Data: 31.03.2016

Palestrante: Dr. Rita Tojeiro (St. Andrews)

Link: https://youtu.be/33LrscNfMkk

Resumo: The great era of massive galaxy spectroscopic surveys has opened many doors across galaxy evolution and observational cosmology studies. Accurate three-dimensional positions of millions of galaxies allow us to map the large-scale structure and expansion history of the Universe. In parallel, galaxy spectra allow us to infer many physical properties of galaxies, including their time-resolved star-formation histories. In this webinar I will show how combining these two probes – the large-scale structure and time-resolved star-formation histories – offers a unique perspective in helping us answer a variety of questions, from the growth rate of structure to halo assembly bias.