Extended Data Table 4 Absorption lines that we use in this work and their oscillator strengths

From: Large metallicity variations in the Galactic interstellar medium

  1. We use f-values from refs. 60,61,62,63. For Ni transitions, we used the f-values from ref. 62 based on observational data, which agree with ref. 64, instead of the theoretical measurements of ref. 60.
Source data
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