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Huertas Company, M. ; Gravet, R. ; Cabrera Vives, G. ; Pérez González, Pablo Guillermo ; Kartaltepe, J. S. ; Barro, G. ; Bernardi, M. ; Mei, S. ; Shankar, F. ; Dimauro, P. ; Bell, E. F. ; Kocevski, D. ; Koo, D. C. ; Faber, S. M. ; Mcintosh, D. H. | University Chicago Press | 2015-11We present a catalog of visual-like H-band morphologies of ~50.000 galaxies (H_f160wtexto impreso
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
Huertas Company, M. ; Bernardi, M. ; Pérez González, Pablo Guillermo ; Ashby, M. L. N. ; Barro, G. ; Conselice, C. ; Daddi, E. ; Dekel, A. ; Dimauro, P. ; Faber, S. M. ; Grogin, N. A. ; Kartaltepe, J. S. ; Kocevski, D. D. ; Koekemoer, A. M. ; Koo, D. C. ; Mei, S. ; Shankar, F. | Wiley | 2016-11-11We quantify the evolution of the stellar mass functions (SMFs) of star-forming and quiescent galaxies as a function of morphology from z ? 3 to the present. Our sample consists of ?50?000 galaxies in the CANDELS fields (?880 arcmin^2), which we [...]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[...]texto impreso
Barro, G. ; Kriek, M. ; Pérez González, Pablo Guillermo ; Díaz Santos, T. ; Price, S. H. ; Rujopakarn, W. ; Pandya, V. ; Koo, D. C. ; Faber, S. M. ; Dekel, A. ; Primack, J. R. ; Kocevski, D. D. | IOP Publishing | 2017-12-20We present high spatial resolution (FWHM similar to 0."14) observations of the CO(8-7) line in GDS-14876, a compact star-forming galaxy at z = 2.3 with a total stellar mass of log(M-*/M-circle dot) = 10.9. The spatially resolved velocity map of [...]
