Table 2: Observed line transitions in the program stars.
Ion $\lambda_{\rm air}$ (Å) Identification

Fe II 
10 485.940 ${\rm e^6D_{5/2}{-}^6D^0_{5/2}}$
Fe II  10 490.942 ${\rm z^4F_{7/2}{-}b^4G_{7/2}}$
Fe II  10 499.297 ${\rm z^4F_{7/2}{-}b^4G_{5/2}}$
Fe II  10 501.499 ${\rm z^4F_{7/2}{-}b^4G_{9/2}}$
N I  10 507.000 ${\rm ^4P^0_3{-}^4D_5}$
N I  10 513.410 ${\rm ^4P^0_1{-}^4D_1}$
N I  10 520.580 ${\rm ^4P^0_3{-}^4D_3}$
Fe II  10 525.122 ${\rm w^2D_{3/2}{-}^4P_{5/2}}$
N I  10 533.760 ${\rm ^4P^0_3{-}^4D_1}$
N I  10 539.574 ${\rm ^4P^0_5{-}^4D_7}$
Fe II  10 546.348 ${\rm e^6D_{9/2}{-}y^6F^0_{11/2}}$
N I  10 549.640 ${\rm ^4P^0_5{-}^4D_5}$
N I  10 563.330 ${\rm ^4P^0_5{-}^4D_3}$
Fe II  10 591.170 ${\rm e^6D_{5/2}{-}^6D^0_{3/2}}$
Fe II  10 655.649 ${\rm d^2F_{7/2}{-}z^2F^0_{7/2}}$
He I  10 667.65 ${\rm 3p~^3P^0{-}6s~^3S}$
C I  10 683.080 ${\rm ^3P^0_1{-}^3D_2}$
C I  10 685.340 ${\rm ^3P^0_0{-}^3D_1}$
C I  10 691.240 ${\rm ^3P^0_2{-}^3D_3}$
C I  10 707.32 ${\rm ^3P^0_1{-}^3D_1}$
Fe II  10 709.730 ${\rm e^6D_{7/2}{-}y^6F^0_{5/2}}$
Fe II  10 711.060 ${\rm e^6D_{3/2}{-}^6D^0_{5/2}}$
N I  10 713.548 ${\rm ^4P^0_3{-}^4P_5}$
N I  10 717.950 ${\rm ^4P^0_3{-}^4P_3}$
C I  10 729.53 ${\rm ^3P^0_2{-}^3D_2}$
Fe II  10 749.781 ${\rm e^6D_{7/2}{-}y^6F^0_{7/2}}$
N I  10 757.887 ${\rm ^4P^0_5{-}^4P_5}$
Fe II  10 820.88 ${\rm e^6D_{3/2}{-}^6D^0_{3/2}}$
Fe II  10 826.483 ${\rm e^6D_{7/2}{-}y^6F^0_{9/2}}$
Fe II  10 829.550 ${\rm z^4D_{3/2}{-}b^4G_{5/2}}$
He I  10 830.34 ${\rm 2s~^3S{-}2p~^3P^0}$
Fe II  10 862.644 ${\rm z^4F_{5/2}{-}b^4G_{7/2}}$
Fe II  10 871.601 ${\rm z^4F_{5/2}{-}b^4G_{5/2}}$
Fe II  10 899.370 ${\rm e^6D_{3/2}{-}y^6F^0_{1/2}}$
He I  10 912.99 ${\rm 3d~^3D{-}6f~^3F^0}$
Mg II  10 914.280 ${\rm ^2D_5{-}^2P^0_3}$
He I  10 917.062 ${\rm 3d~^1D{-}6f~^1F^0}$
Pa $\gamma $ 10 938.095 6-3
Mg II  10 951.770 ${\rm ^2D_3{-}^2P^0_1}$


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