Abstract
We will review some recent advances in understanding the evolution of stellar populations in galaxies at relatively higher redshifts (z 0.5). We will focus on mass assembly, down-sizing and high-z zoo which have been among the most major topics and have seen great observational achievements in the past few years. In particular, wide-field near-infrared surveys, large spectroscopic surveys, and the Spitzer observations at infrared wavelengths, have unveiled underlying stellar masses and dusty star formation in high-z galaxies, which have been crucial in making such recent progresses.
| Original language | English |
|---|---|
| Pages (from-to) | 537-545 |
| Number of pages | 9 |
| Journal | Proceedings of the International Astronomical Union |
| Volume | 2 |
| Issue number | S241 |
| DOIs | |
| Publication status | Published - 2006 Dec |
| Externally published | Yes |
Keywords
- Cosmology: large-scale structure of universe
- Galaxies: clusters: general
- Galaxies: evolution
- Galaxies: formation
- Galaxies: high-redshift
- Galaxies: luminosity function
- Galaxies: stellar content
- Mass function
ASJC Scopus subject areas
- Astronomy and Astrophysics
- Space and Planetary Science