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Table 2

Stellar properties of the sample.

Name d [pc] SpT Teff L M t [Myr]
Kiso A-0904 06 A(1) K6
Kiso A-0904 06 B(1) K6
Brun 216(2) F8
Brun 252(3) G1
Haro 5-38 K7
HD 294260 G1
HD 294268 G0
PDS 110 F6
PDS 113(4) F3+F4
RV Ori K5
RY Ori F5
TX Ori K4
V 351 Ori A9
V 499 Ori K6
V 543 Ori(1) K4
V 578 Ori K7
V 599 Ori(2) A5
V 606 Ori K5
V 1012 Ori(2) A3
V 1044 Ori G6
V 1650 Ori(3) F8
V 1787 Ori A5
V 1788 Ori A0
V2149 Ori A(3) F8
V2149 Ori B(3) F8

Notes. (1)Teff is taken from Briceño et al. (2019). (2)All values from Vioque et al. (2018). (3)Values from Valegård et al. (2021). (4)Spectroscopic binary (SB2) from Klochkova & Chentsov (2008); we detect both components in the X-shooter spectra. Stellar parameters are given for one component, assuming the stars have roughly equal luminosity. The method used to obtain the stellar parameters is described in Sect. 3, unless differently indicated in the footnotes. The columns are: source name, distance, effective temperature, stellar luminosity, mass, and age.

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