SCUBA-2 overdensities associated with candidate protoclusters selected from Planck data

dc.contributor.authorVaccari, M.
dc.contributor.authorCheng, T.
dc.contributor.authorClements, D. L.
dc.date.accessioned2021-02-08T12:32:46Z
dc.date.available2021-02-08T12:32:46Z
dc.date.issued2020
dc.description.abstractWe measure the 850-μm source densities of 46 candidate protoclusters selected from the Planck high-z catalogue (PHz) and the Planck Catalogue of Compact Sources (PCCS) that were followed up with Herschel-SPIRE and SCUBA-2. This paper aims to search for overdensities of 850-μm sources in order to select the fields that are most likely to be genuine protoclusters. Of the 46 candidate protoclusters, 25 have significant overdensities (>5 times the field counts), 11 have intermediate overdensities (3–5 times the field counts), and 10 have no overdensity (<3 times the field counts) of 850-μm sources.en_US
dc.identifier.citationVaccari, M. et al. (2020). SCUBA-2 overdensities associated with candidate protoclusters selected from Planck data. Monthly Notices of the Royal Astronomical Society, 494(4), 5985–5991en_US
dc.identifier.issn1365-2966
dc.identifier.urihttps://doi.org/10.1093/mnras/staa1096
dc.identifier.urihttp://hdl.handle.net/10566/5864
dc.language.isoenen_US
dc.publisherOxford University Pressen_US
dc.subjectGalaxies: high-redshiften_US
dc.subjectGalaxies: starbursten_US
dc.subjectSubmillimetre: galaxiesen_US
dc.subjectPlanck dataen_US
dc.subjectSCUBA-2en_US
dc.titleSCUBA-2 overdensities associated with candidate protoclusters selected from Planck dataen_US
dc.typeArticleen_US

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