Band-4+5 Receiver Front-End: Idea and Initial Development in East Asia Consortium

We propose an upgrade to the ALMA Wideband Sensitivity Upgrade (WSU) by developing a new receiver with increased RF and IF bandwidth. The new receiver will cover the RF frequency of the original Band-4 and Band-5 with continuous frequency tuning over dual polarizations, dual sidebands with instantaneous intermediate frequency (IF) bandwidth up to 16 GHz per sideband and per polarization. Both the SIS-based receiver and HEMT-based receiver schemes are considered. The SIS-based receiver is considered as the baseline design, a sideband separation downconverter with the input fed by the ellipsoidal mirror pairs, corrugated feedhorn and the orthomode transducer form the cold cartridge assembly (CCA). The niobium-based SIS junctions will be fabricated to form mixer chips, and integrated into the mixer blocks with WR-5.44 waveguide 3-dB quadrature hybrid couplers, cryogenic IF low-noise amplifiers, and 2-20 GHz coaxial 3-dB quadrature hybrid couplers to form sideband separating down-converters. For the HEMT-based receiver scheme, the cryogenic InP HEMT low-noise amplifiers (LNAs) chains cover 125 - 211 GHz operated in 15-K ambient temperature will be the key components, to suppress multiple reflection ripples, cryogenic 2SB mixers are considered. To avoid the possible interference between LO and IF signals, the LO fundamental frequency are chosen in 24 - 32 GHz, followed by a frequency tripler to form the phase-lock loop with 72 - 96 GHz frequency tuning range.

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Publication Details

Journal
Zenodo (CERN European Organization for Nuclear Research)
Published
2024-09-04
DOI
https://doi.org/10.5281/zenodo.13681506
Primary Topic
Optical Polarization and Ellipsometry
Type
article
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article

Band-4+5 Receiver Front-End: Idea and Initial Development in East Asia Consortium

Zenodo (CERN European Organization for Nuclear Research)
Optical Polarization and Ellipsometry
article

Band-4+5 Receiver Front-End: Idea and Initial Development in East Asia Consortium

article en

Abstract

We propose an upgrade to the ALMA Wideband Sensitivity Upgrade (WSU) by developing a new receiver with increased RF and IF bandwidth. The new receiver will cover the RF frequency of the original Band-4 and Band-5 with continuous frequency tuning over dual polarizations, dual sidebands with instantaneous intermediate frequency (IF) bandwidth up to 16 GHz per sideband and per polarization. Both the SIS-based receiver and HEMT-based receiver schemes are considered. The SIS-based receiver is considered as the baseline design, a sideband separation downconverter with the input fed by the ellipsoidal mirror pairs, corrugated feedhorn and the orthomode transducer form the cold cartridge assembly (CCA). The niobium-based SIS junctions will be fabricated to form mixer chips, and integrated into the mixer blocks with WR-5.44 waveguide 3-dB quadrature hybrid couplers, cryogenic IF low-noise amplifiers, and 2-20 GHz coaxial 3-dB quadrature hybrid couplers to form sideband separating down-converters. For the HEMT-based receiver scheme, the cryogenic InP HEMT low-noise amplifiers (LNAs) chains cover 125 - 211 GHz operated in 15-K ambient temperature will be the key components, to suppress multiple reflection ripples, cryogenic 2SB mixers are considered. To avoid the possible interference between LO and IF signals, the LO fundamental frequency are chosen in 24 - 32 GHz, followed by a frequency tripler to form the phase-lock loop with 72 - 96 GHz frequency tuning range.

Zenodo (CERN European Organization for Nuclear Research)
Institute of Astronomy and Astrophysics, Academia Sinica (TW), Yuan Ze University (TW)
Openalex Percentile: Top 67%
Optical Polarization and Ellipsometry
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