Showing 1–20 of 30 results
/ Date/ Name
Apr 24, 2026The circumstellar environment of the young, low-mass dipper star JH 223. Accretion and large-scale magnetic field topologyNov 4, 2025Demonstration of Sub-Percent Energy Resolution in the NEXT-100 DetectorNov 3, 2025First results of the NEXT-100 detector using $^{83m}$Kr decaysMay 23, 2025The NEXT-100 DetectorMay 2, 2025High Voltage Delivery and Distribution for the NEXT-100 Time Projection ChamberFeb 18, 2025Performance of an Optical TPC Geant4 Simulation with Opticks GPU-Accelerated Photon PropagationFeb 14, 2025Reconstructing neutrinoless double beta decay event kinematics in a xenon gas detector with vertex taggingNov 29, 2024A New Look at Disk Winds and External Photoevaporation in the $σ$-Orionis ClusterNov 20, 2024EWOCS-III: JWST observations of the supermassive star cluster Westerlund 1Aug 20, 2024EWOCS-II: X-ray properties of the Wolf-Rayet stars in the young Galactic super star cluster Westerlund 1May 30, 2024Measurement of Energy Resolution with the NEXT-White Silicon PhotomultipliersMay 20, 2024Fluorescence Imaging of Individual Ions and Molecules in Pressurized Noble Gases for Barium Tagging in $^{136}$XeMar 6, 2024Long period modulation of the classical T Tauri star CI Tau: evidence for an eccentric close-in massive planet at 0.17 auDec 14, 2023EWOCS-I: The catalog of X-ray sources in Westerlund 1 from the Extended Westerlund 1 and 2 Open Clusters SurveyJan 11, 2023New members of the Lupus I cloud based on Gaia astrometry Physical and accretion properties from X-Shooter spectraJun 6, 2022The Gaia-ESO Public Spectroscopic Survey: Implementation, data products, open cluster survey, science, and legacyMay 11, 2021The Gaia-ESO survey: Mixing processes in low-mass stars traced by lithium abundance in cluster and field starsFeb 6, 2020The Gaia-ESO Survey: detection and characterization of single line spectroscopic binariesJan 9, 2020The Gaia-ESO Survey: a new approach to chemically characterising young open clustersJul 17, 2018The Gaia-ESO Survey: the N/O abundance ratio in the Milky Way