4.7 Article

An IR-selected galaxy cluster at z=1.41

Journal

ASTROPHYSICAL JOURNAL
Volume 634, Issue 2, Pages L129-L132

Publisher

IOP PUBLISHING LTD
DOI: 10.1086/499045

Keywords

galaxies : clusters : general; galaxies : evolution; galaxies : formation

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We report the discovery of a galaxy cluster at z = 1.41. ISCS J143809 + 341419 was found in the Spitzer/IRAC Shallow Survey of the Bootes field in the NOAO Deep Wide- Field Survey carried out using IRAC. The cluster candidate was initially identified as a high-density region of objects with photometric redshifts in the range 1.31 < z < 1.5. Optical spectroscopy of a limited number of objects in the region shows that five galaxies within an similar to 120 diameter region lie at z = 1.41 +/- 0.01. Most of these member galaxies have broadband colors consistent with the expected spectral energy distribution of a passively evolving elliptical galaxy formed at high redshift. The redshift of ISCS J143809 + 341419 is the highest currently known for a spectroscopically confirmed cluster of galaxies.

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