most citedThree years of Sun-as-a-star radial-velocity observations on the approach to solar minimum

149 citations · 396 across the 8 of their papers we have counts for

collaborators

10 papers

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.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…

astro-ph.SR2019149 cited

Three years of Sun-as-a-star radial-velocity observations on the approach to solar minimum

A. Collier Cameron, A. Mortier, D. Phillips +33

The time-variable velocity fields of solar-type stars limit the precision of radial-velocity determinations of their planets' masses, obstructing detection of Earth twins. Since 20…

astro-ph.IM201941 cited

A new wavelength calibration for echelle spectrographs using Fabry-Perot etalons

F. Cersullo, A. Coffinet, B. Chazelas +2

The study of Earth-mass extrasolar planets via the radial-velocity technique and the measurement of the potential cosmological variability of fundamental constants call for very-hi…

astro-ph.EP201952 cited

Hot, rocky and warm, puffy super-Earths orbiting TOI-402 (HD 15337)

X. Dumusque, O. Turner, C. Dorn +30

TESS is revolutionising the search for planets orbiting bright and nearby stars. In sectors 3 and 4, TESS observed TOI-402 (TIC-120896927), a bright V=9.1 K1 dwarf also known as HD…

astro-ph.EP201918 cited

K2-291 b: A rocky super-Earth in a 2.2 day orbit

Molly R. Kosiarek, Sarah Blunt, Mercedes Lopez-Morales +43

K2-291 (EPIC 247418783) is a solar-type star with a radius of R_star = 0.899 0.034 R_sun and mass of M_star=0.934 0.038 M_sun. From K2 C13 data, we found one super-Eart…