All Tables

Table 1: Observational and measurement data. Given are: star name (observed at t - Terskol (Russia), f - FEROS, H - HARPS La Silla (Chile), b - Bohyunsan (S. Korea), spectral and luminosity class, reddening, EWs (in mÅ) of CN and CH molecules, their calculated column densities (in 10¹² cm^-2), and EWs (in mÅ) of diffuse 5797 and 5780 bands with errors in each bracket. We also designate the lines of sight with EW $_{\rm CN}$ > 14 mÅ^a and EW $_{\rm CH}$ > 20 mÅ^b. With symbol: we mark lines of sight with uncertain column density of CN molecule based on measurements of R(0) line and uncertain column densities of CH molecule based on measurements of saturated CH A-X band at 4300 Å. In the case of the 5797 DIB blended with the stellar C IV 5801.313 Å line we avoid the EW measurement as being very uncertain (bl).