TARGET:          455 Bruchsalia
SESSION NUMBER:  239
DATE/TIME:       2008 May 23 @ 06:46
FILTER:          C
TELESCOPE:       0.35m SCT
FOCAL LENGTH:    135.56
CAMERA:          SBIG ST-8E
TEMP (C):        -30
EXPOSURE (s):    120
APPROX. RA:      14:02
APPROX. DEC:     - 1
EXPOSURE JD:     Mid-exposure
JD CORR METHOD:  Light-time
JD CORRECTION:   JD = JD(raw) - 0.01211d
UNITY CORR:      -5 * log(SunDist * EarthDist): -3.9837
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: -7.467
BASE CORRECTION: +0.000
PHASE/DIST CORR: +0.000
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)
 
*********************************************************************************************
TARGET:          455 Bruchsalia
SESSION NUMBER:  243
DATE/TIME:       2008 May 29 @ 08:25
FILTER:          C
TELESCOPE:       0.35m SCT
FOCAL LENGTH:    135.67
CAMERA:          Alta U6 1 x binning
TEMP (C):        -30
EXPOSURE (s):    90
APPROX. RA:      13:58
APPROX. DEC:     - 1
EXPOSURE JD:     Mid-exposure
JD CORR METHOD:  Light-time
JD CORRECTION:   JD = JD(raw) - 0.01230d
UNITY CORR:      -5 * log(SunDist * EarthDist): -4.0067
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: -7.365
BASE CORRECTION: +0.102
PHASE/DIST CORR: +0.091
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)
 
*********************************************************************************************
TARGET:          455 Bruchsalia
SESSION NUMBER:  249
DATE/TIME:       2008 Jun 01 @ 06:24
FILTER:          C
TELESCOPE:       0.35m SCT
FOCAL LENGTH:    135.39
CAMERA:          Alta U6 1 x binning
TEMP (C):        -30
EXPOSURE (s):    120
APPROX. RA:      13:56
APPROX. DEC:     - 1
EXPOSURE JD:     Mid-exposure
JD CORR METHOD:  Light-time
JD CORRECTION:   JD = JD(raw) - 0.01241d
UNITY CORR:      -5 * log(SunDist * EarthDist): -4.0209
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: -8.033
BASE CORRECTION: -0.566
PHASE/DIST CORR: +0.135
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)
 
*********************************************************************************************
TARGET:          455 Bruchsalia
SESSION NUMBER:  256
DATE/TIME:       2008 Jun 04 @ 06:25
FILTER:          C
TELESCOPE:       0.35m SCT
FOCAL LENGTH:    135.63
CAMERA:          Alta U6 1 x binning
TEMP (C):        -30
EXPOSURE (s):    90
APPROX. RA:      13:55
APPROX. DEC:     - 1
EXPOSURE JD:     Mid-exposure
JD CORR METHOD:  Light-time
JD CORRECTION:   JD = JD(raw) - 0.01253d
UNITY CORR:      -5 * log(SunDist * EarthDist): -4.0361
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: -8.520
BASE CORRECTION: -1.053
PHASE/DIST CORR: +0.179
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)
 
*********************************************************************************************
TARGET:          455 Bruchsalia
SESSION NUMBER:  258
DATE/TIME:       2008 Jun 05 @ 06:15
FILTER:          C
TELESCOPE:       0.35m SCT
FOCAL LENGTH:    135.54
CAMERA:          Alta U6 1 x binning
TEMP (C):        -30
EXPOSURE (s):    90
APPROX. RA:      13:54
APPROX. DEC:     - 1
EXPOSURE JD:     Mid-exposure
JD CORR METHOD:  Light-time
JD CORRECTION:   JD = JD(raw) - 0.01257d
UNITY CORR:      -5 * log(SunDist * EarthDist): -4.0409
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: -9.371
BASE CORRECTION: -1.904
PHASE/DIST CORR: +0.193
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)
 
*********************************************************************************************
TARGET:          455 Bruchsalia
SESSION NUMBER:  260
DATE/TIME:       2008 Jun 06 @ 06:33
FILTER:          C
TELESCOPE:       0.35m SCT
FOCAL LENGTH:    135.41
CAMERA:          Alta U6 1 x binning
TEMP (C):        -30
EXPOSURE (s):    90
APPROX. RA:      13:54
APPROX. DEC:     - 1
EXPOSURE JD:     Mid-exposure
JD CORR METHOD:  Light-time
JD CORRECTION:   JD = JD(raw) - 0.01262d
UNITY CORR:      -5 * log(SunDist * EarthDist): -4.0474
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: -8.547
BASE CORRECTION: -1.080
PHASE/DIST CORR: +0.208
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)
 
*********************************************************************************************
TARGET:          455 Bruchsalia
SESSION NUMBER:  262
DATE/TIME:       2008 Jun 07 @ 06:25
FILTER:          C
TELESCOPE:       0.35m SCT
FOCAL LENGTH:    135.51
CAMERA:          Alta U6 1 x binning
TEMP (C):        -30
EXPOSURE (s):    90
APPROX. RA:      13:53
APPROX. DEC:     - 1
EXPOSURE JD:     Mid-exposure
JD CORR METHOD:  Light-time
JD CORRECTION:   JD = JD(raw) - 0.01266d
UNITY CORR:      -5 * log(SunDist * EarthDist): -4.0521
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: -7.655
BASE CORRECTION: -0.188
PHASE/DIST CORR: +0.222
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)
 
*********************************************************************************************
TARGET:          455 Bruchsalia
SESSION NUMBER:  264
DATE/TIME:       2008 Jun 08 @ 06:04
FILTER:          C
TELESCOPE:       0.35m SCT
FOCAL LENGTH:    135.58
CAMERA:          Alta U6 1 x binning
TEMP (C):        -30
EXPOSURE (s):    90
APPROX. RA:      13:53
APPROX. DEC:     - 1
EXPOSURE JD:     Mid-exposure
JD CORR METHOD:  Light-time
JD CORRECTION:   JD = JD(raw) - 0.01270d
UNITY CORR:      -5 * log(SunDist * EarthDist): -4.0585
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: -7.523
BASE CORRECTION: -0.056
PHASE/DIST CORR: +0.236
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)
 
*********************************************************************************************
TARGET:          455 Bruchsalia
SESSION NUMBER:  268
DATE/TIME:       2008 Jun 10 @ 05:22
FILTER:          C
TELESCOPE:       0.35m SCT
FOCAL LENGTH:    135.34
CAMERA:          Alta U6 1 x binning
TEMP (C):        -30
EXPOSURE (s):    90
APPROX. RA:      13:52
APPROX. DEC:     - 2
EXPOSURE JD:     Mid-exposure
JD CORR METHOD:  Light-time
JD CORRECTION:   JD = JD(raw) - 0.01280d
UNITY CORR:      -5 * log(SunDist * EarthDist): -4.0706
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: -8.599
BASE CORRECTION: -1.132
PHASE/DIST CORR: +0.264
P/D ADJUST (-/DAY):+0.013
P/D ADJUST (+/DAY):-0.013
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:          455 Bruchsalia
SESSION NUMBER:  270
DATE/TIME:       2008 Jun 24 @ 05:43
FILTER:          C
TELESCOPE:       0.35m SCT
FOCAL LENGTH:    135.33
CAMERA:          Alta U6 1 x binning
TEMP (C):        -30
EXPOSURE (s):    90
APPROX. RA:      13:50
APPROX. DEC:     - 2
EXPOSURE JD:     Mid-exposure
JD CORR METHOD:  Light-time
JD CORRECTION:   JD = JD(raw) - 0.01353d
UNITY CORR:      -5 * log(SunDist * EarthDist): -4.1633
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: -8.280
BASE CORRECTION: -0.813
PHASE/DIST CORR: +0.446
P/D ADJUST (-/DAY):+0.012
P/D ADJUST (+/DAY):-0.012
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)
 
*********************************************************************************************