Complementary detectors for AGATA@GANIL campaign AGATA Week October 2016

Mechanical and electronic integration The AGATA campaign is organized by sub-campaigns defining the coupling of AGATA with an apparatus that is restrictive in the local installation  ACC validation in collaboration with GANIL via its SC  specific call VAMOS++ (2015-2017) NEDA (2018) MUGAST (2019-20XX) VAMOS GFM (2019-20XX) EXOGAM clovers LaBr3 scintillators Silicon detectors DIAMANT Plunger Gaz-Detector Additional detectors added by the spokesperson must be compatible with the main “ancillary” Mechanical and electronic integration

VAMOS++ (2015-2017) EXOGAM : VME-VXI - GANIL 2nd arm : VME-VXI -GANIL SPIDER : VME-VXI –GANIL DC : VME-VXI –GANIL ChIO : VME – VXI - GANIL

E710-July 2016 C. Michelagnoli et al.

2017 2018 e693 Jungclauss e705 Regan e673 John e706 Korten e676 Leoni DSSD-AGATA e693 Jungclauss AGATA-FATIMA e705 Regan VAMOS-AGATA-FATIMA e673 John e706 Korten VAMOS-AGATA-PARIS e676 Leoni AGATA-DIAMANT-PARIS e709 Bednarczyk VAMOS-AGATA e711 Doncel VAMOS-AGATA-Compact e674 Lemasson AGATA-NEDA-DIAMANT e699 Lenzi e703 Nyberg e725 Cederwall e731 Boso e730 Clement AGATA-NEDA-DIAMANT-PARIS e727 Fornal 2017 2018

VAMOS++ (2015-2017) EXOGAM : VME-VXI - GANIL 2nd arm : VME-VXI -GANIL LaBr3 : FATIMA – VME – GANIL PARIS – VME-VXI - GANIL SPIDER : VME-VXI –GANIL DC : VME-VXI –GANIL ChIO : VME – VXI - GANIL

2017 run LaBr3 campaign – VAMOS backlog FATIMA-PARIS detectors coupled to AGATA and VAMOS (4 experiments) Mechanical integration into EXOGAM frames Electronic coupling Magnetic shielding Starting the integration in the cave in October Be ready by March 2017 See O. Dorvaux and M. Rudigier’s talks Courtesy I. Burrows

2018 run NEDA campaign 8 experiments approved using AGATA+NEDA (+DIAMANT) (+LaBr3) (+plunger) STFC-LNL-GANIL IPNL-CSNSM-GANIL Design phase for the mechanical integration (STFC-IPNL-GANIL) Electronic Development in progress (NEDA collaboration) Detailed planning for the 2017 installation and 2018 to be clarified when GANIL schedule is clarified J. Nyberg et al. : Studies of excited states in 102,103Sn to deduce two-body neutron interactions, single-particle energies and N=Z=50 core excitations S. Lenzi et al. : Effects of Isospin Symmetry Breaking in the A=63 mirror nuclei M. Bentley et al. : Prompt gamma/proton spectroscopy in 65As – isospin symmetry at the limits of proton-binding B. Cederwall et al. : Search for isoscalar pairing in the N=Z nucleus 88Ru B. Fornal et al. : Gamma decay from near-threshold states in 14C: a probe of clusterization phenomena in open quantum systems E. Clément et al : Shell evolution of neutron-deficient Xe isotopes: Octupole and Quadrupole Correlations above 100Sn A. Boso et al :Isospin Symmetry Breaking and Shape Coexistence in Mirror Nuclei 71Kr-71Br M. Palacz et al : Purity of the g9/2 configuration based on lifetime measurements and energies of excited states in 94Pd See the next talks by Th. Dupasquier, G. de France, J. Ljungvall, G. Jaworski

2019-(2020) run MUGAST-GFM VAMOS in GFM for prompt spectroscopy of Heavy Elements Nucleons transfer spectroscopy using SPIRAL1 ISOL beams See Ch. Theisen’s talk See D. Mengoni’s talk 4th PAC late 2017 : to be defined between MUGAST and/or VAMOS GFM Experiments to be run in 2019 Inputs are how and when SPIRAL1 upgrade and SPIRAL2 start 10 LoI using the Gaz-filled mode of VAMOS 16 LoI using Post-accelerated beams from SPIRAL1

Removable spacers on outer detectors? NEDA FATIMA Removable spacers on outer detectors? Clash with EXOGAM support structure

PARIS Existing EXOGAM structure PARIS detectors FATIMA Simple ‘L’ shaped brackets to allow detector faces to target distance to be varied between 15 & 23cm PARIS