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The Javalambre Photometric Local Universe Survey (J-PLUS) is a 12-band photometric survey using the 83-cm JAST telescope. Data Release 3 includes 47.4 million sources. J-PLUS DR3 only provides star-galaxy classification so that quasars are…

Context. In modern astronomy, machine learning has proved to be efficient and effective to mine the big data from the newesttelescopes. Spectral surveys enable us to characterize millions of objects, while long exposure time observations…

We present the photometric calibration of the twelve optical passbands for the Javalambre Photometric Local Universe Survey (J-PLUS) third data release (DR3), comprising 1642 pointings of two square degrees each. We selected nearly 1.5…

We present the white dwarf catalog derived from the third data release of the Javalambre Photometric Local Universe Survey (J-PLUS DR3), which covers 3284 deg2 using 12 optical filters. A particular focus is given to the classification of…

Our goal is to morphologically classify the sources identified in the images of the J-PLUS early data release (EDR) into compact (stars) or extended (galaxies) using a suited Bayesian classifier. J-PLUS sources exhibit two distinct…

We present the photometric calibration of the twelve optical passbands observed by the Javalambre Photometric Local Universe Survey (J-PLUS). The proposed calibration method has four steps: (i) definition of a high-quality set of…

In this pilot study, we investigate the PN population in M~33, a nearby spiral galaxy ($\simeq 840$~kpc), using data from the DR3 of the Javalambre-Photometric Local Universe Survey (J-PLUS), a 12-band photometric dataset extensively used…

J-PLUS is an ongoing 12-band photometric optical survey, observing thousands of square degrees of the Northern hemisphere from the dedicated JAST/T80 telescope at the Observatorio Astrof\'isico de Javalambre. T80Cam is a 2 sq.deg…

Astrophysics of Galaxies · Physics 2019-08-13 A. J. Cenarro , M. Moles , D. Cristóbal-Hornillos , A. Marín-Franch , A. Ederoclite , J. Varela , C. López-Sanjuan , C. Hernández-Monteagudo , R. E. Angulo , H. Vázquez Ramió , K. Viironen , S. Bonoli , A. A. Orsi , G. Hurier , I. San Roman , N. Greisel , G. Vilella-Rojo , L. A. Díaz-García , R. Logroño-García , S. Gurung-López , D. Spinoso , D. Izquierdo-Villalba , J. A. L. Aguerri , C. Allende Prieto , C. Bonatto , J. M. Carvano , A. L. Chies-Santos , S. Daflon , R. A. Dupke , J. Falcón-Barroso , D. R. Gonçalves , Y. Jiménez-Teja , A. Molino , V. M. Placco , E. Solano , D. D. Whitten , J. Abril , J. L. Antón , R. Bello , S. Bielsa de Toledo , J. Castillo-Ramírez , S. Chueca , T. Civera , M. C. Díaz-Martín , M. Domínguez-Martínez , J. Garzarán-Calderaro , J. Hernández-Fuertes , R. Iglesias-Marzoa , C. Iñiguez , J. M. Jiménez Ruiz , K. Kruuse , J. L. Lamadrid , N. Lasso-Cabrera , G. López-Alegre , A. López-Sainz , N. Maícas , A. Moreno-Signes , D. J. Muniesa , S. Rodríguez-Llano , F. Rueda-Teruel , S. Rueda-Teruel , I. Soriano-Laguía , V. Tilve , L. Valdivielso , A. Yanes-Díaz , J. S. Alcaniz , C. Mendes de Oliveira , L. Sodré , P. Coelho , R. Lopes de Oliveira , A. Tamm , H. S. Xavier , L. R. Abramo , S. Akras , E. J. Alfaro , A. Alvarez-Candal , B. Ascaso , M. A. Beasley , T. C. Beers , M. Borges Fernandes , G. R. Bruzual , M. L. Buzzo , J. M. Carrasco , J. Cepa , A. Cortesi , M. V. Costa-Duarte , M. De Prá , G. Favole , A. Galarza , L. Galbany , K. Garcia , R. M. González Delgado , J. I. González-Serrano , L. A. Gutiérrez-Soto , J. A. Hernandez-Jimenez , A. Kanaan , H. Kuncarayakti , R. C. G. Landim , J. Laur , J. Licandro , G. B. Lima Neto , J. D. Lyman , J. Maíz Apellániz , J. Miralda-Escudé , D. Morate , J. P. Nogueira-Cavalcante , P. M. Novais , M. Oncins , I. Oteo , R. A. Overzier , C. B. Pereira , A. Rebassa-Mansergas , R. R. R. Reis , F. Roig , M. Sako , N. Salvador-Rusiñol , L. Sampedro , P. Sánchez-Blázquez , W. A. Santos , L. Schmidtobreick , B. B. Siffert , E. Telles

Over the past decades, several studies have discovered a population of galaxies undergoing very strong star formation events, called extreme emission line galaxies (EELGs). In this work, we exploit the capabilities of the Javalambre…

From the approximately $\sim$3,500 planetary nebulae (PNe) discovered in our Galaxy, only 14 are known to be members of the Galactic halo. Nevertheless, a systematic search for halo PNe has never been performed. In this study, we present…

Context. The Javalambre Photometric Local Universe Survey (J-PLUS) has obtained precise photometry in twelve specially designed filters for large numbers of Galactic stars. Deriving their precise stellar atmospheric parameters and…

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…

Cosmology and Nongalactic Astrophysics · Physics 2021-09-08 S. Bonoli , A. Marín-Franch , J. Varela , H. Vázquez Ramió , L. R. Abramo , A. J. Cenarro , R. A. Dupke , J. M. Vílchez , D. Cristóbal-Hornillos , R. M. González Delgado , C. Hernández-Monteagudo , C. López-Sanjuan , D. J. Muniesa , T. Civera , A. Ederoclite , A. Hernán-Caballero , V. Marra , P. O. Baqui , A. Cortesi , E. S. Cypriano , S. Daflon , A. L. de Amorim , L. A. Díaz-García , J. M. Diego , G. Martínez-Solaeche , E. Pérez , V. M. Placco , F. Prada , C. Queiroz , J. Alcaniz , A. Alvarez-Candal , J. Cepa , A. L. Maroto , F. Roig , B. B. Siffert , K. Taylor , N. Benitez , M. Moles , L. Sodré , S. Carneiro , C. Mendes de Oliveira , E. Abdalla , R. E. Angulo , M. Aparicio Resco , A. Balaguera-Antolínez , F. J. Ballesteros , D. Brito-Silva , T. Broadhurst , E. R. Carrasco , T. Castro , R. Cid Fernandes , P. Coelho , R. B. de Melo , L. Doubrawa , A. Fernandez-Soto , F. Ferrari , A. Finoguenov , R. García-Benito , J. Iglesias-Páramo , Y. Jiménez-Teja , F. S. Kitaura , J. Laur , P. A. A. Lopes , G. Lucatelli , V. J. Martínez , M. Maturi , M. Quartin , C. Pigozzo , J. E. Rodrìguez-Martìn , V. Salzano , A. Tamm , E. Tempel , K. Umetsu , L. Valdivielso , R. von Marttens , A. Zitrin , M. C. Díaz-Martín , G. López-Alegre , A. López-Sainz , A. Yanes-Díaz , F. Rueda-Teruel , S. Rueda-Teruel , J. Abril Ibañez , J. L Antón Bravo , R. Bello Ferrer , S. Bielsa , J. M. Casino , J. Castillo , S. Chueca , L. Cuesta , J. Garzarán Calderaro , R. Iglesias-Marzoa , C. Íniguez , J. L. Lamadrid Gutierrez , F. Lopez-Martinez , D. Lozano-Pérez , N. Maícas Sacristán , E. L. Molina-Ibáñez , A. Moreno-Signes , S. Rodríguez Llano , M. Royo Navarro , V. Tilve Rua , U. Andrade , E. J. Alfaro , S. Akras , P. Arnalte-Mur , B. Ascaso , C. E. Barbosa , J. Beltrán Jiménez , M. Benetti , C. A. P. Bengaly , A. Bernui , J. J. Blanco-Pillado , M. Borges Fernandes , J. N. Bregman , G. Bruzual , G. Calderone , J. M. Carvano , L. Casarini , A. L Chies-Santos , G. Coutinho de Carvalho , P. Dimauro , S. Duarte Puertas , D. Figueruelo , J. I. González-Serrano , M. A. Guerrero , S. Gurung-López , D. Herranz , M. Huertas-Company , J. A. Irwin , D. Izquierdo-Villalba , A. Kanaan , C. Kehrig , C. C. Kirkpatrick , J. Lim , A. R. Lopes , R. Lopes de Oliveira , A. Marcos-Caballero , D. Martínez-Delgado , E. Martínez-González , G. Martínez-Somonte , N. Oliveira , A. A. Orsi , R. A. Overzier , M. Penna-Lima , R. R. R. Reis , D. Spinoso , S. Tsujikawa , P. Vielva , A. Z. Vitorelli , J. Q. Xia , H. B. Yuan , A. Arroyo-Polonio , M. L. L. Dantas , C. A. Galarza , D. R. Gonçalves , R. S. Gonçalves , J. E. Gonzalez , A. H. Gonzalez , N. Greisel , R. G. Landim , D. Lazzaro , G. Magris , R. Monteiro-Oliveira , C. B. Pereira , M. J. Rebouças , J. M. Rodriguez-Espinosa , S. Santos da Costa , E. Telles

Context: The Javalambre Photometric Local Universe Survey (J-PLUS) is an observational campaign that aims to obtain photometry in 12 ultraviolet-visible filters (0.3-1 {\mu}m) of approximately 8 500 deg{^2} of the sky observable from…

We aim to use multi-band imaging from the Phase-3 Verification Data of the J-PLUS survey to derive accurate photometric redshifts (photo-z) and look for potential new members in the surroundings of the nearby galaxy clusters A2589…

The Beijing-Arizona Sky Survey (BASS) Data Release 3 (DR3) catalogue was released in 2019, which contains the data from all BASS and the Mosaic z-band Legacy Survey (MzLS) observations during 2015 January and 2019 March, about 200 million…

We present a catalog of stellar parameters (effective temperature $T_{\rm eff}$, surface gravity $\log g$, age, and metallicity [Fe/H]) and elemental-abundance ratios ([C/Fe], [Mg/Fe], and [$\alpha$/Fe]) for some five million stars (4.5…

We present a dedicated automated pipeline to construct spatially resolved emission H$\alpha$+[NII] maps and to derive the spectral energy distributions (SEDs) in 12 optical filters (five broad and seven narrow/medium) of H$\alpha$ emission…

The Southern Photometric Local Universe Survey (S-PLUS) is a novel project that aims to map the Southern Hemisphere using a twelve filter system, comprising five broad-band SDSS-like filters and seven narrow-band filters optimized for…

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