LoTSS jellyfish galaxies

I. D. Roberts; R. J. van Weeren; S. L. McGee; A. Botteon; A. Drabent; A. Ignesti; H. J. A. Rottgering; T. W. Shimwell; C. Tasse

doi:10.1051/0004-6361/202140784e

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Volume 655 (November 2021)

A&A, 655 (2021) C2

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Erratum

This article is an erratum for:
[https://doi.org/10.1051/0004-6361/202140784]

Issue		A&A Volume 655, November 2021


Article Number		C2
Number of page(s)		1
Section		Extragalactic astronomy
DOI		https://doi.org/10.1051/0004-6361/202140784e
Published online		22 November 2021

A&A 655, C2 (2021)

I. Radio tails in low redshift clusters (Corrigendum)

I. D. Roberts¹, R. J. van Weeren¹, S. L. McGee², A. Botteon¹, A. Drabent³, A. Ignesti⁴, H. J. A. Rottgering¹, T. W. Shimwell¹^,5 and C. Tasse⁶^,7

¹ Leiden Observatory, Leiden University, PO Box 9513, 2300 RA Leiden, The Netherlands
e-mail: iroberts@strw.leidenuniv.nl
² University of Birmingham School of Physics and Astronomy, Edgbaston, Birmingham, UK
³ Thüringer Landessternwarte, Sternwarte 5, 07778 Tautenburg, Germany
⁴ INAF- Osservatorio astronomico di Padova, Vicolo Osservatorio 5, 35122 Padova, Italy
⁵ ASTRON, the Netherlands Institute for Radio Astronomy, Postbus 2, 7990 AA Dwingeloo, The Netherlands
⁶ GEPI & USN, Observatoire de Paris, CNRS, Université Paris Diderot, 5 place Jules Janssen, 92190 Meudon, France
⁷ Centre for Radio Astronomy Techniques and Technologies, Department of Physics and Electronics, Rhodes University, Grahamstown 6140, South Africa

Key words: galaxies: clusters: general / galaxies: evolution / galaxies: irregular / radio continuum: galaxies / errata, addenda

Erratum for: A&A 650, A111 (2021), https://doi.org/10.1051/0004-6361/202140784

After publication, important typos in two sections of this article were identified by the authors. These typos are corrected below. It is important to note that these changes have no influence on the scientific conclusions of the paper, but correcting them does add clarity for future readers of the manuscript.

Section 5: The number of jellyfish galaxies listed in Table 2 are incorrect and reflect an earlier, pre-publication, version of the manuscript. The corrected version of Table 2 is as follows:

Table 1.

Galaxy distribution in phase space regions.

Section 7.2: For the three fits to the 144 MHz luminosity - SFR relation listed in Sect. 7.2, the ‘x’ and ‘y’ variables were inadvertently swapped in the text (the fits were done correctly). The best-fit relations (in order of appearance) should be listed as follows:

$\begin{matrix} log L_{144} = 1.07 \pm 0.01 \times log SFR + 22.07 \pm 0.01, \end{matrix}$ $\begin{aligned} \log L_{144} = 1.07 \pm 0.01 \times \log \mathrm{SFR} + 22.07 \pm 0.01, \end{aligned}$

$\begin{matrix} log L_{144} = 1.07 \pm 0.08 \times log SFR + 22.07 \pm 0.02, \end{matrix}$ $\begin{aligned} \log L_{144} = 1.07 \pm 0.08 \times \log \mathrm{SFR} + 22.07 \pm 0.02, \end{aligned}$

$\begin{matrix} log L_{144} = 0.82 \pm 0.08 \times log SFR + 22.24 \pm 0.03 . \end{matrix}$ $\begin{aligned} \log L_{144} = 0.82 \pm 0.08 \times \log \mathrm{SFR} + 22.24 \pm 0.03. \end{aligned}$

© ESO 2021

All Tables

Table 1.

Galaxy distribution in phase space regions.

In the text

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