Structure Formation and Cosmology with high-z Clusters
Lecture4 - USP
Lecture4 - USP
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Typical LBG LBG C<strong>and</strong>idate Selection SelectionLyman Break Color! Select galaxies in• “Drop-out color-color galaxies” diagramselected in color-color! Require non-detectiondiagramin optical b<strong>and</strong>s• Require non-detection in! (deep) Potential optical b<strong>and</strong>• Potential Contaminants: contaminants:SNe, Supernovae cool stars,photometric Cool Galactic scatter, starsspurious Photometric detections scatterPotential Issues:Missing filtersSpurious optical detectionsRest-frame UV Continuum ColorBowensBouwenset al.et al.2011(2011)