TARGET:          7304 Namiki
SESSION NUMBER:  50
DATE/TIME:       2007 May 15 @ 04:51
FILTER:          C
TELESCOPE:       300 mm f11.5 cass
FOCAL LENGTH:    136.27
CAMERA:          AltaU6 1x bin
TEMP (C):        -30
EXPOSURE (s):    120
APPROX. RA:      14:30
APPROX. DEC:     +10
EXPOSURE JD:     Mid-exposure
JD CORR METHOD:  Light-time
JD CORRECTION:   JD = JD(raw) - 0.00317d
UNITY CORR:      -5 * log(SunDist * EarthDist): 0.4119
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: -7.849
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:          7304 Namiki
SESSION NUMBER:  57
DATE/TIME:       2007 May 19 @ 09:53
FILTER:          C
TELESCOPE:       300 mm f11.5 cass
FOCAL LENGTH:    136.50
CAMERA:          AltaU6 1x bin
TEMP (C):        -30
EXPOSURE (s):    120
APPROX. RA:      14:30
APPROX. DEC:     + 9
EXPOSURE JD:     Mid-exposure
JD CORR METHOD:  Light-time
JD CORRECTION:   JD = JD(raw) - 0.00322d
UNITY CORR:      -5 * log(SunDist * EarthDist): 0.3777
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: -8.362
BASE CORRECTION: -0.513
PHASE/DIST CORR: +0.069
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:          7304 Namiki
SESSION NUMBER:  59
DATE/TIME:       2007 May 20 @ 04:35
FILTER:          C
TELESCOPE:       300 mm f11.5 cass
FOCAL LENGTH:    136.55
CAMERA:          AltaU6 1x bin
TEMP (C):        -30
EXPOSURE (s):    120
APPROX. RA:      14:30
APPROX. DEC:     + 9
EXPOSURE JD:     Mid-exposure
JD CORR METHOD:  Light-time
JD CORRECTION:   JD = JD(raw) - 0.00323d
UNITY CORR:      -5 * log(SunDist * EarthDist): 0.3738
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: -8.512
BASE CORRECTION: -0.663
PHASE/DIST CORR: +0.083
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)
 
*********************************************************************************************
 
-------------------------------------------
  J.D.          Obj-CAvg    Err    Session
-------------------------------------------
2454235.66778     +0.997   0.013        50
2454235.67182     +0.970   0.012        50
2454235.67584     +0.976   0.011        50
2454235.67988     +0.952   0.011        50
2454235.68392     +0.934   0.011        50
2454235.68848     +0.882   0.010        50
2454235.69252     +0.857   0.010        50
2454235.69656     +0.777   0.009        50
2454235.70060     +0.727   0.008        50
2454235.70459     +0.696   0.008        50
2454235.70910     +0.618   0.008        50
2454235.71309     +0.556   0.007        50
2454235.71708     +0.513   0.007        50
2454235.72107     +0.450   0.006        50
2454235.72515     +0.426   0.006        50
2454239.86160     +0.470   0.006        57
2454239.86560     +0.524   0.007        57
2454239.86960     +0.582   0.007        57
2454239.87359     +0.630   0.007        57
2454239.87758     +0.719   0.008        57
2454239.88210     +0.805   0.009        57
2454239.88610     +0.835   0.009        57
2454239.89009     +0.889   0.009        57
2454239.89409     +0.930   0.010        57
2454239.89809     +0.977   0.011        57
2454239.90261     +1.018   0.012        57
2454239.90660     +1.031   0.013        57
2454239.91060     +1.065   0.014        57
2454239.91460     +1.055   0.015        57
2454239.91859     +1.042   0.015        57
2454239.92710     +1.017   0.014        57
2454239.93110     +0.989   0.015        57
2454239.93510     +0.925   0.015        57
2454239.93910     +0.873   0.014        57
2454239.94364     +0.846   0.015        57
2454239.94764     +0.795   0.015        57
2454239.95164     +0.724   0.015        57
2454240.65804     +1.079   0.015        59
2454240.66206     +1.078   0.013        59
2454240.66607     +1.030   0.012        59
2454240.67006     +0.996   0.011        59
2454240.67405     +0.936   0.010        59
2454240.67856     +0.921   0.010        59
2454240.68510     +0.846   0.009        59
2454240.68910     +0.794   0.009        59
2454240.69309     +0.722   0.008        59
2454240.69758     +0.674   0.008        59
2454240.70160     +0.614   0.007        59
2454240.70561     +0.583   0.007        59
2454240.70816     +0.546   0.007        59
2454240.71215     +0.496   0.007        59
2454240.71668     +0.463   0.006        59
 
END OF FIXED DATA SECTION. DO NOT MAKE ANY CHANGES ABOVE THIS LINE.

 

 

 

Contents © 2008 James W Brinsfield / Via Capote Observatory