My interestes lie in supernovae as distance indicators (cosmology), the physics of supernovae (such as explosion mechanism and progenitors), and other stellar transients in general (e.g., kilonovae, tidal disruption events, etc.). I am also interested in machine learning and coding in Python.
I am the developer of the PISCOLA transient light-curve fitter and HostPhot for galaxy photometry, and I am an active member in collaborations such as ePESSTO+, POSIE, ZTF and SAINTS.
Currently, I am a research fellow at Trinity College Dublin (TCD) and previously was a postdoctoral researcher at the Institute of Space Sciences (ICE-CSIC) in Barcelona, Spain. At the moment, my work focuses on using type Ia supernovae with near-infrared data to test the current standard cosmological model as part of the Aarhus-Barcelona Flows project and SAINTS collaboration.
For more information, check my CV.
PhD in Astronomy, 2021
University of Southampton
MSc in Astrophysics, 2017
Pontificia Universidad Católica de Chile
BSc in Astronomy, 2015
Universidad de Chile
Advance coding with Python (pandas, astropy, scikit-learn, etc.) including open-source software development and JOSS referee
Experience with different data-analysis and statistical tools (e.g., Bayesian analysis)
Experience with different Linux distros
Machine and deep learning for regression, outlier detection, classification, etc. Former LSSTC Data Science Fellow
Spanish (native), English (fluent), French (basic) and Catalan (basic)
I love playing the drums, it is one of my hobbies. Checkout my band Time Illusions!
API to download SVO filters
API to access TNS data
API to access WISeREP data
Global and local photometry of galaxies hosting supernovae or other transients
Type Ia supernova light curve fitting code
Type II supernova fitting code
INT-IDS data-reduction pipeline
ePESSTO+ data-reduction pipeline
Pipeline for extracting supernova light curves with TESS data