Radio Identifications of UGC Galaxies - Starbursts and Monsters

Details Radio Identifications of UGC Galaxies - Starbursts and Monsters Radio Identifications of UGC Galaxies - Starbursts and Monsters

Nov 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995adil...jc...01c&link_type=abstract

NCSA Astronomy Digital Image Library

Astronomy and Astrophysics

Astronomy

Astronomical Catalogs, Black Holes (Astronomy), Galactic Clusters, Radio Galaxies, Sky Surveys (Astronomy), Spiral Galaxies, Starburst Galaxies, Very Large Array (Vla)

Scientific paper

Radio identifications of galaxies in the Uppsala General Catalogue of Galaxies with delta < +82 degrees were made from the Green Bank 1400 MHz sky maps. Every source having peak flux density S(P) >= 150 mJy in the approximately 12 arcmin FWHM map point-source response and position < 5 arcmin in both coordinates from the optical position of any UGC galaxy was considered a candidate identification to ensure that very extended (up to 1 Mpc) and asymmetric sources would not be missed. Maps in the literature or new 1.49 GHz VLA C-array maps made with 18 arcsec FWHM resolution were used to confirm or reject candidate identifications. The maps in this directory include both confirmed identifications and candidates rejected because of confusion or low flux density. For more information on this study, please see the following reference: Condon, J. J., and Broderick, J. J., 1988, AJ, 96, 30. The images and related TeX file come from the NRAO CDROM "Images From the Radio Universe" (c. 1992 National Radio Astronomy Observatory, used with permission).

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