학술논문

The miniJPAS survey: a preview of the Universe in 56 colours
Document Type
Working Paper
Author
Bonoli, S.Marín-Franch, A.Varela, J.Ramió, H. VázquezAbramo, L. R.Cenarro, A. J.Dupke, R. A.Vílchez, J. M.Cristóbal-Hornillos, D.Delgado, R. M. GonzálezHernández-Monteagudo, C.López-Sanjuan, C.Muniesa, D. J.Civera, T.Ederoclite, A.Hernán-Caballero, A.Marra, V.Baqui, P. O.Cortesi, A.Cypriano, E. S.Daflon, S.de Amorim, A. L.Díaz-García, L. A.Diego, J. M.Martínez-Solaeche, G.Pérez, E.Placco, V. M.Prada, F.Queiroz, C.Alcaniz, J.Alvarez-Candal, A.Cepa, J.Maroto, A. L.Roig, F.Siffert, B. B.Taylor, K.Benitez, N.Moles, M.Sodré Jr., L.Carneiro, S.de Oliveira, C. MendesAbdalla, E.Angulo, R. E.Resco, M. AparicioBalaguera-Antolínez, A.Ballesteros, F. J.Brito-Silva, D.Broadhurst, T.Carrasco, E. R.Castro, T.Fernandes, R. CidCoelho, P.de Melo, R. B.Doubrawa, L.Fernandez-Soto, A.Ferrari, F.Finoguenov, A.García-Benito, R.Iglesias-Páramo, J.Jiménez-Teja, Y.Kitaura, F. S.Laur, J.Lopes, P. A. A.Lucatelli, G.Martínez, V. J.Maturi, M.Quartin, M.Pigozzo, C.Rodrìguez-Martìn, J. E.Salzano, V.Tamm, A.Tempel, E.Umetsu, K.Valdivielso, L.von Marttens, R.Zitrin, A.Díaz-Martín, M. C.López-Alegre, G.López-Sainz, A.Yanes-Díaz, A.Rueda-Teruel, F.Rueda-Teruel, S.Ibañez, J. AbrilBravo, J. L AntónFerrer, R. BelloBielsa, S.Casino, J. M.Castillo, J.Chueca, S.Cuesta, L.Calderaro, J. GarzaránIglesias-Marzoa, R.Íniguez, C.Gutierrez, J. L. LamadridLopez-Martinez, F.Lozano-Pérez, D.Sacristán, N. MaícasMolina-Ibáñez, E. L.Moreno-Signes, A.Llano, S. RodríguezNavarro, M. RoyoRua, V. TilveAndrade, U.Alfaro, E. J.Akras, S.Arnalte-Mur, P.Ascaso, B.Barbosa, C. E.Jiménez, J. BeltránBenetti, M.Bengaly, C. A. P.Bernui, A.Blanco-Pillado, J. J.Fernandes, M. BorgesBregman, J. N.Bruzual, G.Calderone, G.Carvano, J. M.Casarini, L.Chies-Santos, A. Lde Carvalho, G. CoutinhoDimauro, P.Puertas, S. DuarteFigueruelo, D.González-Serrano, J. I.Guerrero, M. A.Gurung-López, S.Herranz, D.Huertas-Company, M.Irwin, J. A.Izquierdo-Villalba, D.Kanaan, A.Kehrig, C.Kirkpatrick, C. C.Lim, J.Lopes, A. R.de Oliveira, R. LopesMarcos-Caballero, A.Martínez-Delgado, D.Martínez-González, E.Martínez-Somonte, G.Oliveira, N.Orsi, A. A.Overzier, R. A.Penna-Lima, M.Reis, R. R. R.Spinoso, D.Tsujikawa, S.Vielva, P.Vitorelli, A. Z.Xia, J. Q.Yuan, H. B.Arroyo-Polonio, A.Dantas, M. L. L.Galarza, C. A.Gonçalves, D. R.Gonçalves, R. S.Gonzalez, J. E.Gonzalez, A. H.Greisel, N.Landim, R. G.Lazzaro, D.Magris, G.Monteiro-Oliveira, R.Pereira, C. B.Rebouças, M. J.Rodriguez-Espinosa, J. M.da Costa, S. SantosTelles, E.
Source
A&A 653, A31 (2021)
Subject
Astrophysics - Cosmology and Nongalactic Astrophysics
Astrophysics - Astrophysics of Galaxies
Astrophysics - Instrumentation and Methods for Astrophysics
Language
Abstract
The Javalambre-Physics of the Accelerating Universe Astrophysical Survey (J-PAS) will soon start to scan thousands of square degrees of the northern extragalactic sky with a unique set of $56$ optical filters from a dedicated $2.55$m telescope, JST, at the Javalambre Astrophysical Observatory. Before the arrival of the final instrument (a 1.2 Gpixels, 4.2deg$^2$ field-of-view camera), the JST was equipped with an interim camera (JPAS-Pathfinder), composed of one CCD with a 0.3deg$^2$ field-of-view and resolution of 0.23 arcsec pixel$^{-1}$. To demonstrate the scientific potential of J-PAS, with the JPAS-Pathfinder camera we carried out a survey on the AEGIS field (along the Extended Groth Strip), dubbed miniJPAS. We observed a total of $\sim 1$ deg$^2$, with the $56$ J-PAS filters, which include $54$ narrow band (NB, $\rm{FWHM} \sim 145$Angstrom) and two broader filters extending to the UV and the near-infrared, complemented by the $u,g,r,i$ SDSS broad band (BB) filters. In this paper we present the miniJPAS data set, the details of the catalogues and data access, and illustrate the scientific potential of our multi-band data. The data surpass the target depths originally planned for J-PAS, reaching $\rm{mag}_{\rm {AB}}$ between $\sim 22$ and $23.5$ for the NB filters and up to $24$ for the BB filters ($5\sigma$ in a $3$~arcsec aperture). The miniJPAS primary catalogue contains more than $64,000$ sources extracted in the $r$ detection band with forced photometry in all other bands. We estimate the catalogue to be complete up to $r=23.6$ for point-like sources and up to $r=22.7$ for extended sources. Photometric redshifts reach subpercent precision for all sources up to $r=22.5$, and a precision of $\sim 0.3$% for about half of the sample. (Abridged)
Comment: The miniJPAS data and associated value added catalogues are publicly accessible via this url: http://archive.cefca.es/catalogues/minijpas-pdr201912