The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: Cosmological analysis of the DR12 galaxy sample
- Autores
- Alam, Shadab; Ata, Metin; Bailey, Stephen; Beutler, Florian; Bizyaev, Dmitry; Blazek, Jonathan A.; Bolton, Adam S.; Brownstein, Joel R.; Burden, Angela; Chuang, Chia Hsun; Comparat, Johan; Cuesta, Antonio J.; Dawson, Kyle S.; Eisenstein, Daniel J.; Escoffier, Stephanie; Gil Marín, Héctor; Grieb, Jan Niklas; Hand, Nick; Ho, Shirley; Kinemuchi, Karen; Kirkby, David; Kitaura, Francisco; Malanushenko, Elena; Malanushenko, Viktor; Maraston, Claudia; McBride, Cameron K.; Nichol, Robert C.; Olmstead, Matthew D.; Oravetz, Daniel; Padmanabhan, Nikhil; Palanque Delabrouille, Nathalie; Pan, Kaike; Pellejero Ibanez, Marcos; Percival, Will J.; Petitjean, Patrick; Prada, Francisco; Price Whelan, Adrian M.; Reid, Beth A.; Rodriguez Torres, Sergio A.; Roe, Natalie A.; Ross, Ashley; Ross, Nicholas P.; Rossi, Graziano; Rubiño Martin, Jose Alberto; Sánchez, Ariel G.; Saito, Shun; Salazar-Albornoz, Salvador; Samushia, Lado; Satpathy, Siddharth; Scoccola, Claudia Graciela; Schlegel, David J.; Schneider, Donald P.; Seo, Hee Jong; Simmons, Audrey; Slosar, Anze; Strauss, Michael A.; Swanson, Molly E. C.; Thomas, Daniel; Tinker, Jeremy L.; Tojeiro, Rita; Magaña, Mariana Vargas; Vazquez, Jose Alberto; Verde, Licia; Wake, David A.; Wang, Yuting; Weinberg, David H.; White, Martin; Wood Vasey, Michael W.; Yèche, Christophe; Zehavi, Idit; Zhai, Zhongxu; Zhao, Gong Bo
- Año de publicación
- 2017
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- We present cosmological results from the final galaxy clustering data set of the Baryon Oscillation Spectroscopic Survey, part of the Sloan Digital Sky Survey III. Our combined galaxy sample comprises 1.2 million massive galaxies over an effective area of 9329 deg2 and volume of 18.7 Gpc3, divided into three partially overlapping redshift slices centred at effective redshifts 0.38, 0.51 and 0.61. We measure the angular diameter distance DM and Hubble parameterHfrom the baryon acoustic oscillation (BAO) method, in combinationwith a cosmic microwave background prior on the sound horizon scale, after applying reconstruction to reduce non-linear effects on the BAO feature. Using the anisotropic clustering of the pre-reconstruction density field, we measure the product DMH from the Alcock-Paczynski (AP) effect and the growth of structure, quantified by fσ8(z), from redshift-space distortions (RSD). We combine individual measurements presented in seven companion papers into a set of consensus values and likelihoods, obtaining constraints that are tighter and more robust than those from any one method; in particular, the AP measurement from sub-BAO scales sharpens constraints from post-reconstruction BAOs by breaking degeneracy between DM and H. Combined with Planck 2016 cosmic microwave background measurements, our distance scale measurements simultaneously imply curvature ωK = 0.0003 ± 0.0026 and a dark energy equation-of-state parameter ω =-1.01 ± 0.06, in strong affirmation of the spatially flat cold dark matter (CDM) model with a cosmological constant (ΛCDM). Our RSD measurements of fσ8, at 6 per cent precision, are similarly consistent with this model. When combined with supernova Ia data, we find H0 = 67.3 ± 1.0 kms-1 Mpc-1 even for our most general dark energy model, in tension with some direct measurements. Adding extra relativistic species as a degree of freedom loosens the constraint only slightly, to H0 = 67.8 ± 1.2 kms-1 Mpc-1. Assuming flat ΛCDM, we find ωm = 0.310 ± 0.005 and H0 = 67.6 ± 0.5 kms-1 Mpc-1, and we find a 95 per cent upper limit of 0.16 eV c-2 on the neutrino mass sum.
Fil: Alam, Shadab. University of Carnegie Mellon; Estados Unidos
Fil: Ata, Metin. Leibniz-institute Für Astrophysik Potsdam; Alemania
Fil: Bailey, Stephen. Lawrence Berkeley National Laboratory; Estados Unidos
Fil: Beutler, Florian. Lawrence Berkeley National Laboratory; Estados Unidos
Fil: Bizyaev, Dmitry. Apache Point Observatory and New Mexico State University; México. Moscow State University; Rusia
Fil: Blazek, Jonathan A.. Ohio State University; Estados Unidos
Fil: Bolton, Adam S.. University of Utah; Estados Unidos. National Optical Astronomy Observatory; Estados Unidos
Fil: Brownstein, Joel R.. University of Utah; Estados Unidos
Fil: Burden, Angela. University of Yale; Estados Unidos
Fil: Chuang, Chia Hsun. Leibniz-institute Für Astrophysik Potsdam; Alemania. Universidad Autónoma de Madrid; España
Fil: Comparat, Johan. Universidad Autónoma de Madrid; España
Fil: Cuesta, Antonio J.. Universidad de Barcelona; España
Fil: Dawson, Kyle S.. University of Utah; Estados Unidos
Fil: Eisenstein, Daniel J.. Harvard-Smithsonian Center for Astrophysics; Estados Unidos
Fil: Escoffier, Stephanie. Centre National de la Recherche Scientifique; Francia. Universidad de Aix-Marsella; Francia
Fil: Gil Marín, Héctor. Universite Pierre et Marie Curie; Francia. Universite Paris Sorbonne; Francia
Fil: Grieb, Jan Niklas. Max Planck Institut Fur Extraterrestrische Physi; Alemania. Universitats-Sternwarte München; Alemania
Fil: Hand, Nick. University of California at Berkeley; Estados Unidos
Fil: Ho, Shirley. University of Carnegie Mellon; Estados Unidos
Fil: Kinemuchi, Karen. Apache Point Observatory and New Mexico State University; México
Fil: Kirkby, David. University of California at Irvine; Estados Unidos
Fil: Kitaura, Francisco. University of California at Berkeley; Estados Unidos. Lawrence Berkeley National Laboratory; Estados Unidos. Leibniz-institute Für Astrophysik Potsdam; Alemania
Fil: Malanushenko, Elena. Apache Point Observatory and New Mexico State University; México
Fil: Malanushenko, Viktor. Apache Point Observatory and New Mexico State University; México
Fil: Maraston, Claudia. University of Portsmouth; Reino Unido
Fil: McBride, Cameron K.. Harvard-Smithsonian Center for Astrophysics; Estados Unidos
Fil: Nichol, Robert C.. University of Portsmouth; Reino Unido
Fil: Olmstead, Matthew D.. Department of Chemistry and Physics, King’s College, Wilkes Barre; Estados Unidos
Fil: Oravetz, Daniel. Apache Point Observatory and New Mexico State University; México
Fil: Padmanabhan, Nikhil. University of Yale; Estados Unidos
Fil: Palanque Delabrouille, Nathalie. No especifíca;
Fil: Pan, Kaike. Apache Point Observatory and New Mexico State University; México
Fil: Pellejero Ibanez, Marcos. Universidad de La Laguna; España. Instituto Astrofísico de Canarias; España
Fil: Percival, Will J.. University of Portsmouth; Reino Unido
Fil: Petitjean, Patrick. Universite Pierre et Marie Curie; Francia
Fil: Prada, Francisco. Universidad Autónoma de Madrid; España
Fil: Price Whelan, Adrian M.. University of Princeton; Estados Unidos
Fil: Reid, Beth A.. Lawrence Berkeley National Laboratory; Estados Unidos. University of California at Berkeley; Estados Unidos
Fil: Rodriguez Torres, Sergio A.. Universidad Autónoma de Madrid; España
Fil: Roe, Natalie A.. Lawrence Berkeley National Laboratory; Estados Unidos
Fil: Ross, Ashley. Ohio State University; Estados Unidos. University Of Portsmouth; Reino Unido
Fil: Ross, Nicholas P.. University of Edinburgh; Reino Unido
Fil: Rossi, Graziano. Sejong University; Corea del Sur
Fil: Rubiño Martin, Jose Alberto. Universidad de La Laguna; España. Instituto Astrofísico de Canarias; España
Fil: Sánchez, Ariel G.. Max Planck Institut Fur Extraterrestrische Physik; Alemania
Fil: Saito, Shun. Gobierno de la Republica Federal de Alemania. Max Planck Institut Fur Astrophysik; Alemania. University Of Tokyo; Japón
Fil: Salazar-Albornoz, Salvador. Ludwig Maximilians Universitat; Alemania. Max Planck Institut Fur Extraterrestrische Physik; Alemania
Fil: Samushia, Lado. Kansas State University; Estados Unidos
Fil: Satpathy, Siddharth. University of Carnegie Mellon; Estados Unidos
Fil: Scoccola, Claudia Graciela. Universidad Autónoma de Madrid; España. Universidad Nacional de la Plata. Facultad de Cs.astronómicas y Geofísicas. Observatorio Astronómica D/la Plata - Sede Central; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata; Argentina
Fil: Schlegel, David J.. Lawrence Berkeley National Laboratory; Estados Unidos
Fil: Schneider, Donald P.. State University of Pennsylvania; Estados Unidos
Fil: Seo, Hee Jong. Ohio University; Estados Unidos
Fil: Simmons, Audrey. Apache Point Observatory and New Mexico State University; México
Fil: Slosar, Anze. Brookhaven National Laboratory; Estados Unidos
Fil: Strauss, Michael A.. University of Princeton; Estados Unidos
Fil: Swanson, Molly E. C.. Harvard-Smithsonian Center for Astrophysics; Estados Unidos
Fil: Thomas, Daniel. University Of Portsmouth; Reino Unido
Fil: Tinker, Jeremy L.. University of New York; Estados Unidos
Fil: Tojeiro, Rita. University of St. Andrews; Reino Unido
Fil: Magaña, Mariana Vargas. University of Carnegie Mellon; Estados Unidos. Universidad Nacional Autónoma de México; México
Fil: Vazquez, Jose Alberto. Brookhaven National Laboratory; Estados Unidos
Fil: Verde, Licia. University of Oslo; Noruega. Universidad de Barcelona; España. Harvard University; Estados Unidos
Fil: Wake, David A.. University of Wisconsin; Estados Unidos. The Open University; Reino Unido
Fil: Wang, Yuting. University Of Portsmouth; Reino Unido
Fil: Weinberg, David H.. Ohio State University; Estados Unidos
Fil: White, Martin. Lawrence Berkeley National Laboratory; Estados Unidos. University of California at Berkeley; Estados Unidos
Fil: Wood Vasey, Michael W.. University of Pittsburgh; Estados Unidos
Fil: Yèche, Christophe. Centre de Saclay; Francia
Fil: Zehavi, Idit. Case Western Reserve University; Estados Unidos
Fil: Zhai, Zhongxu. University of New York; Estados Unidos
Fil: Zhao, Gong Bo. Chinese Academy of Sciences; República de China. University of Portsmouth; Reino Unido - Materia
-
COSMOLOGY: OBSERVATIONS
DISTANCE SCALE
LARGE-SCALE STRUCTURE OF UNIVERSE - 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:11336/112633
Ver los metadatos del registro completo
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The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: Cosmological analysis of the DR12 galaxy sampleAlam, ShadabAta, MetinBailey, StephenBeutler, FlorianBizyaev, DmitryBlazek, Jonathan A.Bolton, Adam S.Brownstein, Joel R.Burden, AngelaChuang, Chia HsunComparat, JohanCuesta, Antonio J.Dawson, Kyle S.Eisenstein, Daniel J.Escoffier, StephanieGil Marín, HéctorGrieb, Jan NiklasHand, NickHo, ShirleyKinemuchi, KarenKirkby, DavidKitaura, FranciscoMalanushenko, ElenaMalanushenko, ViktorMaraston, ClaudiaMcBride, Cameron K.Nichol, Robert C.Olmstead, Matthew D.Oravetz, DanielPadmanabhan, NikhilPalanque Delabrouille, NathaliePan, KaikePellejero Ibanez, MarcosPercival, Will J.Petitjean, PatrickPrada, FranciscoPrice Whelan, Adrian M.Reid, Beth A.Rodriguez Torres, Sergio A.Roe, Natalie A.Ross, AshleyRoss, Nicholas P.Rossi, GrazianoRubiño Martin, Jose AlbertoSánchez, Ariel G.Saito, ShunSalazar-Albornoz, SalvadorSamushia, LadoSatpathy, SiddharthScoccola, Claudia GracielaSchlegel, David J.Schneider, Donald P.Seo, Hee JongSimmons, AudreySlosar, AnzeStrauss, Michael A.Swanson, Molly E. C.Thomas, DanielTinker, Jeremy L.Tojeiro, RitaMagaña, Mariana VargasVazquez, Jose AlbertoVerde, LiciaWake, David A.Wang, YutingWeinberg, David H.White, MartinWood Vasey, Michael W.Yèche, ChristopheZehavi, IditZhai, ZhongxuZhao, Gong BoCOSMOLOGY: OBSERVATIONSDISTANCE SCALELARGE-SCALE STRUCTURE OF UNIVERSEhttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1We present cosmological results from the final galaxy clustering data set of the Baryon Oscillation Spectroscopic Survey, part of the Sloan Digital Sky Survey III. Our combined galaxy sample comprises 1.2 million massive galaxies over an effective area of 9329 deg2 and volume of 18.7 Gpc3, divided into three partially overlapping redshift slices centred at effective redshifts 0.38, 0.51 and 0.61. We measure the angular diameter distance DM and Hubble parameterHfrom the baryon acoustic oscillation (BAO) method, in combinationwith a cosmic microwave background prior on the sound horizon scale, after applying reconstruction to reduce non-linear effects on the BAO feature. Using the anisotropic clustering of the pre-reconstruction density field, we measure the product DMH from the Alcock-Paczynski (AP) effect and the growth of structure, quantified by fσ8(z), from redshift-space distortions (RSD). We combine individual measurements presented in seven companion papers into a set of consensus values and likelihoods, obtaining constraints that are tighter and more robust than those from any one method; in particular, the AP measurement from sub-BAO scales sharpens constraints from post-reconstruction BAOs by breaking degeneracy between DM and H. Combined with Planck 2016 cosmic microwave background measurements, our distance scale measurements simultaneously imply curvature ωK = 0.0003 ± 0.0026 and a dark energy equation-of-state parameter ω =-1.01 ± 0.06, in strong affirmation of the spatially flat cold dark matter (CDM) model with a cosmological constant (ΛCDM). Our RSD measurements of fσ8, at 6 per cent precision, are similarly consistent with this model. When combined with supernova Ia data, we find H0 = 67.3 ± 1.0 kms-1 Mpc-1 even for our most general dark energy model, in tension with some direct measurements. Adding extra relativistic species as a degree of freedom loosens the constraint only slightly, to H0 = 67.8 ± 1.2 kms-1 Mpc-1. Assuming flat ΛCDM, we find ωm = 0.310 ± 0.005 and H0 = 67.6 ± 0.5 kms-1 Mpc-1, and we find a 95 per cent upper limit of 0.16 eV c-2 on the neutrino mass sum.Fil: Alam, Shadab. University of Carnegie Mellon; Estados UnidosFil: Ata, Metin. Leibniz-institute Für Astrophysik Potsdam; AlemaniaFil: Bailey, Stephen. Lawrence Berkeley National Laboratory; Estados UnidosFil: Beutler, Florian. Lawrence Berkeley National Laboratory; Estados UnidosFil: Bizyaev, Dmitry. Apache Point Observatory and New Mexico State University; México. Moscow State University; RusiaFil: Blazek, Jonathan A.. Ohio State University; Estados UnidosFil: Bolton, Adam S.. University of Utah; Estados Unidos. National Optical Astronomy Observatory; Estados UnidosFil: Brownstein, Joel R.. University of Utah; Estados UnidosFil: Burden, Angela. University of Yale; Estados UnidosFil: Chuang, Chia Hsun. Leibniz-institute Für Astrophysik Potsdam; Alemania. Universidad Autónoma de Madrid; EspañaFil: Comparat, Johan. Universidad Autónoma de Madrid; EspañaFil: Cuesta, Antonio J.. Universidad de Barcelona; EspañaFil: Dawson, Kyle S.. University of Utah; Estados UnidosFil: Eisenstein, Daniel J.. Harvard-Smithsonian Center for Astrophysics; Estados UnidosFil: Escoffier, Stephanie. Centre National de la Recherche Scientifique; Francia. Universidad de Aix-Marsella; FranciaFil: Gil Marín, Héctor. Universite Pierre et Marie Curie; Francia. Universite Paris Sorbonne; FranciaFil: Grieb, Jan Niklas. Max Planck Institut Fur Extraterrestrische Physi; Alemania. Universitats-Sternwarte München; AlemaniaFil: Hand, Nick. University of California at Berkeley; Estados UnidosFil: Ho, Shirley. University of Carnegie Mellon; Estados UnidosFil: Kinemuchi, Karen. Apache Point Observatory and New Mexico State University; MéxicoFil: Kirkby, David. University of California at Irvine; Estados UnidosFil: Kitaura, Francisco. University of California at Berkeley; Estados Unidos. Lawrence Berkeley National Laboratory; Estados Unidos. Leibniz-institute Für Astrophysik Potsdam; AlemaniaFil: Malanushenko, Elena. Apache Point Observatory and New Mexico State University; MéxicoFil: Malanushenko, Viktor. Apache Point Observatory and New Mexico State University; MéxicoFil: Maraston, Claudia. University of Portsmouth; Reino UnidoFil: McBride, Cameron K.. Harvard-Smithsonian Center for Astrophysics; Estados UnidosFil: Nichol, Robert C.. University of Portsmouth; Reino UnidoFil: Olmstead, Matthew D.. Department of Chemistry and Physics, King’s College, Wilkes Barre; Estados UnidosFil: Oravetz, Daniel. Apache Point Observatory and New Mexico State University; MéxicoFil: Padmanabhan, Nikhil. University of Yale; Estados UnidosFil: Palanque Delabrouille, Nathalie. No especifíca;Fil: Pan, Kaike. Apache Point Observatory and New Mexico State University; MéxicoFil: Pellejero Ibanez, Marcos. Universidad de La Laguna; España. Instituto Astrofísico de Canarias; EspañaFil: Percival, Will J.. University of Portsmouth; Reino UnidoFil: Petitjean, Patrick. Universite Pierre et Marie Curie; FranciaFil: Prada, Francisco. Universidad Autónoma de Madrid; EspañaFil: Price Whelan, Adrian M.. University of Princeton; Estados UnidosFil: Reid, Beth A.. Lawrence Berkeley National Laboratory; Estados Unidos. University of California at Berkeley; Estados UnidosFil: Rodriguez Torres, Sergio A.. Universidad Autónoma de Madrid; EspañaFil: Roe, Natalie A.. Lawrence Berkeley National Laboratory; Estados UnidosFil: Ross, Ashley. Ohio State University; Estados Unidos. University Of Portsmouth; Reino UnidoFil: Ross, Nicholas P.. University of Edinburgh; Reino UnidoFil: Rossi, Graziano. Sejong University; Corea del SurFil: Rubiño Martin, Jose Alberto. Universidad de La Laguna; España. Instituto Astrofísico de Canarias; EspañaFil: Sánchez, Ariel G.. Max Planck Institut Fur Extraterrestrische Physik; AlemaniaFil: Saito, Shun. Gobierno de la Republica Federal de Alemania. Max Planck Institut Fur Astrophysik; Alemania. University Of Tokyo; JapónFil: Salazar-Albornoz, Salvador. Ludwig Maximilians Universitat; Alemania. Max Planck Institut Fur Extraterrestrische Physik; AlemaniaFil: Samushia, Lado. Kansas State University; Estados UnidosFil: Satpathy, Siddharth. University of Carnegie Mellon; Estados UnidosFil: Scoccola, Claudia Graciela. Universidad Autónoma de Madrid; España. Universidad Nacional de la Plata. Facultad de Cs.astronómicas y Geofísicas. Observatorio Astronómica D/la Plata - Sede Central; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata; ArgentinaFil: Schlegel, David J.. Lawrence Berkeley National Laboratory; Estados UnidosFil: Schneider, Donald P.. State University of Pennsylvania; Estados UnidosFil: Seo, Hee Jong. Ohio University; Estados UnidosFil: Simmons, Audrey. Apache Point Observatory and New Mexico State University; MéxicoFil: Slosar, Anze. Brookhaven National Laboratory; Estados UnidosFil: Strauss, Michael A.. University of Princeton; Estados UnidosFil: Swanson, Molly E. C.. Harvard-Smithsonian Center for Astrophysics; Estados UnidosFil: Thomas, Daniel. University Of Portsmouth; Reino UnidoFil: Tinker, Jeremy L.. University of New York; Estados UnidosFil: Tojeiro, Rita. University of St. Andrews; Reino UnidoFil: Magaña, Mariana Vargas. University of Carnegie Mellon; Estados Unidos. Universidad Nacional Autónoma de México; MéxicoFil: Vazquez, Jose Alberto. Brookhaven National Laboratory; Estados UnidosFil: Verde, Licia. University of Oslo; Noruega. Universidad de Barcelona; España. Harvard University; Estados UnidosFil: Wake, David A.. University of Wisconsin; Estados Unidos. The Open University; Reino UnidoFil: Wang, Yuting. University Of Portsmouth; Reino UnidoFil: Weinberg, David H.. Ohio State University; Estados UnidosFil: White, Martin. Lawrence Berkeley National Laboratory; Estados Unidos. University of California at Berkeley; Estados UnidosFil: Wood Vasey, Michael W.. University of Pittsburgh; Estados UnidosFil: Yèche, Christophe. Centre de Saclay; FranciaFil: Zehavi, Idit. Case Western Reserve University; Estados UnidosFil: Zhai, Zhongxu. University of New York; Estados UnidosFil: Zhao, Gong Bo. Chinese Academy of Sciences; República de China. University of Portsmouth; Reino UnidoWiley Blackwell Publishing, Inc2017-09info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/112633Alam, Shadab; Ata, Metin; Bailey, Stephen; Beutler, Florian; Bizyaev, Dmitry; et al.; The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: Cosmological analysis of the DR12 galaxy sample; Wiley Blackwell Publishing, Inc; Monthly Notices of the Royal Astronomical Society; 470; 3; 9-2017; 2617-26520035-8711CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.1093/mnras/stx721info:eu-repo/semantics/altIdentifier/url/https://academic.oup.com/mnras/article-abstract/470/3/2617/3091741?redirectedFrom=fulltextinfo:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-10-22T11:27:55Zoai:ri.conicet.gov.ar:11336/112633instacron: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 11:27:56.091CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
| dc.title.none.fl_str_mv |
The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: Cosmological analysis of the DR12 galaxy sample |
| title |
The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: Cosmological analysis of the DR12 galaxy sample |
| spellingShingle |
The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: Cosmological analysis of the DR12 galaxy sample Alam, Shadab COSMOLOGY: OBSERVATIONS DISTANCE SCALE LARGE-SCALE STRUCTURE OF UNIVERSE |
| title_short |
The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: Cosmological analysis of the DR12 galaxy sample |
| title_full |
The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: Cosmological analysis of the DR12 galaxy sample |
| title_fullStr |
The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: Cosmological analysis of the DR12 galaxy sample |
| title_full_unstemmed |
The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: Cosmological analysis of the DR12 galaxy sample |
| title_sort |
The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: Cosmological analysis of the DR12 galaxy sample |
| dc.creator.none.fl_str_mv |
Alam, Shadab Ata, Metin Bailey, Stephen Beutler, Florian Bizyaev, Dmitry Blazek, Jonathan A. Bolton, Adam S. Brownstein, Joel R. Burden, Angela Chuang, Chia Hsun Comparat, Johan Cuesta, Antonio J. Dawson, Kyle S. Eisenstein, Daniel J. Escoffier, Stephanie Gil Marín, Héctor Grieb, Jan Niklas Hand, Nick Ho, Shirley Kinemuchi, Karen Kirkby, David Kitaura, Francisco Malanushenko, Elena Malanushenko, Viktor Maraston, Claudia McBride, Cameron K. Nichol, Robert C. Olmstead, Matthew D. Oravetz, Daniel Padmanabhan, Nikhil Palanque Delabrouille, Nathalie Pan, Kaike Pellejero Ibanez, Marcos Percival, Will J. Petitjean, Patrick Prada, Francisco Price Whelan, Adrian M. Reid, Beth A. Rodriguez Torres, Sergio A. Roe, Natalie A. Ross, Ashley Ross, Nicholas P. Rossi, Graziano Rubiño Martin, Jose Alberto Sánchez, Ariel G. Saito, Shun Salazar-Albornoz, Salvador Samushia, Lado Satpathy, Siddharth Scoccola, Claudia Graciela Schlegel, David J. Schneider, Donald P. Seo, Hee Jong Simmons, Audrey Slosar, Anze Strauss, Michael A. Swanson, Molly E. C. Thomas, Daniel Tinker, Jeremy L. Tojeiro, Rita Magaña, Mariana Vargas Vazquez, Jose Alberto Verde, Licia Wake, David A. Wang, Yuting Weinberg, David H. White, Martin Wood Vasey, Michael W. Yèche, Christophe Zehavi, Idit Zhai, Zhongxu Zhao, Gong Bo |
| author |
Alam, Shadab |
| author_facet |
Alam, Shadab Ata, Metin Bailey, Stephen Beutler, Florian Bizyaev, Dmitry Blazek, Jonathan A. Bolton, Adam S. Brownstein, Joel R. Burden, Angela Chuang, Chia Hsun Comparat, Johan Cuesta, Antonio J. Dawson, Kyle S. Eisenstein, Daniel J. Escoffier, Stephanie Gil Marín, Héctor Grieb, Jan Niklas Hand, Nick Ho, Shirley Kinemuchi, Karen Kirkby, David Kitaura, Francisco Malanushenko, Elena Malanushenko, Viktor Maraston, Claudia McBride, Cameron K. Nichol, Robert C. Olmstead, Matthew D. Oravetz, Daniel Padmanabhan, Nikhil Palanque Delabrouille, Nathalie Pan, Kaike Pellejero Ibanez, Marcos Percival, Will J. Petitjean, Patrick Prada, Francisco Price Whelan, Adrian M. Reid, Beth A. Rodriguez Torres, Sergio A. Roe, Natalie A. Ross, Ashley Ross, Nicholas P. Rossi, Graziano Rubiño Martin, Jose Alberto Sánchez, Ariel G. Saito, Shun Salazar-Albornoz, Salvador Samushia, Lado Satpathy, Siddharth Scoccola, Claudia Graciela Schlegel, David J. Schneider, Donald P. Seo, Hee Jong Simmons, Audrey Slosar, Anze Strauss, Michael A. Swanson, Molly E. C. Thomas, Daniel Tinker, Jeremy L. Tojeiro, Rita Magaña, Mariana Vargas Vazquez, Jose Alberto Verde, Licia Wake, David A. Wang, Yuting Weinberg, David H. White, Martin Wood Vasey, Michael W. Yèche, Christophe Zehavi, Idit Zhai, Zhongxu Zhao, Gong Bo |
| author_role |
author |
| author2 |
Ata, Metin Bailey, Stephen Beutler, Florian Bizyaev, Dmitry Blazek, Jonathan A. Bolton, Adam S. Brownstein, Joel R. Burden, Angela Chuang, Chia Hsun Comparat, Johan Cuesta, Antonio J. Dawson, Kyle S. Eisenstein, Daniel J. Escoffier, Stephanie Gil Marín, Héctor Grieb, Jan Niklas Hand, Nick Ho, Shirley Kinemuchi, Karen Kirkby, David Kitaura, Francisco Malanushenko, Elena Malanushenko, Viktor Maraston, Claudia McBride, Cameron K. Nichol, Robert C. Olmstead, Matthew D. Oravetz, Daniel Padmanabhan, Nikhil Palanque Delabrouille, Nathalie Pan, Kaike Pellejero Ibanez, Marcos Percival, Will J. Petitjean, Patrick Prada, Francisco Price Whelan, Adrian M. Reid, Beth A. Rodriguez Torres, Sergio A. Roe, Natalie A. Ross, Ashley Ross, Nicholas P. Rossi, Graziano Rubiño Martin, Jose Alberto Sánchez, Ariel G. Saito, Shun Salazar-Albornoz, Salvador Samushia, Lado Satpathy, Siddharth Scoccola, Claudia Graciela Schlegel, David J. Schneider, Donald P. Seo, Hee Jong Simmons, Audrey Slosar, Anze Strauss, Michael A. Swanson, Molly E. C. Thomas, Daniel Tinker, Jeremy L. Tojeiro, Rita Magaña, Mariana Vargas Vazquez, Jose Alberto Verde, Licia Wake, David A. Wang, Yuting Weinberg, David H. White, Martin Wood Vasey, Michael W. Yèche, Christophe Zehavi, Idit Zhai, Zhongxu Zhao, Gong Bo |
| 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 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 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 |
| topic |
COSMOLOGY: OBSERVATIONS DISTANCE SCALE LARGE-SCALE STRUCTURE OF UNIVERSE |
| purl_subject.fl_str_mv |
https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 |
| dc.description.none.fl_txt_mv |
We present cosmological results from the final galaxy clustering data set of the Baryon Oscillation Spectroscopic Survey, part of the Sloan Digital Sky Survey III. Our combined galaxy sample comprises 1.2 million massive galaxies over an effective area of 9329 deg2 and volume of 18.7 Gpc3, divided into three partially overlapping redshift slices centred at effective redshifts 0.38, 0.51 and 0.61. We measure the angular diameter distance DM and Hubble parameterHfrom the baryon acoustic oscillation (BAO) method, in combinationwith a cosmic microwave background prior on the sound horizon scale, after applying reconstruction to reduce non-linear effects on the BAO feature. Using the anisotropic clustering of the pre-reconstruction density field, we measure the product DMH from the Alcock-Paczynski (AP) effect and the growth of structure, quantified by fσ8(z), from redshift-space distortions (RSD). We combine individual measurements presented in seven companion papers into a set of consensus values and likelihoods, obtaining constraints that are tighter and more robust than those from any one method; in particular, the AP measurement from sub-BAO scales sharpens constraints from post-reconstruction BAOs by breaking degeneracy between DM and H. Combined with Planck 2016 cosmic microwave background measurements, our distance scale measurements simultaneously imply curvature ωK = 0.0003 ± 0.0026 and a dark energy equation-of-state parameter ω =-1.01 ± 0.06, in strong affirmation of the spatially flat cold dark matter (CDM) model with a cosmological constant (ΛCDM). Our RSD measurements of fσ8, at 6 per cent precision, are similarly consistent with this model. When combined with supernova Ia data, we find H0 = 67.3 ± 1.0 kms-1 Mpc-1 even for our most general dark energy model, in tension with some direct measurements. Adding extra relativistic species as a degree of freedom loosens the constraint only slightly, to H0 = 67.8 ± 1.2 kms-1 Mpc-1. Assuming flat ΛCDM, we find ωm = 0.310 ± 0.005 and H0 = 67.6 ± 0.5 kms-1 Mpc-1, and we find a 95 per cent upper limit of 0.16 eV c-2 on the neutrino mass sum. Fil: Alam, Shadab. University of Carnegie Mellon; Estados Unidos Fil: Ata, Metin. Leibniz-institute Für Astrophysik Potsdam; Alemania Fil: Bailey, Stephen. Lawrence Berkeley National Laboratory; Estados Unidos Fil: Beutler, Florian. Lawrence Berkeley National Laboratory; Estados Unidos Fil: Bizyaev, Dmitry. Apache Point Observatory and New Mexico State University; México. Moscow State University; Rusia Fil: Blazek, Jonathan A.. Ohio State University; Estados Unidos Fil: Bolton, Adam S.. University of Utah; Estados Unidos. National Optical Astronomy Observatory; Estados Unidos Fil: Brownstein, Joel R.. University of Utah; Estados Unidos Fil: Burden, Angela. University of Yale; Estados Unidos Fil: Chuang, Chia Hsun. Leibniz-institute Für Astrophysik Potsdam; Alemania. Universidad Autónoma de Madrid; España Fil: Comparat, Johan. Universidad Autónoma de Madrid; España Fil: Cuesta, Antonio J.. Universidad de Barcelona; España Fil: Dawson, Kyle S.. University of Utah; Estados Unidos Fil: Eisenstein, Daniel J.. Harvard-Smithsonian Center for Astrophysics; Estados Unidos Fil: Escoffier, Stephanie. Centre National de la Recherche Scientifique; Francia. Universidad de Aix-Marsella; Francia Fil: Gil Marín, Héctor. Universite Pierre et Marie Curie; Francia. Universite Paris Sorbonne; Francia Fil: Grieb, Jan Niklas. Max Planck Institut Fur Extraterrestrische Physi; Alemania. Universitats-Sternwarte München; Alemania Fil: Hand, Nick. University of California at Berkeley; Estados Unidos Fil: Ho, Shirley. University of Carnegie Mellon; Estados Unidos Fil: Kinemuchi, Karen. Apache Point Observatory and New Mexico State University; México Fil: Kirkby, David. University of California at Irvine; Estados Unidos Fil: Kitaura, Francisco. University of California at Berkeley; Estados Unidos. Lawrence Berkeley National Laboratory; Estados Unidos. Leibniz-institute Für Astrophysik Potsdam; Alemania Fil: Malanushenko, Elena. Apache Point Observatory and New Mexico State University; México Fil: Malanushenko, Viktor. Apache Point Observatory and New Mexico State University; México Fil: Maraston, Claudia. University of Portsmouth; Reino Unido Fil: McBride, Cameron K.. Harvard-Smithsonian Center for Astrophysics; Estados Unidos Fil: Nichol, Robert C.. University of Portsmouth; Reino Unido Fil: Olmstead, Matthew D.. Department of Chemistry and Physics, King’s College, Wilkes Barre; Estados Unidos Fil: Oravetz, Daniel. Apache Point Observatory and New Mexico State University; México Fil: Padmanabhan, Nikhil. University of Yale; Estados Unidos Fil: Palanque Delabrouille, Nathalie. No especifíca; Fil: Pan, Kaike. Apache Point Observatory and New Mexico State University; México Fil: Pellejero Ibanez, Marcos. Universidad de La Laguna; España. Instituto Astrofísico de Canarias; España Fil: Percival, Will J.. University of Portsmouth; Reino Unido Fil: Petitjean, Patrick. Universite Pierre et Marie Curie; Francia Fil: Prada, Francisco. Universidad Autónoma de Madrid; España Fil: Price Whelan, Adrian M.. University of Princeton; Estados Unidos Fil: Reid, Beth A.. Lawrence Berkeley National Laboratory; Estados Unidos. University of California at Berkeley; Estados Unidos Fil: Rodriguez Torres, Sergio A.. Universidad Autónoma de Madrid; España Fil: Roe, Natalie A.. Lawrence Berkeley National Laboratory; Estados Unidos Fil: Ross, Ashley. Ohio State University; Estados Unidos. University Of Portsmouth; Reino Unido Fil: Ross, Nicholas P.. University of Edinburgh; Reino Unido Fil: Rossi, Graziano. Sejong University; Corea del Sur Fil: Rubiño Martin, Jose Alberto. Universidad de La Laguna; España. Instituto Astrofísico de Canarias; España Fil: Sánchez, Ariel G.. Max Planck Institut Fur Extraterrestrische Physik; Alemania Fil: Saito, Shun. Gobierno de la Republica Federal de Alemania. Max Planck Institut Fur Astrophysik; Alemania. University Of Tokyo; Japón Fil: Salazar-Albornoz, Salvador. Ludwig Maximilians Universitat; Alemania. Max Planck Institut Fur Extraterrestrische Physik; Alemania Fil: Samushia, Lado. Kansas State University; Estados Unidos Fil: Satpathy, Siddharth. University of Carnegie Mellon; Estados Unidos Fil: Scoccola, Claudia Graciela. Universidad Autónoma de Madrid; España. Universidad Nacional de la Plata. Facultad de Cs.astronómicas y Geofísicas. Observatorio Astronómica D/la Plata - Sede Central; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata; Argentina Fil: Schlegel, David J.. Lawrence Berkeley National Laboratory; Estados Unidos Fil: Schneider, Donald P.. State University of Pennsylvania; Estados Unidos Fil: Seo, Hee Jong. Ohio University; Estados Unidos Fil: Simmons, Audrey. Apache Point Observatory and New Mexico State University; México Fil: Slosar, Anze. Brookhaven National Laboratory; Estados Unidos Fil: Strauss, Michael A.. University of Princeton; Estados Unidos Fil: Swanson, Molly E. C.. Harvard-Smithsonian Center for Astrophysics; Estados Unidos Fil: Thomas, Daniel. University Of Portsmouth; Reino Unido Fil: Tinker, Jeremy L.. University of New York; Estados Unidos Fil: Tojeiro, Rita. University of St. Andrews; Reino Unido Fil: Magaña, Mariana Vargas. University of Carnegie Mellon; Estados Unidos. Universidad Nacional Autónoma de México; México Fil: Vazquez, Jose Alberto. Brookhaven National Laboratory; Estados Unidos Fil: Verde, Licia. University of Oslo; Noruega. Universidad de Barcelona; España. Harvard University; Estados Unidos Fil: Wake, David A.. University of Wisconsin; Estados Unidos. The Open University; Reino Unido Fil: Wang, Yuting. University Of Portsmouth; Reino Unido Fil: Weinberg, David H.. Ohio State University; Estados Unidos Fil: White, Martin. Lawrence Berkeley National Laboratory; Estados Unidos. University of California at Berkeley; Estados Unidos Fil: Wood Vasey, Michael W.. University of Pittsburgh; Estados Unidos Fil: Yèche, Christophe. Centre de Saclay; Francia Fil: Zehavi, Idit. Case Western Reserve University; Estados Unidos Fil: Zhai, Zhongxu. University of New York; Estados Unidos Fil: Zhao, Gong Bo. Chinese Academy of Sciences; República de China. University of Portsmouth; Reino Unido |
| description |
We present cosmological results from the final galaxy clustering data set of the Baryon Oscillation Spectroscopic Survey, part of the Sloan Digital Sky Survey III. Our combined galaxy sample comprises 1.2 million massive galaxies over an effective area of 9329 deg2 and volume of 18.7 Gpc3, divided into three partially overlapping redshift slices centred at effective redshifts 0.38, 0.51 and 0.61. We measure the angular diameter distance DM and Hubble parameterHfrom the baryon acoustic oscillation (BAO) method, in combinationwith a cosmic microwave background prior on the sound horizon scale, after applying reconstruction to reduce non-linear effects on the BAO feature. Using the anisotropic clustering of the pre-reconstruction density field, we measure the product DMH from the Alcock-Paczynski (AP) effect and the growth of structure, quantified by fσ8(z), from redshift-space distortions (RSD). We combine individual measurements presented in seven companion papers into a set of consensus values and likelihoods, obtaining constraints that are tighter and more robust than those from any one method; in particular, the AP measurement from sub-BAO scales sharpens constraints from post-reconstruction BAOs by breaking degeneracy between DM and H. Combined with Planck 2016 cosmic microwave background measurements, our distance scale measurements simultaneously imply curvature ωK = 0.0003 ± 0.0026 and a dark energy equation-of-state parameter ω =-1.01 ± 0.06, in strong affirmation of the spatially flat cold dark matter (CDM) model with a cosmological constant (ΛCDM). Our RSD measurements of fσ8, at 6 per cent precision, are similarly consistent with this model. When combined with supernova Ia data, we find H0 = 67.3 ± 1.0 kms-1 Mpc-1 even for our most general dark energy model, in tension with some direct measurements. Adding extra relativistic species as a degree of freedom loosens the constraint only slightly, to H0 = 67.8 ± 1.2 kms-1 Mpc-1. Assuming flat ΛCDM, we find ωm = 0.310 ± 0.005 and H0 = 67.6 ± 0.5 kms-1 Mpc-1, and we find a 95 per cent upper limit of 0.16 eV c-2 on the neutrino mass sum. |
| publishDate |
2017 |
| dc.date.none.fl_str_mv |
2017-09 |
| 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/11336/112633 Alam, Shadab; Ata, Metin; Bailey, Stephen; Beutler, Florian; Bizyaev, Dmitry; et al.; The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: Cosmological analysis of the DR12 galaxy sample; Wiley Blackwell Publishing, Inc; Monthly Notices of the Royal Astronomical Society; 470; 3; 9-2017; 2617-2652 0035-8711 CONICET Digital CONICET |
| url |
http://hdl.handle.net/11336/112633 |
| identifier_str_mv |
Alam, Shadab; Ata, Metin; Bailey, Stephen; Beutler, Florian; Bizyaev, Dmitry; et al.; The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: Cosmological analysis of the DR12 galaxy sample; Wiley Blackwell Publishing, Inc; Monthly Notices of the Royal Astronomical Society; 470; 3; 9-2017; 2617-2652 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/stx721 info:eu-repo/semantics/altIdentifier/url/https://academic.oup.com/mnras/article-abstract/470/3/2617/3091741?redirectedFrom=fulltext |
| dc.rights.none.fl_str_mv |
info:eu-repo/semantics/openAccess https://creativecommons.org/licenses/by-nc-sa/2.5/ar/ |
| eu_rights_str_mv |
openAccess |
| rights_invalid_str_mv |
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/ |
| dc.format.none.fl_str_mv |
application/pdf application/pdf |
| dc.publisher.none.fl_str_mv |
Wiley Blackwell Publishing, Inc |
| publisher.none.fl_str_mv |
Wiley Blackwell Publishing, Inc |
| dc.source.none.fl_str_mv |
reponame:CONICET Digital (CONICET) instname:Consejo Nacional de Investigaciones Científicas y Técnicas |
| reponame_str |
CONICET Digital (CONICET) |
| collection |
CONICET Digital (CONICET) |
| instname_str |
Consejo Nacional de Investigaciones Científicas y Técnicas |
| repository.name.fl_str_mv |
CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicas |
| repository.mail.fl_str_mv |
dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar |
| _version_ |
1846781852262596608 |
| score |
12.982451 |