0       lon0       xBary       yBary       zBary        JD0
  -11.184665   14.479122    0.082568   -0.193344   -0.978353  2456568.633788
# Heliocentric elements and errors
Epoch:              2456568.5000  =  2013/10/03
Mean Anomaly:          294.32795 +/-     0.043
Argument of Peri:      353.89827 +/-     0.053
Long of Asc Node:       93.19553 +/-     0.001
Inclination:            11.12988 +/-     0.000
Eccentricity:         0.06727787 +/-    0.0001
Semi-Major Axis:     43.57024616 +/-    0.0029
Time of Perihelion: 2475731.4130 +/-      15.2
Perihelion:          40.63893299 +/-    0.0040
Aphelion:            46.50155933 +/-    0.0043
Period (y)              287.6029 +/-      0.03
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X           40.45563911 +/-    0.0006
Ecliptic Y           10.36479393 +/-    0.0002
Ecliptic Z           -8.06028166 +/-    0.0001
Ecliptic XDOT        -0.00080209 +/-    0.0000
Ecliptic YDOT         0.00254218 +/-    0.0000
Ecliptic ZDOT         0.00012967 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   42.53303713 +/-    0.0006
Geocenter to KBO     41.55403072 +/-    0.0006
# Hcoef:  6.49

The following table shows the complete astrometric record for 13TY187. 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 (13TY187) followed by the observatory code and reference code for the source of the astrometry.

2013 10  03.13301  01 10 35.654  -04 36 41.50  23.9g 13TY187   W84  C~4yRE      
2013 10  04.18259  01 10 31.000  -04 37 11.12  23.5g 13TY187   W84  C~4yRE      
2013 10  04.18259  01 10 31.00   -04 37 11.1   23.5g 13TY187   W84  C~3clQ      
2014 10  01.32552  01 15 37.746  -04 01 45.47  22.4r 13TY187   W84  C~4yRE      
2014 10  01.32552  01 15 37.75   -04 01 45.5   22.5r 13TY187   W84  C~3clQ      
2014 10  01.32688  01 15 37.754  -04 01 45.30  23.6g 13TY187   W84  C~4yRE      
2014 10  14.24606  01 14 40.112  -04 07 38.50  22.2z 13TY187   W84  C~4yRE      
2014 10  28.25014  01 13 37.875  -04 13 01.58  23.0i 13TY187   W84  C~4yRE      
2014 11  16.16555  01 12 22.217  -04 17 55.86  22.3i 13TY187   W84  C~4yRE      
2014 11  16.16555  01 12 22.22   -04 17 55.9   22.5i 13TY187   W84  C~3clQ      
2014 11  17.15825  01 12 18.674  -04 18 06.10  23.3g 13TY187   W84  C~4yRE      
2014 11  21.04127  01 12 05.410  -04 18 40.31  22.7z 13TY187   W84  C~4yRE      
2014 11  27.10989  01 11 46.478  -04 19 15.67  22.5r 13TY187   W84  C~4yRE      
2014 11  27.10989  01 11 46.48   -04 19 15.7   22.6r 13TY187   W84  C~3clQ      
2015 09  04.27970  01 22 16.464  -03 14 08.41  22.9z 13TY187   W84  C~4yRE      
2015 09  04.27970  01 22 16.46   -03 14 08.4   23.0z 13TY187   W84  C~3clQ      
2015 09  04.28108  01 22 16.455  -03 14 08.34  22.8i 13TY187   W84  C~4yRE      
2015 09  04.28108  01 22 16.45   -03 14 08.3   22.9i 13TY187   W84  C~3clQ      
2016 08  16.37184  01 27 54.199  -02 31 48.59  22.3i 13TY187   W84  C~4yRE      
2016 08  16.37184  01 27 54.20   -02 31 48.6   22.1i 13TY187   W84  C~3clQ      
2016 08  16.37321  01 27 54.193  -02 31 48.81  21.7z 13TY187   W84  C~4yRE      
2016 08  16.37321  01 27 54.19   -02 31 48.8   21.9z 13TY187   W84  C~3clQ      
2016 08  16.37458  01 27 54.191  -02 31 48.77  22.4i 13TY187   W84  C~4yRE      
2016 08  16.37458  01 27 54.19   -02 31 48.8   22.4i 13TY187   W84  C~3clQ      
2016 08  24.38707  01 27 36.947  -02 35 14.39  22.3z 13TY187   W84  C~4yRE      
2016 08  24.38707  01 27 36.95   -02 35 14.4   22.3z 13TY187   W84  C~3clQ      
2016 08  26.35469  01 27 31.988  -02 36 07.61  22.8r 13TY187   W84  C~4yRE      
2016 08  26.35469  01 27 31.99   -02 36 07.6   22.9r 13TY187   W84  C~3clQ      
2016 08  30.36370  01 27 21.040  -02 37 58.33  23.8g 13TY187   W84  C~4yRE      
2016 10  21.18835  01 23 53.034  -03 02 20.40  22.4z 13TY187   W84  C~4yRE      
2016 10  23.17622  01 23 44.084  -03 03 06.62  22.5r 13TY187   W84  C~4yRE      
2016 10  23.17622  01 23 44.08   -03 03 06.6   22.5r 13TY187   W84  C~3clQ      
2016 10  28.14953  01 23 21.985  -03 04 55.33  22.5i 13TY187   W84  C~4yRE      
2016 10  28.14953  01 23 21.99   -03 04 55.3   22.5i 13TY187   W84  C~3clQ      
2016 10  28.25215  01 23 21.525  -03 04 57.51  23.0r 13TY187   W84  C~4yRE      
2016 10  28.25215  01 23 21.52   -03 04 57.5   22.8r 13TY187   W84  C~3clQ      
2016 10  28.25352  01 23 21.539  -03 04 57.64  23.2g 13TY187   W84  C~4yRE      
2016 10  29.24398  01 23 17.177  -03 05 18.00  22.8i 13TY187   W84  C~4yRE      
2016 10  29.24398  01 23 17.18   -03 05 18.0   22.7i 13TY187   W84  C~3clQ      
2017 08  27.34312  01 32 21.869  -02 02 10.68  22.6i 13TY187   W84  C~4yRE      
2017 08  27.34452  01 32 21.871  -02 02 10.68  23.0r 13TY187   W84  C~4yRE      
2017 08  27.34588  01 32 21.857  -02 02 10.79  23.8g 13TY187   W84  C~4yRE      
2017 08  28.38473  01 32 19.158  -02 02 38.69  23.8g 13TY187   W84  C~4yRE      
2017 08  28.41462  01 32 19.092  -02 02 39.57  22.3z 13TY187   W84  C~4yRE      
2018 09  22.34498  01 35 49.616  -01 39 53.88  21.3z 13TY187   W84  C~4yRE      
2018 10  10.29117  01 34 32.886  -01 48 24.67  22.4i 13TY187   W84  C~4yRE      
2018 10  10.29256  01 34 32.887  -01 48 24.61  22.8r 13TY187   W84  C~4yRE      
2020 09  14.52179  01 46 07.489  -00 26 42.94  22.7w 13TY187   F51  C~48At      
2020 09  14.53333  01 46 07.477  -00 26 43.10  22.8w 13TY187   F51  C~48At      
2020 09  14.54435  01 46 07.417  -00 26 43.08  22.7w 13TY187   F51  C~48At      

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    -0.17       0.00    -0.13
     2   0.0029      0.00    -0.12       0.00    -0.15
     3   0.0029      0.00    -0.12       0.00    -0.13
     4   0.9944      0.00     0.01       0.00     0.12
     5   0.9944      0.00     0.07       0.00     0.09
     6   0.9944      0.00     0.22       0.00     0.33
     7   1.0297      0.00     0.10       0.00     0.09
     8   1.0681      0.00     0.02       0.00    -0.02
     9   1.1199      0.00     0.10       0.00     0.05
    10   1.1199      0.00     0.06       0.00     0.09
    11   1.1226      0.00    -0.10       0.00     0.00
    12   1.1332      0.00     0.13       0.00    -0.01
    13   1.1498      0.00     0.06       0.00    -0.04
    14   1.1498      0.00     0.03       0.00    -0.01
    15   1.9196      0.00     0.12       0.00    -0.08
    16   1.9196      0.00     0.06       0.00    -0.07
    17   1.9196      0.00    -0.02       0.00     0.07
    18   1.9196      0.00     0.05       0.00     0.03
    19   2.8699      0.00     0.03       0.00     0.08
    20   2.8699      0.00     0.02       0.00     0.09
    21   2.8699      0.00    -0.08       0.00    -0.08
    22   2.8699      0.00    -0.03       0.00    -0.09
    23   2.8699      0.00    -0.04       0.00    -0.05
    24   2.8699      0.00    -0.02       0.00    -0.02
    25   2.8919      0.00     0.15       0.00    -0.02
    26   2.8919      0.00     0.11       0.00    -0.01
    27   2.8973      0.00     0.07       0.00    -0.12
    28   2.8973      0.00     0.04       0.00    -0.13
    29   2.9082      0.00    -0.12       0.00     0.02
    30   3.0501      0.00     0.07       0.00     0.12
    31   3.0556      0.00    -0.20       0.00     0.02
    32   3.0556      0.00    -0.26       0.00     0.04
    33   3.0692      0.00     0.02       0.00     0.06
    34   3.0692      0.00    -0.05       0.00     0.03
    35   3.0695      0.00    -0.14       0.00    -0.01
    36   3.0695      0.00    -0.07       0.00    -0.02
    37   3.0695      0.00     0.23       0.00    -0.12
    38   3.0722      0.00     0.04       0.00    -0.08
    39   3.0722      0.00    -0.00       0.00    -0.08
    40   3.8993      0.00    -0.05       0.00     0.04
    41   3.8993      0.00     0.03       0.00     0.08
    42   3.8993      0.00    -0.12       0.00     0.01
    43   3.9021      0.00    -0.11       0.00     0.13
    44   3.9022      0.00     0.12       0.00     0.06
    45   4.9698      0.00     0.20       0.00    -0.06
    46   5.0189      0.00    -0.12       0.00    -0.01
    47   5.0189      0.00    -0.01       0.00     0.09
    48   6.9497      0.00    -0.17       0.00    -0.25
    49   6.9498      0.00     0.28       0.00    -0.08
    50   6.9498      0.00    -0.03       0.00     0.25

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.

13TY187    quality flag:3

Type:      CLASSICAL CLASSICAL CLASSICAL

axisobj        43.815    43.815    43.815
ecceobj         0.067     0.067     0.067
incobj         11.135    11.135    11.135
qmin           39.501    39.497    39.510
qmax           47.805    47.842    47.777
amean          43.546    43.546    43.546
amin           43.201    43.205    43.205
amax           43.909    43.912    43.909
emean           0.073     0.073     0.073
emin            0.057     0.057     0.057
emax            0.089     0.090     0.089
imean           9.425     9.425     9.425
imin            8.734     8.735     8.733
imax           10.086    10.083    10.091
excite_mean     0.180     0.180     0.180
fracstop        1.000     1.000     1.000
cjmean          3.058     3.058     3.058

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       175.6     175.6     175.6
kozaiamp        180.0     180.0     180.0