TARGET:          4585 Ainonai
SESSION NUMBER:  245
DATE/TIME:       2008 May 30 @ 07:23
FILTER:          C
TELESCOPE:       0.35m SCT
FOCAL LENGTH:    135.30
CAMERA:          Alta U6 1 x binning
TEMP (C):        -30
EXPOSURE (s):    240
APPROX. RA:      15:43
APPROX. DEC:     -12
EXPOSURE JD:     Mid-exposure
JD CORR METHOD:  Light-time
JD CORRECTION:   JD = JD(raw) - 0.00650d
UNITY CORR:      -5 * log(SunDist * EarthDist): -1.8924
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: -8.550
BASE CORRECTION: +0.000
PHASE/DIST CORR: +0.000
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:          4585 Ainonai
SESSION NUMBER:  246
DATE/TIME:       2008 May 31 @ 05:25
FILTER:          C
TELESCOPE:       0.35m SCT
FOCAL LENGTH:    135.25
CAMERA:          Alta U6 1 x binning
TEMP (C):        -30
EXPOSURE (s):    240
APPROX. RA:      15:42
APPROX. DEC:     -12
EXPOSURE JD:     Mid-exposure
JD CORR METHOD:  Light-time
JD CORRECTION:   JD = JD(raw) - 0.00651d
UNITY CORR:      -5 * log(SunDist * EarthDist): -1.8933
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: -7.586
BASE CORRECTION: +0.964
PHASE/DIST CORR: +0.020
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:          4585 Ainonai
SESSION NUMBER:  248
DATE/TIME:       2008 Jun 01 @ 06:53
FILTER:          C
TELESCOPE:       0.35m SCT
FOCAL LENGTH:    135.37
CAMERA:          Alta U6 1 x binning
TEMP (C):        -30
EXPOSURE (s):    240
APPROX. RA:      15:41
APPROX. DEC:     -12
EXPOSURE JD:     Mid-exposure
JD CORR METHOD:  Light-time
JD CORRECTION:   JD = JD(raw) - 0.00651d
UNITY CORR:      -5 * log(SunDist * EarthDist): -1.8942
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: -7.321
BASE CORRECTION: +1.229
PHASE/DIST CORR: +0.044
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:          4585 Ainonai
SESSION NUMBER:  252
DATE/TIME:       2008 Jun 02 @ 06:42
FILTER:          C
TELESCOPE:       0.35m SCT
FOCAL LENGTH:    135.15
CAMERA:          Alta U6 1 x binning
TEMP (C):        -30
EXPOSURE (s):    240
APPROX. RA:      15:40
APPROX. DEC:     -12
EXPOSURE JD:     Mid-exposure
JD CORR METHOD:  Light-time
JD CORRECTION:   JD = JD(raw) - 0.00652d
UNITY CORR:      -5 * log(SunDist * EarthDist): -1.8960
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: -7.402
BASE CORRECTION: +1.148
PHASE/DIST CORR: +0.066
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:          4585 Ainonai
SESSION NUMBER:  253
DATE/TIME:       2008 Jun 03 @ 06:53
FILTER:          C
TELESCOPE:       0.35m SCT
FOCAL LENGTH:    135.33
CAMERA:          Alta U6 1 x binning
TEMP (C):        -30
EXPOSURE (s):    240
APPROX. RA:      15:39
APPROX. DEC:     -12
EXPOSURE JD:     Mid-exposure
JD CORR METHOD:  Light-time
JD CORRECTION:   JD = JD(raw) - 0.00653d
UNITY CORR:      -5 * log(SunDist * EarthDist): -1.8989
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: -8.579
BASE CORRECTION: -0.029
PHASE/DIST CORR: +0.089
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:          4585 Ainonai
SESSION NUMBER:  255
DATE/TIME:       2008 Jun 04 @ 06:48
FILTER:          C
TELESCOPE:       0.35m SCT
FOCAL LENGTH:    135.14
CAMERA:          Alta U6 1 x binning
TEMP (C):        -30
EXPOSURE (s):    240
APPROX. RA:      15:38
APPROX. DEC:     -12
EXPOSURE JD:     Mid-exposure
JD CORR METHOD:  Light-time
JD CORRECTION:   JD = JD(raw) - 0.00655d
UNITY CORR:      -5 * log(SunDist * EarthDist): -1.9017
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: -7.673
BASE CORRECTION: +0.877
PHASE/DIST CORR: +0.111
P/D ADJUST (-/DAY):+0.023
P/D ADJUST (+/DAY):-0.023
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:          4585 Ainonai
SESSION NUMBER:  257
DATE/TIME:       2008 Jun 05 @ 06:41
FILTER:          C
TELESCOPE:       0.35m SCT
FOCAL LENGTH:    135.46
CAMERA:          Alta U6 1 x binning
TEMP (C):        -30
EXPOSURE (s):    240
APPROX. RA:      15:37
APPROX. DEC:     -12
EXPOSURE JD:     Mid-exposure
JD CORR METHOD:  Light-time
JD CORRECTION:   JD = JD(raw) - 0.00656d
UNITY CORR:      -5 * log(SunDist * EarthDist): -1.9045
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: -8.506
BASE CORRECTION: +0.044
PHASE/DIST CORR: +0.134
P/D ADJUST (-/DAY):+0.023
P/D ADJUST (+/DAY):-0.023
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:          4585 Ainonai
SESSION NUMBER:  259
DATE/TIME:       2008 Jun 06 @ 07:04
FILTER:          C
TELESCOPE:       0.35m SCT
FOCAL LENGTH:    135.07
CAMERA:          Alta U6 1 x binning
TEMP (C):        -30
EXPOSURE (s):    240
APPROX. RA:      15:37
APPROX. DEC:     -13
EXPOSURE JD:     Mid-exposure
JD CORR METHOD:  Light-time
JD CORRECTION:   JD = JD(raw) - 0.00657d
UNITY CORR:      -5 * log(SunDist * EarthDist): -1.9073
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: -7.512
BASE CORRECTION: +1.038
PHASE/DIST CORR: +0.157
P/D ADJUST (-/DAY):+0.023
P/D ADJUST (+/DAY):-0.023
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)
 
*********************************************************************************************