Description
The Simons Observatory is a new observatory in Chile consisting of multiple telescopes observing the Cosmic Microwave Background and millimetre sky at 27-280 GHz. Here, I will review the status of commissioning and early science activities for the Large Aperture Telescope and three Small Aperture Telescopes (SATs), all of which have now been deployed. In particular, I will highlight early data products and analysis from the SAT survey, aimed at future constraints on primordial B-mode polarisation.
Author
Erik Rosenberg
(University of Manchester)
