SIMBAD references

We present Hα-region integral-field spectroscopy for 137 low-inclination, intermediate to late-type galaxies. Spectroscopic data, obtained with SparsePak and the Bench Spectrograph on the WIYN 3.5 m telescope, span 6475-6880 Å with an instrumental resolution of 13 km s^–1 (σ). The spectral range includes Hα and [N II]λλ6548, 6584 for every source, and in most cases includes [S II]λλ6717, 6731. We present and publicly release 18,288 calibrated spectra and visually inspected Gaussian line fits to the Hα emission. Most measurements yield a signal-to-noise ratio above 5 in integrated Hα line flux, adequate to derive reliable line centroids and widths. Second kinematic components are required to adequately describe the emission-line profile in 15% of reliable data. The Hα velocity dispersion distribution peaks at 18 km s^–1, modestly increasing with Hα surface brightness, reaching 20 km s^–1 at Σ_Hα = 10⁴⁰ erg s^–1 kpc^–2. Lower-flux secondary components, when present, have widths of ∼50 km s^–1. These results agree well with previous echelle measurements of nearby galaxies. Velocity-field analysis yields kinematic inclinations, with a sample mean of 26°. Large kinematic asymmetries systematically affect kinematic inclination estimates in a small fraction of our sample. When deviations from circular motion are below 10% of the projected velocity, kinematic inclinations are consistent, within errors, to estimates from inverting the Tully-Fisher relation. This confirms previous disk-submaximality estimates for galaxies with regular kinematics based on inclinations derived from inverting the Tully-Fisher relation.