TARGET:          4483 Petofi
SESSION NUMBER:  76
DATE/TIME:       2007 Jul 16 @ 07:32
FILTER:          C
TELESCOPE:       300 mm f11.5 cass
FOCAL LENGTH:    136.43
CAMERA:          AltaU6 1x bin
TEMP (C):        -30
EXPOSURE (s):    180
APPROX. RA:      16:47
APPROX. DEC:     +23
EXPOSURE JD:     Mid-exposure
JD CORR METHOD:  Light-time
JD CORRECTION:   JD = JD(raw) - 0.00708d
UNITY CORR:      -5 * log(SunDist * EarthDist): -1.8754
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: -7.477
BASE CORRECTION: +0.000
PHASE/DIST CORR: +0.000
P/D ADJUST (-/DAY):+0.011
P/D ADJUST (+/DAY):-0.011
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:          4483 Petofi
SESSION NUMBER:  77
DATE/TIME:       2007 Jul 17 @ 07:31
FILTER:          C
TELESCOPE:       300 mm f11.5 cass
FOCAL LENGTH:    136.91
CAMERA:          AltaU6 1x bin
TEMP (C):        -30
EXPOSURE (s):    180
APPROX. RA:      16:47
APPROX. DEC:     +22
EXPOSURE JD:     Mid-exposure
JD CORR METHOD:  Light-time
JD CORRECTION:   JD = JD(raw) - 0.00711d
UNITY CORR:      -5 * log(SunDist * EarthDist): -1.8813
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: -8.125
BASE CORRECTION: -0.648
PHASE/DIST CORR: +0.011
P/D ADJUST (-/DAY):+0.011
P/D ADJUST (+/DAY):-0.011
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
-------------------------------------------
2454297.73773     +2.831   0.037        76
2454297.74313     +2.817   0.035        76
2454297.74854     +2.621   0.027        76
2454297.75394     +2.408   0.023        76
2454297.75935     +2.249   0.020        76
2454297.76475     +2.104   0.018        76
2454297.77016     +1.983   0.016        76
2454297.77557     +1.952   0.016        76
2454297.78097     +1.923   0.015        76
2454297.78638     +1.915   0.016        76
2454297.79254     +1.958   0.016        76
2454297.79794     +2.021   0.017        76
2454297.80334     +2.173   0.020        76
2454297.80876     +2.383   0.024        76
2454297.81417     +2.571   0.029        76
2454297.81957     +2.788   0.035        76
2454297.82497     +2.806   0.036        76
2454297.83039     +2.693   0.033        76
2454297.83580     +2.533   0.029        76
2454297.84120     +2.461   0.029        76
2454297.84735     +2.316   0.027        76
2454297.85277     +2.264   0.025        76
2454297.85817     +2.137   0.023        76
2454297.86358     +1.990   0.021        76
2454297.86898     +1.944   0.021        76
2454297.87439     +1.912   0.021        76
2454298.73428     +2.580   0.040        77
2454298.73967     +2.557   0.039        77
2454298.74508     +2.411   0.035        77
2454298.75047     +2.324   0.033        77
2454298.75586     +2.168   0.028        77
2454298.76125     +2.116   0.026        77
2454298.76664     +2.033   0.025        77
2454298.77203     +1.922   0.024        77
2454298.77742     +1.923   0.024        77
2454298.78281     +1.921   0.024        77
2454298.78893     +1.968   0.026        77
2454298.79432     +2.116   0.030        77
2454298.79970     +2.245   0.036        77
2454298.80834     +2.412   0.054        77
2454298.81373     +2.494   0.091        77
2454298.81912     +2.818   0.099        77
2454298.82451     +2.809   0.181        77
2454298.82989     +2.365   0.181        77
2454298.83528     +2.423   0.072        77
2454298.84466     +2.273   0.054        77
2454298.85004     +2.117   0.045        77
2454298.85543     +2.019   0.040        77
2454298.86082     +1.938   0.039        77
2454298.86620     +1.879   0.039        77
 
END OF FIXED DATA SECTION. DO NOT MAKE ANY CHANGES ABOVE THIS LINE.

 

 

 

Contents © 2008 James W Brinsfield / Via Capote Observatory