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dc.contributor.authorMuterspaugh, Matthew W.
dc.contributor.authorLane, Benjamin F.
dc.contributor.authorKulkarni, S. R.
dc.contributor.authorKonacki, Maciej
dc.contributor.authorBurke, Bernard F.
dc.contributor.authorColavita, M. M.
dc.contributor.authorShao, M.
dc.contributor.authorHartkopf, William I.
dc.contributor.authorBoss, Alan P.
dc.contributor.authorWilliamson, M.
dc.date.accessioned2015-01-30T20:32:20Z
dc.date.available2015-01-30T20:32:20Z
dc.date.issued2010-12
dc.date.submitted2010-07
dc.identifier.issn0004-6256
dc.identifier.issn1538-3881
dc.identifier.urihttp://hdl.handle.net/1721.1/93249
dc.description.abstractThe Palomar High-precision Astrometric Search for Exoplanet Systems monitored 51 subarcsecond binary systems to evaluate whether tertiary companions as small as Jovian planets orbited either the primary or secondary stars, perturbing their otherwise smooth Keplerian motions. Six binaries are presented that show evidence of substellar companions orbiting either the primary or secondary star. Of these six systems, the likelihoods of two of the detected perturbations to represent real objects are considered to be "high confidence," while the remaining four systems are less certain and will require continued observations for confirmation.en_US
dc.description.sponsorshipNational Science Foundation (U.S.) (grant AST 0300096)en_US
dc.description.sponsorshipNational Science Foundation (U.S.) (grant AST 0507590)en_US
dc.description.sponsorshipNational Science Foundation (U.S.) (grant AST 0505366)en_US
dc.description.sponsorshipFoundation for Polish Science (FOCUS grant and fellowship)en_US
dc.description.sponsorshipPoland. Ministry of Science and Higher Education (grant N203 3020 35)en_US
dc.language.isoen_US
dc.publisherInstitute of Physics/American Astronomical Societyen_US
dc.relation.isversionofhttp://dx.doi.org/10.1088/0004-6256/140/6/1657en_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.sourceAmerican Astronomical Societyen_US
dc.titleTHE PHASES DIFFERENTIAL ASTROMETRY DATA ARCHIVE. V. CANDIDATE SUBSTELLAR COMPANIONS TO BINARY SYSTEMSen_US
dc.typeArticleen_US
dc.identifier.citationMuterspaugh, Matthew W., Benjamin F. Lane, S. R. Kulkarni, Maciej Konacki, Bernard F. Burke, M. M. Colavita, M. Shao, William I. Hartkopf, Alan P. Boss, and M. Williamson. “THE PHASES DIFFERENTIAL ASTROMETRY DATA ARCHIVE. V. CANDIDATE SUBSTELLAR COMPANIONS TO BINARY SYSTEMS.” The Astronomical Journal 140, no. 6 (October 20, 2010): 1657–1671. © 2010 American Astronomical Society.en_US
dc.contributor.departmentKavli Institute for Astrophysics and Space Researchen_US
dc.contributor.departmentMassachusetts Institute of Technology. Department of Physicsen_US
dc.contributor.mitauthorBurke, Bernard F.en_US
dc.relation.journalAstronomical Journalen_US
dc.eprint.versionFinal published versionen_US
dc.type.urihttp://purl.org/eprint/type/JournalArticleen_US
eprint.statushttp://purl.org/eprint/status/PeerRevieweden_US
dspace.orderedauthorsMuterspaugh, Matthew W.; Lane, Benjamin F.; Kulkarni, S. R.; Konacki, Maciej; Burke, Bernard F.; Colavita, M. M.; Shao, M.; Hartkopf, William I.; Boss, Alan P.; Williamson, M.en_US
dc.identifier.orcidhttps://orcid.org/0000-0002-3182-3304
mit.licensePUBLISHER_POLICYen_US


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