activity
19962026
most citedSix transiting planets and a chain of Laplace resonances in TOI-178

195 citations · 3k across the 73 of their papers we have counts for

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Showing 2019Show all

17 papers · 1 filter

astro-ph.EP201920 cited

An extremely low-density and temperate giant exoplanet

A. Santerne, L. Malavolta, M. R. Kosiarek +68

Transiting extrasolar planets are key objects in the study of the formation, migration, and evolution of planetary systems. In particular, the exploration of the atmospheres of gia…

astro-ph.EP201914 cited

From the stellar properties of HD219134 to the internal compositions of its transiting exoplanets

Roxanne Ligi, Caroline Dorn, Aurélien Crida +8

The harvest of exoplanet discoveries has opened the area of exoplanet characterisation. But this cannot be achieved without a careful analysis of the host star parameters. The syst…

astro-ph.EP201915 cited

Using HARPS-N to characterise the long-period planets in the PH-2 and Kepler-103 systems

Sophie C. Dubber, Annelies Mortier, Ken Rice +26

We present confirmation of the planetary nature of PH-2b, as well as the first mass estimates for the two planets in the Kepler-103 system. PH-2b and Kepler-103c are both long-peri…

astro-ph.SR201917 cited

Testing the Spectroscopic Extraction of Suppression of Convective Blueshift

M. Miklos, T. W. Milbourne, R. D. Haywood +21

Efforts to detect low-mass exoplanets using stellar radial velocities (RVs) are currently limited by magnetic photospheric activity. Suppression of convective blueshift is the domi…

astro-ph.EP2019

Catalog for the ESPRESSO blind radial velocity exoplanet survey

S. Hojjatpanah, P. Figueira, N. C. Santos +19

One of the main scientific drivers for ESPRESSO,Échelle SPectrograph, is the detection and characterization of Earth-class exoplanets. With this goal in mind, the ESPRESSO Guarante…

astro-ph.EP2019

An 11 Earth-Mass, Long-Period Sub-Neptune Orbiting a Sun-like Star

Andrew W. Mayo, Vinesh M. Rajpaul, Lars A. Buchhave +27

Although several thousands of exoplanets have now been detected and characterized, observational biases have led to a paucity of long-period, low-mass exoplanets with measured mass…