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PublicationWe present the stellar mass-metallicity relation (MZR) and mass-metallicity-star formation relation ("fundamental metallicity relation"; FMR) of 18 massive (log(M/M\(_\odot\)) = 9.5-11 …
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PublicationRecent JWST observations reveal massive, UV-bright galaxies at z>10 with little apparent dust attenuation, whereas ALMA detections at z≃7 show similarly massive systems that are …
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PublicationWe investigate the impacts of the evolution of dust mass and grain size distribution within a Milky Way-like (MW-like) galaxy simulation on global attenuation curves, focusing …
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PublicationWe present deep ALMA Band 7 observations of the [OIII] \(88μ\)m line and underlying dust continuum emission in four UV-bright, gravitationally lensed (magnification …
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PublicationWe present deep ALMA Band 7 observations of the [OIII] \(88μ\)m line and underlying dust continuum emission in four UV-bright, gravitationally lensed (magnification …
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PublicationWe present deep ALMA Band 7 observations of the [OIII] \(88μ\)m line and underlying dust continuum emission in four UV-bright, gravitationally lensed (magnification …
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PublicationDetermining the physical properties of galaxies during the first billion years after the big bang is key to understanding both early galaxy evolution and how galaxies contributed to …
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PublicationJWST has revealed a new high-redshift population called little red dots (LRDs). Since LRDs may be in the early phase of black hole growth, identifying them in …
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PublicationStar formation in galaxies is regulated by the interplay of a range of processes that shape the multiphase gas in the interstellar and circumgalactic media. Using the Cosmology …
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PublicationDespite the implied presence of dust through reddened UV emission in high-redshift galaxies, no dust emission has been detected in the (sub)millimetre regime beyond …
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PublicationWe perform the first direct cosmological and astrophysical parameter inference from the combination of galaxy luminosity functions and colours using a simulation-based inference approach. Using the SYNTHESIZER …
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PublicationWe present an Atacama Large Millimeter/submillimeter Array (ALMA) Band 9 continuum detection (\(3.3 \sigma\)) of MACS0416_Y1 that confirms the suspected warm dust (91 …
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PublicationMeasuring the ionizing photon production efficiency \(ξ_{\mathrm{ion,0}}\) -- the ratio of ionizing photon output rate \(Q_{\rm H^0}\) to UV continuum luminosity …
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PublicationIn recent years, observations with the JWST have started to map out the rapid metal enrichment of the early Universe, while (sub)millimeter observations have simultaneously begun to …
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PublicationCharacterizing dust attenuation is crucial for revealing the intrinsic physical properties of galaxies. We present an analysis of dust attenuation in 18 spectroscopically confirmed star-forming main-sequence …
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PublicationThe number density of UV luminous galaxies discovered by the James Webb Space Telescope at ultra high redshift (z ≳ 10) is higher, and declines much more slowly with …
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PublicationWe deploy the new ARKENSTONE galactic wind model in cosmological simulations for the first time, allowing us to robustly resolve the evolution and impact of high specific energy …
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PublicationWe present new ALMA [OIII]\(_{88}\) observations of eight previously [CII]\(_{158}\)-detected galaxies at \(6.8 \lesssim z \lesssim 7.7\). Six of our targets -- the primary …
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Publication… Universe Collaboration.
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PublicationWe report the first successful Atacama Large Millimeter/submillimeter Array (ALMA) follow-up observations of a secure z > 10 JWST-selected galaxy, by robustly detecting (6.6σ) the …
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PublicationWe present Keck/MOSFIRE H-band spectroscopic measurements covering the [CIII]1907, CIII]1909 doublet for a sample of 8 z~7 spectroscopically-confirmed star-forming galaxies drawn …
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PublicationSynthesizer is a fast, flexible, modular, and extensible Python package that empowers astronomers to turn theoretical galaxy models into realistic synthetic observations - including spectra, photometry, images, and spectral …
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PublicationDetermining the dust properties of high-redshift galaxies from their far-infrared continuum emission is challenging due to limited multi-frequency data. As a result, the dust spectral …
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PublicationWe present measurements of the dust attenuation curves of 12 massive ( …
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PublicationContext. Molecular Clouds (MCs) are the place where stars are formed and their feedback starts to take place, regulating the evolution of galaxies. Therefore, MCs represent the critical …
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PublicationWe present deep ALMA observations targeting the [CII]\(_{158\mu m}\,\) line in JADES-GS-z14-0, the most distant known galaxy at z=14.1793. We do …
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PublicationMetallicity is a crucial tracer of galaxy evolution, providing insights into gas accretion, star formation, and feedback. At high redshift, these processes reveal how early galaxies assembled and …
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PublicationSome hydrogen-rich core-collapse supernovae (type IIP SNe) exhibit evidence for a sustained energy source powering their light curves, resulting in a brighter and/or longer-lasting …
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PublicationWe present high resolution (\(\sim0.14\)" = 710 pc) ALMA [CII] 158\(\mu\)m and dust continuum follow-up observations of REBELS-25, a [CII]-luminous ( …
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PublicationWe present Atacama Large Millimetre/submillimetre Array (ALMA) observations of the [O III] 88 \(\mu {\rm m}\) emission of a sample of thirteen galaxies at \(z = 6\) to …
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PublicationOur knowledge of galaxy formation and evolution has incredibly progressed through multi-wavelength observational constraints of the interstellar medium (ISM) of galaxies at all cosmic epochs. However, little …
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PublicationWe exploit moderately resolved [OIII], [CII] and dust continuum ALMA observations to derive the gas density (\(n\)), the gas-phase metallicity (\(Z\)) and the deviation from the Kennicutt …
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PublicationWe present new ALMA Band 8 (rest-frame \(90\,\mu\)m) observations of three massive (\(M_\star \approx 10^{10}\,M_\odot\)) galaxies at \(z\approx7\) previously detected …