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

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.

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


Authors

L. Wang

P. Norberg

M. Bethermin

N. Bourne

A. Cooray

W. Cowley

L. Dunne

SIMON DYE Simon.Dye@nottingham.ac.uk
Professor of Astrophysics

S. Eales

D. Farrah

C. Lacey

J. Loveday

S. Maddox

S. Oliver

M. Viero



Abstract

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 equatorial fields and Stripe 82. Our stacking method not only recovers the mean 250 μm luminosities of galaxies that are too faint to be individually detected, but also their underlying distribution functions.
Results. We find very good agreement with previous measurements in the overlapping luminosity range. More importantly, we are able to derive the LF down to much fainter luminosities (~ 25 times fainter) than achieved by previous studies. We find strong positive luminosity evolution L*250(z)∝(1+z)4.89±1.07 and moderate negative density evolution Φ*250(z)∝(1+z)-1.02±0.54 over the redshift range 0.02 <z< 0.5.

Citation

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. (in press). The faint end of the 250μm luminosity function at z< 0.5. Astronomy and Astrophysics, 592, Article L5. https://doi.org/10.1051/0004-6361/201629076

Journal Article Type Article
Acceptance Date Jul 1, 2016
Online Publication Date Aug 2, 2016
Deposit Date Apr 27, 2017
Publicly Available Date Apr 27, 2017
Journal Astronomy & Astrophysics
Electronic ISSN 1432-0746
Publisher EDP Sciences
Peer Reviewed Peer Reviewed
Volume 592
Article Number L5
DOI https://doi.org/10.1051/0004-6361/201629076
Keywords submillimeter: galaxies, galaxies: statistics, methods: statistical, galaxies: evolution, galaxies: abundances, galaxies: luminosity function, mass function
Public URL https://nottingham-repository.worktribe.com/output/806934
Publisher URL http://www.aanda.org/articles/aa/abs/2016/08/aa29076-16/aa29076-16.html
Contract Date Apr 27, 2017

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