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A&A Supplement Series, Vol. 126, December I 1997, 325-334

Received January 19; accepted March 10, 1997

A catalogue of compact radio sources in and behind the Large Magellanic Cloudgif

M. Marxtex2html_wrap1189, J.M. Dickeytex2html_wrap1191, and U. Meboldtex2html_wrap1189

Send offprint request: M. Marx
tex2html_wrap1195  Radioastronomisches Institut der Universität Bonn, Auf dem Hügel 71, D-53121 Bonn, Germany
tex2html_wrap1195  Department of Astronomy, University of Minnesota, Minneapolis, Minnesota 55455, U.S.A.


We present the results of a continuum snapshot survey of a tex2html_wrap_inline1167 region of the Large Magellanic Cloud including the area of the giant molecular cloud and the 30 Doradus nebula. The observations have been carried out with the Australia Telescope Compact Array (ATCA)gif at 1.4 and 2.4 GHz. Most fields are complete to about 6 mJy peak flux density at 1.4 GHz and to about 3 mJy at 2.4 GHz. The positions, peak and integral flux densities of 113 compact (< 54'') sources detected at 1.4 GHz and of 70 sources (<34'') detected at 2.4 GHz are presented. Positions are accurate to about 3'' and peak flux densities are accurate to about 10% or better, depending on the source position relative to the pointing centers. 32 of the sources detected at 1.4 GHz are coincident with Htex2html_wrap_inline1175 objects in the catalogue of Davies et al.; these are possibly intrinsic to the LMC. However, we suppose that most are background objects, since the number vs. flux agrees with predictions of extragalactic source counts from other surveys.

keywords: Magellanic Clouds -- radio continuum: galaxies -- surveys -- HII regions -- methods: statistical

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