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M. Skarka

86 papers hereh-index 181.1k citations149 works total

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

author position
  • sole author3
  • first author12
  • middle author50
  • last author8

Across the 73 of 86 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR54
  • astro-ph.EP22
  • astro-ph.IM7
  • astro-ph.GA2
  • astro-ph.HE1
same name
  • M. Skarka — 11 papers

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
20122026
most citedThe first view of δ Scuti and γ Doradus stars with the TESS mission

125 citations · 1.3k across the 85 of their papers we have counts for

collaborators
Showing 2014Show all

4 papers · 1 filter

astro-ph.SR2014★ 50 cited

Apsidal motion and light a curve solution for eighteen SMC eccentric eclipsing binaries

P. Zasche, M. Wolf, J. Vrastil +3

Aims: The Danish 1.54-meter telescope at the La Silla observatory was used for photometric monitoring of selected eccentric eclipsing binaries located in the Small Magellanic Cloud…

astro-ph.SR2014★ 15 cited

Characteristics of bright ab-type RR Lyrae stars from the ASAS and WASP surveys

Marek Skarka

In this article, we present results based on high-density, high-precision Wide-Angle Search for Planets (WASP) light curves supplemented with lower-precision photometry from the Al…

astro-ph.SR2014★ 6 cited

Photometric study of the star with changing Blazhko effect: TV~Bootis

M. Skarka, M. Zejda

This study investigates periodic modulation of the light curve of the RRc star TV Boo and its physical parameters based on photometric data. This phenomenon, known as Blazhko effec…

astro-ph.SR2014★ 30 cited

Bright Blazhko RRab Lyrae stars observed by ASAS and the SuperWASP surveys

Marek Skarka

Period study of 321 fundamental mode galactic field RR Lyrae type stars (RRab), which had appropriate data in ASAS and SuperWASP surveys, brighter than 12.5 mag in maximum light wa…

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