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A low-mass planet candidate orbiting Proxima Centauri at a distance of 1.5 AU.

Authors :
Damasso, Mario
Del Sordo, Fabio
Anglada-Escudé, Guillem
Giacobbe, Paolo
Sozzetti, Alessandro
Morbidelli, Alessandro
Pojmanski, Grzegorz
Barbato, Domenico
Butler, R. Paul
Jones, Hugh R. A.
Hambsch, Franz-Josef
Jenkins, James S.
López-González, María José
Morales, Nicolás
Peña Rojas, Pablo A.
Rodríguez-López, Cristina
Rodríguez, Eloy
Amado, Pedro J.
Anglada, Guillem
Feng, Fabo
Source :
Science Advances. 1/30/2020, Vol. 6 Issue 3, p1-13. 13p.
Publication Year :
2020

Abstract

The article repots on orbit Proxima Centauri at a distance of 1.5 AU. Topic include measurements with the High Accuracy Radial Velocity Planet Searcher (HARPS) and Ultraviolet and Visual Echelle Spectrograph (UVES); and investigating the nature of this signal in detail, checked its evolution and stability over time by analyzing the stacked Bayesian GLS (SBGLS).

Details

Language :
English
ISSN :
23752548
Volume :
6
Issue :
3
Database :
Academic Search Index
Journal :
Science Advances
Publication Type :
Academic Journal
Accession number :
141331920
Full Text :
https://doi.org/10.1126/sciadv.aax7467