pdosmall.gif (6581 bytes)

The Minor Planet Observer
and
Palmer Divide Observatory

2007 Shoemaker Grant Recipient

Planetary.gif (18781 bytes)

 

External Links
(opens new window)

Buy MPO Software

MPO Support

CALL web site

Society for Astronomical Sciences

99999999999999999999

 

Binzel Method - Target Field

PRSimpTargetField.gif (79664 bytes)

By measuring a series of C and V images of the target field (comparisons and targets), you find several values that help reduce to standard magnitudes.

  1. The average differential value in C between target and the comparisons (<Diff> in the Reductions Values form)

  2. The average instrumental magnitude of the target in V (<Std Inst> in the Reductions Values form).

  3. The "anchor point" in V, which is found using the <Std Inst> and Ref Offset values in the Reductions Values form.

  4. The shift required to convert the value from step 1 to the value in step 3 (assuming the target was the same brightness in all measurements). This shift is stored in the Std. Shift field of the Reductions Values form.

Once all these values are found and saved, it's easy to convert C observations of the target to the Johnson V system.

 

This site is best viewed at 1024x768 and higher

This page was last updated on 01/19/11 05:14 -0700.
All contents copyright (c) 2005-2011, Brian D. Warner
Trademarks are the property of their respective owners