Asteroid phase-curves from Gaia-calibrated data
Abstract
We use asteroid differential photometry gathered in the past decades together with the Gaia stellar catalogue (as photometric standards) to obtain relative magnitudes. The obtained magnitudes are then used to fit the multi-opposition phase curves in several ways depending on data quality.
- Publication:
-
European Planetary Science Congress
- Pub Date:
- September 2017
- Bibcode:
- 2017EPSC...11..743O