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Rieke, G. H. ; Alonso Herrero, A. ; Weiner, B. J. ; Pérez González, Pablo Guillermo ; Blaylock, M. ; Donley, J. L. ; Marcillac, D. | American Astronomical Society | 2009-02-10We show that measures of star formation rates (SFRs) for infrared galaxies using either single-band 24 ?m or extinction-corrected Pa? luminosities are consistent in the total infrared luminosity = L(TIR) ~ 10^10 L_? range. MIPS 24 ?m photometry [...]texto impreso
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
Donley, J. L. ; Rieke, G. H. ; Pérez González, Pablo Guillermo ; Rigby, J. R. ; Alonso Herrero, A. | American Astronomical Society | 2007-05-01We define a sample of 62 galaxies in the Chandra Deep Field-North whose Spitzer IRAC SEDs exhibit the characteristic power-law emission expected of luminous AGNs. We study the multiwavelength properties of this sample and compare the AGNs select[...]texto impreso
Donley, J. L. ; Rieke, G. H. ; Pérez González, Pablo Guillermo ; Barro, Guillermo | American Astronomical Society | 2008-11-01Infrared selection is a potentially powerful way to identify heavily obscured AGNs missed in even the deepest X-ray surveys. Using a 24 ?m-selected sample in GOODS-S, we test the reliability and completeness of three infrared AGN selection metho[...]texto 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[...]
