TARGET:          7638 Gladman
SESSION NUMBER:  296
DATE/TIME:       2008 Oct 02 @ 06:04
FILTER:          C
TELESCOPE:       0.35m SCT
FOCAL LENGTH:    135.72
CAMERA:          Alta U6 1 x binning
TEMP (C):        -20
EXPOSURE (s):    240
APPROX. RA:      22:22
APPROX. DEC:     -14
EXPOSURE JD:     Mid-exposure
JD CORR METHOD:  Light-time
JD CORRECTION:   JD = JD(raw) - 0.00554d
UNITY CORR:      -5 * log(SunDist * EarthDist): -1.2520
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: -7.964
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:          7638 Gladman
SESSION NUMBER:  300
DATE/TIME:       2008 Oct 07 @ 05:19
FILTER:          C
TELESCOPE:       0.35m SCT
FOCAL LENGTH:    135.15
CAMERA:          Alta U6 1 x binning
TEMP (C):        -20
EXPOSURE (s):    240
APPROX. RA:      22:21
APPROX. DEC:     -14
EXPOSURE JD:     Mid-exposure
JD CORR METHOD:  Light-time
JD CORRECTION:   JD = JD(raw) - 0.00565d
UNITY CORR:      -5 * log(SunDist * EarthDist): -1.2839
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: -7.480
BASE CORRECTION: +0.484
PHASE/DIST CORR: +0.107
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:          7638 Gladman
SESSION NUMBER:  306
DATE/TIME:       2008 Oct 19 @ 05:09
FILTER:          C
TELESCOPE:       0.35m SCT
FOCAL LENGTH:    134.73
CAMERA:          Alta U6 1 x binning
TEMP (C):        -20
EXPOSURE (s):    240
APPROX. RA:      22:21
APPROX. DEC:     -12
EXPOSURE JD:     Mid-exposure
JD CORR METHOD:  Light-time
JD CORRECTION:   JD = JD(raw) - 0.00602d
UNITY CORR:      -5 * log(SunDist * EarthDist): -1.3906
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: -7.180
BASE CORRECTION: +0.784
PHASE/DIST CORR: +0.356
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)