Integral field optical spectroscopy of a representative sample of ULIRGs - I. The data

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Volume 505 / No 3 (October III 2009)

A&A, 505 3 (2009) 1319-1343

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Table 3:

Integral field spectroscopy observations log. The galaxies are sorted by decreasing nuclear distance.
IRAS Name	INTEGRAL	INTEGRAL	Date	Exp. time	Comment on IFU data
	(Bundle)	(FoV arcsec²)	month/year	(s)
IRAS 13156+0435	SB2, SB3	32.9 $\times$ 25.3, 69.1 $\times$ 60.5	03/02	17 400^a	[O III] non detected in N comp.
IRAS 13342+3932	SB3	101.7 $\times$ 89.0	03/02	6 $\times$ 1500
IRAS 18580+6527	SB2	47.8 $\times$ 36.7	04/01	7 $\times$ 1500
IRAS 16007+3743^b	SB2	49.6 $\times$ 38.1	04/01	6 $\times$ 1500
IRAS 06268+3509	SB2	46.3 $\times$ 35.6	03/02	6 $\times$ 1500
IRAS 08572+3915^b	SB2	18.0 $\times$ 13.9	04/99	9 $\times$ 1800
IRAS 14348-1447^a	SB2	1.3 $\times$ 1.0	04/98	4 $\times$ 1800
Arp 299^c	SB2, SB3	3.3 $\times$ 2.5, 6.9 $\times$ 6.0	01/04	12 600^d
IRAS 13469+5833	SB1	21.3 $\times$ 17.4	03/02	5 $\times$ 1800	Sky line to H $\alpha$ +[N II] complex
					Not enough S/N
IRAS 12112+0305^a ^e	SB2	27.9 $\times$ 19.5	04/98	5 $\times$ 1800, 4 $\times$ 1500
Mrk 463	SB2	15.7 $\times$ 12.1	04/01	5 $\times$ 900
IRAS 06487+2208	SB1	19.7 $\times$ 16.1	03/02	5 $\times$ 1500
IRAS 11087+5351	SB1	19.5 $\times$ 16.0	03/02	6 $\times$ 1500
Mrk 273^a	SB2	12.0 $\times$ 9.2	04/98	3 $\times$ 1500
Arp 220^a	SB2, SB3	5.9 $\times$ 4.5, 12.4 $\times$ 10.8	05/00	48 000^f	[O III] not detected, H $\beta$ not covered
IRAS 17208-0014^a	SB2	13.5 $\times$ 10.4	04/99	4 $\times$ 1950
IRAS 15250+3609^a	SB2	17.1 $\times$ 13.2	04/98	5 $\times$ 1800
IRAS 12490-1009	SB2	29.7 $\times$ 22.8	03/02	4 $\times$ 1500
IRAS 14060+2919	SB2	1.9 $\times$ 1.4	03/02	4 $\times$ 1800
IRAS 09427+1929	SB3	87.4 $\times$ 76.4	03/02	2320^g	Short inhomogeneous exposures
IRAS 15206+3342^a	SB2	35.7 $\times$ 27.4	04/99	4 $\times$ 1800
Mrk 231	SB1	6.5 $\times$ 5.3	03/02	4 $\times$ 900	H $\beta$ not covered
					Broad emission lines

^a 3 $\times$ 1500 s for the South component with the SB2 bundle; 3 $\times$ 1800 for the North component with the SB2 bundle, 5 $\times$ 1500 s for the entire system with the SB3 bundle.
^b Previously published galaxy. See Colina et al. (2005), Monreal-Ibero et al. (2007) and references therein.
^c García-Marín et al. (2006).
^d 3 $\times$ 1200 s for each individual galaxy of the system, NGC 3690 and IC 694 observed with the SB2 bundle. 3 $\times$ 1800 s for the entire system as observed with the SB3 bundle.
^e For IRAS 12112+0305 we present the results obtained by combining two different pointings of the SB2 INTEGRAL bundle.
^f 6 $\times$ 1500 s for the nuclear region observed with the SB2 bundle, 26 $\times$ 1500 s for the nucleus and the extended nebula as observed with the SB3 bundle.
^g 1500 s, 520 s, 300 s.

Source LaTeX | All tables | In the text

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