Infrared signature of active massive black holes in nearby dwarf galaxies

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Volume 602 (June 2017)

A&A, 602 (2017) A28

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Table 4

16 known AGN with IR signatures of active massive black holes.

Name	RA	Dec	Classification	log(M_BHIR)	log(M_BH)	Reference
	J2000	J2000		M _⊙	M _⊙

NGC 5253	13^h39^m55.80^s	−31d38m24.0s	Sy2	5.602^a	−	Koulouridis (2014)
CIRCINUS	14^h13^m09.30^s	−65d20m21.0s	Sy2	6.306^a	6.23	McConnell et al. (2013)
NGC 2964	09^h42^m54.23^s	+31d50m50.6s	−	6.497^a	7.34;6.11	Beifiori et al. (2012)
ESO 060- G 019	08^h57^m26.72^s	−69d03m36.3s	−	6.015^a	7.83	Davis et al. (2014)
IC 1953	03^h33^m41.87^s	−21d28m43.1s	−	5.990^a	7.33	Davis et al. (2014)
NGC 4194	12^h14^m09.47^s	+54d31m36.6s	AGN	7.235^a	−	SIMBAD info page
NGC 3690 NED01	11^h28^m31.02^s	+58d33m40.7s	Sy2	7.877^a	7.52	Alonso-Herrero et al. (2014)
NGC 3690 NED02	11^h28^m33.63^s	+58d33m46.6s	LINER	7.864^a	7.48;8.85	Alonso-Herrero et al. (2014);
						Zhao et al. (1997)
IRAS 11485-2018	11^h51^m11.60^s	−20d36m02.0s	AGN	5.591	−	Sargsyan et al. (2011)
NGC 1275	03^h19^m48.16^s	+41d30m42.1s	LINER;Sy1	7.752^a	9.28;8.51	McKernan et al. (2010);
						Panessa et al. (2006)
POX052	12^h02^m56.91^s	−20d56m02.7s	Sy1	5.597	5.2	Barth et al. (2004)
MRK 0315	23^h04^m02.62^s	+22d37m27.5s	Sy1	7.259	−	Veron-Cetty & Vernon (2010)
UGC 04211	08^h04^m46.38^s	+10d46m36.2s	Sy2	7.156	−	Veron-Cetty & Vernon (2010)
SBS 1415+437	14^h17^m01.41^s	+43d30m05.5s	QUASAR	5.934	−	Bukhmastova (2001)
ESO 253- G 003	05^h25^m18.08^s	−46d00m21.0s	Sy2	8.090^a	−	Veron-Cetty & Vernon (2010)
FCSS J033846.0-352252	03^h38^m45.97^s	−35d22m52.3s	Sy2	7.281	−	Veron-Cetty & Vernon (2010)

Notes. In Col. (5), M_BHIR denotes the central black hole mass estimates based on IR luminosity (assuming L_bol = 0.1 L_Edd), while in Col. (6), M_BH refers to the central black hole mass estimates based on other conventional (non-infrared) methods.

^(a)

These sources are extended and larger than the largest WISE aperture (24.75 arcsec radius aperture); therefore, the infrared black hole mass estimates for these sources are only lower limits.

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