Volume 640, August 2020
|Number of page(s)||1|
|Section||Galactic structure, stellar clusters and populations|
|Published online||26 August 2020|
Full 5D characterisation of the Sagittarius stream with Gaia DR2 RR Lyrae (Corrigendum)
Dept. FQA, Institut de Ciències del Cosmos (ICCUB), Universitat de Barcelona (IEEC-UB), Martí Franquès 1, 08028 Barcelona, Spain
2 Departamento de Astronomía, Instituto de Física, Universidad de la República, Iguá 4225, CP 11400 Montevideo, Uruguay
3 Kapteyn Astronomical Institute, University of Groningen, Landleven 12, 9747 AD Groningen, The Netherlands
Key words: Galaxy: halo / stars: variables: RR Lyrae / galaxies: dwarf / astrometry / errata, addenda
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.
- Evans, D. W., Riello, M., De Angeli, F., et al. 2018, A&A, 616, A4 [NASA ADS] [CrossRef] [EDP Sciences] [Google Scholar]
- Maíz Apellániz, J., & Weiler, M. 2018, A&A, 619, A180 [NASA ADS] [CrossRef] [EDP Sciences] [Google Scholar]
- Westera, P., Lejeune, T., Buser, R., Cuisinier, F., & Bruzual, G. 2002, A&A, 381, 524 [NASA ADS] [CrossRef] [EDP Sciences] [Google Scholar]
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).
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© ESO 2020
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