The Bulletin of The Korean Astronomical Society (천문학회보)
- Volume 35 Issue 1
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- Pages.36.1-36.1
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- 2010
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- 1226-2692(pISSN)
Introduction of High Resolution Spectrograph by using Optical Freauency Comb.
- Han, In-Woo (Korea Astronomy and Space Science Institute) ;
- Kim, Kang-Min (Korea Astronomy and Space Science Institute) ;
- Yoon, Tai-Hyun (Korea University)
- Published : 2010.04.06
Abstract
OFC (Optical Frequency Comb) is an optical spectrum which consists of equidistant lines in frequency space. OFC can thus be used as an optical ruler. Since it was demonstrated in late 1990s, it is revolutionizing many fields in frequency metrology such as the measurement of absolute optical frequencies, the measure ratios of optical frequencies with extremely high precision. It is also used in high-precision spectroscopy. In astronomy, OFC can be used as a very accurate and stable wavelength standard for a high resolution spectrograph to measure the radial velocity of celestial bodies with extremely high accuracy of about several tens cm/s. In our presentation, we will introduce some basic concepts of OFC and some issues to use it in astronomical spectrograph. We will also present our plan to develop a high resolution spectrograph with OFC.
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