Showing 1–20 of 61 results
/ Date/ Name
Sep 2, 2022Automatic model-based telluric correction for the ESPRESSO data reduction software. Model description and application to radial velocity computationMay 25, 2020Revisiting Proxima with ESPRESSOSep 17, 2020The MUSE Deep Lensed Field on the Hubble Frontier Field MACS~J0416Feb 3, 2021Stellar astrophysics in the near UV with VLT-CUBESSep 4, 2017Solving the conundrum of intervening strong MgII absorbers towards GRBs and quasarsJul 29, 2016XQ-100: A legacy survey of one hundred 3.5 < z < 4.5 quasars observed with VLT/XSHOOTERJul 15, 2024Extragalactic 85Rb/87Rb and 6Li/7Li ratios in the Small Magellanic CloudOct 21, 2025Unveiling the nature of HE 0107-5240Oct 12, 2012Interacting Supernovae and Supernova Impostors. SN 2009ip, is this the end?Jan 6, 2023The pristine nature of SMSS 1605$-$1443 revealed by ESPRESSOMay 3, 2023Evidence of First Stars-enriched Gas in High-redshift AbsorbersAug 2, 2022CUBES, the Cassegrain U-Band Efficient SpectrographJan 10, 2020Candidate Population III stellar complex at z=6.629 in the MUSE Deep Lensed FieldAug 10, 2020The spectroscopic follow-up of the QUBRICS bright quasar surveyMar 18, 2021The Luminosity Function of bright QSOs at z~4 and implications for the cosmic ionizing backgroundNov 16, 2015The evolution of neutral gas in damped Lyman $α$ systems from the XQ-100 surveyDec 20, 2017Direct Lyman continuum and Lyman-alpha escape observed at redshift 4Mar 4, 2016High-resolution spectroscopy of a young, low-metallicity optically-thin L=0.02L* star-forming galaxy at z=3.12Nov 11, 2016Exploring the Thermal State of the Low-Density Intergalactic Medium at z=3 with an Ultra-High Signal-to-Noise QSO SpectrumJul 24, 2024End-to-End simulation framework for astronomical spectrographs: SOXS, CUBES and ANDES