Herschel-ATLAS/GAMA: how does the far-IR luminosity function depend on galaxy group properties?

Herschel-ATLAS/GAMA: how does the far-IR luminosity function depend on galaxy group properties?

We use the Herschel Astrophysical Terahertz Large Area Survey (H-ATLAS) Phase I data to study the conditional luminosity function of far-IR (250 μm) selected galaxies in optically selected galaxy groups from the Galaxy And Mass Assembly (GAMA) spectroscopic survey, as well as environmental effects o...

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Bibliographic Details
Main Authors: Guo, Q., Lacey, C., Norberg, P., Cole, S., Baugh, C., Frenk, C., Cooray, A., Dye, S., Bourne, N., Dunne, L., Eales, S., Ivison, R.J., Maddox, S.J., Alpasan, M., Baldry, I., Bland-Hawthorn, J., Driver, S.P., Robotham, A.
Format: Article
Published: Oxford University Press 2014
Subjects:
galaxies: clusters: general
galaxies: formation
galaxies: haloes
galaxies: luminosity function
mass function
cosmology: theory
infrared: galaxies
Online Access:https://eprints.nottingham.ac.uk/42410/

Internet

https://eprints.nottingham.ac.uk/42410/

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