Paris, November 5th, ILIAS/N5: The GW antenna network Raffaele Flaminio EGO and LAPP/CNRS Summary - History - GWA Objectives & Contents - Management - Budget - Goals of this meeting

Paris, November 5th, GW net: Some history Several attempt to get funds from the EU in the 90’s failed In 2002 EU launched FP6 ApPEC launched a coordinated action in the European astroparticle physics community to prepare a proposal for an I3 called ILIAS (Integrated Large Infrastructures for Astroparticle Science) to be submitted to the EU Long process started - proposal preparation: 9/2002 – 3/ proposal submission: March partly approved in August 2003 (GW contents approved) - negotiations: fall 2003/spring projects start: April 1 st 2004 GWA Budget: 550 kEuros / ~ 200 scientists ….. Why do it ? A) GW experimental community enters the EU world B) Do some coordinated work all together

Paris, November 5th, GW net: Main objectives Increase the level of European coordination in the field Enhance the performance of existing detectors Prepare the future of this discipline in Europe Provide a link between the various experimental projects and theoretical groups Encourage the researchers mobility Open existing facilities to more people from more countries Help the structuring an European GW research community - Ease the collaboration with related field such as Gamma-ray and Neutrino astronomy - Develop coordinated collaborations with non-European communities (USA, Japan, Australia)

Paris, November 5th, GW net: Proposed activities Develop the exchange of information among teams on items such as: - Commissioning and operation of existing detectors - Joint operation and data analysis - R&D for detectors upgrade and future projects Three working groups proposed : ­ WG1: Detectors commissioning and characterization ­ WG2: Joint operation of detectors and network data analysis ­ WG3: An European strategy for future detectors Beside working group activities: ­ Have bi-annual meetings involving the responsibles of the main projects and research poles ­ Organize an annual general meeting

Paris, November 5th, GW net: Objectives and Deliverables WG1 “Commissioning and operation of existing detectors” - Speed-up the VIRGO/GEO commissioning by means of a deeper collaboration - Provide inputs for establishing priorities in the short term improvement of existing detectors - Common characterization methodologies - Regular reports describing and comparing detectors performances WG2 “Joint operation of detectors and network data analysis” ­ Support joint observations among GW detectors and with gamma, neutrino and optical telescopes ­ Support the development of a network data analysis pipeline - Data analysis pipeline to perform joint analysis of data produced by a network of GW detectors ­ First astrophysical results deduced from joint observations WG3 “An European strategy for future detectors” ­ Determine objectives attainable trough short-term improvements ­ Draft a plan for an European network of GW detectors at the 2010 horizon - Short term plan after 18 months - Long term plan: ‘White book’ defining the GW community strategic objectives over 10 years period

Paris, November 5th, GW net: Management structure Each working group typically consists of at least 10 experts One chairperson and co-chairperson per working group (task leaders) One executive board ensuring the coordination of the whole network formed by representative from main GW projects + working group conveners (~ 10 persons) One institution in charge of the budget administration (EGO)

Paris, November 5th, Executive board Set-up at the beginning of the project: * ILIAS-GWA coordinator: K. Danzmann (AEI Hannover) * Virgo representatives: R.Flaminio (CNRS LAPP), M.Punturo (INFN Perugia) * GEO representatives: B.Willke (AEI Hannover), S.Rowan (University of Glasgow) * Resonant antennas representatives: M.Cerdonio (INFN Padova), E.Coccia (INFN Roma) * LISA representative: S.Vitale (University of Trento) * Invited members: o EGO director: F.Menzinger o JRA3 Representative: G.Cagnoli (University of Glasgow) o Leaders of the three working groups (see below) o N6 Representative: ? Problem: attempts to establish a contact with the theoretical network have failed so far. Main outcome of the first EB meeting (Cascina, May 11 th, 2004): - working group members and chairmen (two/group) established - call for the annual general meeting in November (attached to the Virgo week in Orsay) - discussion on priorities (WG1) - decision to allow members of WG1 to access technical data of the all the antenna - good news: British and German groups asking support to participate to the upgrade of Virgo

Paris, November 5th, WP1: Detectors commissioning and characterization WP2: Joint operation of detectors and network data analysis WP3: An European strategy for future detectors Appointed participants: * M. Barsuglia (LAL Orsay) * A.Freise (EGO) * H.Grote (AEI Hannover) * S. Hild (AEI Hannover) * P.La Penna (EGO) * G.Losurdo (INFN Firenze) * H.Lueck (AEI Hannover) * J. Smith (AEI Hannover) * L.Taffarello (INFN Padova) * M.Visco (INFN Roma) Appointed participants: * P.Astone (INFN Roma) * L.Baggio (INFN Trento) * L.Brocco (INFN Roma) * F. Marion (LAPP Annecy) * M.A.Papa (AEI Golm) * G.A. Prodi (INFN Trento) * B.S. Sathyaprakash (Uni. of Cardiff) * A.Vicere (INFN Firenze) * G.Woan ( University of Glasgow) Appointed participants: * H.Lueck (AEI Hannover) * K.Strain (University of Glasgow) * M.Punturo (INFN Perugia) * R.Flaminio (EGO) * V.Fafone (INFN Frascati) * M.Bonaldi (IFN Trento) * D.Enard (EGO) * L. Gottardi (Leiden) Working groups composition

Paris, November 5th, Financial situation ActivitiesAllocationCommitmentPayment Executive board meeting ,03 WG ,158847,77 WG ,70- WG ,443542,94 Annual general meeting ,84- Audit ,00- Management ,64 TOTAL , ,38

Paris, November 5th, Goals of this meeting Main goal: review working groups activity - problems ? - how to improve ? - need to reinforce the working groups ? Discuss mid-term report preparation Discuss the dissemination of on-going activities: web site(s) Next general meeting