TARGET:          1194 Aletta
SESSION NUMBER:  103
DATE/TIME:       2007 Nov 13 @ 05:09
FILTER:          C
TELESCOPE:       300 mm f11.5 cass
FOCAL LENGTH:    136.92
CAMERA:          AltaU6 1x bin
TEMP (C):        -30
EXPOSURE (s):    240
APPROX. RA:      22:43
APPROX. DEC:     + 5
EXPOSURE JD:     Mid-exposure
JD CORR METHOD:  Light-time
JD CORRECTION:   JD = JD(raw) - 0.01534d
UNITY CORR:      -5 * log(SunDist * EarthDist): -4.6383
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: -7.453
BASE CORRECTION: +0.000
PHASE/DIST CORR: +0.000
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:          1194 Aletta
SESSION NUMBER:  106
DATE/TIME:       2007 Nov 14 @ 05:14
FILTER:          C
TELESCOPE:       300 mm f11.5 cass
FOCAL LENGTH:    136.92
CAMERA:          AltaU6 1x bin
TEMP (C):        -30
EXPOSURE (s):    240
APPROX. RA:      22:44
APPROX. DEC:     + 5
EXPOSURE JD:     Mid-exposure
JD CORR METHOD:  Light-time
JD CORRECTION:   JD = JD(raw) - 0.01542d
UNITY CORR:      -5 * log(SunDist * EarthDist): -4.6489
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: -7.575
BASE CORRECTION: -0.122
PHASE/DIST CORR: +0.014
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:          1194 Aletta
SESSION NUMBER:  109
DATE/TIME:       2007 Nov 15 @ 05:02
FILTER:          C
TELESCOPE:       300 mm f11.5 cass
FOCAL LENGTH:    136.92
CAMERA:          AltaU6 1x bin
TEMP (C):        -30
EXPOSURE (s):    240
APPROX. RA:      22:44
APPROX. DEC:     + 5
EXPOSURE JD:     Mid-exposure
JD CORR METHOD:  Light-time
JD CORRECTION:   JD = JD(raw) - 0.01549d
UNITY CORR:      -5 * log(SunDist * EarthDist): -4.6595
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: -7.660
BASE CORRECTION: -0.207
PHASE/DIST CORR: +0.029
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:          1194 Aletta
SESSION NUMBER:  112
DATE/TIME:       2007 Nov 16 @ 04:56
FILTER:          C
TELESCOPE:       300 mm f11.5 cass
FOCAL LENGTH:    136.92
CAMERA:          AltaU6 1x bin
TEMP (C):        -30
EXPOSURE (s):    240
APPROX. RA:      22:44
APPROX. DEC:     + 5
EXPOSURE JD:     Mid-exposure
JD CORR METHOD:  Light-time
JD CORRECTION:   JD = JD(raw) - 0.01557d
UNITY CORR:      -5 * log(SunDist * EarthDist): -4.6700
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: -8.060
BASE CORRECTION: -0.607
PHASE/DIST CORR: +0.043
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)
 
*********************************************************************************************
 
-------------------------------------------
  J.D.          Obj-CAvg    Err    Session
-------------------------------------------
2454417.58809     +1.868   0.024       103
2454417.59504     +1.907   0.025       103
2454417.60200     +1.925   0.024       103
2454417.61229     +1.864   0.022       103
2454417.61942     +1.877   0.023       103
2454417.62656     +1.927   0.024       103
2454417.63369     +1.983   0.025       103
2454417.64083     +2.000   0.027       103
2454417.64866     +1.981   0.025       103
2454417.65579     +2.043   0.025       103
2454417.66293     +1.974   0.024       103
2454417.67006     +2.016   0.025       103
2454417.67720     +2.007   0.026       103
2454417.68503     +1.994   0.025       103
2454417.69216     +2.027   0.027       103
2454417.69931     +2.003   0.025       103
2454417.70644     +2.009   0.025       103
2454417.71358     +1.947   0.028       103
2454417.72143     +1.959   0.025       103
2454417.72857     +1.956   0.026       103
2454417.73573     +1.915   0.026       103
2454417.74286     +1.905   0.026       103
2454417.75000     +1.881   0.026       103
2454417.75784     +1.940   0.029       103
2454417.76499     +1.883   0.027       103
2454417.77215     +1.862   0.027       103
2454417.77931     +1.890   0.029       103
2454417.78647     +1.866   0.029       103
2454417.79432     +1.811   0.028       103
2454417.80147     +1.808   0.031       103
2454418.60083     +1.841   0.023       106
2454418.60807     +1.803   0.022       106
2454418.61524     +1.840   0.023       106
2454418.62240     +1.865   0.023       106
2454418.62957     +1.842   0.023       106
2454418.64215     +1.804   0.022       106
2454418.64929     +1.781   0.021       106
2454418.65642     +1.809   0.021       106
2454418.67141     +1.731   0.021       106
2454418.67856     +1.726   0.021       106
2454418.68574     +1.693   0.020       106
2454418.69299     +1.723   0.021       106
2454418.70013     +1.691   0.020       106
2454418.70800     +1.728   0.021       106
2454418.71517     +1.732   0.022       106
2454418.72233     +1.684   0.020       106
2454418.72950     +1.758   0.021       106
2454418.73666     +1.740   0.022       106
2454418.74451     +1.747   0.022       106
2454418.75170     +1.766   0.024       106
2454418.75887     +1.753   0.024       106
2454418.76601     +1.741   0.024       106
2454418.77315     +1.746   0.024       106
2454418.78101     +1.754   0.026       106
2454418.78815     +1.728   0.025       106
2454418.79532     +1.728   0.027       106
2454419.58556     +1.768   0.020       109
2454419.59273     +1.792   0.020       109
2454419.59992     +1.778   0.023       109
2454419.61231     +1.845   0.021       109
2454419.62009     +1.839   0.021       109
2454419.62782     +1.813   0.020       109
2454419.63558     +1.819   0.020       109
2454419.64331     +1.825   0.020       109
2454419.65173     +1.834   0.021       109
2454419.65946     +1.837   0.020       109
2454419.66719     +1.831   0.021       109
2454419.67490     +1.866   0.022       109
2454419.68261     +1.833   0.021       109
2454419.69102     +1.772   0.020       109
2454419.69874     +1.815   0.020       109
2454419.70645     +1.847   0.021       109
2454419.71417     +1.882   0.022       109
2454419.72190     +1.970   0.029       109
2454419.73031     +1.970   0.025       109
2454419.73802     +1.940   0.024       109
2454419.74574     +1.986   0.026       109
2454419.75345     +2.003   0.029       109
2454419.76117     +2.030   0.028       109
2454419.76958     +2.064   0.029       109
2454419.77730     +2.120   0.033       109
2454419.78502     +2.083   0.033       109
2454420.57623     +1.928   0.025       112
2454420.58400     +2.005   0.027       112
2454420.59175     +1.978   0.025       112
2454420.59948     +2.008   0.027       112
2454420.60719     +2.042   0.027       112
2454420.61562     +1.953   0.025       112
2454420.62334     +2.048   0.027       112
2454420.63107     +2.044   0.028       112
2454420.63879     +2.038   0.027       112
2454420.64651     +2.028   0.027       112
2454420.65493     +1.995   0.024       112
2454420.66266     +2.079   0.026       112
2454420.67038     +2.097   0.028       112
2454420.69163     +2.012   0.025       112
2454420.69935     +2.036   0.027       112
2454420.70708     +1.988   0.025       112
2454420.71478     +1.974   0.025       112
2454420.73095     +1.904   0.023       112
2454420.73868     +1.945   0.025       112
2454420.74640     +1.870   0.024       112
2454420.75412     +1.912   0.025       112
2454420.76185     +1.814   0.024       112
2454420.77026     +1.818   0.024       112
2454420.77800     +1.826   0.027       112
2454420.78572     +1.854   0.027       112
2454420.79345     +1.861   0.032       112
 
END OF FIXED DATA SECTION. DO NOT MAKE ANY CHANGES ABOVE THIS LINE.

 

 

 

Contents © 2008 James W Brinsfield / Via Capote Observatory