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M. K. Szyma'nski

3 papers hereh-index 211 citations4 works total

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

author position
  • middle author3

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

fields
  • astro-ph.SR2
  • astro-ph.GA1
same name
  • M. K. Szyma'nski — 5 papers, h 1
  • M. K. Szyma'nski — 5 papers, 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

most citedThe OGLE Collection of Variable Stars: Over 18 000 Rotating Variables toward the Galactic Bulge

1 citations · 1 across the 2 of their papers we have counts for

collaborators

3 papers

astro-ph.SR2024

Millinovae: A New Class of Transient Supersoft X-ray Sources without a Classical Nova Eruption

Przemek Mróz, Krzysztof Król, Hélène Szegedi +18

Some accreting binary systems containing a white dwarf (such as classical novae or persistent supersoft sources) are seen to emit low-energy X-rays with temperatures of ~10^6 K and…

astro-ph.GA2024

Analysis of the full Spitzer microlensing sample I: Dark remnant candidates and Gaia predictions

Krzysztof A. Rybicki, Yossi Shvartzvald, Jennifer C. Yee +70

In the pursuit of understanding the population of stellar remnants within the Milky Way, we analyze the sample of ∼950 microlensing events observed by the Spitzer Space Teles…

astro-ph.SR2024★ 1 cited

The OGLE Collection of Variable Stars: Over 18 000 Rotating Variables toward the Galactic Bulge

P. Iwanek, I. Soszyński, K. Stępień +14

Stellar rotation, a key factor influencing stellar structure and evolution, also drives magnetic activity, which is manifested as spots or flares on stellar surface. Here, we prese…

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