TARGET:          2005Hencke

SESSION NUMBER:  97

DATE/TIME:       2007 Oct 14 @ 06:42

FILTER:          C

TELESCOPE:       300 mm f11.5 cass

FOCAL LENGTH:    136.79

CAMERA:          AltaU6 1x bin

TEMP (C):        -30

EXPOSURE (s):    240

APPROX. RA:      22:48

APPROX. DEC:     +13

EXPOSURE JD:     Mid-exposure

JD CORR METHOD:  Light-time

JD CORRECTION:   JD = JD(raw) - 0.00794d

UNITY CORR:      -5 * log(SunDist * EarthDist): -2.4617

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: -8.314

BASE CORRECTION: +0.000

PHASE/DIST CORR: +0.000

P/D ADJUST (-/DAY):+0.019

P/D ADJUST (+/DAY):-0.019

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:          2005Hencke

SESSION NUMBER:  98

DATE/TIME:       2007 Nov 01 @ 06:23

FILTER:          C

TELESCOPE:       300 mm f11.5 cass

FOCAL LENGTH:    136.54

CAMERA:          AltaU6 1x bin

TEMP (C):        -30

EXPOSURE (s):    240

APPROX. RA:      22:46

APPROX. DEC:     +11

EXPOSURE JD:     Mid-exposure

JD CORR METHOD:  Light-time

JD CORRECTION:   JD = JD(raw) - 0.00863d

UNITY CORR:      -5 * log(SunDist * EarthDist): -2.6235

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: -7.873

BASE CORRECTION: +0.441

PHASE/DIST CORR: +0.342

P/D ADJUST (-/DAY):+0.019

P/D ADJUST (+/DAY):-0.019

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:          2005Hencke

SESSION NUMBER:  99

DATE/TIME:       2007 Nov 06 @ 05:56

FILTER:          C

TELESCOPE:       300 mm f11.5 cass

FOCAL LENGTH:    136.91

CAMERA:          AltaU6 1x bin

TEMP (C):        -30

EXPOSURE (s):    240

APPROX. RA:      22:47

APPROX. DEC:     +11

EXPOSURE JD:     Mid-exposure

JD CORR METHOD:  Light-time

JD CORRECTION:   JD = JD(raw) - 0.00887d

UNITY CORR:      -5 * log(SunDist * EarthDist): -2.6774

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: -7.501

BASE CORRECTION: +0.813

PHASE/DIST CORR: +0.434

P/D ADJUST (-/DAY):+0.018

P/D ADJUST (+/DAY):-0.018

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:          2005Hencke

SESSION NUMBER:  100

DATE/TIME:       2007 Nov 11 @ 06:07

FILTER:          C

TELESCOPE:       300 mm f11.5 cass

FOCAL LENGTH:    136.91

CAMERA:          AltaU6 1x bin

TEMP (C):        -30

EXPOSURE (s):    240

APPROX. RA:      22:49

APPROX. DEC:     +11

EXPOSURE JD:     Mid-exposure

JD CORR METHOD:  Light-time

JD CORRECTION:   JD = JD(raw) - 0.00912d

UNITY CORR:      -5 * log(SunDist * EarthDist): -2.7338

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: -7.746

BASE CORRECTION: +0.568

PHASE/DIST CORR: +0.524

P/D ADJUST (-/DAY):+0.018

P/D ADJUST (+/DAY):-0.018

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:          2005Hencke

SESSION NUMBER:  115

DATE/TIME:       2007 Nov 22 @ 05:16

FILTER:          C

TELESCOPE:       300 mm f11.5 cass

FOCAL LENGTH:    136.92

CAMERA:          AltaU6 1x bin

TEMP (C):        -30

EXPOSURE (s):    240

APPROX. RA:      22:56

APPROX. DEC:     +10

EXPOSURE JD:     Mid-exposure

JD CORR METHOD:  Light-time

JD CORRECTION:   JD = JD(raw) - 0.00973d

UNITY CORR:      -5 * log(SunDist * EarthDist): -2.8648

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: -8.103

BASE CORRECTION: +0.211

PHASE/DIST CORR: +0.709

P/D ADJUST (-/DAY):+0.016

P/D ADJUST (+/DAY):-0.016

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:          2005Hencke

SESSION NUMBER:  118

DATE/TIME:       2007 Nov 27 @ 05:06

FILTER:          C

TELESCOPE:       300 mm f11.5 cass

FOCAL LENGTH:    136.92

CAMERA:          AltaU6 1x bin

TEMP (C):        -30

EXPOSURE (s):    240

APPROX. RA:      23:01

APPROX. DEC:     +10

EXPOSURE JD:     Mid-exposure

JD CORR METHOD:  Light-time

JD CORRECTION:   JD = JD(raw) - 0.01001d

UNITY CORR:      -5 * log(SunDist * EarthDist): -2.9243

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: -7.841

BASE CORRECTION: +0.473

PHASE/DIST CORR: +0.787

P/D ADJUST (-/DAY):+0.015

P/D ADJUST (+/DAY):-0.015

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)

*********************************************************************************************