Showing 1–14 of 14 results
/ Date/ Name
Mar 22, 2023The impact of AGN-driven winds on physical and observable galaxy sizesNov 21, 2022Predicting sub-millimeter flux densities from global galaxy propertiesNov 28, 2018The Origins of the Circumgalactic Medium in the FIRE SimulationsOct 2, 2019The Fates of the Circumgalactic Medium in the FIRE SimulationsMay 30, 2019Predictions for the spatial distribution of the dust continuum emission in 1<z<5 star-forming galaxiesSep 20, 2012On the shape of the mass-function of dense clumps in the Hi-GAL fields. I. SED determination and global properties of the mass-functionsNov 12, 2013On the shape of the mass-function of dense clumps in the Hi-GAL fields. II. Using Bayesian inference to study the clump mass functionSep 14, 2023Energy balance SED modelling can be effective at high redshifts regardless of UV-FIR offsetsNov 3, 2022Dust temperature uncertainties hamper the inference of dust and molecular gas masses from the dust continuum emission of quiescent high-redshift galaxiesOct 13, 2023Disappearing galaxies: the orientation dependence of JWST-bright, HST-dark, star-forming galaxy selectionAug 19, 2016Low-Redshift Lyman Limit Systems as Diagnostics of Cosmological Inflows and OutflowsMay 11, 2010A Herschel study of YSO evolutionary stages and formation timelines in two fields of the Hi-GAL surveyOct 24, 2023Beware the recent past: a bias in spectral energy distribution modelling due to bursty star formationJun 17, 2024Deciphering the imprint of AGN feedback in Seyfert galaxies: Nuclear-scale molecular gas deficits