EDP Sciences
LOFAR Surveys: a new window on the Universe
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Erratum
This article is an erratum for: [this article]

Issue
A&A
Volume 624, April 2019
LOFAR Surveys: a new window on the Universe
Article Number C1
Number of page(s) 1
Section Cosmology (including clusters of galaxies)
DOI https://doi.org/10.1051/0004-6361/201833900e
Published online 02 April 2019

Some errors have occurred during the production of the original article. The left panel of Fig. 8 was incomplete. Here we publish the correct Fig. 8. Also, Eq. (5) was incorrect, it should read:

thumbnail Fig. 8.

Scatter plots of spectral index and radio SB (IR) as a function of X-ray SB (IX). The regions for extracting data are shown in the overlaid image (left panel). The data points are plotted in the same colour as the regions in the overlaid image (i.e. black circles for the central regions, magenta squares for the regions in the SW direction, and red diamonds for the regions in the NE direction). The best-fit parameters are obtained for the central regions.

Open with DEXTER


© ESO 2019

All Figures

thumbnail Fig. 8.

Scatter plots of spectral index and radio SB (IR) as a function of X-ray SB (IX). The regions for extracting data are shown in the overlaid image (left panel). The data points are plotted in the same colour as the regions in the overlaid image (i.e. black circles for the central regions, magenta squares for the regions in the SW direction, and red diamonds for the regions in the NE direction). The best-fit parameters are obtained for the central regions.

Open with DEXTER
In the text

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