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...
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 |
Language: | English |
Published: |
EDP Sciences
2016
|
Online Access: | http://eprints.nottingham.ac.uk/42356/ http://eprints.nottingham.ac.uk/42356/ http://eprints.nottingham.ac.uk/42356/ http://eprints.nottingham.ac.uk/42356/1/%28Dye%20faint%20end%29.pdf |
Similar Items
-
Herschel-ATLAS: multi-wavelength SEDs and physical properties of 250 μm selected galaxies at z < 0.5
by: Smith, D., et al.
Published: (2012) -
Herschel-ATLAS/GAMA: how does the far-IR luminosity function depend on galaxy group properties?
by: Guo, Q., et al.
Published: (2014) -
Not for the faint of heart
by: Ann-Marie, Urban, et al.
Published: (2014) -
Ultraviolet luminosity density of the universe during the epoch of reionization
by: Mitchell-Wynne, Ketron, et al.
Published: (2015) -
The HerMES submillimetre local and low-redshift luminosity functions*
by: Marchetti, L., et al.
Published: (2015)