Table 5: Results of the weak-shear analysis and of the mass reconstruction. Column 1: quasar name. Column 2: number of galaxies per arcmin² corresponding to the galaxy overdensity. Column 3: position of the galaxy overdensity center relative to the quasar images. Column 4: photometric redshift of the galaxy overdensity and corresponding error bar ("^*'': value inferred from previous paper, see text for references). Column 5: magnitude range for the background galaxies used for the weak-shear analysis. Column 6: number of galaxies used for the weak-shear analysis and the mass reconstruction. Column 7: ICF width of the mass reconstruction in arcsecond. Column 8: upper limit of the mass integrated from the mass reconstruction in a radius of 500 kpc and centered at the galaxy group position. Column 9: galaxy cluster velocity dispersion corresponding to the mass given in Col. 8. Column 10: shear orientation in degree.
Quasar No. gal. Relative $z_{\rm phot}$ Sources No. gal ICF Mass $\sigma_v$ PA $_\gamma$

/( $^\prime$ )² position $\pm$ $\Delta z$ mag. range for WS ('') (10¹⁴ $M_\odot$ h^-1) (km s^-1 h^-1)

CTQ 414
28 12 $^{\prime \prime }$ SE $0.5\pm0.1$ $25<R \leq 28$ 578 180 <1.6 <720 24 $^\circ$

HE 0230-2130 21.1 38 $^{\prime \prime }$ W 1.0 $^\star$ $25<R \leq 28$ 633 120 4.0 1130 45 $^\circ$

LBQS 1009-0252 _ _ 1 $^\star$ $25<R \leq 28$ 351 100 <2.4 <880 -33 $^\circ$

B 1030+074 10 120 $^{\prime \prime }$ SE 0.6 $^\star$ $23< R \leq28$ 416 120 <2.3 <860 33 $^\circ$

HE 1104-1805 9 40 $^{\prime \prime }$ N $2.0\pm0.1$ $24< R \leq28$ _ _ _ _ 90 $^\circ$

18 78 $^{\prime \prime }$ SW _ _ _ _ _ _ _

B 1359+154 4 7 $^{\prime \prime }$ NE $1.3\pm0.2$ $23< R \leq28$ 749 300 <10.7 <1800 -12 $^\circ$

H 1413+117 43 14 $^{\prime \prime }$ SE $0.8\pm0.3$ $25<R \leq 28$ 453 100 <1.8 760 45 $^\circ$

32 36 $^{\prime \prime }$ SW $1.7\pm0.2$ _ _ _ _ _ _

HE 2149-2745 22 7 $^{\prime \prime }$ SE $0.7\pm0.1$ $25<R \leq 28$ 81 60 3.2 1010 45 $^\circ$

**Table 5:** Results of the weak-shear analysis and of the mass reconstruction. Column 1: quasar name. Column 2: number of galaxies per arcmin² corresponding to the galaxy overdensity. Column 3: position of the galaxy overdensity center relative to the quasar images. Column 4: photometric redshift of the galaxy overdensity and corresponding error bar ("^*'': value inferred from previous paper, see text for references). Column 5: magnitude range for the background galaxies used for the weak-shear analysis. Column 6: number of galaxies used for the weak-shear analysis and the mass reconstruction. Column 7: ICF width of the mass reconstruction in arcsecond. Column 8: upper limit of the mass integrated from the mass reconstruction in a radius of 500 kpc and centered at the galaxy group position. Column 9: galaxy cluster velocity dispersion corresponding to the mass given in Col. 8. Column 10: shear orientation in degree.
Quasar	No. gal.	Relative	$z_{\rm phot}$	Sources	No. gal	ICF	Mass	$\sigma_v$	PA $_\gamma$
	/( $^\prime$ )²	position	$\pm$ $\Delta z$	mag. range	for WS	('')	(10¹⁴ $M_\odot$ h^-1)	(km s^-1 h^-1)
CTQ 414	28	12 $^{\prime \prime }$ SE	$0.5\pm0.1$	$25<R \leq 28$	578	180	<1.6	<720	24 $^\circ$
HE 0230-2130	21.1	38 $^{\prime \prime }$ W	1.0 $^\star$	$25<R \leq 28$	633	120	4.0	1130	45 $^\circ$
LBQS 1009-0252	_	_	1 $^\star$	$25<R \leq 28$	351	100	<2.4	<880	-33 $^\circ$
B 1030+074	10	120 $^{\prime \prime }$ SE	0.6 $^\star$	$23< R \leq28$	416	120	<2.3	<860	33 $^\circ$
HE 1104-1805	9	40 $^{\prime \prime }$ N	$2.0\pm0.1$	$24< R \leq28$	_	_	_	_	90 $^\circ$
	18	78 $^{\prime \prime }$ SW	_	_	_	_	_	_	_
B 1359+154	4	7 $^{\prime \prime }$ NE	$1.3\pm0.2$	$23< R \leq28$	749	300	<10.7	<1800	-12 $^\circ$
H 1413+117	43	14 $^{\prime \prime }$ SE	$0.8\pm0.3$	$25<R \leq 28$	453	100	<1.8	760	45 $^\circ$
	32	36 $^{\prime \prime }$ SW	$1.7\pm0.2$	_	_	_	_	_	_
HE 2149-2745	22	7 $^{\prime \prime }$ SE	$0.7\pm0.1$	$25<R \leq 28$	81	60	3.2	1010	45 $^\circ$

Source LaTeX | All tables | In the text