Abstract
We report an on-going blank-field multi-wavelength deep and wide survey of the Subaru/XMM-Newton Deep Survey Field (SXDF). The SXDF has been the focus of a wide range of multi-wavelength observing programs spanning the X-ray to the radio. These observations cover a large enough area (the initial optical imaging covers ∼1.3 deg2) and depth (B = 28.2) that they are not affected by large-scale structures (which exist on tens of Mpc scales) and allow us to study the distribution and evolution of high-z galaxies and AGNs, and thus constrain theories for their formation. Our early results include: i) an indication of the primeval Large Scale Structure (LSS) at z ∼ 5.7, ii) an indication for the down-sizing of galaxy formation at z ∼ 1, iii) identifications of passively evolving systems, and evidence for early formation and the passive evolution of present-day early-type galaxies, and iv) discovery of a large number of optically obscured QSOs. As for the next step forward - we express our hope to use the next generation optical/IR Extremely Large Telescopes (ELTs) to obtain larger and deeper spectroscopy samples of the high-z objects.
Original language | English |
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Pages (from-to) | 171-175 |
Number of pages | 5 |
Journal | Proceedings of the International Astronomical Union |
Volume | 1 |
Issue number | S232 |
DOIs | |
Publication status | Published - 2005 |
Keywords
- Active
- Cosmology: large-scale structure
- Evolution
- Galaxies: distance and redshifts
ASJC Scopus subject areas
- Medicine (miscellaneous)
- Astronomy and Astrophysics
- Nutrition and Dietetics
- Public Health, Environmental and Occupational Health
- Space and Planetary Science