The Edinburgh-Cape Blue Object Survey - I. Description of the survey


Autoria(s): Stobie, R. S.; Kilkenny, D.; O'Donoghue, D.; Chen, A.; Koen, C.; Morgan, D. H.; Barrow, J.; Buckley, D. A. H.; Cannon, R. D.; Cass, C. J. P.; Cranston, M. R.; Drinkwater, M.; Hartley, M.; Hawkins, M. R. S.; Hughes, S.; Humphries, C. M.; MacGillivray, H. T.; McKenzie, P. B.; Parker, Q. A.; Read, M.; Russell, K. S.; Savage, A.; Thomson, E. B.; Tritton, S. B.; Waldron, J. D.; Warner, B.; Watson, F. G.
Data(s)

01/06/1997

Resumo

The Edinburgh-Cape Blue Object Survey is a major survey to discover blue stellar objects brighter than B similar to 18 in the southern sky. It is planned to cover an area of sky of 10 000 deg(2) with \b\ > 30 degrees and delta < 0 degrees. The blue stellar objects are selected by automatic techniques from U and B pairs of UK Schmidt Telescope plates scanned with the COSMOS measuring machine. Follow-up photometry and spectroscopy are being obtained with the SAAO telescopes to classify objects brighter than B = 16.5. This paper describes the survey, the techniques used to extract the blue stellar objects, the photometric methods and accuracy, the spectroscopic classification, and the limits and completeness of the survey.

Identificador

http://espace.library.uq.edu.au/view/UQ:57705

Idioma(s)

eng

Publicador

Blackwell Scientific

Palavras-Chave #Astronomy & Astrophysics #Surveys #Stars, Early-type #Stars, Horizontal Branch #Subdwarfs #White Dwarfs #Quasars, General #High Galactic Latitudes #Star-count Data #White-dwarf #Stellar Objects #Catalog #Spectra #System #Bright #Pole #0201 Astronomical and Space Sciences
Tipo

Journal Article