2012 a year of transition Paschal Coyle Mauro

2012 a year of transition Paschal Coyle, Mauro Taiuti, E. de Wolf IB-meeting, 29 January 2013, CPPM

KM 3 Ne. T in 2012 ASC Rome Erlangen agreement SPB Catania Neutrino 2012 Kyoto SPB Rome Jan Feb Mar Apr May Jun KM 3 Ne. T Day Bologna ORCA kick-off Paris Jul Collaboration meeting Marseille Aug Sep ORCA w/s Catania KFA Catania Oct Nov Dec Jan Validation programmes continued steadily divergence 29 January 2013 bi-lateral meetings Mo. U, SSC-replies, 1 st ORCA-report, PP-deliverables, ESFRI questionnaire, MT selection, Community building 1 st KM 3 Ne. T-phase 1 IB meeting, CPPM 2

KM 3 Ne. T Research Infrastructure 29 January 2013 1 st KM 3 Ne. T-phase 1 IB meeting, CPPM 3

ESS-Consortium KM 3 Ne. T-ERIC and ESS-ERIC neutrino detector KM 3 Ne. T-Gr site shore station JB shore station ESS node data centre data repository KM 3 Ne. T-Fr site neutrino detector JB ESS node shore station KM 3 Ne. T-It site ESS-Consortium JB 29 January 2013 ESS node neutrino detector 4

Technology KM 3 Ne. T neutrino detector • String with multi-PMT optical modules is basic technology • Programme for qualification is being executed • Time constraints of ERDF funds in France and Italy to be met: – Pre-procurement of components with long delivery times has started – Staged technical reports for external review 29 January 2013 1 st KM 3 Ne. T-phase 1 IB meeting, CPPM 5

KM 3 Ne. T Collaboration January 2013: 39 Institutes, 182 members 29 January 2013 1 st KM 3 Ne. T-phase 1 IB meeting, CPPM 6

KM 3 Ne. T-phase 1 Mo. U-v 8. 1 Organization Breakdown Structure : k a e r the b e r o f e ab am d e n T e t g n IB a r e r i e o a m h f t h e g s -c a e B i On I n t i a l n i o b si t. M cti c n e e l o j E p o s • Pr re / n s o k i t s c a • Ele t Mo. U - t f a r D • Mo. U-v 4. 3 Mo. U-v 4. 6 Jan Feb 29 January 2013 Mar Mo. U-v 4. 9 Elections stopped Apr Mo. U-v 5. 1 May Jun Jul Aug Sep 1 st KM 3 Ne. T-phase 1 IB meeting, CPPM Oct Mo. U-v 8 Nov Dec Mo. U-v 8. 1 Elections Jan 7

• KM 3 Ne. T on European Roadmap since 2006 • Assessment of the maturity (progress toward implementation) of KM 3 Ne. T has started (governance, HR, project management) • Review interview on 14 February 2013 in Brussels – 15 min presentation – 90 min questions ak e r b he • Questionnaire has been filled a after t nd provided e g • Supporting documents have been a e h t n O – TDR – – SSC Review documents + Replies on recommendations Decision of ASC/KFA on KM 3 Ne. T-ERIC (minutes meetings) Mo. U-v 8 GNO-Lo. I • This Collaboration meeting and the election of management were announced (minutes will be important) • IB needs to establish who will be the representatives for KM 3 Ne. T for this interview (total of 1+3 is allowed) 29 January 2013 1 st KM 3 Ne. T-phase 1 IB meeting, CPPM 8

GNO-I • Global Neutrino Observatory (GNO) • October 2012: Lo. I sent to boards of Antares, Baikal, Ice. Cube, KM 3 Ne. T • Proposal to form GNO-I – Forum for exchange and consultation • MANTS meetings, regular teleconferences – Framework for coordination cooperative actions and self-organization ak e r b he t r e t f nda a Combined sky maps, cross-check results, alert/multi-messenger policies, exchange/check software, common software pool, common effort to connect better to particle physics tools, standards for data representation, exchange of expertise, GNO-internal advisory committees – – – ge a e h t Onstudents Exchange of Ph. D Common organization tools/topical workshops Creation of common web page/outreach Coordination of relations to other fields of science Annual award for the best Ph. D thesis Exploring options for closer cooperation within GNO-II • Form a GNO-board • Prepare a Mo. U for GNO-I • All partners are positive about the proposal, they are waiting for the 29 January 2013 1 st KM 3 Ne. T-phase 1 IB meeting, CPPM reaction of KM 3 Ne. T 9