Showing 1–14 of 14 results
/ Date/ Name
Feb 2, 2022The REBELS ALMA Survey: cosmic dust temperature evolution out to z $\sim$ 7Sep 17, 2024Characterizing the contribution of dust-obscured star formation at $z \gtrsim$ 5 using 18 serendipitously identified [CII] emittersSep 25, 2024ALMA observations of super-early galaxies: attenuation-free model predictionsJun 30, 2025Beneath the Surface: >85% of z>5.9 QSOs in Massive Host Galaxies are UV-FaintApr 18, 2023The ALMA REBELS Survey: Discovery of a massive, highly star-forming and morphologically complex ULIRG at $z =7.31$Sep 21, 2021Normal, Dust-Obscured Galaxies in the Epoch of ReionizationSep 29, 2023The ALMA REBELS survey: obscured star formation in massive Lyman-break galaxies at z = 4-8 revealed by the IRX-$β$ and $M_{\star}$ relationsSep 27, 2023The ALMA Reionization Era Bright Emission Line Survey (REBELS): The molecular gas content of galaxies at z~7Feb 28, 2022Spectroscopic confirmation of a gravitationally lensed Lyman break galaxy at z$_{[CII]}$ = 6.827 using NOEMAFeb 22, 2022The ALMA REBELS Survey: the dust content of $z \sim 7$ Lyman Break GalaxiesJun 4, 2022The ALMA REBELS Survey: Average [CII] $158\,\rm{μm}$ sizes of Star-Forming Galaxies from $z\sim 7$ to $z\sim 4$Jun 25, 2021Reionization Era Bright Emission Line Survey: Selection and Characterization of Luminous Interstellar Medium Reservoirs in the z>6.5 UniverseFeb 15, 2022The ALMA REBELS Survey. Epoch of Reionization giants: properties of dusty galaxies at $z \approx 7$Aug 4, 2025The ALMA REBELS survey: [OIII]$_{88μ\text{m}}$ line scans of UV-bright $z \gtrsim 7.6$ galaxies