4.7 Article

The Edinburgh-Cape Blue Object Survey - III. Zone 2; galactic latitudes-30° > b >-40°

Journal

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
Volume 431, Issue 1, Pages 240-251

Publisher

OXFORD UNIV PRESS
DOI: 10.1093/mnras/stt158

Keywords

surveys; stars: early-type; stars: horizontal branch; subdwarfs; white dwarfs; quasars: general

Funding

  1. National Research Foundation
  2. University of the Western Cape, South Africa
  3. STFC [ST/H004211/1, ST/H000496/1, ST/K001116/1, ST/H00047X/1, ST/L001136/1] Funding Source: UKRI
  4. Science and Technology Facilities Council [ST/K001116/1, ST/H004211/1, ST/H000496/1, ST/H00047X/1, ST/L001136/1] Funding Source: researchfish

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The Edinburgh-Cape Blue Object Survey seeks to identify point sources with an ultraviolet excess. Results for zone 2 of the survey are presented here, covering that part of the South Galactic Cap between 30 degrees and 40 degrees from the Galactic plane and south of about -12 degrees.3 of declination. Edinburgh-Cape zone 2 comprises 66 UK Schmidt Telescope fields covering about 1730 deg(2), in which we find some 892 blue objects, including 423 hot subdwarfs (similar to 47 per cent); 128 white dwarfs (similar to 14 per cent); 25 cataclysmic variables (similar to 3 per cent); 119 binaries (similar to 13 per cent), mostly composed of a hot subdwarf and a main-sequence F or G star; 66 horizontal branch stars (similar to 7 per cent) and 48 'star-like' extragalactic objects (similar to 5 per cent). A further 362 stars observed in the survey, mainly low-metallicity F- and G-type stars, are also listed. Both low-dispersion spectroscopic classification and UBV photometry are presented for almost all of the hot objects and either spectroscopy or photometry (or both) for the cooler ones.

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