Notes.The table gives the number of detected transitions for each species, the range of upper level energies, the typical v_lsr and FWHM, the total line flux in K   km   s^-1 and in Wm^-2, where the exponential is given in brackets, and a note on the dominant line profile components. The line counts include hyperfine components and blends. Blends between species are excluded from the per-species flux sums, but included in the total line flux measured in the survey. The species are grouped similarly to Sect. 3.6. Dashes represent cases where a good single Gaussian fit was not obtained, mostly due to blending.

Reference. ^s1Winnewisser et al. (1997); ^s2Cazzoli et al. (2004); ^s3Klapper et al. (2001); ^s4Klapper et al. (2003); ^s5Pickett et al. (2005); ^s6Johns (1985); ^s7Blake et al. (1986a); ^s8Müller et al. (2005); ^s9Mürtz et al. (1998); ^s10Müller et al. (2004); ^s11Müller et al. (2000b); ^s12Lattanzi et al. (2007); ^s13Pagani et al. (2009); ^s14Cooksy et al. (1986b); ^s15Cooksy et al. (1986a); ^s16Müller (2010); ^s17McCarthy et al. (2006); ^s18Padovani et al. (2009); ^s19Thorwirth et al. (2003); ^s20Cazzoli & Puzzarini (2005); ^s21Thorwirth et al. (2000); ^s22Klisch et al. (1995); ^s23Flores-Mijangos et al. (2004); ^s24Müller et al. (1999); ^s25Yu et al. (2010); ^s26Huang et al. (2011); ^s27Kim & Yamamoto (2003); ^s28Belov (1995); ^s29Bogey et al. (1997); ^s30Müller et al. (2000a); ^s31Brown & Müller (2009); ^s32Nolt et al. (1987); ^s33Araki et al. (2001); ^s34Brünken et al. (2004); ^s35Takano et al. (1998); ^s36Fusina et al. (1988).