**Table 1:** The properties for 12 type II AGNs with HBLRs.
name	z	log ( $L_{\rm [O~III]}$ )	${\it FWHM}_{\rm [O~III]}$	$\sigma_{\ast}$	${\it FWHM}_{\mbox{H$\beta$\ }}$	log ( $M_{\mbox{H$\beta$\ }}/\mbox{$M_{\odot}$\ }$ )	log ( $M_{\sigma_*}/\mbox{$M_{\odot}$\ }$ )	Ref.
		$\mbox{erg s$^{-1}$\ }$	$\mbox{km s$^{-1}$\ }$	$\mbox{km s$^{-1}$\ }$	$\mbox{km s$^{-1}$\ }$
(1)	(2)	(3)	(4)	(5)	(6)	(7)	(8)	(9)
NGC1068	0.004	42.645^a	-	128	3030	7.88	7.35	1,1,2
NGC7212	0.027	42.636^a	-	137	5420	8.37	7.47	1,1,2
NGC7674	0.029	42.495^a	-	144	2830	7.82	7.56	1,1,2
Mrk3	0.014	43.221^a	-	269	6000	9.17	8.65	1,1,2
Mrk348	0.015	41.912^a	-	185	9350	8.17	7.99	1,1,2
Mrk463E	0.050	42.785^a	-	137	2770	7.81	7.88	1,1,2
Mrk477	0.038	43.543^a	-	117	4130	8.84	7.19	1,1,2
Mrk1210	0.013	42.195^a	-	77	3080	7.90	6.46	1,1,2
J0842+3625	0.561	43.601^b	303.76	129.30^c	4900( $H_{\gamma}$ )	8.99	7.37	3,3,4
J1039+6430	0.402	42.901^b	385.75	164.15^c	3070	7.89	7.79	3,3,4
J1543+4935	0.512	42.789^b	709.72	302.01^c	4300	8.19	8.84	3,3,4
J1641+3858	0.596	43.474^b	395.72	168.39^c	3200( $H_{\gamma}$ )	8.62	7.83	3,3,4

Notes. - Col. (1), name; Col. (2), redshift; Col. 3, the [O III] luminosity; Col. (4), FWHM of the narrow [O III] line; Col. (5), stellar velocity dispersion; Col. (6), FWHM of H $\beta$ from HBLRs; Col. (7), SMBH masses derived from the polarimetric broad line; Col. (8), SMBH masses derived from the $\mbox{$M_{\rm BH}$\ }-\sigma_*$ relation. Col. (9), reference for Cols. (3,5,6): (1) Bian & Gu (2007); (2) Tran (1995); (3) this work; (4) Zakamska et al. (2005). ^a: the intrinsic extinction-corrected [O III] luminosity; ^b: the intrinsic extinction-uncorrected [O III] luminosity; ^c: the stellar velocity dispersion is derived from the FWHM of the narrow/core [O III].

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