One or more bound planets per Milky Way star from microlensing observations - Wikidata - wikimedia - TriplyDB

One or more bound planets per Milky Way star from microlensing observations

One or more bound planets per Milky Way star from microlensing observations

http://www.wikidata.org/entity/Q28257232

about

Can dust coagulation trigger streaming instability?Post-main-sequence planetary system evolution The search for signs of life on exoplanets at the interface of chemistry and planetary science The EChO science case Extrasolar planets: Cloudy with a chance of dustballs On the probability of habitable planets The frequency of planetary debris around young white dwarfs The future of spectroscopic life detection on exoplanets.An Earth-mass planet orbiting α Centauri B.Exoplanet habitability.Exoplanet detection. A terrestrial planet in a ~1-AU orbit around one member of a ~15-AU binary.Galactic planetary science.Possible climates on terrestrial exoplanets.A Statistical Approach to Illustrate the Challenge of Astrobiology for Public Outreach.The origins of life: old problems, new chemistries.Kinetic modeling of x-ray laser-driven solid Al plasmas via particle-in-cell simulation.Exoplanet Biosignatures: Observational Prospects.HATS-2b: A transiting extrasolar planet orbiting aK-type star showing starspot activity Prospect for UV observations from the Moon Life-bearing primordial planets in the solar vicinity On the abundance of extraterrestrial life after the Kepler mission Cavity and other radial substructures in the disk around HD 97048 HADES RV Programme with HARPS-N at TNG Faint-source-star planetary microlensing: the discovery of the cold gas-giant planet OGLE-2014-BLG-0676Lb The OGLE-III planet detection efficiency from six years of microlensing observations (2003–2008)A giant planet beyond the snow line in microlensing event OGLE-2011-BLG-0251 A brown dwarf orbiting an M-dwarf: MOA 2009–BLG–411L OGLE-2008-BLG-510: first automated real-time detection of a weak microlensing anomaly -- brown dwarf or stellar binary?The role of protostellar jets in star formation and the evolution of the early solar system: Astrophysical and meteoritical perspectives ExELS: an exoplanet legacy science proposal for the ESA Euclid mission - II. Hot exoplanets and sub-stellar systems Simultaneous optical and near-infrared linear spectropolarimetry of the earthshine ExELS: an exoplanet legacy science proposal for the ESA Euclid mission – I. Cold exoplanets MASSIVE: A Bayesian analysis of giant planet populations around low-mass stars Global energy budgets and ‘Trenberth diagrams’ for the climates of terrestrial and gas giant planets

P2860

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P2860

One or more bound planets per Milky Way star from microlensing observations

http://www.wikidata.org/entity/Q28257232

description

2012 nî lūn-bûn

@nan

2012 թուականի Յունուարին հրատարակուած գիտական յօդուած

@hyw

2012 թվականի հունվարին հրատարակված գիտական հոդված

@hy

2012年の論文

@ja

2012年論文

@yue

2012年論文

@zh-hant

2012年論文

@zh-hk

2012年論文

@zh-mo

2012年論文

@zh-tw

2012年论文

@wuu

name

One or more bound planets per Milky Way star from microlensing observations

@ast

One or more bound planets per Milky Way star from microlensing observations

@en

One or more bound planets per Milky Way star from microlensing observations

@nl

type

label

One or more bound planets per Milky Way star from microlensing observations

@ast

One or more bound planets per Milky Way star from microlensing observations

@en

One or more bound planets per Milky Way star from microlensing observations

@nl

prefLabel

One or more bound planets per Milky Way star from microlensing observations

@ast

One or more bound planets per Milky Way star from microlensing observations

@en

One or more bound planets per Milky Way star from microlensing observations

@nl

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P2860

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P1433

P1476

One or more bound planets per Milky Way star from microlensing observations

@en

P2093

A Cassan

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A Williams

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B Watson

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C Vinter

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Ch Coutures

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D Dominis Prester

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D Kubas

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D P Bennett

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D Warren

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G Pietrzyński

http://www.w3.org/2001/XMLSchema#string

P2860

OGLE-2005-BLG-071Lb, the most massive M dwarf planetary companion?

Unbound or distant planetary mass population detected by gravitational microlensing

LENS-LIKE ACTION OF A STAR BY THE DEVIATION OF LIGHT IN THE GRAVITATIONAL FIELD

Discovery of a Jupiter/Saturn analog with gravitational microlensing

Discovery of a cool planet of 5.5 Earth masses through gravitational microlensing

A Jupiter-mass companion to a solar-type star

Discovering planetary systems through gravitational microlenses

The occurrence and mass distribution of close-in super-Earths, Neptunes, and Jupiters.

Detection of Planetary Transits Across a Sun-like Star

Microlens OGLE-2005-BLG-169 Implies That Cool Neptune-like Planets Are Common

P2888

P304

167–169

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P31

scholarly article

P356

10.1038/NATURE10684

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P407

P433

7380

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P478

481

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P50

Igor Soszyński

Andrzej Udalski

P577

2012-01-11T00:00:00Z

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P5875

221740325

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P6179

1036550028

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P698

22237108

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P818

1202.0903

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P819

2012Natur.481..167C

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