Optical multiband surface photometry of a sample of Seyfert galaxies - I. Large-scale morphology and local environment analysis of matched Seyfert and inactive galaxy samples

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Volume 526 (February 2011)

A&A, 526 (2011) A43

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Table 4

Close companions of the Sy galaxy sample.

Galaxy	Companion	ΔD		\|ΔV_r\|	Ref.

		[arcmin]	[kpc]	[km s^-1]
(1)	(2)	(3)	(4)	(5)	(6)	(7)

III Zw 2	III Zw 2B	0.572	54.38	199 ± 106	10	10
Mrk 348	2MASX J00485285+3157309	1.218	20.05	321 ± 51	12	19
I Zw 1	J005334+124133^a	0.260	17.38	170 ± 110^b	5
Mrk 573	APMUKS(BJ) B014126.68+020933.5	3.734	70.95	≈100^b	16
Mrk 590	SDSS J021429.36–004604.7	1.053	31.17	234 ± 39	8	1
NGC 3227	NGC 3226	2.177	12.78	181 ± 38	14	14
	2MASX J10232246+1954510	3.515	20.63	42 ± 37	8	4
	2MASX J10232162+2001380	9.961	58.47	9 ± 38	8	4
	SDSS J102434.71+200157.8	18.122	106.38	128 ± 42	8	4
	SDSS J102315.38+201040.5	19.109	112.17	41 ± 40	8	4
NGC 4151	SDSS J121021.06+391252.1	11.688	57.62	75 ± 35	8	3
	SDSS J120959.87+391147.7	14.053	69.28	343 ± 43	8	3
NGC 4593	MCG –01–32–033	3.809	45.67	149 ± 67	21	13
Mrk 279	MCG +12–13–024	0.761	26.88	159 ± 25	20	7
NGC 5548	SDSS J141824.74+250650.7	5.867	122.74	206 ± 22	8	4
	2MASX J14173385+2506515	5.959	124.66	40 ± 59	8	4
Ark 479	SDSS J153550.82+143035.3	0.622	14.60	48 ± 50	9	2
Mrk 506	CGCG 170–019	0.763	37.20	561 ± 58	8	9
	SDSS J172229.44+305231.6	2.277	111.00	505 ± 58	8	2
3C 390.3	PGC 062330	1.802	112.68	549 ± 57	11	18
NGC 7469	IC 5283	1.315	23.29	87 ± 37	15	14
Mrk 315	[CAM2005] DWARF	1.024	44.10	193 ± 35	6	6
NGC 7603^c	NGC 7603:[LG2002] 3	0.620	20.27	87 476 ± 388	8	17
	SDSS J231859.26+001405.4	0.860	28.12	56 018 ± 461	8	17
	NGC 7603B	0.985	32.21	7535 ± 47	8	1

Notes. (3) and (4) Projected linear separation taken from NED; (5) Absolute radial velocity difference calculated using redshift sources specified in Cols. 6 and 7; (6) and (7) References regarding the redshift sources of the primary and the companion, respectively, generally taken through NED.

^(a)

We list the J2000 coordinates taken from Aladin for the name of the anonymous companion.

^(b)

The absolute radial velocity difference itself was taken from the source given in Col. 6.

^(c)

Anomalous redshift galaxy system, not taken into account in the companion statistics.

References. (1) Abazajian et al. (2003); (2) Abazajian et al. (2009); (3) Adelman-McCarthy et al. (2007); (4) Adelman-McCarthy et al. (2008); (5) Canalizo & Stockton (2001); (6) Ciroi et al. (2005); (7) de Grijp et al. (1987); (8) de Vaucouleurs et al. (1991); (9) Falco et. al (1999); (10) Heckman et al. (1984); (11) Hewitt & Burbidge (1991); (12) Huchra et. al (1999); (13) Jones et al. (2009); (14) Keel (1996a); (15) Keel (1996b); (16) Kuo et al. (2008); (17) López-Corredoira & Gutiérrez (2004); (18) Penston & Penston (1973); (19) Petrosian (1982); (20) Strauss & Huchra (1988); (21) Strauss et al. (1992).

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