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Quasi-stellar objects and galaxy mass density profiles derived using the submillimetre galaxies magnification bias

dc.contributor.authorCrespo Iglesias, David 
dc.contributor.authorGonzález-Nuevo González, Joaquín 
dc.contributor.authorBonavera, Laura 
dc.contributor.authorMuñiz Cueli, Marcos 
dc.contributor.authorCasas González, José Manuel 
dc.contributor.authorGoitia, E.
dc.date.accessioned2023-05-18T08:22:05Z
dc.date.available2023-05-18T08:22:05Z
dc.date.issued2022
dc.identifier.citationAstronomy and Astrophysics, 667 (2022); doi:10.1051/0004-6361/202244016
dc.identifier.issn0004-6361
dc.identifier.urihttp://hdl.handle.net/10651/68170
dc.description.sponsorshipMCIN/AEI/10.13039/501100011033/FEDER, UE [project PID2021-125630NB-I00]
dc.language.isoeng
dc.relation.ispartofAstronomy and Astrophysics
dc.rights© 2022 Los autores
dc.rightsCC Reconocimiento 4.0 Internacional
dc.rights.urihttp://creativecommons.org/licenses/by/4.0/
dc.sourceScopus
dc.source.urihttps://www.scopus.com/inward/record.uri?eid=2-s2.0-85145200041&doi=10.1051%2f0004-6361%2f202244016&partnerID=40&md5=f17583457393c35e536ee34a93f12f4a
dc.titleQuasi-stellar objects and galaxy mass density profiles derived using the submillimetre galaxies magnification bias
dc.typejournal article
dc.identifier.doi10.1051/0004-6361/202244016
dc.relation.projectIDMCIN/FEDER/PID2021-125630NB-I00
dc.relation.publisherversionhttp://dx.doi.org/10.1051/0004-6361/202244016
dc.rights.accessRightsopen access
dc.type.hasVersionVoR


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