1 citations · 1 across the 1 of their papers we have counts for
4 papers
LEADER: fast estimates of asteroid shape elongation and spin latitude distributions from scarce photometry
Hari Nortunen, Mikko Kaasalainen
Many asteroid databases with lightcurve brightness measurements (e.g. WISE, Pan-STARRS1) contain enormous amounts of data for asteroid shape and spin modelling. While lightcurve in…
Distribution of shape elongations of main belt asteroids derived from Pan-STARRS1 photometry
H. Cibulková, H. Nortunen, J. Ďurech +10
Context. A lot of photometric data is produced by surveys such as Pan-STARRS, LONEOS, WISE or Catalina. These data are a rich source of information about the physical properties of…
Shape and spin distributions of asteroid populations from brightness variation estimates and large databases
H. Nortunen, M. Kaasalainen, J. Ďurech +3
Context. Many databases on asteroid brightnesses (e.g. ALCDEF, WISE) are potential sources for extensive asteroid shape and spin modelling. Individual lightcurve inversion models r…
Shape and spin distributions of large object populations from random projection areas
Hari Nortunen, Mikko Kaasalainen
We model the shape and spin characteristics of an object population when there are not enough data to model its single members. The data are random projection areas of the members.…