Extragalactic Large-Scale Structures behind the Southern Milky Way. IV. Redshifts Obtained with MEFOS
arXiv:astro-ph/0311195 · doi:10.1051/0004-6361:20034600
Abstract
Abbreviated: As part of our efforts to unveil extragalactic large-scale structures behind the southern Milky Way, we here present redshifts for 764 galaxies in the Hydra/Antlia, Crux and Great Attractor region (266deg < l < 338deg, |b| < 10deg), obtained with the Meudon-ESO Fibre Object Spectrograph (MEFOS) at the 3.6-m telescope of ESO. The observations are part of a redshift survey of partially obscured galaxies recorded in the course of a deep optical galaxy search behind the southern Milky Way. A total of 947 galaxies have been observed, a small percentage of the spectra (N=109, 11.5%) were contaminated by foreground stars, and 74 galaxies (7.8%) were too faint to allow a reliable redshift determination. With MEFOS we obtained spectra down to the faintest galaxies of our optical galaxy survey, and hence probe large-scale structures out to larger distances (v <~ 30000 km/s) than our other redshift follow-ups. The most distinct large-scale structures revealed in the southern Zone of Avoidance are discussed in context to known structures adjacent to the Milky Way.
arXiv comment11 pages, 7 figures; accepted for publication in A&A. Tables 1 and 2 will be available in electronic format at the CDS. Figure 1 at full resolution, and both tables are available at http://mensa.ast.uct.ac.za/~pwoudt/data/H4462/)
References in corpus (11)
- Maps of Dust IR Emission for Use in Estimation of Reddening and CMBR Foregrounds
- The 2dF Galaxy Redshift Survey: Spectra and redshifts
- Galaxy Clustering in Early SDSS Redshift Data
- The SBF Survey of Galaxy Distances. II. Local and Large-Scale Flows
- The Universe behind the Milky Way
- Large-Scale Mass Distribution Behind the Galactic Plane
- A catalogue of galaxies behind the southern Milky Way. - II. The Crux and Great Attractor regions (l = 289deg - 338deg)
- A Catalog of Galaxies behind the Southern Milky Way. - I. The Hydra/Antlia Extension (l: 266 - 296 deg)
- Discovery of Extreme Examples of Superclustering in Aquarius
- Extragalactic Large-Scale Structures behind the Southern Milky Way. -- II. Redshifts Obtained at the SAAO in the Crux Region
- Parkes HI observations of galaxies behind the southern Milky Way. - I. The Hydra/Antlia region (l : 266 to 296 deg)
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