Orbit Fit and Astrometric record for 03QW111

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: 03QW111   
# Created Fri May  2 02:36:52 2008
# Orbit generated from Bernstein formalism
# Fitting   20 observations of   22
# Arc:   4.13y
# First observation: 2003/08/25
#  Last observation: 2007/10/11
Preliminary a, adot, b, bdot, g, gdot:
  -0.000095   0.020986  -0.000001  -0.000028   0.022616   0.000000
# Chi-squared of fit:    31.85 DOF:   34 RMS:  0.22
# Min/Max residuals:    -0.40    0.43
# Exact a, adot, b, bdot, g, gdot:
  1.415379E-05  2.083145E-02 -1.379190E-06 -2.739721E-05  2.271071E-02 -2.241601E-03
# Covariance matrix:
  3.7760E-13 -4.0506E-13 -4.8337E-16 -1.0200E-16  5.3969E-15 -4.0984E-12
 -4.0506E-13  7.7856E-13  5.8854E-16  2.7451E-16  3.8468E-14  9.2323E-12
 -4.8337E-16  5.8854E-16  2.2896E-13 -7.5140E-14 -2.4293E-15  6.7859E-15
 -1.0200E-16  2.7451E-16 -7.5140E-14  3.6236E-14  2.3605E-16  3.4622E-15
  5.3969E-15  3.8468E-14 -2.4293E-15  2.3605E-16  2.5146E-13  5.3256E-13
 -4.0984E-12  9.2323E-12  6.7859E-15  3.4622E-15  5.3256E-13  1.1483E-10
#      lat0       lon0       xBary       yBary       zBary        JD0
   -2.726519  -22.951617    0.098491   -0.048008   -1.009225  2452876.734503
# Heliocentric elements and errors
Epoch:              2452870.5000  =  2003/08/19
Mean Anomaly:          258.99252 +/-     0.078
Argument of Peri:       21.96237 +/-     0.070
Long of Asc Node:       68.50677 +/-     0.011
Inclination:             2.66672 +/-     0.000
Eccentricity:         0.11560375 +/-    0.0005
Semi-Major Axis:     43.53981395 +/-    0.0040
Time of Perihelion: 2482313.3142 +/-      22.4
Perihelion:          38.50644799 +/-    0.0211
Aphelion:            48.57317990 +/-    0.0213
Period (y)              287.3016 +/-      0.04
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X           41.38975038 +/-    0.0009
Ecliptic Y          -17.63152886 +/-    0.0004
Ecliptic Z           -2.09462672 +/-    0.0001
Ecliptic XDOT         0.00072534 +/-    0.0000
Ecliptic YDOT         0.00241209 +/-    0.0000
Ecliptic ZDOT         0.00000973 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   45.03742563 +/-    0.0008
Geocenter to KBO     44.03207927 +/-    0.0010
# Hcoef:  6.37

The following table shows the complete astrometric record for 03QW111. 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 (03QW111) followed by the observatory code and reference code for the source of the astrometry.

2003 08  25.23376  22 39 11.59   -11 27 14.7   21.6R 03QW111   807  Ci4592      
2003 08  25.33868  22 39 11.12   -11 27 17.5         03QW111   807  Ci4592      
2003 09  03.06904  22 38 33.66   -11 30 58.5   22.7R 03QW111   304  Ci4592      
2003 09  03.29799  22 38 32.63   -11 31 03.9         03QW111   304  Ci4592      
2003 10  23.06714  22 35 33.90   -11 47 04.7   23.0R 03QW111   304  Ci9432      
2003 10  23.09793  22 35 33.83   -11 47 04.8         03QW111   304  Ci9432      
2004 07  16.33143  22 46 05.21   -10 45 03.4   22.1R 03QW111   807  Co3932      
2004 07  16.38293  22 46 05.05   -10 45 04.6         03QW111   807  Co3932      
2004 10  12.13108  22 40 30.33   -11 18 31.2   22.8R 03QW111   695  Cr8411      
2004 10  12.23634  22 40 29.99   -11 18 32.6         03QW111   695  Cr8411      
2005 08  08.10293  22 49 20.74   -10 26 12.5   21.8R 03QW111   807  Co3932      
2005 08  08.21996  22 49 20.27   -10 26 15.6         03QW111   807  Co3932      
2005 08  09.10840  22 49 16.90   -10 26 37.6         03QW111   807  Co3932      
2006 07  25.37402  22 54 39.928  -09 53 15.38  22.9R 03QW111   500              
2006 07  25.37842  22 54 39.912  -09 53 15.50        03QW111   500              
2006 07  25.38722  22 54 39.885  -09 53 15.69        03QW111   500              
2006 07  28.33854  22 54 30.57   -09 54 19.5   22.8R 03QW111   304  Cr5531      
2006 07  28.39394  22 54 30.38   -09 54 20.5         03QW111   304  Cr5531      
2007 09  12.35681  22 56 00.48   -09 45 40.5   22.7r 03QW111   695  Cv8576      
2007 09  12.40050  22 56 00.31   -09 45 41.2   23.0r 03QW111   695  Cv8576      
2007 10  11.13460  22 54 08.03   -09 56 21.2   23.0R 03QW111   688  Cw0394      
2007 10  11.21226  22 54 07.76   -09 56 22.7         03QW111   688  Cw0394      

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     0.07       0.00     0.28
  2   0.0003     -7.46    -0.19      -0.01     0.25
  3   0.0242   -600.80 (   0.05)      0.63 (   1.34)
  4   0.0248   -616.86 (  -0.24)      1.27 (   1.84)
  5   0.1611  -3411.85    -0.02      86.18    -0.09
  6   0.1612  -3412.84     0.11      86.46     0.09
  7   0.8928   6595.42     0.29      53.27     0.15
  8   0.8929   6592.78    -0.01      53.05     0.05
  9   1.1332   1269.66    -0.07      52.12    -0.06
 10   1.1335   1264.50    -0.13      52.69     0.20
 11   1.9545   9696.73     0.19       2.73    -0.16
 12   1.9548   9689.12    -0.14       2.51    -0.24
 13   1.9572   9634.65     0.08       1.14    -0.40
 14   2.9162  14825.63    -0.23      21.80    -0.38
 15   2.9162  14825.36    -0.27      21.78    -0.39
 16   2.9162  14824.92    -0.27      21.76    -0.39
 17   2.9243  14672.54     0.20      15.89    -0.20
 18   2.9245  14669.55     0.19      16.05     0.05
 19   4.0496  16106.68    -0.13     -17.92     0.16
 20   4.0497  16104.08     0.29     -17.59     0.43
 21   4.1284  14316.57     0.07      31.85     0.35
 22   4.1286  14312.29    -0.03      32.00     0.28

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.

03QW111    quality flag:3

Type:         7:4EEE    7:4EEE    7:4EEE

axisobj       43.943    43.943    43.943
ecceobj        0.114     0.114     0.114
incobj         2.667     2.667     2.667
qmin          38.234    38.234    38.234
qmax          49.550    49.551    49.553
amean         43.727    43.727    43.727
amin          43.333    43.339    43.327
amax          44.176    44.148    44.172
emean          0.110     0.110     0.110
emin           0.097     0.097     0.097
emax           0.122     0.122     0.122
imean          1.136     1.134     1.137
imin           0.241     0.241     0.240
imax           1.887     1.888     1.886
fracstop       1.000     1.000     1.000
cjmean         3.083     3.083     3.083

libcent 0      179.4     178.6     179.3
libamp  0      108.1     106.5     108.4
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      139.0     146.2     136.7
kozaiamp       180.0     180.0     179.9