16:30 Break up into four sub-groups based on following topics:
What families of progenitor models are excluded?
What is the FRB emission mechanism
Are there multiple populations of FRBs
(How) does the DM distribution relate to the FRB distance scale?
17:45 Panel discussion
Here, a representative from each of the discussions will be on the panel
plus a moderator their job is to summarize the essential elements from
the discussions. We'll then have a large-group follow-up discussion on
these points. As a goal for ourselves, let's record action
items from each discussion.
16:30 Small Group Breakouts #2:
What are DM/RM/tsc telling us about IGM and/or local FRB environments?
What biases are there in the FRB sample?
Will FRBs be good cosmological probes?
What other astrophysics can we do with FRBs?