Author/Authors :
Daniel Stern، نويسنده , , S. A. Stanford، نويسنده , , Peter R. Eisenhardt، نويسنده , , Mark Brodwin، نويسنده , , Anthony H. Gonzalez، نويسنده , , B. T. Jannuzi، نويسنده , , Arjun Dey، نويسنده , , Michael J. I. Brown، نويسنده , , Eric McKenzie، نويسنده , , Richard Elston، نويسنده ,
Abstract :
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 1.3 < z < 1.5. Optical spectroscopy of a limited number of objects in the region shows that five galaxies within an 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.
Keywords :
Formation , general , Evolution , galaxies , Clusters
