Bibcode
Hempel, A.; Schaerer, D.; Egami, E.; Pelló, R.; Wise, M.; Richard, J.; Le Borgne, J.-F.; Kneib, J.-P.
Bibliographical reference
Astronomy and Astrophysics, Volume 477, Issue 1, January I 2008, pp.55-66
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1
2008
Journal
Citations
5
Refereed citations
4
Description
Aims:We study the properties and nature of extremely red galaxies (ERO,
R-K≥5.6) found behind two lensing clusters and compare them with
other known galaxy populations. Methods: New HST/ACS, Spitzer
(IRAC and MIPS), and Chandra/ACIS observations of the two lensing
clusters Abell 1835 and AC114 have been obtained, combined with our
earlier optical and near-IR observations and used to study EROs in these
deep fields. Results: We have found 6 and 9 EROs in Abell 1835 and
AC114. Several (7) of these objects are undetected up to the I and/or
z850 band, and are hence “optical” drop-out
sources (at a 3σ limit). The photometric redshifts of most of our
sources (80%) are z˜ 0.7-1.5. According to simple colour-colour
diagrams, the majority of our objects would be classified as hosting old
stellar populations (“ellipticals”). However, there are
clear signs of dusty starbursts for several among them. These objects
correspond to the most extreme ones in R-K colour. After correcting for
lens magnification, we estimate a surface density of (0.97±0.31)
arcmin-2 for EROs with (R-K ≥ 5.6) at K<20.5. As in
earlier studies, an overlap of different populations is found. Among our
15 EROs 6 (40%) also classify as distant red galaxies. Eleven of 13 EROs
(85%) with available IRAC photometry also fulfil the selection criteria
for IRAC selected EROs (IEROs) of Yan et al. (2004, ApJ, 616, 63). SED
modelling shows that ~36% of the IEROs in our sample are luminous or
ultra-luminous infrared galaxies ((U)LIRG). Some very red DRGs are found
to be very dusty starbursts, even (U)LIRGs. No AGNs is found, although
faint activity cannot be excluded for all objects. From mid-IR and X-ray
data, 5 objects are clearly classified as starbursts. The derived
properties are quite similar to those of DRGs and IEROs, except for 5
extreme objects in terms of colours, for which a very high extinction
(AV ⪆ 3) is found.
Tables 1-6 are only available in electronic form at http://www.aanda.org
Based on observations collected at the Very Large Telescope (Antu/UT1),
European Southern Observatory, Paranal, Chile (ESO Programs 69.A-0508,
70.A-0355, 73.A-0471), the NASA/ESA Hubble Space Telescope obtained at
the Space Telescope Science Institute which is operated by AURA under
NASA contract NAS5-26555, the Spitzer Space Telescope, which is operated
by the Jet Propulsion Laboratory, California Institute of Technology
under NASA contract 1407, and the Chandra satellite.