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Galaxy And Mass Assembly (GAMA): The star formation rate dependence of the stellar initial mass function

, , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , and . (2011)cite arxiv:1104.2379 Comment: 18 pages, 15 figures, accepted for publication in MNRAS. Image resolution has been reduced. For the full resolution version, see http://www.gama-survey.org/pubs/papers/imf_sfr.pdf.

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P-MaNGA Galaxies: Emission Lines Properties - Gas Ionisation and Chemical Abundances from Prototype Observations, , , , , , , , , and 20 other author(s). (2014)cite arxiv:1410.7781Comment: 37 pages, 28 figures, resubmitted to MNRAS after addressing the referee report.Comparison of Stellar Population Model Predictions Using Optical and Infrared Spectroscopy, , , , and . (2017)cite arxiv:1709.09300Comment: 26 pages, 21 figures, accepted for publication in MNRAS.The Dark Energy Survey: more than dark energy - an overview, , , , , , , , , and 131 other author(s). Monthly Notices of the Royal Astronomical Society, 460 (2): 1270--1299 (Aug 19, 2016)Galaxy And Mass Assembly (GAMA): The star formation rate dependence of the stellar initial mass function, , , , , , , , , and 28 other author(s). (2011)cite arxiv:1104.2379 Comment: 18 pages, 15 figures, accepted for publication in MNRAS. Image resolution has been reduced. For the full resolution version, see http://www.gama-survey.org/pubs/papers/imf_sfr.pdf.