Planets Around Solar Twins/Analogs (PASTA) - II. Chemical abundances, systematic offsets, and clues as to planet formation

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Volume 701 (September 2025)

A&A, 701 (2025) A107

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Table B.1

Atomic spectral lines and EWs (extract).

λ^a [Å]	Ion^a	$X_{exc}^{a} [eV]$ $X_{{\rm{exc}}}^a\left[ {{\rm{eV}}} \right]$	log ɡf^a	$C_{6}^{a}$	Solar^b	HD 10180	HD 20782	HD 31527	HD 42618	HD 45184	HD 70573	…
EW^c [mÅ]					EW	EW	EW	EW	EW	EW	EW	…
5044.211	26.0	2.8512	–2.058	2.71E–31	80.0	71.4	70.0	64.2	66.1	67.6	65.4	…
5054.642	26.0	3.6400	–1.921	4.68E–32	45.3	43.6	37.2	30.7	34.2	37.0	29.9	…
⋮	⋮	⋮	⋮	⋮	⋮	⋮	⋮	⋮	⋮	⋮	⋮	…

Notes. ^(a)Columns 1–5 give wavelength (in Å), ion identifier, excitation potential (eV), log ɡf, and van der Waals damping constant C₆. Ion notation: 26.0 = Fe I, 6.0 = C I, etc.

^(b)Columns 6–31 give equivalent widths (EW, in mÅ) for the Sun and the 25 target stars, following the header order.

^(c)EW: Equivalent width in mÅ.

The full table is available in machine-readable form at the CDS.

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