[ASTRO\]SOURCE /DOPPLER Type Value Can be used to be abe to take into account LSR velocities or redshift in the frequency coverage computations (NOEMA and PICOVELETA) without defining a full source (i.e. coordinates, V(LSR/G) and V(G/OBS) veloci- ties are not computed. In that case V(SOU/OBS)=V(S/LSR). Type can be REDSHIFT or LSR Value is the value (real) in the corresponding type of doppler.