The Southern Photometric Local Universe Survey (S-PLUS): improved SEDs, morphologies, and redshifts with 12 optical filters

Autor:	Nina S. T. Hirata, Alexandre S. Oliveira, Fernando Roig, J. Caffer, Zach Cano, Denise R. Gonçalves, Daniela Lazzaro, Carlos A. Fernandes, E. Pattaro, C. H. Veiga, F. Urrutia-Viscarra, P. Amram, Silvia Rossi, J. D. Hernández-Fernández, Ramachrisna Teixeira, M. Castejon, A. Schnorr Müller, R. Magalhães, C. Labayru, Lilianne Mariko Izuti Nakazono, R. Cid Fernandes, Jordi Miralda-Escudé, D. F. De Paula, Vinicius M. Placco, G. B. Lima Neto, Eduardo S. Pereira, H. J. Rocha Pinto, O. L. Dors, M. Jaque Arancibia, Pedro H. Bernardinelli, S. S. Eikenberry, Stavros Akras, C. Lima-Dias, Rodolfo H. Barbá, V. Branco, Karín Menéndez-Delmestre, Thiago S. Gonçalves, R. Silva, Yara L. Jaffé, Alvaro Alvarez-Candal, R. Monteiro-Oliveira, Pieter Westera, Ana L. Chies-Santos, Anthony H. Gonzalez, Leandro Alberto Sesto, William Schoenell, Eduardo S. Cypriano, T. Ribeiro, Roberto K. Saito, Kanak Saha, Angela Krabbe, Devin D. Whitten, D. Brito-Silva, E. A. Hartmann, A. Campillay, L. Sampedro, C. L. Barbosa, G. Damke, S. Bonoli, J. A. Hernandez-Jimenez, L. J. de Melo de Azevedo, Richard L. Donnerstein, Irapuan Rodrigues, C. Queiroz, F. Almeida-Fernandes, Beatriz Luci Fernandes, Antonio Kanaan, Paula Coelho, Christina C. Thöne, Leandro Kerber, Javier Alonso-García, H. Farías, Analia Viviana Smith Castelli, Ribamar R. R. Reis, Fabricio Ferrari, M. Vika, Martin Makler, Simone Daflon, Arianna Cortesi, Roderik Overzier, Bruno Quint, F. R. Faifer, S. Fontes, Dennis Zaritsky, A. Z. Vitorelli, D. Ortíz, Rafael M. Santucci, C. Mendes de Oliveira, L. Katena, R. S. de Souza, V. Jatenco-Pereira, Luca Izzo, H. S. Xavier, M. V. Costa-Duarte, H. D. Perottoni, Marina Trevisan, W. A. Santos, L. Sodré, Timothy C. Beers, R. A. Ortega-Minakata, R. Lopes de Oliveira, K. G. Diem, David Alexander Kann, Amanda R. Lopes, Carlos Gabriel Escudero, M. L. L. Dantas, R. C. Thom de Souza, A. Galarza, Jane Gregorio-Hetem, N. Muñoz-Elgueta, S. Alencar, G. Fabiano de Souza, Eduardo Telles, R. S. Nemmen, Teresa Santos-Silva, J. M. Carvano, C. B. Pereira, F. R. Herpich, S. V. Werner, C. E. Barbosa, Beatriz B. Siffert, Y. Jimenez-Teja, E. Vinicius-Lima, R. de la Reza, Paulo A. A. Lopes, Alessandro Ederoclite, Antonio D. Montero-Dorta, S. Torres-Flores, Luis Raul Weber Abramo, A. Werle, M. L. Buzzo, P. M. Novais, J. S. Alcaniz, C. Bonatto, M. Borges Fernandes, L. Azanha, L. A. Gutiérrez-Soto, A. de Ugarte Postigo, Leonardo A. Almeida, J. L. Nilo Castellón, R. de Menezes, Reginaldo Bezerra dos Santos, R. A. Dupke, Alberto Molino, L. Riguccini
Přispěvatelé:	Universidad de La Serena (Chile), Centro de Estudios de Física del Cosmos de Aragón, Conselho Nacional de Desenvolvimento Científico e Tecnológico (Brasil), Coordenação de Aperfeiçoamento de Pessoal de Nível Superior (Brasil), Fundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de Janeiro, Financiadora de Estudos e Projetos (Brasil), National Science Foundation (US), Southern Office of Aerospace Research and Development (US), Consejo Superior de Investigaciones Científicas (España), Ministerio de Economía y Competitividad (España), European Commission, Universidad Nacional Autónoma de México, Alfred P. Sloan Foundation, National Aeronautics and Space Administration (US), Ministry of Education, Culture, Sports, Science and Technology (Japan), Max Planck Society, Higher Education Funding Council for England, American Museum of Natural History, Leibniz Institute for Astrophysics Potsdam, University of Basel, University of Cambridge, Case Western Reserve University, University of Chicago, Drexel University (US), Joint Institute for Nuclear Astrophysics - Center for the Evolution of the Elements (US), Kavli Institute for Particle Astrophysics and Cosmology, Chinese Academy of Sciences, Los Alamos National Laboratory, Max Planck Institute for Astronomy, Max Planck Institute for Astrophysics, New Mexico State University, The Ohio State University, University of Pittsburgh, University of Portsmouth, Princeton University, U.S. Naval Observatory, University of Washington, Fermilab, Institute for Advanced Study (Germany), Johns Hopkins University, Institut de Planétologie et d'Astrophysique de Grenoble (IPAG), Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Observatoire des Sciences de l'Univers de Grenoble (OSUG ), Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut national des sciences de l'Univers (INSU - CNRS)-Institut national de recherche en sciences et technologies pour l'environnement et l'agriculture (IRSTEA)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes [2016-2019] (UGA [2016-2019])-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut national de recherche en sciences et technologies pour l'environnement et l'agriculture (IRSTEA)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes [2016-2019] (UGA [2016-2019]), Laboratoire d'Astrophysique de Marseille (LAM), Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)
Rok vydání:	2019
Předmět:	Ciencias Astronómicas Cosmology and Nongalactic Astrophysics (astro-ph.CO) media_common.quotation_subject purl.org/becyt/ford/1.7 [https] FOS: Physical sciences Astrophysics::Cosmology and Extragalactic Astrophysics Astrophysics Surveys clusters: general [Galaxies] purl.org/becyt/ford/1 [https] PROCESSAMENTO DE IMAGENS clusters Optical filter Instrumentation and Methods for Astrophysics (astro-ph.IM) Astrophysics::Galaxy Astrophysics Solar and Stellar Astrophysics (astro-ph.SR) media_common Physics High Energy Astrophysical Phenomena (astro-ph.HE) [SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph] general [Stars] photometry [Galaxies] Astrophysics::Instrumentation and Methods for Astrophysics Astronomy and Astrophysics general [Quasars] Galaxies: photometry general – galaxies Astrophysics - Astrophysics of Galaxies Redshift Universe photometry – quasars Quasars: general Astrophysics - Solar and Stellar Astrophysics [SDU]Sciences of the Universe [physics] Space and Planetary Science Stars: general general Astrophysics of Galaxies (astro-ph.GA) surveys – stars Galaxies: clusters: general Astrophysics - High Energy Astrophysical Phenomena Astrophysics - Instrumentation and Methods for Astrophysics Astrophysics - Cosmology and Nongalactic Astrophysics
Zdroj:	Biblioteca Digital de Teses e Dissertações da FEI Centro Universitário da Fundação Educacional Inaciana (FEI) instacron:FEI SEDICI (UNLP) Universidad Nacional de La Plata instacron:UNLP Digital.CSIC. Repositorio Institucional del CSIC instname Monthly Notices of the Royal Astronomical Society Monthly Notices of the Royal Astronomical Society, 2019, 489, pp.241-267. ⟨10.1093/mnras/stz1985⟩ Repositório Institucional da USP (Biblioteca Digital da Produção Intelectual) Universidade de São Paulo (USP) instacron:USP CONICET Digital (CONICET) Consejo Nacional de Investigaciones Científicas y Técnicas instacron:CONICET
ISSN:	0035-8711 1365-2966
Popis:	The Southern Photometric Local Universe Survey (S-PLUS) is imaging similar to 9300 deg(2) of the celestial sphere in 12 optical bands using a dedicated 0.8mrobotic telescope, the T80-South, at the Cerro Tololo Inter-american Observatory, Chile. The telescope is equipped with a 9.2k x 9.2k e2v detector with 10 mu m pixels, resulting in a field of view of 2 deg(2) with a plate scale of 0.55 arcsec pixel-1. The survey consists of four main subfields, which include two non-contiguous fields at high Galactic latitudes (vertical bar b vertical bar > 30 degrees, 8000 deg(2)) and two areas of the Galactic Disc and Bulge (for an additional 1300 deg(2)). S-PLUS uses the Javalambre 12-band magnitude system, which includes the 5 ugriz broad-band filters and 7 narrow-band filters centred on prominent stellar spectral features: the Balmer jump/[OII], Ca H + K, Hd, G band, Mg b triplet, H alpha, and the Ca triplet. S-PLUS delivers accurate photometric redshifts (dz /(1 + z) = 0.02 or better) for galaxies with r < 19.7 AB mag and z < 0.4, thus producing a 3D map of the local Universe over a volume of more than 1 (Gpc/h)(3). The final S-PLUS catalogue will also enable the study of star formation and stellar populations in and around the Milky Way and nearby galaxies, as well as searches for quasars, variable sources, and low-metallicity stars. In this paper we introduce the main characteristics of the survey, illustrated with science verification data highlighting the unique capabilities of S-PLUS. We also present the first public data release of similar to 336 deg(2) of the Stripe 82 area, in 12 bands, to a limiting magnitude of r = 21, available at datalab.noao.edu/splus.© 2019 The Author(s).Published by Oxford University Press on behalf of the Royal Astronomical Society The S-PLUS project, including the T80S robotic telescope and the S-PLUS scientific survey, was founded as a partnership between the Fundacao de Amparo a Pesquisa do Estado de Sao Paulo (FAPESP), the Observatorio Nacional (ON), the Federal University of Sergipe (UFS), and the Federal University of Santa Catarina (UFSC), with important financial and practical contributions from other collaborating institutes in Brazil, Chile (Universidad de La Serena), and Spain (Centro de Estudios de Fisica del Cosmos de Aragon, CEFCA). The members of the collaboration are grateful for the support received from the Conselho Nacional de Desenvolvimento Cientifico e Tecnologico (CNPq; grants 312333/2014-5, 306968/2014-2, 142436/2014-3, 459553/2014-3, 400738/2014-7, 302037/2015-2, 312307/2015-2, 300336/2016-0, 304184/2016-0, 304971/2016-2, 401669/2016-5, 308968/2016-6, 309456/2016-9, 421687/2016-9, 150237/2017-0, 311331/2017-3, 304819/2017-4, and 200289/2017-9), FAPESP (grants 2009/54202-8, 2011/51680-6, 2014/07684-5, 2014/11806-9, 2014/13723-3, 2014/18632-6, 2016/17119-9, 2016/12331-0, 2016/21532-9, 2016/21664-2, 2016/23567-4, 2017/01461-2, 2017/23766-0, 2018/02444-7, and 2018/21661-9), the Coordenacao de Aperfeicoamento de Pessoal de Nivel Superior (CAPES; grants 88881.030413/2013-01 and 88881.156185/2017-01), the Fundacao de Amparo a Pesquisa do Estado do Rio de Janeiro (FAPERJ; grants 202.876/2015, 202.835/2016, and 203.186/2016), the Financiadora de Estudos e Projetos (FINEP; grants 1217/13-01.13.0279.00 and 0859/10-01.10.0663.00), the Direccion de Investigacion y Desarrollo de la Universidad de La Serena (DIDULS/ULS; projects PR16143 and PTE16146 and the Programa de Investigadores Asociados), and the Direccion de Postgrado y Postitulo. TCB, VMP, and DDW acknowledge the support from the Physics Frontier Center for the Evolution of the Elements (JINA-CEE) through the US National Science Foundation (grant PHY 14-30152). JLNC is grateful for financial support received from the Southern Office of Aerospace Research and development (SOARD; grants FA9550-15-1-0167 and FA9550-18-1-0018) of the Air Force Office of the Scientific Research International Office of the United States (AFOSR/IO). YJT and RAD acknowledge support from the Spanish National Research Council (CSIC) I-COOP + 2016 program (grant COOPB20263), and the Spanish Ministry of Economy, Industry, and Competitiveness (MINECO; grants AYA2013-48623-C2-1-P and AYA2016-81065-C2-1-P). RAOM acknowledges support from the Direccion General de Asuntos del Personal Academico of the Universidad Nacional Autonoma de Mexico (DGAPA-UNAM) through a post-doctoral fellowship from the Programa de Becas Posdoctorales en la UNAM. This work has made use of data from the Sloan Digital Sky Survey. Funding for the SDSS and SDSS-II has been provided by the Alfred P. Sloan Foundation, the Participating Institutions, the National Science Foundation, the U.S. Department of Enenergy, the National Aeronautics and Space Administration, the Japanese Monbukagakusho, the Max Planck Society, and the Higher Education Funding Council for England. The SDSS Web Site is http://www.sdss.org/.The SDSS is managed by the Astrophysical Research Consortium for the Participating Institutions. The Participating Institutions are the American Museum of Natural History, Astrophysical Institute Potsdam, University of Basel, University of Cambridge, Case Western Reserve University, University of Chicago, Drexel University, Fermilab, the Institute for Advanced Study, the Japan Participation Group, Johns Hopkins University, the Joint Institute for Nuclear Astrophysics, the Kavli Institute for Particle Astrophysics and Cosmology, the Korean Scientist Group, the Chinese Academy of Sciences (LAMOST), Los Alamos National Laboratory, the Max-Planck-Institute for Astronomy (MPIA), the Max-Planck-Institute for Astrophysics (MPA), the New Mexico State University, Ohio State University, University of Pittsburgh, University of Portsmouth, Princeton University, the United States Naval Observatory, and the University of Washington. This publication makes use of data products from the Widefield Infrared Survey Explorer, which is a joint project of the University of California, Los Angeles, and the Jet Propulsion Laboratory/California Institute of Technology, funded by the National Aeronautics and Space Administration. We are grateful for the contributions of CTIO staff in helping in the construction, commissioning, and maintenance of the telescope and camera and we are particularly thankful to the CTIO director, Steve Heathcote, for his support at every phase, without which this project would not have been completed. We thank Cesar Iniguez for making the 2D measurements of the filter transmissions at CEFCA. We warmly thank David Cristobal-Hornillos and his group for helping us to install and run the reduction package JYPE version 0.9.9 in the S-PLUS computer system in Chile. We warmly thank Mariano Moles, Javier Cenarro, Tamara Civera, Sergio Chueca, Javier Hernandez Fuertes, Antonio Marin Franch, Jesus Varella, and Hector Vazquez Ramio -the success of the S-PLUS project relies on the dedication of these and other CEFCA staff members in building OAJ and running J-PLUS and J-PAS. We deeply thank Rene Laporte and INPE, as well as Keith Taylor, for their contributions to the T80S camera.
Databáze:	OpenAIRE
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