Orbit Fit and Astrometric record for 14XW40

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: 14XW40    
# Created Thu Nov 15 02:09:52 2018
# Orbit generated from Bernstein formalism
# Fitting   39 observations of   39
# Arc:   3.36y
# First observation: 2014/12/01
#  Last observation: 2018/04/10
Preliminary a, adot, b, bdot, g, gdot:
   0.000003   0.026919   0.000019   0.002018   0.025435   0.000000
# Chi-squared of fit:    35.33 DOF:   72 RMS:  0.17
# Min/Max residuals:    -0.55    0.37
# Exact a, adot, b, bdot, g, gdot:
  1.766752E-05  2.598065E-02  9.928662E-07  1.964580E-03  2.473960E-02 -5.840143E-03
# Covariance matrix:
  1.8793E-13 -1.8405E-12 -4.2322E-14 -5.6892E-14 -3.9969E-13 -3.2550E-11
 -1.8405E-12  7.7973E-11  3.2388E-12  2.4516E-12  2.3393E-11  1.3547E-09
 -4.2322E-14  3.2388E-12  1.9018E-13  7.7651E-14  1.0204E-12  5.6002E-11
 -5.6892E-14  2.4516E-12  7.7651E-14  1.4683E-13  7.3656E-13  4.2629E-11
 -3.9969E-13  2.3393E-11  1.0204E-12  7.3656E-13  7.2349E-12  4.0540E-10
 -3.2550E-11  1.3547E-09  5.6002E-11  4.2629E-11  4.0540E-10  2.3566E-08
#      lat0       lon0       xBary       yBary       zBary        JD0
  -16.037530  159.835582    0.985990    0.004500    0.015058  2456993.083978
# Heliocentric elements and errors
Epoch:              2456990.5000  =  2014/11/29
Mean Anomaly:          323.37299 +/-     0.230
Argument of Peri:      349.01134 +/-     0.637
Long of Asc Node:      234.34572 +/-     0.005
Inclination:            16.50475 +/-     0.000
Eccentricity:         0.30799706 +/-    0.0057
Semi-Major Axis:     50.35385493 +/-    0.1687
Time of Perihelion: 2470268.9214 +/-      50.0
Perihelion:          34.84501586 +/-    0.3104
Aphelion:            65.86269400 +/-    0.3625
Period (y)              357.3200 +/-      1.80
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X          -36.11512148 +/-    0.0040
Ecliptic Y           14.31194137 +/-    0.0014
Ecliptic Z          -11.16698612 +/-    0.0012
Ecliptic XDOT        -0.00046860 +/-    0.0000
Ecliptic YDOT        -0.00289744 +/-    0.0000
Ecliptic ZDOT         0.00038761 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   40.42072790 +/-    0.0036
Geocenter to KBO     40.42102602 +/-    0.0044
# Hcoef:  6.27

The following table shows the complete astrometric record for 14XW40. 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 (14XW40) followed by the observatory code and reference code for the source of the astrometry.

2014 12  01.58320  10 21 25.841  -06 59 22.04  22.2w 14XW40    F51  C~1vXx      
2014 12  01.59510  10 21 25.861  -06 59 22.47  22.3w 14XW40    F51  C~1vXx      
2014 12  01.60775  10 21 25.854  -06 59 22.92  22.2w 14XW40    F51  C~1vXx      
2014 12  01.62143  10 21 25.876  -06 59 23.32  22.4w 14XW40    F51  C~1vXx      
2014 12  01.63438  10 21 25.868  -06 59 23.57  22.6w 14XW40    F51  C~1vXx      
2014 12  01.64628  10 21 25.865  -06 59 23.98  22.6w 14XW40    F51  C~1vXx      
2015 01  20.49294  10 19 51.316  -07 08 38.94  22.4w 14XW40    F51  C~1vXx      
2015 01  20.50612  10 19 51.272  -07 08 38.94  22.5w 14XW40    F51  C~1vXx      
2015 01  20.51925  10 19 51.232  -07 08 38.85  22.6w 14XW40    F51  C~1vXx      
2015 01  20.53241  10 19 51.169  -07 08 38.78  22.4w 14XW40    F51  C~1vXx      
2015 01  26.45070  10 19 27.753  -07 07 48.60  22.3w 14XW40    F51  C~1vXx      
2015 01  26.46209  10 19 27.702  -07 07 48.54  22.2w 14XW40    F51  C~1vXx      
2015 01  26.47344  10 19 27.657  -07 07 48.21  22.1w 14XW40    F51  C~1vXx      
2015 01  26.48481  10 19 27.606  -07 07 48.19  22.5w 14XW40    F51  C~1vXx      
2015 02  17.15939  10 17 50.41   -07 01 29.3   23.3g 14XW40    W84  C~2iOT      
2015 02  17.24529  10 17 50.01   -07 01 27.3   23.2g 14XW40    W84  C~2iOT      
2015 02  17.31416  10 17 49.67   -07 01 25.6   23.6g 14XW40    W84  C~2iOT      
2015 02  17.36113  10 17 49.45   -07 01 24.6   23.7g 14XW40    W84  C~2iOT      
2015 02  20.42149  10 17 34.938  -07 00 08.92  22.2w 14XW40    F51  C~1vXx      
2015 02  20.43447  10 17 34.882  -07 00 08.34  22.0w 14XW40    F51  C~1vXx      
2015 02  20.44716  10 17 34.817  -07 00 08.19  22.3w 14XW40    F51  C~1vXx      
2015 02  20.45984  10 17 34.750  -07 00 07.82  22.2w 14XW40    F51  C~1vXx      
2015 02  22.07772  10 17 27.07   -06 59 26.0         14XW40    W84  C~2iOT      
2015 02  22.21347  10 17 26.45   -06 59 22.0         14XW40    W84  C~2iOT      
2015 02  22.28233  10 17 26.11   -06 59 20.3         14XW40    W84  C~2iOT      
2015 02  22.39578  10 17 25.592  -06 59 17.36  22.1w 14XW40    F51  C~1vXx      
2015 02  22.40870  10 17 25.492  -06 59 17.42  22.0w 14XW40    F51  C~1vXx      
2015 02  22.42194  10 17 25.439  -06 59 16.95  22.0w 14XW40    F51  C~1vXx      
2015 02  22.43491  10 17 25.390  -06 59 16.36  22.1w 14XW40    F51  C~1vXx      
2015 02  24.12978  10 17 17.37   -06 58 30.5         14XW40    W84  C~2iOT      
2015 02  24.19143  10 17 17.06   -06 58 28.9         14XW40    W84  C~2iOT      
2015 02  27.12117  10 17 03.20   -06 57 06.6         14XW40    W84  C~2iOT      
2015 02  27.18962  10 17 02.86   -06 57 04.6         14XW40    W84  C~2iOT      
2015 03  20.34669  10 15 28.098  -06 45 41.29  22.2w 14XW40    F51  C~1vXx      
2015 03  20.35939  10 15 28.059  -06 45 41.08  22.1w 14XW40    F51  C~1vXx      
2015 03  20.37208  10 15 28.000  -06 45 40.55  22.1w 14XW40    F51  C~1vXx      
2015 03  20.41946  10 15 27.801  -06 45 38.78  22.2w 14XW40    F51  C~1vXx      
2018 04  10.15781  10 32 02.318  -07 58 06.93  22.1R 14XW40    G37              
2018 04  10.20545  10 32 02.143  -07 58 05.16        14XW40    G37              

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    -0.22       0.00     0.05
  2   0.0000      0.44     0.05      -0.29     0.05
  3   0.0001      0.51    -0.05      -0.74    -0.10
  4   0.0001      0.96     0.21      -0.99    -0.02
  5   0.0001      0.95     0.02      -1.27     0.01
  6   0.0002      1.06    -0.03      -1.66    -0.10
  7   0.1366  -1093.82    -0.26   -1045.81     0.21
  8   0.1367  -1094.42    -0.13   -1046.06     0.17
  9   0.1367  -1095.01     0.02   -1046.20     0.24
 10   0.1368  -1095.90    -0.14   -1046.49     0.16
 11   0.1530  -1437.64     0.08   -1131.44     0.18
 12   0.1530  -1438.36     0.05   -1131.67     0.10
 13   0.1530  -1439.11     0.01   -1131.62     0.31
 14   0.1531  -1439.82     0.00   -1131.88     0.20
 15   0.2124  -2922.82     0.17   -1327.38    -0.00
 16   0.2126  -2929.09     0.37   -1327.78     0.02
 17   0.2128  -2934.42     0.22   -1328.12     0.02
 18   0.2129  -2937.83     0.34   -1328.43    -0.08
 19   0.2213  -3166.51    -0.06   -1340.05    -0.19
 20   0.2214  -3167.51    -0.06   -1339.83     0.08
 21   0.2214  -3168.46    -0.04   -1340.06    -0.11
 22   0.2214  -3169.52    -0.14   -1340.09    -0.10
 23   0.2259  -3291.22    -0.17   -1344.62    -0.55
 24   0.2262  -3301.28     0.14   -1344.41     0.04
 25   0.2264  -3306.61     0.08   -1344.75    -0.12
 26   0.2267  -3314.87     0.17   -1344.95     0.05
 27   0.2268  -3316.22    -0.19   -1345.56    -0.53
 28   0.2268  -3317.13    -0.09   -1345.43    -0.36
 29   0.2268  -3318.03     0.01   -1345.16    -0.05
 30   0.2315  -3445.95     0.19   -1347.87     0.03
 31   0.2316  -3450.83     0.04   -1348.14    -0.12
 32   0.2397  -3673.06    -0.17   -1350.03     0.04
 33   0.2399  -3678.51    -0.34   -1350.09     0.01
 34   0.2978  -5244.20    -0.17   -1252.22     0.16
 35   0.2978  -5244.81     0.12   -1252.25     0.03
 36   0.2978  -5245.83     0.01   -1252.09     0.07
 37   0.2980  -5249.25    -0.03   -1251.57     0.17
 38   3.3554  10105.40     0.13     265.47     0.07
 39   3.3556  10102.32    -0.13     266.15    -0.04

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.

14XW40    quality flag:3

Type:       SCATNEAR  SCATNEAR  SCATNEAR

axisobj        49.843    50.240    49.488
ecceobj         0.302     0.317     0.287
incobj         16.500    16.501    16.499
qmin           33.196    32.547    33.978
qmax           67.913    68.940    66.476
amean          50.035    50.306    49.793
amin           49.441    49.475    49.210
amax           50.879    51.163    50.436
emean           0.308     0.329     0.297
emin            0.286     0.308     0.277
emax            0.337     0.351     0.318
imean          17.440    16.772    17.207
imin           16.061    15.362    16.308
imax           18.446    18.077    18.180
excite_mean     0.430     0.438     0.420
fracstop        1.000     1.000     1.000
cjmean          2.941     2.936     2.950

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       167.4     174.2     171.1
kozaiamp        180.0     179.9     180.0