A millimeter survey of ultra-compact HII-regions and associated molecular clouds

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Table 2:

Spectral resolution and bandwidth available with the receiver/backend combinations used.
		Channel spacing		Bandwidth
receiver	backend	MHz	km s^-1	MHz	km s^-1	transition
	VESPA	1.25	1.6	288	370	H $30\alpha$ , HCO⁺(3-2)
HERA	WILMA	2.0	2.6	930	1200	H $30\alpha$ , HCO⁺(3-2)
	FB	4.0	5.2	1024	1300	H $30\alpha$
A 100, B 100	VESPA	0.078	0.26	140	480	H $39\alpha$ , HCO⁺(1-0)
A 230, B 230	VESPA	0.313	0.36	220	249	H¹³CO⁺(3-2), HC¹⁸O⁺(3-2)

Notes. VESPA and WILMA are autocorrelators, FB is a low resolution filterbank.

Source LaTeX | All tables | In the text

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