Description
With high-quality data and a large sample from Euclid, providing powerful statistical insights, this project aims to quantify how the fraction of dust-obscured star formation varies with stellar mass and evolves over cosmic time. Dust plays a crucial role in the evolution of massive galaxies, strongly correlating with stellar mass and affecting our ability to trace star formation history. Using Euclid deep field catalogs, integrated with other multi-wavelength datasets, we will derive stellar masses, star formation rates, and dust obscuration through multiple indicators, including optical colors, infrared luminosity ratios, and spectral energy distribution (SED) fitting.
| Talk category | NOVA Network 1 |
|---|---|
| Preference for a talk or poster | Poster |
Primary authors
Sara Tacchetto
Prof.
Lingyu Wang
