Millimeter imaging of submillimeter galaxies in the COSMOS field: redshift distribution

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Volume 548 (December 2012)

A&A, 548 (2012) A4

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Table 5

Master table of interferometrically observed SMGs in the COSMOS field.

Source	Other names	(sub)mm-interferometry		Statistical
		observed	detected	interferometric sample


AzTEC-1^(1,5)	COSLA-60⁽⁴⁾, AzTEC/C5⁽²⁾	SMA, CARMA, PdBI	^√	1.1mm, 870 μm, least-biased-870 μm
AzTEC-2^(1,5)	COSLA-4⁽⁴⁾, AzTEC/C3⁽²⁾	SMA, CARMA	^√	1.1mm, 870 μm, least-biased-870 μm
AzTEC-3^(1,5)	AzTEC/C138⁽²⁾	SMA, CARMA, PdBI	^√	1.1 mm
AzTEC-4^(1,5)	AzTEC/C4⁽²⁾	SMA	^√	1.1 mm
AzTEC-5^(1,5)	AzTEC/C42⁽²⁾	SMA	^√	1.1 mm
AzTEC-6^(1,5)	AzTEC/C106⁽²⁾	SMA	^√	1.1 mm
AzTEC-7^(1,5)		SMA	^√	1.1 mm
AzTEC-8^(1,6)	COSLA-73⁽⁴⁾, AzTEC/C2⁽²⁾	SMA	^√	1.1mm, 870 μm, least-biased-870 μm
AzTEC-9^(1,6)	COSLA-3⁽⁴⁾, AzTEC/C14⁽²⁾	SMA	^√	1.1mm, 870 μm, least-biased-870 μm
AzTEC-10^(1,6)		SMA	^√	1.1 mm
AzTEC-11^(1,6)	AzTEC-11-N⁽⁶⁾, AzTEC-11-S⁽⁶⁾, AzTEC/C22⁽²⁾	SMA	^√	1.1 mm
AzTEC-12^(1,6)	AzTEC/C18⁽²⁾	SMA	^√	1.1 mm
AzTEC-13^(1,6)	COSLA-158⁽⁴⁾	SMA	^√	1.1mm, 870 μm, least-biased-870 μm
AzTEC-14^(1,6)	AzTEC-14-E⁽⁶⁾, AzTEC-14-W⁽⁶⁾	SMA	^√	1.1 mm
AzTEC-15^(1,6)	AzTEC/C10⁽²⁾	SMA	^√	1.1 mm
AzTEC-16^(1,13)	–	CARMA	^√	–
J1000+0234^(1,14)	AzTEC/C17⁽²⁾	VLA	^√	–
AzTEC/C1^(2,7)	COSLA-89⁽⁴⁾	CARMA	^√	870 μm
Cosbo-1^(3,16)	COSLA-1⁽⁴⁾, AzTEC/C7⁽²⁾	SMA	^√	870 μm, least-biased-870 μm
Cosbo-3^(3,7)	COSLA-2⁽⁴⁾, AzTEC/C6⁽²⁾	CARMA	^√	870 μm, least-biased-870 μm
Cosbo-8^(3,7)	AzTEC/C118⁽²⁾	CARMA	^√	–
Cosbo-14^(3,16)		SMA	^√	–
COSLA-5^(4,17)	Cosbo-12⁽³⁾	PdBI	^√	870 μm
COSLA-6^(4,17)	COSLA-6-N⁽¹⁷⁾, COSLA-6-S⁽¹⁷⁾	PdBI	^√	870 μm, least-biased-870 μm
COSLA-8^(4,17)		PdBI	^√	870 μm
COSLA-9^(4,17)	AzTEC/C8⁽²⁾, COSLA-9-N⁽¹⁷⁾, COSLA-9-S⁽¹⁷⁾	PdBI	^√	870 μm
COSLA-10^(4,17)	Cosbo-6⁽³⁾	PdBI	–	–
COSLA-11^(4,17)	COSLA-11-N⁽¹⁷⁾, COSLA-11-S⁽¹⁷⁾	PdBI	^√	870 μm
COSLA-12^(4,17)		PdBI	–	–
COSLA-13^(4,17)	AzTEC/C145⁽²⁾, Cosbo-5⁽³⁾	PdBI	^√	870 μm
COSLA-14^(4,17)	AzTEC/C176⁽²⁾, Cosbo-10⁽³⁾	PdBI	–	–
COSLA-16^(4,17)	COSLA-16-N⁽¹⁷⁾, COSLA-16-S⁽¹⁷⁾	PdBI	^√	870 μm
COSLA-17^(4,17)	AzTEC/C12⁽²⁾, COSLA-17-N⁽¹⁷⁾, COSLA-17-S⁽¹⁷⁾	PdBI	^√	870 μm, least-biased-870 μm
COSLA-18^(4,17)	AzTEC/C98⁽²⁾	PdBI	^√	870 μm
COSLA-19^(4,17)	AzTEC/C34⁽²⁾, Cosbo-4⁽³⁾	PdBI	^√	870 μm
COSLA-23^(4,17)	Cosbo-2⁽³⁾, COSLA-23-N⁽¹⁷⁾, COSLA-23-S⁽¹⁷⁾	PdBI	^√	870 μm, least-biased-870 μm
COSLA-25^(4,17)		PdBI	–	–
COSLA-30^(4,17)		PdBI	–	–
COSLA-33^(4,17)		PdBI	^√	870 μm
COSLA-35^(4,17)	AzTEC/C38⁽²⁾	PdBI	^√	870 μm
COSLA-38^(4,17)	Cosbo-19⁽³⁾	PdBI	^√	870 μm
COSLA-40^(4,17)	AzTEC/C117⁽²⁾	PdBI	^√	870 μm
COSLA-47^(4,17)	AzTEC/C80⁽²⁾	PdBI	^√	870 μm, least-biased-870 μm
COSLA-48^(4,17)	AzTEC/C160, Cosbo-7⁽³⁾	PdBI	–	–
COSLA-50^(4,17)		PdBI	–	–
COSLA-51^(4,17)		PdBI	–	–
COSLA-54^(4,17)	AzTEC/C13⁽²⁾	PdBI	^√	870 μm, least-biased-870 μm
COSLA-62^(4,17)		PdBI	–	–
COSLA-128^(4,17)		PdBI	^√	870 μm, least-biased-870 μm
COSLA-161^(4,17)	AzTEC/C158⁽²⁾, Cosbo-13S⁽³⁾	PdBI	^√	870 μm, least-biased-870 μm

References. (1) Scott et al. (2008); (2) Aretxaga et al. (2011); (3) Bertoldi et al. (2007); (4) Navarette et al. (in prep.); (5) Younger et al. (2007); (6) Younger et al. (2009); (7) Smolčić et al. (2011); (8) Baloković et al. (in prep.); (9) Capak et al. (2010); Riechers et al. (2010); (10) Karim et al. (in prep.); (11) Younger et al. (2009); (12) Riechers et al. (in prep.); (13) Sheth et al., in prep.; (14) Capak et al. (2009); Schinnerer et al. (2009); (15) Smolčić et al., 2012; (16) Aravena et al. (2010); (17) this work.

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