| Issue |
A&A
Volume 527, March 2011
|
|
|---|---|---|
| Article Number | C2 | |
| Number of page(s) | 2 | |
| Section | Cosmology (including clusters of galaxies) | |
| DOI | https://doi.org/10.1051/0004-6361/20053650e | |
| Published online | 26 January 2011 | |
X-ray properties in massive galaxy clusters: XMM-Newton observations of the REFLEX-DXL sample (Corrigendum)
1
Max-Planck-Institut für extraterrestrische Physik,
Giessenbachstraße,
85748
Garching,
Germany
e-mail: yyzhang@astro.uni-bonn.de
2
National Museum of Emerging Science and Innovation,
Tokyo,
Japan
3
Tokyo University of Science, Tokyo, Japan
4
INAF – Osservatorio Astronomico di Brera,
Merate/Milano,
Italy
5
Liverpool John Moores University, Liverpool, UK
The article by Zhang et al. (2006, A&A, 456, 55) contains an error in Fig. 5 on page 64, in which we inadvertently re-called the mass distribution of RXCJ0528.9−3972. We note that this does not affect any results in Zhang et al. (2006). Nevertheless, we regret this error and provide an update of Fig. 5 here.
Key words: cosmology: observations / galaxies: clusters: general / X-rays: galaxies: clusters / dark matter / errata, addenda
© ESO, 2011
 |
Fig. 5 Measured mass profiles of the REFLEX-DXL clusters and their best fits by the extended-NFW models. Residuals scaled by the data uncertainties are plotted in the upper part of the diagrams. |
References
- Zhang, Y.-Y., Böhringer, H., Finoguenov, A., et al. 2006, A&A, 456, 55 [NASA ADS] [CrossRef] [EDP Sciences] [Google Scholar]
All Figures
|
Fig. 5 Measured mass profiles of the REFLEX-DXL clusters and their best fits by the extended-NFW models. Residuals scaled by the data uncertainties are plotted in the upper part of the diagrams. |
| In the text | |
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