Massive deep-frozen bone allografts : contamination, immunogenicity and clinical use
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GERELATEERDE DOCUMENTEN
License: Licence agreement concerning inclusion of doctoral thesis in the Institutional Repository of the University of
License: Licence agreement concerning inclusion of doctoral thesis in the Institutional Repository of the University of Leiden Downloaded from: https://hdl.handle.net/1887/3765.
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Studies of the stellar composition, using optical and near-infrared broadband photometry, reinforced this picture of relatively low- mass, moderately star forming objects (Sawicki
2 Ultradeep NIR ISAAC observations of the HDF-South: observations, reduction, multicolor catalog, and photometric redshifts Furthermore, the predicted color correction is small
-A steep galaxy mass function at high redshift: if much of the U V light which is used to measure the SFR at high redshifts comes from small galaxies which would fall below
We focus on the galaxies that populate the blue peak of galaxies at low and high redshift. We wish to understand the nature of the blue color-magnitude relation, the evolution of
Figure 3 — The range in best-fit extinction and age values of various DRGs, for constant star forming models (Bruzual & Charlot 2003) including dust Calzetti et al (2000).. We
