TauREx 2D: Modelling 2D effects in retrievals
<div data-canvas-width="636.8035259153738">New-generation spectrographs dedicated to the study of exoplanetary atmospheres, require a higher precision in the atmospheric</div> <div data-canvas-width="636.8035259153735">models to better interpret the new spectra. Thanks to future space missions like JWST, ARIEL and Twinkle, indeed, the observed</div> <div data-canvas-width="636.8035259153738">spectra will be precise enough to reveal features which cannot be modeled with a one-dimensional plane parallel atmosphere,</div> <div data-canvas-width="636.8035259153739">especially in the case of Ultra Hot Jupiters. Bayesian frameworks are computationally intensive and prevent us from using complete</div> <div data-canvas-width="636.803525915374">three-dimensional self-consistent models to retrieve an exoplanetary atmosphere, and, they constrain us to use simplified models to</div> <div data-canvas-width="636.8035259153739">converge to a set of atmospheric parameters. We propose the TauREx2D retrieval code, which uses two-dimensional atmospheric</div> <div data-canvas-width="636.8035259153738">models as a good compromise between computational power and model precision to better infer exoplanetary atmospheres. Finally,</div> <div data-canvas-width="636.8035259153736">we apply such a model on synthetic spectrum computed from a GCM simulation of WASP121b and show the parameters retrieved by</div> <div data-canvas-width="167.95345291125463">the new TauREx 2D retrieval code.</div>