Volume 589, May 2016
|Number of page(s)||2|
|Published online||05 April 2016|
The Penn State – Toruń Centre for Astronomy Planet Search stars (Corrigendum)
III. The sample of evolved stars⋆
1 Toruń Centre for Astronomy, Nicolaus Copernicus University in Toruń, Grudziadzka 5, 87-100 Toruń, Poland
2 McDonald Observatory and Department of Astronomy, University of Texas at Austin, 2515 Speedway, Stop C1402, Austin, Texas, 78712-1206, USA
3 Instituto de Astrofísica de Canarias, C/vía Láctea, s/n, 38205 La Laguna, Tenerife, Spain
4 Departamento de Astrofísica, Universidad de La Laguna, 38206 La Laguna, Tenerife, Spain
5 Department of Astronomy and Astrophysics, Pennsylvania State University, 525 Davey Laboratory, University Park, PA 16802, USA
6 Center for Exoplanets and Habitable Worlds, Pennsylvania State University, 525 Davey Laboratory, University Park, PA 16802, USA
Key words: stars: atmospheres / stars: fundamental parameters / stars: late-type / stars: general / errata, addenda
Table 2 in our recent paper (Niedzielski et al. 2016) erroneously includes 20 stars that were finally adopted for detailed spectroscopic analysis (including 11 SB1s mentioned in the text) and are listed in Table 1 as well. Consequently, the corrected Table 2 (available in electronic version) contains 33 rather than 53 stars. They are 18 SB2 stars, 14 ones with variable CCFs (possibly SB2) and one with a weak CCF.
An photometric estimate of Teff and log g for stars with unstable CCF.
© ESO, 2016
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