Chairs: Garreth Martin, Aritra Ghosh, Burcin Mutlu-Pakdil, Marc Huertas-Company

This session will focus on galaxy morphology and low surface brightness (LSB) features (e.g., tidal streams, tails). 

The imaging quality that LSST will deliver will provide significantly more morphological and LSB information for a far greater number of objects than any previous large survey. The goal of this session is to hear from researchers in the field about how they're preparing to model/classify galaxy/LSB features in the big data era of the LSST.

Please contact the session chair with any questions, or if you'd like to volunteer to speak or help with this session.

Contributed talks:

• Tracing the environmental dependence of low surface brightness galaxy properties (Unnikrishnan Sureshkumar) - 10:30~10:44

• A comparison of observable and simulated intracluster light fractions (Sarah Brough) - 10:44~10:58

• Galactic Cirrus in Deep Optical Observations (Aleksandr Mosenkov, remote) - 10:58~11:12

• Confirmation of Dwarf Stellar Halos Built by Accretion at the dwarf galaxy scale (Catherine Fielder, remote) - 11:12~11:26

• Tracing the intra-halo light with deep Hyper Suprime-Cam images (Lucia Paz Garate Nunez, remote) - 11:26~11:40

• Morphology data challenge discussion - 11:40 ~ 12:00