activity
20022026
most citedDiscovery of magnetic fields in the beta Cephei star xi^1 CMa and in several Slowly Pulsating B stars

128 citations · 1.4k across the 35 of their papers we have counts for

collaborators
Showing astro-ph.SRShow all

19 papers · 1 filter

astro-ph.SR2026

High-precision K2/TESS Photometry and HERMES Spectroscopy of Four Bright Field Stars

Otto Trust, Santosh Joshi, Benard Nsamba +13

Space-based photometry from K2 and TESS, coupled with high-resolution spectroscopy, provides a unique opportunity to re-examine the variability and chemical nature of four bright s…

astro-ph.SR2025★ 8 cited

LAMOST medium-resolution observations of the Pleiades

A. Frasca, J. Y. Zhang, J. Alonso-Santiago +4

In this work we present the results of our analysis of medium-resolution LAMOST spectra of late-type candidate members of the Pleiades. We have used the code ROTFIT to determine th…

astro-ph.SR2023★ 25 cited

MELCHIORS: The Mercator Library of High Resolution Stellar Spectroscopy

P. Royer, T. Merle, K. Dsilva +71

Over the past decades, libraries of stellar spectra have been used in a large variety of science cases, including as sources of reference spectra for a given object or a given spec…

astro-ph.SR2021★ 28 cited

A homogeneous spectroscopic analysis of a Kepler legacy sample of dwarfs for gravity-mode asteroseismology

Sarah Gebruers, Ilya Straumit, Andrew Tkachenko +12

Asteroseismic modelling of the internal structure of main-sequence stars born with a convective core has so far been based on homogeneous analyses of space photometric Kepler light…

astro-ph.SR2020★ 65 cited

Phase II of the LAMOST-Kepler/K2 survey. I. Time series of medium-resolution spectroscopic observations

Weikai Zong, Jian-Ning Fu, Peter De Cat +20

Phase \RNum{2} of the LAMOST-{\sl Kepler/K}2 survey (LK-MRS), initiated in 2018, aims at collecting medium-resolution spectra (; hereafter MRS) for more than s…

astro-ph.SR2020★ 42 cited

Overview of the LAMOST- project

J. N. Fu, P. De Cat, W. Zong +9

The NASA mission obtained long-term high-quality photometric observations for a large number of stars in its original field of view from 2009 to 2013. In order to provide…