• Large scale structure of the Universe – galaxy filaments and the properties of various astrophysical sources in relation to them.

    • The filament network should be connected, i.e., loose ends and lone filamentary scraps should be rare or even nonexistent. We achieved this [1] by morphological transformations of celestial projections within an image analysis framework.

    Continuous galaxy filament network
    1. Continuous Filament Network of the Local Universe
      A. Tugay & M. Tarnopolski
      Astrophysical Journal, 952, 3, 14 pp., 2023 (Open Access)
      PDF   NASA ADS logo ADS

  • Ultra-high energy cosmic rays (UHECRs) and ultra-high energy neutrinos (UHEν) – in particular, the connection between UHEν and GRBs, blazars and matter distribution.

  • Solar variability – in particular, the statistics and forecasting of the sunspot number (SSN).

© 2022–, Mariusz Tarnopolski
Sources of figures