Probing ∼L* Lyman-break galaxies at z≈ 7 in GOODS-South with WFC3 on Hubble Space Telescope

Wilkins, Stephen M, Bunker, Andrew J, Ellis, Richard S, Stark, Daniel, Stanway, Elizabeth R, Chiu, Kuenley, Lorenzoni, Silvio and Jarvis, Matt J (2010) Probing ∼L* Lyman-break galaxies at z≈ 7 in GOODS-South with WFC3 on Hubble Space Telescope. Monthly Notices of the Royal Astronomical Society, 403 (2). pp. 938-944. ISSN 0035-8711

[img]
Preview
PDF - Published Version
Download (4MB) | Preview

Abstract

We analyse recently acquired near-infrared Hubble Space Telescope imaging of the Great Observatories Origins Deep Survey (GOODS)-South field to search for star-forming galaxies at z≈ 7.0. By comparing Wide Field Camera 3 (WFC3) 0.98 μm Y-band images with Advanced Camera for Surveys (ACS) z-band (0.85 μm) images, we identify objects with colours consistent with Lyman-break galaxies at z≃ 6.4–7.4. This new data cover an area five times larger than that previously reported in the WFC3 imaging of the Hubble Ultra Deep Field and affords a valuable constraint on the bright end of the luminosity function. Using additional imaging of the region in the ACS B, V and i bands from GOODS v2.0 and the WFC3J band, we attempt to remove any low-redshift interlopers. Our selection criteria yields six candidates brighter than YAB= 27.0, of which all except one are detected in the ACS z-band imaging and are thus unlikely to be transients. Assuming all six candidates are at z≈ 7, this implies a surface density of objects brighter than YAB= 27.0 of 0.30 ± 0.12 arcmin−2, a value significantly smaller than the prediction from z≈ 6 luminosity function. This suggests continued evolution of the bright end of the luminosity function between z= 6 and 7, with number densities lower at higher redshift.

Item Type: Article
Schools and Departments: School of Mathematical and Physical Sciences > Physics and Astronomy
Subjects: Q Science > QB Astronomy
Depositing User: Stephen Wilkins
Date Deposited: 26 Apr 2013 10:56
Last Modified: 07 Mar 2017 10:34
URI: http://sro.sussex.ac.uk/id/eprint/44510

View download statistics for this item

📧 Request an update