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Volumn 340, Issue 6132, 2013, Pages 572-576

Observed properties of extrasolar planets

Author keywords

[No Author keywords available]

Indexed keywords

METAL;

EID: 84877316061     PISSN: 00368075     EISSN: 10959203     Source Type: Journal    
DOI: 10.1126/science.1233545     Document Type: Review
Times cited : (187)

References (62)
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    • Updates to (1) are available at
    • Updates to (1) are available at http://exoplanets.org.
  • 4
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    • The current catalog of planets discovered with the Kepler telescope are available at
    • The current catalog of planets discovered with the Kepler telescope are available at http://exoplanetarchive.ipac.caltech.edu/cgi-bin/ExoTables/nph- exotbls?dataset=cumulative.
  • 7
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    • note
    • The false positive probabilities (FPPs) for Kepler telescope planet candidates are typically small because of detailed vetting of the photometry, including analysis of the transit shape and astrometric displacement. FPPs depend on the host star brightness and crowding in the field as well as on planet size; giant planets often have larger FPPs.
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    • (2012)
    • Dong, S.1    Zhu, Z.2
  • 30
  • 43
    • 84877356165 scopus 로고    scopus 로고
    • note
    • All elements except for hydrogen and helium are considered "metals" by astronomers. "Metallicity" refers to the abundance of metals (often iron) relative to solar proportions.
  • 45
    • 84877315306 scopus 로고    scopus 로고
    • note
    • Self-pollution was ruled out because evolved subgiant planet-host stars are as metal-rich as are main sequence -planet hosts, despite convective zone mixing in evolved stars that would have diluted their surface-layer pollution signature (53).
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    • note
    • For planets smaller than 4 RE, I adopt Kepler telescope occurrence measurements for orbital periods of 5 to 50 days, which include corrections for missed planet detections in the Kepler telescope pipeline (16). For larger planets, I use measurements of a larger number of stars, but for all orbital periods <50 days (17).
  • 60
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    • The properties of extrasolar planets plotted in Figs. 3 and 4 were downloaded from the Exoplanet Orbit Database on 14 February Additionally, Kepler-discovered planets with ≥2-σ mass measurements from (58) were included for Fig. 3
    • The properties of extrasolar planets plotted in Figs. 3 and 4 were downloaded from the Exoplanet Orbit Database (http://exoplanets.org) on 14 February 2013. Additionally, Kepler-discovered planets with ≥2-σ mass measurements from (58) were included for Fig. 3.
    • (2013)


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.