Orbit Fit and Astrometric record for 01UC17

The following information shows the result of the orbit fit based on Gary Bernstein's method. Most of the information should be self-explanatory.

# Object: 01UC17    
# Created Fri May  2 02:36:35 2008
# Orbit generated from Bernstein formalism
# Fitting    8 observations of    8
# Arc:   1.10d
# First observation: 2001/10/17
#  Last observation: 2001/10/18
# WARNING Fitting with energy constraint
# WARNING and with gdot fixed = 0
# Chi-squared of fit:    10.76 DOF:   12 RMS:  0.21
# Min/Max residuals:    -0.43    0.33
# Exact a, adot, b, bdot, g, gdot:
  1.723740E-05  3.259990E-02 -9.022104E-07 -7.598581E-04  2.996900E-02  0.000000E+00
# Covariance matrix:
  4.2735E-11  7.9123E-08 -7.9023E-14 -8.6212E-11  1.2605E-08  0.0000E+00
  7.9123E-08  1.4932E-04 -1.4862E-10 -1.6206E-07  2.3700E-05  0.0000E+00
 -7.9023E-14 -1.4862E-10  5.3482E-13 -2.2099E-10 -2.3609E-11  0.0000E+00
 -8.6212E-11 -1.6206E-07 -2.2099E-10  1.3950E-07 -2.5748E-08  0.0000E+00
  1.2605E-08  2.3700E-05 -2.3609E-11 -2.5748E-08  3.7651E-06  0.0000E+00
  0.0000E+00  0.0000E+00  0.0000E+00  0.0000E+00  0.0000E+00  3.5419E-04
#      lat0       lon0       xBary       yBary       zBary        JD0
   -2.643504   23.810027    0.003837   -0.045841   -0.991330  2452199.663483
# Heliocentric elements and errors
Epoch:              2452190.5000  =  2001/10/08
Mean Anomaly:          355.68462 +/-   232.153
Argument of Peri:      247.09563 +/-   299.015
Long of Asc Node:      141.31703 +/-    14.229
Inclination:             2.89356 +/-     0.377
Eccentricity:         0.03348634 +/-    0.5749
Semi-Major Axis:     35.55034081 +/-   18.9059
Time of Perihelion: 2453118.5706 +/-  204769.5
Perihelion:          34.35989003 +/-   27.4165
Aphelion:            36.74079160 +/-   28.2761
Period (y)              211.9697 +/-    169.09
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X           31.40679339 +/-    1.9745
Ecliptic Y           13.85965900 +/-    0.8711
Ecliptic Z           -1.53902978 +/-    0.0996
Ecliptic XDOT        -0.00121392 +/-    0.0016
Ecliptic YDOT         0.00272404 +/-    0.0011
Ecliptic ZDOT        -0.00006913 +/-    0.0001
# Distances at JD0 (AU)
Heliocenter to KBO   34.36343160 +/-    1.8385
Geocenter to KBO     33.36781305 +/-    2.1605
# Hcoef:  7.70

The following table shows the complete astrometric record for 01UC17. 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 (01UC17) followed by the observatory code and reference code for the source of the astrometry.

2001 10  17.16274  01 32 05.23   +06 46 56.5         01UC17    809  Cd9575      
2001 10  17.27628  01 32 04.60   +06 46 52.6         01UC17    809  Cd9575      
2001 10  18.07605  01 32 00.21   +06 46 26.6         01UC17    809  Cd9575      
2001 10  18.07605  01 32 00.22   +06 46 26.4   22.9R 01UC17    I03  Ck3831      
2001 10  18.18551  01 31 59.57   +06 46 22.9   22.5R 01UC17    809  Cd9575      
2001 10  18.18551  01 31 59.61   +06 46 23.4   22.3R 01UC17    I03  Ck3831      
2001 10  18.25983  01 31 59.17   +06 46 20.3         01UC17    809  Cd9575      
2001 10  18.25983  01 31 59.20   +06 46 20.8   22.8R 01UC17    I03  Ck3831      

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    -0.01       0.00     0.10
  2   0.0003    -10.16     0.01      -0.19    -0.10
  3   0.0025    -80.53     0.00      -0.41     0.02
  4   0.0025    -80.46     0.06      -0.66    -0.22
  5   0.0028    -90.75    -0.43      -0.36     0.04
  6   0.0028    -90.02     0.31      -0.12     0.29
  7   0.0030    -97.25    -0.27      -0.60    -0.21
  8   0.0030    -96.65     0.33      -0.30     0.09

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.

01UC17    quality flag:3

Type:      CLASSICAL CLASSICAL CLASSICAL

axisobj       40.579    40.579    40.579
ecceobj        0.165     0.165     0.165
incobj         2.847     2.847     2.847
qmin          33.330    32.922    32.857
qmax          48.093    48.778    51.529
amean         40.264    40.393    41.254
amin          39.449    39.480    39.699
amax          40.916    41.311    42.427
emean          0.148     0.146     0.180
emin           0.119     0.107     0.140
emax           0.175     0.184     0.215
imean          1.686     2.046     1.422
imin           0.052     0.117     0.000
imax           2.870     3.561     2.905
fracstop       1.000     1.000     1.000
cjmean         3.034     3.036     3.032

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      179.4     172.7     189.5
kozaiamp       180.0     180.0     180.0