A study of occultation-derived diameters and albedos of TNOs in comparison with those from other techniques

Tesis del Departamento de Sistema Solar, Instituto de Astrofísica de Andalucía. Universidad de Granada. Programa de doctorado en Física y Ciencias Espaciales. Leída en el Salón de Grados de la Facultad de Ciencias, el 25 de noviembre del 2025, a las 11:00 h.-- This thesis is partly based on observations collected at the Centro Astronómico Hispano en Andalucía (CAHA) at Calar Alto, operated jointly by Junta de Andalucía and Consejo Superior de Investigaciones Científicas (CSIC). This research is also partially based on observations carried out at the Observatorio de Sierra Nevada (OSN) operated by Instituto de Astrofísica de Andalucía (IAA-CSIC) and on observations made with the Liverpool Telescope (LT) at the Roque de los Muchachos Observatory (ORM) on the island of La Palma as part of the Observatorios de Canarias (OCAN) operated by the Instituto de Astrofísica de Canarias (IAC). This work has made use of data from the European Space Agency (ESA) Gaia mission (Gaia Collaboration et al., 2023), processed by the Gaia Data Processing and Analysis Consortium (DPAC). Funding for the DPAC has been provided by national institutions, in particular the institutions participating in the Gaia Multilateral Agreement. The contributions of (both amateur and professional) occultation observers and data collectors/validators is also acknowledged. Thank you!