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Optical Design of the TolTEC Millimeter-wave Camera

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arxiv 1807.00097 v1 pith:ZNCG3ZI6 submitted 2018-06-30 astro-ph.IM astro-ph.CO

Sean Bryan , Jason Austermann , Daniel Ferrusca , Philip Mauskopf , Jeff McMahon , Alfredo Montana , Sara Simon , Giles Novak
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David Sanchez-Arguelles Grant Wilson (for the TolTEC Team)
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keywords designinstrumentmodelopticalcameramillimeter-wavetoltecatmospheric
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TolTEC is a new camera being built for the 50-meter Large Millimeter-wave Telescope (LMT) in Puebla, Mexico to survey distant galaxies and star-forming regions in the Milky Way. The optical design simultaneously couples the field of view onto focal planes at 150, 220, and 280 GHz. The optical design and detector properties, as well as a data-driven model of the atmospheric emission of the LMT site, inform the sensitivity model of the integrated instrument. This model is used to optimize the instrument design, and to calculate the mapping speed as an early forecast of the science reach of the instrument.

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