Orbit Fit and Astrometric record for 11UP410

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: 11UP410   
# Created Fri Mar 29 01:14:10 2024
# Orbit generated by ELGB
# -->Covariance matrix from a Bernstein fit
# Fitting     34 observations of     34
# Arc:   7.43y
# First observation: 2011/09/05
#  Last observation: 2019/02/08
# Chi-squared of fit:    14.12 DOF:     62 RMS:  0.11
# Min/Max residuals:    -0.25    0.27
# Exact a, adot, b, bdot, g, gdot:
  1.784088E-05  3.585529E-02 -5.156965E-07 -1.502276E-03  3.062631E-02 -1.803260E-03
# Covariance matrix:
  1.9417E-13 -7.3832E-14 -2.5214E-15  4.2259E-15  1.0459E-13 -3.4801E-13
 -7.3832E-14  1.4909E-13  4.0456E-15 -7.1769E-15  3.0553E-14  6.2329E-13
 -2.5214E-15  4.0456E-15  6.2338E-14 -1.6996E-14  4.0461E-17  1.9370E-14
  4.2259E-15 -7.1769E-15 -1.6996E-14  1.4972E-14 -3.4124E-16 -3.4172E-14
  1.0459E-13  3.0553E-14  4.0461E-17 -3.4124E-16  1.3518E-13  5.0357E-14
 -3.4801E-13  6.2329E-13  1.9370E-14 -3.4172E-14  5.0357E-14  2.9529E-12
#      lat0       lon0       xBary       yBary       zBary        JD0
    1.383460   33.331660    0.780838    0.015255   -0.632585  2455810.024946
# Heliocentric elements and errors
Epoch:              2455810.5000  =  2011/09/06
Mean Anomaly:          340.52627 +/-     0.013
Argument of Peri:      178.34708 +/-     0.019
Long of Asc Node:      241.79417 +/-     0.002
Inclination:             2.72758 +/-     0.000
Eccentricity:         0.18064252 +/-    0.0000
Semi-Major Axis:     39.90067039 +/-    0.0024
Time of Perihelion: 2460790.3391 +/-       8.6
Perihelion:          32.69291272 +/-    0.0024
Aphelion:            47.10842806 +/-    0.0032
Period (y)              252.0452 +/-      0.02
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X           28.23374030 +/-    0.0003
Ecliptic Y           17.63288669 +/-    0.0002
Ecliptic Z            0.78832571 +/-    0.0000
Ecliptic XDOT        -0.00189641 +/-    0.0000
Ecliptic YDOT         0.00259663 +/-    0.0000
Ecliptic ZDOT        -0.00013809 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   33.29695476 +/-    0.0003
Geocenter to KBO     32.65172662 +/-    0.0004
# Hcoef:  8.36

The following table shows the complete astrometric record for 11UP410. 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 (11UP410) followed by the observatory code and reference code for the source of the astrometry.

2011 09  05.52418  02 02 29.121  +13 55 31.79        11UP410   568  C~1C6L      
2011 10  24.40337  01 58 31.895  +13 34 38.54  23.5r 11UP410   568  C~1C6L      
2011 10  24.44610  01 58 31.649  +13 34 37.14  23.4r 11UP410   568  C~1C6L      
2011 10  24.48881  01 58 31.396  +13 34 35.78  23.4r 11UP410   568  C~1C6L      
2011 10  26.42314  01 58 20.223  +13 33 33.96  23.3r 11UP410   568  C~1C6L      
2011 10  28.30027  01 58 09.406  +13 32 33.72        11UP410   568  C~1C6L      
2011 10  28.48012  01 58 08.348  +13 32 28.04        11UP410   568  C~1C6L      
2011 10  30.30008  01 57 57.905  +13 31 29.56        11UP410   568  C~1C6L      
2011 10  30.52443  01 57 56.590  +13 31 22.44  23.3r 11UP410   568  C~1C6L      
2011 10  31.50734  01 57 50.958  +13 30 50.94  23.5r 11UP410   568  C~1C6L      
2011 11  24.29629  01 55 43.637  +13 18 39.92  23.4r 11UP410   568  C~1C6L      
2011 11  30.34253  01 55 16.049  +13 15 55.50  23.6r 11UP410   568  C~1C6L      
2011 11  30.35120  01 55 16.015  +13 15 55.15  23.6r 11UP410   568  C~1C6L      
2012 01  25.28222  01 53 51.888  +13 05 14.50  23.7r 11UP410   568  C~1C6L      
2012 01  26.26707  01 53 53.654  +13 05 20.58  23.9r 11UP410   568  C~1C6L      
2012 01  27.32416  01 53 55.660  +13 05 27.75  23.5r 11UP410   568  C~1C6L      
2012 02  21.23299  01 55 19.792  +13 11 42.38  23.5r 11UP410   568  C~1C6L      
2012 08  17.56010  02 11 14.576  +14 35 22.27  23.3r 11UP410   568  C~1C6L      
2012 08  23.53769  02 11 06.103  +14 34 47.31  24.0r 11UP410   568  C~1C6L      
2012 08  24.51776  02 11 04.339  +14 34 39.57  23.5r 11UP410   568  C~1C6L      
2012 08  24.57339  02 11 04.234  +14 34 39.11  23.7r 11UP410   568  C~1C6L      
2012 10  17.36532  02 07 19.745  +14 15 45.33  23.3r 11UP410   568  C~1C6L      
2012 10  17.40813  02 07 19.500  +14 15 44.11  23.2r 11UP410   568  C~1C6L      
2012 10  17.42550  02 07 19.396  +14 15 43.49  23.3r 11UP410   568  C~1C6L      
2012 10  20.46016  02 07 01.952  +14 14 10.73  23.7r 11UP410   568  C~1C6L      
2012 10  20.50496  02 07 01.687  +14 14 09.34  23.4r 11UP410   568  C~1C6L      
2013 01  04.33671  02 01 40.545  +13 43 07.60  23.3r 11UP410   568  C~1C6L      
2013 01  14.35870  02 01 37.032  +13 42 15.19  23.8r 11UP410   568  C~1C6L      
2013 02  02.25552  02 02 03.501  +13 43 32.15  23.5r 11UP410   568  C~1C6L      
2013 12  05.41625  02 11 10.33   +14 28 48.1         11UP410   568  C~1CKy      
2013 12  05.42432  02 11 10.29   +14 28 47.8         11UP410   568  C~1CKy      
2013 12  05.43226  02 11 10.25   +14 28 47.6         11UP410   568  C~1CKy      
2019 02  08.138400 02 51 04.543  +17 07 21.98  24.1G 11UP410   G37  C~2zmc      
2019 02  08.237780 02 51 04.747  +17 07 22.93        11UP410   G37  C~2zmc      

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     0.15       0.00    -0.00
     2   0.1338      0.00    -0.09       0.00     0.17
     3   0.1339      0.00    -0.01       0.00     0.13
     4   0.1341      0.00    -0.04       0.00     0.14
     5   0.1394      0.00    -0.21       0.00     0.11
     6   0.1445      0.00    -0.18       0.00     0.02
     7   0.1450      0.00    -0.22       0.00     0.10
     8   0.1500      0.00     0.00       0.00     0.03
     9   0.1506      0.00    -0.04       0.00     0.11
    10   0.1533      0.00     0.06       0.00     0.14
    11   0.2184      0.00     0.05       0.00    -0.15
    12   0.2350      0.00     0.02       0.00    -0.07
    13   0.2350      0.00     0.08       0.00    -0.19
    14   0.3881      0.00     0.06       0.00    -0.01
    15   0.3908      0.00     0.15       0.00    -0.05
    16   0.3937      0.00     0.06       0.00    -0.14
    17   0.4619      0.00    -0.12       0.00    -0.19
    18   0.9501      0.00     0.06       0.00    -0.01
    19   0.9665      0.00    -0.00       0.00     0.03
    20   0.9692      0.00    -0.06       0.00     0.02
    21   0.9693      0.00    -0.00       0.00     0.00
    22   1.1166      0.00    -0.02       0.00    -0.09
    23   1.1167      0.00     0.05       0.00    -0.02
    24   1.1168      0.00     0.00       0.00    -0.11
    25   1.1251      0.00     0.05       0.00    -0.07
    26   1.1252      0.00     0.02       0.00    -0.07
    27   1.3328      0.00     0.02       0.00    -0.09
    28   1.3603      0.00     0.20       0.00    -0.05
    29   1.4120      0.00     0.07       0.00    -0.04
    30   2.2502      0.00    -0.02       0.00     0.16
    31   2.2502      0.00    -0.09       0.00     0.06
    32   2.2503      0.00    -0.17       0.00     0.06
    33   7.4267      0.00    -0.25       0.00    -0.22
    34   7.4270      0.00     0.27       0.00     0.23

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.

11UP410    quality flag:3

Type:           3:2E      3:2E      3:2E

axisobj        39.980    39.980    39.980
ecceobj         0.181     0.181     0.182
incobj          2.726     2.726     2.726
qmin           32.284    32.279    32.281
qmax           47.358    47.306    47.365
amean          39.458    39.458    39.458
amin           38.956    38.950    38.949
amax           40.023    40.012    40.032
emean           0.165     0.165     0.165
emin            0.147     0.146     0.148
emax            0.184     0.184     0.184
imean           4.600     4.597     4.600
imin            3.711     3.713     3.715
imax            5.258     5.258     5.260
excite_mean     0.184     0.184     0.184
fracstop        1.000     1.000     1.000
cjmean          3.013     3.013     3.013

libcent 0       179.9     179.6     180.0
libamp  0       113.9     114.5     113.8
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       180.6     180.1     180.4
kozaiamp        180.0     179.9     180.0