1 code implementation • 6 Jul 2022 • Mario Morvan, Nikolaos Nikolaou, Kai Hou Yip, Ingo Waldmann
Astrophysical light curves are particularly challenging data objects due to the intensity and variety of noise contaminating them.
no code implementations • 8 Sep 2021 • Mahed Abroshan, Kai Hou Yip, Cem Tekin, Mihaela van der Schaar
Secondly, such datasets are usually imperfect, additionally cursed with missing values in the attributes of features.
1 code implementation • 23 Nov 2020 • Kai Hou Yip, Quentin Changeat, Nikolaos Nikolaou, Mario Morvan, Billy Edwards, Ingo P. Waldmann, Giovanna Tinetti
We then present an extensive analysis of the predictions of DNNs, which can inform us - among other things - of the credibility limits for atmospheric parameters for a given instrument and model.
no code implementations • 29 Oct 2020 • Nikolaos Nikolaou, Ingo P. Waldmann, Angelos Tsiaras, Mario Morvan, Billy Edwards, Kai Hou Yip, Giovanna Tinetti, Subhajit Sarkar, James M. Dawson, Vadim Borisov, Gjergji Kasneci, Matej Petkovic, Tomaz Stepisnik, Tarek Al-Ubaidi, Rachel Louise Bailey, Michael Granitzer, Sahib Julka, Roman Kern, Patrick Ofner, Stefan Wagner, Lukas Heppe, Mirko Bunse, Katharina Morik
For instance, the most prolific method for detecting exoplanets and inferring several of their characteristics, transit photometry, is very sensitive to the presence of stellar spots.
no code implementations • 12 Apr 2019 • Kai Hou Yip, Nikolaos Nikolaou, Piero Coronica, Angelos Tsiaras, Billy Edwards, Quentin Changeat, Mario Morvan, Beth Biller, Sasha Hinkley, Jeffrey Salmond, Matthew Archer, Paul Sumption, Elodie Choquet, Remi Soummer, Laurent Pueyo, Ingo P. Waldmann
Further advances in exoplanet detection and characterisation require sampling a diverse population of extrasolar planets.
Earth and Planetary Astrophysics Instrumentation and Methods for Astrophysics