Mapping the radial structure of AGN tori | Astronomy & Astrophysics (A&A)

Home

All issues

Volume 536 (December 2011)

A&A, 536 (2011) A78

Full HTML

Free Access

Table 1

Properties of our targets and their point-source flux from our UKIRT images or 2MASS images.

Name	z^a	Scale^b	E_B − V^c	Date	Flux (mJy)^d					A_V	R_{τ_K} fit^e (≡ R_in)		νL_ν(5500 Å)^f

	corr.	(pc/mas)	(mag)	(UT)	Z	Y	J	H	K	(mag)	(pc)	(mas)	(erg s^-1)^b

NGC 4151	0.00414	0.0855	0.028	2009-06-17	39.7	42.4	59.4	96.3	173.		0.033	0.383	(8.3 ± 1.3) × 10⁴²
NGC 3783^g	0.0108	0.221	0.119	1999-04-11	–	–	19.1	33.5	62.5		0.061	0.274	(2.8 ± 0.4) × 10⁴³
ESO323-G77^g	0.0159	0.324	0.101	1999-05-03	–	–	28.6	63.4	107.	1.2 ± 0.4	0.10	0.321	(8.4 ± 1.9) × 10⁴³
H0557-385	0.0342	0.681	0.043	2009-12-13	4.03	4.43	7.21	15.3	36.8	1.5 ± 0.5	0.12	0.181	(1.2 ± 0.3) × 10⁴⁴
IRAS09149^g, ^h	0.0579	1.12	0.182	2000-01-05	–	–	35.3	59.1	116.		0.47	0.419	(1.7 ± 0.2) × 10⁴⁵
IRAS13349ⁱ	0.108	1.98	0.012	2009-06-17	7.75	8.71	12.6	26.3	62.3	0.93 ± 0.31	0.49	0.248	(1.9 ± 0.4) × 10⁴⁵

Notes.

^(a)

CMB corrected value from NED.

^(b)

H₀ = 70 km s^-1 Mpc^-1, Ω_m = 0.3, and Ω_Λ = 0.7.

^(c)

Galactic reddening from Schlegel et al. (1998).

^(d)

Flux measurement uncertainty is ~5% (see Sect. 3 in Kishimoto et al. 2009a).

^(e)

The K-band reverberation radius R_{τ_K} from UV luminosity using the fit by Suganuma et al. (2006), which is defined as R_in in this paper (see Eq. (1)).

^(f)

Optical luminosity at rest wavelength 5500 Å.

^(g)

From 2MASS images.

^(h)

IRAS09149-6206.

⁽ⁱ⁾

IRAS13349+2438.

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.