The Submillimeter Array 1.3 mm line survey of Arp 220

S. Martín; M. Krips; J. Martín-Pintado; S. Aalto; J.-H. Zhao; A. B. Peck; G. R. Petitpas; R. Monje; T. R. Greve; T. An

doi:10.1051/0004-6361/201015855

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Volume 527 (March 2011)

A&A, 527 (2011) A36

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Table 1

Observational details of each frequency setup.

Date	Frequency	Config.^a	τ₂₂₅^b	Flux	Gain	Bandpass
	(BAND)	(# Ant.)

2007 May 06	215.032 GHz (USB)	SC (7)	0.10	Titan	J1613+342	3c273
	217.016 GHz (USB)	SC (6)	0.09	Uranus	J1613+342	Uranus
2007 May 07	219.000 GHz (USB)	SC (5)	0.05	Callisto	J1613+342	3c273
2007 May 08	220.984 GHz (USB)	SC (5)	0.05	Callisto	J1613+342	3c273
2008 Feb. 26	213.048 GHz (USB)	C (7)	0.16	Titan	J1504+104	3c273
	222.968 GHz (LSB)	C (8)	0.17	Callisto	J1504+104	J1924-292, Callisto
2008 Mar. 03	224.952 GHz (LSB)	C (8)	0.19	Titan	J1504+104	3c273
	226.936 GHz (LSB)	C (8)	0.20	Titan	J1504+104	J1924-292, Callisto
2008 Mar. 04	222.968 GHz (LSB)	C (8)	0.21	Titan	J1504+104	3c273, Titan
2008 Mar. 05	228.920 GHz (LSB)	C (7)	0.20	Titan	J1504+104	3c273, Titan
	230.904 GHz (LSB)	C (7)	0.20	Callisto	J1504+104	3c273, Callisto, J1924-292

Notes.

^(a)

Array configuration (SC: Subcompact – C: Compact) and number of antennae available.

^(b)

Average zenith opacity at 225 GHz during observations.

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