The Cosmology Large Angular Scale Surveyor (CLASS) project aims to make a unique measurement of the Cosmic Microwave Background (CMB) that will transform our understanding of the universe and fundamental physics with far-reaching impacts on the scientific community, the next generation of scientists, and the public. As electromagnetic radiation, the CMB has both an intensity and a polarization, and it is the polarization of the CMB that CLASS will map over 70% of the sky.

Acknowledgements

We acknowledge the National Science Foundation Division of Astronomical Sciences for their support of CLASS under Grant Numbers 0959349, 1429236, 1636634, and 1654494. The CLASS project employs detector technology developed under several previous and ongoing NASA grants. Detector development work at JHU was funded by NASA grant number NNX14AB76A. We further acknowledge the very generous support of Jim and Heather Murren (JHU A&S ’88), Matthew Polk (JHU A&S Physics BS ’71), David Nicholson, and Michael Bloomberg (JHU Engineering ’64). CLASS is located in the Parque Astronómica Atacama in northern Chile under the auspices of the Comisión Nacional de Investigación Científica y Tecnológica de Chile (CONICYT).