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16. Study of the insertion/deinsertion mechanism of sodium into [Na.sub.0.44]Mn[O.sub.2]

Author

Sauvage, F., Laffont, L., Tarascon, J.-M., and Baudrin, E.

Subjects
Sodium compounds -- Chemical properties, Sodium compounds -- Electric properties, Hydrogen chloride -- Chemical properties, Electrochemical analysis, Chemistry
Abstract

Pure [Na.sub.0.44]Mn[O.sub.2] samples are prepared using a solid-state route by carefully tuning the synthesis conditions. The analysis has shown that the insertion process within the [Na.sub.[x.sup.-]]Mn[O.sub.2] system is fully reversible and that HCl treatment has a detrimental effect on the electrochemical properties due to structural and textural evolutions.

Published
2007

28. Puumala hantavirus infection in humans and in the reservoir host, Ardennes region, France. (Dispatches)

Author

Sauvage, F., Penalba, C., Vuillaume, P., Boue, F., Coudrier, D., Pontier, D., and Artois, M.

Subjects
Hantavirus infections -- Diagnosis, Hantavirus infections -- Development and progression, Communicable diseases -- Research
Abstract

We compared the occurrence of nephropathia epidemica cases, over a multi-annual population cycle, in northeastern France with the hantavirus serology for bank voles captured in the same area. We discuss [...]

Published
2002

34. Stop-less Lyot coronagraph for exoplanet characterization: first on-sky validation in VLT/SPHERE

Author

Vigan, Arthur, N'Diaye, M., Dohlen, K., Beuzit, J.-L., Costille, A., Caillat, A., Baruffolo, A., Blanchard, P., Carle, M., Ferrari, M., Fusco, T., Gluck, L., Hugot, E., Jaquet, M., Langlois, M., Le Mignant, D., Llored, M., Madec, F., Mouillet, D., Origné, A., Puget, P., Salasnich, B., Sauvage, J.-F., Navarro, Ramon, Burge, James, Sauvage, F., Laboratoire d'Astrophysique de Marseille (LAM), Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS), Space Telescope Science Institute (STSci), Institut de Planétologie et d'Astrophysique de Grenoble (IPAG), Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Observatoire des Sciences de l'Univers de Grenoble (OSUG ), Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut national des sciences de l'Univers (INSU - CNRS)-Institut national de recherche en sciences et technologies pour l'environnement et l'agriculture (IRSTEA)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes [2016-2019] (UGA [2016-2019])-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut national de recherche en sciences et technologies pour l'environnement et l'agriculture (IRSTEA)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes [2016-2019] (UGA [2016-2019]), INAF - Osservatorio Astronomico di Padova (OAPD), Istituto Nazionale di Astrofisica (INAF), Chimie, Ingénierie Moléculaire et Matériaux d'Angers (CIMMA), Université d'Angers (UA)-Centre National de la Recherche Scientifique (CNRS), Caratterizzazione e Sviluppo di Materiali per la Fotonica e l'Optoelecttronica (CSMFO), CNR Istituto di Fotonica e Nanotecnologie [Trento] (IFN), Consiglio Nazionale delle Ricerche [Roma] (CNR)-Consiglio Nazionale delle Ricerche [Roma] (CNR), Netherlands Institute for Radio Astronomy (ASTRON), National Research Council of Italy | Consiglio Nazionale delle Ricerche (CNR)-National Research Council of Italy | Consiglio Nazionale delle Ricerche (CNR), Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Aix Marseille Université (AMU)-Centre National d'Études Spatiales [Toulouse] (CNES), Laboratoire d'Astrophysique de Grenoble (LAOG), Université Joseph Fourier - Grenoble 1 (UJF)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Chimie, Ingénierie Moléculaire et Matériaux d'Angers (CIMMA), Centre National de la Recherche Scientifique (CNRS)-Université d'Angers (UA), Centre National d'Études Spatiales [Toulouse] (CNES)-Université Grenoble Alpes (UGA)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire des Sciences de l'Univers de Grenoble (OSUG), Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP)-Institut national de recherche en sciences et technologies pour l'environnement et l'agriculture (IRSTEA)-Université Joseph Fourier - Grenoble 1 (UJF)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP)-Institut national de recherche en sciences et technologies pour l'environnement et l'agriculture (IRSTEA)-Université Joseph Fourier - Grenoble 1 (UJF)-Centre National de la Recherche Scientifique (CNRS), ITA, USA, and FRA

Subjects
Physics, Lyot stop, business.industry, media_common.quotation_subject, Phase (waves), 01 natural sciences, Exoplanet, law.invention, 010309 optics, Speckle pattern, Optics, Apodization, law, Sky, 0103 physical sciences, business, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], 010303 astronomy & astrophysics, Coronagraph, Long-slit spectroscopy, media_common
Abstract

International audience; The VLT/SPHERE instrument includes a unique long-slit spectroscopy (LSS) mode coupled with Lyot coronagraphy dedicated to the spectral characterization of directly imaged giant exoplanets. The performance of this mode is limited by its non-optimal coronagraph, but in a previous work we demonstrated that it could be significantly improved at small inner-working angles using the stop-less Lyot coronagraph (SLLC). A prototype of the SLLC was installed in VLT/SPHERE in 2014 during the reintegration of the instrument in Paranal, and it was extensively tested in 2015 to characterize its performance. The performance is tested in both imaging and spectroscopy using data acquired on the internal source of SPHERE. In imaging, we obtain a raw contrast gain of a factor 10 at 0.3" with the SLLC. We also demonstrate that no Lyot stop is required to reach the full performance, which validates the SLLC concept. Comparison with a realistic simulation model shows that we are currently limited by the internal phase aberrations of SPHERE. In spectroscopy, we obtain a gain of 1 mag in a limited range of angular separations. Simulations show that although the main limitation comes from phase errors, the performance in the non-SLLC case is very close to the ultimate limit of the LSS mode. We present the very first on-sky data with the SLLC, which appear extremely promising for the future scientific exploitation of an apodized LSS mode in SPHERE. Finally, we explore a new possibility for the speckle subtraction in the LSS mode that could significantly improve the data analysis with respect to methods based on spectral differences.

Published
2016

36. Identification de nouveaux gènes impliqués dans les carcinomes basocellulaires sporadiques

Author

Parmentier, L., primary, Bonilla, X., additional, King, B., additional, Bezrukov, F., additional, Kaya, G., additional, Zoete, V., additional, Seplyarskiy, V., additional, Sharpe, H., additional, McKee, T., additional, Letourneau, A., additional, Ribaux, P., additional, Papodin, K., additional, Basset-Seguin, N., additional, Ben Chaabene, R., additional, Santoni, F., additional, Guipponi, M., additional, Andrianova, M., additional, Garieri, M., additional, Verdan, C., additional, Grosdemange, K., additional, Sumara, O., additional, Eilers, M., additional, Aifantis, I., additional, Michielin, O., additional, de Sauvage, F., additional, Antonarakis, S., additional, and Nikolaev, S., additional

Published
2016
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37. Transcription of a β-1,3-glucanase gene in grape berries in a late developmental period, or earlier after wounding treatments

Author

Kraeva, E., Tesnière, C., Terrier, N., charles romieu, Sauvage, F. X., Bierne, J., and Deloire, A.

Subjects
food and beverages
Abstract

The hydrolytic enzymes β-1,3-glucanases (EC3.2.1.39) an known to be involved in plant defense reactions against pathogens and in developmental events. We have obtained two partial cDNA clones, corresponding to Vitis vinifera β-1,3-glucanase gene sequences (VvGlu1/7 and VvGlu26). The expression of VvGlu1/7 was studied in grape berries at different developmental stages and in wounded berries with or without salicylic acid elicitation. No constitutive expression was observed in young berries, whereas the induction of VvGlu1/7 transcription was detected during fruit ripening. By contrast, synthesis of mRNA coding for this isoform was generated in the first stage of rapid berry growth in response to wounding treatments with and without salicylic acid., VITIS - Journal of Grapevine Research, Vol. 37 No. 3 (1998): Vitis

Published
2015
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38. Phase stability frustration on ultra-nanosized anatase TiO 2

Author

Patra, S., Davoisne, C., Bouyanfif, Houssny, Foix, D., Sauvage, F., Réseau sur le stockage électrochimique de l'énergie (RS2E), Université de Nantes (UN)-Aix Marseille Université (AMU)-Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-Collège de France (CdF (institution))-Université de Picardie Jules Verne (UPJV)-Ecole Nationale Supérieure de Chimie de Montpellier (ENSCM)-Ecole Nationale Supérieure de Chimie de Paris - Chimie ParisTech-PSL (ENSCP), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université de Pau et des Pays de l'Adour (UPPA)-Institut de Chimie du CNRS (INC)-Université de Montpellier (UM)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Institut National Polytechnique (Toulouse) (Toulouse INP), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP ), Université Grenoble Alpes (UGA)-Université Grenoble Alpes (UGA), Laboratoire réactivité et chimie des solides - UMR CNRS 7314 (LRCS), Université de Picardie Jules Verne (UPJV)-Institut de Chimie du CNRS (INC)-Centre National de la Recherche Scientifique (CNRS), Advanced Lithium Energy Storage Systems - ALISTORE-ERI (ALISTORE-ERI), Institut de Chimie du CNRS (INC)-Centre National de la Recherche Scientifique (CNRS), Institut des sciences analytiques et de physico-chimie pour l'environnement et les materiaux (IPREM), Université de Pau et des Pays de l'Adour (UPPA)-Institut de Chimie du CNRS (INC)-Centre National de la Recherche Scientifique (CNRS), ANR-10-LABX-0076,STORE-EX,Laboratory of excellency for electrochemical energy storage(2010), Université de Picardie Jules Verne (UPJV)-Institut de Chimie du CNRS (INC)-Aix Marseille Université (AMU)-Université de Pau et des Pays de l'Adour (UPPA)-Université de Nantes (UN)-Université de Montpellier (UM)-Centre National de la Recherche Scientifique (CNRS)-Sorbonne Université (SU)-Ecole Nationale Supérieure de Chimie de Paris - Chimie ParisTech-PSL (ENSCP), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-Collège de France (CdF (institution))-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP ), Université Grenoble Alpes (UGA)-Université Grenoble Alpes (UGA)-Institut National Polytechnique (Toulouse) (Toulouse INP), Université Fédérale Toulouse Midi-Pyrénées-Université Fédérale Toulouse Midi-Pyrénées-Ecole Nationale Supérieure de Chimie de Montpellier (ENSCM), and Université de Picardie Jules Verne (UPJV)-Centre National de la Recherche Scientifique (CNRS)-Institut de Chimie du CNRS (INC)

Subjects
[CHIM.THEO]Chemical Sciences/Theoretical and/or physical chemistry, [CHIM.MATE]Chemical Sciences/Material chemistry
Abstract

cited By 8; International audience; This work sheds light on the exceptional robustness of anatase TiO 2 when it is downsized to an extreme value of 4â €‰nm. Since at this size the surface contribution to the volume becomes predominant, it turns out that the material becomes significantly resistant against particles coarsening with temperature, entailing a significant delay in the anatase to rutile phase transition, prolonging up to 1000â €‰°C in air. A noticeable alteration of the phase stability diagram with lithium insertion is also experienced. Lithium insertion in such nanocrystalline anatase TiO 2 converts into a complete solid solution until almost Li 1 TiO 2, a composition at which the tetragonal to orthorhombic transition takes place without the formation of the emblematic and unwished rock salt Li 1 TiO 2 phase. Consequently, excellent reversibility in the electrochemical process is experienced in the whole portion of lithium content.

Published
2015

41. Planck pre-launch status: The Planck mission

Author

Tauber, J, Mandolesi, N, Puget, J, Banos, T, Bersanelli, M, Bouchet, F, Butler, R, Charra, J, Crone, G, Dodsworth, J, Efstathiou, G, Gispert, R, Guyot, G, Gregorio, A, Juillet, J, Lamarre, J, Laureijs, R, Lawrence, C, NØRGAARD NIELSEN, H, Passvogel, T, Reix, J, Texier, D, Vibert, L, Zacchei, A, Ade, P, Aghanim, N, Aja, B, Alippi, E, Aloy, L, Armand, P, Arnaud, M, Arondel, A, ARREOLA VILLANUEVA, A, Artal, E, Artina, E, Arts, A, Ashdown, M, Aumont, J, Azzaro, M, Bacchetta, A, Baccigalupi, C, Baker, M, Balasini, M, Balbi, A, Banday, A, Barbier, G, Barreiro, R, Bartelmann, M, Battaglia, P, Battaner, E, Benabed, K, Beney, J, Beneyton, R, Bennett, K, Benoit, A, Bernard, J, Bhandari, P, Bhatia, R, Biggi, M, Biggins, R, Billig, G, Blanc, Y, Blavot, H, Bock, J, Bonaldi, A, Bond, R, Bonis, J, Borders, J, Borrill, J, Boschini, L, Boulanger, F, Bouvier, J, Bouzit, M, Bowman, R, Bréelle, E, Bradshaw, T, Braghin, M, Bremer, M, Brienza, D, Broszkiewicz, D, Burigana, C, Burkhalter, M, Cabella, P, Cafferty, T, Cairola, M, Caminade, S, Camus, P, Cantalupo, C, Cappellini, B, Cardoso, J, Carr, R, Catalano, A, Cayón, L, Cesa, M, Chaigneau, M, Challinor, A, Chamballu, A, Chambelland, J, Charra, M, Chiang, L, Chlewicki, G, Christensen, P, Church, S, Ciancietta, E, Cibrario, M, Cizeron, R, Clements, D, Collaudin, B, Colley, J, Colombi, S, Colombo, A, Colombo, F, Corre, O, Couchot, F, Cougrand, B, Coulais, A, Couzin, P, Crane, B, Crill, B, Crook, M, Crumb, D, Cuttaia, F, Dörl, U, DA SILVA, P, Daddato, R, Damasio, C, Danese, L, D'Aquino, G, D'Arcangelo, O, Dassas, K, Davies, R, Davies, W, Davis, R, DE BERNARDIS, P, DE CHAMBURE, D, DE GASPERIS, G, DE LA FUENTE, M, DE PACO, P, DE ROSA, A, DE TROIA, G, DE ZOTTI, G, Dehamme, M, Delabrouille, J, Delouis, J, Désert, F, DI GIROLAMO, G, Dickinson, C, Doelling, E, Dolag, K, Domken, I, Douspis, M, Doyle, D, Du, S, Dubruel, D, Dufour, C, Dumesnil, C, Dupac, X, Duret, P, Eder, C, Elfving, A, Enlin, T, Eng, P, English, K, Eriksen, H, Estaria, P, Falvella, M, Ferrari, F, Finelli, F, Fishman, A, Fogliani, S, Foley, S, Fonseca, A, Forma, G, Forni, O, Fosalba, P, Fourmond, J, Frailis, M, Franceschet, C, Franceschi, E, François, S, Frerking, M, GÓMEZ REÑASCO, M, Górski, K, Gaier, T, Galeotta, S, Ganga, K, GARCÍA LÁZARO, J, Garnica, A, Gaspard, M, Gavila, E, Giard, M, Giardino, G, Gienger, G, GIRAUD HERAUD, Y, Glorian, J, Griffin, M, Gruppuso, A, Guglielmi, L, Guichon, D, Guillaume, B, Guillouet, P, Haissinski, J, Hansen, F, Hardy, J, Harrison, D, Hazell, A, Hechler, M, Heckenauer, V, Heinzer, D, Hell, R, HENROT VERSILLÉ, S, HERNÁNDEZ MONTEAGUDO, C, Herranz, D, Herreros, J, Hervier, V, Heske, A, Heurtel, A, Hildebrandt, S, Hills, R, Hivon, E, Hobson, M, Hollert, D, Holmes, W, Hornstrup, A, Hovest, W, Hoyland, R, Huey, G, Huffenberger, K, Hughes, N, Israelsson, U, Jackson, B, Jaffe, A, Jaffe, T, Jagemann, T, Jessen, N, Jewell, J, Jones, W, Juvela, M, Kaplan, J, Karlman, P, Keck, F, Keihänen, E, King, M, Kisner, T, Kletzkine, P, Kneissl, R, Knoche, J, Knox, L, Koch, T, Krassenburg, M, KURKI SUONIO, H, Lähteenmäki, A, Lagache, G, Lagorio, E, Lami, P, Lande, J, Lange, A, Langlet, F, Lapini, R, Lapolla, M, Lasenby, A, LE JEUNE, M, Leahy, J, Lefebvre, M, Legrand, F, LE MEUR, G, Leonardi, R, Leriche, B, Leroy, C, Leutenegger, P, Levin, S, Lilje, P, Lindensmith, C, LINDEN VØRNLE, M, Loc, A, Longval, Y, Lubin, P, Luchik, T, Luthold, I, MACIAS PEREZ, J, Maciaszek, T, Mactavish, C, Madden, S, Maffei, B, Magneville, C, Maino, D, Mambretti, A, Mansoux, B, Marchioro, D, Maris, M, Marliani, F, Marrucho, J, MARTÍ CANALES, J, MARTÍNEZ GONZÁLEZ, E, MARTÍN POLEGRE, A, Martin, P, Marty, C, Marty, W, Masi, S, Massardi, M, Matarrese, S, Matthai, F, Mazzotta, P, Mcdonald, A, Mcgrath, P, Mediavilla, A, Meinhold, P, Mélin, J, Melot, F, Mendes, L, Mennella, A, Mervier, C, Meslier, L, Miccolis, M, MIVILLE DESCHENES, M, Moneti, A, Montet, D, Montier, L, Mora, J, Morgante, G, Morigi, G, Morinaud, G, Morisset, N, Mortlock, D, Mottet, S, Mulder, J, Munshi, D, Murphy, A, Murphy, P, Musi, P, Narbonne, J, Naselsky, P, Nash, A, Nati, F, Natoli, P, Netterfield, B, Newell, J, Nexon, M, Nicolas, C, Nielsen, P, Ninane, N, Noviello, F, Novikov, D, Novikov, I, O'Dwyer, I, Oldeman, P, Olivier, P, Ouchet, L, Oxborrow, C, PÉREZ CUEVAS, L, Pagan, L, Paine, C, Pajot, F, Paladini, R, Pancher, F, Panh, J, Parks, G, Parnaudeau, P, Partridge, B, Parvin, B, Pascual, J, Pasian, F, Pearson, D, Pearson, T, Pecora, M, Perdereau, O, Perotto, L, Perrotta, F, Piacentini, F, Piat, M, Pierpaoli, E, Piersanti, O, Plaige, E, Plaszczynski, S, Platania, P, Pointecouteau, E, Polenta, G, Ponthieu, N, Popa, L, Poulleau, G, Poutanen, T, Prézeau, G, Pradell, L, Prina, M, Prunet, S, Rachen, J, Rambaud, D, Rame, F, Rasmussen, I, Rautakoski, J, Reach, W, Rebolo, R, Reinecke, M, Reiter, J, Renault, C, Ricciardi, S, Rideau, P, Riller, T, Ristorcelli, I, Riti, J, Rocha, G, Roche, Y, Pons, R, Rohlfs, R, Romero, D, Roose, S, Rosset, C, Rouberol, S, ROWAN ROBINSON, M, RUBIÑO MARTÍN, J, Rusconi, P, Rusholme, B, Salama, M, Salerno, E, Sandri, M, Santos, D, Sanz, J, Sauter, L, Sauvage, F, Savini, G, Schmelzel, M, Schnorhk, A, Schwarz, W, Scott, D, Seiffert, M, Shellard, P, Shih, C, Sias, M, Silk, J, Silvestri, R, Sippel, R, Smoot, G, Starck, J, Stassi, P, Sternberg, J, Stivoli, F, Stolyarov, V, Stompor, R, Stringhetti, L, Strommen, D, Stute, T, Sudiwala, R, Sugimura, R, Sunyaev, R, Sygnet, J, Türler, M, Taddei, E, Tallon, J, Tamiatto, C, Taurigna, M, Taylor, D, Terenzi, L, Thuerey, S, Tillis, J, Tofani, G, Toffolatti, L, Tommasi, E, Tomasi, M, Tonazzini, E, Torre, J, Tosti, S, Touze, F, Tristram, M, Tuovinen, J, Tuttlebee, M, Umana, G, Valenziano, L, Vallée, D, VAN DER VLIS, M, VAN LEEUWEN, F, Vanel, J, VAN TENT, B, Varis, J, Vassallo, E, Vescovi, C, Vezzu, F, Vibert, D, Vielva, P, Vierra, J, Villa, F, Vittorio, N, Vuerli, C, Wade, L, Walker, A, Wandelt, B, Watson, C, Werner, D, White, M, White, S, Wilkinson, A, Wilson, P, Woodcraft, A, Yoffo, B, Yun, M, Yurchenko, V, Yvon, D, Zhang, B, Zimmermann, O, Zonca, A, Zorita, D, TAUBER J. A, MANDOLESI N, PUGET J. L, BANOS T, BERSANELLI M, BOUCHET F. R, BUTLER R. C, CHARRA J, CRONE G, DODSWORTH J, EFSTATHIOU G, GISPERT R, GUYOT G, GREGORIO A, JUILLET J. J, LAMARRE J. M, LAUREIJS R. J, LAWRENCE C. R, NØRGAARD NIELSEN H. U, PASSVOGEL T, REIX J. M, TEXIER D, VIBERT L, ZACCHEI A, ADE P. A. R, AGHANIM N, AJA B, ALIPPI E, ALOY L, ARMAND P, ARNAUD M, ARONDEL A, ARREOLA VILLANUEVA A, ARTAL E, ARTINA E, ARTS A, ASHDOWN M, AUMONT J, AZZARO M, BACCHETTA A, BACCIGALUPI C, BAKER M, BALASINI M, BALBI A, BANDAY A. J, BARBIER G, BARREIRO R. B, BARTELMANN M, BATTAGLIA P, BATTANER E, BENABED K, BENEY J. L, BENEYTON R, BENNETT K, BENOIT A, BERNARD J. P, BHANDARI P, BHATIA R, BIGGI M, BIGGINS R, BILLIG G, BLANC Y, BLAVOT H, BOCK J. J, BONALDI A, BOND R, BONIS J, BORDERS J, BORRILL J, BOSCHINI L, BOULANGER F, BOUVIER J, BOUZIT M, BOWMAN R, BRÉELLE E, BRADSHAW T, BRAGHIN M, BREMER M, BRIENZA, DANIELE, BROSZKIEWICZ D, BURIGANA C, BURKHALTER M, CABELLA, PAOLO, CAFFERTY T, CAIROLA M, CAMINADE S, CAMUS P, CANTALUPO C. M, CAPPELLINI B, CARDOSO J. F, CARR R, CATALANO, Andrea, CAYÓN L, CESA M, CHAIGNEAU M, CHALLINOR A, CHAMBALLU A, CHAMBELLAND J. P, CHARRA M, CHIANG L. Y, CHLEWICKI G, CHRISTENSEN P. R, CHURCH S, CIANCIETTA E, CIBRARIO M, CIZERON R, CLEMENTS D, COLLAUDIN B, COLLEY J. M, COLOMBI S, COLOMBO A, COLOMBO F, CORRE O, COUCHOT F, COUGRAND B, COULAIS A, COUZIN P, CRANE B, CRILL B, CROOK M, CRUMB D, CUTTAIA F, DÖRL U, DA SILVA P, DADDATO R, DAMASIO C, DANESE L, D'AQUINO G, D'ARCANGELO O, DASSAS K, DAVIES R. D, DAVIES W, DAVIS R. J, DE BERNARDIS, Paolo, DE CHAMBURE D, DE GASPERIS G, DE LA FUENTE M. L, DE PACO P, DE ROSA A, DE TROIA, Grazia, DE ZOTTI G, DEHAMME M, DELABROUILLE J, DELOUIS J. M, DÉSERT F. 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B, MELOT F, MENDES L, MENNELLA A, MERVIER C, MESLIER L, MICCOLIS M, MIVILLE DESCHENES M. A, MONETI A, MONTET D, MONTIER L, MORA J, MORGANTE G, MORIGI G, MORINAUD G, MORISSET N, MORTLOCK D, MOTTET S, MULDER J, MUNSHI D, MURPHY A, MURPHY P, MUSI P, NARBONNE J, NASELSKY P, NASH A, NATI, FEDERICO, NATOLI P, NETTERFIELD B, NEWELL J, NEXON M, NICOLAS C, NIELSEN P. H, NINANE N, NOVIELLO F, NOVIKOV D, NOVIKOV I, O'DWYER I. J, OLDEMAN P, OLIVIER P, OUCHET L, OXBORROW C. A, PÉREZ CUEVAS L, PAGAN L, PAINE C, PAJOT F, PALADINI R, PANCHER F, PANH J, PARKS G, PARNAUDEAU P, PARTRIDGE B, PARVIN B, PASCUAL J. P, PASIAN F, PEARSON D. P, PEARSON T, PECORA M, PERDEREAU O, PEROTTO L, PERROTTA F, PIACENTINI, Francesco, PIAT M, PIERPAOLI E, PIERSANTI O, PLAIGE E, PLASZCZYNSKI S, PLATANIA P, POINTECOUTEAU E, POLENTA, GIANLUCA, PONTHIEU N, POPA L, POULLEAU G, POUTANEN T, PRÉZEAU G, PRADELL L, PRINA M, PRUNET S, RACHEN J. P, RAMBAUD D, RAME F, RASMUSSEN I, RAUTAKOSKI J, REACH W. T, REBOLO R, REINECKE M, REITER J, RENAULT C, RICCIARDI, Sara, RIDEAU P, RILLER T, RISTORCELLI I, RITI J. B, ROCHA G, ROCHE Y, PONS R, ROHLFS R, ROMERO D, ROOSE S, ROSSET C, ROUBEROL S, ROWAN ROBINSON M, RUBIÑO MARTÍN J. A, RUSCONI P, RUSHOLME B, SALAMA M, SALERNO E, SANDRI M, SANTOS D, SANZ J. L, SAUTER L, SAUVAGE F, SAVINI, Giorgio, SCHMELZEL M, SCHNORHK A, SCHWARZ W, SCOTT D, SEIFFERT M. D, SHELLARD P, SHIH C, SIAS M, SILK J. I, SILVESTRI R, SIPPEL R, SMOOT G. F, STARCK J. L, STASSI P, STERNBERG J, STIVOLI, federico, STOLYAROV V, STOMPOR R, STRINGHETTI L, STROMMEN D, STUTE T, SUDIWALA R, SUGIMURA R, SUNYAEV R, SYGNET J. F, TÜRLER M, TADDEI E, TALLON J, TAMIATTO C, TAURIGNA M, TAYLOR D, TERENZI L, THUEREY S, TILLIS J, TOFANI G, TOFFOLATTI L, TOMMASI E, TOMASI M, TONAZZINI E, TORRE J. P, TOSTI S, TOUZE F, TRISTRAM M, TUOVINEN J, TUTTLEBEE M, UMANA G, VALENZIANO L, VALLÉE D, VAN DER VLIS M, VAN LEEUWEN F, VANEL J. C, VAN TENT B, VARIS J, VASSALLO E, VESCOVI C, VEZZU F, VIBERT D, VIELVA P, VIERRA J, VILLA F, VITTORIO N, VUERLI C, WADE L. A, WALKER A. R, WANDELT B. D, WATSON C, WERNER D, WHITE M, WHITE S. D. M, WILKINSON A, WILSON P, WOODCRAFT A, YOFFO B, YUN M, YURCHENKO V, YVON D, ZHANG B, ZIMMERMANN O, ZONCA A, and ZORITA D.

Abstract

The European Space Agency's Planck satellite, launched on 14 May 2009, is the third-generation space experiment in the field of cosmic microwave background (CMB) research. It will image the anisotropies of the CMB over the whole sky, with unprecedented sensitivity (${{\Delta T}\over T}$ ~ 2 × 10-6) and angular resolution (~5 arcmin). Planck will provide a major source of information relevant to many fundamental cosmological problems and will test current theories of the early evolution of the Universe and the origin of structure. It will also address a wide range of areas of astrophysical research related to the Milky Way as well as external galaxies and clusters of galaxies. The ability of Planck to measure polarization across a wide frequency range (30-350 GHz), with high precision and accuracy, and over the whole sky, will provide unique insight, not only into specific cosmological questions, but also into the properties of the interstellar medium. This paper is part of a series which describes the technical capabilities of the Planck scientific payload. It is based on the knowledge gathered during the on-ground calibration campaigns of the major subsystems, principally its telescope and its two scientific instruments, and of tests at fully integrated satellite level. It represents the best estimate before launch of the technical performance that the satellite and its payload will achieve in flight. In this paper, we summarise the main elements of the payload performance, which is described in detail in the accompanying papers. In addition, we describe the satellite performance elements which are most relevant for science, and provide an overview of the plans for scientific operations and data analysis.

Published
2010

42. Ag6Mo2O7F3Cl: A New Silver Cathode Material for Enhanced ICD Primary Lithium Batteries

Author

Sauvage, F., Bodenez, V., Tarascon, J.-M., and Poeppelmeier, K. R.

Abstract

As a potential cathode material for the ICD lithium battery, one advantage of Ag6Mo2O7F3Cl (SMOFC) is its enhanced gravimetric capacity of ca.133 mAh/g above 3 V (vs Li+/Li) delivered by two biphasic transitions at 3.46 and 3.39 V (vs Li+/Li). The unique crystal structure of SMOFC enables a high silver ion conduction: σ⊥[001]= 3.10−2S/cm (±2.10−2S/cm) and σ//[001]= 4.10−3S/cm (±2.10−3S/cm) and, hence, an excellent discharge rate capability. Lithium insertion has been monitored by in situXRD measurements with HRTEM investigations. There is a linear isotropic collapse of the structure leading to a fully amorphous structure beyond four inserted lithiums.

Published
2024
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43. Methods for the detection and the characterization of low mass companions using the IFS of SPHERE

Author

Zurlo, A., Mesa, D., Gratton, R., Claudi, R., Desidera, S., Giro, E., Beuzit, J.-L., Dohlen, K., Mouillet, D., Puget, P., Wildi, F., Feldt, M., Moeller-Nilsson, O., Baruffolo, A., Fantinel, D., Salasnich, B., Kasper, M., Costille, A., Sauvage, J.-F., Vigan, Arthur, Moutou, C., Langlois, M., Antichi, J., Pavlov, A., Zimmerman, N., Turatto, M., Ramsay, Suzanne, Mclean, Ian, Takami, Hideki, Sauvage, F., Laboratoire d'Astrophysique de Marseille (LAM), Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS), Department of Biochemistry and Molecular Biology, Mayo Clinic, INAF - Osservatorio Astronomico di Padova (OAPD), Istituto Nazionale di Astrofisica (INAF), Institut de Planétologie et d'Astrophysique de Grenoble (IPAG ), Observatoire des Sciences de l'Univers de Grenoble (OSUG), Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut national des sciences de l'Univers (INSU - CNRS)-Institut national de recherche en sciences et technologies pour l'environnement et l'agriculture (IRSTEA)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-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 des sciences de l'Univers (INSU - CNRS)-Institut national de recherche en sciences et technologies pour l'environnement et l'agriculture (IRSTEA)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS), Observatoire Astronomique de l'Université de Genève (ObsGE), Université de Genève = University of Geneva (UNIGE), Max-Planck-Institut für Astronomie (MPIA), Max-Planck-Gesellschaft, INAF - Osservatorio Astrofisico di Arcetri (OAA), Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Aix Marseille Université (AMU)-Centre National d'Études Spatiales [Toulouse] (CNES), and Université de Genève (UNIGE)

Subjects
Physics, Astrophysics::Instrumentation and Methods for Astrophysics, Astrophysics, Star (graph theory), Exoplanet, law.invention, Telescope, Speckle pattern, Stars, Integral field spectrograph, Planet, law, Astrophysics::Solar and Stellar Astrophysics, Deconvolution, Astrophysics::Earth and Planetary Astrophysics, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
Abstract

International audience; SPHERE is an instrument aimed to the search for low mass companions around young stars in the solar neighborhood. To achieve this goal light from the host star (and in particular the speckle pattern due to the telescope aberrations) should be strongly attenuated while avoiding to cancel out the light from the faint companion. Different techniques can be used to fulfill this aim exploiting the multi-wavelength datacube produced by the Integral Field Spectrograph that is one of the scientific modules that composes SPHERE. In particular we have tested the application of the Spectral Deconvolution and of the Principal Components Analysis techniques. Both of them allow us to obtained a contrast better than 10-5 with respect to the central star at separations of the order of 0.4 arcsec. A further improvement of one order of magnitude can be obtained by combining one of these techniques to the Angular Differential Imaging. To investigate the expected performance of IFS in characterizing detected objects we injected in laboratory data synthetics planets with different intrinsic fluxes and projected separations from the host star. We performed a complete astrometric and photometric analysis of these images to evaluate the expected errors on these measurements, the spectral fidelity and the differences between the reduction methods. The main issue is to avoid the strong self-cancellation that is inherent to all the reduction methods. We have in particular tested two possible solutions: the use of a mask during the reduction on the positions of the companions or, alternatively, using a KLIP procedure for the IFS. This latter seems to give better results in respect o the classical PCA, allowing us to obtain a good spectral reconstruction for simulated objects down to a contrast of ~10-5.

Published
2014

44. SPHERE/IRDIS: final performance assessment of the dual-band imaging and long slit spectroscopy modes

Author

Vigan, Arthur, Langlois, M., Dohlen, K., Zurlo, A., Moutou, C., Costille, A., Gry, C., Madec, F., Le Mignant, D., Gluck, Laurence, Sauvage, J.-F., Ramsay, Suzanne, McLean, Ian, Takami, Hideki, Sauvage, F., Laboratoire d'Astrophysique de Marseille (LAM), Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Aix Marseille Université (AMU)-Centre National d'Études Spatiales [Toulouse] (CNES), and Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)

Subjects
Physics, business.industry, Near-infrared spectroscopy, Astrophysics::Instrumentation and Methods for Astrophysics, 01 natural sciences, Exoplanet, law.invention, 010309 optics, Optics, Planet, law, Observatory, 0103 physical sciences, Astrophysics::Earth and Planetary Astrophysics, Multi-band device, business, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], 010303 astronomy & astrophysics, Spectrograph, Coronagraph, Long-slit spectroscopy
Abstract

International audience; The near-infrared imager and spectrograph IRDIS is one of the three science sub-systems of VLT/SPHERE dedicated to the detection and characterization of giant exoplanets at large orbital radii. It offers a wide range of observational modes including dual-band imaging (DBI) with very low differential aberrations, and long slit spectroscopy (LSS) coupled with a classical Lyot coronagraph at low (R = ~50) and medium (R = ~330) resolution. Over the course of 2012 and 2013, IRDIS has been extensively tested in laboratory during the integration and optimization of the SPHERE system. At the beginning of 2014, the instrument has been shipped to Chile and has been reintegrated at the Paranal observatory. We present here a detailed summary of the performance of the DBI and LSS modes obtained in laboratory. We provide a wide range of results covering different observing conditions and setups for the DBI mode, and we show that the instrument reaches the technical specifications in terms of contrast. We also identify some of the limitations that prevent going down much further in contrast while testing in the laboratory. For the LSS mode, we present results obtained both at low and medium resolution in the main setups that will be offered to future users. We demonstrate that the LSS mode will provide a useful characterization tool for the planets detected in DBI mode. Finally, we present the first results obtained on-sky during the first commissioning run of SPHERE at the VLT.

Published
2014

45. Comparaison de la toxicité de l’amphotéricine B liposomale et désoxycholate sur des cellules épithéliales alvéolaires par mesures de l’impédance cellulaire en temps réel et du niveau d’expression de gènes de cytokines pro-inflammatoires

Author

Menotti, J., primary, Alanio, A., additional, Sturny-Leclere, A., additional, Vitry, S., additional, Sauvage, F., additional, Dromer, F., additional, Barratt, G., additional, and Bretagne, S., additional

Published
2016
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48. Une analyse préliminaire de dix ans de suivi individuel de campagnole roussatre, le réservoir du hantavirus Puumala, dans la zone d'endémie (Ardennes)

Author

Margin-Bottom, P., Laurent Crespin, Augot, D., François Boué, Pons, J. -. B., Marianneau, P., Sauvage, F., Laboratoire de Biométrie et Biologie Evolutive - UMR 5558 (LBBE), Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut National de Recherche en Informatique et en Automatique (Inria)-VetAgro Sup - Institut national d'enseignement supérieur et de recherche en alimentation, santé animale, sciences agronomiques et de l'environnement (VAS)-Centre National de la Recherche Scientifique (CNRS), Unité de Recherche d'Épidémiologie Animale (UR EpiA), Institut National de la Recherche Agronomique (INRA), Agence nationale de sécurité sanitaire de l'alimentation, de l'environnement et du travail (ANSES), Unité de Virologie, and Institut de Recherches Biomédicales des Armées

Subjects
[SDV]Life Sciences [q-bio], HANTAVIRUS, ZOONOSE, ESPECE RESERVOIR, ComputingMilieux_MISCELLANEOUS
Abstract

National audience

Published
2013

49. Strain effect on extracellular laccase activities from <italic>Botrytis cinerea</italic>.

Author

Quijada‐Morin, N., Garcia, F., Lambert, K., Walker, A.‐S., Tiers, L., Viaud, M., Sauvage, F.‐X., Hirtz, C., and Saucier, C.

Subjects
LACCASE, BOTRYTIS cinerea, EXTRACELLULAR enzymes, FUNGAL enzymes, OXIDATION of phenols, GLYCOSYLATION
Abstract

Abstract: Background and Aims: Laccase enzymes produced by Botrytis cinerea are involved in the oxidation of phenolic substances during the development of grey mould, which causes significant economic losses. The aim of this work was to study the structural and activity characteristics of the laccase enzymes secreted by three B. cinerea strains that are involved in the development of grey mould. Methods and Results: Laccase enzymes obtained from three B. cinerea strains [one reference strain (B05.10) and two strains obtained from two French vineyards (VA612 and RM344)] were characterised. Analysis by LC‐QTOF‐MS revealed that the three strains contained a mixture of Laccase‐2‐BcLCC2 and Laccase‐3‐BcLCC7. The structural characteristics of the laccases from the three strains, such as molecular weight and glycosylation degree, were identical. Nevertheless, their catalytic activities were significantly different. Conclusions: Differences in catalytic activities could be due either to possible differences in the relative amount of Laccase‐2‐BcLCC2 and Laccase‐3‐BcLCC7 produced by each strain or to differences in the glycosidic fraction of the enzymes. Significance of the Study: The severity of the infection caused by B. cinerea may be not only related to the infection level but also to the strain involved. [ABSTRACT FROM AUTHOR]

Published
2018
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