Hubble Space Telescope Imaging of Bright Lyman-break Galaxy Candidates from the Sloan Digital Sky Survey: Not LBGs After All
arXiv:0805.1894 · doi:10.1088/0004-6256/136/1/498
Abstract
We present deep Hubble Space Telescope ACS and NICMOS images of six bright Lyman-break galaxy candidates that were previously discovered in the Sloan Digital Sky Survey. We find that five of the objects are consistent with unresolved point sources. Although somewhat atypical of the class, they are most likely LoBAL quasars, perhaps FeLoBALs. The sixth object, J1147, has a faint companion galaxy located ~0.8 arcsec to the southwest. The companion contributes ~8% of the flux in the observed-frame optical and infrared. It is unknown whether this companion is located at the same redshift as J1147.
arXiv comment16 pages, 8 figures, 3 tables; accepted for publication in AJ
References in corpus (11)
- The Sloan Digital Sky Survey: Technical Summary
- Detailed Structural Decomposition of Galaxy Images
- Rest-Frame Ultraviolet Spectra of z~3 Lyman Break Galaxies
- The First Data Release of the Sloan Digital Sky Survey
- Multi-wavelength Observations of Dusty Star Formation at Low and High Redshift
- The Sloan Digital Sky Survey Quasar Catalog I. Early Data Release
- The z=2.72 galaxy cB58: a gravitational fold arc lensed by the cluster MS 1512+36
- A Search for Nitrogen Enriched Quasars in the Sloan Digital Sky Survey Early Data Release
- Bright Lyman Break Galaxy Candidates in the Sloan Digital Sky Survey First Data Release
- SDSS J1553+0056: A BALQSO mimicking a Lyman-break galaxy
- Rest-frame optical and far-infrared observations of extremely bright Lyman-break galaxy candidates at z ~ 2.5