Free Access
Erratum
This article is an erratum for:
[https://doi.org/10.1051/0004-6361/202037819]


Issue
A&A
Volume 640, August 2020
Article Number C5
Number of page(s) 1
Section Galactic structure, stellar clusters and populations
DOI https://doi.org/10.1051/0004-6361/202037819e
Published online 26 August 2020

A mistake has been identified in the text describing the process involved in obtaining Eq. (A.1). The Gaia passbands that were used to calculate the observed colours (GBP − GRP) in the simulations are the ones by Evans et al. (2018), instead of Maíz Apellániz & Weiler (2018), as was originally reported. Consequently, Fig. A.1 has been corrected to include the points with the Evans et al. (2018) passbands.

This modification only affects the text in Appendix A and does not affect the coefficients of Eq. (A.1). Therefore, it does not affect our analysis or any other part of the manuscript either.

References

  1. Evans, D. W., Riello, M., De Angeli, F., et al. 2018, A&A, 616, A4 [NASA ADS] [CrossRef] [EDP Sciences] [Google Scholar]
  2. Maíz Apellániz, J., & Weiler, M. 2018, A&A, 619, A180 [NASA ADS] [CrossRef] [EDP Sciences] [Google Scholar]
  3. Westera, P., Lejeune, T., Buser, R., Cuisinier, F., & Bruzual, G. 2002, A&A, 381, 524 [NASA ADS] [CrossRef] [EDP Sciences] [Google Scholar]

Appendix A: Reddening to absorption transformations

thumbnail Fig. A.1.

Fitted relationship between and the observed GBP − GRP colour (affected by reddening) derived from simulations using BaSeL-3.1 synthetic spectral energy distributions (Westera et al. 2002) and Gaia DR2 passbands from Evans et al. (2018).

Open with DEXTER


© ESO 2020

All Figures

thumbnail Fig. A.1.

Fitted relationship between and the observed GBP − GRP colour (affected by reddening) derived from simulations using BaSeL-3.1 synthetic spectral energy distributions (Westera et al. 2002) and Gaia DR2 passbands from Evans et al. (2018).

Open with DEXTER
In the text

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