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A direct and robust method to observationally constrain the halo mass function via the submillimeter magnification bias: proof of concept

dc.contributor.authorMuñiz Cueli, Marcos 
dc.contributor.authorBonavera, Laura 
dc.contributor.authorGonzález-Nuevo González, Joaquín 
dc.contributor.authorLapi, A.
dc.date.accessioned2021-07-26T07:50:16Z
dc.date.available2021-07-26T07:50:16Z
dc.date.issued2021
dc.identifier.citationAstronomy and Astrophysics, 645 (2021); doi:10.1051/0004-6361/202039326
dc.identifier.issn0004-6361
dc.identifier.urihttp://hdl.handle.net/10651/59969
dc.description.sponsorshipMMC, LB and JGN acknowledge the PGC 2018 project PGC2018-101948-B-I00 (MICINN/FEDER). AL acknowledges support from PRIN MIUR 2017 prot. 20173ML3WW002, ‘Opening the ALMA window on the cosmic evolution of gas, stars and supermassive black holes’, the MIUR grant ‘Finanziamento annuale individuale attivitá base di ricerca’, and the EU H2020-MSCA-ITN-2019 Project 860744 ‘BiD4BEST: Big Data applications for Black hole Evolution Studies’.
dc.language.isoeng
dc.relation.ispartofAstronomy and Astrophysics
dc.rights© ESO 2021
dc.rightsCC Reconocimiento - No Comercial - Sin Obra Derivada 4.0 Internacional
dc.rights.urihttp://creativecommons.org/licenses/by-nc-nd/4.0/
dc.sourceScopus
dc.source.urihttps://www.scopus.com/inward/record.uri?eid=2-s2.0-85099917523&doi=10.1051%2f0004-6361%2f202039326&partnerID=40&md5=aed6ea20e4a026a54bfe8ef0bd7d441a
dc.titleA direct and robust method to observationally constrain the halo mass function via the submillimeter magnification bias: proof of concept
dc.typejournal article
dc.identifier.doi10.1051/0004-6361/202039326
dc.relation.projectIDMICINN/FEDER/PGC2018-101948-B-I00
dc.relation.projectIDinfo:eu‐repo/grantAgreement/EC/H2020/860744
dc.relation.publisherversionhttp://dx.doi.org/10.1051/0004-6361/202039326
dc.rights.accessRightsopen access
dc.type.hasVersionAM


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