Welcome

I have worked on and studied cosmology from 2005 to 2019 at: the Physics Institute of the University of Sao Paulo (IF-USP); the Astronomy Institute of the University of Sao Paulo (IAG-USP); the Department of Physics & Astronomy of University College London (UCL); and at the Department of Physics & Astronomy of the University of Pennsylvania (Upenn). I have worked on the J-PAS project and also developed the FLASK code for simulating large-scale-structure observables.

  • Power-spectrum estimator optimization

    Using realistic simulations and including sistematic effects, I intend to test different methods of estimating the matter power-spectrum from galaxy surveys and optimize it for the largest-scales and for the upcoming surveys such as SuMIRe, J-PAS and Euclid.

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  • FLASK

    The Full-sky Lognormal Astro-fields Simulations Kit is a public code created by me that quickly generates full-sky lognormal or Gaussian realizations of multiple correlated large-scale structure fields. It can be used to estimate covariance matrices, test analysis and verify systematic effects.

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  • The J-PAS project

    The Javalambre Physics of the accelerating universe Astrophysical Survey is a project by Spain and Brazil whose main objective is to measure the expansion rate of the Universe through the Baryon Acoustic Oscillations scale imprinted in the galaxy distribution.

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