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We have identified galaxies near two quasars which are at the redshift ofdamped Lyman-alpha (DLA) systems in the UV spectra of the quasars. Bothgalaxies are actively forming stars. One galaxy has a luminosity close to thebreak in the local galaxy luminosity function, L*, the other is significantlyfainter than L* and appears to be interacting with a nearby companion. Despitethe strong selection effects favoring spectroscopic identification of the mostluminous DLA galaxies, many of the spectroscopically-identified DLA galaxies inthe literature are sub-L*, suggesting that the majority of the DLA populationis probably sub-L*, in contrast to MgII absorbers at similar redshifts whosemean luminosity is close to L*.Comment: 9 pages, to appear in AJ, November 2003 issu

Imaging and Spectroscopy of Galaxies Associated with Twoz~0.7 Damped Ly Absorption Systems