By NelmaS on Dom, 25/02/2018 - 15:21
High resolution NIR spectrographs have played an important role in the detection and characterization of exoplanet atmospheres. Throughout my PhD I have tried two techniques to extract the faint blended spectra of Brown Dwarf companions in CRIRES data. I will present the two techniques attempted, direct subtraction and chi squared synthethic recovery, discuss some of their limitiations and highlight the main reasons for the unsuccessful detections.
27 de fevereiro de 2018 | 13:30
Centro de Astrofísica da Universidade do Porto (Classroom)
Rua das Estrelas, 4150-762 Porto