CHEMOUT: CHEMical complexity in star-forming regions of the OUTer Galaxy - V. Chemical composition gradients as a function of the galactocentric radius

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Table 1

Observational set ups of CHEMOUT used in this paper.


Spectral windows (GHz)	Beam size (″)	V_res (km s⁻¹)	B_eff	F_eff	T_sys
85.310–87.130^a	28	~0.16	0.80	0.95	~120–200
88.590–90.410^a	27	~0.16	0.80	0.95	~120–200
90.400–98.180^b	25	~0.6	0.80	0.95	~100–150
140.720–148.500^b	17	~0.4	0.73	0.93	~150–300
148.470–150.290^a	15	~0.096	0.73	0.93	>300
151.750–153.570^a	15	~0.096	0.73	0.93	>300

Notes. The observational parameters presented include the frequency ranges observed (at 3 and 2 mm), velocity resolution (V_res) of the spectra, main beam efficiency (B_eff), forward efficiency (F_eff), and system temperature (T_sys). ^(a)Project 004-18 ^(b)Project 042-21.

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