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Table 2.
Description of the ALMA observations and the continuum results.
| Object | Project ID | νobs(a) | bmin, bmax | tint(b) | θmaj × θmin | Icont, peak | rmscont(c) | Scont(d) |
|---|---|---|---|---|---|---|---|---|
| [GHz] | [m] | [h] | [arcsec2] | [mJy beam−1] | [mJy beam−1] | [mJy] | ||
| NGC 1377 | 2018.1.00423.S | 167.76 | 67/585 | 1.1 | 0 51 × 0 43 |
0.198 | 0.011 | 0.30 ± 0.013 |
| 2018.1.01488.S | 216.71 | 15/13900 | 1.1 | 0 10 × 0 08 |
0.178 | 0.018 | 0.28 ± 0.02 | |
| 2018.1.01488.S | 691.47 | 37/1154 | 1.1 | 0 19 × 0 15 |
9.65 | 0.407 | 31.5 ± 2.4 | |
| NGC 4418 | 2018.1.00939.S | 167.575 | 155/1500 | 0.4 | 0 21 × 0 16 |
18.4 | 0.076 | 23.4 ± 0.15 |
| 2012.1.00377.S | 216.71 | 15/1600 | 0.1 | 0 37 × 0 23 |
24.1 | 0.643 | 45.0 ± 1.18 | |
| NGC 1266 | 2018.1.00423.S | 167.55 | 66/565 | 0.9 | 0 52 × 0 47 |
2.59 | 0.013 | 3.84 ± 0.11 |
| 2011.1.00511.S | 216.71 | 21/384 | 1.4 | 1 26 × 0 82 |
5.22 | 0.120 | 5.74 ± 0.24 |
Notes.
(c)
Noise level determined using CLASS package in GILDAS (http://www.iram.fr/IRAMFR/GILDAS).
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