A HARPS view on K2-3
| Author | dc.contributor.author | Almenara, J. M. | |
| Author | dc.contributor.author | Astudillo Defru, N. | |
| Author | dc.contributor.author | Bonfils, X. | |
| Author | dc.contributor.author | Forveille, T. | |
| Author | dc.contributor.author | Santerne, A. | |
| Author | dc.contributor.author | Albrecht, S. | |
| Author | dc.contributor.author | Barros, S. C. C. | |
| Author | dc.contributor.author | Bouchy, F. | |
| Author | dc.contributor.author | Delfosse, X. | |
| Author | dc.contributor.author | Demangeon, O. | |
| Author | dc.contributor.author | Diaz, R. F. | |
| Author | dc.contributor.author | Hébrard, G. | |
| Author | dc.contributor.author | Mayor, M. | |
| Author | dc.contributor.author | Neves, V. | |
| Author | dc.contributor.author | Rojo Rubke, Patricio | |
| Author | dc.contributor.author | Santos, N. C. | |
| Author | dc.contributor.author | Wünsche, A. | |
| Admission date | dc.date.accessioned | 2015-12-04T18:51:19Z | |
| Available date | dc.date.available | 2015-12-04T18:51:19Z | |
| Publication date | dc.date.issued | 2015 | |
| Cita de ítem | dc.identifier.citation | Astronomy & Astrophysics, 581, L7 (2015) | en_US |
| Identifier | dc.identifier.issn | 1432-0746 | |
| Identifier | dc.identifier.other | 10.1051/0004-6361/201525918 | |
| Identifier | dc.identifier.uri | https://repositorio.uchile.cl/handle/2250/135501 | |
| Abstract | dc.description.abstract | K2 space observations recently found that three super-Earths transit the nearby M dwarf K2-3. The apparent brightness and the small physical radius of their host star rank these planets amongst the most favourable for follow-up characterisations. The outer planet orbits close to the inner edge of the habitable zone and might become one of the first exoplanets searched for biomarkers using transmission spectroscopy.We used the HARPS velocimeter to measure the mass of the planets. The mass of planet b is 8:4 2:1 M , while our determination of those planets c and d are a ected by the stellar activity. With a density of 4:32+2:0 0:76 g cm3, planet b is probably mostly rocky, but it could contain up to 50% water. | en_US |
| Patrocinador | dc.description.sponsorship | NASA Science Mission directorate NAS5-26555 NASA Office of Space Science NNX09AF08G CONICYT Becas-Chile 72120460 European Research Council 337591-ExTrA Fundacao para a Ciencia e a Tecnologia (FCT) through Investigador FCT IF /00169/2012 "Programa Operacional de Factores de Competitividade -COMPETE" | en_US |
| Lenguage | dc.language.iso | en | en_US |
| Publisher | dc.publisher | EDP Sciences | en_US |
| Type of license | dc.rights | Atribución-NoComercial-SinDerivadas 3.0 Chile | * |
| Type of license | dc.rights | Atribución-NoComercial-SinDerivadas 3.0 Chile | * |
| Link to License | dc.rights.uri | http://creativecommons.org/licenses/by-nc-nd/3.0/cl/ | * |
| Link to License | dc.rights.uri | http://creativecommons.org/licenses/by-nc-nd/3.0/cl/ | * |
| Source | dc.source | Astronomy & Astrophysics | |
| Keywords | dc.subject | Planetary systems | en_US |
| Keywords | dc.subject | Stars: late-type | en_US |
| Keywords | dc.subject | Techniques: radial velocities | en_US |
| Keywords | dc.subject | Techniques: photometric | en_US |
| Título | dc.title | A HARPS view on K2-3 | en_US |
| Document type | dc.type | Artículo de revista | |
| dcterms.accessRights | dcterms.accessRights | Acceso abierto | |
| Indexation | uchile.index | Artículo de publicación ISI |
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Except where otherwise noted, this item's license is described as Atribución-NoComercial-SinDerivadas 3.0 Chile