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dc.contributor.authorVanderburg, Andrew
dc.contributor.authorHuang, Chelsea
dc.contributor.authorRicker, George R.
dc.contributor.authorVanderspek, Roland K.
dc.contributor.authorSeager, Sara
dc.contributor.authorBurke, Christopher J.
dc.contributor.authorBurt, Jennifer A.
dc.contributor.authorCrossfield, Ian
dc.contributor.authorDynes, Scott
dc.contributor.authorGuerrero, Natalia
dc.contributor.authorShporer, Avi
dc.date.accessioned2020-04-17T14:09:36Z
dc.date.available2020-04-17T14:09:36Z
dc.date.issued2019-08
dc.identifier.issn2041-8213
dc.identifier.issn2041-8205
dc.identifier.urihttps://hdl.handle.net/1721.1/124716
dc.description.abstractTransiting Exoplanet Survey Satellite (TESS) observations have revealed a compact multiplanet system around the sixth-magnitude star HR 858 (TIC 178155732, TOI 396), located 32 pc away. Three planets, each about twice the size of Earth, transit this slightly evolved, late F-type star, which is also a member of a visual binary. Two of the planets may be in mean motion resonance. We analyze the TESS observations, using novel methods to model and remove instrumental systematic errors, and combine these data with follow-up observations taken from a suite of ground-based telescopes to characterize the planetary system. The HR 858 planets are enticing targets for precise radial velocity observations, secondary eclipse spectroscopy, and measurements of the Rossiter-McLaughlin effect. ©2019en_US
dc.language.isoen
dc.publisherAmerican Astronomical Societyen_US
dc.relation.isversionof10.3847/2041-8213/AB322Den_US
dc.rightsArticle is made available in accordance with the publisher's policy and may be subject to US copyright law. Please refer to the publisher's site for terms of use.en_US
dc.sourceThe American Astronomical Societyen_US
dc.titleTESS spots a compact system of super-Earths around the naked-eye star HR 858en_US
dc.typeArticleen_US
dc.identifier.citationVanderburg, Andrew, et al. "TESS spots a compact system of super-Earths around the naked-eye star HR 858." Astrophysical journal. Letters 881, 1 (August 2019): letter 19 doi 10.3847/2041-8213/AB322D ©2019 Author(s)en_US
dc.contributor.departmentMassachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciencesen_US
dc.contributor.departmentMIT Kavli Institute for Astrophysics and Space Researchen_US
dc.relation.journalAstrophysical journal. Lettersen_US
dc.eprint.versionFinal published versionen_US
dc.type.urihttp://purl.org/eprint/type/JournalArticleen_US
eprint.statushttp://purl.org/eprint/status/PeerRevieweden_US
dc.date.updated2020-04-07T19:00:12Z
dspace.orderedauthorsAndrew Vanderburg ; Chelsea X. Huang ; Joseph E. Rodriguez ; Juliette C. Becker ; George R. Ricker ; Roland K. Vanderspek ; David W. Latham ; Sara Seager ; Joshua N. Winn ; Jon M. Jenkins ; Brett Addison ; Allyson Bieryla ; Cesar Briceño ; Brendan P. Bowler ; Timothy M. Brown ; Christopher J. Burke ; Jennifer A. Burt ; Douglas A. Caldwell ; Jake T. Clark ; Ian Crossfield ; Jason A. Dittmann ; Scott Dynes ; Benjamin J. Fulton ; Natalia Guerrero ; Daniel Harbeck ; Jonathan Horner ; Stephen R. Kane ; John Kielkopf ; Adam L. Kraus ; Laura Kreidberg ; Nicolas Law ; Andrew W. Mann ; Matthew W. Mengel ; Timothy D. Morton ; Jack Okumura ; Logan A. Pearce ; Peter Plavchan ; Samuel N. Quinn ; Markus Rabus ; Mark E. Rose ; Pam Rowden ; Avi Shporer ; Robert J. Siverd ; Jeffrey C. Smith ; Keivan Stassun ; C. G. Tinney ; Rob Wittenmyer ; Duncan J. Wright ; Hui Zhang ; George Zhou ; Carl A. Ziegleren_US
dspace.date.submission2020-04-07T19:00:22Z
mit.journal.volume881en_US
mit.journal.issue1en_US
mit.licensePUBLISHER_POLICY
mit.metadata.statusComplete


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