Title: Stellar population studies in the J-PAS survey
Abstract: The Javalambre Physics of the Accelerating Universe Astrophysical Survey (J-PAS) is a large scale multi-filter survey that has started to observe 8500 deg² of the northern sky with 54 narrow-band filters in the optical range (3500-9600Å). In our Galaxy Evolution group at IAA-CSIC, we aimed at developing and testing methodologies in order to perform stellar populations studies using this kind of data. More precisely, Luis introduced our SED-fitting codes and the potential of J-PAS to determine the integrated properties of the stellar content of galaxies up to redshift z~1 (including age, metallicity, stellar mass, etc.), techniques for the determination of the stellar mass and luminosity functions of galaxies in this kind of surveys, and how to constrain the stellar population properties of spatially resolved galaxies up to 2-3 half light radius only using the miniJPAS/J-PAS images by means of a tool that we are developing in our group (IFU-like studies).
Rosa, Rubén and Julio the Course on gender analysis in research, held online at the IAA. Organized by the equality commission of the IAA-CSIC, and is set up with the aim of achieving three different objectives.
Paper presentation by Rosa on our recent work on the JPAS seminars on June 22th, 2020: The miniJPAS survey: Paving the way to characterizing galaxy populations in J-PAS with 56 colors
Gines & Julio attend the 1st IAA-CSIC Severo Ochoa School on Statistics, Data Mining and Machine Learning
Ginés and Julio attended the 1st IAA-CSIC Severo Ochoa School on Statistics, Data Mining and Machine Learning, held at the IAA from 4th to 7th of November 2019.