Candidate high-z proto-clusters among the Planck compact sources, as revealed by Herschel-SPIRE
(2018)
Journal Article
Greenslade, J., Clements, D., Cheng, T., De Zotti, G., Scott, D., Valiante, E., Eales, S., Bremer, M., Dannerbauer, H., Birkinshaw, M., Farrah, D., Harrison, D., Michałowski, M., Valtchanov, I., Oteo, I., Baes, M., Cooray, A., Negrello, M., Wang, L., van der Werf, P., …Dye, S. (2018). Candidate high-z proto-clusters among the Planck compact sources, as revealed by Herschel-SPIRE. Monthly Notices of the Royal Astronomical Society, https://doi.org/10.1093/mnras/sty023
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... Read More about Candidate high-z proto-clusters among the Planck compact sources, as revealed by Herschel-SPIRE.