**Table 3:** Measured radio flux densities or peak brightnesses of J1101+7225, obtained with single-dish telescopes, local interferometers, and VLBI. The VLBI flux densities are our fitted core flux densities as presented in Tables 5 and 7.
Obs. type	Freq. [GHz]	Flux dens. [mJy]
single-dish	0.038	$(1.41\times 10^4\pm 800)$	(a)
single-dish	0.178	$(3900\pm 600)$	(b)
single-dish	1.4	$(1451\pm 30)$	(c)
single-dish	2.7	$(1070\pm 35)$	(d)
single-dish	5	$(858\pm 76)$	(e)
single-dish	22	$(820\pm 100)$	(f)
local interf.	1.4	$(748\pm 40)$ /beam	(g), res $\sim$ 1.5''
local interf.	8.4	$(349 \pm 20)$ /beam	(h), res $\sim$ 0.2''
VLBI	1.66	( $396\pm 20$ )	EVN Feb. 2002
VLBI	2.3	$(520\pm25)$ /beam	B02, res $\sim$ 3 mas
VLBI	5	( $139\pm7)$	- 1991.4 -
VLBI	5	$(282\pm14)$	- 1993.4 -
VLBI	5	$(337\pm17)$	- 1996.6 -
VLBI	5	$(439\pm22)$	- 1999.9 -
VLBI	8.4	$(383\pm20)$ /beam	B02, res $\sim$ 1 mas

References and comments: (a) Rees (1990), catalogue revised by Hales et al. (1995); (b) Gower et al. (1967); (c) White & Becker (1992); (d) Kühr et al. (1981); (e) Gregory et al. (1996); (f) Teräsranta et al. (2001); (g) Xu et al.(1995) gave this peak brightness of a map, which was convolved to a circular beam of 1.5'' FWHM; (h) Patnaik et al. (1992) found this peak brightness to be 80% of the total flux density of 436 mJy.
The values are plotted over frequency in Fig. 1. For the interferometric observations 5% flux density errors are given.

Source LaTeX | All tables | In the text

	1 Introduction
	2 Observations
	3 Radio properties of the quasar J1101+7225
	4 Discussion of the results
	References