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Table 1

Summary of the results of our KI observations and radio data for the present and remaining previous targets.

Name Date (UT) za Scaleb EB − Vc Bpd PA V2 Rringe Radio fluxf AV


corr. (pc mas-1) (mag) (m) (°) (mas) (pc) (mJy) (GHz) (mag)

AKN120 2009-11-07 0.0327 0.653 0.128 74.6 31.9 0.843  ±  0.097 0.56  ±  0.19 0.36  ±  0.12 9.3g 1.4
IC4329A 2010-05-01 0.0170 0.345 0.059 69.8 49.6 0.868  ±  0.084 0.54  ±  0.18 0.19  ±  0.06 10.7h 8.4 2  ±  1n
MRK6 2010-05-01 0.0188 0.382 0.136 71.5  −1.4 0.909  ±  0.048 0.44  ±  0.12 0.17  ±  0.05 39.5i 8.4
3C273 2010-05-02 0.159 2.75 0.021 83.5 39.9 0.958  ±  0.034 0.25  ±  0.10 0.69  ±  0.28 3.20E4j 4.8
NGC 4151 2010-05-01 0.00414 0.0855 0.028 72.4 51.0 0.920  ±  0.017 0.40  ±  0.05 0.034  ±  0.004 125.k 4.9
2010-05-01 81.3 40.7 0.878  ±  0.049 0.45  ±  0.10 0.038  ±  0.008
2010-05-02 84.9 21.7 0.883  ±  0.048 0.42  ±  0.09 0.036  ±  0.008

NGC 4051 0.00309 0.0639 6.0k 4.9
MRK231 0.0427 0.841 173.l 5.0
IRAS 13349o 0.109 1.98 19.9m 1.4

Notes. 

(a)

CMB corrected value from NED.

(b)

H0 = 70 km s-1 Mpc-1, Ωm = 0.3, and ΩΛ = 0.7.

(c)

Galactic reddening from Schlegel et al. (1998).

(d)

Projected baseline lengths.

(e)

Thin-ring radius.

(f)

Radio flux observed at frequency given. For radio-quiet objects, flux from linear (double or triple) structure at  ~ 100 pc scale is given, except for AKN120, IC4329A, and IRAS 13349+2438, for which flux from a source unresolved at resolution of 6″ (3.9 kpc), 1″ (350 pc), and 5.4″ (11 kpc), respectively, is given.

(o)

IRAS 13349+2438.

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