UKIRT Widefield Infrared Survey for Fe
arXiv:1406.4271 · doi:10.1093/mnras/stu1146
Abstract
The United Kingdom Infrared Telescope (UKIRT) Widefield Infrared Survey for Fe (UWIFE) is a 180 deg imaging survey of the first Galactic quadrant (7 < l < 62; |b| < 1.5) using a narrow-band filter centered on the [Fe II] 1.644 μm emission line. The [Fe II] 1.644 μm emission is a good tracer of dense, shock-excited gas, and the survey will probe violent environments around stars: star-forming regions, evolved stars, and supernova remnants, among others. The UWIFE survey is designed to complement the existing UKIRT Widefield Infrared Survey for H2 (UWISH2; Froebrich et al. 2011). The survey will also complement existing broad-band surveys. The observed images have a nominal 5σ detection limit of 18.7 mag for point sources, with the median seeing of 0.83". For extended sources, we estimate surface brightness limit of 8.1 x 10 W m arcsec . In this paper, we present the overview and preliminary results of this survey.
MNRAS Accepted, 13 pages, A pdf version with high-res figures is available at the survey web page (http://gems0.kasi.re.kr/uwife/)
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- Massive young stellar object W42-MME: The discovery of an infrared jet using VLT/NACO near-infrared images
- Unraveling the inner substructure of new candidate hub-filament system in the HII region G25.4NW
- [Fe II] 1.64 um Imaging Observations of the Outflow Features around Ultracompact H II Regions in the 1st Galactic Quadrant
- Extended Ionized Fe Objects in the UWIFE Survey