Open Access

Table 3

NLTE atomic models used in this study.

Species Reference H I collisions
C I* Amarsi et al. (2019a,c) AK
O I* Przybilla et al. (2000),
Sitnova & Mashonkina (2018) BVM19
Na I Alexeeva et al. (2014) BBD10
Mg I–II Bergemann et al. (2017a) BBS12
Si I–II Mashonkina (2020) BYB14
Ca I–II Mashonkina et al. (2007, 2017b) BVY17
Sc II Zhang et al. (2008) SH84 (0.1)
Ti I–II Sitnova et al. (2016) SYB20
Cr I–II Bergemann & Cescutti (2010) SH84 (0.0)
Mn I–II Bergemann et al. (2019) BV17, BGE19
Fe I–II Mashonkina et al. (2011, 2019) YBK18,
YBK19
Co I–II Bergemann et al. (2010) SH84 (0.05)
Zr II Velichko et al. (2010) SH84 (0.1)
Nd II Mashonkina et al. (2005) SH84 (0.1)
Ba II Gallagher et al. (2020) BY17, BY18
Eu II Mashonkina & Gehren (2000) SH84 (0.1)
Pb I Mashonkina et al. (2012) SH84 (0.1)
Th II Mashonkina et al. (2012) SH84 (0.1)

Notes. Collisions with H I were treated following AK (Amarsi et al. 2019a; Kaulakys 1991), BVM19 (Belyaev et al. 2019), BBD10 (Barklem et al. 2010), BYB14 (Belyaev et al. 2014), BVY17 (Belyaev et al. 2017), SH84 (Zhang et al. 2008), SYB20 (Sitnova et al. 2020), YBK18 (Yakovleva et al. 2018), YBK19 (Yakovleva et al. 2019), BGE19 (Bergemann et al. 2019), BV17 (Belyaev & Voronov 2017), BBS12 (Barklem et al. 2012), BY17 (Belyaev & Yakovleva 2017), BY18 (Belyaev & Yakovleva 2018), and SH84 (0.1) (Steenbock & Holweger 1984) with a scaling factor of SH = 0.1. SH84 (0.0) (Steenbock & Holweger 1984) and with a scaling factor of SH = 0.0. The * indicates that 3D, NLTE abundances were computed, see Table 4.

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.