Orbit Fit and Astrometric record for 15BS518

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: 15BS518   
# Created Fri Nov 22 02:10:15 2024
# Orbit generated by ELGB
# -->Covariance matrix from a Bernstein fit
# Fitting     49 observations of     49
# Arc:  16.16y
# First observation: 2004/12/21
#  Last observation: 2021/02/16
# Chi-squared of fit:    42.37 DOF:     92 RMS:  0.16
# Min/Max residuals:    -0.74    0.39
# Exact a, adot, b, bdot, g, gdot:
  1.554125E-05  2.398371E-02 -5.590478E-06 -9.781168E-03  2.539011E-02 -1.928231E-03
# Covariance matrix:
  4.6130E-13 -6.8844E-14 -4.4984E-14  1.5745E-14 -3.5115E-14 -9.4809E-14
 -6.8844E-14  1.9905E-14  1.7324E-14 -6.5885E-15  3.5683E-14  3.8998E-14
 -4.4984E-14  1.7324E-14  3.7357E-13 -3.7037E-14  2.2436E-14  4.1427E-14
  1.5745E-14 -6.5885E-15 -3.7037E-14  5.3407E-15 -1.1719E-14 -1.5288E-14
 -3.5115E-14  3.5683E-14  2.2436E-14 -1.1719E-14  1.8075E-13  6.5603E-14
 -9.4809E-14  3.8998E-14  4.1427E-14 -1.5288E-14  6.5603E-14  9.1045E-14
#      lat0       lon0       xBary       yBary       zBary        JD0
   19.090912  159.726274    0.924864    0.109388   -0.315743  2453360.932345
# Heliocentric elements and errors
Epoch:              2453360.5000  =  2004/12/21
Mean Anomaly:          306.68360 +/-     0.016
Argument of Peri:      201.54703 +/-     0.020
Long of Asc Node:       17.47583 +/-     0.000
Inclination:            28.50169 +/-     0.000
Eccentricity:         0.11102849 +/-    0.0000
Semi-Major Axis:     42.14314335 +/-    0.0028
Time of Perihelion: 2468160.0044 +/-       9.6
Perihelion:          37.46405386 +/-    0.0028
Aphelion:            46.82223283 +/-    0.0034
Period (y)              273.5890 +/-      0.03
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X          -34.91099376 +/-    0.0006
Ecliptic Y           13.87985598 +/-    0.0002
Ecliptic Z           12.88150222 +/-    0.0002
Ecliptic XDOT        -0.00103613 +/-    0.0000
Ecliptic YDOT        -0.00238176 +/-    0.0000
Ecliptic ZDOT        -0.00106464 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   39.71606468 +/-    0.0005
Geocenter to KBO     39.38549113 +/-    0.0007
# Hcoef:  6.64

The following table shows the complete astrometric record for 15BS518. 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 (15BS518) followed by the observatory code and reference code for the source of the astrometry.

2004 12  21.431602 11 16 29.64   +25 29 18.7   22.4V 15BS518   645  C~2scb      
2004 12  21.432431 11 16 29.66   +25 29 18.7         15BS518   645  C~2scb      
2004 12  21.434919 11 16 29.65   +25 29 18.9         15BS518   645  C~2scb      
2014 03  20.48157  11 50 23.846  +15 58 34.73  22.8G 15BS518   F51  C~2r7b      
2014 03  25.30529  11 49 58.441  +16 00 24.07  23.1G 15BS518   F51  C~2r7b      
2014 03  25.31935  11 49 58.419  +16 00 24.04  22.3G 15BS518   F51  C~2r7b      
2014 03  25.33163  11 49 58.374  +16 00 24.02  22.2G 15BS518   F51  C~2r7b      
2014 03  25.34400  11 49 58.286  +16 00 24.46  22.7G 15BS518   F51  C~2r7b      
2015 01  28.51210  11 58 28.642  +14 21 10.51  22.6w 15BS518   F51  C~1vYB      
2015 01  28.52384  11 58 28.604  +14 21 10.90  22.6w 15BS518   F51  C~1vYB      
2015 01  28.53552  11 58 28.572  +14 21 11.10  22.5w 15BS518   F51  C~1vYB      
2015 02  16.40991  11 57 18.593  +14 30 46.76  22.2w 15BS518   F51  C~1vYB      
2015 02  16.42133  11 57 18.537  +14 30 47.41  22.4w 15BS518   F51  C~1vYB      
2015 02  16.43280  11 57 18.478  +14 30 47.63  22.4w 15BS518   F51  C~1vYB      
2015 02  16.44425  11 57 18.452  +14 30 47.70  22.4w 15BS518   F51  C~1vYB      
2015 02  18.43530  11 57 09.653  +14 31 50.58  22.4w 15BS518   F51  C~1vYB      
2015 02  18.44608  11 57 09.624  +14 31 50.96  22.4w 15BS518   F51  C~1vYB      
2015 02  18.45717  11 57 09.563  +14 31 51.20  22.4w 15BS518   F51  C~1vYB      
2015 02  18.46794  11 57 09.511  +14 31 51.36  22.5w 15BS518   F51  C~1vYB      
2015 03  25.49867  11 54 13.047  +14 48 16.21  22.4w 15BS518   F51  C~1vYB      
2015 03  25.51012  11 54 12.977  +14 48 16.16  22.3w 15BS518   F51  C~1vYB      
2015 03  25.52157  11 54 12.919  +14 48 16.58  22.4w 15BS518   F51  C~1vYB      
2015 03  25.53304  11 54 12.868  +14 48 16.88  22.3w 15BS518   F51  C~1vYB      
2016 02  03.53429  12 02 20.129  +13 11 25.75  22.8G 15BS518   F51  C~2r7b      
2016 02  04.43958  12 02 17.053  +13 11 52.02  22.0G 15BS518   F51  C~2r7b      
2016 02  11.47077  12 01 51.099  +13 15 22.33  22.6G 15BS518   F51  C~2r7b      
2016 02  11.48220  12 01 51.035  +13 15 22.43  22.6G 15BS518   F51  C~2r7b      
2016 02  11.49355  12 01 51.000  +13 15 23.02  22.7G 15BS518   F51  C~2r7b      
2016 02  11.50493  12 01 50.960  +13 15 23.42  22.7G 15BS518   F51  C~2r7b      
2016 04  22.36259  11 56 06.992  +13 42 54.39  23.2G 15BS518   F51  C~2r7b      
2016 04  26.28088  11 55 50.813  +13 43 16.69  22.3G 15BS518   F51  C~2r7b      
2017 03  04.50351  12 04 23.134  +12 13 03.23  22.6G 15BS518   F51  C~2r7b      
2017 03  04.53963  12 04 22.923  +12 13 03.99  22.3G 15BS518   F51  C~2r7b      
2017 03  04.55143  12 04 22.871  +12 13 04.60  22.4G 15BS518   F51  C~2r7b      
2017 03  04.56324  12 04 22.813  +12 13 04.81  22.5G 15BS518   F51  C~2r7b      
2017 03  21.34044  12 02 56.555  +12 20 45.90  22.4G 15BS518   F51  C~2r7b      
2017 03  21.35189  12 02 56.494  +12 20 46.19  22.4G 15BS518   F51  C~2r7b      
2017 03  21.36331  12 02 56.424  +12 20 46.37  22.7G 15BS518   F51  C~2r7b      
2017 03  21.37474  12 02 56.369  +12 20 46.72  22.5G 15BS518   F51  C~2r7b      
2017 03  30.35636  12 02 09.563  +12 24 15.07  22.5G 15BS518   F51  C~2r7b      
2017 04  20.26618  12 00 28.026  +12 29 46.04  22.7G 15BS518   F51  C~2r7b      
2017 04  20.27840  12 00 27.955  +12 29 46.06  22.6G 15BS518   F51  C~2r7b      
2017 04  20.29052  12 00 27.901  +12 29 46.40  22.3G 15BS518   F51  C~2r7b      
2017 04  20.30271  12 00 27.839  +12 29 46.52  22.6G 15BS518   F51  C~2r7b      
2018 04  10.17713  12 05 26.217  +11 13 56.30  22.0R 15BS518   G37  C~2r7b      
2018 04  10.22933  12 05 25.968  +11 13 57.40        15BS518   G37  C~2r7b      
2021 02  16.579402 12 22 03.634  +07 07 33.16  22.3w 15BS518   F51  C~4ZGQ      
2021 02  16.591703 12 22 03.585  +07 07 33.37  22.2w 15BS518   F51  C~4ZGQ      
2021 02  16.616347 12 22 03.492  +07 07 34.02  22.2w 15BS518   F51  C~4ZGQ      

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    -0.04
     2   0.0000      0.00     0.13       0.00    -0.07
     3   0.0000      0.00     0.01       0.00     0.06
     4   9.2431      0.00    -0.23       0.00     0.04
     5   9.2563      0.00    -0.74       0.00     0.32
     6   9.2564      0.00     0.05       0.00    -0.02
     7   9.2564      0.00     0.36       0.00    -0.31
     8   9.2564      0.00     0.03       0.00    -0.13
     9  10.1029      0.00    -0.10       0.00     0.13
    10  10.1029      0.00    -0.13       0.00     0.18
    11  10.1030      0.00    -0.07       0.00     0.04
    12  10.1546      0.00     0.16       0.00    -0.19
    13  10.1547      0.00     0.08       0.00     0.10
    14  10.1547      0.00    -0.05       0.00    -0.05
    15  10.1547      0.00     0.32       0.00    -0.34
    16  10.1602      0.00    -0.20       0.00     0.06
    17  10.1602      0.00     0.10       0.00     0.10
    18  10.1602      0.00    -0.06       0.00    -0.01
    19  10.1603      0.00    -0.11       0.00    -0.19
    20  10.2562      0.00     0.13       0.00     0.25
    21  10.2562      0.00    -0.00       0.00    -0.05
    22  10.2562      0.00     0.04       0.00     0.11
    23  10.2563      0.00     0.19       0.00     0.16
    24  11.1187      0.00     0.23       0.00     0.13
    25  11.1212      0.00     0.07       0.00    -0.02
    26  11.1404      0.00     0.04       0.00    -0.02
    27  11.1405      0.00    -0.23       0.00    -0.27
    28  11.1405      0.00    -0.07       0.00    -0.03
    29  11.1405      0.00     0.02       0.00     0.03
    30  11.3345      0.00    -0.11       0.00    -0.04
    31  11.3452      0.00    -0.10       0.00     0.22
    32  12.2001      0.00     0.26       0.00     0.13
    33  12.2002      0.00    -0.16       0.00    -0.16
    34  12.2002      0.00    -0.05       0.00     0.10
    35  12.2002      0.00    -0.03       0.00    -0.04
    36  12.2462      0.00     0.03       0.00     0.01
    37  12.2462      0.00     0.02       0.00     0.02
    38  12.2462      0.00    -0.12       0.00    -0.09
    39  12.2463      0.00    -0.03       0.00    -0.03
    40  12.2708      0.00     0.15       0.00    -0.12
    41  12.3281      0.00     0.14       0.00     0.09
    42  12.3281      0.00    -0.10       0.00    -0.02
    43  12.3282      0.00    -0.09       0.00     0.20
    44  12.3282      0.00    -0.20       0.00     0.20
    45  13.2998      0.00     0.22       0.00    -0.22
    46  13.2999      0.00     0.39       0.00    -0.01
    47  16.1565      0.00    -0.15       0.00     0.05
    48  16.1565      0.00    -0.15       0.00    -0.07
    49  16.1566      0.00    -0.05       0.00    -0.07

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.

15BS518    quality flag:3

Type:       SCATEXTD  SCATEXTD  SCATEXTD

axisobj        41.796    41.796    41.796
ecceobj         0.105     0.105     0.105
incobj         28.605    28.605    28.605
qmin           36.428    36.423    36.470
qmax           47.688    47.674    47.674
amean          41.918    41.923    41.920
amin           41.583    41.571    41.576
amax           42.298    42.299    42.297
emean           0.112     0.112     0.112
emin            0.096     0.098     0.097
emax            0.128     0.127     0.128
imean          28.331    28.344    28.341
imin           28.005    28.006    28.013
imax           28.711    28.738    28.707
excite_mean     0.488     0.488     0.488
fracstop        1.000     1.000     1.000
cjmean          2.782     2.781     2.781

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       181.6     181.4     181.4
kozaiamp        180.0     180.0     180.0