Author: "Campagne, Jean-Eric" - Searchworks@Jio Institute Digital Library Search Results

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1. Denoising: from classical methods to deep CNNs

Author: Campagne, Jean-Eric
Subjects: Computer Science - Computer Vision and Pattern Recognition, Mathematics - History and Overview
Abstract: This paper aims to explore the evolution of image denoising in a pedagological way. We briefly review classical methods such as Fourier analysis and wavelet bases, highlighting the challenges they faced until the emergence of neural networks, notably the U-Net, in the 2010s. The remarkable performance of these networks has been demonstrated in studies such as Kadkhodaie et al. (2024). They exhibit adaptability to various image types, including those with fixed regularity, facial images, and bedroom scenes, achieving optimal results and biased towards geometry-adaptive harmonic basis. The introduction of score diffusion has played a crucial role in image generation. In this context, denoising becomes essential as it facilitates the estimation of probability density scores. We discuss the prerequisites for genuine learning of probability densities, offering insights that extend from mathematical research to the implications of universal structures., Comment: This document uses works by authors not yet presented to the community and may appear to be original
Published: 2024

2. JAX-COSMO: An End-to-End Differentiable and GPU Accelerated Cosmology Library

Author: Campagne, Jean-Eric, Lanusse, François, Zuntz, Joe, Boucaud, Alexandre, Casas, Santiago, Karamanis, Minas, Kirkby, David, Lanzieri, Denise, Li, Yin, and Peel, Austin
Subjects: Astrophysics - Cosmology and Nongalactic Astrophysics, Astrophysics - Instrumentation and Methods for Astrophysics
Abstract: We present jax-cosmo, a library for automatically differentiable cosmological theory calculations. It uses the JAX library, which has created a new coding ecosystem, especially in probabilistic programming. As well as batch acceleration, just-in-time compilation, and automatic optimization of code for different hardware modalities (CPU, GPU, TPU), JAX exposes an automatic differentiation (autodiff) mechanism. Thanks to autodiff, jax-cosmo gives access to the derivatives of cosmological likelihoods with respect to any of their parameters, and thus enables a range of powerful Bayesian inference algorithms, otherwise impractical in cosmology, such as Hamiltonian Monte Carlo and Variational Inference. In its initial release, jax-cosmo implements background evolution, linear and non-linear power spectra (using halofit or the Eisenstein and Hu transfer function), as well as angular power spectra with the Limber approximation for galaxy and weak lensing probes, all differentiable with respect to the cosmological parameters and their other inputs. We illustrate how autodiff can be a game-changer for common tasks involving Fisher matrix computations, or full posterior inference with gradient-based techniques. In particular, we show how Fisher matrices are now fast, exact, no longer require any fine tuning, and are themselves differentiable. Finally, using a Dark Energy Survey Year 1 3x2pt analysis as a benchmark, we demonstrate how jax-cosmo can be combined with Probabilistic Programming Languages to perform posterior inference with state-of-the-art algorithms including a No U-Turn Sampler, Automatic Differentiation Variational Inference,and Neural Transport HMC. We further demonstrate that Normalizing Flows using Neural Transport are a promising methodology for model validation in the early stages of analysis.
Published: 2023
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3. Predicting regrowth of low-grade gliomas after radiotherapy

Author: Plaszczynski, Stephane, Grammaticos, Basile, Pallud, Johan, Campagne, Jean-Eric, and Badoual, Mathilde
Subjects: Physics - Medical Physics
Abstract: Diffuse low grade gliomas are invasive and incurable brain tumours that inevitably transform into higher grade ones. A classical treatment to delay this transition is radiotherapy (RT). Following RT, the tumour gradually shrinks during a period of typically 6 months to 4 years before regrowing. To improve the patient's health-related quality of life and help clinicians build personalised follow-ups, one would benefit from predictions of the time during which the tumour is expected to decrease. The challenge is to provide a reliable estimate of this regrowth time shortly after RT (i.e. with few data), although patients react differently to the treatment. To this end, we analyse the tumour size dynamics from a batch of 20 high-quality longitudinal data, and propose a simple and robust analytical model, with just 4 parameters. From the study of their correlations, we build a statistical constraint that helps determine the regrowth time even for patients for which we have only a few measurements of the tumour size. We validate the procedure on the data and predict the regrowth time at the moment of the first MRI after RT, with precision of, typically, 6 months. Using virtual patients, we study whether some forecast is still possible just three months after RT. We obtain some reliable estimates of the regrowth time in 75\% of the cases, in particular for all "fast-responders". The remaining 25\% represent cases where the actual regrowth time is large and can be safely estimated with another measurement a year later. These results show the feasibility of making personalised predictions of the tumour regrowth time shortly after RT.
Published: 2022
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4. The LSST-DESC 3x2pt Tomography Optimization Challenge

Author: Zuntz, Joe, Lanusse, François, Malz, Alex I., Wright, Angus H., Slosar, Anže, Abolfathi, Bela, Alonso, David, Bault, Abby, Bom, Clécio R., Brescia, Massimo, Broussard, Adam, Campagne, Jean-Eric, Cavuoti, Stefano, Cypriano, Eduardo S., Fraga, Bernardo M. O., Gawiser, Eric, Gonzalez, Elizabeth J., Green, Dylan, Hatfield, Peter, Iyer, Kartheik, Kirkby, David, Nicola, Andrina, Nourbakhsh, Erfan, Park, Andy, Teixeira, Gabriel, Heitmann, Katrin, Kovacs, Eve, and Mao, Yao-Yuan
Subjects: Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: This paper presents the results of the Rubin Observatory Dark Energy Science Collaboration (DESC) 3x2pt tomography challenge, which served as a first step toward optimizing the tomographic binning strategy for the main DESC analysis. The task of choosing an optimal tomographic binning scheme for a photometric survey is made particularly delicate in the context of a metacalibrated lensing catalogue, as only the photometry from the bands included in the metacalibration process (usually riz and potentially g) can be used in sample definition. The goal of the challenge was to collect and compare bin assignment strategies under various metrics of a standard 3x2pt cosmology analysis in a highly idealized setting to establish a baseline for realistically complex follow-up studies; in this preliminary study, we used two sets of cosmological simulations of galaxy redshifts and photometry under a simple noise model neglecting photometric outliers and variation in observing conditions, and contributed algorithms were provided with a representative and complete training set. We review and evaluate the entries to the challenge, finding that even from this limited photometry information, multiple algorithms can separate tomographic bins reasonably well, reaching figures-of-merit scores close to the attainable maximum. We further find that adding the g band to riz photometry improves metric performance by ~15% and that the optimal bin assignment strategy depends strongly on the science case: which figure-of-merit is to be optimized, and which observables (clustering, lensing, or both) are included., Comment: 30 pages (incl. 12 in appendix), 12 figures. Version accepted for publication in the Open Journal of Astrophysics
Published: 2021
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5. The Tianlai Dish Pathfinder Array: design, operation and performance of a prototype transit radio interferometer

Author: Wu, Fengquan, Li, Jixia, Zuo, Shifan, Chen, Xuelei, Das, Santanu, Marriner, John P., Oxholm, Trevor M., Phan, Anh, Stebbins, Albert, Timbie, Peter T., Ansari, Reza, Campagne, Jean-Eric, Chen, Zhiping, Cong, Yanping, Huang, Qizhi, Li, Yichao, Liu, Tao, Liu, Yingfeng, Niu, Chenhui, Osinga, Calvin, Perdereau, Olivier, Peterson, Jeffrey B., Shi, Huli, Siebert, Gage, Sun, Shijie, Tian, Haijun, Tucker, Gregory S., Wang, Qunxiong, Wang, Rongli, Wang, Yougang, Wu, Yanlin, Xu, Yidong, Yu, Kaifeng, Yu, Zijie, Zhang, Jiao, Zhang, Juyong, and Zhu, Jialu
Subjects: Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: The Tianlai Dish Pathfinder Array is a radio interferometer designed to test techniques for 21~cm intensity mapping in the post-reionization universe as a means for measuring large-scale cosmic structure. It performs drift scans of the sky at constant declination. We describe the design, calibration, noise level, and stability of this instrument based on the analysis of about $\sim 5 \%$ of 6,200 hours of on-sky observations through October, 2019. Beam pattern determinations using drones and the transit of bright sources are in good agreement, and compatible with electromagnetic simulations. Combining all the baselines, we make maps around bright sources and show that the array behaves as expected. A few hundred hours of observations at different declinations have been used to study the array geometry and pointing imperfections, as well as the instrument noise behaviour. We show that the system temperature is below 80~K for most feed antennas, and that noise fluctuations decrease as expected with integration time, at least up to a few hundred seconds. Analysis of long integrations, from 10 nights of observations of the North Celestial Pole, yielded visibilities with amplitudes of 20-30~mK, consistent with the expected signal from the NCP radio sky with $<10\,$mK precision for $1 ~\mathrm{MHz} \times 1~ \mathrm{min}$ binning. Hi-pass filtering the spectra to remove smooth spectrum signal yields a residual consistent with zero signal at the $0.5\,$mK level., Comment: 30 pages, 38 figures
Published: 2020
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6. Fink, a new generation of broker for the LSST community

Author: Möller, Anais, Peloton, Julien, Ishida, Emille E. O., Arnault, Chris, Bachelet, Etienne, Blaineau, Tristan, Boutigny, Dominique, Chauhan, Abhishek, Gangler, Emmanuel, Hernandez, Fabio, Hrivnac, Julius, Leoni, Marco, Leroy, Nicolas, Moniez, Marc, Pateyron, Sacha, Ramparison, Adrien, Turpin, Damien, Ansari, Réza, Allam Jr., Tarek, Bajat, Armelle, Biswas, Biswajit, Boucaud, Alexandre, Bregeon, Johan, Campagne, Jean-Eric, Cohen-Tanugi, Johann, Coleiro, Alexis, Dornic, Damien, Fouchez, Dominique, Godet, Olivier, Gris, Philippe, Karpov, Sergey, Gomez-Moran, Ada Nebot, Neveu, Jérémy, Plaszczynski, Stephane, Savchenko, Volodymyr, and Webb, Natalie
Subjects: Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - High Energy Astrophysical Phenomena
Abstract: Fink is a broker designed to enable science with large time-domain alert streams such as the one from the upcoming Vera C. Rubin Observatory Legacy Survey of Space and Time (LSST). It exhibits traditional astronomy broker features such as automatised ingestion, annotation, selection and redistribution of promising alerts for transient science. It is also designed to go beyond traditional broker features by providing real-time transient classification which is continuously improved by using state-of-the-art Deep Learning and Adaptive Learning techniques. These evolving added values will enable more accurate scientific output from LSST photometric data for diverse science cases while also leading to a higher incidence of new discoveries which shall accompany the evolution of the survey. In this paper we introduce Fink, its science motivation, architecture and current status including first science verification cases using the Zwicky Transient Facility alert stream., Comment: accepted in MNRAS
Published: 2020
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7. Adversarial training applied to Convolutional Neural Network for photometric redshift predictions

Author: Campagne, Jean-Eric
Subjects: Astrophysics - Instrumentation and Methods for Astrophysics, Electrical Engineering and Systems Science - Image and Video Processing
Abstract: The use of Convolutional Neural Networks (CNN) to estimate the galaxy photometric redshift probability distribution by analysing the images in different wavelength bands has been developed in the recent years thanks to the rapid development of the Machine Learning (ML) ecosystem. Authors have set-up CNN architectures and studied their performances and some sources of systematics using standard methods of training and testing to ensure the generalisation power of their models. So far so good, but one piece was missing : does the model generalisation power is well measured? The present article shows clearly that very small image perturbations can fool the model completely and opens the Pandora's box of \textit{adversarial} attack. Among the different techniques and scenarios, we have chosen to use the Fast Sign Gradient one-step Method and its Projected Gradient Descent iterative extension as adversarial generator tool kit. However, as unlikely as it may seem these adversarial samples which fool not only a single model, reveal a weakness both of the model and the classical training. A revisited algorithm is shown and applied by injecting a fraction of adversarial samples during the training phase. Numerical experiments have been conducted using a specific CNN model for illustration although our study could be applied to other models - not only CNN ones - and in other contexts - not only redshift measurements - as it deals with the complexity of the boundary decision surface., Comment: 12 pages, 6 figures
Published: 2020

8. Core Cosmology Library: Precision Cosmological Predictions for LSST

Author: Chisari, Nora Elisa, Alonso, David, Krause, Elisabeth, Leonard, C. Danielle, Bull, Philip, Neveu, Jérémy, Villarreal, Antonia, Singh, Sukhdeep, McClintock, Thomas, Ellison, John, Du, Zilong, Zuntz, Joe, Mead, Alexander, Joudaki, Shahab, Lorenz, Christiane S., Troester, Tilman, Sanchez, Javier, Lanusse, Francois, Ishak, Mustapha, Hlozek, Renée, Blazek, Jonathan, Campagne, Jean-Eric, Almoubayyed, Husni, Eifler, Tim, Kirby, Matthew, Kirkby, David, Plaszczynski, Stéphane, Slosar, Anze, Vrastil, Michal, and Wagoner, Erika L.
Subjects: Astrophysics - Cosmology and Nongalactic Astrophysics, Astrophysics - Instrumentation and Methods for Astrophysics
Abstract: The Core Cosmology Library (CCL) provides routines to compute basic cosmological observables to a high degree of accuracy, which have been verified with an extensive suite of validation tests. Predictions are provided for many cosmological quantities, including distances, angular power spectra, correlation functions, halo bias and the halo mass function through state-of-the-art modeling prescriptions available in the literature. Fiducial specifications for the expected galaxy distributions for the Large Synoptic Survey Telescope (LSST) are also included, together with the capability of computing redshift distributions for a user-defined photometric redshift model. A rigorous validation procedure, based on comparisons between CCL and independent software packages, allows us to establish a well-defined numerical accuracy for each predicted quantity. As a result, predictions for correlation functions of galaxy clustering, galaxy-galaxy lensing and cosmic shear are demonstrated to be within a fraction of the expected statistical uncertainty of the observables for the models and in the range of scales of interest to LSST. CCL is an open source software package written in C, with a python interface and publicly available at https://github.com/LSSTDESC/CCL., Comment: 38 pages, 18 figures, matches ApJS accepted version
Published: 2018
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9. Progress in the Construction and Testing of the Tianlai Radio Interferometers

Author: Das, Santanu, Anderson, Christopher J., Ansari, Reza, Campagne, Jean-Eric, Charlet, Daniel, Chen, Xuelei, Chen, Zhiping, Cianciara, Aleksander J., Colom, Pierre, Cong, Yanping, Gayley, Kevin G., Geng, Jingchao, Hao, Jie, Huang, Qizhi, Keith, Celeste S., Li, Chao, Li, Jixia, Li, Yichao, Liu, Chao, Liu, Tao, Magneville, Christophe, Marriner, John P., Martin, Jean-Michel, Moniez, Marc, Oxholm, Trevor M., Pen, Ue-Li, Perdereau, Olivier, Peterson, Jeffrey B., Shi, Huli, Shu, Lin, Stebbins, Albert, Sun, Shijie, Timbie, Peter T., Torchinsky, Steve, Tucker, Gregory S., Wang, Guisong, Wang, Rongli, Wang, Xin, Wang, Yougang, Wu, Fengquan, Xu, Yidong, Yu, Kaifeng, Zhang, Jiao, Zhang, Juyong, Zhang, Le, Zhu, Jialu, and Zuo, Shifan
Subjects: Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: The Tianlai Pathfinder is designed to demonstrate the feasibility of using a wide field of view radio interferometers to map the density of neutral hydrogen in the Universe after the Epoch of Reionizaton. This approach, called 21~cm intensity-mapping, promises an inexpensive means for surveying the large-scale structure of the cosmos. The Tianlai Pathfinder presently consists of an array of three, 15~m $\times$ 40~m cylinder telescopes and an array of sixteen, 6~m diameter dish antennas located in a radio-quiet part of western China. The two types of arrays were chosen to determine the advantages and disadvantages of each approach. The primary goal of the Pathfinder is to make 3D maps by surveying neutral hydrogen over large areas of the sky %$20,000 {\rm deg}^2$ in two different redshift ranges: first at $1.03 > z > 0.78$ ($700 - 800$~MHz) and later at $0.21 > z > 0.12$ ($1170 - 1270$~MHz). The most significant challenge to $21$~cm intensity-mapping is the removal of strong foreground radiation that dwarfs the cosmological signal. It requires exquisite knowledge of the instrumental response, i.e. calibration. In this paper, we provide an overview of the status of the Pathfinder and discuss the details of some of the analysis that we have carried out to measure the beam function of both arrays. We compare electromagnetic simulations of the arrays to measurements, discuss measurements of the gain and phase stability of the instrument, and provide a brief overview of the data processing pipeline., Comment: 18 pages, 10 figures
Published: 2018

10. Sky reconstruction for the Tianlai cylinder array

Author: Zhang, Jiao, Zuo, Shifan, Ansari, Reza, Chen, Xuelei, Li, Yichao, Wu, Fengquan, Campagne, Jean-Eric, and Magneville, Christophe
Subjects: Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: In this paper, we apply our sky map reconstruction method for transit type interferometers to the Tianlai cylinder array. The method is based on the spherical harmonic decomposition, and can be applied to cylindrical array as well as dish arrays and we can compute the instrument response, synthesised beam, transfer function and the noise power spectrum. We consider cylinder arrays with feed spacing larger than half wavelength, and as expected, we find that the arrays with regular spacing have grating lobes which produce spurious images in the reconstructed maps. We show that this problem can be overcome, using arrays with different feed spacing on each cylinder. We present the reconstructed maps, and study the performance in terms of noise power spectrum, transfer function and beams for both regular and irregular feed spacing configurations., Comment: 15 pages, 12 figures, accepted by RAA
Published: 2016
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11. Sky reconstruction from transit visibilities: PAON-4 and Tianlai Dish Array

Author: Zhang, Jiao, Ansari, Reza, Chen, Xuelei, Campagne, Jean-Eric, Magneville, Christophe, and Wu, Fengquan
Subjects: Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: The spherical harmonics $m$-mode decomposition is a powerful sky map reconstruction method suitable for radio interferometers operating in transit mode. It can be applied to various configurations, including dish arrays and cylinders. We describe the computation of the instrument response function, the point spread function (PSF), transfer function, the noise covariance matrix and noise power spectrum. The analysis in this paper is focused on dish arrays operating in transit mode. We show that arrays with regular spacing have more pronounced side lobes as well as structures in their noise power spectrum, compared to arrays with irregular spacing, specially in the north-south direction. A good knowledge of the noise power spectrum $C^{\mathrm{noise}}(\ell)$ is essential for intensity mapping experiments as non uniform $C^{\mathrm{noise}}(\ell)$ is a potential problem for the measurement of the HI power spectrum. Different configurations have been studied to optimise the PAON-4 and Tianlai dish array layouts. We present their expected performance and their sensitivities to the 21-cm emission of the Milky Way and local extragalactic HI clumps, Comment: 20 pages, 18 figures - Submitted to MNRAS ( the appendix A,B are not included in the accepted version)
Published: 2016
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12. BAORadio: A digital pipeline for radio interferometry and 21 cm mapping of large scale structures

Author: Ansari, Réza, Campagne, Jean-Eric, Colom, Pierre, Magneville, Christophe, Martin, Jean-Michel, Moniez, Marc, Rich, James, and Yèche, Christophe
Subjects: Astrophysics - Cosmology and Nongalactic Astrophysics, Astrophysics - Instrumentation and Methods for Astrophysics
Abstract: 3D mapping of matter distribution in the universe through the 21 cm radio emission of atomic hydrogen HI is a complementary approach to optical surveys for the study of the Large Scale Structures, in particular for measuring the BAO (Baryon Acoustic Oscillation) scale up to redshifts z < 3, and therefore constraining dark energy parameters. We propose a novel method to map the HI mass distribution in three dimensions in radio, without detecting or identifying individual compact sources. This method would require an instrument with a large instantaneous bandwidth (> 100 MHz) and high sensitivity, while a rather modest angular resolution (~ 10 arcmin) should be sufficient. These requirements can be met by a dense interferometric array or a phased array (FPA) in the focal plane of a large primary reflector, representing a total collecting area of a few thousand square meters with few hundred simultaneous beams covering a 20 to 100 square degrees field of view. We describe the development and qualification of an electronic and data processing system for digital radio interferometry and beam forming suitable for such instruments with several hundred receiver elements., Comment: 11 pages, 5 figures
Published: 2012
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13. The \theta_{13} and \delta_{CP} sensitivities of the SPL-Frejus project revisited

Author: Campagne, Jean Eric and Cazes, Antoine
Subjects: High Energy Physics - Experiment
Abstract: An optimization of the CERN SPL beam line has been performed guided by the sensitivities to the \theta_{13} mixing angle and to the \delta_{CP} Dirac CP violating phase. A UNO-like 440 ktons water Cerenkov detector located at 130 km from the target in a new foreseen Frejus laboratory has been used as a generic detector. Concerning the \delta_{CP} independent \theta_{13} sensitivity, a gain of about 20% may be reached using a 3.5 GeV proton beam with a 40 m long, 2 m radius decay tunnel compared to the up to now considered 2.2 GeV beam energy and 20 m long, 1 m radius decay tunnel. This may motivate new machine developments to upgrade the nominal SPL proton beam energy., Comment: 17 pages, 19 figures, submitted to European Physical Journal C
Published: 2004
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14. JAX-COSMO: An End-to-End Differentiable and GPU Accelerated Cosmology Library

Author: Campagne, Jean-Eric, primary, Lanusse, François, additional, Zuntz, Joe, additional, Boucaud, Alexandre, additional, Casas, Santiago, additional, Karamanis, Minas, additional, Kirkby, David, additional, Lanzieri, Denise, additional, Peel, Austin, additional, and Li, Yin, additional
Published: 2023
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15. Predicting regrowth of low-grade gliomas after radiotherapy

Author: Plaszczynski, Stéphane, primary, Grammaticos, Basile, additional, Pallud, Johan, additional, Campagne, Jean-Eric, additional, and Badoual, Mathilde, additional
Published: 2023
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16. The Tianlai dish pathfinder array: design, operation, and performance of a prototype transit radio interferometer

Author: Wu, Fengquan, primary, Li, Jixia, additional, Zuo, Shifan, additional, Chen, Xuelei, additional, Das, Santanu, additional, Marriner, John P, additional, Oxholm, Trevor M, additional, Phan, Anh, additional, Stebbins, Albert, additional, Timbie, Peter T, additional, Ansari, Reza, additional, Campagne, Jean-Eric, additional, Chen, Zhiping, additional, Cong, Yanping, additional, Huang, Qizhi, additional, Kwak, Juhun, additional, Li, Yichao, additional, Liu, Tao, additional, Liu, Yingfeng, additional, Niu, Chenhui, additional, Osinga, Calvin, additional, Perdereau, Olivier, additional, Peterson, Jeffrey B, additional, Podczerwinski, John, additional, Shi, Huli, additional, Siebert, Gage, additional, Sun, Shijie, additional, Tian, Haijun, additional, Tucker, Gregory S, additional, Wang, Qunxiong, additional, Wang, Rongli, additional, Wang, Yougang, additional, Wu, Yanlin, additional, Xu, Yidong, additional, Yu, Kaifeng, additional, Yu, Zijie, additional, Zhang, Jiao, additional, Zhang, Juyong, additional, and Zhu, Jialu, additional
Published: 2021
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17. fink, a new generation of broker for the LSST community

Author: Möller, Anais, primary, Peloton, Julien, additional, Ishida, Emille E O, additional, Arnault, Chris, additional, Bachelet, Etienne, additional, Blaineau, Tristan, additional, Boutigny, Dominique, additional, Chauhan, Abhishek, additional, Gangler, Emmanuel, additional, Hernandez, Fabio, additional, Hrivnac, Julius, additional, Leoni, Marco, additional, Leroy, Nicolas, additional, Moniez, Marc, additional, Pateyron, Sacha, additional, Ramparison, Adrien, additional, Turpin, Damien, additional, Ansari, Réza, additional, Allam Jr, Tarek, additional, Bajat, Armelle, additional, Biswas, Biswajit, additional, Boucaud, Alexandre, additional, Bregeon, Johan, additional, Campagne, Jean-Eric, additional, Cohen-Tanugi, Johann, additional, Coleiro, Alexis, additional, Dornic, Damien, additional, Fouchez, Dominique, additional, Godet, Olivier, additional, Gris, Philippe, additional, Karpov, Sergey, additional, Nebot Gomez-Moran, Ada, additional, Neveu, Jérémy, additional, Plaszczynski, Stephane, additional, Savchenko, Volodymyr, additional, and Webb, Natalie, additional
Published: 2020
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18. Core Cosmology Library: Precision Cosmological Predictions for LSST

Author: Sub String Theory Cosmology and ElemPart, Theoretical Physics, Chisari, Nora Elisa, Alonso, David, Krause, Elisabeth, Leonard, C. Danielle, Bull, Philip, Neveu, Jérémy, Villarreal, Antonio, Singh, Sukhdeep, McClintock, Thomas, Ellison, John, Du, Zilong, Zuntz, Joe, Mead, Alexander, Joudaki, Shahab, Lorenz, Christiane S., Troester, Tilman, Sanchez, Javier, Lanusse, Francois, Ishak, Mustapha, Hlozek, Renée, Blazek, Jonathan, Campagne, Jean-Eric, Almoubayyed, Husni, Eifler, Tim, Kirby, Matthew, Kirkby, David, Plaszczynski, Stéphane, Slosar, Anze, Vrastil, Michal, Wagoner, Erika L., Sub String Theory Cosmology and ElemPart, Theoretical Physics, Chisari, Nora Elisa, Alonso, David, Krause, Elisabeth, Leonard, C. Danielle, Bull, Philip, Neveu, Jérémy, Villarreal, Antonio, Singh, Sukhdeep, McClintock, Thomas, Ellison, John, Du, Zilong, Zuntz, Joe, Mead, Alexander, Joudaki, Shahab, Lorenz, Christiane S., Troester, Tilman, Sanchez, Javier, Lanusse, Francois, Ishak, Mustapha, Hlozek, Renée, Blazek, Jonathan, Campagne, Jean-Eric, Almoubayyed, Husni, Eifler, Tim, Kirby, Matthew, Kirkby, David, Plaszczynski, Stéphane, Slosar, Anze, Vrastil, Michal, and Wagoner, Erika L.
Published: 2018

19. Progress in the construction and testing of the Tianlai radio interferometers

Author: Timbie, Peter T., primary, Cianciara, Aleksander J., primary, Anderson, Christopher J., primary, Chen, Xuelei, primary, Chen, Zhiping, primary, Das, Santanu, primary, Gayley, Kevin G., primary, Keith, Celeste S., primary, Li, Jixia, primary, Liu, Chao, primary, Liu, Tao, primary, Marriner, John P., primary, Peterson, Jeffrey B., primary, Shi, Huli, primary, Stebbins, Albert J., primary, Wang, Yougang, primary, Wu, Fengquan, primary, Zhang, Juyong, primary, Li, Yichao, primary, Zuo, Shifan, primary, Huang, Qizhi, primary, Xu, Yidong, primary, Cong, Yanping, primary, Yu, Kaifeng, primary, Ansari, Reza, primary, Magneville, Christophe, primary, Charlet, Daniel, primary, Campagne, Jean-Eric, primary, Colom, Pierre, primary, Hao, Jie, primary, Torchinsky, Steve, primary, Martin, Jean-Michel, primary, Moniez, Marc, primary, Oxholm, Trevor M., primary, Pen, Ue-li, primary, Perdereau, Olivier, primary, Tucker, Gregory S., primary, Wang, Xin, primary, Zhang, Jiao, primary, Zhang, Le, primary, Zhu, Jialu, primary, Wang, Rongli, primary, Geng, Jingchao, primary, Li, Chao, primary, Shu, Lin, primary, Sun, Shijie, primary, and Wang, Guisong, primary
Published: 2018
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20. On sky characterization of the BAORadio wide band digital backend

Author: Ansari, R., Campagne, Jean-Eric, Colom, P., Ferrari, C., Magneville, Ch., Martin, J. M., Moniez, M., Torrentó, A. S., Laboratoire de l'Accélérateur Linéaire (LAL), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), Institut de Physique Nucléaire d'Orsay (IPNO), and BAORadio
Subjects: [PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]
Abstract: 18 pages, 17 figures; International audience; We have observed regions of three galaxy clusters at z∼ [0.06, 0.09] (Abell85, Abell1205, Abell2440), as well as calibration sources with the Nancay radiotelescope (NRT) to search for 21 cm emission and fully characterize the FPGA based BAORadio digital backend. The total observation time of few hours per source have been distributed over few months, from March 2011 to January 2012, due to scheduling constraints of the NRT, which is a transit telescope. Data have been acquired in parallel with the NRT standard correlator (ACRT) back-end, as well as with the BAORadio data acquisition system. The latter enables wide band instantaneous observation of the [1250, 1500]MHz frequency range, as well as the use of powerful RFI mitigation methods thanks to its fine time sampling. A number of questions related to instrument stability, data processing and calibration are discussed. We have obtained the radiometer curves over the integration time range [0.01,10 000] seconds and we show that sensitivities of few mJy over most of the wide frequency band can be reached with the NRT.It is clearly shown that in blind line search, which is the context of HI intensity mapping for Baryon Acoustic Oscillations, the new acquisition system and processing pipeline outperforms the standard one. We report a positive detection of 21 cm emission at 3 sigma-level from galaxies in the outer region of Abell85 at 1352 MHz (14 400 km/s) corresponding to a line strength of 0.8 Jy km/s. We observe also an excess power around 1318 MHz (21 600 km/s), although at lower statistical significance, compatible with emission from Abell1205 galaxies. Detected radio line emissions have been cross matched with optical catalogs and we have derived hydrogen mass estimates.
Published: 2016

21. The SPL-Fréjus physics potential

Author: Campagne, Jean-Eric
Published: 2006
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22. Sky reconstruction for the Tianlai cylinder array

Author: Zhang, Jiao, primary, Zuo, Shi-Fan, additional, Ansari, Reza, additional, Chen, Xuelei, additional, Li, Yi-Chao, additional, Wu, Feng-Quan, additional, Campagne, Jean-Eric, additional, and Magneville, Christophe, additional
Published: 2016
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23. Sky reconstruction from transit visibilities: PAON-4 and Tianlai dish array

Author: Zhang, Jiao, primary, Ansari, Reza, additional, Chen, Xuelei, additional, Campagne, Jean-Eric, additional, Magneville, Christophe, additional, and Wu, Fengquan, additional
Published: 2016
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24. BAORadio: A digital pipeline for radio interferometry and 21 cm mapping of large scale structures BAORadio : Une chaîne numérique pour la radio-interférométrie et la cartographie des grandes structures à 21 cm

Author: Ansari, R., Campagne, Jean-Eric, Colom, P., Magneville, C., Martin, J.-M., Moniez, M., Rich, J., Yèche, C., Laboratoire de l'Accélérateur Linéaire (LAL), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), Laboratoire d'études spatiales et d'instrumentation en astrophysique (LESIA), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, Galaxies, Etoiles, Physique, Instrumentation (GEPI), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, LSST, and Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)
Subjects: [PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], [PHYS]Physics [physics], [PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM], [SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], Dark energy, Énergie noire, 21 cm radio interferometry Cosmologie, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], Radio-interférométrie à 21 cm, Cosmology, [SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]
Abstract: 3D mapping of matter distribution in the Universe through the 21 cm radio emission of atomic hydrogen (HI) is a complementary approach to optical surveys for the study of the Large Scale Structures, in particular for measuring the BAO (Baryon Acoustic Oscillation) scale up to redshifts z≲3, and therefore constraining dark energy parameters. We propose a novel method to map the HI mass distribution in three dimensions in radio, without detecting or identifying individual compact sources. This method would require an instrument with a large instantaneous bandwidth (≳100 MHz) and high sensitivity, while a rather modest angular resolution (∼10 arcmin) should be sufficient. These requirements can be met by a dense interferometric array or a phased array (FPA) in the focal plane of a large primary reflector, representing a total collecting area of a few thousand square meters with few hundred simultaneous beams covering a 20 to 100 square degrees field of view. We describe the development and qualification of an electronic and data processing system for digital radio interferometry and beam forming suitable for such instruments with several hundred receiver elements. La cartographie de lʼunivers en radio, à travers lʼobservation de la raie à 21 cm de lʼhydrogène atomique, constitue une approche complémentaire aux relevés optiques pour lʼétude des grandes structures, et en particulier des oscillations acoustiques baryoniques (BAO). Nous proposons une méthode originale de la mesure de la distribution de lʼhydrogène atomique neutre à travers une cartographie à 3 dimensions de lʼémission du gaz à 21 cm, sans identification de sources compactes. Cette méthode nécessite un instrument avec une grande sensibilité et une grande largeur de bande instantanée (≳100 MHz), alors quʼelle peut se contenter dʼune résolution angulaire moyenne (∼10 arcmin). Ces performances peuvent être obtenues avec un réseau interférométrique compact ou un réseau phasé au foyer dʼun grand réflecteur, représentant une surface collectrice de quelques milliers de m2 avec quelques centaines de lobes simultanés couvrant un champ de vue de 20 à 100 deg2. Nous décrivons le développement et la qualification dʼun système électronique et de traitement pour la radio-interférométrie et la synthèse de lobe numérique, adapté à ce type dʼinstrument avec plusieurs centaines dʼéléments de réception.
Published: 2012

25. Large Synoptic Survey Telescope: Dark Energy Science Collaboration

Author: Abate, A., Ansari, R., Campagne, Jean-Eric, Moniez, M., Perdereau, O., Plaszczynski, Stéphane, Tristram, M., Boutigny, D., Antilogus, P., Astier, P., Bongard, S., Guy, J., Pain, R., Russo, S., Ricol, J.S., Ealet, A., Escoffier, S., Fouchez, D., Tao, C., Tilquin, A., Laboratoire de l'Accélérateur Linéaire (LAL), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), Centre de Calcul de l'IN2P3 (CC-IN2P3), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE), Centre National de la Recherche Scientifique (CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Pierre et Marie Curie - Paris 6 (UPMC), Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Joseph Fourier - Grenoble 1 (UJF)-Centre National de la Recherche Scientifique (CNRS), Centre de Physique des Particules de Marseille (CPPM), Aix Marseille Université (AMU)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), IN2P3, LSST, Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), and Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Centre National de la Recherche Scientifique (CNRS)
Subjects: [PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], [SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], [PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]
Abstract: See paper for full list of authors - 133 pages; a White Paper describing the goals of the LSST Dark Energy Science Collaboration and its work plan for the next three years; This white paper describes the LSST Dark Energy Science Collaboration (DESC), whose goal is the study of dark energy and related topics in fundamental physics with data from the Large Synoptic Survey Telescope (LSST). It provides an overview of dark energy science and describes the current and anticipated state of the field. It makes the case for the DESC by laying out a robust analytical framework for dark energy science that has been defined by its members and the comprehensive three-year work plan they have developed for implementing that framework. The analysis working groups cover five key probes of dark energy: weak lensing, large scale structure, galaxy clusters, Type Ia supernovae, and strong lensing. The computing working groups span cosmological simulations, galaxy catalogs, photon simulations and a systematic software and computational framework for LSST dark energy data analysis. The technical working groups make the connection between dark energy science and the LSST system. The working groups have close linkages, especially through the use of the photon simulations to study the impact of instrument design and survey strategy on analysis methodology and cosmological parameter estimation. The white paper describes several high priority tasks identified by each of the 16 working groups. Over the next three years these tasks will help prepare for LSST analysis, make synergistic connections with ongoing cosmological surveys and provide the dark energy community with state of the art analysis tools. Members of the community are invited to join the LSST DESC, according to the membership policies described in the white paper. Applications to sign up for associate membership may be made by submitting the Web form at http://www.slac.stanford.edu/exp/lsst/desc/signup.html with a short statement of the work they wish to pursue that is relevant to the LSST DESC.
Published: 2012

26. BAORadio : Cartographie 3D de la distribution de gaz HI dans l'univers

Author: Ansari, R., Campagne, Jean-Eric, Colom, P., Magneville, C., Martin, J.M., Moniez, M., Rich, J., Yèche, C., Starita, Sabine, Laboratoire de l'Accélérateur Linéaire (LAL), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), Galaxies, Etoiles, Physique, Instrumentation (GEPI), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, and Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)
Subjects: [SDU.ASTR.CO] Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], [PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], [PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM], cartographie à 21 cm, [SDU.ASTR.HE] Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], [SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], [SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], cosmologie, [SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM], [PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], [SDU.ASTR.IM] Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM], [PHYS.ASTR.CO] Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], énergie noire, radio-interférométrie, [PHYS.ASTR.IM] Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM], [PHYS.ASTR.HE] Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]
Abstract: Communications consultables sur http://ursi-france.institut-telecom.fr; International audience; La cartographie de l'univers en radio, à travers l'observation de la raie à 21 cm de l'hydrogène atomique, constitue une approche complémentaire aux relevés optiques pour l'étude des grandes structures, et en particulier des oscillations acoustiques baryoniques (BAO). Nous proposons une méthode originale de la mesure de la distribution de l'hydrogène atomique neutre à travers une cartographie à 3 dimensions de l'émission du gaz à 21 cm, sans passer par l'identiﬁcation des sources compactes (galaxies . . . ). Cette méthode nécessite un instrument à grande sensibilité et ayant une grande largeur de bande instantanée (≿ 100 MHz), alors qu'elle peut se contenter d'une résolution angulaire moyenne (10 arcmin). L'instrument devra avoir une surface de collection de quelques milliers de m2 et quelques centaines de lobes simultanés. Ces contraintes peuvent être satisfaites avec un réseau dense de récepteurs en mode interférométrique ou un réseau phasé au foyer d'une grande antenne.
Published: 2011

27. Status of PMm2

Author: Campagne, Jean-Eric, PMm2, Laboratoire de l'Accélérateur Linéaire (LAL), and Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11)
Subjects: [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]
Published: 2009

28. PMm2, a R&D Program for any detectors using 'large' number of photodetectors

Author: Campagne, Jean-Eric, Laboratoire de l'Accélérateur Linéaire (LAL), and Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11)
Subjects: [PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph], [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]
Published: 2007

29. CERN to MEgaton Mass PHYSics

Author: Campagne, Jean-Eric, Laboratoire de l'Accélérateur Linéaire (LAL), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), and Starita, Sabine
Subjects: [PHYS.PHYS.PHYS-ACC-PH]Physics [physics]/Physics [physics]/Accelerator Physics [physics.acc-ph], [PHYS.PHYS.PHYS-ACC-PH] Physics [physics]/Physics [physics]/Accelerator Physics [physics.acc-ph]
Published: 2006

30. Large water Cerenkov detectors

Author: Campagne, Jean-Eric, Jung, C.K., Kaneyuki, K., Laboratoire de l'Accélérateur Linéaire (LAL), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), and Starita, Sabine
Subjects: [PHYS.PHYS.PHYS-INS-DET] Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]
Abstract: Groupe Opera; A brief Status Report on the present projects of Water Cerenkov Megaton scale detectors in the world
Published: 2006

31. MEMPHYS:A large scale water Cerenkov detector at Frejus

Author: De Bellefon, A., Bouchez, J., Busto, J., Campagne, Jean-Eric, Cavata, C., Dolbeau, J., Dumarchez, J., Gorodetzky, P., Katsanevas, S., Mezzetto, M., Mosca, L., Patzak, T., Salin, P., Tonazzo, A., Volpe, C., AstroParticule et Cosmologie (APC (UMR_7164)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Département d'Astrophysique, de physique des Particules, de physique Nucléaire et de l'Instrumentation Associée (DAPNIA), Commissariat à l'énergie atomique et aux énergies alternatives (CEA), Centre de Physique des Particules de Marseille (CPPM), Aix Marseille Université (AMU)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de l'Accélérateur Linéaire (LAL), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Istituto Nazionale di Fisica Nucleare (INFN), APC - Neutrinos, Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-AstroParticule et Cosmologie (APC (UMR_7164)), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, Institut de Physique Nucléaire d'Orsay (IPNO), Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), Centre National de la Recherche Scientifique (CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Pierre et Marie Curie - Paris 6 (UPMC), Centre National de la Recherche Scientifique (CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Pierre et Marie Curie - Paris 6 (UPMC)-AstroParticule et Cosmologie (APC (UMR_7164)), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Aix Marseille Université (AMU), National Institute for Nuclear Physics (INFN), and PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris
Subjects: Physics::Instrumentation and Detectors, Astrophysics::High Energy Astrophysical Phenomena, [PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex], Physics::Accelerator Physics, High Energy Physics::Experiment, Nuclear Experiment, High Energy Physics - Experiment
Abstract: A water \v{C}erenkov detector project, of megaton scale, to be installed in the Fr\'ejus underground site and dedicated to nucleon decay, neutrinos from supernovae, solar and atmospheric neutrinos, as well as neutrinos from a super-beam and/or a beta-beam coming from CERN, is presented and compared with competitor projects in Japan and in the USA. The performances of the European project are discussed, including the possibility to measure the mixing angle $\theta_{13}$ and the CP-violating phase $\delta$., Comment: 1+33 pages, 14 figures, Expression of Interest of MEMPHYS project
Published: 2006

32. Beams for European Neutrino Experiments (BENE) - Midterm scientific report

Author: Baldini, A., Bennett, R., Blondel, A., Campagne, Jean-Eric, Cavata, C., Donini, A., Dracos, M., Dumarchez, J., Edgecock, R., Efthymiopoulos, I., Garoby, R., Huber, P., Long, K., Lindroos, M., Méot, F., Mezzetto, M., Palladino, V., Rees, G., Sievers, P., Strolin, P., Volpe, C., Laboratoire de l'Accélérateur Linéaire (LAL), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), Commissariat à l'énergie atomique et aux énergies alternatives (CEA), Département Recherches Subatomiques (DRS-IPHC), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Louis Pasteur - Strasbourg I-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE), Centre National de la Recherche Scientifique (CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Pierre et Marie Curie - Paris 6 (UPMC), European Organization for Nuclear Research (CERN), Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Joseph Fourier - Grenoble 1 (UJF)-Centre National de la Recherche Scientifique (CNRS), Institut de Physique Nucléaire d'Orsay (IPNO), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Centre National de la Recherche Scientifique (CNRS), and Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA)
Subjects: [PHYS.PHYS.PHYS-ACC-PH]Physics [physics]/Physics [physics]/Accelerator Physics [physics.acc-ph], High Energy Physics::Experiment, Accelerators and Storage Rings
Abstract: PTH; The activities of BENE during 2004 and 2005 are reviewed. Neutrino oscillation experiments at accelerators offer the richest possibilities of precision studies of neutrino mixing and mass differences, with the potential of important discoveries including leptonic CP or T violation. Two main options for a major initiative have been studied: 1) a high-energy Neutrino Factory coupled to a large dense magnetized detector; 2) a lower energy betabeam and conventional superbeam, coupled to a very large low-density, non-magnetic, detector. Both offer significant scientific breakthroughs over other planned facilities. Much remains to be done to optimize and establish the cost, performance, and feasibility of either solution so as to allow comparison and decision. The proposal of a FP7 Design Study of a Neutrino Facility to be completed by the end of the decade is being prepared. Its success will require strong support and engagement at CERN and other European laboratories and funding agencies. International contributors are already engaged in the framework of an international scoping study. The recommendations and milestones proposed by BENE towards a complete conceptual design are summarized.
Published: 2006

33. Sur la route de MEMPHYS

Author: Campagne, Jean-Eric, Laboratoire de l'Accélérateur Linéaire (LAL), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), and Starita, Sabine
Subjects: [PHYS.HPHE] Physics [physics]/High Energy Physics - Phenomenology [hep-ph], [PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]
Published: 2005

34. The SPL-Fréjus: physics potential, Fréjus site and French photodetector R&D

Author: Campagne, Jean-Eric, Starita, Sabine, Laboratoire de l'Accélérateur Linéaire (LAL), and Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11)
Subjects: [PHYS.HPHE] Physics [physics]/High Energy Physics - Phenomenology [hep-ph], [PHYS.PHYS.PHYS-INS-DET] Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], [PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph], [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]
Published: 2005

35. The ��_{13} and ��_{CP} sensitivities of the SPL-Frejus project revisited

Author: Campagne, Jean Eric and Cazes, Antoine
Subjects: High Energy Physics - Experiment (hep-ex), Physics::Instrumentation and Detectors, Physics::Accelerator Physics, FOS: Physical sciences, High Energy Physics::Experiment
Abstract: An optimization of the CERN SPL beam line has been performed guided by the sensitivities to the ��_{13} mixing angle and to the ��_{CP} Dirac CP violating phase. A UNO-like 440 ktons water Cerenkov detector located at 130 km from the target in a new foreseen Frejus laboratory has been used as a generic detector. Concerning the ��_{CP} independent ��_{13} sensitivity, a gain of about 20% may be reached using a 3.5 GeV proton beam with a 40 m long, 2 m radius decay tunnel compared to the up to now considered 2.2 GeV beam energy and 20 m long, 1 m radius decay tunnel. This may motivate new machine developments to upgrade the nominal SPL proton beam energy., 17 pages, 19 figures, submitted to European Physical Journal C
Published: 2004
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36. Porting ALIROOT to CMT for OPERA

Author: Campagne, Jean-Eric, Laboratoire de l'Accélérateur Linéaire (LAL), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), OPERA, and Kerec, Hélène
Subjects: [PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], [PHYS.ASTR.CO] Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]
Published: 2002

37. Les neutrinos atmospheriques : quelles erreurs et comment sont elles estimees ?

Author: Campagne, Jean-Eric, Laboratoire de l'Accélérateur Linéaire (LAL), and Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11)
Subjects: [PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]
Published: 2002

38. The changeable sheet detector in OPERA

Author: Guler, M., Serin-Zeyrek, M., Tolun, P., Zeyrek, M T., Duchesneau, D., Degre, A., Favier, J., Pessard, H., Muciaccia, M T., Righini, P., Simone, S., Lu, S L., Zhou, S J., Winter, K., Borer, K., Haeberli, C., Hess, M., Klingenberg, R., Moser, U., Pretzl, K., Waelchli, T., Weber, M., Giacomelli, G., Mandrioli, G., Patrizii, L., Serra, P., Sioli, M., Sirri, G., Van Beek, G., Vilain, P., Wilquet, G., Spinetti, M., Votano, L., Ogawa, S., Shibuya, H., Autiero, D., Camilleri, L., Di Lella, L., Dupraz, J., Fabre, J P., Petti, R., Schilly, P., Sohlbach, H., Woltersdorf, H., Goldberg, J., Khalifa, M., Busser, F W., Garfagnini, A., Geiser, A., Hopfner, K., Koppitz, B., Naroska, B., Schmidt-Parzefall, W., Van Staa, R., Kodama, K., Ushida, N., Aoki, S., Hara, T., Chaussard, L., Chemarin, M., Déclais, Y., Jonsson, P., Katsanevas, S., Laktineh, I., Marteau, J., Moret, G., D'Ambrosio, N., Boschan, P., Frekers, D., Kellmann, T., Kueckmann, J., Schmand, J., Wortche, H J., Wolff, T., Hoshino, K., Komatsu, M., Miyanishi, M., Nakamura, M., Nakano, T., Niwa, K., Sato, O., Bruski, N., Buontempo, S., Carbonara, F., Cocco, A G., De Lellis, G., De Rosa, G., Ereditato, A., Fiorillo, G., Kawamura, T., Messina, M., Migliozzi, P., Saggese, L., Strolin, P., Tioukov, V., Boucrot, J., Campagne, Jean-Eric, Merkel, B., Repellin, J P., Veillet, J J., Brugnera, R., Dal Corso, F., Dusini, S., Fanin, C., Stanco, L., Rosa, G., Beyer, M., Schroder, H., Waldi, R., Barbuto, E., Bozza, C., Grella, G., Romano, G., Sorrentino, S., Arnold, R., Baussan, E., Dracos, M., Guyonnet, J.L., Strub, R., He, M., Li, J Y., Feng, C F., Fu, Y., Xue, L., Sato, Y., Tezuka, I., Stipcevic, M., Ljubicic, A., Jakovcic, K., Kerec, Hélène, Institut de Physique Nucléaire de Lyon (IPNL), Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de l'Accélérateur Linéaire (LAL), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Institut de Recherches Subatomiques (IReS), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Cancéropôle du Grand Est-Université Louis Pasteur - Strasbourg I-Centre National de la Recherche Scientifique (CNRS), OPERA, Centre National de la Recherche Scientifique (CNRS)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), and Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11)
Subjects: Physics::Instrumentation and Detectors, [PHYS.PHYS.PHYS-INS-DET] Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], Astrophysics::High Energy Astrophysical Phenomena, High Energy Physics::Phenomenology, High Energy Physics::Experiment, [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]
Abstract: Neutrinos
Published: 2002

39. Chemical purification of molybdenum samples for the NEMO3 experiment

Author: Arnold, R., Augier, C., Baker, J., Barabash, A., Bing, O., Blum, D., Brudanin, V., Caffrey, A.J., Campagne, Jean-Eric, Caurier, E., Dassie, D., Egorov, V., Errahnmane, K., Filipova, T., Guyonnet, J.L., Hubert, F., Hubert, P., Jullian, Sophie, Kochetov, O., Kisel, I., Kornoukhov, V.N., Kovalenko, V., Kuzichev, V.F., Lalanne, D., Laplanche, F., Leccia, F., Linck, I., Longuemare, C., Marquet, Ch., Mauger, F., Nicholson, H.W., Nikolic-Audit, I., Pilugin, I., Piquemal, F., Reyss, J.-L., Riddle, C.L., Sarazin, X., Scheibling, F., Stekl, I., Suhonen, J., Sutton, C.S., Szklarz, G., Timkin, V., Tretyak, V., Umatov, V., Vanyushin, I., Vorobel, V., Vylov, Ts., Institut de Recherches Subatomiques (IReS), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Cancéropôle du Grand Est-Université Louis Pasteur - Strasbourg I-Centre National de la Recherche Scientifique (CNRS), Laboratoire de l'Accélérateur Linéaire (LAL), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), Centre d'Etudes Nucléaires de Bordeaux Gradignan (CENBG), Université Sciences et Technologies - Bordeaux 1-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de physique corpusculaire de Caen (LPCC), Université de Caen Normandie (UNICAEN), Normandie Université (NU)-Normandie Université (NU)-École Nationale Supérieure d'Ingénieurs de Caen (ENSICAEN), Normandie Université (NU)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Laboratoire des Sciences du Climat et de l'Environnement [Gif-sur-Yvette] (LSCE), Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ), Océan et Interfaces (OCEANIS), Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ), NEMO, Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), and Normandie Université (NU)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)
Subjects: [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]
Published: 2001

40. Influence of neutrons and $\gamma$-rays in the Frejus underground laboratory on the NEMO experiment

Author: Marquet, Catherine, Piquemal, F., Arnold, R., Augier, C., Baker, J., Barabash, A., Bing, O., Blum, D., Brudanin, V., Caffrey, J., Campagne, Jean-Eric, Caurier, E., Dassie, D., Egorov, V., Errahmane, K., Eschbach, R., Filipova, T., Guyonnet, J.L., Jollet, C., Jullian, Sophie, Hubert, F., Hubert, P., Kisel, I., Kochetov, O., Kornoukhov, V.N., Kovalenko, V., Lalanne, D., Laplanche, D., Leccia, F., Linck, I., Longuemare, C., Mauger, F., Nicholson, H.W., Nikolic-Audit, I., Ohsumi, H., Pilugin, I., Reyss, J.L., Sarazin, X., Scheibling, F., Stekl, I., Suhonen, J., Sutton, C.S., Szklarz, G., Timkin, V., Tretyak, V., Umatov, V., Vala, L., Vanyushin, I., Vareille, A., Vorobel, V., Vylov, T., Centre d'Etudes Nucléaires de Bordeaux Gradignan (CENBG), Université Sciences et Technologies - Bordeaux 1-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Institut de Recherches Subatomiques (IReS), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Cancéropôle du Grand Est-Université Louis Pasteur - Strasbourg I-Centre National de la Recherche Scientifique (CNRS), Laboratoire de l'Accélérateur Linéaire (LAL), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), Laboratoire de physique corpusculaire de Caen (LPCC), Université de Caen Normandie (UNICAEN), Normandie Université (NU)-Normandie Université (NU)-École Nationale Supérieure d'Ingénieurs de Caen (ENSICAEN), Normandie Université (NU)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), NEMO, Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), and Normandie Université (NU)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)
Subjects: [PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]
Published: 2001

41. Limits on different majoron decay modes of $^{100}$Mo, $^{116}$Cd, $^{82}$Se and $^{96}$Zr for neutrinoless double beta decays in the NEMO-2 experiment

Author: VASILEV, V., ARNOLD, R., AUGIER, C., BAKER, J., BARABASH, A., BLUM, D., BRUDANIN, V., CAFFREY, A.J., CAMPAGNE, Jean-Eric, CAURIER, E., DASSIE, D., EGOROV, V., FILIPOVA, T., GURRIARAN, R., GUYONNET, J.L., HUBERT, F., HUBERT, P., JULLIAN, Sophie, KISEL, I., KOCHETOV, O., KORNOUKHOV, V.N., KOVALENKO, V., LALANNE, D., LAPLANCHE, F., LECCIA, F., LINCK, I., LONGUEMARE, C., MARQUET, Catherine, MAUGER, F., NICHOLSON, H.W., PILUGIN, I., PIQUEMAL, F., REYSS, J.L., SARAZIN, X., SCHEIBLING, F., SUHONEN, J., SUTTON, C.S., SZKLARZ, G., TIMKIN, V., TORRES, R., UMATOV, V., VANYUSHIN, I., VAREILLE, A., VYLOV, Ts., Institut de Recherches Subatomiques (IReS), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Cancéropôle du Grand Est-Université Louis Pasteur - Strasbourg I-Centre National de la Recherche Scientifique (CNRS), Laboratoire de l'Accélérateur Linéaire (LAL), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), Centre d'Etudes Nucléaires de Bordeaux Gradignan (CENBG), Université Sciences et Technologies - Bordeaux 1-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de physique corpusculaire de Caen (LPCC), Université de Caen Normandie (UNICAEN), Normandie Université (NU)-Normandie Université (NU)-École Nationale Supérieure d'Ingénieurs de Caen (ENSICAEN), Normandie Université (NU)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), NEMO, Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), and Normandie Université (NU)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)
Subjects: [PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex], Nuclear Physics
Published: 2001

42. Status report on the OPERA experiment

Author: Kellmann, T., van Beek, G., Vilain, P., Wilquet, G., Lu, S.L., Ren, J., Zhou, S.J., Feng, C., Fu, Y., He, M., Li, J.Y., Xue, L., Jakovcic, K., Ljubicic, A., Stipcevic, M., Degre, A., Duchesneau, D., Favier, J., Lavy, M., Mugnier, P., Pessard, H., Arnold, R., Baussan, E., Dracos, M., Engel, J.P., Guyonnet, J.L., Chaussard, L., Déclais, Y., Heritier, C., Jonsson, P., Katsanevas, S., Laktineh, I., Marteau, J., Moret, G., Boucrot, J., Campagne, Jean-Eric, Merkel, B., Repellin, J.P., Veillet, J.J., Schauties, H., Sohlbach, H., Woltersdorf, H., Aplin, S., Bagdasarova, I., Ballhausen, C., Buesser, F.W., Ebert, J., Koppitz, B., Naroska, B., Saveliev, V., Schmidt-Parzefall, W., van Staa, R., Winter, K., Laboratoire d'Annecy de Physique des Particules (LAPP), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS), Institut de Recherches Subatomiques (IReS), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Cancéropôle du Grand Est-Université Louis Pasteur - Strasbourg I-Centre National de la Recherche Scientifique (CNRS), Institut de Physique Nucléaire de Lyon (IPNL), Centre National de la Recherche Scientifique (CNRS)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Laboratoire de l'Accélérateur Linéaire (LAL), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), OPERA, Laboratoire d'Annecy de Physique des Particules (LAPP/Laboratoire d'Annecy-le-Vieux de Physique des Particules), Centre National de la Recherche Scientifique (CNRS)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), and Flores, Sylvie
Subjects: [PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], [PHYS.ASTR.CO] Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], Physics::Instrumentation and Detectors, Astrophysics::High Energy Astrophysical Phenomena, High Energy Physics::Phenomenology, High Energy Physics::Experiment
Abstract: Neutrinos
Published: 2001

43. Status of the NEMO-3 experiment for the study of neutrinoless double beta decay

Author: Augier, C., Baker, J., Barabash, A., Blum, D., Brudanin, V., Caffrey, A.J., Campagne, Jean-Eric, Caurier, E., Dassie, D., Egorov, V., Filipova, T., Gurriaran, R., Guyonnet, J.L., Hubert, F., Hubert, P., Jullian, Sophie, Kochetov, O., Kisel, I., Kornoukhov, V.N., Kovalenko, V., Lalanne, D., Laplanche, F., Leccia, F., Linck, I., Longuemare, C., Marquet, Catherine, Mauger, F., Nicholson, H.W., Pilugin, I., Piquemal, F., Reyss, J.L., Sarazin, X., Scheibling, F., Suhonen, J., Sutton, C.S., Szklarz, G., Timkin, V., Torres, R., Tretyak, V.I., Umatov, V., Vanyushin, I., Vareille, A., Vasilyev, Y., Laboratoire de l'Accélérateur Linéaire (LAL), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), Centre d'Etudes Nucléaires de Bordeaux Gradignan (CENBG), Université Sciences et Technologies - Bordeaux 1-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de physique corpusculaire de Caen (LPCC), Université de Caen Normandie (UNICAEN), Normandie Université (NU)-Normandie Université (NU)-École Nationale Supérieure d'Ingénieurs de Caen (ENSICAEN), Normandie Université (NU)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), and NEMO
Subjects: Physics, Particle physics, 010308 nuclear & particles physics, Detector, [PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex], 7. Clean energy, 01 natural sciences, Nuclear physics, Double beta decay, 0103 physical sciences, Electromagnetic shielding, Underground laboratory, Neutrino, 010306 general physics
Abstract: The NEMO collaboration is presently mounting the NEMO3 detector in the Frejus Underground Laboratory (Laboratoire Souterrain de Modane or LSM). This detector is devoted to search of neutrinoless double beta decay of various isotopes and especially Molybdenium 100. It will be able to reach a sensitivity to neutrino effective mass in the order of 0.1 eV. The NEMO3 detector is composed of 20 sectors. Three of them take data in Modane since the end of April, without shielding or magnetic field. The full detector is planned to be in operation by the end of the year.
Published: 2000

44. Double beta decay with the NEMO experiment : status of the Nemo 3 detector

Author: ARNOLD, R., AUGIER, C., BAKER, J., BARABASH, A., BLUM, D., BRUDANIN, V., CAFFREY, A.J., CAMPAGNE, Jean-Eric, CAURIER, E., DASSIE, D., EGOROV, V., FILIPOVA, T., GURRIARAN, R., GUYONNET, J.L., HUBERT, F., HUBERT, P., JULLIAN, Sophie, KISEL, I., KOCHETOV, O., KORNOUKHOV, V.N., KOVALENKO, V., LALANNE, D., LAPLANCHE, F., LECCIA, F., LINCK, I., LONGUEMARE, C., MARQUET, Catherine, MAUGER, F., NICHOLSON, H.W., PILUGIN, I., PIQUEMAL, F., REYSS, J-L., SARAZIN, X., SCHEIBLING, F., SUHONEN, J., SUTTON, C.S., SZKLARZ, G., TIMKIN, V., TORRES, R., UMATOV, V., VANYUSHIN, I., VAREILLE, A., VASILYEV, V., VYLOV, Ts., Laboratoire de l'Accélérateur Linéaire (LAL), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), Institut de Recherches Subatomiques (IReS), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Cancéropôle du Grand Est-Université Louis Pasteur - Strasbourg I-Centre National de la Recherche Scientifique (CNRS), Centre d'Etudes Nucléaires de Bordeaux Gradignan (CENBG), Université Sciences et Technologies - Bordeaux 1-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de physique corpusculaire de Caen (LPCC), Université de Caen Normandie (UNICAEN), Normandie Université (NU)-Normandie Université (NU)-École Nationale Supérieure d'Ingénieurs de Caen (ENSICAEN), Normandie Université (NU)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), NEMO, Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), and Normandie Université (NU)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)
Subjects: [PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]
Published: 2000

45. An appearance experiment to search for $\nu_{\mu} \leftrightarrow \nu_{\tau}$ oscillations in the CNGS beam : experimental proposal

Author: Guler, M., Serin-Zeyrek, M., Tolun, P., Zeyrek, M T., Duchesneau, D., Degre, A., Favier, J., Pessard, H., Muciaccia, M T., Righini, P., Simone, S., Lu, S L., Zhou, S J., Winter, K., Borer, K., Haeberli, C., Hess, M., Klingenberg, R., Moser, U., Pretzl, K., Waelchli, T., Weber, M., Giacomelli, G., Mandrioli, G., Patrizii, L., Serra, P., Sioli, M., Sirri, G., Van Beek, G., Vilain, P., Wilquet, G., Spinetti, M., Votano, L., Ogawa, S., Shibuya, H., Autiero, D., Camilleri, L., Di Lella, L., Dupraz, J., Fabre, J P., Petti, R., Schilly, P., Sohlbach, H., Woltersdorf, H., Goldberg, J., Khalifa, M., Busser, F W., Garfagnini, A., Geiser, A., Hopfner, K., Koppitz, B., Naroska, B., Schmidt-Parzefall, W., Van Staa, R., Kodama, K., Ushida, N., Aoki, S., Hara, T., Chaussard, L., Chemarin, M., Déclais, Y., Jonsson, P., Katsanevas, S., Laktineh, I., Marteau, J., Moret, G., D'Ambrosio, N., Boschan, P., Frekers, D., Kellmann, T., Kueckmann, J., Schmand, J., Wortche, H J., Wolff, T., Hoshino, K., Komatsu, M., Miyanishi, M., Nakamura, M., Nakano, T., Niwa, K., Sato, O., Bruski, N., Buontempo, S., Carbonara, F., Cocco, A G., De Lellis, G., De Rosa, G., Ereditato, A., Fiorillo, G., Kawamura, T., Messina, M., Migliozzi, P., Saggese, L., Strolin, P., Tioukov, V., Boucrot, J., Campagne, Jean-Eric, Merkel, B., Repellin, J P., Veillet, J J., Brugnera, R., Dal Corso, F., Dusini, S., Fanin, C., Stanco, L., Rosa, G., Beyer, M., Schroder, H., Waldi, R., Barbuto, E., Bozza, C., Grella, G., Romano, G., Sorrentino, S., Arnold, R., Baussan, E., Dracos, M., Guyonnet, J.L., Strub, R., He, M., Li, J Y., Feng, C F., Fu, Y., Xue, L., Sato, Y., Tezuka, I., Stipcevic, M., Ljubicic, A., Jakovcic, K., Kerec, Hélène, Laboratoire d'Annecy de Physique des Particules (LAPP), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS), Institut de Physique Nucléaire de Lyon (IPNL), Centre National de la Recherche Scientifique (CNRS)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Laboratoire de l'Accélérateur Linéaire (LAL), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), Institut de Recherches Subatomiques (IReS), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Cancéropôle du Grand Est-Université Louis Pasteur - Strasbourg I-Centre National de la Recherche Scientifique (CNRS), OPERA, Laboratoire d'Annecy de Physique des Particules (LAPP/Laboratoire d'Annecy-le-Vieux de Physique des Particules), Centre National de la Recherche Scientifique (CNRS)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), and Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)
Subjects: [PHYS.HEXP] Physics [physics]/High Energy Physics - Experiment [hep-ex], Physics::Instrumentation and Detectors, Astrophysics::High Energy Astrophysical Phenomena, High Energy Physics::Phenomenology, [PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex], High Energy Physics::Experiment
Abstract: Neutrinos
Published: 2000

46. Towards an experiment to study atmospheric neutrino oscillations with a massive magnetized iron detector (Progress Report)

Author: Ambrosio, M., Amelchakov, M., Antonioli, P., Aprile, E., Aramo, C., Aynutdinov, V., Bari, G., Benacoeur, R., Bencivenni, G., Bologna, G., Bonesini, M., Bruni, G., Bruski, N., Buesser, F.W., Campagne, Jean-Eric, Chernov, D., Chemarin, M., Curioni, A., Chaussard, L., Déclais, Y., Duchesneau, D., Ezubchenko, A., Favier, J., Frekers, D., Galeotti, P., Garfagnini, A., Geiser, A., Gharbi, F., Giusti, P., Golubkov, D., Golouvev, N., Gninenko, S., Gustavino, C., Heinzelmann, G., Hermel, R., Hoepfner, K., Jonsson, P., Katsanevas, S., Kindin, V., Kirsanov, M., Klanner, R., Koppitz, B., Kokoulin, R., Kompaniets, K., Konovalov, A., Kovzelev, A., Laktineh, I., Mannocchi, G., Marteau, J., Merkel, B., Monacelli, P., Moret, G., Murtas, F., Murtas, G.P., Nania, R., Naroska, B., Negri, P., Ordine, A., Paganoni, M., Pesci, A., Pessard, H., Periale, L., Petrukhin, A., Picchi, P., Pullia, A., Ragazzi, S., Redaelli, N., Repellin, J-P., Rondeshagen, D., Ronga, F., Sartorelli, G., Satta, L., Schmidt-Parzefall, W., Spinetti, M., Souga, C., Tabarelli De Fatis, T., Terranova, F., Trabelski, A., Trinchero, G., Van Staa, R., Veillet, J.J., Villone, B., Votano, L., Winter, K., Woerche, H.J., Wolff, T., Yanson, E., Yashin, I., Flores, Sylvie, Laboratoire de l'Accélérateur Linéaire (LAL), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), Institut de Physique Nucléaire de Lyon (IPNL), Centre National de la Recherche Scientifique (CNRS)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Laboratoire d'Annecy de Physique des Particules (LAPP), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS), and MONOLITH
Subjects: [PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], [PHYS.ASTR.CO] Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]
Published: 1999

47. A long baseline $\nu_\tau$ appearance experiment in the CNGS beam from CERN to Gran Sasso - (Progress Report)

Author: Kodama, M., Ushida, N., Guler, M., Pesen, E., Serin-Zeyrek, M., Sever, R., Tolun, P., Zeyrek, M.T., Duchesneau, D., Favier, J., Pessard, H., Muciaccia, M.T., Righini, P., Simone, S., Haeberli, C., Hess, M., Klingenberg, R., Moser, U., Pretsl, K., Weber, M., Benussi, L., Van Beek, G., Vilain, P., Wilquet, G., Spinetti, M., Votano, L., Kazamura, T., Ogawa, S., Shibuya, H., Dupraz, J., Fabre, J-P., Schilly, P., Stiegler, U., Goldberg, J., Khalifa, M., Buesser, F.W., Geiser, A., Hoepfner, K., Koppitz, B., Naroska, B., Schmidt-Parzefall, W., Van Staa, R., Aoki, S., Hara, T., Chaussard, L., Chemarin, M., Déclais, Y., Jonsson, P., Katsanevas, S., Laktineh, I., Marteau, J., Moret, G., Artamonov, A., Gorbounov, P., Khovansky, V., D'Ambrosio, N., Oschan, P., Frekers, D., Rondeshagen, D., Schmand, J., Wortche, H.J., Wolff, T., Hoshino, K., Komatsu, M., Miyanishi, M., Nakamura, M., Nakano, T., Niwa, K., Sato, O., Ruski, N., Uontempo, S., Carbonara, F., Cocco, A.G., Cuomo, V., De Lellis, G., Eroditato, A., Fiorillo, G., Listone, R., Messina, M., Migliozzi, P., Sorrentino, S., Strolin, P., Tioukov, V., Campagne, Jean-Eric, Merkel, B., Repellin, J-P., Veillet, J-J., Rosa, G., Barbuto, E., Bozza, C., Grella, G., Romano, G., Sato, Y., Tezuka, I., Laboratoire d'Annecy de Physique des Particules (LAPP), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS), Institut de Physique Nucléaire de Lyon (IPNL), Centre National de la Recherche Scientifique (CNRS)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Laboratoire de l'Accélérateur Linéaire (LAL), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), and OPERA
Subjects: [PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]
Published: 1999

48. Testing the Pauli exclusion principle with the NEMO-2 detector

Author: Arnold, R., Augier, C., Baker, J., Barabash, A., Blum, D., Brudanin, V., Caffrey, A.J., Campagne, Jean-Eric, Caurier, E., Dassie, D., Egorov, V., Filipova, T., Gurriaran, R., Guyonnet, J.L., Hubert, F., Hubert, P., Jullian, Sophie, Kochetov, O., Kisel, I., Kornoukhov, V.N., Kovalenko, V., Lalanne, D., Laplanche, F., Leccia, F., Linck, I., Longuemare, C., Marquet, Catherine, Mauger, F., Nicholson, H.W., Pilugin, I., Piquemal, F., Reyss, J.L., Sarazin, X., Scheibling, F., Suhonen, J., Sutton, C.S., Szklarz, G., Timkin, V., Torres, R., Tretyak, V.I., Umatov, V., Vanyushin, I., Vareille, A., Vasilyev, Y., Heyd, Yvette, Institut de Recherches Subatomiques (IReS), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Cancéropôle du Grand Est-Université Louis Pasteur - Strasbourg I-Centre National de la Recherche Scientifique (CNRS), Laboratoire de l'Accélérateur Linéaire (LAL), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), Centre d'Etudes Nucléaires de Bordeaux Gradignan (CENBG), Université Sciences et Technologies - Bordeaux 1-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de physique corpusculaire de Caen (LPCC), Université de Caen Normandie (UNICAEN), Normandie Université (NU)-Normandie Université (NU)-École Nationale Supérieure d'Ingénieurs de Caen (ENSICAEN), Normandie Université (NU)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), NEMO, Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), and Normandie Université (NU)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)
Subjects: [PHYS.NEXP] Physics [physics]/Nuclear Experiment [nucl-ex], [PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]
Published: 1999

49. Progress report towards an experiment to study atmospheric neutrino oscillations with a massive magnetized iron detector

Author: Ambrosio, M., Amelchakov, M., Antonioli, P., Aprile, E., Aramo, C., Aynutdinov, V., Bari, G., Benaceur, R., Bencivenni, G., Bologna, G., Bonesini, M., Bruni, G., Bruski, N., Busser, F W., Campagne, Jean-Eric, Chernov, D., Chemarin, M., Curioni, A., Chaussard, L., Déclais, Y., Duchesneau, D., Ezubchenko, A., Favier, J., Frekers, D., Galeotti, P., Garfagnini, A., Geiser, A., Gharbi, F., Giusti, P., Golubkov, D., Goloubev, N., Gninenko, S., Gustavino, C., Heinzelmann, G., Hermel, R., Hopfner, K., Jonsson, P., Katsanevas, S., Kindin, V., Kirsanov, M., Klanner, R., Koppitz, B., Kokoulin, R., Kompaniets, K., Konovalov, A., Kovzelev, A., Laktineh, I., Mannocchi, G., Marteau, J., Merkel, B., Monacelli, P., Moret, G., Murtas, F., Murtas, G P., Nania, R., Naroska, B., Negri, P., Ordine, A., Paganoni, M., Pesci, A., Pessard, H., Periale, L., Petrukhin, a A., Picchi, P., Pullia, A., Ragazzi, S., Redaelli, N., Repellin, J P., Rondeshagen, D., Ronga, F., Sartorelli, G., Satta, L., Schmidt-Parzefall, W., Spinetti, M., Souga, C., Tabarelli de Fatis, T., Terranova, F., Trabelsi, A., Trinchero, G., van Staa, R., Veillet, J J., Villone, B., Votano, L., Winter, K., Wortche, H J., Wolff, T., Yanson, E., Laboratoire de l'Accélérateur Linéaire (LAL), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), Institut de Physique Nucléaire de Lyon (IPNL), Centre National de la Recherche Scientifique (CNRS)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Laboratoire d'Annecy de Physique des Particules (LAPP), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS), OPERA, and Kerec, Hélène
Subjects: [PHYS.HEXP] Physics [physics]/High Energy Physics - Experiment [hep-ex], [PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]
Published: 1999

50. Double-beta decay of $^{82}$Se

Author: Arnold, R., Augier, C., Baker, J., Barabash, A., Blum, D., Brudanin, V., Caffrey, A.J., Campagne, Jean-Eric, Caurier, E., Dassie, D., Egorov, V., Eschbach, R., Filipova, T., Gurriaran, R., Guyonnet, J.L., Hubert, F., Hubert, P., Jullian, Sophie, Kisel, I., Kochetov, O., Kornoukhov, V.N., Kovalenko, V., Lalanne, D., Laplanche, F., Leccia, F., Linck, I., Longuemare, C., Marquet, Catherine, Mauger, F., Mennrath, P., Nicholson, H.W., Pilugin, I., Piquemal, F., Purtov, O., Reyss, J-L., Sarazin, X., Scheibling, F., Suhonen, J., Sutton, C.S., Szklarz, G., Timkin, V., Torres, R., Tretyak, V.I., Umatov, V., Vanyushin, I., Vareille, A., Vaslyev, Y., Vylov, T., Zerkin, V., Institut de Recherches Subatomiques (IReS), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Cancéropôle du Grand Est-Université Louis Pasteur - Strasbourg I-Centre National de la Recherche Scientifique (CNRS), Laboratoire de l'Accélérateur Linéaire (LAL), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), Centre d'Etudes Nucléaires de Bordeaux Gradignan (CENBG), Université Sciences et Technologies - Bordeaux 1-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de physique corpusculaire de Caen (LPCC), Université de Caen Normandie (UNICAEN), Normandie Université (NU)-Normandie Université (NU)-École Nationale Supérieure d'Ingénieurs de Caen (ENSICAEN), Normandie Université (NU)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), NEMO, Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Normandie Université (NU)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), and Chambon, Pascale
Subjects: [PHYS.NEXP] Physics [physics]/Nuclear Experiment [nucl-ex], [PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]
Published: 1998

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