1 INTRODUCTION
2 DATA
2.1 Galaxy Sample
2.2 Photometric Properties
2.3 Visual Morphologies
2.4 Stellar Masses
2.5 Star-Formation Rates
2.6 Sampling and Volume Corrections
3 SELECTING QUENCHED GALAXIES
3.1 Quantifying “Young”
3.2 Quenched Galaxy Sample
4 THE PHYSICAL PROPERTIES OF QUENCHED GALAXIES
4.1 Global Colours
4.2 Visual and Quantitative Morphology
4.3 Incidence of AGN
5 DISCUSSION
5.1 The Relationship Between Quenching and Morphology
5.2 Where Do Post-Starburst Galaxies Fit In?
5.3 What Quenches Star Formation?
6 CONCLUSIONS