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SUMMARY:Global Neutrino Network (GNN) Meeting 2026 (formerly MANTS)
DTSTART:20260525T070000Z
DTEND:20260526T160000Z
DTSTAMP:20260513T190800Z
UID:indico-event-7529@indico.nikhef.nl
CONTACT:dosamt@nikhef.nl
DESCRIPTION:This annual meeting has been established in order to best conn
 ect the neutrino telescope community and brings together all neutrino coll
 aborations\, which constitute the GNN. It fosters the exchange between the
  collaborations to best exploit synergies from hardware developments to hi
 gh-level analyses to future visions.A note for new people: this meeting al
 lows for sharing things privately under MOU that could be of interest to o
 ther neutrino collaborations in the network. This includes in-progress wor
 k\, and you usually do not need your collaboration's speakers committee pe
 rmission\, nor to approve plots or slides in advance as you would for norm
 al conferences. (If in doubt\, check with your collaboration\, of course.)
 The GNN meeting will this year be held in Amsterdam at Nikhef. The meeting
  fee includes the lunches and dinner.How to get here: Nikhef is well conne
 cted by public transport\, it takes ~15 minutes from Amsterdam Centrum to 
  get there\, you can find descriptions of the connections here.Visum: If 
 you need an invitation letter for a visum please contact Joan Berger (jber
 ger at nikhef.nl).Note about the payment: An early version of the payment 
 link did not lead to the 'confirmed payment' page due to a typo and thus t
 he registration is incorrectly listed as 'awaiting payment'. If the money 
 was subtracted from your bank account we also received it despite the stat
 ement. The problem should be fixed by now.Questions / Topics to be discuss
 ed: We will be able to discuss a wide variety of topics that are relevant 
 to the collaborations and for the GNN community. Below are some of the top
 ics/questions open for discussion. We can cover them in presentations and 
 during discussion time during the meeting\, including an "Unconference" se
 ssion with break-out discussions and ad-hoc plenary presentations from the
 se discussions. Feel free to submit/add your own questions you would like 
 to discuss - we will add them here. Contact Claudio Kopper via chat (if yo
 u have this) or via email at claudio.kopper@fau.de ! Selection of questio
 ns: How do we find Galactic neutrino sources?Can we detect kHz periodic s
 ignals of MeV neutrinos?What is the status of the common NMO working group
 ?How do we deal with realtime analysis and/or time-dependent sources and h
 ow do we collaborate on them?How far did we get with common data formats f
 or realtime alerts?How do we deal with atmospheric fluxes? Is Daemonflux a
  good description? How do detector systematics fit into this? And do we ne
 ed a joint WG on this?How do you deal with water properties / ice properti
 es / medium properties\, how do they affect your reconstructions / systema
 tics)How can AI methods help us and how are they already being used?How do
  you start a joint working group (and how do you keep it alive??)What can 
 we achieve if we combine detectors? (PLeNuM\, …)How should we approach c
 ombined EHE (extremely high energy) fits across multiple detectors?How can
  we efficiently simulate the extreme tail of the muon flux\, including unc
 ertainties from hadronic interaction models?How can we improve simulations
  of hadronic showers and charm production in DIS?How can we collaborate mo
 re effectively in searching for the atmospheric prompt flux?How can we bet
 ter model the atmospheric self-veto effect\, particularly important for do
 wn-going neutrino backgrounds?What's the status of KM3-230213A? Any news o
 n it to report?Any updates on the common data formats?  \n\nhttps://indi
 co.nikhef.nl/event/7529/
LOCATION:Nikhef
URL:https://indico.nikhef.nl/event/7529/
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