Published in Physics-Uspekhi, 48 (11), 1109-1127, 2005
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Translated by K.A. Postnov; edited by A.M. Semikhatov
astro-ph/0603154
Abstract. Selected results obtained in major observational sky surveys (DSS, 2MASS, 2dF, SDSS) and deep field observations (HDF, GOODS, HUDF, etc.) are reviewed. Modern surveys provide information on the characteristics and space distribution of millions of galaxies. Deep fields allow one to study galaxies at the stage of formation and to trace their evolution over billions of years. The wealth of observational data is altering the face of modern astronomy: the formulation of problems and their solutions are changing and all the previous knowledge, from planetary studies in the solar system to the most distant galaxies and quasars, is being revised.
Table of Contents
INTRODUCTION
GENERAL CHARACTERISTICS OF SURVEYS AND DEEP
FIELDS
SKY SURVEYS
Photographic surveys
APM
DSS and DPOSS
2MASS
2dF and 6dF
SDSS
DEEP FIELDS
WHDF
HDF
CDF
FDF
SDF and SXDS
COMBO-17
GOODS
HUDF
Other projects
SOME RESULTS
Galaxy counts
Galaxy distribution
Evolution of the luminosity function
Evolution of the galaxy structure
The most distant galaxies
History of star formation in the Universe
CONCLUSION
REFERENCES