Literature DB >> 20485423

Extrasolar planets: Larger than they ought to be.

Pin-Gao Gu.   

Abstract

Year:  2010        PMID: 20485423     DOI: 10.1038/465300a

Source DB:  PubMed          Journal:  Nature        ISSN: 0028-0836            Impact factor:   49.962


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  3 in total

1.  A transiting giant planet with a temperature between 250 K and 430 K.

Authors:  H J Deeg; C Moutou; A Erikson; Sz Csizmadia; B Tingley; P Barge; H Bruntt; M Havel; S Aigrain; J M Almenara; R Alonso; M Auvergne; A Baglin; M Barbieri; W Benz; A S Bonomo; P Bordé; F Bouchy; J Cabrera; L Carone; S Carpano; D Ciardi; M Deleuil; R Dvorak; S Ferraz-Mello; M Fridlund; D Gandolfi; J-C Gazzano; M Gillon; P Gondoin; E Guenther; T Guillot; R den Hartog; A Hatzes; M Hidas; G Hébrard; L Jorda; P Kabath; H Lammer; A Léger; T Lister; A Llebaria; C Lovis; M Mayor; T Mazeh; M Ollivier; M Pätzold; F Pepe; F Pont; D Queloz; M Rabus; H Rauer; D Rouan; B Samuel; J Schneider; A Shporer; B Stecklum; R Street; S Udry; J Weingrill; G Wuchterl
Journal:  Nature       Date:  2010-03-18       Impact factor: 49.962

2.  The use of transit timing to detect terrestrial-mass extrasolar planets.

Authors:  Matthew J Holman; Norman W Murray
Journal:  Science       Date:  2005-02-25       Impact factor: 47.728

3.  Infrared radiation from an extrasolar planet.

Authors:  Drake Deming; Sara Seager; L Jeremy Richardson; Joseph Harrington
Journal:  Nature       Date:  2005-03-23       Impact factor: 49.962

  3 in total

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