After stars formed in the early Universe, their ultraviolet light is expected, eventually, to have
penetrated the primordial hydrogen gas and altered the excitation state of its 21-centimetre …

Our paper reviews the use of conductive polymer composite materials in various
applications for semi conductive, static-dissipative, anti-corrosive, electromagnetic …

The cosmological 21 cm signal is one of the most promising avenues to study the Epoch of
Reionization. One class of experiments aiming to detect this signal is global signal …

Changing observing strategies and the increased sensitivity of radio astronomy
observatories have made radio frequency interference an important operational factor. All …

The deuterium abundance in the primordial gas formed during the big bang is dependent on
the baryon-to-photon ratio during nucleosynthesis. We report a measurement of the …

Radio astronomy studies cosmic sources through their radio emissions. As passive users,
astronomers have to deal with an increasingly corrupted radio spectrum. The research …

We report measurements of the 327 MHz line of deuterium for regions in the Galactic plane
at 171, 183, and 195 longitude using an array of 24 stations of fixed phased-antenna …

We report sensitive spectrum measurements from 70 to 1500 MHz of the radio interference
(RFI) environment at locations in Westford, Massachusetts and Hancock, New Hampshire …

Radio astronomy is a subfield of astronomy, which studies celestial objects with highly
sensitive radio receivers and large radio telescopes. These radio astronomical …

Mitigation techniques fall into three general categories:– Preventing radio frequency
interference (RFI) signals from entering the astronomical data, including reduction of the …