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In March 2013, the Sydney--AAO Multi-object Integral field spectrograph(SAMI) began a major survey of 3400 galaxies at the AAT, the largest of itskind to date. At the time of writing, over a third of the targets have beenobserved and the scientific impact has been immediate. The Manga galaxy surveyhas now started at the SDSS telescope and will target an even larger sample ofnearby galaxies. In Australia, the community is now gearing up to deliver amajor new facility called Hector that will allow integral field spectroscopy of100 galaxies observed simultaneously. By the close of the decade, it will bepossible to obtain integral field spectroscopy of 100,000 galaxies over 3000square degrees of sky down to r=17 (median). Many of these objects will have HIimaging from the new ASKAP radio surveys. We discuss the motivation for such asurvey and the use of new cosmological simulations that are properly matched tothe integral field observations. The Hector survey will open up a new andunique parameter space for galaxy evolution studies.

The Hector Survey: integral field spectroscopy of 100,000 galaxies