Fivet, VQuinet, PPalmeri, PBiemont, EAsplund, MartinGrevesse, NSauval, A JEngstrom, LLundberg, HHartman, HNilsson, H2015-12-130035-8711http://hdl.handle.net/1885/80009The solar photospheric abundance of ruthenium is revised on the basis of a new set of oscillator strengths derived for Ru i transitions with wavelengths in the spectral range 2250-4710 Å. The new abundance value (in the usual logarithmic scale where theKeywords: Atomic data; Atomic processes; Sun: abundancesExperimental and theoretical radiative decay rates for highly excited ruthenium atomic levels and the solar abundance of ruthenium200910.1111/j.1365-2966.2009.14761.x2016-02-24