Pre-deployment verification and predicted mapping speed of MUSCAT

T. L.R. Brien; P. A.R. Ade; P. S. Barry; E. Castillo-Dominguez; D. Ferrusca; V. Gomez-Rivera; P. Hargrave; J. L. Hernandez Rebollar; A. Hornsby; D. H. Hughes; J. M. Jauregui-Garcia; P. Mauskopf; D. Murias; A. Papageorgiou; E. Pascale; A. Perez; S. Rowe; M. W.L. Smith; M. Tapia; C. Tucker; M. Velazquez; S. Ventura; S. Doyle

doi:10.1117/12.2561305

Pre-deployment verification and predicted mapping speed of MUSCAT

T. L.R. Brien, P. A.R. Ade, P. S. Barry, E. Castillo-Dominguez, D. Ferrusca, V. Gomez-Rivera, P. Hargrave, J. L. Hernandez Rebollar, A. Hornsby, D. H. Hughes, J. M. Jauregui-Garcia, P. Mauskopf, D. Murias, A. Papageorgiou, E. Pascale, A. Perez, S. Rowe, M. W.L. Smith, M. Tapia, C. TuckerM. Velazquez, S. Ventura, S. Doyle

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

3 Scopus citations

Abstract

The Mexico-UK Submillimetre Camera for AsTronomy (MUSCAT) is a 1.1 mm receiver consisting of 1,500 lumped-element kinetic inductance detectors (LEKIDs) for the Large Millimeter Telescope (LMT; Volcan Sierra Negra in Puebla, Mexico). MUSCAT utilises the maximum field of view of the LMT's upgraded 50-metre primary mirror and is the first Mexico-UK collaboration to deploy a millimetre/sub-mm receiver on the Large Millimeter Telescope. Using a simplistic simulator, we estimate a predicted mapping speed for MUSCAT by combining the measured performance of MUSCAT with the observed sky conditions at the LMT. We compare this to a previously calculated bolometric-model mapping speed and find that our mapping speed is in good agreement when this is scaled by a previously reported empirical factor. Through this simulation we show that signal contamination due to sky fluctuations can be effectively removed through the use of principle component analysis.

Original language	English (US)
Title of host publication	Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy X
Editors	Jonas Zmuidzinas, Jian-Rong Gao
Publisher	SPIE
ISBN (Electronic)	9781510636934
DOIs	https://doi.org/10.1117/12.2561305
State	Published - 2020
Externally published	Yes
Event	Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy X 2020 - Virtual, Online, United States Duration: Dec 14 2020 → Dec 22 2020

Publication series

Name	Proceedings of SPIE - The International Society for Optical Engineering
Volume	11453
ISSN (Print)	0277-786X
ISSN (Electronic)	1996-756X

Conference

Conference	Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy X 2020
Country/Territory	United States
City	Virtual, Online
Period	12/14/20 → 12/22/20

ASJC Scopus subject areas

Electronic, Optical and Magnetic Materials
Condensed Matter Physics
Computer Science Applications
Applied Mathematics
Electrical and Electronic Engineering

Access to Document

10.1117/12.2561305

Cite this

Brien, T. L. R., Ade, P. A. R., Barry, P. S., Castillo-Dominguez, E., Ferrusca, D., Gomez-Rivera, V., Hargrave, P., Hernandez Rebollar, J. L., Hornsby, A., Hughes, D. H., Jauregui-Garcia, J. M., Mauskopf, P., Murias, D., Papageorgiou, A., Pascale, E., Perez, A., Rowe, S., Smith, M. W. L., Tapia, M., ... Doyle, S. (2020). Pre-deployment verification and predicted mapping speed of MUSCAT. In J. Zmuidzinas, & J.-R. Gao (Eds.), Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy X Article 1145303 (Proceedings of SPIE - The International Society for Optical Engineering; Vol. 11453). SPIE. https://doi.org/10.1117/12.2561305

Pre-deployment verification and predicted mapping speed of MUSCAT. / Brien, T. L.R.; Ade, P. A.R.; Barry, P. S. et al.
Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy X. ed. / Jonas Zmuidzinas; Jian-Rong Gao. SPIE, 2020. 1145303 (Proceedings of SPIE - The International Society for Optical Engineering; Vol. 11453).

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

Brien, TLR, Ade, PAR, Barry, PS, Castillo-Dominguez, E, Ferrusca, D, Gomez-Rivera, V, Hargrave, P, Hernandez Rebollar, JL, Hornsby, A, Hughes, DH, Jauregui-Garcia, JM, Mauskopf, P, Murias, D, Papageorgiou, A, Pascale, E, Perez, A, Rowe, S, Smith, MWL, Tapia, M, Tucker, C, Velazquez, M, Ventura, S & Doyle, S 2020, Pre-deployment verification and predicted mapping speed of MUSCAT. in J Zmuidzinas & J-R Gao (eds), Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy X., 1145303, Proceedings of SPIE - The International Society for Optical Engineering, vol. 11453, SPIE, Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy X 2020, Virtual, Online, United States, 12/14/20. https://doi.org/10.1117/12.2561305

Brien TLR, Ade PAR, Barry PS, Castillo-Dominguez E, Ferrusca D, Gomez-Rivera V et al. Pre-deployment verification and predicted mapping speed of MUSCAT. In Zmuidzinas J, Gao JR, editors, Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy X. SPIE. 2020. 1145303. (Proceedings of SPIE - The International Society for Optical Engineering). doi: 10.1117/12.2561305

@inproceedings{a2db1c4e8e2b44069e8157ca3b2b37d7,

title = "Pre-deployment verification and predicted mapping speed of MUSCAT",

abstract = "The Mexico-UK Submillimetre Camera for AsTronomy (MUSCAT) is a 1.1 mm receiver consisting of 1,500 lumped-element kinetic inductance detectors (LEKIDs) for the Large Millimeter Telescope (LMT; Volcan Sierra Negra in Puebla, Mexico). MUSCAT utilises the maximum field of view of the LMT's upgraded 50-metre primary mirror and is the first Mexico-UK collaboration to deploy a millimetre/sub-mm receiver on the Large Millimeter Telescope. Using a simplistic simulator, we estimate a predicted mapping speed for MUSCAT by combining the measured performance of MUSCAT with the observed sky conditions at the LMT. We compare this to a previously calculated bolometric-model mapping speed and find that our mapping speed is in good agreement when this is scaled by a previously reported empirical factor. Through this simulation we show that signal contamination due to sky fluctuations can be effectively removed through the use of principle component analysis.",

author = "Brien, {T. L.R.} and Ade, {P. A.R.} and Barry, {P. S.} and E. Castillo-Dominguez and D. Ferrusca and V. Gomez-Rivera and P. Hargrave and {Hernandez Rebollar}, {J. L.} and A. Hornsby and Hughes, {D. H.} and Jauregui-Garcia, {J. M.} and P. Mauskopf and D. Murias and A. Papageorgiou and E. Pascale and A. Perez and S. Rowe and Smith, {M. W.L.} and M. Tapia and C. Tucker and M. Velazquez and S. Ventura and S. Doyle",

note = "Funding Information: We acknowledge RCUK and CONACYT through the Newton Fund (grant no. ST/P002803/1), CONACYT for supporting the fellowship for the instrument scientist (grant no. 053), Chase Research Cryogenics for the development of the sub-kelvin coolers and to XILINX Inc. for the donation of the FPGAs used for the ROACH2 boards. Publisher Copyright: {\textcopyright} COPYRIGHT SPIE. Downloading of the abstract is permitted for personal use only.; Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy X 2020 ; Conference date: 14-12-2020 Through 22-12-2020",

year = "2020",

doi = "10.1117/12.2561305",

language = "English (US)",

series = "Proceedings of SPIE - The International Society for Optical Engineering",

publisher = "SPIE",

editor = "Jonas Zmuidzinas and Jian-Rong Gao",

booktitle = "Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy X",

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TY - GEN

T1 - Pre-deployment verification and predicted mapping speed of MUSCAT

AU - Brien, T. L.R.

AU - Ade, P. A.R.

AU - Barry, P. S.

AU - Castillo-Dominguez, E.

AU - Ferrusca, D.

AU - Gomez-Rivera, V.

AU - Hargrave, P.

AU - Hernandez Rebollar, J. L.

AU - Hornsby, A.

AU - Hughes, D. H.

AU - Jauregui-Garcia, J. M.

AU - Mauskopf, P.

AU - Murias, D.

AU - Papageorgiou, A.

AU - Pascale, E.

AU - Perez, A.

AU - Rowe, S.

AU - Smith, M. W.L.

AU - Tapia, M.

AU - Tucker, C.

AU - Velazquez, M.

AU - Ventura, S.

AU - Doyle, S.

N1 - Funding Information: We acknowledge RCUK and CONACYT through the Newton Fund (grant no. ST/P002803/1), CONACYT for supporting the fellowship for the instrument scientist (grant no. 053), Chase Research Cryogenics for the development of the sub-kelvin coolers and to XILINX Inc. for the donation of the FPGAs used for the ROACH2 boards. Publisher Copyright: © COPYRIGHT SPIE. Downloading of the abstract is permitted for personal use only.

PY - 2020

Y1 - 2020

N2 - The Mexico-UK Submillimetre Camera for AsTronomy (MUSCAT) is a 1.1 mm receiver consisting of 1,500 lumped-element kinetic inductance detectors (LEKIDs) for the Large Millimeter Telescope (LMT; Volcan Sierra Negra in Puebla, Mexico). MUSCAT utilises the maximum field of view of the LMT's upgraded 50-metre primary mirror and is the first Mexico-UK collaboration to deploy a millimetre/sub-mm receiver on the Large Millimeter Telescope. Using a simplistic simulator, we estimate a predicted mapping speed for MUSCAT by combining the measured performance of MUSCAT with the observed sky conditions at the LMT. We compare this to a previously calculated bolometric-model mapping speed and find that our mapping speed is in good agreement when this is scaled by a previously reported empirical factor. Through this simulation we show that signal contamination due to sky fluctuations can be effectively removed through the use of principle component analysis.

AB - The Mexico-UK Submillimetre Camera for AsTronomy (MUSCAT) is a 1.1 mm receiver consisting of 1,500 lumped-element kinetic inductance detectors (LEKIDs) for the Large Millimeter Telescope (LMT; Volcan Sierra Negra in Puebla, Mexico). MUSCAT utilises the maximum field of view of the LMT's upgraded 50-metre primary mirror and is the first Mexico-UK collaboration to deploy a millimetre/sub-mm receiver on the Large Millimeter Telescope. Using a simplistic simulator, we estimate a predicted mapping speed for MUSCAT by combining the measured performance of MUSCAT with the observed sky conditions at the LMT. We compare this to a previously calculated bolometric-model mapping speed and find that our mapping speed is in good agreement when this is scaled by a previously reported empirical factor. Through this simulation we show that signal contamination due to sky fluctuations can be effectively removed through the use of principle component analysis.

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U2 - 10.1117/12.2561305

DO - 10.1117/12.2561305

M3 - Conference contribution

AN - SCOPUS:85100035623

T3 - Proceedings of SPIE - The International Society for Optical Engineering

BT - Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy X

A2 - Zmuidzinas, Jonas

A2 - Gao, Jian-Rong

PB - SPIE

T2 - Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy X 2020

Y2 - 14 December 2020 through 22 December 2020

ER -

Pre-deployment verification and predicted mapping speed of MUSCAT

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