All-sky ultraviolet surveys: the needs and the means

被引:0
|
作者
Gomez de Castro, Ana I. [1 ]
Brosch, Noah [2 ]
Shustov, Boris [3 ]
机构
[1] Univ Complutense Madrid, AEGORA Res Grp, Fac CC Matemat, Plaza Ciencias 3, E-28040 Madrid, Spain
[2] Tel Aviv Univ, Tel Aviv, Israel
[3] Russian Acad Sci, Inst Astron, Pyatnitskaya 48, Moscow 119017, Russia
基金
俄罗斯科学基金会;
关键词
Ultraviolet:; general; GALAXY-EVOLUTION-EXPLORER; UV; TELESCOPES; ASTRONOMY;
D O I
10.1007/s10509-018-3412-0
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
This is a crucial time in the history of astronomy with major all-sky surveying work being carried out in all spectral bands, as well as in astrometry. The results of this activity are advancing all fields of astrophysical research, from the investigation of exo-planetary systems to the study of the chemical evolution of the Universe. Full sky surveys are available from the radio domain to X-ray wavelengths but not in the ultraviolet range (UV). While large UV missions are currently under discussion within the astrophysical community and at the major Space Agencies, the efficient use of resources requires preparatory work that can fill the UV surveying gap. This article summarizes the research and on-going activities in this field.
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页数:8
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