OLIVA, ErnestoErnestoOLIVA0000-0002-6040-5849ORIGLIA, LiviaLiviaORIGLIA0000-0002-8637-2109SCUDERI, SalvatoreSalvatoreSCUDERI0000-0001-9275-9492BENATTI, SERENASERENABENATTI0000-0003-2763-9560Carleo, I.I.Carleo0000-0003-1492-1591Lapenna, E.E.Lapenna0000-0002-4638-3495Mucciarelli, A.A.Mucciarelli0000-0002-9825-7407BAFFA, CarloCarloBAFFABiliotti, V.V.Biliotti0000-0001-6407-8032CARBONARO, LUCALUCACARBONARO0000-0002-9123-0412Falcini, G.G.Falcini0000-0002-4935-100XGIANI, ElisabettaElisabettaGIANI0000-0002-6725-3825Iuzzolino, M.M.IuzzolinoMassi, F.F.MassiSANNA, NicolettaNicolettaSANNASozzi, M.M.SozziTozzi, A.A.TozziGhedina, A.A.GhedinaGhinassi, F.F.GhinassiLodi, M.M.LodiHarutyunyan, A.A.HarutyunyanPedani, M.M.Pedani2020-03-202020-03-202015http://hdl.handle.net/20.500.12386/23440Tables 1 and 2 list the wavelengths and relative photon fluxes of the OH airglow lines (Table 1) and the wavelengths and relative photon fluxes of other airglow lines (Table 2), measured in the Near-Infrared with the echelle spectrometer GIANO at the Telescopio Nazionale Galileo. The intensities of the lines (flux) are expressed in units of photons/m<SUP>2</SUP>/s, normalised to the intensity of the brightest line (in Table1), which is set to 10<SUP>4</SUP>. The wavelengths are in vacuum and expressed in Angstrom. The Wavelengths in Table 1 are computed from the most complete and accurate OH molecular parameters available in the literature (Bernath & Colin, 2009, J. Mol. Spec., 257, 20). Table 4 contains the observed spectrum in the Y,J and H photometric bands. The wavelengths are in vaccuum and in Angstrom. The spectral flux is expressed in units of photons/m<SUP>2</SUP>/s/Angstrom, please note that the flux calibration is uncertain (see the paper for details). <P />(3 data files). <P />enDatabasehttp://vizier.u-strasbg.fr/viz-bin/VizieR?-source=J/A+A/581/A472015yCat..35810047O