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Low-ionization galaxies and evolution in a pilot survey up to z=1

Research in Astronomy and Astrophysics 2011年第3期11卷 245-270页

作者： Edmond Giraud Qiu-Sheng Gu Jorge Melnick Hernan Quintana Fernando Selman Ignacio Toledo Paula Zelaya lpta Universit6 Montpellier 2 - CNRS/IN2P3 34095 Montpellier France edmond.giraud@ lpta. in2p3.fr Department of Astronomy Nanjing University Nanjing 210093 China European Southern Observatory /klonso de Cbrdova 3107 Santiago Chile Department of Astronomy and Astrophysics R Universidad Catolica de Chile Casilla 306Santiago Chile

We present galactic spectroscopic data from a pencil beam of 10.75×7.5 centered on the X-ray cluster RXJ0054.0–2823 at z=0.29.We study the spectral evolution of galaxies from z=1 down to the cluster redshift in a magnitude-limited sample at R≤23,for which the statistical properties of the sample are well understood.We divide emission-line galaxies into star-forming galaxies,Low Ionization Nuclear Emission line Regions（LINERs） ,and Seyferts by using emission-line ratios of[OII],Hβ,and[OIII],and derive stellar fractions from population synthesis models. We focus our analysis on absorption and low-ionization galaxies.For absorption-line galaxies,we recover the well-known result that these galaxies have had no detectable evolution since z～0.6-0.7,but we also find that in the range z=0.65-1,at least 50% of the stars in bright absorption systems are younger than 2.5 Gyr.Faint absorption-line galaxies in the cluster at z=0.29 also had significant star formation during the previous 2-3 Gyr,but their brighter counterparts seem to be only composed of old stars.At z～0.8,our dynamically young cluster had a truncated red-sequence.This result seems to be consistent with a scenario where the final assembly of E/S0 took place at z1.In the volume-limited range 0.35≤z≤0.65,we find that 23% of the early-type galaxies have LINER-like spectra with Hβin absorption and have a significant component of A stars.The vast majority of LINERs in our sample have significant populations of young and intermediate-aged stars and are thus not related to AGNs,but to the population of‘retired galaxies’recently identified by Cid Fernandes et al.in the Sloan Digital Sky Survey（SDSS） .Early-type LINERs with various fractions of A stars and E＋A galaxies appear to play an important role in the formation of the red sequence.

关键词： cosmology：observations—galaxies：evolution—large scale structures —evolution—RX J0054.0–2823

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