Unclustered Radcliffe Wave Sample

Properties of young pre-main sequence stars in the "unclustered" Radcliffe Wave sample from Tu et al. 2022. Original selection of the pre-main sequence is taken from Zari et al. 2018. Data columns are as follows: (1-2) Galactic Longitude and Latitude (deg) (3-4) Right Ascension and Declination (deg) (5) Gaia DR2 Source ID (6-7) Gaia DR2 Parallax and Parallax Uncertainty (8-11) Gaia DR2 Proper motions (in Galactic coordinates) and their uncertainties (mas/year) (12-13) Gaia DR2 Radial Velocity and Radial Velocity Uncertainty (km/s) (14) G-band mean magnitude (mag) (15) Gaia BP-band mean magnitude (mag) (16) Gaia RP-band mean magnitude (mag) (17) Extinction in the Gaia G-band (mag), taken from Zari et al. 2018 (18) Color excess in BP-RP (mag), taken from Zari et al. 2018 (19-21) Heliocentric Galactic Cartesian Positions (pc) (22-30) Galactocentric velocities (km/s) and their uncertainties (31-48) Actions and angles in the (r, phi, z) directions and their upper and lower uncertainties. The direct orbit integration transforms the radial velocities nonlinearly, which is why there are two different uncertainties per value. "_ue" indicates upper error on the measured value and "_le" indicates lower error on the measured value