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

Details 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 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

2008-11-06

arxiv.org/abs/0811.1045v2

Astronomy and Astrophysics

Astrophysics

accepted for publication in A&A, updated with referee comments, 12 pages, 10 figures

Scientific paper

10.1051/0004-6361/200811255

We quantify the effects of \emph{morphological k-correction} at $11$ could be underestimating the elliptical population. [abridged]

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