Probing the effects of external irradiation on low-mass protostars through unbiased line surveys

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Table 2

Observational parameters of the APEX observations (this work; IRS7B line survey and CrA source survey) and the ASTE line survey of IRS7B (Watanabe et al. 2012).

Window	Frequency range	Beam size
	[GHz]	[′′]	[AU]

IRS7B survey	217.2–245.5^a	26–29	3300–3800
1.4 mm	216.1–220.1	29	3700
0.9 mm	336.9–340.9	19	2400
0.8 mm	361.8–365.8^b	17	2200

ASTE 0.8 mm	332.0–364.0	21–23	2700–3000
ASTE 0.7 mm	435.0–437.0	17	2300
ASTE 0.7 mm	459.2–461.2	16	2100

Notes.

^(a)

The 217.2–217.9 GHz portion is only covered at a low S/N level.

^(b)

In most sources only 361.8–364.3 GHz, due to high noise levels and baseline issues in the upper sideband.

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