Orbit Fit and Astrometric record for 07TB434

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: 07TB434   
# Created Sat Apr 27 01:13:02 2024
# Orbit generated from Bernstein formalism
# Fitting      4 observations of      4
# Arc:   1.17d
# First observation: 2007/10/14
#  Last observation: 2007/10/15
# WARNING Fitting with energy constraint
# WARNING and with gdot fixed = 0
# WARNING MRQMIN stopped after  13 iterations -- oscilliatory solution
# Chi-squared of fit:    12.79 DOF:      4 RMS:  0.32
# Min/Max residuals:    -0.59    0.60
# Exact a, adot, b, bdot, g, gdot:
  3.688368E-05  2.874825E-01  4.912739E-06  4.954939E-02  1.335180E-01  0.000000E+00
# Covariance matrix:
  4.8373E-09  4.0220E-05 -3.3271E-11  4.6248E-09  6.4505E-06  0.0000E+00
  4.0220E-05  3.3445E-01 -2.7666E-07  3.8458E-05  5.3639E-02  0.0000E+00
 -3.3271E-11 -2.7666E-07  7.3535E-13 -2.0270E-10 -4.4371E-08  0.0000E+00
  4.6248E-09  3.8458E-05 -2.0270E-10  2.1428E-07  6.1678E-06  0.0000E+00
  6.4505E-06  5.3639E-02 -4.4371E-08  6.1678E-06  8.6026E-03  0.0000E+00
  0.0000E+00  0.0000E+00  0.0000E+00  0.0000E+00  0.0000E+00  3.1321E-02
#      lat0       lon0       xBary       yBary       zBary        JD0
    0.266421   13.198533   -0.130140    0.004672   -0.991417  2454387.770714
# Heliocentric elements and errors
Epoch:              2454380.5000  =  2007/10/07
Mean Anomaly:           31.09730 +/-    47.185
Argument of Peri:      328.22278 +/-   136.691
Long of Asc Node:       12.68174 +/-     2.115
Inclination:             9.78289 +/-    19.291
Eccentricity:         0.02903607 +/-    1.6868
Semi-Major Axis:      8.69367962 +/-   12.0679
Time of Perihelion: 2462934.4915 +/-   57379.0
Perihelion:           8.44124931 +/-   18.7710
Aphelion:             8.94610993 +/-   19.2163
Period (y)               25.6338 +/-     53.37
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X            8.22651405 +/-    5.0654
Ecliptic Y            2.05852090 +/-    1.1876
Ecliptic Z            0.03487983 +/-    0.0242
Ecliptic XDOT        -0.00134428 +/-    0.0040
Ecliptic YDOT         0.00573689 +/-    0.0076
Ecliptic ZDOT         0.00101592 +/-    0.0007
# Distances at JD0 (AU)
Heliocenter to KBO    8.48022749 +/-    4.9223
Geocenter to KBO      7.48962439 +/-    5.2028
# Hcoef: 14.75

The following table shows the complete astrometric record for 07TB434. 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 (07TB434) followed by the observatory code and reference code for the source of the astrometry.

2007 10  14.26996  00 48 09.37   +05 27 23.0   23.5R 07TB434   568  Cz4329      
2007 10  14.33345  00 48 08.14   +05 27 17.1         07TB434   568  Cz4329      
2007 10  14.39537  00 48 06.93   +05 27 11.3         07TB434   568  Cz4329      
2007 10  15.44444  00 47 46.23   +05 25 32.6         07TB434   568  Cz4329      

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    -0.59       0.00     0.20
     2   0.0002    -19.21     0.06       1.71    -0.01
     3   0.0003    -38.12     0.60       3.40    -0.21
     4   0.0032   -361.26    -0.06      32.75     0.02

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.

07TB434    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