A short overview of the work of the Euclid Consortium Diversity Committee
The presentation describes the main aspects of the electronic unit that controls the infrared instrument on board the Euclid space telescope, which the Polytechnic University of Cartagena is responsible for, in collaboration with the Institute of Astrophysics of the Canary Islands.
The talk describes the work of the “Barcelona Team” in the Filter Wheel Assembly of the NISP Instrument.
During this talk, I will briefly describe the characteristics and main contributions of the Spanish Science Data Center.
The Spanish teams at the University of Barcelona and Universidade da Coruña working in the Gaia Data Processing and Analysis Consortium are also contributing to the Euclid mission. The tasks they are contributing related to Euclid instrumentation include the evaluation of the NISP filters cut-on and cut-off limits, and obtaining the spectral energy distribution for some sources to be used to...
In this talk I will review the main simulations (Flagship) that have been produced to prepare the Euclid mission.
The observations of clusters of galaxies with Euclid is fundamental to achieve the major goals of this mission. I will give an overview of the major aims of the Science Working Group „Clusters of Galaxies“. Both I will present science cases directly related to the major goals of Euclid and projects/ideas related to legacy science.
In this talk we briefly review the strong lensing science to be done with Euclid
I will briefly review the different galaxy formation related science cases that Euclid will address, with a special focus on galaxy morphology
The Local Universe Science Working Group (LU-SWG) is the Euclid consortium's team that works in galaxy evolution in the nearby Universe (z < 0.3). Euclid will provide an unmatched view of these objects considering our combination of spatial resolution, sky coverage and photometric depth. Remarkably, we also have the power of transforming the survey removing nuisances such us different sky...
We as the Euclid ILS team, hereby present our preliminary results of one of the Euclid ERO programme, probing the young free-floating planets in the hotbed of the sigma Orionis cluster. We used known, spectroscopically-confirmed substellar benchmarks to proceed with high-purity selection for new members in the Euclid catalogue and we were able to probe down to objects with 4 Jovian masses. The...
