J-PLUS: The star formation main sequence and rate density at d  ≲  75 Mpc

Vilella-Rojo, G.; Logroño-García, R.; López-Sanjuan, Carlos; Viironen, Kerttu; Varela, Jesús; Moles, Mariano; Cenarro, A. J.; Cristóbal-Hornillos, David; Ederoclite, Alessandro; Hernández-Monteagudo, Carlos; Marín-Franch, Antonio; Vázquez Ramió, H.; Galbany, Lluís; González Delgado, Rosa M.; Hernán-Caballero, Antonio; Lumbreras-Calle, A.; Sánchez-Blázquez, P.; Sobral, D.; Vílchez Medina, José Manuel; Alcaniz, Jailson; Angulo, R.E.; Dupke, Renato A.; Sodré, L.

J-PLUS: The star formation main sequence and rate density at d ≲ 75 Mpc

Aims. Our goal is to estimate the star formation main sequence (SFMS) and the star formation rate density (SFRD) at z = 0.017 (d . 75 Mpc) using the Javalambre Photometric Local Universe Survey (J-PLUS) first data release, that probes 897.4 deg2 with twelve optical bands. Methods. We extract the Ha...

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Autores:	Vilella-Rojo, G., Logroño-García, R., López-Sanjuan, Carlos, Viironen, Kerttu, Varela, Jesús, Moles, Mariano, Cenarro, A. J., Cristóbal-Hornillos, David, Ederoclite, Alessandro, Hernández-Monteagudo, Carlos, Marín-Franch, Antonio, Vázquez Ramió, H., Galbany, Lluís, González Delgado, Rosa M., Hernán-Caballero, Antonio, Lumbreras-Calle, A., Sánchez-Blázquez, P., Sobral, D., Vílchez Medina, José Manuel, Alcaniz, Jailson, Angulo, R.E., Dupke, Renato A., Sodré, L.
Tipo de recurso:	artículo
Estado:	Versión publicada
Fecha de publicación:	2021
País:	España
Institución:	Consejo Superior de Investigaciones Científicas (CSIC)
Repositorio:	DIGITAL.CSIC. Repositorio Institucional del CSIC
OAI Identifier:	oai:digital.csic.es:10261/247359
Acceso en línea:	http://hdl.handle.net/10261/247359
Access Level:	acceso abierto
Palabra clave:	Galaxies: general Galaxies: evolution Galaxies: fundamental parameters Galaxies: star formation Galaxies: luminosity function Mass function

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network_acronym_str	ES
network_name_str	España
repository_id_str
dc.title.none.fl_str_mv	J-PLUS: The star formation main sequence and rate density at d ≲ 75 Mpc
title	J-PLUS: The star formation main sequence and rate density at d ≲ 75 Mpc
spellingShingle	J-PLUS: The star formation main sequence and rate density at d ≲ 75 Mpc Vilella-Rojo, G. Galaxies: general Galaxies: evolution Galaxies: fundamental parameters Galaxies: star formation Galaxies: luminosity function Mass function
title_short	J-PLUS: The star formation main sequence and rate density at d ≲ 75 Mpc
title_full	J-PLUS: The star formation main sequence and rate density at d ≲ 75 Mpc
title_fullStr	J-PLUS: The star formation main sequence and rate density at d ≲ 75 Mpc
title_full_unstemmed	J-PLUS: The star formation main sequence and rate density at d ≲ 75 Mpc
title_sort	J-PLUS: The star formation main sequence and rate density at d ≲ 75 Mpc
dc.creator.none.fl_str_mv	Vilella-Rojo, G. Logroño-García, R. López-Sanjuan, Carlos Viironen, Kerttu Varela, Jesús Moles, Mariano Cenarro, A. J. Cristóbal-Hornillos, David Ederoclite, Alessandro Hernández-Monteagudo, Carlos Marín-Franch, Antonio Vázquez Ramió, H. Galbany, Lluís González Delgado, Rosa M. Hernán-Caballero, Antonio Lumbreras-Calle, A. Sánchez-Blázquez, P. Sobral, D. Vílchez Medina, José Manuel Alcaniz, Jailson Angulo, R.E. Dupke, Renato A. Sodré, L.
author	Vilella-Rojo, G.
author_facet	Vilella-Rojo, G. Logroño-García, R. López-Sanjuan, Carlos Viironen, Kerttu Varela, Jesús Moles, Mariano Cenarro, A. J. Cristóbal-Hornillos, David Ederoclite, Alessandro Hernández-Monteagudo, Carlos Marín-Franch, Antonio Vázquez Ramió, H. Galbany, Lluís González Delgado, Rosa M. Hernán-Caballero, Antonio Lumbreras-Calle, A. Sánchez-Blázquez, P. Sobral, D. Vílchez Medina, José Manuel Alcaniz, Jailson Angulo, R.E. Dupke, Renato A. Sodré, L.
author_role	author
author2	Logroño-García, R. López-Sanjuan, Carlos Viironen, Kerttu Varela, Jesús Moles, Mariano Cenarro, A. J. Cristóbal-Hornillos, David Ederoclite, Alessandro Hernández-Monteagudo, Carlos Marín-Franch, Antonio Vázquez Ramió, H. Galbany, Lluís González Delgado, Rosa M. Hernán-Caballero, Antonio Lumbreras-Calle, A. Sánchez-Blázquez, P. Sobral, D. Vílchez Medina, José Manuel Alcaniz, Jailson Angulo, R.E. Dupke, Renato A. Sodré, L.
author2_role	author author author author author author author author author author author author author author author author author author author author author author
dc.contributor.none.fl_str_mv	European Commission Ministerio de Ciencia, Innovación y Universidades (España) Ministerio de Economía y Competitividad (España) Fondo de Inversiones de Teruel Conselho Nacional de Desenvolvimento Científico e Tecnológico (Brasil) Financiadora de Estudos e Projetos (Brasil) Consejo Superior de Investigaciones Científicas [https://ror.org/02gfc7t72]
dc.subject.none.fl_str_mv	Galaxies: general Galaxies: evolution Galaxies: fundamental parameters Galaxies: star formation Galaxies: luminosity function Mass function
topic	Galaxies: general Galaxies: evolution Galaxies: fundamental parameters Galaxies: star formation Galaxies: luminosity function Mass function
description	Aims. Our goal is to estimate the star formation main sequence (SFMS) and the star formation rate density (SFRD) at z = 0.017 (d . 75 Mpc) using the Javalambre Photometric Local Universe Survey (J-PLUS) first data release, that probes 897.4 deg2 with twelve optical bands. Methods. We extract the Ha emission flux of 805 local galaxies from the J-PLUS filter J0660, being the continuum level estimated with the other eleven J-PLUS bands, and the dust attenuation and nitrogen contamination corrected with empirical relations. Stellar masses (M), Ha luminosities (LHa), and star formation rates (SFRs) were estimated by accounting for parameters covariances. Our sample comprises 689 blue galaxies and 67 red galaxies, classified in the (u - g) vs. (g - z) color–color diagram, plus 49 AGN. Results. The SFMS is explored at log M 8 and it is clearly defined by the blue galaxies, with the red galaxies located below them. The SFMS is described as log SFR = 0.83 log M -8.44. We find a good agreement with previous estimations of the SFMS, especially those based on integral field spectroscopy. The Ha luminosity function of the AGN-free sample is well described by a Schechter function with log L * Ha = 41.34, log f * = -2.43, and a = -1.25. Our measurements provide a lower characteristic luminosity than several previous studies in the literature. Conclusions. The derived star formation rate density at d . 75 Mpc is log SFR = -2.10 ± 0.11, with red galaxies accounting for 15% of the SFRD. Our value is lower than previous estimations at similar redshift, and provides a local reference for evolutionary studies regarding the star formation history of the Universe © 2021 EDP Sciences. All rights reserved.
publishDate	2021
dc.date.none.fl_str_mv	2021 2021 2021
dc.type.none.fl_str_mv	info:eu-repo/semantics/article http://purl.org/coar/resource_type/c_6501 Publisher's version info:eu-repo/semantics/publishedVersion
format	article
status_str	publishedVersion
dc.identifier.none.fl_str_mv	http://hdl.handle.net/10261/247359
url	http://hdl.handle.net/10261/247359
dc.language.none.fl_str_mv	Inglés
language_invalid_str_mv	Inglés
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dc.rights.none.fl_str_mv	info:eu-repo/semantics/openAccess
eu_rights_str_mv	openAccess
dc.publisher.none.fl_str_mv	EDP Sciences
publisher.none.fl_str_mv	EDP Sciences
dc.source.none.fl_str_mv	reponame:DIGITAL.CSIC. Repositorio Institucional del CSIC instname:Consejo Superior de Investigaciones Científicas (CSIC)
instname_str	Consejo Superior de Investigaciones Científicas (CSIC)
reponame_str	DIGITAL.CSIC. Repositorio Institucional del CSIC
collection	DIGITAL.CSIC. Repositorio Institucional del CSIC
repository.name.fl_str_mv
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spelling	J-PLUS: The star formation main sequence and rate density at d ≲ 75 MpcVilella-Rojo, G.Logroño-García, R.López-Sanjuan, CarlosViironen, KerttuVarela, JesúsMoles, MarianoCenarro, A. J.Cristóbal-Hornillos, DavidEderoclite, AlessandroHernández-Monteagudo, CarlosMarín-Franch, AntonioVázquez Ramió, H.Galbany, LluísGonzález Delgado, Rosa M.Hernán-Caballero, AntonioLumbreras-Calle, A.Sánchez-Blázquez, P.Sobral, D.Vílchez Medina, José ManuelAlcaniz, JailsonAngulo, R.E.Dupke, Renato A.Sodré, L.Galaxies: generalGalaxies: evolutionGalaxies: fundamental parametersGalaxies: star formationGalaxies: luminosity functionMass functionAims. Our goal is to estimate the star formation main sequence (SFMS) and the star formation rate density (SFRD) at z = 0.017 (d . 75 Mpc) using the Javalambre Photometric Local Universe Survey (J-PLUS) first data release, that probes 897.4 deg2 with twelve optical bands. Methods. We extract the Ha emission flux of 805 local galaxies from the J-PLUS filter J0660, being the continuum level estimated with the other eleven J-PLUS bands, and the dust attenuation and nitrogen contamination corrected with empirical relations. Stellar masses (M), Ha luminosities (LHa), and star formation rates (SFRs) were estimated by accounting for parameters covariances. Our sample comprises 689 blue galaxies and 67 red galaxies, classified in the (u - g) vs. (g - z) color–color diagram, plus 49 AGN. Results. The SFMS is explored at log M 8 and it is clearly defined by the blue galaxies, with the red galaxies located below them. The SFMS is described as log SFR = 0.83 log M -8.44. We find a good agreement with previous estimations of the SFMS, especially those based on integral field spectroscopy. The Ha luminosity function of the AGN-free sample is well described by a Schechter function with log L * Ha = 41.34, log f * = -2.43, and a = -1.25. Our measurements provide a lower characteristic luminosity than several previous studies in the literature. Conclusions. The derived star formation rate density at d . 75 Mpc is log SFR = -2.10 ± 0.11, with red galaxies accounting for 15% of the SFRD. Our value is lower than previous estimations at similar redshift, and provides a local reference for evolutionary studies regarding the star formation history of the Universe © 2021 EDP Sciences. All rights reserved.Based on observations made with the JAST/T80 telescope for J-PLUS project at the Observatorio Astrofísico de Javalambre in Teruel, a Spanish Infraestructura Cientifico-Técnica Singular (ICTS) owned, managed and operated by the Centro de Estudios de Física del Cosmos de Aragón (CEFCA). Data has been processed and provided by CEFCA’s Unit of Processing and Archiving Data (UPAD). Funding for the J-PLUS Project has been provided by the Governments of Spain and Aragón through the Fondo de Inversiones de Teruel; the Aragón Government through the Research Groups E96, E103, and E16_17R; the Spanish Ministry of Science, Innovation and Universities (MCIU/AEI/FEDER, UE) with grants PGC2018-097585-B-C21 and PGC2018-097585-B-C22; the Spanish Ministry of Economy and Competitiveness (MINECO) under AYA2015-66211-C2-1-P, AYA2015-66211-C2-2, AYA2012-30789, and ICTS-2009-14; and European FEDER funding (FCDD10- 4E-867, FCDD13-4E-2685). The Brazilian agencies FINEP, FAPESP, and the National Observatory of Brazil have also contributed to this project. J.M.V. acknowledges financial support from the State Agency for Research of the Spanish MCIU through the “Center of Excellence Severo Ochoa” award to the Instituto de Astrofísica de Andalucía (SEV 2017-0709), and grant AYA2016-79724-C4-4P. R.A.D. acknowledges support from the Conselho Nacional de Desenvolvimento Científico e Tecnolágico –CNPq through BP grant 308105/2018-4, and the Financiadora de Estudos e Projetos – FINEP grants REF. 1217/13 – 01.13.0279.00 and REF 0859/10 – 01.10.0663.00 for hardware support for the J-PLUS project through the National Observatory of Brazil. We thank the help of Prof. G. Gavazzi in the analysis and understanding of Hα3 data. This research has made use of the NASA/IPAC Extragalactic Database (NED), which is operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration. This research made use of Astropy, a community-developed core Python package for Astron omy (Astropy Collaboration 2013), and Matplotlib, a 2D graphics package used for Python for publication-quality image generation across user interfaces and operating systems (Hunter 2007). Some of the data sets discussed in the manuscript were recovered with WebPlotDigitizer (https://automeris.io/WebPlotDigitizer/index.html), a free software developed to facilitate easy and accurate data extraction from a variety of plot types.Peer reviewedEDP SciencesEuropean CommissionMinisterio de Ciencia, Innovación y Universidades (España)Ministerio de Economía y Competitividad (España)Fondo de Inversiones de TeruelConselho Nacional de Desenvolvimento Científico e Tecnológico (Brasil)Financiadora de Estudos e Projetos (Brasil)Consejo Superior de Investigaciones Científicas [https://ror.org/02gfc7t72]202120212021info:eu-repo/semantics/articlehttp://purl.org/coar/resource_type/c_6501Publisher's versioninfo:eu-repo/semantics/publishedVersionhttp://hdl.handle.net/10261/247359reponame:DIGITAL.CSIC. 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J-PLUS: The star formation main sequence and rate density at d ≲ 75 Mpc

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