J. L. Bouly
Joseph Fourier University
Network
Latest external collaboration on country level. Dive into details by clicking on the dots.
Publication
Featured researches published by J. L. Bouly.
Journal of Instrumentation | 2011
F. J. Iguaz; D. Attié; D Calvet; P. Colas; F. Druillole; E. Ferrer-Ribas; I. Giomataris; J.-P. Mols; J. Pancin; T. Papaevangelou; J. Billard; G. Bosson; J. L. Bouly; O. Bourrion; Ch. Fourel; C. Grignon; O. Guillaudin; F. Mayet; J. P. Richer; D. Santos; C. Golabek; L. Lebreton
The aim of the MIMAC project is to detect non-baryonic Dark Matter with a directional TPC using a high precision Micromegas readout plane. We will describe in detail the recent developments done with bulk Micromegas detectors as well as the characterisation measurements performed in an Argon(95%)-Isobutane(5%) mixture. Track measurements with alpha particles will be shown.
Journal of Instrumentation | 2012
O. Bourrion; C. Vescovi; J. L. Bouly; A. Benoît; M. Calvo; L. Gallin-Martel; J. F. Macías-Pérez; Alessandro Monfardini
A prototype of digital frequency multiplexing electronics allowing the real time monitoring of microwave kinetic inductance detector (MKIDs) arrays for mm-wave astronomy has been developed. Thanks to the frequency multiplexing, it can monitor simultaneously 400 pixels over a 500 MHz bandwidth and requires only two coaxial cables for instrumenting such a large array. The chosen solution and the achieved performances are presented in this paper.
Journal of Physics: Conference Series | 2011
D. Santos; J. Billard; G. Bosson; J. L. Bouly; O. Bourrion; Ch. Fourel; C. Grignon; O. Guillaudin; F. Mayet; J. P. Richer; A. Delbart; E. Ferrer; I. Giomataris; F. J. Iguaz; J.P. Mols; C. Golabek; L. Lebreton
Directional detection of non-baryonic Dark Matter is a promising search strategy for discriminating WIMP events from background. However, this strategy requires both a precise measurement of the energy down to a few keV and 3D reconstruction of tracks down to a few mm. To achieve this goal, the MIMAC project has been developed. It is based on a gaseous micro-TPC matrix, filled with 3He, CF4 and/or C4H10. The first results on low energy nuclear recoils (1H and 19F) obtained with a low mono-energetic neutron field are presented. The discovery potential of this search strategy is discussed and illustrated by a realistic case accessible to MIMAC.
Nuclear Instruments & Methods in Physics Research Section A-accelerators Spectrometers Detectors and Associated Equipment | 2010
O. Bourrion; G. Bosson; C. Grignon; J. L. Bouly; J. P. Richer; O. Guillaudin; F. Mayet; D. Santos
Directional detection of galactic dark matter requires 3D reconstruction of low energy nuclear recoils tracks. A dedicated acquisition electronics with auto triggering feature and a real time track reconstruction software have been developed within the framework of the MIMAC project of detector. This auto-triggered acquisition electronic uses embedded processing to reduce data transfer to its useful part only, i.e. decoded coordinates of hit tracks and corresponding energy measurements. An acquisition software with online monitoring and 3D track reconstruction is also presented.
Journal of Instrumentation | 2011
O. Bourrion; G. Bosson; C. Grignon; J. L. Bouly; J. P. Richer; O. Guillaudin; F. Mayet; J. Billard; D. Santos
Directional detection of non-baryonic Dark Matter requires 3D reconstruction of low energy nuclear recoils tracks. A gaseous micro-TPC matrix, filled with either 3He, CF4 or C4H10 has been developed within the MIMAC project. A dedicated acquisition electronics and a real time track reconstruction software have been developed to monitor a 512 channel prototype. This auto-triggered electronic uses embedded processing to reduce the data transfer to its useful part only, i.e. decoded coordinates of hit tracks and corresponding energy measurements. An acquisition software with on-line monitoring and 3D track reconstruction is also presented.
arXiv: Instrumentation and Detectors | 2013
D. Santos; G. Bosson; J. L. Bouly; O. Bourrion; Ch. Fourel; O. Guillaudin; J. Lamblin; F. Mayet; J. F. Muraz; J. P. Richer; Q. Riffard; L. Lebreton; D. Maire; J. Busto; J. Brunner; D. Fouchez
Directional detection of non-baryonic Dark Matter is a promising search strategy for discriminating WIMP events from neutrons, the ultimate background for dark matter direct detection. This strategy requires both a precise measurement of the energy down to a few keV and 3D reconstruction of tracks down to a few mm. The MIMAC (MIcro-tpc MAtrix of Chambers) collaboration has developed in the last years an original prototype detector based on the direct coupling of large pixelized micromegas with a special developed fast self-triggered electronics showing the feasibility of a new generation of directional detectors. The first bi-chamber prototype has been installed at Modane, underground laboratory in June 2012. The first undergournd background events, the gain stability and calibration are shown. The first spectrum of nuclear recoils showing 3D tracks coming from the radon progeny is presented.
arXiv: Instrumentation and Detectors | 2013
D. Santos; J. Billard; G. Bosson; J. L. Bouly; O. Bourrion; Ch. Fourel; O. Guillaudin; J. Lamblin; J. F. Muraz; F. Mayet; J. P. Richer; Q. Riffard; E. Ferrer; I. Giomataris; F. J. Iguaz; L. Lebreton; D. Maire
The dark matter directional detection opens a new field in cosmology bringing the possibility to build a map of nuclear recoils that would be able to explore the galactic dark matter halo giving access to a particle characterization of such matter and the shape of the halo. The MIMAC (MIcro-tpc MAtrix of Chambers) collaboration has developed in the last years an original prototype detector based on the direct coupling of large pixelized micromegas with a devoted fast self-triggered electronics showing the feasibility of a new generation of directional detectors. The discovery potential of this search strategy is discussed and illustrated. In June 2012, the first bi-chamber prototype has been installed at Modane Underground Laboratory (LSM) and the first underground background events, the gain stability and calibration are shown.
Journal of Instrumentation | 2011
O. Bourrion; Ch. Bernard; D. Bondoux; J. L. Bouly; J. Bouvier; B. Boyer; M. Brinet; M. Buénerd; G. Damieux; L. Derome; L. Eraud; R. Foglio; D. Fombaron; D. Grondin; M.H. Lee; L. Lutz; M. Marton; A. Menchaca-Rocha; A. Pelissier; J. N. Périé; A. Putze; S. Roudier; Y. Sallaz-Damaz; E. S. Seo; J.-P. Scordilis; Y.S. Yoon
A proximity focusing Cherenkov imager called CHERCAM, has been built for the charge measurement of nuclear cosmic rays with the CREAM instrument. It consists of a silica aerogel radiator plane across from a detector plane equipped with 1,600 1`` diameter photomultipliers. The two planes are separated by a ring expansion gap. The Cherenkov light yield is proportional to the charge squared of the incident particle. The expected relative light collection accuracy is in the few percents range. It leads to an expected single element separation over the range of nuclear charge Z of main interest 1 ? Z26. CHERCAM is designed to fly with the CREAM balloon experiment. The design of the instrument and the implemented technical solutions allowing its safe operation in high altitude conditions (radiations, low pressure, cold) are presented.
Eas Publications Series | 2012
D. Santos; J. Billard; G. Bosson; J. L. Bouly; O. Bourrion; Ch. Fourel; O. Guillaudin; F. Mayet; J. P. Richer; A. Delbart; E. Ferrer; I. Giomataris; F. J. Iguaz; J.P. Mols; C. Golabek; L. Lebreton
Eas Publications Series | 2012
E. Ferrer-Ribas; D. Attié; D Calvet; P. Colas; F. Druillole; Y. Giomataris; F. J. Iguaz; J.-P. Mols; J. Pancin; T. Papaevangelou; J. Billard; G. Bosson; J. L. Bouly; O. Bourrion; Ch. Fourel; C. Grignon; O. Guillaudin; F. Mayet; J. P. Richer; D. Santos; C. Golabek; L. Lebreton