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...

Disgrifiad llawn

Wedi'i Gadw mewn:
Manylion Llyfryddiaeth
Cyhoeddwyd yn:Nat Photonics
Prif Awduron: 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
Fformat: Artigo
Iaith:Inglês
Cyhoeddwyd: 2018
Pynciau:
Article
Mynediad Ar-lein:https://ncbi.nlm.nih.gov/pmc/articles/PMC6364311/
https://ncbi.nlm.nih.gov/pubmed/30740138
https://ncbi.nlm.nih.govhttp://dx.doi.org/10.1038/s41566-018-0312-3
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