Showing 1–20 of 60 results
/ Date/ Name
Apr 13, 2026The RoPES project with HARPS and HARPS-N III. Two candidate planets orbiting the G-type star HD 161098Oct 20, 2025Euclid preparation: The flat-sky approximation for the clustering of Euclid's photometric galaxiesOct 10, 2025Euclid preparation. Cosmology Likelihood for Observables in Euclid (CLOE). 3. Inference and ForecastsAug 19, 2025Two warm Earth-sized exoplanets and an Earth-sized candidate in the M5V-M6V binary system TOI-2267Jun 10, 2025Euclid preparation: The NISP spectroscopy channel, on ground performance and calibrationMay 7, 2025Euclid preparation. The impact of redshift interlopers on the two-point correlation function analysisMar 19, 2025Euclid Quick Data Release (Q1): First visual morphology catalogueMar 11, 2025HADES RV Programme with HARPS-N at TNG. XVI. A super-Earth in the habitable zone of the GJ 3998 multi-planet systemFeb 10, 2025Euclid: A complete Einstein ring in NGC 6505Jul 19, 2024ANDES, the high resolution spectrograph for the ELT: science goals, project overview and future developmentsMay 22, 2024Euclid: Early Release Observations -- Programme overview and pipeline for compact- and diffuse-emission photometryOct 24, 2023Euclid preparation. LII. Forecast impact of super-sample covariance on 3x2pt analysis with EuclidMar 9, 2022HADES RV Programme with HARPS-N at TNG XV. Planetary occurrence rates around early-M dwarfsNov 11, 2021The Gamow Explorer: A gamma-ray burst observatory to study the high redshift universe and enable multi-messenger astrophysicsMar 17, 2021HADES RV Programme with HARPS-N at TNG XIII. A sub-Neptune around the M dwarf GJ 720 AFeb 18, 2021A super-Earth on a close-in orbit around the M1V star GJ 740. A HADES and CARMENES collaborationNov 6, 2020Measuring and characterizing the line profile of HARPS with a laser frequency combOct 28, 2020HADES RV Programme with HARPS-N at TNG XII. The abundance signature of M dwarf stars with planetsDec 17, 2018Stellar activity analysis of Barnard's Star: Very slow rotation and evidence for long-term activity cycleFeb 13, 2018The QUIJOTE Experiment: Prospects for CMB B-MODE polarization detection and foregrounds characterization