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Radek Poleski

Researcher at Ohio State University

Publications -  72
Citations -  1512

Radek Poleski is an academic researcher from Ohio State University. The author has contributed to research in topics: Gravitational microlensing & Planet. The author has an hindex of 18, co-authored 72 publications receiving 1335 citations. Previous affiliations of Radek Poleski include University of Warsaw.

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MOA-2011-BLG-262Lb: A Sub-Earth-Mass Moon Orbiting a Gas Giant Primary or a High Velocity Planetary System in the Galactic Bulge

David P. Bennett, +101 more
TL;DR: In this paper, the first microlensing candidate for a free-floating exoplanet-exomoon system, MOA-2011-BLG-262, with a primary lens mass of M host ~ 4 Jupiter masses hosting a sub-Earth mass moon was presented.
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Binary microlensing event OGLE-2009-BLG-020 gives a verifiable mass, distance and orbit predictions

TL;DR: In this article, the first example of binary microlensing for which the parameter measurements can be verified (or contradicted) by future Doppler observations is presented, made possible by a confluence of two relatively unusual circumstances.
Posted Content

The wide field infrared survey telescope: 100 hubbles for the 2020s

Rachel Akeson, +104 more
TL;DR: The Wide Field Infrared Survey Telescope (WFIRST) as discussed by the authors is a 2.4m space telescope with a 0.281 deg^2 field of view for near-IR imaging and slitless spectroscopy and a coronagraph designed for > 10^8 starlight suppresion.
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Spitzer parallax of OGLE-2015-BLG-0966 : a cold Neptune in the Galactic disk

Rachel Street, +110 more
TL;DR: In this paper, the authors reported the detection of a cold Neptune mplanet = 21 ± 2 M⊕ orbiting a 0.38 m⊙ M dwarf lying 2.5-3.3 kpc toward the Galactic center as part of a campaign combining ground-based and Spitzer observations.
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A terrestrial planet in a ~1-AU orbit around one member of a ∼15-AU binary

Andrew Gould, +68 more
- 04 Jul 2014 - 
TL;DR: In this paper, a cold terrestrial planet orbiting one member of a binary star system was detected using gravitational microlensing, and the planet has low mass (twice Earth's) and lies projected at ~0.8 astronomical units (AU) from its host star, about the distance between Earth and the Sun.