with the H$+$K grating which covers the H and K band simultaneously at R$\sim$1500 (corresponding to FWHM$\approx$200 km s$^{-1}$) and is sufficient to resolve all emission lines spectrally in our targets. Some galaxies, in particular those observed during the visitor run 079.A-617, were observed in the H and K-band individually. Where appropriate, for example owing to the redshift of the source, we also observed in the J band. The spectral resolving power in the J, H, and K band is R$\sim$2000, R$\sim$3000, and R$\sim$4000, respectively. Table \[tab:sample\] lists all bands in which each target was observed. The bands covered for each source can also be found in the detailed descriptions of individual sources in Appendix \[sec:individualobjects\].

New and archival VLA observations {#ssec:vlaobs}
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We also collected a set of new VLA continuum imaging for parts of our sample through program AN 0129, to increase the number of targets with arcsecond resolution radio morphologies. C. Carilli kindly shared his radio imaging of 17 sources with us, which had previously been discussed by @carilli97 and @pentericci00, and we obtained the cm imaging of another eight sources from the VLA archive. Tab. \[tab:radioobs\] lists the sets of the new and archival radio images 