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Large Equivalent Width of Lyα Emitters<br />
Lyα Equivalent Width<br />
~ Lyα Line Luminosity<br />
/ Adjacent Top Continuum heavy IMF x=0.5<br />
Luminosity i per wavelength<br />
~ Number of Ionizing<br />
~240Å<br />
Photon / Non‐Ionizing Photon<br />
(for Photo Ionization)<br />
Salpeter IMF x=2.35<br />
Constant Continuous SF, 1/20 Z solar<br />
M l =1 M sun , M u =120 M sun<br />
Shimasaku+06<br />
Z=5.7 LAE<br />
Malhotra et sl. 2002; Charlot and Fall 1993