Table 1.
General information about the sample and the data
| ID | RAALMA | DecALMA | AGN (a) | PSFALMA,nat | PSFALMA,tap | IFU | IFUband | PSFIFU |
|---|---|---|---|---|---|---|---|---|
| [J2000] | [J2000] | [arcsec] | [arcsec] | [arcsec] | ||||
| ALESS17.1 | 53.030410 | −27.855765 | X-ray | 0.17 × 0.15 | 0.66 × 0.62 | SINFONI | H | 0.65 |
| ALESS66.1 | 53.383053 | −27.902645 | No | 0.17 × 0.13 | 0.47 × 0.45 | SINFONI | K | 0.48 |
| ALESS67.1 | 53.179981 | −27.920649 | X-ray | 0.18 × 0.15 | 0.66 × 0.62 | SINFONI | HK | 0.66 |
| ALESS75.1 | 52.863303 | −27.930928 | IR | 0.17 × 0.12 | 0.57 × 0.54 | SINFONI | HK | 0.56 |
| AS2UDS292.0 | 34.322638 | −5.2300513 | X-ray | 0.22 × 0.19 | 0.46 × 0.42 | KMOS | K | 0.46 |
| AS2UDS412.0 | 34.422392 | −5.1810288 | No | 0.25 × 0.23 | 0.56 × 0.52 | KMOS | K | 0.55 |
Notes.
The AGN classification in the X-ray is based on catalog matching; ALESS SMGs are matched to the Chandra 7 Ms catalog and classified as AGN based on the criteria set in Luo et al. (2017). The AS2UDS SMGs are matched to the Chandra X-UDS catalog (Kocevski et al. 2018) with a simple luminosity cut of L2 − 10 kev > 3 × 1042 erg s−1, which is one of the criteria used in Luo et al. (2017). The steep slope in mid-infrared has suggested that ALESS75.1 is an IR AGN (Simpson et al. 2014; Stanley et al. 2018).
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