1. Complementary detectors for AGATA@GANIL campaign
AGATA Week October 2016

2. 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++ ( )
NEDA (2018)
MUGAST ( XX)
VAMOS GFM ( XX)
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

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

4. E710-July 2016 C. Michelagnoli et al.

5. 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

6. 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

7. 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

8. 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

9. 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

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

12. 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