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Far-infrared transparent conductors
The long-standing challenge in designing far-infrared transparent conductors (FIRTC) is the combination of high plasma absorption edge ( λ p ) and high...
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Beamforming of Electrically Tunable Plasmonic Graphene Strip Nanoantennas in the Terahertz, Far-Infrared, and Mid-Infrared Ranges
Abstract —The purpose of this work is to study, using automated modeling methods, the possibility of scanning in frequency and beamforming of...
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A Vacuum Waveguide Filter Bank Spectrometer for Far-Infrared Astrophysics
Traditional technologies for far-infrared (FIR) spectroscopy generally involve bulky dispersive optics. Integrated filter bank spectrometers promise...
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Laser Spectroscopy in the Submillimeter and Far-Infrared Regions
Recent technical developments in sub-millimeter and far-infrared laser spectroscopy are described. This includes new laser sources, both side-band...
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Far infrared properties of OH megamaser host galaxies
The hosts of OH megamaser (OHM) are luminous infrared galaxies (LIRGs), in fact 1/3 of them are ultra-luminous infrared galaxies (ULIRGs), which...
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Parallel Plate Capacitor Aluminum KIDs for Future Far-Infrared Space-Based Observatories
Future space-based far-infrared astrophysical observatories will require exquisitely sensitive detectors consistent with the low optical backgrounds....
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High-Sensitivity Kinetic Inductance Detector Arrays for the PRobe Far-Infrared Mission for Astrophysics
Far-infrared (far-IR) astrophysics missions featuring actively cooled telescopes will offer orders of magnitude observing speed improvement at...
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Observational Manifestations of First Galaxies in the Far Infrared Range
High-redshift galaxies ( z ≳ 9) are currently observed in the near-infrared (1.4-2 μm), mid-infrared (IR) (5-28.8 μm), and submillimeter (500-1000 μm)...
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Far-Infrared and Submillimetre Lighthouses
Evidence is discussed which strongly suggests that the sources discovered in deep submillimetre (submm) surveys form a major population of distant...
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The Contribution of AGN to the Far Infrared Background
We use synthesis models for the X-ray background, together with quasar Spectral Energy Distributions, to estimate the contribution of Active Galactic...
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Tunable frequency selective surface using crossed shaped graphene metasurface geometry for far infrared frequency spectrum
The mathematical and numerical analysis of the Graphene infrared tunable frequency selective surface (FSS) for far-infrared spectrum has been...
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Infrared Model Dielectric Functions
This chapter reviews a selection of dielectric function models progressed for lineshape analysis of (far) infrared ellipsometry data. Contributions...
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The far-infrared spectroscopic surveyor (FIRSS)
We are standing at the crossroads of powerful new facilities emerging in the next decade on the ground and in space like ELT, SKA, JWST, and Athena....
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Far-infrared frequency mode conversion using bulk acoustic phonon modes
The ability to design, fabricate and control systems which can convert photons with dissimilar frequencies has technological implications in...
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Graphene-based triple-band switch with circuit model method in far-infrared region
In this paper, a tunable triple-band plasmonic switch based on an array of graphene rings has been studied in the far-infrared region. The...
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Infrared Spectroscopy
Coblentz determined the relation between infrared spectra and molecular identity. Infrared spectroscopy became a tool for chemical analysis widely...
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Single-Cycle Infrared Waveform Generation and Control
Tailoring the electric-field waveform of few-cycle light pulses lays the foundation for controlling nonlinear optical phenomena on their genuine,...
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Bringing high spatial resolution to the far-infrared
The far-infrared (FIR) regime is one of the wavelength ranges where no astronomical data with sub-arcsecond spatial resolution exist. None of the...
