![Figure 1 from UVI colour gradients of 0.4 < z < 1.4 star-forming main- sequence galaxies in CANDELS: dust extinction and star formation profiles | Semantic Scholar Figure 1 from UVI colour gradients of 0.4 < z < 1.4 star-forming main- sequence galaxies in CANDELS: dust extinction and star formation profiles | Semantic Scholar](https://d3i71xaburhd42.cloudfront.net/fedb2038f2bcf11cdfd189e170fc9d6534aa961c/3-Figure1-1.png)
Figure 1 from UVI colour gradients of 0.4 < z < 1.4 star-forming main- sequence galaxies in CANDELS: dust extinction and star formation profiles | Semantic Scholar
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PG quasars lie above the star-forming galaxy main sequence at z ≈ 0 as... | Download Scientific Diagram
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Figure C2. The star formation main sequence for JINGLE, HRS, KINGFISH,... | Download Scientific Diagram
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The relationship between SFR and stellar mass for star-forming SDSS... | Download Scientific Diagram
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The growth of the central region by acquisition of counterrotating gas in star-forming galaxies | Nature Communications
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Jayne Birkby on Twitter: "Wang gets us all familiar with the galaxy main sequence - a tight correlation between star formation rate and the stellar mass of star forming galaxies #NAC2018 https://t.co/08QoHoY4MB" /
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