143 results on '"E. Giani"'
Search Results
2. Telemedicine and COVID-19 pandemic: the perfect storm to mark a change in diabetes care results from a world-wide cross-sectional web-based survey
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E, Giani, primary, K, Dovc, additional, Santos, TJ Dos, additional, A, Chobot, additional, K, Braune, additional, R, Cardona-Hernandez, additional, Beaufort, C De, additional, and A, Scaramuzza, additional
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- 2022
- Full Text
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3. Development and Implementation of the AIDA International Registry for Patients With Still's Disease
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Vitale, A. Della Casa, F. Lopalco, G. Pereira, R.M. Ruscitti, P. Giacomelli, R. Ragab, G. La Torre, F. Bartoloni, E. Del Giudice, E. Lomater, C. Emmi, G. Govoni, M. Maggio, M.C. Maier, A. Makowska, J. Ogunjimi, B. Sfikakis, P.P. Sfriso, P. Gaggiano, C. Iannone, F. Dagostin, M.A. Di Cola, I. Navarini, L. Ahmed Mahmoud, A.A. Cardinale, F. Riccucci, I. Paroli, M.P. Marucco, E.M. Mattioli, I. Sota, J. Abbruzzese, A. Antonelli, I.P.B. Cipriani, P. Tufan, A. Fabiani, C. Ramadan, M.M. Cattalini, M. Kardas, R.C. Sebastiani, G.D. Giardini, H.A.M. Hernández-Rodríguez, J. Mastrorilli, V. Więsik-Szewczyk, E. Frassi, M. Caggiano, V. Telesca, S. Giordano, H.F. Guadalupi, E. Giani, T. Renieri, A. Colella, S. Cataldi, G. Gentile, M. Fabbiani, A. Al-Maghlouth, I.A. Frediani, B. Balistreri, A. Rigante, D. Cantarini, L. The Autoinflammatory Diseases Alliance (AIDA) Network
- Abstract
Objective: Aim of this paper is to present the design, construction, and modalities of dissemination of the AutoInflammatory Disease Alliance (AIDA) International Registry for patients with systemic juvenile idiopathic arthritis (sJIA) and adult-onset Still's disease (AOSD), which are the pediatric and adult forms of the same autoinflammatory disorder. Methods: This Registry is a clinical, physician-driven, population- and electronic-based instrument implemented for the retrospective and prospective collection of real-world data. The collection of data is based on the Research Electronic Data Capture (REDCap) tool and is intended to obtain evidence drawn from routine patients' management. The collection of standardized data is thought to bring knowledge about real-life clinical research and potentially communicate with other existing and future Registries dedicated to Still's disease. Moreover, it has been conceived to be flexible enough to easily change according to future scientific acquisitions. Results: Starting from June 30th to February 7th, 2022, 110 Centers from 23 Countries in 4 continents have been involved. Fifty-four of these have already obtained the approval from their local Ethics Committees. Currently, the platform counts 290 users (111 Principal Investigators, 175 Site Investigators, 2 Lead Investigators, and 2 data managers). The Registry collects baseline and follow-up data using 4449 fields organized into 14 instruments, including patient's demographics, history, clinical manifestations and symptoms, trigger/risk factors, therapies and healthcare access. Conclusions: This international Registry for patients with Still's disease will allow a robust clinical research through collection of standardized data, international consultation, dissemination of knowledge, and implementation of observational studies based on wide cohorts of patients followed-up for very long periods. Solid evidence drawn from “real-life” data represents the ultimate goal of this Registry, which has been implemented to significantly improve the overall management of patients with Still's disease. NCT 05200715 available at https://clinicaltrials.gov/. Copyright © 2022 Vitale, Della Casa, Lopalco, Pereira, Ruscitti, Giacomelli, Ragab, La Torre, Bartoloni, Del Giudice, Lomater, Emmi, Govoni, Maggio, Maier, Makowska, Ogunjimi, Sfikakis, Sfriso, Gaggiano, Iannone, Dagostin, Di Cola, Navarini, Ahmed Mahmoud, Cardinale, Riccucci, Paroli, Marucco, Mattioli, Sota, Abbruzzese, Antonelli, Cipriani, Tufan, Fabiani, Ramadan, Cattalini, Kardas, Sebastiani, Giardini, Hernández-Rodríguez, Mastrorilli, Więsik-Szewczyk, Frassi, Caggiano, Telesca, Giordano, Guadalupi, Giani, Renieri, Colella, Cataldi, Gentile, Fabbiani, Al-Maghlouth, Frediani, Balistreri, Rigante and Cantarini.
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- 2022
4. The GAPS Programme at TNG. XXIX. No detection of reflected light from 51 Peg b using optical high-resolution spectroscopy
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Scandariato, G, Borsa, F, Sicilia, D, Malavolta, L, Biazzo, K, Bonomo, A, Bruno, G, Claudi, R, Covino, E, Di Marcantonio, P, Esposito, M, Frustagli, G, Lanza, A, Maldonado, J, Maggio, A, Mancini, L, Micela, G, Nardiello, D, Rainer, M, Singh, V, Sozzetti, A, Affer, L, Benatti, S, Bignamini, A, Biliotti, V, Capuzzo-Dolcetta, R, Carleo, I, Cosentino, R, Damasso, M, Desidera, S, Garcia de Gurtubai, A, Ghedina, A, Giacobbe, P, Giani, E, Harutyunyan, A, Hernandez, N, Hernandez Diaz, M, Knapic, C, Leto, G, Martìnez Fiorenzano, A, Molinari, E, Nascimbeni, V, Pagano, I, Pedani, M, Piotto, G, Poretti, E, Stoev, H, G. Scandariato, F. Borsa, D. Sicilia, L. Malavolta, K. Biazzo, A. S. Bonomo, G. Bruno, R. Claudi, E. Covino, P. Di Marcantonio, M. Esposito, G. Frustagli, A. F. Lanza, J. Maldonado, A. Maggio, L. Mancini, G. Micela, D. Nardiello, M. Rainer, V. Singh, A. Sozzetti, L. Affer, S. Benatti, A. Bignamini, V. Biliotti, R. Capuzzo-Dolcetta, I. Carleo, R. Cosentino, M. Damasso, S. Desidera, A. Garcia de Gurtubai, A. Ghedina, P. Giacobbe, E. Giani, A. Harutyunyan, N. Hernandez, M. Hernandez Diaz, C. Knapic, G. Leto, A. F. Martìnez Fiorenzano, E. Molinari, V. Nascimbeni, I. Pagano, M. Pedani, G. Piotto, E. Poretti, H. Stoev, Scandariato, G, Borsa, F, Sicilia, D, Malavolta, L, Biazzo, K, Bonomo, A, Bruno, G, Claudi, R, Covino, E, Di Marcantonio, P, Esposito, M, Frustagli, G, Lanza, A, Maldonado, J, Maggio, A, Mancini, L, Micela, G, Nardiello, D, Rainer, M, Singh, V, Sozzetti, A, Affer, L, Benatti, S, Bignamini, A, Biliotti, V, Capuzzo-Dolcetta, R, Carleo, I, Cosentino, R, Damasso, M, Desidera, S, Garcia de Gurtubai, A, Ghedina, A, Giacobbe, P, Giani, E, Harutyunyan, A, Hernandez, N, Hernandez Diaz, M, Knapic, C, Leto, G, Martìnez Fiorenzano, A, Molinari, E, Nascimbeni, V, Pagano, I, Pedani, M, Piotto, G, Poretti, E, Stoev, H, G. Scandariato, F. Borsa, D. Sicilia, L. Malavolta, K. Biazzo, A. S. Bonomo, G. Bruno, R. Claudi, E. Covino, P. Di Marcantonio, M. Esposito, G. Frustagli, A. F. Lanza, J. Maldonado, A. Maggio, L. Mancini, G. Micela, D. Nardiello, M. Rainer, V. Singh, A. Sozzetti, L. Affer, S. Benatti, A. Bignamini, V. Biliotti, R. Capuzzo-Dolcetta, I. Carleo, R. Cosentino, M. Damasso, S. Desidera, A. Garcia de Gurtubai, A. Ghedina, P. Giacobbe, E. Giani, A. Harutyunyan, N. Hernandez, M. Hernandez Diaz, C. Knapic, G. Leto, A. F. Martìnez Fiorenzano, E. Molinari, V. Nascimbeni, I. Pagano, M. Pedani, G. Piotto, E. Poretti, and H. Stoev
- Abstract
Context. The analysis of exoplanetary atmospheres by means of high-resolution spectroscopy is an expanding research field which provides information on the chemical composition, thermal structure, atmospheric dynamics, and orbital velocity of exoplanets. Aims. In this work, we aim to detect the light reflected by the exoplanet 51 Peg b by employing optical high-resolution spectroscopy. Methods. To detect the light reflected by the planetary dayside, we used optical High Accuracy Radial velocity Planet Searcher and High Accuracy Radial velocity Planet Searcher for the Northern hemisphere spectra taken near the superior conjunction of the planet, when the flux contrast between the planet and the star is maximum. To search for the weak planetary signal, we cross-correlated the observed spectra with a high signal-to-noise ratio stellar spectrum. Results. We homogeneously analyze the available datasets and derive a 10-5 upper limit on the planet-to-star flux contrast in the optical. Conclusions. The upper limit on the planet-to-star flux contrast of 10-5 translates into a low albedo of the planetary atmosphere (Ag 0.05-0.15 for an assumed planetary radius in the range of 1.5-0.9 RJup, as estimated from the planet's mass).
- Published
- 2021
5. Persisting gender-related differences in low-grade inflammation and dyslipidemia in children, adolescents and young adults with type 1 diabetes
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D. Smigoc Schweiger, Tadej Battelino, E. Giani, Maddalena Macedoni, Primož Kotnik, Natasa Bratina, E. Plesnik, Urh Groselj, Tinka Hovnik, and Klemen Dovc
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Low grade inflammation ,Type 1 diabetes ,Pediatrics ,medicine.medical_specialty ,business.industry ,medicine ,Early adolescents ,Young adult ,Cardiology and Cardiovascular Medicine ,medicine.disease ,Gender related ,business ,Dyslipidemia - Published
- 2021
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6. Trattamento della metatarsalgia
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G. Bruno, E. Giani, A. Leli, A. Amanti, and B. Rossi
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Metatarsalgia ,medicine.medical_specialty ,Heel ,biology ,business.industry ,Radiography ,Forefoot ,Hyperkeratosis ,030204 cardiovascular system & hematology ,medicine.disease ,biology.organism_classification ,Surgery ,body regions ,03 medical and health sciences ,Valgus ,Hallux rigidus ,0302 clinical medicine ,medicine.anatomical_structure ,Orthopedic surgery ,medicine ,030212 general & internal medicine ,business - Abstract
Central metatarsalgia is a disease of the second, third and fourth metatarsal heads, described as pain in the forefoot, which extends from the plantar to the heel and on the dorsum of the foot; in some cases, it may be associated to hyperkeratosis. It is often accompanied by other symptoms like hallux rigidus and hallux valgus and/or the claw-foot syndrome. Usually the surgeon is able to clinically diagnose it with a radiographic foot survey, which allows him to calculate the “metatarsal formula”. Surgical treatment is suggested in case conservative treatment fails. The operation consists of radical surgical techniques, such as resection and realignment of the bone, as well as conservative techniques like distal and proximal osteotomies.
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- 2016
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7. M58 Internal Corrosion Control in Water Distribution Systems, Second Edition
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Richard E. Giani
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Distribution system ,Materials science ,Metallurgy ,Corrosion - Published
- 2017
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8. Disk and wind interaction in the young stellar object MWC 297 spatially resolved with AMBER/VLTI
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F. Malbet, M. Benisty, W.-J. de Wit, S. Kraus, A. Meilland, F. Millour, E. Tatulli, J.-P. Berger, O. Chesneau, K.-H. Hofmann, A. Isella, A. Natta, R. G. Petrov, T. Preibisch, P. Stee, L. Testi, G. Weigelt, P. Antonelli, U. Beckmann, Y. Bresson, A. Chelli, M. Dugué, G. Duvert, S. Gennari, L. Glück, P. Kern, S. Lagarde, E. Le Coarer, F. Lisi, K. Perraut, P. Puget, F. Rantakyrö, S. Robbe-Dubois, A. Roussel, G. Zins, M. Accardo, B. Acke, K. Agabi, E. Altariba, B. Arezki, E. Aristidi, C. Baffa, J. Behrend, T. Blöcker, S. Bonhomme, S. Busoni, F. Cassaing, J.-M. Clausse, J. Colin, C. Connot, A. Delboulbé, A. Domiciano de Souza, T. Driebe, P. Feautrier, D. Ferruzzi, T. Forveille, E. Fossat, R. Foy, D. Fraix-Burnet, A. Gallardo, E. Giani, C. Gil, A. Glentzlin, M. Heiden, M. Heininger, O. Hernandez Utrera, D. Kamm, M. Kiekebusch, D. Le Contel, J.-M. Le Contel, T. Lesourd, B. Lopez, M. Lopez, Y. Magnard, A. Marconi, G. Mars, G. Martinot-Lagarde, P. Mathias, P. Mège, J.-L. Monin, D. Mouillet, D. Mourard, E. Nussbaum, K. Ohnaka, J. Pacheco, C. Perrier, Y. Rabbia, S. Rebattu, F. Reynaud, A. Richichi, A. Robini, M. Sacchettini, D. Schertl, M. Schöller, W. Solscheid, A. Spang, P. Stefanini, M. Tallon, I. Tallon-Bosc, D. Tasso, F. Vakili, O. von der Lühe, J.-C. Valtier, M. Vannier, and N. Ventura
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Physics ,010308 nuclear & particles physics ,Astrophysics::High Energy Astrophysical Phenomena ,Young stellar object ,Continuum (design consultancy) ,Visibility (geometry) ,Equator ,Astronomy and Astrophysics ,Astrophysics::Cosmology and Extragalactic Astrophysics ,Astrophysics ,01 natural sciences ,Spectral line ,Wavelength ,Space and Planetary Science ,0103 physical sciences ,Thick disk ,Astrophysics::Solar and Stellar Astrophysics ,Astrophysics::Earth and Planetary Astrophysics ,010303 astronomy & astrophysics ,Astrophysics::Galaxy Astrophysics ,Line (formation) - Abstract
The young stellar object MWC 297 has been observed with the VLT interferometer equipped with the AMBER instrument. MWC 297 has been spatially resolved in the continuum with a visibility of 0.50 as well as in the Br gamma emission line where the visibility decrease to a lower value of 0.33. This change in the visibility with the wavelength can be interpreted by the presence of an optically thick disk responsible for the visibility in the continuum and of a stellar wind traced by Br gamma and whose apparent size is 40% larger. We validate this interpretation by building a model of the stellar environment that combines a geometrically thin, optically thick accretion disk model consisting of gas and dust, and a latitude-dependent stellar wind outflowing above the disk surface. The continuum emission and visibilities obtained from this model are fully consistent with the interferometric AMBER data. They agree also with existing optical, near-infrared spectra and other broad-band near-infrared interferometric visibilities. A picture emerges in which MWC 297 is surrounded by an equatorial flat disk that is possibly still accreting and an outflowing wind which has a much higher velocity in the polar region than at the equator. [abridged]
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- 2007
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9. The EChO science case
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Giovanna Tinetti, Pierre Drossart, Paul Eccleston, Paul Hartogh, Kate Isaak, Martin Linder, Christophe Lovis, Giusi Micela, Marc Ollivier, Ludovic Puig, Ignasi Ribas, Ignas Snellen, Bruce Swinyard, France Allard, Joanna Barstow, James Cho, Athena Coustenis, Charles Cockell, Alexandre Correia, Leen Decin, Remco de Kok, Pieter Deroo, Therese Encrenaz, Francois Forget, Alistair Glasse, Caitlin Griffith, Tristan Guillot, Tommi Koskinen, Helmut Lammer, Jeremy Leconte, Pierre Maxted, Ingo Mueller-Wodarg, Richard Nelson, Chris North, Enric Pallé, Isabella Pagano, Guseppe Piccioni, David Pinfield, Franck Selsis, Alessandro Sozzetti, Lars Stixrude, Jonathan Tennyson, Diego Turrini, Mariarosa Zapatero-Osorio, Jean-Philippe Beaulieu, Denis Grodent, Manuel Guedel, David Luz, Hans Ulrik Nørgaard-Nielsen, Tom Ray, Hans Rickman, Avri Selig, Mark Swain, Marek Banaszkiewicz, Mike Barlow, Neil Bowles, Graziella Branduardi-Raymont, Vincent Coudé du Foresto, Jean-Claude Gerard, Laurent Gizon, Allan Hornstrup, Christopher Jarchow, Franz Kerschbaum, Géza Kovacs, Pierre-Olivier Lagage, Tanya Lim, Mercedes Lopez-Morales, Giuseppe Malaguti, Emanuele Pace, Enzo Pascale, Bart Vandenbussche, Gillian Wright, Gonzalo Ramos Zapata, Alberto Adriani, Ruymán Azzollini, Ana Balado, Ian Bryson, Raymond Burston, Josep Colomé, Martin Crook, Anna Di Giorgio, Matt Griffin, Ruud Hoogeveen, Roland Ottensamer, Ranah Irshad, Kevin Middleton, Gianluca Morgante, Frederic Pinsard, Mirek Rataj, Jean-Michel Reess, Giorgio Savini, Jan-Rutger Schrader, Richard Stamper, Berend Winter, L. Abe, M. Abreu, N. Achilleos, P. Ade, V. Adybekian, L. Affer, C. Agnor, M. Agundez, C. Alard, J. Alcala, C. Allende Prieto, F. J. Alonso Floriano, F. Altieri, C. A. Alvarez Iglesias, P. Amado, A. Andersen, A. Aylward, C. Baffa, G. Bakos, P. Ballerini, M. Banaszkiewicz, R. J. Barber, D. Barrado, E. J. Barton, V. Batista, G. Bellucci, J. A. Belmonte Avilés, D. Berry, B. Bézard, D. Biondi, M. Błęcka, I. Boisse, B. Bonfond, P. Bordé, P. Börner, H. Bouy, L. Brown, L. Buchhave, J. Budaj, A. Bulgarelli, M. Burleigh, A. Cabral, M. T. Capria, A. Cassan, C. Cavarroc, C. Cecchi-Pestellini, R. Cerulli, J. Chadney, S. Chamberlain, N. Christian Jessen, A. Ciaravella, A. Claret, R. Claudi, A. Coates, R. Cole, A. Collur, D. Cordier, E. Covino, C. Danielski, M. Damasso, H. J. Deeg, E. Delgado-Mena, C. Del Vecchio, O. Demangeon, A. De Sio, J. De Wit, M. Dobrijévi, P. Doel, C. Dominic, E. Dorfi, S. Eales, C. Eiroa, M. Espinoza Contreras, M. Esposito, V. Eymet, N. Fabrizio, M. Fernández, B. Femenía Castella, P. Figueira, G. Filacchione, L. Fletcher, M. Focardi, S. Fossey, P. Fouqué, J. Frith, M. Galand, L. Gambicorti, P. Gaulme, R. J. García López, A. Garcia-Piquer, W. Gear, J. -C. Gerard, L. Gesa, E. Giani, F. Gianotti, M. Gillon, E. Giro, M. Giuranna, H. Gomez, I. Gomez-Leal, J. Gonzalez Hernandez, B. GonzÁlez Merino, R. Graczyk, D. Grassi, J. Guardia, P. Guio, J. Gustin, P. Hargrave, J. Haigh, E. Hébrard, U. Heiter, R. L. Heredero, E. Herrero, F. Hersant, D. Heyrovsky, M. Hollis, B. Hubert, R. Hueso, G. Israelian, N. Iro, P. Irwin, S. Jacquemoud, G. Jones, H. Jones, K. Justtanont, T. Kehoe, F. Kerschbaum, E. Kerins, P. Kervell, D. Kipping, T. Koskinen, N. Krupp, O. Lahav, B. Laken, N. Lanza, E. Lellouch, G. Leto, J. Licandro Goldaracena, C. Lithgow Bertelloni, S. J. Liu, U. Lo Cicero, N. Lodieu, P. Lognonné, M. Lopez Puertas, M. A. Lopez Valverde, I. Lundgaard Rasmussen, A. Luntzer, P. Machado, C. Mac Tavish, A. Maggio, J. P. Maillard, W. Magnes, J. Maldonado, U. Mall, J. B. Marquette, P. Mauskopf, F. Massi, A. S. Maurin, A. Medvedev, C. Michaut, P. Miles Paez, M. Montalto, P. Montañés Rodríguez, M. Monteiro, D. Montes, H. Morais, J. C. Morale, M. Morales-Calderón, G. Morello, A. Moro Martín, J. Moses, A. Moya Bedon, F. Murgas Alcaino, E. Oliva, G. Orton, F. Palla, M. Pancrazzi, E. Pantin, V. Parmentier, H. Parviainen, Y. Pena Ramirez, J. Peralta, S. Perez-Hoyos, R. Petrov, S. Pezzuto, R. Pietrzak, E. Pilat-Lohinger, N. Piskunov, R. Prinja, L. Prisinzano, I. Polichtchouk, E. Poretti, A. Radioti, A. Ramos, T. Rank-Luftinger, P. Read, K. Readorn, R. Rebolo Lopez, J. Rebordao, M. Rengel, L. Rezac, M. Rocchetto, F. Rodler, J. Sanchez Bejar, A. Sanchez Lavega, E. Sanroma, N. Santos, J. Sanz Forcada, G. Scandariato, F.- X. Schmider, A. Scholz, S. Scuderi, J. Sethenadh, S. Shore, A. Showman, B. Sicardy, P. Sitek, A. Smith, L. Soret, S. Sousa, A. Stiepen, M. Stolarski, G. Strazzulla, H. M. Tabernero, P. Tanga, M. Tecsa, J. Temple, L. Terenzi, M. Tessenyi, L. Testi, S. Thompson, H. Thrastarson, B. W. Tingley, M. Trifoglio, J. Martin Torres, A. Tozzi, D. Turrini, R. Varley, F. Vakili, M. de Val-Borro, M. L. Valdivieso, O. Venot, E. Villaver, S. Vinatier, S. Viti, I. Waldmann, D. Waltham, D. Ward-Thompson, R. Waters, C. Watkins, D. Watson, P. Wawer, A. Wawrzaszk, G. White, T. Widemann, W. Winek, T. Wi.niowski, R. Yelle, Y. Yung, and S. N. Yurchenko
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13. Climate action ,7. Clean energy - Published
- 2015
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10. Didactic/research
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L. Amistadi, E. Giani, M. Landsberger, S. Marini, M. Marzo, D. Nencini, V. P. Mosco, E. Narne, L. A. Pezzetti, G. Rakowitz, SCAVUZZO, GIUSEPPINA, L., Amistadi, E., Giani, M., Landsberger, S., Marini, M., Marzo, D., Nencini, V. P., Mosco, E., Narne, L. A., Pezzetti, G., Rakowitz, and Scavuzzo, Giuseppina
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research ,Architectural composition ,Didactic - Abstract
Considering the involvement of the researchers at all levels of the didactic, it may be assumed that the transmissibility of the architectonic composition is a question of priority for them, at least for two areas of the relationship research/didactic: research about the didactic and research through the didactic experimentation. Didactic and research come closer when it is understood that nothing is transmissible except thought means not teaching something already worked out, or well know, but to transmit an attitude towards to search. Contemporary pedagogy, appropriating Derrida's deconstruction, indicates in the form of awakening the method for a discipline that eschews the evidence, the convention, which is not deaf to the contingent event and everything that can be generated but has not yet been revealed.
- Published
- 2013
11. Contribution � l��tude de la transmission h�r�ditaire du rhume et de l�asthme des foins
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P. Carbonera and E. Giani
- Published
- 2015
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12. An asymmetry detected in the disk of κ Canis Majoris with AMBER/VLTI
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A. Meilland, F. Millour, P. Stee, A. Domiciano de Souza, R. G. Petrov, D. Mourard, S. Jankov, S. Robbe-Dubois, A. Spang, E. Aristidi, P. Antonelli, U. Beckmann, Y. Bresson, A. Chelli, M. Dugué, G. Duvert, S. Gennari, L. Glück, P. Kern, S. Lagarde, E. Le Coarer, F. Lisi, F. Malbet, K. Perraut, P. Puget, F. Rantakyrö, A. Roussel, E. Tatulli, G. Weigelt, G. Zins, M. Accardo, B. Acke, K. Agabi, E. Altariba, B. Arezki, C. Baffa, J. Behrend, T. Blöcker, S. Bonhomme, S. Busoni, F. Cassaing, J.-M. Clausse, J. Colin, C. Connot, A. Delboulbé, T. Driebe, P. Feautrier, D. Ferruzzi, T. Forveille, E. Fossat, R. Foy, D. Fraix-Burnet, A. Gallardo, E. Giani, C. Gil, A. Glentzlin, M. Heiden, M. Heininger, O. Hernandez Utrera, K.-H. Hofmann, D. Kamm, M. Kiekebusch, S. Kraus, D. Le Contel, J.-M. Le Contel, T. Lesourd, B. Lopez, M. Lopez, Y. Magnard, A. Marconi, G. Mars, G. Martinot-Lagarde, P. Mathias, P. Mège, J.-L. Monin, D. Mouillet, E. Nussbaum, K. Ohnaka, J. Pacheco, C. Perrier, Y. Rabbia, S. Rebattu, F. Reynaud, A. Richichi, A. Robini, M. Sacchettini, D. Schertl, M. Schöller, W. Solscheid, P. Stefanini, M. Tallon, I. Tallon-Bosc, D. Tasso, L. Testi, F. Vakili, O. von der Lühe, J.-C. Valtier, M. Vannier, and N. Ventura
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Physics ,010308 nuclear & particles physics ,Be star ,media_common.quotation_subject ,Continuum (design consultancy) ,Astronomy and Astrophysics ,Astrophysics ,01 natural sciences ,Asymmetry ,Stars ,Polar wind ,Space and Planetary Science ,0103 physical sciences ,Astrophysics::Solar and Stellar Astrophysics ,Spectral energy distribution ,Astrophysics::Earth and Planetary Astrophysics ,Spectral resolution ,010303 astronomy & astrophysics ,Astrophysics::Galaxy Astrophysics ,media_common ,Line (formation) - Abstract
Aims. We study the geometry and kinematics of the circumstellar environment of the Be star Kappa CMa in the Br gamma emission line and its nearby continuum. Methods. We use the VLTI/AMBER instrument operating in the K band which provides a spatial resolution of about 6 mas with a spectral resolution of 1500 to study the kinematics within the disk and to infer its rotation law. In order to obtain more kinematical constraints we also use an high spectral resolution Pa beta line profile obtain in December 2005 at the Observatorio do Pico do Dios, Brazil and we compile V/R line profile variations and spectral energy distribution data points from the literature. Results. Using differential visibilities and differential phases across the Br gamma line we detect an asymmetry in the disk. Moreover, we found that kappa CMa seems difficult to fit within the classical scenario for Be stars, illustrated recently by alpha Arae observations, i.e. a fast rotating B star close to its breakup velocity surrounded by a Keplerian circumstellar disk with an enhanced polar wind. Finally we discuss the possibility for kappa CMa to be a critical rotator with a Keplerian rotating disk and try to see if the detected asymmetry can be interpreted within the "one-armed" viscous disk framework.
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- 2006
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13. The Risk Map of Italian Cultural Heritage
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A. Giovagnoli, G. Accardo, and E. Giani
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Process (engineering) ,business.industry ,Library science ,Distribution (economics) ,Building and Construction ,Conservation ,Cultural heritage ,Thematic map ,Homogeneous ,Risk map ,Information system ,Christian ministry ,Sociology ,business ,Environmental planning - Abstract
The Risk Map of Italian Cultural Heritage is a current research project of the Istituto Centrale del Restauro (ICR), with the aim of developing a more rational and economical means of undertaking the maintenance, conservation, and restoration of the architectural and archaeological monuments of Italy.The first step of the project has been to create a geographical information system (GIS), which collects, processes, and manages both cartographic and alphanumerical data coming from peripheral units based in many Italian towns by the ‘Soprintendenze’, being the territorial departments of the Ministry of Culture. The connection between environmental danger and risk to the monuments is highlighted through a mapping process, by overlapping computerized maps having a thematic content (such as air pollution, climate, and earthquakes) and the distribution of cultural assets. The second step has ensured that the above data were homogeneous through defining standardized schedules at different levels of detai...
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- 2003
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14. Quality Issues in Chip‐on‐board (COB) Technology
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E. Giani and J.P. Mathurin
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Engineering ,business.industry ,media_common.quotation_subject ,Condensed Matter Physics ,Chip ,Statistical process control ,Atomic and Molecular Physics, and Optics ,Manufacturing engineering ,Surfaces, Coatings and Films ,Electronic, Optical and Magnetic Materials ,On board ,Quality (business) ,Electrical and Electronic Engineering ,business ,media_common - Abstract
Critical processing steps of COB manufacturing, as implemented at Epitek, are reported. They include testing of incoming boards, cleaning, bonding parameters, bonding defects and statistical process control.
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- 1994
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15. Long-lasting immunogenicity and safety of a 2009 pandemic influenza A(H1N1) MF59-adjuvanted vaccine when co-administered with a 2009-2010 seasonal influenza vaccine in young patients with type 1 diabetes mellitus
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G V, Zuccotti, E, Pariani, A, Scaramuzza, L, Santoro, E, Giani, M, Macedoni, A, Gazzarri, G, Anselmi, A, Amendola, and A, Zanetti
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Male ,Squalene ,Adolescent ,Patient Selection ,Polysorbates ,Young Adult ,Diabetes Mellitus, Type 1 ,Influenza A Virus, H1N1 Subtype ,Treatment Outcome ,Adjuvants, Immunologic ,Italy ,Influenza Vaccines ,Influenza, Human ,Humans ,Female ,Prospective Studies ,Child ,Pandemics - Abstract
To evaluate the long-lasting immunogenicity and safety of a pandemic vaccine co-administered with a seasonal influenza vaccine in young subjects with Type 1 diabetes.Eighty patients (mean age: 16.7 ± 5.5 years, disease duration: 10.2 ± 4.7 years) were randomly assigned to receive a single or a double dose (1 month apart) of MF59-adjuvanted influenza A(H1N1) vaccine, simultaneously with a single dose of a virosome-adjuvanted trivalent influenza vaccine for the 2009-2010 season.One month after immunization, the rate of seroconversion to 2009 pandemic A(H1N1) was 92.5% with an overall 100% proportion of vaccinees with protective antibody titres (≥ 1:40). No significant differences were observed between vaccinees who received the one-dose or the two-dose schedule. Seasonal vaccine induced a significant increase of both seroprotection rates and antibody levels. Local adverse events at the injection site of pandemic and seasonal vaccines were reported by 66.3% and 50% of subjects, respectively. Solicited systemic adverse events, mainly mild in intensity, were reported by 26.7% of vaccinees. No subjects had an influenza-like illness during the 6-month follow-up.One injection of 2009 pandemic influenza A(H1N1) MF59-adjuvanted vaccine is immunogenic and safe in young patients with Type 1 diabetes who are at increased risk of influenza morbidities. Pandemic vaccine can be safely co-administered with seasonal influenza vaccine.
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- 2011
16. Unilateral NMR Microclimate Monitoring and SEM-EDS analysis for monitoring the state of conservation of an ancient deteriorated wall painting in hypogeous environment
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N. Proietti, V. Di Tullio, E. Giani, D. Poggi, and D. Capitani
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- 2011
17. Monitoraggio del contenuto d'umidità con NMR unilaterale in ambienti ipogei: il caso dell'affresco
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V. Di Tullio, N. Proietti, D. Capitani, and E. Giani
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- 2010
18. Il nuovo certificato di assistenza al parto : CedAP
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TRIASSI, MARIA, R. ARSIERI, A. PUGLIESE, M. SAPORITO, A. ANNECCHIARICO, E. GIANI, Triassi, Maria, R., Arsieri, A., Pugliese, M., Saporito, A., Annecchiarico, and E., Giani
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- 1998
19. An integrated approach to mapping moisture and salt content in two frescoes in the Basilica of San Clemente
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R. Olmi, C. Riminesi, S. Priori, N. Proietti, D. Capitani, A.L. Segre, E. Giani, and P. Santopadre
- Abstract
Two physical non-invasive techniques bave been used to measure the moisture content in two frescoes in the Basilica of San Clemente in Rome: evanescent-field dielectrometry (EFD) and unilateral nuclear magnetic resonance (uNMR). Both techniques are portable and allow mapping the moisture content in frescoed walls and murai paintings. The integration of the two techniques results in a true synergistic effect, by exploiting their peculiar characteristics: uNMR is inherently independent on the materia!characteristics, as it is directly sensitive to the water content, and allows the obtainment of a 2D map of the water content relative to a depth of a few millimeters; EFD measures the sub-superficial moisture content (up to about 2 cm) and allows the detection of soluble salts in the wall, but its response slightly depends on the material density, as moisture and salt content are obtained from the dielectric properties of the wall. Moreover, uNMR operates without needing to contact the surface of the fresco, and thus allows the obtainment of information also about criticai regions where, for example, there is a risk of det chment of the painted layer. EFD, that needs a direct contact with the wall, is very fast (a few seconds per measureod point, with in-line elaboration), also allowing the study of the dynamics of water absorption after a consolidation treatment. The integration between the two techniques allows the full characterization of a fresco with regard to the water content and a screening of the locations where an invasive chemical analysis of the salts is in order.
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- 2008
20. Optical configuration and analysis of the AMBER/VLTI instrument
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S. Robbe-Dubois, S. Lagarde, R. G. Petrov, F. Lisi, U. Beckmann, P. Antonelli, Y. Bresson, G. Martinot-Lagarde, A. Roussel, P. Salinari, M. Vannier, A. Chelli, M. Dugué, G. Duvert, S. Gennari, L. Glück, P. Kern, E. Le Coarer, F. Malbet, F. Millour, K. Perraut, P. Puget, F. Rantakyrö, E. Tatulli, G. Weigelt, G. Zins, M. Accardo, B. Acke, K. Agabi, E. Altariba, B. Arezki, E. Aristidi, C. Baffa, J. Behrend, T. Blöcker, S. Bonhomme, S. Busoni, F. Cassaing, J.-M. Clausse, J. Colin, C. Connot, L. Delage, A. Delboulbé, A. Domiciano de Souza, T. Driebe, P. Feautrier, D. Ferruzzi, T. Forveille, E. Fossat, R. Foy, D. Fraix-Burnet, A. Gallardo, E. Giani, C. Gil, A. Glentzlin, M. Heiden, M. Heininger, O. Hernandez Utrera, K.-H. Hofmann, D. Kamm, M. Kiekebusch, S. Kraus, D. Le Contel, J.-M. Le Contel, T. Lesourd, B. Lopez, M. Lopez, Y. Magnard, A. Marconi, G. Mars, P. Mathias, P. Mège, J.-L. Monin, D. Mouillet, D. Mourard, E. Nussbaum, K. Ohnaka, J. Pacheco, C. Perrier, Y. Rabbia, S. Rebattu, F. Reynaud, A. Richichi, A. Robini, M. Sacchettini, D. Schertl, M. Schöller, W. Solscheid, A. Spang, P. Stee, P. Stefanini, M. Tallon, I. Tallon-Bosc, D. Tasso, L. Testi, F. Vakili, O. von der Lühe, J.-C. Valtier, N. Ventura, Laboratoire Universitaire d'Astrophysique de Nice (LUAN), 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)-Centre National de la Recherche Scientifique (CNRS), Laboratoire Gemini (LG), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de la Côte d'Azur, Université Côte d'Azur (UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Centre National de la Recherche Scientifique (CNRS), INAF - Osservatorio Astrofisico di Arcetri (OAA), Istituto Nazionale di Astrofisica (INAF), Max-Planck-Institut für Radioastronomie (MPIFR), Division technique INSU/SDU (DTI), Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), European Southern Observatory (ESO), Institute of Astronomy [Leuven], Catholic University of Leuven - Katholieke Universiteit Leuven (KU Leuven), Laboratoire Hippolyte Fizeau (FIZEAU), Université Côte d'Azur (UCA)-Université Côte d'Azur (UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de la Côte d'Azur, Université Côte d'Azur (UCA)-Centre National de la Recherche Scientifique (CNRS), Université Côte d'Azur (UCA)-Université Côte d'Azur (UCA)-Centre National de la Recherche Scientifique (CNRS), Galilée (Galilée), Laboratoire de Cosmologie, Astrophysique Stellaire & Solaire, de Planétologie et de Mécanique des Fluides (CASSIOPEE), Université Côte d'Azur (UCA)-Université Côte d'Azur (UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), 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, and Université Côte d'Azur (UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-Centre National de la Recherche Scientifique (CNRS)
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FOS: Physical sciences ,Astrophysics ,01 natural sciences ,Stability (probability) ,010309 optics ,[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO] ,Optics ,numerical ,interferometers ,instrumentation: high angular resolution ,0103 physical sciences ,Visibility ,010303 astronomy & astrophysics ,Physics ,Basis (linear algebra) ,Spatial filter ,[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph] ,business.industry ,Emphasis (telecommunications) ,Astrophysics (astro-ph) ,Astronomy and Astrophysics ,Differential phase ,Transmission (telecommunications) ,Space and Planetary Science ,methods : analytical ,business ,Realization (systems) ,laboratory - Abstract
This paper describes the design goals and engineering efforts that led to the realization of AMBER (Astronomical Multi BEam combineR) and to the achievement of its present performance. On the basis of the general instrumental concept, AMBER was decomposed into modules whose functions and detailed characteristics are given. Emphasis is put on the spatial filtering system, a key element of the instrument. We established a budget for transmission and contrast degradation through the different modules, and made the detailed optical design. The latter confirmed the overall performance of the instrument and defined the exact implementation of the AMBER optics. The performance was assessed with laboratory measurements and commissionings at the VLTI, in terms of spectral coverage and resolution, instrumental contrast higher than 0.80, minimum magnitude of 11 in K, absolute visibility accuracy of 1%, and differential phase stability of 1E-3 rad over one minute., Comment: 14 pages
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- 2007
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21. Near-infrared interferometry of eta Carinae with spectral resolutions of 1 500 and 12 000 using AMBER/VLTI
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G. Weigelt, S. Kraus, T. Driebe, R. G. Petrov, K.-H. Hofmann, F. Millour, O. Chesneau, D. Schertl, F. Malbet, D. J. Hillier, T. Gull, K. Davidson, A. Domiciano de Souza, P. Antonelli, U. Beckmann, Y. Bresson, A. Chelli, M. Dugué, G. Duvert, S. Gennari, L. Glück, P. Kern, S. Lagarde, E. Le Coarer, F. Lisi, K. Perraut, P. Puget, F. Rantakyrö, S. Robbe-Dubois, A. Roussel, E. Tatulli, G. Zins, M. Accardo, B. Acke, K. Agabi, E. Altariba, B. Arezki, E. Aristidi, C. Baffa, J. Behrend, T. Blöcker, S. Bonhomme, S. Busoni, F. Cassaing, J.-M. Clausse, J. Colin, C. Connot, A. Delboulbé, P. Feautrier, D. Ferruzzi, T. Forveille, E. Fossat, R. Foy, D. Fraix-Burnet, A. Gallardo, E. Giani, C. Gil, A. Glentzlin, M. Heiden, M. Heininger, O. Hernandez Utrera, D. Kamm, M. Kiekebusch, D. Le Contel, J.-M. Le Contel, T. Lesourd, B. Lopez, M. Lopez, Y. Magnard, A. Marconi, G. Mars, G. Martinot-Lagarde, P. Mathias, P. Mège, J.-L. Monin, D. Mouillet, D. Mourard, E. Nussbaum, K. Ohnaka, J. Pacheco, C. Perrier, Y. Rabbia, S. Rebattu, F. Reynaud, A. Richichi, A. Robini, M. Sacchettini, M. Schöller, W. Solscheid, A. Spang, P. Stee, P. Stefanini, M. Tallon, I. Tallon-Bosc, D. Tasso, L. Testi, F. Vakili, O. von der Lühe, J.-C. Valtier, M. Vannier, N. Ventura, K. Weis, M. Wittkowski, Max-Planck-Institut für Radioastronomie (MPIFR), Laboratoire Universitaire d'Astrophysique de Nice (LUAN), Université Nice Sophia Antipolis (... - 2019) (UNS), Université Côte d'Azur (UCA)-Université Côte d'Azur (UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Laboratoire d'Astrophysique de Grenoble (LAOG), Université Joseph Fourier - Grenoble 1 (UJF)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Laboratoire Gemini (LG), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de la Côte d'Azur, Université Côte d'Azur (UCA)-Université Côte d'Azur (UCA)-Centre National de la Recherche Scientifique (CNRS), Département Fresnel (FRESNEL), Observatoire de la Côte d'Azur, Laboratoire de Cosmologie, Astrophysique Stellaire & Solaire, de Planétologie et de Mécanique des Fluides (CASSIOPEE), Université Côte d'Azur (UCA)-Université Côte d'Azur (UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de la Côte d'Azur, Université Côte d'Azur (UCA)-Centre National de la Recherche Scientifique (CNRS), INAF - Osservatorio Astrofisico di Arcetri (OAA), Istituto Nazionale di Astrofisica (INAF), European Southern Observatory (ESO), ONERA - The French Aerospace Lab [Châtillon], ONERA, Observatoire de la Côte d'Azur (OCA), Centre National de la Recherche Scientifique (CNRS), Canada-France-Hawaii Telescope Corporation (CFHT), National Research Council of Canada (NRC)-Centre National de la Recherche Scientifique (CNRS)-University of Hawai'i [Honolulu] (UH), Centre de Recherche Astrophysique de Lyon (CRAL), Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-École normale supérieure - Lyon (ENS Lyon), Association EURATOM-CEA (CEA/DSM/DRFC), Commissariat à l'énergie atomique et aux énergies alternatives (CEA), Division technique INSU/SDU (DTI), Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Laboratoire Astrophysique de Toulouse-Tarbes (LATT), Centre National de la Recherche Scientifique (CNRS)-Observatoire Midi-Pyrénées (OMP), Université Fédérale Toulouse Midi-Pyrénées-Université Fédérale Toulouse Midi-Pyrénées-Institut national des sciences de l'Univers (INSU - CNRS)-Université Toulouse III - Paul Sabatier (UT3), Université Fédérale Toulouse Midi-Pyrénées, Astrophysique Relativiste Théories Expériences Métrologie Instrumentation Signaux (ARTEMIS), PHOTONIQUE, XLIM (XLIM), Université de Limoges (UNILIM)-Centre National de la Recherche Scientifique (CNRS)-Université de Limoges (UNILIM)-Centre National de la Recherche Scientifique (CNRS), 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)-Centre National de la Recherche Scientifique (CNRS), Université Côte d'Azur (UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Centre National de la Recherche Scientifique (CNRS), COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de la Côte d'Azur, Université Côte d'Azur (UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-Centre National de la Recherche Scientifique (CNRS), ONERA-Université Paris Saclay (COmUE), 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), Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Toulouse III - Paul Sabatier (UT3), Université Nice Sophia Antipolis (1965 - 2019) (UNS), COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-Centre National de la Recherche Scientifique (CNRS), 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), Université de Lyon-Université de Lyon-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire Midi-Pyrénées (OMP), Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3), and Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Centre National de la Recherche Scientifique (CNRS)
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[SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO] ,Astrophysics::High Energy Astrophysical Phenomena ,Continuum (design consultancy) ,Astrophysics ,01 natural sciences ,7. Clean energy ,circumstellar matter ,emission-line Be ,outflows ,[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO] ,Atmospheric radiative transfer codes ,0103 physical sciences ,Astrophysics::Solar and Stellar Astrophysics ,Emission spectrum ,Spectral resolution ,010303 astronomy & astrophysics ,infrared: stars ,Astrophysics::Galaxy Astrophysics ,Physics ,Very Large Telescope ,[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph] ,010308 nuclear & particles physics ,Near-infrared spectroscopy ,Gamma ray ,Astronomy and Astrophysics ,Position angle ,stars: individual: ηCarinae ,winds ,13. Climate action ,Space and Planetary Science ,techniques: interferometric ,stars: mass-loss - Abstract
Aims. We present the first NIR spectro-interferometry of the LBV ? Carinae. The observations were performed with the AMBER instrument of the ESO Very Large Telescope Interferometer (VLTI) using baselines from 42 to 89 m. The aim of this work is to study the wavelength dependence of ? Car's optically thick wind region with a high spatial resolution of 5 mas (11 AU) and high spectral resolution. Methods: The observations were carried out with three 8.2 m Unit Telescopes in the K-band. The raw data are spectrally dispersed interferograms obtained with spectral resolutions of 1500 (MR-K mode) and 12 000 (HR-K mode). The MR-K observations were performed in the wavelength range around both the He I 2.059 ?m and the Br? 2.166 ?m emission lines, the HR-K observations only in the Br? line region. Results: The spectrally dispersed AMBER interferograms allow the investigation of the wavelength dependence of the visibility, differential phase, and closure phase of ? Car. In the K-band continuum, a diameter of 4.0±0.2 mas (Gaussian FWHM, fit range 28-89 m baseline length) was measured for ? Car's optically thick wind region. If we fit Hillier et al. (2001, ApJ, 553, 837) model visibilities to the observed AMBER visibilities, we obtain 50% encircled-energy diameters of 4.2, 6.5 and 9.6 mas in the 2.17 ?m continuum, the He I, and the Br? emission lines, respectively. In the continuum near the Br? line, an elongation along a position angle of 120°±15° was found, consistent with previous VINCI/VLTI measurements by van Boekel et al. (2003, A&A, 410, L37). We compare the measured visibilities with predictions of the radiative transfer model of Hillier et al. (2001), finding good agreement. Furthermore, we discuss the detectability of the hypothetical hot binary companion. For the interpretation of the non-zero differential and closure phases measured within the Br? line, we present a simple geometric model of an inclined, latitude-dependent wind zone. Our observations support theoretical models of anisotropic winds from fast-rotating, luminous hot stars with enhanced high-velocity mass loss near the polar regions. Based on observations collected at the European Southern Observatory, Paranal, Chile, within the AMBER guaranteed time programme 074.A-9025 and the VLTI science demonstration programme 074.A-9024.
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- 2007
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22. Direct constraint on the distance of Gamma2 Velorum from AMBER/VLTI observations
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F. Millour, R. G. Petrov, O. Chesneau, D. Bonneau, L. Dessart, C. Bechet, I. Tallon-Bosc, M. Tallon, E. Thiébaut, F. Vakili, F. Malbet, D. Mourard, P. Antonelli, U. Beckmann, Y. Bresson, A. Chelli, M. Dugué, G. Duvert, S. Gennari, L. Glück, P. Kern, S. Lagarde, E. Le Coarer, F. Lisi, K. Perraut, P. Puget, F. Rantakyrö, S. Robbe-Dubois, A. Roussel, E. Tatulli, G. Weigelt, G. Zins, M. Accardo, B. Acke, K. Agabi, E. Altariba, B. Arezki, E. Aristidi, C. Baffa, J. Behrend, T. Blöcker, S. Bonhomme, S. Busoni, F. Cassaing, J.-M. Clausse, J. Colin, C. Connot, A. Delboulbé, A. Domiciano de Souza, T. Driebe, P. Feautrier, D. Ferruzzi, T. Forveille, E. Fossat, R. Foy, D. Fraix-Burnet, A. Gallardo, E. Giani, C. Gil, A. Glentzlin, M. Heiden, M. Heininger, O. Hernandez Utrera, K.-H. Hofmann, D. Kamm, M. Kiekebusch, S. Kraus, D. Le Contel, J.-M. Le Contel, T. Lesourd, B. Lopez, M. Lopez, Y. Magnard, A. Marconi, G. Mars, G. Martinot-Lagarde, P. Mathias, P. Mège, J.-L. Monin, D. Mouillet, E. Nussbaum, K. Ohnaka, J. Pacheco, C. Perrier, Y. Rabbia, S. Rebattu, F. Reynaud, A. Richichi, A. Robini, M. Sacchettini, D. Schertl, M. Schöller, W. Solscheid, A. Spang, P. Stee, P. Stefanini, D. Tasso, L. Testi, O. von der Lühe, J.-C. Valtier, M. Vannier, N. Ventura, Laboratoire d'Astrophysique de Grenoble (LAOG), Université Joseph Fourier - Grenoble 1 (UJF)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Laboratoire Universitaire d'Astrophysique de Nice (LUAN), 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)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Cosmologie, Astrophysique Stellaire & Solaire, de Planétologie et de Mécanique des Fluides (CASSIOPEE), COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de la Côte d'Azur, COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-Université Côte d'Azur (UCA)-Centre National de la Recherche Scientifique (CNRS), Laboratoire Gemini (LG), 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)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-Centre National de la Recherche Scientifique (CNRS), Steward Observatory (STEWARD OBSERVATORY), University of Arizona, Centre de Recherche Astrophysique de Lyon (CRAL), École normale supérieure de Lyon (ENS de Lyon)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), INAF - Osservatorio Astrofisico di Arcetri (OAA), Istituto Nazionale di Astrofisica (INAF), Max-Planck-Institut für Radioastronomie (MPIFR), European Southern Observatory (ESO), PHOTONIQUE, XLIM (XLIM), Université de Limoges (UNILIM)-Centre National de la Recherche Scientifique (CNRS)-Université de Limoges (UNILIM)-Centre National de la Recherche Scientifique (CNRS), Laboratoire Astrophysique de Toulouse-Tarbes (LATT), Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire Midi-Pyrénées (OMP), Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Centre National de la Recherche Scientifique (CNRS), Division technique INSU/SDU (DTI), Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Observatoire des Sciences de l'Univers de Grenoble (OSUG), Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut national des sciences de l'Univers (INSU - CNRS)-Institut national de recherche en sciences et technologies pour l'environnement et l'agriculture (IRSTEA)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS), Observatoire de la Côte d'Azur (OCA), ONERA - The French Aerospace Lab [Châtillon], ONERA-Université Paris Saclay (COmUE), AMBER, Université Nice Sophia Antipolis (... - 2019) (UNS), Université Côte d'Azur (UCA)-Université Côte d'Azur (UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Université Côte d'Azur (UCA)-Université Côte d'Azur (UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de la Côte d'Azur, Université Côte d'Azur (UCA)-Centre National de la Recherche Scientifique (CNRS), 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)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-École normale supérieure - Lyon (ENS Lyon), Centre National de la Recherche Scientifique (CNRS)-Observatoire Midi-Pyrénées (OMP), Université Fédérale Toulouse Midi-Pyrénées-Université Fédérale Toulouse Midi-Pyrénées-Institut national des sciences de l'Univers (INSU - CNRS)-Université Toulouse III - Paul Sabatier (UT3), Université Fédérale Toulouse Midi-Pyrénées, 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), Centre National de la Recherche Scientifique (CNRS), ONERA, Université Côte d'Azur (UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-Centre National de la Recherche Scientifique (CNRS), Université Côte d'Azur (UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Centre National de la Recherche Scientifique (CNRS), 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), and Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Toulouse III - Paul Sabatier (UT3)
- Subjects
Physics ,[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph] ,010308 nuclear & particles physics ,[SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO] ,Astrophysics (astro-ph) ,FOS: Physical sciences ,Astronomy and Astrophysics ,Observable ,Ranging ,Astrophysics ,Spectral bands ,Position angle ,01 natural sciences ,[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO] ,Space and Planetary Science ,0103 physical sciences ,Binary system ,010303 astronomy & astrophysics - Abstract
International audience; In this work, we present the first AMBER observations, of the Wolf-Rayet and O (WR+O) star binary system y² Velorum. The AMBER instrument was used with the telescopes UT2, UT3, and UT4 on baselines ranging from 46m to 85m. It delivered spectrally dispersed visibilities, as well as differential and closure phases, with a resolution R = 1500 in the spectral band 1.95-2.17 micron. We interpret these data in the context of a binary system with unresolved components, neglecting in a first approximation the wind-wind collision zone flux contribution. We show that the AMBER observables result primarily from the contribution of the individual components of the WR+O binary system. We discuss several interpretations of the residuals, and speculate on the detection of an additional continuum component, originating from the free-free emission associated with the wind-wind collision zone (WWCZ), and contributing at most to the observed K-band flux at the 5% level. The expected absolute separation and position angle at the time of observations were 5.1±0.9mas and 66±15° respectively. However, we infer a separation of 3.62+0.11-0.30 mas and a position angle of 73+9-11°. Our analysis thus implies that the binary system lies at a distance of 368+38-13 pc, in agreement with recent spectrophotometric estimates, but significantly larger than the Hipparcos value of 258+41-31 pc.
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- 2007
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23. Constraining the wind launching region in Herbig Ae stars: AMBER/VLTI spectroscopy of HD104237
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E. Tatulli, A. Isella, A. Natta, L. Testi, A. Marconi, F. Malbet, P. Stee, R. G. Petrov, F. Millour, A. Chelli, G. Duvert, P. Antonelli, U. Beckmann, Y. Bresson, M. Dugué, S. Gennari, L. Glück, P. Kern, S. Lagarde, E. Le Coarer, F. Lisi, K. Perraut, P. Puget, F. Rantakyrö, S. Robbe-Dubois, A. Roussel, G. Weigelt, G. Zins, M. Accardo, B. Acke, K. Agabi, E. Altariba, B. Arezki, E. Aristidi, C. Baffa, J. Behrend, T. Blöcker, S. Bonhomme, S. Busoni, F. Cassaing, J.-M. Clausse, J. Colin, C. Connot, A. Delboulbé, A. Domiciano de Souza, T. Driebe, P. Feautrier, D. Ferruzzi, T. Forveille, E. Fossat, R. Foy, D. Fraix-Burnet, A. Gallardo, E. Giani, C. Gil, A. Glentzlin, M. Heiden, M. Heininger, O. Hernandez Utrera, K.-H. Hofmann, D. Kamm, M. Kiekebusch, S. Kraus, D. Le Contel, J.-M. Le Contel, T. Lesourd, B. Lopez, M. Lopez, Y. Magnard, G. Mars, G. Martinot-Lagarde, P. Mathias, P. Mège, J.-L. Monin, D. Mouillet, D. Mourard, E. Nussbaum, K. Ohnaka, J. Pacheco, C. Perrier, Y. Rabbia, S. Rebattu, F. Reynaud, A. Richichi, A. Robini, M. Sacchettini, D. Schertl, M. Schöller, W. Solscheid, A. Spang, P. Stefanini, M. Tallon, I. Tallon-Bosc, D. Tasso, F. Vakili, O. von der Lühe, J.-C. Valtier, M. Vannier, N. Ventura, Laboratoire Hippolyte Fizeau (FIZEAU), Université Nice Sophia Antipolis (... - 2019) (UNS), Université Côte d'Azur (UCA)-Université Côte d'Azur (UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de la Côte d'Azur, Université Côte d'Azur (UCA)-Centre National de la Recherche Scientifique (CNRS), Galilée (Galilée), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de la Côte d'Azur, Université Côte d'Azur (UCA)-Université Côte d'Azur (UCA)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Cosmologie, Astrophysique Stellaire & Solaire, de Planétologie et de Mécanique des Fluides (CASSIOPEE), Laboratoire Gemini (LG), COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de la Côte d'Azur, Université Côte d'Azur (UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-Centre National de la Recherche Scientifique (CNRS), and Université Côte d'Azur (UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Centre National de la Recherche Scientifique (CNRS)
- Subjects
Physics ,010308 nuclear & particles physics ,Astrophysics::High Energy Astrophysical Phenomena ,Near-infrared spectroscopy ,Astronomical unit ,Continuum (design consultancy) ,Astrophysics (astro-ph) ,FOS: Physical sciences ,Astronomy and Astrophysics ,Astrophysics ,Astrophysics::Cosmology and Extragalactic Astrophysics ,01 natural sciences ,Stars ,[SDU]Sciences of the Universe [physics] ,Space and Planetary Science ,0103 physical sciences ,Peak intensity ,Astrophysics::Solar and Stellar Astrophysics ,Astrophysics::Earth and Planetary Astrophysics ,Spectral resolution ,Spectroscopy ,010303 astronomy & astrophysics ,Astrophysics::Galaxy Astrophysics ,Line (formation) - Abstract
We investigate the origin of the $\mathrm{Br}\gamma$ emission of the Herbig Ae star HD104237 on Astronomical Unit (AU) scales. Using AMBER/VLTI at a spectral resolution R=1500 spatially resolve the emission in both the BrGamma line and the adjacent continuum. The visibility does not vary between the continuum and the BrGamma line, even though the line is strongly detected in the spectrum, with a peak intensity 35% above the continuum. This demonstrates that the line and continuum emission have similar size scales. We assume that the K-band continuum excess originates in a ``puffed-up'' inner rim of the circumstellar disk, and discuss the likely origin of BrGamma. We conclude that this emission most likely arises from a compact disk wind, launched from a region 0.2-0.5 AU from the star, with a spatial extent similar to that of the near infrared continuum emission region, i.e, very close to the inner rim location., Comment: 4 pages, 2 figures, accepted in A&A
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- 2006
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24. Learning health informatics and telematics by web_DKN based knowledge construction and discovery
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U, Giani, E, Giani, A, Lamura, and P, Martone
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Education, Distance ,Internet ,Models, Educational ,Italy ,Humans ,Medical Informatics - Published
- 2000
25. LonGSp: the Gornergrat Longslit Infrared Spectrometer
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E. Giani, Franco Lisi, V. Biliotti, L. Vanzi, Leslie K. Hunt, M. Sozzi, Alessandro Marconi, Sandro Gennari, G. Marcucci, Filippo Mannucci, and Carlo Baffa
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Physics ,Spectrometer ,Pixel ,business.industry ,Astrophysics (astro-ph) ,Detector ,Infrared telescope ,FOS: Physical sciences ,General Physics and Astronomy ,Field of view ,Astrophysics ,Grating ,Cardinal point ,Optics ,Observatory ,business - Abstract
We present a near-infrared cooled grating spectrometer that has been developed at the Arcetri Astrophysical Observatory for the 1.5 m Infrared Telescope at Gornergrat (TIRGO). The spectrometer is equipped with cooled reflective optics and a grating in Littrow configuration. The detector is an engineering grade Rockwell NICMOS3 array (256x256 pixels of 40 $\mu$m). The scale on the focal plane is 1.73 arcsec/pixel and the field of view along the slit is 70 arcsec. The accessible spectral range is 0.95-2.5 $\mu$m with a dispersion, at first order, of about 11.5 angstroms/pixel. This paper presents a complete description of the instrument, including its optics and cryo-mechanical system, along with astronomical results from test observations, started in 1994. Since January 1996, LonGSp is offered to TIRGO users and employed in several Galactic and extragalactic programs., Comment: 5 pages LaTeX with 5 eps figures (included). To appear in Astronomy and Astrophysics, Supp. Require LaTeX style l-aa (from A&A)
- Published
- 1997
26. Diets Rich in Saturated, Monounsaturated and Polyunsaturated Fatty Acids Differently Affect Plasma Lipids, Platelet and Arterial Wall Eicosanoids in Rabbits
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I. Masi, Corrado L. Galli, E. Giani, Cesare R. Sirtori, and Elena Tremoli
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Male ,Platelet Aggregation ,Thromboxane ,Dietary lipid ,Medicine (miscellaneous) ,Biology ,Animals ,Platelet ,Food science ,Aorta ,Phospholipids ,Triglycerides ,Unsaturated fatty acid ,chemistry.chemical_classification ,Nutrition and Dietetics ,Fatty Acids ,digestive, oral, and skin physiology ,food and beverages ,Dietary Fats ,Epoprostenol ,Lipids ,Thromboxane B2 ,Cholesterol ,chemistry ,Biochemistry ,Saturated fatty acid ,Fatty Acids, Unsaturated ,lipids (amino acids, peptides, and proteins) ,Rabbits ,Lipoproteins, HDL ,Corn oil ,Olive oil ,Polyunsaturated fatty acid - Abstract
New Zealand male rabbits, on a moderate dietary fat intake (10.2% w/w) received, as the major dietary lipid, butter, olive oil and corn oil, respectively, for a period of 8 weeks. At the end of the dietary treatment, plasma total cholesterol was significantly decreased in the corn oil group, compared to butter, whereas the olive-oil-consuming rabbits had an intermediate cholesterolemia; the corn oil and olive oil groups had significantly elevated high-density lipoprotein (HDL) cholesterolemia, compared to the butter group. Maximal platelet aggregability, with collagen and arachidonic acid, did not appear to differ in the three treatment groups. Thromboxane B2 release in the sera of treated rabbits was slightly higher after corn oil administration. The arterial release of prostacyclin (PGI2), tested by perfusing platelet-rich plasma through the aorta of donor rabbits, was lowest in the corn oil group. Corn oil is the most effective dietary fat in reducing cholesterolemia, but it may also reduce PGI2 release from arteries. Butter has the most unfavorable effect on lipidemia and HDL-cholesterol, whereas dietary olive oil shows an intermediate lipid-lowering activity but preserves arterial PGI2 production.
- Published
- 1986
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27. Effects of CDP-choline on platelet aggregation and the antiaggregatory activity of arterial wall in the rat
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E. Giani, Corrado L. Galli, and I. Masi
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Male ,Cytidine Diphosphate Choline ,Time Factors ,Platelet Aggregation ,Thromboxane ,Aorta, Thoracic ,In Vitro Techniques ,Pharmacology ,Epithelium ,Choline ,chemistry.chemical_compound ,medicine.artery ,medicine ,Animals ,Thoracic aorta ,Platelet ,Aorta ,Biological activity ,Arteries ,Epoprostenol ,Rats ,Perfusion ,Thromboxane B2 ,chemistry ,Anesthesia ,Citicoline ,medicine.drug - Abstract
The effects of the acute (250 mg/kg) and chronic (250 mg/kg for two weeks) treatments with CDP-choline on platelet aggregation and thromboxane formation and on the platelet antiaggregatory activity of thoracic aorta, have been studied in the rat. The acute administration resulted mainly in reduced platelet reactivity to aggregating agents, with no change of platelet thromboxane formation. The antiaggregatory activity of aortic walls was also concomitantly reduced. After chronic treatment, the major effect was a greater antiaggregatory activity of the vessel wall in respect of the control values, whereas platelet function was not affected. CDP-choline treatment, thus exerts favourable effects especially in the acute treatment, by reducing platelet reactivity.
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- 1986
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28. Sputtered Ni-Cr-based resistors terminated on sputtered aluminum and screeen-printed Pt-Ag conductors
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E. Giani and S.M. Leung
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Thin layers ,Materials science ,Metals and Alloys ,Surfaces and Interfaces ,Sputter deposition ,Surfaces, Coatings and Films ,Electronic, Optical and Magnetic Materials ,law.invention ,law ,Sputtering ,Soldering ,Materials Chemistry ,Composite material ,Resistor ,Thin film ,Temperature coefficient ,Electrical conductor - Abstract
The standard technology to fabricate thin film resistors is to deposit a layer of resistive material, usually by evaporation or sputtering, followed by thin layers of nickel and gold. Gold plating is then used to augment the thickness of the gold layer, typically to 1 μm. The three-layer structure is then selectively etched to yield resistors with terminations suitable for wire bonding and soldering. We have used a somewhat unconventional approach in which a film 1–2 μm thick of aluminum is first sputtered onto 99.5% Al2O3 substrates, then etched to produce the desired conductor pattern. Isotropic (wet) etching is used to produce sloping edges to contact better the Ni-Cr based resistor material which is sputter deposited and patterned using a lift-off technique. We have also combined the thin and thick film technologies by terminating our thin film resistors on Pt-Ag conductors which are screen printed onto the substrate prior to sputter deposition of the resistors. Aluminum terminations can be wire bonded, or, when soldering is required, coated with sputtered or plated nickel. When a layer of suitable adhesion promoter is sputtered between aluminum and nickel, adhesion of aluminum to nickel is greatly improved. The use of a sputtering target made of an Ni-Cr-based alloy has enabled us to obtain resistors in the 50 Ω/□ range which can be mass produced with near-zero temperature coefficient of resistance (TCR). Such resistors show stability within better than 0.02% after 1000 h at 398 K under load. Also reported are resistance spread and shift, due to annealing, as a function of aspect ratio (ratio between length and width of resistor) for both aluminum and Pt-Ag terminations, as well as TCR as a function of annealing temperature.
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- 1986
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29. Thin films of solid electrolyte Ag19I15P2O7 II: Thin film electrolytic cells
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M.R. Arora and E. Giani
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Materials science ,Electrolytic cell ,Charge recovery ,Metals and Alloys ,Analytical chemistry ,chemistry.chemical_element ,Surfaces and Interfaces ,Electrolyte ,Surfaces, Coatings and Films ,Electronic, Optical and Magnetic Materials ,chemistry ,Thin film rechargeable lithium battery ,Cathode material ,Materials Chemistry ,Thin film ,Tellurium - Abstract
Flash-evaporated films of Ag 19 I 15 P 2 O 7 were employed in thin film coulometers (Ag/Ag 19 I 15 P 2 O 7 /Au) and batteries (Ag/Ag 19 I 15 P 2 O 7 /Te). When large current densities, exceeding about 1 mA cm -2 , are employed in transporting silver through the electrolyte films, dendritic growth of the silver deposit occurs and shorting problems arise within a few cycles. At low current densities (not more than 100 μA cm -2 ) the coulometers can be charged and discharged over several hundred cycles without any undesirable effects. When these coulometers are given a “conditioning treatment” their charge recovery behavior is greatly improved. Thin film batteries employing tellurium as the cathode material yielded energy densities of about 0.01–0.02 W h cm -3 . All the electrolytic cells showed good stability when stored over long periods of time in ambient atmosphere.
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- 1980
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30. Dietary heated fat alters and vitamin E restores the thromboxane/prostacyclin balance in the rat
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I. Masi, Corrado L. Galli, and E. Giani
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medicine.medical_specialty ,Thromboxane ,Chemistry ,Vitamin E ,medicine.medical_treatment ,Prostacyclin ,Cell Biology ,Biochemistry ,Endocrinology ,Internal medicine ,medicine ,Balance (ability) ,medicine.drug - Published
- 1986
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31. Enhancement of F-centre colouration during plastic deformation of alkali halides
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P. Camagni, M. Boni, and E. Giani
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Materials science ,Annealing (metallurgy) ,Kinetics ,Mineralogy ,General Chemistry ,Activation energy ,Atmospheric temperature range ,Condensed Matter Physics ,Chemical physics ,Radiolysis ,Hardening (metallurgy) ,General Materials Science ,Dislocation ,Deformation (engineering) - Abstract
Stimulated growth of F -centres was observed by irradiating alkali-halide single crystals during uniaxial deformation at controlled rates. Quantitative monitoring of the phenomena was performed for pure KCl at L.N.T. as well as in the range from R.T. to 106°C. Distinct forms for the kinetics of growth were obtained in the two regions. A correlation was also established between the growth of excess colouration and the evolution of stress, in the higher temperature range. The data on the kinetics, stress dependence and temperature dependence suggest that the production of excess F -centres arises from the radiolysis of vacancy-producing debris (possibly, dislocation dipoles) that are also effective agents of hardening. The process is limited by thermally activated annealing, with an activation energy appropriate for free-vacancy migrations. It is suggested that the limiting reaction is a recombination of the excess negative-ion vacancies with an antimorph defect, contained in a complementary type of dislocation debris.
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- 1975
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32. Screen Printed Thick Film Resistors — Better Yields with Shorter Set‐up Times
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E. Giani and J.P. Mathurin
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Engineering ,Yield (engineering) ,Inkwell ,Physics::Instrumentation and Detectors ,business.industry ,Acoustics ,Electrical engineering ,Function (mathematics) ,Condensed Matter Physics ,Atomic and Molecular Physics, and Optics ,Surfaces, Coatings and Films ,Electronic, Optical and Magnetic Materials ,law.invention ,Set (abstract data type) ,law ,Range (statistics) ,Electrical and Electronic Engineering ,Resistor ,business ,Sheet resistance - Abstract
A set of rules is presented for printing thick film resistors, whose implementation minimises losses due to resistors firing too high or too low, and also results in the shortest possible set‐up times. To the best of the authors' knowledge, some of the concepts and relations reported here are nowhere to be found spelled out in the published literature, let alone presented in quantitative form. One example is the relationship between sheet resistance vs resistor length curves and the mesh/emulsion of the screen used to obtain such curves. Another example is the relationship between the choice (or lack of it) of resistors used to set up thickness at the beginning of a print, and the spread in resistance values. Then there are better known relationships, like the dependence of thickness on resistor width or print direction—still no quantitative data are available and the potential relevance of these effects is generally not appreciated. Long set‐up times and yield losses need not exist, as they arise from non‐rigorous printing rules which call for a standard dry thickness (usually 25±3 µm) regardless of resistor dimensions, print direction and ink jar value, and which only call for a range of screen mesh/emulsion values, rather than for specific ones. In fact, for any given sheet resistance vs resistor length curve, only one choice of screen mesh/emulsion and resistor thickness is logically possible. Also reported are experimental data relating resistor thickness to resistor length as a function of screen mesh/emulsion, resistor width and print direction as well as data on sheet resistance as a function of resistor dry thickness. Finally, results from thirty‐eight production runs are reported and discussed.
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- 1989
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33. Pirprofen in the Treatment of Sports Injuries
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Alberto Ventura, E. Porretti, V. Azzolini, F. Braconaro, P. Volpi, E. Giani, V. Maresca, and U. Garagiola
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Adult ,Male ,medicine.medical_specialty ,Sports injury ,Clinical variables ,Adolescent ,Movement ,medicine.medical_treatment ,Pain ,Biochemistry ,Oral administration ,Pirprofen ,Gastro ,Internal medicine ,Humans ,Multicenter Studies as Topic ,Medicine ,Chemotherapy ,Dose-Response Relationship, Drug ,Phenylpropionates ,biology ,business.industry ,Athletes ,Anti-Inflammatory Agents, Non-Steroidal ,Biochemistry (medical) ,Cell Biology ,General Medicine ,Middle Aged ,biology.organism_classification ,Surgery ,Single centre ,Acute Disease ,Athletic Injuries ,Chronic Disease ,Female ,business ,medicine.drug - Abstract
Patients with sports injuries were treated with pirprofen, a non-steroidal anti-inflammatory drug, in two separate studies. In the single centre study, 39 athletes were treated with 1000 mg/day pirprofen for 2 weeks. In the multicentre study, a further 80 athletes were treated with a variable dosage (600 − 1200 mg/day) until the disappearance of symptoms, but for no longer than 2 weeks. Efficacy was considered excellent or good in 99/119 (83%) of the patients treated. The clinical variables of pain and mobility significantly ( P
- Published
- 1989
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34. Sex differences in platelet thromboxane and arterial prostacyclin production in control and n-6 fatty acid supplemented rats
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I. Masi, Claudio Colombo, E. Giani, and Corrado L. Galli
- Subjects
Blood Platelets ,Male ,medicine.medical_specialty ,Platelet Aggregation ,Thromboxane ,Prostacyclin ,6-Ketoprostaglandin F1 alpha ,Arachidonic Acids ,Biology ,Fatty Acids, Nonesterified ,Biochemistry ,chemistry.chemical_compound ,Endocrinology ,Internal medicine ,medicine ,Animals ,Platelet ,Phospholipids ,chemistry.chemical_classification ,Sex Characteristics ,Arachidonic Acid ,Fatty acid metabolism ,Fatty Acids ,Fatty acid ,Arteries ,Dietary Fats ,Epoprostenol ,Rats ,Thromboxane B2 ,chemistry ,cardiovascular system ,lipids (amino acids, peptides, and proteins) ,Arachidonic acid ,Female ,Cholesterol Esters ,Eicosanoid Production ,medicine.drug - Abstract
Sex differences in eicosanoid production in platelets and vessel walls have been studied in control and n-6 fatty acid supplemented rats. In platelet rich plasma (PRP) of control female rats, arachidonic acid (AA) levels in phospholipids (PL), thromboxane B2 (TxB2) formation following collagen stimulation and aggregatory responses to collagen were higher than in PRP of male rats. 6 keto PGF1 alpha release from PRP-perfused isolated aortas were the same for both sexes, but the antiaggregatory activity of the wall was higher in males than in females, in association with a greater sensitivity of male platelets to prostacyclin. The administration of n-6 fatty acid supplements increased AA level in PL, TxB2 production and aggregation only in male platelets. Production of 6 keto PGF1 alpha and the antiaggregatory activity of aortic walls were reduced after dietary treatment in males, but biochemical and functional parameters were not correlated in females. The results indicate complex sex-related differences in fatty acid metabolism and eicosanoid production, and in responses to n-6 dietary fatty acids in platelets and the vascular system in the rat.
- Published
- 1984
35. [Jaundice caused by ajmaline: pathogenetic theory concerning 5 cases]
- Author
-
E, Giani, C, Cestari, A, Lomazzi, S, Magni, P, Pioltelli, L, Ratti, and C A, Dinelli
- Subjects
Adult ,Male ,Ajmaline ,Drug Combinations ,Barbiturates ,Humans ,Jaundice ,Arrhythmias, Cardiac ,Female ,Middle Aged ,Anti-Arrhythmia Agents ,Aged - Published
- 1981
36. [Preventive medicine in secondary spondyloarthrosis caused by chronic microtraumatism in helicopter personnel]
- Author
-
P, Lanciani and E, Giani
- Subjects
Occupational Diseases ,Aircraft ,Spinal Injuries ,Arthritis ,Chronic Disease ,Posture ,Aerospace Medicine ,Humans ,Spinal Diseases - Abstract
After an examination of the three operational stages in the modern concept of preventive medicine, the main pathogenetic cofactors in secondary arthrosis following chronic microtraumatisation are identified, described and evaluated in order to establish the correct preventive approach to the condition in helicopter pilots.
- Published
- 1983
37. Heated fat, vitamin E and vascular eicosanoids
- Author
-
I. Masi, Corrado L. Galli, and E. Giani
- Subjects
Blood Platelets ,Male ,medicine.medical_specialty ,Hot Temperature ,Time Factors ,Platelet Aggregation ,Thromboxane ,medicine.medical_treatment ,Prostacyclin ,6-Ketoprostaglandin F1 alpha ,In Vitro Techniques ,Biochemistry ,chemistry.chemical_compound ,Internal medicine ,medicine ,Animals ,Vitamin E ,Platelet ,Nutritional Physiological Phenomena ,Cooking ,Aorta ,chemistry.chemical_classification ,Triglyceride ,Chemistry ,Organic Chemistry ,Body Weight ,Fatty Acids ,Fatty acid ,Thromboxanes ,Cell Biology ,Organ Size ,Dietary Fats ,Lipids ,Diet ,Rats ,Thromboxane B2 ,Endocrinology ,Fatty Acids, Unsaturated ,lipids (amino acids, peptides, and proteins) ,Eicosanoid Production ,Lipidology ,medicine.drug - Abstract
A semisynthetic diet containing adequate amounts of vitamin E and 10% (w/w) of a mixture of polyunsaturated oils subjected to heating and characterized by elevated indexes of thermal alteration (polar component, dimer triglyceride, altered triglyceride contents and reduced alpha-tocopherol levels) was fed to growing male rats for a period of eight weeks. It resulted in a selective alteration of the production of vascular eicosanoids (elevation of platelet thromboxane formation and decrease of vascular prostacyclin release) compared to the values found in rats fed a diet containing a fresh mixture of polyunsaturated oils. Major nutritional parameters, plasma lipids and the fatty acid profiles of plasma, liver and heart lipids were not different in the two groups of animals. Supplementation of an excess vitamin E (300 mg/kg) to the diet containing heated fat neutralized the adverse effects of heated fat on vascular eicosanoid production.
- Published
- 1985
38. Platelets from aged rats aggregate more, but are more sensitive to prostacyclin
- Author
-
I. Masi, E. Giani, and Corrado L. Galli
- Subjects
Senescence ,Blood Platelets ,Male ,medicine.medical_specialty ,Aging ,Platelet Aggregation ,Physiology ,Thromboxane ,Prostacyclin ,Aorta, Thoracic ,6-Ketoprostaglandin F1 alpha ,Biology ,Biochemistry ,Endocrinology ,Internal medicine ,Blood plasma ,medicine ,Cyclic AMP ,Animals ,Platelet ,Phospholipids ,chemistry.chemical_classification ,Fatty Acids ,Fatty acid ,Rats, Inbred Strains ,Epoprostenol ,Rats ,Thromboxane B2 ,chemistry ,Eicosanoid ,lipids (amino acids, peptides, and proteins) ,Cholesterol Esters ,Collagen ,Perfusion ,medicine.drug - Abstract
The balance between vascular eicosanoids has been explored in young (1 month of age) and aged (11 month of age) rats. PRP from mature rats was more reactive to collagen (lower threshold, greater amplitude of aggregation curve and higher TxB2 formation) than PRP from young animals. Release of 6-keto-PGF1α from PRP-perfused isolated aortas (pg/ul) was higher and the inhibition of PRP aggregation after perfusion correspondingly greater, in mature rats. Platelets from aged rats were more sensitive to exogenous prostacyclin (higher inhibition of aggregation and greater accumulation of cAMP). The fatty acid compositions of plasma and platelet lipids were not different in the two age groups. Compensatory mechanisms were operating in the aged rats, counteracting the greater platelet aggregability with higher vascular prostacyclin production and greater sensitivity of platelets to this eicosanoid.
- Published
- 1985
39. Oral polyunsaturated phosphatidylcholine reduces platelet lipid and cholesterol contents in healthy volunteers
- Author
-
Cesare R. Sirtori, Paola Maderna, Gemma Gianfranceschi, E. Giani, Corrado L. Galli, and Elena Tremoli
- Subjects
Adult ,Blood Glucose ,Blood Platelets ,Male ,medicine.medical_specialty ,Platelet Aggregation ,Linoleic acid ,Phospholipid ,Administration, Oral ,Biochemistry ,chemistry.chemical_compound ,High-density lipoprotein ,Reference Values ,Internal medicine ,medicine ,Humans ,Cholesterol ,Organic Chemistry ,Cell Biology ,Epoprostenol ,Lipids ,Thromboxane B2 ,Endocrinology ,chemistry ,Platelet-rich plasma ,Low-density lipoprotein ,Fatty Acids, Unsaturated ,Phosphatidylcholines ,lipids (amino acids, peptides, and proteins) ,Lipoprotein - Abstract
The effects of orally administered polyunsaturated phosphatidylcholine (PPC) on plasma lipids, lipoproteins and platelet function and composition were studied in seven healthy male volunteers. PPC (Nattermann & Cie, GmbH, Cologne, Federal Republic of Germany), 10 g/day, was given for a 6-week period after a 4-week wash out; laboratory tests were repeated after a further 4-week period after the end of treatment. PPC did not appear, during treatment, to modify the levels of plasma total cholesterol and triglycerides. High density lipoprotein (HDL) cholesterol levels were, however, increased after six weeks of PPC. The most dramatic changes occurred in platelet membrane composition: the total lipid/total protein and the cholesterol/protein ratios were reduced significantly, whereas increases of the phospholipid/total lipid ratio and of the linoleic acid membrane content were observed. Platelet function tests, both in whole blood and in platelet rich plasma, were not modified. Similarly, the thromboxane B2 formation after standard stimuli and the sensitivity to exogenous prostaglandin I2 also were unchanged. During the final wash out period following treatment, a reduction of plasma total and low density lipoprotein (LDL) cholesterol levels also was recorded. PPC appears to be capable of modulating lipid exchanges between cell membranes and the plasma compartment.
- Published
- 1985
40. [Dietary factors and risk of atherosclerosis]
- Author
-
C, Galli, E, Giani, and I, Masi
- Subjects
Risk ,Cholesterol ,Arteriosclerosis ,Humans ,Dietary Fats ,Diet - Published
- 1984
41. Precursor-Product Relationship in Vascular Eicosanoid Formation after Manipulation of Dietary Fatty Acids in Experimental Animals
- Author
-
Corrado L. Galli, I. Masi, and E. Giani
- Subjects
chemistry.chemical_classification ,chemistry.chemical_compound ,chemistry ,Eicosanoid ,Essential fatty acid ,Biochemistry ,Dietary Fatty Acid ,Fatty acid ,Prostaglandin ,lipids (amino acids, peptides, and proteins) ,Arachidonic acid ,Long chain ,Polyunsaturated fatty acid - Abstract
The metabolic relationship between the long chain polyunsaturated fatty acid (PUFA), arachidonic acid (AA), and the prostaglandin system was discovered two decades ago. Although information on the eicosanoid family has considerably grown since then, our understanding of the complex relationships between the intake of the fatty acid precursors with the diet and the balance in the formation of various eicosanoids in a given tissue or district is still quite limited.
- Published
- 1985
- Full Text
- View/download PDF
42. Effects of Iloprost Treatment in the Rat on Prostacyclin Release from Isolated Aortas
- Author
-
E. Giani, C. Mosconi, Corrado L. Galli, and I. Masi
- Subjects
Platelet reactivity ,Chemistry ,cardiovascular system ,medicine ,lipids (amino acids, peptides, and proteins) ,Platelet ,Endogeny ,Prostacyclin ,Pharmacology ,In vitro ,medicine.drug ,Iloprost - Abstract
The observation of an enhanced platelet reactivity after infusion of prostacyclin in clinical studies [1] suggests the possibility that the administration of this compound might inhibit the endogenous release of prostacyclin and, consequently, result in hyperactive platelets. In order to explore this possibility, we have studied the effects of acute and chronic administration of Iloprost in the rat, on the release of 6-keto-PGF1α from in vitro perfused aortas.
- Published
- 1987
- Full Text
- View/download PDF
43. [Pyloric stenosis from caustics]
- Author
-
E, GIANI
- Subjects
Caustics ,Constriction, Pathologic ,Pyloric Stenosis ,Pylorus - Published
- 1956
44. [ON THE BEHAVIOR OF STROMAL METACHROMASIA AND MAST CELLS IN TUMORS OF MESENCHYMAL ORIGIN]
- Author
-
E, GIANI
- Subjects
Neoplasms, Connective Tissue ,Osteosarcoma ,Staining and Labeling ,Breast Neoplasms ,Sarcoma ,Kidney Neoplasms ,Parotid Neoplasms ,Connective Tissue ,Head and Neck Neoplasms ,Neoplasms ,Intestinal Neoplasms ,Uterine Neoplasms ,Pathology ,Humans ,Female ,Mast Cells ,Coloring Agents - Published
- 1964
45. [Value of Rehn's test in cranial trauma, preliminary note]
- Author
-
E, GIANI and M, SCARANO
- Subjects
Brain Injuries ,Brain ,Humans ,Wounds and Injuries ,Shock - Published
- 1956
46. [Effect of pentothal-curare on peristalsis of the intestine in vitro]
- Author
-
E, GIANI
- Subjects
Intestines ,Barbiturates ,Peristalsis ,In Vitro Techniques ,Thiopental ,Curare - Published
- 1951
47. [Prevention of peritoneal adhesions by various steroids (cortisone, prednisone and triamcinolone); experimental studies]
- Author
-
M, DELLA CORTE and E, GIANI
- Subjects
Cortisone ,Fludrocortisone ,Prednisolone ,Prednisone ,Steroids ,Tissue Adhesions ,Connective Tissue Diseases ,Peritoneal Diseases ,Triamcinolone - Published
- 1958
48. [Injury of the left cerebral hemisphere by the trident from an underwater fishing gun]
- Author
-
E, GIANI
- Subjects
Brain Injuries ,Humans - Published
- 1960
49. [Fibrocystic mastopathy in a supernumerary breast]
- Author
-
E, GIANI
- Subjects
Breast Diseases ,Nipples ,Humans ,Female ,Fibrocystic Breast Disease - Published
- 1960
50. [Data on the effect of various antibiotics on the process of blood coagulation]
- Author
-
E, GIANI
- Subjects
Humans ,Dermatologic Agents ,Antibiotics, Antitubercular ,Blood Coagulation ,Anti-Bacterial Agents ,Erythromycin - Published
- 1958
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