dc.contributor.author | Cunnington, S | en_US |
dc.contributor.author | Wolz, L | en_US |
dc.contributor.author | Pourtsidou, A | en_US |
dc.contributor.author | Bacon, D | en_US |
dc.date.accessioned | 2019-08-05T10:53:54Z | |
dc.date.available | 2019-07-05 | en_US |
dc.date.issued | 2019-10 | en_US |
dc.identifier.issn | 0035-8711 | en_US |
dc.identifier.uri | https://qmro.qmul.ac.uk/xmlui/handle/123456789/58782 | |
dc.format.extent | 5452 - 5472 | en_US |
dc.relation.ispartof | MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | en_US |
dc.rights | This article is published and distributed under the terms of the Oxford University Press, Standard Journals Publication Model (https://academic.oup.com/journals/pages/open_access/funder_policies/chorus/standard_publication_model) | |
dc.subject | techniques: photometric | en_US |
dc.subject | techniques: spectroscopic | en_US |
dc.subject | galaxies: distances and redshifts | en_US |
dc.subject | large-scale structure of Universe | en_US |
dc.subject | cosmology: observations | en_US |
dc.subject | radio lines: galaxies | en_US |
dc.title | Impact of foregrounds on Hi intensity mapping cross-correlations with optical surveys | en_US |
dc.type | Article | |
dc.rights.holder | © 2019 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society | |
dc.identifier.doi | 10.1093/mnras/stz1916 | en_US |
pubs.author-url | http://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcApp=PARTNER_APP&SrcAuth=LinksAMR&KeyUT=WOS:000484349700078&DestLinkType=FullRecord&DestApp=ALL_WOS&UsrCustomerID=612ae0d773dcbdba3046f6df545e9f6a | en_US |
pubs.issue | 4 | en_US |
pubs.notes | Not known | en_US |
pubs.publication-status | Published | en_US |
pubs.volume | 488 | en_US |
rioxxterms.funder | Default funder | en_US |
rioxxterms.identifier.project | Default project | en_US |