4.7 Article

YOUNG GALAXY CANDIDATES IN THE HUBBLE FRONTIER FIELDS. II. MACS J0416-2403

Journal

ASTROPHYSICAL JOURNAL
Volume 815, Issue 1, Pages -

Publisher

IOP PUBLISHING LTD
DOI: 10.1088/0004-637X/815/1/18

Keywords

cosmology: observations; galaxies: clusters: individual (MACS0416); galaxies: high-redshift; gravitational lensing: strong

Funding

  1. Space Telescope Science Institute (STScI) [AR-13279]
  2. NASA [NAS 5-26555]
  3. Basal-CATA [PFB-06/2007, FP7-SPACE-2012-ASTRODEEP-312725]
  4. NSFC [11103017, 11233002]
  5. NASA - STScI [HST-HF2-51334.01-A]
  6. CONICYT-Chile [FONDECYT 1141218, FONDECYT 3140542, Gemini-CONICYT 32120003, Anillo ACT1101]
  7. Ministry of Economy, Development, and Tourism's Millennium Science Initiative [IC120009]
  8. Spanish consolider project [CAD2010-00064, AYA2012-39475-C02-01]
  9. Brazilian funding agency-FAPESP [2014/11806-9]

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We searched for z greater than or similar to 7 Lyman-break galaxies in the optical-to-mid-infrared Hubble Frontier Field and associated parallel field observations of the strong-lensing cluster MACS J0416-2403. We discovered 22 candidates, of which 6 lie at z greater than or similar to 9 and 1 lies at z greater than or similar to 10. Based on the Hubble and Spitzer photometry, all have secure photometric redshifts and a negligible probability of being at lower redshifts according to their peak-probability ratios, R. This substantial increase in the number of known high-redshift galaxies allows a solid determination of the luminosity function (LF) at z greater than or similar to 8. The number of high-z candidates in the parallel field is considerably higher than that in the Abell 2744 parallel field. Our candidates have median stellar masses of (M-*) similar to log 8.44(-0.31)(+0.55)M(circle dot), star formation rates (SFRs) of similar to 1.8(-0.4)(+0.5) M-circle dot yr(-1), and SFR-weighted ages of less than or similar to 300(-140)(+70) Myr. Finally, we are able to put strong constraints on the z = 7, 8, 9, and 10 LFs. One of the objects in the cluster field is a z similar or equal to 10 candidate, with a magnification of mu similar to 20 +/- 13. This object is likely the faintest z similar to 10 object known to date, allowing a first look into the extreme faint end (L similar to 0.04 L*) of the z similar to 10 LF (It is named Tayna in the Aymara language).

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