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(Referência obtida automaticamente do Web of Science, por meio da informação sobre o financiamento pela FAPESP e o número do processo correspondente, incluída na publicação pelos autores.)

The miniJPAS survey: A preview of the Universe in 56 colors

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Autor(es):
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Bonoli, S. [1, 2, 3] ; Marin-Franch, A. [4] ; Varela, J. [4] ; Vazquez Ramio, H. [4] ; Abramo, L. R. [5] ; Cenarro, A. J. [4] ; Dupke, R. A. [6, 7, 8] ; Vilchez, J. M. [9] ; Cristobal-Hornillos, D. [3] ; Gonzalez Delgado, R. M. [9] ; Hernandez-Monteagudo, C. [4] ; Lopez-Sanjuan, C. [4] ; Muniesa, D. J. [3] ; Civera, T. [3] ; Ederoclite, A. [10] ; Hernan-Caballero, A. [3] ; Marra, V [11, 12] ; Baqui, P. O. [11, 12] ; Cortesi, A. [13] ; Cypriano, E. S. [10] ; Daflon, S. [8] ; de Amorim, A. L. [14] ; Diaz-Garcia, L. A. [15] ; Diego, J. M. [16] ; Martinez-Solaeche, G. [9] ; Perez, E. [9] ; Placco, V. M. [17, 18] ; Prada, F. [9] ; Queiroz, C. [5] ; Alcaniz, J. [19, 8] ; Alvarez-Candal, A. [8, 20, 21] ; Cepa, J. [22, 23] ; Maroto, A. L. [24] ; Roig, F. [8] ; Siffert, B. B. [25] ; Taylor, K. [26] ; Benitez, N. [9] ; Moles, M. [3, 9] ; Sodre Jr, L. ; Carneiro, S. [27] ; de Oliveira, C. Mendes [28] ; Abdalla, E. [5] ; Angulo, R. E. [1, 2] ; Aparicio Resco, M. [24] ; Balaguera-Antolinez, A. [22, 23] ; Ballesteros, F. J. [29] ; Brito-Silva, D. [28] ; Broadhurst, T. [1, 2, 30] ; Carrasco, E. R. [31] ; Castro, T. [32, 33, 34, 35] ; Fernandes, R. Cid [14] ; Coelho, P. [28] ; de Melo, R. B. [7, 8] ; Doubrawa, L. [28] ; Fernandez-Soto, A. [36, 16] ; Ferrari, F. [37] ; Finoguenov, A. [38] ; Garcia-Benito, R. [9] ; Iglesias-Paramo, J. [9] ; Jimenez-Teja, Y. [9] ; Kitaura, F. S. [22, 23] ; Laur, J. [39] ; Lopes, P. A. A. [13] ; Lucatelli, G. [37] ; Martinez, V. J. [36, 29, 40] ; Maturi, M. [41, 42] ; Quartin, M. [43, 13] ; Pigozzo, C. [27] ; Rodriguez-Martin, J. E. [9] ; Salzano, V [44] ; Tamm, A. [39] ; Tempel, E. [39] ; Umetsu, K. [15] ; Valdivielso, L. [3] ; von Marttens, R. [8] ; Zitrin, A. [45] ; Diaz-Martin, M. C. [3] ; Lopez-Alegre, G. [3] ; Lopez-Sainz, A. [3] ; Yanes-Diaz, A. [3] ; Rueda-Teruel, F. [3] ; Rueda-Teruel, S. [3] ; Abril Ibanez, J. [46, 3] ; Anton Bravo, J. L. [3] ; Bello Ferrer, R. [3] ; Bielsa, S. [3] ; Casino, J. M. [3] ; Castillo, J. [3] ; Chueca, S. [3] ; Cuesta, L. [3] ; Garzaran Calderaro, J. [3] ; Iglesias-Marzoa, R. [3] ; Iniguez, C. [3] ; Lamadrid Gutierrez, J. L. [3] ; Lopez-Martinez, F. [3] ; Lozano-Perez, D. [3] ; Maicas Sacristan, N. [3] ; Molina-Ibanez, E. L. [3] ; Moreno-Signes, A. [3] ; Llano, S. Rodriguez [3] ; Royo Navarro, M. [3] ; Tilve Rua, V [3] ; Andrade, U. [8] ; Alfaro, E. J. [9] ; Akras, S. [37] ; Arnalte-Mur, P. [29, 40] ; Ascaso, B. [47] ; Barbosa, C. E. [28] ; Beltran Jimenez, J. [48] ; Benetti, M. [49, 50] ; Bengaly, C. A. P. [8] ; Bernui, A. [8] ; Blanco-Pillado, J. J. [1, 30] ; Borges Fernandes, M. [8] ; Bregman, J. N. [6] ; Bruzual, G. [51] ; Calderone, G. [33] ; Carvano, J. M. [8] ; Casarini, L. [52] ; Chies-Santos, A. L. [19] ; de Carvalho, G. Coutinho [53] ; Dimauro, P. [8] ; Duarte Puertas, S. [9] ; Figueruelo, D. [48] ; Gonzalez-Serrano, I, J. ; Guerrero, M. A. [9] ; Gurung-Lopez, S. [54, 3] ; Herranz, D. [55] ; Huertas-Company, M. [22, 56, 23, 57] ; Irwin, J. A. [7] ; Izquierdo-Villalba, D. [3] ; Kanaan, A. [14] ; Kehrig, C. [9] ; Kirkpatrick, C. C. [38] ; Lim, J. [58] ; Lopes, A. R. [8] ; de Oliveira, R. Lopes [52, 8] ; Marcos-Caballero, A. [30] ; Martinez-Delgado, D. [9] ; Martinez-Gonzalez, E. [55] ; Martinez-Somonte, G. [59, 55, 60] ; Oliveira, N. [8] ; Orsi, A. A. [3] ; Overzier, R. A. [8] ; Penna-Lima, M. [61] ; Reis, R. R. R. [43, 13] ; Spinoso, D. [3] ; Tsujikawa, S. [62] ; Vielva, P. [55] ; Vitorelli, A. Z. [28] ; Xia, J. Q. [63] ; Yuan, H. B. [63] ; Arroyo-Polonio, A. [9] ; Dantas, M. L. L. [28] ; Galarza, C. A. [8] ; Goncalves, D. R. [13] ; Goncalves, R. S. [8] ; Gonzalez, J. E. [19, 8] ; Gonzalez, A. H. [64] ; Greisel, N. [3] ; Landim, R. G. [65] ; Lazzaro, D. [8] ; Magris, G. [66] ; Monteiro-Oliveira, R. [28] ; Pereira, C. B. [8] ; Reboucas, M. J. [67] ; Rodriguez-Espinosa, J. M. [23] ; da Costa, S. Santos [8] ; Telles, E. [8]
Número total de Autores: 169
Afiliação do(s) autor(es):
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[1] Basque Fdn Sci, Ikerbasque, Bilbao 48013 - Spain
[2] Donostia Int Phys Ctr DIPC, Manuel Lardizabal Ibilbidea 4, San Sebastian - Spain
[3] Ctr Estudios Fis Cosmos Aragon CEFCA, Plaza San Juan 1, Teruel 44001 - Spain
[4] CSIC, Unidad Asociada, Ctr Estudios Fis Cosmos Aragon CEFCA, Plaza San Juan 1, Teruel 44001 - Spain
[5] Univ Sao Paulo, Inst Fis, Rua Matao 1371, BR-05508090 Sao Paulo - Brazil
[6] Univ Alabama, Dept Phys & Astron, Box 870324, Tuscaloosa, AL 35487 - USA
[7] Univ Brasilia, Inst Fis, Caixa Postal 04455, BR-70919970 Brasilia, DF - Brazil
[8] Minist Ciencia Tecnol Inovacao & Comunicacoes, Observ Nacl, Rua Gen Jose Cristino 77, BR-20921400 Rio De Janeiro - Brazil
[9] CSIC, Inst Astrofis Andalucia, Apdo 3004, Granada 18080 - Spain
[10] Univ Sao Paulo, Inst Astron, Inst Astron Geofis & Ciencias Atmosfer, Sao Paulo - Brazil
[11] Univ Fed Espirito Santo, Dept Fis, BR-29075910 Vitoria, ES - Brazil
[12] Univ Fed Espirito Santo, PPGCosmo, Nucleo Astrofis & Cosmol, BR-29075910 Vitoria, ES - Brazil
[13] Beijing Normal Univ, Dept Astron, Beijing 100875 - Peoples R China
[14] Univ Trieste, Sez Astron, Dipartimento Fis, Via Tiepolo 11, I-34143 Trieste - Italy
[15] Acad Sinica, Inst Astron & Astrophys ASIAA, AS NTU, 11F Astron Math Bldg, 1, Section4, Roosevelt Rd, Taipei 10617 - Taiwan
[16] Inst Fis Cantabria CSIC UC, Avda Los Castros S-N, Santander 39005 - Spain
[17] NSFs NOIRLab, Community Sci & Data Ctr, 950 N Cherry Ave, Tucson, AZ 85719 - USA
[18] Univ Fed Rio de Janeiro, Inst Fis, BR-21941972 Rio De Janeiro 21941972, RJ - Brazil
[19] Univ Fed Rio Grande do Norte, Dept Fis Teor & Expt, BR-59072970 Natal, RN - Brazil
[20] Univ Complutense Madrid, Dept Fis Teor, IPARCOS, Madrid 28040 - Spain
[21] Univ Complutense Madrid, IPARCOS, Inst Fis Particulas & Cosmos, Madrid 28040 - Spain
[22] Inst Astrofis Canarias, Tenerife 38200 - Spain
[23] UPMC Univ Paris 06, Sorbonne Univ, CNRS, LERMA, Observ Paris, PSL Res Univ, F-75014 Paris - France
[24] Univ Fed Santa Catarina, Dept Fis, CFM, Florianpolis, SC - Brazil
[25] Univ Fed Rio de Janeiro, Campus Duque de Caxias, BR-25265970 Duque De Caxias, RJ - Brazil
[26] Heidelberg Univ, Zentrum Astron, Philosophenweg 12, D-69120 Heidelberg - Germany
[27] Univ Fed Bahia, Inst Fis, BR-40210340 Salvador, BA - Brazil
[28] Sodre Jr, Jr., L., Univ Sao Paulo, Inst Astron, Inst Astron Geofis & Ciencias Atmosfer, Sao Paulo - Brazil
[29] Univ Valencia, Dept Astron & Astrofis, Burjassot 46100 - Spain
[30] Univ La Laguna, Dept Astrofis, Tenerife 38206 - Spain
[31] Univ Estado Rio de Janeiro, Dept Fis Matemat & Comp, BR-27537000 Resende, RJ - Brazil
[32] INAF Osservatorio Astron Trieste, Via Tiepolo 11, I-34131 Trieste - Italy
[33] IFPU Inst Fundamental Phys Universe, Via Beirut 2, I-34151 Trieste - Italy
[34] Univ Tartu, Tartu Observ, Observ 1, EE-61602 Toravere - Estonia
[35] Ist Nazl Fis Nucl, Sez Trieste, I-34100 Trieste - Italy
[36] Univ Basque Country, Dept Theoret Phys, UPV EHU, Bilbao 48080 - Spain
[37] Univ Fed Rio Grande IMEF FURG, Inst Matemat Estat & Fis, Rio Grande, RS - Brazil
[38] Tech Univ Munich, Phys Dept, James Franck Str, D-85748 Garching - Germany
[39] European Southern Observ ESO, Alonso de Cordova 3107, Santiago - Chile
[40] CIDA, Ctr Invest Astron, Merida - Venezuela
[41] Heidelberg Univ, Inst Theoret Phys, Philosophenweg 16, D-69120 Heidelberg - Germany
[42] Univ Helsinki, Dept Phys, Gustaf Hallstromin Katu 2, Helsinki 00014 - Finland
[43] Univ Fed Rio de Janeiro, Observ Valongo, BR-20080090 Rio de Janeiro, RJ - Brazil
[44] Univ Napoli Federico II, Dipartimento Fis E Pancini, Via Cinthia, I-80126 Naples - Italy
[45] Ben Gurion Univ Negev, Dept Phys, IL-84105 Beer Sheva - Israel
[46] Univ Michigan, Dept Astron, 311 West Hall, 1085 South Univ Ave, Ann Arbor, MI 48109 - USA
[47] Univ Hong Kong, Dept Phys, Pokfulam Rd, Hong Kong - Peoples R China
[48] ESAC, Ctr Astrobiol CSIC INTA ESA, Madrid - Spain
[49] Ist Nazl Fis Nucl INFN, Sez Napoli, Via Cinthia 9, I-80126 Naples - Italy
[50] Waseda Univ, Dept Phys, Shinjuku Ku, 3-4-1 Okubo, Tokyo 1698555 - Japan
[51] Univ Florida, Dept Astron, 211 Bryant Space Ctr, Gainesville, FL 32611 - USA
[52] Univ Fed Sergipe, Dept Fis, Av Marechal Rondon S-N, BR-49000000 Sao Cristovao, SE - Brazil
[53] Univ Valencia, Observ Astron, Ed Inst Invest, Parc Cient, Valencia 46980 - Spain
[54] NSFs NOIRLab, Gemini Observ, Casilla 603, La Serena - Chile
[55] Gonzalez-Serrano, J., I, Inst Fis Cantabria CSIC UC, Avda Los Castros S-N, Santander 39005 - Spain
[56] Univ Fed Rio Grande do Sul UFRGS, Inst Fis, Dept Astron, Av Bento Goncalves 9500, Porto Alegre, RS - Brazil
[57] Univ Paris, 5 Rue Thomas Mann, F-75013 Paris - France
[58] Ctr Brasileiro Pesquisas Fis, Dept Theoret Phys, Rua Dr Xavier Sigaud 150, BR-22290180 Rio De Janeiro, RJ - Brazil
[59] Univ Salamanca, Dept Fis Fundamental, Salamanca 37008 - Spain
[60] Univ Salamanca, IUFFyM, Salamanca 37008 - Spain
[61] Instruments4, 4121 Pembury Pl, La Canada Flintridge, CA 91011 - USA
[62] Univ Cantabria, Dept Fis Moderna, Avda Castros S-N, Santander 39005 - Spain
[63] Univ Alicante, Inst Univ Fis Aplicada Ciencias & Tecnol, Alicante 03080 - Spain
[64] Univ Paris Diderot, AstroParticule & Cosmol, Sorbonne Paris Cite, CNRS IN2P3, CEA Irfu, Observ Paris, APC, F-75205 Paris 13 - France
[65] Univ Valencia, Unidad Asociada Grp Astrofis Extragalact & Cosmol, IFCA CSIC, Valencia - Spain
[66] UNAM, Inst Radioastron & Astrofis, Campus Morelia, Morelia 58089, Michoacan - Mexico
[67] Univ Szczecin, Inst Phys, Wielkopolska 15, PL-70451 Szczecin - Poland
Número total de Afiliações: 67
Tipo de documento: Artigo Científico
Fonte: Astronomy & Astrophysics; v. 653, SEP 3 2021.
Citações Web of Science: 3
Resumo

The Javalambre-Physics of the Accelerating Universe Astrophysical Survey (J-PAS) will scan thousands of square degrees of the northern sky with a unique set of 56 filters using the dedicated 2.55 m Javalambre Survey Telescope (JST) at the Javalambre Astrophysical Observatory. Prior to the installation of the main camera (4.2 deg(2) field-of-view with 1.2 Gpixels), the JST was equipped with the JPAS-Pathfinder, a one CCD camera with a 0.3 deg(2) field-of-view and plate scale of 0.23 arcsec pixel(-1). To demonstrate the scientific potential of J-PAS, the JPAS-Pathfinder camera was used to perform miniJPAS, a similar to 1 deg(2) survey of the AEGIS field (along the Extended Groth Strip). The field was observed with the 56 J-PAS filters, which include 54 narrow band (FWHM similar to 145 angstrom) and two broader filters extending to the UV and the near-infrared, complemented by the u, g, r, i SDSS broad band filters. In this miniJPAS survey overview paper, we present the miniJPAS data set (images and catalogs), as we highlight key aspects and applications of these unique spectro-photometric data and describe how to access the public data products. The data parameters reach depths of mag(AB) similar or equal to 22-23.5 in the 54 narrow band filters and up to 24 in the broader filters (5 sigma in a 3 `' aperture). The miniJPAS primary catalog contains more than 64 000 sources detected in the r band and with matched photometry in all other bands. This catalog is 99% complete at r = 23.6 (r = 22.7) mag for point-like (extended) sources. We show that our photometric redshifts have an accuracy better than 1% for all sources up to r = 22.5, and a precision of <= 0.3% for a subset consisting of about half of the sample. On this basis, we outline several scientific applications of our data, including the study of spatially-resolved stellar populations of nearby galaxies, the analysis of the large scale structure up to z similar to 0.9, and the detection of large numbers of clusters and groups. Sub-percent redshift precision can also be reached for quasars, allowing for the study of the large-scale structure to be pushed to z > 2. The miniJPAS survey demonstrates the capability of the J-PAS filter system to accurately characterize a broad variety of sources and paves the way for the upcoming arrival of J-PAS, which will multiply this data by three orders of magnitude. (AU)

Processo FAPESP: 18/05392-8 - Uma nova biblioteca de modelos de população estelar puramente teóricos
Beneficiário:Paula Rodrigues Teixeira Coelho
Modalidade de apoio: Auxílio à Pesquisa - Regular
Processo FAPESP: 11/18729-1 - Gravitação e cosmologia: questões estruturais e aplicações
Beneficiário:Elcio Abdalla
Modalidade de apoio: Auxílio à Pesquisa - Temático
Processo FAPESP: 15/11442-0 - Quasares e galáxias como traçadores das estruturas em grandes escalas
Beneficiário:Carolina Queiroz de Abreu Silva
Modalidade de apoio: Bolsas no Brasil - Doutorado
Processo FAPESP: 17/02375-2 - Modelos de população estelar teóricos vs. semi-empíricos: um experimento controlado
Beneficiário:Paula Rodrigues Teixeira Coelho
Modalidade de apoio: Auxílio à Pesquisa - Pesquisador Visitante - Internacional