The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: single-probe measurements from CMASS anisotropic galaxy clustering
- Autores
- Chuang, Chia-Hsun; Prada, Francisco; Pellejero Ibanez, Marcos; Beutler, Florian; Cuesta, Antonio; Eisenstein, Daniel J.; Escoffier, Stephanie; Ho, Shirley; Kitaura, Francisco-Shu; Kneib, Jean Paul; Manera, Marc; Nuza, Sebastian Ernesto; Rodriguez Torres, Sergio A.; Ross, Ashley; Rubiño Martín, J. A.; Samushia, Lado; Schlegel, David J.; Schneider, Donald P.; Wang, Yuting; Weaber, Benjamin A.; Zao, Gongbo; Brownstein, Joel R.; Dawson, Kyle S.; Maraston, Claudia; Olmestead, Matthew D.; Thomas, Daniel
- Año de publicación
- 2016
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- With the largest spectroscopic galaxy survey volume drawn from the SDSS-III Baryon Oscillation Spectroscopic Survey (BOSS), we can extract cosmological constraints from the measurements of redshift and geometric distortions at quasi-linear scales (e.g. above 50 h−1 Mpc). We analyse the broad-range shape of the monopole and quadrupole correlation functions of the BOSS Data Release 12 (DR12) CMASS galaxy sample, at the effective redshift z = 0.59, to obtain constraints on the Hubble expansion rate H(z), the angular- diameter distance DA(z), the normalized growth rate f(z)σ8(z), and the physical matter density Ωm h2. We obtain robust measurements by including a polynomial as the model for the systematic errors, and find it works very well against the systematic effects, e.g. ones induced by stars and seeing. We provide accurate measurements {DA(0.59)rs,fid/rs, H(0.59)rs/rs,fid, f(0.59)σ8(0.59), Ωm h2} = {1427 ± 26 Mpc, 97.3 ± 3.3 km s−1 Mpc−1, 0.488 ± 0.060, 0.135 ± 0.016}, where rs is the comoving sound horizon at the drag epoch and rs,fid = 147.66 Mpc is the sound scale of the fiducial cosmology used in this study. The parameters which are not well constrained by our galaxy clustering analysis are marginalized over with wide flat priors. Since no priors from other data sets, e.g. cosmic microwave background (CMB), are adopted and no dark energy models are assumed, our results from BOSS CMASS galaxy clustering alone may be combined with other data sets, i.e. CMB, SNe, lensing or other galaxy clustering data to constrain the parameters of a given cosmological model. The uncertainty on the dark energy equation of state parameter, w, from CMB+CMASS is about 8 per cent. The uncertainty on the curvature fraction, Ωk, is 0.3 per cent. We do not find deviation from flat ΛCDM.
Fil: Chuang, Chia-Hsun. Universidad Autónoma de Madrid; España
Fil: Prada, Francisco. Universidad Autónoma de Madrid; España
Fil: Pellejero Ibanez, Marcos. Instituto de Astrofísica de Canarias; España
Fil: Beutler, Florian. Lawrence Berkeley National Lab,; Estados Unidos
Fil: Cuesta, Antonio. Universidad de Barcelona; España
Fil: Eisenstein, Daniel J.. Harvard-Smithsonian Center for Astrophysics; Estados Unidos
Fil: Escoffier, Stephanie. Aix-Marseille Universite,; Francia
Fil: Ho, Shirley. Carnegie Mellon University; Estados Unidos
Fil: Kitaura, Francisco-Shu. Leibniz-Institut fur Astrophysik Potsdam; Alemania
Fil: Kneib, Jean Paul. Aix Marseille Universite,; Francia
Fil: Manera, Marc. University College London,; Reino Unido
Fil: Nuza, Sebastian Ernesto. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina
Fil: Rodriguez Torres, Sergio A.. Universidad Autónoma de Madrid; España
Fil: Ross, Ashley. Ohio State University; Estados Unidos
Fil: Rubiño Martín, J. A.. Instituto de Astrof´ısica de Canarias; España
Fil: Samushia, Lado. Kansas State University; Estados Unidos
Fil: Schlegel, David J.. Lawrence Berkeley National Laboratory; Estados Unidos
Fil: Schneider, Donald P.. State University Of Pennsylvania; Estados Unidos
Fil: Wang, Yuting. National Astronomy Observatories; China
Fil: Weaber, Benjamin A.. University of New York; Estados Unidos
Fil: Zao, Gongbo. National Astronomy Observatories; China
Fil: Brownstein, Joel R.. University of Utah; Estados Unidos
Fil: Dawson, Kyle S.. University of Utah; Estados Unidos
Fil: Maraston, Claudia. University of Portsmouth; Reino Unido
Fil: Olmestead, Matthew D.. King’s College; Estados Unidos
Fil: Thomas, Daniel. University of Portsmouth; Reino Unido - Materia
-
COSMOLOGY: OBSERVATIONS
DISTANCE SCALE
LARGE-SCALE STRUCTURE OF UNIVERSE
COSMOLOGICAL PARAMETERS - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
- Repositorio
.jpg)
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/18434
Ver los metadatos del registro completo
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The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: single-probe measurements from CMASS anisotropic galaxy clusteringChuang, Chia-HsunPrada, FranciscoPellejero Ibanez, MarcosBeutler, FlorianCuesta, AntonioEisenstein, Daniel J.Escoffier, StephanieHo, ShirleyKitaura, Francisco-ShuKneib, Jean PaulManera, MarcNuza, Sebastian ErnestoRodriguez Torres, Sergio A.Ross, AshleyRubiño Martín, J. A.Samushia, LadoSchlegel, David J.Schneider, Donald P.Wang, YutingWeaber, Benjamin A.Zao, GongboBrownstein, Joel R.Dawson, Kyle S.Maraston, ClaudiaOlmestead, Matthew D.Thomas, DanielCOSMOLOGY: OBSERVATIONSDISTANCE SCALELARGE-SCALE STRUCTURE OF UNIVERSECOSMOLOGICAL PARAMETERShttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1With the largest spectroscopic galaxy survey volume drawn from the SDSS-III Baryon Oscillation Spectroscopic Survey (BOSS), we can extract cosmological constraints from the measurements of redshift and geometric distortions at quasi-linear scales (e.g. above 50 h−1 Mpc). We analyse the broad-range shape of the monopole and quadrupole correlation functions of the BOSS Data Release 12 (DR12) CMASS galaxy sample, at the effective redshift z = 0.59, to obtain constraints on the Hubble expansion rate H(z), the angular- diameter distance DA(z), the normalized growth rate f(z)σ8(z), and the physical matter density Ωm h2. We obtain robust measurements by including a polynomial as the model for the systematic errors, and find it works very well against the systematic effects, e.g. ones induced by stars and seeing. We provide accurate measurements {DA(0.59)rs,fid/rs, H(0.59)rs/rs,fid, f(0.59)σ8(0.59), Ωm h2} = {1427 ± 26 Mpc, 97.3 ± 3.3 km s−1 Mpc−1, 0.488 ± 0.060, 0.135 ± 0.016}, where rs is the comoving sound horizon at the drag epoch and rs,fid = 147.66 Mpc is the sound scale of the fiducial cosmology used in this study. The parameters which are not well constrained by our galaxy clustering analysis are marginalized over with wide flat priors. Since no priors from other data sets, e.g. cosmic microwave background (CMB), are adopted and no dark energy models are assumed, our results from BOSS CMASS galaxy clustering alone may be combined with other data sets, i.e. CMB, SNe, lensing or other galaxy clustering data to constrain the parameters of a given cosmological model. The uncertainty on the dark energy equation of state parameter, w, from CMB+CMASS is about 8 per cent. The uncertainty on the curvature fraction, Ωk, is 0.3 per cent. We do not find deviation from flat ΛCDM.Fil: Chuang, Chia-Hsun. Universidad Autónoma de Madrid; EspañaFil: Prada, Francisco. Universidad Autónoma de Madrid; EspañaFil: Pellejero Ibanez, Marcos. Instituto de Astrofísica de Canarias; EspañaFil: Beutler, Florian. Lawrence Berkeley National Lab,; Estados UnidosFil: Cuesta, Antonio. Universidad de Barcelona; EspañaFil: Eisenstein, Daniel J.. Harvard-Smithsonian Center for Astrophysics; Estados UnidosFil: Escoffier, Stephanie. Aix-Marseille Universite,; FranciaFil: Ho, Shirley. Carnegie Mellon University; Estados UnidosFil: Kitaura, Francisco-Shu. Leibniz-Institut fur Astrophysik Potsdam; AlemaniaFil: Kneib, Jean Paul. Aix Marseille Universite,; FranciaFil: Manera, Marc. University College London,; Reino UnidoFil: Nuza, Sebastian Ernesto. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; ArgentinaFil: Rodriguez Torres, Sergio A.. Universidad Autónoma de Madrid; EspañaFil: Ross, Ashley. Ohio State University; Estados UnidosFil: Rubiño Martín, J. A.. Instituto de Astrof´ısica de Canarias; EspañaFil: Samushia, Lado. Kansas State University; Estados UnidosFil: Schlegel, David J.. Lawrence Berkeley National Laboratory; Estados UnidosFil: Schneider, Donald P.. State University Of Pennsylvania; Estados UnidosFil: Wang, Yuting. National Astronomy Observatories; ChinaFil: Weaber, Benjamin A.. University of New York; Estados UnidosFil: Zao, Gongbo. National Astronomy Observatories; ChinaFil: Brownstein, Joel R.. University of Utah; Estados UnidosFil: Dawson, Kyle S.. University of Utah; Estados UnidosFil: Maraston, Claudia. University of Portsmouth; Reino UnidoFil: Olmestead, Matthew D.. King’s College; Estados UnidosFil: Thomas, Daniel. University of Portsmouth; Reino UnidoWiley Blackwell Publishing, Inc2016-10info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/18434Chuang, Chia-Hsun; Prada, Francisco; Pellejero Ibanez, Marcos; Beutler, Florian; Cuesta, Antonio; et al.; The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: single-probe measurements from CMASS anisotropic galaxy clustering; Wiley Blackwell Publishing, Inc; Monthly Notices Of The Royal Astronomical Society; 461; 4; 10-2016; 3781-37930035-8711CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.1093/mnras/stw1535info:eu-repo/semantics/altIdentifier/url/https://arxiv.org/abs/1312.4889info:eu-repo/semantics/altIdentifier/url/https://academic.oup.com/mnras/article-abstract/461/4/3781/2608598/The-clustering-of-galaxies-in-the-SDSS-III-Baryon?redirectedFrom=PDFinfo:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-10-22T11:47:45Zoai:ri.conicet.gov.ar:11336/18434instacron:CONICETInstitucionalhttp://ri.conicet.gov.ar/Organismo científico-tecnológicoNo correspondehttp://ri.conicet.gov.ar/oai/requestdasensio@conicet.gov.ar; lcarlino@conicet.gov.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:34982025-10-22 11:47:45.92CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
| dc.title.none.fl_str_mv |
The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: single-probe measurements from CMASS anisotropic galaxy clustering |
| title |
The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: single-probe measurements from CMASS anisotropic galaxy clustering |
| spellingShingle |
The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: single-probe measurements from CMASS anisotropic galaxy clustering Chuang, Chia-Hsun COSMOLOGY: OBSERVATIONS DISTANCE SCALE LARGE-SCALE STRUCTURE OF UNIVERSE COSMOLOGICAL PARAMETERS |
| title_short |
The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: single-probe measurements from CMASS anisotropic galaxy clustering |
| title_full |
The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: single-probe measurements from CMASS anisotropic galaxy clustering |
| title_fullStr |
The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: single-probe measurements from CMASS anisotropic galaxy clustering |
| title_full_unstemmed |
The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: single-probe measurements from CMASS anisotropic galaxy clustering |
| title_sort |
The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: single-probe measurements from CMASS anisotropic galaxy clustering |
| dc.creator.none.fl_str_mv |
Chuang, Chia-Hsun Prada, Francisco Pellejero Ibanez, Marcos Beutler, Florian Cuesta, Antonio Eisenstein, Daniel J. Escoffier, Stephanie Ho, Shirley Kitaura, Francisco-Shu Kneib, Jean Paul Manera, Marc Nuza, Sebastian Ernesto Rodriguez Torres, Sergio A. Ross, Ashley Rubiño Martín, J. A. Samushia, Lado Schlegel, David J. Schneider, Donald P. Wang, Yuting Weaber, Benjamin A. Zao, Gongbo Brownstein, Joel R. Dawson, Kyle S. Maraston, Claudia Olmestead, Matthew D. Thomas, Daniel |
| author |
Chuang, Chia-Hsun |
| author_facet |
Chuang, Chia-Hsun Prada, Francisco Pellejero Ibanez, Marcos Beutler, Florian Cuesta, Antonio Eisenstein, Daniel J. Escoffier, Stephanie Ho, Shirley Kitaura, Francisco-Shu Kneib, Jean Paul Manera, Marc Nuza, Sebastian Ernesto Rodriguez Torres, Sergio A. Ross, Ashley Rubiño Martín, J. A. Samushia, Lado Schlegel, David J. Schneider, Donald P. Wang, Yuting Weaber, Benjamin A. Zao, Gongbo Brownstein, Joel R. Dawson, Kyle S. Maraston, Claudia Olmestead, Matthew D. Thomas, Daniel |
| author_role |
author |
| author2 |
Prada, Francisco Pellejero Ibanez, Marcos Beutler, Florian Cuesta, Antonio Eisenstein, Daniel J. Escoffier, Stephanie Ho, Shirley Kitaura, Francisco-Shu Kneib, Jean Paul Manera, Marc Nuza, Sebastian Ernesto Rodriguez Torres, Sergio A. Ross, Ashley Rubiño Martín, J. A. Samushia, Lado Schlegel, David J. Schneider, Donald P. Wang, Yuting Weaber, Benjamin A. Zao, Gongbo Brownstein, Joel R. Dawson, Kyle S. Maraston, Claudia Olmestead, Matthew D. Thomas, Daniel |
| author2_role |
author author author author author author author author author author author author author author author author author author author author author author author author author |
| dc.subject.none.fl_str_mv |
COSMOLOGY: OBSERVATIONS DISTANCE SCALE LARGE-SCALE STRUCTURE OF UNIVERSE COSMOLOGICAL PARAMETERS |
| topic |
COSMOLOGY: OBSERVATIONS DISTANCE SCALE LARGE-SCALE STRUCTURE OF UNIVERSE COSMOLOGICAL PARAMETERS |
| purl_subject.fl_str_mv |
https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 |
| dc.description.none.fl_txt_mv |
With the largest spectroscopic galaxy survey volume drawn from the SDSS-III Baryon Oscillation Spectroscopic Survey (BOSS), we can extract cosmological constraints from the measurements of redshift and geometric distortions at quasi-linear scales (e.g. above 50 h−1 Mpc). We analyse the broad-range shape of the monopole and quadrupole correlation functions of the BOSS Data Release 12 (DR12) CMASS galaxy sample, at the effective redshift z = 0.59, to obtain constraints on the Hubble expansion rate H(z), the angular- diameter distance DA(z), the normalized growth rate f(z)σ8(z), and the physical matter density Ωm h2. We obtain robust measurements by including a polynomial as the model for the systematic errors, and find it works very well against the systematic effects, e.g. ones induced by stars and seeing. We provide accurate measurements {DA(0.59)rs,fid/rs, H(0.59)rs/rs,fid, f(0.59)σ8(0.59), Ωm h2} = {1427 ± 26 Mpc, 97.3 ± 3.3 km s−1 Mpc−1, 0.488 ± 0.060, 0.135 ± 0.016}, where rs is the comoving sound horizon at the drag epoch and rs,fid = 147.66 Mpc is the sound scale of the fiducial cosmology used in this study. The parameters which are not well constrained by our galaxy clustering analysis are marginalized over with wide flat priors. Since no priors from other data sets, e.g. cosmic microwave background (CMB), are adopted and no dark energy models are assumed, our results from BOSS CMASS galaxy clustering alone may be combined with other data sets, i.e. CMB, SNe, lensing or other galaxy clustering data to constrain the parameters of a given cosmological model. The uncertainty on the dark energy equation of state parameter, w, from CMB+CMASS is about 8 per cent. The uncertainty on the curvature fraction, Ωk, is 0.3 per cent. We do not find deviation from flat ΛCDM. Fil: Chuang, Chia-Hsun. Universidad Autónoma de Madrid; España Fil: Prada, Francisco. Universidad Autónoma de Madrid; España Fil: Pellejero Ibanez, Marcos. Instituto de Astrofísica de Canarias; España Fil: Beutler, Florian. Lawrence Berkeley National Lab,; Estados Unidos Fil: Cuesta, Antonio. Universidad de Barcelona; España Fil: Eisenstein, Daniel J.. Harvard-Smithsonian Center for Astrophysics; Estados Unidos Fil: Escoffier, Stephanie. Aix-Marseille Universite,; Francia Fil: Ho, Shirley. Carnegie Mellon University; Estados Unidos Fil: Kitaura, Francisco-Shu. Leibniz-Institut fur Astrophysik Potsdam; Alemania Fil: Kneib, Jean Paul. Aix Marseille Universite,; Francia Fil: Manera, Marc. University College London,; Reino Unido Fil: Nuza, Sebastian Ernesto. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina Fil: Rodriguez Torres, Sergio A.. Universidad Autónoma de Madrid; España Fil: Ross, Ashley. Ohio State University; Estados Unidos Fil: Rubiño Martín, J. A.. Instituto de Astrof´ısica de Canarias; España Fil: Samushia, Lado. Kansas State University; Estados Unidos Fil: Schlegel, David J.. Lawrence Berkeley National Laboratory; Estados Unidos Fil: Schneider, Donald P.. State University Of Pennsylvania; Estados Unidos Fil: Wang, Yuting. National Astronomy Observatories; China Fil: Weaber, Benjamin A.. University of New York; Estados Unidos Fil: Zao, Gongbo. National Astronomy Observatories; China Fil: Brownstein, Joel R.. University of Utah; Estados Unidos Fil: Dawson, Kyle S.. University of Utah; Estados Unidos Fil: Maraston, Claudia. University of Portsmouth; Reino Unido Fil: Olmestead, Matthew D.. King’s College; Estados Unidos Fil: Thomas, Daniel. University of Portsmouth; Reino Unido |
| description |
With the largest spectroscopic galaxy survey volume drawn from the SDSS-III Baryon Oscillation Spectroscopic Survey (BOSS), we can extract cosmological constraints from the measurements of redshift and geometric distortions at quasi-linear scales (e.g. above 50 h−1 Mpc). We analyse the broad-range shape of the monopole and quadrupole correlation functions of the BOSS Data Release 12 (DR12) CMASS galaxy sample, at the effective redshift z = 0.59, to obtain constraints on the Hubble expansion rate H(z), the angular- diameter distance DA(z), the normalized growth rate f(z)σ8(z), and the physical matter density Ωm h2. We obtain robust measurements by including a polynomial as the model for the systematic errors, and find it works very well against the systematic effects, e.g. ones induced by stars and seeing. We provide accurate measurements {DA(0.59)rs,fid/rs, H(0.59)rs/rs,fid, f(0.59)σ8(0.59), Ωm h2} = {1427 ± 26 Mpc, 97.3 ± 3.3 km s−1 Mpc−1, 0.488 ± 0.060, 0.135 ± 0.016}, where rs is the comoving sound horizon at the drag epoch and rs,fid = 147.66 Mpc is the sound scale of the fiducial cosmology used in this study. The parameters which are not well constrained by our galaxy clustering analysis are marginalized over with wide flat priors. Since no priors from other data sets, e.g. cosmic microwave background (CMB), are adopted and no dark energy models are assumed, our results from BOSS CMASS galaxy clustering alone may be combined with other data sets, i.e. CMB, SNe, lensing or other galaxy clustering data to constrain the parameters of a given cosmological model. The uncertainty on the dark energy equation of state parameter, w, from CMB+CMASS is about 8 per cent. The uncertainty on the curvature fraction, Ωk, is 0.3 per cent. We do not find deviation from flat ΛCDM. |
| publishDate |
2016 |
| dc.date.none.fl_str_mv |
2016-10 |
| dc.type.none.fl_str_mv |
info:eu-repo/semantics/article info:eu-repo/semantics/publishedVersion http://purl.org/coar/resource_type/c_6501 info:ar-repo/semantics/articulo |
| format |
article |
| status_str |
publishedVersion |
| dc.identifier.none.fl_str_mv |
http://hdl.handle.net/11336/18434 Chuang, Chia-Hsun; Prada, Francisco; Pellejero Ibanez, Marcos; Beutler, Florian; Cuesta, Antonio; et al.; The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: single-probe measurements from CMASS anisotropic galaxy clustering; Wiley Blackwell Publishing, Inc; Monthly Notices Of The Royal Astronomical Society; 461; 4; 10-2016; 3781-3793 0035-8711 CONICET Digital CONICET |
| url |
http://hdl.handle.net/11336/18434 |
| identifier_str_mv |
Chuang, Chia-Hsun; Prada, Francisco; Pellejero Ibanez, Marcos; Beutler, Florian; Cuesta, Antonio; et al.; The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: single-probe measurements from CMASS anisotropic galaxy clustering; Wiley Blackwell Publishing, Inc; Monthly Notices Of The Royal Astronomical Society; 461; 4; 10-2016; 3781-3793 0035-8711 CONICET Digital CONICET |
| dc.language.none.fl_str_mv |
eng |
| language |
eng |
| dc.relation.none.fl_str_mv |
info:eu-repo/semantics/altIdentifier/doi/10.1093/mnras/stw1535 info:eu-repo/semantics/altIdentifier/url/https://arxiv.org/abs/1312.4889 info:eu-repo/semantics/altIdentifier/url/https://academic.oup.com/mnras/article-abstract/461/4/3781/2608598/The-clustering-of-galaxies-in-the-SDSS-III-Baryon?redirectedFrom=PDF |
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info:eu-repo/semantics/openAccess https://creativecommons.org/licenses/by-nc-sa/2.5/ar/ |
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openAccess |
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application/pdf application/pdf |
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Wiley Blackwell Publishing, Inc |
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Wiley Blackwell Publishing, Inc |
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CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicas |
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dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar |
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