4.7 Article

The UV-Excess survey of the northern Galactic plane

期刊

出版社

WILEY-BLACKWELL
DOI: 10.1111/j.1365-2966.2009.15273.x

关键词

surveys; stars: general; ISM: general; Galaxy: disc; Galaxy: stellar content; Galaxy: structure

资金

  1. Science and Technology Facilities Council [PP/D00148X/1, ST/H001913/1, ST/F003277/1, PP/E003435/1, ST/G003084/1, PP/D005914/1, ST/H004157/1, PP/C002229/1, ST/G002622/1, ST/F003196/1, ST/F002599/1, ST/H004165/1] Funding Source: researchfish
  2. UK Space Agency [ST/H00002X/1] Funding Source: researchfish
  3. STFC [PP/D005914/1, PP/E003435/1, ST/F002599/1, PP/C002229/1, ST/F003196/1, ST/H001913/1, PP/D00148X/1, ST/G003084/1, ST/H004157/1, ST/F003277/1, ST/H004165/1, ST/G002622/1] Funding Source: UKRI

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The UV-Excess survey of the northern Galactic plane images a 10 degrees x 185 degrees wide band, centred on the Galactic equator using the 2.5-m Isaac Newton Telescope in four bands (U, g, r, He 15875) down to similar to 21-22 mag (similar to 20 in He 15875). 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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