Volume 636, April 2020
|Number of page(s)||1|
|Section||Galactic structure, stellar clusters and populations|
|Published online||07 April 2020|
Measuring the local matter density using Gaia DR2 (Corrigendum)
The Oskar Klein Centre for Cosmoparticle Physics, Department of Physics, Stockholm University, AlbaNova 10691, Stockholm, Sweden
Key words: Galaxy: kinematics and dynamics / Galaxy: disk / solar neighborhood / astrometry / errata, addenda
This is an erratum for Widmark (2019), with two corrections to the text in the article.
Firstly, in the bottom row and second column of Table 3 of the article, there is a numerical range that reads 6.3–6.3, which should instead read 6.0–6.3.
Secondly, the matrix elements of Eq. (21) all contain a factor of kμ/ϖ. These factors should really be squared, such that the equation reads
These corrections apply only to the text in the article. In the analysis, the correct numbers and expressions are used, so the results of Widmark (2019) are not affected.
© ESO 2020
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.