Galaxy truncations or ''edges'' are used as a tracer of size in the Fornax Cluster environment and compared with field measurements from the literature.
Contacts: Nushkia Chamba (nushkia.chamba@astro.su.se or on the LSST Slack)
Time: Morning (9 am PT)
Main communication channel: Slack #desc-dkm-lsb-galaxies
GitHub repo: N/A
In-person/Virtual/Hybrid: Virtual
Zoom room (if applicable): https://stanford.zoom.us/j/94814361452?pwd=UEpxTVFlVXY4QWJ0MHZmOSt4MXZTQT09
Goals and deliverable
Writing text for the paper and discussing main results for interpretation and analysis. Potentially making a new plot.
Resources and skills needed
Interest in low surface brightness galaxies, dwarfs, dark matter. Experts in large scale structure, cluster or related fields are very welcome!
The environmental impact on galaxy edges
Galaxy truncations or ''edges'' are used as a tracer of size in the Fornax Cluster environment and compared with field measurements from the literature.
Contacts: Nushkia Chamba (nushkia.chamba@astro.su.se or on the LSST Slack) Time: Morning (9 am PT) Main communication channel: Slack #desc-dkm-lsb-galaxies GitHub repo: N/A In-person/Virtual/Hybrid: Virtual Zoom room (if applicable): https://stanford.zoom.us/j/94814361452?pwd=UEpxTVFlVXY4QWJ0MHZmOSt4MXZTQT09
Goals and deliverable
Writing text for the paper and discussing main results for interpretation and analysis. Potentially making a new plot.
Resources and skills needed
Interest in low surface brightness galaxies, dwarfs, dark matter. Experts in large scale structure, cluster or related fields are very welcome!
Detailed description
DESC Project description on confluence: https://confluence.slac.stanford.edu/x/iuE7Eg