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The Infrared Astrometry today

Published online by Cambridge University Press:  01 October 2007

A. S. Kharin ,
I. P. Vedenicheva  and
A. V. Zolotukhina
A. S. Kharin
Affiliation:
Main Astronomical Observatory, National Academy of Sciences of Ukraine27 Akademika Zabolotnoho Str., 03680 Kiev, Ukraine email: [email protected]
I. P. Vedenicheva
Affiliation:
Main Astronomical Observatory, National Academy of Sciences of Ukraine27 Akademika Zabolotnoho Str., 03680 Kiev, Ukraine email: [email protected]
A. V. Zolotukhina
Affiliation:
Main Astronomical Observatory, National Academy of Sciences of Ukraine27 Akademika Zabolotnoho Str., 03680 Kiev, Ukraine email: [email protected]
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Abstract

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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.

Keywords

infrared: generalcatalogsastrometry
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 3 , Symposium S248: A Giant Step: from Milli- to Micro-arcsecond Astrometry , October 2007 , pp. 326 - 327
Copyright
Copyright © International Astronomical Union 2008

References

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