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10.2 Corrections to the PA-profiles

Note: in this section, we will use primes to denote the CCD coordinate system, to keep the notation consistent with that of the astrometry section (Sect. [*], p. [*]). For example, we will use the term ``the CCD x'-axis'', or just ``the x'-axis'', to denote what would otherwise just be called ``the CCD x-axis''. Unprimed quantities will refer to the ideal plate coordinate system.



 

Properties of E and S0 Galaxies in the Clusters HydraI and Coma
Master's Thesis, University of Copenhagen, July 1997

Bo Milvang-Jensen (milvang@astro.ku.dk)