TARGET:          1379 Lomosonowa
SESSION NUMBER:  170
DATE/TIME:       2008 Feb 29 @ 04:37
FILTER:          C
TELESCOPE:       300 mm f11.5 cass
FOCAL LENGTH:    136.37
CAMERA:          AltaU6 1x bin
TEMP (C):        -30
EXPOSURE (s):    90
APPROX. RA:      09:25
APPROX. DEC:     + 5
EXPOSURE JD:     Mid-exposure
JD CORR METHOD:  Light-time
JD CORRECTION:   JD = JD(raw) - 0.00820d
UNITY CORR:      -5 * log(SunDist * EarthDist): -2.6413
NOTE: The unity correction is NOT included in the reduced 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: -8.118
BASE CORRECTION: +0.000
PHASE/DIST CORR: +0.000
P/D ADJUST (-/DAY):+0.021
P/D ADJUST (+/DAY):-0.021
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)
 
*********************************************************************************************
TARGET:          1379 Lomosonowa
SESSION NUMBER:  171
DATE/TIME:       2008 Mar 04 @ 06:56
FILTER:          C
TELESCOPE:       300 mm f11.5 cass
FOCAL LENGTH:    136.30
CAMERA:          AltaU6 1x bin
TEMP (C):        -30
EXPOSURE (s):    90
APPROX. RA:      09:22
APPROX. DEC:     + 6
EXPOSURE JD:     Mid-exposure
JD CORR METHOD:  Light-time
JD CORRECTION:   JD = JD(raw) - 0.00828d
UNITY CORR:      -5 * log(SunDist * EarthDist): -2.6583
NOTE: The unity correction is NOT included in the reduced 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: -9.551
BASE CORRECTION: -1.433
PHASE/DIST CORR: +0.088
P/D ADJUST (-/DAY):+0.022
P/D ADJUST (+/DAY):-0.022
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)
 
*********************************************************************************************
TARGET:          1379 Lomosonowa
SESSION NUMBER:  172
DATE/TIME:       2008 Mar 05 @ 05:57
FILTER:          C
TELESCOPE:       300 mm f11.5 cass
FOCAL LENGTH:    136.46
CAMERA:          AltaU6 1x bin
TEMP (C):        -30
EXPOSURE (s):    90
APPROX. RA:      09:21
APPROX. DEC:     + 6
EXPOSURE JD:     Mid-exposure
JD CORR METHOD:  Light-time
JD CORRECTION:   JD = JD(raw) - 0.00829d
UNITY CORR:      -5 * log(SunDist * EarthDist): -2.6619
NOTE: The unity correction is NOT included in the reduced 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: -8.749
BASE CORRECTION: -0.631
PHASE/DIST CORR: +0.109
P/D ADJUST (-/DAY):+0.022
P/D ADJUST (+/DAY):-0.022
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)
 
*********************************************************************************************
TARGET:          1379 Lomosonowa
SESSION NUMBER:  179
DATE/TIME:       2008 Mar 10 @ 12:40
FILTER:          C
TELESCOPE:       0.35
FOCAL LENGTH:    77.00
CAMERA:          ST-8XME
TEMP (C):        -15
EXPOSURE (s):    120
APPROX. RA:      09:18
APPROX. DEC:     + 7
EXPOSURE JD:     Mid-exposure
JD CORR METHOD:  Light-time
JD CORRECTION:   JD = JD(raw) - 0.00844d
UNITY CORR:      -5 * log(SunDist * EarthDist): -2.6957
NOTE: The unity correction is NOT included in the reduced 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: -7.961
BASE CORRECTION: +0.157
PHASE/DIST CORR: +0.227
P/D ADJUST (-/DAY):+0.022
P/D ADJUST (+/DAY):-0.022
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)
 
*********************************************************************************************
TARGET:          1379 Lomosonowa
SESSION NUMBER:  181
DATE/TIME:       2008 Mar 12 @ 06:21
FILTER:          C
TELESCOPE:       300 mm f11.5 cass
FOCAL LENGTH:    136.88
CAMERA:          AltaU6 1x bin
TEMP (C):        -30
EXPOSURE (s):    120
APPROX. RA:      09:18
APPROX. DEC:     + 7
EXPOSURE JD:     Mid-exposure
JD CORR METHOD:  Light-time
JD CORRECTION:   JD = JD(raw) - 0.00849d
UNITY CORR:      -5 * log(SunDist * EarthDist): -2.7081
NOTE: The unity correction is NOT included in the reduced 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: -8.836
BASE CORRECTION: -0.718
PHASE/DIST CORR: +0.265
P/D ADJUST (-/DAY):+0.022
P/D ADJUST (+/DAY):-0.022
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)
 
*********************************************************************************************
TARGET:          1379 Lomosonowa
SESSION NUMBER:  183
DATE/TIME:       2008 Mar 13 @ 12:31
FILTER:          C
TELESCOPE:       .35
FOCAL LENGTH:    77.00
CAMERA:          ST-8XME
TEMP (C):        -15
EXPOSURE (s):    120
APPROX. RA:      09:17
APPROX. DEC:     + 7
EXPOSURE JD:     Mid-exposure
JD CORR METHOD:  Light-time
JD CORRECTION:   JD = JD(raw) - 0.00853d
UNITY CORR:      -5 * log(SunDist * EarthDist): -2.7175
NOTE: The unity correction is NOT included in the reduced 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: -8.487
BASE CORRECTION: -0.369
PHASE/DIST CORR: +0.293
P/D ADJUST (-/DAY):+0.022
P/D ADJUST (+/DAY):-0.022
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)
 
*********************************************************************************************
TARGET:          1379 Lomosonowa
SESSION NUMBER:  185
DATE/TIME:       2008 Mar 16 @ 10:00
FILTER:          C
TELESCOPE:       0.35
FOCAL LENGTH:    77.00
CAMERA:          SBIG ST-8E
TEMP (C):         -5
EXPOSURE (s):    240
APPROX. RA:      09:16
APPROX. DEC:     + 8
EXPOSURE JD:     Mid-exposure
JD CORR METHOD:  Light-time
JD CORRECTION:   JD = JD(raw) - 0.00863d
UNITY CORR:      -5 * log(SunDist * EarthDist): -2.7420
NOTE: The unity correction is NOT included in the reduced 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: -8.067
BASE CORRECTION: +0.051
PHASE/DIST CORR: +0.357
P/D ADJUST (-/DAY):+0.022
P/D ADJUST (+/DAY):-0.022
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)
 
*********************************************************************************************
TARGET:          1379 Lomosonowa
SESSION NUMBER:  193
DATE/TIME:       2008 Mar 21 @ 06:03
FILTER:          C
TELESCOPE:       300 mm f11.5 cass
FOCAL LENGTH:    139.97
CAMERA:          AltaU6 1x bin
TEMP (C):        -30
EXPOSURE (s):    90
APPROX. RA:      09:15
APPROX. DEC:     + 9
EXPOSURE JD:     Mid-exposure
JD CORR METHOD:  Light-time
JD CORRECTION:   JD = JD(raw) - 0.00883d
UNITY CORR:      -5 * log(SunDist * EarthDist): -2.7880
NOTE: The unity correction is NOT included in the reduced 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: -8.316
BASE CORRECTION: -0.198
PHASE/DIST CORR: +0.463
P/D ADJUST (-/DAY):+0.021
P/D ADJUST (+/DAY):-0.021
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)
 
*********************************************************************************************
TARGET:          1379 Lomosonowa
SESSION NUMBER:  199
DATE/TIME:       2008 Mar 27 @ 05:58
FILTER:          C
TELESCOPE:       300 mm f11.5 cass
FOCAL LENGTH:    139.92
CAMERA:          AltaU6 1x bin
TEMP (C):        -30
EXPOSURE (s):    90
APPROX. RA:      09:15
APPROX. DEC:     +10
EXPOSURE JD:     Mid-exposure
JD CORR METHOD:  Light-time
JD CORRECTION:   JD = JD(raw) - 0.00910d
UNITY CORR:      -5 * log(SunDist * EarthDist): -2.8500
NOTE: The unity correction is NOT included in the reduced 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: -7.581
BASE CORRECTION: +0.537
PHASE/DIST CORR: +0.591
P/D ADJUST (-/DAY):+0.021
P/D ADJUST (+/DAY):-0.021
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)
 
*********************************************************************************************
TARGET:          1379 Lomosonowa
SESSION NUMBER:  200
DATE/TIME:       2008 Mar 27 @ 10:00
FILTER:          C
TELESCOPE:       0.35
FOCAL LENGTH:    77.00
CAMERA:          SBIG ST-8E
TEMP (C):        -15
EXPOSURE (s):    120
APPROX. RA:      09:15
APPROX. DEC:     +10
EXPOSURE JD:     Mid-exposure
JD CORR METHOD:  Light-time
JD CORRECTION:   JD = JD(raw) - 0.00911d
UNITY CORR:      -5 * log(SunDist * EarthDist): -2.8519
NOTE: The unity correction is NOT included in the reduced 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: -7.996
BASE CORRECTION: +0.122
PHASE/DIST CORR: +0.594
P/D ADJUST (-/DAY):+0.021
P/D ADJUST (+/DAY):-0.021
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)
 
*********************************************************************************************
TARGET:          1379 Lomosonowa
SESSION NUMBER:  204
DATE/TIME:       2008 Mar 28 @ 10:00
FILTER:          C
TELESCOPE:       0.35
FOCAL LENGTH:    77.00
CAMERA:          SBIG ST-8E
TEMP (C):        -15
EXPOSURE (s):    120
APPROX. RA:      09:15
APPROX. DEC:     +10
EXPOSURE JD:     Mid-exposure
JD CORR METHOD:  Light-time
JD CORRECTION:   JD = JD(raw) - 0.00916d
UNITY CORR:      -5 * log(SunDist * EarthDist): -2.8628
NOTE: The unity correction is NOT included in the reduced 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: -8.403
BASE CORRECTION: -0.285
PHASE/DIST CORR: +0.615
P/D ADJUST (-/DAY):+0.021
P/D ADJUST (+/DAY):-0.021
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)
 
*********************************************************************************************
TARGET:          1379 Lomosonowa
SESSION NUMBER:  205
DATE/TIME:       2008 Apr 07 @ 06:05
FILTER:          C
TELESCOPE:       300 mm f11.5 cass
FOCAL LENGTH:    136.99
CAMERA:          AltaU6 1x bin
TEMP (C):        -30
EXPOSURE (s):    90
APPROX. RA:      09:16
APPROX. DEC:     +11
EXPOSURE JD:     Mid-exposure
JD CORR METHOD:  Light-time
JD CORRECTION:   JD = JD(raw) - 0.00969d
UNITY CORR:      -5 * log(SunDist * EarthDist): -2.9787
NOTE: The unity correction is NOT included in the reduced 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: -7.312
BASE CORRECTION: +0.806
PHASE/DIST CORR: +0.813
P/D ADJUST (-/DAY):+0.020
P/D ADJUST (+/DAY):-0.020
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)
 
*********************************************************************************************
 
-------------------------------------------
  J.D.          Obj-CAvg    Err    Session
-------------------------------------------
2454525.61941     +0.398   0.013       170
2454525.62055     +0.374   0.012       170
2454525.62169     +0.376   0.012       170
2454525.62283     +0.371   0.012       170
2454525.62397     +0.393   0.012       170
2454525.62588     +0.396   0.012       170
2454525.62702     +0.348   0.011       170
2454525.62816     +0.350   0.011       170
2454525.62930     +0.374   0.011       170
2454525.63044     +0.376   0.011       170
2454525.63234     +0.351   0.011       170
2454525.63348     +0.344   0.010       170
2454525.63462     +0.348   0.010       170
2454525.63576     +0.342   0.010       170
2454525.63690     +0.326   0.010       170
2454525.63876     +0.334   0.010       170
2454525.63990     +0.335   0.010       170
2454525.64103     +0.337   0.010       170
2454525.64216     +0.340   0.010       170
2454525.64329     +0.320   0.010       170
2454525.64517     +0.323   0.010       170
2454525.64631     +0.321   0.009       170
2454525.64744     +0.313   0.009       170
2454525.64857     +0.305   0.009       170
2454525.64970     +0.306   0.009       170
2454525.65158     +0.319   0.009       170
2454525.65271     +0.298   0.009       170
2454525.65384     +0.276   0.009       170
2454525.65497     +0.282   0.009       170
2454525.65610     +0.272   0.009       170
2454525.65795     +0.282   0.009       170
2454525.65909     +0.276   0.009       170
2454525.66023     +0.298   0.009       170
2454525.66137     +0.255   0.009       170
2454525.66251     +0.265   0.009       170
2454525.66437     +0.282   0.009       170
2454525.66551     +0.257   0.009       170
2454525.66665     +0.268   0.008       170
2454525.66780     +0.265   0.008       170
2454525.66894     +0.248   0.008       170
2454525.67083     +0.261   0.008       170
2454525.67197     +0.264   0.008       170
2454525.67310     +0.256   0.008       170
2454525.67426     +0.238   0.008       170
2454525.67538     +0.245   0.008       170
2454525.67722     +0.232   0.008       170
2454525.67836     +0.233   0.008       170
2454525.67950     +0.226   0.008       170
2454525.68064     +0.238   0.008       170
2454525.68178     +0.251   0.008       170
2454525.68336     +0.231   0.008       170
2454525.68452     +0.230   0.008       170
2454525.68564     +0.227   0.008       170
2454525.68675     +0.218   0.008       170
2454525.68789     +0.229   0.008       170
2454525.68970     +0.210   0.008       170
2454525.69082     +0.216   0.008       170
2454525.69195     +0.222   0.007       170
2454525.69310     +0.200   0.007       170
2454525.69424     +0.201   0.007       170
2454525.69607     +0.212   0.007       170
2454525.69719     +0.202   0.007       170
2454525.69833     +0.215   0.007       170
2454525.69947     +0.208   0.007       170
2454525.70058     +0.215   0.007       170
2454525.70237     +0.203   0.007       170
2454525.70350     +0.213   0.007       170
2454525.70464     +0.215   0.007       170
2454525.70577     +0.215   0.007       170
2454525.70692     +0.203   0.007       170
2454525.70874     +0.210   0.007       170
2454525.70985     +0.200   0.007       170
2454525.71099     +0.194   0.007       170
2454525.71213     +0.189   0.007       170
2454525.71326     +0.191   0.007       170
2454525.71486     +0.185   0.006       170
2454525.71600     +0.190   0.007       170
2454525.71714     +0.204   0.007       170
2454525.71827     +0.186   0.006       170
2454525.71939     +0.196   0.006       170
2454525.72092     +0.203   0.006       170
2454525.72206     +0.185   0.006       170
2454525.72320     +0.181   0.006       170
2454525.72431     +0.187   0.006       170
2454525.72543     +0.190   0.006       170
2454525.72701     +0.190   0.006       170
2454525.72812     +0.179   0.006       170
2454525.72925     +0.179   0.006       170
2454525.73038     +0.184   0.006       170
2454525.73151     +0.176   0.006       170
2454525.73337     +0.186   0.006       170
2454525.73448     +0.183   0.006       170
2454525.73561     +0.185   0.006       170
2454525.73673     +0.181   0.006       170
2454525.73786     +0.173   0.007       170
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2454563.82267     +0.484   0.021       205
2454563.82380     +0.499   0.018       205
2454563.82579     +0.454   0.018       205
 
END OF FIXED DATA SECTION. DO NOT MAKE ANY CHANGES ABOVE THIS LINE.

 

 

 

Contents © 2008 James W Brinsfield / Via Capote Observatory