Mexico-UK Submillimeter Camera for AsTronomy focal plane performance at the Large Millimeter Telescope

The Mexico-UK Submillimeter Camera for AsTronomy (MUSCAT) is a continuum camera in the 1.1-mm band for the Large Millimeter Telescope (LMT), with 1458 lumped-element kinetic inductance detectors distributed across six arrays. Installed on the telescope at the end of 2021, we present the characterization of the detector beams of four of the six arrays based on the beam map observations of bright point sources developed during the first commissioning campaign between February and June 2022. With all the observations, we estimate the average positions of each detector with an average error in azimuth of less than 0.70 arcsec and less than 1.05 arcsec in elevation. From the positions, we created the coadded maps of all the detectors, from which we selected only eight observations to calculate the mean beam width of MUSCAT-LMT, of 6.32±0.36 arcsec⁡×5.78±0.19 arcsec. By stacking the maps, we identify the sidelobes with three main structures whose amplitudes are ∼3% with respect to the main beam.

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Journal
Journal of Astronomical Telescopes Instruments and Systems
Published
2024-10-25
DOI
https://doi.org/10.1117/1.jatis.10.4.045003
Primary Topic
Superconducting and THz Device Technology
Type
article
Field-Weighted Citation Impact
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article

Mexico-UK Submillimeter Camera for AsTronomy focal plane performance at the Large Millimeter Telescope

David W. Hughes, Emmaly Aguilar Pérez, P. Mauskopf, Salvador Ventura-González et al.
Journal of Astronomical Telescopes Instruments and Systems
Superconducting and THz Device Technology
article

Mexico-UK Submillimeter Camera for AsTronomy focal plane performance at the Large Millimeter Telescope

David W. Hughes, Emmaly Aguilar Pérez, P. Mauskopf, Salvador Ventura-González, Christopher Dodd, José Luis Hernández-Rebollar, P. A. R. Ade, Amber Hornsby, Kamal Souccar, Edgar Castillo-Domínguez, Miguel Velázquez, C. Tucker, A. Torres-Campos, N. Peretto, Peter Hargrave, Ανδρέας Παπαγεωργίου, Dulce Murias, Ian J. Walker, Thomas L. R. Brien, E. Pascale, David Sánchez-Argüelles, Julian S. House, Víctor Gómez-Rivera, M. W. L. Smith, Iván Rodríguez, José Miguel Jáuregui-García, A. Luna, D. Ferrusca, P. S. Barry, Marcial Tapia, R. V. Sudiwala, Stephen Eales, S. Doyle, A. Pérez, C. Dunscombe, Samuel Rowe
article en

Abstract

The Mexico-UK Submillimeter Camera for AsTronomy (MUSCAT) is a continuum camera in the 1.1-mm band for the Large Millimeter Telescope (LMT), with 1458 lumped-element kinetic inductance detectors distributed across six arrays. Installed on the telescope at the end of 2021, we present the characterization of the detector beams of four of the six arrays based on the beam map observations of bright point sources developed during the first commissioning campaign between February and June 2022. With all the observations, we estimate the average positions of each detector with an average error in azimuth of less than 0.70 arcsec and less than 1.05 arcsec in elevation. From the positions, we created the coadded maps of all the detectors, from which we selected only eight observations to calculate the mean beam width of MUSCAT-LMT, of 6.32±0.36 arcsec⁡×5.78±0.19 arcsec. By stacking the maps, we identify the sidelobes with three main structures whose amplitudes are ∼3% with respect to the main beam.

Journal of Astronomical Telescopes Instruments and SystemsVol. 10(04)
University of Massachusetts Amherst (US), Commissariat à l'Énergie Atomique et aux Énergies Alternatives (FR), Université Paris-Saclay (FR), Centro de Investigaciones en Optica (MX), National Institute of Astrophysics, Optics and Electronics (MX), University of Oxford (GB), CEA Paris-Saclay (FR), Institut de Recherche sur les Lois Fondamentales de l'Univers (FR), Arizona State University (US), Cardiff University (GB), Sapienza University of Rome (IT), University of California, Berkeley (US)
Science and Technology Facilities Council
Affordable and clean energy
Openalex Percentile: Top 86%
Superconducting and THz Device Technology
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