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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Detalles Bibliográficos
Autores principales: 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
Formato: Online Artículo Texto
Lenguaje:English
Publicado: 2018
Materias:
Article
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC6364311/
https://www.ncbi.nlm.nih.gov/pubmed/30740138
http://dx.doi.org/10.1038/s41566-018-0312-3

Internet

https://www.ncbi.nlm.nih.gov/pmc/articles/PMC6364311/
https://www.ncbi.nlm.nih.gov/pubmed/30740138
http://dx.doi.org/10.1038/s41566-018-0312-3

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