Evolution of the frequency of luminous (≥L* v) close galaxy pairs at z < 1.2 in the COSMOS field

J. S. Kartaltepe, D. B. Sanders, N. Z. Scoville, D. Calzetti, P. Capak, A. Koekemoer, B. Mobasher, T. Murayama, M. Salvato, S. S. Sasaki, Y. Taniguchi

研究成果: Article査読

132 被引用数 (Scopus)

抄録

We measure the fraction of luminous galaxies in pairs at projected separations of 5-20 kpc out to z = 1.2 in the Cosmic Evolution Survey (COSMOS) field using ACS images and photometric redshifts derived from an extensive multiwavelength data set. Analysis of a complete sample of 106,188 galaxies more luminous than My = -1.9.8 (∼L* V) in the redshift range 0.1 < z < 1.2 yields 1749 galaxy pairs. These data are supplemented by a local (z = 0-0.1)value for the galaxy pair fraction derived from the Sloan Digital Sky Survey. After statistically correcting the COSMOS pair sample for chance line-of-sight superpositions, the evolution in the pair fraction is fit by a power law ∝(1 + z) n=3.1*0.1. If this strongly evolving pair fraction continues out to higher redshift, ∼50% of all luminous galaxies at z ∼ 2 are in close pairs. This clearly signifies that galaxy mergers are a very significant and possibly dominant mechanism for galaxy evolution during the epoch of galaxy formation at z = 1-3.

本文言語English
ページ(範囲)320-328
ページ数9
ジャーナルAstrophysical Journal, Supplement Series
172
1
DOI
出版ステータスPublished - 2007

ASJC Scopus subject areas

  • 天文学と天体物理学
  • 宇宙惑星科学

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