The planetary-mass-limit VLT/SINFONI library - Spectral extraction and atmospheric characterization via forward modeling

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Table A.4

Table A.4 lists the properties of the companion objects in our sample.

Name	Distance host (au)	Spectral type host	[M/H] host	[M/H] companion	C/O companion	comment
2M 0103 AB b	84 ± 1	M6	−	${0.15}_{- 0.05}^{+ 0.2}$ $0.15_{ - 0.05}^{ + 0.2}$	${0.6}_{- 0.05}^{+ 0.0}$ $0.6_{ - 0.05}^{ + 0.0}$	−
AB Pic b	273 ± 1	K2	0.04 ± 0.02	$- {0.08}_{- 0.03}^{+ 0.57}$ $- 0.08_{ - 0.03}^{ + 0.57}$	${0.45}_{- 0.0}^{+ 0.11}$ $0.45_{ - 0.0}^{ + 0.11}$	−
CD-35 2722 b	67 ± 1	M1	−	$- {0.0}_{- 0.1}^{+ 0.01}$ $- 0.0_{ - 0.1}^{ + 0.01}$	${0.5}_{- 0.0}^{+ 0.01}$ $0.5_{ - 0.0}^{ + 0.01}$	−
DH Tau b	330 ± 5	M0.5	−	$- {0.11}_{- 0.02}^{+ 0.04}$ $- 0.11_{ - 0.02}^{ + 0.04}$	${0.4}_{- 0.0}^{+ 0.0}$ $0.4_{ - 0.0}^{ + 0.0}$	S/N< 80
FU Tau b	800 ± 10	M7.25	−	${0.61}_{- 0.9}^{+ 0.13}$ $0.61_{ - 0.9}^{ + 0.13}$	${0.65}_{- 0.35}^{+ 0.01}$ $0.65_{ - 0.35}^{ + 0.01}$	S/N< 80
HIP 78530 b	623 ± 8	B9	–0.5 ± 0.03	−	−	T_eff > 2000K
HR 7329 b	136±10	A0	−	−	−	T_eff > 2000K

Notes: Host star metallicities were taken from Swastik et al. (2021). Additionally, we have included the C/O ratio and metallicity measurements from our work, along with specific annotations where relevant.

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