**Table 1:** Results of radio observations with the VLA.
HSC	$\alpha_{\rm J2000.0}$ , $\delta_{\rm J2000.0}$	Flux density
		(mJy)
North	$20^{\rm h}32^{\rm m}$ 26 $.\!\!^{\rm s}$ $874\pm0$ $.\!\!^{\rm s}$ 001	$S_{\rm 6~cm} = 2.01\pm 0.03$
	$+41^{\circ}04^{\prime}$ 33 ${\rlap.}^{\prime \prime}$ $02\pm 0$ ${\rlap.}^{\prime \prime}$ 01	$S_{\rm 3.5~cm} = 1.33 \pm 0.03$

South^*	$20^{\rm h}32^{\rm m}$ 24 $.\!\!^{\rm s}$ $97\pm0$ $.\!\!^{\rm s}$ 02	$S_{\rm 6~cm} \leq 0.16^{**}$
	$+40^{\circ} 53^{\prime}$ 05 ${\rlap.}^{\prime \prime}$ $9\pm0$ ${\rlap.}^{\prime \prime}$ 2	$S_{\rm 3.5~cm} \leq 0.11^{**}$

^* Position taken from Martí et al. (2005).
^** Upper limits are given as $4 \sigma$ from VLA data of this paper.