Table 2.
SINFONI observations of the 12 SUPER type-2 AGN.
| Target | Obs mode | H band | K band | ||||||
|---|---|---|---|---|---|---|---|---|---|
| mag (AB) | texp [hr] | θPSF [″] | Detected lines | mag (AB) | texp [hr] | θPSF [″] | Detected lines | ||
| (θPSF [kpc]) | (θPSF [kpc]) | ||||||||
| XID36 | AO | 21.45 | 5.3 | 0.29 × 0.26 | Hβ, [O III] | 21.13 | 2.0 | 0.15 × 0.15 | Hα, [N II], [S II] |
| (2.4 × 2.1) | 1.2 × 1.2 | ||||||||
| XID57 | AO | – | 3.0 | 0.32 × 0.30 | – | – | 1.0 | 0.33 × 0.27 | – |
| (2.6 × 2.5) | (2.7 × 2.2) | ||||||||
| XID419 | AO | 22.69 ( * ) | 0.8 | 0.47 × 0.52 | [O III] | 21.85 ( * ) | 1.0 | 0.24 × 0.22 | Hα, [N II] |
| (3.9 × 4.3) | (2.0 × 1.8) | ||||||||
| XID427 | AO | 22.72 | 1.0 | 0.23 × 0.20 | – | 21.90 ( * ) | 1.0 | 0.28 × 0.20 | – |
| (1.9 × 1.6) | (2.3 × 1.6) | ||||||||
| XID522 | AO | – | 1.0 | 0.25 × 0.20 | – | – | 1.0 | 0.25 × 0.19 | – |
| (2.0 × 1.6) | (2.0 × 1.6) | ||||||||
| XID614 | AO | 22.41 ( * ) | 11.5 | 0.38 × 0.37 | Hβ, [O III] | 21.79 | 3.5 | 0.27 × 0.28 | Hα, [N II] |
| (3.1 × 3.0) | (2.2 × 2.3) | ||||||||
| cid_1057 | AO | 21.80 ( * ) | 2.0 | 0.32 × 0.30 | Hβ, [O III] | 20.91 | 0.7 | 0.46 × 0.43 | – |
| (2.6 × 2.5) | (3.8 × 3.6) | ||||||||
| cid_451 | AO | 21.73 | 5.0 | 0.28 × 0.30 | [O III] | 21.69 ( * ) | 2.0 | 0.28 × 0.27 | Hα, [N II] |
| (2.3 × 2.4) | (2.3 × 2.2) | ||||||||
| cid_2682 | AO | 21.58 | 5.6 | 0.33 × 0.28 | [O III] | 21.01 ( * ) | 1.8 | 0.28 × 0.25 | Hα, [N II] |
| (2.7 × 2.3) | (2.3 × 2.0) | ||||||||
| cid_1143 | AO | 22.44 | 5.5 | 0.41 × 0.38 | Hβ, [O III] | 22.66 | 2.0 | 0.30 × 0.30 | Hα( † ) |
| (3.3 × 3.1) | (2.4 × 2.4) | ||||||||
| cid_1253 | noAO | 22.45 | 4.0 | 0.68 × 0.63 | – | 21.61 | 1.0 | 0.66 × 0.61 | – |
| (5.6 × 5.2) | (5.5 × 5.1) | ||||||||
| HK band | |||||||||
| mag (AB) | texp [hr] | θPSF [″] | Detected lines | ||||||
| (θPSF [kpc]) | |||||||||
| cid_971 | noAO | – | 1.8 | 0.42 × 0.39 | – | ||||
| (3.4 × 3.2) | |||||||||
Notes. For each target, we list the observing mode (AO/noAO) and the following parameters for each adopted grating (H, K, HK): The absolute (AB) magnitude measured from SINFONI-integrated spectra accounting for the corresponding filter transmission curve, total on-source exposure time texp, spatial resolution θPSF (computed as PSF FWHM), and detected emission lines for the objects with [O III] detected at S/N > 2. For these sources, a dagger indicates marginal detections (S/N < 2) of Hα. The AB magnitudes marked with an asterisk required a correction factor (∼2) to match the previous synthetic measurements (Circosta et al. 2018).
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