Showing 1–15 of 15 results
/ Date/ Name
Oct 1, 2025Ly-alpha emission reveals two satellite halos around massive groups at z ~ 3: the puzzling case of a quiescent central galaxySep 4, 2025A large thermal energy reservoir in the nascent intracluster medium at a redshift of 4.3Jul 15, 2025The ALMA-CRISTAL survey: Resolved kinematic studies of main sequence star-forming galaxies at 4<z<6Apr 24, 2025Hot Diggity Dog: Simultaneous CO and Dust Modeling of the Most Luminous WISE Hot Dust-Obscured Galaxy Unveils Extreme Molecular Gas ExcitationApr 18, 2025Resolving the black hole sphere of influence in a hyper-luminous obscured quasar at redshift 4.6Feb 14, 2025Spatially resolved dust properties over 50 kpc in a hyperluminous galaxy merger at $z = 4.6$Dec 5, 2024Overdensity of Lyman-Break Galaxy Candidates Around Hot Dust-Obscured GalaxiesMay 9, 2024REBELS-25: Discovery of a dynamically cold disc galaxy at z = 7.31Jan 13, 2023A NOEMA molecular line scan of the Hubble Deep Field North: Improved constraints on the CO luminosity functions and cosmic density of molecular gasAug 17, 2022The ALMA REBELS Survey: The Dust-obscured Cosmic Star Formation Rate Density at Redshift 7Mar 28, 2022The ALMA REBELS Survey: Dust Continuum Detections at z > 6.5May 26, 2021Measuring the average molecular gas content of star-forming galaxies at $z=3-4$Sep 22, 2020The ALMA Spectroscopic Survey Large Program: The Infrared Excess of z=1.5-10 UV-selected Galaxies and the Implied High-Redshift Star Formation HistorySep 9, 2020The ALMA Spectroscopic Survey in the HUDF: CO Excitation and Atomic Carbon in Star-Forming Galaxies at $z=1-3$Mar 21, 2019The ALMA Spectroscopic Survey in the HUDF: Nature and physical properties of gas-mass selected galaxies using MUSE spectroscopy