{ "id": "1701.08484", "version": "v1", "published": "2017-01-30T05:22:46.000Z", "updated": "2017-01-30T05:22:46.000Z", "title": "Young Galaxy Candidates in the Hubble Frontier Fields IV. MACS J1149.5+2223", "authors": [ "W. Zheng", "A. Zitrin", "L. Infante", "N. Laporte", "X. X. Huang", "J. Moustakas", "H. C. Ford", "X. W. Shu", "J. X. Wang", "J. M. Diego", "F. E. Bauer", "P. T. Iribarren", "T. Broadhurst", "A. Molino" ], "comment": "To appear in the Astrophysical Journal. 14 pages, 6 figures, 3 tables", "categories": [ "astro-ph.GA", "astro-ph.CO" ], "abstract": "We search for high-redshift dropout galaxies behind the Hubble Frontier Fields (HFF) galaxy cluster MACS J1149.5+2223, a powerful cosmic lens that has revealed a number of unique objects in its field. Using the deep images from the Hubble and Spitzer space telescopes, we find 11 galaxies at z>7 in the MACS J1149.5+2223 cluster field, and 11 in its parallel field. The high-redshift nature of the bright z~9.6 galaxy MACS1149-JD, previously reported by Zheng et al. (2012), is further supported by non-detection in the extremely deep optical images from the HFF campaign. With the new photometry, the best photometric redshift solution for MACS1149-JD reduces slightly to z=9.44 +/- 0.12. The young galaxy has an estimated stellar mass of (7 +/- 2)X10E8 Msun, and was formed at z=13.2 +1.9-1.6 when the Universe was ~300 Myr old. Data available for the first four HFF clusters have already enabled us to find faint galaxies to an intrinsic magnitude of M(UV) ~ -15.5, approximately a factor of ten deeper than the parallel fields.", "revisions": [ { "version": "v1", "updated": "2017-01-30T05:22:46.000Z" } ], "analyses": { "keywords": [ "hubble frontier fields", "young galaxy candidates", "parallel field", "best photometric redshift solution", "spitzer space telescopes" ], "note": { "typesetting": "TeX", "pages": 14, "language": "en", "license": "arXiv", "status": "editable" } } }