The faint end of the 250μm luminosity function at z< 0.5

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The faint end of the 250μm luminosity function at z< 0.5

Aims. We aim to study the 250 μm luminosity function (LF) down to much fainter luminosities than achieved by previous efforts. Methods. We developed a modified stacking method to reconstruct the 250 μm LF using optically selected galaxies from the SDSS survey and Herschel maps of the GAMA equatoria...

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Bibliographic Details
Main Authors:	Wang, L., Norberg, P., Bethermin, M., Bourne, N., Cooray, A., Cowley, W., Dunne, L., Dye, S., Eales, S., Farrah, D., Lacey, C., Loveday, J., Maddox, S., Oliver, S., Viero, M.
Format:	Article
Published:	EDP Sciences 2016
Subjects:	submillimeter: galaxies galaxies: statistics methods: statistical galaxies: evolution galaxies: abundances galaxies: luminosity function mass function
Online Access:	https://eprints.nottingham.ac.uk/42356/

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