Spectroscopic Identification of Massive Galaxies at z~2.3 with Strongly Suppressed Star Formation

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Accepted for publication in ApJ Letters

Scientific paper

10.1086/508371

We present first results of a spectroscopic survey targeting K-selected galaxies at z=2.0-2.7 using the GNIRS instrument on Gemini-South. We obtained near-infrared spectra with a wavelength coverage of 1.0-2.5 micron for 26 K-bright galaxies (K<19.7) selected from the MUSYC survey using photometric redshifts. We successfully derived spectroscopic redshifts for all 26 galaxies using rest-frame optical emission lines or the redshifted Balmer/4000 Angstrom break. Twenty galaxies have spectroscopic redshifts in the range 2.0

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