A robust morphological classification of high-redshift galaxies using support vector machines on seeing limited images. II. Quantifying morphological k-correction in the COSMOS field at 1<z<2: Ks band vs. I band

M. Huertas-Company; L. Tasca; D. Rouan; D. Pelat; J. P. Kneib; O. Le Fevre; P. Capak; J. Kartaltepe; A. Koekemoer; H. J. McCracken; M. Salvato; D. B. Sanders; C. Willott

doi:10.1051/0004-6361/200811255

arXiv · 0811.1045

A robust morphological classification of high-redshift galaxies using support vector machines on seeing limited images. II. Quantifying morphological k-correction in the COSMOS field at 1<z<2: Ks band vs. I band

M. Huertas-Company·L. Tasca·D. Rouan·D. Pelat·J. P. Kneib·O. Le Fevre·P. Capak·J. Kartaltepe·A. Koekemoer·H. J. McCracken·M. Salvato·D. B. Sanders·C. Willott

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Abstract

We quantify the effects of \emph{morphological k-correction} at $1 1$ could be underestimating the elliptical population. [abridged]

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M. Huertas-Company, L. Tasca, D. Rouan, D. Pelat, J. P. Kneib, O. Le Fevre, P. Capak, J. Kartaltepe, A. Koekemoer, H. J. McCracken, M. Salvato, D. B. Sanders, C. Willott. 2009-02-24. A robust morphological classification of high-redshift galaxies using support vector machines on seeing limited images. II. Quantifying morphological k-correction in the COSMOS field at 1<z<2: Ks band vs. I band. https://doi.org/10.1051/0004-6361%2F200811255

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