The UV-Excess survey of the northern Galactic plane |
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| Authors: | C. R. Purcell S. N. Longmore M. G. Burton A. J. Walsh V. Minier M. R. Cunningham R. Balasubramanyam |
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| Affiliation: | University of Manchester, Jodrell Bank Observatory, Macclesfield, Cheshire SK11 9DL;School of Physics, University of New South Wales, Sydney, NSW 2052, Australia;Harvard–Smithsonian Center For Astrophysics, 60 Garden Street, Cambridge, MA 02138, USA;CSIRO Australia Telescope National Facility, PO Box 76, Epping, NSW 1710, Australia;Centre for Astronomy, James Cook University, Townsville, QLD 4811, Australia;Service d'Astrophysique, DAPNIA/DSM/CEA Saclay, 91191 Gif-sur-Yvette, France;AIM, UnitéMixte de Recherche, CEA-CNRS-UniversitéParis VII, UMR 7158, CEA/Saclay, 91191 Gif-sur-Yvette, France;Raman Research Institute, Sadashivanagar, Bangalore 560 080, India |
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| Abstract: | The UV-Excess survey of the northern Galactic plane images a 10°× 185° wide band, centred on the Galactic equator using the 2.5-m Isaac Newton Telescope in four bands ( i 5875) down to ∼21–22 mag ( in i 5875). The setup and data reduction procedures are described. Simulations of the colours of main-sequence stars, giant, supergiants, DA and DB white dwarfs and AM Canum Venaticorum stars are made, including the effects of reddening. A first look at the data of the survey (currently 30 per cent complete) is given. |
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| Keywords: | surveys stars: formation stars: pre-main-sequence ISM: abundances ISM: molecules |
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