Orbit Fit and Astrometric record for 16EF367

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: 16EF367   
# Created Wed Nov 27 02:10:35 2024
# Orbit generated from Bernstein formalism
# Fitting     32 observations of     32
# Arc:  11.11d
# First observation: 2016/03/04
#  Last observation: 2016/03/15
Preliminary a, adot, b, bdot, g, gdot:
  -0.000000   0.044548   0.000001  -0.008785   0.030372   0.000000
# WARNING MRQMIN stopped after  13 iterations -- oscilliatory solution
# WARNING Fitting with energy constraint
# Chi-squared of fit:    21.15 DOF:     59 RMS:  0.14
# Min/Max residuals:    -0.33    0.57
# Exact a, adot, b, bdot, g, gdot:
  1.948141E-05  3.618300E-02 -4.331430E-06 -8.384428E-03  2.902688E-02  8.368879E-03
# Covariance matrix:
  3.0740E-12  4.3409E-09  2.5642E-13 -2.1346E-10  7.1649E-10 -1.1135E-08
  4.3409E-09  6.6739E-06  3.9296E-10 -3.2653E-07  1.0960E-06 -2.1781E-05
  2.5642E-13  3.9296E-10  1.8454E-13 -2.6901E-11  6.4550E-11 -1.2689E-09
 -2.1346E-10 -3.2653E-07 -2.6901E-11  1.6493E-08 -5.3649E-08  1.0394E-06
  7.1649E-10  1.0960E-06  6.4550E-11 -5.3649E-08  1.8008E-07 -3.4884E-06
 -1.1135E-08 -2.1781E-05 -1.2689E-09  1.0394E-06 -3.4884E-06  1.8953E-04
#      lat0       lon0       xBary       yBary       zBary        JD0
   -8.775943  151.148184   -0.217997   -0.146967   -0.953057  2457451.926989
# Heliocentric elements and errors
Epoch:              2457450.5000  =  2016/03/03
Mean Anomaly:            8.14279 +/-    10.654
Argument of Peri:      177.96373 +/-    50.089
Long of Asc Node:      298.86833 +/-     1.618
Inclination:            15.55191 +/-     0.660
Eccentricity:         0.57869636 +/-    0.2569
Semi-Major Axis:     78.26625729 +/-   33.3844
Time of Perihelion: 2451730.0375 +/-    6528.7
Perihelion:          32.97385917 +/-   24.5398
Aphelion:           123.55865540 +/-   56.4098
Period (y)              692.4207 +/-    443.03
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X          -30.77509181 +/-    0.4359
Ecliptic Y           16.70143265 +/-    0.2402
Ecliptic Z           -5.25634174 +/-    0.0768
Ecliptic XDOT        -0.00222462 +/-    0.0011
Ecliptic YDOT        -0.00267795 +/-    0.0007
Ecliptic ZDOT        -0.00090199 +/-    0.0002
# Distances at JD0 (AU)
Heliocenter to KBO   35.40724865 +/-    0.3957
Geocenter to KBO     34.45082958 +/-    0.5036
# Hcoef:  8.72

The following table shows the complete astrometric record for 16EF367. 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 (16EF367) followed by the observatory code and reference code for the source of the astrometry.

2016 03  04.42620  10 00 18.25   +02 50 59.2   23.9i 16EF367   T09  C~8AhO      
2016 03  04.43733  10 00 18.19   +02 50 59.5   23.6i 16EF367   T09  C~8AhO      
2016 03  04.45194  10 00 18.12   +02 50 59.9   23.8i 16EF367   T09  C~8AhO      
2016 03  07.27865  10 00 03.84   +02 52 16.4   25.1g 16EF367   T09  C~8AhO      
2016 03  07.28113  10 00 03.81   +02 52 16.6   25.1g 16EF367   T09  C~8AhO      
2016 03  07.28866  10 00 03.77   +02 52 16.9   25.1g 16EF367   T09  C~8AhO      
2016 03  07.29878  10 00 03.72   +02 52 17.1   25.4g 16EF367   T09  C~8AhO      
2016 03  07.30953  10 00 03.67   +02 52 17.3   25.1g 16EF367   T09  C~8AhO      
2016 03  07.31343  10 00 03.66   +02 52 17.3   25.2g 16EF367   T09  C~8AhO      
2016 03  07.32114  10 00 03.61   +02 52 17.6   25.1g 16EF367   T09  C~8AhO      
2016 03  07.32499  10 00 03.60   +02 52 17.8   24.9g 16EF367   T09  C~8AhO      
2016 03  07.32886  10 00 03.58   +02 52 17.8   24.8g 16EF367   T09  C~8AhO      
2016 03  09.153116 09 59 54.499  +02 53 08.05  23.8r 16EF367   W84  C~8HEL      
2016 03  09.166380 09 59 54.427  +02 53 08.34  23.7i 16EF367   W84  C~8HEL      
2016 03  09.200558 09 59 54.276  +02 53 09.13  23.8r 16EF367   W84  C~8HEL      
2016 03  09.29953  09 59 53.79   +02 53 11.5   24.3r 16EF367   T09  C~8AhO      
2016 03  09.30973  09 59 53.73   +02 53 12.0   24.5r 16EF367   T09  C~8AhO      
2016 03  09.33622  09 59 53.61   +02 53 12.7   24.7r 16EF367   T09  C~8AhO      
2016 03  09.34016  09 59 53.60   +02 53 12.8   24.5r 16EF367   T09  C~8AhO      
2016 03  12.39109  09 59 38.76   +02 54 36.3   23.6z 16EF367   T09  C~8AhO      
2016 03  12.42050  09 59 38.62   +02 54 37.0   23.6z 16EF367   T09  C~8AhO      
2016 03  12.44690  09 59 38.49   +02 54 37.8   23.7z 16EF367   T09  C~8AhO      
2016 03  12.45077  09 59 38.47   +02 54 37.8   23.6z 16EF367   T09  C~8AhO      
2016 03  12.45461  09 59 38.45   +02 54 38.0   23.6z 16EF367   T09  C~8AhO      
2016 03  12.46234  09 59 38.43   +02 54 38.1   24.2z 16EF367   T09  C~8AhO      
2016 03  12.47390  09 59 38.36   +02 54 38.5   23.8z 16EF367   T09  C~8AhO      
2016 03  15.49118  09 59 24.17   +02 56 00.9   23.8y 16EF367   T09  C~8AhO      
2016 03  15.49888  09 59 24.13   +02 56 01.4   23.4y 16EF367   T09  C~8AhO      
2016 03  15.50274  09 59 24.12   +02 56 01.2   23.1y 16EF367   T09  C~8AhO      
2016 03  15.50659  09 59 24.12   +02 56 00.9   23.3y 16EF367   T09  C~8AhO      
2016 03  15.51045  09 59 24.06   +02 56 01.7   23.7y 16EF367   T09  C~8AhO      
2016 03  15.53155  09 59 23.95   +02 56 02.0   23.7y 16EF367   T09  C~8AhO      

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     0.05       0.00    -0.05
     2   0.0000     -0.95     0.02      -0.03    -0.06
     3   0.0001     -2.07     0.10      -0.02    -0.02
     4   0.0078   -229.25     0.17      -2.95    -0.06
     5   0.0078   -229.74    -0.12      -2.92    -0.03
     6   0.0078   -230.41    -0.18      -2.85     0.05
     7   0.0079   -231.18    -0.13      -2.92    -0.01
     8   0.0079   -231.95    -0.03      -2.99    -0.07
     9   0.0079   -232.09     0.14      -3.05    -0.12
    10   0.0079   -232.90    -0.04      -3.03    -0.09
    11   0.0079   -233.11     0.06      -2.89     0.05
    12   0.0079   -233.39     0.10      -3.00    -0.05
    13   0.0129   -378.42    -0.14      -3.35     0.19
    14   0.0130   -379.53    -0.19      -3.45     0.09
    15   0.0131   -381.92     0.15      -3.50     0.07
    16   0.0133   -389.57     0.03      -3.82    -0.10
    17   0.0134   -390.59    -0.17      -3.66     0.06
    18   0.0134   -392.52     0.02      -3.64     0.10
    19   0.0135   -392.69     0.16      -3.59     0.15
    20   0.0218   -630.17    -0.11      -2.86     0.09
    21   0.0219   -632.38    -0.02      -2.94     0.01
    22   0.0220   -634.49    -0.07      -2.87     0.07
    23   0.0220   -634.77    -0.05      -2.97    -0.03
    24   0.0220   -635.12    -0.10      -2.89     0.05
    25   0.0220   -635.44     0.19      -2.90     0.04
    26   0.0220   -636.56    -0.04      -2.89     0.05
    27   0.0303   -864.52     0.11       0.22    -0.05
    28   0.0303   -865.26    -0.05       0.48     0.20
    29   0.0303   -865.33     0.17       0.24    -0.05
    30   0.0303   -865.23     0.57      -0.04    -0.33
    31   0.0303   -866.35    -0.26       0.40     0.10
    32   0.0304   -868.00    -0.32       0.10    -0.22

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.