Orbit Fit and Astrometric record for 19EW9

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: 19EW9     
# Created Tue Apr  1 01:11:13 2025
# Orbit generated by ELGB
# -->Covariance matrix from a Bernstein fit
# Fitting     23 observations of     23
# Arc:  13.07y
# First observation: 2012/01/28
#  Last observation: 2025/02/23
# Chi-squared of fit:    14.27 DOF:     40 RMS:  0.14
# Min/Max residuals:    -0.62    0.25
# Exact a, adot, b, bdot, g, gdot:
  1.256370E-05  1.736136E-02  3.064451E-06  3.402730E-03  2.077064E-02 -3.995126E-03
# Covariance matrix:
  6.7325E-13 -1.3488E-13  5.7238E-14 -1.9185E-14  6.5940E-14 -3.6003E-13
 -1.3488E-13  5.5396E-14 -2.9756E-14  9.9218E-15  1.1335E-13  1.8824E-13
  5.7238E-14 -2.9756E-14  3.4737E-13 -4.5456E-14 -6.7849E-14 -1.1285E-13
 -1.9185E-14  9.9218E-15 -4.5456E-14  7.7478E-15  2.2447E-14  3.7629E-14
  6.5940E-14  1.1335E-13 -6.7849E-14  2.2447E-14  7.6059E-13  4.3285E-13
 -3.6003E-13  1.8824E-13 -1.1285E-13  3.7629E-14  4.3285E-13  7.1394E-13
#      lat0       lon0       xBary       yBary       zBary        JD0
   -0.307089  168.762123    0.641614   -0.004003   -0.748173  2455955.153343
# Heliocentric elements and errors
Epoch:              2455954.5000  =  2012/01/28
Mean Anomaly:          268.83777 +/-     0.046
Argument of Peri:      115.77100 +/-     0.026
Long of Asc Node:      169.54304 +/-     0.000
Inclination:            11.14299 +/-     0.000
Eccentricity:         0.23807948 +/-    0.0000
Semi-Major Axis:     46.16593735 +/-    0.0070
Time of Perihelion: 2484967.5484 +/-      24.3
Perihelion:          35.17477504 +/-    0.0056
Aphelion:            57.15709965 +/-    0.0088
Period (y)              313.6828 +/-      0.07
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X          -47.82690588 +/-    0.0020
Ecliptic Y           10.15845991 +/-    0.0004
Ecliptic Z           -0.25789725 +/-    0.0000
Ecliptic XDOT         0.00006366 +/-    0.0000
Ecliptic YDOT        -0.00234233 +/-    0.0000
Ecliptic ZDOT         0.00045143 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   48.89466938 +/-    0.0019
Geocenter to KBO     48.14506106 +/-    0.0020
# Hcoef:  7.17

The following table shows the complete astrometric record for 19EW9. 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 (19EW9) followed by the observatory code and reference code for the source of the astrometry.

2012 01  28.652577 11 18 11.55   +04 09 48.3         19EW9     T14  C~8Sg5      
2012 01  28.658049 11 18 11.52   +04 09 48.7         19EW9     T14  C~8Sg5      
2016 03  17.424991 11 31 29.29   +03 38 27.0         19EW9     T09  C~8Sg5      
2016 03  17.567553 11 31 28.70   +03 38 31.0         19EW9     T09  C~8Sg5      
2017 03  24.211426 11 35 12.559  +03 28 01.52  24.0V 19EW9     W84  C~8Sg5      
2018 03  18.50304  11 39 47.15   +03 11 41.4   23.6i 19EW9     T09  C~8Sg5      
2018 03  18.56001  11 39 46.92   +03 11 42.9   23.7i 19EW9     T09  C~8Sg5      
2018 03  18.57604  11 39 46.86   +03 11 43.2   24.0i 19EW9     T09  C~8Sg5      
2018 04  24.351987 11 37 34.68   +03 27 00.9         19EW9     T09  C~8Sg5      
2018 04  24.485347 11 37 34.28   +03 27 03.6         19EW9     T09  C~8Sg5      
2019 02  05.455206 11 46 30.81   +02 39 45.9         19EW9     T09  C~8Sg5      
2019 02  05.508896 11 46 30.65   +02 39 47.1         19EW9     T09  C~8Sg5      
2019 03  02.43089  11 45 04.91   +02 50 16.2   23.4y 19EW9     T09  C~8Sg5      
2019 03  02.51613  11 45 04.56   +02 50 19.1   22.9y 19EW9     T09  C~8Sg5      
2019 03  02.52968  11 45 04.51   +02 50 19.7   23.6y 19EW9     T09  C~8Sg5      
2019 03  02.55653  11 45 04.42   +02 50 20.4   23.5y 19EW9     T09  C~8Sg5      
2019 03  08.34835  11 44 41.74   +02 53 02.1   24.0r 19EW9     T09  C~8Sg5      
2019 03  08.35813  11 44 41.71   +02 53 02.4   24.0r 19EW9     T09  C~8Sg5      
2019 03  08.40222  11 44 41.54   +02 53 03.8   23.8r 19EW9     T09  C~8Sg5      
2019 03  08.43185  11 44 41.41   +02 53 04.4   23.9r 19EW9     T09  C~8Sg5      
2025 02  23.429490 12 11 30.504  +01 21 10.23  23.7G 19EW9     G37  C~8iif      
2025 02  23.471790 12 11 30.342  +01 21 11.18        19EW9     G37  C~8iif      
2025 02  23.523080 12 11 30.160  +01 21 12.39        19EW9     G37  C~8iif      

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     0.09       0.00    -0.14
     2   0.0000      0.00    -0.13       0.00     0.15
     3   4.1335      0.00     0.18       0.00    -0.09
     4   4.1339      0.00    -0.07       0.00    -0.02
     5   5.1514      0.00     0.06       0.00    -0.00
     6   6.1351      0.00    -0.09       0.00     0.13
     7   6.1353      0.00    -0.08       0.00     0.04
     8   6.1353      0.00    -0.00       0.00    -0.11
     9   6.2360      0.00     0.06       0.00    -0.02
    10   6.2364      0.00    -0.03       0.00     0.01
    11   7.0220      0.00     0.08       0.00     0.06
    12   7.0222      0.00     0.06       0.00     0.08
    13   7.0904      0.00     0.11       0.00    -0.62
    14   7.0907      0.00    -0.11       0.00    -0.08
    15   7.0907      0.00    -0.06       0.00     0.15
    16   7.0908      0.00     0.17       0.00     0.11
    17   7.1066      0.00    -0.19       0.00     0.07
    18   7.1067      0.00    -0.05       0.00     0.09
    19   7.1068      0.00     0.06       0.00     0.25
    20   7.1069      0.00    -0.10       0.00     0.02
    21  13.0726      0.00     0.11       0.00     0.16
    22  13.0727      0.00    -0.05       0.00    -0.02
    23  13.0729      0.00    -0.04       0.00    -0.18

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.

19EW9    quality flag:3

Type:       SCATNEAR  SCATNEAR  SCATNEAR

axisobj        46.110    46.110    46.110
ecceobj         0.238     0.238     0.238
incobj         11.157    11.157    11.157
qmin           34.704    34.778    34.645
qmax           58.342    58.327    58.312
amean          46.220    46.250    46.199
amin           45.541    45.750    45.739
amax           46.810    46.811    46.810
emean           0.231     0.229     0.230
emin            0.216     0.212     0.212
emax            0.248     0.247     0.249
imean          11.035    11.131    10.880
imin           10.055    10.234     9.639
imax           11.945    12.130    11.991
excite_mean     0.300     0.300     0.298
fracstop        1.000     1.000     1.000
cjmean          3.018     3.019     3.019

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       180.3     181.6     184.6
kozaiamp        179.9     180.0     179.9