The Mass-Luminosity Relation For Galaxies in the Deep Lens Survey
The Mass-Luminosity Relation For Galaxies in the Deep Lens Survey
The Mass-Luminosity Relation For Galaxies in the Deep Lens Survey
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Characterize <strong>the</strong> galaxy-dark matter<br />
connection<br />
by <strong>in</strong>vestigat<strong>in</strong>g, e.g., <strong>the</strong> M tot - L relation us<strong>in</strong>g<br />
lens<strong>in</strong>g to measure <strong>the</strong> total mass.<br />
Observational results have studied low redshift galaxies or <strong>the</strong> most<br />
massive galaxies at higher redshifts, but we can now extend <strong>the</strong> mass<br />
and redshift ranges with current deep and wide surveys.<br />
● Galaxy-galaxy weak lens<strong>in</strong>g (GGWL) background<br />
● Overview of <strong>the</strong> <strong>Deep</strong> <strong>Lens</strong> <strong>Survey</strong> (DLS)<br />
● GGWL signal b<strong>in</strong>ned by color and lum<strong>in</strong>osity<br />
● M tot - L relation<br />
● Summary and future outlook<br />
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