Abstract
We describe the development of a broadband astro-comb providing wavelength coverage of 500 - 620 nm, which is deployed as a wavelength calibration source for the HARPS-N spectrograph to detect and characterize long-period exoplanets.
© 2013 Optical Society of America
PDF ArticleMore Like This
Chih-Hao Li, Alexander G. Glenday, Nicholas Langellier, Alexander Zibrov, Guoqing Chang, Li-Jin Chen, Gabor Furesz, Franz Kärtner, David F. Phillips, Dimitar Sasselov, Andrew Szentgyorgyi, and Ronald L. Walsworth
CTu1I.2 CLEO: Science and Innovations (CLEO:S&I) 2013
Chih-Hao Li, Alexander G. Glenday, Guoqing Chang, Li-Jin Chen, Gabor Furesz, Nicholas Langellier, Alexander Zibrov, Franz Kärtner, David F. Phillips, Dimitar Sasselov, Andrew Szentgyorgyi, and Ronald L. Walsworth
FW5D.2 Frontiers in Optics (FiO) 2014
Guoqing Chang, Chih-Hao Li, Alexander Glenday, Gabor Furesz, Nicholas Langellier, Jinkang Lim, Hung-Wen Chen, David F. Phillips, Dimitar Sasselov, Andrew Szentgyorgyi, Ronald L. Walsworth, and Franz X. Kärtner
ATh3A.2 Advanced Solid State Lasers (ASSL) 2014