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478 results on '"Cascone, E."'

101. Post-conjunction detection of Œ≤ Pictoris b with VLT/SPHERE

Author: Lagrange, A., Boccaletti, A., Langlois, M., Chauvin, G., Gratton, R., Beust, H., Desidera, S., Milli, J., Bonnefoy, M., Cheetham, A., Feldt, M., Meyer, M., Vigan, A., Biller, B., Bonavita, M., Baudino, J., Cantalloube, F., Cudel, M., Daemgen, S., Delorme, P., D'Orazi, V., Girard, J., Fontanive, C., Hagelberg, J., Janson, M., Keppler, M., Koypitova, T., Galicher, R., Lannier, J., Le Coroller, H., Ligi, R., Maire, A., Mesa, D., Messina, S., Müeller, A., Peretti, S., Perrot, C., Rouan, D., Salter, G., Samland, M., Schmidt, T., Sissa, E., Zurlo, A., Beuzit, J., Mouillet, D., Dominik, C., Henning, T., Lagadec, E., Ménard, F., Schmid, H., Turatto, M., Udry, S., Bohn, A., Charnay, B., Gomez Gonzales, C., Gry, C., Kenworthy, M., Kral, Q., Mordasini, C., Moutou, C., van der Plas, G., Schlieder, J., Abe, L., Antichi, J., Baruffolo, A., Baudoz, P., Baudrand, J., Blanchard, P., Bazzon, A., Buey, T., Carbillet, M., Carle, M., Charton, J., Cascone, E., Claudi, R., Costille, A., Deboulbe, A., De Caprio, V., Dohlen, K., Fantinel, D., Feautrier, P., Fusco, T., Gigan, P., Giro, E., Gisler, D., Gluck, L., Hubin, N., Hugot, E., Jaquet, M., Kasper, M., Madec, F., Magnard, Y., Martinez, P., Maurel, D., Le Mignant, D., Möller-Nilsson, O., Llored, M., Moulin, T., Origné, A., Pavlov, A., Perret, D., Petit, C., Pragt, J., Szulagyi, J., and Wildi, F.
Subjects: Astrophysics::Solar and Stellar Astrophysics, Astrophysics::Earth and Planetary Astrophysics, Astrophysics::Galaxy Astrophysics
Abstract: Context. With an orbital distance comparable to that of Saturn in the solar system, Œ≤ Pictoris b is the closest (semi-major axis ‚âÉ9 au) exoplanet that has been imaged to orbit a star. Thus it offers unique opportunities for detailed studies of its orbital, physical, and atmospheric properties, and of disk-planet interactions. With the exception of the discovery observations in 2003 with NaCo at the Very Large Telescope (VLT), all following astrometric measurements relative to Œ≤ Pictoris have been obtained in the southwestern part of the orbit, which severely limits the determination of the planet's orbital parameters. Aims: We aimed at further constraining Œ≤ Pictoris b orbital properties using more data, and, in particular, data taken in the northeastern part of the orbit. Methods: We used SPHERE at the VLT to precisely monitor the orbital motion of beta Œ≤ Pictoris b since first light of the instrument in 2014. Results: We were able to monitor the planet until November 2016, when its angular separation became too small (125 mas, i.e., 1.6 au) and prevented further detection. We redetected Œ≤ Pictoris b on the northeast side of the disk at a separation of 139 mas and a PA of 30¬∞ in September 2018. The planetary orbit is now well constrained. With a semi-major axis (sma) of a = 9.0 ¬± 0.5 au (1œÉ), it definitely excludes previously reported possible long orbital periods, and excludes Œ≤ Pictoris b as the origin of photometric variations that took place in 1981. We also refine the eccentricity and inclination of the planet. From an instrumental point of view, these data demonstrate that it is possible to detect, if they exist, young massive Jupiters that orbit at less than 2 au from a star that is 20 pc away. Based on observations collected at the European Southern Observatory under programmes 198.C-0209, 1100.C-0481.
Published: 2019

102. A new shaking table apparatus for large scale physical modelling of geotechnical systems

Author: Cascone, E., Aliberti, D., Bandini, V., Biondi, G., Casablanca, O., Di Filippo, G., Ingegneri, S., and Genovese, F.
Subjects: Shaking table, Laminar box, Physical modelling, Shaking table, Laminar box, Physical modelling
Published: 2019

103. SPHERE dynamical and spectroscopic characterization of HD142527B

Author: Claudi, R., Maire, A. -L., Mesa, D., Cheetham, A., Fontanive, C., Gratton, R., Zurlo, A., Avenhaus, H., Bhowmik, T., Biller, B., Boccaletti, A., Bonavita, M., Bonnefoy, M., Cascone, E., Chauvin, G., Delboulbe, A., Desidera, S., D'Orazi, V., Feautrier, P., Feldt, M., Dotti, F. Flammini, Girard, J. H., Giro, E., Janson, Markus, Hagelberg, J., Keppler, M., Kopytova, T., Lacour, S., Lagrange, A. -M., Langlois, M., Lannier, J., Le Coroller, H., Menard, F., Messina, S., Meyer, M., Millward, M., Olofsson, J., Pavlov, A., Peretti, S., Perrot, C., Pinte, C., Pragt, J., Ramos, J., Rochat, S., Rodet, L., Roelfsema, R., Rouan, D., Salter, G., Schmidt, T., Sissa, E., Thebault, P., Udry, S., Vigan, A., Claudi, R., Maire, A. -L., Mesa, D., Cheetham, A., Fontanive, C., Gratton, R., Zurlo, A., Avenhaus, H., Bhowmik, T., Biller, B., Boccaletti, A., Bonavita, M., Bonnefoy, M., Cascone, E., Chauvin, G., Delboulbe, A., Desidera, S., D'Orazi, V., Feautrier, P., Feldt, M., Dotti, F. Flammini, Girard, J. H., Giro, E., Janson, Markus, Hagelberg, J., Keppler, M., Kopytova, T., Lacour, S., Lagrange, A. -M., Langlois, M., Lannier, J., Le Coroller, H., Menard, F., Messina, S., Meyer, M., Millward, M., Olofsson, J., Pavlov, A., Peretti, S., Perrot, C., Pinte, C., Pragt, J., Ramos, J., Rochat, S., Rodet, L., Roelfsema, R., Rouan, D., Salter, G., Schmidt, T., Sissa, E., Thebault, P., Udry, S., and Vigan, A.
Abstract: Aims. HD142527 is one of the most frequently studied Herbig Ae/Be stars with a transitional disk that hosts a large cavity that is up to about 100 au in radius. For this reason, it has been included in the guaranteed time observation (GTO) SpHere INfrared survey for Exoplanets (SHINE) as part of the Spectro-Polarimetric High-contrast Exoplanet REsearch (SPHERE) at the Very Large Telescope (VLT) in order to search for low-mass companions that might explain the presence of the gap. SHINE is a large survey within about 600 young nearby stars are observed with SPHERE with the aim to constrain the occurrence and orbital properties of the giant planet population at large (>5 au) orbital separation around young stars. Methods. We used the IRDIFS observing mode of SPHERE (IRDIS short for infrared dual imaging and spectrograph plus IFS or integral field spectrograph) without any coronagraph in order to search for and characterize companions as close as 30 mas of the star. Furthermore, we present the first observations that ever used the sparse aperture mask (SAM) for SPHERE both in IRDIFS and IRDIFS_EXT modes. All the data were reduced using the dedicated SPHERE pipeline and dedicated algorithms that make use of the principal component analysis (PCA) and reference differential imaging (RDI) techniques. Results. We detect the accreting low-mass companion HD142527B at a separation of 73 mas (11.4 au) from the star. No other companions with mass greater than 10 M-J are visible in the field of view of IFS (similar to 100 au centered on the star) or in the IRDIS field of view (similar to 400 au centered on the star). Measurements from IFS, SAM IFS, and IRDIS suggest an M6 spectral type for HD142527B, with an uncertainty of one spectral subtype, compatible with an object of M = 0.11 +/- 0.06 M-circle dot and R = 0.15 +/- 0.07 R-circle dot. The determination of the mass remains a challenge using contemporary evolutionary models, as they do not account for the energy input due to
Published: 2019
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104. Post-conjunction detection of beta Pictoris b with VLT/SPHERE

Author: Lagrange, A. -M., Boccaletti, A., Langlois, M., Chauvin, G., Gratton, R., Beust, H., Desidera, S., Milli, J., Bonnefoy, M., Cheetham, A., Feldt, M., Meyer, M., Vigan, A., Biller, B., Bonavita, M., Baudino, J. -L., Cantalloube, F., Cudel, M., Daemgen, S., Delorme, P., D'Orazi, V., Girard, J., Fontanive, C., Hagelberg, J., Janson, Markus, Keppler, M., Koypitova, T., Galicher, R., Lannier, J., Le Coroller, H., Ligi, R., Maire, A. -L., Mesa, D., Messina, S., Müeller, A., Peretti, S., Perrot, C., Rouan, D., Salter, G., Samland, M., Schmidt, T., Sissa, E., Zurlo, A., Beuzit, J. -L., Mouillet, D., Dominik, C., Henning, T., Lagadec, E., Ménard, F., Schmid, H. -M., Turatto, M., Udry, S., Bohn, A. J., Charnay, B., Gonzales, C. A. Gomez, Gry, C., Kenworthy, M., Kral, Q., Mordasini, C., Moutou, C., van der Plas, G., Schlieder, J. E., Abe, L., Antichi, J., Baruffolo, A., Baudoz, P., Baudrand, J., Blanchard, P., Bazzon, A., Buey, T., Carbillet, M., Carle, M., Charton, J., Cascone, E., Claudi, R., Costille, A., Deboulbe, A., De Caprio, V., Dohlen, K., Fantinel, D., Feautrier, P., Fusco, T., Gigan, P., Giro, E., Gisler, D., Gluck, L., Hubin, N., Hugot, E., Jaquet, M., Kasper, M., Madec, F., Magnard, Y., Martinez, P., Maurel, D., Le Mignant, D., Möller-Nilsson, O., Llored, M., Moulin, T., Origné, A., Pavlov, A., Perret, D., Petit, C., Pragt, J., Szulagyi, J., Wildi, F., Lagrange, A. -M., Boccaletti, A., Langlois, M., Chauvin, G., Gratton, R., Beust, H., Desidera, S., Milli, J., Bonnefoy, M., Cheetham, A., Feldt, M., Meyer, M., Vigan, A., Biller, B., Bonavita, M., Baudino, J. -L., Cantalloube, F., Cudel, M., Daemgen, S., Delorme, P., D'Orazi, V., Girard, J., Fontanive, C., Hagelberg, J., Janson, Markus, Keppler, M., Koypitova, T., Galicher, R., Lannier, J., Le Coroller, H., Ligi, R., Maire, A. -L., Mesa, D., Messina, S., Müeller, A., Peretti, S., Perrot, C., Rouan, D., Salter, G., Samland, M., Schmidt, T., Sissa, E., Zurlo, A., Beuzit, J. -L., Mouillet, D., Dominik, C., Henning, T., Lagadec, E., Ménard, F., Schmid, H. -M., Turatto, M., Udry, S., Bohn, A. J., Charnay, B., Gonzales, C. A. Gomez, Gry, C., Kenworthy, M., Kral, Q., Mordasini, C., Moutou, C., van der Plas, G., Schlieder, J. E., Abe, L., Antichi, J., Baruffolo, A., Baudoz, P., Baudrand, J., Blanchard, P., Bazzon, A., Buey, T., Carbillet, M., Carle, M., Charton, J., Cascone, E., Claudi, R., Costille, A., Deboulbe, A., De Caprio, V., Dohlen, K., Fantinel, D., Feautrier, P., Fusco, T., Gigan, P., Giro, E., Gisler, D., Gluck, L., Hubin, N., Hugot, E., Jaquet, M., Kasper, M., Madec, F., Magnard, Y., Martinez, P., Maurel, D., Le Mignant, D., Möller-Nilsson, O., Llored, M., Moulin, T., Origné, A., Pavlov, A., Perret, D., Petit, C., Pragt, J., Szulagyi, J., and Wildi, F.
Abstract: Context. With an orbital distance comparable to that of Saturn in the solar system, beta Pictoris b is the closest (semi-major axis similar or equal to 9 au) exoplanet that has been imaged to orbit a star. Thus it offers unique opportunities for detailed studies of its orbital, physical, and atmospheric properties, and of disk-planet interactions. With the exception of the discovery observations in 2003 with NaCo at the Very Large Telescope (VLT), all following astrometric measurements relative to beta Pictoris have been obtained in the southwestern part of the orbit, which severely limits the determination of the planet's orbital parameters. Aims. We aimed at further constraining beta Pictoris b orbital properties using more data, and, in particular, data taken in the northeastern part of the orbit. Methods. We used SPHERE at the VLT to precisely monitor the orbital motion of beta beta Pictoris b since first light of the instrument in 2014. Results. We were able to monitor the planet until November 2016, when its angular separation became too small (125 mas, i.e., 1.6 au) and prevented further detection. We redetected beta Pictoris b on the northeast side of the disk at a separation of 139 mas and a PA of 30 degrees in September 2018. The planetary orbit is now well constrained. With a semi-major axis (sma) of a = 9.0 +/- 0.5 au (1 sigma), it definitely excludes previously reported possible long orbital periods, and excludes beta Pictoris b as the origin of photometric variations that took place in 1981. We also refine the eccentricity and inclination of the planet. From an instrumental point of view, these data demonstrate that it is possible to detect, if they exist, young massive Jupiters that orbit at less than 2 au from a star that is 20 pc away.
Published: 2019
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105. Introduction to CTA Science

Author: Acharya, B. S., Agudo, I., Al Samarai, I., Alfaro, R., Alfaro, J., Alispach, C., Batista, R. Alves, Amans, J. -P, Amato, E., Ambrosi, G., Antolini, E., Antonelli, L. A., Aramo, C., Araya, M., Armstrong, T., Arqueros, F., Arrabito, L., Asano, K., Ashley, M., Backes, M., Balazs, C., Balbo, M., Ballester, O., Ballet, J., Bamba, A., Barkov, M., Barres de Almeida, U., Barrio, J. A., Bastieri, D., Becherini, Yvonne, Belfiore, A., Benbow, W., Berge, D., Bernardini, E., Bernardini, M. G., Bernardos, M., Bernloehr, K., Bertucci, B., Biasuzzi, B., Bigongiari, C., Biland, A., Bissaldi, E., Biteau, J., Blanch, O., Blazek, J., Boisson, C., Bolmont, J., Bonanno, G., Bonardi, A., Bonavolonta, C., Bonnoli, G., Bosnjak, Z., Bottcher, M., Braiding, C., Bregeon, J., Brill, A., Brown, A. M., Brun, P., Brunetti, G., Buanes, T., Buckley, J., Bugaev, V., Buehler, R., Bulgarelli, A., Bulik, T., Burton, M., Burtovoi, A., Busetto, G., Canestrari, R., Capalbi, M., Capitanio, F., Caproni, A., Caraveo, P., Cardenas, V., Carlile, C., Carosi, R., Carquin, E., Carr, J., Casanova, S., Cascone, E., Catalani, F., Catalano, O., Cauz, D., Cerruti, M., Chadwick, P., Chaty, S., Chaves, R. C. G., Chen, A., Chen, X., Chernyakova, M., Chikawa, M., Christov, A., Chudoba, J., Cieslar, M., Coco, V., Colafrancesco, S., Colin, P., Conforti, V., Connaughton, V., Conrad, J., Contreras, J. L., Cortina, J., Costa, A., Costantini, H., Cotter, G., Covino, S., Crocker, R., Cuadra, J., Cuevas, O., Cumani, P., D'Ai, A., D'Ammando, F., D'Avanzo, P., D'Urso, D., Daniel, M., Davids, I., Dawson, B., Dazzi, F., De Angelis, A., de Cassia dos Anjos, R., De Cesare, G., De Franco, A., De Gouveia Dal Pino, E. M., de la Calle, I., Lopez, R. de los Reyes, De Lotto, B., De Luca, A., De Lucia, M., de Naurois, M., de Ona Wilhelmi, E., De Palma, F., De Persio, F., de Souza, V., Deil, C., Del Santo, M., Delgado, C., della Volpe, D., Di Girolamo, T., Di Pierro, F., Di Venere, L., Diaz, C., Dib, C., Diebold, S., Djannati-Atai, A., Dominguez, A., Prester, D. Dominis, Dorner, D., Doro, M., Drass, H., Dravins, D., Dubus, G., Dwarkadas, V. V., Ebr, J., Eckner, C., Egberts, K., Einecke, S., Ekoume, T. R. N., Elsaesser, D., Ernenwein, J. -P, Espinoza, C., Evoli, C., Fairbairn, M., Falceta-Goncalves, D., Falcone, A., Farnier, C., Fasola, G., Fedorova, E., Fegan, S., Fernandez-Alonso, M., Fernandez-Barral, A., Ferrand, G., Fesquet, M., Filipovic, M., Fioretti, V., Fontaine, G., Fornasa, M., Fortson, L., Freixas Coromina, L., Fruck, C., Fujita, Y., Fukazawa, Y., Funk, S., Fuessling, M., Gabici, S., Gadola, A., Gallant, Y., Garcia, B., Garcia Lopez, R., Garczarczyk, M., Gaskins, J., Gasparetto, T., Gaug, M., Gerard, L., Giavitto, G., Giglietto, N., Giommi, P., Giordano, F., Giro, E., Giroletti, M., Giuliani, A., Glicenstein, J. -F, Gnatyk, R., Godinovic, N., Goldoni, P., Gomez-Vargas, G., Gonzalez, M. M., Gonzalez, J. M., Gotz, D., Graham, J., Grandi, P., Granot, J., Green, A. J., Greenshaw, T., Griffiths, S., Gunji, S., Hadasch, D., Hara, S., Hardcastle, M. J., Hassan, T., Hayashi, K., Hayashida, M., Heller, M., Helo, J. C., Hermann, G., Hinton, J., Hnatyk, B., Hofmann, W., Holder, J., Horan, D., Horandel, J., Horns, D., Horvath, P., Hovatta, T., Hrabovsky, M., Hrupec, D., Humensky, T. B., Huetten, M., Iarlori, M., Inada, T., Inome, Y., Inoue, S., Inoue, T., Inoue, Y., Iocco, F., Ioka, K., Iori, M., Ishio, K., Iwamura, Y., Jamrozy, M., Janecek, P., Jankowsky, D., Jean, P., Jung-Richardt, I., Jurysek, J., Kaaret, P., Karkar, S., Katagiri, H., Katz, U., Kawanaka, N., Kazanas, D., Khelifi, B., Kieda, D. B., Kimeswenger, S., Kimura, S., Kisaka, S., Knapp, J., Knodlseder, J., Koch, B., Kohri, K., Komin, N., Kosack, K., Kraus, M., Krause, M., Krauss, F., Kubo, H., Mezek, G. Kukec, Kuroda, H., Kushida, J., La Palombara, N., Lamanna, G., Lang, R. G., Lapington, J., Le Blanc, O., Leach, S., Lees, J. -P, Lefaucheur, J., Leigui de Oliveira, M. A., Lenain, J. -P, Lico, R., Limon, M., Lindfors, E., Lohse, T., Lombardi, S., Longo, F., Lopez, M., Lopez-Coto, R., Lu, C. -C, Lucarelli, F., Luque-Escamilla, P. L., Lyard, E., Maccarone, M. C., Maier, G., Majumdar, P., Malaguti, G., Mandat, D., Maneva, G., Manganaro, M., Mangano, S., Marcowith, A., Marin, J., Markoff, S., Marti, J., Martin, P., Martinez, M., Martinez, G., Masetti, N., Masuda, S., Maurin, G., Maxted, N., Mazin, D., Medina, C., Melandri, A., Mereghetti, S., Meyer, M., Minaya, I. A., Mirabal, N., Mirzoyan, R., Mitchell, A., Mizuno, T., Moderski, R., Mohammed, M., Mohrmann, L., Montaruli, T., Moralejo, A., Morcuende-Parrilla, D., Mori, K., Morlino, G., Morris, P., Morselli, A., Moulin, E., Mukherjee, R., Mundell, C., Murach, T., Muraishi, H., Murase, K., Nagai, A., Nagataki, S., Nagayoshi, T., Naito, T., Nakamori, T., Nakamura, Y., Niemiec, J., Nieto, D., Nikolajuk, M., Nishijima, K., Noda, K., Nosek, D., Novosyadlyj, B., Nozaki, S., O'Brien, P., Oakes, L., Ohira, Y., Ohishi, M., Ohm, S., Okazaki, N., Okumura, A., Ong, R. A., Orienti, M., Orito, R., Osborne, J. P., Ostrowski, M., Otte, N., Oya, I., Padovani, M., Paizis, A., Palatiello, M., Palatka, M., Paoletti, R., Paredes, J. M., Pareschi, G., Parsons, R. D., Pe'er, A., Pech, M., Pedaletti, G., Perri, M., Persic, M., Petrashyk, A., Petrucci, P., Petruk, O., Peyaud, B., Pfeifer, M., Piano, G., Pisarski, A., Pita, S., Pohl, M., Polo, M., Pozo, D., Prandini, E., Prast, J., Principe, G., Prokhorov, Dmitry, Prokoph, H., Prouza, M., Puehlhofer, G., Punch, Michael, Puerckhauer, S., Queiroz, F., Quirrenbach, A., Raino, S., Razzaque, S., Reimer, O., Reimer, A., Reisenegger, A., Renaud, M., Rezaeian, A. H., Rhode, W., Ribeiro, D., Ribo, M., Richtler, T., Rico, J., Rieger, F., Riquelme, M., Rivoire, S., Rizi, V., Rodriguez, J., Fernandez, G. Rodriguez, Rodriguez Vazquez, J. J., Rojas, G., Romano, P., Romeo, G., Rosado, J., Rovero, A. C., Rowell, G., Rudak, B., Rugliancich, A., Rulten, C., Sadeh, I., Safi-Harb, S., Saito, T., Sakaki, N., Sakurai, S., Salina, G., Sanchez-Conde, M., Sandaker, H., Sandoval, A., Sangiorgi, P., Sanguillon, M., Sano, H., Santander, M., Sarkar, S., Satalecka, K., Saturni, F. G., Schioppa, E. J., Schlenstedt, S., Schneider, M., Schoorlemmer, H., Schovanek, P., Schulz, A., Schussler, F., Schwanke, U., Sciacca, E., Scuderi, S., Seitenzahl, I., Semikoz, D., Sergijenko, O., Servillat, M., Shalchi, A., Shellard, R. C., Sidoli, L., Siejkowski, H., Sillanpaa, A., Sironi, G., Sitarek, J., Sliusar, V., Slowikowska, A., Sol, H., Stamerra, A., Stanic, S., Starling, R., Stawarz, L., Stefanik, S., Stephan, M., Stolarczyk, T., Stratta, G., Straumann, U., Suomijarvi, T., Supanitsky, A. D., Tagliaferri, G., Tajima, H., Tavani, M., Tavecchio, F., Tavernet, J. -P, Tayabaly, K., Tejedor, L. A., Temnikov, P., Terada, Y., Terrier, R., Terzic, T., Teshima, M., Testa, V., Thoudam, Satyendra, Tian, W., Tibaldo, L., Tluczykont, M., Todero Peixoto, C. J., Tokanai, F., Tomastik, J., Tonev, D., Tornikoski, M., Torres, D. F., Torresi, E., Tosti, G., Tothill, N., Tovmassian, G., Travnicek, P., Trichard, C., Trifoglio, M., Pujadas, I. Troyano, Tsujimoto, S., Umana, G., Vagelli, V., Vagnetti, F., Valentino, M., Vallania, P., Valore, L., van Eldik, C., Vandenbroucke, J., Varner, G. S., Vasileiadis, G., Vassiliev, V., Vazquez Acosta, M., Vecchi, M., Vega, A., Vercellone, S., Veres, P., Vergani, S., Verzi, V., Vettolani, G. P., Viana, A., Vigorito, C., Villanueva, J., Voelk, H., Vollhardt, A., Vorobiov, S., Vrastil, M., Vuillaume, T., Wagner, S. J., Wagner, R., Walter, R., Ward, J. E., Warren, D., Watson, J. J., Werner, F., White, M., White, R., Wierzcholska, A., Wilcox, P., Will, M., Williams, D. A., Wischnewski, R., Wood, M., Yamamoto, T., Yamazaki, R., Yanagita, S., Yang, L., Yoshida, T., Yoshiike, S., Yoshikoshi, T., Zacharias, M., Zaharijas, G., Zampieri, L., Zandanel, F., Zanin, R., Zavrtanik, M., Zavrtanik, D., Zdziarski, A. A., Zech, A., Zechlin, H., Zhdanov, V. I., Ziegler, A., Zorn, J., Acharya, B. S., Agudo, I., Al Samarai, I., Alfaro, R., Alfaro, J., Alispach, C., Batista, R. Alves, Amans, J. -P, Amato, E., Ambrosi, G., Antolini, E., Antonelli, L. A., Aramo, C., Araya, M., Armstrong, T., Arqueros, F., Arrabito, L., Asano, K., Ashley, M., Backes, M., Balazs, C., Balbo, M., Ballester, O., Ballet, J., Bamba, A., Barkov, M., Barres de Almeida, U., Barrio, J. A., Bastieri, D., Becherini, Yvonne, Belfiore, A., Benbow, W., Berge, D., Bernardini, E., Bernardini, M. G., Bernardos, M., Bernloehr, K., Bertucci, B., Biasuzzi, B., Bigongiari, C., Biland, A., Bissaldi, E., Biteau, J., Blanch, O., Blazek, J., Boisson, C., Bolmont, J., Bonanno, G., Bonardi, A., Bonavolonta, C., Bonnoli, G., Bosnjak, Z., Bottcher, M., Braiding, C., Bregeon, J., Brill, A., Brown, A. M., Brun, P., Brunetti, G., Buanes, T., Buckley, J., Bugaev, V., Buehler, R., Bulgarelli, A., Bulik, T., Burton, M., Burtovoi, A., Busetto, G., Canestrari, R., Capalbi, M., Capitanio, F., Caproni, A., Caraveo, P., Cardenas, V., Carlile, C., Carosi, R., Carquin, E., Carr, J., Casanova, S., Cascone, E., Catalani, F., Catalano, O., Cauz, D., Cerruti, M., Chadwick, P., Chaty, S., Chaves, R. C. G., Chen, A., Chen, X., Chernyakova, M., Chikawa, M., Christov, A., Chudoba, J., Cieslar, M., Coco, V., Colafrancesco, S., Colin, P., Conforti, V., Connaughton, V., Conrad, J., Contreras, J. L., Cortina, J., Costa, A., Costantini, H., Cotter, G., Covino, S., Crocker, R., Cuadra, J., Cuevas, O., Cumani, P., D'Ai, A., D'Ammando, F., D'Avanzo, P., D'Urso, D., Daniel, M., Davids, I., Dawson, B., Dazzi, F., De Angelis, A., de Cassia dos Anjos, R., De Cesare, G., De Franco, A., De Gouveia Dal Pino, E. M., de la Calle, I., Lopez, R. de los Reyes, De Lotto, B., De Luca, A., De Lucia, M., de Naurois, M., de Ona Wilhelmi, E., De Palma, F., De Persio, F., de Souza, V., Deil, C., Del Santo, M., Delgado, C., della Volpe, D., Di Girolamo, T., Di Pierro, F., Di Venere, L., Diaz, C., Dib, C., Diebold, S., Djannati-Atai, A., Dominguez, A., Prester, D. Dominis, Dorner, D., Doro, M., Drass, H., Dravins, D., Dubus, G., Dwarkadas, V. V., Ebr, J., Eckner, C., Egberts, K., Einecke, S., Ekoume, T. R. N., Elsaesser, D., Ernenwein, J. -P, Espinoza, C., Evoli, C., Fairbairn, M., Falceta-Goncalves, D., Falcone, A., Farnier, C., Fasola, G., Fedorova, E., Fegan, S., Fernandez-Alonso, M., Fernandez-Barral, A., Ferrand, G., Fesquet, M., Filipovic, M., Fioretti, V., Fontaine, G., Fornasa, M., Fortson, L., Freixas Coromina, L., Fruck, C., Fujita, Y., Fukazawa, Y., Funk, S., Fuessling, M., Gabici, S., Gadola, A., Gallant, Y., Garcia, B., Garcia Lopez, R., Garczarczyk, M., Gaskins, J., Gasparetto, T., Gaug, M., Gerard, L., Giavitto, G., Giglietto, N., Giommi, P., Giordano, F., Giro, E., Giroletti, M., Giuliani, A., Glicenstein, J. -F, Gnatyk, R., Godinovic, N., Goldoni, P., Gomez-Vargas, G., Gonzalez, M. M., Gonzalez, J. M., Gotz, D., Graham, J., Grandi, P., Granot, J., Green, A. J., Greenshaw, T., Griffiths, S., Gunji, S., Hadasch, D., Hara, S., Hardcastle, M. J., Hassan, T., Hayashi, K., Hayashida, M., Heller, M., Helo, J. C., Hermann, G., Hinton, J., Hnatyk, B., Hofmann, W., Holder, J., Horan, D., Horandel, J., Horns, D., Horvath, P., Hovatta, T., Hrabovsky, M., Hrupec, D., Humensky, T. B., Huetten, M., Iarlori, M., Inada, T., Inome, Y., Inoue, S., Inoue, T., Inoue, Y., Iocco, F., Ioka, K., Iori, M., Ishio, K., Iwamura, Y., Jamrozy, M., Janecek, P., Jankowsky, D., Jean, P., Jung-Richardt, I., Jurysek, J., Kaaret, P., Karkar, S., Katagiri, H., Katz, U., Kawanaka, N., Kazanas, D., Khelifi, B., Kieda, D. B., Kimeswenger, S., Kimura, S., Kisaka, S., Knapp, J., Knodlseder, J., Koch, B., Kohri, K., Komin, N., Kosack, K., Kraus, M., Krause, M., Krauss, F., Kubo, H., Mezek, G. Kukec, Kuroda, H., Kushida, J., La Palombara, N., Lamanna, G., Lang, R. G., Lapington, J., Le Blanc, O., Leach, S., Lees, J. -P, Lefaucheur, J., Leigui de Oliveira, M. A., Lenain, J. -P, Lico, R., Limon, M., Lindfors, E., Lohse, T., Lombardi, S., Longo, F., Lopez, M., Lopez-Coto, R., Lu, C. -C, Lucarelli, F., Luque-Escamilla, P. L., Lyard, E., Maccarone, M. C., Maier, G., Majumdar, P., Malaguti, G., Mandat, D., Maneva, G., Manganaro, M., Mangano, S., Marcowith, A., Marin, J., Markoff, S., Marti, J., Martin, P., Martinez, M., Martinez, G., Masetti, N., Masuda, S., Maurin, G., Maxted, N., Mazin, D., Medina, C., Melandri, A., Mereghetti, S., Meyer, M., Minaya, I. A., Mirabal, N., Mirzoyan, R., Mitchell, A., Mizuno, T., Moderski, R., Mohammed, M., Mohrmann, L., Montaruli, T., Moralejo, A., Morcuende-Parrilla, D., Mori, K., Morlino, G., Morris, P., Morselli, A., Moulin, E., Mukherjee, R., Mundell, C., Murach, T., Muraishi, H., Murase, K., Nagai, A., Nagataki, S., Nagayoshi, T., Naito, T., Nakamori, T., Nakamura, Y., Niemiec, J., Nieto, D., Nikolajuk, M., Nishijima, K., Noda, K., Nosek, D., Novosyadlyj, B., Nozaki, S., O'Brien, P., Oakes, L., Ohira, Y., Ohishi, M., Ohm, S., Okazaki, N., Okumura, A., Ong, R. A., Orienti, M., Orito, R., Osborne, J. P., Ostrowski, M., Otte, N., Oya, I., Padovani, M., Paizis, A., Palatiello, M., Palatka, M., Paoletti, R., Paredes, J. M., Pareschi, G., Parsons, R. D., Pe'er, A., Pech, M., Pedaletti, G., Perri, M., Persic, M., Petrashyk, A., Petrucci, P., Petruk, O., Peyaud, B., Pfeifer, M., Piano, G., Pisarski, A., Pita, S., Pohl, M., Polo, M., Pozo, D., Prandini, E., Prast, J., Principe, G., Prokhorov, Dmitry, Prokoph, H., Prouza, M., Puehlhofer, G., Punch, Michael, Puerckhauer, S., Queiroz, F., Quirrenbach, A., Raino, S., Razzaque, S., Reimer, O., Reimer, A., Reisenegger, A., Renaud, M., Rezaeian, A. H., Rhode, W., Ribeiro, D., Ribo, M., Richtler, T., Rico, J., Rieger, F., Riquelme, M., Rivoire, S., Rizi, V., Rodriguez, J., Fernandez, G. Rodriguez, Rodriguez Vazquez, J. J., Rojas, G., Romano, P., Romeo, G., Rosado, J., Rovero, A. C., Rowell, G., Rudak, B., Rugliancich, A., Rulten, C., Sadeh, I., Safi-Harb, S., Saito, T., Sakaki, N., Sakurai, S., Salina, G., Sanchez-Conde, M., Sandaker, H., Sandoval, A., Sangiorgi, P., Sanguillon, M., Sano, H., Santander, M., Sarkar, S., Satalecka, K., Saturni, F. G., Schioppa, E. J., Schlenstedt, S., Schneider, M., Schoorlemmer, H., Schovanek, P., Schulz, A., Schussler, F., Schwanke, U., Sciacca, E., Scuderi, S., Seitenzahl, I., Semikoz, D., Sergijenko, O., Servillat, M., Shalchi, A., Shellard, R. C., Sidoli, L., Siejkowski, H., Sillanpaa, A., Sironi, G., Sitarek, J., Sliusar, V., Slowikowska, A., Sol, H., Stamerra, A., Stanic, S., Starling, R., Stawarz, L., Stefanik, S., Stephan, M., Stolarczyk, T., Stratta, G., Straumann, U., Suomijarvi, T., Supanitsky, A. D., Tagliaferri, G., Tajima, H., Tavani, M., Tavecchio, F., Tavernet, J. -P, Tayabaly, K., Tejedor, L. A., Temnikov, P., Terada, Y., Terrier, R., Terzic, T., Teshima, M., Testa, V., Thoudam, Satyendra, Tian, W., Tibaldo, L., Tluczykont, M., Todero Peixoto, C. J., Tokanai, F., Tomastik, J., Tonev, D., Tornikoski, M., Torres, D. F., Torresi, E., Tosti, G., Tothill, N., Tovmassian, G., Travnicek, P., Trichard, C., Trifoglio, M., Pujadas, I. Troyano, Tsujimoto, S., Umana, G., Vagelli, V., Vagnetti, F., Valentino, M., Vallania, P., Valore, L., van Eldik, C., Vandenbroucke, J., Varner, G. S., Vasileiadis, G., Vassiliev, V., Vazquez Acosta, M., Vecchi, M., Vega, A., Vercellone, S., Veres, P., Vergani, S., Verzi, V., Vettolani, G. P., Viana, A., Vigorito, C., Villanueva, J., Voelk, H., Vollhardt, A., Vorobiov, S., Vrastil, M., Vuillaume, T., Wagner, S. J., Wagner, R., Walter, R., Ward, J. E., Warren, D., Watson, J. J., Werner, F., White, M., White, R., Wierzcholska, A., Wilcox, P., Will, M., Williams, D. A., Wischnewski, R., Wood, M., Yamamoto, T., Yamazaki, R., Yanagita, S., Yang, L., Yoshida, T., Yoshiike, S., Yoshikoshi, T., Zacharias, M., Zaharijas, G., Zampieri, L., Zandanel, F., Zanin, R., Zavrtanik, M., Zavrtanik, D., Zdziarski, A. A., Zech, A., Zechlin, H., Zhdanov, V. I., Ziegler, A., and Zorn, J.
Published: 2019
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106. Melt crystallisation of polymer materials: The role of the thermal conductivity and its influence on the microstructure

Author: Raimo, M., Cascone, E., and Martuscelli, E.
Published: 2001

107. New spectro-photometric characterization of the substellar object HR 2562 B using SPHERE

Author: Mesa, D., Baudino, J. -L., Charnay, B., D’Orazi, V., Desidera, S., Boccaletti, A., Gratton, R., Bonnefoy, M., Delorme, P., Langlois, M., Vigan, A., Zurlo, A., Maire, A. -L., Janson, M., Antichi, J., Baruffolo, A., Bruno, P., Cascone, E., Chauvin, G., Claudi, R. U., De Caprio, V., Fantinel, D., Farisato, G., Feldt, M., Giro, E., Hagelberg, J., Incorvaia, S., Lagadec, E., Lagrange, A. -M., Lazzoni, C., Lessio, L., Salasnich, B., Scuderi, S., and Turatto, E. Sissa and M.
Published: 2018

108. Submarine slopes of the Messina seaport area: a model for the evaluation of the post-seismic serviceability conditions

Author: Biondi, G., Cascone, E, and Di Filippo, G.
Subjects: Messina seaport, Liquefiable soils, performance-based analysis, Messina seaport, Liquefiable soils, seismic slope stability, performance-based analysis, seismic slope stability
Published: 2018

109. VLT/SPHERE exploration of the young multiplanetary system PDS70

Author: Mesa, D., primary, Keppler, M., additional, Cantalloube, F., additional, Rodet, L., additional, Charnay, B., additional, Gratton, R., additional, Langlois, M., additional, Boccaletti, A., additional, Bonnefoy, M., additional, Vigan, A., additional, Flasseur, O., additional, Bae, J., additional, Benisty, M., additional, Chauvin, G., additional, de Boer, J., additional, Desidera, S., additional, Henning, T., additional, Lagrange, A.-M., additional, Meyer, M., additional, Milli, J., additional, Müller, A., additional, Pairet, B., additional, Zurlo, A., additional, Antoniucci, S., additional, Baudino, J.-L., additional, Brown Sevilla, S., additional, Cascone, E., additional, Cheetham, A., additional, Claudi, R. U., additional, Delorme, P., additional, D’Orazi, V., additional, Feldt, M., additional, Hagelberg, J., additional, Janson, M., additional, Kral, Q., additional, Lagadec, E., additional, Lazzoni, C., additional, Ligi, R., additional, Maire, A.-L., additional, Martinez, P., additional, Menard, F., additional, Meunier, N., additional, Perrot, C., additional, Petrus, S., additional, Pinte, C., additional, Rickman, E. L., additional, Rochat, S., additional, Rouan, D., additional, Samland, M., additional, Sauvage, J.-F., additional, Schmidt, T., additional, Udry, S., additional, Weber, L., additional, and Wildi, F., additional
Published: 2019
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110. SPHERE: the exoplanet imager for the Very Large Telescope

Author: Beuzit, J.-L., primary, Vigan, A., additional, Mouillet, D., additional, Dohlen, K., additional, Gratton, R., additional, Boccaletti, A., additional, Sauvage, J.-F., additional, Schmid, H. M., additional, Langlois, M., additional, Petit, C., additional, Baruffolo, A., additional, Feldt, M., additional, Milli, J., additional, Wahhaj, Z., additional, Abe, L., additional, Anselmi, U., additional, Antichi, J., additional, Barette, R., additional, Baudrand, J., additional, Baudoz, P., additional, Bazzon, A., additional, Bernardi, P., additional, Blanchard, P., additional, Brast, R., additional, Bruno, P., additional, Buey, T., additional, Carbillet, M., additional, Carle, M., additional, Cascone, E., additional, Chapron, F., additional, Charton, J., additional, Chauvin, G., additional, Claudi, R., additional, Costille, A., additional, De Caprio, V., additional, de Boer, J., additional, Delboulbé, A., additional, Desidera, S., additional, Dominik, C., additional, Downing, M., additional, Dupuis, O., additional, Fabron, C., additional, Fantinel, D., additional, Farisato, G., additional, Feautrier, P., additional, Fedrigo, E., additional, Fusco, T., additional, Gigan, P., additional, Ginski, C., additional, Girard, J., additional, Giro, E., additional, Gisler, D., additional, Gluck, L., additional, Gry, C., additional, Henning, T., additional, Hubin, N., additional, Hugot, E., additional, Incorvaia, S., additional, Jaquet, M., additional, Kasper, M., additional, Lagadec, E., additional, Lagrange, A.-M., additional, Le Coroller, H., additional, Le Mignant, D., additional, Le Ruyet, B., additional, Lessio, G., additional, Lizon, J.-L., additional, Llored, M., additional, Lundin, L., additional, Madec, F., additional, Magnard, Y., additional, Marteaud, M., additional, Martinez, P., additional, Maurel, D., additional, Ménard, F., additional, Mesa, D., additional, Möller-Nilsson, O., additional, Moulin, T., additional, Moutou, C., additional, Origné, A., additional, Parisot, J., additional, Pavlov, A., additional, Perret, D., additional, Pragt, J., additional, Puget, P., additional, Rabou, P., additional, Ramos, J., additional, Reess, J.-M., additional, Rigal, F., additional, Rochat, S., additional, Roelfsema, R., additional, Rousset, G., additional, Roux, A., additional, Saisse, M., additional, Salasnich, B., additional, Santambrogio, E., additional, Scuderi, S., additional, Segransan, D., additional, Sevin, A., additional, Siebenmorgen, R., additional, Soenke, C., additional, Stadler, E., additional, Suarez, M., additional, Tiphène, D., additional, Turatto, M., additional, Udry, S., additional, Vakili, F., additional, Waters, L. B. F. M., additional, Weber, L., additional, Wildi, F., additional, Zins, G., additional, and Zurlo, A., additional
Published: 2019
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111. Monte Carlo studies for the optimisation of the Cherenkov Telescope Array layout

Author: Acharyya, A., primary, Agudo, I., additional, Angüner, E.O., additional, Alfaro, R., additional, Alfaro, J., additional, Alispach, C., additional, Aloisio, R., additional, Alves Batista, R., additional, Amans, J.-P., additional, Amati, L., additional, Amato, E., additional, Ambrosi, G., additional, Antonelli, L.A., additional, Aramo, C., additional, Armstrong, T., additional, Arqueros, F., additional, Arrabito, L., additional, Asano, K., additional, Ashkar, H., additional, Balazs, C., additional, Balbo, M., additional, Balmaverde, B., additional, Barai, P., additional, Barbano, A., additional, Barkov, M., additional, Barres de Almeida, U., additional, Barrio, J.A., additional, Bastieri, D., additional, Becerra González, J., additional, Becker Tjus, J., additional, Bellizzi, L., additional, Benbow, W., additional, Bernardini, E., additional, Bernardos, M.I., additional, Bernlöhr, K., additional, Berti, A., additional, Berton, M., additional, Bertucci, B., additional, Beshley, V., additional, Biasuzzi, B., additional, Bigongiari, C., additional, Bird, R., additional, Bissaldi, E., additional, Biteau, J., additional, Blanch, O., additional, Blazek, J., additional, Boisson, C., additional, Bonanno, G., additional, Bonardi, A., additional, Bonavolontá, C., additional, Bonnoli, G., additional, Bordas, P., additional, Böttcher, M., additional, Bregeon, J., additional, Brill, A., additional, Brown, A.M., additional, Brügge, K., additional, Brun, P., additional, Bruno, P., additional, Bulgarelli, A., additional, Bulik, T., additional, Burton, M., additional, Burtovoi, A., additional, Busetto, G., additional, Cameron, R., additional, Canestrari, R., additional, Capalbi, M., additional, Caproni, A., additional, Capuzzo-Dolcetta, R., additional, Caraveo, P., additional, Caroff, S., additional, Carosi, R., additional, Casanova, S., additional, Cascone, E., additional, Cassol, F., additional, Catalani, F., additional, Catalano, O., additional, Cauz, D., additional, Cerruti, M., additional, Chaty, S., additional, Chen, A., additional, Chernyakova, M., additional, Chiaro, G., additional, Cieślar, M., additional, Colak, S.M., additional, Conforti, V., additional, Congiu, E., additional, Contreras, J.L., additional, Cortina, J., additional, Costa, A., additional, Costantini, H., additional, Cotter, G., additional, Cristofari, P., additional, Cumani, P., additional, Cusumano, G., additional, D’Aí, A., additional, D’Ammando, F., additional, Dangeon, L., additional, Da Vela, P., additional, Dazzi, F., additional, De Angelis, A., additional, De Caprio, V., additional, de Cássia dos Anjos, R., additional, De Frondat, F., additional, de Gouveia Dal Pino, E.M., additional, De Lotto, B., additional, De Martino, D., additional, de Naurois, M., additional, de Oña Wilhelmi, E., additional, de Palma, F., additional, de Souza, V., additional, Del Santo, M., additional, Delgado, C., additional, della Volpe, D., additional, Di Girolamo, T., additional, Di Pierro, F., additional, Di Venere, L., additional, Díaz, C., additional, Diebold, S., additional, Djannati-Ataï, A., additional, Dmytriiev, A., additional, Dominis Prester, D., additional, Donini, A., additional, Dorner, D., additional, Doro, M., additional, Dournaux, J.-L., additional, Ebr, J., additional, Ekoume, T.R.N., additional, Elsässer, D., additional, Emery, G., additional, Falceta-Goncalves, D., additional, Fedorova, E., additional, Fegan, S., additional, Feng, Q., additional, Ferrand, G., additional, Fiandrini, E., additional, Fiasson, A., additional, Filipovic, M., additional, Fioretti, V., additional, Fiori, M., additional, Flis, S., additional, Fonseca, M.V., additional, Fontaine, G., additional, Freixas Coromina, L., additional, Fukami, S., additional, Fukui, Y., additional, Funk, S., additional, Füßling, M., additional, Gaggero, D., additional, Galanti, G., additional, Garcia López, R.J., additional, Garczarczyk, M., additional, Gascon, D., additional, Gasparetto, T., additional, Gaug, M., additional, Ghalumyan, A., additional, Gianotti, F., additional, Giavitto, G., additional, Giglietto, N., additional, Giordano, F., additional, Giroletti, M., additional, Gironnet, J., additional, Glicenstein, J.-F., additional, Gnatyk, R., additional, Goldoni, P., additional, González, J.M., additional, González, M.M., additional, Gourgouliatos, K.N., additional, Grabarczyk, T., additional, Granot, J., additional, Green, D., additional, Greenshaw, T., additional, Grondin, M.-H., additional, Gueta, O., additional, Hadasch, D., additional, Hassan, T., additional, Hayashida, M., additional, Heller, M., additional, Hervet, O., additional, Hinton, J., additional, Hiroshima, N., additional, Hnatyk, B., additional, Hofmann, W., additional, Horvath, P., additional, Hrabovsky, M., additional, Hrupec, D., additional, Humensky, T.B., additional, Hütten, M., additional, Inada, T., additional, Iocco, F., additional, Ionica, M., additional, Iori, M., additional, Iwamura, Y., additional, Jamrozy, M., additional, Janecek, P., additional, Jankowsky, D., additional, Jean, P., additional, Jouvin, L., additional, Jurysek, J., additional, Kaaret, P., additional, Kadowaki, L.H.S., additional, Karkar, S., additional, Kerszberg, D., additional, Khélifi, B., additional, Kieda, D., additional, Kimeswenger, S., additional, Kluźniak, W., additional, Knapp, J., additional, Knödlseder, J., additional, Kobayashi, Y., additional, Koch, B., additional, Kocot, J., additional, Komin, N., additional, Kong, A., additional, Kowal, G., additional, Krause, M., additional, Kubo, H., additional, Kushida, J., additional, Kushwaha, P., additional, La Parola, V., additional, La Rosa, G., additional, Lallena Arquillo, M., additional, Lang, R.G., additional, Lapington, J., additional, Le Blanc, O., additional, Lefaucheur, J., additional, Leigui de Oliveira, M.A., additional, Lemoine-Goumard, M., additional, Lenain, J.-P., additional, Leto, G., additional, Lico, R., additional, Lindfors, E., additional, Lohse, T., additional, Lombardi, S., additional, Longo, F., additional, Lopez, A., additional, López, M., additional, Lopez-Oramas, A., additional, López-Coto, R., additional, Loporchio, S., additional, Luque-Escamilla, P.L., additional, Lyard, E., additional, Maccarone, M.C., additional, Mach, E., additional, Maggio, C., additional, Majumdar, P., additional, Malaguti, G., additional, Mallamaci, M., additional, Mandat, D., additional, Maneva, G., additional, Manganaro, M., additional, Mangano, S., additional, Marculewicz, M., additional, Mariotti, M., additional, Martí, J., additional, Martínez, M., additional, Martínez, G., additional, Martínez-Huerta, H., additional, Masuda, S., additional, Maxted, N., additional, Mazin, D., additional, Meunier, J.-L., additional, Meyer, M., additional, Micanovic, S., additional, Millul, R., additional, Minaya, I.A., additional, Mitchell, A., additional, Mizuno, T., additional, Moderski, R., additional, Mohrmann, L., additional, Montaruli, T., additional, Moralejo, A., additional, Morcuende, D., additional, Morlino, G., additional, Morselli, A., additional, Moulin, E., additional, Mukherjee, R., additional, Munar, P., additional, Mundell, C., additional, Murach, T., additional, Nagai, A., additional, Nagayoshi, T., additional, Naito, T., additional, Nakamori, T., additional, Nemmen, R., additional, Niemiec, J., additional, Nieto, D., additional, Nievas Rosillo, M., additional, Nikołajuk, M., additional, Ninci, D., additional, Nishijima, K., additional, Noda, K., additional, Nosek, D., additional, Nöthe, M., additional, Nozaki, S., additional, Ohishi, M., additional, Ohtani, Y., additional, Okumura, A., additional, Ong, R.A., additional, Orienti, M., additional, Orito, R., additional, Ostrowski, M., additional, Otte, N., additional, Ou, Z., additional, Oya, I., additional, Pagliaro, A., additional, Palatiello, M., additional, Palatka, M., additional, Paoletti, R., additional, Paredes, J.M., additional, Pareschi, G., additional, Parmiggiani, N., additional, Parsons, R.D., additional, Patricelli, B., additional, Pe’er, A., additional, Pech, M., additional, Peñil Del Campo, P., additional, Pérez-Romero, J., additional, Perri, M., additional, Persic, M., additional, Petrucci, P.-O., additional, Petruk, O., additional, Pfrang, K., additional, Piel, Q., additional, Pietropaolo, E., additional, Pohl, M., additional, Polo, M., additional, Poutanen, J., additional, Prandini, E., additional, Produit, N., additional, Prokoph, H., additional, Prouza, M., additional, Przybilski, H., additional, Pühlhofer, G., additional, Punch, M., additional, Queiroz, F., additional, Quirrenbach, A., additional, Rainò, S., additional, Rando, R., additional, Razzaque, S., additional, Reimer, O., additional, Renault-Tinacci, N., additional, Renier, Y., additional, Ribeiro, D., additional, Ribó, M., additional, Rico, J., additional, Rieger, F., additional, Rizi, V., additional, Rodriguez Fernandez, G., additional, Rodriguez-Ramirez, J.C., additional, Rodrí-guez Vázquez, J.J., additional, Romano, P., additional, Romeo, G., additional, Roncadelli, M., additional, Rosado, J., additional, Rowell, G., additional, Rudak, B., additional, Rugliancich, A., additional, Rulten, C., additional, Sadeh, I., additional, Saha, L., additional, Saito, T., additional, Sakurai, S., additional, Salesa Greus, F., additional, Sangiorgi, P., additional, Sano, H., additional, Santander, M., additional, Santangelo, A., additional, Santos-Lima, R., additional, Sanuy, A., additional, Satalecka, K., additional, Saturni, F.G., additional, Sawangwit, U., additional, Schlenstedt, S., additional, Schovanek, P., additional, Schussler, F., additional, Schwanke, U., additional, Sciacca, E., additional, Scuderi, S., additional, Sedlaczek, K., additional, Seglar-Arroyo, M., additional, Sergijenko, O., additional, Seweryn, K., additional, Shalchi, A., additional, Shellard, R.C., additional, Siejkowski, H., additional, Sillanpää, A., additional, Sinha, A., additional, Sironi, G., additional, Sliusar, V., additional, Slowikowska, A., additional, Sol, H., additional, Specovius, A., additional, Spencer, S., additional, Spengler, G., additional, Stamerra, A., additional, Stanič, S., additional, Stawarz, Ł., additional, Stefanik, S., additional, Stolarczyk, T., additional, Straumann, U., additional, Suomijarvi, T., additional, Świerk, P., additional, Szepieniec, T., additional, Tagliaferri, G., additional, Tajima, H., additional, Tam, T., additional, Tavecchio, F., additional, Taylor, L., additional, Tejedor, L.A., additional, Temnikov, P., additional, Terzic, T., additional, Testa, V., additional, Tibaldo, L., additional, Todero Peixoto, C.J., additional, Tokanai, F., additional, Tomankova, L., additional, Tonev, D., additional, Torres, D.F., additional, Tosti, G., additional, Tosti, L., additional, Tothill, N., additional, Toussenel, F., additional, Tovmassian, G., additional, Travnicek, P., additional, Trichard, C., additional, Umana, G., additional, Vagelli, V., additional, Valentino, M., additional, Vallage, B., additional, Vallania, P., additional, Valore, L., additional, Vandenbroucke, J., additional, Varner, G.S., additional, Vasileiadis, G., additional, Vassiliev, V., additional, Vázquez Acosta, M., additional, Vecchi, M., additional, Vercellone, S., additional, Vergani, S., additional, Vettolani, G.P., additional, Viana, A., additional, Vigorito, C.F., additional, Vink, J., additional, Vitale, V., additional, Voelk, H., additional, Vollhardt, A., additional, Vorobiov, S., additional, Wagner, S.J., additional, Walter, R., additional, Werner, F., additional, White, R., additional, Wierzcholska, A., additional, Will, M., additional, Williams, D.A., additional, Wischnewski, R., additional, Yang, L., additional, Yoshida, T., additional, Yoshikoshi, T., additional, Zacharias, M., additional, Zampieri, L., additional, Zavrtanik, M., additional, Zavrtanik, D., additional, Zdziarski, A.A., additional, Zech, A., additional, Zechlin, H., additional, Zenin, A., additional, Zhdanov, V.I., additional, Zimmer, S., additional, and Zorn, J., additional
Published: 2019
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112. Orbiting a binary: SPHERE characterisation of the HD 284149 system

Author: Bonavita, M., d'Orazi, V., Mesa, D., Fontanive, C., Desidera, S., Messina, S., Daemgen, S., Gratton, R., Vigan, Arthur, Bonnefoy, M., Zurlo, A., Antichi, J., Avenhaus, H., Baruffolo, A., Baudino, J. L., Beuzit, J. L., Boccaletti, A., Bruno, P., Buey, T., Carbillet, M., Cascone, E., Chauvin, G., Claudi, R. U., de Caprio, V., Fantinel, D., Farisato, G., Feldt, M., Galicher, R., Giro, E., Gry, C., Hagelberg, J., Incorvaia, S., Janson, M., Jaquet, M., Lagrange, A. M., Langlois, M., Lannier, J., Le Coroller, H., Lessio, L., Ligi, R., Maire, A. L., Meyer, M., Menard, F., Perrot, C., Peretti, S., Petit, C., Ramos, J., Roux, A., Salasnich, B., Salter, G., Samland, M., Scuderi, S., Schlieder, J., Surez, M., Turatto, M., Weber, L., INAF - Osservatorio Astronomico di Padova (OAPD), Istituto Nazionale di Astrofisica (INAF), SUPA, Institute for Astronomy, University of Edinburgh, Monash University [Melbourne], Institute for Astronomy [Edinburgh] (IfA), INAF - Osservatorio Astrofisico di Catania (OACT), Institute of Astronomy [ETH Zürich], Department of Physics [ETH Zürich] (D-PHYS), Eidgenössische Technische Hochschule - Swiss Federal Institute of Technology [Zürich] (ETH Zürich)- Eidgenössische Technische Hochschule - Swiss Federal Institute of Technology [Zürich] (ETH Zürich), 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), Institut de Planétologie et d'Astrophysique de Grenoble (IPAG), Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Observatoire des Sciences de l'Univers de Grenoble (OSUG ), Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut national des sciences de l'Univers (INSU - CNRS)-Institut national de recherche en sciences et technologies pour l'environnement et l'agriculture (IRSTEA)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes [2016-2019] (UGA [2016-2019])-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut national de recherche en sciences et technologies pour l'environnement et l'agriculture (IRSTEA)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes [2016-2019] (UGA [2016-2019]), Universidad Diego Portales [Santiago] (UDP), INAF - Osservatorio Astrofisico di Arcetri (OAA), Eidgenössische Technische Hochschule - Swiss Federal Institute of Technology [Zürich] (ETH Zürich), University of Oxford, Laboratoire d'études spatiales et d'instrumentation en astrophysique = Laboratory of Space Studies and Instrumentation in Astrophysics (LESIA), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), Observatoire de la Côte d'Azur (OCA), Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), INAF - Osservatorio Astronomico di Capodimonte (OAC), Max-Planck-Institut für Astronomie (MPIA), Max-Planck-Gesellschaft, INAF - Osservatorio Astronomico di Milano (OAM), Department of Astronomy, Stockholm University, Max Planck Institute for Radio Astronomy, Département de Physique Nucléaire (ex SPhN) (DPHN), Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, Laboratoire Franco-Chilien d'Astronomie (LFCA), Universidad de Chile = University of Chile [Santiago] (UCHILE)-Pontificia Universidad Católica de Chile (UC)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Universidad de Concepción - University of Concepcion [Chile], Observatoire Astronomique de l'Université de Genève (ObsGE), Université de Genève = University of Geneva (UNIGE), ONERA, NASA Goddard Space Flight Center (GSFC), Centre de Recherche en Acquisition et Traitement de l'Image pour la Santé (CREATIS), Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut National des Sciences Appliquées de Lyon (INSA Lyon), Université de Lyon-Institut National des Sciences Appliquées (INSA)-Institut National des Sciences Appliquées (INSA)-Université Jean Monnet - Saint-Étienne (UJM)-Institut National de la Santé et de la Recherche Médicale (INSERM)-Centre National de la Recherche Scientifique (CNRS), Centre National d'Études Spatiales [Toulouse] (CNES)-Observatoire des Sciences de l'Univers de Grenoble (OSUG ), Institut national des sciences de l'Univers (INSU - CNRS)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)-Institut National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement (INRAE)-Université Grenoble Alpes (UGA)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)-Institut National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement (INRAE)-Université Grenoble Alpes (UGA), University of Oxford [Oxford], Laboratoire d'études spatiales et d'instrumentation en astrophysique (LESIA (UMR_8109)), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), Universidad de Concepción [Chile]-Pontificia Universidad Católica de Chile (UC)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Universidad de Chile, Université de Genève (UNIGE), Université Jean Monnet [Saint-Étienne] (UJM)-Hospices Civils de Lyon (HCL)-Institut National des Sciences Appliquées de Lyon (INSA Lyon), Université de Lyon-Institut National des Sciences Appliquées (INSA)-Université de Lyon-Institut National des Sciences Appliquées (INSA)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Centre National de la Recherche Scientifique (CNRS)-Institut National de la Santé et de la Recherche Médicale (INSERM), Joseph Louis LAGRANGE (LAGRANGE), 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, 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), Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Aix Marseille Université (AMU)-Centre National d'Études Spatiales [Toulouse] (CNES), and Institut National des Sciences Appliquées (INSA)-Université de Lyon-Institut National des Sciences Appliquées (INSA)-Université de Lyon-Université Claude Bernard Lyon 1 (UCBL)
Subjects: [PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM], stars: individual: HD 284149, stars: rotation, techniques: high angular resolution, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], binaries: visual, brown dwarfs
Abstract: International audience; Aims. In this paper we present the results of the SPHERE observation of the HD 284149 system, aimed at a more detailed characterisation of both the primary and its brown dwarf companion. Methods. We observed HD 284149 in the near-infrared with SPHERE, using the imaging mode (IRDIS+IFS) and the long-slit spectroscopy mode (IRDIS-LSS). The data were reduced using the dedicated SPHERE pipeline, and algorithms such as PCA and TLOCI were applied to reduce the speckle pattern. Results. The IFS images revealed a previously unknown low-mass (~0.16 M ⊙ ) stellar companion ( HD 294149 B) at ~0.1′′, compatible with previously observed radial velocity differences, as well as proper motion differences between Gaia and Tycho -2 measurements. The known brown dwarf companion ( HD 284149 b) is clearly visible in the IRDIS images. This allowed us to refine both its photometry and astrometry. The analysis of the medium resolution IRDIS long slit spectra also allowed a refinement of temperature and spectral type estimates. A full reassessment of the age and distance of the system was also performed, leading to more precise values of both mass and semi-major axis. Conclusions. As a result of this study, HD 284149 ABb therefore becomes the latest addition to the (short) list of brown dwarfs on wide circumbinary orbits, providing new evidence to support recent claims that object in such configuration occur with a similar frequency to wide companions to single stars.
Published: 2017

113. Flow and deformation failure of sandy slopes

Author: Biondi, G, Cascone, E, and Maugeri, M
Published: 2002
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114. High-contrast study of the candidate planets and protoplanetary disk around HD 100546

Author: Sissa, E., Gratton, R., Garufi, A., Rigliaco, E., Zurlo, A., Mesa, D., Langlois, M., de Boer, J., Desidera, S., Ginski, C., Lagrange, A. -M., Maire, A. -L., Vigan, A., Dima, M., Antichi, J., Baruffolo, A., Bazzon, A., Benisty, M., Beuzit, J. -L., Biller, B., Boccaletti, A., Bonavita, M., Bonnefoy, M., Brandner, W., Bruno, P., Buenzli, E., Cascone, E., Chauvin, G., Cheetham, A., Claudi, R. U., Cudel, M., De Caprio, V., Dominik, C., Fantinel, D., Farisato, G., Feldt, M., Fontanive, C., Galicher, R., Giro, E., Hagelberg, J., Incorvaia, S., Janson, Markus, Kasper, M., Keppler, M., Kopytova, T., Lagadec, E., Lannier, J., Lazzoni, C., LeCoroller, H., Lessio, L., Ligi, R., Marzari, F., Menard, F., Meyer, M. R., Mouillet, D., Peretti, S., Perrot, C., Potiron, P. J., Rouan, D., Salasnich, B., Salter, G., Samland, M., Schmidt, T., Scuderi, S., Wildi, F., Sissa, E., Gratton, R., Garufi, A., Rigliaco, E., Zurlo, A., Mesa, D., Langlois, M., de Boer, J., Desidera, S., Ginski, C., Lagrange, A. -M., Maire, A. -L., Vigan, A., Dima, M., Antichi, J., Baruffolo, A., Bazzon, A., Benisty, M., Beuzit, J. -L., Biller, B., Boccaletti, A., Bonavita, M., Bonnefoy, M., Brandner, W., Bruno, P., Buenzli, E., Cascone, E., Chauvin, G., Cheetham, A., Claudi, R. U., Cudel, M., De Caprio, V., Dominik, C., Fantinel, D., Farisato, G., Feldt, M., Fontanive, C., Galicher, R., Giro, E., Hagelberg, J., Incorvaia, S., Janson, Markus, Kasper, M., Keppler, M., Kopytova, T., Lagadec, E., Lannier, J., Lazzoni, C., LeCoroller, H., Lessio, L., Ligi, R., Marzari, F., Menard, F., Meyer, M. R., Mouillet, D., Peretti, S., Perrot, C., Potiron, P. J., Rouan, D., Salasnich, B., Salter, G., Samland, M., Schmidt, T., Scuderi, S., and Wildi, F.
Abstract: The nearby Herbig Be star HD 100546 is known to be a laboratory for the study of protoplanets and their relation with the circum stellar disk, which is carved by at least two gaps. We observed the HD 100546 environment with high-contrast imaging exploiting several different observing modes of SPHERE, including data sets with and without coronagraphs, dual band imaging, integral field spectroscopy and polarimetry. The picture emerging from these different data sets is complex. Flux-conservative algorithm images clearly show the disk up to 200 au. More aggressive algorithms reveal several rings and warped arms that are seen overlapping the main disk. Some of these structures are found to lie at considerable height over the disk mid-plane at about 30 au. Our images demon-strate that the brightest wings close to the star in the near side of the disk are a unique structure, corresponding to the outer edge of the intermediate disk at similar to 40 au. Modeling of the scattered light from the disk with a geometrical algorithm reveals that a moderately thin structure (H/r = 0.18 at 40 au) can well reproduce the light distribution in the flux-conservative images. We suggest that the gap between 44 and 113 au spans between the 1:2 and 3:2 resonance orbits of a massive body located at similar to 70 au, which might coincide with the candidate planet HD 100546b detected with previous thermal infrared (IR) observations. In this picture, the two wings can be the near side of a ring formed by disk material brought out of the disk at the 1:2 resonance with the same massive object. While we find no clear evidence confirming detection of the planet candidate HD 100546c in our data, we find a diffuse emission close to the expected position of HD 100546b. This source can be described as an extremely reddened substellar object surrounded by a dust cloud or its circumplanetary disk. Its astrometry is broadly consistent with a circular orbital motion on the disk plane, a result that could
Published: 2018
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115. New spectro-photometric characterization of the substellar object HR2562B using SPHERE

Author: Mesa, D., Baudino, J. -L., Charnay, B., D'Orazi, V., Desidera, S., Boccaletti, A., Gratton, R., Bonnefoy, M., Delorme, P., Langlois, M., Vigan, A., Zurlo, A., Maire, A. -L., Janson, Markus, Antichi, J., Baruffolo, A., Bruno, P., Cascone, E., Chauvin, G., Claudi, R. U., De Caprio, V., Fantinel, D., Farisato, G., Feldt, M., Giro, E., Hagelberg, J., Incorvaia, S., Lagadec, E., Lagrange, A. -M., Lazzoni, C., Lessio, L., Salasnich, B., Scuderi, S., Sissa, E., Turatto, M., Mesa, D., Baudino, J. -L., Charnay, B., D'Orazi, V., Desidera, S., Boccaletti, A., Gratton, R., Bonnefoy, M., Delorme, P., Langlois, M., Vigan, A., Zurlo, A., Maire, A. -L., Janson, Markus, Antichi, J., Baruffolo, A., Bruno, P., Cascone, E., Chauvin, G., Claudi, R. U., De Caprio, V., Fantinel, D., Farisato, G., Feldt, M., Giro, E., Hagelberg, J., Incorvaia, S., Lagadec, E., Lagrange, A. -M., Lazzoni, C., Lessio, L., Salasnich, B., Scuderi, S., Sissa, E., and Turatto, M.
Abstract: Aims. HR2562 is an F5V star located at similar to 33 pc from the Sun hosting a substellar companion that was discovered using the Gemini planet imager (GPI) instrument. The main objective of the present paper is to provide an extensive characterization of the substellar companion, by deriving its fundamental properties. Methods. We observed HR2562 with the near-infrared branch composed by the integral field spectrograph (IFS) and the infrared dual band spectrograph (IRDIS) of the spectro-polarimetric high-contrast exoplanet research (SPHERE) instrument at the very large telescope (VLT). During our observations IFS was operating in the YJ band, while IRDIS was observing with the H broadband filter. The data were reduced with the dedicated SPHERE GTO pipeline, which is custom designed for this instrument. On the reduced images, we then applied the post-processing procedures that are specifically prepared to subtract the speckle noise. Results. The companion is clearly detected in both IRDIS and IFS datasets. We obtained photometry in three different spectral bands. The comparison with template spectra allowed us to derive a spectral type of T2-T3 for the companion. Using both evolutionary and atmospheric models we inferred the main physical parameters of the companion obtaining a mass of 32 +/- 14 M-Jup, T-eff = 1100 +/- 200 K, and log g = 4.75 +/- 0.41.
Published: 2018
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116. Dynamical models to explain observations with SPHERE in planetary systems with double debris belts

Author: Lazzoni, C., Desidera, S., Marzari, F., Boccaletti, A., Langlois, M., Mesa, D., Gratton, R., Kral, Q., Pawellek, N., Olofsson, J., Bonnefoy, M., Chauvin, G., Lagrange, A. M., Vigan, A., Sissa, E., Antichi, J., Avenhaus, H., Baruffolo, A., Baudino, J. L., Bazzon, A., Beuzit, J. L., Biller, B., Bonavita, M., Brandner, W., Bruno, P., Buenzli, E., Cantalloube, F., Cascone, E., Cheetham, A., Claudi, R. U., Cudel, M., Daemgen, S., De Caprio, V., Delorme, P., Fantinel, D., Farisato, G., Feldt, M., Galicher, R., Ginski, C., Girard, J., Giro, E., Janson, Markus, Hagelberg, J., Henning, T., Incorvaia, S., Kasper, M., Kopytova, T., Lannier, J., LeCoroller, H., Lessio, L., Ligi, R., Maire, A. L., Menard, F., Meyer, M., Milli, J., Mouillet, D., Peretti, S., Perrot, C., Rouan, D., Samland, M., Salasnich, B., Salter, G., Schmidt, T., Scuderi, S., Sezestre, E., Turatto, M., Udry, S., Wildi, F., Zurlo, A., Lazzoni, C., Desidera, S., Marzari, F., Boccaletti, A., Langlois, M., Mesa, D., Gratton, R., Kral, Q., Pawellek, N., Olofsson, J., Bonnefoy, M., Chauvin, G., Lagrange, A. M., Vigan, A., Sissa, E., Antichi, J., Avenhaus, H., Baruffolo, A., Baudino, J. L., Bazzon, A., Beuzit, J. L., Biller, B., Bonavita, M., Brandner, W., Bruno, P., Buenzli, E., Cantalloube, F., Cascone, E., Cheetham, A., Claudi, R. U., Cudel, M., Daemgen, S., De Caprio, V., Delorme, P., Fantinel, D., Farisato, G., Feldt, M., Galicher, R., Ginski, C., Girard, J., Giro, E., Janson, Markus, Hagelberg, J., Henning, T., Incorvaia, S., Kasper, M., Kopytova, T., Lannier, J., LeCoroller, H., Lessio, L., Ligi, R., Maire, A. L., Menard, F., Meyer, M., Milli, J., Mouillet, D., Peretti, S., Perrot, C., Rouan, D., Samland, M., Salasnich, B., Salter, G., Schmidt, T., Scuderi, S., Sezestre, E., Turatto, M., Udry, S., Wildi, F., and Zurlo, A.
Abstract: Context. A large number of systems harboring a debris disk show evidence for a double belt architecture. One hypothesis for explaining the gap between the debris belts in these disks is the presence of one or more planets dynamically carving it. For this reason these disks represent prime targets for searching planets using direct imaging instruments, like the Spectro-Polarimetric High-constrast Exoplanet Research (SPHERE) at the Very Large Telescope. Aims. The goal of this work is to investigate this scenario in systems harboring debris disks divided into two components, placed, respectively, in the inner and outer parts of the system. All the targets in the sample were observed with the SPHERE instrument, which performs high-contrast direct imaging, during the SHINE guaranteed time observations. Positions of the inner and outer belts were estimated by spectral energy distribution fitting of the infrared excesses or, when available, from resolved images of the disk. Very few planets have been observed so far in debris disks gaps and we intended to test if such non-detections depend on the observational limits of the present instruments. This aim is achieved by deriving theoretical predictions of masses, eccentricities, and semi-major axes of planets able to open the observed gaps and comparing such parameters with detection limits obtained with SPHERE. Methods. The relation between the gap and the planet is due to the chaotic zone neighboring the orbit of the planet. The radial extent of this zone depends on the mass ratio between the planet and the star, on the semi-major axis, and on the eccentricity of the planet, and it can be estimated analytically. We first tested the different analytical predictions using a numerical tool for the detection of chaotic behavior and then selected the best formula for estimating a planet's physical and dynamical properties required to open the observed gap. We then apply the formalism to the case of one single planet on a circul
Published: 2018
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117. Prospects for CTA observations of the young SNR RX J1713.7-3946

Author: Cta Consortium, The, Acero, F., Aloisio, R., Amans, J., Amato, E., Antonelli, L. A., Aramo, C., Armstrong, T., Arqueros, F., Asano, K., Ashley, M., Backes, M., Balazs, C., Balzer, A., Bamba, A., Barkov, M., Barrio, J. A., Benbow, W., Bernlöhr, K., Beshley, V., Bigongiari, C., Biland, A., Bilinsky, A., Bissaldi, E., Biteau, J., Blanch, O., Blasi, P., Blazek, J., Boisson, C., Bonanno, G., Bonardi, A., Bonavolontà, C., Bonnoli, G., Braiding, C., Brau-Nogué, S., Bregeon, J., Brown, A. M., Bugaev, V., Bulgarelli, A., Bulik, T., Burton, M., Burtovoi, A., Busetto, G., Böttcher, M., Cameron, R., Capalbi, M., Caproni, A., Caraveo, P., Carosi, R., Cascone, E., Cerruti, M., Chaty, S., Chen, A., Chen, X., Chernyakova, M., Chikawa, M., Chudoba, J., Cohen-Tanugi, J., Colafrancesco, S., Conforti, V., Contreras, J. L., Costa, A., Cotter, G., Covino, S., Covone, G., Cumani, P., Cusumano, G., D Ammando, F., D Urso, D., Daniel, M., Dazzi, F., Angelis, A., Cesare, G., Franco, A., Frondat, F., Gouveia Dal Pino, E. M., Lisio, C., Los Reyes Lopez, R., Lotto, B., Naurois, M., Palma, F., Del Santo, M., Delgado, C., Della Volpe, D., Di Girolamo, T., Di Giulio, C., Di Pierro, F., Di Venere, L., Doro, M., Dournaux, J., Dumas, D., Dwarkadas, V., Díaz, C., Ebr, J., Egberts, K., Einecke, S., Elsässer, D., Eschbach, S., Falceta-Goncalves, D., Fasola, G., Fedorova, E., Fernández-Barral, A., Ferrand, G., Fesquet, M., Fiandrini, E., Fiasson, A., Filipovíc, M. D., Fioretti, V., Font, L., Fontaine, G., Franco, F. J., Freixas Coromina, L., Fujita, Y., Fukui, Y., Funk, S., Förster, A., Gadola, A., Garcia López, R., Garczarczyk, M., Giglietto, N., Giordano, F., Giuliani, A., Glicenstein, J., Gnatyk, R., Goldoni, P., Grabarczyk, T., Graciani, R., Graham, J., Grandi, P., Granot, J., Green, A. J., Griffiths, S., Gunji, S., Hakobyan, H., Hara, S., Hassan, T., Hayashida, M., Heller, M., Helo, J. C., Hinton, J., Hnatyk, B., Huet, J., Huetten, M., Humensky, T. B., Hussein, M., Hörandel, J., Ikeno, Y., Inada, T., Inome, Y., Inoue, S., Inoue, T., Inoue, Y., Ioka, K., Iori, M., Jacquemier, J., Janecek, P., Jankowsky, D., Jung, I., Kaaret, P., Katagiri, H., Kimeswenger, S., Kimura, S., Knödlseder, J., Koch, B., Kocot, J., Kohri, K., Komin, N., Konno, Y., Kosack, K., Koyama, S., Kraus, M., Kubo, H., Kukec Mezek, G., Kushida, J., La Palombara, N., Lalik, K., Lamanna, G., Landt, H., Lapington, J., Laporte, P., Lee, S., Lees, J., Lefaucheur, J., Lenain, J. -P, Leto, G., Lindfors, E., Lohse, T., Lombardi, S., Longo, F., Lopez, M., Lucarelli, F., Luque-Escamilla, P. L., López-Coto, R., Maccarone, M. C., Maier, G., Malaguti, G., Mandat, D., Maneva, G., Mangano, S., Marcowith, A., Martí, J., Martínez, M., Martínez, G., Masuda, S., Maurin, G., Maxted, N., Melioli, C., Mineo, T., Mirabal, N., Mizuno, T., Moderski, R., Mohammed, M., Montaruli, T., Moralejo, A., Mori, K., Morlino, G., Morselli, A., Moulin, E., Mukherjee, R., Mundell, C., Muraishi, H., Murase, K., Nagataki, S., Nagayoshi, T., Naito, T., Nakajima, D., Nakamori, T., Nemmen, R., Niemiec, J., Nieto, D., Nievas-Rosillo, M., Nikołajuk, M., Nishijima, K., Noda, K., Nogues, L., Nosek, D., Novosyadlyj, B., Nozaki, S., Ohira, Y., Ohishi, M., Ohm, S., Okumura, A., Ong, R. A., Orito, R., Orlati, A., Ostrowski, M., Oya, I., Padovani, M., Palacio, J., Palatka, M., Paredes, J. M., Pavy, S., Pe Er, A., Persic, M., Petrucci, P., Petruk, O., Pisarski, A., Pohl, M., Porcelli, A., Prandini, E., Prast, J., Principe, G., Prouza, M., Pueschel, E., Pühlhofer, G., Quirrenbach, A., Rameez, M., Reimer, O., Renaud, M., Ribó, M., Rico, J., Rizi, V., Rodriguez, J., Rodriguez Fernandez, G., Rodríguez Vázquez, J. J., Romano, P., Romeo, G., Rosado, J., Rousselle, J., Rowell, G., Rudak, B., Sadeh, I., Safi-Harb, S., Saito, T., Sakaki, N., Sanchez, D., Sangiorgi, P., Sano, H., Santander, M., Sarkar, S., Sawada, M., Schioppa, E. J., Schoorlemmer, H., Schovanek, P., Schussler, F., Sergijenko, O., Servillat, M., Shalchi, A., Shellard, R. C., Siejkowski, H., Sillanpää, A., Simone, D., Sliusar, V., Sol, H., Stanič, S., Starling, R., Stawarz, Ł., Stefanik, S., Stephan, M., Stolarczyk, T., Szanecki, M., Szepieniec, T., Tagliaferri, G., Tajima, H., Takahashi, M., Takeda, J., Tanaka, M., Tanaka, S., Tejedor, L. A., Telezhinsky, I., Temnikov, P., Terada, Y., Tescaro, D., Teshima, M., Testa, V., Thoudam, S., Tokanai, F., Torres, D. F., Torresi, E., Tosti, G., Townsley, C., Travnicek, P., Trichard, C., Trifoglio, M., Tsujimoto, S., Vagelli, V., Vallania, P., Valore, L., Driel, W., Eldik, C., Vandenbroucke, J., Vassiliev, V., Vecchi, M., Vercellone, S., Vergani, S., Vigorito, C., Vorobiov, S., Vrastil, M., Vázquez Acosta, M. L., Wagner, S. J., Wagner, R., Wakely, S. P., Walter, R., Ward, J. E., Watson, J. J., Weinstein, A., White, M., White, R., Wierzcholska, A., Wilcox, P., Williams, D. A., Wischnewski, R., Wojcik, P., Yamamoto, T., Yamamoto, H., Yamazaki, R., Yanagita, S., Yang, L., Yoshida, T., Yoshida, M., Yoshiike, S., Yoshikoshi, T., Zacharias, M., Zampieri, L., Zanin, R., Zavrtanik, M., Zavrtanik, D., Zdziarski, A., Zech, A., Zechlin, H., Zhdanov, V., Ziegler, A., and Zorn, J.
Subjects: High Energy Astrophysical Phenomena (astro-ph.HE), Astrophysics::High Energy Astrophysical Phenomena, FOS: Physical sciences, Astrophysics - High Energy Astrophysical Phenomena, Astrophysics::Galaxy Astrophysics
Abstract: We perform simulations for future Cherenkov Telescope Array (CTA) observations of RX~J1713.7$-$3946, a young supernova remnant (SNR) and one of the brightest sources ever discovered in very-high-energy (VHE) gamma rays. Special attention is paid to explore possible spatial (anti-)correlations of gamma rays with emission at other wavelengths, in particular X-rays and CO/H{\sc i} emission. We present a series of simulated images of RX J1713.7$-$3946 for CTA based on a set of observationally motivated models for the gamma-ray emission. In these models, VHE gamma rays produced by high-energy electrons are assumed to trace the non-thermal X-ray emission observed by {\it XMM-Newton}, whereas those originating from relativistic protons delineate the local gas distributions. The local atomic and molecular gas distributions are deduced by the NANTEN team from CO and H{\sc i} observations. Our primary goal is to show how one can distinguish the emission mechanism(s) of the gamma rays (i.e., hadronic vs leptonic, or a mixture of the two) through information provided by their spatial distribution, spectra, and time variation. This work is the first attempt to quantitatively evaluate the capabilities of CTA to achieve various proposed scientific goals by observing this important cosmic particle accelerator., Comment: 19 pages, 5 figures. Accepted for publication in ApJ
Published: 2017
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118. Prospects for Cherenkov Telescope Array Observations of the Young Supernova Remnant RX J1713.7-3946

Author: Acero, F., Aloisio, R., Amans, J., Amato, E., Antonelli, L. A., Aramo, C., Armstrong, T., Arqueros, F., Asano, K., Ashley, M., Backes, M., Balazs, C., Balzer, A., Bamba, A., Barkov, M., Barrio, J. A., Benbow, W., Bernl?Hr, K., Beshley, V., Bigongiari, C., Biland, A., Bilinsky, A., Bissaldi, E., Biteau, J., Blanch, O., Blasi, P., Blazek, J., Boisson, C., Bonanno, G., Bonardi, A., Bonavolont?, C., Bonnoli, G., Braiding, C., Brau-Nogu?, S., Bregeon, J., Brown, A. M., Bugaev, V., Bulgarelli, A., Bulik, T., Burton, M., Burtovoi, A., Busetto, G., B?Ttcher, M., Cameron, R., Capalbi, M., Caproni, A., Caraveo, P., Carosi, R., Cascone, E., Cerruti, M., Chaty, S., Chen, A., Chen, X., Chernyakova, M., Chikawa, M., Chudoba, J., Cohen-Tanugi, J., Colafrancesco, S., Conforti, V., Contreras, J. L., Costa, A., Cotter, G., Covino, S., Covone, G., Cumani, P., Cusumano, G., D?Ammando, F., D?Urso, D., Daniel, M., Dazzi, F., De Angelis, A., De Cesare, G., De Franco, A., De Frondat, F., De Gouveia Dal Pino, E. M., De Lisio, C., De Los Reyes Lopez, R., De Lotto, B., De Naurois, M., De Palma, F., Del Santo, M., Delgado, C., Della Volpe, D., Di Girolamo, T., Di Giulio, C., Di Pierro, F., Di Venere, L., Doro, M., Dournaux, J., Dumas, D., Dwarkadas, V., D?Az, C., Ebr, J., Egberts, K., Einecke, S., Els?Sser, D., Eschbach, S., Falceta-Goncalves, D., Fasola, G., Fedorova, E., Fern?Ndez-Barral, A., Ferrand, G., Fesquet, M., Fiandrini, E., Fiasson, A., Filipov?C, M. D., Fioretti, V., Font, L., Fontaine, G., Franco, F. J., Coromina, L. Freixas, Fujita, Y., Fukui, Y., Funk, S., F?Rster, A., Gadola, A., L?Pez, R. Garcia, Garczarczyk, M., Giglietto, N., Giordano, F., Giuliani, A., Glicenstein, J., Gnatyk, R., Goldoni, P., Grabarczyk, T., Graciani, R., Graham, J., Grandi, P., Granot, J., Green, A. J., Griffiths, S., Gunji, S., Hakobyan, H., Hara, S., Hassan, T., Hayashida, M., Heller, M., Helo, J. C., Hinton, J., Hnatyk, B., Huet, J., Huetten, Moritz, Humensky, T. B., Hussein, M., H?Randel, J., Ikeno, Y., Inada, T., Inome, Y., Inoue, S., Inoue, T., Inoue, Y., Ioka, K., Iori, M., Jacquemier, J., Janecek, P., Jankowsky, D., Jung, I., Kaaret, P., Katagiri, H., Kimeswenger, S., Kimura, S., Kn?Dlseder, J., Koch, B., Kocot, J., Kohri, K., Komin, N., Konno, Y., Kosack, K., Koyama, S., Kraus, M., Kubo, H., Mezek, G. Kukec, Kushida, J., Palombara, N. La, Lalik, K., Lamanna, G., Landt, H., Lapington, J., Laporte, P., Lee, S., Lees, J., Lefaucheur, J., Lenain, J.-P., Leto, G., Lindfors, E., Lohse, T., Lombardi, S., Longo, F., Lopez, M., Lucarelli, F., Luque-Escamilla, P. L., L?Pez-Coto, R., Maccarone, M. C., Maier, G., Malaguti, G., Mandat, D., Maneva, G., Mangano, S., Marcowith, A., Mart?, J., Mart?Nez, M., Mart?Nez, G., Masuda, S., Maurin, G., Maxted, N., Melioli, C., Mineo, T., Mirabal, N., Mizuno, T., Moderski, R., Mohammed, M., Montaruli, T., Moralejo, A., Mori, K., Morlino, G., Morselli, A., Moulin, E., Mukherjee, R., Mundell, C., Muraishi, H., Murase, K., Nagataki, S., Nagayoshi, T., Naito, T., Nakajima, D., Nakamori, T., Nemmen, R., Niemiec, J., Nieto, D., Nievas-Rosillo, M., Niko?Ajuk, M., Nishijima, K., Noda, K., Nogues, L., Nosek, D., Novosyadlyj, B., Nozaki, S., Ohira, Y., Ohishi, M., Ohm, S., Okumura, A., Ong, R. A., Orito, R., Orlati, A., Ostrowski, M., Oya, I., Padovani, M., Palacio, J., Palatka, M., Paredes, J. M., Pavy, S., Pe?Er, A., Persic, M., Petrucci, P., Petruk, O., Pisarski, A., Pohl, M., Porcelli, A., Prandini, E., Prast, J., Principe, G., Prouza, M., Pueschel, E., P?Hlhofer, G., Quirrenbach, A., Rameez, M., Reimer, O., Renaud, M., Rib?, M., Rico, J., Rizi, V., Rodriguez, J., Fernandez, G. Rodriguez, V?Zquez, J. J. Rodr?Guez, Romano, P., Romeo, G., Rosado, J., Rousselle, J., Rowell, G., Rudak, B., Sadeh, I., Safi-Harb, S., Saito, T., Sakaki, N., Sanchez, D., Sangiorgi, P., Sano, H., Santander, M., Sarkar, S., Sawada, M., Schioppa, E. J., Schoorlemmer, H., Schovanek, P., Schussler, F., Sergijenko, O., Servillat, M., Shalchi, A., Shellard, R. C., Siejkowski, H., Sillanp??, A., Simone, D., Sliusar, V., Sol, H., Stani?, S., Starling, R., Stawarz, ?., Stefanik, S., Stephan, M., Stolarczyk, T., Szanecki, M., Szepieniec, T., Tagliaferri, G., Tajima, H., Takahashi, M., Takeda, J., Tanaka, M., Tanaka, S., Tejedor, L. A., Telezhinsky, I., Temnikov, P., Terada, Y., Tescaro, D., Teshima, M., Testa, V., Thoudam, S., Tokanai, F., Torres, D. F., Torresi, E., Tosti, G., Townsley, C., Travnicek, P., Trichard, C., Trifoglio, M., Tsujimoto, S., Vagelli, V., Vallania, P., Valore, L., Van Driel, W., Van Eldik, C., Vandenbroucke, J., Vassiliev, V., Vecchi, M., Vercellone, S., Vergani, S., Vigorito, C., Vorobiov, S., Vrastil, M., Acosta, M. L. V?Zquez, Wagner, S. J., Wagner, R., Wakely, S. P., Walter, R., Ward, J. E., Watson, J. J., Weinstein, A., White, M., White, R., Wierzcholska, A., Wilcox, P., Williams, D. A., Wischnewski, R., Wojcik, P., Yamamoto, T., Yamamoto, H., Yamazaki, R., Yanagita, S., Yang, L., Yoshida, T., Yoshida, M., Yoshiike, S., Yoshikoshi, T., Zacharias, M., Zampieri, L., Zanin, R., Zavrtanik, M., Zavrtanik, D., Zdziarski, A., Zech, A., Zechlin, H., Zhdanov, V., Ziegler, A., and Zorn, J.
Abstract: The astrophysical journal 840(2), 74 (2017). doi:10.3847/1538-4357/aa6d67, We perform simulations for future Cherenkov Telescope Array (CTA) observations of RX J1713.7−3946, a young supernova remnant (SNR) and one of the brightest sources ever discovered in very high energy (VHE) gamma rays. Special attention is paid to exploring possible spatial (anti)correlations of gamma rays with emission at other wavelengths, in particular X-rays and CO/H i emission. We present a series of simulated images of RX J1713.7−3946 for CTA based on a set of observationally motivated models for the gamma-ray emission. In these models, VHE gamma rays produced by high-energy electrons are assumed to trace the nonthermal X-ray emission observed by XMM-Newton, whereas those originating from relativistic protons delineate the local gas distributions. The local atomic and molecular gas distributions are deduced by the NANTEN team from CO and H i observations. Our primary goal is to show how one can distinguish the emission mechanism(s) of the gamma rays (i.e., hadronic versus leptonic, or a mixture of the two) through information provided by their spatial distribution, spectra, and time variation. This work is the first attempt to quantitatively evaluate the capabilities of CTA to achieve various proposed scientific goals by observing this important cosmic particle accelerator., Published by IOP, Chicago, Ill. [u.a.]
Published: 2017
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119. Seismic response of saturated cohesionless slopes

Author: Biondi, G, Cascone, E, Maugeri, M, and Motta, E
Published: 2000
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120. Seismic stability of retaining walls with surcharge

Author: Caltabiano, S., Cascone, E., and Maugeri, M.
Published: 2000
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121. Supernova rates from the SUDARE VST-OmegaCAM search

Author: Cappellaro, E., Botticella, M. T., Pignata, G., Grado, A., Greggio, L., Limatola, L., Vaccari, M., Baruffolo, A., Benetti, S., Bufano, F., Cascone, E., Della Valle, M., Jarvis, M., Marchetti, L., Napolitano, N. R., Pastorello, A., Radovich, M., Schipani, P., Spiro, S., Tomasella, L., Turatto, M., CAPACCIOLI, MASSIMO, COVONE, GIOVANNI, DE CICCO, DEMETRA, FALOCCO, SERENA, PAOLILLO, MAURIZIO, Cappellaro, E., Botticella, M. T., Pignata, G., Grado, A., Greggio, L., Limatola, L., Vaccari, M., Baruffolo, A., Benetti, S., Bufano, F., Capaccioli, Massimo, Cascone, E., Covone, Giovanni, DE CICCO, Demetra, Falocco, Serena, Della Valle, M., Jarvis, M., Marchetti, L., Napolitano, N. R., Paolillo, Maurizio, Pastorello, A., Radovich, M., Schipani, P., Spiro, S., Tomasella, L., and Turatto, M.
Subjects: supernovae: general, galaxies: star formation, Galaxy: stellar content, surveys
Abstract: We describe the observing strategy, data reduction tools and early results of a supernova (SN) search project, named SUDARE, conducted with the ESO VST telescope aimed at measuring the rate of the different types of SNe in the redshift range 0.2
Published: 2015

122. High-contrast study of the candidate planets and protoplanetary disk around HD 100546

Author: Sissa, E., primary, Gratton, R., additional, Garufi, A., additional, Rigliaco, E., additional, Zurlo, A., additional, Mesa, D., additional, Langlois, M., additional, de Boer, J., additional, Desidera, S., additional, Ginski, C., additional, Lagrange, A.-M., additional, Maire, A.-L., additional, Vigan, A., additional, Dima, M., additional, Antichi, J., additional, Baruffolo, A., additional, Bazzon, A., additional, Benisty, M., additional, Beuzit, J.-L., additional, Biller, B., additional, Boccaletti, A., additional, Bonavita, M., additional, Bonnefoy, M., additional, Brandner, W., additional, Bruno, P., additional, Buenzli, E., additional, Cascone, E., additional, Chauvin, G., additional, Cheetham, A., additional, Claudi, R. U., additional, Cudel, M., additional, De Caprio, V., additional, Dominik, C., additional, Fantinel, D., additional, Farisato, G., additional, Feldt, M., additional, Fontanive, C., additional, Galicher, R., additional, Giro, E., additional, Hagelberg, J., additional, Incorvaia, S., additional, Janson, M., additional, Kasper, M., additional, Keppler, M., additional, Kopytova, T., additional, Lagadec, E., additional, Lannier, J., additional, Lazzoni, C., additional, LeCoroller, H., additional, Lessio, L., additional, Ligi, R., additional, Marzari, F., additional, Menard, F., additional, Meyer, M. R., additional, Mouillet, D., additional, Peretti, S., additional, Perrot, C., additional, Potiron, P. J., additional, Rouan, D., additional, Salasnich, B., additional, Salter, G., additional, Samland, M., additional, Schmidt, T., additional, Scuderi, S., additional, and Wildi, F., additional
Published: 2018
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123. Discovery of a planetary-mass companion within the gap of the transition disk around PDS 70

Author: Keppler, M., primary, Benisty, M., additional, Müller, A., additional, Henning, Th., additional, van Boekel, R., additional, Cantalloube, F., additional, Ginski, C., additional, van Holstein, R. G., additional, Maire, A.-L., additional, Pohl, A., additional, Samland, M., additional, Avenhaus, H., additional, Baudino, J.-L., additional, Boccaletti, A., additional, de Boer, J., additional, Bonnefoy, M., additional, Chauvin, G., additional, Desidera, S., additional, Langlois, M., additional, Lazzoni, C., additional, Marleau, G.-D., additional, Mordasini, C., additional, Pawellek, N., additional, Stolker, T., additional, Vigan, A., additional, Zurlo, A., additional, Birnstiel, T., additional, Brandner, W., additional, Feldt, M., additional, Flock, M., additional, Girard, J., additional, Gratton, R., additional, Hagelberg, J., additional, Isella, A., additional, Janson, M., additional, Juhasz, A., additional, Kemmer, J., additional, Kral, Q., additional, Lagrange, A.-M., additional, Launhardt, R., additional, Matter, A., additional, Ménard, F., additional, Milli, J., additional, Mollière, P., additional, Olofsson, J., additional, Pérez, L., additional, Pinilla, P., additional, Pinte, C., additional, Quanz, S. P., additional, Schmidt, T., additional, Udry, S., additional, Wahhaj, Z., additional, Williams, J. P., additional, Buenzli, E., additional, Cudel, M., additional, Dominik, C., additional, Galicher, R., additional, Kasper, M., additional, Lannier, J., additional, Mesa, D., additional, Mouillet, D., additional, Peretti, S., additional, Perrot, C., additional, Salter, G., additional, Sissa, E., additional, Wildi, F., additional, Abe, L., additional, Antichi, J., additional, Augereau, J.-C., additional, Baruffolo, A., additional, Baudoz, P., additional, Bazzon, A., additional, Beuzit, J.-L., additional, Blanchard, P., additional, Brems, S. S., additional, Buey, T., additional, De Caprio, V., additional, Carbillet, M., additional, Carle, M., additional, Cascone, E., additional, Cheetham, A., additional, Claudi, R., additional, Costille, A., additional, Delboulbé, A., additional, Dohlen, K., additional, Fantinel, D., additional, Feautrier, P., additional, Fusco, T., additional, Giro, E., additional, Gluck, L., additional, Gry, C., additional, Hubin, N., additional, Hugot, E., additional, Jaquet, M., additional, Le Mignant, D., additional, Llored, M., additional, Madec, F., additional, Magnard, Y., additional, Martinez, P., additional, Maurel, D., additional, Meyer, M., additional, Möller-Nilsson, O., additional, Moulin, T., additional, Mugnier, L., additional, Origné, A., additional, Pavlov, A., additional, Perret, D., additional, Petit, C., additional, Pragt, J., additional, Puget, P., additional, Rabou, P., additional, Ramos, J., additional, Rigal, F., additional, Rochat, S., additional, Roelfsema, R., additional, Rousset, G., additional, Roux, A., additional, Salasnich, B., additional, Sauvage, J.-F., additional, Sevin, A., additional, Soenke, C., additional, Stadler, E., additional, Suarez, M., additional, Turatto, M., additional, and Weber, L., additional
Published: 2018
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124. Discovery of a brown dwarf companion to the star HIP 64892

Author: Cheetham, A., primary, Bonnefoy, M., additional, Desidera, S., additional, Langlois, M., additional, Vigan, A., additional, Schmidt, T., additional, Olofsson, J., additional, Chauvin, G., additional, Klahr, H., additional, Gratton, R., additional, D’Orazi, V., additional, Henning, T., additional, Janson, M., additional, Biller, B., additional, Peretti, S., additional, Hagelberg, J., additional, Ségransan, D., additional, Udry, S., additional, Mesa, D., additional, Sissa, E., additional, Kral, Q., additional, Schlieder, J., additional, Maire, A.-L., additional, Mordasini, C., additional, Menard, F., additional, Zurlo, A., additional, Beuzit, J.-L., additional, Feldt, M., additional, Mouillet, D., additional, Meyer, M., additional, Lagrange, A.-M., additional, Boccaletti, A., additional, Keppler, M., additional, Kopytova, T., additional, Ligi, R., additional, Rouan, D., additional, Le Coroller, H., additional, Dominik, C., additional, Lagadec, E., additional, Turatto, M., additional, Abe, L., additional, Antichi, J., additional, Baruffolo, A., additional, Baudoz, P., additional, Blanchard, P., additional, Buey, T., additional, Carbillet, M., additional, Carle, M., additional, Cascone, E., additional, Claudi, R., additional, Costille, A., additional, Delboulbé, A., additional, De Caprio, V., additional, Dohlen, K., additional, Fantinel, D., additional, Feautrier, P., additional, Fusco, T., additional, Giro, E., additional, Gluck, L., additional, Hubin, N., additional, Hugot, E., additional, Jaquet, M., additional, Kasper, M., additional, Llored, M., additional, Madec, F., additional, Magnard, Y., additional, Martinez, P., additional, Maurel, D., additional, Le Mignant, D., additional, Möller-Nilsson, O., additional, Moulin, T., additional, Origné, A., additional, Pavlov, A., additional, Perret, D., additional, Petit, C., additional, Pragt, J., additional, Puget, P., additional, Rabou, P., additional, Ramos, J., additional, Rigal, F., additional, Rochat, S., additional, Roelfsema, R., additional, Rousset, G., additional, Roux, A., additional, Salasnich, B., additional, Sauvage, J.-F., additional, Sevin, A., additional, Soenke, C., additional, Stadler, E., additional, Suarez, M., additional, Weber, L., additional, and Wildi, F., additional
Published: 2018
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125. First scattered light detection of a nearly edge-on transition disk around the T Tauri star RY Lupi

Author: Langlois, M., primary, Pohl, A., additional, Lagrange, A.-M., additional, Maire, A.- L., additional, Mesa, D., additional, Boccaletti, A., additional, Gratton, R., additional, Denneulin, L., additional, Klahr, H., additional, Vigan, A., additional, Benisty, M., additional, Dominik, C., additional, Bonnefoy, M., additional, Menard, F., additional, Avenhaus, H., additional, Cheetham, A., additional, Van Boekel, R., additional, de Boer, J., additional, Chauvin, G., additional, Desidera, S., additional, Feldt, M., additional, Galicher, R., additional, Ginski, C., additional, Girard, J. H., additional, Henning, T., additional, Janson, M., additional, Kopytova, T., additional, Kral, Q., additional, Ligi, R., additional, Messina, S., additional, Peretti, S., additional, Pinte, C., additional, Sissa, E., additional, Stolker, T., additional, Zurlo, A., additional, Magnard, Y., additional, Blanchard, P., additional, Buey, T., additional, Suarez, M., additional, Cascone, E., additional, Moller-Nilsson, O., additional, Weber, L., additional, Petit, C., additional, and Pragt, J., additional
Published: 2018
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126. New spectro-photometric characterization of the substellar object HR 2562 B using SPHERE

Author: Mesa, D., primary, Baudino, J.-L., additional, Charnay, B., additional, D’Orazi, V., additional, Desidera, S., additional, Boccaletti, A., additional, Gratton, R., additional, Bonnefoy, M., additional, Delorme, P., additional, Langlois, M., additional, Vigan, A., additional, Zurlo, A., additional, Maire, A.-L., additional, Janson, M., additional, Antichi, J., additional, Baruffolo, A., additional, Bruno, P., additional, Cascone, E., additional, Chauvin, G., additional, Claudi, R.U., additional, De Caprio, V., additional, Fantinel, D., additional, Farisato, G., additional, Feldt, M., additional, Giro, E., additional, Hagelberg, J., additional, Incorvaia, S., additional, Lagadec, E., additional, Lagrange, A.-M., additional, Lazzoni, C., additional, Lessio, L., additional, Salasnich, B., additional, Scuderi, S., additional, Sissa, E., additional, and Turatto, M., additional
Published: 2018
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127. Dynamical models to explain observations with SPHERE in planetary systems with double debris belts

Author: Lazzoni, C., primary, Desidera, S., additional, Marzari, F., additional, Boccaletti, A., additional, Langlois, M., additional, Mesa, D., additional, Gratton, R., additional, Kral, Q., additional, Pawellek, N., additional, Olofsson, J., additional, Bonnefoy, M., additional, Chauvin, G., additional, Lagrange, A. M., additional, Vigan, A., additional, Sissa, E., additional, Antichi, J., additional, Avenhaus, H., additional, Baruffolo, A., additional, Baudino, J. L., additional, Bazzon, A., additional, Beuzit, J. L., additional, Biller, B., additional, Bonavita, M., additional, Brandner, W., additional, Bruno, P., additional, Buenzli, E., additional, Cantalloube, F., additional, Cascone, E., additional, Cheetham, A., additional, Claudi, R. U., additional, Cudel, M., additional, Daemgen, S., additional, De Caprio, V., additional, Delorme, P., additional, Fantinel, D., additional, Farisato, G., additional, Feldt, M., additional, Galicher, R., additional, Ginski, C., additional, Girard, J., additional, Giro, E., additional, Janson, M., additional, Hagelberg, J., additional, Henning, T., additional, Incorvaia, S., additional, Kasper, M., additional, Kopytova, T., additional, LeCoroller, H., additional, Lessio, L., additional, Ligi, R., additional, Maire, A. L., additional, Ménard, F., additional, Meyer, M., additional, Milli, J., additional, Mouillet, D., additional, Peretti, S., additional, Perrot, C., additional, Rouan, D., additional, Samland, M., additional, Salasnich, B., additional, Salter, G., additional, Schmidt, T., additional, Scuderi, S., additional, Sezestre, E., additional, Turatto, M., additional, Udry, S., additional, Wildi, F., additional, and Zurlo, A., additional
Published: 2018
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128. Orbiting a binary

Author: Bonavita, M., primary, D’Orazi, V., additional, Mesa, D., additional, Fontanive, C., additional, Desidera, S., additional, Messina, S., additional, Daemgen, S., additional, Gratton, R., additional, Vigan, A., additional, Bonnefoy, M., additional, Zurlo, A., additional, Antichi, J., additional, Avenhaus, H., additional, Baruffolo, A., additional, Baudino, J. L., additional, Beuzit, J. L., additional, Boccaletti, A., additional, Bruno, P., additional, Buey, T., additional, Carbillet, M., additional, Cascone, E., additional, Chauvin, G., additional, Claudi, R. U., additional, De Caprio, V., additional, Fantinel, D., additional, Farisato, G., additional, Feldt, M., additional, Galicher, R., additional, Giro, E., additional, Gry, C., additional, Hagelberg, J., additional, Incorvaia, S., additional, Janson, M., additional, Jaquet, M., additional, Lagrange, A. M., additional, Langlois, M., additional, Lannier, J., additional, Le Coroller, H., additional, Lessio, L., additional, Ligi, R., additional, Maire, A. L., additional, Meyer, M., additional, Menard, F., additional, Perrot, C., additional, Peretti, S., additional, Petit, C., additional, Ramos, J., additional, Roux, A., additional, Salasnich, B., additional, Salter, G., additional, Samland, M., additional, Scuderi, S., additional, Schlieder, J., additional, Surez, M., additional, Turatto, M., additional, and Weber, L., additional
Published: 2017
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129. Discovery of a warm, dusty giant planet around HIP 65426

Author: Chauvin, G., Desidera, S., Lagrange, A. -M., Vigan, A., Gratton, R., Langlois, M., Bonnefoy, M., Beuzit, J. -L., Feldt, M., Mouillet, D., Meyer, M., Cheetham, A., Biller, B., Boccaletti, A., D'Orazi, V., Galicher, R., Hagelberg, J., Maire, A. -L., Mesa, D., Olofsson, J., Samland, M., Schmidt, T. O. B., Sissa, E., Bonavita, M., Charnay, B., Cudel, M., Daemgen, S., Delorme, P., Janin-Potiron, P., Janson, M., Keppler, M., Le, Coroller, H., Ligi, R., Marleau, G. D., Messina, S., Mollière, P., Mordasini, C., Müller, A., Peretti, S., Perrot, C., Rodet, L., Rouan, D., Zurlo, A., Dominik, C., Henning, T., Menard, F., Schmid, H. -M., Turatto, M., Udry, S., Vakili, F., Abe, L., Antichi, J., Baruffolo, A., Baudoz, P., Baudrand, J., Blanchard, P., Bazzon, A., Buey, T., Carbillet, M., Carle, M., Charton, J., Cascone, E., Claudi, R., Costille, A., Deboulbe, A., De, Caprio, V., Dohlen, K., Fantinel, D., Feautrier, P., Fusco, T., Gigan, P., Giro, E., Gisler, D., Gluck, L., Hubin, N., Hugot, E., Jaquet, M., Kasper, M., Madec, F., Magnard, Y., Martinez, P., Maurel, D., Le, Mignant, D., Möller-Nilsson, O., Llored, M., Moulin, T., Origné, A., Pavlov, A., Perret, D., Petit, C., Pragt, J., Puget, P., Rabou, P., Ramos, J., Rigal, R., Rochat, S., Roelfsema, R., Rousset, G., Roux, A., Salasnich, B., Sauvage, J. -F., Sevin, A., Soenke, C., Stadler, E., Suarez, M., Weber, L., Wildi, F., Antoniucci, S., Augereau, J. -C., Baudino, J. -L., Brandner, W., Engler, N., Girard, J., Gry, C., Kral, Q., Kopytova, T., Lagadec, E., Milli, J., Moutou, C., Schlieder, J., Szulágyi, J., Thalmann, C., Wahhaj, Z., Chauvin, G., Desidera, S., Lagrange, A. -M., Vigan, A., Gratton, R., Langlois, M., Bonnefoy, M., Beuzit, J. -L., Feldt, M., Mouillet, D., Meyer, M., Cheetham, A., Biller, B., Boccaletti, A., D'Orazi, V., Galicher, R., Hagelberg, J., Maire, A. -L., Mesa, D., Olofsson, J., Samland, M., Schmidt, T. O. B., Sissa, E., Bonavita, M., Charnay, B., Cudel, M., Daemgen, S., Delorme, P., Janin-Potiron, P., Janson, M., Keppler, M., Le, Coroller, H., Ligi, R., Marleau, G. D., Messina, S., Mollière, P., Mordasini, C., Müller, A., Peretti, S., Perrot, C., Rodet, L., Rouan, D., Zurlo, A., Dominik, C., Henning, T., Menard, F., Schmid, H. -M., Turatto, M., Udry, S., Vakili, F., Abe, L., Antichi, J., Baruffolo, A., Baudoz, P., Baudrand, J., Blanchard, P., Bazzon, A., Buey, T., Carbillet, M., Carle, M., Charton, J., Cascone, E., Claudi, R., Costille, A., Deboulbe, A., De, Caprio, V., Dohlen, K., Fantinel, D., Feautrier, P., Fusco, T., Gigan, P., Giro, E., Gisler, D., Gluck, L., Hubin, N., Hugot, E., Jaquet, M., Kasper, M., Madec, F., Magnard, Y., Martinez, P., Maurel, D., Le, Mignant, D., Möller-Nilsson, O., Llored, M., Moulin, T., Origné, A., Pavlov, A., Perret, D., Petit, C., Pragt, J., Puget, P., Rabou, P., Ramos, J., Rigal, R., Rochat, S., Roelfsema, R., Rousset, G., Roux, A., Salasnich, B., Sauvage, J. -F., Sevin, A., Soenke, C., Stadler, E., Suarez, M., Weber, L., Wildi, F., Antoniucci, S., Augereau, J. -C., Baudino, J. -L., Brandner, W., Engler, N., Girard, J., Gry, C., Kral, Q., Kopytova, T., Lagadec, E., Milli, J., Moutou, C., Schlieder, J., Szulágyi, J., Thalmann, C., and Wahhaj, Z.
Abstract: Aims. The SHINE program is a high-contrast near-infrared survey of 600 young, nearby stars aimed at searching for and characterizing new planetary systems using VLT/SPHERE's unprecedented high-contrast and high-angular-resolution imaging capabilities. It is also intended to place statistical constraints on the rate, mass and orbital distributions of the giant planet population at large orbits as a function of the stellar host mass and age to test planet-formation theories. Methods. We used the IRDIS dual-band imager and the IFS integral field spectrograph of SPHERE to acquire high-contrast coronagraphic differential near-infrared images and spectra of the young A2 star HIP 65426. It is a member of the ~17 Myr old Lower Centaurus-Crux association. Results. At a separation of 830 mas (92 au projected) from the star, we detect a faint red companion. Multi-epoch observations confirm that it shares common proper motion with HIP 65426. Spectro-photometric measurements extracted with IFS and IRDIS between 0.95 and 2.2 μm indicate a warm, dusty atmosphere characteristic of young low-surface-gravity L5-L7 dwarfs. Hot-start evolutionary models predict a luminosity consistent with a 6-12 MJup, Teff = 1300-1600 K and R = 1.5 ± 0.1 RJup giant planet. Finally, the comparison with Exo-REM and PHOENIX BT-Settl synthetic atmosphere models gives consistent effective temperatures but with slightly higher surface gravity solutions of log (g) = 4.0-5.0 with smaller radii (1.0-1.3 RJup). Conclusions. Given its physical and spectral properties, HIP 65426 b occupies a rather unique placement in terms of age, mass, and spectral-type among the currently known imaged planets. It represents a particularly interesting case to study the presence of clouds as a function of particle size, composition, and location in the atmosphere, to search for signatures of non-equilibrium chemistry, and finally to test the theory of planet formation and evolution. © ESO, 2017.
Published: 2017

130. Supernova rates from the SUDARE VST-omegacam search II. Rates in a galaxy sample

Author: Botticella, M. T., Cappellaro, E., Greggio, L., Pignata, G., Della Valle, M., Grado, A., Limatola, L., Baruffolo, A., Benetti, S., Bufano, F., Capaccioli, M., Cascone, E., Covone, G., De Cicco, D., Falocco, Serena, Haeussler, B., Harutyunyan, V., Jarvis, M., Marchetti, L., Napolitano, N. R., Paolillo, M., Pastorello, A., Radovich, M., Schipani, P., Tomasella, L., Turatto, M., Vaccari, M., Botticella, M. T., Cappellaro, E., Greggio, L., Pignata, G., Della Valle, M., Grado, A., Limatola, L., Baruffolo, A., Benetti, S., Bufano, F., Capaccioli, M., Cascone, E., Covone, G., De Cicco, D., Falocco, Serena, Haeussler, B., Harutyunyan, V., Jarvis, M., Marchetti, L., Napolitano, N. R., Paolillo, M., Pastorello, A., Radovich, M., Schipani, P., Tomasella, L., Turatto, M., and Vaccari, M.
Abstract: Aims. This is the second paper of a series in which we present measurements of the supernova (SN) rates from the SUDARE survey. The aim of this survey is to constrain the core collapse (CC) and Type Ia SN progenitors by analysing the dependence of their explosion rate on the properties of the parent stellar population averaging over a population of galaxies with different ages in a cosmic volume and in a galaxy sample. In this paper, we study the trend of the SN rates with the intrinsic colours, the star formation activity and the masses of the parent galaxies. To constrain the SN progenitors we compare the observed rates with model predictions assuming four progenitor models for SNe Ia with different distribution functions of the time intervals between the formation of the progenitor and the explosion, and a mass range of 8-40 M for CC SN progenitors. Methods. We considered a galaxy sample of approximately 130 000 galaxies and a SN sample of approximately 50 events. The wealth of photometric information for our galaxy sample allows us to apply the spectral energy distribution (SED) fitting technique to estimate the intrinsic rest frame colours, the stellar mass and star formation rate (SFR) for each galaxy in the sample. The galaxies have been separated into star-forming and quiescent galaxies, exploiting both the rest frame U-V vs. V-J colour-colour diagram and the best fit values of the specific star formation rate (sSFR) from the SED fitting. Results. We found that the SN Ia rate per unit mass is higher by a factor of six in the star-forming galaxies with respect to the passive galaxies, identified as such both on the U-V vs. V-J colour-colour diagram and for their sSFR. The SN Ia rate per unit mass is also higher in the less massive galaxies that are also younger. These results suggest a distribution of the delay times (DTD) less populated at long delay times than at short delays. The CC SN rate per unit mass is proportional to both the sSFR and the galaxy mass, QC 20170607
Published: 2017
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131. Upper limits for mass and radius of objects around Proxima Cen from SPHERE/VLT

Author: Mesa, D., Zurlo, A., Milli, J., Gratton, R., Desidera, S., Langlois, M., Vigan, A., Bonavita, Mariangela, Antichi, J., Avenhaus, H., Baruffolo, A., Biller, B., Boccaletti, A., Bruno, P., Cascone, E., Chauvin, G., Claudi, R. U., De Caprio, V., Fantinel, D., Farisato, G., Girard, J., Giro, E., Hagelberg, Janis, Incorvaia, S., Janson, Markus, Kral, Q., Lagadec, E., Lagrange, A. -M., Lessio, L., Meyer, M., Peretti, S., Perrot, C., Salasnich, B., Schlieder, J., Schmid, H. -M., Scuderi, S., Sissa, E., Thalmann, C., Turatto, M., Mesa, D., Zurlo, A., Milli, J., Gratton, R., Desidera, S., Langlois, M., Vigan, A., Bonavita, Mariangela, Antichi, J., Avenhaus, H., Baruffolo, A., Biller, B., Boccaletti, A., Bruno, P., Cascone, E., Chauvin, G., Claudi, R. U., De Caprio, V., Fantinel, D., Farisato, G., Girard, J., Giro, E., Hagelberg, Janis, Incorvaia, S., Janson, Markus, Kral, Q., Lagadec, E., Lagrange, A. -M., Lessio, L., Meyer, M., Peretti, S., Perrot, C., Salasnich, B., Schlieder, J., Schmid, H. -M., Scuderi, S., Sissa, E., Thalmann, C., and Turatto, M.
Abstract: The recent discovery of an earth-like planet around Proxima Centauri has drawn much attention to this star and its environment. We performed a series of observations of Proxima Centauri using Spectro-Polarimetric High-contrast Exoplanet REsearch (SPHERE), the planet-finder instrument installed at the European Southern Observatory (ESO) Very Large Telescope (VLT) UT3, using its near-infrared modules, InfraRed Dual-band Imager and Spectrograph (IRDIS) and IFS. No planet was detected directly, but we set upper limits on the mass up to 7 au by exploiting the AMES-COND models. Our IFS observations reveal that no planet more massive than similar to 6-7 M-Jup can be present within 1 au. The dual-band imaging camera IRDIS also enables us to probe larger separations than other techniques such as radial velocity or astrometry. We obtained mass limits of the order of 4 M-Jup at separations of 2 au or larger, representing the most stringent mass limits at separations larger than 5 au available at the moment. We also made an attempt to estimate the radius of possible planets around Proxima using the reflected light. Since the residual noise for the observations is dominated by photon noise and thermal background, longer exposures in good observing conditions could improve the achievable contrast limit further.
Published: 2017
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132. First light of the VLT planet finder SPHERE. III. New spectrophotometry and astrometry of the HR 8799 exoplanetary system

Author: Zurlo, A., Vigan, Arthur, Galicher, R., Maire, A.L., Mesa, D., Gratton, R., Chauvin, G., Kasper, M., Moutou, C., Bonnefoy, M., Desidera, S., Abe, L., Apai, D., Baruffolo, A., Baudoz, P., Baudrand, J., Beuzit, J.L., Blancard, P., Boccaletti, A., Cantalloube, F., Carle, M., Cascone, E., Charton, P., Claudi, R.U., Costille, A., De Caprio, V., Dohlen, K., Dominik, C., Fantinel, D., Feautrier, P., Feldt, M., Fusco, T., Gigan, P., Girard, J.H., Gisler, D., Gluck, L., Gry, C., Henning, T., Hugot, E., Janson, M., Jaquet, M., Lagrange, A.M., Langlois, M., Llored, M., Madec, F., Magnard, Y., Martinez, P., Maurel, D., Mawet, D., Meyer, M.R., Milli, J., Moeller-Nilsson, O., Mouillet, D., Origné, A., Pavlov, A., Petit, C., Puget, P., Quanz, S.P., Rabou, P., Ramos, J., Rousset, G., Roux, A., Salasnich, B., Salter, G., Sauvage, J.F., Schmid, H.M., Soenke, C., Stadler, E., Suarez, M., Turatto, M., Udry, S., F., Vakili, Wahhaj, Z., Wildi, F., Antichi, J., Universidad Diego Portales [Santiago] (UDP), Departamento de Astronomía, Universidad de Chile = University of Chile [Santiago] (UCHILE), 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), INAF - Osservatorio Astronomico di Padova (OAPD), Istituto Nazionale di Astrofisica (INAF), European Southern Observatory, European Southern Observatory (ESO), Laboratoire d'études spatiales et d'instrumentation en astrophysique (LESIA), Centre National de la Recherche Scientifique (CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Pierre et Marie Curie - Paris 6 (UPMC), Institut de Planétologie et d'Astrophysique de Grenoble (IPAG), Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Observatoire des Sciences de l'Univers de Grenoble (OSUG ), Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut national des sciences de l'Univers (INSU - CNRS)-Institut national de recherche en sciences et technologies pour l'environnement et l'agriculture (IRSTEA)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes [2016-2019] (UGA [2016-2019])-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut national de recherche en sciences et technologies pour l'environnement et l'agriculture (IRSTEA)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes [2016-2019] (UGA [2016-2019]), ESO, Physics Department [Garching], Technische Universität Munchen - Université Technique de Munich [Munich, Allemagne] (TUM)-Technische Universität Munchen - Université Technique de Munich [Munich, Allemagne] (TUM), Joseph Louis LAGRANGE (LAGRANGE), 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), Steward Observatory (STEWARD OBSERVATORY), University of Arizona, Lunar and Planetary Laboratory [Tucson] (LPL), ONERA - The French Aerospace Lab [Châtillon], ONERA-Université Paris Saclay (COmUE), Anton Pannekoek Institute for Astronomy, University of Amsterdam [Amsterdam] (UvA), Max-Planck-Institut für Astronomie (MPIA), Max-Planck-Gesellschaft, Kiepenheuer-Institut für Sonnenphysik (KIS), AlbaNova University Center (ALBANOVA), Stockholm University, Centre de Recherche Astrophysique de Lyon (CRAL), École normale supérieure - Lyon (ENS Lyon)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS), California Institute of Technology (CALTECH), Institute of Astronomy [ETH Zürich], Department of Physics [ETH Zürich] (D-PHYS), Eidgenössische Technische Hochschule - Swiss Federal Institute of Technology [Zürich] (ETH Zürich)- Eidgenössische Technische Hochschule - Swiss Federal Institute of Technology [Zürich] (ETH Zürich), Observatoire Astronomique de l'Université de Genève (ObsGE), Université de Genève (UNIGE), Universidad de Chile, 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), 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), Centre National d'Études Spatiales [Toulouse] (CNES)-Université Grenoble Alpes (UGA)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire des Sciences de l'Univers de Grenoble (OSUG), Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP)-Institut national de recherche en sciences et technologies pour l'environnement et l'agriculture (IRSTEA)-Université Joseph Fourier - Grenoble 1 (UJF)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP)-Institut national de recherche en sciences et technologies pour l'environnement et l'agriculture (IRSTEA)-Université Joseph Fourier - Grenoble 1 (UJF)-Centre National de la Recherche Scientifique (CNRS), Technical University of Munich (TUM)-Technical University of Munich (TUM), Université Nice Sophia Antipolis (... - 2019) (UNS), Université Côte d'Azur (UCA)-Université Côte d'Azur (UCA)-Observatoire de la Côte d'Azur, Université Côte d'Azur (UCA)-Centre National de la Recherche Scientifique (CNRS), ONERA, Université de Lyon-Université de Lyon-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Eidgenössische Technische Hochschule - Swiss Federal Institute of Technology in Zürich [Zürich] (ETH Zürich)-Eidgenössische Technische Hochschule - Swiss Federal Institute of Technology in Zürich [Zürich] (ETH Zürich), 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), 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), École normale supérieure de Lyon (ENS de Lyon)-Université Claude Bernard Lyon 1 (UCBL), and Université de Genève = University of Geneva (UNIGE)
Subjects: TRAITEMENT IMAGE, [SPI.OPTI]Engineering Sciences [physics]/Optics / Photonic, SPECTROSCOPIE, ANALYSE DONNEES, ASTROMETRIE, Astrophysics::Earth and Planetary Astrophysics, Astrophysics::Galaxy Astrophysics, HAUTE RESOLUTION, EXOPLANETE
Abstract: International audience; Context. The planetary system discovered around the young A-type HR 8799 provides a unique laboratory to: a) test planet formation theories; b) probe the diversity of system architectures at these separations, and c) perform comparative (exo)planetology.Aims. We present and exploit new near-infrared images and integral-field spectra of the four gas giants surrounding HR 8799 obtained with SPHERE, the new planet finder instrument at the Very Large Telescope, during the commissioning and science verification phase of the instrument (July–December 2014). With these new data, we contribute to completing the spectral energy distribution (SED) of these bodies in the 1.0–2.5 μm range. We also provide new astrometric data, in particular for planet e, to further constrain the orbits.Methods. We used the infrared dual-band imager and spectrograph (IRDIS) subsystem to obtain pupil-stabilized, dual-band H2H3 (1.593 μm, 1.667 μm), K1K2 (2.110 μm, 2.251 μm), and broadband J (1.245 μm) images of the four planets. IRDIS was operated in parallel with the integral field spectrograph (IFS) of SPHERE to collect low-resolution (R ~ 30), near-infrared (0.94–1.64 μm) spectra of the two innermost planets HR 8799 d and e. The data were reduced with dedicated algorithms, such as the Karhunen-Loève image projection (KLIP), to reveal the planets. We used the so-called negative planets injection technique to extract their photometry, spectra, and measure their positions. We illustrate the astrometric performance of SPHERE through sample orbital fits compatible with SPHERE and literature data.Results. We demonstrated the ability of SPHERE to detect and characterize planets in this kind of systems, providing spectra and photometry of its components. The spectra improve upon the signal-to-noise ratio of previously obtained data and increase the spectral coverage down to the Y band. In addition, we provide the first detection of planet e in the J band. Astrometric positions for planets HR 8799 bcde are reported for the epochs of July, August, and December 2014. We measured the photometric values in J, H2H3, K1K2 bands for the four planets with a mean accuracy of 0.13 mag. We found upper limit constraints on the mass of a possible planet f of 3–7 MJup . Our new measurements are more consistent with the two inner planets d and e being in a 2d:1e or 3d:2e resonance. The spectra of HR 8799 d and e are well matched by those of L6-8 field dwarfs. However, the SEDs of these objects are redder than field L dwarfs longward of 1.6 μm.
Published: 2016

133. Discovery of a warm, dusty giant planet around HIP 65426

Author: Chauvin, G., primary, Desidera, S., additional, Lagrange, A.-M., additional, Vigan, A., additional, Gratton, R., additional, Langlois, M., additional, Bonnefoy, M., additional, Beuzit, J.-L., additional, Feldt, M., additional, Mouillet, D., additional, Meyer, M., additional, Cheetham, A., additional, Biller, B., additional, Boccaletti, A., additional, D’Orazi, V., additional, Galicher, R., additional, Hagelberg, J., additional, Maire, A.-L., additional, Mesa, D., additional, Olofsson, J., additional, Samland, M., additional, Schmidt, T. O. B., additional, Sissa, E., additional, Bonavita, M., additional, Charnay, B., additional, Cudel, M., additional, Daemgen, S., additional, Delorme, P., additional, Janin-Potiron, P., additional, Janson, M., additional, Keppler, M., additional, Le Coroller, H., additional, Ligi, R., additional, Marleau, G. D., additional, Messina, S., additional, Mollière, P., additional, Mordasini, C., additional, Müller, A., additional, Peretti, S., additional, Perrot, C., additional, Rodet, L., additional, Rouan, D., additional, Zurlo, A., additional, Dominik, C., additional, Henning, T., additional, Menard, F., additional, Schmid, H.-M., additional, Turatto, M., additional, Udry, S., additional, Vakili, F., additional, Abe, L., additional, Antichi, J., additional, Baruffolo, A., additional, Baudoz, P., additional, Baudrand, J., additional, Blanchard, P., additional, Bazzon, A., additional, Buey, T., additional, Carbillet, M., additional, Carle, M., additional, Charton, J., additional, Cascone, E., additional, Claudi, R., additional, Costille, A., additional, Deboulbe, A., additional, De Caprio, V., additional, Dohlen, K., additional, Fantinel, D., additional, Feautrier, P., additional, Fusco, T., additional, Gigan, P., additional, Giro, E., additional, Gisler, D., additional, Gluck, L., additional, Hubin, N., additional, Hugot, E., additional, Jaquet, M., additional, Kasper, M., additional, Madec, F., additional, Magnard, Y., additional, Martinez, P., additional, Maurel, D., additional, Le Mignant, D., additional, Möller-Nilsson, O., additional, Llored, M., additional, Moulin, T., additional, Origné, A., additional, Pavlov, A., additional, Perret, D., additional, Petit, C., additional, Pragt, J., additional, Puget, P., additional, Rabou, P., additional, Ramos, J., additional, Rigal, R., additional, Rochat, S., additional, Roelfsema, R., additional, Rousset, G., additional, Roux, A., additional, Salasnich, B., additional, Sauvage, J.-F., additional, Sevin, A., additional, Soenke, C., additional, Stadler, E., additional, Suarez, M., additional, Weber, L., additional, Wildi, F., additional, Antoniucci, S., additional, Augereau, J.-C., additional, Baudino, J.-L., additional, Brandner, W., additional, Engler, N., additional, Girard, J., additional, Gry, C., additional, Kral, Q., additional, Kopytova, T., additional, Lagadec, E., additional, Milli, J., additional, Moutou, C., additional, Schlieder, J., additional, Szulágyi, J., additional, Thalmann, C., additional, and Wahhaj, Z., additional
Published: 2017
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134. Prospects for Cherenkov Telescope Array Observations of the Young Supernova Remnant RX J1713.7−3946

Author: Acero, F., primary, Aloisio, R., additional, Amans, J., additional, Amato, E., additional, Antonelli, L. A., additional, Aramo, C., additional, Armstrong, T., additional, Arqueros, F., additional, Asano, K., additional, Ashley, M., additional, Backes, M., additional, Balazs, C., additional, Balzer, A., additional, Bamba, A., additional, Barkov, M., additional, Barrio, J. A., additional, Benbow, W., additional, Bernlöhr, K., additional, Beshley, V., additional, Bigongiari, C., additional, Biland, A., additional, Bilinsky, A., additional, Bissaldi, E., additional, Biteau, J., additional, Blanch, O., additional, Blasi, P., additional, Blazek, J., additional, Boisson, C., additional, Bonanno, G., additional, Bonardi, A., additional, Bonavolontà, C., additional, Bonnoli, G., additional, Braiding, C., additional, Brau-Nogué, S., additional, Bregeon, J., additional, Brown, A. M., additional, Bugaev, V., additional, Bulgarelli, A., additional, Bulik, T., additional, Burton, M., additional, Burtovoi, A., additional, Busetto, G., additional, Böttcher, M., additional, Cameron, R., additional, Capalbi, M., additional, Caproni, A., additional, Caraveo, P., additional, Carosi, R., additional, Cascone, E., additional, Cerruti, M., additional, Chaty, S., additional, Chen, A., additional, Chen, X., additional, Chernyakova, M., additional, Chikawa, M., additional, Chudoba, J., additional, Cohen-Tanugi, J., additional, Colafrancesco, S., additional, Conforti, V., additional, Contreras, J. L., additional, Costa, A., additional, Cotter, G., additional, Covino, S., additional, Covone, G., additional, Cumani, P., additional, Cusumano, G., additional, D’Ammando, F., additional, D’Urso, D., additional, Daniel, M., additional, Dazzi, F., additional, De Angelis, A., additional, De Cesare, G., additional, De Franco, A., additional, De Frondat, F., additional, de Gouveia Dal Pino, E. M., additional, De Lisio, C., additional, de los Reyes Lopez, R., additional, De Lotto, B., additional, de Naurois, M., additional, De Palma, F., additional, Del Santo, M., additional, Delgado, C., additional, della Volpe, D., additional, Di Girolamo, T., additional, Di Giulio, C., additional, Di Pierro, F., additional, Di Venere, L., additional, Doro, M., additional, Dournaux, J., additional, Dumas, D., additional, Dwarkadas, V., additional, Díaz, C., additional, Ebr, J., additional, Egberts, K., additional, Einecke, S., additional, Elsässer, D., additional, Eschbach, S., additional, Falceta-Goncalves, D., additional, Fasola, G., additional, Fedorova, E., additional, Fernández-Barral, A., additional, Ferrand, G., additional, Fesquet, M., additional, Fiandrini, E., additional, Fiasson, A., additional, Filipovíc, M. D., additional, Fioretti, V., additional, Font, L., additional, Fontaine, G., additional, Franco, F. J., additional, Coromina, L. Freixas, additional, Fujita, Y., additional, Fukui, Y., additional, Funk, S., additional, Förster, A., additional, Gadola, A., additional, López, R. Garcia, additional, Garczarczyk, M., additional, Giglietto, N., additional, Giordano, F., additional, Giuliani, A., additional, Glicenstein, J., additional, Gnatyk, R., additional, Goldoni, P., additional, Grabarczyk, T., additional, Graciani, R., additional, Graham, J., additional, Grandi, P., additional, Granot, J., additional, Green, A. J., additional, Griffiths, S., additional, Gunji, S., additional, Hakobyan, H., additional, Hara, S., additional, Hassan, T., additional, Hayashida, M., additional, Heller, M., additional, Helo, J. C., additional, Hinton, J., additional, Hnatyk, B., additional, Huet, J., additional, Huetten, M., additional, Humensky, T. B., additional, Hussein, M., additional, Hörandel, J., additional, Ikeno, Y., additional, Inada, T., additional, Inome, Y., additional, Inoue, S., additional, Inoue, T., additional, Inoue, Y., additional, Ioka, K., additional, Iori, M., additional, Jacquemier, J., additional, Janecek, P., additional, Jankowsky, D., additional, Jung, I., additional, Kaaret, P., additional, Katagiri, H., additional, Kimeswenger, S., additional, Kimura, S., additional, Knödlseder, J., additional, Koch, B., additional, Kocot, J., additional, Kohri, K., additional, Komin, N., additional, Konno, Y., additional, Kosack, K., additional, Koyama, S., additional, Kraus, M., additional, Kubo, H., additional, Mezek, G. Kukec, additional, Kushida, J., additional, Palombara, N. La, additional, Lalik, K., additional, Lamanna, G., additional, Landt, H., additional, Lapington, J., additional, Laporte, P., additional, Lee, S., additional, Lees, J., additional, Lefaucheur, J., additional, Lenain, J.-P., additional, Leto, G., additional, Lindfors, E., additional, Lohse, T., additional, Lombardi, S., additional, Longo, F., additional, Lopez, M., additional, Lucarelli, F., additional, Luque-Escamilla, P. L., additional, López-Coto, R., additional, Maccarone, M. C., additional, Maier, G., additional, Malaguti, G., additional, Mandat, D., additional, Maneva, G., additional, Mangano, S., additional, Marcowith, A., additional, Martí, J., additional, Martínez, M., additional, Martínez, G., additional, Masuda, S., additional, Maurin, G., additional, Maxted, N., additional, Melioli, C., additional, Mineo, T., additional, Mirabal, N., additional, Mizuno, T., additional, Moderski, R., additional, Mohammed, M., additional, Montaruli, T., additional, Moralejo, A., additional, Mori, K., additional, Morlino, G., additional, Morselli, A., additional, Moulin, E., additional, Mukherjee, R., additional, Mundell, C., additional, Muraishi, H., additional, Murase, K., additional, Nagataki, S., additional, Nagayoshi, T., additional, Naito, T., additional, Nakajima, D., additional, Nakamori, T., additional, Nemmen, R., additional, Niemiec, J., additional, Nieto, D., additional, Nievas-Rosillo, M., additional, Nikołajuk, M., additional, Nishijima, K., additional, Noda, K., additional, Nogues, L., additional, Nosek, D., additional, Novosyadlyj, B., additional, Nozaki, S., additional, Ohira, Y., additional, Ohishi, M., additional, Ohm, S., additional, Okumura, A., additional, Ong, R. A., additional, Orito, R., additional, Orlati, A., additional, Ostrowski, M., additional, Oya, I., additional, Padovani, M., additional, Palacio, J., additional, Palatka, M., additional, Paredes, J. M., additional, Pavy, S., additional, Pe’er, A., additional, Persic, M., additional, Petrucci, P., additional, Petruk, O., additional, Pisarski, A., additional, Pohl, M., additional, Porcelli, A., additional, Prandini, E., additional, Prast, J., additional, Principe, G., additional, Prouza, M., additional, Pueschel, E., additional, Pühlhofer, G., additional, Quirrenbach, A., additional, Rameez, M., additional, Reimer, O., additional, Renaud, M., additional, Ribó, M., additional, Rico, J., additional, Rizi, V., additional, Rodriguez, J., additional, Fernandez, G. Rodriguez, additional, Vázquez, J. J. Rodríguez, additional, Romano, P., additional, Romeo, G., additional, Rosado, J., additional, Rousselle, J., additional, Rowell, G., additional, Rudak, B., additional, Sadeh, I., additional, Safi-Harb, S., additional, Saito, T., additional, Sakaki, N., additional, Sanchez, D., additional, Sangiorgi, P., additional, Sano, H., additional, Santander, M., additional, Sarkar, S., additional, Sawada, M., additional, Schioppa, E. J., additional, Schoorlemmer, H., additional, Schovanek, P., additional, Schussler, F., additional, Sergijenko, O., additional, Servillat, M., additional, Shalchi, A., additional, Shellard, R. C., additional, Siejkowski, H., additional, Sillanpää, A., additional, Simone, D., additional, Sliusar, V., additional, Sol, H., additional, Stanič, S., additional, Starling, R., additional, Stawarz, Ł., additional, Stefanik, S., additional, Stephan, M., additional, Stolarczyk, T., additional, Szanecki, M., additional, Szepieniec, T., additional, Tagliaferri, G., additional, Tajima, H., additional, Takahashi, M., additional, Takeda, J., additional, Tanaka, M., additional, Tanaka, S., additional, Tejedor, L. A., additional, Telezhinsky, I., additional, Temnikov, P., additional, Terada, Y., additional, Tescaro, D., additional, Teshima, M., additional, Testa, V., additional, Thoudam, S., additional, Tokanai, F., additional, Torres, D. F., additional, Torresi, E., additional, Tosti, G., additional, Townsley, C., additional, Travnicek, P., additional, Trichard, C., additional, Trifoglio, M., additional, Tsujimoto, S., additional, Vagelli, V., additional, Vallania, P., additional, Valore, L., additional, van Driel, W., additional, van Eldik, C., additional, Vandenbroucke, J., additional, Vassiliev, V., additional, Vecchi, M., additional, Vercellone, S., additional, Vergani, S., additional, Vigorito, C., additional, Vorobiov, S., additional, Vrastil, M., additional, Acosta, M. L. Vázquez, additional, Wagner, S. J., additional, Wagner, R., additional, Wakely, S. P., additional, Walter, R., additional, Ward, J. E., additional, Watson, J. J., additional, Weinstein, A., additional, White, M., additional, White, R., additional, Wierzcholska, A., additional, Wilcox, P., additional, Williams, D. A., additional, Wischnewski, R., additional, Wojcik, P., additional, Yamamoto, T., additional, Yamamoto, H., additional, Yamazaki, R., additional, Yanagita, S., additional, Yang, L., additional, Yoshida, T., additional, Yoshida, M., additional, Yoshiike, S., additional, Yoshikoshi, T., additional, Zacharias, M., additional, Zampieri, L., additional, Zanin, R., additional, Zavrtanik, M., additional, Zavrtanik, D., additional, Zdziarski, A., additional, Zech, A., additional, Zechlin, H., additional, Zhdanov, V., additional, Ziegler, A., additional, and Zorn, J., additional
Published: 2017
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135. Supernova rates from the SUDARE VST-Omegacam search II. Rates in a galaxy sample

Author: Botticella, M. T., primary, Cappellaro, E., additional, Greggio, L., additional, Pignata, G., additional, Della Valle, M., additional, Grado, A., additional, Limatola, L., additional, Baruffolo, A., additional, Benetti, S., additional, Bufano, F., additional, Capaccioli, M., additional, Cascone, E., additional, Covone, G., additional, De Cicco, D., additional, Falocco, S., additional, Haeussler, B., additional, Harutyunyan, V., additional, Jarvis, M., additional, Marchetti, L., additional, Napolitano, N. R., additional, Paolillo, M., additional, Pastorello, A., additional, Radovich, M., additional, Schipani, P., additional, Tomasella, L., additional, Turatto, M., additional, and Vaccari, M., additional
Published: 2017
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136. Upper limits for mass and radius of objects around Proxima Cen from SPHERE/VLT

Author: Mesa, D., primary, Zurlo, A., additional, Milli, J., additional, Gratton, R., additional, Desidera, S., additional, Langlois, M., additional, Vigan, A., additional, Bonavita, M., additional, Antichi, J., additional, Avenhaus, H., additional, Baruffolo, A., additional, Biller, B., additional, Boccaletti, A., additional, Bruno, P., additional, Cascone, E., additional, Chauvin, G., additional, Claudi, R. U., additional, De Caprio, V., additional, Fantinel, D., additional, Farisato, G., additional, Girard, J., additional, Giro, E., additional, Hagelberg, J., additional, Incorvaia, S., additional, Janson, M., additional, Kral, Q., additional, Lagadec, E., additional, Lagrange, A.-M., additional, Lessio, L., additional, Meyer, M., additional, Peretti, S., additional, Perrot, C., additional, Salasnich, B., additional, Schlieder, J., additional, Schmid, H.-M., additional, Scuderi, S., additional, Sissa, E., additional, Thalmann, C., additional, and Turatto, M., additional
Published: 2017
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137. ASTRI SST-2M: THE DESIGN EVOLUTION FROM THE PROTOTYPE TO THE ARRAY TELESCOPE.

Author: Marchiori, G., Busatta, A., Marcuzzi, E., Manfrin, C., Folla, I., Pareschi, G., Scuderi, S., Giro, E., Canestrari, R., Tosti, G., Antolini, E., Sironi, G., and Cascone, E.
Published: 2018
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138. Approccio integrato al monitoraggio di frane a cinematica intermittente

Author: BUDETTA P., CALCATERRA D., CALÒ F., PARISE M., RAMONDINI M., CASCONE E., PISCITELLI E., IULIANO S., TERRANOVA C., Budetta, Paolo, Calcaterra, Domenico, Calò, F., Parise, M., Ramondini, Massimo, Cascone, E., Piscitelli, E., Iuliano, S., and Terranova, C.
Subjects: Frane complesse, DInSAR, monitoraggio
Published: 2009

139. Draco project: activities results and future perspectives

Author: VUERLI C, PASIAN F, TAFFONI G, BARISANI A, BARUFFOLO A, BENACCHIO L, BARBIERI M, CANCIAN M, VOLPATO A, PASTORE S, FONTANA A, GALLOZZI S, DE SANTIS C, CASCONE E, CAPASSO G, MANNA V, RUBANO C, TAGLIAFERRI R, VIGLIAR M, BECCIANI U, COSTA A, CALANDUCCI A., LONGO, GIUSEPPE, Vuerli, C, Pasian, F, Taffoni, G, Barisani, A, Baruffolo, A, Benacchio, L, Barbieri, M, Cancian, M, Volpato, A, Pastore, S, Fontana, A, Gallozzi, S, DE SANTIS, C, Cascone, E, Capasso, G, Manna, V, Longo, Giuseppe, Rubano, C, Tagliaferri, R, Vigliar, M, Becciani, U, Costa, A, and Calanducci, A.
Published: 2007

140. La medicina territoriale sportello di salute per la partecipazione del cittadino in qualità di cliente-fruitore: comunicazione sanitaria integrata e carta dei servizi

Author: TRIASSI, MARIA, CASCONE E, GIANCOTTI E, GIORDANO V., Triassi, Maria, Cascone, E, Giancotti, E, and Giordano, V.
Subjects: medicina territoriale
Published: 2006

141. Electrophoresis of proteins and DNA on horizontal sodium dodecyl sulfate polycrylamide gels

Author: IZZO V, COSTA MA, DI FIORE R, DURO G, CASCONE E, BELLAVIA, Daniele, COLOMBO, Paolo, GIOVIALE, Maria Concetta, BARBIERI, Rainero, ROMANO, Maurizio, IZZO V, COSTA MA, DI FIORE R, DURO G, BELLAVIA D, CASCONE E, COLOMBO P, GIOVIALE MC, BARBIERI R, and Romano, M.
Published: 2006

142. Characterizing HR 3549 B using SPHERE

Author: Mesa, D., primary, Vigan, A., additional, D’Orazi, V., additional, Ginski, C., additional, Desidera, S., additional, Bonnefoy, M., additional, Gratton, R., additional, Langlois, M., additional, Marzari, F., additional, Messina, S., additional, Antichi, J., additional, Biller, B., additional, Bonavita, M., additional, Cascone, E., additional, Chauvin, G., additional, Claudi, R. U., additional, Curtis, I., additional, Fantinel, D., additional, Feldt, M., additional, Garufi, A., additional, Galicher, R., additional, Henning, Th., additional, Incorvaia, S., additional, Lagrange, A.-M., additional, Millward, M., additional, Perrot, C., additional, Salasnich, B., additional, Scuderi, S., additional, Sissa, E., additional, Wahhaj, Z., additional, and Zurlo, A., additional
Published: 2016
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143. The new SOXS instrument for the ESO NTT

Author: Schipani, P., additional, Claudi, R., additional, Campana, S., additional, Baruffolo, A., additional, Basa, S., additional, Basso, S., additional, Cappellaro, E., additional, Cascone, E., additional, Cosentino, R., additional, D'Alessio, F., additional, De Caprio, V., additional, Della Valle, M., additional, de Ugarte Postigo, A., additional, D'Orsi, S., additional, Franzen, R., additional, Fynbo, J., additional, Gal-Yam, A., additional, Gardiol, D., additional, Giro, E., additional, Hamuy, M., additional, Iuzzolino, M., additional, Loreggia, D., additional, Mattila, S., additional, Munari, M., additional, Pignata, G., additional, Riva, M., additional, Savarese, S., additional, Schmidt, B., additional, Scuderi, S., additional, Smartt, S., additional, and Vitali, F., additional
Published: 2016
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144. Pushing down with the contrast: scientific performances with SPHERE-IFS

Author: Claudi, R., additional, Antichi, J., additional, Baruffolo, A., additional, Bruno, P., additional, Cascone, E., additional, DeCaprio, V., additional, DePascale, M., additional, Desidera, S., additional, D'Orazi, V., additional, Fantinel, D., additional, Farisato, G., additional, Giro, E., additional, Gratton, R., additional, Lessio, L., additional, Maire, A.L., additional, Mesa, D., additional, Salasnich, B., additional, Scuderi, S., additional, Sissa, E., additional, Turatto, M., additional, Zurlo, A., additional, Beuzit, JL, additional, Boccaletti, A., additional, Chauvin, G., additional, Dohlen, K., additional, Finger, G., additional, Girard, J. H., additional, Kasper, M., additional, Hubin, N., additional, Langlois, M., additional, Lizon, J. L., additional, Mouillet, D., additional, Puget, P., additional, and Wildi, F., additional
Published: 2016
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145. MAORY: adaptive optics module for the E-ELT

Author: Diolaiti, E., additional, Ciliegi, P., additional, Abicca, R., additional, Agapito, G., additional, Arcidiacono, C., additional, Baruffolo, A., additional, Bellazzini, M., additional, Biliotti, V., additional, Bonaglia, M., additional, Bregoli, G., additional, Briguglio, R., additional, Brissaud, O., additional, Busoni, L., additional, Carbonaro, L., additional, Carlotti, A., additional, Cascone, E., additional, Correia, J.-J., additional, Cortecchia, F., additional, Cosentino, G., additional, De Caprio, V., additional, de Pascale, M., additional, De Rosa, A., additional, Del Vecchio, C., additional, Delboulbé, A., additional, Di Rico, G., additional, Esposito, S., additional, Fantinel, D., additional, Feautrier, P., additional, Felini, C., additional, Ferruzzi, D., additional, Fini, L., additional, Fiorentino, G., additional, Foppiani, I., additional, Ghigo, M., additional, Giordano, C., additional, Giro, E., additional, Gluck, L., additional, Hénault, F., additional, Jocou, L., additional, Kerber, F., additional, La Penna, P., additional, Lafrasse, S., additional, Lauria, M., additional, le Coarer, E., additional, Le Louarn, M., additional, Lombini, M., additional, Magnard, Y., additional, Maiorano, E., additional, Mannucci, F., additional, Mapelli, M., additional, Marchetti, E., additional, Maurel, D., additional, Michaud, L., additional, Morgante, G., additional, Moulin, T., additional, Oberti, S., additional, Pareschi, G., additional, Patti, M., additional, Puglisi, A., additional, Rabou, P., additional, Ragazzoni, R., additional, Ramsay, S., additional, Riccardi, A., additional, Ricciardi, S., additional, Riva, M., additional, Rochat, S., additional, Roussel, F., additional, Roux, A., additional, Salasnich, B., additional, Saracco, P., additional, Schreiber, L., additional, Spavone, M., additional, Stadler, E., additional, Sztefek, M.-H., additional, Ventura, N., additional, Vérinaud, C., additional, Xompero, M., additional, Fontana, A., additional, and Zerbi, F. M., additional
Published: 2016
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146. First light of the VLT planet finder SPHERE

Author: Maire, A.-L., primary, Bonnefoy, M., additional, Ginski, C., additional, Vigan, A., additional, Messina, S., additional, Mesa, D., additional, Galicher, R., additional, Gratton, R., additional, Desidera, S., additional, Kopytova, T. G., additional, Millward, M., additional, Thalmann, C., additional, Claudi, R. U., additional, Ehrenreich, D., additional, Zurlo, A., additional, Chauvin, G., additional, Antichi, J., additional, Baruffolo, A., additional, Bazzon, A., additional, Beuzit, J.-L., additional, Blanchard, P., additional, Boccaletti, A., additional, de Boer, J., additional, Carle, M., additional, Cascone, E., additional, Costille, A., additional, De Caprio, V., additional, Delboulbé, A., additional, Dohlen, K., additional, Dominik, C., additional, Feldt, M., additional, Fusco, T., additional, Girard, J. H., additional, Giro, E., additional, Gisler, D., additional, Gluck, L., additional, Gry, C., additional, Henning, T., additional, Hubin, N., additional, Hugot, E., additional, Jaquet, M., additional, Kasper, M., additional, Lagrange, A.-M., additional, Langlois, M., additional, Le Mignant, D., additional, Llored, M., additional, Madec, F., additional, Martinez, P., additional, Mawet, D., additional, Milli, J., additional, Möller-Nilsson, O., additional, Mouillet, D., additional, Moulin, T., additional, Moutou, C., additional, Origné, A., additional, Pavlov, A., additional, Petit, C., additional, Pragt, J., additional, Puget, P., additional, Ramos, J., additional, Rochat, S., additional, Roelfsema, R., additional, Salasnich, B., additional, Sauvage, J.-F., additional, Schmid, H. M., additional, Turatto, M., additional, Udry, S., additional, Vakili, F., additional, Wahhaj, Z., additional, Weber, L., additional, and Wildi, F., additional
Published: 2016
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147. Development of a Beowulf cluster for high performance parallel image processing

Author: SEDMAK, GIORGIO, CASCONE E, RUSSO G, ZAGGIA S., Sedmak, Giorgio, Cascone, E, Russo, G, and Zaggia, S.
Published: 2004

148. Cluster Beowulf per analisi astrofisiche

Author: BARONE F., CASCONE E., DE ROSA, ROSARIO, ESPOSITO R., MILANO L., PARDI S., TORTONE G., TAURINO F., RUSSO, GUIDO, Barone, F., Cascone, E., DE ROSA, Rosario, Esposito, R., Milano, L., Pardi, S., Russo, Guido, Tortone, G., and Taurino, F.
Published: 2003

149. The dual-mirror Small Size Telescope for the Cherenkov Telescope Array

Author: Pareschi, Giovanni, Agnetta, G., Antonelli, L. A., Bastieri, D., Bellassai, G., Belluso, M., Bigongiari, C., Billotta, S., Biondo, B., Bonanno, G., Bonnoli, G., Bruno, P., Bulgarelli, A., Canestrari, R., Capalbi, M., Caraveo, P., Carosi, A., Cascone, E., Catalano, O., Cereda, M., Conconi, P., Conforti, V., Cusumano, G., Caprio, V., Luca, A., Di Paola, A., Di Pierro, F., Fantinel, D., Fiorini, M., Fugazza, D., Gardiol, D., Ghigo, M., Gianotti, F., Giarrusso, S., Giro, E., Grillo, A., Impiombato, D., Incorvaia, S., La Barbera, A., La Palombara, N., La Parola, V., La Rosa, G., Lessio, L., Leto, G., Lombardi, S., Lucarelli, F., Maccarone, M. C., Malaguti, G., Malaspina, G., Mangano, V., Marano, D., Martinetti, E., Rachele Millul, Mineo, T., Mistò, A., Morello, C., Morlino, G., Panzera, M. R., Rodeghiero, G., Romano, P., Russo, F., Sacco, B., Sartore, N., Schwarz, J., Segreto, A., Sironi, G., Sottile, G., Stamerra, A., Strazzeri, E., Stringhetti, L., Tagliaferri, G., Testa, V., Timpanaro, M. C., Toso, G., Tosti, G., Trifoglio, M., Vallania, P., Vercellone, S., Zitelli, V., Amans, J. P., Boisson, C., Costille, C., Dournaux, J. L., Dumas, D., Fasola, G., Hervet, O., Huet, J. M., Laporte, P., Rulten, C., Sol, H., Zech, A., White, R., Hinton, J., Ross, D., Sykes, J., Ohm, S., Schmoll, J., Chadwick, P., Greenshaw, T., Daniel, M., Cotter, G., Varner, G. S., Funk, S., Vandenbroucke, J., Sapozhnikov, L., Buckley, J., Moore, P., Williams, D., Markoff, S., Vink, J., Berge, D., Hidaka, N., Okumura, A., and Tajima, H.
Subjects: High Energy Astrophysical Phenomena (astro-ph.HE), High Energy Physics - Experiment (hep-ex), Physics - Instrumentation and Detectors, FOS: Physical sciences, Instrumentation and Detectors (physics.ins-det), Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - High Energy Astrophysical Phenomena, Instrumentation and Methods for Astrophysics (astro-ph.IM), High Energy Physics - Experiment
Abstract: In this paper, the development of the dual mirror Small Size Telescopes (SST) for the Cherenkov Telescope Array (CTA) is reviewed. Up to 70 SST, with a primary mirror diameter of 4 m, will be produced and installed at the CTA southern site. These will allow investigation of the gamma-ray sky at the highest energies accessible to CTA, in the range from about 1 TeV to 300 TeV. The telescope presented in this contribution is characterized by two major innovations: the use of a dual mirror Schwarzschild-Couder configuration and of an innovative camera using as sensors either multi-anode photomultipliers (MAPM) or silicon photomultipliers (SiPM). The reduced plate-scale of the telescope, achieved with the dual-mirror optics, allows the camera to be compact (40 cm in diameter), and low-cost. The camera, which has about 2000 pixels of size 6x6 mm^2, covers a field of view of 10{\deg}. The dual mirror telescopes and their cameras are being developed by three consortia, ASTRI (Astrofisica con Specchi a Tecnologia Replicante Italiana, Italy/INAF), GATE (Gamma-ray Telescope Elements, France/Paris Observ.) and CHEC (Compact High Energy Camera, universities in UK, US and Japan) which are merging their efforts in order to finalize an end-to-end design that will be constructed for CTA. A number of prototype structures and cameras are being developed in order to investigate various alternative designs. In this contribution, these designs are presented, along with the technological solutions under study., Comment: In Proceedings of the 33rd International Cosmic Ray Conference (ICRC2013), Rio de Janeiro (Brazil). All CTA contributions at arXiv:1307.2232
Published: 2013

150. The ASTRI SST-2M prototype: camera designOptomechanical Engineering 2013

Author: Hatheway, Alson E., De Caprio, V., Belluso, M., Bonanno, G., Canestrari, R., Cascone, E., Catalano, O., La Rosa, G., Pareschi, G., Rodeghiero, Gabriele, and Sottile, G.
Published: 2013

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