Showing 1–20 of 54 results
/ Date/ Name
Oct 15, 2024Ultra Long Period Cepheids as standard candles from Gaia to Rubin-LSSTJun 18, 2024Light curve's recovery with Rubin-LSST: II. UnVEiling the darknesS of The gAlactic buLgE (VESTALE) with RR LyraeDec 16, 2025Why the Northern Hemisphere Needs a 30-40 m Telescope and the Science at Stake: Resolved Stellar Populations Studies in M31 and its SatellitesMay 11, 2015On a new theoretical framework for RR Lyrae stars I: the metallicity dependenceAug 2, 2016The Gaia spectrophotometric standard stars survey - III. Short-term variability monitoringJun 29, 2014Optical and Near-Infrared UBVRIJHK Photometry for the RR Lyrae stars in the Nearby Globular Cluster M4 (NGC 6121)Jun 19, 2018Impact of distance determinations on Galactic structure. II. Old tracersAug 6, 2019On the use of field RR Lyrae as Galactic probes: I. The Oosterhoff dichotomy based on fundamental variablesApr 26, 2019New type II Cepheids from VVV data towards the Galactic centerSep 15, 2020Evolutionary and pulsation properties of Type II CepheidsDec 7, 2018unVEil the darknesS of The gAlactic buLgE (VESTALE)May 28, 2015On the distance of the globular cluster M4 (NGC 6121) using RR Lyrae stars: II. Mid-infrared period-luminosity relationsFeb 10, 2018On the RR Lyrae stars in globulars: V. the complete Near-Infrared (JHKs) census of omega Centauri RR Lyrae variablesMay 8, 2024Cepheids as distance indicators and stellar tracersApr 16, 2021On the Use of Field RR Lyrae as Galactic Probes. III. The $α$-element abundancesDec 3, 2020On the Use of Field RR Lyrae as Galactic Probes. II. A new $Δ$S calibration to estimate their metallicityJul 6, 2020Using classical Cepheids to study the far side of the Milky Way disk: I. Spectroscopic classification and the metallicity gradientMay 23, 2020On the Metamorphosis of the Bailey diagram for RR Lyrae starsJul 2, 2021On the use of field RR Lyrae as Galactic probes: IV. New insights into and around the Oosterhoff dichotomyFeb 16, 2022A new and homogeneous metallicity scale for Galactic classical Cepheids II. The abundance of iron and alpha elements