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SUMMARY:Linking the low surface brightness Universe and galactic growth - 
 Elisabeth Sola / IoA
DTSTART:20241204T134000Z
DTEND:20241204T140500Z
UID:TALK225223@talks.cam.ac.uk
CONTACT:Xander Byrne
DESCRIPTION:In hierarchical models of galaxy formation and evolution\, gal
 axies grow through gas accretion and merger events. The tidal debris produ
 ced during these mergers serves as a fossil record of a galaxy’s assembl
 y history\, with characteristics that depend on the nature of the merger. 
 Exploring these faint Low Surface Brightness (LSB) structures around galax
 ies of varying masses and environments is essential to fully understanding
  galactic evolution. Advances in dedicated instruments and data reduction 
 pipelines from past\, ongoing\, and future surveys have significantly expa
 nded our ability to explore the LSB Universe.\nIn this talk\, I will discu
 ss how LSB features can be leveraged to investigate galactic growth\, usin
 g deep imaging data from the Canada-France-Hawaii Telescope (CFHT) and ESA
 ’s Euclid space telescope\, combined with an innovative online annotatio
 n tool.
LOCATION:The Hoyle Lecture Theatre + Zoom 
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