Showing 1–20 of 47 results
/ Date/ Name
Feb 14, 2019A morphological study of galaxies in ZwCl0024+1652, a galaxy cluster at redshift z $\sim$ 0.4Feb 2, 2022Identification and spectroscopic characterization of 128 new Herbig starsFeb 10, 2015GLACE survey: OSIRIS/GTC Tuneable Filter H$α$ imaging of the rich galaxy cluster ZwCl 0024.0+1652 at z = 0.395. Part I -- Survey presentation, TF data reduction techniques and catalogueSep 8, 2010Search for H alpha emitters in Galaxy Clusters with Tunable FiltersJun 23, 2021The OTELO survey: the star formation rate evolution of low-mass galaxiesApr 21, 2024The Lockman--SpReSO project. Main properties of infrared selected star-forming galaxiesMar 18, 2024GLACE survey: OSIRIS/GTC tuneable imaging of the galaxy cluster ZwCl 0024.0+1652 II. The mass--metallicity relationship and the effect of the environmentMay 27, 2021The OTELO survey: Revealing a population of low-luminosity current/active star-forming galaxies at z$\sim0.9$Mar 27, 2025The OTELO survey: New evidence of downsizing from the specific star formation rates, stellar mass functions, and star formation histories of a sample of low-mass galaxies at 0.38<z<1.43Jan 9, 2024The Lockman-SpReSO project. Galactic flows in a sample of far-infrared galaxiesDec 8, 2020GLACE survey: galaxy activity in ZwCl0024+1652 cluster from strong optical emission linesApr 30, 2015San Pedro Martir observations of microvariability in obscured quasarsSep 12, 2025GLACE survey: OSIRIS/GTC multi-object spectroscopy of the rich galaxy cluster ZwCl 0024.0+1652 at z~0.4. III. The mass-SFR relation and the quenching of cluster galaxiesMay 7, 2021The landscape of promising non-supersymmetric string modelsFeb 16, 2023Higgs-portal dark matter from non-supersymmetric stringsJan 29, 2019U(1)' coupling constant at low energies from heterotic orbifoldsAug 20, 2018Charting the flavor landscape of MSSM-like Abelian heterotic orbifoldsApr 28, 2025The Non-SUSY Orbifolder: a tool to build promising non-supersymmetric string modelsMay 4, 2020Catalogue of new Herbig Ae/Be and classical Be stars. A machine learning approach to Gaia DR2Sep 24, 2021Galaxy And Mass Assembly (GAMA): The environmental impact on SFR and metallicity in galaxy groups