Candidate high-z proto-clusters among the Planck compact sources, as revealed by Herschel-SPIRE

Candidate high-z proto-clusters among the Planck compact sources, as revealed by Herschel-SPIRE

By determining the nature of all the Planck compact sources within 808.4 deg2 of large Herschel surveys, we have identified 27 candidate proto-clusters of dusty star forming galaxies (DSFGs) that are at least 3σ overdense in either 250, 350 or 500 μm sources. We find roughly half of all the Planck c...

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Bibliographic Details
Main Authors: Greenslade, J., Clements, D.L., Cheng, T., De Zotti, G., Scott, D., Valiante, E., Eales, S., Bremer, M.N., Dannerbauer, H., Birkinshaw, M., Farrah, D., Harrison, D.L., Michałowski, M.J., Valtchanov, I., Oteo, I., Baes, M., Cooray, A., Negrello, M., Wang, L., van der Werf, P., Dunne, L., Dye, S.
Format: Article
Published: Oxford University Press 2018
Subjects:
galaxies: clusters: general; submillimetre: galaxies; infrared: galaxies; galaxies: evolution
Online Access:https://eprints.nottingham.ac.uk/50331/

Internet

https://eprints.nottingham.ac.uk/50331/

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