Author: "Leclercq F" - Searchworks@Jio Institute Digital Library Search Results

580 results on '"Leclercq F"'

1. A negligible contribution of two luminous $z$ ~ 7.5 galaxies to the ionizing photon budget of reionization

Author: Gazagnes, S., Chisholm, J., Endsley, Ryan, Berg, D. A., Leclercq, F., Jurlin, N., Saldana-Lopez, A., Finkelstein, S. L., Flury, S. R., Guseva, N. G., Henry, A., Izotov, Y. I., Jung, I., Matthee, J., and Schaerer, D.
Subjects: Astrophysics - Astrophysics of Galaxies
Abstract: We present indirect constraints on the absolute escape fraction of ionizing photons ($f_{\rm esc}^{\rm LyC}$) of the system GN 42912 which comprises two luminous galaxies ($M_{\rm UV}$ magnitudes of -20.89 and -20.37) at $z\sim7.5$, GN 42912-NE and GN 42912-SW, to determine their contribution to the ionizing photon budget of the Epoch of Reionization (EoR). The high-resolution James Webb Space Telescope NIRSpec and NIRCam observations reveal the two galaxies are separated by only ~0.1$"$ (0.5 kpc) on the sky and have a 358 km s$^{-1}$ velocity separation. GN 42912-NE and GN 42912-SW are relatively massive for this redshift (log($M_\ast/M_\odot$) $\sim$ 8.4 and 8.9, respectively), with gas-phase metallicities of 18 per cent and 23 per cent solar, O$_{32}$ ratios of 5.3 and $>5.8$, and $\beta$ slopes of $-1.92$ and $-1.51$, respectively. We use the Mg II$\lambda\lambda$2796,2803 doublet to constrain $f_{\rm esc}^{\rm LyC}$. Mg II has an ionization potential close to that of neutral hydrogen and, in the optically thin regime, can be used as an indirect tracer of the LyC leakage. We establish realistic conservative upper limits on $f_{\rm esc}^{\rm LyC}$ of 8.5 per cent for GN 42912-NE and 14 per cent for GN 42912-SW. These estimates align with $f_{\rm esc}^{\rm LyC}$ trends observed with $\beta$, O$_{32}$, and the H$\beta$ equivalent width at $z<4$. The small inferred ionized region sizes ($<0.3$ pMpc) around both galaxies indicate they have not ionized a significant fraction of the surrounding neutral gas. While these $z>7$ $f_{\rm esc}^{\rm LyC}$ constraints do not decisively determine a specific reionization model, they support a minor contribution from these two relatively luminous galaxies to the EoR., Comment: 18 pages, submitted to MNRAS
Published: 2024

2. Witnessing an extreme, highly efficient galaxy formation mode with resolved Ly$\alpha$ and LyC emission

Author: Marques-Chaves, R., Schaerer, D., Vanzella, E., Verhamme, A., Dessauges-Zavadsky, M., Chisholm, J., Leclercq, F., Upadhyaya, A., Alvarez-Marquez, J., Colina, L., Garel, T., and Messa, M.
Subjects: Astrophysics - Astrophysics of Galaxies
Abstract: J1316+2614 at z=3.613 is the UV-brightest ($M_{UV}$ = -24.7) and strongest Lyman continuum (LyC, $f_{esc}^{LyC} \approx$ 90%) emitting star-forming galaxy known, showing also signatures of inflowing gas from its blue-dominated Ly$\alpha$ profile. Here, we present high-resolution imaging with the HST and VLT of the LyC, Ly$\alpha$, rest-UV, and optical emission of J1316+2614. Detailed analysis of the LyC and UV light distributions reveals compact yet resolved profiles, with LyC and UV morphologies showing identical half-light radii of $\simeq$ 220 pc. The continuum-subtracted Ly$\alpha$ emission reveals an extended filamentary structure of $\simeq$ 6.0 kpc oriented south-north with only weak/residual flux within the stellar core, suggesting a Ly$\alpha$ "hole". J1316+2614 presents remarkably high SFR and stellar mass surface densities of log($\Sigma_{SFR}$ [$M_{\odot}$/yr/kpc^2]) = 3.47$\pm$0.11 and log($\Sigma_{M}$ [$M_{\odot}$/pc^2]) = 4.20$\pm$0.06, respectively, which are among the highest observed in star-forming galaxies. Our findings indicate that J1316+2614 is a powerful, young, and compact starburst, leaking significant LyC photons due to the lack of gas and dust within the starburst. We explore the conditions for gas expulsion using a simple energetic balance and find that, given the strong binding force in J1316+2614, a high star formation efficiency ($\epsilon_{SF} \geq 0.7$) is necessary to remove the gas and explain its exposed nature. Our results thus suggest a close link between high $\epsilon_{SF}$ and high $f_{esc}^{LyC}$. This high efficiency can also naturally explain the remarkably high SFR, UV-luminosity, and efficient mass growth of J1316+2614, where at least 62% of its mass formed in the last 6 Myr. J1316+2614 may exemplify an intense, feedback-free starburst with a high $\epsilon_{SF}$, similar to those proposed for UV-bright galaxies at high redshifts. (ABRIDGED), Comment: 15 pages and 9 figures. Accepted for publication in A&A
Published: 2024
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3. Euclid. I. Overview of the Euclid mission

Author: Euclid Collaboration, Mellier, Y., Abdurro'uf, Barroso, J. A. Acevedo, Achúcarro, A., Adamek, J., Adam, R., Addison, G. E., Aghanim, N., Aguena, M., Ajani, V., Akrami, Y., Al-Bahlawan, A., Alavi, A., Albuquerque, I. S., Alestas, G., Alguero, G., Allaoui, A., Allen, S. W., Allevato, V., Alonso-Tetilla, A. V., Altieri, B., Alvarez-Candal, A., Alvi, S., Amara, A., Amendola, L., Amiaux, J., Andika, I. T., Andreon, S., Andrews, A., Angora, G., Angulo, R. E., Annibali, F., Anselmi, A., Anselmi, S., Arcari, S., Archidiacono, M., Aricò, G., Arnaud, M., Arnouts, S., Asgari, M., Asorey, J., Atayde, L., Atek, H., Atrio-Barandela, F., Aubert, M., Aubourg, E., Auphan, T., Auricchio, N., Aussel, B., Aussel, H., Avelino, P. P., Avgoustidis, A., Avila, S., Awan, S., Azzollini, R., Baccigalupi, C., Bachelet, E., Bacon, D., Baes, M., Bagley, M. B., Bahr-Kalus, B., Balaguera-Antolinez, A., Balbinot, E., Balcells, M., Baldi, M., Baldry, I., Balestra, A., Ballardini, M., Ballester, O., Balogh, M., Bañados, E., Barbier, R., Bardelli, S., Baron, M., Barreiro, T., Barrena, R., Barriere, J. -C., Barros, B. J., Barthelemy, A., Bartolo, N., Basset, A., Battaglia, P., Battisti, A. J., Baugh, C. M., Baumont, L., Bazzanini, L., Beaulieu, J. -P., Beckmann, V., Belikov, A. N., Bel, J., Bellagamba, F., Bella, M., Bellini, E., Benabed, K., Bender, R., Benevento, G., Bennett, C. L., Benson, K., Bergamini, P., Bermejo-Climent, J. R., Bernardeau, F., Bertacca, D., Berthe, M., Berthier, J., Bethermin, M., Beutler, F., Bevillon, C., Bhargava, S., Bhatawdekar, R., Bianchi, D., Bisigello, L., Biviano, A., Blake, R. P., Blanchard, A., Blazek, J., Blot, L., Bosco, A., Bodendorf, C., Boenke, T., Böhringer, H., Boldrini, P., Bolzonella, M., Bonchi, A., Bonici, M., Bonino, D., Bonino, L., Bonvin, C., Bon, W., Booth, J. T., Borgani, S., Borlaff, A. S., Borsato, E., Bose, B., Botticella, M. T., Boucaud, A., Bouche, F., Boucher, J. S., Boutigny, D., Bouvard, T., Bouwens, R., Bouy, H., Bowler, R. A. A., Bozza, V., Bozzo, E., Branchini, E., Brando, G., Brau-Nogue, S., Brekke, P., Bremer, M. N., Brescia, M., Breton, M. -A., Brinchmann, J., Brinckmann, T., Brockley-Blatt, C., Brodwin, M., Brouard, L., Brown, M. L., Bruton, S., Bucko, J., Buddelmeijer, H., Buenadicha, G., Buitrago, F., Burger, P., Burigana, C., Busillo, V., Busonero, D., Cabanac, R., Cabayol-Garcia, L., Cagliari, M. S., Caillat, A., Caillat, L., Calabrese, M., Calabro, A., Calderone, G., Calura, F., Quevedo, B. Camacho, Camera, S., Campos, L., Canas-Herrera, G., Candini, G. P., Cantiello, M., Capobianco, V., Cappellaro, E., Cappelluti, N., Cappi, A., Caputi, K. I., Cara, C., Carbone, C., Cardone, V. F., Carella, E., Carlberg, R. G., Carle, M., Carminati, L., Caro, F., Carrasco, J. M., Carretero, J., Carrilho, P., Duque, J. Carron, Carry, B., Carvalho, A., Carvalho, C. S., Casas, R., Casas, S., Casenove, P., Casey, C. M., Cassata, P., Castander, F. J., Castelao, D., Castellano, M., Castiblanco, L., Castignani, G., Castro, T., Cavet, C., Cavuoti, S., Chabaud, P. -Y., Chambers, K. C., Charles, Y., Charlot, S., Chartab, N., Chary, R., Chaumeil, F., Cho, H., Chon, G., Ciancetta, E., Ciliegi, P., Cimatti, A., Cimino, M., Cioni, M. -R. L., Claydon, R., Cleland, C., Clément, B., Clements, D. L., Clerc, N., Clesse, S., Codis, S., Cogato, F., Colbert, J., Cole, R. E., Coles, P., Collett, T. E., Collins, R. S., Colodro-Conde, C., Colombo, C., Combes, F., Conforti, V., Congedo, G., Conseil, S., Conselice, C. J., Contarini, S., Contini, T., Conversi, L., Cooray, A. R., Copin, Y., Corasaniti, P. -S., Corcho-Caballero, P., Corcione, L., Cordes, O., Corpace, O., Correnti, M., Costanzi, M., Costille, A., Courbin, F., Mifsud, L. Courcoult, Courtois, H. M., Cousinou, M. -C., Covone, G., Cowell, T., Cragg, C., Cresci, G., Cristiani, S., Crocce, M., Cropper, M., Crouzet, P. E, Csizi, B., Cuby, J. -G., Cucchetti, E., Cucciati, O., Cuillandre, J. -C., Cunha, P. A. C., Cuozzo, V., Daddi, E., D'Addona, M., Dafonte, C., Dagoneau, N., Dalessandro, E., Dalton, G. B., D'Amico, G., Dannerbauer, H., Danto, P., Das, I., Da Silva, A., da Silva, R., Doumerg, W. d'Assignies, Daste, G., Davies, J. E., Davini, S., Dayal, P., de Boer, T., Decarli, R., De Caro, B., Degaudenzi, H., Degni, G., de Jong, J. T. A., de la Bella, L. F., de la Torre, S., Delhaise, F., Delley, D., Delucchi, G., De Lucia, G., Denniston, J., De Paolis, F., De Petris, M., Derosa, A., Desai, S., Desjacques, V., Despali, G., Desprez, G., De Vicente-Albendea, J., Deville, Y., Dias, J. D. F., Díaz-Sánchez, A., Diaz, J. J., Di Domizio, S., Diego, J. M., Di Ferdinando, D., Di Giorgio, A. M., Dimauro, P., Dinis, J., Dolag, K., Dolding, C., Dole, H., Sánchez, H. Domínguez, Doré, O., Dournac, F., Douspis, M., Dreihahn, H., Droge, B., Dryer, B., Dubath, F., Duc, P. -A., Ducret, F., Duffy, C., Dufresne, F., Duncan, C. A. J., Dupac, X., Duret, V., Durrer, R., Durret, F., Dusini, S., Ealet, A., Eggemeier, A., Eisenhardt, P. R. M., Elbaz, D., Elkhashab, M. Y., Ellien, A., Endicott, J., Enia, A., Erben, T., Vigo, J. A. Escartin, Escoffier, S., Sanz, I. Escudero, Essert, J., Ettori, S., Ezziati, M., Fabbian, G., Fabricius, M., Fang, Y., Farina, A., Farina, M., Farinelli, R., Farrens, S., Faustini, F., Feltre, A., Ferguson, A. M. N., Ferrando, P., Ferrari, A. G., Ferré-Mateu, A., Ferreira, P. G., Ferreras, I., Ferrero, I., Ferriol, S., Ferruit, P., Filleul, D., Finelli, F., Finkelstein, S. L., Finoguenov, A., Fiorini, B., Flentge, F., Focardi, P., Fonseca, J., Fontana, A., Fontanot, F., Fornari, F., Fosalba, P., Fossati, M., Fotopoulou, S., Fouchez, D., Fourmanoit, N., Frailis, M., Fraix-Burnet, D., Franceschi, E., Franco, A., Franzetti, P., Freihoefer, J., Frenk, C. . S., Frittoli, G., Frugier, P. -A., Frusciante, N., Fumagalli, A., Fumagalli, M., Fumana, M., Fu, Y., Gabarra, L., Galeotta, S., Galluccio, L., Ganga, K., Gao, H., García-Bellido, J., Garcia, K., Gardner, J. P., Garilli, B., Gaspar-Venancio, L. -M., Gasparetto, T., Gautard, V., Gavazzi, R., Gaztanaga, E., Genolet, L., Santos, R. Genova, Gentile, F., George, K., Gerbino, M., Ghaffari, Z., Giacomini, F., Gianotti, F., Gibb, G. P. S., Gillard, W., Gillis, B., Ginolfi, M., Giocoli, C., Girardi, M., Giri, S. K., Goh, L. W. K., Gómez-Alvarez, P., Gonzalez-Perez, V., Gonzalez, A. H., Gonzalez, E. J., Gonzalez, J. C., Beauchamps, S. Gouyou, Gozaliasl, G., Gracia-Carpio, J., Grandis, S., Granett, B. R., Granvik, M., Grazian, A., Gregorio, A., Grenet, C., Grillo, C., Grupp, F., Gruppioni, C., Gruppuso, A., Guerbuez, C., Guerrini, S., Guidi, M., Guillard, P., Gutierrez, C. M., Guttridge, P., Guzzo, L., Gwyn, S., Haapala, J., Haase, J., Haddow, C. R., Hailey, M., Hall, A., Hall, D., Hamaus, N., Haridasu, B. S., Harnois-Déraps, J., Harper, C., Hartley, W. G., Hasinger, G., Hassani, F., Hatch, N. A., Haugan, S. V. H., Häußler, B., Heavens, A., Heisenberg, L., Helmi, A., Helou, G., Hemmati, S., Henares, K., Herent, O., Hernández-Monteagudo, C., Heuberger, T., Hewett, P. C., Heydenreich, S., Hildebrandt, H., Hirschmann, M., Hjorth, J., Hoar, J., Hoekstra, H., Holland, A. D., Holliman, M. S., Holmes, W., Hook, I., Horeau, B., Hormuth, F., Hornstrup, A., Hosseini, S., Hu, D., Hudelot, P., Hudson, M. J., Huertas-Company, M., Huff, E. M., Hughes, A. C. N., Humphrey, A., Hunt, L. K., Huynh, D. D., Ibata, R., Ichikawa, K., Iglesias-Groth, S., Ilbert, O., Ilić, S., Ingoglia, L., Iodice, E., Israel, H., Israelsson, U. E., Izzo, L., Jablonka, P., Jackson, N., Jacobson, J., Jafariyazani, M., Jahnke, K., Jain, B., Jansen, H., Jarvis, M. J., Jasche, J., Jauzac, M., Jeffrey, N., Jhabvala, M., Jimenez-Teja, Y., Muñoz, A. Jimenez, Joachimi, B., Johansson, P. H., Joudaki, S., Jullo, E., Kajava, J. J. E., Kang, Y., Kannawadi, A., Kansal, V., Karagiannis, D., Kärcher, M., Kashlinsky, A., Kazandjian, M. V., Keck, F., Keihänen, E., Kerins, E., Kermiche, S., Khalil, A., Kiessling, A., Kiiveri, K., Kilbinger, M., Kim, J., King, R., Kirkpatrick, C. C., Kitching, T., Kluge, M., Knabenhans, M., Knapen, J. H., Knebe, A., Kneib, J. -P., Kohley, R., Koopmans, L. V. E., Koskinen, H., Koulouridis, E., Kou, R., Kovács, A., Kovačić, I., Kowalczyk, A., Koyama, K., Kraljic, K., Krause, O., Kruk, S., Kubik, B., Kuchner, U., Kuijken, K., Kümmel, M., Kunz, M., Kurki-Suonio, H., Lacasa, F., Lacey, C. G., La Franca, F., Lagarde, N., Lahav, O., Laigle, C., La Marca, A., La Marle, O., Lamine, B., Lam, M. C., Lançon, A., Landt, H., Langer, M., Lapi, A., Larcheveque, C., Larsen, S. S., Lattanzi, M., Laudisio, F., Laugier, D., Laureijs, R., Laurent, V., Lavaux, G., Lawrenson, A., Lazanu, A., Lazeyras, T., Boulc'h, Q. Le, Brun, A. M. C. Le, Brun, V. Le, Leclercq, F., Lee, S., Graet, J. Le, Legrand, L., Leirvik, K. N., Jeune, M. Le, Lembo, M., Mignant, D. Le, Lepinzan, M. D., Lepori, F., Reun, A. Le, Leroy, G., Lesci, G. F., Lesgourgues, J., Leuzzi, L., Levi, M. E., Liaudat, T. I., Libet, G., Liebing, P., Ligori, S., Lilje, P. B., Lin, C. -C., Linde, D., Linder, E., Lindholm, V., Linke, L., Li, S. -S., Liu, S. J., Lloro, I., Lobo, F. S. N., Lodieu, N., Lombardi, M., Lombriser, L., Lonare, P., Longo, G., López-Caniego, M., Lopez, X. Lopez, Alvarez, J. Lorenzo, Loureiro, A., Loveday, J., Lusso, E., Macias-Perez, J., Maciaszek, T., Maggio, G., Magliocchetti, M., Magnard, F., Magnier, E. A., Magro, A., Mahler, G., Mainetti, G., Maino, D., Maiorano, E., Malavasi, N., Mamon, G. A., Mancini, C., Mandelbaum, R., Manera, M., Manjón-García, A., Mannucci, F., Mansutti, O., Outeiro, M. Manteiga, Maoli, R., Maraston, C., Marcin, S., Marcos-Arenal, P., Margalef-Bentabol, B., Marggraf, O., Marinucci, D., Marinucci, M., Markovic, K., Marleau, F. R., Marpaud, J., Martignac, J., Martín-Fleitas, J., Martin-Moruno, P., Martin, E. L., Martinelli, M., Martinet, N., Martin, H., Martins, C. J. A. P., Marulli, F., Massari, D., Massey, R., Masters, D. C., Matarrese, S., Matsuoka, Y., Matthew, S., Maughan, B. J., Mauri, N., Maurin, L., Maurogordato, S., McCarthy, K., McConnachie, A. W., McCracken, H. J., McDonald, I., McEwen, J. D., McPartland, C. J. R., Medinaceli, E., Mehta, V., Mei, S., Melchior, M., Melin, J. -B., Ménard, B., Mendes, J., Mendez-Abreu, J., Meneghetti, M., Mercurio, A., Merlin, E., Metcalf, R. B., Meylan, G., Migliaccio, M., Mignoli, M., Miller, L., Miluzio, M., Milvang-Jensen, B., Mimoso, J. P., Miquel, R., Miyatake, H., Mobasher, B., Mohr, J. J., Monaco, P., Monguió, M., Montoro, A., Mora, A., Dizgah, A. Moradinezhad, Moresco, M., Moretti, C., Morgante, G., Morisset, N., Moriya, T. J., Morris, P. W., Mortlock, D. J., Moscardini, L., Mota, D. F., Mottet, S., Moustakas, L. A., Moutard, T., Müller, T., Munari, E., Murphree, G., Murray, C., Murray, N., Musi, P., Nadathur, S., Nagam, B. C., Nagao, T., Naidoo, K., Nakajima, R., Nally, C., Natoli, P., Navarro-Alsina, A., Girones, D. Navarro, Neissner, C., Nersesian, A., Nesseris, S., Nguyen-Kim, H. N., Nicastro, L., Nichol, R. C., Nielbock, M., Niemi, S. -M., Nieto, S., Nilsson, K., Noller, J., Norberg, P., Nouri-Zonoz, A., Ntelis, P., Nucita, A. A., Nugent, P., Nunes, N. J., Nutma, T., Ocampo, I., Odier, J., Oesch, P. A., Oguri, M., Oliveira, D. Magalhaes, Onoue, M., Oosterbroek, T., Oppizzi, F., Ordenovic, C., Osato, K., Pacaud, F., Pace, F., Padilla, C., Paech, K., Pagano, L., Page, M. J., Palazzi, E., Paltani, S., Pamuk, S., Pandolfi, S., Paoletti, D., Paolillo, M., Papaderos, P., Pardede, K., Parimbelli, G., Parmar, A., Partmann, C., Pasian, F., Passalacqua, F., Paterson, K., Patrizii, L., Pattison, C., Paulino-Afonso, A., Paviot, R., Peacock, J. A., Pearce, F. R., Pedersen, K., Peel, A., Peletier, R. F., Ibanez, M. Pellejero, Pello, R., Penny, M. T., Percival, W. J., Perez-Garrido, A., Perotto, L., Pettorino, V., Pezzotta, A., Pezzuto, S., Philippon, A., Pierre, M., Piersanti, O., Pietroni, M., Piga, L., Pilo, L., Pires, S., Pisani, A., Pizzella, A., Pizzuti, L., Plana, C., Polenta, G., Pollack, J. E., Poncet, M., Pöntinen, M., Pool, P., Popa, L. A., Popa, V., Popp, J., Porciani, C., Porth, L., Potter, D., Poulain, M., Pourtsidou, A., Pozzetti, L., Prandoni, I., Pratt, G. W., Prezelus, S., Prieto, E., Pugno, A., Quai, S., Quilley, L., Racca, G. D., Raccanelli, A., Rácz, G., Radinović, S., Radovich, M., Ragagnin, A., Ragnit, U., Raison, F., Ramos-Chernenko, N., Ranc, C., Rasera, Y., Raylet, N., Rebolo, R., Refregier, A., Reimberg, P., Reiprich, T. H., Renk, F., Renzi, A., Retre, J., Revaz, Y., Reylé, C., Reynolds, L., Rhodes, J., Ricci, F., Ricci, M., Riccio, G., Ricken, S. O., Rissanen, S., Risso, I., Rix, H. -W., Robin, A. C., Rocca-Volmerange, B., Rocci, P. -F., Rodenhuis, M., Rodighiero, G., Monroy, M. Rodriguez, Rollins, R. P., Romanello, M., Roman, J., Romelli, E., Romero-Gomez, M., Roncarelli, M., Rosati, P., Rosset, C., Rossetti, E., Roster, W., Rottgering, H. J. A., Rozas-Fernández, A., Ruane, K., Rubino-Martin, J. A., Rudolph, A., Ruppin, F., Rusholme, B., Sacquegna, S., Sáez-Casares, I., Saga, S., Saglia, R., Sahlén, M., Saifollahi, T., Sakr, Z., Salvalaggio, J., Salvaterra, R., Salvati, L., Salvato, M., Salvignol, J. -C., Sánchez, A. G., Sanchez, E., Sanders, D. B., Sapone, D., Saponara, M., Sarpa, E., Sarron, F., Sartori, S., Sartoris, B., Sassolas, B., Sauniere, L., Sauvage, M., Sawicki, M., Scaramella, R., Scarlata, C., Scharré, L., Schaye, J., Schewtschenko, J. A., Schindler, J. -T., Schinnerer, E., Schirmer, M., Schmidt, F., Schmidt, M., Schneider, A., Schneider, M., Schneider, P., Schöneberg, N., Schrabback, T., Schultheis, M., Schulz, S., Schuster, N., Schwartz, J., Sciotti, D., Scodeggio, M., Scognamiglio, D., Scott, D., Scottez, V., Secroun, A., Sefusatti, E., Seidel, G., Seiffert, M., Sellentin, E., Selwood, M., Semboloni, E., Sereno, M., Serjeant, S., Serrano, S., Setnikar, G., Shankar, F., Sharples, R. M., Short, A., Shulevski, A., Shuntov, M., Sias, M., Sikkema, G., Silvestri, A., Simon, P., Sirignano, C., Sirri, G., Skottfelt, J., Slezak, E., Sluse, D., Smith, G. P., Smith, L. C., Smith, R. E., Smit, S. J. A., Soldano, F., Solheim, B. G. B., Sorce, J. G., Sorrenti, F., Soubrie, E., Spinoglio, L., Mancini, A. Spurio, Stadel, J., Stagnaro, L., Stanco, L., Stanford, S. A., Starck, J. -L., Stassi, P., Steinwagner, J., Stern, D., Stone, C., Strada, P., Strafella, F., Stramaccioni, D., Surace, C., Sureau, F., Suyu, S. H., Swindells, I., Szafraniec, M., Szapudi, I., Taamoli, S., Talia, M., Tallada-Crespí, P., Tanidis, K., Tao, C., Tarrío, P., Tavagnacco, D., Taylor, A. N., Taylor, J. E., Taylor, P. L., Teixeira, E. M., Tenti, M., Idiago, P. Teodoro, Teplitz, H. I., Tereno, I., Tessore, N., Testa, V., Testera, G., Tewes, M., Teyssier, R., Theret, N., Thizy, C., Thomas, P. D., Toba, Y., Toft, S., Toledo-Moreo, R., Tolstoy, E., Tommasi, E., Torbaniuk, O., Torradeflot, F., Tortora, C., Tosi, S., Tosti, S., Trifoglio, M., Troja, A., Trombetti, T., Tronconi, A., Tsedrik, M., Tsyganov, A., Tucci, M., Tutusaus, I., Uhlemann, C., Ulivi, L., Urbano, M., Vacher, L., Vaillon, L., Valageas, P., Valdes, I., Valentijn, E. A., Valenziano, L., Valieri, C., Valiviita, J., Broeck, M. Van den, Vassallo, T., Vavrek, R., Vega-Ferrero, J., Venemans, B., Venhola, A., Ventura, S., Kleijn, G. Verdoes, Vergani, D., Verma, A., Vernizzi, F., Veropalumbo, A., Verza, G., Vescovi, C., Vibert, D., Viel, M., Vielzeuf, P., Viglione, C., Viitanen, A., Villaescusa-Navarro, F., Vinciguerra, S., Visticot, F., Voggel, K., von Wietersheim-Kramsta, M., Vriend, W. J., Wachter, S., Walmsley, M., Walth, G., Walton, D. M., Walton, N. A., Wander, M., Wang, L., Wang, Y., Weaver, J. R., Weller, J., Wetzstein, M., Whalen, D. J., Whittam, I. H., Widmer, A., Wiesmann, M., Wilde, J., Williams, O. R., Winther, H. -A., Wittje, A., Wong, J. H. W., Wright, A. H., Yankelevich, V., Yeung, H. W., Yoon, M., Youles, S., Yung, L. Y. A., Zacchei, A., Zalesky, L., Zamorani, G., Vitorelli, A. Zamorano, Marc, M. Zanoni, Zennaro, M., Zerbi, F. M., Zinchenko, I. A., Zoubian, J., Zucca, E., and Zumalacarregui, M.
Subjects: Astrophysics - Cosmology and Nongalactic Astrophysics, Astrophysics - Astrophysics of Galaxies, Astrophysics - Instrumentation and Methods for Astrophysics
Abstract: The current standard model of cosmology successfully describes a variety of measurements, but the nature of its main ingredients, dark matter and dark energy, remains unknown. Euclid is a medium-class mission in the Cosmic Vision 2015-2025 programme of the European Space Agency (ESA) that will provide high-resolution optical imaging, as well as near-infrared imaging and spectroscopy, over about 14,000 deg^2 of extragalactic sky. In addition to accurate weak lensing and clustering measurements that probe structure formation over half of the age of the Universe, its primary probes for cosmology, these exquisite data will enable a wide range of science. This paper provides a high-level overview of the mission, summarising the survey characteristics, the various data-processing steps, and data products. We also highlight the main science objectives and expected performance., Comment: Accepted for publication in the A&A special issue`Euclid on Sky'
Published: 2024

4. Ubiquitous broad-line emission and the relation between ionized gas outflows and Lyman continuum escape in Green Pea galaxies

Author: Amorín, R. O., Rodríguez-Henríquez, M., Fernández, V., Vílchez, J. M., Marques-Chaves, R., Schaerer, D., Izotov, Y. I., Firpo, V., Guseva, N., Jaskot, A. E., Komarova, L., Muñoz-Vergara, D., Oey, M. S., Bait, O., Carr, C., Chisholm, J., Ferguson, H., Flury, S. R., Giavalisco, M., Hayes, M. J., Henry, A., Ji, Z., King, W., Leclercq, F., Östlin, G., Pentericci, L., Saldana-Lopez, A., Thuan, T. X., Trebitsch, M., Wang, B., Worseck, G., and Xu, X.
Subjects: Astrophysics - Astrophysics of Galaxies, Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: We report observational evidence of highly turbulent ionized gas kinematics in a sample of 20 Lyman continuum (LyC) emitters (LCEs) at low redshift ($z\sim 0.3$). Detailed Gaussian modeling of optical emission line profiles in high-dispersion spectra consistently shows that both bright recombination and collisionally excited lines can be fitted as one or two narrow components with intrinsic velocity dispersion of $\sigma$ $\sim$ 40-100 km s$^{-1}$, in addition to a broader component with $\sigma \sim$ 100-300 km s$^{-1}$, which contributes up to $\sim$40% of the total flux and is preferentially blueshifted from the systemic velocity. We interpret the narrow emission as highly ionized gas close to the young massive star clusters and the broader emission as a signpost of unresolved ionized outflows, resulting from massive stars and supernova feedback. We find a significant correlation between the width of the broad emission and the LyC escape fraction, with strong LCEs exhibiting more complex and broader line profiles than galaxies with weaker or undetected LyC emission. We provide new observational evidence supporting predictions from models and simulations; our findings suggest that gas turbulence and outflows resulting from strong radiative and mechanical feedback play a key role in clearing channels through which LyC photons escape from galaxies. We propose that the detection of blueshifted broad emission in the nebular lines of compact extreme emission-line galaxies can provide a new indirect diagnostic of Lyman photon escape, which could be useful to identify potential LyC leakers in the epoch of reionization with the JWST., Comment: 11 Pages, 7 Figures. A&A in Press
Published: 2024
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5. Equivalent widths of Lyman $\alpha$ emitters in MUSE-Wide and MUSE-Deep

Author: Kerutt, J., Wisotzki, L., Verhamme, A., Schmidt, K. B., Leclercq, F., Herenz, E. C., Urrutia, T., Garel, T., Hashimoto, T., Maseda, M., Matthee, J., Kusakabe, H., Schaye, J., Richard, J., Guiderdoni, B., Mauerhofer, V., Nanayakkara, T., and Vitte, E.
Subjects: Astrophysics - Astrophysics of Galaxies
Abstract: The aim of this study is to better understand the connection between the Lyman $\alpha$ rest-frame equivalent width (EW$_0$) and spectral properties as well as ultraviolet (UV) continuum morphology by obtaining reliable EW$_0$ histograms for a statistical sample of galaxies and by assessing the fraction of objects with large equivalent widths. We used integral field spectroscopy from MUSE combined with broad-band data from the Hubble Space Telescope (HST) to measure EW$_0$. We analysed the emission lines of $1920$ Lyman $\alpha$ emitters (LAEs) detected in the full MUSE-Wide (one hour exposure time) and MUSE-Deep (ten hour exposure time) surveys and found UV continuum counterparts in archival HST data. We fitted the UV continuum photometric images using the Galfit software to gain morphological information on the rest-UV emission and fitted the spectra obtained from MUSE to determine the double peak fraction, asymmetry, full-width at half maximum, and flux of the Lyman $\alpha$ line. The two surveys show different histograms of Lyman $\alpha$ EW$_0$. In MUSE-Wide, $20\%$ of objects have EW$_0 > 240$ \r{A}, while this fraction is only $11\%$ in MUSE-Deep and $\approx 16\%$ for the full sample. This includes objects without HST continuum counterparts (one-third of our sample), for which we give lower limits for EW$_0$. The object with the highest securely measured EW$_0$ has EW$_0=589 \pm 193$ \r{A} (the highest lower limit being EW$_0=4464$ \r{A}). We investigate the connection between EW$_0$ and Lyman $\alpha$ spectral or UV continuum morphological properties. The survey depth has to be taken into account when studying EW$_0$ distributions. We find that in general, high EW$_0$ objects can have a wide range of spectral and UV morphological properties, which might reflect that the underlying causes for high EW$_0$ values are equally varied. (abridged), Comment: 28 pages, 21 + 1 figures, 7 + 1 tables, accepted for publication in A&A
Published: 2022
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6. The Lensed Lyman-Alpha MUSE Arcs Sample (LLAMAS) : I. Characterisation of extended Lyman-alpha haloes and spatial offsets

Author: Claeyssens, A., Richard, J., Blaizot, J., Garel, T., Kusakabe, H., Bacon, R., Bauer, F. E., Guaita, L., Jeanneau, A., Lagattuta, D., Leclercq, F., Maseda, M., Matthee, J., Nanayakkara, T., Pello, R., Thai, T. T., Tuan-Anh, P., Verhamme, A., Vitte, E., and Wisotzki, L.
Subjects: Astrophysics - Astrophysics of Galaxies
Abstract: We present the Lensed Lyman-Alpha MUSE Arcs Sample (LLAMAS) selected from MUSE and HST observations of 17 lensing clusters. The sample consists of 603 continuum-faint (-23
Published: 2022
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7. Recovery and analysis of rest-frame UV emission lines in 2052 galaxies observed with MUSE at $1.5 < z < 6.4$

Author: Schmidt, K. B., Kerutt, J., Wisotzki, L., Urrutia, T., Feltre, A., Maseda, M. V., Nanayakkara, T., Bacon, R., Boogaard, L. A., Conseil, S., Contini, T., Herenz, E. C., Kollatschny, W., Krumpe, M., Leclercq, F., Mahler, G., Matthee, J., Mauerhofer, V., Richard, J., and Schaye, J.
Subjects: Astrophysics - Astrophysics of Galaxies, Astrophysics - Instrumentation and Methods for Astrophysics
Abstract: [Abbreviated] Rest-frame UV emission lines probe physical parameters of the emitting star-forming galaxies and their environments. The strongest main UV line, Ly$\alpha$, has been instrumental in advancing the general knowledge of galaxy formation in the early universe. However, observing Ly$\alpha$ emission becomes increasingly challenging at $z \gtrsim 6$ when the neutral hydrogen fraction of the CGM and IGM increases. Secondary weaker UV emission lines provide important alternative methods for studying galaxy properties at high redshift. We present a large sample of rest-frame UV emission line sources at intermediate redshift for calibrating and exploring the connection between secondary UV lines and the emitting galaxies' physical properties and their Ly$\alpha$ emission. The sample of 2052 emission line sources with $1.5 < z < 6.4$ was selected through untargeted source detection in three-dimensional MUSE data cubes. We searched optimally extracted 1D spectra of the full sample for UV emission features via emission line template matching, resulting in a sample of more than 100 rest-frame UV emission line detections. We show that the detection efficiency of (non-Ly$\alpha$) UV emission lines increases with survey depth, and that the UV emission line strength often correlate with the strength of Ciii]. We measured the velocity offsets of resonant emission lines with respect to systemic tracers as well as the electron density and the gas-phase abundance. Lastly, using "PhotoIonization Model Probability Density Functions" we find that the UV line emitters generally have ionization parameter log10(U) $\approx$ -2.5 and metal mass fractions that scatter around Z $\approx$ 10$^{-2}$, that is Z $\approx$ 0.66Z$\odot$. Value-added catalogs of the full sample of MUSE objects studied in this work and a collection of UV line emitters from the literature are provided with this paper., Comment: Accepted by A&A. Contains 54 pages, 21 figures, and appendices. Catalogs described in Tables B.1 and C.1 will be made available with published paper
Published: 2021
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8. The Multiple Merger Assembly of a Hyper-luminous Obscured Quasar at redshift 4.6

Author: Diaz-Santos, T., Assef, R. J., Blain, A. W., Aravena, M., Stern, D., Tsai, C. -W., Eisenhardt, P., Wu, J., Jun, H. D., Dibert, K., Inami, H., Lansbury, G., and Leclercq, F.
Subjects: Astrophysics - Astrophysics of Galaxies
Abstract: Galaxy mergers and gas accretion from the cosmic web drove the growth of galaxies and their central black holes at early epochs. We report spectroscopic imaging of a multiple merger event in the most luminous known galaxy, WISE J224607.56-052634.9 (W2246-0526), a dust-obscured quasar at redshift 4.6, 1.3 Gyr after the Big Bang. Far-infrared dust continuum observations show three galaxy companions around W2246-0526 with disturbed morphologies, connected by streams of dust likely produced by the dynamical interaction. The detection of tidal dusty bridges shows that W2246-0526 is accreting its neighbors, suggesting merger activity may be a dominant mechanism through which the most luminous galaxies simultaneously obscure and feed their central supermassive black holes., Comment: To be published in Science on the 15th of November 2018
Published: 2018
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9. Nearly all the sky is covered by Lyman-alpha emission around high redshift galaxies

Author: Wisotzki, L., Bacon, R., Brinchmann, J., Cantalupo, S., Richter, P., Schaye, J., Schmidt, K. B., Urrutia, T., Weilbacher, P. M., Akhlaghi, M., Bouche, N., Contini, T., Guiderdoni, B., Herenz, E. C., Inami, H., Kerutt, J., Leclercq, F., Marino, R. A., Maseda, M., Monreal-Ibero, A., Nanayakkara, T., Richard, J., Saust, R., Steinmetz, M., and Wendt, M.
Subjects: Astrophysics - Astrophysics of Galaxies
Abstract: Galaxies are surrounded by large reservoirs of gas, mostly hydrogen, fed by inflows from the intergalactic medium and by outflows due to galactic winds. Absorption-line measurements along the sightlines to bright and rare background quasars indicate that this circumgalactic medium pervades far beyond the extent of starlight in galaxies, but very little is known about the spatial distribution of this gas. A new window into circumgalactic environments was recently opened with the discovery of ubiquitous extended Lyman-alpha emission from hydrogen around high-redshift galaxies, facilitated by the extraordinary sensitivity of the MUSE instrument at the ESO Very Large Telescope. Due to the faintness of this emission, such measurements were previously limited to especially favourable systems or to massive statistical averaging. Here we demonstrate that low surface brightness Lyman-alpha emission surrounding faint galaxies at redshifts between 3 and 6 adds up to a projected sky coverage of nearly 100%. The corresponding rate of incidence (the mean number of Lyman-alpha emitters penetrated by any arbitrary line of sight) is well above unity and similar to the incidence rate of high column density absorbers frequently detected in the spectra of distant quasars. This similarity suggests that most circumgalactic atomic hydrogen at these redshifts has now been detected also in emission., Comment: published in Nature, online on 01 Oct 2018, in print on 11 Oct 2018. This is the Authors' version, for the published version see https://www.nature.com/articles/s41586-018-0564-6 ; free viewing access via https://rdcu.be/8eCx
Published: 2018
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10. Recovering the systemic redshift of galaxies from their Lyman-alpha line profile

Author: Verhamme, A., Garel, T., Ventou, E., Contini, T., Bouché, N., Herenz, E. C., Richard, J., Bacon, R., Schmidt, K. B., Maseda, M., Marino, R. A., Brinchmann, J., Cantalupo, S., Caruana, J., Clément, B., Diener, C., Drake, A. B., Hashimoto, T., Inami, H., Kerutt, J., Kollatschny, W., Leclercq, F., Patrício, V., Schaye, J., Wisotzki, L., and Zabl, J.
Subjects: Astrophysics - Astrophysics of Galaxies
Abstract: The Lyman alpha (lya) line of Hydrogen is a prominent feature in the spectra of star-forming galaxies, usually redshifted by a few hundreds of km/s compared to the systemic redshift. This large offset hampers follow-up surveys, galaxy pair statistics and correlations with quasar absorption lines when only lya is available. We propose diagnostics that can be used to recover the systemic redshift directly from the properties of the lya line profile. We use spectroscopic observations of Lyman-Alpha Emitters (LAEs) for which a precise measurement of the systemic redshift is available. Our sample contains 13 sources detected between z~3 and z~6 as part of various Multi Unit Spectroscopic Explorer (MUSE) Guaranteed Time Observations (GTO). We also include a compilation of spectroscopic lya data from the literature spanning a wide redshift range (z~0-8). First, restricting our analysis to double-peaked lya spectra, we find a tight correlation between the velocity offset of the red peak with respect to the systemic redshift, Vpeak, and the separation of the peaks. Secondly, we find a correlation between Vpeak and the full width at half maximum of the lya line. Fitting formulas, to estimate systemic redshifts of galaxies with an accuracy of +-100 km/s when only the lya emission line is available, are given for the two methods., Comment: letter, accepted for publication in MNRAS
Published: 2018
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11. Audiométrie vocale dans le bruit : valeurs normales par classe d’âge

Author: Decambron, M., Leclercq, F., Renard, C., and Vincent, C.
Published: 2022
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12. Speech audiometry in noise: SNR Loss per age-group in normal hearing subjects

Author: Decambron, M., Leclercq, F., Renard, C., and Vincent, C.
Published: 2022
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13. The MUSE Hubble Ultra Deep Field Survey VI: The Faint-End of the Lya Luminosity Function at 2.91 < z < 6.64 and Implications for Reionisation

Author: Drake, A. B., Garel, T., Wisotzki, L., Leclercq, F., Hashimoto, T., Richard, J., Bacon, R., Blaizot, J., Caruana, J., Conseil, S., Contini, T., Guiderdoni, B., Herenz, E. C., Inami, H., Lewis, J., Mahler, G., Marino, R. A., Pello, R., Schaye, J., Verhamme, A., Ventou, E., and Weilbacher, P. M.
Subjects: Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: We present the deepest study to date of the Lya luminosity function (LF) in a blank field using blind integral field spectroscopy from MUSE. We constructed a sample of 604 Lya emitters (LAEs) across the redshift range 2.91 < z < 6.64 using automatic detection software in the Hubble Ultra Deep Field. We calculate accurate total Lya fluxes capturing low surface brightness extended Lya emission now known to be a generic property of high-redshift star-forming galaxies. We simulated realistic extended LAEs to characterise the selection function of our samples, and performed flux-recovery experiments to test and correct for bias in our determination of total Lya fluxes. We find an accurate completeness correction accounting for extended emission reveals a very steep faint-end slope of the LF, alpha, down to luminosities of log10 L erg s^-1< 41.5, applying both the 1/Vmax and maximum likelihood estimators. Splitting the sample into three broad redshift bins, we see the faint-end slope increasing from -2.03+1.42-inf at z ~ 3.44 to -2.86+0.76-inf at z ~ 5.48, however no strong evolution is seen between the 68% confidence regions in L*-alpha parameter space. Using the Lya line flux as a proxy for star formation activity, and integrating the observed LFs, we find that LAEs' contribution to the cosmic SFRD rises with redshift until it is comparable to that from continuum-selected samples by z ~ 6. This implies that LAEs may contribute more to the star-formation activity of the early Universe than previously thought - any additional interglactic medium correction would act to further boost the Lya luminosities. Finally, assuming fiducial values for the escape of Lya and LyC radiation, and the clumpiness of the IGM, we integrated the maximum likelihood LF at 5.00 < z < 6.64 and find we require only a small extrapolation beyond the data (< 1 dex in L) for LAEs alone to maintain an ionised IGM at z ~ 6., Comment: 16 pages, 10 figures. Accepted for publication in A&A special issue: "The MUSE Hubble Ultra Deep Field Survey" (MUSE UDF Series Paper VI)
Published: 2017
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14. The MUSE Hubble Ultra Deep Field Survey: II. Spectroscopic redshifts and comparisons to color selections of high-redshift galaxies

Author: Inami, H., Bacon, R., Brinchmann, J., Richard, J., Contini, T., Conseil, S., Hamer, S., Akhlaghi, M., Bouche, N., Clement, B., Desprez, G., Drake, A. B., Hashimoto, T., Leclercq, F., Maseda, M., Michel-Dansac, L., Paalvast, M., Tresse, L., Ventou, E., Kollatschny, W., Boogaard, L. A., Finley, H., Marino, R. A., Schaye, J., and Wisotzki, L.
Subjects: Astrophysics - Astrophysics of Galaxies
Abstract: We have conducted a two-layered spectroscopic survey (1'x1' ultra deep and 3'x3' deep regions) in the Hubble Ultra Deep Field (HUDF) with the Multi Unit Spectroscopic Explorer (MUSE). The combination of a large field of view, high sensitivity, and wide wavelength coverage provides an order of magnitude improvement in spectroscopically confirmed redshifts in the HUDF; i.e., 1206 secure spectroscopic redshifts for HST continuum selected objects, which corresponds to 15% of the total (7904). The redshift distribution extends well beyond z>3 and to HST/F775W magnitudes as faint as ~30 mag (AB, 1-sigma). In addition, 132 secure redshifts were obtained for sources with no HST counterparts that were discovered in the MUSE data cubes by a blind search for emission-line features. In total, we present 1338 high quality redshifts, which is a factor of eight increase compared with the previously known spectroscopic redshifts in the same field. We assessed redshifts mainly with the spectral features [OII] at z<1.5 (473 objects) and Lya at 2.9~20% up to 28-29 mag and ~27 mag, respectively. We used the determined redshifts to test continuum color selection (dropout) diagrams of high-z galaxies. The selection condition for F336W dropouts successfully captures ~80% of the targeted z~2.7 galaxies. However, for higher redshift selections (F435W, F606W, and F775W dropouts), the success rates decrease to ~20-40%. We empirically redefine the selection boundaries to make an attempt to improve them to ~60%. The revised boundaries allow bluer colors that capture Lya emitters with high Lya equivalent widths falling in the broadbands used for the color-color selection. Along with this paper, we release the redshift and line flux catalog., Comment: 26 pages, 26 figures, 4 tables, accepted for publication in A&A (MUSE UDF Series Paper II), the redshift catalogs will be available at the CDS
Published: 2017
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15. Strong lensing analysis of Abell 2744 with MUSE and Hubble Frontier Fields images

Author: Mahler, G., Richard, J., Clément, B., Lagattuta, D., Schmidt, K., Patrício, V., Soucail, G., Bacon, R., Pello, R., Bouwens, R., Maseda, M., Martinez, J., Carollo, M., Inami, H., Leclercq, F., and Wisotzki, L.
Subjects: Astrophysics - Astrophysics of Galaxies
Abstract: We present an analysis of MUSE observations obtained on the massive Frontier Fields cluster Abell 2744. This new dataset covers the entire multiply-imaged region around the cluster core. We measure spectroscopic redshifts for HST-selected continuum sources together with line emitters blindly detected in the datacube. The combined catalog consists of 514 spectroscopic redshifts (with 414 new identifications), including 156 cluster members and 326 magnified background sources. We use this redshift information to perform a strong-lensing analysis of all multiple images previously found in the deep Frontier Field images, and add three new MUSE-detected multiply-imaged systems with no obvious HST counterpart. The combined strong lensing constraints include a total of 60 systems producing 188 images altogether, out of which 29 systems and 83 images are spectroscopically confirmed, making Abell 2744 one of the most well-constrained clusters to date. A parametric mass model including two cluster-scale components in the core and several group-scale substructures at larger radii accurately reproduces all the spectroscopic multiple systems, reaching an rms of 0.67" in the image plane. Overall, the large number of spectroscopic redshifts gives us a robust model and we estimate the systematics on the mass density and magnification within the cluster core to be typically ~9%., Comment: 34 pages, 20 figures. Accepted for publication in MNRAS. Full high resolution pdf and other data are available at http://muse-vlt.eu/science/a2744/
Published: 2017
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16. Witnessing an extreme, highly efficient galaxy formation mode with resolved Lyman-α and Lyman-continuum emission.

Author: Marques-Chaves, R., Schaerer, D., Vanzella, E., Verhamme, A., Dessauges-Zavadsky, M., Chisholm, J., Leclercq, F., Upadhyaya, A., Álvarez-Márquez, J., Colina, L., Garel, T., and Messa, M.
Abstract: J1316+2614 at z = 3.613 is the UV-brightest (MUV = −24.7) and strongest Lyman continuum-emitting (fescLyC ≈ 90%) star-forming galaxy known; it also shows signatures of inflowing gas from its blue-dominated Lyα profile. We present high-resolution imaging with the Hubble Space Telescope (HST) and the Very Large Telescope (VLT) of the LyC, Lyα, rest-UV, and optical emission of J1316+2614. Detailed analysis of the LyC and UV light distributions reveals compact yet resolved profiles, with LyC and UV morphologies showing identical half-light radii of reff ≃ 220 pc. The continuum-subtracted Lyα emission, obtained with the HST ramp-filter FR551N, reveals an extended filamentary structure of ≃6.0 kpc oriented south to north with only residual flux within the stellar core, suggesting a Lyα 'hole'. Our spectral energy distribution analysis shows that J1316+2614 is characterised by a young (5.7 ± 1.0 Myr), nearly un-obscured stellar population with a high star-formation rate (SFR = 898 ± 181 M⊙ yr−1) and a stellar mass of M⋆young = (4.8 ± 0.3) × 109 M⊙. Additionally, the spectral energy distribution analysis supports the absence of an underlying old stellar population (M⋆old ≤ 2.8 × 109 M⊙, 3σ). J1316+2614 presents remarkably high SFR and stellar mass surface densities of log(Σ SFR[M⊙ yr−1 kpc−2]) = 3.47 ± 0.11 and log(ΣM⋆[M⊙pc−2]) = 4.20 ± 0.06, respectively, which are among the highest observed in star-forming galaxies and are more typically observed in local young massive star clusters and globular clusters. Our findings indicate that J1316+2614 is a powerful, young, and compact starburst that is leaking a significant amount of LyC photons due to a lack of gas and dust within the starburst. We explored the conditions for gas expulsion using a simple energetic balance and find that, given the strong binding force in J1316+2614, a high star-formation efficiency (ϵSF ≥ 0.7) is necessary to explain the removal of gas and its exposed nature. Our results thus suggest a close link between high ϵSF and high fescLyC. This high efficiency can also naturally explain the remarkably high SFR, UV luminosity, and efficient mass growth of J1316+2614, which acquired at least 62% of its mass in the last 6 Myr. J1316+2614 may exemplify an intense, feedback-free starburst with a high ϵSF, similar to those proposed for UV-bright galaxies at high redshifts. [ABSTRACT FROM AUTHOR]
Published: 2024
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17. A public grid of radiative transfer simulations for Lyα and metal lines in idealised galactic outflows.

Author: Garel, T., Michel-Dansac, L., Verhamme, A., Mauerhofer, V., Katz, H., Blaizot, J., Leclercq, F., and Salvignol, G.
Abstract: The vast majority of star-forming galaxies are surrounded by large reservoirs of gas ejected from the interstellar medium. Ultraviolet absorption and emission lines represent powerful diagnostics to constrain the cool phase of these outflows, through resonant transitions of hydrogen and metal ions. The interpretation of these observations is often remarkably difficult as it requires detailed modelling of the propagation of the continuum and emission lines in the gas. To this aim, we present a large public grid of ≈20 000 simulated spectra that includes H I Lyα and five metal transitions associated with Mg II, C II, Si II, and Fe II which is accessible online. The spectra have been computed with the RASCAS Monte Carlo radiative transfer code for 5760 idealised spherically symmetric configurations surrounding a central point source emission, and characterised by their column density, Doppler parameter, dust opacity, wind velocity, as well as various density and velocity gradients. Designed to predict and interpret Lyα and metal line profiles, our grid exhibits a wide diversity of resonant absorption and emission features, as well as fluorescent lines. We illustrate how it can help better constrain the wind properties by performing a joint modelling of observed Lyα, C II, and Si II spectra. Using CLOUDY simulations and virial scaling relations, we also show that Lyα is expected to be a faithful tracer of the gas at T ≈ 104 − 105 K, even if the medium is highly ionised. While C II is found to probe the same range of temperatures as Lyα, other metal lines merely trace cooler phases (T ≈ 104 K). As their gas opacity strongly depends on gas temperature, incident radiation field, metallicity and dust depletion, we caution that optically thin metal lines do not necessarily originate from low H I column densities and may not accurately probe Lyman continuum leakage. [ABSTRACT FROM AUTHOR]
Published: 2024
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18. Recommandations de la Société française d’ORL et de chirurgie de la face et du cou (SFORL) et de la Société française d’audiologie (SFA) pour la pratique de l’audiométrie vocale dans le bruit chez l’adulte

Author: Joly, C.-A., Reynard, P., Mezzi, K., Bakhos, D., Bergeron, F., Bonnard, D., Borel, S., Bouccara, D., Coez, A., Dejean, F., Del Rio, M., Leclercq, F., Henrion, P., Marx, M., Mom, T., Mosnier, I., Potier, M., Renard, C., Roy, T., Sterkers-Artières, F., Venail, F., Verheyden, P., Veuillet, E., Vincent, C., and Thai-Van, H.
Published: 2022
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19. Kernel-based emulator for the 3D matter power spectrum from CLASS

Author: Mootoovaloo, A., Jaffe, A.H., Heavens, A.F., and Leclercq, F.
Published: 2022
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20. Guidelines of the French Society of Otorhinolaryngology-Head and Neck Surgery (SFORL) and the French Society of Audiology (SFA) for Speech-in-Noise Testing in Adults

Author: Joly, C.-A., Reynard, P., Mezzi, K., Bakhos, D., Bergeron, F., Bonnard, D., Borel, S., Bouccara, D., Coez, A., Dejean, F., Del Rio, M., Leclercq, F., Henrion, P., Marx, M., Mom, T., Mosnier, I., Potier, M., Renard, C., Roy, T., Sterkers-Artières, F., Venail, F., Verheyden, P., Veuillet, E., Vincent, C., and Thai-Van, H.
Published: 2022
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21. Extended Lyman alpha haloes around individual high-redshift galaxies revealed by MUSE

Author: Wisotzki, L., Bacon, R., Blaizot, J., Brinchmann, J., Herenz, E. C., Schaye, J., Bouché, N., Cantalupo, S., Contini, T., Carollo, C. M., Caruana, J., Courbot, J. -B., Emsellem, E., Kamann, S., Kerutt, J., Leclercq, F., Lilly, S. J., Patrício, V., Sandin, C., Steinmetz, M., Straka, L. A., Urrutia, T., Verhamme, A., Weilbacher, P. M., and Wendt, M.
Subjects: Astrophysics - Astrophysics of Galaxies
Abstract: We report the detection of extended Ly alpha emission around individual star-forming galaxies at redshifts z = 3-6 in an ultradeep exposure of the Hubble Deep Field South obtained with MUSE on the ESO-VLT. The data reach a limiting surface brightness (1sigma) of ~1 x 10^-19 erg s^-1 cm^-2 arcsec^-2 in azimuthally averaged radial profiles, an order of magnitude improvement over previous narrowband imaging. Our sample consists of 26 spectroscopically confirmed Ly alpha-emitting, but mostly continuum-faint (m_AB >~ 27) galaxies. In most objects the Ly alpha emission is considerably more extended than the UV continuum light. While 5 of the faintest galaxies in the sample show no significantly detected Ly alpha haloes, the derived upper limits suggest that this is just due to insufficient S/N. Ly alpha haloes therefore appear to be (nearly) ubiquitous even for low-mass (~10^8-10^9 M_sun) star-forming galaxies at z>3. We decompose the Ly alpha emission of each object into a compact `continuum-like' and an extended halo component, and infer sizes and luminosities of the haloes. The extended Ly alpha emission approximately follows an exponential surface brightness distribution with a scale length of a few kpc. While these haloes are thus quite modest in terms of their absolute sizes, they are larger by a factor of 5-15 than the corresponding rest-frame UV continuum sources as seen by HST. They are also much more extended, by a factor ~5, than Ly alpha haloes around low-redshift star-forming galaxies. Between ~40% and >90% of the observed Ly alpha flux comes from the extended halo component, with no obvious correlation of this fraction with either the absolute or the relative size of the Ly alpha halo. Our observations provide direct insights into the spatial distribution of at least partly neutral gas residing in the circumgalactic medium of low to intermediate mass galaxies at z > 3., Comment: accepted by Astronomy & Astrophysics
Published: 2015
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22. Ubiquitous broad-line emission and the relation between ionized gas outflows and Lyman continuum escape in Green Pea galaxies

Author: Amorin, R.O., primary, Rodriguez-Henriquez, M., additional, Fernandez, V., additional, Vílchez, J.M., additional, Marques-Chaves, R., additional, Schaerer, D., additional, Izotov, Y.I., additional, Firpo, V., additional, Guseva, N., additional, Jaskot, A.E., additional, Komarova, L., additional, Muñoz-Vergara, D., additional, Oey, M.S., additional, Bait, O., additional, Carr, C., additional, Chisholm, J., additional, Ferguson, H., additional, Flury, S.R., additional, Giavalisco, M., additional, Hayes, M.J., additional, Henry, A., additional, Ji, Z., additional, King, W., additional, Leclercq, F., additional, Ostlin, G., additional, Pentericci, L., additional, Saldana-Lopez, A., additional, Thuan, T.X., additional, Trebitsch, M., additional, Wang, B., additional, Worseck, G., additional, and Xu, X., additional
Published: 2024
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23. ACCEPTCARDIO1: Criteria associated with patient willingness to participate in biomedical research in cardiology

Author: Soltani, S., primary, Morand, O., additional, Galtier, E., additional, Desmoulins, G., additional, Cardeur, L., additional, Faucanie, M., additional, Molinari, N., additional, Vidal, C., additional, Vachier, I., additional, Bourdin, A., additional, Delbaere, Q., additional, Leclercq, F., additional, Pasquié, J.-L., additional, and Roubille, F., additional
Published: 2024
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24. Ticagrelor versus clopidogrel for complex percutaneous coronary intervention in chronic coronary syndrome: A post-hoc analysis of the ALPHEUS study

Author: Lattuca, B., primary, Mazeau, C., additional, Cayla, G., additional, Ducrocq, G., additional, Guedeney, P., additional, Kala, P., additional, Nejjari, M., additional, Morel, O., additional, Leclercq, F., additional, Payot, L., additional, Beygui, F., additional, Rangé, G., additional, Motovska, Z., additional, Vicaut, E., additional, Collet, J.-P., additional, Montalescot, G., additional, and Silvain, J., additional
Published: 2024
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25. Simplification des procédures TAVI : mise au point

Author: Akodad, M., Lefèvre, T., Lounes, Y., and Leclercq, F.
Published: 2019
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26. Bipolar outflows out to 10 kpc for massive galaxies at redshift z ≈ 1

Author: Guo, Y, Bacon, R, Bouché, N, Wisotzki, L, Schaye, J, Blaizot, J, Verhamme, A, Cantalupo, S, Boogaard, L, Brinchmann, J, Cherrey, M, Kusakabe, H, Langan, I, Leclercq, F, Matthee, J, Michel-Dansac, L, Schroetter, I, Wendt, M, Guo Y., Bacon R., Bouché N. F., Wisotzki L., Schaye J., Blaizot J., Verhamme A., Cantalupo S., Boogaard L. A., Brinchmann J., Cherrey M., Kusakabe H., Langan I., Leclercq F., Matthee J., Michel-Dansac L., Schroetter I., Wendt M., Guo, Y, Bacon, R, Bouché, N, Wisotzki, L, Schaye, J, Blaizot, J, Verhamme, A, Cantalupo, S, Boogaard, L, Brinchmann, J, Cherrey, M, Kusakabe, H, Langan, I, Leclercq, F, Matthee, J, Michel-Dansac, L, Schroetter, I, Wendt, M, Guo Y., Bacon R., Bouché N. F., Wisotzki L., Schaye J., Blaizot J., Verhamme A., Cantalupo S., Boogaard L. A., Brinchmann J., Cherrey M., Kusakabe H., Langan I., Leclercq F., Matthee J., Michel-Dansac L., Schroetter I., and Wendt M.
Abstract: Galactic outflows are believed to play a critical role in the evolution of galaxies by regulating their mass build-up and star formation1. Theoretical models assume bipolar shapes for the outflows that extend well into the circumgalactic medium (CGM), up to tens of kiloparsecs (kpc) perpendicular to the galaxies. They have been directly observed in the local Universe in several individual galaxies, for example, around the Milky Way and M82 (refs. 2,3). At higher redshifts, cosmological simulations of galaxy formation predict an increase in the frequency and efficiency of galactic outflows owing to the increasing star-formation activity4. Galactic outflows are usually of low gas density and low surface brightness and therefore difficult to observe in emission towards high redshifts. Here we present an ultra-deep Multi-Unit Spectroscopic Explorer (MUSE) image of the mean Mg II emission surrounding a sample of galaxies at z ≈ 1 that strongly suggests the presence of outflowing gas on physical scales of more than 10 kpc. We find a strong dependence of the detected signal on the inclination of the central galaxy, with edge-on galaxies clearly showing enhanced Mg II emission along the minor axis, whereas face-on galaxies show much weaker and more isotropic emission. We interpret these findings as supporting the idea that outflows typically have a bipolar cone geometry perpendicular to the galactic disk. We demonstrate that this CGM-scale outflow is prevalent among galaxies with stellar mass M * ≳ 109.5 M ⊙.
Published: 2023

27. Ticagrelor versus clopidogrel for complex percutaneous coronary intervention in chronic coronary syndrome: a post-hoc analysis of the ALPHEUS study

Author: Lattuca, B, primary, Mazeau, C, additional, Guedeney, P, additional, Kala, P, additional, Nejjari, M, additional, Morel, O, additional, Leclercq, F, additional, Payot, L, additional, Beygui, F, additional, Range, G, additional, Motovska, Z, additional, Vicaut, E, additional, Collet, J P, additional, Montalescot, G, additional, and Silvain, J, additional
Published: 2023
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28. Up to 6-year performance and clinical outcomes of balloon expandable transcatheter aortic valve according to the implantation strategy: insight from the DIRECTAVI trial

Author: Leclercq, F, primary, Jammoul, N, additional, Dupasquier, V, additional, Akodad, M, additional, Meunier, P A, additional, Soltani, S, additional, Moulis, L, additional, Macia, J C, additional, Robert, P, additional, Schmutz, L, additional, Piot, C, additional, Targosz, F, additional, Benkemoun, H, additional, Roubille, F, additional, and Cayla, G, additional
Published: 2023
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29. The multiple merger assembly of a hyperluminous obscured quasar at redshift 4.6

Author: Díaz-Santos, T., Assef, R. J., Blain, A. W., Aravena, M., Stern, D., Tsai, C.-W., Eisenhardt, P., Wu, J., Jun, H. D., Dibert, K., Inami, H., Lansbury, G., and Leclercq, F.
Published: 2018

30. New developments of Fudaa-LSPIV, a user-friendly software to perform river velocity measurements in various flow conditions

Author: Jodeau, M., primary, Bel, C., additional, Antoine, G., additional, Bodart, G., additional, Le Coz, J., additional, Faure, J.-B., additional, Hauet, A., additional, Leclercq, F., additional, Haddad, H., additional, Legout, C., additional, and Marchand, B., additional
Published: 2020
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31. Speech audiometry in noise: Development of the French-language VRB (vocale rapide dans le bruit) test

Author: Leclercq, F., Renard, C., and Vincent, C.
Published: 2018
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32. Audiométrie vocale dans le bruit : mise au point du test VRB (vocale rapide dans le bruit)

Author: Leclercq, F., Renard, C., and Vincent, C.
Published: 2018
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33. Wearable cardioverter defibrillator shortens the length of stay: a single center real-world experience

Author: Cardelli, L S, primary, Casella, G, additional, Roubille, F, additional, Pasquie, J L, additional, and Leclercq, F, additional
Published: 2023
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34. Prise en charge du syndrome coronaire aigu avec sus-décalage de ST en France : variations régionales en 2010

Author: Sokoloff, A., Lefèvre, G., Teixeira, N., Puymirat, E., Beygui, F., Vanzetto, G., Richard, P., Khalife, K., Blanchard, D., Gilard, M., Coste, P., Farah, B., Elbaz, M., Leclercq, F., Ferrari, E., Bonnet, J.-L., Meyer, P., Belle, L., Funck, F., Motreff, P., Virot, P., Geugniaud, P.-Y., Ferrières, J., Simon, T., and Danchin, N.
Published: 2015
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35. Quelle place pour les stents biorésorbables dans la prise en charge du syndrome coronarien aigu avec sus-décalage du segment ST ?

Author: Lattuca, B., Schmutz, L., Ledermann, B., Cornillet, L., Messner-Pellenc, P., Leclercq, F., and Cayla, G.
Published: 2015
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36. Evaluation of factors influencing immunosuppressant adherence among heart transplant patients: FIAHT study

Author: Barone, J., primary, Chapet, N., additional, Moulis, L., additional, Maire, A., additional, Villiet, M., additional, Jalabert, A., additional, De Barry, G., additional, Breuker, C., additional, Roubille, F., additional, Leclercq., F, additional, Pasquié, J.-L., additional, Agullo, A., additional, Battistella, P., additional, and Castet-Nicolas, A., additional
Published: 2023
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37. Clinical and ethical implications of withdrawal treatment at the end of heart failure clinical trials

Author: Martinez, D., primary, Huet, F., additional, Dupasquier, V., additional, Aguilhon, S., additional, Soltani, S., additional, Leclercq, F., additional, Molinari, N., additional, Chapet, N., additional, Delbaere, Q., additional, and Roubille, F., additional
Published: 2023
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38. The Lensed Lyman-Alpha MUSE Arcs Sample (LLAMAS)

Author: Claeyssens, A., primary, Richard, J., additional, Blaizot, J., additional, Garel, T., additional, Kusakabe, H., additional, Bacon, R., additional, Bauer, F. E., additional, Guaita, L., additional, Jeanneau, A., additional, Lagattuta, D., additional, Leclercq, F., additional, Maseda, M., additional, Matthee, J., additional, Nanayakkara, T., additional, Pello, R., additional, Thai, T. T., additional, Tuan-Anh, P., additional, Verhamme, A., additional, Vitte, E., additional, and Wisotzki, L., additional
Published: 2022
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39. MusE GAs FLOw and Wind (MEGAFLOW) VIII. Discovery of a Mgii emission halo probed by a quasar sightline

Author: Zabl, J, Bouche, N, Wisotzki, L, Schaye, J, Leclercq, F, Garel, T, Wendt, M, Schroetter, I, Muzahid, S, Cantalupo, S, Contini, T, Bacon, R, Brinchmann, J, Richard, J, Zabl J., Bouche N. F., Wisotzki L., Schaye J., Leclercq F., Garel T., Wendt M., Schroetter I., Muzahid S., Cantalupo S., Contini T., Bacon R., Brinchmann J., Richard J., Zabl, J, Bouche, N, Wisotzki, L, Schaye, J, Leclercq, F, Garel, T, Wendt, M, Schroetter, I, Muzahid, S, Cantalupo, S, Contini, T, Bacon, R, Brinchmann, J, Richard, J, Zabl J., Bouche N. F., Wisotzki L., Schaye J., Leclercq F., Garel T., Wendt M., Schroetter I., Muzahid S., Cantalupo S., Contini T., Bacon R., Brinchmann J., and Richard J.
Abstract: Using deep ($11.2, m{h}$) VLT/MUSE data from the MEGAFLOW survey, we report the first detection of extended $ m{Mg, small {II}}$ emission from a galaxy's halo that is probed by a quasar sightline. The $ m{Mg, small {II}}, lambda lambda , 2796, 2803$ emission around the z = 0.702 galaxy ($log (M_∗/ m{M_odot })=10.05_{-0.11}^{+0.15}{}$) is detected out to $approx 25, hbox{kpc}$ from the central galaxy and covers $1.0 imes 10^3, hbox{kpc}^2$ above a surface brightness of $14 imes 10^{-19}, m{erg}, m{s}^{-1}, m{cm}^{-2}, m{arcsec}^{-2}{}$ ($2, sigma$; integrated over $1200, m{km, s}^{-1}= 19mathring{ m A}$ and averaged over $1.5, m{arcsec}^{2}$). The $ m{Mg, small {II}}$ emission around this highly inclined galaxy (i ? 75 deg) is strongest along the galaxy's projected minor axis, consistent with the $ m{Mg, small {II}}$ gas having been ejected from the galaxy into a bi-conical structure. The quasar sightline, which is aligned with the galaxy's minor axis, shows strong $ m{Mg, small {II}}$ absorption ($hbox{$EW_0^{lambda 2796}$}{}=1.8{}, mathring{ m A}$) at an impact parameter of $39{}, hbox{kpc}$ from the galaxy. Comparing the kinematics of both the emission and the absorption - probed with VLT/UVES - to the expectation from a simple toy model of a bi-conical outflow, we find good consistency when assuming a relatively slow outflow ($v_ m{out}=130{}, m{km, s}^{-1}$). We investigate potential origins of the extended $ m{Mg, small {II}}$ emission using simple toy models. With continuum scattering models we encounter serious difficulties in explaining the luminosity of the $ m{Mg, small {II}}$ halo and in reconciling density estimates from emission and absorption. Instead, we find that shocks might be a more viable source to power the extended $ m{Mg, small {II}}$ (and non-resonant $[ m{O, small {II}}]$) emission.
Published: 2021

40. Incidence des pathologies médico-chirurgicales observées à bord des sous-marins nucléaires lanceurs d’engins français de nouvelle génération entre mai 1997 et décembre 2013

Author: REPELLIN, M., primary, CASTELNÉRAC, A., additional, LECLERCQ, F., additional, LAFFERRERIE, C., additional, TRÉVIDIC, F., additional, and CUVILLIER, J.-M., additional
Published: 2017
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41. Critical Slowing Down in a Simple Fluid System as Measured by Neutron Spin Echo Technique. Crossover Between Hydrodynamics and Critical Dynamics

Author: Leclercq, F., Pouget, S., Damay, P., Beig, R., editor, Englert, B. -G., editor, Frisch, U., editor, Hänggi, P., editor, Hepp, K., editor, Hillebrandt, W., editor, Imboden, D., editor, Jaffe, R. L., editor, Lipowsky, R., editor, v. Löhneysen, H., editor, Ojima, I., editor, Sornette, D., editor, Theisen, S., editor, Weise, W., editor, Wess, J., editor, Zittartz, J., editor, Mezei, Ferenc, editor, Pappas, Catherine, editor, and Gutberlet, Thomas, editor
Published: 2003
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42. The MUSE eXtremely deep field: first panoramic view of an Mg ̄ II emitting intragroup medium

Author: Leclercq, F, Verhamme, A, Epinat, B, Simmonds, C, Matthee, J, Bouch??, N, Garel, T, Urrutia, T, Wisotzki, L, Zabl, J, Bacon, R, Abril-Melgarejo, V, Boogaard, L, Brinchmann, J, Cantalupo, S, Contini, T, Kerutt, J, Kusakabe, H, Maseda, M, Michel-Dansac, L, Muzahid, S, Nanayakkara, T, Richard, J, Schaye, J, Floriane Leclercq, Anne Verhamme, Benoit Epinat, Charlotte Simmonds, Jorryt Matthee, Nicolas F. Bouch??, Thibault Garel, Tanya Urrutia, Lutz Wisotzki, Johannes Zabl, Roland Bacon, Valentina Abril-Melgarejo, Leindert Boogaard, Jarle Brinchmann, Sebastiano Cantalupo, Thierry Contini, Josephine Kerutt, Haruka Kusakabe, Michael Maseda, L??o Michel-Dansac, Sowgat Muzahid, Themiya Nanayakkara, Johan Richard, Joop Schaye, Leclercq, F, Verhamme, A, Epinat, B, Simmonds, C, Matthee, J, Bouch??, N, Garel, T, Urrutia, T, Wisotzki, L, Zabl, J, Bacon, R, Abril-Melgarejo, V, Boogaard, L, Brinchmann, J, Cantalupo, S, Contini, T, Kerutt, J, Kusakabe, H, Maseda, M, Michel-Dansac, L, Muzahid, S, Nanayakkara, T, Richard, J, Schaye, J, Floriane Leclercq, Anne Verhamme, Benoit Epinat, Charlotte Simmonds, Jorryt Matthee, Nicolas F. Bouch??, Thibault Garel, Tanya Urrutia, Lutz Wisotzki, Johannes Zabl, Roland Bacon, Valentina Abril-Melgarejo, Leindert Boogaard, Jarle Brinchmann, Sebastiano Cantalupo, Thierry Contini, Josephine Kerutt, Haruka Kusakabe, Michael Maseda, L??o Michel-Dansac, Sowgat Muzahid, Themiya Nanayakkara, Johan Richard, and Joop Schaye
Abstract: Using the exquisite data from the MUSE eXtremely Deep Field (MXDF), we report the discovery of an Mg ̄II emission nebula with an area above a 2I significance level of 1000 proper kpc2. This provides the first panoramic view of the spatial distribution of magnesium in the intragroup medium of a low-mass group of five star-forming galaxies at za" =a" 1.31. The galaxy group members are separated by less than 50 physical kpc in projection and ~120 km sa1 in velocity space. The most massive galaxy has a stellar mass of 109.35a Ma and shows an Mg ̄II P-Cygni line profile, indicating the presence of an outflow, which is consistent with the spatially resolved spectral analysis showing ~+120 km sa1 shift of the Mg ̄II emission lines with respect to the systemic redshift. The other galaxies are less massive and only show Mg ̄II in emission. The detected Mg ̄II nebula has a maximal projected extent of ~70 kpc, including a low-surface-brightness (~2 A- 10a19 erg sa1 cma2 arcseca2) gaseous bridge between two subgroups of galaxies. The presence of absorption features in the spectrum of a background galaxy located at an impact parameter of 19 kpc from the closest galaxy of the group indicates the presence of gas enriched in magnesium even beyond the detected nebula seen in emission, which suggests that we are observing the tip of a larger intragroup medium. The observed Mg ̄II velocity gradient suggests an overall rotation of the structure along the major axis of the most massive galaxy. Our MUSE data also reveal extended Fe ̄II∗ emission in the vicinity of the most massive galaxy, aligned with its minor axis and pointing towards a neighboring galaxy. Extended [O ̄II] emission is found around the galaxy group members and at the location of the Mg ̄II bridge. Our results suggest that both tidal stripping effects from galaxy interactions and outflows are enriching the intragroup medium of this system.
Published: 2022

43. Heart rate as a determinant of L-type Ca2+ channel activity: Mechanisms and implication in force-frequency relation

Author: Lemaire, S., Piot, C., Leclercq, F., Leuranguer, V., Nargeot, J., Richard, S., Hasenfuss, G., editor, and Just, H., editor
Published: 2000
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44. Equivalent widths of Lyman α emitters in MUSE-Wide and MUSE-Deep

Author: Kerutt, J., primary, Wisotzki, L., additional, Verhamme, A., additional, Schmidt, K. B., additional, Leclercq, F., additional, Herenz, E. C., additional, Urrutia, T., additional, Garel, T., additional, Hashimoto, T., additional, Maseda, M., additional, Matthee, J., additional, Kusakabe, H., additional, Schaye, J., additional, Richard, J., additional, Guiderdoni, B., additional, Mauerhofer, V., additional, Nanayakkara, T., additional, and Vitte, E., additional
Published: 2022
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45. Deciphering stellar metallicities in the early Universe

Author: Matthee, J., Feltre, A., Maseda, M.V., Nanayakkara, T., Boogaard, L.A., Bacon, R., Verhamme, A., Leclercq, F., Kusakabe, H., Urrutia, T., Wisotzki, L., Centre de Recherche Astrophysique de Lyon (CRAL), École normale supérieure de Lyon (ENS de Lyon)-Université Claude Bernard Lyon 1 (UCBL), and Université de Lyon-Université de Lyon-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)
Subjects: [SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph], Astrophysics::High Energy Astrophysical Phenomena, Galaxies: Formation, FOS: Physical sciences, Astronomy and Astrophysics, Techniques: Spectroscopic, Astrophysics::Cosmology and Extragalactic Astrophysics, Galaxies: High-Redshift, Astrophysics - Astrophysics of Galaxies, [SDU]Sciences of the Universe [physics], Space and Planetary Science, Astrophysics of Galaxies (astro-ph.GA), Astrophysics::Solar and Stellar Astrophysics, Galaxies: Stellar Content, Astrophysics::Earth and Planetary Astrophysics, Astrophysics::Galaxy Astrophysics
Abstract: Directly characterising the first generations of stars in distant galaxies is a key quest of observational cosmology. We present a case study of ID53 at z=4.77, the UV-brightest (but L*) star-forming galaxy at z>3 in the MUSE eXtremely Deep Field with a mass of $10^9$ M$_{\odot}$. In addition to very strong Lyman-$\alpha$ (Ly$\alpha$) emission, we clearly detect the (stellar) continuum and an NV P-Cygni feature, interstellar absorption, fine-structure emission and nebular CIV emission lines in the 140 hr spectrum. Continuum emission from two spatially resolved components in Hubble Space Telescope data are blended in the MUSE data, but we show that the nebular CIV emission originates from a subcomponent of the galaxy. The UV spectrum can be fit with recent BPASS stellar population models combined with single-burst or continuous star formation histories (SFHs), a standard initial mass function, and an attenuation law. Models with a young age and low metallicity (log10(age/yr)=6.5-7.6 and [Z/H]=-2.15 to -1.15) are preferred. The intrinsic H$\alpha$ luminosity of the best-fit models is an order of magnitude higher than the H$\alpha$ luminosity inferred from Spitzer/IRAC data, which either suggests a high escape fraction of ionising photons, a high relative attenuation of nebular to stellar dust, or a complex SFH. The metallicity appears lower than the metallicity in more massive galaxies at z=3-5, consistent with the scenario according to which younger galaxies have lower metallicities. This chemical immaturity likely facilitates Ly$\alpha$ escape, explaining why the Ly$\alpha$ equivalent width is anti-correlated with stellar metallicity. Finally, we stress that uncertainties in SFHs impose a challenge for future inferences of the stellar metallicity of young galaxies. This highlights the need for joint (spatially resolved) analyses of stellar spectra and photo-ionisation models., Comment: Main results: Figures 3 and 5 show that the observed nebular CIV emission varies spatially within the galaxy and Figure 8 shows the rest-frame UV spectrum is best-fit with very young stellar populations. Accepted for publication in A&A
Published: 2022

46. Les patients bénéficiant d’une coronarographie sont-ils bien informés ? Évaluation de l’efficacité de l’information écrite. Étude prospective unicentrique

Author: Vergès, M., Leclercq, F., Davy, J.-M., Piot, C., Gervasoni, R., Pasquie, J.-L., Cornillet, L., Sportouch-Dukhan, C., Raczka, F., Cung, T.-T., Macia, J.-C., and Roubille, F.
Published: 2011
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47. Effects of alirocumab on cardiovascular and metabolic outcomes after acute coronary syndrome in patients with or without diabetes: a prespecified analysis of the ODYSSEY OUTCOMES randomised controlled trial

Author: Ray, K, Colhoun, H, Szarek, M, Baccara-Dinet, M, Bhatt, D, Bittner, V, Budaj, A, Diaz, R, Goodman, S, Hanotin, C, Harrington, R, Jukema, J, Loizeau, V, Lopes, R, Moryusef, A, Murin, J, Pordy, R, Ristic, A, Roe, M, Tunon, J, White, H, Zeiher, A, Schwartz, G, Steg, P, Tricoci, P, Mahaffey, K, Edelberg, J, Lecorps, G, Sasiela, W, Tamby, J, Aylward, P, Drexel, H, Sinnaeve, P, Dilic, M, Gotcheva, N, Prieto, J, Yong, H, Lopez-Jaramillo, P, Pecin, I, Reiner, Z, Ostadal, P, Viigimaa, M, Nieminen, M, Chumburidze, V, Marx, N, Danchin, N, Liberopoulos, E, Montenegro Valdovinos, P, Tse, H, Kiss, R, Xavier, D, Zahger, D, Valgimigli, M, Kimura, T, Kim, H, Kim, S, Erglis, A, Laucevicius, A, Kedev, S, Yusoff, K, Ramos Lopez, G, Alings, M, Halvorsen, S, Correa Flores, R, Morais, J, Dorobantu, M, Karpov, Y, Chua, T, Fras, Z, Dalby, A, de Silva, H, Hagstrom, E, Landmesser, U, Chiang, C, Sritara, P, Guneri, S, Parkhomenko, A, Moriarty, P, Vogel, R, Chaitman, B, Kelsey, S, Olsson, A, Rouleau, J, Simoons, M, Alexander, K, Meloni, C, Rosenson, R, Sijbrands, E, Alexander, J, Armaganijan, L, Bagai, A, Bahit, M, Brennan, J, Clifton, S, Devore, A, Deloatch, S, Dickey, S, Dombrowski, K, Ducrocq, G, Eapen, Z, Endsley, P, Eppinger, A, Harrison, R, Hess, C, Hlatky, M, Jordan, J, Knowles, J, Kolls, B, Kong, D, Leonardi, S, Lillis, L, Maron, D, Marcus, J, Mathews, R, Mehta, R, Mentz, R, Moreira, H, Patel, C, Bernardez-Pereira, S, Perkins, L, Povsic, T, Puymirat, E, Schuyler Jones, W, Shah, B, Sherwood, M, Stringfellow, K, Sujjavanich, D, Toma, M, Trotter, C, Van Diepen, S, Wilson, M, Yan, A, Schiavi, L, Garrido, M, Alvarisqueta, A, Sassone, S, Bordonava, A, Alves De Lima, A, Schmidberg, J, Duronto, E, Caruso, O, Novaretto, L, Hominal, M, Montana, O, Caccavo, A, Gomez Vilamajo, O, Lorenzatti, A, Cartasegna, L, Paterlini, G, Mackinnon, I, Caime, G, Amuchastegui, M, Salomone, O, Codutti, O, Jure, H, Bono, J, Hrabar, A, Vallejos, J, Ahuad Guerrero, R, Novoa, F, Patocchi, C, Zaidman, C, Giuliano, M, Dran, R, Vico, M, Carnero, G, Guzman, P, Medrano Allende, J, Garcia Brasca, D, Bustamante Labarta, M, Nani, S, Blumberg, E, Colombo, H, Liberman, A, Fuentealba, V, Luciardi, H, Waisman, G, Berli, M, Garcia Duran, R, Cestari, H, Luquez, H, Giordano, J, Saavedra, S, Zapata, G, Costamagna, O, Llois, S, Waites, J, Collins, N, Soward, A, Hii, C, Shaw, J, Arstall, M, Horowitz, J, Ninio, D, Rogers, J, Colquhoun, D, Oqueli Flores, R, Roberts-Thomson, P, Raffel, O, Lehman, S, Aroney, C, Coverdale, S, Garrahy, P, Starmer, G, Sader, M, Carroll, P, Dick, R, Zweiker, R, Hoppe, U, Huber, K, Berger, R, Delle-Karth, G, Frey, B, Weidinger, F, Faes, D, Hermans, K, Pirenne, B, Leone, A, Hoffer, E, Vrolix, M, De Wolf, L, Wollaert, B, Castadot, M, Dujardin, K, Beauloye, C, Vervoort, G, Striekwold, H, Convens, C, Roosen, J, Barbato, E, Claeys, M, Cools, F, Terzic, I, Barakovic, F, Midzic, Z, Pojskic, B, Fazlibegovic, E, Kulic, M, Durak-Nalbantic, A, Vulic, D, Muslibegovic, A, Goronja, B, Reis, 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Y., Tang I-Shing J., Micko K., Nociar J., Pella D., Fulop P., Hranai M., Palka J., Mazur J., Majercak I., Dzupina A., Fazekas F., Gonsorcik J., Bugan V., Selecky J., Kamensky G., Strbova J., Smik R., Dukat A., Zuran I., Poklukar J., Cernic Suligoj N., Cevc M., Cyster H. P., Ranjith N., Corbett C., Bayat J., Makotoko E. M., du Toit Theron H., Kapp I. E., de V Basson M. M., Lottering H., Van Aswegen D., Van Zyl L. J., Sebastian P. J., Pillay T., Saaiman J. A., Commerford P. J., Cassimjee S., Riaz G., Ebrahim I. O., Sarvan M., Mynhardt J. H., Reuter H., Moodley R., Vida M., Cequier Fillat A. R., Bodi Peris V., Fuentes Jimenez F., Marin F., Cruz Fernandez J. M., Hidalgo Urbano R. J., Gil-Extremera B., Toledo P., Worner Diz F., Garcia-Dorado D., Iniguez A., Gonzalez-Juanatey J. R., Fernandez Portales J., Civeira Murillo F., Matas Pericas L., Zamorano J. L., De Mora Martin M., Bruguera Cortada J., Alonso Martin J. J., Serrano Antolin J. M., De Berrazueta Fernandez J. R., Vazquez de Prada J. A., Diaz Fernandez J. F., Garcia Lledo J. A., Cosin Sales J., Botas Rodriguez J., Gusi Tragant G., Benedicto A., Gonzalez-Juanatey C., Camprubi Potau M., Plaza Perez I., De La Tassa C. M., Loma-Osorio Rincon P., Balaguer Recena J., Escudier J. M., Payeras A. C., Alonso Orcajo N., Valdivielso P., Constantine G., Haniffa R., Tissera N., Amarasekera S., Ponnamperuma C., Fernando N., Fernando K., Jayawardena J., Wijeyasingam S., Ranasinghe G., Ekanayaka R., Mendis S., Senaratne V., Mayurathan G., Sirisena T., Rajapaksha A., Herath J. I., Amarasena N., Berglund S., Rasmanis G., Vedin O., Witt N., Mourtzinis G., Nicol P., Hansen O., Romeo S., Agergaard Jensen S., Torstensson I., Ahremark U., Sundelin T., Moccetti T., Muller C., Mach F., Binde R., Tsai W. -C., Ueng K. -C., Lai W. -T., Liu M. -E., Hwang J. -J., Yin W. -H., Hsieh I. -C., Hsieh M. -J., Lin W. H., Kuo J. -Y., Huang T. -Y., Fang C. -Y., Kaewsuwanna P., Soonfuang W., Jintapakorn W., Sukonthasarn A., Wongpraparut N., Sastravaha K., Sansanayudh N., Kehasukcharoen W., Piyayotai D., Chotnoparatpat P., Camsari A., Kultursay H., Mutlu B., Ersanli M., Demirtas M., Kirma C., Ural E., Koldas L., Karpenko O., Prokhorov A., Vakaluyk I., Myshanych H., Reshotko D., Batushkin V., Rudenko L., Kovalskyi I., Kushnir M., Tseluyko V., Mostovoy Y., Stanislavchuk M., Kyiak Y., Karpenko Y., Malynovsky Y., Klantsa A., Kutniy O., Amosova E., Tashchuk V., Leshchuk O., Rishko M., Kopytsya M., Yagensky A., Vatutin M., Bagriy A., Barna O. M., Ushakov O., Dzyak G., Goloborodko B., Rudenko A., Zheleznyy V., Trevelyan J., Zaman A., Lee K., Moriarty A., Aggarwal R. K., Clifford P., Wong Y. -K., Iqbal S. M., Subkovas E., Braganza D., Sarkar D., Storey R., Griffiths H., McClure S., Muthusamy R., Smith S., Kurian J., Levy T., Barr C., Kadr H., Gerber R., Simaitis A., Soran H., Mathur A., Brodison A., Ayaz M., Cheema M., Oliver R., Thackray S., Mudawi T., Rahman G., Sultan A., Sharman D., Sprigings D., Butler R., Wilkinson P., Lip G. Y., Halcox J., Gallagher S., Ossei-Gerning N., Vardi G., Baldari D., Brabham D., Treasure II C., Dahl C., Palmer B., Wiseman A., Puri S., Mohart A. E., Ince C., Flores E., Wright S., Cheng S. -C., Rosenberg M., Rogers W., Kosinski E., Forgosh L., Waltman J., Khan M., Shoukfeh M., Dagher G., Cambier P., Lieber I., Kumar P., East C., Krichmar P., Hasan M., White L., Knickelbine T., Haldis T., Gillespie E., Amidon T., Suh D., Arif I., Abdallah M., Akhter F., Carlson E., D'Urso M., El-Ahdab F., Nelson W., Moriarty K., Harris B., Cohen S., Carter L., Doty D., Sabatino K., Haddad T., Malik A., Rao S., Mulkay A., Jovin I., Klancke K., Malhotra V., Devarapalli S. K., Koren M., Chandna H., Dodds III G., Goraya T., Bengston J., Janik M., Moran J., Sumner A., Kobayashi J., Davis W., Yazdani S., Pasquini J., Thakkar M., Vedere A., Leimbach W., Rider J., Fenton S., Singh N., Shah A. V., Janosik D., Pepine C., Berman B., Gelormini J., Daniels C., Richard K., Keating F., Kondo N. I., Shetty S., Levite H., Waider W., Takata T., Abu-Fadel M., Shah V., Aggarwal R., Izzo M., Kumar A., Hattler B., Do R., Link C., Bortnick A., Kinzfogl III G., Ghitis A., Larry J., Teufel E., Kuhlman P., Mclaurin B., Zhang W., Thew S., Abbas J., White M., Islam O., Subherwal S., Ranadive N., Vakili B., Gring C., Henderson D., Schuchard T., Farhat N., Kline G., Mahal S., Whitaker J., Speirs S., Andersen R., Daboul N., Horwitz P., Zahr F., Ponce G., Jafar Z., Mcgarvey J., Panchal V., Voyce S., Blok T., Sheldon W., Azizad M. M., Schmalfuss C., Picone M., Pederson R., Herzog W., Friedman K., Lindsey J., Nowins R., Timothy E., Leonard P., Lepor N., El Shahawy M., Weintraub H., Irimpen A., Alonso A., May W., Christopher D., Galski T., Chu A., Mody F., Ramin E., Hodes Z., Rossi J., Rose G., Fairlamb J., Lambert C., Raisinghani A., Abbate A., Vetrovec G., King M., Carey C., Gerber J., Younis L., Park H. T., Vidovich M., Knutson T., Friedman D., Chaleff F., Loussararian A., Rozeman P., Kimmelstiel C., Kuvin J., Silver K., Foster M., Tonnessen G., Espinoza A., Amlani M., Wali A., Malozzi C., Jong G. T., Massey C., Wattanakit K., O'Donnell P. J., Singal D., Jaffrani N., Banuru S., Fisher D., Xenakis M., Perlmutter N., Bhagwat R., Strader J., Blonder R., Akyea-Djamson A., Labroo A., Marais H. J., Claxton E., Weiss R., Kathryn R., Berk M., Rossi P., Joshi P., Khera A., Khaira A. S., Kumkumian G., Lupovitch S., Purow J., Welka S., Hoffman D., Fischer S., Soroka E., Eagerton D., Pancholy S., Ray M., Erenrich N., Farrar M., Pollock S., French W. J., Diamantis S., Guy D., Gimple L., Neustel M., Schwartz S., Pereira E., Albert S., Spriggs D., Strain J., Mittal S., Vo A., Chane M., Hall J., Vijay N., Lotun K., Lester F. M., Nahhas A., Pope T., Nager P., Vohra R., Sharma M., Bashir R., Ahmed H., Berlowitz M., Fishberg R., Barrucco R., Yang E., Radin M., Sporn D., Stapleton D., Eisenberg S., Landzberg J., Mcgough M., Turk S., Schwartz M., Sundram P. S., Jain D., Zainea M., Bayron C., Karlsberg R., Dohad S., Lui H., Keen W., Westerhausen D., Khurana S., Agarwal H., Birchem J., Penny W., Chang M., Murphy S., Henry J., Schifferdecker B., Gilbert J. M., Chalavarya G., Eaton C., Schmedtje J. F., Christenson S., Dotani I., Denham D., Macdonell A., Gibson P., Rahman A., Al Joundi T., Assi N., Conrad G., Kotha P., Love M., Giesler G., Rubenstein H., Gamil D., Akright L., Krawczyk J., Cobler J., Wells T., Welker J., Foster R., Gilmore R., Anderson J., Jacoby D., Gardner G., Dandillaya R., Vora K., Kostis J., Hunter J., Laxson D., Ball E., Lopes R., Egydio F., Kawakami A., Oliveira J., Wozniak J., Matthews A., Ratky C., Valiris J., Berdan L., Hepditch A., Quintero K., Rorick T., Westbrook M., Pascual A., Rovito C., Bezault M., Drouet E., Simon T., Alsweiler C., Luyten A., Butters J., Griffith L., Shaw M., Grunberg L., Islam S., Bregeault M. -F., Bougon N., Faustino D., Fontecave S., Murphy J., Verrier M., Agnetti V., Andersen D., Badreddine E., Bekkouche M., Bouancheau C., Brigui I., Brocklehurst M., Cianciarulo J., Devaul D., Domokos S., Gache C., Gobillot C., Guillou S., Healy J., Heath M., Jaiwal G., Javierre C., Labeirie J., Monier M., Morales U., Mrabti A., Mthombeni B., Okan B., Smith L., Sheller J., Sopena S., Pellan V., Benbernou F., Bengrait N., Lamoureux M., Kralova K., Scemama M., Bejuit R., Coulange A., Berthou C., Repincay J., Lorenzato C., Etienne A., Gouet V., Normand M., Ourliac A., Rondel C., Adamo A., Beltran P., Barraud P., Dubois-Gache H., Halle B., Metwally L., Mourgues M., Sotty M., Vincendet M., Cotruta R., Chengyue Z., Fournie-Lloret D., Morrello C., Perthuis A., Picault P., Zobouyan I., Dempsey M. 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F., Christenson S., Dotani I., Denham D., Macdonell A., Gibson P., Rahman A., Al Joundi T., Assi N., Conrad G., Kotha P., Love M., Giesler G., Rubenstein H., Gamil D., Akright L., Krawczyk J., Cobler J., Wells T., Welker J., Foster R., Gilmore R., Anderson J., Jacoby D., Gardner G., Dandillaya R., Vora K., Kostis J., Hunter J., Laxson D., Ball E., Lopes R., Egydio F., Kawakami A., Oliveira J., Wozniak J., Matthews A., Ratky C., Valiris J., Berdan L., Hepditch A., Quintero K., Rorick T., Westbrook M., Pascual A., Rovito C., Bezault M., Drouet E., Simon T., Alsweiler C., Luyten A., Butters J., Griffith L., Shaw M., Grunberg L., Islam S., Bregeault M. -F., Bougon N., Faustino D., Fontecave S., Murphy J., Verrier M., Agnetti V., Andersen D., Badreddine E., Bekkouche M., Bouancheau C., Brigui I., Brocklehurst M., Cianciarulo J., Devaul D., Domokos S., Gache C., Gobillot C., Guillou S., Healy J., Heath M., Jaiwal G., Javierre C., Labeirie J., Monier M., Morales U., Mrabti A., Mthombeni B., Okan B., Smith L., Sheller J., Sopena S., Pellan V., Benbernou F., Bengrait N., Lamoureux M., Kralova K., Scemama M., Bejuit R., Coulange A., Berthou C., Repincay J., Lorenzato C., Etienne A., Gouet V., Normand M., Ourliac A., Rondel C., Adamo A., Beltran P., Barraud P., Dubois-Gache H., Halle B., Metwally L., Mourgues M., Sotty M., Vincendet M., Cotruta R., Chengyue Z., Fournie-Lloret D., Morrello C., Perthuis A., Picault P., Zobouyan I., Dempsey M. A., and McClanahan M. A.
Abstract: Background: After acute coronary syndrome, diabetes conveys an excess risk of ischaemic cardiovascular events. A reduction in mean LDL cholesterol to 1·4–1·8 mmol/L with ezetimibe or statins reduces cardiovascular events in patients with an acute coronary syndrome and diabetes. However, the efficacy and safety of further reduction in LDL cholesterol with an inhibitor of proprotein convertase subtilisin/kexin type 9 (PCSK9) after acute coronary syndrome is unknown. We aimed to explore this issue in a prespecified analysis of the ODYSSEY OUTCOMES trial of the PCSK9 inhibitor alirocumab, assessing its effects on cardiovascular outcomes by baseline glycaemic status, while also assessing its effects on glycaemic measures including risk of new-onset diabetes. Methods: ODYSSEY OUTCOMES was a randomised, double-blind, placebo-controlled trial, done at 1315 sites in 57 countries, that compared alirocumab with placebo in patients who had been admitted to hospital with an acute coronary syndrome (myocardial infarction or unstable angina) 1–12 months before randomisation and who had raised concentrations of atherogenic lipoproteins despite use of high-intensity statins. Patients were randomly assigned (1:1) to receive alirocumab or placebo every 2 weeks; randomisation was stratified by country and was done centrally with an interactive voice-response or web-response system. Alirocumab was titrated to target LDL cholesterol concentrations of 0·65–1·30 mmol/L. In this prespecified analysis, we investigated the effect of alirocumab on cardiovascular events by glycaemic status at baseline (diabetes, prediabetes, or normoglycaemia)—defined on the basis of patient history, review of medical records, or baseline HbA1c or fasting serum glucose—and risk of new-onset diabetes among those without diabetes at baseline. The primary endpoint was a composite of death from coronary heart disease, non-fatal myocardial infarction, fatal or non-fatal ischaemic stroke, or unstable angina requiring
Published: 2019

48. Les effets pro-arythmiques des médicaments

Author: Pasquié, J.-L., Massin, F., Leclercq, F., Cung, T.-T., Davy, J.-M., and Grolleau, R.
Published: 2010
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49. Can troponin elevation predict worse prognosis in patients with acute pericarditis?

Author: Machado, S., Roubille, F., Gahide, G., Vernhet-Kovacsik, H., Cornillet, L., Cung, T.T., Sportouch-Dukhan, C., Raczka, F., Pasquié, J.L., Gervasoni, R., Macia, J.C., Cransac, F., Davy, J.-M., Piot, C., and Leclercq, F.
Published: 2010
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50. Atrial fibrillation screening on holter monitoring after percutaneous patent foramen ovale closure: a prospective study

Author: Leclercq, F, primary, Odorico, X, additional, Arquizan, C, additional, Macia, J C, additional, Lattuca, B, additional, Schmutz, L, additional, Roubille, F, additional, Pages, L, additional, Marin, G, additional, Cayla, G, additional, and Akodad, M, additional
Published: 2021
Full Text: View/download PDF

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