Analysis results from the NGC 3259 Binospec IFU datacube. First (top) row: 1. Stellar population velocity (V_stars). 2. Stellar population velocity dispersion (σ_stars). 3. Simple stellar population age (T_SSP). 4. SSP ([Z/H]_SSP) metallicity. Second row: 1. Hα emission line velocity (V_gas). 2. Hα emission line velocity dispersion (σ_gas); 3. Reduced χ² in each spaxel. 4. Hα emission line flux. Third row: emission line ratios: 1. [O III]/Hβ. 2. [N II]/Hα; 3. Balmer decrement for the narrow-line component, Hα/Hβ. 4. [O III] emission line flux. Fourth (bottom) row: BPT diagrams (1 & 2) with the position of each spaxel with color-coded inclination-corrected distance from the galaxy center, underlying grey points represent position of galaxies from RCSED (Chilingarian et al. 2017). 3–4: Color-coded classification of spaxels according to their position on the BPT diagram. In each panel (rows 1–3) we show the center of the broad-line point source with a black cross.