The SAMI Galaxy Survey: spatially resolving the main sequence of star formation

Grants

Funding Acknowledgements

We thank the referee for their thoughtful suggestions to improve the manuscript. Support for A.M.M. is provided by National Aeronautics and Space Administration (NASA) through Hubble Fellowship grant #HST-HF2-51377 awarded by the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., for NASA, under contract NAS5-26555. S.M.C. acknowledges the support of an Australian Research Council Future Fellowship (FT100100457). S.B. acknowledges funding support from the Australian Research Council through a Future Fellowship (FT140101166). B.C. is the recipient of an Australian Research Council Future Fellowship (FT120100660). C.F. gratefully acknowledges funding provided by the Australian Research Council's Discovery Projects (grants DP150104329 and DP170100603). M.S.O. acknowledges the funding support from the Australian Research Council through a Future Fellowship (FT140100255). R.Mc.D. is the recipient of an Australian Research Council Future Fellowship (project number FT150100333). N.S. acknowledges support of a University of Sydney Postdoctoral Research Fellowship. J.v.d.S. is funded under Bland-Hawthorn's Australian Research Council (ARC) Laureate Fellowship (FL140100278).The SAMI Galaxy Survey is based on observations made at the Anglo-Australian Telescope. The SAMI was developed jointly by the University of Sydney and the Australian Astronomical Observatory. The SAMI input catalogue is based on data taken from the Sloan Digital Sky Survey, the GAMA Survey, and the VST ATLAS Survey. The SAMI Galaxy Survey is funded by the Australian Research Council Centre of Excellence for All-sky Astrophysics (CAASTRO), through project number CE110001020, and other participating institutions. The SAMI Galaxy Survey website is http://sami-survey.org/.GAMA is a joint European-Australasian project based around a spectroscopic campaign using the Anglo-Australian Telescope. The GAMA input catalogue is based on data taken from the Sloan Digital Sky Survey and the UKIRT Infrared Deep Sky Survey. Complementary imaging of the GAMA regions is being obtained by a number of independent survey programmes including GALEX MIS, VST KiDS, VISTA VIKING, WISE, Herschel-ATLAS, GMRT, and ASKAP providing ultraviolet to radio coverage. GAMA is funded by the STFC (UK), the ARC (Australia), the AAO, and the participating institutions. The GAMA website is http://www.gama-survey.org/. This work is based on observations made with ESO Telescopes at the La Silla Paranal Observatory under programme IDs 179.A-2004 and 177.A-3016.