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Table 2

Point-source flux from UKIRT imaging data and the KI results corrected for host galaxy and unresolved AD component.

Name Date Flux (mJy)a Magnitude Hostb AD V2 corrected Rring corr. RτK fitd


(UT) Z Y J H K J K (%) fractionc (pc) (pc)

AKN120 2009-12-13 11.7 11.8 16.4 26.6 60.7 12.4 10.1 0.6  ±  0.1 0.17  ±  0.05 0.822  ±  0.117 0.38  ±  0.14 0.15
IC4329A 2010-06-13 15.0 16.0 23.9 41.6 75.5 12.0 9.8 0.9  ±  0.2 0.29  ±  0.09 0.839  ±  0.119 0.21  ±  0.08 0.13
Mrk6e 1999-02-27 16.3 29.1 53.6 12.4 10.2 0.2  ±  0.1 0.21  ±  0.05 0.890  ±  0.061 0.18  ±  0.05 0.097
3C273 2010-06-14 29.0 29.1 33.2 45.7 81.9 11.7 9.7  < 0.1 0.28  ±  0.09 0.942  ±  0.047 0.81  ±  0.34 1.1
NGC 4151 2010-06-14 51.1 54.0 81.8 136. 264. 10.7 8.5 0.2  ±  0.1 0.14  ±  0.05 0.912  ±  0.021f 0.037  ±  0.007g 0.037

Notes. 

(a)

Flux measurement uncertainty is  ~ 5% (see Sect. 3 in Paper I).

(b)

Host galaxy flux fraction at K-band estimated for the KI’s 50 mas FOV in the AO-corrected images.

(c)

AD flux fraction of the point source at K-band.

(d)

RτK from UV luminosity using the fit by Suganuma et al. (2006).

(e)

From 2MASS images.

(f)

Value for the shortest baseline data.

(g)

Best-fit value for 2010-05-01 data.

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