TY - JOUR
T1 - Young Galaxy Candidates in the Hubble Frontier Fields. IV. MACS J1149.5+2223
AU - Zheng, Wei
AU - Zitrin, Adi
AU - Infante, Leopoldo
AU - Laporte, Nicolas
AU - Huang, Xingxing
AU - Moustakas, John
AU - Ford, Holland C.
AU - Shu, Xinwen
AU - Wang, Junxian
AU - Diego, Jose M.
AU - Bauer, Franz E.
AU - Iribarren, Paulina Troncoso
AU - Broadhurst, Tom
AU - Molino, Alberto
N1 - Publisher Copyright: © 2017. The American Astronomical Society. All rights reserved.
PY - 2017/2/20
Y1 - 2017/2/20
N2 - 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., 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 , and was formed at 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 , approximately a factor of 10 deeper than the parallel fields.
AB - 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., 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 , and was formed at 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 , approximately a factor of 10 deeper than the parallel fields.
KW - cosmology: observations
KW - galaxies: clusters: individual (MACS J1149.5+2223)
KW - galaxies: highredshift
KW - gravitational lensing: strong
UR - http://www.scopus.com/inward/record.url?scp=85014345394&partnerID=8YFLogxK
U2 - 10.3847/1538-4357/aa5d55
DO - 10.3847/1538-4357/aa5d55
M3 - Article
SN - 0004-637X
VL - 836
JO - Astrophysical Journal
JF - Astrophysical Journal
IS - 2
M1 - 210
ER -