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S

S. Duscha

Researcher at ASTRON

Publications -  63
Citations -  3161

S. Duscha is an academic researcher from ASTRON. The author has contributed to research in topics: LOFAR & Radio telescope. The author has an hindex of 32, co-authored 62 publications receiving 2752 citations.

Papers
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Journal ArticleDOI

Initial deep LOFAR observations of epoch of reionization windows. I. The north celestial pole

Sarod Yatawatta, +105 more
TL;DR: In this article, the authors present results from observations of the NCP window using the LOFAR highband antenna (HBA) array in the frequency range 115 MHz to 163 MHz.
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Synchronous X-ray and Radio Mode Switches: a Rapid Global Transformation of the Pulsar Magnetosphere

W. Hermsen, +114 more
- 25 Jan 2013 - 
TL;DR: Through simultaneous observations, synchronous switching in the radio and x-ray emission properties of pulsar PSR B0943+10 is detected, indicating rapid, global changes to the conditions in the magnetosphere, which challenge all proposed pulsar emission theories.
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A large light-mass component of cosmic rays at 10 17 –10 17.5 electronvolts from radio observations

Stijn Buitink, +124 more
- 03 Mar 2016 - 
TL;DR: Radio measurements of Xmax with a mean uncertainty of 16 grams per square centimetre for air showers initiated by cosmic rays with energies of 1017–1017.5 electronvolts enable us to determine the mass spectrum of the cosmic rays: a mixed composition, with a light-mass fraction (protons and helium nuclei) of about 80 per cent.
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Detecting cosmic rays with the LOFAR radio telescope

Pim Schellart, +106 more
TL;DR: In this article, the authors describe the dataset, as well as the analysis pipeline, and serve as a reference for future papers based on these data, including removal of radio frequency interference, correcting for the antenna response and identification of the pulsed signal.
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Calibrating high-precision Faraday rotation measurements for LOFAR and the next generation of low-frequency radio telescopes

Carlos Sotomayor-Beltran, +81 more
TL;DR: In this paper, the authors present ionFR, a code that calculates the amount of ionospheric Faraday rotation for a specific epoch, geographic location, and line-of-sight.