The Infrared Astrometry today

Infrared Astrometry is one of the seven subdivisions of astrometry that detects emission in the range from 0.7 to 350 μm. Specific features and some problems of this one are discussed here and more details are provided on our web site “INFRARED ASTROMETRY” with the following URL http://www.mao.kiev....

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Veröffentlicht in:Proceedings of the International Astronomical Union 2007-10, Vol.3 (S248), p.326-327
Hauptverfasser: Kharin, A. S., Vedenicheva, I. P., Zolotukhina, A. V.
Format: Artikel
Sprache:eng
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Zusammenfassung:Infrared Astrometry is one of the seven subdivisions of astrometry that detects emission in the range from 0.7 to 350 μm. Specific features and some problems of this one are discussed here and more details are provided on our web site “INFRARED ASTROMETRY” with the following URL http://www.mao.kiev.ua/IR. This web page includes 7 sections that will be expanded and regularly updated.
ISSN:1743-9213
1743-9221
DOI:10.1017/S1743921308019479