- 1INAF- Italian National Institute for Astrophysics, Astrophysical Observatory of Turin, (paola.ardizzone@inaf.it)
- 2University of Turin, Physics Department, Italy
- 3Astronomical Institute, Slovak Academy of Sciences, Slovakia
- 4Konan University, Department of Physics, Japan
- 5Korea Astronomy and Space Science Institute, Republic of Korea
- 6Astronomical Institute, Czech Academy of Sciences, Czech Republic
- 7University of Lodz Doctoral School of Exact and Natural Sciences, Poland
- 8Astrophysics Division, National Centre for Nuclear Research, Poland
- 9National Centre for Nuclear Research, Astrophysics Division, Poland
The DIMS project (Dark matter and Interstellar Meteoroid Study) is an international collaboration with a twofold scientific goal: the search for hypothetical macroscopic dark matter candidates and the study of meteoroids of interstellar origin. To pursue these objectives, DIMS deployed highly sensitive CMOS cameras, that were operated from 2021 to 2025 in central Japan and at the Telescope Array site in Utah.
In this contribution we present the architecture of the pipeline developed for the analysis of DIMS observations of meteor events, that includes custom astrometry and elliptical aperture photometry, together with the adaptation of the PRISMA fireball network pipeline to the DIMS case. We discuss the preliminary results of multi-station triangulation, atmospheric dynamic model, and reconstructions of pre-atmospheric orbits of a selected sample of events. In particular, we focus on the search of interstellar meteor candidates and the assessment of measurement uncertainties.
How to cite: Ardizzone, P. S., Barghini, D., Bertaina, M. E., Gardiol, D., Durisova, S., Hajdukova, M., Kajino, F., Kim, S.-W., Koten, P., Przybylak, M., Shinozaki, K., and Vrabel, M.: Study of Interstellar Meteor Candidates Based on Optical Meteor Observations from the DIMS Project, Europlanet Science Congress 2026, The Hague, The Netherlands, 7–11 Sep 2026, EPSC2026-642, https://doi.org/10.5194/epsc2026-642, 2026.