Emily Lunde,1 Marc Berthoud,2 N. S. DeNigris,3 Simon Doyle,4 Daniel Ferrusca Sr.,5 Joseph E. Golechttps://orcid.org/0000-0002-4421-0267,6 Stephen Kuczarski,3 Dennis Leehttps://orcid.org/0000-0002-3455-1826,2 Zhiyuan Ma,3 Philip Mauskopf,1 Michael McCrackan,3 Jeffrey McMahon,6 Giles Novak,2 Giampaolo Pisano,4 Sara Simon,6 Kamal Souccar,3 Carole Tucker,4 Matthew Underhill,1 Eric Van Camp,2 Grant W. Wilson3
1Arizona State Univ. (United States) 2Northwestern Univ. (United States) 3Univ. of Massachusetts Amherst (United States) 4Cardiff Univ. (United Kingdom) 5Instituto Nacional de Astrofísica, Óptica y Electrónica (Mexico) 6Univ. of Chicago (United States)
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The TolTEC camera is an imaging polarimeter installed at the Large Millimeter Telescope (LMT) in Mexico during December 2021. This new camera uses polarization-sensitive Kinetic Inductance Detectors (KIDs) coupled to the 50 m LMT to produce high resolution images simultaneously at 1.1, 1.4, and 2.0 mm wavelengths. We present a description of the cryogenic camera optics, the warm coupling optics, and the techniques used for on-site alignment of TolTEC with the telescope and characterization of the optics.
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Emily Lunde, Marc Berthoud, N. S. DeNigris, Simon Doyle, Daniel Ferrusca Sr., Joseph E. Golec, Stephen Kuczarski, Dennis Lee, Zhiyuan Ma, Philip Mauskopf, Michael McCrackan, Jeffrey McMahon, Giles Novak, Giampaolo Pisano, Sara Simon, Kamal Souccar, Carole Tucker, Matthew Underhill, Eric Van Camp, Grant W. Wilson, "The TolTEC camera: optical alignment and characterization," Proc. SPIE 12190, Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy XI, 1219016 (31 August 2022); https://doi.org/10.1117/12.2630340