activity
20182022
most citedOne year of AU Mic with HARPS: I -- measuring the masses of the two transiting planets

52 citations · 129 across the 5 of their papers we have counts for

collaborators

8 papers

astro-ph.EP202252 cited

One year of AU Mic with HARPS: I -- measuring the masses of the two transiting planets

Norbert Zicher, Oscar Barragán, Baptiste Klein +11

The system of two transiting Neptune-sized planets around the bright, young M-dwarf AU Mic provides a unique opportunity to test models of planet formation, early evolution, and st…

astro-ph.EP2021

A SOPHIE RV search for giant planets around young nearby stars (YNS). A combination with the HARPS YNS survey

A. Grandjean, A. -M. Lagrange, N. Meunier +9

The search of close (a<=5 au) giant planet(GP) companions with radial velocity(RV) around young stars and the estimate of their occurrence rates is important to constrain the migra…

astro-ph.EP202040 cited

Hot Exoplanet Atmospheres Resolved with Transit Spectroscopy (HEARTS) VI. Non-detection of sodium with HARPS on the bloated super-Neptune WASP-127b

J. V. Seidel, M. Lendl, V. Bourrier +17

WASP-127b is one of the puffiest exoplanets found to date, with a mass only Neptune masses, but a radius larger than Jupiter. It is also located at the border of the Neptune…

astro-ph.EP2020

Direct confirmation of the radial-velocity planet Pic c

M. Nowak, S. Lacour, A. -M. Lagrange +90

Methods used to detect giant exoplanets can be broadly divided into two categories: indirect and direct. Indirect methods are more sensitive to planets with a small orbital period,…

astro-ph.EP201936 cited

A HARPS RV search for planets around young nearby stars

A. Grandjean, A. -M. Lagrange, M. Keppler +9

Young nearby stars are good candidates in the search for planets with both radial velocity (RV) and direct imaging techniques. This, in turn, allows for the computation of the gian…

astro-ph.EP20191 cited

Constraining the properties of HD 206893 B. A combination of radial velocity, direct imaging, and astrometry data

A. Grandjean, A. -M. Lagrange, H. Beust +25

High contrast imaging enables the determination of orbital parameters for substellar companions (planets, brown dwarfs) from the observed relative astrometry and the estimation of…