Published September 10, 2010 | Version v1
Journal article

UV-DROPOUT GALAXIES IN THE GOODS-SOUTH FIELD FROM WFC3 EARLY RELEASE SCIENCE OBSERVATIONS

  • 1. Department of Physics and Astronomy, University of California, Riverside, CA 92521 (United States)
  • 2. Department of Physics and Astronomy, University of California, Davis, CA 92616 (United States)
  • 3. School of Earth and Space Exploration, Arizona State University, Tempe, AZ 85287-1404 (United States)
  • 4. Center for Cosmology and AstroParticle Physics, Ohio State University, Columbus, OH 43210 (United States)
  • 5. Observatories of the Carnegie Institute of Washington, Pasadena, CA 91101 (United States)
  • 6. Department of Astronomy, University of Virginia, Charlottesville, VA 22904-4325 (United States)
  • 7. Space Telescope Science Institute, Baltimore, MD 21218 (United States)
  • 8. Department of Astronomy, University of Washington, Seattle, WA 98195-1580 (United States)
  • 9. Department of Astronomy, University of Massachusetts, Amherst, MA 01003 (United States)
  • 10. School of Physics and Astronomy, Cardiff University, Cardiff CF24 3AA (United Kingdom)
  • 11. Research School of Astronomy and Astrophysics, The Australian National University, ACT 2611 (Australia)
  • 12. Association of Universities for Research in Astronomy, Washington, DC 20005 (United States)
  • 13. Institute for Astronomy, University of Hawaii, Honolulu, HI 96822 (United States)
  • 14. Department of Astronomy, New Mexico State University, Las Cruces, NM 88003 (United States)
  • 15. NASA-Goddard Space Flight Center, Greenbelt, MD 20771 (United States)
  • 16. Istituto di Astrofisica Spaziale e Fisica Cosmica, INAF, Via Gobetti 101, 40129 Bologna (Italy)
  • 17. National Optical Astronomy Observatories, Tucson, AZ 85726-6732 (United States)

Description

We combine new high sensitivity ultraviolet (UV) imaging from the Wide Field Camera 3 (WFC3) on the Hubble Space Telescope (HST) with existing deep HST/Advanced Camera for Surveys optical images from the Great Observatories Origins Deep Survey (GOODS) program to identify UV-dropouts, which are Lyman break galaxy (LBG) candidates at z ≅ 1-3. These new HST/WFC3 observations were taken over 50 arcmin2 in the GOODS-South field as a part of the Early Release Science program. The uniqueness of these new UV data is that they are observed in three UV/optical (WFC3 UVIS) channel filters (F225W, F275W, and F336W), which allows us to identify three different sets of UV-dropout samples. We apply Lyman break dropout selection criteria to identify F225W-, F275W-, and F336W-dropouts, which are z ≅ 1.7, 2.1, and 2.7 LBG candidates, respectively. We use multi-wavelength imaging combined with available spectroscopic and photometric redshifts to carefully access the validity of our UV-dropout candidates. Our results are as follows: (1) these WFC3 UVIS filters are very reliable in selecting LBGs with z ≅ 2.0, which helps to reduce the gap between the well-studied z ∼> 3 and z ∼ 0 regimes; (2) the combined number counts with average redshift z ≅ 2.2 agree very well with the observed change in the surface densities as a function of redshift when compared with the higher redshift LBG samples; and (3) the best-fit Schechter function parameters from the rest-frame UV luminosity functions at three different redshifts fit very well with the evolutionary trend of the characteristic absolute magnitude, M*, and the faint-end slope, α, as a function of redshift. This is the first study to illustrate the usefulness of the WFC3 UVIS channel observations to select z ∼< 3 LBGs. The addition of the new WFC3 on the HST has made it possible to uniformly select LBGs from z ≅ 1 to z ≅ 9 and significantly enhance our understanding of these galaxies using HST sensitivity and resolution.

Availability note (English)

Available from http://dx.doi.org/10.1088/0004-637X/720/2/1708

Additional details

Identifiers

Publishing Information

Journal Title
Astrophysical Journal
Journal Volume
720
Journal Issue
2
Journal Page Range
p. 1708-1716
ISSN
0004-637X
CODEN
ASJOAB

INIS

Country of Publication
United States
Country of Input or Organization
International Atomic Energy Agency (IAEA)
INIS RN
42055894
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Descriptors DEI
GALACTIC EVOLUTION; GALAXIES; LUMINOSITY; MASS; RED SHIFT; TELESCOPES; ULTRAVIOLET RADIATION; WAVELENGTHS
Descriptors DEC
ELECTROMAGNETIC RADIATION; EVOLUTION; OPTICAL PROPERTIES; PHYSICAL PROPERTIES; RADIATIONS