Complex organic molecules in strongly UV-irradiated gas

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Table 1

Observed frequency ranges and telescope parameters.

Rec.^a	Backend	Freq.^b	δv ^c	^d	HPBW^e
		[GHz]	[km s^-1]		[arcsec]

E0	FFTS	80−117	0.75−0.51	0.87−0.82	31−21

E1	WILMA	128−176	4.7−3.4	0.80−0.74	19−14

E2	FFTS	202−275	0.30−0.22	0.70−0.56	12−9

E3	FFTS	275−305	0.22−0.20	0.56−0.50	9−8
E3	FFTS	328−359	0.18−0.17	0.46−0.40	8−7

Notes.

^(a)

Emir receiver.

^(b)

Observed frequency range.

^(c)

Spectral resolution in velocity units (δv) in the observed frequency ranges.

^(d)

Antenna efficiencies.

^(e)

The half power beam width can be well fitted by HPBW[arcsec] ≈ 2460/Frequency[GHz].

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