Results 21 to 30 of about 38,151 (299)
125 - 211 GHz low noise MMIC amplifier design for radio astronomy [PDF]
To achieve the low noise and wide bandwidth required for millimeter wavelength astronomy applications, superconductor-insulator-superconductor (SIS) mixer based receiver systems have typically been used.
Cleary, Kieran +7 more
core +2 more sources
Introduction to Millimeter/Sub-millimeter Astronomy [PDF]
This is an introduction to the basic elements needed for the measurements and interpretation of data in the millimeter and sub-mm wavelength range. A more complete version will be published in the proceedings of the Saas Fee Winter School 2008.
openaire +2 more sources
A broadband FFT spectrometer for radio and millimeter astronomy [PDF]
Astronomy and Astrophysics, in ...
Benz, Arnold O. +6 more
openaire +2 more sources
Herschel Far-Infrared and Sub-millimeter Photometry for the KINGFISH Sample of Nearby Galaxies [PDF]
New far-infrared and sub-millimeter photometry from the Herschel Space Observatory is presented for 61 nearby galaxies from the Key Insights on Nearby Galaxies: A Far-Infrared Survey with Herschel (KINGFISH) sample.
A. D. Bolatto +66 more
core +4 more sources
Digital compensation of the side-band-rejection ratio in a fully analog 2SB sub-millimeter receiver [PDF]
In observational radio astronomy, sideband-separating receivers are preferred, particularly under high atmospheric noise, which is usually the case in the sub-millimeter range.
Alvear, A. +9 more
core +2 more sources
Development of Wideband Tunable E-Band (60-70 GHz) Gunn Oscillator [PDF]
A Gunn waveguide-oscillator, mechanically tunable from 60 to 70 GHz, has been developed for use as a local oscillator (LO) in millimeter radio telescope.
Hyunjoo Kim +3 more
doaj
In the next decades millimeter and sub-mm astronomy requires large format imaging arrays and broad-band spectrometers to complement the high spatial and spectral resolution of the Atacama Large Millimeter/sub-millimeter Array.
Baryshev, A. M. +6 more
core +1 more source
We present a high-angular resolution (∼1″) and wide-field ( $2\buildrel{\,\prime}\over{.} 9\times 1\buildrel{\,\prime}\over{.} 9$ ) image of the 1.3 mm continuum, CO( J = 2–1) and SiO( J = 5–4) line emissions toward an embedded protocluster, FIR 3, FIR 4,
Asako Sato +8 more
doaj +1 more source
Electromagnetic reprogrammable coding-metasurface holograms
Realizing metasurfaces with reconfigurability, high efficiency, and control over phase and amplitude is a challenge. Here, Li et al. introduce a reprogrammable hologram based on a 1-bit coding metasurface, where the state of each unit cell of the coding ...
Lianlin Li +9 more
doaj +1 more source
A Low Noise Receiver for Submillimeter Astronomy [PDF]
A broadband, low noise heterodyne receiver, suitable for astronomical use, has been built using a Pb alloy superconducting tunnel junction (SIS). The RF coupling is quasioptical via a bowtie antenna on a quartz lens and is accomplished without any tuning
Miller, R. E. +3 more
core +1 more source

