Cosmology from LOFAR Two-metre Sky Survey Data Release 2: Cross-correlation with the cosmic microwave background (Corrigendum)

S. J. Nakoneczny; D. Alonso; M. Bilicki; D. J. Schwarz; C. L. Hale; A. Pollo; C. Heneka; P. Tiwari; J. Zheng; M. Brüggen; M. J. Jarvis; T. W. Shimwell

doi:10.1051/0004-6361/202450585e

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Erratum

This article is an erratum for:
[https://doi.org/10.1051/0004-6361/202347728]

Issue		A&A Volume 686, June 2024


Article Number		C2
Number of page(s)		1
Section		Cosmology (including clusters of galaxies)
DOI		https://doi.org/10.1051/0004-6361/202450585e
Published online		31 May 2024

A&A, 686, C2 (2024)

Cosmology from LOFAR Two-metre Sky Survey Data Release 2: Cross-correlation with the cosmic microwave background (Corrigendum)

S. J. Nakoneczny¹^,2, D. Alonso³, M. Bilicki⁴, D. J. Schwarz⁵, C. L. Hale⁶, A. Pollo²^,7, C. Heneka⁸, P. Tiwari⁹, J. Zheng⁵, M. Brüggen¹⁰, M. J. Jarvis³^,11 and T. W. Shimwell¹²^,13

¹ Division of Physics, Mathematics and Astronomy, California Institute of Technology, 1200 E California Blvd, Pasadena, CA 91125, USA
e-mail: nakonecz@caltech.edu
² Department of Astrophysics, National Centre for Nuclear Research, Pasteura 7, 02-093 Warsaw, Poland
³ Sub-department of Astrophysics, University of Oxford, Denys Wilkinson Building, Keble Road, Oxford OX1 2DL, UK
⁴ Center for Theoretical Physics, Polish Academy of Sciences, Al. Lotników 32/46, 02-668 Warsaw, Poland
⁵ Fakultät für Physik, Universität Bielefeld, Postfach 100131, 33501 Bielefeld, Germany
⁶ Institute for Astronomy, School of Physics and Astronomy, University of Edinburgh, Royal Observatory Edinburgh, Blackford Hill, Edinburgh EH9 3HJ, UK
⁷ Astronomical Observatory of the Jagiellonian University, 31-007 Cracow, Poland
⁸ Institute for Theoretical Physics, Heidelberg University, Philosophenweg 16, 69120 Heidelberg, Germany
⁹ Department of Physics, Guangdong Technion – Israel Institute of Technology, Shantou, Guangdong 515063, PR China
¹⁰ Hamburg Observatory, University of Hamburg, Gojenbersgweg 112, 21029 Hamburg, Germany
¹¹ Department of Physics, University of the Western Cape, Bellville 7535, South Africa
¹² ASTRON, Netherlands Institute for Radio Astronomy, Oude Hoogeveensedijk 4, 7991 PD Dwingeloo, The Netherlands
¹³ Leiden Observatory, Leiden University, PO Box 9513 2300 RA Leiden, The Netherlands

Key words: cosmic background radiation / methods: statistical / radio continuum: galaxies / large-scale structure of Universe / cosmology: observations / errata, addenda

Erratum for: A&A, 681, A105 (2024), https://doi.org/10.1051/0004-6361/202347728

Fig. 7.

Constraints on σ₈ using $C_{l}^{g g}$ $C_\ell^{gg}$ and $C_{l}^{g κ}$ $C_\ell^{g\kappa}$ at the fiducial ℓ < (250, 500), the b_g, D/D(z) bias modelling, HALOFIT matter power spectrum, and Planck cosmology assumed for parameters other than σ₈. The top bar shows constraints form the LoTSS DR1 (Alonso et al. 2021), and the three bottom bars present Planck (Planck Collaboration I 2020), KiDS (Heymans et al. 2021), and DES (Abbott et al. 2022).

Figure 7 in the original paper had switched plus and minus values of the error bars. Figure 7 shows the correct results.

References

Abbott, T. M. C., Aguena, M., Alarcon, A., et al. 2022, Phys. Rev. D, 105, 023520 [CrossRef] [Google Scholar]
Alonso, D., Bellini, E., Hale, C., Jarvis, M. J., & Schwarz, D. J. 2021, MNRAS, 502, 876 [NASA ADS] [CrossRef] [Google Scholar]
Heymans, C., Tröster, T., Asgari, M., et al. 2021, A&A, 646, A140 [NASA ADS] [CrossRef] [EDP Sciences] [Google Scholar]
Planck, Collaboration I. 2020, A&A, 641, A1 [NASA ADS] [CrossRef] [EDP Sciences] [Google Scholar]

© The Authors 2024

Open Access article, published by EDP Sciences, under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.

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All Figures

Fig. 7.

Constraints on σ₈ using $C_{l}^{g g}$ $C_\ell^{gg}$ and $C_{l}^{g κ}$ $C_\ell^{g\kappa}$ at the fiducial ℓ < (250, 500), the b_g, D/D(z) bias modelling, HALOFIT matter power spectrum, and Planck cosmology assumed for parameters other than σ₈. The top bar shows constraints form the LoTSS DR1 (Alonso et al. 2021), and the three bottom bars present Planck (Planck Collaboration I 2020), KiDS (Heymans et al. 2021), and DES (Abbott et al. 2022).

In the text

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[1] Abbott, T. M. C., Aguena, M., Alarcon, A., et al. 2022, Phys. Rev. D, 105, 023520 [CrossRef] [Google Scholar]

[2] Alonso, D., Bellini, E., Hale, C., Jarvis, M. J., & Schwarz, D. J. 2021, MNRAS, 502, 876 [NASA ADS] [CrossRef] [Google Scholar]

[3] Heymans, C., Tröster, T., Asgari, M., et al. 2021, A&A, 646, A140 [NASA ADS] [CrossRef] [EDP Sciences] [Google Scholar]

[4] Planck, Collaboration I. 2020, A&A, 641, A1 [NASA ADS] [CrossRef] [EDP Sciences] [Google Scholar]