The star formation reference survey - I. Survey description and basic data

@article{Ashby2011TheSF,
  title={The star formation reference survey - I. Survey description and basic data},
  author={M. Ashby and S. Mahajan and H. A. Smith and S. Willner and G. Fazio and S. Raychaudhury and A. Zezas and P. Barmby and P. Bonfini and C. Cao and E. Gonz{\'a}lez-Alfonso and D. Ishihara and H. Kaneda and V. Lyttle and S. Madden and C. Papovich and E. Sturm and J. Surace and H. Wu and Y.-N. Zhu Harvard-Smithsonian Center for Astrophysics and Usa and U. Birmingham and Uk and U. O. Crete and Greece. and U. W. Ontario and Canada. and Shandong University at Weihai and China. and Universidad de Alcal'a de Henares and Deptamento de F'isica and Spain. and N. University and Japan. and CEASaclay and France. and Texas AM University and Mpe and H Germany and Spitzer Science Center and National Astronomical Observatories},
  journal={Publications of the Astronomical Society of the Pacific},
  year={2011},
  volume={123},
  pages={1011-1029}
}
ABSTRACT.Star formation is arguably the most important physical process in the cosmos. It is a fundamental driver of galaxy evolution and the ultimate source of most of the energy emitted by galaxies in the local universe. A correct interpretation of star formation rate (SFR) measures is therefore essential to our understanding of galaxy formation and evolution. Unfortunately, however, no single SFR estimator is universally available or even applicable in all circumstances: the numerous… Expand
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