Orbit Fit and Astrometric record for 15GY58

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: 15GY58    
# Created Wed May  8 01:17:06 2024
# Orbit generated from Bernstein formalism
# Fitting     39 observations of     39
# Arc:   2.35y
# First observation: 2015/02/17
#  Last observation: 2017/06/24
Preliminary a, adot, b, bdot, g, gdot:
  -0.000123   0.023241   0.000004   0.000514   0.023616   0.000000
# Chi-squared of fit:    13.21 DOF:     72 RMS:  0.10
# Min/Max residuals:    -0.40    0.25
# Exact a, adot, b, bdot, g, gdot:
  1.549965E-05  2.314530E-02  5.208450E-07  5.132608E-04  2.367921E-02  1.644492E-03
# Covariance matrix:
  1.5222E-13 -5.8112E-15 -1.5796E-15  2.1204E-15  1.1405E-13  1.5901E-12
 -5.8112E-15  2.6718E-13 -3.5500E-15  9.1642E-15  1.6600E-13  7.1161E-12
 -1.5796E-15 -3.5500E-15  8.1040E-14 -5.9428E-14 -3.8269E-15 -1.3087E-13
  2.1204E-15  9.1642E-15 -5.9428E-14  8.1021E-14  7.5526E-15  3.5350E-13
  1.1405E-13  1.6600E-13 -3.8269E-15  7.5526E-15  2.2671E-13  5.7976E-12
  1.5901E-12  7.1161E-12 -1.3087E-13  3.5350E-13  5.7976E-12  2.7495E-10
#      lat0       lon0       xBary       yBary       zBary        JD0
    2.630785 -154.303386    0.829821    0.024521   -0.530658  2457071.097458
# Heliocentric elements and errors
Epoch:              2457070.5000  =  2015/02/17
Mean Anomaly:           47.54090 +/-     0.275
Argument of Peri:        9.40448 +/-     0.352
Long of Asc Node:      141.47083 +/-     0.012
Inclination:             2.91186 +/-     0.000
Eccentricity:         0.06913493 +/-    0.0006
Semi-Major Axis:     44.73525987 +/-    0.0049
Time of Perihelion: 2442638.1086 +/-      83.4
Perihelion:          41.64249099 +/-    0.0277
Aphelion:            47.82802875 +/-    0.0279
Period (y)              299.2149 +/-      0.05
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X          -38.85572800 +/-    0.0008
Ecliptic Y          -17.77494940 +/-    0.0004
Ecliptic Z            1.93842376 +/-    0.0000
Ecliptic XDOT         0.00098803 +/-    0.0000
Ecliptic YDOT        -0.00249821 +/-    0.0000
Ecliptic ZDOT         0.00006810 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   42.77234984 +/-    0.0007
Geocenter to KBO     42.23114381 +/-    0.0008
# Hcoef:  8.15

The following table shows the complete astrometric record for 15GY58. 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 (15GY58) followed by the observatory code and reference code for the source of the astrometry.

2015 02  17.59668  13 39 08.665  -07 28 48.92  24.9r 15GY58    568  C~2nvb      
2015 02  17.63771  13 39 08.580  -07 28 48.20  24.6r 15GY58    568  C~2nvb      
2015 02  20.63083  13 39 02.486  -07 28 01.67  24.3r 15GY58    568  C~2nvb      
2015 03  18.57516  13 37 43.527  -07 19 05.14  24.6r 15GY58    568  C~2nvb      
2015 03  18.62254  13 37 43.337  -07 19 04.01  24.4r 15GY58    568  C~2nvb      
2015 03  20.57938  13 37 35.831  -07 18 16.08  24.4r 15GY58    568  C~2nvb      
2015 04  11.51365  13 36 03.146  -07 08 46.33  24.6r 15GY58    568  C~2nvb      
2015 04  13.37789  13 35 54.876  -07 07 57.08  24.5r 15GY58    568  C~2nvb      
2015 04  13.41891  13 35 54.708  -07 07 55.91  24.4r 15GY58    568  C~2nvb      
2015 04  13.42365  13 35 54.650  -07 07 55.93  24.1r 15GY58    568  C~2nvb      
2015 04  13.42846  13 35 54.655  -07 07 55.74  24.0r 15GY58    568  C~2nvb      
2015 04  13.43331  13 35 54.624  -07 07 55.60  24.1r 15GY58    568  C~2nvb      
2015 04  13.43815  13 35 54.604  -07 07 55.40  24.5r 15GY58    568  C~2nvb      
2015 04  13.52145  13 35 54.218  -07 07 53.28  24.4r 15GY58    568  C~2nvb      
2015 04  19.48929  13 35 27.603  -07 05 16.78  22.6r 15GY58    568  C~2nvb      
2015 05  18.34130  13 33 27.721  -06 54 04.60  24.3r 15GY58    568  C~2nvb      
2015 06  20.29133  13 32 00.307  -06 47 01.24  24.7r 15GY58    568  C~2nvb      
2015 06  20.33212  13 32 00.241  -06 47 00.95  24.5r 15GY58    568  C~2nvb      
2015 06  22.33610  13 31 57.442  -06 46 51.19  24.8r 15GY58    568  C~2nvb      
2015 07  14.28829  13 31 48.467  -06 47 17.12  25.5r 15GY58    568  C~2nvb      
2015 07  20.28135  13 31 53.139  -06 48 06.47  24.4r 15GY58    568  C~2nvb      
2016 02  04.58367  13 44 27.573  -07 58 19.80  24.7w 15GY58    568  C~2nvb      
2016 02  10.57151  13 44 21.929  -07 57 22.51  24.6w 15GY58    568  C~2nvb      
2016 02  10.61301  13 44 21.896  -07 57 21.93  24.8w 15GY58    568  C~2nvb      
2016 03  11.59678  13 43 10.483  -07 48 48.32  24.8w 15GY58    568  C~2nvb      
2016 04  03.46957  13 41 40.650  -07 39 26.87  24.7w 15GY58    568  C~2nvb      
2016 04  09.45073  13 41 14.482  -07 36 50.42  24.6w 15GY58    568  C~2nvb      
2016 05  01.45743  13 39 37.190  -07 27 30.31  24.7w 15GY58    568  C~2nvb      
2016 05  02.33152  13 39 33.476  -07 27 09.44  24.8w 15GY58    568  C~2nvb      
2016 05  02.36396  13 39 33.317  -07 27 08.76  23.9w 15GY58    568  C~2nvb      
2016 05  07.33487  13 39 12.449  -07 25 13.35  23.6w 15GY58    568  C~2nvb      
2016 05  29.33959  13 37 51.933  -07 18 09.18  24.9w 15GY58    568  C~2nvb      
2016 06  04.40200  13 37 34.348  -07 16 43.50  24.7w 15GY58    568  C~2nvb      
2016 06  27.33817  13 36 51.640  -07 13 49.63  24.8w 15GY58    568  C~2nvb      
2016 07  07.32804  13 36 46.135  -07 13 54.01  25.2w 15GY58    568  C~2nvc      
2017 03  29.51368  13 47 08.094  -08 08 49.55  24.9w 15GY58    568  C~2nvc      
2017 03  30.48302  13 47 04.066  -08 08 25.30        15GY58    568  C~2nvc      
2017 03  30.48771  13 47 04.053  -08 08 25.16  24.7w 15GY58    568  C~2nvc      
2017 06  24.30392  13 41 56.248  -07 41 01.24  25.0w 15GY58    568  C~2nvc      

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    -0.04
     2   0.0001     -1.44    -0.09       0.21     0.05
     3   0.0083   -102.76     0.16      10.83     0.07
     4   0.0793  -1391.88     0.02      85.91     0.03
     5   0.0795  -1394.93    -0.07      85.94    -0.03
     6   0.0848  -1516.39    -0.01      90.15    -0.03
     7   0.1449  -3008.54    -0.19     120.83     0.08
     8   0.1500  -3141.14     0.01     122.02     0.07
     9   0.1501  -3143.89     0.23     122.20     0.25
    10   0.1501  -3144.69    -0.23     121.87    -0.08
    11   0.1501  -3144.69     0.12     122.07     0.12
    12   0.1501  -3145.17    -0.01     122.03     0.09
    13   0.1501  -3145.52    -0.01     122.11     0.16
    14   0.1504  -3151.64    -0.09     122.00     0.04
    15   0.1667  -3577.70    -0.08     123.89    -0.06
    16   0.2457  -5485.72     0.15     100.45    -0.40
    17   0.3359  -6853.54     0.02      19.74    -0.11
    18   0.3360  -6854.56    -0.04      19.65    -0.06
    19   0.3415  -6896.99     0.04      13.51     0.03
    20   0.4016  -7012.10     0.05     -59.49    -0.03
    21   0.4180  -6929.20    -0.02     -80.03    -0.02
    22   0.9637   5060.89     0.09      54.74    -0.06
    23   0.9801   4962.02    -0.13      78.16    -0.12
    24   0.9802   4961.35     0.11      78.52     0.11
    25   1.0623   3786.10    -0.04     176.99    -0.06
    26   1.1249   2337.95     0.02     220.50    -0.01
    27   1.1413   1918.63     0.06     226.28     0.01
    28   1.2015    367.16    -0.15     226.61    -0.04
    29   1.2039    308.12     0.10     226.12     0.06
    30   1.2040    305.66    -0.11     225.90    -0.12
    31   1.2176    -25.45     0.22     221.34    -0.04
    32   1.2779  -1295.58    -0.00     183.37     0.02
    33   1.2945  -1570.50    -0.06     168.45    -0.02
    34   1.3573  -2225.85     0.07     100.11     0.00
    35   1.3846  -2300.61    -0.10      66.31    -0.10
    36   2.1107   7514.71    -0.12     319.98     0.14
    37   2.1133   7450.10     0.01     321.27    -0.03
    38   2.1133   7449.87     0.10     321.34     0.03
    39   2.3483   2588.29    -0.01     215.96     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.

15GY58    quality flag:3

Type:      CLASSICAL CLASSICAL CLASSICAL

axisobj        44.301    44.317    44.285
ecceobj         0.062     0.064     0.061
incobj          2.918     2.918     2.918
qmin           40.810    40.747    40.798
qmax           48.625    48.701    48.604
amean          44.587    44.604    44.551
amin           44.236    44.238    44.186
amax           44.959    44.970    44.934
emean           0.066     0.068     0.064
emin            0.051     0.052     0.047
emax            0.082     0.083     0.082
imean           2.208     2.211     2.187
imin            1.601     1.609     1.576
imax            2.830     2.831     2.820
excite_mean     0.077     0.078     0.075
fracstop        1.000     1.000     1.000
cjmean          3.102     3.102     3.101

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       188.5     187.9     178.4
kozaiamp        179.9     180.0     180.0