Quasi-Optical System for the ASTE Telescope with 1:3 Bandwidth at Sub-mm Wave

S.O. Dabironezare; G. Carluccio; A. Pascual Laguna; S. Hähnle; J. Baselmans; N. Llombart

doi:10.1109/IRMMW-THz.2019.8874065

Quasi-Optical System for the ASTE Telescope with 1:3 Bandwidth at Sub-mm Wave

S.O. Dabironezare, G. Carluccio, A. Pascual Laguna, S. Hähnle, J. Baselmans, N. Llombart

Tera-Hertz Sensing

Research output: Chapter in Book/Conference proceedings/Edited volume › Conference contribution › Scientific › peer-review

3 Citations (Scopus)

60 Downloads (Pure)

Abstract

DESHIMA is a spectrometer for astronomical applications targeting sources at sub-mm wavelengths from 240GHz to 720GHz that will operate in the ASTE telescope in Atacama Desert, Chile. In this work, a quasi-optical system based on a hyper-hemispherical leaky lens antenna and a series of Dragonian reflectors is presented as the coupling chain for the EM radiation captured by the telescope into the detector. The design procedure is based on a field matching technique in reception. The achieved average illumination efficiency over the band is approximately 70%. The directivity patterns in the sky are also estimated. The side lobe, and cross-polarization levels, over the whole frequency band, are below-16dB, and-18dB, respectively. The measurement of the system is on-going, and will be presented at the conference.

Original language	English
Title of host publication	IRMMW-THz 2019 - 44th International Conference on Infrared, Millimeter, and Terahertz Waves
Publisher	IEEE
Pages	1-2
Number of pages	2
ISBN (Electronic)	978-1-5386-8285-2
ISBN (Print)	978-1-5386-8286-9
DOIs	https://doi.org/10.1109/IRMMW-THz.2019.8874065
Publication status	Published - 2019
Event	44th International Conference on Infrared, Millimeter, and Terahertz Waves, IRMMW-THz 2019 - Paris, France Duration: 1 Sept 2019 → 6 Sept 2019

Publication series

Name	International Conference on Infrared, Millimeter, and Terahertz Waves, IRMMW-THz
Volume	2019-September
ISSN (Print)	2162-2027
ISSN (Electronic)	2162-2035

Conference

Conference	44th International Conference on Infrared, Millimeter, and Terahertz Waves, IRMMW-THz 2019
Country/Territory	France
City	Paris
Period	1/09/19 → 6/09/19

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10.1109/IRMMW-THz.2019.8874065

IRMMWTHz2019Accepted author manuscript, 569 KB

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Dabironezare, S. O., Carluccio, G., Pascual Laguna, A., Hähnle, S., Baselmans, J., & Llombart, N. (2019). Quasi-Optical System for the ASTE Telescope with 1:3 Bandwidth at Sub-mm Wave. In IRMMW-THz 2019 - 44th International Conference on Infrared, Millimeter, and Terahertz Waves (pp. 1-2). Article 8874065 (International Conference on Infrared, Millimeter, and Terahertz Waves, IRMMW-THz; Vol. 2019-September). IEEE. https://doi.org/10.1109/IRMMW-THz.2019.8874065

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title = "Quasi-Optical System for the ASTE Telescope with 1:3 Bandwidth at Sub-mm Wave",

abstract = "DESHIMA is a spectrometer for astronomical applications targeting sources at sub-mm wavelengths from 240GHz to 720GHz that will operate in the ASTE telescope in Atacama Desert, Chile. In this work, a quasi-optical system based on a hyper-hemispherical leaky lens antenna and a series of Dragonian reflectors is presented as the coupling chain for the EM radiation captured by the telescope into the detector. The design procedure is based on a field matching technique in reception. The achieved average illumination efficiency over the band is approximately 70%. The directivity patterns in the sky are also estimated. The side lobe, and cross-polarization levels, over the whole frequency band, are below-16dB, and-18dB, respectively. The measurement of the system is on-going, and will be presented at the conference.",

author = "S.O. Dabironezare and G. Carluccio and {Pascual Laguna}, A. and S. H{\"a}hnle and J. Baselmans and N. Llombart",

year = "2019",

doi = "10.1109/IRMMW-THz.2019.8874065",

language = "English",

isbn = "978-1-5386-8286-9",

series = "International Conference on Infrared, Millimeter, and Terahertz Waves, IRMMW-THz",

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booktitle = "IRMMW-THz 2019 - 44th International Conference on Infrared, Millimeter, and Terahertz Waves",

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Dabironezare, SO, Carluccio, G, Pascual Laguna, A, Hähnle, S, Baselmans, J & Llombart, N 2019, Quasi-Optical System for the ASTE Telescope with 1:3 Bandwidth at Sub-mm Wave. in IRMMW-THz 2019 - 44th International Conference on Infrared, Millimeter, and Terahertz Waves., 8874065, International Conference on Infrared, Millimeter, and Terahertz Waves, IRMMW-THz, vol. 2019-September, IEEE, pp. 1-2, 44th International Conference on Infrared, Millimeter, and Terahertz Waves, IRMMW-THz 2019, Paris, France, 1/09/19. https://doi.org/10.1109/IRMMW-THz.2019.8874065

Quasi-Optical System for the ASTE Telescope with 1:3 Bandwidth at Sub-mm Wave. / Dabironezare, S.O.; Carluccio, G.; Pascual Laguna, A. et al.
IRMMW-THz 2019 - 44th International Conference on Infrared, Millimeter, and Terahertz Waves. IEEE, 2019. p. 1-2 8874065 (International Conference on Infrared, Millimeter, and Terahertz Waves, IRMMW-THz; Vol. 2019-September).

Research output: Chapter in Book/Conference proceedings/Edited volume › Conference contribution › Scientific › peer-review

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T1 - Quasi-Optical System for the ASTE Telescope with 1:3 Bandwidth at Sub-mm Wave

AU - Dabironezare, S.O.

AU - Carluccio, G.

AU - Pascual Laguna, A.

AU - Hähnle, S.

AU - Baselmans, J.

AU - Llombart, N.

PY - 2019

Y1 - 2019

N2 - DESHIMA is a spectrometer for astronomical applications targeting sources at sub-mm wavelengths from 240GHz to 720GHz that will operate in the ASTE telescope in Atacama Desert, Chile. In this work, a quasi-optical system based on a hyper-hemispherical leaky lens antenna and a series of Dragonian reflectors is presented as the coupling chain for the EM radiation captured by the telescope into the detector. The design procedure is based on a field matching technique in reception. The achieved average illumination efficiency over the band is approximately 70%. The directivity patterns in the sky are also estimated. The side lobe, and cross-polarization levels, over the whole frequency band, are below-16dB, and-18dB, respectively. The measurement of the system is on-going, and will be presented at the conference.

AB - DESHIMA is a spectrometer for astronomical applications targeting sources at sub-mm wavelengths from 240GHz to 720GHz that will operate in the ASTE telescope in Atacama Desert, Chile. In this work, a quasi-optical system based on a hyper-hemispherical leaky lens antenna and a series of Dragonian reflectors is presented as the coupling chain for the EM radiation captured by the telescope into the detector. The design procedure is based on a field matching technique in reception. The achieved average illumination efficiency over the band is approximately 70%. The directivity patterns in the sky are also estimated. The side lobe, and cross-polarization levels, over the whole frequency band, are below-16dB, and-18dB, respectively. The measurement of the system is on-going, and will be presented at the conference.

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M3 - Conference contribution

SN - 978-1-5386-8286-9

T3 - International Conference on Infrared, Millimeter, and Terahertz Waves, IRMMW-THz

SP - 1

EP - 2

BT - IRMMW-THz 2019 - 44th International Conference on Infrared, Millimeter, and Terahertz Waves

PB - IEEE

T2 - 44th International Conference on Infrared, Millimeter, and Terahertz Waves, IRMMW-THz 2019

Y2 - 1 September 2019 through 6 September 2019

ER -

Dabironezare SO, Carluccio G, Pascual Laguna A, Hähnle S, Baselmans J , Llombart N. Quasi-Optical System for the ASTE Telescope with 1:3 Bandwidth at Sub-mm Wave. In IRMMW-THz 2019 - 44th International Conference on Infrared, Millimeter, and Terahertz Waves. IEEE. 2019. p. 1-2. 8874065. (International Conference on Infrared, Millimeter, and Terahertz Waves, IRMMW-THz). doi: 10.1109/IRMMW-THz.2019.8874065

Quasi-Optical System for the ASTE Telescope with 1:3 Bandwidth at Sub-mm Wave

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