White dwarf planetary system variability and architecture
Lead Research Organisation:
University College London
Department Name: Physics and Astronomy
Abstract
Student will use existing data to constrain light curve transit and stellar variability in polluted white dwarf systems, and explore multi-wavelength observations for other indicators of dynamical interactions and planetary architecture. Projects will be based purely on observational data including but not limited to, high-cadence photometry, space-based photometry, optical spectroscopy, and infrared photometry.
Organisations
People |
ORCID iD |
| Jay Farihi (Primary Supervisor) | |
| Robert Akshay (Student) |
Studentship Projects
| Project Reference | Relationship | Related To | Start | End | Student Name |
|---|---|---|---|---|---|
| ST/V507167/1 | 01/10/2020 | 30/09/2024 | |||
| 2733522 | Studentship | ST/V507167/1 | 01/10/2022 | 31/03/2026 | Robert Akshay |
| ST/W50788X/1 | 01/10/2021 | 30/09/2025 | |||
| 2733522 | Studentship | ST/W50788X/1 | 01/10/2022 | 31/03/2026 | Robert Akshay |