The evolution of the dust and gas content in galaxies
A&A, 562 (2014) A30
Published online: 2014-02-03
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Multiwavelength dissection of a massive heavily dust-obscured galaxy and its blue companion at z∼2
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From Haloes to Galaxies. II. The Fundamental Relations in Star Formation and Quenching
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The ALMA Spectroscopic Survey in the HUDF: The Cosmic Dust and Gas Mass Densities in Galaxies up to z ∼ 3
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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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The Evolution of the Star-Forming Interstellar Medium Across Cosmic Time
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A Significant Excess in Major Merger Rate for AGNs with the Highest Eddington Ratios at z < 0.2
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GOODS-ALMA: The slow downfall of star formation in z = 2–3 massive galaxies
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Detecting outliers in astronomical images with deep generative networks
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New Analytic Solutions for Galaxy Evolution. II. Wind Recycling, Galactic Fountains, and Late-type Galaxies
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S2COSMOS: Evolution of gas mass with redshift using dust emission
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Both starvation and outflows drive galaxy quenching
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In pursuit of giants
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The ISM scaling relations in DustPedia late-type galaxies: A benchmark study for the Local Universe
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Local Starburst Conditions and Formation of GRB 980425/SN 1998bw within a Collisional Ring
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SOFIA/HAWC+ View of an Extremely Luminous Infrared Galaxy: WISE 1013+6112
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Semi-analytic forecasts forJWST– I. UV luminosity functions atz = 4–10
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Disentangling the physical parameters of gaseous nebulae and galaxies
Akio K Inoue and Daichi KashinoMonthly Notices of the Royal Astronomical Society 486 (1) 1053 (2019)
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Impact of galactic interactions on the evolution of the far-infrared–radio correlation
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