Issue |
A&A
Volume 501, Number 1, July I 2009
|
|
---|---|---|
Page(s) | 75 - 88 | |
Section | Extragalactic astronomy | |
DOI | https://doi.org/10.1051/0004-6361/200809591 | |
Published online | 05 May 2009 |
Online Material
Table 4: Parameters for the underlying stellar host derived from the 2D Sérsic fit.
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Figure 10:
Atlas of galaxy images I: Galaxies with Q=1. Broad-band galaxy images ( left), the best 2D Sérsic model ( centre) and the residual image ( right) of the 20 galaxies fitted with quality index Q=1 in the full sample of 28 BCGs. Broad-band images and 2D Sérsic models are showed in surface brightness grey scale (magnitude per square arcseconds). Realistic Poissonian noise are included in the 2D models. Residual images, i.e. galaxy-model, are displayed in an inverted linear grey scale (counts) which covers the range |
Open with DEXTER |
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Figure 10: continued. |
Open with DEXTER |
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Figure 10: continued. |
Open with DEXTER |
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Figure 10: continued. |
Open with DEXTER |
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Figure 10: continued. |
Open with DEXTER |
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Figure 11: Atlas of galaxy images II: Galaxies with Q=2. Broad-band galaxy images ( left), the best 2D Sérsic model ( centre) and the residual image ( right) of the 8 galaxies fitted with quality index Q=2 in the full sample of 28 BCGs. The description is the same as in Fig. 10. |
Open with DEXTER |
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Figure 11: continued. |
Open with DEXTER |
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