The catalog is based on the spectral extraction performed automatically by the HARPS-N Data Reduction pipeline. The basic processing steps consist in bias subtraction (the bias is computed on the over-scan regions of the frame), spectrum extraction, flat fielding, wavelength calibration, and normalization of the blaze continuum. The blaze-corrected spectrum is derived by dividing the extracted order spectra by the blaze function. The dust-scattered solar light is removed using a high-resolution solar analogue spectrum (Land 107-684) degraded to the same spectral resolution. Table C1 reports the wavelength corresponding to the sky emission and the relative intensity. Table C2 provides the observed wavelength ({lambda}), the relative intensity (I_rel_), the name of the molecule, and the transition (if mentioned in the reference).

Pamela Cambianica, pamela.cambianica(at)inaf.it