Showing 1–20 of 44 results
/ Date/ Name
Sep 30, 2020A new high-precision strong lensing model of the galaxy cluster MACS J0416.1-2403Mar 17, 2023The GLASS-JWST Early Release Science Program. III. Strong lensing model of Abell 2744 and its infalling regionsJan 9, 2024Augmenting the power of time-delay cosmography in lens galaxy clusters by probing their member galaxies. II. Cosmic chronometersMar 19, 2025Euclid Quick Data Release (Q1). The first catalogue of strong-lensing galaxy clustersFeb 13, 2024An improved Magellan weak lensing analysis of the galaxy cluster Abell 2744Jul 23, 2022Early Results from GLASS-JWST. I: Confirmation of Lensed $z\geqslant7$ Lyman-Break Galaxies Behind the Abell 2744 Cluster With NIRISSOct 3, 2023Exploring the low-mass regime of galaxy-scale strong lensing: Insights into the mass structure of cluster galaxiesNov 22, 2022The production of ionizing photons in UV-faint z~3-7 galaxiesNov 16, 2022Early results from GLASS-JWST. XIV: A spectroscopically confirmed protocluster 650 million years after the Big BangJan 17, 2023Early Results from GLASS-JWST. XXI: Rapid assembly of a galaxy at z=6.23 revealed by its C/O abundanceAug 26, 2020Cluster Strong Lensing with Hierarchical InferenceOct 24, 2024The Dual Nature of GHZ9: Coexisting Active Galactic Nuclei and Star Formation Activity in a Remote X-ray Source at z = 10.145Dec 1, 2025Image simulations of highly magnified clumpy galaxiesNov 10, 2021VLT/MUSE observations of SDSS J1029+2623: towards a high-precision strong lensing modelApr 19, 2022Galaxies in the central regions of simulated galaxy clustersFeb 21, 2024Diverse Oxygen Abundance in Early Galaxies Unveiled by Auroral Line Analysis with JWSTDec 13, 2022Early Results from GLASS-JWST. XIX: A High Density of Bright Galaxies at $z\approx10$ in the Abell 2744 RegionOct 27, 2022The nature of an ultra-faint galaxy in the cosmic Dark Ages seen with JWSTMar 15, 2024A luminous and young galaxy at z=12.33 revealed by a JWST/MIRI detection of Hα and [OIII]May 12, 2025Galaxy cluster virial quantities from extrapolating strong lensing mass profiles