Preliminary strawman schedule, to be adjusted as needed
Signal Prediction - ModelingTG1
What's going on in the supernova to make the neutrinos we will see?
Convenors: Evan O'Connor, Jim Kneller
Signal Prediction - Pre-supernovaTG2
What would neutrinos cooling the core of a pre-SN star look like?
Convenors: Cecilia Lunardini, Andrey Sheshukov
Signal Prediction - Detector ResponseTG3
Given a neutrino flux, how to get that modeled in the detectors participating in SNEWS?
Convenors: Segev BenZvi
Alert Formation - ImplementationTG4
The communications between experiments and SNEWS, and how SNEWS itself is built do to the job.
Convenor: Alec Habig
Alert Formation - Triangulation and PointingTG5
What can SNEWS do to point back on the sky to the source of the neutrinos?
Convenors: Kate Scholberg, Jeff Tseng
Alert Formation - Fire DrillsTG6
How can we practice doing all this stuff?
Convenor: Erin O'Sullivan
Follow-up: Multi- Messenger Follow-UpTG7
Coordinating the SN followup with things other than neutrinos
Convenor: Danny Milisavljevic
Follow-up: Outreach & CommunicationTG8
Making sure the wider community knows what we're up to.
Convenor: Justin Vasel
Logistics of operating SNEWS