Fig. 2.
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Integrated H- and K-band spectra extracted from SINFONI datacubes of cid_1143 (top), cid_2682 (middle), and cid_451 (bottom), with a radius aperture of 0.25″, after subtracting continuum emission that was modelled with a first-degree polynomial. Same as in Fig. 2. In the K-band spectrum of cid_1143, we fit only the Hα line emission due to the low S/N (S/N < 2) of this dataset.
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