The Evolution of the Galaxy Sizes in the NTT Deep Field: a Comparison with CDM Models

Details The Evolution of the Galaxy Sizes in the NTT Deep Field: a Comparison with CDM Models The Evolution of the Galaxy Sizes in the NTT Deep Field: a Comparison with CDM Models

1999-10-29

arxiv.org/abs/astro-ph/9910537v1

Astronomy and Astrophysics

Astrophysics

16 pages, 11 figures, ApJ in press, Dec 1999

Scientific paper

10.1086/308122

The sizes of the field galaxies with I<25 have been measured in the NTT Deep Field. Intrinsic sizes have been obtained after deconvolution of the PSF with a multigaussian method. The reliability of the method has been tested using both simulated data and HST observations of the same field. The distribution of the half light radii is peaked at r_{hl} 0.3 arcsec, in good agreement with that derived from HST images at the same magnitude. An approximate morphological classification has been obtained using the asymmetry and concentration parameters. The intrinsic sizes of the galaxies are shown as a function of their redshifts and absolute magnitudes using photometric redshifts derived from the multicolor catalog. While the brighter galaxies with morphological parameters typical of the normal spirals show a flat distribution in the range r_{d}=1-6 kpc, the fainter population at 0.4

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