Showing 1–16 of 16 results
/ Date/ Name
Dec 4, 2025Little red dot variability over a century reveals black hole envelope via a giant Einstein crossNov 18, 2025VENUS: A Strongly Lensed Clumpy Galaxy at $z\sim11-12$ behind the Galaxy Cluster MACS J0257.1-2325Jun 19, 2025Taking a Break at Cosmic Noon: Continuum-selected Low-mass Galaxies Require Long Burst CyclesMay 20, 2025The first direct imaging of the silhouette of a damped Lyman $α$ system along the line-of-sight to a background galaxySep 26, 2024A Giant Disk Galaxy Two Billion Years After The Big BangSep 5, 2023Accelerated Formation of Ultra-Massive Galaxies in the First Billion YearsAug 4, 2022Schrodinger's Galaxy Candidate: Puzzlingly Luminous at $z\approx17$, or Dusty/Quenched at $z\approx5$?Mar 17, 2022The UV 2175Å Attenuation Bump and its Correlation with PAH Emission at z~2Mar 10, 2022The MUSE Extremely Deep Field: a first panoramic view of an Mg II emitting intragroup mediumNov 29, 2021Deciphering stellar metallicities in the early Universe: Case study of a young galaxy at z = 4.77 in the MUSE eXtremely Deep FieldMay 26, 2021Measuring the average molecular gas content of star-forming galaxies at $z=3-4$Aug 4, 2020The nature of CR7 revealed with MUSE: a young starburst powering extended Lyman-$α$ emission at z=6.6Mar 21, 2019The ALMA Spectroscopic Survey in the HUDF: Nature and physical properties of gas-mass selected galaxies using MUSE spectroscopyFeb 15, 2019Exploring HeII$λ$1640 emission line properties at ${z\sim2-4}$Nov 1, 2018The clustering of typical Ly$α$ emitters from $z \sim 2.5 - 6$: host halo masses depend on Ly$α$ and UV luminositiesMay 2, 2017The clustering of H$β$+[OIII] and [OII] emitters since $z \sim 5$: dependencies with line luminosity and stellar mass