  We recently discovered an extragalactic transient, AT2020caa, using the
community alert broker ANTARES. This transient apparently exhibited two
outbursts in a time span of a year (between 2020 and 2021). Based on a
decade-long historical light curve of the candidate host galaxy, we rule out an
activity from the galaxy nucleus to explain these outbursts. The measured peak
magnitudes (assuming the known spectroscopic redshift of the candidate host
galaxy) put AT2020caa in the realm of thermonuclear supernovae (SNe) or
luminous core-collapse SNe. A handful of the latter are known to show prior
outbursts (POs), thought to be linked to mass loss in massive stars. Using
Gemini/GMOS, we obtained a spectrum of the current outburst that shows it to be
a Type Ia supernova (SNIa). We examine the nature of AT2020caa's PO and
conclude that it is likely a separate SN within the same galaxy.
