Zobrazeno 1 - 10
of 96
pro vyhledávání: '"Rodriguez Espinosa, J. M."'
Autor:
González-Morán, A. L., Haro, P. Arrabal, Muñóz-Tuñón, C., Rodríguez-Espinosa, J. M., Sánchez-Almeida, J., Calhau, J., Gaztañaga, E., Castander, F. J., Renard, P., Cabayol, L., Fernandez, E., Padilla, C., Garcia-Bellido, J., Miquel, R., De Vicente, J., Sanchez, E., Sevilla-Noarbe, I., Navarro-Gironés, D.
We present an application of unsupervised Machine Learning Clustering to the PAU Survey of galaxy spectral energy distribution (SED) within the COSMOS field. The clustering algorithm is implemented and optimized to get the relevant groups in the data
Externí odkaz:
http://arxiv.org/abs/2307.13840
Autor:
Benítez, E., Jiménez-Bailón, E., Negrete, C. A., Ruschel-Dutra, D., Rodríguez-Espinosa, J. M., Cruz-González, I., Rodríguez, L. F., Chavushyan, V. H., Marziani, P., Gutiérrez, L., González-Martin, O., Jiang, B. W., D'Onofrio, M.
We have studied the nuclear region of the previously detected dual AGN system in the galaxy pair IRAS 05589+2828 and 2MASX J06021107+2828382 through new optical spectroscopy observations, along with radio and X-ray archival data. Our multiwavelength
Externí odkaz:
http://arxiv.org/abs/2208.06451
Autor:
Almeida, J. Sanchez, Calhau, J., Munoz-Tunon, C., Gonzalez-Moran, A. L., Rodriguez-Espinosa, J. M.
Aiming at the detection of cosmological gas being accreted onto galaxies of the local Universe, we examined the Halpha emission in the halo of 164 galaxies in the field of view of the Multi-Unit Spectroscopic Explorer Wide survey (\musew ) with obser
Externí odkaz:
http://arxiv.org/abs/2205.12782
Autor:
Cabello, C., Gallego, J., Cardiel, N., Pascual, S., Guzmán, R., Herrero, A., Manrique, A., Marín-Franch, A., Mas-Hesse, J. M., Rodríguez-Espinosa, J. M., Salvador-Solé, E.
Publikováno v:
A&A 659, A116 (2022)
Identifying very high-redshift galaxies is crucial for understanding the formation and evolution of galaxies. However, many questions still remain, and the uncertainty on the epoch of reionization is large. In this approach, some models allow a doubl
Externí odkaz:
http://arxiv.org/abs/2112.04505
Autor:
Rodríguez-Muñoz, L., Rodighiero, G., Pérez-González, P. G., Talia, M., Baronchelli, I., Morselli, L., Renzini, A., Puglisi, A., Grazian, A., Zanella, A., Mancini, C., Feltre, A., Romano, M., García, A. Vidal, Franceschini, A., Pampliega, B. Alcalde, Cassata, P., Costantin, L., Sánchez, H. Domínguez, Espino-Briones, N., Iani, E., Koekemoer, A., Lumbreras-Calle, A., Rodríguez-Espinosa, J. M.
We use a sample of 706 galaxies, selected as [OII]$\lambda$3727 ([OII]) emitters in the Survey for High-$z$ Absorption Red and Dead Sources (SHARDS) on the CANDELS/GOODS-N field, to study the differential attenuation of the nebular emission with resp
Externí odkaz:
http://arxiv.org/abs/2112.01885
Autor:
Jin, S., Dannerbauer, H., Emonts, B., Serra, P., Lagos, C. D. P., Thomson, A. P., Bassini, L., Lehnert, M., Allison, J. R., Champagne, J. B., Indermuhle, B., Norris, R. P., Seymour, N., Shimakawa, R., Casey, C. M., De Breuck, C., Drouart, G., Hatch, N., Kodama, T., Koyama, Y., Macgregor, P., Miley, G., Overzier, R., Perez-Martinez, J. M., Rodriguez-Espinosa, J. M., Rottgering, H., Portal, M. Sanchez, Ziegler, B.
Publikováno v:
A&A 652, A11 (2021)
We report a detailed CO(1-0) survey of a galaxy protocluster field at $z=2.16$, based on 475 hours of observations with the Australia Telescope Compact Array. We constructed a large mosaic of 13 individual pointings, covering an area of 21 arcmin$^2$
Externí odkaz:
http://arxiv.org/abs/2103.08884
Autor:
Bonoli, S., Marín-Franch, A., Varela, J., Ramió, H. Vázquez, Abramo, L. R., Cenarro, A. J., Dupke, R. A., Vílchez, J. M., Cristóbal-Hornillos, D., Delgado, R. M. González, Hernández-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. Mendes, Abdalla, E., Angulo, R. E., Resco, M. Aparicio, Balaguera-Antolínez, A., Ballesteros, F. J., Brito-Silva, D., Broadhurst, T., Carrasco, E. R., Castro, T., Fernandes, R. Cid, Coelho, 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. Abril, Bravo, J. L Antón, Ferrer, R. Bello, Bielsa, S., Casino, J. M., Castillo, J., Chueca, S., Cuesta, L., Calderaro, J. Garzarán, Iglesias-Marzoa, R., Íniguez, C., Gutierrez, J. L. Lamadrid, Lopez-Martinez, F., Lozano-Pérez, D., Sacristán, N. Maícas, Molina-Ibáñez, E. L., Moreno-Signes, A., Llano, S. Rodríguez, Navarro, M. Royo, Rua, V. Tilve, Andrade, U., Alfaro, E. J., Akras, S., Arnalte-Mur, P., Ascaso, B., Barbosa, C. E., Jiménez, J. Beltrán, Benetti, M., Bengaly, C. A. P., Bernui, A., Blanco-Pillado, J. J., Fernandes, M. Borges, Bregman, J. N., Bruzual, G., Calderone, G., Carvano, J. M., Casarini, L., Chies-Santos, A. L, de Carvalho, G. Coutinho, Dimauro, P., Puertas, S. Duarte, Figueruelo, 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. Lopes, Marcos-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. Santos, Telles, E.
Publikováno v:
A&A 653, A31 (2021)
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,
Externí odkaz:
http://arxiv.org/abs/2007.01910
Autor:
Benítez, E., Cruz-González, I., Rodríguez-Espinosa, J. M., González-Martín, O., Negrete, C. A., Gutiérrez, L., Jiménez-Bailón, E., Ruschel-Dutra, D., Rodríguez, L. F., Loinard, L., Binette, L.
Publikováno v:
Monthly Notices of the Royal Astronomical Society Main Journal 2019
A detailed multi-wavelength study of the properties of the triple-peaked AGN Mrk\,622 showing different aspects of the nuclear emission region is presented. Radio, near- and mid-infrared, optical and X-ray data has been considered for the analysis. I
Externí odkaz:
http://arxiv.org/abs/1910.04916
Autor:
González-Martín, O., Masegosa, J., García-Bernete, I., Almeida, C. Ramos, Rodríguez-Espinosa, J. M., Márquez, I., Esparza-Arredondo, D., Osorio-Clavijo, N., Martínez-Paredes, M., Victoria-Ceballos, C., Pasetto, A., Dultzin, D.
This is the second in a series of papers devoted to explore a set of six dusty models of active galactic nuclei (AGN) with available spectral energy distributions (SEDs). These models are the smooth torus by Fritz et al. (2006), the clumpy torus by N
Externí odkaz:
http://arxiv.org/abs/1908.11389
Autor:
González-Martín, O., Masegosa, J., García-Bernete, I., Almeida, C. Ramos, Rodríguez-Espinosa, J. M., Márquez, I., Esparza-Arredondo, D., Osorio-Clavijo, N., Martínez-Paredes, M., Victoria-Ceballos, C., Pasetto, A., Dultzin, D.
At distances from the active galaxy nucleus (AGN) where the ambient temperature falls below ~1500-1800 K, dust is able to survive. It is thus possible to have a large dusty structure present which surrounds the AGN. This is the first of two papers ai
Externí odkaz:
http://arxiv.org/abs/1908.11381