When observing through the atmosphere, the apparent position of an object is biased because of differential color refraction.
The bias is a function of the color of the observed target (which is generally unknown) and that of the stars used for the astrometric solution.
The bias is larger at lower elevation.
This term is to be computed by observers, when feasible.
ADES should have a note to specify that the observation was in fact color corrected and the correction should be reported in the remarks field.
When observing through the atmosphere, the apparent position of an object is biased because of differential color refraction. The bias is a function of the color of the observed target (which is generally unknown) and that of the stars used for the astrometric solution. The bias is larger at lower elevation.
This term is to be computed by observers, when feasible. ADES should have a note to specify that the observation was in fact color corrected and the correction should be reported in the remarks field.