부산대학교 도서관

We report the discovery using Hubble Space Telescope imaging and Keck spectroscopy of a very bright, highly magnified (~30*) Lyman Break Galaxy (LBG) at z=3.07 in the field of the massive z=0.33 cluster MACSJ2135.2-0102. The system comprises two high-surface brightness arcs with a maximum extent of 3", bracketing a central object which we identify as a massive early-type galaxy at z=0.73. We construct a lens model which reproduces the main features of the system using a combination of a galaxy-scale lens and the foreground cluster. We show that the morphological, spectral and photometric properties of the arcs are consistent with them arising from the lensing of a single ~L* LBG. The most important feature of this system is that the lensing magnification results in an apparent magnitude of r=20.3, making this one of the brightest LBGs known. Such a high magnification provides the opportunity of obtaining very high signal to noise (and potentially spatially resolved) spectroscopy of a high redshift galaxy to study its physical properties. We present initial imaging and spectroscopy demonstrating the basic properties of the system and discuss the opportunities for future observations.
Comment: In press at ApJL, 4 pages, 2 figures