Table 1: Details of the WSRT and VLA radio sources associated with SMM J16359+6612 (SMM-A, B, C) and SMM J16359+66118(arclet #289).
Name RA ( $\rm + 16^{h} 35^{m}$ ) Dec ( $+ 66^{\circ}$ ) $S_{\rm T}$ $S_{\rm Pk}$ Maj axis Min axis PA

J2000 (s) J2000 ( $^\prime$ , $^{\prime\prime}$ ) $\mu$ Jy $\mu$ Jy '' '' deg

WSRT J163550+661205 (SMM-C) $51.1\pm0.1$ 12, $08.0\pm1.0$ $110\pm17$ $110\pm17$ - - -

WSRT J163553+661226 (SMM-B) $53.9\pm0.1$ 12, $26.4\pm0.6$ $391\pm43$ $217\pm16$ $15\pm2$ $9\pm2$ $165\pm12$

WSRT J163555+661237 (SMM-A) $55.6\pm0.2$ 12, $37.7\pm1.0$ $99\pm17$ $99\pm17$ - - -

VLA J163550+661206 (SMM-C) $50.5\pm0.2$ 12, $06.8\pm0.1$ $24\pm10$ $24\pm6$ - - -

VLA J163554+661223 (SMM-B) $54.5\pm0.1$ 12, $25.3\pm1.1$ $124\pm18$ $51\pm6$ $16\pm3$ $10\pm3$ $39\pm12$

VLA J163555+661236 (SMM-A) $55.7\pm0.1$ 12, $37.1\pm0.5$ $28\pm6$ $28\pm6$ - - -

WSRT J163555+661152 (#289) $55.2\pm0.1$ 11, $52.9\pm0.6$ $170\pm29$ $175\pm17$ $6\pm4$ - $43\pm20$

VLA J163555+661150 (#289) $55.1\pm0.2$ 11, $50.1\pm0.6$ $35\pm10$ $37\pm6$ $8\pm3$ - $65\pm10$

**Table 1:** Details of the WSRT and VLA radio sources associated with SMM J16359+6612 (SMM-A, B, C) and SMM J16359+66118(arclet #289).
Name	RA ( $\rm + 16^{h} 35^{m}$ )	Dec ( $+ 66^{\circ}$ )	$S_{\rm T}$	$S_{\rm Pk}$	Maj axis	Min axis	PA
	J2000 (s)	J2000 ( $^\prime$ , $^{\prime\prime}$ )	$\mu$ Jy	$\mu$ Jy	''	''	deg
WSRT J163550+661205 (SMM-C)	$51.1\pm0.1$	12, $08.0\pm1.0$	$110\pm17$	$110\pm17$	-	-	-
WSRT J163553+661226 (SMM-B)	$53.9\pm0.1$	12, $26.4\pm0.6$	$391\pm43$	$217\pm16$	$15\pm2$	$9\pm2$	$165\pm12$
WSRT J163555+661237 (SMM-A)	$55.6\pm0.2$	12, $37.7\pm1.0$	$99\pm17$	$99\pm17$	-	-	-
VLA J163550+661206 (SMM-C)	$50.5\pm0.2$	12, $06.8\pm0.1$	$24\pm10$	$24\pm6$	-	-	-
VLA J163554+661223 (SMM-B)	$54.5\pm0.1$	12, $25.3\pm1.1$	$124\pm18$	$51\pm6$	$16\pm3$	$10\pm3$	$39\pm12$
VLA J163555+661236 (SMM-A)	$55.7\pm0.1$	12, $37.1\pm0.5$	$28\pm6$	$28\pm6$	-	-	-
WSRT J163555+661152 (#289)	$55.2\pm0.1$	11, $52.9\pm0.6$	$170\pm29$	$175\pm17$	$6\pm4$	-	$43\pm20$
VLA J163555+661150 (#289)	$55.1\pm0.2$	11, $50.1\pm0.6$	$35\pm10$	$37\pm6$	$8\pm3$	-	$65\pm10$

Source LaTeX | All tables | In the text

	1 Introduction
	2 Radio observations
	3 Results and discussion
	4 Conclusions
	References