Journal
ASTROPHYSICAL JOURNAL LETTERS
Volume 716, Issue 2, Pages L152-L156Publisher
IOP PUBLISHING LTD
DOI: 10.1088/2041-8205/716/2/L152
Keywords
galaxies: clusters: individual; galaxies: luminosity function, mass function; X-rays: galaxies: clusters
Categories
Funding
- World Premier International Research Center Initiative (WPI Initiative), MEXT, Japan
- National Astronomical Observatory of Japan [S09B-042]
Ask authors/readers for more resources
We report on a confirmed galaxy cluster at z = 1.62. We discovered two concentrations of galaxies at z similar to 1.6 in the Subaru/XMM-Newton deep field based on deep multi-band photometric data. We made a near-IR spectroscopic follow-up observation of them and confirmed several massive galaxies at z = 1.62. One of the two is associated with an extended X-ray emission at 4.5 sigma on a scale of 0'.5, which is typical of high-z clusters. The X-ray detection suggests that it is a gravitationally bound system. The other one shows a hint of an X-ray signal, but only at 1.5 sigma, and we obtained only one secure redshift at z = 1.62. We are not yet sure if this is a collapsed system. The possible twins exhibit a clear red sequence at K < 22 and seem to host relatively few number of faint red galaxies. Massive red galaxies are likely old galaxies-they have colors consistent with the formation redshift of z(f) = 3, and a spectral fit of the brightest confirmed member yields an age of 1.8(-0.2)(+0.1) Gyr with a mass of 2.5(-0.1)(+0.2) x 10(11) M-circle dot. Our results show that it is feasible to detect clusters at z > 1.5 in X-rays and also to perform detailed analysis of galaxies in them with the existing near-IR facilities on large telescopes.
Authors
I am an author on this paper
Click your name to claim this paper and add it to your profile.
Reviews
Recommended
No Data Available