Searching for exoplanets using a microresonator astrocomb

Orbiting planets induce a weak radial velocity (RV) shift in the host star that provides a powerful method of planet detection. Importantly, the RV technique provides information about the exoplanet mass, which is unavailable with the complementary technique of transit photometry. However, RV detect...

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Veröffentlicht in:	Nature photonics 2019-01, Vol.13 (1), p.25-30
Hauptverfasser:	Suh, Myoung-Gyun, Yi, Xu, Lai, Yu-Hung, Leifer, S., Grudinin, Ivan S., Vasisht, G., Martin, Emily C., Fitzgerald, Michael P., Doppmann, G., Wang, J., Mawet, D., Papp, Scott B., Diddams, Scott A., Beichman, C., Vahala, Kerry
Format:	Artikel
Sprache:	eng
Schlagworte:	140/125 639/624 639/624/1075/1079 639/624/400/1118 639/624/400/385 Applied and Technical Physics Celestial bodies Extrasolar planets Filtration Letter Photometry Physics Physics and Astronomy Planet detection Power consumption Quantum Physics Radial velocity Spectrographs
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