Presentation
29 August 2022 The Large Millimeter Telescope: Current status and telescope performance
Author Affiliations +
Abstract
The Large Millimeter Telescope (LMT) Alfonso Serrano is a bi-national (Mexico and USA) telescope facility constructed on the summit of Sierra Negra, at an altitude of 4600m, in the Mexican state of Puebla. The LMT is a 50-m diameter single-dish telescope, with an active surface control-system to correct gravitational and thermal deformations of the primary reflector, designed and optimized to conduct scientific observations using heterodyne and continuum receivers, as well as VLBI observations, at frequencies between ~70 and 350 GHz.  We describe the current status and technical performance of the recently commissioned LMT 50-m, the instrumentation development program, and future engineering upgrades that will optimize the optical efficiency of the telescope and increase its scientific productivity.
Conference Presentation
© (2022) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
David H. Hughes, F. Peter Schloerb, Emmaly Aguilar Perez, Itziar Aretxaga, Edgar Castillo-Domínguez, Miguel Chávez Dagostino, Edgar Colín, Daniel Ferrusca Rodriguez Sr., David M. Gale, Víctor Gómez-Rivera, Arturo Gómez-Ruiz, José Luis Hernández Rebollar, Alfredo Montaña, Emir Marcos Moreno Nolasco, Lee G. Mundy, Gopal Narayanan, Alexandra Pope, Iván Rodríguez-Montoya, David Sánchez-Argüelles, David R. Smith, Kamal Souccar, Miguel Veláquez de la Rosa Becerra, Grant W. Wilson, and Min S. Yun "The Large Millimeter Telescope: Current status and telescope performance", Proc. SPIE 12182, Ground-based and Airborne Telescopes IX, 1218213 (29 August 2022); https://doi.org/10.1117/12.2630664
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KEYWORDS
Telescopes

Cameras

Receivers

Optical instrument design

Reflectors

Sensors

Spectroscopes

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