Showing 1–20 of 36 results
/ Date/ Name
Sep 20, 2023An optimal ALMA image of the Hubble Ultra Deep Field in the era of JWST: obscured star formation and the cosmic far-infrared backgroundOct 24, 2018The SCUBA-2 Web Survey: I. Observations of CO(3-2) in hyper-luminous QSO fieldsAug 14, 2017An application of an optimal statistic for characterising relative orientationsFeb 26, 2020Megaparsec-scale structure around the proto-cluster core SPT2349$-$56 at $z\,{=}\,4.3$Oct 5, 2017High-resolution SMA imaging of bright submillimetre sources from the SCUBA-2 Cosmology Legacy SurveyApr 18, 2018Using ALMA to resolve the nature of the early star-forming large-scale structure PLCK G073.4-57.5Sep 9, 2021Rapid build-up of the stellar content in the protocluster core SPT2349$-$56 at $z\,{=}\,4.3$Jan 28, 2019A machine learning approach for identifying the counterparts of submillimetre galaxies and applications to the GOODS-North fieldFeb 11, 2018The Spectrum of the UniverseNov 30, 2024An ALMA spectroscopic survey of the Planck high-redshift object PLCK G073.4-57.5 confirms two protoclustersMar 15, 2024Mitigation and optimization of induced seismicity using physics-based forecastingFeb 25, 2022Multi-Phase ISM in the z = 5.7 Hyperluminous Starburst SPT0346-52Jan 3, 2023Brightest Cluster Galaxy Formation in the z=4.3 Protocluster SPT2349-56: Discovery of a Radio-Loud AGNMar 28, 2022Chaotic and Clumpy Galaxy Formation in an Extremely Massive Reionization-Era HaloJun 5, 2023Spatial variations in aromatic hydrocarbon emission in a dust-rich galaxySep 20, 2024Kinematic analysis of $\mathbf{z = 4.3}$ galaxies in the SPT2349$-$56 protocluster coreSep 4, 2025A large thermal energy reservoir in the nascent intracluster medium at a redshift of 4.3Oct 6, 2020Overdensities of Submillimetre-Bright Sources around Candidate Protocluster Cores Selected from the South Pole Telescope SurveyNov 21, 2025An Overabundance of Radio-AGN in the SPT2349-56 Protocluster: Preheating the Intra-Cluster MediumDec 4, 2024Improving Optical Photo-z Constraints for Dusty Star-forming Galaxies Using Submillimeter-based Priors