Modelling radio luminosity functions of radio-loud AGN by the cosmological evolution of supermassive black holes

dc.contributor.author	Tucci, M.
dc.contributor.author	Toffolatti, Luigi
dc.date.accessioned	2022-02-01T08:05:32Z
dc.date.available	2022-02-01T08:05:32Z
dc.date.issued	2021
dc.identifier.citation	Astronomy and Astrophysics, 650 (2021); doi:10.1051/0004-6361/202039884
dc.identifier.issn	0004-6361
dc.identifier.uri	http://hdl.handle.net/10651/61662
dc.description.sponsorship	LT acknowledges the Spanish Ministerio de Ciencia, Innovación y Universidades for partial financial support under projects PGC2018-101814-B-I00 and PGC2018-101948-B-I00.
dc.language.iso	eng
dc.relation.ispartof	Astronomy and Astrophysics
dc.rights	© ESO 2021
dc.source	Scopus
dc.source.uri	https://www.scopus.com/inward/record.uri?eid=2-s2.0-85108533860&doi=10.1051%2f0004-6361%2f202039884&partnerID=40&md5=e3e133d82c6d1aa081b08b27dd71688b
dc.title	Modelling radio luminosity functions of radio-loud AGN by the cosmological evolution of supermassive black holes
dc.type	journal article
dc.identifier.doi	10.1051/0004-6361/202039884
dc.relation.projectID	MICIU/PGC2018-101814-B-I00
dc.relation.projectID	MICIU/PGC2018-101948-B-I00
dc.relation.publisherversion	http://dx.doi.org/10.1051/0004-6361/202039884
dc.rights.accessRights	open access
dc.type.hasVersion	AM

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