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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 . $ {{\overset{\prime\prime}{.}}} $51 × 0 . $ {{\overset{\prime\prime}{.}}} $43 0.198 0.011 0.30 ± 0.013
2018.1.01488.S 216.71 15/13900 1.1 0 . $ {{\overset{\prime\prime}{.}}} $10 × 0 . $ {{\overset{\prime\prime}{.}}} $08 0.178 0.018 0.28 ± 0.02
2018.1.01488.S 691.47 37/1154 1.1 0 . $ {{\overset{\prime\prime}{.}}} $19 × 0 . $ {{\overset{\prime\prime}{.}}} $15 9.65 0.407 31.5 ± 2.4
NGC 4418 2018.1.00939.S 167.575 155/1500 0.4 0 . $ {{\overset{\prime\prime}{.}}} $21 × 0 . $ {{\overset{\prime\prime}{.}}} $16 18.4 0.076 23.4 ± 0.15
2012.1.00377.S 216.71 15/1600 0.1 0 . $ {{\overset{\prime\prime}{.}}} $37 × 0 . $ {{\overset{\prime\prime}{.}}} $23 24.1 0.643 45.0 ± 1.18
NGC 1266 2018.1.00423.S 167.55 66/565 0.9 0 . $ {{\overset{\prime\prime}{.}}} $52 × 0 . $ {{\overset{\prime\prime}{.}}} $47 2.59 0.013 3.84 ± 0.11
2011.1.00511.S 216.71 21/384 1.4 1 . $ {{\overset{\prime\prime}{.}}} $26 × 0 . $ {{\overset{\prime\prime}{.}}} $82 5.22 0.120 5.74 ± 0.24

Notes.

(a)

Central frequency of the spectral window which include the targeted line.

(b)

On-source observation time.

(c)

Noise level determined using CLASS package in GILDAS (http://www.iram.fr/IRAMFR/GILDAS).

(d)

Flux density determined with CASA from the region with over 3σ emission for each source.

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