activity
20172020
most citedWASP-107b's density is even lower: a case study for the physics of planetary gas envelope accretion and orbital migration

97 citations · 174 across the 3 of their papers we have counts for

collaborators

5 papers

astro-ph.EP202097 cited

WASP-107b's density is even lower: a case study for the physics of planetary gas envelope accretion and orbital migration

Caroline Piaulet, Björn Benneke, Ryan A. Rubenzahl +21

With a mass in the Neptune regime and a radius of Jupiter, WASP-107b presents a challenge to planet formation theories. Meanwhile, the planet's low surface gravity and the star's b…

astro-ph.EP2020

Physical Parameters of the Multi-Planet Systems HD 106315 and GJ 9827

Molly R. Kosiarek, David A. Berardo, Ian J. M. Crossfield +42

HD 106315 and GJ 9827 are two bright, nearby stars that host multiple super-Earths and sub-Neptunes discovered by K2 that are well suited for atmospheric characterization. We refin…

astro-ph.SR20207 cited

An extensive spectroscopic time series of three Wolf-Rayet stars -- II. A search for wind asymmetries in the dust-forming WC7 binary WR137

N. St-Louis, C. Piaulet, N. D. Richardson +39

We present the results of a four-month, spectroscopic campaign of the Wolf-Rayet dust-making binary, WR137. We detect only small-amplitude, random variability in the CIII5696 emiss…

astro-ph.EP2019

Water Vapor and Clouds on the Habitable-Zone Sub-Neptune Exoplanet K2-18b

Björn Benneke, Ian Wong, Caroline Piaulet +13

Results from the Kepler mission indicate that the occurrence rate of small planets ( ) in the habitable zone of nearby low-mass stars may be as high as 80%. Despite t…

astro-ph.SR201770 cited

BRITE-Constellation high-precision time-dependent photometry of the early-O-type supergiant Puppis unveils the photospheric drivers of its small- and large-scale wind structures

Tahina Ramiaramanantsoa, Anthony F. J. Moffat, Robert Harmon +33

From months of dual-band optical photometric monitoring at the mmag level, BRITE-Constellation has revealed two simultaneous types of variability in the O4I(n)fp star