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Deep Near-Infrared Spectroscopy of Passively Evolving Galaxies at Z & 1.4^1
Astrophysical Journal (2011)
  • M. Onodera
  • A. Renzini
  • M. Carollo
  • M. Cappellari
  • C. Mancini
  • V. Strazzullo
  • E. Daddi
  • N. Arimoto
  • R. Gobat
  • Y. Yamada
  • H. J. McCracken
  • O. Ilbert
  • P. Capak
  • A. Cimatti
  • Mauro Giavalisco, University of Massachusetts - Amherst
  • M. Giavalisco
  • A. M. Koekemoer
  • X. Kong
  • S. Lilly
  • K. Motohara
  • K. Ohta
  • D. B. Sanders
  • N. Scoville
  • N. Tamura
  • Y. Taniguchi
We present the results of new near-IR spectroscopic observations of passive galaxies at z & 1.4 in a concentration of BzK-selected galaxies in the COSMOS field. The observations have been conducted with Subaru/ MOIRCS, and have resulted in absorption lines and/or continuum detection for 18 out of 34 objects. This allows us to measure spectroscopic redshifts for a sample that is almost complete to KAB = 21. COSMOS photometric redshifts are found in fair agreement overall with the spectroscopic redshifts, with a standard deviation of ∼ 0.05; however, ∼ 30% of objects have photometric redshifts systematically underestimated by up to ∼ 25%. We show that these systematic offsets in photometric redshifts can be removed by using these objects as a training set. All galaxies fall in four distinct redshift spikes at z = 1.43, 1.53, 1.67 and 1.82, with this latter one including 7 galaxies. SED fits to broad-band fluxes indicate stellar masses in the range of ∼ 4–40×1010M⊙ and that star formation was quenched ∼ 1 Gyr before the cosmic epoch at which they are observed. The spectra of several individual galaxies have allowed us to measure their HδF indices and the strengths of the 4000 Å break, which confirms their identification as passive galaxies, as does a composite spectrum resulting from the coaddition of 17 individual spectra. The effective radii of the galaxies have been measured on the COSMOS HST/ACS iF814W-band image, confirming the coexistence at these redshifts of passive galaxies which are substantially more compact than their local counterparts with others that follow the local effective radius-stellar mass relation. For the galaxy with best S/N spectrum we were able to measure a velocity dispersion of 270±105 km s-1 (error bar including systematic errors), indicating that this galaxy lies closely on the virial relation given its stellar mass and effective radius.
  • galaxies: evolution,
  • galaxies: formation,
  • galaxies: high-redshift
Publication Date
Publisher Statement
This paper was harvested from and ArXiv identifier is arXiv:1206.1540
Citation Information
M. Onodera, A. Renzini, M. Carollo, M. Cappellari, et al.. "Deep Near-Infrared Spectroscopy of Passively Evolving Galaxies at Z & 1.4^1" Astrophysical Journal (2011)
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