6dF Galaxies
Overview
The Six-degree Field (6dF) Galaxy Survey mapped roughly half the sky from the Anglo-Australian Observatory. The survey used the 1.2-meter UK Schmidt Telescope at Siding Spring Observatory in New South Wales, Australia, and allowed for a six degree field of view per observation.
This catalog overlaps with the Tully Galaxies, and there is a noticeable difference in the quality of these datasets. Tully is much tighter and the structure is more apparent, while the 6dF data are more spread out with noticeable fingers of god. This is because of local motions within galaxy clusters have not been corrected in these data. (see explanation in the 2MASS Galaxies).
In addition, the 6dF Galaxies cover only the southern sky. It will only overlap with half of the Tully or 2MASS galaxy surveys.
Completeness
Unlike the Tully galaxies, these data show an incompleteness in the sample. Most of the rich structure is visible closer to the Milky Way, where we see more of the dimmer galaxies. Toward the edge of the data set we see galaxies by their lonesome. This is because these data are not as complete. We’re only seeing the brighter galaxies to this distance, and therefore less complex structures are visible.
Profiles
Dossier
Census: |
117,441 galaxies |
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Asset File: |
|
OpenSpace Version: |
3 |
Reference: |
The 6dF Galaxy Survey - Final Redshift Release (DR3) and Southern Large-scale Structures |
Prepared by: |
Brian Abbott, Sohum Udani (AMNH) |
Source Version: |
1.05 |
License: |