Terahertz hot electron bolometer waveguide mixers for GREAT
arXiv:1204.2381 · doi:10.1051/0004-6361/201218916
Abstract
Supplementing the publications based on the first-light observations with the German Receiver for Astronomy at Terahertz frequencies (GREAT) on SOFIA, we present background information on the underlying heterodyne detector technology. We describe the superconducting hot electron bolometer (HEB) detectors that are used as frequency mixers in the L1 (1400 GHz), L2 (1900 GHz), and M (2500 GHz) channels of GREAT. Measured performance of the detectors is presented and background information on their operation in GREAT is given. Our mixer units are waveguide-based and couple to free-space radiation via a feedhorn antenna. The HEB mixers are designed, fabricated, characterized, and flight-qualified in-house. We are able to use the full intermediate frequency bandwidth of the mixers using silicon-germanium multi-octave cryogenic low-noise amplifiers with very low input return loss. Superconducting HEB mixers have proven to be practical and sensitive detectors for high-resolution THz frequency spectroscopy on SOFIA. We show that our niobium-titanium-nitride (NbTiN) material HEBs on silicon nitride (SiN) membrane substrates have an intermediate frequency (IF) noise roll-off frequency above 2.8 GHz, which does not limit the current receiver IF bandwidth. Our mixer technology development efforts culminate in the first successful operation of a waveguide-based HEB mixer at 2.5 THz and deployment for radioastronomy. A significant contribution to the success of GREAT is made by technological development, thorough characterization and performance optimization of the mixer and its IF interface for receiver operation on SOFIA. In particular, the development of an optimized mixer IF interface contributes to the low passband ripple and excellent stability, which GREAT demonstrated during its initial successful astronomical observation runs.
Accepted for publication in A&A (SOFIA/GREAT special issue)
References in corpus (2)
Cited by in corpus (12)
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- The upGREAT dual frequency heterodyne arrays for SOFIA
- Hot electron bolometer heterodyne receiver with a 4.7-THz quantum cascade laser as a local oscillator
- Room Temperature Terahertz Spectrometer with Quantum-Level Sensitivity
- The SOFIA Observatory at the Start of Routine Science Operations : Mission capabilities and performance
- Engineering physics of superconducting hot-electron bolometer mixers
- Unveiling the chemistry of interstellar CH: Spectroscopy of the 2 THz ground state line
- 4GREAT -- a four-color receiver for high-resolution airborne terahertz spectroscopy
- Nonequilibrium interpretation of DC properties of NbN superconducting hot electron bolometers
- Plasmonic Heterodyne Spectrometry for Resolving the Spectral Signatures of Ammonia over a 1-5 THz Frequency Range
- Improved Nb SIS devices for heterodyne mixers between 700 GHz and 1.3 THz with NbTiN transmission lines using a normal metal energy relaxation layer