activity
20032014
most citedThe spectral evolution of impulsive solar X-ray flares

157 citations · 506 across the 8 of their papers we have counts for

collaborators

8 papers

astro-ph.HE2014★ 15 cited

Short-duration Radio Bursts with Apparent Extragalactic Dispersion

Pascal Saint-Hilaire, Arnold O. Benz, Christian Monstein

We present the results of the longest yet undertaken search for apparently extragalactic radio bursts at the Bleien Radio Observatory covering 21000 hours (898 days). The data were…

astro-ph.GA2012★ 24 cited

Submillimeter Line Emission from LMC 30Dor: The Impact of a Starburst on a Low Metallicity Environment

Jorge L. Pineda, Norikazu Mizuno, Markus Roellig +4

(Abridged) The 30 Dor region in the Large Magellanic Cloud (LMC) is the most vigorous star-forming region in the Local Group. Star formation in this region is taking place in low-m…

astro-ph.GA2010★ 101 cited

Herschel/HIFI discovery of interstellar chloronium (HCl)

D. C. Lis, J. C. Pearson, D. A. Neufeld +102

We report the first detection of chloronium, HCl, in the interstellar medium, using the HIFI instrument aboard the \emph{Herschel} Space Observatory. The li…

astro-ph2005★ 68 cited

A broadband FFT spectrometer for radio and millimeter astronomy

Arnold O. Benz, Paolo C. Grigis, V. Hungerbuhler +4

The core architecture, tests in the lab and first results of a Fast Fourier Transform (FFT) spectrometer are described. It is based on a commercially available fast digital sampler…

astro-ph2005★ 97 cited

Size dependence of solar X-ray flare properties

Marina Battaglia, Paolo C. Grigis, Arnold O. Benz

Non-thermal and thermal parameters of 85 solar flares of GOES class B1 to M6 (background subtracted classes A1 to M6) have been compared to each other. The hard X-ray flux has been…

astro-ph2005★ 35 cited

The spectral evolution of impulsive solar X-ray flares. II.Comparison of observations with models

Paolo C. Grigis, Arnold O. Benz

We study the evolution of the spectral index and the normalization (flux) of the non-thermal component of the electron spectra observed by RHESSI during 24 solar hard X-ray flares.…