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

dc.contributor.authorIbar, Eduardo
dc.date.accessioned2021-07-28T16:33:33Z
dc.date.available2021-07-28T16:33:33Z
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. We find that the enhanced number densities are unlikely to be the result of sample variance. Compared with the number counts of another sample selected from Planck’s compact source catalogues, this [PHz+PCCS]-selected sample has a higher fraction of candidate protoclusters with significant overdensities, though both samples show overdensities of 850-μm sources above intermediate level. Based on the estimated star-formation rate densities (SFRDs), we suggest that both samples can efficiently select protoclusters with starbursting galaxies near the redshift at which the global field SFRD peaks (2 < z < 3). Based on the confirmation of overdensities found here, future follow-up observations on other PHz targets may greatly increase the number of genuine DSFG-rich clusters/protoclusters.en_ES
dc.identifier.doihttps://doi.org/10.1093/mnras/staa1096
dc.identifier.urihttp://repositoriobibliotecas.uv.cl/handle/uvscl/2213
dc.language.isoenen_ES
dc.publisherRoyal Astronomical Societyen_ES
dc.sourceMonthly Notices of the Royal Astronomical Societyen_ES
dc.subjectGALAXIES: HIGH-REDSHIFTen_ES
dc.subjectGALAXIES: STARBURSTen_ES
dc.subjectSUBMILLIMETRE: GALAXIESen_ES
dc.titleSCUBA-2 overdensities associated with candidate protoclusters selected from Planck dataen_ES
dc.typeArticuloen_ES
uv.catalogadorRCR DIBRAen_ES

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