VLT-SINFONI integral field spectroscopy of low-z luminous and ultraluminous infrared galaxies - I. Atlas of the 2D gas structure

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Volume 546 (October 2012)

A&A, 546 (2012) A64

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Table 1

The SINFONI sample.

ID1	ID2	α	δ	z	D	Scale	log L_IR	Classification	References
Common	IRAS	(J2000)	(J2000)		(Mpc)	(pc/arcsec)	(L_⊙)
(1)	(2)	(3)	(4)	(5)	(6)	(7)	(8)	(9)	(10)

IRAS 06206-6315	IRAS 06206-6315	06^h21^m01.21^s	–63°17′235	0.092441	425	1726	12.31	Sy2	1, 2, 3
NGC 2369	IRAS 07160-6215	07^h16^m37.73^s	–62°20′374	0.010807	48.6	230	11.17	Composite	4
NGC 3110	IRAS 10015-0614	10^h04^m02.11^s	–06°28′292	0.016858	78.4	367	11.34	Composite	4
NGC 3256	IRAS 10257-4338	10^h27^m51.27^s	–43°54′138	0.009354	44.6	212	11.74	HII, Starburst	1, 5
ESO 320-G030	IRAS 11506-3851	11^h53^m11.72^s	–39°07′489	0.010781	51.1	242	11.35	HII	4
IRAS 12112+0305	IRAS 12112+0305	12^h13^m46.00^s	+02°48′380	0.073317	337	1416	12.38	LINER	1, 2
IRASF 12115-4656	IRAS 12115-4657	12^h14^m12.84^s	–47°13′432	0.018489	84.4	394	11.10	HII	1
NGC 5135	IRAS 13229-2934	13^h25^m44.06^s	–29°50′012	0.013693	63.5	299	11.33	HII, Sy2	1, 6
IRAS 14348-1447	IRAS 14348-1447	14^h37^m38.40^s	–15°00′200	0.083000	382	1575	12.41	LINER	1, 2
IRASF 17138-1017	IRAS 17138-1017	17^h16^m35.79^s	–10°20′394	0.017335	75.3	353	11.42	HII	1
IRAS 17208-0014	IRAS 17208-0014	17^h23^m21.95^s	–00°17′009	0.042810	189	844	12.43	LINER	1, 6
IC 4687	IRAS 18093-5744	18^h13^m39.63^s	–57°43′313	0.017345	75.1	352	11.44	HII	1, 6
IRAS 21130-4446	IRAS 21130-4446	21^h16^m18.52^s	–44°33′380	0.092554	421	1712	12.22	HII	7
NGC 7130	IRAS 21453-3511	21^h48^m19.50^s	–34°57′047	0.016151	66.3	312	11.34	HII, Sy2, LINER	1, 6
IC 5179	IRAS 22132-3705	22^h16^m09.10^s	–36°50′374	0.011415	45.6	216	11.12	HII	4
IRAS 22491-1808	IRAS 22491-1808	22^h51^m49.26^s	–17°52′235	0.077760	347	1453	12.23	HII	1, 2
IRAS 23128-5919	IRAS 23128-5919	23^h15^m46.78^s	–59°03′156	0.044601	195	869	12.04	Sy2, LINER	1, 3, 6

Notes. Columns (3) and (4): right ascension and declination from the NASA Extragalactic Database (NED). Column (5): redshift from NED. Columns (6) and (7): luminosity distance and scale from Ned Wright’s Cosmology Calculator (Wright 2006) given h₀ = 0.70, Ω_M = 0.7, Ω_M = 0.3. Column (8): L_IR(8–1000 μm) calculated from the IRAS flux densities f₁₂, f₂₅, f₆₀ and f₁₀₀ (Sanders et al. 2003), using the expression in Sanders & Mirabel (1996). Column (9): spectroscopic classification based on the nuclear optical spectra from the literature. Galaxies classified as composite are likely to be a combination of AGN activity and star formation.

References. 1: Sanders et al. (2003), 2: Lutz et al. (1999), 3: Duc et al. (1997), 4: Pereira-Santaella et al. (2011), 5: Wamsteker et al. (1985), 6: Véron-Cetty & Véron (2006), 7: Farrah et al. (2003).

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