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J. Ridder

34 papers hereh-index 5918k citations272 works total

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

author position
  • first author1
  • middle author19
  • last author1

Across the 21 of 34 papers where every author was matched, so the position is known.

fields
  • astro-ph11
  • astro-ph.SR11
  • astro-ph.IM6
  • astro-ph.GA4
  • astro-ph.EP2
same name
  • J. Ridder — 3 papers, h 5
  • J. Ridder — 1 paper, h 3
  • J. Ridder — 1 paper, h 2

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
20022026
most citedGaia Data Release 2: Mapping the Milky Way disc kinematics

423 citations · 1.9k across the 33 of their papers we have counts for

collaborators
Showing 2005 · astro-phShow all

3 papers · 2 filters

astro-ph2005★ 14 cited

Multiperiodicity in the large-amplitude rapidly-rotating βCeph ei star HD 203664

C. Aerts, P. De Cat, J. De Ridder +4

We perform a seismic study of the young massive βCephei star HD 203664 with the goal to constrain its interior structure. Our study is based on a time series of 328 new Geneva 7-…

astro-ph2005

Estimating stellar oscillation-related parameters and their uncertainties with the moment method

Joris De Ridder, Geert Molenberghs, Conny Aerts

The moment method is a well known mode identification technique in asteroseismology (where `mode' is to be understood in an astronomical rather than in a statistical sense), which…

astro-ph2005★ 100 cited

Asteroseismology of the Beta Cephei star 12 (DD) Lacertae: photometric observations, pulsational frequency analysis and mode identification

G. Handler, M. Jerzykiewicz, E. Rodriguez +28

We report a multisite photometric campaign for the Beta Cephei star 12 Lacertae. 750 hours of high-quality differential photoelectric Stromgren, Johnson and Geneva time-series phot…

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