The MUSE Hubble Ultra Deep Field Survey - XI. Constraining the low-mass end of the stellar mass – star formation rate relation at z < 1
A&A, 619 (2018) A27
Published online: 2018-11-07
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The ALMA Spectroscopic Survey in the Hubble Ultra Deep Field: CO Excitation and Atomic Carbon in Star-forming Galaxies at z = 1–3
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The Variability of Star Formation Rate in Galaxies. II. Power Spectrum Distribution on the Main Sequence
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The ALMA Spectroscopic Survey in the Hubble Ultra Deep Field: Constraining the Molecular Content at log(M*/M⊙) ∼ 9.5 with CO Stacking of MUSE-detected z ∼ 1.5 Galaxies
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An Evolving and Mass-dependent σsSFR–M⋆ Relation for Galaxies
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Statistical Stellar Mass Corrections for High-z Galaxies Observed with JWST Broadband Filters Due to Template Degeneracies
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The ALMA Spectroscopic Survey in the HUDF: Nature and Physical Properties of Gas-mass Selected Galaxies Using MUSE Spectroscopy
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Nonparametric Star Formation History Reconstruction with Gaussian Processes. I. Counting Major Episodes of Star Formation
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Stochastic modelling of star-formation histories I: the scatter of the star-forming main sequence
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Metallicity of stars formed throughout the cosmic history based on the observational properties of star-forming galaxies
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The origin of scatter in the star formation rate–stellar mass relation
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The relative specific Type Ia supernovae rate from three years of ASAS-SN
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The MUSE Hubble Ultra Deep Field Survey
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Impact of inter-correlated initial binary parameters on double black hole and neutron star mergers
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