Galaxy Evolution in a Pilot Survey up to z=1 and CDM Halos
We study spectral evolution of galaxies in a magnitude limited sample of 550 galaxies from z=1 down to z=0.3 on a pencil beam of ≈10′×10′. We concentrate on the large apparent cosmological structures along the line of sight, and we bin our individual galaxy spectra to obtain representative high S/N...
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Main Authors: | E. Giraud, J. Melnick, Q.-S. Gu, H. Quintana, F. Selman, I. Toledo, P. Zelaya |
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Format: | Article |
Language: | English |
Published: |
Wiley
2011-01-01
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Series: | Advances in Astronomy |
Online Access: | http://dx.doi.org/10.1155/2011/508381 |
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