Young stellar object candidates toward the Orion region selected from GALEX

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Table 2

Physical properties derived from the best SED fits for 65 sources.

ID(2MASS)	l	b	T _eff ^a	L _bol	ΔL_bol	A _V	Type	Ref.
	(deg)	(deg)	(K)	(L_⊙)	(L_⊙)	(mag)

J05071385-1020045	210.512	–27.796	4700	0.035	0.003	1.0
J05141589-0138583	202.856	–22.279	4400	2.355	0.275	0.0
J05160402+0618525	195.751	–17.904	3600	1.343	0.155	1.25	TTS	Tak10
J05170743-1143036	213.069	–26.18	4200	0.029	0.003	0.0
J05173566-1140050	213.073	–26.054	3800	0.024	0.003	0.0

Notes. This table is published in its entirety at the CDS. A portion is shown here for guidance regarding its form and content.

^(a)

Uncertainty in T_eff is ±50 K.

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