Hyperfine interaction constants and hyperfine components of MnI lines in the near-infrared J and H bands were obtained by fitting the solar spectrum. I identified the 17744-A solar absorption line as resulting from MnI and I discarded the identifications of the 13281.65-A and 16929.85-A solar features as a result of FeI and MnI, respectively
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J. Meléndez (1999) studied this question.
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