  The Cerro Chajnantor Atacama Telescope-prime (CCAT-prime) is a new 6-m,
off-axis, low-emissivity, large field-of-view submillimeter telescope scheduled
for first light in the last quarter of 2021. In summary, (a) CCAT-prime
uniquely combines a large field-of-view (up to 8-deg), low emissivity telescope
(< 2%) and excellent atmospheric transmission (5600-m site) to achieve
unprecedented survey capability in the submillimeter. (b) Over five years,
CCAT-prime first generation science will address the physics of star formation,
galaxy evolution, and galaxy cluster formation; probe the re-ionization of the
Universe; improve constraints on new particle species; and provide for improved
removal of dust foregrounds to aid the search for primordial gravitational
waves. (c) The Observatory is being built with non-federal funds (~ \$40M in
private and international investments). Public funding is needed for
instrumentation (~ \$8M) and operations (\$1-2M/yr). In return, the community
will be able to participate in survey planning and gain access to curated data
sets. (d) For second generation science, CCAT-prime will be uniquely positioned
to contribute high-frequency capabilities to the next generation of CMB surveys
in partnership with the CMB-S4 and/or the Simons Observatory projects or
revolutionize wide-field, sub-millimetter line intensity mapping surveys.
