Showing 1–20 of 44 results
/ Date/ Name
Jan 17, 2019Stellar populations of galaxies in the ALHAMBRA survey up to $z \sim 1$. IV. Properties of quiescent galaxies on the stellar mass$-$size planeFeb 25, 2021The miniJPAS survey: Identification and characterization of galaxy populations with the J-PAS photometric systemJul 15, 2020The miniJPAS survey: star-galaxy classification using machine learningNov 28, 2017Stellar populations of galaxies in the ALHAMBRA survey up to $z \sim 1$. II. Stellar content of quiescent galaxies within the dust-corrected stellar mass$-$colour and the $UVJ$ colour$-$colour diagramsSep 3, 2014The ALHAMBRA survey: Accurate merger fractions by PDF analysis of photometric close pairsNov 12, 2025J-PAS: A Neural Network Approach to Single Stellar Population CharacterizationSep 3, 2025J-PLUS: The stellar mass function of quiescent and star-forming galaxies at 0.05 <= z <= 0.2Aug 6, 2021The miniJPAS survey: the photometric redshift catalogueApr 4, 2022The miniJPAS survey: Identification and characterization of the emission line galaxies down to $z < 0.35$ in the AEGIS fieldJan 23, 2023J-NEP: 60-band photometry and photometric redshifts for the James Webb Space Telescope North Ecliptic Pole Time-Domain FieldMay 26, 2015Extracting H$α$ flux from photometric data in the J-PLUS surveyAug 12, 2015The ALHAMBRA survey : Estimation of the clustering signal encoded in the cosmic varianceNov 28, 2016The ALHAMBRA survey : $B-$band luminosity function of quiescent and star-forming galaxies at $0.2 \leq z < 1$ by PDF analysisNov 29, 2023The miniJPAS survey. Evolution of the luminosity and stellar mass functions of galaxies up to $z \sim 0.7$Apr 8, 2018J-PLUS: The Javalambre Photometric Local Universe SurveySep 4, 2025J-PAS: Discovery of RaJav, a bright spatially extended Ly$α$ Nebula at z=2.25Jul 1, 2022The miniJPAS Survey: Detection of double-core Lyα morphology of two high-redshift (z>3) QSOsMay 19, 2025Spatially resolved stellar populations and emission lines properties in nearby galaxies with J-PLUS -- I. Method and first results for the M101 groupApr 1, 2026OJALÁ: Optimizing J-PAS Astronomy for Large-scale Analysis. A foundation model for the SED of galaxies, QSOs and starsJul 12, 2022The miniJPAS survey: The role of group environment in quenching the star formation