here - Institute for Astronomy Umleitung
here - Institute for Astronomy Umleitung
here - Institute for Astronomy Umleitung
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Title: Science Case<br />
Reference: MUSE-MEM-SCI-052<br />
Issue: 1.3<br />
Date: 04/02/2004<br />
Page: 23/100<br />
Preparation). This extends the results from Moller & Fynbo (2001) to z=3. The peak in PDF<br />
at higher fluxes corresponds roughly to the values calculated in Figure 2-8, supporting the<br />
idea that large areas may ‘light up’ if these surface brightnesses can be detected.<br />
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