Diving Beneath the Sea of Stellar Activity: Chromatic Radial Velocities of the Young AU Mic
Planetary System - IOPscience This site uses cookies. By continuing to use this site you agree …

We present a spectroscopic analysis of a 1-yr intensive monitoring campaign of the 22-Myr
old planet-hosting M dwarf AU Mic using the HARPS spectrograph. In a companion paper …

In this paper, we present an analysis of near-infrared spectropolarimetric and velocimetric
data of the young M dwarf AU Mic, collected with SPIRou at the Canada–France–Hawaii …

We present radial velocity measurements of a sample of M5V–M9V stars from our Red-
Optical Planet Survey, operating at 0.652–1.025 μm. Radial velocities for 15 stars, with rms …

AU Mic b is a Neptune-sized planet on an 8.47-day orbit around the nearest pre-main
sequence (~ 20 Myr) star to the Sun, the bright (V= 8.81) M dwarf AU Mic. The planet was …

We obtained spectra of the pre-main-sequence star AU Microscopii during a transit of its
Neptune-sized planet to investigate its orbit and atmosphere. We used the high-dispersion …

AU Mic is a young (∼ 24 Myr), pre-main-sequence M dwarf star that was observed in the first
month of science observations of the Transiting Exoplanet Survey Satellite (TESS) and …

We present spectroscopic rotation velocities (v sin i) for 56 M dwarf stars using high-
resolution Hobby–Eberly Telescope High Resolution Spectrograph red spectroscopy. In …

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 …

We present a velocimetric and spectropolarimetric analysis of 27 observations of the 22-Myr
M1 star AU Microscopii (AU Mic) collected with the high-resolution YJHK (0.98–2.35 μm) …