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Solving for closure errors due to polarization leakage in radio interferometry of unpolarized sources

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arxiv astro-ph/0106348 v1 pith:PJCSKGBE submitted 2001-06-20 astro-ph

classification astro-ph
keywords closureleakageunpolarizederrorspolarizationradiosourcesco-polar
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Mechanical and electronic imperfections can result into polarization leakage in individual antennas of a radio interferometer. Such leakages manifest themselves as closure errors even in co-polar visibility measurements of unpolarized sources. This paper describes and tests a method for the study of polarization leakage for radio interferometric telescopes using {\it only} the nominally co-polar visibilities for unpolarized calibrators. Interpretation of the resulting closure phases on the Poincar\'e sphere is presented. Since unpolarized sources are used, the actual solutions for leakage parameters is subject to a degeneracy which is discussed. This however, does not affect the correction of closure errors in our scheme.

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Cited by 2 Pith papers

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  1. The Southern-sky MWA Rapid Two-metre (SMART) pulsar survey--IV. Survey update and an atlas of 205 non-recycled southern pulsars

    astro-ph.HE 2026-07 accept novelty 6.0 of 10

    Atlas of 205 non-recycled southern pulsars at 140–170 MHz from MWA SMART data, with profiles, DMs, RMs, fluxes and public data products for SKA-Low.

  2. Measuring Magnetic Field Strengths in Galactic Star-forming Regions via the Zeeman Effect with the SKA

    astro-ph.GA 2026-06 unverdicted novelty 2.0 of 10

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