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K2-263 b: a 50 d period sub-Neptune with a mass measurement using HARPS-N
Indexado
WoS WOS:000449764000032
Scopus SCOPUS_ID:85060873232
DOI 10.1093/MNRAS/STY2360
Año 2018
Tipo artículo de investigación

Citas Totales

Autores Afiliación Chile

Instituciones Chile

% Participación
Internacional

Autores
Afiliación Extranjera

Instituciones
Extranjeras


Abstract



This paper reports on the validation and mass measurement of K2-263 b, a sub-Neptune orbiting a quiet G9V star. Using K2 data from campaigns C5 and C16, we find this planet to have a period of 50.818947 +/- 0.000094 d and a radius of 2.41 +/- 0.12 R-circle plus. We followed this system with HARPS-N to obtain 67 precise radial velocities (RVs). A combined fit of the transit and radial velocity data reveals that K2-263 b has a mass of 14.8 +/- 3.1 M-circle plus. Its bulk density (5.7(-1.41.6) g cm(-3) ) implies that this planet has a significant envelope of water or other volatiles around a rocky core. K2-263 b likely formed in a similar way as the cores of the four giant planets in our own Solar System, but for some reason, did not accrete much gas. The planetary mass was confirmed by an independent Gaussian process-based fit to both the RVs and the spectroscopic activity indicators. K2-263 b belongs to only a handful of confirmed K2 exoplanets with periods longer than 40 d. It is among the longest periods for a small planet with a precisely determined mass using RVs.

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Disciplinas de Investigación



WOS
Astronomy & Astrophysics
Scopus
Sin Disciplinas
SciELO
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Publicaciones WoS (Ediciones: ISSHP, ISTP, AHCI, SSCI, SCI), Scopus, SciELO Chile.

Colaboración Institucional



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Autores - Afiliación



Ord. Autor Género Institución - País
1 Mortier, A. Mujer Univ St Andrews - Reino Unido
University of St Andrews - Reino Unido
2 Bonomo, Aldo S. Hombre Istituto Nazionale di Astrofisica - Italia
Istituto Nazionale Di Astrofisica, Rome - Italia
3 Rajpaul, Vinesh M. - UNIV CAMBRIDGE - Reino Unido
Department of Physics - Reino Unido
4 Buchhave, L. A. Hombre Tech Univ Denmark - Dinamarca
Danmarks Tekniske Universitet - Dinamarca
Technical University of Denmark - Dinamarca
5 Vanderburg, Andrew Hombre Univ Texas Austin - Estados Unidos
The University of Texas at Austin - Estados Unidos
6 Zeng, Li - Harvard University - Estados Unidos
7 Lopez-Morales, Mercedes Mujer Harvard Smithsonian Ctr Astrophys - Estados Unidos
Harvard-Smithsonian Center for Astrophysics - Estados Unidos
Harvard University - Estados Unidos
8 Malavolta, Luca Hombre Istituto Nazionale di Astrofisica - Italia
Univ Padua - Italia
Osservatorio Astronomico di Padova - Italia
Università degli Studi di Padova - Italia
9 Cameron, A. Hombre Univ St Andrews - Reino Unido
University of St Andrews - Reino Unido
10 Dressing, Courtney D. Mujer UNIV CALIF BERKELEY - Estados Unidos
University of California, Berkeley - Estados Unidos
11 Gu, P. -G. Hombre ESO - Chile
Univ Porto - Portugal
European Southern Observatory Santiago - Chile
Universidade do Porto, Centro de Astrofísica - Portugal
Centro de Astrofísica da Universidade do Porto - Portugal
12 Nascimbeni, V. Hombre Istituto Nazionale di Astrofisica - Italia
Univ Padua - Italia
Osservatorio Astronomico di Padova - Italia
Università degli Studi di Padova - Italia
13 Rice, Ken - UNIV EDINBURGH - Reino Unido
University of Edinburgh, Institute for Astronomy - Reino Unido
University of Edinburgh - Reino Unido
The University of Edinburgh - Reino Unido
14 Sozzetti, A. Hombre Istituto Nazionale di Astrofisica - Italia
Istituto Nazionale Di Astrofisica, Rome - Italia
15 Watson, Christopher A. Hombre Queens Univ Belfast - Reino Unido
Queen's University Belfast - Reino Unido
16 Affer, Laura Mujer INAF Osservatorio Astron Palermo - Italia
Osservatorio Astronomico di Palermo Guiseppe S. Vaiana - Italia
Istituto Nazionale di Astrofisica - Italia
Istituto Nazionale Di Astrofisica, Rome - Italia
17 Bouchy, Francois Hombre Univ Geneva - Suiza
Université de Genève - Suiza
Faculty of Science - Suiza
18 Charbonneau, David Hombre Harvard Smithsonian Ctr Astrophys - Estados Unidos
Harvard-Smithsonian Center for Astrophysics - Estados Unidos
Harvard University - Estados Unidos
19 Harutyunyan, Avet - Istituto Nazionale di Astrofisica - España
Fundación Galileo Galilei - España
20 Haywood, Raphaelle D. - Harvard Smithsonian Ctr Astrophys - Estados Unidos
Harvard-Smithsonian Center for Astrophysics - Estados Unidos
Harvard University - Estados Unidos
21 Johnson, John A. Hombre Harvard Smithsonian Ctr Astrophys - Estados Unidos
Harvard-Smithsonian Center for Astrophysics - Estados Unidos
Harvard University - Estados Unidos
22 Latham, David W. Hombre Harvard Smithsonian Ctr Astrophys - Estados Unidos
Harvard-Smithsonian Center for Astrophysics - Estados Unidos
Harvard University - Estados Unidos
23 Lovis, Christophe Hombre Univ Geneva - Suiza
Université de Genève - Suiza
Faculty of Science - Suiza
24 Martinez Fiorenzano, A. Hombre Istituto Nazionale di Astrofisica - España
Fundación Galileo Galilei - España
25 Mayor, M. - Univ Geneva - Suiza
Université de Genève - Suiza
Faculty of Science - Suiza
26 Micela, G. Mujer INAF Osservatorio Astron Palermo - Italia
Osservatorio Astronomico di Palermo Guiseppe S. Vaiana - Italia
Istituto Nazionale di Astrofisica - Italia
Istituto Nazionale Di Astrofisica, Rome - Italia
27 MOLINARI-LABBE, ESTEBAN RICARDO Hombre INAF Osservatorio Astron Cagliari - Italia
Osservatorio Astronomico di Cagliari - Italia
28 Motalebi, Fatemeh Mujer Univ Geneva - Suiza
Université de Genève - Suiza
Faculty of Science - Suiza
29 Pepe, Francesco A. Hombre Univ Geneva - Suiza
Université de Genève - Suiza
Faculty of Science - Suiza
30 Piotto, Giampaolo Hombre Istituto Nazionale di Astrofisica - Italia
Univ Padua - Italia
Osservatorio Astronomico di Padova - Italia
Università degli Studi di Padova - Italia
31 Phillips, D. Hombre Harvard Smithsonian Ctr Astrophys - Estados Unidos
Harvard-Smithsonian Center for Astrophysics - Estados Unidos
Harvard University - Estados Unidos
32 Poretti, Ennio Hombre Istituto Nazionale di Astrofisica - España
Istituto Nazionale di Astrofisica - Italia
Fundación Galileo Galilei - España
Osservatorio Astronomico di Brera - Italia
33 Sasselov, Dimitar Hombre Harvard Smithsonian Ctr Astrophys - Estados Unidos
Harvard-Smithsonian Center for Astrophysics - Estados Unidos
Harvard University - Estados Unidos
34 Ségransan, Damien Hombre Univ Geneva - Suiza
Université de Genève - Suiza
Faculty of Science - Suiza
35 Celino, J. J. Hombre Univ Geneva - Suiza
Université de Genève - Suiza
Faculty of Science - Suiza

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Citas identificadas: Las citas provienen de documentos incluidos en la base de datos de DATACIENCIA

Citas Identificadas: 7.14 %
Citas No-identificadas: 92.86 %

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Citas identificadas: Las citas provienen de documentos incluidos en la base de datos de DATACIENCIA

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Citas No-identificadas: 92.86 %

Financiamiento



Fuente
European Union
National Aeronautics and Space Administration (NASA)
Swiss National Science Foundation
STFC
Science and Technology Facilities Council
National Aeronautics and Space Administration
FP7/2007
Seventh Framework Programme
John Templeton Foundation
NASA Science Mission directorate
Emmanuel College, University of Cambridge
University of Edinburgh
California Institute of Technology
NASA Exoplanet Science Institute
Jet Propulsion Laboratory
Queen's University Belfast
University of Geneva
Smithsonian Astrophysical Observatory
NASA Office of Space Science
Kepler Mission under NASA
INAF/Frontiera
Italian Ministry of Education, University
Queen’s University Belfast
Scottish Universities Physics Alliance (SUPA)
Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung
Prodex Program of the Swiss Space Office (SSO)
Scottish Universities Physics Alliance
Swiss Space Office
Université de Genève
Harvard University Origins of Life Initiative (HUOLI)
Italian National Astrophysical Institute (INAF)
Smithsonian Astrophysical Observatory (SAO)
University of St Andrews
INAF/Frontiera through the 'Progetti Premiali' funding scheme of the Italian Ministry of Education, University, and Research
Harvard University Origins of Life Initiative
Université de Genève
Royal Astronomical Society and Emmanuel College, Cambridge
Science AMP; Technology Facilities Council (STFC)
Royal Astronomical Society
John Temple-ton Foundation
Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung

Muestra la fuente de financiamiento declarada en la publicación.

Agradecimientos



Agradecimiento
The HARPS-N project has been funded by the Prodex Program of the Swiss Space Office (SSO), the Harvard University Origins of Life Initiative (HUOLI), the Scottish Universities Physics Alliance (SUPA), the University of Geneva, the Smithsonian Astrophysical Observatory (SAO), and the Italian National Astrophysical Institute (INAF), the University of St Andrews, Queen's University Belfast, and the University of Edinburgh.r The research leading to these results received funding from the European Union Seventh Framework Programme (FP7/2007-2013) under grant agreement number 313014 (ETAEARTH). VMR acknowledges the Royal Astronomical Society and Emmanuel College, Cambridge, for financial support. This work was performed in part under contract with the California Institute of Technology (Caltech)/Jet Propulsion Laboratory (JPL) funded by NASA through the Sagan Fellowship Program executed by the NASA Exoplanet Science Institute (AV, RDH). LM acknowledges the support by INAF/Frontiera through the 'Progetti Premiali' funding scheme of the Italian Ministry of Education, University, and Research. ACC acknowledges support from the Science & Technology Facilities Council (STFC) consolidated grant number ST/R000824/1. DWL acknowledges partial support from the Kepler mission under NASA Cooperative Agreement NNX13AB58A with the Smithsonian Astrophysical Observatory. CAW acknowledges support by STFC grant ST/P000312/1. Some of this work has been carried out within the framework of the NCCR PlanetS, supported by the Swiss National Science Foundation. This publication was made possible through the support of a grant from the John Templeton Foundation. The opinions expressed are those of the authors and do not necessarily reflect the views of the John Templeton Foundation.r This material is based upon work supported by the National Aeronautics and Space Administration (NASA) under grants No. NNX15AC90G and NNX17AB59G issued through the Exoplanets Research Program. This research has made use of the SIMBAD database, operated at CDS, Strasbourg, France, NASA's Astro-physics Data System and the NASA Exoplanet Archive, which is operated by the California Institute of Technology, under contract with NASA under the Exoplanet Exploration Program. Based on observations made with the Italian Telescopio Nazionale Galileo (TNG) operated on the island of La Palma by the Fundacion Galileo Galilei of the INAF (Istituto Nazionale di Astrofisica) at the Spanish Observatorio del Roque de los Muchachos of the Instituto de Astrofisica de Canarias. This paper includes data collected by the K2 mission. Funding for the K2 mission is provided by the NASA Science Mission directorate. Some of the data presented in this paper were obtained from the Mikulski Archive for Space Telescopes (MAST). STScI is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS5-26555. Support for MAST for non-HST data is provided by the NASA Office of Space Science via grant NNX13AC07G and by other grants and contracts. K2-263 was observed as part of the following Guest Programmes: GO5007_LC (PI: Winn), GO5029_LC (PI: Charbonneau), GO5033_LC (PI: Howard), GO5104_LC (PI: Dragomir), GO5106_LC (PI: Jackson), GO5060_LC (PI: Coughlin), GO16009_LC (PI: Charbonneau), GO16011_LC (PI: Fabrycky), GO16015_LC (PI: Boyajian), GO16020_LC (PI: Adams), GO16021_LC (PI: Howard), GO16101_LC (PI: Winn), GO16009_SC (PI: Charbonneau), GO16015_SC (PI: Boyajian), and GO16101_SC (PI: Winn).
The HARPS-N project has been funded by the Prodex Program of the Swiss Space Office (SSO), the Harvard University Origins of Life Initiative (HUOLI), the Scottish Universities Physics Alliance (SUPA), the University of Geneva, the Smithsonian Astrophysical Observatory (SAO), and the Italian National Astrophysical Institute (INAF), the University of St Andrews, Queen’s University Belfast, and the University of Edinburgh.

Muestra la fuente de financiamiento declarada en la publicación.