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Galaxy And Mass Assembly (GAMA): The connection between metals, specific-SFR, and HI gas in galaxies: the Z-SSFR relation

, , , , , , , , , , , , and . (2013)cite arxiv:1304.3889Comment: Accepted for publication as a letter in MNRAS. 5 pages and 4 figures.

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Herschel Far-IR counterparts of SDSS galaxies: Analysis of commonly used Star Formation Rate estimates, , , , , , , , , and 6 other author(s). (2014)cite arxiv:1403.3615Comment: 24 pages, 23 figures, accepted for publication in MNRAS.Galaxy And Mass Assembly: Evolution of the Halpha luminosity function and star formation rate density up to z<0.35, , , , , , , , , and 21 other author(s). (2013)cite arxiv:1305.5308Comment: 27 pages, 20 figures, accepted for publication in MNRAS.VALES: II. The physical conditions of interstellar gas in normal star-forming galaxies up to z=0.2 revealed by ALMA, , , , , , , , , and 11 other author(s). (2016)cite arxiv:1611.05867Comment: Accepted for publication in A&A. Abstract abridged for arXiv. 13 pages, including 5 figures and 2 tables.Galaxy And Mass Assembly (GAMA): The connection between metals, specific-SFR, and HI gas in galaxies: the Z-SSFR relation, , , , , , , , , and 3 other author(s). (2013)cite arxiv:1304.3889Comment: Accepted for publication as a letter in MNRAS. 5 pages and 4 figures.Galaxy And Mass Assembly (GAMA): growing up in a bad neighbourhood - how do low-mass galaxies become passive?, , , , , , , , , and 6 other author(s). (2015)cite arxiv:1511.02245Comment: 20 pages, 12 figures, Accepted to MNRAS.