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Michael 'Misha' Rashkovetskyi

Michael 'Misha' Rashkovetskyi

Areas of Expertise

  • Cosmology
  • Large-scale structure
  • Dark energy
  • Cosmic microwave background
  • Hubble tension

Education

  • Ph.D. Astronomy and Astrophysics, Harvard University, 2025
  • M.A. Astronomy and Astrophysics, Harvard University, 2022
  • B.Sc. Physics, Tel Aviv University, 2020

Dr. Rashkovetskyi started as a CCAPP Postdoctoral Fellow on July 28, 2025. He is currently working on the splitting of the Dark Energy Spectroscopic Instrument (DESI) galaxies based on a thermal Sunyaev-Zeldovich map to extract more information from galaxy clustering. He defended his PhD in May 2025 at Center for Astrophysics | Harvard & Smithsonian with Prof. Daniel Eisenstein. He has developed the covariance matrix pipeline for 2-point correlation functions for DESI 2024 (DR1) and DR2 baryon acoustic oscillations measurements. Earlier, he conducted a follow-up study of small-scale baryon inhomogeneities at recombination time as a possible relief of the Hubble tension.

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