Galaxy–galaxy lensing with the DES-CMASS catalogue: measurement and constraints on the galaxy-matter cross-correlation

Detalhes bibliográficos
Autor(a) principal: Lee, S.
Data de Publicação: 2022
Outros Autores: Troxel, M. A., Choi, A., Elvin-Poole, J., Hirata, C., Honscheid, K., Huff, E. M., MacCrann, N., Ross, A. J., Eifler, T. F., Chang, C., Miquel, R., Omori, Y., Prat, J., Bernstein, G. M., Davis, C., DeRose, J., Gatti, M., Rau, M. M., Samuroff, S., Sánchez, C., Vielzeuf, P., Zuntz, J., Aguena, M., Allam, S., Amon, A., Andrade-Oliveira, F. [UNESP], Bertin, E., Brooks, D., Burke, D. L., Rosell, A. Carnero, Kind, M. Carrasco, Carretero, J., Castander, F. J., Cawthon, R., Conselice, C., Costanzi, M., da Costa, L. N., Pereira, M. E.S., de Vicente, J., Desai, S., Diehl, H. T., Dietrich, J. P., Doel, P., Everett, S., Evrard, A. E., Ferrero, I., Flaugher, B., Fosalba, P., Frieman, J., García-Bellido, J., Gaztanaga, E., Gerdes, D. W., Giannantonio, T., Gruen, D., Gruendl, R. A., Gschwend, J., Gutierrez, G., Hartley, W. G., Hinton, S. R., Hollowood, D. L., Hoyle, B., Huterer, D., James, D. J., Kuehn, K., Kuropatkin, N., Lahav, O., Lima, M., Maia, M. A.G., March, M., Marshall, J. L., Menanteau, F., Mohr, J. J., Morgan, R., Palmese, A., Paz-Chinchón, F., Pieres, A., Malagón, A.A. Plazas, Roodman, A., Sanchez, E., Scarpine, V., Schubnell, M., Serrano, S., Sevilla-Noarbe, I., Sheldon, E., Smith, M., Suchyta, E., Swanson, M. E.C., Tarle, G., Thomas, D., To, C., Varga, T. N., Weller, J.
Tipo de documento: Artigo
Idioma: eng
Título da fonte: Repositório Institucional da UNESP
Texto Completo: http://dx.doi.org/10.1093/mnras/stab3028
http://hdl.handle.net/11449/230081
Resumo: The DMASS sample is a photometric sample from the DES Year 1 data set designed to replicate the properties of the CMASS sample from BOSS, in support of a joint analysis of DES and BOSS beyond the small overlapping area. In this paper, we present the measurement of galaxy–galaxy lensing using the DMASS sample as gravitational lenses in the DES Y1 imaging data. We test a number of potential systematics that can bias the galaxy–galaxy lensing signal, including those from shear estimation, photometric redshifts, and observing conditions. After careful systematic tests, we obtain a highly significant detection of the galaxy–galaxy lensing signal, with total S/N = 25.7. With the measured signal, we assess the feasibility of using DMASS as gravitational lenses equivalent to CMASS, by estimating the galaxy-matter cross-correlation coefficient rcc. By jointly fitting the galaxy–galaxy lensing measurement with the galaxy clustering measurement from CMASS, we obtain rcc = 1.09+−001211 for the scale cut of 4 h−1 Mpc and rcc = 1.06+−001312 for 12 h−1 Mpc in fixed cosmology. By adding the angular galaxy clustering of DMASS, we obtain rcc = 1.06 ± 0.10 for the scale cut of 4 h−1 Mpc and rcc = 1.03 ± 0.11 for 12 h−1 Mpc. The resulting values of rcc indicate that the lensing signal of DMASS is statistically consistent with the one that would have been measured if CMASS had populated the DES region within the given statistical uncertainty. The measurement of galaxy–galaxy lensing presented in this paper will serve as part of the data vector for the forthcoming cosmology analysis in preparation.
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spelling Galaxy–galaxy lensing with the DES-CMASS catalogue: measurement and constraints on the galaxy-matter cross-correlationGravitational lensingLarge-scale structure of the UniverseThe DMASS sample is a photometric sample from the DES Year 1 data set designed to replicate the properties of the CMASS sample from BOSS, in support of a joint analysis of DES and BOSS beyond the small overlapping area. In this paper, we present the measurement of galaxy–galaxy lensing using the DMASS sample as gravitational lenses in the DES Y1 imaging data. We test a number of potential systematics that can bias the galaxy–galaxy lensing signal, including those from shear estimation, photometric redshifts, and observing conditions. After careful systematic tests, we obtain a highly significant detection of the galaxy–galaxy lensing signal, with total S/N = 25.7. With the measured signal, we assess the feasibility of using DMASS as gravitational lenses equivalent to CMASS, by estimating the galaxy-matter cross-correlation coefficient rcc. By jointly fitting the galaxy–galaxy lensing measurement with the galaxy clustering measurement from CMASS, we obtain rcc = 1.09+−001211 for the scale cut of 4 h−1 Mpc and rcc = 1.06+−001312 for 12 h−1 Mpc in fixed cosmology. By adding the angular galaxy clustering of DMASS, we obtain rcc = 1.06 ± 0.10 for the scale cut of 4 h−1 Mpc and rcc = 1.03 ± 0.11 for 12 h−1 Mpc. The resulting values of rcc indicate that the lensing signal of DMASS is statistically consistent with the one that would have been measured if CMASS had populated the DES region within the given statistical uncertainty. The measurement of galaxy–galaxy lensing presented in this paper will serve as part of the data vector for the forthcoming cosmology analysis in preparation.Department of Physics Duke UniversityCenter for Cosmology and Astro-Particle Physics Ohio State UniversityDepartment of Physics Ohio State UniversityJet Propulsion Laboratory California Institute of Technology, 4800 Oak Grove Dr.Department of Applied Mathematics and Theoretical Physics University of CambridgeDepartment of Astronomy/Steward Observatory University of Arizona, 933 North Cherry AvenueDepartment of Astronomy and Astrophysics University of ChicagoKavli Institute for Cosmological Physics University of ChicagoInstitució Catalana de Recerca i Estudis AvançatsInstitut de Física d’Altes Energies (IFAE) Barcelona Institute of Science and Technology Campus UAB, BellaterraKavli Institute for Particle Astrophysics & Cosmology Stanford University, PO Box 2450Department of Physics and Astronomy University of PennsylvaniaDepartment of Astronomy University of California Berkeley 501 Campbell HallSanta Cruz Institute for Particle PhysicsDepartment of Physics Carnegie Mellon UniversityInstitute for Astronomy University of EdinburghDepartamento de Física Matemática Instituto de Física Universidade de São Paulo, CP 66318,SPLaboratório Interinstitucional de e-Astronomia - LIneA, Rua Gal. José Cristino 77, RJFermi National Accelerator Laboratory, PO Box 500Instituto de Física Teórica Universidade Estadual PaulistaCNRS UMR 7095 Institut d’Astrophysique de ParisSorbonne Universités UPMC Univ Paris 06 UMR 7095 Institut d’Astrophysique de ParisDepartment of Physics & Astronomy University College London, Gower StreetSLAC National Accelerator LaboratoryInstituto de Astrofisica de Canarias, TenerifeUniversidad de La Laguna Dpto. Astrofisica, TenerifeCenter for Astrophysical Surveys National Center for Supercomputing Applications, 1205 West Clark StrDepartment of Astronomy University of Illinois at Urbana-Champaign, 1002 W. Green StreetInstitut d’Estudis Espacials de Catalunya (IEEC)Institute of Space Sciences (ICE CSIC) Campus UAB, Carrer de Can Magrans, s/nPhysics Department 2320 Chamberlin Hall University of Wisconsin-Madison, 1150 University AvenueJodrell Bank Center for Astrophysics School of Physics and Astronomy University of Manchester, Oxford RoadUniversity of Nottingham School of Physics and AstronomyAstronomy Unit Department of Physics University of Trieste, via Tiepolo 11INAF-Osservatorio Astronomico di Trieste, via G. B. Tiepolo 11Institute for Fundamental Physics of the Universe, Via Beirut 2Observatório Nacional, Rua Gal. José Cristino 77, RJDepartment of Physics University of MichiganCentro de Investigaciones Energéticas Medioambientales y Tecnológicas (CIEMAT)Department of Physics IIT Hyderabad, TelanganaFaculty of Physics Ludwig-Maximilians-Universität, Scheinerstr. 1Department of Astronomy University of MichiganInstitute of Theoretical Astrophysics University of Oslo, PO Box 1029 BlindernInstituto de Fisica Teorica UAM/CSIC Universidad Autonoma de MadridInstitute of Astronomy University of Cambridge, Madingley RoadKavli Institute for Cosmology University of Cambridge, Madingley RoadDepartment of Physics Stanford University, 382 Via Pueblo MallDepartment of Astronomy University of Geneva, ch. d’Écogia 16School of Mathematics and Physics University of QueenslandMax Planck Institute for Extraterrestrial Physics, GiessenbachstrasseCenter for Astrophysics Harvard & Smithsonian, 60 Garden StreetAustralian Astronomical Optics Macquarie UniversityLowell Observatory, 1400 Mars Hill RdGeorge P. and Cynthia Woods Mitchell Institute for Fundamental Physics and Astronomy Department of Physics and Astronomy Texas A&M UniversityDepartment of Astrophysical Sciences Princeton University Peyton HallBrookhaven National Laboratory, Bldg 510School of Physics and Astronomy University of SouthamptonComputer Science and Mathematics Division Oak Ridge National LaboratoryInstitute of Cosmology and Gravitation University of PortsmouthUniversitäts-Sternwarte Fakultät für Physik Ludwig-Maximilians Universität München, Scheinerstr. 1Instituto de Física Teórica Universidade Estadual PaulistaDuke UniversityOhio State UniversityCalifornia Institute of TechnologyUniversity of CambridgeUniversity of ArizonaUniversity of ChicagoInstitució Catalana de Recerca i Estudis AvançatsBarcelona Institute of Science and TechnologyStanford UniversityUniversity of Pennsylvania501 Campbell HallSanta Cruz Institute for Particle PhysicsCarnegie Mellon UniversityUniversity of EdinburghUniversidade de São Paulo (USP)Laboratório Interinstitucional de e-Astronomia - LIneAFermi National Accelerator LaboratoryUniversidade Estadual Paulista (UNESP)Institut d’Astrophysique de ParisUniversity College LondonSLAC National Accelerator LaboratoryInstituto de Astrofisica de CanariasDpto. AstrofisicaNational Center for Supercomputing ApplicationsUniversity of Illinois at Urbana-ChampaignInstitut d’Estudis Espacials de Catalunya (IEEC)CSIC)University of Wisconsin-MadisonUniversity of ManchesterSchool of Physics and AstronomyUniversity of TriesteINAF-Osservatorio Astronomico di TriesteInstitute for Fundamental Physics of the UniverseObservatório NacionalUniversity of MichiganMedioambientales y Tecnológicas (CIEMAT)IIT HyderabadLudwig-Maximilians-UniversitätUniversity of OsloUniversidad Autonoma de MadridUniversity of GenevaUniversity of QueenslandMax Planck Institute for Extraterrestrial PhysicsHarvard & SmithsonianMacquarie UniversityLowell ObservatoryTexas A&M UniversityPeyton HallBrookhaven National LaboratoryUniversity of SouthamptonOak Ridge National LaboratoryUniversity of PortsmouthLudwig-Maximilians Universität MünchenLee, S.Troxel, M. A.Choi, A.Elvin-Poole, J.Hirata, C.Honscheid, K.Huff, E. M.MacCrann, N.Ross, A. J.Eifler, T. F.Chang, C.Miquel, R.Omori, Y.Prat, J.Bernstein, G. M.Davis, C.DeRose, J.Gatti, M.Rau, M. M.Samuroff, S.Sánchez, C.Vielzeuf, P.Zuntz, J.Aguena, M.Allam, S.Amon, A.Andrade-Oliveira, F. [UNESP]Bertin, E.Brooks, D.Burke, D. L.Rosell, A. CarneroKind, M. CarrascoCarretero, J.Castander, F. J.Cawthon, R.Conselice, C.Costanzi, M.da Costa, L. N.Pereira, M. E.S.de Vicente, J.Desai, S.Diehl, H. T.Dietrich, J. P.Doel, P.Everett, S.Evrard, A. E.Ferrero, I.Flaugher, B.Fosalba, P.Frieman, J.García-Bellido, J.Gaztanaga, E.Gerdes, D. W.Giannantonio, T.Gruen, D.Gruendl, R. A.Gschwend, J.Gutierrez, G.Hartley, W. G.Hinton, S. R.Hollowood, D. L.Hoyle, B.Huterer, D.James, D. J.Kuehn, K.Kuropatkin, N.Lahav, O.Lima, M.Maia, M. A.G.March, M.Marshall, J. L.Menanteau, F.Mohr, J. J.Morgan, R.Palmese, A.Paz-Chinchón, F.Pieres, A.Malagón, A.A. PlazasRoodman, A.Sanchez, E.Scarpine, V.Schubnell, M.Serrano, S.Sevilla-Noarbe, I.Sheldon, E.Smith, M.Suchyta, E.Swanson, M. E.C.Tarle, G.Thomas, D.To, C.Varga, T. N.Weller, J.2022-04-29T08:37:33Z2022-04-29T08:37:33Z2022-01-01info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/article2033-2047http://dx.doi.org/10.1093/mnras/stab3028Monthly Notices of the Royal Astronomical Society, v. 509, n. 2, p. 2033-2047, 2022.1365-29660035-8711http://hdl.handle.net/11449/23008110.1093/mnras/stab30282-s2.0-85121374172Scopusreponame:Repositório Institucional da UNESPinstname:Universidade Estadual Paulista (UNESP)instacron:UNESPengMonthly Notices of the Royal Astronomical Societyinfo:eu-repo/semantics/openAccess2022-04-29T08:37:34Zoai:repositorio.unesp.br:11449/230081Repositório InstitucionalPUBhttp://repositorio.unesp.br/oai/requestopendoar:29462024-08-06T00:06:47.555596Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)false
dc.title.none.fl_str_mv Galaxy–galaxy lensing with the DES-CMASS catalogue: measurement and constraints on the galaxy-matter cross-correlation
title Galaxy–galaxy lensing with the DES-CMASS catalogue: measurement and constraints on the galaxy-matter cross-correlation
spellingShingle Galaxy–galaxy lensing with the DES-CMASS catalogue: measurement and constraints on the galaxy-matter cross-correlation
Lee, S.
Gravitational lensing
Large-scale structure of the Universe
title_short Galaxy–galaxy lensing with the DES-CMASS catalogue: measurement and constraints on the galaxy-matter cross-correlation
title_full Galaxy–galaxy lensing with the DES-CMASS catalogue: measurement and constraints on the galaxy-matter cross-correlation
title_fullStr Galaxy–galaxy lensing with the DES-CMASS catalogue: measurement and constraints on the galaxy-matter cross-correlation
title_full_unstemmed Galaxy–galaxy lensing with the DES-CMASS catalogue: measurement and constraints on the galaxy-matter cross-correlation
title_sort Galaxy–galaxy lensing with the DES-CMASS catalogue: measurement and constraints on the galaxy-matter cross-correlation
author Lee, S.
author_facet Lee, S.
Troxel, M. A.
Choi, A.
Elvin-Poole, J.
Hirata, C.
Honscheid, K.
Huff, E. M.
MacCrann, N.
Ross, A. J.
Eifler, T. F.
Chang, C.
Miquel, R.
Omori, Y.
Prat, J.
Bernstein, G. M.
Davis, C.
DeRose, J.
Gatti, M.
Rau, M. M.
Samuroff, S.
Sánchez, C.
Vielzeuf, P.
Zuntz, J.
Aguena, M.
Allam, S.
Amon, A.
Andrade-Oliveira, F. [UNESP]
Bertin, E.
Brooks, D.
Burke, D. L.
Rosell, A. Carnero
Kind, M. Carrasco
Carretero, J.
Castander, F. J.
Cawthon, R.
Conselice, C.
Costanzi, M.
da Costa, L. N.
Pereira, M. E.S.
de Vicente, J.
Desai, S.
Diehl, H. T.
Dietrich, J. P.
Doel, P.
Everett, S.
Evrard, A. E.
Ferrero, I.
Flaugher, B.
Fosalba, P.
Frieman, J.
García-Bellido, J.
Gaztanaga, E.
Gerdes, D. W.
Giannantonio, T.
Gruen, D.
Gruendl, R. A.
Gschwend, J.
Gutierrez, G.
Hartley, W. G.
Hinton, S. R.
Hollowood, D. L.
Hoyle, B.
Huterer, D.
James, D. J.
Kuehn, K.
Kuropatkin, N.
Lahav, O.
Lima, M.
Maia, M. A.G.
March, M.
Marshall, J. L.
Menanteau, F.
Mohr, J. J.
Morgan, R.
Palmese, A.
Paz-Chinchón, F.
Pieres, A.
Malagón, A.A. Plazas
Roodman, A.
Sanchez, E.
Scarpine, V.
Schubnell, M.
Serrano, S.
Sevilla-Noarbe, I.
Sheldon, E.
Smith, M.
Suchyta, E.
Swanson, M. E.C.
Tarle, G.
Thomas, D.
To, C.
Varga, T. N.
Weller, J.
author_role author
author2 Troxel, M. A.
Choi, A.
Elvin-Poole, J.
Hirata, C.
Honscheid, K.
Huff, E. M.
MacCrann, N.
Ross, A. J.
Eifler, T. F.
Chang, C.
Miquel, R.
Omori, Y.
Prat, J.
Bernstein, G. M.
Davis, C.
DeRose, J.
Gatti, M.
Rau, M. M.
Samuroff, S.
Sánchez, C.
Vielzeuf, P.
Zuntz, J.
Aguena, M.
Allam, S.
Amon, A.
Andrade-Oliveira, F. [UNESP]
Bertin, E.
Brooks, D.
Burke, D. L.
Rosell, A. Carnero
Kind, M. Carrasco
Carretero, J.
Castander, F. J.
Cawthon, R.
Conselice, C.
Costanzi, M.
da Costa, L. N.
Pereira, M. E.S.
de Vicente, J.
Desai, S.
Diehl, H. T.
Dietrich, J. P.
Doel, P.
Everett, S.
Evrard, A. E.
Ferrero, I.
Flaugher, B.
Fosalba, P.
Frieman, J.
García-Bellido, J.
Gaztanaga, E.
Gerdes, D. W.
Giannantonio, T.
Gruen, D.
Gruendl, R. A.
Gschwend, J.
Gutierrez, G.
Hartley, W. G.
Hinton, S. R.
Hollowood, D. L.
Hoyle, B.
Huterer, D.
James, D. J.
Kuehn, K.
Kuropatkin, N.
Lahav, O.
Lima, M.
Maia, M. A.G.
March, M.
Marshall, J. L.
Menanteau, F.
Mohr, J. J.
Morgan, R.
Palmese, A.
Paz-Chinchón, F.
Pieres, A.
Malagón, A.A. Plazas
Roodman, A.
Sanchez, E.
Scarpine, V.
Schubnell, M.
Serrano, S.
Sevilla-Noarbe, I.
Sheldon, E.
Smith, M.
Suchyta, E.
Swanson, M. E.C.
Tarle, G.
Thomas, D.
To, C.
Varga, T. N.
Weller, J.
author2_role author
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dc.contributor.none.fl_str_mv Duke University
Ohio State University
California Institute of Technology
University of Cambridge
University of Arizona
University of Chicago
Institució Catalana de Recerca i Estudis Avançats
Barcelona Institute of Science and Technology
Stanford University
University of Pennsylvania
501 Campbell Hall
Santa Cruz Institute for Particle Physics
Carnegie Mellon University
University of Edinburgh
Universidade de São Paulo (USP)
Laboratório Interinstitucional de e-Astronomia - LIneA
Fermi National Accelerator Laboratory
Universidade Estadual Paulista (UNESP)
Institut d’Astrophysique de Paris
University College London
SLAC National Accelerator Laboratory
Instituto de Astrofisica de Canarias
Dpto. Astrofisica
National Center for Supercomputing Applications
University of Illinois at Urbana-Champaign
Institut d’Estudis Espacials de Catalunya (IEEC)
CSIC)
University of Wisconsin-Madison
University of Manchester
School of Physics and Astronomy
University of Trieste
INAF-Osservatorio Astronomico di Trieste
Institute for Fundamental Physics of the Universe
Observatório Nacional
University of Michigan
Medioambientales y Tecnológicas (CIEMAT)
IIT Hyderabad
Ludwig-Maximilians-Universität
University of Oslo
Universidad Autonoma de Madrid
University of Geneva
University of Queensland
Max Planck Institute for Extraterrestrial Physics
Harvard & Smithsonian
Macquarie University
Lowell Observatory
Texas A&M University
Peyton Hall
Brookhaven National Laboratory
University of Southampton
Oak Ridge National Laboratory
University of Portsmouth
Ludwig-Maximilians Universität München
dc.contributor.author.fl_str_mv Lee, S.
Troxel, M. A.
Choi, A.
Elvin-Poole, J.
Hirata, C.
Honscheid, K.
Huff, E. M.
MacCrann, N.
Ross, A. J.
Eifler, T. F.
Chang, C.
Miquel, R.
Omori, Y.
Prat, J.
Bernstein, G. M.
Davis, C.
DeRose, J.
Gatti, M.
Rau, M. M.
Samuroff, S.
Sánchez, C.
Vielzeuf, P.
Zuntz, J.
Aguena, M.
Allam, S.
Amon, A.
Andrade-Oliveira, F. [UNESP]
Bertin, E.
Brooks, D.
Burke, D. L.
Rosell, A. Carnero
Kind, M. Carrasco
Carretero, J.
Castander, F. J.
Cawthon, R.
Conselice, C.
Costanzi, M.
da Costa, L. N.
Pereira, M. E.S.
de Vicente, J.
Desai, S.
Diehl, H. T.
Dietrich, J. P.
Doel, P.
Everett, S.
Evrard, A. E.
Ferrero, I.
Flaugher, B.
Fosalba, P.
Frieman, J.
García-Bellido, J.
Gaztanaga, E.
Gerdes, D. W.
Giannantonio, T.
Gruen, D.
Gruendl, R. A.
Gschwend, J.
Gutierrez, G.
Hartley, W. G.
Hinton, S. R.
Hollowood, D. L.
Hoyle, B.
Huterer, D.
James, D. J.
Kuehn, K.
Kuropatkin, N.
Lahav, O.
Lima, M.
Maia, M. A.G.
March, M.
Marshall, J. L.
Menanteau, F.
Mohr, J. J.
Morgan, R.
Palmese, A.
Paz-Chinchón, F.
Pieres, A.
Malagón, A.A. Plazas
Roodman, A.
Sanchez, E.
Scarpine, V.
Schubnell, M.
Serrano, S.
Sevilla-Noarbe, I.
Sheldon, E.
Smith, M.
Suchyta, E.
Swanson, M. E.C.
Tarle, G.
Thomas, D.
To, C.
Varga, T. N.
Weller, J.
dc.subject.por.fl_str_mv Gravitational lensing
Large-scale structure of the Universe
topic Gravitational lensing
Large-scale structure of the Universe
description The DMASS sample is a photometric sample from the DES Year 1 data set designed to replicate the properties of the CMASS sample from BOSS, in support of a joint analysis of DES and BOSS beyond the small overlapping area. In this paper, we present the measurement of galaxy–galaxy lensing using the DMASS sample as gravitational lenses in the DES Y1 imaging data. We test a number of potential systematics that can bias the galaxy–galaxy lensing signal, including those from shear estimation, photometric redshifts, and observing conditions. After careful systematic tests, we obtain a highly significant detection of the galaxy–galaxy lensing signal, with total S/N = 25.7. With the measured signal, we assess the feasibility of using DMASS as gravitational lenses equivalent to CMASS, by estimating the galaxy-matter cross-correlation coefficient rcc. By jointly fitting the galaxy–galaxy lensing measurement with the galaxy clustering measurement from CMASS, we obtain rcc = 1.09+−001211 for the scale cut of 4 h−1 Mpc and rcc = 1.06+−001312 for 12 h−1 Mpc in fixed cosmology. By adding the angular galaxy clustering of DMASS, we obtain rcc = 1.06 ± 0.10 for the scale cut of 4 h−1 Mpc and rcc = 1.03 ± 0.11 for 12 h−1 Mpc. The resulting values of rcc indicate that the lensing signal of DMASS is statistically consistent with the one that would have been measured if CMASS had populated the DES region within the given statistical uncertainty. The measurement of galaxy–galaxy lensing presented in this paper will serve as part of the data vector for the forthcoming cosmology analysis in preparation.
publishDate 2022
dc.date.none.fl_str_mv 2022-04-29T08:37:33Z
2022-04-29T08:37:33Z
2022-01-01
dc.type.status.fl_str_mv info:eu-repo/semantics/publishedVersion
dc.type.driver.fl_str_mv info:eu-repo/semantics/article
format article
status_str publishedVersion
dc.identifier.uri.fl_str_mv http://dx.doi.org/10.1093/mnras/stab3028
Monthly Notices of the Royal Astronomical Society, v. 509, n. 2, p. 2033-2047, 2022.
1365-2966
0035-8711
http://hdl.handle.net/11449/230081
10.1093/mnras/stab3028
2-s2.0-85121374172
url http://dx.doi.org/10.1093/mnras/stab3028
http://hdl.handle.net/11449/230081
identifier_str_mv Monthly Notices of the Royal Astronomical Society, v. 509, n. 2, p. 2033-2047, 2022.
1365-2966
0035-8711
10.1093/mnras/stab3028
2-s2.0-85121374172
dc.language.iso.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv Monthly Notices of the Royal Astronomical Society
dc.rights.driver.fl_str_mv info:eu-repo/semantics/openAccess
eu_rights_str_mv openAccess
dc.format.none.fl_str_mv 2033-2047
dc.source.none.fl_str_mv Scopus
reponame:Repositório Institucional da UNESP
instname:Universidade Estadual Paulista (UNESP)
instacron:UNESP
instname_str Universidade Estadual Paulista (UNESP)
instacron_str UNESP
institution UNESP
reponame_str Repositório Institucional da UNESP
collection Repositório Institucional da UNESP
repository.name.fl_str_mv Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)
repository.mail.fl_str_mv
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