The evolutionary paths among galaxy types on the Red Sequence at 0.3 < Z < 1.5

M. C. Eliche-Moral, M. Prieto, M. Balcells, D. Abreu, G. Barro, D. Cristóbal-Hornillos, L. Domínguez Palmero, P. Erwin, J. Gallego, R. Guzán, A. Hempel, C. López-Sanjuan, P. G. Pérez-González, J. Zamorano

Research output: Contribution to journalArticlepeer-review


We have studied the main evolutionary paths among the galaxy types residing on the massive end of the Red Sequence and nearby locations on the Green Valley during the last ∼9 Gyr. The morphological and star formation properties of a sample of these galaxies at 0.3 < z < 1.5 with stellar masses M * > 5 × 1010 M have been analysed. We present direct observational evidence for the first time of the existence of two main evolutionary paths among the different red galaxy types since z ∼ 1.5, which provide some clues on the nature of the processes that have governed the assembly of present-day massive quiescent galaxies. The results are in excellent agreement with the hierarchical evolutionary framework proposed in the Eliche-Moral et al. (2010) model. Data from SHARDS (one of the ESO/GTC Large Programmes approved in 2009A) will complement and improve the present findings, shedding some light into many of the still unsettled questions concerning the migration of galaxies from the Blue Cloud to the Red Sequence at z < 1.5.

Original languageEnglish
Pages (from-to)24-25
Number of pages2
JournalRevista Mexicana de Astronomia y Astrofisica: Serie de Conferencias
Publication statusPublished - 2013


  • CD
  • Galaxies: Elliptical and lenticular
  • Galaxies: Evolution
  • Galaxies: Formation
  • Galaxies: Interactions
  • Galaxies: Luminosity function
  • Mass function

ASJC Scopus subject areas

  • Space and Planetary Science
  • Astronomy and Astrophysics


Dive into the research topics of 'The evolutionary paths among galaxy types on the Red Sequence at 0.3 < Z < 1.5'. Together they form a unique fingerprint.

Cite this