Multiplicity datasets using Gaia DR3: CARMENES M-dwarf pairs; ultra-wide pairs (ρ ≥ 1000 arcsec); and systems within 10 pc. They include WDS identifiers (or, if absent, the stellar name in parentheses), separations in au, masses in solar masses, binding energies (|U*₉|) in units of 10³³ J, and information on the presence or absence of planets.