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We present the results of a spectroscopic survey with the Keck I telescope ofmore than 280 star-forming galaxies and AGN at redshifts 1.4<z<3.0 in theGOODS-N field. Candidates are selected by their UGR colors using the ``BM/BX''criteria to target redshift 1.4<z<2.5 galaxies and the LBG criteria to targetredshift z~3 galaxies; combined these samples account for ~25-30% of the R andK-band counts to R=25.5 and K(AB)=24.4, respectively. The sample of 212 BM/BXgalaxies and 74 LBGs is presently the largest spectroscopic sample of galaxiesat z>1.4 in GOODS-N. Extensive multi-wavelength data allow us to investigatethe stellar populations, stellar masses, bolometric luminosities (L_bol), andextinction of z~2 galaxies. Deep Chandra and Spitzer data indicate that thesample includes galaxies with a wide range in L_bol, from 10^10 L_sun to >10^12L_sun, and covering 4 orders of magnitude in dust obscuration (L_bol/L_UV). Thesample includes galaxies with a large dynamic range in evolutionary state, fromvery young galaxies (ages <50 Myr) with small stellar masses (M* ~ 10^9 M_sun)to evolved galaxies (ages >2 Gyr) with stellar masses comparable to the mostmassive galaxies at these redshifts (M* > 10^11 M_sun). Spitzer data indicatethat the optical sample includes some fraction of the obscured AGN populationat high redshifts: at least 3 of 11 AGN in the z>1.4 sample are undetected inthe deep X-ray data but exhibit power-law SEDs longward of ~2 micron(rest-frame) indicative of obscured AGN. The results of our survey indicatethat rest-frame UV selection and spectroscopy presently constitute the mosttime-wise efficient method of culling large samples of high redshift galaxieswith a wide range in intrinsic properties, and the data presented here will addsignificantly to the multi-wavelength legacy of the GOODS survey. [Abridged]Comment: 25 pages, 5 figures, 5 tables; accepted for publication in Ap

A Spectroscopic Survey of Redshift 1.4≲z≲3.0 Galaxies in the GOODS‐North Field: Survey Description, Catalogs, and Properties