| dc.contributor.author | Vaccari, M. | |
| dc.contributor.author | Cheng, T. | |
| dc.contributor.author | Clements, D. L. | |
| dc.date.accessioned | 2021-02-08T12:32:46Z | |
| dc.date.available | 2021-02-08T12:32:46Z | |
| dc.date.issued | 2020 | |
| dc.identifier.citation | Vaccari, M. et al. (2020). SCUBA-2 overdensities associated with candidate protoclusters selected from Planck data. Monthly Notices of the Royal Astronomical Society, 494(4), 5985–5991 | en_US |
| dc.identifier.issn | 1365-2966 | |
| dc.identifier.uri | https://doi.org/10.1093/mnras/staa1096 | |
| dc.identifier.uri | http://hdl.handle.net/10566/5864 | |
| dc.description.abstract | We 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.language.iso | en | en_US |
| dc.publisher | Oxford University Press | en_US |
| dc.subject | Galaxies: high-redshift | en_US |
| dc.subject | Galaxies: starburst | en_US |
| dc.subject | Submillimetre: galaxies | en_US |
| dc.subject | Planck data | en_US |
| dc.subject | SCUBA-2 | en_US |
| dc.title | SCUBA-2 overdensities associated with candidate protoclusters selected from Planck data | en_US |
| dc.type | Article | en_US |
