dc.contributor.author | Nagel, E | en_US |
dc.contributor.author | Czesla, S | en_US |
dc.contributor.author | Schmitt, JHMM | en_US |
dc.contributor.author | Dreizler, S | en_US |
dc.contributor.author | Anglada-Escude, G | en_US |
dc.contributor.author | Rodriguez, E | en_US |
dc.contributor.author | Ribas, I | en_US |
dc.contributor.author | Reiners, A | en_US |
dc.contributor.author | Quirrenbach, A | en_US |
dc.contributor.author | Amado, PJ | en_US |
dc.contributor.author | Caballero, JA | en_US |
dc.contributor.author | Aceituno, J | en_US |
dc.contributor.author | Bejar, VJS | en_US |
dc.contributor.author | Cortes-Contreras, M | en_US |
dc.contributor.author | Gonzalez-Cuestato, L | en_US |
dc.contributor.author | Guenther, W | en_US |
dc.contributor.author | Henning, T | en_US |
dc.contributor.author | Jeffers, SV | en_US |
dc.contributor.author | Kaminski, A | en_US |
dc.contributor.author | Kuerster, M | en_US |
dc.contributor.author | Lafarga, M | en_US |
dc.contributor.author | Lopez-Gonzalez, MJ | en_US |
dc.contributor.author | Montes, D | en_US |
dc.contributor.author | Morales, JC | en_US |
dc.contributor.author | Passegger, VM | en_US |
dc.contributor.author | Rodriguez-Lopez, C | en_US |
dc.contributor.author | Schweitzer, A | en_US |
dc.contributor.author | Zechmeister, M | en_US |
dc.date.accessioned | 2019-05-16T10:40:47Z | |
dc.date.available | 2018-12-13 | en_US |
dc.date.issued | 2019-02-13 | en_US |
dc.identifier.issn | 1432-0746 | en_US |
dc.identifier.other | ARTN A153 | |
dc.identifier.other | ARTN A153 | |
dc.identifier.other | ARTN A153 | en_US |
dc.identifier.uri | https://qmro.qmul.ac.uk/xmlui/handle/123456789/57585 | |
dc.relation.ispartof | ASTRONOMY & ASTROPHYSICS | en_US |
dc.subject | planetary systems | en_US |
dc.subject | stars: individual: GJ 4276 | en_US |
dc.subject | stars: low-mass | en_US |
dc.subject | methods: data analysis | en_US |
dc.subject | methods: observational | en_US |
dc.subject | techniques: radial velocities | en_US |
dc.title | The CARMENES search for exoplanets around M dwarfs The enigmatic planetary system GJ 4276: one eccentric planet or two planets in a 2:1 resonance? | en_US |
dc.type | Article | |
dc.rights.holder | © ESO 2019 | |
dc.identifier.doi | 10.1051/0004-6361/201834569 | en_US |
pubs.author-url | http://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcApp=PARTNER_APP&SrcAuth=LinksAMR&KeyUT=WOS:000458472000001&DestLinkType=FullRecord&DestApp=ALL_WOS&UsrCustomerID=612ae0d773dcbdba3046f6df545e9f6a | en_US |
pubs.notes | Not known | en_US |
pubs.publication-status | Published | en_US |
pubs.volume | 622 | en_US |
rioxxterms.funder | Default funder | en_US |
rioxxterms.identifier.project | Default project | en_US |
qmul.funder | Astronomy Research at Queen Mary::Science and Technology Facilities Council | en_US |