Table 1.
NOEMA and 30m observations.
Survey | Telescope | Lines | Δtobs (in SWAN FoV) | Native resolution |
---|---|---|---|---|
SWAN | NOEMA | C2H(1−0), HNCO(4−3), HCN(1−0), HCO+(1−0), | 214 h | 2.4″ − 3.0″ |
HNC(1−0), N2H+(1−0), C18O(1−0), HNCO(5−4), | ||||
13CO(1−0) | ||||
SWAN-new | IRAM-30m | Same as SWAN-NOEMA | 55 h | 23.6″ − 29.8″ |
CLAWS | IRAM-30m | C18O(1−0), 13CO(1−0), N2H+(1−0) | ∼14 h | 27 − 32″ |
EMPIRE | IRAM-30m | HCN(1−0), HNC(1−0), HCO+(1−0) | ∼14 h | 26 − 34″ |
Notes. Observational data used in the SWAN survey, including archival data from EMPIRE (Jiménez-Donaire et al. 2019) and CLAWS (den Brok et al. 2022). The observing time tobs refers to the estimated observing time inside the FoV of SWAN (see Fig. 1). All 30m datasets (SWAN-new, EMPIRE, CLAWS) are combined to the “SWAN-30m” dataset before merging with the NOEMA data via joint deconvolution. Native resolution refers to the resolution after imaging.
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