Galaxy cluster mass density profile derived using the submillimetre galaxies magnification bias

dc.contributor.author	Fernández, L.
dc.contributor.author	Muñiz Cueli, Marcos
dc.contributor.author	González-Nuevo González, Joaquín
dc.contributor.author	Bonavera, Laura
dc.contributor.author	Crespo Iglesias, David
dc.contributor.author	Casas González, José Manuel
dc.contributor.author	Lapi, A.
dc.date.accessioned	2022-09-06T07:29:18Z
dc.date.available	2022-09-06T07:29:18Z
dc.date.issued	2022
dc.identifier.citation	Astronomy and Astrophysics, 658 (2022); doi:10.1051/0004-6361/202141905
dc.identifier.issn	0004-6361
dc.identifier.uri	http://hdl.handle.net/10651/64669
dc.description.sponsorship	MICINN/FEDER [PGC2018-101948-B-I00]; Universidad de Oviedo [PAPI-20-PF-23]; EU [860744]; PRIN MUR 2017 [20173ML3WW]; CINECA award under the ISCRA initiative
dc.language.iso	eng
dc.relation.ispartof	Astronomy and astrophysics
dc.rights	© ESO 2022
dc.source	Scopus
dc.source.uri	https://www.scopus.com/inward/record.uri?eid=2-s2.0-85123853423&doi=10.1051%2f0004-6361%2f202141905&partnerID=40&md5=d9e0e7f2ed706c300d33f35a0988a2f3
dc.title	Galaxy cluster mass density profile derived using the submillimetre galaxies magnification bias
dc.type	journal article
dc.identifier.doi	10.1051/0004-6361/202141905
dc.relation.projectID	MICINN/FEDER/PGC2018-101948-B-I00
dc.relation.projectID	info:eu‐repo/grantAgreement/EC/H2020/860744
dc.relation.publisherversion	http://dx.doi.org/10.1051/0004-6361/202141905
dc.rights.accessRights	open access
dc.type.hasVersion	VoR

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