Transit timing & ephemerides
We refine transit times and ephemerides from space- and ground-based observations, supporting reliable scheduling and long-baseline studies of planetary systems.
We study small signals in noisy scientific data: measuring exoplanet transits, identifying stellar-activity systematics, and building reliable machine-learning and Bayesian workflows that can be tested, reproduced, and reused.
Astronomy supplies the precision-measurement problems; scientific machine learning supplies tools for inference, diagnostics and scale. The group connects the two without treating either the data or the model as a black box.
We refine transit times and ephemerides from space- and ground-based observations, supporting reliable scheduling and long-baseline studies of planetary systems.
We model how starspots and instrumental effects distort measured transit times and depths, then propagate those uncertainties into the scientific result.
We develop interpretable, validation-focused ML and Bayesian methods for time series, imaging and other scientific data where errors have physical meaning.
We contribute to exoplanet atmospheric-characterisation studies and multi-site stellar-occultation campaigns for trans-Neptunian objects.
Funded work is separated from proposals still under evaluation. Roles and funders are drawn from the principal investigator's maintained academic record.
Space- and ground-based photometric time series, timing measurements and public scientific archives.
Python workflows for transit modelling, Bayesian analysis, Gaussian processes, simulation and machine learning.
Version-controlled analysis, documented assumptions, reproducible notebooks and reusable teaching materials.
Generated from NASA ADS and filtered against ORCID and a maintained collision list. See the NASA ADS record for source metadata.
Current (2026–2027, İSTÜN): Physics I & II, Computer Programming I & II, Object-Oriented Programming, Data Structures & Algorithms, Robotics, and Machine Learning—in English and Turkish.
Student work can connect coursework to research through transit light curves, starspot simulations, scientific time-series modelling and reproducible Python pipelines.
Open materials are available through Algorithm Analysis with Python and the full course list.
Ground-based observations and ephemeris refinement in support of ESA's Ariel mission; co-author contributions to ExoClock III and IV.
Participation in international transit-timing work connecting new photometry with long-baseline exoplanet records.
Community work on machine learning in planetary science, including an invited contribution at EPSC-DPS 2025.
Analysis and coordination supporting physical characterisation of trans-Neptunian objects.
International Astronomical Union (IAU), European Astronomical Society (EAS), Turkish Astronomical Society (TAD), and European Association for Astronomy Education (EAAE). Referee for international astronomy and planetary-science journals.
Students at İSTÜN and researchers interested in exoplanet data analysis, transit timing, stellar activity or validation-focused machine learning are welcome to propose a focused project or collaboration.
The principal investigator's appointment is listed in the İSTÜN academic staff directory and Türkiye's YÖKSİS registry. Publications are linked through ORCID, NASA ADS and DOI records.