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In this work, we examine the list of 63 candidates to T Tauri star (TTS) inthe TAMC identified by their ultraviolet (UV) and infrared colours (IR)measured from data obtained by the Galaxy Evolution Explorer all sky survey(GALEX-AIS) and the Two Microns All Sky Survey (2MASS), respectively. Theobjective of this work is twofold: evaluate whether they are pre-main sequence(PMS) stars and evaluate the goodness of the UV-IR colour-colour diagram todetect PMS stars in wide-fields.  The astrometric properties of these sources have been retrieved from the GaiaDR3 catalogue and used to evaluate their membership probability. Severalclassification algorithms have been tested to search for the kinematical groupsbut the final classification has been made with k-means++ algorithms.Membership probability has been evaluated by applying Logistic Regression. Inaddition, spectroscopic information available in the archive of the Large SkyArea Multi Object Fiber Spectroscopic Telescope has been used to ascertaintheir PMS nature when available.  About 20% of the candidates share the kinematics of the TAMC members. Amongthem, HD 281691 is a G8-type field star located in front of the cloud and HOAur is likely a halo star given the very low metallicity provided by Gaia. Therest are three known PMS stars (HD 30171, V600 Aur and J04590305+3003004), twopreviously unknown accreting M-type stars (J04510713+1708468 andJ05240794+2542438) and, five additional sources, which are very likely PMSstars. Most of these new sources are concentrated at low galactic latitudesover the Auriga-Perseus region.

Uncovering a new group of T Tauri stars in the Taurus-Auriga molecular complex from Gaia and GALEX data