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Sensitivity coefficients to $α$-variation for astrophysically relevant transitions in Ni II

We calculated the dependence of the transition frequencies on the fine-structure constant $α$ ($q$-factors) for Ni~II. Nickel is one of the few elements with high sensitivity to $α$-variation, whose lines are observed at high redshifts. This makes it a sensitive probe for $α$-variation on the cosmological timescale. The electronic structure of Ni II ion was treated within the configuration interaction (CI) method using Dirac-Coulomb Hamiltonian.