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Table 1

Atmospheric parameters and chemical abundances for our reference stars.

Star Cool giants Cool dwarfs Hot dwarf


Arcturus μ Leo 61 Cyg A ϵ Eri Sun Procyon
Teff (K) 4286 4474 4374 5076 5771 6554
log(g) (g in cm s−2) 1.60 2.51 4.63 4.61 4.44 4.00 Fe/H>Fe/H
(dex) –0.55 0.22 –0.36 –0.12 0.00 –0.04 α/Fe>α/Fe
(dex) 0.22 0.12 0.02 –0.01 0.00 –0.07
Vmicro (km s−1) 1.95(a) 1.95(a) 1.07(b) 1.14(b) 0.87(c) 1.69(d)
Vmacro (km s−1) 4.30(a) 2.58(a) 1.83(c) 2.91(c) 3.57(c) 4.60(d)
Vsin i (km s−1) 3.80(a) 5.06(a) 0.70(e) 2.40(c) 1.60(c) 2.80(d)
[C/Fe] (dex) 0.43(f) –0.18(g) 0.60(h) –0.06(h) 0.00 -0.05(h)
[N/Fe] (dex) 0.00 0.37(g) 0.00 0.00 0.00 0.00
[O/Fe] (dex) 0.50(f) –0.13(g) 0.47(h) –0.17(h) 0.00 0.14 (h)
[Ca/Fe] (dex) 0.12 0.03 –0.03 0.04 0.00 0.03
12 C/13 C 6.30(i) 20.0(i) 89.9 89.9 89.9 89.9

References. The data come from Jofré et al. (2018) or are assumed solar-scaled abundances except the following: (a) Hekker & Meléndez (2007), (b) Jofré et al. (2015), (c) Valenti & Fischer (2005), (d) Bruntt et al. (2010), (e) Benz & Mayor (1984), (f) Ramírez & Allende Prieto (2011), (g)Gratton & Sneden (1990), (h)Luck (2017), and (i) Smith et al. (2013).

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