P. W. LucasL. C. SmithC. Contreras PeñaD. FroebrichJ. E. DrewM. S. N. KumarBorissova, JuraJuraBorissovaD. MinnitiKurtev, RadostinRadostinKurtevM. Monguió2025-12-072025-12-072017-01-0110.1093/mnras/stx20582-s2.0-85041186814https://cris-uv-2.scimago.es/handle/123456789/7696WOS:000413088400044We present a catalogue of 618 high-amplitude infrared variable stars (1 < ΔK < 5mag) detected by the two widely separated epochs of 2.2 μm data in the UKIDSS Galactic plane survey, from searches covering ~1470 deg2. Most were discovered by a search of all fields at 30 < l < 230°. Sources include new dusty Mira variables, three new cataclysmic variable candidates, a blazar and a peculiar source that may be an interacting binary system. However, ~60 per cent are young stellar obbjects (YSOs), based on spatial association with star-forming regions at distances ranging from 300 pc to over 10 kpc. This confirms our initial result in Contreras Peña et al. (Paper I) that YSOs dominate the high-amplitude infrared variable sky in the Galactic disc. It is also supported by recently published VISTA Variables in the Via Lactea (VVV) results at 295 < l < 350°. The spectral energy distributions of the YSOs indicate class I or flat-spectrum systems in most cases, as in the VVV sample. A large number of variable YSOs are associated with the Cygnus X complex and other groups are associated with the North America/Pelican nebula, the Gemini OB1 molecular cloud, the Rosette complex, the Cone nebula, theW51 star-forming region and the S86 and S236 HII regions. Most of the YSO variability is likely due to variable/episodic accretion on time-scales of years, albeit usually less extreme than classical FUors and EXors. Luminosities at the 2010 Wide-field Infrared Survey Explorer epoch range from ~0.1 to 103 L⊙ but only rarely exceed 102.5 L⊙.enacceso abiertoAstronomy And AstrophysicsSpace And Planetary Sciencearticle