LabCompass

M. Rashkovetskyi

Physics and Astronomy · The Ohio State University

Early career · publishing since 2017Rising activity

Publications

48

Citations

3,718

Est. group size

~9

Recurring co-author estimate

Active years

10

Publishing since 2017

Research summary
AI-generated

M. Rashkovetskyi works in astrophysics and cosmology, with research spanning pulsar behavior (rotating neutron stars that emit beams of radio waves) and large-scale cosmological analyses such as galaxy correlation functions and the Hubble tension (a discrepancy in measurements of how fast the universe is expanding). Recent work focuses heavily on statistical methods for analyzing large galaxy survey data, particularly from the DESI (Dark Energy Spectroscopic Instrument) project. This research would suit students interested in both observational cosmology and statistical/computational methods for analyzing astronomical survey data.

Pulsar astrophysicsCosmological large-scale structureGalaxy survey statistics (DESI)Hubble tension and cosmological parametersRadio astronomy

Publication output was sparse and irregular from 2017-2022 but has grown sharply since 2023, with a large increase in output through 2024-2025.

Generated by claude-sonnet-5 from public bibliographic data · Jul 20, 2026

Publication cadence
Publications per year over the last 10 years — averaging 8.8/year recently
2017: 2 publications172018: 1 publication18192020: 1 publication202021: 1 publication21222023: 5 publications232024: 8 publications242025: 25 publications25252026: 6 publications26
Recent publications
Publishes in
  • Journal of Cosmology and Astroparticle Physics×18
  • arXiv (Cornell University)×13
  • Physical review. D/Physical review. D.×6
  • Monthly Notices of the Royal Astronomical Society×4
  • The Astronomical Journal×3
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This profile was generated automatically from public scholarly data (OpenAlex). Group size and activity levels are estimates derived from co-authorship patterns.

Last updated Jul 19, 2026.

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