Orbit Fit and Astrometric record for 16GX367

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: 16GX367   
# Created Tue Apr  1 01:10:47 2025
# Orbit generated from Bernstein formalism
# Fitting     24 observations of     24
# Arc:  34.95d
# First observation: 2016/03/07
#  Last observation: 2016/04/11
Preliminary a, adot, b, bdot, g, gdot:
   0.000001   0.017521  -0.000003  -0.001749   0.019860   0.000000
# WARNING Fitting with energy constraint
# Chi-squared of fit:     7.48 DOF:     43 RMS:  0.10
# Min/Max residuals:    -0.25    0.23
# Exact a, adot, b, bdot, g, gdot:
  1.247115E-05  1.550255E-02 -1.790860E-06 -1.568335E-03  1.940546E-02 -6.185370E-03
# Covariance matrix:
  4.3210E-13  4.7178E-11 -8.3197E-14 -4.3693E-12  1.3251E-11  2.6372E-09
  4.7178E-11  1.5332E-07 -1.6240E-10 -1.3775E-08  3.0873E-08  2.3351E-06
 -8.3197E-14 -1.6240E-10  4.0957E-13  1.1856E-11 -3.3239E-11 -2.7845E-09
 -4.3693E-12 -1.3775E-08  1.1856E-11  1.2811E-09 -2.7726E-09 -2.0868E-07
  1.3251E-11  3.0873E-08 -3.3239E-11 -2.7726E-09  6.2741E-09  5.0308E-07
  2.6372E-09  2.3351E-06 -2.7845E-09 -2.0868E-07  5.0308E-07  5.4788E-05
#      lat0       lon0       xBary       yBary       zBary        JD0
   11.679207 -150.536243    0.666820    0.148079   -0.715656  2457455.109939
# Heliocentric elements and errors
Epoch:              2457450.5000  =  2016/03/03
Mean Anomaly:          290.38565 +/-    62.375
Argument of Peri:      229.49816 +/-    18.764
Long of Asc Node:       92.05413 +/-     0.527
Inclination:            12.84219 +/-     0.058
Eccentricity:         0.37839765 +/-    0.3802
Semi-Major Axis:     51.81904275 +/-   15.4228
Time of Perihelion: 2483797.3534 +/-   20468.1
Perihelion:          32.21083861 +/-   21.9081
Aphelion:            71.42724688 +/-   28.9826
Period (y)              373.0287 +/-    166.54
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X          -44.90596359 +/-    0.1793
Ecliptic Y          -24.60368758 +/-    0.1013
Ecliptic Z           10.43163029 +/-    0.0426
Ecliptic XDOT         0.00178077 +/-    0.0009
Ecliptic YDOT        -0.00151298 +/-    0.0005
Ecliptic ZDOT        -0.00039334 +/-    0.0002
# Distances at JD0 (AU)
Heliocenter to KBO   52.25615676 +/-    0.1616
Geocenter to KBO     51.53189302 +/-    0.2103
# Hcoef:  7.59

The following table shows the complete astrometric record for 16GX367. 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 (16GX367) followed by the observatory code and reference code for the source of the astrometry.

2016 03  07.60915  14 05 59.59   -00 20 12.3   25.4g 16GX367   T09  C~89Tb      
2016 03  07.61343  14 05 59.57   -00 20 12.2   25.6g 16GX367   T09  C~89Tb      
2016 03  07.64412  14 05 59.50   -00 20 11.7   25.6g 16GX367   T09  C~89Tb      
2016 03  16.46636  14 05 36.08   -00 16 47.7   24.0z 16GX367   T09  C~89Tb      
2016 03  16.49362  14 05 35.98   -00 16 47.0   24.9z 16GX367   T09  C~89Tb      
2016 03  16.51315  14 05 35.94   -00 16 46.5   24.3z 16GX367   T09  C~89Tb      
2016 03  16.54620  14 05 35.84   -00 16 46.0   24.9z 16GX367   T09  C~89Tb      
2016 03  16.56805  14 05 35.78   -00 16 45.4   24.2z 16GX367   T09  C~89Tb      
2016 03  16.59256  14 05 35.71   -00 16 45.0   25.0z 16GX367   T09  C~89Tb      
2016 04  08.53538  14 04 19.59   -00 07 52.2   24.4r 16GX367   T09  C~89Tb      
2016 04  08.54322  14 04 19.57   -00 07 52.2   24.7r 16GX367   T09  C~89Tb      
2016 04  08.54746  14 04 19.56   -00 07 52.2   24.7r 16GX367   T09  C~89Tb      
2016 04  08.55823  14 04 19.50   -00 07 51.8   24.7r 16GX367   T09  C~89Tb      
2016 04  08.56882  14 04 19.47   -00 07 51.8   24.6r 16GX367   T09  C~89Tb      
2016 04  08.57093  14 04 19.46   -00 07 51.8   24.9r 16GX367   T09  C~89Tb      
2016 04  11.43756  14 04 08.93   -00 06 48.7   24.3i 16GX367   T09  C~89Tb      
2016 04  11.46218  14 04 08.84   -00 06 48.0   24.4i 16GX367   T09  C~89Tb      
2016 04  11.48411  14 04 08.76   -00 06 47.5   24.2i 16GX367   T09  C~89Tb      
2016 04  11.50575  14 04 08.68   -00 06 47.0   24.5i 16GX367   T09  C~89Tb      
2016 04  11.50846  14 04 08.67   -00 06 47.0   24.5i 16GX367   T09  C~89Tb      
2016 04  11.52732  14 04 08.60   -00 06 46.7   24.5i 16GX367   T09  C~89Tb      
2016 04  11.53541  14 04 08.56   -00 06 46.5   24.9i 16GX367   T09  C~89Tb      
2016 04  11.54904  14 04 08.51   -00 06 46.2   24.2i 16GX367   T09  C~89Tb      
2016 04  11.55443  14 04 08.49   -00 06 46.0   24.1i 16GX367   T09  C~89Tb      

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     0.03       0.00     0.11
     2   0.0000     -0.32    -0.10      -0.01     0.06
     3   0.0001     -1.47     0.06       0.10    -0.09
     4   0.0242   -401.68     0.05      69.80     0.05
     5   0.0243   -403.33    -0.25      69.94     0.01
     6   0.0244   -404.07    -0.02      70.20     0.14
     7   0.0245   -405.65     0.03      70.15    -0.13
     8   0.0245   -406.70     0.07      70.40    -0.03
     9   0.0246   -407.82     0.16      70.41    -0.18
    10   0.0874  -1663.52    -0.15     174.77     0.23
    11   0.0874  -1663.80     0.04     174.67     0.12
    12   0.0874  -1663.94     0.15     174.61     0.06
    13   0.0875  -1664.92    -0.18     174.68     0.10
    14   0.0875  -1665.34     0.03     174.52    -0.07
    15   0.0875  -1665.48     0.01     174.47    -0.12
    16   0.0954  -1835.52     0.01     178.96    -0.16
    17   0.0954  -1837.03    -0.01     179.14     0.01
    18   0.0955  -1838.33     0.02     179.20     0.05
    19   0.0955  -1839.63     0.03     179.25     0.08
    20   0.0955  -1839.77     0.05     179.20     0.03
    21   0.0956  -1840.86     0.10     179.12    -0.07
    22   0.0956  -1841.49    -0.04     179.10    -0.10
    23   0.0957  -1842.30    -0.02     179.12    -0.09
    24   0.0957  -1842.65    -0.05     179.20    -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.

16GX367    quality flag:0

Type:      ERR2LARGE ERR2LARGE ERR2LARGE

axisobj         0.000     0.000     0.000
ecceobj        -1.000    -1.000    -1.000
incobj         -1.000    -1.000    -1.000
qmin            0.000     0.000     0.000
qmax            0.000     0.000     0.000
amean           0.000     0.000     0.000
amin            0.000     0.000     0.000
amax            0.000     0.000     0.000
emean           0.000     0.000     0.000
emin            0.000     0.000     0.000
emax            0.000     0.000     0.000
imean           0.000     0.000     0.000
imin            0.000     0.000     0.000
imax            0.000     0.000     0.000
excite_mean     0.000     0.000     0.000
fracstop        0.000     0.000     0.000
cjmean          0.000     0.000     0.000

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         0.0       0.0       0.0
kozaiamp          0.0       0.0       0.0