This work presents four high-amplitude variable YSOs (≃ 3 mag at near-
or mid-IR wavelengths) arising from the SPICY catalog. Three outbursts show a
duration that is longer than 1 year, and are still ongoing. And additional YSO
brightened over the last two epochs of NEOWISE observations and the duration of
the outburst is thus unclear. Analysis of the spectra of the four sources
confirms them as new members of the eruptive variable class. We find two YSOs
that can be firmly classified as bona fide FUors and one object that falls in
the V1647 Ori-like class. Given the uncertainty in the duration of its
outburst, an additional YSO can only be classified as a candidate FUor.
Continued monitoring and follow-up of these particular sources is important to
better understand the accretion process of YSOs.Comment: 10 pages, 10 figures, Accepted for publication at the Journal of the
Korean Astronomical Societ