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A small fraction of the atomic-cooling halos assembling at z<15 may form outof minihalos that never experienced any prior star formation, and could inprinciple host small galaxies of chemically unenriched stars. Since theprospects of detecting isolated population III stars appear bleak even with theupcoming James Webb Space Telescope (JWST), these population III galaxies mayoffer one of the best probes of population III stars in the foreseeable future.By projecting the results from population III galaxy simulations throughcluster magnification maps, we predict the fluxes and surface number densitiesof pop III galaxy galaxies as a function of their typical star formationefficiency. We argue that a small number of lensed population III galaxies inprinciple could turn up at z=7-10 in the ongoing Hubble Space Telescope surveyCLASH, which covers a total of 25 low-redshift galaxy clusters.

Detecting population III galaxies with HST and JWST