1,183 results on '"Baudin, F"'
Search Results
202. Red giants observed by CoRoT and APOGEE: The evolution of the Milky Way’s radial metallicity gradient
- Author
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Anders, F., primary, Chiappini, C., additional, Minchev, I., additional, Miglio, A., additional, Montalbán, J., additional, Mosser, B., additional, Rodrigues, T. S., additional, Santiago, B. X., additional, Baudin, F., additional, Beers, T. C., additional, da Costa, L. N., additional, García, R. A., additional, García-Hernández, D. A., additional, Holtzman, J., additional, Maia, M. A. G., additional, Majewski, S., additional, Mathur, S., additional, Noels-Grotsch, A., additional, Pan, K., additional, Schneider, D. P., additional, Schultheis, M., additional, Steinmetz, M., additional, Valentini, M., additional, and Zamora, O., additional
- Published
- 2017
- Full Text
- View/download PDF
203. Antifungal therapy for patients with proven or suspected Candida peritonitis: Amarcand2, a prospective cohort study in French intensive care units
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Montravers, P., primary, Perrigault, P.F., additional, Timsit, J.F., additional, Mira, J.P., additional, Lortholary, O., additional, Leroy, O., additional, Gangneux, J.P., additional, Guillemot, D., additional, Bensoussan, C., additional, Bailly, S., additional, Azoulay, E., additional, Constantin, J.M., additional, Dupont, H., additional, Aait Hssain, A., additional, Adda, M., additional, Allaouchiche, B., additional, Ammenouche, N., additional, Angel, G., additional, Argaud, L., additional, Badetti, C., additional, Baldesi, O., additional, Barthet, M.C., additional, Bastien, O., additional, Baudin, F., additional, Bellec, F., additional, Blasco, G., additional, Bollaert, P.E., additional, Bonadona, A., additional, Bretonniere, C., additional, Brocas, E., additional, Brua, S., additional, Bruder, N., additional, Brunin, G., additional, Cabaret, P., additional, Carpentier, D., additional, Cartier, J.C., additional, Cerf, C., additional, Chabanne, R., additional, Charles, P.E., additional, Cheval, C., additional, Cinotti, R., additional, Cohen, Y., additional, Cousson, J., additional, Delpierre, E., additional, Demory, D., additional, Diconne, E., additional, Du Cheyron, D., additional, Dubost, C., additional, Dumenil, A.S., additional, Durand, M., additional, Duroy, E., additional, Forel, J.M., additional, Foucher-Lezla, A.L., additional, Fratea, S., additional, Gally, J., additional, Gaudard, P., additional, Geffe, P., additional, Gergaud, S., additional, Gette, S., additional, Girault, C., additional, Goubaux, B., additional, Gouin, P., additional, Grenot, R., additional, Grossmith, G., additional, Guelon, D., additional, Guerin-Robardey, A.M., additional, Guervilly, C., additional, Hayl-Slayman, D., additional, Hilbert, G., additional, Houissa, H., additional, Hraiech, S., additional, Ichai, P., additional, Jung, B., additional, Kaidomar, M., additional, Karoubi, P., additional, Kherchache, A., additional, Lambiotte, F., additional, Lamhaut, L., additional, Launoy, A., additional, Lebreton, F., additional, Lefrant, J.Y., additional, Lemaire, C., additional, Lepape, A., additional, Lepoivre, T., additional, Lesieur, O., additional, Levy, B., additional, Luyt, C.E., additional, Mahe, P.J., additional, Mahul, P., additional, Mateu, P., additional, Megarbane, B., additional, Merle, J.C., additional, Montcriol, A., additional, Mootien, Y., additional, Navellou, J.C., additional, Ouattara, A., additional, Page, B., additional, Petitpas, F., additional, Plantefeve, G., additional, Quinart, A., additional, Quintard, H., additional, Ragonnet, B., additional, Roquilly, A., additional, Ruiz, J., additional, Saliba, F., additional, Samba, D., additional, Schmitt, Z., additional, Seguin, P., additional, Sejourne, C., additional, Tellier, A.C., additional, Thevenot, F., additional, Tonnelier, J.M., additional, Van Grunderbeek, N., additional, Vincent, J.F., additional, Wiramus, S., additional, and Zogheib, E., additional
- Published
- 2017
- Full Text
- View/download PDF
204. Galactic archaeology with asteroseismology and spectroscopy: Red giants observed by CoRoT and APOGEE
- Author
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Anders, F., primary, Chiappini, C., additional, Rodrigues, T. S., additional, Miglio, A., additional, Montalbán, J., additional, Mosser, B., additional, Girardi, L., additional, Valentini, M., additional, Noels, A., additional, Morel, T., additional, Johnson, J. A., additional, Schultheis, M., additional, Baudin, F., additional, de Assis Peralta, R., additional, Hekker, S., additional, Themeßl, N., additional, Kallinger, T., additional, García, R. A., additional, Mathur, S., additional, Baglin, A., additional, Santiago, B. X., additional, Martig, M., additional, Minchev, I., additional, Steinmetz, M., additional, da Costa, L. N., additional, Maia, M. A. G., additional, Allende Prieto, C., additional, Cunha, K., additional, Beers, T. C., additional, Epstein, C., additional, García Pérez, A. E., additional, García-Hernández, D. A., additional, Harding, P., additional, Holtzman, J., additional, Majewski, S. R., additional, Mészáros, Sz., additional, Nidever, D., additional, Pan, K., additional, Pinsonneault, M., additional, Schiavon, R. P., additional, Schneider, D. P., additional, Shetrone, M. D., additional, Stassun, K., additional, Zamora, O., additional, and Zasowski, G., additional
- Published
- 2016
- Full Text
- View/download PDF
205. Traitement et évolution des infections ostéoarticulaires aiguës communautaires chez l’enfant sain : étude rétrospective monocentrique de 64 cas
- Author
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Lemoine, A., primary, Baudin, F., additional, Vialle, R., additional, and Grimprel, E., additional
- Published
- 2016
- Full Text
- View/download PDF
206. Stellar classification of CoRoT targets
- Author
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Damiani, C., primary, Meunier, J.-C., additional, Moutou, C., additional, Deleuil, M., additional, Ysard, N., additional, Baudin, F., additional, and Deeg, H., additional
- Published
- 2016
- Full Text
- View/download PDF
207. Paléoenvironnements et caractérisation des roches mères carbonatées du bassin aquitain
- Author
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Bastianini, L., Hoareau, Guilhem, Caline, B., Martinez, C., Baudin, F., Guy, L., Bonnel, Cédric, Laboratoire des Fluides Complexes et leurs Réservoirs (LFCR), Centre National de la Recherche Scientifique (CNRS)-Université de Pau et des Pays de l'Adour (UPPA)-TOTAL FINA ELF, Centre scientifique et Technique Jean Feger (CSTJF), TOTAL FINA ELF, Institut d'astrophysique spatiale (IAS), Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris-Sud - Paris 11 (UP11), Solvay Silica, and Solvay (France)
- Subjects
[PHYS]Physics [physics] ,[PHYS.MECA.MEMA]Physics [physics]/Mechanics [physics]/Mechanics of materials [physics.class-ph] ,[SDU.STU.GP]Sciences of the Universe [physics]/Earth Sciences/Geophysics [physics.geo-ph] ,[SPI.MECA.MEMA]Engineering Sciences [physics]/Mechanics [physics.med-ph]/Mechanics of materials [physics.class-ph] ,[PHYS.MECA.GEME]Physics [physics]/Mechanics [physics]/Mechanical engineering [physics.class-ph] ,[SPI.MECA.MEFL]Engineering Sciences [physics]/Mechanics [physics.med-ph]/Fluids mechanics [physics.class-ph] - Abstract
ACT; International audience
- Published
- 2015
208. French Intensive Care Society, International congress - Réanimation 2016
- Author
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Jaillette, E, Girault, C, Brunin, G, Zerimech, F, Chiche, A, Broucqsault Dedrie, C, Fayolle, C, Minacori, F, Alves, I, Barrailler, S, Robriquet, L, Delaporte, E, Thellier, D, Delcourte, C, Duhamel, A, Nseir, S, Valette, X, Desmeulles, I, Savary, B, Masson, R, Seguin, A, Daubin, C, Sauneuf, B, Verrier, P, Pottier, V, Orabona, M, Samba, D, Viquesnel, G, Lermuzeaux, M, Hazera, P, Hanouz, J, Parienti, J, Du Cheyron, D, Demoule, A, Clavel, M, Rolland Debord, C, Perbet, S, Terzi, N, Kouatchet, A, Wallet, F, Roze, H, Vargas, F, Guérin, C, Dellamonica, J, Jaber, S, Similowski, T, Quenot, J, Binquet, C, Vinsonneau, C, Barbar, S, Vinault, S, Deckert, V, Lemaire, S, Hssain, A, Bruyère, R, Souweine, B, Lagrost, L, Adrie, C, Jung, B, Daurat, A, De Jong, A, Chanques, G, Mahul, M, Monnin, M, Molinari, N, Lheureux, O, Trepo, E, Hites, M, Cotton, F, Wolff, F, Surin, R, Créteur, J, Vincent, J, Gustot, T, Jacobs, F, Taccone, F, Neuville, M, Timsit, J, El Helali, N, Le Monnier, A, Magalhaes, E, Radjou, A, Smonig, R, Soubirou, J, Voiriot, G, Sonneville, R, Bouadma, L, Mourvillier, B, Gélisse, E, Brasseur, A, Roisin, S, De Backer, D, Van Ruychevelt, V, Carlier, E, Piagnerelli, M, Vanhaeverbeek, M, Danguy, C, Biston, P, Au, S, Begot, E, Dalmay, F, Repessé, X, Prat, G, Bouferrache, K, Slama, M, Vieillard Baron, A, Monnet, X, Marik, P, Teboul, J, Jozwiak, M, Richard, C, Chauvet, J, El Dash, S, Delastre, O, Bouffandeau, B, Jusserand, D, Michot, J, Bauer, F, Brazier, F, Mercado, P, Kontar, L, Titeca, D, De Cagny, B, Bacari Risal, G, Riviere, A, Maizel, J, Guillot, C, Le Reun, C, Lampin, M, Sadik, A, Botte, A, Leteurtre, S, Collins, A, Kempeneers, C, Cajgfinger, N, Ohlmann, C, Pouyau, R, Subtil, F, Baudin, F, Massenavette, B, Javouhey, E, Milesi, C, Essouri, S, Liet, J, Afanetti, M, Durand, S, Durand, P, Roze, J, Dupont, D, Cambonie, G, Soyer, B, Rusca, M, Lukaszewicz, A, Crassard, I, Guichard, J, Bresson, D, de la Garanderie, D, Cantier, M, Sabben, C, Louedec, L, Delbosc, S, Journé, C, Ou, P, Klein, I, Chau, F, Lefort, A, Desilles, J, Michel, J, Mazighi, M, Salem, O, Demeret, S, Bolgert, F, Sharshar, T, Grabli, D, Arib, S, Crippa, I, Soummer, A, Engrand, N, Guedin, P, Aldea, S, Cerf, C, Desailly, V, Pasquier, P, Brun, P, Roux, D, Latournerie, G, Kasprzyk, L, Grosjean, V, Latreche, A, Habert, P, Huot, S, Jobin, T, Tesnière, A, Dreyfuss, D, Ricard, J, Mignon, A, Gaudry, S, Laithier, F, Kimmoun, A, Chouihed, T, Albizzati, S, Camenzind, E, Vanhuyse, F, Levy, B, Cour, M, Venet, F, Hernu, R, Demaret, J, Monneret, G, Argaud, L, Dumas, F, Lamhaut, L, Rosencher, J, Pène, F, Varenne, O, Carli, P, Jouven, X, Spaulding, C, Cariou, A, Geri, G, Bonnetain, F, Marijon, E, Empana, J, Mirouse, A, Resche Rigon, M, Mayaux, J, Rabbat, A, Meert, A, Benoit, D, Bruneel, F, Azoulay, E, Dupuis, C, Schwebel, C, Ruckly, S, Goldgran Toledano, D, Marcotte, G, Lafarge, A, Pichereau, C, Theodose, I, Scotto, M, Kemlin, D, Ghrenassia, E, Schlemmer, B, Vimpere, D, Galicier, L, Contou, D, Guérot, E, Grimaldi, D, Ricome, S, Maury, E, Plantefève, G, Dessap, A, Brun Buisson, C, de Prost, N, Dubé, B, Delemazure, J, Dres, M, Rousseau, L, Drouot, X, Diaz, V, Rebollar, Y, Frat, J, Thille, A, Aissa, D, Coquet, P, Ruiz, J, Ferre, F, Hoarau, L, Riu Poulenc, B, Bataille, B, Silva, S, Baudel, J, Bigé, N, Tahiri, J, Dubée, V, Guidet, B, Ait Oufella, H, Jinglun, L, Shen, F, Bailly, S, Leroy, O, Montravers, P, Constantin, J, Dupont, H, Guillemot, D, Lortholary, O, Perrigault, P, Gangneux, J, Razazi, K, Mekontso Dessap, A, Jansen, C, Lecronier, M, Sandrine, V, Mira, J, Blein, S, Marin, N, Rousseau, C, Charpentier, J, Pachot, A, Hraiech, S, Bordes, J, De, L, Mège, J, Forel, J, Guervilly, C, Adda, M, Raoult, D, Papazian, L, Kentish Barnes, N, Cohen Solal, Z, Souppart, V, Kerhuel, L, Haubertin, C, Exbrayat, I, Rozières, E, Argain, A, Suc, A, Vignes, M, Cougot, P, Fourcade, O, Brunel, E, Messika, J, Tubach, F, Dubief, E, Pasquet, B, Guillo, S, Pierron, C, Grimaud, M, Farnoux, C, Maillard, A, Decavèle, M, Prodanovic, H, Idbaih, A, Alentorn, A, Delattre, J, De Montmollin, E, Brule, N, Conrad, M, Dailler, F, Navellou, J, Alves, M, Tonnelier, J, Picard, G, Rogemond, V, Honnorat, J, Marzorati, C, Lebert, C, Perez, P, Citerio, G, Legriel, S, Tripon, S, Mallet, M, Rudler, M, Imbert Bismut, F, Thabut, D, Canet, E, Faguer, S, Moreau, A, Barbier, F, Merceron, S, Guitton, C, Labadie, F, Lemiale, V, Faucher, E, Klouche, K, Chevret, S, Ragot, S, Coudroy, R, Boulain, T, Jamet, A, Mercat, A, Brochard, L, Roux, A, Franchineau, G, Brechot, N, Lebreton, G, Hekimian, G, Nieszkowska, A, Leprince, P, Trouillet, J, Combes, A, Schmidt, M, Barrot, L, Piton, G, Bailey, M, Panwar, R, Belin, N, Belon, F, Patry, C, Grandperrin, M, Chaignat, C, Labro, G, Vivet, B, Capellier, G, Daix, T, Guérin, E, Tavernier, E, Mercier, E, Gissot, V, Vallejo, C, François, B, Ravry, C, Pichon, N, Chapellas, C, Fedou, A, Galy, A, Ploy, M, Barraud, O, Vignon, P, Thooft, A, Conotte, R, Colet, J, Le Dorze, M, Tarazona, V, Brumpt, C, Moins Teisserenc, H, Uhel, F, Azzaoui, I, Gregoire, M, Pangault, C, Dulong, J, Cynober, L, Roussel, M, Le Tulzo, Y, Tarte, K, Demiselle, J, Auchabie, J, Dequin, P, Chudeau, N, Fourrier, F, Grange, S, Piquilloud, L, Lautrette, A, Boyer, S, Letheulle, J, Lerolle, N, Truche, A, Clec'H, C, Zaoui, P, Laurent, V, Toledano, D, Ragey, S, Gros, A, Dumenil, A, Jamali, S, Darmon, M, Chouraqui, M, Dewitte, A, Chastel, B, Carles, P, Fleureau, C, Joannes Boyau, O, Ouattara, A, Joseph, A, Garrouste Orgeas, M, Max, A, Lerin, T, Grégoire, C, Kloeckner, M, Bruel, C, Brochon, S, Philippart, F, Pichot, E, Simons, C, Flint, A, Aubron, C, Bellomo, R, Pilcher, D, Cheng, A, Hegarty, C, Martinelli, A, Howden, B, Reade, M, Mcquilten, Z, Bretonnière, C, Villers, D, Soares, M, Gonzalez, F, Vincent, F, Fauché, C, Gay, S, Skowron, O, Levrat, A, Dorez, D, Foucrier, A, Pease, S, Gauss, T, Paugam, C, Gorham, J, Ameye, L, Paesmans, M, Berghmans, T, Sculier, J, Deras, P, Martinez, O, Latry, P, Capdevila, X, Charbit, J, Jaubert, J, Etiennar, C, Ginoux, L, Sebbah, J, Haouache, H, Dhonneur, G, Cheikh, C, Moussaid, I, Ghazaoui, O, Belkadi, K, El Youssoufi, S, Salmi, S, Pajot, L, Zuber, B, Bedos, J, Dupont, B, Eugène, A, Galateau Sallé, F, Michard, B, Lebas, B, Boivin, A, Guillot, M, Harlay, M, Janssen Langenstein, R, Schenck, M, Ellero, B, Woehl Jaegle, M, Besch, C, Castelain, V, Bachellier, P, Schneider, F, Camus, C, Saliba, F, Goubaux, B, Bonadona, A, Lavayssiere, L, Quinart, A, Barbot, O, Dharancy, S, Delafosse, B, Barraud, H, Galbois, A, Veber, B, Cayot, S, Souche, B, Locher, C, Roux, O, Figorilli, F, Putignano, A, Houssel, P, Francoz, C, Weiss, E, Agarwal, B, Jalan, R, Durand, F, Ghezala, H, Daoudi, R, Kaddour, M, Ghadhoune, H, Rachedi, E, Guissouma, J, Ben Slimene, A, Azzeza, W, Brahmi, H, Elghord, H, Kada, A, Chikh, R, Slimani, R, A. Bouyoucef, K, Regaieg, K, Kamilia, C, Baccouche, N, Turki, O, Chaari, A, Ben, H, Bouaziz, M, Medhioub, F, Zekri, M, Rgieg, K, Bhimada, C, Mounir, B, Lang, E, Welschbillig, S, Perrin, M, Devys, J, Benbernou, S, Mokhtari Djebli, H, Ilies, S, Bouyacoub, K, Azza, A, Zogheib, E, Nader, J, Villeret, L, Guilbart, M, Besserve, P, Caus, T, Mastroianni, C, Santi, F, Hékimian, G, Pascal, L, Chastre, J, Perrier, V, Deniau, B, Klasen, F, Ponthus, J, Ngasseu, P, Amilien, V, Barsam, E, Lehericey, P, Tchir, M, Georger, J, Puech, B, Vandroux, D, Roussiaux, A, Belcour, D, Ferdynus, C, Martinet, O, Jabot, J, Fresco, M, Demeilliers Pfister, G, Merle, V, Brunel, V, Dureuil, B, Leydier, S, Clerc Urmes, I, Lemarie, J, Maigrat, C, Cravoisy Popovic, A, Barraud, D, Nace, L, Gibot, S, Agrinier, N, Bollaert, P, Daban, J, Boutonnet, M, Dumas, G, Falzone, E, Jault, P, Lenoir, B, Makunza, J, Mejeni, N, Mazaud, A, Béague, S, Rousselle, A, Durocher, A, Grinea, A, Bedoui, N, Stoian, A, Baboi, L, Gobert, F, Yonis, H, Tapponier, R, Bruyneel, A, Bonus, T, Cuvelier, G, Machayeckhi, S, Olieuz, S, Legrand, A, Feki, F, Jamoussi, A, Merhebene, T, Braham, E, Ghariani, A, Mezni, F, Slim, L, Khelil, J, Besbes, M, Marchalot, A, Beduneau, G, Carpentier, D, Besnier, E, Gastaldi, G, Abily, J, Beuzelin, M, Nay, M, Mankikian, J, Hervé, V, Soulie, M, Cronier, P, Kantor, E, Federici, L, Gilbert, M, Mezhari, I, Choukroun, G, Marque, S, Coppere, Z, Fulgencio, J, Blayau, C, Pham, T, Djibre, M, Reffienna, M, Lefort, S, Debue, A, Daviaud, F, Cabon, S, Addou, Z, Douah, A, Moussati, M, Belhabiche, K, Aouffen, N, Soulier, S, Mauriat, P, Tafer, N, Mortamet, G, Amaddeo, A, Khirani, S, Fauroux, B, Khanes, G, Liutko, O, Bidnenko, S, Doye, E, Voirin, N, Maucort Boulch, D, Kolev Descamp, K, Aouane, I, Essid, A, Hammami, W, Haegy, I, Bataille, J, Bergounioux, J, Morin, L, Ray, S, Maclaren, G, Nadel, S, Kneyber, M, Peters, M, Jansen, K, De Luca, D, Wilson, C, Schlapbach, L, Tissières, P, Girard, A, Savajols, E, Burguet, A, Semama, D, Litzler Renault, S, Fredj, H, Hassouna, M, Hechmi, Y, Cherif, M, Zouheir, J, Dernane, A, Bouakkaz, F, Taleb, L, Zeddine Mouhsen, A, Lyazidi, A, Richard, J, Mouhsen, A, Harmouchi, M, Rattal, M, Huck, M, Leclerc, T, Donat, N, Cirodde, A, Schaal, J, Masson, Y, Hoffmann, C, Cerland, L, Valentino, R, Chabartier, C, Villain Coquet, L, Ferge, J, Brouste, Y, Mehdaoui, H, Louriz, M, Madani, N, Amlaiky, F, Dendane, T, Abidi, K, Zekraoui, A, Zeggwagh, A, Abouqal, R, Brahim, A, Ferhi, F, Bouslama, M, Benjazia, K, Zeineb, A, Mahassen, D, Cadiet, J, Ferron, M, Prat, V, Erraud, A, Aillerie, V, Mevel, M, Grabherr, A, Chatham, J, Gauthier, C, Lauzier, B, Rozec, B, Joffre, J, Loyer, X, Lavillegrand, J, Zeboudj, L, Laurans, L, Esposito, B, Tedgui, A, Mallat, Z, Wei, C, Kattani, N, Louis, H, Orlowski, S, Tharaux, P, Burban, M, Meyer, G, Olland, A, Yver, B, Toti, F, Schini Kerth, V, Monnier, A, Leborgne, P, Meziani, F, Clavier, T, Paulus, M, Castel, H, Richard, V, Pons, S, Skurnik, D, Six, S, Jaffal, K, 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Deboscker, S, Harley, M, Lavigne, T, Brunet, J, Canoville, B, Lellouche, F, L'Her, E, Bouchard, P, Delorme, M, Elfaramawy, T, Gosselin, B, Guegan, S, Michotte, J, Staderini, E, Dugernier, J, Rusu, R, Liistro, G, Reychler, G, Simon, M, Essoukaki, E, Duprez, F, Contal, O, Trabelsi, B, Garsallah, H, Harira, K, Rafat, C, Mariotte, E, Le Jeune, C, Roy, P, Michallet, M, Zerbib, Y, Blot, F, Bornstain, C, Gelinotte, S, Rigaud, J, Tamion, F, Bouteloup, M, Nouira, H, Boisramé Helms, J, Degirmenci, S, Kummerlen, C, Delile, E, Thiébaut, P, Do Rego, J, Coquerel, D, Nevière, R, Ichou, L, Carbonell, N, Rautou, P, Nousbaum, J, Renou, C, Anty, R, Landraud, L, Lecron, J, Helary, M, Paillot, J, Pili Floury, S, Khedher, S, Maoui, A, Ezzamouri, A, Salem, M, Kerdjana, L, Dumitrescu, M, Mimoz, O, Debaene, B, Migeot, V, Dahyot Fizelier, C, Champigneulle, B, Zafrani, L, Lascarrou, J, Lissonde, F, Le Thuaut, A, Reignier, J, Platon, L, Lambert, J, Lagier, D, Brun, J, Sannini, A, Chow Chine, L, Bisbal, M, Faucher, M, Mokart, D, la Mourtada, L, Virgnie, L, Gaudet, A, Parmentier Decrucq, E, De Freitas Caires, N, Dubucquoi, S, Lassalle, P, Mathieu, D, Tapponnier, R, Quintin, L, Pichot, C, Petitjeans, F, Guillon, A, Jouan, Y, Breah, D, Gueugnon, F, Dalloneau, E, Baranek, T, Henry, C, Morello, E, Renauld, J, Pichavant, M, Gosset, P, Courty, Y, Diot, P, Si Tahar, M, Tadié, J, Vuillard, C, La Combe, B, Ponsin, P, Boddaert, G, Grand, B, Baudoin, Y, Bonnet, S, Snouda, S, Abbes, M, Benchiekh, I, Sedghiani, I, Maaroufi, N, Belayachi, J, Debono, L, Auvet, A, Nadal Desbarats, L, Tankovic, J, Dahoumane, R, Oufella, H, Offenstadt, G, Filali, A, Faure, E, Van Grunderbeeck, N, Nigeon, O, Bazus, H, Mallat, J, Thevenin, D, Lempereur Legros, S, Ledoux, D, Nys, M, Clermont, O, Aubry, A, Fernandes, R, Venot, M, Garnaud, C, Cornet, M, Pavese, P, Foroni, L, Boisset, S, le Maubon, D, Abid, M, Ezzouine, H, Edith, C, Sztrymf, B, Brunot, V, Serre, J, Landreau, L, Jean Michel, V, Couturaud, F, Moore, E, Egreteau, P, Boles, J, Herbrecht, J, Kaeuffer, C, Meyer, A, Arfi, K, Lesage, F, Séguret, S, Dupic, L, De Saint Blanquat, L, Baptiste, A, Georges, H, Delannoy, P, Devos, P, Albarracin, D, Ducousso Lacaze, A, Dufour, J, Cabasson, S, Veinstein, A, Chatellier, D, Robert, R, Ha, V, Lau, N, Mimoun, L, Forceville, X, Maamar, A, Chevalier, S, Botoc, V, Rouleau, S, Desachy, A, Calvat, S, Lafon, C, Cracco, C, Temime, J, Molmy, P, Gasan, G, Béranger, A, Chappuy, H, Bertrand, P, Beurton, A, Bodet Contentin, L, Danin, P, Dubois, E, Karaca, Y, Mora, P, Vodovar, D, Desbrosses, Y, Chauchet, A, Daguindau, E, Deconinck, E, Chermak, A, Baron, M, Calvet, L, Sapin, A, Pereira, B, Vettoretti, L, Lacroix, J, Clayton, L, Sabri, E, Bardiaux, L, Tiberghien, P, Hebert, P, Lengliné, E, Socié, G, Borcoman, E, Rusinova, K, Del Galy, A, Mercier, M, Hamel, J, Raveau, T, Moles, M, Clavert, A, Hunault Berger, M, Ifrah, N, Schmidt Tanguy, A, Carreira, S, Lavault, S, Pallanca, O, Morawiec, E, Arnulf, I, D'Humières, T, Carrié, C, Gisbert Mora, C, Bonnardel, E, Biais, M, Hilbert, G, Joannon, T, Marincamp, A, Chiche, J, Ferre, A, Lichtenstein, D, Meziere, G, Gonzalez, C, Hamzaoui, O, Geffriaud, T, Leleu, F, Boissier, F, Cuquemelle, E, Lim, P, Amara, R, Léger, J, Jacob, C, Bouferache, K, Ragot, C, Corradi, L, Maurice, L, Julliand, S, Deho, A, Le Bourgeois, F, Jacquot, A, Valla, F, Letois, F, Salvadori, A, Ottonello, G, Blanot, S, Montmayeur, J, Orliaguet, G, Tarmiz, K, Habas, F, Baleine, J, Lebouhellec, J, Combes, C, Chomton, M, Jouvet, P, Ranchin, B, Macher, M, Gaillot, T, Moine, M, Ageron, F, Jannel, C, Debillon, T, Wroblewski, I, Duprey, M, Jarlier, V, Luyt, C, Longval, T, Schnell, D, Padoin, C, Cohen, Y, Gaies, E, Triki, S, Klouz, A, Moussa, M, Desrumaux, F, May, F, Nguyen, J, Tiercelet, K, Fournier, J, Cherin, M, Kitzis, M, Misset, B, Mathien, C, Poidevin, A, Donatti, L, Mootien, J, Pinto, L, Egard, M, Bodur, G, Barberet, G, Ionescu, C, Ganster, F, Guiot, P, Kuteifan, K, Mpela, A, Chelly, J, Guérin, L, Persichini, R, Hullin, T, Deye, N, Aubertein, P, Paul, M, Bougouin, W, Sandroni, C, Passouant, O, Llitjos, J, Chenevier Gobeaux, C, Batteux, F, Drouet, L, Voicu, S, Henry, P, Dillinger, J, Resiere, D, Dessoy, A, Faivre, V, Damoisel, C, Stiel, L, Galoisy, A, Mauvieux, L, Zobairi, F, Angles Cano, E, Piau, C, Jeannet, R, Feuillard, J, Jolly, L, Boufenzer, A, Carrasco, K, Derive, M, Merdji, H, Belaidouni, N, Toubiana, J, L'Hermitte, Y, Woimant, F, Oppenheim, C, Couvreur, C, Dolveck, F, Devriese, M, Dupeyrat, S, Ray, P, Lefevre, G, Fartoukh, M, Roothaer, N, Carpentier, A, Vaniet, F, Maisonneuve, A, Wiel, E, Canu, S, Hammad, E, Antonini, F, Poirier, M, Vigne, C, Haddam, M, Alingrin, J, Dangers, L, Mangiapan, G, Huet, I, Dhalluin, X, Bautin, N, Quiot, J, De Vecchi, C, Chenivesse, C, Smaoui, M, El Alami, E, Weiss, N, Mochel, F, Galanaud, D, Puybasset, L, Lodey, M, Guiller, E, Vuillaume, C, De Pasquale, F, Demonet, J, Sinnah, F, Dalloz, M, D'Ortho, M, Rouvel Tallec, A, Couret, D, Catan, A, Nativel, B, Planesse, C, Diotel, N, Meilhac, O, Roy Gash, F, Lebard, C, Larbi, A, Gaudin, V, Bonnin, F, Sultan, O, Hoc, C, Mathieu, E, Lapergue, B, Bourdain, F, Caron, M, Parrot, A, Labbe, V, Hafiani, E, Quesnel, C, Genay, S, Décaudin, B, Ethgen, S, Odou, P, Lebuffe, G, Mcquilte, Z, Allaouchiche, B, Verdière, B, Nyunga, M, Banaias, N, Colling, D, Kauv, M, Blondeau, E, Auclin, E, Haw Berlemont, C, Taieb, J, Oudard, S, Morissette, G, Kechaou, W, Litalien, C, Merouani, A, Phan, V, Bouchard, J, Starck, J, Briand, N, Sachs, P, Angoulvant, F, Sommet, J, Holvoet, L, Benkerrou, M, Dreyfus, L, Bordet, F, Touzet, S, Denis, A, Le Coz, J, Chéron, G, Nabbout, R, Patteau, G, Heilbronner, C, Hubert, P, Oualha, M, Crulli, B, Toledano, B, Poirier, N, Vobecky, S, Khouadja, H, Vinet, M, Vinclair, C, Beloncle, F, Radermacher, P, Asfar, P, Coupez, E, Bohé, J, Shinotsuka, C, Caironi, P, Villois, P, Fontana, V, Creteur, J, Pourcine, F, Vong, L, Weyer, C, Akando, B, Abdallah, R, Wetzstein, M, Antier, N, Serroukh, Y, Boudjeltia, K, Joosten, A, Rousseau, A, Delabranche, X, Grunebaum, L, Mootien, Y, Gaci, R, Garric, J, Delbove, A, Darreau, C, Dargent, A, Soudry Faure, A, De Chambrun, M, Demondion, P, Blanchard, J, Chocron, S, Meneveau, N, Corsi, F, Meynieu, P, Repusseau, B, Germain, A, Baudry, G, Hierle, L, Besch, G, Thomas, G, Cassir, N, Dizier, S, Roch, A, Trebbia, G, Govindaradjou, K, Devaquet, J, Picard, C, Parquin, F, Leguen, M, Felten, M, Sage, E, Chapelier, A, Duruisseaux, M, Fleury, J, Antoine, M, Carette, M, Wislez, M, Givel, C, De Margerie Mellon, C, De Kerviler, E, Tandjaoui Lambiotte, Y, Freynet, O, Baux, E, Das, V, Talec, P, Anguel, N, Louis, G, Girerd, N, Tallon, P, Hadchouel Duvergé, A, Salvi, N, Cairet, P, Delacourt, C, Blandine, B, Beraud, L, Lamaziere, A, Lionnet, F, Lehingue, S, D'Journo, X, Jean Marie, F, Thibault, R, Makhlouf, A, Mulliez, A, Dadet, S, Kekstas, G, Preiser, J, Rotovnik, K, Rozalen, I, Kupczyk, K, Krznaric, Z, Cano, N, Pichard, C, Le Roux, B, Jotterand, C, Rooze, S, Moullet, C, Henin, A, Ettori, F, Zemmour, C, Boher, J, Feltry, A, Ben, S, Audibert, J, Conia, A, Gontier, O, Hamrouni, M, Lherm, T, Ouchenir, A, Rétif, J, Proudhom, A, Lagardere, C, Tissot, S, Kalfon, P, Sacre, L, Villa, A, Khadija, A, Garnier, R, Vasset, B, Heinzelman, A, Jouffroy, R, Durand, E, Compagnon, P, Jebri, A, Legout, C, Castot Villepelet, A, Valade, S, Lesieur, O, Delmas, B, Visseaux, B, Cohen, J, Nguyen, L, Morbieu, C, Burdet, C, Lescure, F, Armand Lefevre, L, Yazdanpanah, Y, Houhou Fidouh, N, Cazaux, M, Goff Jérôme, L, Meignin, V, Boutboul, D, Rispail, P, Besnard, N, Ceballos, P, Stoclin, A, Rotolo, F, Wartelle, M, Hicheri, Y, Maillet, S, Chachaty, E, Pignon, J, Bialais, E, Julie, D, Paoloni, L, Wittebolle, X, Hickmann, C, Castanares Zapatero, D, Tordeur, A, Colmant, L, Wittebole, X, Tirone, G, Laterre, P, Ducroux, L, Kemlin, C, Moulton, E, Rosso, C, Le Neindre, A, Mongodi, S, Bouhemad, B, Rodrigues, J, Botteau, C, Waroquier, F, Christiaens, K, Vantrimpont, F, Elkhawand, C, Vermeesh, F, Vermeesh, F., and CITERIO, GIUSEPPE
- Abstract
Determinants of outcome in critically ill patients with hematological malignancy and central neurological failure: data from the TRIAL OH study
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- 2016
209. A calcareous nannofossil and organic geochemical study of marine palaeoenvironmental changes across the Sinemurian/Pliensbachian (early Jurassic, ∼191 Ma) in Portugal
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Plancq, J., Mattioli, E., Pittet, B., Baudin, F., Duarte, L. V., Boussaha, Myriam, Grossi, V., Plancq, J., Mattioli, E., Pittet, B., Baudin, F., Duarte, L. V., Boussaha, Myriam, and Grossi, V.
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- 2016
210. Caractérisation sédimentaire d’une roche mère carbonatée du Bassin aquitain : exemple de la formation Parnac du Quercy
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Bastianini, L., Hoareau, Guilhem, Caline, B., Guy, L., Martinez, M., Baudin, F., Bonnel, Cédric, Laboratoire des Fluides Complexes et leurs Réservoirs (LFCR), TOTAL FINA ELF-Université de Pau et des Pays de l'Adour (UPPA)-Centre National de la Recherche Scientifique (CNRS), Centre scientifique et Technique Jean Feger (CSTJF), TOTAL FINA ELF, Solvay Silica, Solvay (France), DAM Île-de-France (DAM/DIF), Direction des Applications Militaires (DAM), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA), Commissariat à l'énergie atomique et aux énergies alternatives - Laboratoire d'Electronique et de Technologie de l'Information (CEA-LETI), and Direction de Recherche Technologique (CEA) (DRT (CEA))
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[PHYS]Physics [physics] ,[PHYS.MECA.MEMA]Physics [physics]/Mechanics [physics]/Mechanics of materials [physics.class-ph] ,[SDU.STU.GP]Sciences of the Universe [physics]/Earth Sciences/Geophysics [physics.geo-ph] ,[SPI.MECA.MEMA]Engineering Sciences [physics]/Mechanics [physics.med-ph]/Mechanics of materials [physics.class-ph] ,[PHYS.MECA.GEME]Physics [physics]/Mechanics [physics]/Mechanical engineering [physics.class-ph] ,[SPI.MECA.MEFL]Engineering Sciences [physics]/Mechanics [physics.med-ph]/Fluids mechanics [physics.class-ph] - Abstract
AFF; International audience
- Published
- 2014
211. Normal values for fundus perimetry with the MAIA microperimeter and short-term repeatability evaluation
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Baudin, F., primary, Assad, G., additional, Meillon, C., additional, Koehrer, P., additional, Bron, A., additional, and Creuzot, C., additional
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- 2016
- Full Text
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212. Efficacité de la prise en charge des traumatismes graves de l’enfant en salle d’accueil des urgences vitales adulte ou pédiatrique : une étude avant-après
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Baudin, F., primary, Floccard, B., additional, Desgranges, F.-P., additional, Courtil-Teyssedre, S., additional, De Queiroz, M., additional, Richard, N., additional, and Javouhey, E., additional
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- 2016
- Full Text
- View/download PDF
213. Intérêt de l’ustékinumab pour le traitement des uvéites antérieures chez une patiente avec un rhumatisme psoriasique
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Bielefeld, P., primary, Picque, J.B., additional, Devilliers, H., additional, Maupin, E., additional, Baudin, F., additional, Turcu, A., additional, Muller, G., additional, Bron, A., additional, Creuzot-Garcher, C., additional, and Besancenot, J.F., additional
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- 2015
- Full Text
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214. Differential asteroseismic study of seismic twins observed by CoRoT
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Ozel, N., Mosser, B., Dupret, M. A., Bruntt, H., Barban, C., Deheuvels, S., García, R. A., Michel, E., Samadi, R., Baudin, F., Mathur, S., Régulo, C., Auvergne, M., Catala, C., Morel, Pierre, Pichon, B., 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), Astrophysique Interprétation Modélisation (AIM (UMR7158 / UMR_E_9005 / UM_112)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Astrophysique Interprétation Modélisation (AIM (UMR_7158 / UMR_E_9005 / UM_112)), Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7), Centre National de la Recherche Scientifique (CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Observatoire de Paris, and PSL Research University (PSL)-PSL Research University (PSL)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Pierre et Marie Curie - Paris 6 (UPMC)
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techniques: photometric ,Astrophysics::Solar and Stellar Astrophysics ,stars: individual: HD 181420 ,Astrophysics::Earth and Planetary Astrophysics ,stars: evolution ,asteroseismology ,stars: interiors ,[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph] ,stars: individual: HD 175272 - Abstract
International audience; Context. The CoRoT short asteroseismic runs give us the opportunity to observe a large variety of late-type stars through their solar-like oscillations. We report the observation and modeling of the F5V star HD 175272.Aims. Our aim is to define a method for extracting as much information as possible from a noisy oscillation spectrum. Methods. We followed a differential approach that consists of using a well-known star as a reference to characterize another star. We used classical tools such as the envelope autocorrelation function to derive the global seismic parameters of the star. We compared HD 175272 with HD 181420 through a linear approach, because they appear to be asteroseismic twins.Results. The comparison with the reference star enables us to substantially enhance the scientific output for HD 175272. First, we determined its global characteristics through a detailed seismic analysis of HD 181420. Second, with our differential approach, we measured the difference of mass, radius and age between HD 175272 and HD 181420.Conclusions. We have developed a general method able to derive asteroseismic constraints on a star even in case of low-quality data. This method can be applied to stars with interesting properties but low signal-to-noise ratio oscillation spectrum, such as stars hosting an exoplanet or members of a binary system.
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- 2013
215. Microstructures and Textures in a Cu-Ni-Si Alloy Processed by High-Pressure Torsion
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A.Y. Khereddine, F.H. Larbi, H. Azzeddine, T. Baudin, F. Brisset, A.L. Helbert, M.H. Mathon, M. Kawasaki, D. Bradai and T.G. Langdon
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- 2013
216. A study of temperature fluctuations in the atmospheric boundary layer
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Weill, A., Aubry, M., Baudin, F., and Heissat, J.
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- 1976
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217. The ‘MESOGERS 84’ experiment: A report
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Weill, A., Mazaudier, C., Baudin, F., Klapisz, C., Leca, F., Masmoudi, M., Madjar, D. Vidal, Bernard, R., Taconet, O., Gera, B. S., Sauvaget, A., Druilhet, A., Durand, P., Caneil, J. Y., Mery, P., Dubosclard, G., Beljaars, A. C. M., Monna, W. A. A., Van Der Vliet, J. G., Crochet, M., Thomson, D., and Carlson, T.
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- 1988
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218. A mesoscale shear convective cell observed during the C.O.A.S.T. experiment: Acoustic sounder measurements
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Weill, A., Baudin, F., Mazaudier, C., Desbraux, G., Klapisz, C., Driedonks, A. G. M., Goutorbe, J. P., Druilhet, A., and Durand, P.
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- 1988
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219. Turbulence structure in temperature inversions and in convection fields as observed by doppler sodar
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Weill, A., Baudin, F., Goutorbe, J. P., Van Grunderbeeck, P., and Leberre, P.
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- 1978
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220. CoRoT Observations of O Stars: Diverse Origins of Variability
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Blomme, R., Briquet, M., Degroote, P., Mahy, L., Aerts, Conny, Cuypers, J., Godart, M., Gosset, E., Hareter, M., Montalban, J., Morel, T., Nieva, M.F., Noels, A., Oreiro, R., Poretti, E., Przybilla, N., Rainer, M., Rauw, G., Schiller, F., Simon-Diaz, S., Smolders, K., Ventura, P., Vučković, M., Auvergne, M., Baglin, A., Baudin, F., Catala, C., Michel, E., Samadi, R., Rubert, C., St-Louis, N., Moffat, A.F.J., Drissen, L., and Drissen, L.
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Astronomy ,ComputingMethodologies_DOCUMENTANDTEXTPROCESSING ,Astronomical Society of the Pacific Conference Series - Abstract
Contains fulltext : 111302.pdf (Author’s version preprint ) (Open Access) Contains fulltext : 111302.pdf (Publisher’s version ) (Closed access)
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- 2013
221. An in-depth study of HD 174966 with CoRoT photometry and HARPS spectroscopy. Large separation as a new observable for ��Sct stars
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Hern��ndez, A. Garc��a, Moya, A., Michel, E., Su��rez, J. C., Poretti, E., Mart��n-Ru��z, S., Amado, P. J., Garrido, R., Rodr��guez, E., Rainer, M., Uytterhoeven, K., Rodrigo, C., Solano, E., Rod��n, J. R., Mathias, P., Rolland, A., Auvergne, M., Baglin, A., Baudin, F., Catala, C., and Samadi, R.
- Subjects
Astrophysics::Solar and Stellar Astrophysics ,FOS: Physical sciences ,Astrophysics::Earth and Planetary Astrophysics ,Solar and Stellar Astrophysics (astro-ph.SR) - Abstract
The aim of this work was to use a multi-approach technique to derive the most accurate values possible of the physical parameters of the ��Sct star HD174966. In addition, we searched for a periodic pattern in the frequency spectra with the goal of using it to determine the mean density of the star. First, we extracted the frequency content from the CoRoT light curve. Then, we derived the physical parameters of HD174966 and carried a mode identification out from the spectroscopic and photometric observations. We used this information to look for the models fulfilling all the conditions and discussed the inaccuracies of the method because of the rotation effects. In a final step, we searched for patterns in the frequency set using a Fourier transform, discussed its origin and studied the possibility of using the periodicity to obtain information about the physical parameters of the star. A total of 185 peaks were obtained from the Fourier analysis of the CoRoT light curve, being almost all reliable pulsating frequencies. From the spectroscopic observations, 18 oscillation modes were detected and identified, and the inclination angle ($62.5^{\circ}$$^{+7.5}_{-17.5}$) and the rotational velocity of the star (142 km/s) were estimated. From the multi-colour photometric observations, 3 frequencies were detected, which correspond to the main ones in the CoRoT light curve. We looked for periodicities within the 185 frequencies and found a periodic pattern ~64 ��Hz. Using the inclination angle, the rotational velocity and an Echelle diagram, showing a double comb outside the asymptotic regime, we concluded that the periodicity corresponds to a large separation structure. The periodic pattern allowed us to discriminate models from a grid, finding that the value of the mean density is achieved with a 6% uncertainty. So, the pattern could be used as a new observable for A-F type stars., 15 pages, 10 figures, 6 tables
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- 2013
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222. Evaluation of Titanium Direct Bonding MechanismStudy of crystal-crucible detachment: GaSb in SiO2
- Author
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Baudin, F., Delaye, V., Guedj, C., Chevalier, N., Mariolle, D., Imbert, B., Fabbri, J.M., Di Cioccio, L., Brechet, Y., Commissariat à l'énergie atomique et aux énergies alternatives - Laboratoire d'Electronique et de Technologie de l'Information (CEA-LETI), Direction de Recherche Technologique (CEA) (DRT (CEA)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA), Science et Ingénierie des Matériaux et Procédés (SIMaP), and Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut National Polytechnique de Grenoble (INPG)-Institut de Chimie du CNRS (INC)-Centre National de la Recherche Scientifique (CNRS)
- Subjects
[CHIM.MATE]Chemical Sciences/Material chemistry - Abstract
International audience; Direct metal bonding represents an advanced joining technology that allows vertical stacking with electrical conduction and even heat dissipation. For most metals used as bonding layers, direct bonding when operating under ambient conditions involves metal oxides. The bonding interface saddles with a trapped oxide layer that might affect electrical conduction and even complete sealing of bonding interface. Titanium especially because of its high affinity with oxygen makes oxide free direct bonding very difficult. In the mean time, the remarkable getter effect of Ti matrix allows the dissolution of oxygen during post bonding annealing. In this paper, the bonding limits with regards to the titanium thickness have been investigated. The key role of layer roughness on the bonding quality and energy has been pointed out. A titanium thickness below 10 nm appears as a limit for an oxide free bonding in our conditions. (C) 2013 The Electrochemical Society.
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- 2013
223. CoRoT Observations of O Stars: Diverse Origins of Variability
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Blomme, R., Briquet, M., Degroote, P., Mahy, L., Aerts, C., Cuypers, J., Godart, M., Gosset, E., Hareter, M., Montalban, J., Morel, T., Nieva, M. F., Noels, A., Oreiro, R., Poretti, E., Przybilla, N., Rainer, M., Rauw, G., Schiller, F., Simon-Diaz, S., Smolders, K., Ventura, P., Vučković, M., Auvergne, M., Baglin, A., Baudin, F., Catala, C., Michel, E., Samadi, R., Blomme, Briquet, Degroote, Mahy, Aerts, Cuypers, Godart, Gosset, Hareter, Montalban, Morel, Nieva, M. F., Noels, Oreiro, Poretti, Przybilla, Rainer, Rauw, Schiller, Simon-Diaz, Smolders, Ventura, Vučković, Auvergne, Baglin, Baudin, Catala, Michel, and Samadi
- Published
- 2012
224. Purpura thrombotique thrombocytopénique réfractaire révélant un cancer de l’épiglotte
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Baudin, F., Guillot, P., Bedock, B., and Blanc, P.-L.
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- 2012
- Full Text
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225. Amplitudes of solar-like oscillations in red giant stars
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Samadi, R., Belkacem, K., Dupret, M.-A., Ludwig, H.-G., Baudin, F., Caffau, E., Goupil, M.-J., Barban, C., 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), Galaxies, Etoiles, Physique, Instrumentation (GEPI), and Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris
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[PHYS]Physics [physics] ,[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph] ,ComputingMilieux_MISCELLANEOUS - Abstract
International audience
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- 2012
226. Damping rates of solar-like oscillations across the HR diagram
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Belkacem, K., Dupret, M., Baudin, F., Appourchaux, T., Marques, J., Samadi, R., Institut d'astrophysique spatiale (IAS), Université Paris-Sud - Paris 11 (UP11)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Centre National d’Études Spatiales [Paris] (CNES), 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), Space Sciences, Technologies and Astrophysics Research Institute (STAR), Université de Liège, Commissariat à l'énergie atomique et aux énergies alternatives - Laboratoire d'Electronique et de Technologie de l'Information (CEA-LETI), Direction de Recherche Technologique (CEA) (DRT (CEA)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA), Laboratoire d'automatique et de génie des procédés (LAGEP), Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-École Supérieure de Chimie Physique Électronique de Lyon (CPE)-Centre National de la Recherche Scientifique (CNRS), Université Paris-Sud - Paris 11 (UP11)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), and Université de Lyon-Université de Lyon-École Supérieure Chimie Physique Électronique de Lyon-Centre National de la Recherche Scientifique (CNRS)
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[PHYS]Physics [physics] ,[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph] ,ComputingMilieux_MISCELLANEOUS - Abstract
International audience
- Published
- 2012
227. Young [α/Fe]-enhanced stars discovered by CoRoT and APOGEE: What is their origin?
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Chiappini, C., primary, Anders, F., additional, Rodrigues, T. S., additional, Miglio, A., additional, Montalbán, J., additional, Mosser, B., additional, Girardi, L., additional, Valentini, M., additional, Noels, A., additional, Morel, T., additional, Minchev, I., additional, Steinmetz, M., additional, Santiago, B. X., additional, Schultheis, M., additional, Martig, M., additional, da Costa, L. N., additional, Maia, M. A. G., additional, Allende Prieto, C., additional, de Assis Peralta, R., additional, Hekker, S., additional, Themeßl, N., additional, Kallinger, T., additional, García, R. A., additional, Mathur, S., additional, Baudin, F., additional, Beers, T. C., additional, Cunha, K., additional, Harding, P., additional, Holtzman, J., additional, Majewski, S., additional, Mészáros, Sz., additional, Nidever, D., additional, Pan, K., additional, Schiavon, R. P., additional, Shetrone, M. D., additional, Schneider, D. P., additional, and Stassun, K., additional
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- 2015
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228. CoRoT data: final pipe-line for faint stars
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Deru, A., primary, Chaintreuil, S., additional, Baudin, F., additional, Ferrigno, A., additional, and Baglin, A., additional
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- 2015
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229. CoRoT data: final pipe-line for bright stars
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Deru, A., primary, Chaintreuil, S., additional, Baudin, F., additional, Ferrigno, A., additional, and Baglin, A., additional
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- 2015
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230. VizieR Online Data Catalog: Supervised classification of CoRoT variables (Debosscher+, 2009)
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Debosscher, J., Sarro, L.~m., Lopez, M., Deleuil, M., Aerts, C., Auvergne, M., Baglin, A., Baudin, F., Chadid, M., Charpinet, S., Cuypers, J., de Ridder, J., Garrido, R., Hubert, A.~m., Janot-Pacheco, E., Jorda, L., Kaiser, Andreas, Kallinger, T., Kollath, Z., Maceroni, C., Mathias, P., Michel, E., Moutou, C., Neiner, C., Ollivier, M., Samadi, R., Solano, E., Surace, C., Vandenbussche, B., Weiss, W.~w., Institute of Astronomy [Leuven], Catholic University of Leuven - Katholieke Universiteit Leuven (KU Leuven), 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), Instituut voor Sterrenkunde [Leuven], 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), Division technique INSU/SDU (DTI), Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Laboratoire Hippolyte Fizeau (FIZEAU), Université Nice Sophia Antipolis (1965 - 2019) (UNS), COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de la Côte d'Azur, COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-Université Côte d'Azur (UCA)-Centre National de la Recherche Scientifique (CNRS), Laboratoire Astrophysique de Toulouse-Tarbes (LATT), Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire Midi-Pyrénées (OMP), Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Centre National de la Recherche Scientifique (CNRS), Royal Observatory of Belgium [Brussels] (ROB), Instituto de Astrofísica de Andalucía (IAA), Consejo Superior de Investigaciones Científicas [Madrid] (CSIC), Instituto de Astronomia, Geofisica e Ciencias Atmosfericas (IAGCAUSP), Universidade de São Paulo = University of São Paulo (USP), Institut d’Électronique, de Microélectronique et de Nanotechnologie - UMR 8520 (IEMN), Centrale Lille-Institut supérieur de l'électronique et du numérique (ISEN)-Université de Valenciennes et du Hainaut-Cambrésis (UVHC)-Université de Lille-Centre National de la Recherche Scientifique (CNRS)-Université Polytechnique Hauts-de-France (UPHF), Institute for Astronomy [Vienna], University of Vienna [Vienna], Laboratoire des Sciences du Climat et de l'Environnement [Gif-sur-Yvette] (LSCE), Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS), Galaxies, Etoiles, Physique, Instrumentation (GEPI), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Institut d'astrophysique spatiale (IAS), Université Paris-Sud - Paris 11 (UP11)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Centre National d’Études Spatiales [Paris] (CNES), Departamento de Astrofisica [Madrid], Centro de Astrobiologia [Madrid] (CAB), Instituto Nacional de Técnica Aeroespacial (INTA)-Consejo Superior de Investigaciones Científicas [Madrid] (CSIC)-Instituto Nacional de Técnica Aeroespacial (INTA)-Consejo Superior de Investigaciones Científicas [Madrid] (CSIC), Spanish Virtual Observatory - Observatorio Virtual Español (SVO), and Spanish Virtual Observatory - Observatorio Virtual Español
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[INFO]Computer Science [cs] ,Stars: variable ,[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph] - Abstract
International audience; Light curve parameters and classification results are presented for all the objects measured in the first four CoRoT observing runs: IRa01, SRc01, LRc01, and LRa01. The information presented here should allow scientists to make candidate lists of their objects of study and to obtain some basic light curve information. We recall that we did not perform detailed light curve modelling, only a basic one, sufficient for producing variability class memberships for each target. We refer to the paper for a detailed description of the light curve parameters, and the classification results. It is strongly advised to read the paper prior to using the results presented here. (4 data files).
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- 2009
231. Automated supervised classification of variable stars in the CoRoT programme. Method and application to the first four exoplanet fields
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Debosscher, J., Sarro, L. M., Lxf3pez, M., Deleuil, M., Aerts, C., Auvergne, M., Baglin, A., Baudin, F., Chadid, M., Charpinet, S., Cuypers, J., De Ridder, J., Garrido, R., Hubert, A. M., Janot-Pacheco, E., Jorda, L., Kaiser, A., Kallinger, T., Kollath, Z., Maceroni, C., Mathias, P., Michel, E., Moutou, C., Neiner, C., Ollivier, M., Samadi, R., Solano, E., Surace, C., Vandenbussche, B., Weiss, W. W., Debosscher, Sarro, L. M., Lxf3pez, Deleuil, Aerts, Auvergne, Baglin, Baudin, Chadid, Charpinet, Cuypers, De Ridder, Garrido, Hubert, A. M., Janot-Pacheco, Jorda, Kaiser, Kallinger, Kollath, Maceroni, Mathias, Michel, Moutou, Neiner, Ollivier, Samadi, Solano, Surace, Vandenbussche, Weiss, and W. W.
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- 2009
232. The B0.5IVe CoRoT target HD 49 330. I. Photometric analysis from CoRoT data
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Huat, A.L., Hubert, A.M., Floquet, M., Neiner, C., Frémat, Y., Gutiérrez Soto, Juan, Baudin, F., Andrade, L., De Batz, B., Diago Nebot, Pascual David, Emilio, M., Espinosa-Lara, F., Fabregat Llueca, Juan, Janot-Pacheco, E., Leroy, B., Martayan, C., Semaan, T., Suso, J., Michel, E., and Samadi, R.
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Astrophysics::High Energy Astrophysical Phenomena ,Astronomia ,Astrophysics::Solar and Stellar Astrophysics ,Astrophysics::Earth and Planetary Astrophysics ,Astrophysics::Galaxy Astrophysics ,Ciència Ensenyament - Abstract
Context. Be stars undergo outbursts producing a circumstellar disk from the ejected material. The beating of non-radial pulsations has been put forward as a possible mechanism of ejection. Aims. We analyze the pulsational behavior of the early B0.5IVe star HD 49330 observed during the first CoRoT long run towards the Galactical anticenter (LRA1). This Be star is located close to the lower edge of the β Cephei instability strip in the HR diagram and showed a 0.03 mag outburst during the CoRoT observations. It is thus an ideal case for testing the aforementioned hypothesis. Methods. We analyze the CoRoT light curve of HD 49330 usin g Fourier methods and non-lin ear least square fitting. Results. In this star, we find pulsation modes typical of β Cep stars (p modes) and SPB stars (g modes) with amplitude variations along the run directly correlated with the outburst. These results provide new clues about the origin of the Be phenomenon as well as strong constraints on the seismic modelling of Be stars.
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- 2009
233. Asteroseismic analysis of the CoRoT ��-Scuti star HD174936
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Hern��ndez, A. Garc��a, Moya, A., Michel, E., Garrido, R., Su��rez, J. C., Rodr��guez, E., Amado, P. J., Mart��n-Ru��z, S., Rolland, A., Poretti, E., Samadi, R., Baglin, A., Auvergne, M., Catala, C., Lefevre, L., and Baudin, F.
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Astrophysics::Solar and Stellar Astrophysics ,FOS: Physical sciences ,Astrophysics::Earth and Planetary Astrophysics ,Solar and Stellar Astrophysics (astro-ph.SR) - Abstract
We present an analysis of the ��-Scuti star object HD 174936 (ID 7613) observed by CoRoT during the first short run SRc01 (27 days). A total number of 422 frequencies we are extracted from the light curve using standard prewhitening techniques. This number of frequencies was obtained by considering a spectral significance limit of sig = 10 using the software package SigSpec. Our analysis of the oscillation frequency spectrum reveals a spacing periodicity of around 52 \muHz. Although modes considered here are not in the asymptotic regime, a comparison with stellar models confirms that this signature may stem from a quasi-periodic pattern similar to the so-called large separation in solar-like stars., 7 pages, 7 figures, 2 tables. Accepted for publication in A&A CoRoT Special Feature
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- 2009
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234. Data report: bio- and lithofacies, mineralogy, and organic content of Challenger Mound (Porcupine Seabight, SW Ireland
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Leonide, P.S., Floquet, M., Baudin, F., Felderman, T.G., Kano, A., Williams, T., Henriet, J.-P., and Sedimentology
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- 2009
235. The pulsations of the B5IVe star HD 181 231 observed with CoRoT and ground-based spectroscopy
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Neiner, C., Gutiérrez Soto, Juan, Baudin, F., De Batz, B., Frémat, Y., Huat, A.L., Floquet, M., Hubert, A.M., Leroy, B., Diago Nebot, Pascual David, Poretti, E., Carrier, F., Rainer, M., Catala, C., Thizy, O., Buil, C., Ribeiro, J., Andrade, L., Emilio, M., Espinosa-Lara, F., Fabregat Llueca, Juan, Janot-Pacheco, E., Martayan, C., Semaan, T., Suso, J., Baglin, A., Michel, E., and Samadi, R.
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Astronomia ,Astrophysics::Solar and Stellar Astrophysics ,Astrophysics::Earth and Planetary Astrophysics ,Ciència Ensenyament - Abstract
Context. HD 181231 is a B5IVe star, which has been observed with the CoRoT satellite during ∼5 consecutive months and simultaneously from the ground in spectroscopy and spectropolarimetry. Aims. By analysing these data, we aim to detect and characterize as many pulsation frequencies as possible, to search for the presence of beating effects possibly at the origin of the Be phenomenon. Our results will also pr ovide a basis for seismic modelling. Methods. The fundamental parameters of the star are determined from spectral fitting and from the study of the circumstellar emission. The CoRoT photometric data and ground-based spectroscopy are analysed using several Fourier Techniques: CLEAN-NG,PASPER,and TISAFT, as well as a time-frequency technique. A search for a magnetic field is performed by applying the LSD technique to the spectropolarimetric data. Results. We find that HD 181231 is a B5IVe star seen with an inclination of ∼45 degrees. No magnetic field is detected in its photo-sphere. We detect at least 10 independent significant frequencies of variations among the 54 detected frequencies, interpreted in termsof non-radial pulsation modes and rotation. Two longer-term variations are also detected: one at ∼14 days resulting from a beating effect between the two main frequencies of short-term variations, the other at ∼116 days due either to a beating of frequencies or to a zonal pulsation mode. Conclusions. Our analysis of the CoRoT light curve and ground-based spectroscopic data of HD 181231 has led to the determination of the fundamental and pulsational parameters of the star, including beating effects. This will allow a precise seismic modelling of this star.
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- 2009
236. Transiting exoplanets from the CoRoT space mission VIII. CoRoT-7b: the first super-Earth with measured radius
- Author
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Leger, A., Rouan, D., Jodi Schneider, Barge, P., Fridlund, M., Samuel, B., Ollivier, M., Guenther, E., Deleuil, M., Deeg Hj, Auvergne, M., Alonso, R., Aigrain, S., Alapini, A., Almenara Jm, Baglin, A., Barbieri, M., Bruntt, H., Pascal Bordé, Bouchy, F., Cabrera, J., Catala, C., Carone, L., Carpano, S., Csizmadia, S., Dvorak, R., Erikson, A., Ferraz-Mello, S., Foing, B., Grasset, O., Fressin, F., Gandolfi, D., Gillon, M., Gondoin, P., Guillot, T., Hatzes, A., Hebrard, G., Jorda, L., Lammer, H., Llebaria, A., Loeillet, B., Mayor, M., Mazeh, T., Moutou, C., Patzold, M., Pont, F., Queloz, D., Rauer, H., Renner, S., Samadi, R., Shporer, A., Sotin, C., Tingley, B., Wuchterl, G., Adda, M., Agogu, P., Appourchaux, T., Ballans, H., Baron, P., Beaufort, T., Bellenger, R., Berlin, R., Bernardi, P., Blouin, D., Baudin, F., Bodin, P., Boisnard, L., Boit, L., Bonneau, F., Borzeix, S., Briet, R., Buey Jt, Butler, B., Cailleau, D., Cautain, R., Chabaud Py, Chaintreuil, S., Chiavassa, F., Costes V, Parrho Vc, Fialho Fd, Decaudin, M., Defise Jm, Djalal, S., Epstein, G., Exil Ge, Faure, C., Fenouillet, T., Gaboriaud, A., Gallic, A., Gamet, P., Gavalda, P., Grolleau, E., Gruneisen, R., Gueguen, L., Guis, V., V. Guivarc'H, Guterman, P., Hallouard, D., Hasiba, J., Heuripeau, F., Huntzinger, G., Hustaix, H., Imad, C., Imbert, C., Johlander, B., Jouret, M., Journoud, P., Karioty, F., Kerjean, L., Lafaille, V., Lafond, L., Lam-Trong, T., Landiech, P., Lapeyrere, V., Larque, T., Laudet, P., Lautier, N., Lecann, H., Lefevre, L., Leruyet, B., Levacher, P., Magnan, A., Mazy, E., Mertens, F., Mesnager Jm, Meunier Jc, Michel Jp, Monjoin, W., Naudet, D., Nguyen-Kim, K., Orcesi Jl, Ottacher, H., Perez, R., Peter, G., Plasson, P., Plesseria Jy, Pontet, B., Pradines, A., Céline Quentin, Reynaud Jl, Rolland, G., Rollenhagen, F., Romagnan, R., Russ, N., Schmidt, R., Schwartz, N., Sebbag, I., Sedes, G., Smit, H., Steller Mb, Sunter, W., Surace, C., Tello, M., Tiphene, D., Toulouse, P., Ulmer, B., Vandermarcq, O., Vergnault, E., Vuillemin, A., 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), Laboratoire de Planétologie et Géodynamique [UMR 6112] (LPG), Université d'Angers (UA)-Université de Nantes - UFR des Sciences et des Techniques (UN UFR ST), Université de Nantes (UN)-Université de Nantes (UN)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), 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), Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Université de Nantes - UFR des Sciences et des Techniques (UN UFR ST), and Université de Nantes (UN)-Université de Nantes (UN)-Université d'Angers (UA)
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[SDU.STU]Sciences of the Universe [physics]/Earth Sciences ,ComputingMilieux_MISCELLANEOUS - Abstract
International audience
- Published
- 2009
237. First asteroseismic results from CoRoT. Veröffentlichungen der Kommission für Astronomie|Communications in Asteroseismology|Communications in Asteroseismology 156 156
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Baglin, A., Aerts, C., Barban, C., Catala, C., Michel, E., Baudin, F., Carrier, F., Auvergne, M., Briquet, M., Appourchaux, T., and al, et
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Mathematics, Physics and Space Research - Published
- 2008
238. AsteroFLAG - from the Sun to the Stars
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Chaplin, W.J., Appourchaux, T., Arentoft, Torben, Ballot, J., Baudin, F., Bazot, Michael, Bedding, T.R., Christensen-Dalsgaard, Jørgen, Creevey, O.L., Duez, V., Elsworth, Y., Fletcher, S.T., García, R.A., Gough, D.O., Jiménez, A., Jiménez-Reyes, S.J., Houdek, G., Kjeldsen, Hans, Lazrek, M., Leibacher, J.W., Monteiro, M.J.P.F.G., Neiner, C., New, R., Régulo, C., Salabert, D., Samadi, R., Sekii, T., Sousa, S.G., Toutain, T., and Turck-Chièze, S.
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- 2008
239. Simu-LC : a Light-Curve simulator for CoRoT
- Author
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Baudin, F., Samadi, R., Appourchaux, T., and Michel, E.
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Astrophysics (astro-ph) ,FOS: Physical sciences ,Astrophysics - Abstract
Simulating the data that a space instrument like COROT will provide might look presomptuous. Indeed, it is certainly, when comparing to previous comparable instruments like IPHIR or GOLF. These two examples show that the nominal behaviour of the instrument is not always reached, but this does not prevent this instrument to provide very interesting data. However, despite some technical problems, IPHIR and GOLF yielded a wealth of scientific results. Thus, what is the interest of simulating COROT data? How close to reality these simualtions will get? This might not be the most important fact as the preparation of these simulations will help us to prepare the analysis of real data and to be ready in case of unexpected technical behaviour of the instrument perturbating the data, or unexpected physical behaviour of the targets of the instrument. A consequence of that is that the simulation tool must include technical and physical aspects, making the task even more difficult. These aspects cover: photon noise, p modes excitation, granulation signal, stellar activity signal, orbital perturbations, stellar rotation... The software presented here is freely available at: http://www.lesia.obspm.fr/~corotswg/simulightcurve.html, Contribution to "The Corot book" published by ESA (SP 1306; Eds: M. Fridlund, A. Baglin, L. Conroy and J. Lochard). Due to a mistake, the references were not correctly compiled, this version corrects this mistake ; 5 pages ; 3 figures
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- 2007
240. The Corot Book: Chap. V.5/ Extraction of the photometric information : corrections
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Samadi, R., Fialho, F., Costa, J. E. S., Drummond, R., Da Silva, L. Pinheiro, Baudin, F., Boumier, P., and Jorda, L.
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Astrophysics (astro-ph) ,FOS: Physical sciences ,Astrophysics - Abstract
We present here the set of corrections that will be applied to the raw data of the CoRoT mission. The aim is to correct the data for instrumental and environmental perturbations as well as to optimize the duty-cycle, in order to reach the expected performances of the mission. The main corrections are : the correction of the electromagnetic interferences, suppression of outliers, the background correction, the jitter correction and the correction of the integration time variations. We focus here on these corrections and emphasize their efficiency., Contribution to "The Corot book" published by ESA (SP 1306; Eds: M. Fridlund, A. Baglin, L. Conroy and J. Lochard). Due to a mistake, the published version is not the final version that should have been published. This version replaced the one published in ESA-SP 1306 ; 9 pages ; 16 figures
- Published
- 2007
241. OH and H2O maser variations in W33B
- Author
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Chiappini, C., Anders, F., Rodrigues, T., Miglio, A., Montalban, J., Mosser, B., Girardi, L., Valentini, M., Noels, A., Morel, T., Minchev, I., Steinmetz, M., Santiago, B., Schultheis, M., Martig, M., da Costa, L., Maia, M., Allende Prieto, C., de Assis Peralta, R., Hekker, S., Themessl, N., Kallinger, T., Garcia, R., Mathur, S., Baudin, F., Beers, T., Cunha, K., Harding, P., Holtzman, J., Majewski, S., Mészáros, Sz., Nidever, D., Pan, K., Schiavon, R., Shetrone, M., Schneider, D., Stassun, K., Colom, P., Lekht, E., Pashchenko, M., Rudnitskij, G., Leibniz-Institut für Astrophysik Potsdam (AIP), Institut d'Astrophysique et de Géophysique [Liège], Université de Liège, 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), INAF - Osservatorio Astronomico di Padova (OAPD), Istituto Nazionale di Astrofisica (INAF), Département d'astrophysique, Géophysique et Océanographie (AGO), Joseph Louis LAGRANGE (LAGRANGE), Université Nice Sophia Antipolis (1965 - 2019) (UNS), COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de la Côte d'Azur, COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-Université Côte d'Azur (UCA)-Centre National de la Recherche Scientifique (CNRS), Liverpool John Moores University (LJMU), Laboratoire Géosciences Océan (LGO), Université de Bretagne Sud (UBS)-Institut Français de Recherche pour l'Exploitation de la Mer (IFREMER)-Université de Brest (UBO)-Centre National de la Recherche Scientifique (CNRS), Mullard Space Science Laboratory (MSSL), University College of London [London] (UCL), School of Physics and Astronomy, University of Birmingham [Birmingham], Institute for Astronomy [Vienna], University of Vienna [Vienna], Institut de Physique du Globe de Paris (IPG Paris), Space Science Institute [Boulder] (SSI), Commissariat à l'énergie atomique et aux énergies alternatives - Laboratoire d'Electronique et de Technologie de l'Information (CEA-LETI), Direction de Recherche Technologique (CEA) (DRT (CEA)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA), Center for the Study of Cosmic Evolution (CSCE), Michigan State University [East Lansing], Michigan State University System-Michigan State University System, Department of Geography, Department of geography, Université Nice Sophia Antipolis (... - 2019) (UNS), Université Côte d'Azur (UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-Centre National de la Recherche Scientifique (CNRS), Institut Français de Recherche pour l'Exploitation de la Mer - Brest (IFREMER Centre de Bretagne), Institut Français de Recherche pour l'Exploitation de la Mer (IFREMER)-Institut Français de Recherche pour l'Exploitation de la Mer (IFREMER)-Université de Bretagne Sud (UBS)-Université de Brest (UBO)-Centre National de la Recherche Scientifique (CNRS), Institut de Physique du Globe de Paris, Université Côte d'Azur (UCA)-Université Nice Sophia Antipolis (... - 2019) (UNS), COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Observatoire de la Côte d'Azur, Université Côte d'Azur (UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Université de Bretagne Sud (UBS)-Université de Brest (UBO)-Institut Universitaire Européen de la Mer (IUEM), and Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Université de Brest (UBO)-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Centre National de la Recherche Scientifique (CNRS)
- Subjects
individual objects ,85A15 ,lines and bands -ISM ,Astrophysics::High Energy Astrophysical Phenomena ,Central object ,FOS: Physical sciences ,Astrophysics ,01 natural sciences ,W33B ,law.invention ,Radio telescope ,symbols.namesake ,law ,0103 physical sciences ,Astrophysics::Solar and Stellar Astrophysics ,Maser ,masers -ISM ,010303 astronomy & astrophysics ,Solar and Stellar Astrophysics (astro-ph.SR) ,Astrophysics::Galaxy Astrophysics ,magnetic fields -ISM ,Line (formation) ,[PHYS]Physics [physics] ,Physics ,Zeeman effect ,010308 nuclear & particles physics ,molecules -ISM ,Astronomy and Astrophysics ,Astrophysics - Astrophysics of Galaxies ,Magnetic field ,Wavelength ,Astrophysics - Solar and Stellar Astrophysics ,13. Climate action ,Space and Planetary Science ,Astrophysics of Galaxies (astro-ph.GA) ,symbols ,Astrophysics::Earth and Planetary Astrophysics ,[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph] ,Excitation - Abstract
The active star-forming region W33B is a source of OH and H2O maser emission located in distinct zones around the central object. The aim was to obtain the complete Stokes pattern of polarised OH maser emission, to trace its variability and to investigate flares and long-term variability of the H2O maser and evolution of individual emission features. Observations in the OH lines at a wavelength of 18 cm were carried out on the Nan\c{c}ay radio telescope (France) at a number of epochs in 2008--2014; H2O line observations (long-term monitoring) at a wavelength of 1.35 cm were performed on the 22-metre radio telescope of the Pushchino Radio Astronomy Observatory (Russia) between 1981 and 2014. We have observed strong variability of the emission features in the main 1665- and 1667-MHz OH lines as well as in the 1612-MHz satellite line. Zeeman splitting has been detected in the 1665-MHz OH line at 62 km/s and in the 1667-MHz line at 62 and 64 km/s. The magnetic field intensity was estimated to be from 2 to 3 mG. The H2O emission features form filaments, chains with radial-velocity gradients, or more complicated structures including large-scale ones. Long-term observations of the hydroxyl maser in the W33B region have revealed narrowband polarised emission in the 1612-MHz line with a double-peak profile characteristic of Type IIb circumstellar masers. The 30-year monitoring of the water-vapour maser in W33B showed several strong flares of the H2O line. The observed radial-velocity drift of the H2O emission features suggests propagation of an excitation wave in the masering medium with a gradient of radial velocities. In OH and H2O masers some turbulent motions of material are inferred., Comment: 18 pages, 12 figures
- Published
- 2015
242. Studying solar-like oscillations in red giants: MOST spacebased photometry of epsilon Ophiuchi
- Author
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Barban, C., Matthews, J., Ridder, J., Baudin, F., Kuschnig, R., Anwesh Mazumdar, Samadi, R., Guenther, D. B., Moffat, A. F. J., Rucinski, S. M., Sasselov, D., Walker, G. A. H., Weiss, W. W., 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), Pôle Astronomie du LESIA, and 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)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris
- Subjects
[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph] - Abstract
International audience
- Published
- 2006
243. solarFLAG hare and hounds: on the extraction of rotational p-mode splittings from seismic, Sun-as-a-star data
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Chaplin, W. J., Appourchaux, T., Baudin, F., Boumier, P., Elsworth, Y., Fletcher, S. T., Fossat, E., Garcia, R. A., Isaak, G. R., Jimenez, A., Jimenez-Reyes, S. J., Lazrek, M., Leibacher, J. W., Lochard, J., New, R., Palle, P., Regulo, C., Salabert, D., Seghouani, N., Toutain, T., and Wachter, R.
- Subjects
Astrophysics (astro-ph) ,Astrophysics::Solar and Stellar Astrophysics ,FOS: Physical sciences ,Astrophysics::Earth and Planetary Astrophysics ,Astrophysics - Abstract
We report on results from the first solar Fitting at Low-Angular degree Group (solar FLAG) hare-and-hounds exercise. The group is concerned with the development of methods for extracting the parameters of low-l solar p mode data (`peak bagging'), collected by Sun-as-a-star observations. Accurate and precise estimation of the fundamental parameters of the p modes is a vital pre-requisite of all subsequent studies. Nine members of the FLAG (the `hounds') fitted an artificial 3456-d dataset. The dataset was made by the `hare' (WJC) to simulate full-disc Doppler velocity observations of the Sun. The rotational frequency splittings of the l=1, 2 and 3 modes were the first parameter estimates chosen for scrutiny. Significant differences were uncovered at l=2 and 3 between the fitted splittings of the hounds. Evidence is presented that suggests this unwanted bias had its origins in several effects. The most important came from the different way in which the hounds modeled the visibility ratio of the different rotationally split components. Our results suggest that accurate modelling of the ratios is vital to avoid the introduction of significant bias in the estimated splittings. This is of importance not only for studies of the Sun, but also of the solar analogues that will targets for asteroseismic campaigns.
- Published
- 2006
- Full Text
- View/download PDF
244. Solar FLAG hare and hounds: on the extraction of rotational p-mode splittings from seismic, Sun-as-a-star data
- Author
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Chaplin, W. J., Thierry Appourchaux, Baudin, F., Boumier, P., Elsworth, Y., Fletcher, S. T., Fossat, E., García, R. A., Isaak, G. R., Jiménez, A., Jiménez-Reyes, S. J., Lazrek, M., Leibacher, J. W., Lochard, J., New, R., Pallé, P., Régulo, C., Salabert, D., Seghouani, N., Toutain, T., Wachter, R., Laboratoire Hippolyte Fizeau (FIZEAU), Université Nice Sophia Antipolis (... - 2019) (UNS), COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de la Côte d'Azur, Université Côte d'Azur (UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-Centre National de la Recherche Scientifique (CNRS), CEA/DSM Centre de Saclay (CEA/DSM), Commissariat à l'énergie atomique et aux énergies alternatives (CEA), Laboratoire de Cosmologie, Astrophysique Stellaire & Solaire, de Planétologie et de Mécanique des Fluides (CASSIOPEE), Université Nice Sophia Antipolis (1965 - 2019) (UNS), and COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-Université Côte d'Azur (UCA)-Centre National de la Recherche Scientifique (CNRS)
- Subjects
[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph] ,[SDU]Sciences of the Universe [physics] - Abstract
Monthly Notices of the Royal Astronomical Society, 369, pp. 985-996 (2006); International audience
- Published
- 2006
245. Galactic archaeology with asteroseismology and spectroscopy: Red giants observed by CoRoT and APOGEE.
- Author
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Anders, F., Chiappini, C., Rodrigues, T. S., Miglio, A., Montalbán, J., Mosser, B., Girardi, L., Valentini, M., Noels, A., Morel, T., Johnson, J. A., Schultheis, M., Baudin, F., de Assis Peralta, R., Hekker, S., Themeß, N., Kallinger, T., García, R. A., Mathur, S., and Baglin, A.
- Subjects
OPEN clusters of stars ,GALACTIC evolution ,SPACE archaeology ,RED giants ,MILKY Way - Abstract
With the advent of the space missions CoRoT and Kepler, it has recently become feasible to determine precise asteroseismic masses and relative ages for large samples of red giant stars. We present the CoRoGEE dataset, obtained from CoRoT light curves for 606 red giants in two fields of the Galactic disc that have been co-observed by the Apache Point Observatory Galactic Evolution Experiment (APOGEE). We used the Bayesian parameter estimation code PARAM to calculate distances, extinctions, masses, and ages for these stars in a homogeneous analysis, resulting in relative statistical uncertainties of .2% in distance, ~4% in radius, ~9% in mass and ~25% in age. We also assessed systematic age uncertainties stemming from different input physics and mass loss. We discuss the correlation between ages and chemical abundance patterns of field stars over a broad radial range of the Milky Way disc (5 kpc < R
Gal < 14 kpc), focussing on the [ /Fe]-[Fe/H]-age plane in five radial bins of the Galactic disc. We find an overall agreement with the expectations of pure chemical-evolution models computed before the present data were available, especially for the outer regions. However, our data also indicate that a significant fraction of stars now observed near and beyond the solar neighbourhood migrated from inner regions. Mock CoRoGEE observations of a chemodynamical Milky Way disc model indicate that the number of high-metallicity stars in the outer disc is too high to be accounted for even by the strong radial mixing present in the model. The mock observations also show that the age distribution of the [ /Fe]-enhanced sequence in the CoRoGEE inner-disc field is much broader than expected from a combination of radial mixing and observational errors. We suggest that a thick-disc/bulge component that formed stars for more than 3 Gyr may account for these discrepancies. Our results are subject to future improvements due to (a) the still low statistics, because our sample had to be sliced into bins of Galactocentric distances and ages; (b) large uncertainties in proper motions (and therefore guiding radii); and (c) corrections to the asteroseismic mass-scaling relation. The situation will improve not only upon the upcoming Gaia data releases, but also with the foreseen increase in the number of stars with both seismic and spectroscopic information. [ABSTRACT FROM AUTHOR]- Published
- 2017
- Full Text
- View/download PDF
246. Isotopic and faunal record of high paleotemperatures in the Kimmeridgian of subpolar urals
- Author
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Zakharov, V.A., Baudin, F., Dzyuba, O.S., Daux, V., Zverev, K.V., Renard, M., Geological Institute of RAS, Russian Academy of Sciences [Moscow] (RAS), Laboratoire des Sciences du Climat et de l'Environnement [Gif-sur-Yvette] (LSCE), Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS), Géochrononologie Traceurs Archéométrie (GEOTRAC), Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris-Saclay-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)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS), Glaces et Continents, Climats et Isotopes Stables (GLACCIOS), 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), and 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)
- Subjects
[SDU.OCEAN]Sciences of the Universe [physics]/Ocean, Atmosphere ,[SDU.ENVI]Sciences of the Universe [physics]/Continental interfaces, environment ,ComputingMilieux_MISCELLANEOUS - Abstract
International audience
- Published
- 2005
247. Kystes péripupillaires bilatéraux chez un patient de 30 ans
- Author
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Guillemin, M., Blanc, J., Baudin, F., Haddad, D., Bron, A.M., and Creuzot-Garcher, C.
- Published
- 2020
- Full Text
- View/download PDF
248. Oscillation power spectra of the Sun and of Alpha Cen A: observations versus models
- Author
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Samadi, R., Goupil, M. J., Baudin, F., Georgobiani, D., Trampedach, R., Stein, R., and Nordlund, A.
- Subjects
Astrophysics (astro-ph) ,FOS: Physical sciences ,Astrophysics::Solar and Stellar Astrophysics ,Astrophysics - Abstract
Hydrodynamical, 3D simulations of the outer layers of the Sun and Alpha Cen A are used to obtain constraints on the properties of turbulent convection in such stars. These constraints enable us to compute - on the base of a theoretical model of stochastic excitation - the rate P at which p modes are excited by turbulent convection in those two stars. Results are then compared with solar seismic observations and recent observations of Alpha Cen A. For the Sun, a good agreement between observations and computed P is obtained. For Alpha Cen A a large discrepancy is obtained which origin cannot be yet identified: it can either be caused by the present data quality which is not sufficient for our purpose or by the way the intrinsic amplitudes and the life-times of the modes are determined or finally attributed to our present modelling. Nevertheless, data with higher quality or/and more adapted data reductions will likely provide constraints on the p-mode excitation mechanism in Alpha Cen A., 4 pages, 4 figures, proceedings of the SOHO14/GONG 2004 Workshop "Helio- and Asteroseismology: Towards a Golden Future" from July 12-16 2004 at New Haven CT (USA)
- Published
- 2004
249. Flag Hare-And Exercise: on the Extraction of Sectoral Mode Splittings from Full-Disc Sun-As Data
- Author
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Chaplin, W. J., Appourchaux, T., Baudin, F., Boumier, P., Elsworth, Y., Fletcher, S. T., Fossat, E., Rafael A. García, Isaak, G. R., Jiménez, A., Jiménez-Reyes, S. J., Lazrek, M., Lochard, J., New, R., Pallé, P., Régulo, C., Salabert, D., Toutain, T., Laboratoire Hippolyte Fizeau (FIZEAU), Université Nice Sophia Antipolis (... - 2019) (UNS), COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de la Côte d'Azur, Université Côte d'Azur (UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Cosmologie, Astrophysique Stellaire & Solaire, de Planétologie et de Mécanique des Fluides (CASSIOPEE), 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), Ingénieurs, Techniciens et Administratifs, and 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)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris
- Subjects
[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph] - Abstract
Proceedings of the SOHO 14 / GONG 2004 Workshop (ESA SP-559). "Helio- and Asteroseismology: Towards a Golden Future, ed. D. Danesy., n/a, p. 356 (2004); International audience
- Published
- 2004
250. High-resolution geochemical and biotic records of the Tethyan ‘Bonarelli Level’ (OAE2, latest Cenomanian) from the Calabianca-Guidaloca composite section, northwestern Sicily, Italy
- Author
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Scopelliti, G, Bellanca, A, Neri, R, Coccioni, R, Luciani, Valeria, and Baudin, F.
- Subjects
radiolarians ,Cretaceous Oceanic Anoxic Event ,Sicily ,Corg-rich deposits ,Bonarelli level equivalent ,Planktonic foraminifera ,Geochemical proxies ,Palaeoceanography - Published
- 2004
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