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          Institute: MPI für Astronomie     Collection: Publikationen_mpia     Display Documents



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ID: 559163.0, MPI für Astronomie / Publikationen_mpia
Optical and near-IR spectroscopy of candidate red galaxies in two z ~ 2.5 proto-clusters
Authors:Doherty, M.; Tanaka, M.; De Breuck, C.; Ly, C.; Kodama, T.; Kurk, J.; Seymour, N.; Vernet, J.; Stern, D.; Venemans, B.; Kajisawa, M.; Tanaka, I.
Language:English
Date of Publication (YYYY-MM-DD):2010
Title of Journal:Astronomy and Astrophysics
Journal Abbrev.:A&A
Volume:509
Start Page:id.A83
Review Status:Peer-review
Audience:Experts Only
Abstract / Description:We present a spectroscopic campaign to follow-up red colour-selected candidate massive galaxies in two high redshift proto-clusters surrounding radio galaxies. We observed a total of 57 galaxies in the field of MRC 0943-242 (z=2.93) and 33 in the field of MRC 1138-262 (z=2.16) with a mix of optical and near-infrared multi-object spectroscopy. We confirm two red galaxies in the field of MRC 1138-262 at the redshift of the radio galaxy. Based on an analysis of their spectral energy distributions, and their derived star formation rates from the Hα and observed frame 24 μm flux, one object belongs to the class of dust-obscured star-forming red galaxies, while the other is evolved with little ongoing star formation. This result represents the first red and mainly passively evolving galaxy to be confirmed as companion galaxies in a z>2 proto-cluster. Both red galaxies in MRC 1138-262 are massive, of the order of 4-6 × 1011~Mȯ. They lie along a colour-magnitude relation which implies that they formed the bulk of their stellar population around z=4. In the MRC 0943-242 field we find no red galaxies at the redshift of the radio galaxy but we do confirm the effectiveness of our JHK_s selection of galaxies at 2.3<z<3.1, finding that 10 out of 18 (56%) of JHK_s-selected galaxies whose redshifts could be measured fall within this redshift range. We also serendipitously identify an interesting foreground structure of 6 galaxies at z=2.6 in the field of MRC 0943-242. This may be a proto-cluster itself, but complicates any interpretation of the red sequence build-up in MRC 0943-242 until more redshifts can be measured. Based in part on data collected at Subaru Telescope, which is operated by the National Astronomical Observatory of Japan, and in part on data collected with ESO's Very Large Telescope UT1/Antu, under program ID 080.A-0463(B), and with the VLT/Melipal telescope during the first X-shooter commissioning run, and ESO's New Technology Telescope under program ID 076.A-0670(B).
Free Keywords:galaxies: clusters: individual: MRC 1138-262; galaxies: clusters: individual: MRC 0943-242; galaxies: evolution; galaxies: high-redshift; large-scale structure of Universe; infrared: galaxies
External Publication Status:published
Document Type:Article
Communicated by:N. N.
Affiliations:MPI für Astronomie
Identifiers:URL:http://adsabs.harvard.edu/abs/2010A%26A...509A..83... [ID No:1]
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