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SNEWS Meeting @ Neutrino2020

19–20 Jun 2020
Zoom
US/Central timezone

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Contribution List

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  1. 3. Manibrata Sen
    Manibrata Sen
    19/06/2020, 07:00
  2. 4. Laurie Walk
    Dr Walk Laurie
    19/06/2020, 07:20
  3. 5. Tommy Lam
    Tommy Lam (Virginia Tech)
    19/06/2020, 07:40
  4. 15. Pointing with presupernova neutrinos
    Cecilia Lunardini (Arizona State University)
    19/06/2020, 08:15
  5. 16. Shape analysis and combination of presupernova signals
    Andrey Sheshukov (JINR)
    19/06/2020, 08:35
  6. 17. Pre-supernova neutrino alert with SNO+
    Janet Rumleskie (Laurentian University)
    19/06/2020, 08:55
  7. 29. Overview
    Segev BenZvi (University of Rochester)
    19/06/2020, 09:30
  8. 22. Sensitivity of KM3Net to CCSNe: Online and Offline Performance
    Massimiliano Lincetto, marta colomer (km3net)
    19/06/2020, 09:36
  9. 24. Sensitivity of RES-NOVA to supernova neutrinos
    Luca Maria Pattavina (INFN - National Institute for Nuclear Physics)
    19/06/2020, 09:54
  10. 25. Sensitivity of LZ to supernova neutrinos
    Elise McCarthy (University of Rochester)
    19/06/2020, 10:12
  11. 19. Scimma and Hopskotch
    Amanda Depoian (Purdue University), Skylar(Yiyang) Xu (Rice Univeristy)
    19/06/2020, 10:40
  12. 20. Signifcance-based Alerts
    Andrey Sheshukov (JINR)
    19/06/2020, 11:00
  13. 7. Introduction to session
    Jeffrey Tseng (University of Oxford (GB))
    20/06/2020, 07:00
  14. 8. Pointing based on anisotropic interactions
    Kate Scholberg (Duke University)
    20/06/2020, 07:05
  15. 9. Pointing confidence area estimation
    Dr Vladimir Kulikovskiy (INFN Genova), marta colomer (km3net)
    20/06/2020, 07:15
  16. 10. Time measurements from individual experiments
    Clarence Virtue (Laurentian University)
    20/06/2020, 07:30
  17. 11. Pointing with shape information
    Jia-Shian Wang (University of Hong Kong (HK))
    20/06/2020, 07:40
  18. 12. Systematic uncertainties discussion
    20/06/2020, 07:50
  19. 13. Discussion on Next Steps
    Kate Scholberg (Duke University)
    20/06/2020, 08:05
  20. 30. Intro to fire drill overall strategy
    Erin O'Sullivan (Stockholm University)
    20/06/2020, 08:30
  21. 31. Brainstorming - supernova modelling
    Evan O'Connor, James Kneller (NC State University)
    20/06/2020, 08:40
  22. 32. Brainstorming - Detector response
    Segev BenZvi (University of Rochester)
    20/06/2020, 08:45
  23. 33. Brainstorming - Pre-supernova
    Andrey Sheshukov (JINR), Cecilia Lunardini (Arizona State University)
    20/06/2020, 08:50
  24. 34. Brainstorming - implementation
    Alec Thomas Habig (University of Minnesota (US))
    20/06/2020, 08:55
  25. 35. Brainstorming - triangulation
    Jeffrey Tseng (University of Oxford (GB)), Kate Scholberg (Duke University)
    20/06/2020, 09:00
  26. 36. Brainstorming - Multimessenger
    Dan Milisavljevic (Purdue University)
    20/06/2020, 09:05
  27. 37. Brainstorming - Outreach
    Justin Vasel (Indiana University)
    20/06/2020, 09:10
  28. 38. Discussion
    20/06/2020, 09:15
  29. 2. Analytic Model for Supernova Neutrinos
    Tommy Lam (Virginia Tech)
    Signal Prediction - Modeling
    Poster
    Signal Prediction - Modeling

    We report the status of upgrading the analytic supernova model of Mueller et al. (2016) with a focus on neutrino emission. Our simple model is calibrated to existing numerical supernova simulations and will include the dependence on the mass density property of the progenitor to yield neutrino predictions within seconds.

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  30. 23. Detector response of KM3Net, offline implementation
    Massimiliano Lincetto, marta colomer (km3net)
  31. 21. Discussion
    Alec Thomas Habig (University of Minnesota (US))

    Open discussion (everyone).

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  32. 28. Preparing to Observe the Next Galactic Supernova with IceCube
    Spencer Griswold (University of Rochester)
    Alert Formation - Fire Drills
    Poster
    Alert Formation - Fire Drills

    The next Galactic supernova will be a historic opportunity for multi-messenger astronomy. A core collapse will produce a neutrino burst visible up to half a day before electromagnetic radiation from the explosion, providing an early warning for optical follow-up and valuable insight about the proto-neutron star. Since local supernovae are exceedingly rare, it is critical that neutrino...

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