The UV-Excess survey of the northern Galactic plane
The UV-Excess survey of the northern Galactic plane
复制标题
银河系北部平面的紫外线过量调查
DOI：
10.1111/j.1365-2966.2009.15273.x
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发表时间：
2009
影响因子：
4.8
通讯作者：
Groot P
中科院分区：
文献类型：
--
作者：
Groot P
对北方银道面进行的紫外线过量巡天观测，利用2.5米艾萨克·牛顿望远镜在银道赤道上拍摄了一个10°× 185°宽的波段，波段范围从21等到22等（i 5875）。描述了设置和数据简化过程。模拟了主序星、巨星、超巨星、DA和DB白色矮星和AM犬座星的颜色，包括变红的影响。对调查数据（目前已完成30%）作了初步介绍。
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.