A hybrid Fourier transform spectrometer with filterbank post-dispersion is proposed to reduce photon noise by over an order of magnitude while preserving imaging capabilities for R~1000 line intensity mapping.
Snowmass 2021 Cosmic Frontier White Paper: Cosmology with Millimeter-Wave Line Intensity Mapping
4 Pith papers cite this work, alongside 8 external citations. Polarity classification is still indexing.
verdicts
UNVERDICTED 4representative citing papers
TIFUUN is a portable 90-360 GHz integral field spectrometer with up to 18,000 detectors and R up to 1000, optimized for CII line intensity mapping at z~6 on the ASTE telescope.
Optimizing electron-beam lithography via smaller beam step size and avoiding main-field stitching reduces random and systematic frequency scatter four-fold in superconducting microstrip resonators.
Reviews how cross-correlating SKAO 21-cm LIM with other lines like [CII], CO, and Ly-alpha can mitigate systematics, enhance sensitivity, and disentangle cosmological from astrophysical parameters.
citing papers explorer
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Low-noise Fourier Transform Spectroscopy Enabled by Superconducting On-Chip Filterbank Spectrometers
A hybrid Fourier transform spectrometer with filterbank post-dispersion is proposed to reduce photon noise by over an order of magnitude while preserving imaging capabilities for R~1000 line intensity mapping.
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Development of TIFUUN: Terahertz Integral Field Units with Universal Nanotechnology
TIFUUN is a portable 90-360 GHz integral field spectrometer with up to 18,000 detectors and R up to 1000, optimized for CII line intensity mapping at z~6 on the ASTE telescope.
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Enhanced electron-beam lithography to reduce the frequency scatter of 200-400 GHz superconducting microstrip resonators for on-chip filterbank spectrometers
Optimizing electron-beam lithography via smaller beam step size and avoiding main-field stitching reduces random and systematic frequency scatter four-fold in superconducting microstrip resonators.
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Cosmology with Multi-Wavelength Line Intensity Mapping Synergies in the SKAO Era
Reviews how cross-correlating SKAO 21-cm LIM with other lines like [CII], CO, and Ly-alpha can mitigate systematics, enhance sensitivity, and disentangle cosmological from astrophysical parameters.