CHEMOUT: CHEMical complexity in star-forming regions of the OUTer Galaxy - I. Organic molecules and tracers of star-formation activity

Free Access

Table 2

Spectral windows observed and observational parameters.

Spectral windows (GHz)	HPBW (″)	V_res^(a) (kms^-1)	η_MB^(b)
85.310–87.130	28	~0.16	0.85
88.590–90.410	27	~0.16	0.84
151.750–153.570	15	~0.096	0.77
148.470–150.290	15	~0.096	0.77

Notes. ^(a)Velocity resolution in the spectrum. ^(b)Defined as η_MB = B_eff/F_eff, where B_eff is the main beam efficiency and F_eff the forward efficiency.

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.