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pro vyhledávání: '"Fernández-Ontiveros, J. A."'
Autor:
Maturi, M., Finoguenov, A., Lopes, P. A. A., Delgado, R. M. González, Dupke, R. A., Cypriano, E. S., Carrasco, E. R., Diego, J. M., Penna-Lima, M., Vílchez, J. M., Moscardini, L., Marra, V., Bonoli, S., Rodríguez-Martín, J. E., Zitrin, A., Márquez, I., Hernán-Caballero, A., Jiménez-Teja, Y., Abramo, R., Alcaniz, J., Benitez, N., Carneiro, S., Cenarro, J., Cristóbal-Hornillos, D., Ederoclite, A., López-Sanjuan, C., Marín-Franch, A., de Oliveira, C. Mendes, Moles, M., Sodré Jr., L., Taylor, K., Varela, J., Ramió, H. Vázquez, Fernández-Ontiveros, J. A.
Samples of galaxy clusters allow us to better understand the physics at play in galaxy formation and to constrain cosmological models once their mass, position (for clustering studies) and redshift are known. In this context, large optical data sets
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c40015647880e1aa6e797468255979d0
Autor:
Hernán-Caballero, A., Willmer, C. N. A., Varela, J., López-Sanjuan, C., Marín-Franch, A., Vázquez Ramió, H., Civera, T., Ederoclite, A., Muniesa, D., Cenarro, J., Bonoli, S., Dupke, R., Lim, J., Chaves-Montero, J., Laur, J., Hernández-Monteagudo, C., Fernández-Ontiveros, J. A., Fernández-Soto, A., Díaz-García, L. A., González Delgado, Rosa M., Queiroz, C., Vílchez Medina, José Manuel, Abramo, R., Alcaniz, J., Benítez, Narciso, Carneiro, S., Cristóbal-Hornillos, D., Mendes de Oliveira, C., Moles, Mariano, Sodré, L., Taylor, K.
This is an Open Access article, published by EDP Sciences, under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provid
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2231b994dfd603186709699cabbae0de
Autor:
Martínez-Solaeche, G., Delgado, R. M. González, García-Benito, R., Díaz-García, L. A., Rodríguez-Martín, J. E., Pérez, E., de Amorim, A., Puertas, S. Duarte, Sodré, Laerte, Sobral, David, Chaves-Montero, Jonás, Vílchez, J. M., Hernán-Caballero, A., López-Sanjuan, C., Cortesi, A., Bonoli, S., Cenarro, A. J., Dupke, R. A., Marín-Franch, A., Varela, J., Ramió, H. Vázquez, Abramo, L. R., Cristóbal-Hornillos, D., Moles, M., Alcaniz, J., Benitez, N., Ederoclite, A., Marra, V., de Oliveira, C. Mendes, Taylor, K., Fernández-Ontiveros, J. A.
The Javalambre-Physics of the Accelerating Universe Astrophysical Survey (J-PAS) is expected to map thousands of square degrees of the northern sky with 56 narrowband filters in the upcoming years. This will make J-PAS a very competitive and unbiased
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::2822dbe9f8ff85b4d91243d88e088ede
Autor:
Yang, Lin, Yuan, Haibo, Xiang, Maosheng, Duan, Fuqing, Huang, Yang, Liu, Jifeng, Beers, Timothy C., Galarza, Carlos Andrés, Daflon, Simone, Fernández-Ontiveros, J. A., Cenarro, Javier, Cristóbal-Hornillos, David, Hernández-Monteagudo, Carlos, López-Sanjuan, Carlos, Marín-Franch, Antonio, Moles, Mariano, Varela, Jesús, Ramió, Héctor Vázquez, Alcaniz, Jailson, Dupke, Renato, Ederoclite, Alessandro, Sodré, Laerte, Angulo, Raul E.
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 individual elementa
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::50d0db34f9eb58516c4f8e8e27702f02
Autor:
Armus, L., Baes, M., Charmandaris, V., Czerny, B., Efstathiou, A., Fernandez-Ontiveros, J. A., Ferrara, A., Gonzalez-Alfonso, E., Griffin, M., Gruppioni, C., Hatziminaoglou, E., Pozzi, F., Scott, D., Smith, J. -D. T., Spinoglio, L., Suzuki, T., van, der Tak F., Vaccari, M., Vignali, C., Wang, L., Kaneda, Hidehiro, Ishihara, Daisuke, Oyabu, Shinki, Yamagishi, Mitsuyoshi, Wada, Takehiko, Imanishi, Masatoshi, Kohno, Kotaro, Kwon, Jungmi, Nakagawa, Takao, Onaka, Takashi
Publikováno v:
Publications of the Astronomical Society of Australia, 34:e059. Cambridge University Press
The mid-infrared (IR) range contains many spectral features associated with large molecules and dust grains such as polycyclic aromatic hydrocarbons (PAHs) and silicates. These are usually very strong compared to fine-structure gas lines, and thus va
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::671d6d953979ab24e3bafae0b43c8e29