the $J$ and $H$ bands. The measured flux-ratios of the components in each band are combined with the total magnitudes [@Rao2011] to assign individual magnitudes to each of the interacting components. The resulting magnitudes are reported in Table \[tab:refparam\], and complement the optical photometry in the SED-fitting procedure (see Section \[sec:SED\]).

Results {#sec:results}
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[r | c c c | l c c c c c c c c ]{} Quasar field

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& &\

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& $\theta$ & $b$ & $z_{\text{em}}^{\text{SPEC}}$ & Transition & $\lambda _0$ & FWHM & Line-flux\

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& \["\] & \[kpc\] & & & \[Å\] & \[Å\] & \[$\times 10^{-17}$ erg s$^{-1}$ cm$^{-2}$\]\

HE1122-1649 & 3.6 & 25.6 & $0.68249 \pm 0.00003$ & \[<span style="font-variant:small-caps;">O ii</span>\] & 3727,3729 & $6.3 \pm 0.7$ & $17.7 \pm 2.4$\
& & & & H$\beta$ & 4861.39 & $6.0 \pm 0.5$ & $4.8 \pm 0.6$\

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Q0153+0009 & 4.9 & 36.6 & $0.77085 \pm 0.00003$ & H5 & 4340.47 & $9.5 \pm 1.0$ & $3.0 \pm 0.4$\
& & & & H$\beta$ & 4861.33 & $9.5 \pm 0.6$ & $6.3 \pm 0.6$\
& & & & \[<span style="font-variant:small-caps;">O iii</span>\] & 5007 & $9.8 \pm 0.5$ & $7.5 \pm 0.5$\

