activity
19962018
most citedStudy of Exclusive Radiative B Meson Decays

134 citations · 2.6k across the 110 of their papers we have counts for

collaborators

110 papers

physics.ins-det2018★ 2 cited

Feasibility Study for BioLEIR

S. Ghithan, G. Roy, S. Schuh

The biomedical community asked CERN to investigate the possibility to transform the Low Energy Ion Ring (LEIR) accelerator into a multidisciplinary, biomedical research facility (B…

astro-ph.EP2014★ 47 cited

Kepler detection of a new extreme planetary system orbiting the subdwarf-B pulsator KIC10001893

R. Silvotti, S. Charpinet, E. Green +7

KIC10001893 is one out of 19 subdwarf-B (sdB) pulsators observed by the Kepler spacecraft in its primary mission. In addition to tens of pulsation frequencies in the g-mode domain,…

astro-ph.EP2013★ 26 cited

EXOTIME: searching for planets and measuring Pdot in sdB pulsators

Ronny Lutz, Sonja Schuh, Roberto Silvotti

We review the status of the EXOTIME project (EXOplanet search with the TIming MEthod). The two main goals of EXOTIME are to search for sub-stellar companions to sdB stars in wide o…

astro-ph.SR2012★ 1 cited

Acoustic and buoyancy modes throughout stellar evolution - Seismic properties of stars at different stellar ages and masses

Sonja Schuh

Parameter regions in which stars can become pulsationally unstable are found throughout the Hertzsprung-Russel diagram. Stars of high, intermediate, low and very low masses may cro…

astro-ph.SR2012★ 6 cited

Chandra grating spectroscopy of three hot white dwarfs

J. Adamczak, K. Werner, T. Rauch +3

High-resolution soft X-ray spectroscopic observations of single hot white dwarfs are scarce. With the Chandra Low-Energy Transmission Grating, we have observed two white dwarfs, on…

astro-ph.SR2012

Amplitude variation and multiplet structures: Is PG1605+072 a slow rotator?

Jan Langfellner, Sonja Schuh, the MSST +1

The subdwarf B star PG1605+072, with an unusually low log g ~ 5.3, shows a high number of non-radial pulsation modes, making it a promising candidate for asteroseismology. This cou…