Infrared spectroscopy of free-floating planet candidates in Upper Scorpius and Ophiuchus

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Table 3.

Adopted spectral types and estimated effective temperatures and masses for the confirmed members.

ID	SpT	T_eff	Mass 3 Myr	Mass 6 Myr	Mass 10 Myr
		(K)	(M_⊙)	(M_⊙)	(M_⊙)
3213	L2	1880	0.007	0.010	0.012
3214	L2–L4	1560–1880	0.005–0.007	0.007–0.010	0.009–0.012
3345	L6	1220	0.003	0.004	0.006
3355	L1–L3	1740–1970	0.006–0.008	0.008–0.011	0.011–0.013
3378	L2–L4	1560–1880	0.005–0.007	0.007–0.010	0.009–0.012
3404	L3–L4	1560–1740	0.005–0.006	0.007–0.008	0.009–0.011
3314	L0	2060	0.009	0.012	0.014
3231	L1	1970	0.008	0.011	0.013
3091	L0	2060	0.009	0.012	0.014
3210	L0	2060	0.009	0.012	0.014
3244	L1	1970	0.008	0.011	0.013
3421	L1	1970	0.008	0.011	0.013
3326	L2	1880	0.007	0.010	0.012
3144	L4	1560	0.005	0.007	0.009
3200	L0	2060	0.009	0.012	0.014
3299	L4	1560	0.005	0.007	0.009

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