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

التفاصيل البيبلوغرافية
العنوان: The Southern Photometric Local Universe Survey (S-PLUS): improved SEDs, morphologies, and redshifts with 12 optical filters
المؤلفون: de Oliveira, C. M., Ribeiro, T., Schoenell, W., Kanaan, A., Overzier, R. A., Molino, A., Sampedro, L., Coelho, P., Barbosa, C. E., Cortesi, A., Costa-Duarte, M. V., Montero-Dorta, A. D., Riguccini, L., Munoz-Elgueta, N., Telles, E., Vitorelli, A. Z., Hernández-Jiménez, J.A., Pinto, H. J. R., Rossi, S., Muller, A. S., Castelli, A. V. S., Beers, T. C., Thöne, Cristina Carina, Bonoli, S., Veiga, C. H., Vinicius-Lima, E., Werner, S. V., de Souza, G. F., Xavier, H. S., Gonzalez, A. H., Zaritsky, D., Jaffe, Y., Gutiérrez-Soto, L. A., Abramo, L. R., Lopes, PAA, Kerber, L. O., Saito, R. K., Novais, P. M., Menéndez-Delmestre, Karín, Chies-Santos, A.L., Queiroz, C., Pereira, E. S., Ederoclite, A., Bonatto, C., Santucci, R. M., Santos, W. A., de Oliveira, R. L., Cypriano, E. S., Westera, P., Siffert, B. B., Gonçalves, D. R., de Souza, RS, Akras, S., Alcaniz, Jailson S., Reis, R. R. R., Almeida, L. A., Ferrari, F., Almeida-Fernandes, F., Ortega-Minakata, R. A., Barbosa, C. L., Whitten, DD, Gonçalves, T. S., Hartmann, EA, Lima-Dias, C., Nakazono, L. M. I., Perottoni, H. D., Caffer, J., Santos-Silva, T., Cano, Z., Sodre, L., Castejon, M., Alonso-Garcia, J., Dantas, M. L. L., Torres-Flores, S., de la Reza, R., Alencar, S., Diem, K. G., de Azevedo, L. J. D., Alvarez-Candal, A., Dupke, Renato, Donnerstein, R., Amram, P., Faifer, F. R., Eikenberry, S., Azanha, L., Fontes, S., Fernandes, B., Barbá, R. H., Campillay, A., Gregorio-Hetem, J., Hirata, N. S. T., Bernardinelli, P. H., Carvano, J.M., Jiménez-Teja, Y., Izzo, L., Fernandes, M. B., Fernandes, R. C., Branco, V., Krabbe, A. C., Galarza, A., Brito-Silva, D., Daflon, S., Buzzo, M. L., Farias, H., Hernandez-Fernandez, J. D., Kann, D.A., Damke, G., De Paula, D. F., Dors, O. L., Escudero, C. G., Fernandes, C., Nemmen, R. S., Katena, L., Oliveira, A. S., Arancibia, M. J., Pattaro, E., Labayru, C., Quint, B., Jatenco-Pereira, V., Rodrigues, I., Lazzaro, D., Saha, K., Roig-Roig, Ferran, Neto, G. B. L., Sesto, L. A., Santos, R., Lopes, A. R., Teixeira, R., Silva, R., Magalhaes, R., Trevisan, M., de Souza, R. C. T., Makler, M., Castellon, J. L. N., Vika, M., Urrutia-Viscarra, F., de Menezes, R., Ortiz, D., Herpich, F.R., Werle, A., Miralda-Escudé, Jordi, Pereira, C. B., Monteiro-Oliveira, R., Placco, V. M., Ugarte Postigo, Antonio de
المساهمون: 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
بيانات النشر: Oxford University Press
سنة النشر: 2019
المجموعة: Digital.CSIC (Consejo Superior de Investigaciones Científicas / Spanish National Research Council)
مصطلحات موضوعية: galaxies: clusters: general, galaxies: photometry, quasars: general, stars: general, surveys
الوصف: 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 ...
نوع الوثيقة: article in journal/newspaper
اللغة: unknown
تدمد: 0035-8711
Relation: #PLACEHOLDER_PARENT_METADATA_VALUE#; info:eu-repo/grantAgreement/MINECO/Plan Estatal de Investigación Científica y Técnica y de Innovación 2013-2016/AYA2013-48623-C2-1-P; info:eu-repo/grantAgreement/MINECO/Plan Estatal de Investigación Científica y Técnica y de Innovación 2013-2016/AYA2016-81065-C2-1-P; Publisher's version; http://dx.doi.org/10.1093/mnras/stz1985; Sí; Monthly Notices of the Royal Astronomical Society 489: 241-267 (2019); http://hdl.handle.net/10261/204891; http://dx.doi.org/10.13039/100000879; http://dx.doi.org/10.13039/100009153; http://dx.doi.org/10.13039/100007921; http://dx.doi.org/10.13039/100007234; http://dx.doi.org/10.13039/100007812; http://dx.doi.org/10.13039/501100000735; http://dx.doi.org/10.13039/100008375; http://dx.doi.org/10.13039/501100005739; http://dx.doi.org/10.13039/100010220; http://dx.doi.org/10.13039/100006734; http://dx.doi.org/10.13039/100009611; http://dx.doi.org/10.13039/100000001; http://dx.doi.org/10.13039/100000104; http://dx.doi.org/10.13039/501100001700; http://dx.doi.org/10.13039/501100003329; http://dx.doi.org/10.13039/501100004189; http://dx.doi.org/10.13039/100008902; http://dx.doi.org/10.13039/100007880; http://dx.doi.org/10.13039/501100000384; http://dx.doi.org/10.13039/501100004586; http://dx.doi.org/10.13039/501100004809; http://dx.doi.org/10.13039/100006230; http://dx.doi.org/10.13039/501100000780; http://dx.doi.org/10.13039/100008211; http://dx.doi.org/10.13039/501100002322; http://dx.doi.org/10.13039/501100003593; http://dx.doi.org/10.13039/501100003339; http://dx.doi.org/10.13039/501100002367; http://dx.doi.org/10.13039/100008136; http://dx.doi.org/10.13039/100005835
DOI: 10.1093/mnras/stz1985
DOI: 10.13039/100000879
DOI: 10.13039/100009153
DOI: 10.13039/100007921
DOI: 10.13039/100007234
DOI: 10.13039/100007812
DOI: 10.13039/501100000735
DOI: 10.13039/100008375
DOI: 10.13039/501100005739
DOI: 10.13039/100010220
DOI: 10.13039/100006734
DOI: 10.13039/100009611
DOI: 10.13039/100000001
DOI: 10.13039/100000104
DOI: 10.13039/501100001700
DOI: 10.13039/501100003329
DOI: 10.13039/501100004189
DOI: 10.13039/100008902
DOI: 10.13039/100007880
DOI: 10.13039/501100000384
DOI: 10.13039/501100004586
DOI: 10.13039/501100004809
DOI: 10.13039/100006230
DOI: 10.13039/501100000780
DOI: 10.13039/100008211
DOI: 10.13039/501100002322
DOI: 10.13039/501100003593
DOI: 10.13039/501100003339
DOI: 10.13039/501100002367
DOI: 10.13039/100008136
DOI: 10.13039/100005835
الاتاحة: http://hdl.handle.net/10261/204891
https://doi.org/10.1093/mnras/stz1985
https://doi.org/10.13039/100000879
https://doi.org/10.13039/100009153
https://doi.org/10.13039/100007921
https://doi.org/10.13039/100007234
https://doi.org/10.13039/100007812
https://doi.org/10.13039/501100000735
https://doi.org/10.13039/100008375
https://doi.org/10.13039/501100005739
Rights: open
رقم الانضمام: edsbas.B90450E5
قاعدة البيانات: BASE
الوصف
تدمد:00358711
DOI:10.1093/mnras/stz1985