Zobrazeno 1 - 10
of 58
pro vyhledávání: '"B. Alcalde"'
Autor:
Solimano, M., González-López, J., Aravena, M., Pampliega, B. Alcalde, Assef, R. J., Béthermin, M., Boquien, M., Bovino, S., Casey, C. M., Cassata, P., da Cunha, E., Davies, R. L., De Looze, I., Ding, X., Díaz-Santos, T., Faisst, A. L., Ferrara, A., Fisher, D. B., Förster-Schreiber, N. M., Fujimoto, S., Ginolfi, M., Gruppioni, C., Guaita, L., Hathi, N., Herrera-Camus, R., Ibar, E., Inami, H., Jones, G. C., Koekemoer, A. M., Lee, L., Li, J., Liu, D., Liu, Z., Molina, J., Ogle, P., Posses, A. C., Pozzi, F., Relaño, M., Riechers, D. A., Romano, M., Spilker, J., Sulzenauer, N., Telikova, K., Vallini, L., Vasan, K. G. C., Veilleux, S., Vergani, D., Villanueva, V., Wang, W., Yan, L., Zamorani, G.
We present new JWST/NIRSpec IFU observations of the J1000+0234 system at $z=4.54$, the dense core of a galaxy protocluster hosting a massive, dusty star forming galaxy (DSFG) with a low luminosity radio counterpart. The new data reveals two extended,
Externí odkaz:
http://arxiv.org/abs/2407.13020
Autor:
Gottumukkala, R., Barrufet, L., Oesch, P. A., Weibel, A., Allen, N., Pampliega, B. Alcalde, Nelson, E. J., Williams, C. C., Brammer, G., Fudamoto, Y., González, V., Heintz, K. E., Illingworth, G., Magee, D., Naidu, R. P., Shuntov, M., Stefanon, M., Toft, S., Valentino, F., Xiao, M.
With the advent of JWST, we can probe the rest-frame optical emission of galaxies at $z>3$ with high sensitivity and spatial resolution, making it possible to accurately characterise red, optically-faint galaxies and thus move towards a more complete
Externí odkaz:
http://arxiv.org/abs/2310.03787
Autor:
Costantin, L., Pérez-González, P. G., Méndez-Abreu, J., Huertas-Company, M., Pampliega, B. Alcalde, Balcells, M., Barro, G., Ceverino, D., Dimauro, P., Sánchez, H. Domínguez, Espino-Briones, N., Koekemoer, A. M.
We investigate the assembly history of massive disk galaxies and describe how they shape their morphology through cosmic time. Using SHARDS and HST data, we modeled the surface brightness distribution of 91 massive galaxies at redshift $0.14
Externí odkaz:
http://arxiv.org/abs/2202.02332
Autor:
Rodríguez-Muñoz, L., Rodighiero, G., Pérez-González, P. G., Talia, M., Baronchelli, I., Morselli, L., Renzini, A., Puglisi, A., Grazian, A., Zanella, A., Mancini, C., Feltre, A., Romano, M., García, A. Vidal, Franceschini, A., Pampliega, B. Alcalde, Cassata, P., Costantin, L., Sánchez, H. Domínguez, Espino-Briones, N., Iani, E., Koekemoer, A., Lumbreras-Calle, A., Rodríguez-Espinosa, J. M.
We use a sample of 706 galaxies, selected as [OII]$\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:
Haro, P. Arrabal, Espinosa, J. M. Rodríguez, Muñoz-Tuñón, C., Sobral, D., Lumbreras-Calle, A., Boquien, M., Hernán-Caballero, A., Rodríguez-Muñoz, L., Pampliega, B. Alcalde
The differences between the inherent stellar populations (SPs) of LAEs and LBGs are a key factor in understanding early galaxy formation and evolution. We have run a set of SP burst-like models for a sample of 1,558 sources at $3.4
Externí odkaz:
http://arxiv.org/abs/2004.11175
Autor:
Haro, P. Arrabal, Espinosa, J. M. Rodríguez, Muñoz-Tuñón, C., Pérez-González, P. G., Dannerbauer, H., Bongiovanni, Á., Barro, G., Cava, A., Lumbreras-Calle, A., Hernán-Caballero, A., Eliche-Moral, M. C., Sánchez, H. Domínguez, Conselice, C. J., Tresse, L., Pampliega, B. Alcalde, Balcells, M., Daddi, E., Rodighiero, G.
We have undertaken a comprehensive search for both Lyman Alpha Emitters (LAEs) and Lyman Break Galaxies (LBGs) in the SHARDS Survey of the GOODS-N field. SHARDS is a deep imaging survey, made with the 10.4 m Gran Telescopio Canarias (GTC), employing
Externí odkaz:
http://arxiv.org/abs/1805.00477
Autor:
Lumbreras-Calle, A., Muñoz-Tuñón, C., Méndez-Abreu, J., Mas-Hesse, J. M., Pérez-González, P. G., Pampliega, B. Alcalde, Haro, P. Arrabal, Cava, A., Sánchez, H. Domínguez, Eliche-Moral, M. C., Alonso-Herrero, A., Borlaff, A., Gallego, J., Hernán-Caballero, A., Koekemoer, A. M., Rodríguez-Muñoz, L.
Publikováno v:
A&A 621, A52 (2019)
The physical processes driving the evolution of star formation (SF) in galaxies over cosmic time still present many open questions. Recent galaxy surveys allow now to study these processes in great detail at intermediate redshift. In this work, we bu
Externí odkaz:
http://arxiv.org/abs/1803.08045
Autor:
Tress, M., Mármol-Queraltó, E., Ferreras, I., Pérez-González, P. G., Barro, G., Pampliega, B. Alcalde, Cava, A., Domínguez-Sánchez, H., Eliche-Moral, C., Espino-Briones, N., Esquej, P., Hernán-Caballero, A., Rodighiero, G., Rodriguez-Muñoz, L.
Publikováno v:
2018, MNRAS, 475, 2363
We make use of SHARDS, an ultra-deep (<26.5AB) galaxy survey that provides optical photo-spectra at resolution R~50, via medium band filters (FWHM~150A). This dataset is combined with ancillary optical and NIR fluxes to constrain the dust attenuation
Externí odkaz:
http://arxiv.org/abs/1801.01128
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.