Habitable-zone super-Earth candidate in a six-planet system around the K2.5V star HD40307 â †

Astronomy and Astrophysics

Volumn 549, Issue , 2012, Pages

  Tuomi, M ^a,b   Anglada Escude G ^c   Gerlach, E ^d   Jones, H R A ^a   Reiners, A ^c   Rivera, E J ^e   Vogt, S S ^e   Butler, R P ^f  

^a UNIVERSITY OF HERTFORDSHIRE   (United Kingdom)

^b UNIVERSITY OF TURKU   (Finland)

^c UNIVERSITY OF GÖTTINGEN   (Germany)

^d DRESDEN UNIVERSITY OF TECHNOLOGY   (Germany)

^e University of California Santa Cruz   (United States)

^f GEOPHYSICAL LABORATORY   (United States)

Author keywords

Methods: numerical; Methods: statistical; Stars: individual: HD 40307; Techniques: radial velocities

Indexed keywords

ANGULAR SEPARATION; BAYESIAN ANALYSIS; CURRENT DEFINITION; DATA ANALYSIS METHODS; DIRECT IMAGING; DOPPLER MEASUREMENT; DOPPLER SIGNALS; LIQUID WATER; LOW-AMPLITUDE; LOW-MASS; METHODS: NUMERICALS; METHODS:STATISTICAL; MINIMUM MASS; MODEL PARAMETERS; PERIODOGRAM ANALYSIS; PROBABILITY DENSITIES; RADIAL VELOCITY; RELATIVE PROBABILITY; SPACE-BASED; STARS: INDIVIDUAL: HD 40307; TECHNIQUES: RADIAL VELOCITIES;

CHROMOPHORES; DOPPLER EFFECT; LIQUIDS; NUMERICAL METHODS; STARS;

EARTH (PLANET);

EID: 84871281294     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201220268     Document Type: Article

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