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Detailed Properties of High Redshift Galaxies

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Figure 1.1:Star formation density of the universe sinceaxis. The density of star formation peaked during the redshift rangeformation density is derived from measurements of the ultraviolet luminosity density, shown on the rightthe star formation density as
Figure 1.3:Evolution in the mass-metallicity relation with redshift.Solid lines are empirical fits byMaiolino et al
Figure 2.1: True color ACS images of the sample derived from the multi-band data referred to in Table 2.1.The xy scale is in arcseconds
Figure 2.2: Source plane properties of the lensed galaxy sample. From left to right in each row: ACS broad-band emission, line intensity, velocity, and velocity dispersion derived from the OSIRIS nebular emissionline data
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Kinematic Modeling Cl 0024+1709 Conclusions Introduction Emission Line Fitting Discussion A Fundamental Metallicity Relation? Low-Ionization Metal Transitions High-Ionization Lines Implications for Reionization

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