I am currently analyzing the emission line spectra of the approximately 600
galaxies from the sample of Cohen et al. (2000) and Cohen (2001) in the region
of the HDF-North with z<1.5. A progress report on this effort of the Caltech
Faint Galaxy Redshift Survey is presented.Comment: For the proceedings of the meeting held in Cozumel, March 2002 on
Galaxy Evolution: Theory and Observations, to be edited by V. Avila-Reese, C.
Firmani, C. Frenk, & C. Allen, RevMexAA SC (2002
