19–20 Jun 2020
Zoom
US/Central timezone

Scientific Programme

Preliminary strawman schedule, to be adjusted as needed

  • Signal Prediction - Modeling

    TG1

    What's going on in the supernova to make the neutrinos we will see?

    Convenors: Evan O'Connor, Jim Kneller

  • Signal Prediction - Pre-supernova

    TG2

    What would neutrinos cooling the core of a pre-SN star look like?
    Convenors: Cecilia Lunardini, Andrey Sheshukov

  • Signal Prediction - Detector Response

    TG3

    Given a neutrino flux, how to get that modeled in the detectors participating in SNEWS?
    Convenors: Segev BenZvi

  • Alert Formation - Implementation

    TG4

    The communications between experiments and SNEWS, and how SNEWS itself is built do to the job.
    Convenor: Alec Habig

  • Alert Formation - Triangulation and Pointing

    TG5

    What can SNEWS do to point back on the sky to the source of the neutrinos?
    Convenors: Kate Scholberg, Jeff Tseng

  • Alert Formation - Fire Drills

    TG6

    How can we practice doing all this stuff?

    Convenor: Erin O'Sullivan

  • Follow-up: Multi- Messenger Follow-Up

    TG7

    Coordinating the SN followup with things other than neutrinos
    Convenor: Danny Milisavljevic

  • Follow-up: Outreach & Communication

    TG8

    Making sure the wider community knows what we're up to.
    Convenor: Justin Vasel

  • Governance

    TG9

    Logistics of operating SNEWS