Table 4: The published single-dish flux densities at 5 GHz to investigate the source variability. (1) observed at 4.9 GHz and corrected to 5 GHz via a spectral index $\alpha ^{\rm 10.7~GHz}_{\rm 2.7~GHz}\protect$ ; (2) at 4.85 GHz; (3) at 4.75 GHz; (a): Kühr et al. (1981); (b): Gregory et al. (1996); (c): Gregory & Condon (1991); (d): Reich et al. (2000).
$S_{\rm 5~GHz}[{\rm mJy}]$ Date of observation Ref. Ann.

778 $\pm$ 4 between Feb. 1977 and Mar. 1978 (a) (1)

788 $\pm$ 31 Nov. 1986 (b) (2)

953 $\pm$ 73 Oct. 1987 (c) (2)

623 $\pm$ 56 1992.5 = Jul. 1992 (d) (3)

**Table 4:** The published single-dish flux densities at 5 GHz to investigate the source variability. (1) observed at 4.9 GHz and corrected to 5 GHz via a spectral index $\alpha ^{\rm 10.7~GHz}_{\rm 2.7~GHz}\protect$ ; (2) at 4.85 GHz; (3) at 4.75 GHz; (a): Kühr et al. (1981); (b): Gregory et al. (1996); (c): Gregory & Condon (1991); (d): Reich et al. (2000).
$S_{\rm 5~GHz}[{\rm mJy}]$	Date of observation	Ref.	Ann.
778 $\pm$ 4	between Feb. 1977 and Mar. 1978	(a)	(1)
788 $\pm$ 31	Nov. 1986	(b)	(2)
953 $\pm$ 73	Oct. 1987	(c)	(2)
623 $\pm$ 56	1992.5 = Jul. 1992	(d)	(3)

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