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For refcode 1995A&AS..114...21N:
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Copyright by European Southern Observatory (ESO). Reproduced by permission
1995A&AS..114...21N A radio continuum survey of Shapley-Ames galaxies at {lambda}2.8 cm. I. Atlas of radio data S. Niklas, U. Klein, J. Braine and R. Wielebinski Max-Planck-Institut fur Radioastronomie, Auf dem Hugel 69, D-53121 Bonn, Germany Radioastronomisches Institut, Universitat Bonn, Auf dem Hugel 71, D-53121 Bonn, Germany IRAM, 300 Rue de La Piscine, F-38406 St. Martin d'Heres, France Received April 3; accepted May 17, 1995 Abstract. - We present measurements of the radio continuum emission at {lambda}2.8 cm of a nearly complete sample of spiral galaxies. The sample consists of the Shapley-Ames galaxies north of {delta} = -25^deg^ and brighter than B_T_ = +12. The large, nearby galaxies were not observed during the survey, but measured with high sensitivity in individual projects. The radioweak galaxies were also excluded. The observational results and the derived flux densities are given and compared with that of other observations. Peculiarities of the radio emission of individual galaxies are discussed. Key words: galaxies: spiral; general - infrared: galaxies - radio continuum: galaxies
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