EDP Sciences logo
Subscriber Authentication Point
Search
Menu
Home All issues Volume 674 (June 2023) A&A, 674 (2023) C1 Full HTML
Open Access
Erratum
This article is an erratum for:
[https://doi.org/10.1051/0004-6361/202243994]

Issue
A&A
Volume 674, June 2023
Article Number C1
Number of page(s) 3
Section Interstellar and circumstellar matter
DOI https://doi.org/10.1051/0004-6361/202243994e
Published online 07 June 2023

Erratum for: A&A, 666, A12 (2022), https://doi.org/10.1051/0004-6361/202243994

In this erratum we remove duplicate entries from Table D.1 of the original paper for QSO-DLAs. Removing the duplicated entries from Table D.1 has no effect on the results of the original paper.

Additionally, we update the P II column densities for the Milky Way that are taken from Jenkins (2009), adopting the most recent value f = 0.0196 for the λ1301 Å line of Brown et al. (2018). This value is based on comprehensive beam-foil measurements. In the original paper, we homogenized the P II column densities to the oscillator strength f= 0.0053 derived by Kurucz (2017), which is an older value. The updated column densities are given in Table 1. The updated and the old A2P and B2P coefficients resulting from the fit are presented in Table 2, where the difference between the old and new values are small and within the uncertainties. Figure 1 shows the updated fit for [P/Zn] with [Zn/Fe] (left) and the dust depletion δP with [Zn/Fe] (right). The updated table for QSO-DLAs without the duplicates is Table 3.

References

  1. Berg, T. A. M., Ellison, S. L., Prochaska, J. X., Venn, K. A., & Dessauges-Zavadsky, M. 2015, MNRAS, 452, 4326 [NASA ADS] [CrossRef] [Google Scholar]
  2. Brown, M. S., Alkhayat, R. B., Irving, R. E., et al. 2018, ApJ, 868, 42 [NASA ADS] [CrossRef] [Google Scholar]
  3. Cashman, F. H., Kulkarni, V. P., Kisielius, R., Ferland, G. J., & Bogdanovich, P. 2017, ApJS, 230, 8 [NASA ADS] [CrossRef] [Google Scholar]
  4. De Cia, A., Ledoux, C., Mattsson, L., et al. 2016, A&A, 596, A97 [NASA ADS] [CrossRef] [EDP Sciences] [Google Scholar]
  5. Jenkins, E. B. 2009, ApJ, 700, 1299 [Google Scholar]
  6. Kisielius, R., Kulkarni, V. P., Ferland, G. J., Bogdanovich, P., & Lykins, M. L. 2014, ApJ, 780, 76 [Google Scholar]
  7. Kisielius, R., Kulkarni, V. P., Ferland, G. J., et al. 2015, ApJ, 804, 76 [NASA ADS] [CrossRef] [Google Scholar]
  8. Kurucz, R. L. 2017, Canadian J. Phys., 95, 825 [NASA ADS] [CrossRef] [Google Scholar]

© The Authors 2023

Licence Creative CommonsOpen 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.

This article is published in open access under the Subscribe to Open model. Subscribe to A&A to support open access publication.

All Tables

Table 1

Updated column densities for PII.

In the text
Table 2

Coefficients for PII.

In the text
Table 3

QSO-DLA column densities.

In the text

All Figures

thumbnail Fig. 1

Relative abundance of P with respect to Zn against [Zn/Fe] (left). Dust depletion of P against [Zn/Fe] (right). The linear fits for the QSO-DLAs (black triangles and black line), for the LMC (purple stars and purple line), for the SMC (blue triangles and blue line) and for the Milky Way (green points and green line) are shown. The solid red line shows the linear fit to the merged data, resulting in the new A2P and B2P coefficients given in Table 2.
In the text

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.