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Table 2.

Parameters of the spectral lines in the GRIS observing window.

Line Origin λ Transition geff fij Δλ
(Å) i − j (km s−1)
Si I Solar 10 827.09 4s 3P2 − 4p 3P2 1.5 3.47e−01 −89.96
He Ia Solar 10 829.09 2s 3S1 − 2p 3P0 2.0 5.99e−02 −34.60
Ca I Solar 10 829.27 4p 3F3 − 6d 3D2 1.0 0.42e−02 −29.62
He Ib Solar 10 830.25 2s 3S1 − 2p 3P1 1.75 1.78e−01 −2.49
He Ic Solar 10 830.34 2s 3S1 − 2p 3P2 1.25 2.99e−01 0.00
H2O Telluric 10 831.63 35.70
H2O Telluric 10 832.09 48.44
Ca I Solar 10 833.38 4p 3P1 − 3d 3P2 1.5 1.02e−01 84.14
H2O Telluric 10 834.00 101.31
Na I Solar 10 834.84 3d 2D5/2 − 6f 2F5/2 1.03 2.62e−03 124.56
Na I Solar 10 834.84 3d 2D5/2 − 6f 2F7/2 1.07 5.24e−02 124.56
Na I Solar 10 834.90 3d 2D3/2 − 6f 2F5/2 0.90 5.50e−02 126.22
H2O Telluric 10 837.97 211.20
Ca I Solar 10 838.97 4p 3P2 − 3d 3P2 1.5 1.85e−01 238.88

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