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Noeske, K. G. ; Koo, D. C. ; Phillips, A. C. ; Willmer, C. N. A. ; Melbourne, J. ; Gil de Paz, Armando ; Papaderos, P. | American Astronomical Society | 2006-04-01We analyze 26 luminous compact blue galaxies (LCBGs) in the Hubble Space Telescope ACS Ultra Deep Field (UDF) at z ~ 0.2-1.3, to determine whether these truly are small galaxies or, rather, bright central starbursts within existing or forming la[...]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
Cardiel López, Nicolás ; Elbaz, D. ; Schiavon, R. P. ; Willmer, C. N. A. ; Koo, D. C. ; Phillips, A. C. ; Gallego Maestro, Jesús | IOP Publishing | 2003-02-10We use a sample of seven starburst galaxies at intermediate redshifts (z similar to 0.4 and 0.8) with observations ranging from the observed ultraviolet to 1.4 GHz, to compare the star formation rate (SFR) estimators that are used in the differe[...]
