  The ALMA lensing cluster survey (ALCS) is a 96-hr large program dedicated to
uncovering and characterizing intrinsically faint continuum sources and line
emitters with the assistance of gravitational lensing. All 33 cluster fields
were selected from HST/Spitzer treasury programs including CLASH, Hubble
Frontier Fields, and RELICS, which also have Herschel and Chandra coverages.
The total sky area surveyed reaches $\sim$133 arcmin$^2$ down to a depth of
$\sim$60 $\mu$Jy beam$^{-1}$ (1$\sigma$) at 1.2 mm, yielding 141 secure blind
detections of continuum sources and additional 39 sources aided by priors. We
present scientific motivation, survey design, the status of spectroscopy
follow-up observations, and number counts down to $\sim$7 $\mu$Jy. Synergies
with JWST are also discussed.
