3C 286: a bright, compact, stable, and highly polarized calibrator for millimeter-wavelength observations

I. Agudo; C. Thum; H. Wiesemeyer; S. N. Molina; C. Casadio; J. L. Gómez; D. Emmanoulopoulos

doi:10.1051/0004-6361/201218801

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Volume 541 (May 2012)

A&A, 541 (2012) A111

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Table 7

S, p, and χ measurements of 3C 286 along the millimeter and radio spectrum.

λ	S	p	χ	Ref.
mm	Jy	%	°

1^a	0.30 ± 0.03	14.4 ± 1.8	33.1 ± 5.7	1
3^a	0.91 ± 0.02	13.5 ± 0.3	37.3 ± 0.8	1
7	1.49 ± 0.03^b	11.6 ± 0.8^c	33.1 ± 0.6^c	2, 3
9	1.92 ± 0.03^b	...	...	2
13	2.46 ± 0.05^b	11.7 ± 0.3^c	33.2 ± 0.3^c	2, 3
28	4.45 ± 0.06^b	...	...	2
36	5.11 ± 0.07^b	11.7 ± 0.1^c	33.1 ± 0.1^c	2, 3
60	7.49 ± 0.07^b	11.2 ± 0.2^c	33.1 ± 0.2^c	2, 3
110	10.62 ± 0.07^b	...	...	2
180	13.53 ± 0.11^b	...	...	2
210	14.65 ± 0.05^b	...	...	2

Notes.

^(a)

S, p, and χ correspond to fitted values as presented in this work.

^(b)

Average values of S are those presented by Peng et al. (2000).

^(c)

Average values of measurements made during 2009 by Taylor et al. (2001), see http://www.vla.nrao.edu/astro/calib/polar/2009/.

References. (1) This paper; (2) Peng et al. (2000); (3) Taylor et al. (2001).

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