Nearby Optical Galaxies: Selection of the Sample and Identification of Groups

@article{Giuricin2000NearbyOG,
  title={Nearby Optical Galaxies: Selection of the Sample and Identification of Groups},
  author={G. Giuricin and C. Marinoni and L. Ceriani and A. D. O. Astronomy and University of Trieste Sissa and Trieste and I. A. Observatory and I. S. O. Physics and U. Waterloo and Waterloo and Canada.},
  journal={The Astrophysical Journal},
  year={2000},
  volume={543},
  pages={178-194}
}
In this paper we describe the Nearby Optical Galaxy (NOG) sample, which is a complete, distance-limited (cz ≤ 6000 km s-1) and magnitude-limited (B ≤ 14) sample of ~7000 optical galaxies. The sample covers (8.27 sr) of the sky (|b| > 20°) and appears to have a good completeness in redshift (97%). We select the sample on the basis of homogenized corrected total blue magnitudes in order to minimize systematic effects in galaxy sampling. We identify the groups in this sample by means of both the… Expand

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References

SHOWING 1-10 OF 110 REFERENCES
The Nearby Optical Galaxy Sample: The Local Galaxy Luminosity Function
Environmental Effects on Local Active Galactic Nuclei
DWARF GALAXIES OF THE LOCAL GROUP
Loose groups of galaxies in the Perseus-Pisces survey
The redshift-space neighborhoods of 36 loose groups. 2: Analysis
Nearby groups of galaxies. I. The NGC 1023 group.
...
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2
3
4
5
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