Kavli Affiliate: Zeeshan Ahmed
| First 5 Authors: Tanay Bhandarkar, Saianeesh K. Haridas, Jeff Iuliano, Anna Kofman, Alex Manduca
| Summary:
The Simons Observatory (SO) is a ground-based cosmic microwave background
(CMB) survey experiment that currently consists of three 0.42m small-aperture
telescopes (SATs) and one 6m large-aperture telescope (LAT), located at an
elevation of 5200m in the Atacama Desert in Chile. At the LAT’s focal plane, SO
will install >62,000 transition-edge sensor detectors across 13 optics tubes
(OTs) within the Large Aperture Telescope Receiver (LATR), the largest
cryogenic camera ever built to observe the CMB. Here we report on the
validation of the LATR in the laboratory and the subsequent dark testing and
validation within the LAT. We show that the LATR meets cryogenic, optical, and
detector specifications required for high-sensitivity measurements of the CMB.
At the time of writing, the LATR is installed in the LAT with six OTs
(corresponding to >31,000 detectors), and the LAT mirrors and remaining seven
OTs are undergoing development.
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