Produção Nacional
Revisado por pares
The Southern Photometric Local Universe Survey (S-PLUS): improved SEDs, morphologies, and redshifts with 12 optical filters
2019; Oxford University Press; Volume: 489; Issue: 1 Linguagem: Inglês
10.1093/mnras/stz1985
ISSN1365-2966
AutoresC. Mendes de Oliveira, T. Ribeiro, W. Schoenell, A. Kanaan, Roderik Overzier, A. Molino, L. Sampedro, P. Coelho, C. E. Barbosa, A. Cortesi, M. V. Costa-Duarte, F. R. Herpich, J. A. Hernández-Jiménez, Vinicius M. Placco, Henrique S. Xavier, L. Raul Abramo, R. K. Saito, Ana L. Chies-Santos, A. Ederoclite, R. Lopes de Oliveira, D. R. Gonçalves, S. Akras, L. A. Almeida, Felipe Almeida-Fernandes, Timothy C. Beers, C. Bonatto, Silvia Bonoli, E. S. Cypriano, E Vinicius-Lima, Rafael S. de Souza, Gabriel Fabiano De Souza, Fabrício Ferrari, Thiago S. Gonçalves, Anthony H. Gonzalez, L. A. Gutiérrez-Soto, Eduardo A. Hartmann, Yara L. Jaffé, L. O. Kerber, Círia Lima-Dias, P. A. A. Lopes, Karín Menéndez‐Delmestre, L. Nakazono, Patricia Martins de Novais, R. A. Ortega-Minakata, Eduardo S. Pereira, Hélio D. Perottoni, C. Queiroz, Ribamar R. R. Reis, W. A. Santos, T. Santos-Silva, Rafael M. Santucci, C. L. Barbosa, Beatriz B. Siffert, L. Sodré, S. Torres-Flores, P. Westera, Devin D. Whitten, J. S. Alcaniz, J. Alonso-García, S. H. P. Alencar, A. Álvarez-Candal, P. Amram, Luiz Azanha, R. H. Barbá, Pedro H. Bernardinelli, M. Borges Fernandes, V. Branco, D. Brito-Silva, Maria Luísa Buzzo, J Caffer, A. Campillay, Z. Cano, J. M. Carvano, M Castejon, R. Cid Fernandes, M. L. L. Dantas, S. Daflon, G. Damke, R. de la Reza, L J de Melo de Azevedo, Delcides Ferreira Paula, Keith Diem, Richard L. Donnerstein, O. L. Dors, Renato A. Dupke, S. S. Eikenberry, Carlos Escudero, F. R. Faifer, Humberto Farías, B. Fernandes, R. Cid Fernandes, Suely Lima Alves Fontes, Andrés Galarza, Nina S. T. Hirata, L Katena, J. Gregorio‐Hetem, J. D. Hernández-Fernández, L. Izzo, M. Jaque Arancibia, V. Jatenco‐Pereira, Y. Jiménez-Teja, Д. А. Канн, A. C. Krabbe, C Labayru, D. Lazzaro, G. B. Lima Neto, A. R. Lopes, Régis Pires Magalhães, Martı́n Makler, Raniere de Menezes, Jordi Miralda‐Escudé, Rogério Monteiro-Oliveira, Antonio D. Montero-Dorta, N Muñoz-Elgueta, Rodrigo Nemmen, J. L. Nilo Castellón, A. S. Oliveira, Daniel Ortiz, Elizabete Saburi Pattaro, C. B. Pereira, Bruno Quint, L. Riguccini, H. J. Rocha–Pinto, I. Rodrigues, F. Roig, Silvia Rossi, Kanak Saha, R. Génova-Santos, Allan Schnorr-Müller, Leandro Sesto, R. Silva, A. V. Smith Castelli, R. Teixeira, Eduardo Telles, Rodrigo Clemente Thom de Souza, C. C. Thöne, Marina Trevisan, A. de Ugarte Postigo, F. Urrutia-Viscarra, C. H. Veiga, Marina Vika, A Z Vitorelli, Ariel Werle, S V Werner, Dennis Zaritsky,
Tópico(s)Stellar, planetary, and galactic studies
ResumoThe Southern Photometric Local Universe Survey (S-PLUS) is imaging ~9300 deg^2 of the celestial sphere in twelve optical bands using a dedicated 0.8 m robotic telescope, the T80-South, at the Cerro Tololo Inter-American Observatory, Chile. The telescope is equipped with a 9.2k by 9.2k e2v detector with 10 um pixels, resulting in a field-of-view of 2 deg^2 with a plate scale of 0.55"/pixel. The survey consists of four main subfields, which include two non-contiguous fields at high Galactic latitudes (8000 deg^2 at |b| > 30 deg) and two areas of the Galactic plane and bulge (for an additional 1300 deg^2). S-PLUS uses the Javalambre 12-band magnitude system, which includes the 5 u, g, r, i, z broad-band filters and 7 narrow-band filters centered on prominent stellar spectral features: the Balmer jump/[OII], Ca H+K, H-delta, G-band, Mg b triplet, H-alpha, and the Ca triplet. S-PLUS delivers accurate photometric redshifts (delta_z/(1+z) = 0.02 or better) for galaxies with r < 20 AB mag and redshift < 0.5, 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 ~336 deg^2 of the Stripe-82 area, which is available at http://datalab.noao.edu/splus.
Referência(s)