scispace - formally typeset
C

C. H. Ling

Researcher at Massey University

Publications -  67
Citations -  2712

C. H. Ling is an academic researcher from Massey University. The author has contributed to research in topics: Gravitational microlensing & Planet. The author has an hindex of 25, co-authored 65 publications receiving 2495 citations. Previous affiliations of C. H. Ling include Institut d'Astrophysique de Paris & Nagoya University.

Papers
More filters
Journal ArticleDOI

Frequency of solar-like systems and of ice and gas giants beyond the snow line from high-magnification microlensing events in 2005-2008

Andrew Gould, +149 more
TL;DR: In this paper, the authors presented the first measurement of the planet frequency beyond the "snow line," for the planet-to-star mass-ratio interval during 2005-2008 microlensing events during the survey-plus-follow-up high-magnification channel.
Journal ArticleDOI

The Exoplanet Mass-Ratio Function from the MOA-II Survey: Discovery of a Break and Likely Peak at a Neptune Mass

TL;DR: In this article, the authors report the results of the statistical analysis of planetary signals discovered in MOA-II microlensing survey alert system events from 2007 to 2012, finding significant planetary signals in 23 of the 1474 alert events that are well characterized by the MOA II survey data alone, and combine this analysis with the previous analyses of Gould et al. and Cassan et al., bringing the total sample to 30 planets.
Journal ArticleDOI

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.
Journal ArticleDOI

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.