Model of foreground screen for large field radioastronomical data reduction

Details Model of foreground screen for large field radioastronomical data reduction Model of foreground screen for large field radioastronomical data reduction

Aug 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006iaujd..16e..58r&link_type=abstract

Nomenclature, Precession and New Models in Fundamental Astronomy, 26th meeting of the IAU, Joint Discussion 16, 22-23 August 200

Astronomy and Astrophysics

Astronomy

Scientific paper

Here we present an improved model of atmospheric radio-wave radiation, which seem us to be more useful than models frequently presented in the radioastronomical literature. The model was fitted to the data from 32-m Torun radiotelescope and used during the data reduction of our polarimetric survey of the Milky Way. We also detect a polarized component from the atmospheric foreground which seems to be independent of Earth surface radiation.

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