The All-Sky Automated Survey for Supernovae (ASAS-SN) provides long baseline
(${\sim}4$ yrs) light curves for sources brighter than V$\lesssim17$ mag across
the whole sky. The Transiting Exoplanet Survey Satellite (TESS) has started to
produce high-quality light curves with a baseline of at least 27 days,
eventually for most of the sky. The combination of ASAS-SN and TESS light
curves probes both long and short term variability in great detail, especially
towards the TESS continuous viewing zones (CVZ) at the ecliptic poles. We have
produced ${\sim}1.3$ million V-band light curves covering a total of
${\sim}1000 \, \rm deg^2$ towards the southern TESS CVZ and have systematically
searched these sources for variability. We have identified ${\sim} 11,700$
variables, including ${\sim} 7,000$ new discoveries. The light curves and
characteristics of the variables are all available through the ASAS-SN variable
stars database (this https URL). We also introduce an online
resource to obtain pre-computed ASAS-SN V-band light curves
(this https URL) starting with the light curves of the
${\sim}1.3$ million sources studied in this work. This effort will be extended
to provide ASAS-SN light curves for ${\sim}50\;$million sources over the entire
sky.

本文介绍了 All-Sky Automated Survey for Supernovae 和 Transiting Exoplanet Survey Satellite 结合使用所获得的恒星光变曲线数据，并向读者提供了这些数据的在线资源库。