CL0024+1652 as seen by the Galaxy Cluster Evolution survey (GLACE)

Bibcode
2013AN....334..458P
DOI
10.1002/asna.201211880
Pérez-Martínez, R.; Sánchez-Portal, M.; Pintos-Castro, I.; Pérez-García, A. M.; Cepa, J.; GLACE Team
Bibliographical reference

Astronomische Nachrichten, Vol.334, Issue 4-5, p.458

Advertised on:
4
2013
Number of authors
6
IAC number of authors
3
Citations
2
Refereed citations
2
Description
The GaLAxy Cluster Evolution survey (GLACE) is aimed to study the evolution of emission line galaxies in clusters across the cosmic time. It takes advantage of the tunable filter mode of OSIRIS (first light instrument of GTC) to scan Hα/[N II], Hβ, [O II] 3727 and [O III] 5007 searching for star formation activity and AGNs in clusters in three different redshift windows ({z˜ 0.40}, 0.63, and 0.86), providing a unique view of the evolution of cluster galaxies along such redshift range. Moreover, the OSIRIS large field of view (8{×}8 arcmin2) together with GTC large collective area ({D˜ 10 m}) make it possible to detect SFR ˜ 2 M_ȯ yr-1 in an angular area up to 2R_vir. We present here the first results of the program together with a brief description of this novel technique focusing in the cluster CL0024+1654 (z ˜ 0.39).
Related projects
Project Image
Evolution of Galaxies

Galaxy evolution is a crucial topic in modern extragalactic astrophysics, linking cosmology to the Local Universe. Their study requires collecting statistically significant samples of galaxies of different luminosities at different distances. It implies the ability to observe faint objects using different techniques, and at different wavelengths

Jorge
Cepa Nogue
In progress
Type
Refereed
Galaxies
Surveys
Techniques
Formation & Evolution of Galaxies (FYEG)

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