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researcher

W. Weiss

4 papers hereh-index 344 citations9 works total

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

author position
  • middle author2
  • last author1

Across the 3 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph2
  • astro-ph.SR2
same name
  • W. Weiss — 112 papers, h 49
  • W. Weiss — 9 papers, h 13
  • W. Weiss — 5 papers, h 7
  • W. Weiss — 3 papers, h 2
  • W. Weiss — 2 papers, h 3
  • W. Weiss — 1 paper, h 28

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
19982023
most citedGAUDI: a preparatory archive for the COROT mission

39 citations · 42 across the 4 of their papers we have counts for

collaborators

4 papers

astro-ph.SR2023★ 1 cited

Catalogue of BRITE-Constellation targets I. Fields 1 to 14 (November 2013 - April 2016)

K. Zwintz, A. Pigulski, R. Kuschnig +25

The BRIght Target Explorer (BRITE) mission collects photometric time series in two passbands aiming to investigate stellar structure and evolution. Since their launches in the year…

astro-ph.SR2020★ 2 cited

The BRITE-SONG of Aldebaran -- Stellar Music in three voices

P. G. Beck, R. Kuschnig, G. Houdek +20

Solar-like oscillations in red-giant stars are now commonly detected in thousands of stars with space telescopes such as the NASA Kepler mission. Parallel radial velocity and photo…

astro-ph2004★ 39 cited

GAUDI: a preparatory archive for the COROT mission

E. Solano, C. Catala, R. Garrido +34

The GAUDI database (Ground-based Asteroseismology Uniform Database Interface, http://sdc.laeff.esa.es/gaudi/) is a preparatory archive for the COROT (COnvection, ROtation and plane…

astro-ph1998

Multi-Element Doppler Imaging of the Ap star epsilon Ursae Majoris

T. Lueftinger, R. Kuschnig, W. W. Weiss

The surface distribution of five elements: iron, chromium, titanium, magnesium and manganese on the magnetic A0pCr star epsilon UMa, have been calculated using the Doppler imaging…

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