PENELLOPE: The ESO data legacy program to complement the Hubble UV Legacy Library of Young Stars (ULLYSES) - I. Survey presentation and accretion properties of Orion OB1 and σ-Orionis

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Table A.2.

Stellar and accretion properties from the literature for the targets in the σ Ori cluster.

Target	2MASS	RV ^(a)	RV ^(b)	SpT ^(a)	A_V^(a)	M_⋆^(c)	L_⋆^(c)	Disk type ^(c)	log(Ṁ_acc) ^(c)
SO 518	J05382725–0245096	28.8 ± 0.6	30.3	K6.0 ± 1.0	0.0	0.75	0.44	II	−8.54
SO 583	J05383368–0244141	29.5 ± 0.5	31.5	K4.5 ± 1.5	0.0	1.09	2.57	II	−8.13
SO 1153	J05393982–0231217	...	33.4	K5.5 ± 1.0	0.15	0.88	0.52	I	−8.38

Notes.

^(a)

Hernández et al. (2014),

^(b)

SDSS-SAS,

^(c)

Maucó et al. (2018).

Radial Velocities are reported in km s⁻¹, stellar masses are reported in solar masses, and ages are reported in Myr.

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