TARGET:          2235 Vittore
SESSION NUMBER:  511
DATE/TIME:       2009/12/01 @ 09:14
OBSERVER:        J.W. Brinsfield
CONTACT INFO:    J.W. Brinsfield 5180 Via Capote, Thousand Oals, Ca, USA [jbrinsfi@viacapotesky.com]
FILTER:          C
TELESCOPE:       0.35m SCT
FOCAL LENGTH:    135.08
CAMERA:          Alta U6 1 X binning
TEMP (C):        -30
EXPOSURE (s):    180
APPROX. RA:      05:46
APPROX. DEC:     + 0
EXPOSURE JD:     Mid-exposure
JD CORR METHOD:  Light-time
JD CORRECTION:   JD = JD(raw) - 0.00998d
UNITY CORR:      -5 * log(SunDist * EarthDist): -3.2921
NOTE: The unity correction is NOT included in the output magnitudes
MAG. METHOD:     Instrumental
 
NOTE:            For multiple sessions, differential magnitudes include
                 adjustments ADDED to the Obj-CAvg value to compensate
                 for changing phase angle, distance, and refinements to
                 the base average value of the comparison stars.       
                                                                       
                 The phase angle calculations include the effects of   
                 the phase parameter, G. This value is taken from the  
                 MPCORB value at the time the calculations were made.
BASE COMP VALUE: -8.671
BASE CORRECTION: +0.000
PHASE/DIST CORR: +0.000
PHASE SLOPE:     0.15
P/D ADJUST (-/DAY):-0.014
P/D ADJUST (+/DAY):+0.014
THE P/D ADJUSTMENTS ARE INCLUDED IN THE VALUES BELOW.
 
ERROR CALC:      The magnitude error is calculated by the following:
                 Err = sqrt(sqr(ERR[target]) + sqr(Err[Comps]))
                       where Err[Target] = 1.0857/SNR[target]
                             Err[Comps]  = sqrt(sqr(1.0857/SNR[Comp1])... + sqr(1.0857/SNR[CompN])) / N
                 The factor of 1.0857 converts flux to magnitudes (Howell)
Comp1: 054620.18 -03511.3            0.000 R  Y
Comp2: 054624.22 -03602.1            0.000 R  Y
Comp3: 054602.17 -03847.4            0.000 R  Y
Comp4: 054554.89 -03722.8            0.000 R  Y
Comp5: 054608.60 -03857.2            0.000 R  N
*********************************************************************************************
TARGET:          2235 Vittore
SESSION NUMBER:  516
DATE/TIME:       2009/12/15 @ 08:29
OBSERVER:        J.W. Brinsfield
CONTACT INFO:    J.W. Brinsfield 5180 Via Capote, Thousand Oals, Ca, USA [jbrinsfi@viacapotesky.com]
FILTER:          C
TELESCOPE:       0.35m SCT
FOCAL LENGTH:    135.10
CAMERA:          Alta U6 1 X binning
TEMP (C):        -30
EXPOSURE (s):    180
APPROX. RA:      05:35
APPROX. DEC:     - 2
EXPOSURE JD:     Mid-exposure
JD CORR METHOD:  Light-time
JD CORRECTION:   JD = JD(raw) - 0.00977d
UNITY CORR:      -5 * log(SunDist * EarthDist): -3.2323
NOTE: The unity correction is NOT included in the output magnitudes
MAG. METHOD:     Instrumental
 
NOTE:            For multiple sessions, differential magnitudes include
                 adjustments ADDED to the Obj-CAvg value to compensate
                 for changing phase angle, distance, and refinements to
                 the base average value of the comparison stars.       
                                                                       
                 The phase angle calculations include the effects of   
                 the phase parameter, G. This value is taken from the  
                 MPCORB value at the time the calculations were made.
BASE COMP VALUE: -9.150
BASE CORRECTION: -0.479
PHASE/DIST CORR: -0.109
PHASE SLOPE:     0.15
P/D ADJUST (-/DAY):-0.001
P/D ADJUST (+/DAY):-0.001
THE P/D ADJUSTMENTS ARE INCLUDED IN THE VALUES BELOW.
 
ERROR CALC:      The magnitude error is calculated by the following:
                 Err = sqrt(sqr(ERR[target]) + sqr(Err[Comps]))
                       where Err[Target] = 1.0857/SNR[target]
                             Err[Comps]  = sqrt(sqr(1.0857/SNR[Comp1])... + sqr(1.0857/SNR[CompN])) / N
                 The factor of 1.0857 converts flux to magnitudes (Howell)
Comp1: 053508.65 -20712.0            0.000 R  Y
Comp2: 053527.68 -20851.0            0.000 R  Y
Comp3: 053456.03 -20424.2            0.000 R  Y
Comp4: 053516.60 -21216.4            0.000 R  Y
Comp5: 053451.04 -20811.2            0.000 R  Y
*********************************************************************************************
TARGET:          2235 Vittore
SESSION NUMBER:  517
DATE/TIME:       2009/12/16 @ 09:32
OBSERVER:        J.W. Brinsfield
CONTACT INFO:    J.W. Brinsfield 5180 Via Capote, Thousand Oals, Ca, USA [jbrinsfi@viacapotesky.com]
FILTER:          C
TELESCOPE:       0.35m SCT
FOCAL LENGTH:    134.97
CAMERA:          Alta U6 1 X binning
TEMP (C):        -30
EXPOSURE (s):    180
APPROX. RA:      05:34
APPROX. DEC:     - 2
EXPOSURE JD:     Mid-exposure
JD CORR METHOD:  Light-time
JD CORRECTION:   JD = JD(raw) - 0.00977d
UNITY CORR:      -5 * log(SunDist * EarthDist): -3.2294
NOTE: The unity correction is NOT included in the output magnitudes
MAG. METHOD:     Instrumental
 
NOTE:            For multiple sessions, differential magnitudes include
                 adjustments ADDED to the Obj-CAvg value to compensate
                 for changing phase angle, distance, and refinements to
                 the base average value of the comparison stars.       
                                                                       
                 The phase angle calculations include the effects of   
                 the phase parameter, G. This value is taken from the  
                 MPCORB value at the time the calculations were made.
BASE COMP VALUE: -8.864
BASE CORRECTION: -0.193
PHASE/DIST CORR: -0.109
PHASE SLOPE:     0.15
P/D ADJUST (-/DAY):-0.001
P/D ADJUST (+/DAY):-0.001
THE P/D ADJUSTMENTS ARE INCLUDED IN THE VALUES BELOW.
 
ERROR CALC:      The magnitude error is calculated by the following:
                 Err = sqrt(sqr(ERR[target]) + sqr(Err[Comps]))
                       where Err[Target] = 1.0857/SNR[target]
                             Err[Comps]  = sqrt(sqr(1.0857/SNR[Comp1])... + sqr(1.0857/SNR[CompN])) / N
                 The factor of 1.0857 converts flux to magnitudes (Howell)
Comp1: 053451.03 -20811.2            0.000 R  Y
Comp2: 053428.44 -20909.9            0.000 R  N
Comp3: 053440.57 -20937.0            0.000 R  Y
Comp4: 053454.90 -21332.1            0.000 R  Y
Comp5: 053433.26 -21603.8            0.000 R  Y
*********************************************************************************************
TARGET:          2235 Vittore
SESSION NUMBER:  519
DATE/TIME:       2009/12/17 @ 08:30
OBSERVER:        J.W. Brinsfield
CONTACT INFO:    J.W. Brinsfield 5180 Via Capote, Thousand Oals, Ca, USA [jbrinsfi@viacapotesky.com]
FILTER:          C
TELESCOPE:       0.35m SCT
FOCAL LENGTH:    134.73
CAMERA:          Alta U6 1 X binning
TEMP (C):        -30
EXPOSURE (s):    180
APPROX. RA:      05:33
APPROX. DEC:     - 2
EXPOSURE JD:     Mid-exposure
JD CORR METHOD:  Light-time
JD CORRECTION:   JD = JD(raw) - 0.00977d
UNITY CORR:      -5 * log(SunDist * EarthDist): -3.2285
NOTE: The unity correction is NOT included in the output magnitudes
MAG. METHOD:     Instrumental
 
NOTE:            For multiple sessions, differential magnitudes include
                 adjustments ADDED to the Obj-CAvg value to compensate
                 for changing phase angle, distance, and refinements to
                 the base average value of the comparison stars.       
                                                                       
                 The phase angle calculations include the effects of   
                 the phase parameter, G. This value is taken from the  
                 MPCORB value at the time the calculations were made.
BASE COMP VALUE: -8.964
BASE CORRECTION: -0.293
PHASE/DIST CORR: -0.108
PHASE SLOPE:     0.15
P/D ADJUST (-/DAY):+0.002
P/D ADJUST (+/DAY):-0.002
THE P/D ADJUSTMENTS ARE INCLUDED IN THE VALUES BELOW.
 
ERROR CALC:      The magnitude error is calculated by the following:
                 Err = sqrt(sqr(ERR[target]) + sqr(Err[Comps]))
                       where Err[Target] = 1.0857/SNR[target]
                             Err[Comps]  = sqrt(sqr(1.0857/SNR[Comp1])... + sqr(1.0857/SNR[CompN])) / N
                 The factor of 1.0857 converts flux to magnitudes (Howell)
Comp1: 053343.49 -21243.9            0.000 R  Y
Comp2: 053328.02 -21213.0            0.000 R  Y
Comp3: 053352.87 -21416.8            0.000 R  Y
Comp4: 053340.80 -21532.0            0.000 R  Y
Comp5: 053415.76 -21243.1            0.000 R  Y
*********************************************************************************************
TARGET:          2235 Vittore
SESSION NUMBER:  521
DATE/TIME:       2009/12/18 @ 08:28
OBSERVER:        J.W. Brinsfield
CONTACT INFO:    J.W. Brinsfield 5180 Via Capote, Thousand Oals, Ca, USA [jbrinsfi@viacapotesky.com]
FILTER:          C
TELESCOPE:       0.35m SCT
FOCAL LENGTH:    135.34
CAMERA:          Alta U6 1 X binning
TEMP (C):        -28
EXPOSURE (s):    180
APPROX. RA:      05:32
APPROX. DEC:     - 2
EXPOSURE JD:     Mid-exposure
JD CORR METHOD:  Light-time
JD CORRECTION:   JD = JD(raw) - 0.00977d
UNITY CORR:      -5 * log(SunDist * EarthDist): -3.2277
NOTE: The unity correction is NOT included in the output magnitudes
MAG. METHOD:     Instrumental
 
NOTE:            For multiple sessions, differential magnitudes include
                 adjustments ADDED to the Obj-CAvg value to compensate
                 for changing phase angle, distance, and refinements to
                 the base average value of the comparison stars.       
                                                                       
                 The phase angle calculations include the effects of   
                 the phase parameter, G. This value is taken from the  
                 MPCORB value at the time the calculations were made.
BASE COMP VALUE: -8.905
BASE CORRECTION: -0.234
PHASE/DIST CORR: -0.106
PHASE SLOPE:     0.15
P/D ADJUST (-/DAY):+0.002
P/D ADJUST (+/DAY):-0.002
THE P/D ADJUSTMENTS ARE INCLUDED IN THE VALUES BELOW.
 
ERROR CALC:      The magnitude error is calculated by the following:
                 Err = sqrt(sqr(ERR[target]) + sqr(Err[Comps]))
                       where Err[Target] = 1.0857/SNR[target]
                             Err[Comps]  = sqrt(sqr(1.0857/SNR[Comp1])... + sqr(1.0857/SNR[CompN])) / N
                 The factor of 1.0857 converts flux to magnitudes (Howell)
Comp1: 053253.44 -21614.9            0.000 R  Y
Comp2: 053254.04 -21837.5            0.000 R  Y
Comp3: 053302.93 -21604.2            0.000 R  Y
Comp4: 053305.85 -21530.9            0.000 R  Y
Comp5: 053307.61 -22327.9            0.000 R  Y
*********************************************************************************************
TARGET:          2235 Vittore
SESSION NUMBER:  523
DATE/TIME:       2009/12/19 @ 08:26
OBSERVER:        J.W. Brinsfield
CONTACT INFO:    J.W. Brinsfield 5180 Via Capote, Thousand Oals, Ca, USA [jbrinsfi@viacapotesky.com]
FILTER:          C
TELESCOPE:       0.35m SCT
FOCAL LENGTH:    135.00
CAMERA:          Alta U6 1 X binning
TEMP (C):        -25
EXPOSURE (s):    180
APPROX. RA:      05:32
APPROX. DEC:     - 2
EXPOSURE JD:     Mid-exposure
JD CORR METHOD:  Light-time
JD CORRECTION:   JD = JD(raw) - 0.00977d
UNITY CORR:      -5 * log(SunDist * EarthDist): -3.2269
NOTE: The unity correction is NOT included in the output magnitudes
MAG. METHOD:     Instrumental
 
NOTE:            For multiple sessions, differential magnitudes include
                 adjustments ADDED to the Obj-CAvg value to compensate
                 for changing phase angle, distance, and refinements to
                 the base average value of the comparison stars.       
                                                                       
                 The phase angle calculations include the effects of   
                 the phase parameter, G. This value is taken from the  
                 MPCORB value at the time the calculations were made.
BASE COMP VALUE: -9.334
BASE CORRECTION: -0.663
PHASE/DIST CORR: -0.103
PHASE SLOPE:     0.15
P/D ADJUST (-/DAY):+0.003
P/D ADJUST (+/DAY):-0.003
THE P/D ADJUSTMENTS ARE INCLUDED IN THE VALUES BELOW.
 
ERROR CALC:      The magnitude error is calculated by the following:
                 Err = sqrt(sqr(ERR[target]) + sqr(Err[Comps]))
                       where Err[Target] = 1.0857/SNR[target]
                             Err[Comps]  = sqrt(sqr(1.0857/SNR[Comp1])... + sqr(1.0857/SNR[CompN])) / N
                 The factor of 1.0857 converts flux to magnitudes (Howell)
Comp1: 053232.26 -22117.9            0.000 R  Y
Comp2: 053232.93 -21852.4            0.000 R  Y
Comp3: 053234.60 -22154.5            0.000 R  Y
Comp4: 053200.63 -22031.8            0.000 R  Y
Comp5: 053200.87 -21653.2            0.000 R  Y
*********************************************************************************************
TARGET:          2235 Vittore
SESSION NUMBER:  525
DATE/TIME:       2009/12/20 @ 08:22
OBSERVER:        J.W. Brinsfield
CONTACT INFO:    J.W. Brinsfield 5180 Via Capote, Thousand Oals, Ca, USA [jbrinsfi@viacapotesky.com]
FILTER:          C
TELESCOPE:       0.35m SCT
FOCAL LENGTH:    134.99
CAMERA:          Alta U6 1 X binning
TEMP (C):        -28
EXPOSURE (s):    180
APPROX. RA:      05:31
APPROX. DEC:     - 2
EXPOSURE JD:     Mid-exposure
JD CORR METHOD:  Light-time
JD CORRECTION:   JD = JD(raw) - 0.00977d
UNITY CORR:      -5 * log(SunDist * EarthDist): -3.2260
NOTE: The unity correction is NOT included in the output magnitudes
MAG. METHOD:     Instrumental
 
NOTE:            For multiple sessions, differential magnitudes include
                 adjustments ADDED to the Obj-CAvg value to compensate
                 for changing phase angle, distance, and refinements to
                 the base average value of the comparison stars.       
                                                                       
                 The phase angle calculations include the effects of   
                 the phase parameter, G. This value is taken from the  
                 MPCORB value at the time the calculations were made.
BASE COMP VALUE: -9.364
BASE CORRECTION: -0.693
PHASE/DIST CORR: -0.099
PHASE SLOPE:     0.15
P/D ADJUST (-/DAY):+0.005
P/D ADJUST (+/DAY):-0.005
THE P/D ADJUSTMENTS ARE INCLUDED IN THE VALUES BELOW.
 
ERROR CALC:      The magnitude error is calculated by the following:
                 Err = sqrt(sqr(ERR[target]) + sqr(Err[Comps]))
                       where Err[Target] = 1.0857/SNR[target]
                             Err[Comps]  = sqrt(sqr(1.0857/SNR[Comp1])... + sqr(1.0857/SNR[CompN])) / N
                 The factor of 1.0857 converts flux to magnitudes (Howell)
Comp1: 053111.28 -22439.8            0.000 R  Y
Comp2: 053133.18 -22031.5            0.000 R  Y
Comp3: 053135.94 -22932.4            0.000 R  N
Comp4: 053055.11 -22923.5            0.000 R  Y
Comp5: 053049.87 -22701.2            0.000 R  Y
*********************************************************************************************
TARGET:          2235 Vittore
SESSION NUMBER:  526
DATE/TIME:       2009/12/18 @ 07:00
OBSERVER:        J.W. Brinsfield
CONTACT INFO:    J.W. Brinsfield 5180 Via Capote, Thousand Oals, Ca, USA [jbrinsfi@viacapotesky.com]
FILTER:          C
TELESCOPE:       0.35m SCT
FOCAL LENGTH:    55.91
CAMERA:          Alta U6 1 X binning
TEMP (C):        -10
EXPOSURE (s):    120
APPROX. RA:      05:32
APPROX. DEC:     - 2
EXPOSURE JD:     Mid-exposure
JD CORR METHOD:  Light-time
JD CORRECTION:   JD = JD(raw) - 0.00977d
UNITY CORR:      -5 * log(SunDist * EarthDist): -3.2277
NOTE: The unity correction is NOT included in the output magnitudes
MAG. METHOD:     Instrumental
 
NOTE:            For multiple sessions, differential magnitudes include
                 adjustments ADDED to the Obj-CAvg value to compensate
                 for changing phase angle, distance, and refinements to
                 the base average value of the comparison stars.       
                                                                       
                 The phase angle calculations include the effects of   
                 the phase parameter, G. This value is taken from the  
                 MPCORB value at the time the calculations were made.
BASE COMP VALUE: -10.329
BASE CORRECTION: -1.658
PHASE/DIST CORR: -0.106
PHASE SLOPE:     0.15
P/D ADJUST (-/DAY):+0.002
P/D ADJUST (+/DAY):-0.002
THE P/D ADJUSTMENTS ARE INCLUDED IN THE VALUES BELOW.
 
ERROR CALC:      The magnitude error is calculated by the following:
                 Err = sqrt(sqr(ERR[target]) + sqr(Err[Comps]))
                       where Err[Target] = 1.0857/SNR[target]
                             Err[Comps]  = sqrt(sqr(1.0857/SNR[Comp1])... + sqr(1.0857/SNR[CompN])) / N
                 The factor of 1.0857 converts flux to magnitudes (Howell)
Comp1: A                             0.000 R  Y
Comp2: B                             0.000 R  Y
Comp3: C                             0.000 R  Y
Comp4: D                             0.000 R  Y
Comp5: E                             0.000 R  Y
*********************************************************************************************
TARGET:          2235 Vittore
SESSION NUMBER:  528
DATE/TIME:       2009/12/23 @ 07:53
OBSERVER:        J.W. Brinsfield
CONTACT INFO:    J.W. Brinsfield 5180 Via Capote, Thousand Oals, Ca, USA [jbrinsfi@viacapotesky.com]
FILTER:          C
TELESCOPE:       0.35m SCT
FOCAL LENGTH:    134.44
CAMERA:          Alta U6 1 X binning
TEMP (C):        -35
EXPOSURE (s):    180
APPROX. RA:      05:28
APPROX. DEC:     -02
EXPOSURE JD:     Mid-exposure
JD CORR METHOD:  Light-time
JD CORRECTION:   JD = JD(raw) - 0.00978d
UNITY CORR:      -5 * log(SunDist * EarthDist): -3.2266
NOTE: The unity correction is NOT included in the output magnitudes
MAG. METHOD:     Instrumental
 
NOTE:            For multiple sessions, differential magnitudes include
                 adjustments ADDED to the Obj-CAvg value to compensate
                 for changing phase angle, distance, and refinements to
                 the base average value of the comparison stars.       
                                                                       
                 The phase angle calculations include the effects of   
                 the phase parameter, G. This value is taken from the  
                 MPCORB value at the time the calculations were made.
BASE COMP VALUE: -9.413
BASE CORRECTION: -0.742
PHASE/DIST CORR: -0.082
PHASE SLOPE:     0.15
P/D ADJUST (-/DAY):+0.007
P/D ADJUST (+/DAY):-0.007
THE P/D ADJUSTMENTS ARE INCLUDED IN THE VALUES BELOW.
 
ERROR CALC:      The magnitude error is calculated by the following:
                 Err = sqrt(sqr(ERR[target]) + sqr(Err[Comps]))
                       where Err[Target] = 1.0857/SNR[target]
                             Err[Comps]  = sqrt(sqr(1.0857/SNR[Comp1])... + sqr(1.0857/SNR[CompN])) / N
                 The factor of 1.0857 converts flux to magnitudes (Howell)
Comp1: 052923.60 -023436.5           0.000 R  Y
Comp2: 052841.86 -023253.5           0.000 R  Y
Comp3: 052859.73 -022935.1           0.000 R  Y
Comp4: 052847.62 -022953.1           0.000 R  Y
Comp5: 052909.22 -022634.7           0.000 R  Y
*********************************************************************************************
TARGET:          2235 Vittore
SESSION NUMBER:  530
DATE/TIME:       2009/12/24 @ 07:43
OBSERVER:        J.W. Brinsfield
CONTACT INFO:    J.W. Brinsfield 5180 Via Capote, Thousand Oals, Ca, USA [jbrinsfi@viacapotesky.com]
FILTER:          C
TELESCOPE:       0.35m SCT
FOCAL LENGTH:    135.03
CAMERA:          Alta U6 1 X binning
TEMP (C):        -35
EXPOSURE (s):    180
APPROX. RA:      05:28
APPROX. DEC:     -02
EXPOSURE JD:     Mid-exposure
JD CORR METHOD:  Light-time
JD CORRECTION:   JD = JD(raw) - 0.00980d
UNITY CORR:      -5 * log(SunDist * EarthDist): -3.2283
NOTE: The unity correction is NOT included in the output magnitudes
MAG. METHOD:     Instrumental
 
NOTE:            For multiple sessions, differential magnitudes include
                 adjustments ADDED to the Obj-CAvg value to compensate
                 for changing phase angle, distance, and refinements to
                 the base average value of the comparison stars.       
                                                                       
                 The phase angle calculations include the effects of   
                 the phase parameter, G. This value is taken from the  
                 MPCORB value at the time the calculations were made.
BASE COMP VALUE: -8.157
BASE CORRECTION: +0.514
PHASE/DIST CORR: -0.074
PHASE SLOPE:     0.15
P/D ADJUST (-/DAY):+0.008
P/D ADJUST (+/DAY):-0.008
THE P/D ADJUSTMENTS ARE INCLUDED IN THE VALUES BELOW.
 
ERROR CALC:      The magnitude error is calculated by the following:
                 Err = sqrt(sqr(ERR[target]) + sqr(Err[Comps]))
                       where Err[Target] = 1.0857/SNR[target]
                             Err[Comps]  = sqrt(sqr(1.0857/SNR[Comp1])... + sqr(1.0857/SNR[CompN])) / N
                 The factor of 1.0857 converts flux to magnitudes (Howell)
Comp1: 052826.25 -023731.1          14.478 R  Y
Comp2: 052815.20 -024158.2          13.828 R  Y
Comp3: 052826.97 -023513.0          13.355 R  Y
Comp4: 052841.92 -023958.0          13.845 R  Y
Comp5: 052815.43 -024039.5          14.678 R  Y
*********************************************************************************************
 
Non-reduced Magnitudes
-------------------------------------------
J.D.            Obj-CAvg    Err    Session
-------------------------------------------
2455166.75636     +0.268   0.007       511
2455166.75863     +0.246   0.007       511
2455166.76082     +0.270   0.007       511
2455166.76301     +0.258   0.007       511
2455166.76519     +0.241   0.007       511
2455166.76737     +0.265   0.007       511
2455166.76964     +0.248   0.007       511
2455166.77182     +0.258   0.007       511
2455166.77400     +0.258   0.006       511
2455166.77619     +0.258   0.006       511
2455166.77837     +0.263   0.006       511
2455166.78056     +0.257   0.006       511
2455166.78274     +0.254   0.006       511
2455166.78493     +0.251   0.006       511
2455166.78711     +0.268   0.006       511
2455166.79001     +0.267   0.006       511
2455166.79219     +0.245   0.006       511
2455166.79437     +0.262   0.006       511
2455166.79655     +0.252   0.006       511
2455166.79874     +0.253   0.006       511
2455166.80091     +0.264   0.006       511
2455166.80310     +0.262   0.006       511
2455166.80528     +0.270   0.006       511
2455166.80746     +0.261   0.006       511
2455166.80965     +0.263   0.006       511
2455166.81183     +0.281   0.006       511
2455166.81404     +0.267   0.006       511
2455166.81619     +0.269   0.006       511
2455166.81838     +0.280   0.006       511
2455166.82056     +0.268   0.006       511
2455166.82343     +0.270   0.006       511
2455166.82561     +0.284   0.006       511
2455166.82778     +0.275   0.006       511
2455166.82997     +0.271   0.006       511
2455166.83215     +0.281   0.006       511
2455166.83434     +0.275   0.006       511
2455166.83651     +0.273   0.006       511
2455166.83875     +0.275   0.006       511
2455166.84093     +0.291   0.006       511
2455166.84311     +0.287   0.006       511
2455166.84530     +0.304   0.006       511
2455166.84748     +0.288   0.006       511
2455166.84965     +0.295   0.006       511
2455166.85183     +0.307   0.006       511
2455166.85416     +0.297   0.006       511
2455166.85720     +0.303   0.006       511
2455166.85938     +0.318   0.006       511
2455166.86156     +0.309   0.006       511
2455166.86380     +0.306   0.006       511
2455166.86598     +0.342   0.006       511
2455166.86816     +0.326   0.006       511
2455166.87034     +0.308   0.006       511
2455166.87252     +0.323   0.006       511
2455166.87475     +0.309   0.006       511
2455166.87689     +0.335   0.006       511
2455166.87911     +0.323   0.006       511
2455166.88129     +0.331   0.006       511
2455166.88347     +0.338   0.006       511
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2455189.92851     +0.440   0.005       530
2455189.93069     +0.438   0.005       530
 
END OF FIXED DATA SECTION. DO NOT MAKE ANY CHANGES ABOVE THIS LINE.

      

 

 

 

Contents © 2008 James W Brinsfield / Via Capote Observatory