  In this work, we examine the list of 63 candidates to T Tauri star (TTS) in
the 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. The
objective 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 to
detect PMS stars in wide-fields.
  The astrometric properties of these sources have been retrieved from the Gaia
DR3 catalogue and used to evaluate their membership probability. Several
classification algorithms have been tested to search for the kinematical groups
but the final classification has been made with k-means++ algorithms.
Membership probability has been evaluated by applying Logistic Regression. In
addition, spectroscopic information available in the archive of the Large Sky
Area Multi Object Fiber Spectroscopic Telescope has been used to ascertain
their PMS nature when available.
  About 20% of the candidates share the kinematics of the TAMC members. Among
them, HD 281691 is a G8-type field star located in front of the cloud and HO
Aur is likely a halo star given the very low metallicity provided by Gaia. The
rest are three known PMS stars (HD 30171, V600 Aur and J04590305+3003004), two
previously unknown accreting M-type stars (J04510713+1708468 and
J05240794+2542438) and, five additional sources, which are very likely PMS
stars. Most of these new sources are concentrated at low galactic latitudes
over the Auriga-Perseus region.
