Clash: Z ~ 6 young galaxy candidate quintuply lensed by the frontier field cluster RXC J2248.7-4431

  • A. Monna
  • , S. Seitz
  • , N. Greisel
  • , T. Eichner
  • , N. Drory
  • , M. Postman
  • , A. Zitrin
  • , D. Coe
  • , A. Halkola
  • , S. H. Suyu
  • , C. Grillo
  • , P. Rosati
  • , D. Lemze
  • , I. Balestra
  • , J. Snigula
  • , L. Bradley
  • , K. Umetsu
  • , A. Koekemoer
  • , U. Kuchner
  • , L. Moustakas
  • M. Bartelmann, N. Benítez, R. Bouwens, T. Broadhurst, M. Donahue, H. Ford, O. Host, L. Infante, Y. Jimenez-Teja, S. Jouvel, D. Kelson, O. Lahav, E. Medezinski, P. Melchior, M. Meneghetti, J. Merten, A. Molino, J. Moustakas, M. Nonino, W. Zheng

Research output: Contribution to journalArticlepeer-review

57 Scopus citations

Abstract

We present a quintuply lensed z ~ 6 candidate discovered in the field of the galaxy cluster RXC J2248.7-4431 (z ~ 0.348) targeted within the Cluster Lensing and Supernova survey with Hubble (CLASH) and selected in the deep Hubble Space Telescope (HST) frontier fields survey. Thanks to the CLASH 16-band HST imaging, we identify the quintuply lensed z ~ 6 candidate as an optical dropout in the inner region of the cluster, the brightest image having magAB = 24.8 ± 0.1 in the f105w filter. We perform a detailed photometric analysis to verify its high-z and lensed nature. We get as photometric redshift zph ~ 5.9, and given the extended nature and NIR colours of the lensed images, we rule out low-z early-type and galactic star contaminants.We perform a strong lensing analysis of the cluster, using 13 families of multiple lensed images identified in the HST images. Our final best model predicts the high-z quintuply lensed system with a position accuracy of 0.8 arcsec. The magnifications of the five images are between 2.2 and 8.3, which leads to a delensedUVluminosity of L1600 ~ 0.5L * 1600 at z=6.We also estimate the UV slope from the observed NIR colours, finding a steep β =-2.89 ± 0.38. We use singular and composite stellar population SEDs to fit the photometry of the high-z candidate, and we conclude that it is a young (age<300 Myr) galaxy with mass ofM~108 M, subsolar metallicity (Z < 0.2 Z) and low dust content (AV ~ 0.2-0.4).

Original languageEnglish (US)
Pages (from-to)1417-1434
Number of pages18
JournalMonthly Notices of the Royal Astronomical Society
Volume438
Issue number2
DOIs
StatePublished - Mar 2014
Externally publishedYes

All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics
  • Space and Planetary Science

Keywords

  • Galaxies: clusters: general
  • Galaxies: high-redshift
  • Gravitational lensing: strong

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