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Methodological refinement of the submillimeter galaxy magnification bias: II. Cosmological analysis with tomography

dc.contributor.authorBonavera, Laura 
dc.contributor.authorMuñiz Cueli, Marcos 
dc.contributor.authorGonzález-Nuevo González, Joaquín 
dc.contributor.authorCasas González, José Manuel 
dc.contributor.authorCrespo Iglesias, David 
dc.date.accessioned2024-10-22T06:07:58Z
dc.date.available2024-10-22T06:07:58Z
dc.date.issued2024
dc.identifier.citationAstronomy and Astrophysics, 686, (2024); doi:10.1051/0004-6361/202347002
dc.identifier.issn0004-6361
dc.identifier.urihttps://hdl.handle.net/10651/75272
dc.description.sponsorshipAcknowledgements. L.B., J.G.N., J.M.C., and D.C. acknowledge the PID2021-125630NB-I00 project funded by MCIN/AEI/10.13039/501100011033/FEDER, UE. L.B. also acknowledges the CNS2022-135748 project funded by MCIN/AEI/10.13039/501100011033 and by the EU “NextGeneration EU/PRTR”. J.M.C. also acknowledges financial support from the SV-PA-21-AYUD/2021/51301 project. We deeply acknowledge the CINECA award under the ISCRA initiative, for the availability of high performance computing resources and support. In particular the projects “SIS22_lapi”, “SIS23_lapi” in the framework “Convenzione triennale SISSA-CINECA”. The Herschel-ATLAS is a project with Herschel, which is an ESA space observatory with science instruments provided by European-led Principal Investigator consortia and with important participation from NASA. The H-ATLAS website is http://www.h-atlas.org. GAMA is a joint European-Australasian project based around a spectroscopic campaign using the Anglo-Australian Telescope. The GAMA input catalogue is based on data taken from the Sloan Digital Sky Survey and the UKIRT Infrared Deep Sky Survey. Complementary imaging of the GAMA regions is being obtained by a number of independent survey programs including GALEX MIS, VST KIDS, VISTA VIKING, WISE, Herschel-ATLAS, GMRT and ASKAP providing UV to radio coverage. GAMA is funded by the STFC (UK), the ARC (Australia), the AAO, and the participating institutions. The GAMA website is: http://www.gama-survey.org. This research has made use of the python packages ipython (Pérez & Granger 2007), matplotlib (Hunter 2007) and Scipy (Jones et al. 2001)
dc.language.isoeng
dc.relation.ispartofAstronomy and Astrophysics
dc.rights© The Authors 2024
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-s2.0-85194100710&doi=10.1051%2f0004-6361%2f202347002&partnerID=40&md5=9a09fa0c50b458ea49c18adf15f28216
dc.titleMethodological refinement of the submillimeter galaxy magnification bias: II. Cosmological analysis with tomography
dc.typejournal article
dc.identifier.doi10.1051/0004-6361/202347002
dc.relation.projectIDPID2021-125630NB-I00
dc.relation.projectIDCNS2022-135748
dc.relation.projectIDSV-PA-21-AYUD/2021/51301
dc.relation.projectIDSIS22_lapi
dc.relation.projectIDSIS23_lapi
dc.relation.publisherversionhttp://dx.doi.org/10.1051/0004-6361/202347002
dc.rights.accessRightsopen access
dc.type.hasVersionVoR


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