High redshift evolution of optically and IR-selected galaxies: A Comparison with CDM scenarios - INSPIRE

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High redshift evolution of optically and IR-selected galaxies: A Comparison with CDM scenarios

Adriano Fontana
(
- Rome Observ. and
- European Southern Observ. and
- Padua U., Astron. Dept. and
- ST-ECF, Garching and
- Brera Observ.
)
,
Nicola Menci
(
- Rome Observ. and
- European Southern Observ. and
- Padua U., Astron. Dept. and
- ST-ECF, Garching and
- Brera Observ.
)
,
Sandro D'Odorico
(
- Rome Observ. and
- European Southern Observ. and
- Padua U., Astron. Dept. and
- ST-ECF, Garching and
- Brera Observ.
)
,
Emanuele Giallongo
(
- Rome Observ. and
- European Southern Observ. and
- Padua U., Astron. Dept. and
- ST-ECF, Garching and
- Brera Observ.
)
,
Francesco Poli
(
- Rome Observ. and
- European Southern Observ. and
- Padua U., Astron. Dept. and
- ST-ECF, Garching and
- Brera Observ.
)

Sep, 1999

7 pages

Published in:

Mon.Not.Roy.Astron.Soc. 310 (1999) L27

e-Print:

astro-ph/9909126 [astro-ph]

DOI:

10.1046/j.1365-8711.1999.03152.x

Report number:

ESO-1346

View in:

ADS Abstract Service

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Abstract: (arXiv)

A combination of ground-based (NTT and VLT) and HST (HDF-N and HDF-S) public imaging surveys have been used to collect a sample of 1712 I-selected and 319

K\leq 21

galaxies. Photometric redshifts have been obtained for all these galaxies. The results have been compared with the prediction of an analytic rendition of the current CDM hierarchical models for galaxy formation. We focus in particular on two observed quantities: the galaxy redshift distribution at K<21 and the evolution of the UV luminosity density. The derived photometric redshift distribution is in agreement with the hierarchical CDM prediction, with a fraction of only 5% of galaxies detected at z>2. This result strongly supports hierarchical scenarios where present-day massive galaxies are the result of merging processes. The observed UV luminosity density in the I-selected sample is confined within a factor of 4 over the whole range 03. CDM models in

\Lambda

-dominated universe are in better agreement at 3

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