Molecular gas excitation and outflow properties of obscured quasars at z ∼ 0.1

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Table 1.

Main properties of the quasars.

SDSS ID	z	D_L	Scale	log $L_{[OIII]}^{corr}$ $L_{\mathrm{[OIII]}}^{\mathrm{corr}}$	log L_bol	log L_1.4 GHz	log M_*	SFR	Galaxy
	SDSS	(Mpc)	(kpc/″)	(L_⊙)	(erg/s)	(W/Hz)	(M_⊙)	(M_⊙ yr⁻¹)	Morphology
J101043.36+061201.4	0.0977	449	1.807	9.30	45.54	24.37	10.99	30	Interacting ETG
J110012.39+084616.3	0.1004	462	1.851	9.60	45.84	24.18	11.02	34	Barred spiral
J134733.36+121724.3	0.1217^*	568	2.189	9.28	45.52	26.30	11.70	59^†	Merging ETG
J135646.10+102609.0	0.1232	576	2.213	9.29	45.53	24.36	11.27	69	Merging ETG
J143029.88+133912.0	0.0851	388	1.597	9.58	45.82	23.67	11.15	12	Post-merger ETG
J150904.22+043441.8	0.1115	517	2.028	9.79	46.03	23.81	10.94	34	Barred spiral

Notes. The values of L_bol were derived from the extinction-corrected [OIII] luminosities from Kong & Ho (2018), listed in Col. 5, multiplied by the factor of 474 from Lamastra et al. (2009). The rest-frame radio luminosities were calculated from integrated FIRST fluxes (Becker et al. 1995), assuming a spectral index α = −0.7, and the stellar masses and SFRs were taken from RA22. ^*The redshift measured from the CO(2–1) was computed by Lamperti et al. (2022). ^†SFR from Bessiere et al. (2024).

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