**Table 1:** Fe I lines used for setting the wavelength scale in the stellar spectrum and determining the rotational velocity.
$\lambda_{\rm air}$ (Å)	Ref.^a	log gf^b
4592.6512	LT	-2.449
4602.9409	LT	-2.250
4691.412	TW	-1.450
4710.2834	LT	-1.612
5049.8196	LT	-1.420
5051.635	TW	-2.795
5068.7657	LT	-1.055
5098.6959	LT	-2.026
5107.448	TW	-3.087
5107.641	TW^c	-2.418
5110.413	TW	-3.760

^a TW: This work; LT: Learner & Thorne (1988);
^b Kurucz & Bell (1995);
^c blended with Nd II line in stellar spectrum.

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