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researcher

S. Schuh

110 papers hereh-index 369k citations373 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • sole author2
  • first author9
  • middle author24
  • last author6

Across the 41 of 110 papers where every author was matched, so the position is known.

fields
  • hep-ex68
  • astro-ph25
  • astro-ph.SR10
  • astro-ph.EP5
  • physics.ins-det2
same name
  • S. Schuh — 30 papers
  • S. Schuh — 6 papers, h 2
  • S. Schuh — 3 papers, h 4
  • S. Schuh — 2 papers
  • S. Schuh — 1 paper
  • S. Schuh — 1 paper

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

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
Showing 2012Show all

3 papers · 1 filter

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…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.