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Rigby, J. R. ; Marcillac, D. ; Egami, E. ; Rieke, G. H. ; Richard, J. ; Kneib, J. P. ; Fadda, D. ; Willmer, C. N. A. ; Borys, C. ; van der Werf, P. P. ; Pérez González, Pablo Guillermo ; Knudsen, K. K. ; Papovich, C. | American Astronomical Society | 2008-03-01We present Spitzer IRS mid-infrared spectra for 15 gravitationally lensed, 24 ?m-selected galaxies, and combine the results with four additional very faint galaxies with IRS spectra in the literature. The median intrinsic 24 ?m flux density of t[...]texto impreso
Rodríguez Muñoz, L. ; Rodighiero, G. ; Mancini, C. ; Pérez González, Pablo Guillermo ; Rawle, T.D. ; Egami, E. ; Mercurio, A. ; Rosati, P. ; Puglisi, A. ; Franceschini, A. ; Balestra, I. ; Baronchelli, I. ; Biviano, A. ; Ebeling, H. ; Edge, A,C ; Enia, A.F.M. ; Grillo, C. ; Haines, C.P. ; Iani, E. ; Jones, T. ; Nonino, M. ; Valtchanov, I. ; Vulcani, B. ; Zemcov, M. | Oxford University Press. | 2019-05We quantify the star formation (SF) in the inner cores (R/R_(200) ?0.3) of 24 massive galaxy clusters at 0.2texto impreso
Donley, J. L. ; Rieke, G. H. ; Alexander, D. M. ; Egami, E. ; Pérez González, Pablo Guillermo | American Astronomical Society | 2010-08-20We present the active galactic nucleus (AGN), star-forming, and morphological properties of a sample of 13 MIR-luminous (?_24 700 ?Jy) IR-bright/optically-faint galaxies (IRBGs, ?_24/f_R? 1000). While these z ? 2 sources were drawn from deep Cha[...]
