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Searching for Exoplanets Using a Microresonator Astrocomb

Suh, Myoung-Gyun and Yi, Xu and Lai, Yu-Hung and Leifer, S. and Grudinin, Ivan S. and Vasisht, G. and Martin, Emily C. and Fitzgerald, Michael P. and Doppmann, G. and Wang, J. and Mawet, D. and Papp, Scott B. and Diddams, Scott A. and Beichman, C. and Vahala, Kerry (2019) Searching for Exoplanets Using a Microresonator Astrocomb. Nature Photonics, 13 (1). pp. 25-30. ISSN 1749-4885. http://resolver.caltech.edu/CaltechAUTHORS:20180119-080155783

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Abstract

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 detection of an Earth-like planet in the ‘habitable zone’ requires extreme spectroscopic precision that is only possible using a laser frequency comb (LFC). Conventional LFCs require complex filtering steps to be compatible with astronomical spectrographs, but a new chip-based microresonator device, the Kerr soliton microcomb, is an ideal match for astronomical spectrograph resolution and can eliminate these filtering steps. Here, we demonstrate an atomic/molecular line-referenced soliton microcomb for calibration of astronomical spectrographs. These devices can ultimately provide LFC systems that would occupy only a few cubic centimetres, thereby greatly expanding implementation of these technologies into remote and mobile environments beyond the research lab.


Item Type:Article
Related URLs:
URLURL TypeDescription
https://doi.org/10.1038/s41566-018-0312-3DOIArticle
https://rdcu.be/bdIpWPublisherFree ReadCube access
https://arxiv.org/abs/1801.05174arXivDiscussion Paper
ORCID:
AuthorORCID
Suh, Myoung-Gyun0000-0002-9527-0585
Yi, Xu0000-0002-2485-1104
Fitzgerald, Michael P.0000-0002-0176-8973
Mawet, D.0000-0002-8895-4735
Diddams, Scott A.0000-0002-2144-0764
Vahala, Kerry0000-0003-1783-1380
Additional Information:© 2018 Springer Nature Publishing AG. Received 29 April 2018; Accepted 05 November 2018; Published 14 December 2018. We gratefully acknowledge J. Schlieder, A. Howard, F. Hadaegh and the support of the entire Keck summit team. We thank D. Carlson and H. Timmers for preparing the HNLF. The authors wish to recognize and acknowledge the very significant cultural role and reverence that the summit of Mauna Kea has always had within the indigenous Hawaiian community. The data presented herein were obtained at the W.M. Keck Observatory, which is operated as a scientific partnership among the California Institute of Technology, the University of California and NASA. The Observatory was made possible by the generous financial support of the W.M. Keck Foundation. This paper made use of data available in the NASA Exoplanet Archive and the Keck Observatory Archive. S.D. and S.P. acknowledge support from NIST. K.V., M.-G.S., X.Y. and Y.-H.L. thank the Kavli Nanoscience Institute and NASA for support under KJV.JPLNASA-1-JPL.1459106. This research was carried out at JPL and the California Institute of Technology under a contract with NASA and funded through the JPL Research and Technology Development Program. Data availability: The data that support the plots within this paper and other findings of this study are available from the corresponding authors upon reasonable request. Contributions: M.-G.S., S.L., G.V., M.P.F., D.M., S.B.P., S.A.D., C.B. and K.V. conceived the experiments. All co-authors designed and performed experiments. M.-G.S. and X.Y. built the soliton microcomb set-up and EO comb set-up with S.L., I.S.G., S.A.D., S.B.P. and Y.-H.L. providing assistance. G.D. managed operations and the experimental interface of the Keck II telescope. E.C.M., J.W. and C.B. analysed NIRSPEC data. C.B. and K.V. supervised the experiment. M.-G.S., C.B. and K.V. prepared the manuscript with input from all co-authors. Competing interests: The authors declare no competing interests.
Group:Kavli Nanoscience Institute, Infrared Processing and Analysis Center (IPAC)
Funders:
Funding AgencyGrant Number
W. M. Keck FoundationUNSPECIFIED
National Institute of Standards and Technology (NIST)UNSPECIFIED
Kavli Nanoscience InstituteUNSPECIFIED
NASAKJV.JPLNASA-1-JPL.1459106
NASA/JPL/CaltechUNSPECIFIED
JPL Research and Technology Development FundUNSPECIFIED
Subject Keywords:Integrated optics; Nonlinear optics; Optics and photonics; Solitons
Record Number:CaltechAUTHORS:20180119-080155783
Persistent URL:http://resolver.caltech.edu/CaltechAUTHORS:20180119-080155783
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:84406
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:19 Jan 2018 17:56
Last Modified:17 Dec 2018 21:32

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