Table 2.
Parameters of the ALMA observations.
Name | σcont[MSR − HSR] | σCO[MSR − HSR] | σHCO+[MSR − HSR] | BeamMSR | BeamHSR | FOV | LAS |
---|---|---|---|---|---|---|---|
μJy beam−1 | mJy beam−1 | mJy beam−1 | ″ × ″ @° (pc × pc) | ″ × ″ @° (pc × pc) | ″ (kpc) | ″ (pc) | |
NGC 6300 | 36–45 | 0.52–0.62 | 0.79–1.00 | ![]() |
![]() |
17 (1.2) | 4 (280) |
NGC 5643 | 32–38 | 0.52–0.57 | 0.77–1.00 | ![]() |
![]() |
17 (1.4) | 4 (340) |
NGC 7314 | 25–27 | 0.45–0.50 | 0.61–0.69 | ![]() |
![]() |
17 (1.5) | 4 (350) |
NGC 4388 | 36–45 | 0.62–0.63 | 0.84–0.99 | ![]() |
![]() |
17 (1.5) | 4 (360) |
NGC 4941 | 24–33 | 0.48–0.58 | 0.60–0.73 | ![]() |
![]() |
17 (1.7) | 4 (410) |
NGC 7213 | 54–60 | 0.45–0.60 | 0.56–NA | ![]() |
![]() |
17 (1.9) | 4 (440) |
NGC 7582 | 43–46 | 0.55–0.65 | 0.75–0.91 | ![]() |
![]() |
17 (1.9) | 4 (450) |
NGC 6814 | 24–29 | 0.42–0.54 | 0.53–NA | ![]() |
![]() |
17 (1.9) | 4 (460) |
NGC 5506 | 31–36 | 0.51–0.59 | 0.65–0.79 | ![]() |
![]() |
17 (2.2) | 4 (530) |
NGC 7465 | 23–30 | 0.42–0.56 | 0.49–0.67 | ![]() |
![]() |
17 (2.3) | 4 (540) |
NGC 1068 | 46–46 | 0.23–0.23 | 0.28–0.28 | ![]() |
![]() |
17 (1.2) | 1.8 (130) |
NGC 1365 | 30 | 0.60 | – | ![]() |
– | 17 (1.6) | 3 (275) |
NGC 3227 | 31 | 0.51 | – | ![]() |
– | 17 (2.0) | 1 (120) |
Notes. Columns (2)–(4) list the range of 1σ sensitivities for the continuum as well as for the CO and HCO+ line observations. Line sensitivities are derived for channels of 10 km s−1-width (except for NGC 1068, where García-Burillo et al. (2019) used 20 km s−1-wide channels). The range in Cols. (2)–(4) accounts for the moderate spatial resolution data sets (MSR) and the high spatial resolution data sets (HSR) obtained by using a different robust weighting parameter of the visibilities in the UV plane: robust = 1 (0.1) for the MSR (HSR) configuration; these are available for all sources except for NGC 1365 and NGC 3227. Columns (5) and (6) list the range of spatial resolutions (in ″ and pc) reached for the MSR and HSR observations respectively. The field-of-view (FOV) and largest scale recovered (LAS) are listed in Cols. (7) and (8) in ″ and kpc and pc, respectively.
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