MODERN COSMOLOGY

Galaxy surveys 327 Figure 11.4.Measurement of the LF at different redshifts from the CFRS survey (Lilly et al1995). The redshift ...

328 Highlights in modern observational cosmology Figure 11.5.Number counts for different morphological types as derived from the ...

Galaxy surveys 329 Figure 11.6.Evolution of the spectral energy distribution (SED) of a stellar population modelled as a star fo ...

330 Highlights in modern observational cosmology Figure 11.7.Illustration of the Lyman break (‘drop-out’) technique in the HDF-N ...

Galaxy surveys 331 Giavaliscoet al1998) in the universe back to epochs which represent only 20% of the cosmic time (e.g. Steidel ...

332 Highlights in modern observational cosmology Figure 11.8.Illustration of the photometric redshift technique on a variety of ...

Galaxy surveys 333 Figure 11.9.Comparison between the spectroscopic redshift (zspec) and the photometric redshift (zB) in the HD ...

334 Highlights in modern observational cosmology Figure 11.10.Linking the star formation rate (SFR) to the UV luminosity (L 1500 ...

Cluster surveys 335 Figure 11.11. History of the star formation rate (SFR) in the universe (∼80% of the cosmic time): SFR densit ...

336 Highlights in modern observational cosmology Figure 11.12. Evolution of the cosmic structure (projected mass distribution) f ...

Cluster surveys 337 figure 11.12 shows indeed less structure atz=3intheCDM model when compared with OCDM). One of the fundament ...

338 Highlights in modern observational cosmology sensitivity does not depend on redshift. This will possibly be one of the most ...

Cluster surveys 339 Figure 11.13. The best determination to date of the cluster x-ray luminosity function (i.e. the cluster spac ...

340 Highlights in modern observational cosmology Figure 11.14.Constraints in the plane of the cosmological parameters
m−σ 8 deri ...

Cluster surveys 341 Figure 11.15. Constraints to
mand
from CMB anisotropies (Boomerang: De Bernardiset al2000; Maxima: Hananyet ...

342 Highlights in modern observational cosmology scales (see the chapter by Arthur Kosowsky in this volume). The power of these ...

References 343 Hubble E 1926Astrophys. J. 64321 Huchra J P, Geller M J, de Lapparant V and Corwin H G 1990Astrophys. J. Suppl. 4 ...

Chapter 12 Clustering in the universe: from highly nonlinear structures to homogeneity Luigi Guzzo Osservatorio Astronomico di B ...

The clustering of galaxies 345 Figure 12.1.The distribution of the nearly 140 000 galaxies observed so far (September 2000) in t ...

346 Clustering in the universe Figure 12.2. The two-point correlation function of galaxies, as measured from a few representativ ...