A simple method of correcting magnitudes for the errors introduced by atmospheric refraction

Simple item page
dc.creatorKruszewski, A.
dc.creatorSemeniuk, I.
dc.date2003-11-26
dc.date.accessioned2026-07-07T02:11:21Z
dc.date.available2026-07-07T02:11:21Z
dc.descriptionWe show that the errors due to atmospheric refraction are present in the magnitudes determined with the Difference Images Analysis method. In case of single, unblended stars the size of the effect agrees with the theoretical prediction. But when the blending is strong, what is quite common in a dense field, then the effect of atmospheric refraction can be strongly amplified to the extend that some cases of apparently variable stars with largest amplitudes of variations are solely due to refraction. We present a simple method of correcting for this kind of errors.
dc.description8 pages, 3 figures, accepted for publication in Acta Astronomica
dc.identifierhttps://arxiv.org/abs/astro-ph/0311588
dc.identifierhttp://arxiv.org/abs/astro-ph/0311588
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/7052
dc.subjectAstrophysics
dc.titleA simple method of correcting magnitudes for the errors introduced by atmospheric refraction
dc.typetext

Files

Collections

arXiv