Cosmological model dependence of the galaxy luminosity function: far-infrared results in the Lemaître-Tolman-Bondi model

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dc.contributor.authorIribarrem, A
dc.contributor.authorAndreani, P
dc.contributor.authorGruppioni, C
dc.contributor.authorFebruary, S
dc.contributor.authorRibeiro, M B
dc.contributor.authorBerta, S
dc.contributor.authorLe Floc’h, E
dc.contributor.authorMagnelli, B
dc.contributor.authorNordon, R
dc.contributor.authorPopesso, P
dc.contributor.authorPozzi, F
dc.contributor.authorRiguccini, L
dc.date.accessioned2021-10-08T11:01:09Z
dc.date.available2021-10-08T11:01:09Z
dc.date.issued2013
dc.description.abstractAims. This is the first paper of a series aiming at investigating galaxy formation and evolution in the giant-void class of the Lemaître-Tolman-Bondi (LTB) models that best fits current cosmological observations. Here we investigate the luminosity function (LF) methodology, and how its estimates would be affected by a change on the cosmological model assumed in its computation. Are the current observational constraints on the allowed cosmology enough to yield robust LF results?
dc.identifier.apacitationIribarrem, A., Andreani, P., Gruppioni, C., February, S., Ribeiro, M. B., Berta, S., ... Riguccini, L. (2013). Cosmological model dependence of the galaxy luminosity function: far-infrared results in the Lemaître-Tolman-Bondi model. <i>Astronomy and Astrophysics</i>, 558(4), A15 - 177. http://hdl.handle.net/11427/35095en_ZA
dc.identifier.chicagocitationIribarrem, A, P Andreani, C Gruppioni, S February, M B Ribeiro, S Berta, , et al "Cosmological model dependence of the galaxy luminosity function: far-infrared results in the Lemaître-Tolman-Bondi model." <i>Astronomy and Astrophysics</i> 558, 4. (2013): A15 - 177. http://hdl.handle.net/11427/35095en_ZA
dc.identifier.citationIribarrem, A., Andreani, P., Gruppioni, C., February, S., Ribeiro, M.B., Berta, S., & Magnelli, B. et al. 2013. Cosmological model dependence of the galaxy luminosity function: far-infrared results in the Lemaître-Tolman-Bondi model. <i>Astronomy and Astrophysics.</i> 558(4):A15 - 177. http://hdl.handle.net/11427/35095en_ZA
dc.identifier.issn0004-6361
dc.identifier.issn1432-0746
dc.identifier.ris TY - Journal Article AU - Iribarrem, A AU - Andreani, P AU - Gruppioni, C AU - February, S AU - Ribeiro, M B AU - Berta, S AU - Le Floc’h, E AU - Magnelli, B AU - Nordon, R AU - Popesso, P AU - Pozzi, F AU - Riguccini, L AB - Aims. This is the first paper of a series aiming at investigating galaxy formation and evolution in the giant-void class of the Lemaître-Tolman-Bondi (LTB) models that best fits current cosmological observations. Here we investigate the luminosity function (LF) methodology, and how its estimates would be affected by a change on the cosmological model assumed in its computation. Are the current observational constraints on the allowed cosmology enough to yield robust LF results? DA - 2013 DB - OpenUCT DP - University of Cape Town IS - 4 J1 - Astronomy and Astrophysics LK - https://open.uct.ac.za PY - 2013 SM - 0004-6361 SM - 1432-0746 T1 - Cosmological model dependence of the galaxy luminosity function: far-infrared results in the Lemaître-Tolman-Bondi model TI - Cosmological model dependence of the galaxy luminosity function: far-infrared results in the Lemaître-Tolman-Bondi model UR - http://hdl.handle.net/11427/35095 ER - en_ZA
dc.identifier.urihttp://hdl.handle.net/11427/35095
dc.identifier.vancouvercitationIribarrem A, Andreani P, Gruppioni C, February S, Ribeiro MB, Berta S, et al. Cosmological model dependence of the galaxy luminosity function: far-infrared results in the Lemaître-Tolman-Bondi model. Astronomy and Astrophysics. 2013;558(4):A15 - 177. http://hdl.handle.net/11427/35095.en_ZA
dc.language.isoeng
dc.publisher.departmentDepartment of Astronomy
dc.publisher.facultyFaculty of Science
dc.sourceAstronomy and Astrophysics
dc.source.journalissue4
dc.source.journalvolume558
dc.source.paginationA15 - 177
dc.source.urihttps://dx.doi.org/10.1051/0004-6361/201321396
dc.subject.othergalaxies: luminosity function, mass function
dc.subject.othergalaxies: distances and redshifts
dc.subject.otherinfrared: galaxies
dc.subject.othercosmology: theory
dc.subject.othergalaxies: evolution
dc.subject.othergalaxies: luminosity function
dc.subject.othermass function
dc.titleCosmological model dependence of the galaxy luminosity function: far-infrared results in the Lemaître-Tolman-Bondi model
dc.typeJournal Article
uct.type.publicationResearch
uct.type.resourceJournal Article
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