Orbit Fit and Astrometric record for 14VW37

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: 14VW37    
# Created Sun Dec 22 02:10:10 2024
# Orbit generated from Bernstein formalism
# Fitting     64 observations of     64
# Arc:   4.04y
# First observation: 2014/11/12
#  Last observation: 2018/11/26
Preliminary a, adot, b, bdot, g, gdot:
   0.000159   0.029802  -0.000100   0.004209   0.027611   0.000000
# Chi-squared of fit:    14.17 DOF:    122 RMS:  0.08
# Min/Max residuals:    -0.24    0.24
# Exact a, adot, b, bdot, g, gdot:
  1.797597E-05  3.007724E-02  2.580535E-06  4.287192E-03  2.765582E-02  1.163350E-03
# Covariance matrix:
  9.5135E-14 -4.7165E-14 -1.2447E-14 -6.5398E-15  4.2420E-14 -2.5774E-13
 -4.7165E-14  1.0902E-13 -2.3354E-14  2.4486E-14  4.9354E-14  9.8760E-13
 -1.2447E-14 -2.3354E-14  7.7034E-14 -2.8722E-14 -4.6940E-14 -2.4125E-13
 -6.5398E-15  2.4486E-14 -2.8722E-14  2.0706E-14  1.2306E-14  2.5553E-13
  4.2420E-14  4.9354E-14 -4.6940E-14  1.2306E-14  1.2956E-13  5.0769E-13
 -2.5774E-13  9.8760E-13 -2.4125E-13  2.5553E-13  5.0769E-13  1.0306E-11
#      lat0       lon0       xBary       yBary       zBary        JD0
  -49.423506   43.528877   -0.103166   -0.748286   -0.641076  2456973.849725
# Heliocentric elements and errors
Epoch:              2456970.5000  =  2014/11/09
Mean Anomaly:           16.11979 +/-     0.035
Argument of Peri:      256.08036 +/-     0.048
Long of Asc Node:      122.89439 +/-     0.000
Inclination:            48.77544 +/-     0.000
Eccentricity:         0.13263498 +/-    0.0001
Semi-Major Axis:     42.10065701 +/-    0.0024
Time of Perihelion: 2452502.7538 +/-       9.8
Perihelion:          36.51663709 +/-    0.0033
Aphelion:            47.68467694 +/-    0.0037
Period (y)              273.1754 +/-      0.02
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X           17.69290473 +/-    0.0002
Ecliptic Y           16.95369511 +/-    0.0002
Ecliptic Z          -27.46395181 +/-    0.0004
Ecliptic XDOT        -0.00176698 +/-    0.0000
Ecliptic YDOT         0.00242749 +/-    0.0000
Ecliptic ZDOT         0.00018870 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   36.80672907 +/-    0.0003
Geocenter to KBO     36.15875309 +/-    0.0005
# Hcoef:  6.99

The following table shows the complete astrometric record for 14VW37. 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 (14VW37) followed by the observatory code and reference code for the source of the astrometry.

2014 11  12.348947 03 46 05.61   -31 14 33.6   22.6z 14VW37    W84  C~1wab      
2014 11  12.34897  03 46 05.622  -31 14 33.61  22.1z 14VW37    W84  C~4yV3      
2014 11  18.335509 03 45 27.76   -31 15 50.0   24.1g 14VW37    W84  C~1wab      
2014 11  18.33553  03 45 27.752  -31 15 49.94  23.5g 14VW37    W84  C~4yV3      
2014 11  18.33696  03 45 27.744  -31 15 49.88  22.2z 14VW37    W84  C~4yV3      
2015 01  08.153218 03 40 49.43   -30 54 19.8   22.8z 14VW37    W84  C~1wab      
2015 01  08.15323  03 40 49.439  -30 54 19.80  22.4z 14VW37    W84  C~4yV3      
2015 01  09.18421  03 40 45.724  -30 53 20.59  23.0z 14VW37    W84  C~4yV3      
2015 01  10.170671 03 40 42.26   -30 52 23.3   22.6i 14VW37    W84  C~1wab      
2015 01  10.17068  03 40 42.281  -30 52 23.27  22.4i 14VW37    W84  C~4yV3      
2015 01  25.137106 03 40 03.28   -30 36 04.0   23.5g 14VW37    W84  C~1wab      
2015 01  25.13712  03 40 03.277  -30 36 04.12  23.5g 14VW37    W84  C~4yV3      
2015 01  26.14304  03 40 01.596  -30 34 51.92  22.1i 14VW37    W84  C~4yV3      
2015 01  26.144395 03 40 01.59   -30 34 51.8   23.2g 14VW37    W84  C~1wab      
2015 01  26.14440  03 40 01.595  -30 34 51.79  22.8g 14VW37    W84  C~4yV3      
2015 01  26.145745 03 40 01.59   -30 34 51.6   22.3r 14VW37    W84  C~1wab      
2015 01  26.14575  03 40 01.600  -30 34 51.62  22.3r 14VW37    W84  C~4yV3      
2015 02  01.109757 03 39 54.21   -30 27 30.6   22.9z 14VW37    W84  C~1wab      
2015 02  01.10976  03 39 54.207  -30 27 30.58  22.4z 14VW37    W84  C~4yV3      
2015 10  17.36540  03 55 41.114  -30 10 40.10  22.5i 14VW37    W84  C~4yV3      
2015 11  15.345058 03 52 56.38   -30 26 04.6   22.6i 14VW37    W84  C~1wab      
2015 11  15.34507  03 52 56.384  -30 26 04.56  22.5i 14VW37    W84  C~4yV3      
2015 11  16.329769 03 52 50.19   -30 26 18.1   22.7r 14VW37    W84  C~1wab      
2015 11  16.32978  03 52 50.201  -30 26 18.17  22.5r 14VW37    W84  C~4yV3      
2015 11  16.331123 03 52 50.21   -30 26 18.2   23.0g 14VW37    W84  C~1wab      
2015 11  16.33115  03 52 50.203  -30 26 18.16  22.6g 14VW37    W84  C~4yV3      
2015 11  29.297164 03 51 28.27   -30 27 17.0   22.5z 14VW37    W84  C~352R      
2015 11  29.297685 03 51 28.26   -30 27 16.9   22.5z 14VW37    W84  C~1wab      
2015 11  29.29769  03 51 28.273  -30 27 16.97  22.3z 14VW37    W84  C~4yV3      
2016 01  14.166875 03 47 34.22   -30 01 07.2   22.7i 14VW37    W84  C~1wab      
2016 01  14.16690  03 47 34.222  -30 01 07.25  22.8i 14VW37    W84  C~4yV3      
2016 01  14.167743 03 47 34.22   -30 01 07.1   23.3r 14VW37    W84  C~352R      
2016 01  14.168264 03 47 34.21   -30 01 07.0   23.3r 14VW37    W84  C~1wab      
2016 01  14.16827  03 47 34.217  -30 01 07.13  23.1r 14VW37    W84  C~4yV3      
2016 01  14.169641 03 47 34.21   -30 01 07.1   23.6g 14VW37    W84  C~1wab      
2016 01  14.16965  03 47 34.212  -30 01 07.14  23.5g 14VW37    W84  C~4yV3      
2016 11  28.27145  03 58 29.883  -29 37 13.08  22.8r 14VW37    W84  C~4yV3      
2016 11  28.27282  03 58 29.871  -29 37 13.12  23.0g 14VW37    W84  C~4yV3      
2016 12  02.23514  03 58 05.103  -29 36 53.33  22.4i 14VW37    W84  C~4yV3      
2016 12  02.23652  03 58 05.091  -29 36 53.25  22.5r 14VW37    W84  C~4yV3      
2016 12  02.23788  03 58 05.079  -29 36 53.27  22.1i 14VW37    W84  C~4yV3      
2016 12  02.23926  03 58 05.078  -29 36 53.22  23.0g 14VW37    W84  C~4yV3      
2016 12  20.25800  03 56 18.904  -29 30 55.23  22.3z 14VW37    W84  C~4yV3      
2017 01  27.13255  03 53 54.303  -28 57 26.59  23.2g 14VW37    W84  C~4yV3      
2017 02  17.07529  03 53 42.714  -28 30 52.41  22.7r 14VW37    W84  C~4yV3      
2017 02  17.07668  03 53 42.717  -28 30 52.27  22.5i 14VW37    W84  C~4yV3      
2017 02  17.07806  03 53 42.726  -28 30 52.15  23.0g 14VW37    W84  C~4yV3      
2017 11  27.316296 04 05 28.92   -28 45 54.2   23.5r 14VW37    W84  C~352R      
2017 11  27.317685 04 05 28.91   -28 45 54.4   23.2g 14VW37    W84  C~352R      
2017 12  14.240706 04 03 45.46   -28 42 55.8   22.4i 14VW37    W84  C~352R      
2017 12  14.24124  04 03 45.459  -28 42 55.79  22.4i 14VW37    W84  C~4yV3      
2018 01  04.200127 04 01 56.20   -28 30 38.2   22.6z 14VW37    W84  C~352R      
2018 01  23.094190 04 00 49.83   -28 12 34.2   22.2z 14VW37    W84  C~352R      
2018 01  23.09472  04 00 49.830  -28 12 34.17  22.1z 14VW37    W84  C~4yV3      
2018 01  23.095567 04 00 49.81   -28 12 34.1   22.6i 14VW37    W84  C~352R      
2018 01  23.09609  04 00 49.817  -28 12 34.07  22.5i 14VW37    W84  C~4yV3      
2018 02  10.101042 04 00 23.61   -27 50 58.6   22.5r 14VW37    W84  C~352R      
2018 02  10.10157  04 00 23.611  -27 50 58.60  22.5r 14VW37    W84  C~4yV3      
2018 02  10.102407 04 00 23.63   -27 50 58.5   23.5g 14VW37    W84  C~352R      
2018 02  10.10294  04 00 23.627  -27 50 58.46  23.3g 14VW37    W84  C~4yV3      
2018 11  15.34604  04 13 27.983  -27 51 20.39  21.8i 14VW37    W84  C~4yV3      
2018 11  16.33938  04 13 21.942  -27 51 37.64  22.6r 14VW37    W84  C~4yV3      
2018 11  17.27945  04 13 16.206  -27 51 52.76  23.5g 14VW37    W84  C~4yV3      
2018 11  26.31574  04 12 20.228  -27 53 20.36  22.3z 14VW37    W84  C~4yV3      

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    -0.16       0.00    -0.03
     2   0.0000      0.14    -0.02      -0.06    -0.09
     3   0.0164   -482.75     0.09      91.45    -0.06
     4   0.0164   -482.83     0.01      91.54     0.03
     5   0.0164   -482.90     0.05      91.64     0.09
     6   0.1555  -3429.95    -0.11    2492.87    -0.15
     7   0.1555  -3429.84     0.00    2492.83    -0.19
     8   0.1583  -3455.75     0.05    2564.42     0.05
     9   0.1610  -3479.26    -0.20    2633.14     0.02
    10   0.1610  -3478.99     0.06    2633.08    -0.04
    11   0.2020  -3636.24     0.12    3723.09     0.08
    12   0.2020  -3636.31     0.04    3722.99    -0.02
    13   0.2048  -3633.42    -0.01    3798.36     0.01
    14   0.2048  -3633.46    -0.04    3798.50     0.05
    15   0.2048  -3633.39     0.02    3798.49     0.04
    16   0.2048  -3633.39     0.02    3798.69     0.13
    17   0.2048  -3633.28     0.13    3798.63     0.07
    18   0.2211  -3580.61    -0.01    4247.00     0.04
    19   0.2211  -3580.64    -0.04    4247.04     0.07
    20   0.9282   8295.68    -0.05    1016.68    -0.16
    21   1.0075   5970.33    -0.06     908.32    -0.02
    22   1.0075   5970.39     0.00     908.34     0.00
    23   1.0102   5890.57    -0.08     923.83     0.16
    24   1.0102   5890.68     0.03     923.71     0.04
    25   1.0102   5890.78     0.24     923.64    -0.05
    26   1.0102   5890.71     0.17     923.71     0.02
    27   1.0457   4876.95    -0.09    1239.53    -0.13
    28   1.0457   4876.86    -0.13    1239.67    -0.01
    29   1.0457   4876.99    -0.00    1239.54    -0.13
    30   1.1713   2569.62     0.02    3758.73     0.06
    31   1.1713   2569.63     0.03    3758.68     0.00
    32   1.1713   2569.66     0.07    3758.83     0.09
    33   1.1713   2569.57    -0.00    3758.96     0.19
    34   1.1713   2569.61     0.04    3758.81     0.04
    35   1.1713   2569.54    -0.01    3758.87    -0.00
    36   1.1713   2569.55    -0.00    3758.82    -0.05
    37   2.0450  11072.30    -0.02    2100.27    -0.01
    38   2.0450  11072.13    -0.08    2100.29    -0.04
    39   2.0558  10777.51    -0.05    2235.96    -0.10
    40   2.0558  10777.39    -0.06    2236.09    -0.02
    41   2.0558  10777.24    -0.12    2236.13    -0.03
    42   2.0558  10777.24    -0.01    2236.18    -0.03
    43   2.1052   9611.35    -0.06    3070.03     0.05
    44   2.2089   8556.37     0.05    5623.92     0.03
    45   2.2662   8978.67    -0.05    7172.39    -0.05
    46   2.2662   8978.76    -0.01    7172.51    -0.04
    47   2.2662   8978.91     0.09    7172.58    -0.07
    48   3.0417  17339.98     0.12    2935.32     0.24
    49   3.0417  17339.78     0.03    2935.19     0.06
    50   3.0880  16137.95    -0.01    3612.72    -0.02
    51   3.0880  16137.94     0.01    3612.73    -0.04
    52   3.1454  15070.75    -0.24    4835.13    -0.09
    53   3.1971  14654.56     0.09    6169.62     0.03
    54   3.1971  14654.58     0.10    6169.65     0.02
    55   3.1971  14654.35    -0.11    6169.81     0.12
    56   3.1971  14654.45    -0.01    6169.80     0.07
    57   3.2464  14809.05    -0.09    7507.32     0.01
    58   3.2464  14809.07    -0.09    7507.32    -0.03
    59   3.2464  14809.34     0.17    7507.32    -0.09
    60   3.2464  14809.32     0.13    7507.37    -0.08
    61   4.0082  24513.85    -0.00    3533.08     0.08
    62   4.0109  24432.26    -0.01    3548.66    -0.04
    63   4.0135  24355.30     0.01    3564.60    -0.06
    64   4.0382  23628.28     0.02    3774.86     0.01

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.

14VW37    quality flag:3

Type:       SCATEXTD  SCATEXTD  SCATEXTD

axisobj        42.484    42.492    42.476
ecceobj         0.141     0.141     0.141
incobj         48.779    48.779    48.779
qmin           35.764    35.883    35.888
qmax           48.791    48.697    48.603
amean          42.149    42.144    42.128
amin           41.818    41.821    41.790
amax           42.502    42.501    42.501
emean           0.121     0.119     0.119
emin            0.090     0.089     0.093
emax            0.149     0.146     0.145
imean          47.339    47.353    47.348
imin           47.027    47.012    47.027
imax           47.660    47.634    47.597
excite_mean     0.745     0.745     0.745
fracstop        1.000     1.000     1.000
cjmean          2.306     2.306     2.306

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       189.3     185.7     184.0
kozaiamp        179.9     180.0     179.9