Zobrazeno 1 - 10
of 423
pro vyhledávání: '"Giani E."'
Autor:
Scandariato, G., Borsa, F., Sicilia, D., Malavolta, L., Biazzo, K., Bonomo, A. S., Bruno, G., Claudi, R., Covino, E., Di Marcantonio, P., Esposito, M., Frustagli, G., Lanza, A. F., 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., de Gurtubai, A. Garcia, Ghedina, A., Giacobbe, P., Giani, E., Harutyunyan, A., Hernandez, N., Diaz, M. Hernandez, Knapic, C., Leto, G., Fiorenzano, A. F. Martìnez, Molinari, E., Nascimbeni, V., Pagano, I., Pedani, M., Piotto, G., Poretti, E., Stoev, H.
Publikováno v:
A&A 646, A159 (2021)
The analysis of exoplanetary atmospheres by means of high-resolution spectroscopy is an expanding research field which provides information on chemical composition, thermal structure, atmospheric dynamics and orbital velocity of exoplanets. In this w
Externí odkaz:
http://arxiv.org/abs/2012.10435
Autor:
Carleo, I., Malavolta, L., Lanza, A. F., Damasso, M., Desidera, S., Borsa, F., Mallonn, M., Pinamonti, M., Gratton, R., Alei, E., Benatti, S., Mancini, L., Maldonado, J., Biazzo, K., Esposito, M., Frustagli, G., González-Álvarez, E., Micela, G., Scandariato, G., Sozzetti, A., Affer, L., Bignamini, A., Bonomo, A. S., Claudi, R., Cosentino, R., Covino, E., Fiorenzano, A. F. M., Giacobbe, P., Harutyunyan, A., Leto, G., Maggio, A., Molinari, E., Nascimbeni, V., Pagano, I., Pedani, M., Piotto, G., Poretti, E., Rainer, M., Redfield, S., Baffa, C., Baruffolo, A., Buchschacher, N., Billotti, V., Cecconi, M., Falcini, G., Fantinel, D., Fini, L., Galli, A., Ghedina, A., Ghinassi, F., Giani, E., Gonzalez, C., Gonzalez, M., Guerra, J., Diaz, M. Hernandez, Hernandez, N., Iuzzolino, M., Lodi, M., Oliva, E., Origlia, L., Ventura, H. Perez, Puglisi, A., Riverol, C., Riverol, L., Juan, J. San, Sanna, N., Scuderi, S., Seemann, U., Sozzi, M., Tozzi, A.
Publikováno v:
A&A 638, A5 (2020)
The existence of hot Jupiters is still not well understood. Two main channels are thought to be responsible for their current location: a smooth planet migration through the proto-planetary disk or the circularization of an initial high eccentric orb
Externí odkaz:
http://arxiv.org/abs/2002.10562
Autor:
Claudi, R., Benatti, S., Carleo, I., Ghedina, A., Guerra, J., Ghinassi, F., Harutyunyan, A., Micela, G., Molinari, E., Oliva, E., Rainer, M., Tozzi, A., Baffa, C., Baruffolo, A., Biliotti, V., Buchschacher, N., Cecconi, M., Cosentino, R., Falcini, G., Fantinel, D., Fini, L., Giani, E., Gonzalez--Alvarez, E., Gonzalez, M., Gonzalez, C., Gratton, R., Hernandez, N., Iuzzolino, M., Lodi, M., Malavolta, L., Maldonado, J., Origlia, L., Puglisi, A., Sanna, N., Juan, J. San, Scuderi, S., Seemann, U., Sozzetti, A., Sozzi, M., Ventura, H. Perez, Diaz, M. Hernandez, Galli, A., Riverol, L., Riverol, C.
GIARPS (GIAno \& haRPS) is a project devoted to have on the same focal station of the Telescopio Nazionale Galileo (TNG) both high resolution spectrographs, HARPS-N (VIS) and GIANO-B (NIR), working simultaneously. This could be considered the first a
Externí odkaz:
http://arxiv.org/abs/1808.03184
Autor:
Carleo, I., Benatti, S., Lanza, A. F., Gratton, R., Claudi, R., Desidera, S., Mace, G. N., Messina, S., Sanna, N., Sissa, E., Ghedina, A., Ghinassi, F., Guerra, J., Harutyunyan, A., Micela, G., Molinari, E., Oliva, E., Tozzi, A., Baffa, C., Baruffolo, A., Bignamini, A., Buchschacher, N., Cecconi, M., Cosentino, R., Endl, M., Falcini, G., Fantinel, D., Fini, L., Fugazza, D., Galli, A., Giani, E., González, C., González-Álvarez, E., González, M., Hernandez, N., Diaz, M. Hernandez, Iuzzolino, M., Kaplan, K. F., Kidder, B. T., Lodi, M., Malavolta, L., Maldonado, J., Origlia, L., Ventura, H. Perez, Puglisi, A., Rainer, M., Riverol, L., Riverol, C., Juan, J. San, Scuderi, S., Seemann, U., Sokal, K. R., Sozzetti, A., Sozzi, M.
Publikováno v:
A&A 613, A50 (2018)
Context. Stellar activity is currently challenging the detection of young planets via the radial velocity (RV) technique. Aims. We attempt to definitively discriminate the nature of the RV variations for the young active K5 star BD+20 1790, for which
Externí odkaz:
http://arxiv.org/abs/1805.01281
Autor:
Levin, L., Armour, W., Baffa, C., Barr, E., Cooper, S., Eatough, R., Ensor, A., Giani, E., Karastergiou, A., Karuppusamy, R., Keith, M., Kramer, M., Lyon, R., Mackintosh, M., Mickaliger, M., van Nieuwpoort, R, Pearson, M., Prabu, T., Roy, J., Sinnen, O., Spitler, L., Spreeuw, H., Stappers, B. W., van Straten, W., Williams, C., Wang, H., Wiesner, K.
The Square Kilometre Array will be an amazing instrument for pulsar astronomy. While the full SKA will be sensitive enough to detect all pulsars in the Galaxy visible from Earth, already with SKA1, pulsar searches will discover enough pulsars to incr
Externí odkaz:
http://arxiv.org/abs/1712.01008
Autor:
Claudi, R., Benatti, S., Carleo, I., Ghedina, A., Guerra, J., Micela, G., Molinari, E., Oliva, E., Rainer, M., Tozzi, A., Baffa, C., Baruffolo, A., Buchschacher, N., Cecconi, M., Cosentino, R., Fantinel, D., Fini, L., Ghinassi, F., Giani, E., Gonzalez, E., Gonzalez, M., Gratton, R., Harutyunyan, A., Hernandez, N., Lodi, M., Malavolta, L., Maldonado, J., Origlia, L., Sanna, N., Sanjuan, J., Scuderi, S., Seemann, U., Sozzetti, A., Ventura, H. Perez, Diaz, M. Hernandez, Galli, A., Gonzalez, C., Riverol, L., Riverol, C.
Since 2012, thanks to the installation of the high resolution echelle spectrograph in the optical range HARPS-N, the Italian telescope TNG (La Palma) became one of the key facilities for the study of the extrasolar planets. In 2014 TNG also offered G
Externí odkaz:
http://arxiv.org/abs/1707.04553
Autor:
Origlia, L., Oliva, E., Sanna, N., Mucciarelli, A., Dalessandro, E., Scuderi, S., Baffa, C., Biliotti, V., Carbonaro, L., Falcini, G., Giani, E., Iuzzolino, M., Massi, F., Sozzi, M., Tozzi, A., Ghedina, A., Ghinassi, F., Lodi, M., Harutyunyan, A., Pedani, M.
The Scutum complex in the inner disk of the Galaxy has a number of young star clusters dominated by red supergiants that are heavily obscured by dust extinction and observable only at infrared wavelengths. These clusters are important tracers of the
Externí odkaz:
http://arxiv.org/abs/1510.06870
Autor:
Oliva, E., Origlia, L., Scuderi, S., Benatti, S., Carleo, I., Lapenna, E., Mucciarelli, A., Baffa, C., Biliotti, V., Carbonaro, L., Falcini, G., Giani, E., Iuzzolino, M., Massi, F., Sanna, N., Sozzi, M., Tozzi, A, Ghedina, A., Ghinassi, F., Lodi, M., Harutyunyan, A., Pedani, M.
Publikováno v:
A&A 581, A47 (2015)
Aims Determining the intensity of lines and continuum airglow emission in the H-band is important for the design of faint-object infrared spectrographs. Existing spectra at low/medium resolution cannot disentangle the true sky-continuum from instrume
Externí odkaz:
http://arxiv.org/abs/1506.09004
Autor:
Tinetti, Giovanna, Drossart, Pierre, Eccleston, Paul, Hartogh, Paul, Isaak, Kate, Linder, Martin, Lovis, Christophe, Micela, Giusi, Ollivier, Marc, Puig, Ludovic, Ribas, Ignasi, Snellen, Ignas, Allard, Bruce Swinyard. France, Barstow, Joanna, Cho, James, Coustenis, Athena, Cockell, Charles, Correia, Alexandre, Decin, Leen, de Kok, Remco, Deroo, Pieter, Encrenaz, Therese, Forget, Francois, Glasse, Alistair, Griffith, Caitlin, Guillot, Tristan, Koskinen, Tommi, Lammer, Helmut, Leconte, Jeremy, Maxted, Pierre, Mueller-Wodarg, Ingo, Nelson, Richard, North, Chris, Pallé, Enric, Pagano, Isabella, Piccioni, Guseppe, Pinfield, David, Selsis, Franck, Sozzetti, Alessandro, Stixrude, Lars, Tennyson, Jonathan, Turrini, Diego, Beaulieu, Mariarosa Zapatero-Osorio. Jean-Philippe, Grodent, Denis, Guedel, Manuel, Luz, David, Nørgaard-Nielsen, Hans Ulrik, Ray, Tom, Rickman, Hans, Selig, Avri, Banaszkiewicz, Mark Swain. Marek, Barlow, Mike, Bowles, Neil, Branduardi-Raymont, Graziella, Foresto, Vincent Coudé du, Gerard, Jean-Claude, Gizon, Laurent, Hornstrup, Allan, Jarchow, Christopher, Kerschbaum, Franz, Kovacs, Géza, Lagage, Pierre-Olivier, Lim, Tanya, Lopez-Morales, Mercedes, Malaguti, Giuseppe, Pace, Emanuele, Pascale, Enzo, Vandenbussche, Bart, Wright, Gillian, Adriani, Gonzalo Ramos Zapata. Alberto, Azzollini, Ruymán, Balado, Ana, Bryson, Ian, Burston, Raymond, Colomé, Josep, Crook, Martin, Di Giorgio, Anna, Griffin, Matt, Hoogeveen, Ruud, Ottensamer, Roland, Irshad, Ranah, Middleton, Kevin, Morgante, Gianluca, Pinsard, Frederic, Rataj, Mirek, Reess, Jean-Michel, Savini, Giorgio, Schrader, Jan-Rutger, Stamper, Richard, Abe, Berend Winter. L., Abreu, M., Achilleos, N., Ade, P., Adybekian, V., Affer, L., Agnor, C., Agundez, M., Alard, C., Alcala, J., Prieto, C. Allende, Floriano, F. J. Alonso, Altieri, F., Iglesias, C. A. Alvarez, Amado, P., Andersen, A., Aylward, A., Baffa, C., Bakos, G., Ballerini, P., Banaszkiewicz, M., Barber, R. J., Barrado, D., Barton, E. J., Batista, V., Bellucci, G., Avilés, J. A. Belmonte, Berry, D., Bézard, B., Biondi, D., Błęcka, M., Boisse, I., Bonfond, B., Bordé, P., Börner, P., Bouy, H., Brown, L., Buchhave, L., Budaj, J., Bulgarelli, A., Burleigh, M., Cabral, A., Capria, M. T., Cassan, A., Cavarroc, C., Cecchi-Pestellini, C., Cerulli, R., Chadney, J., Chamberlain, S., Charnoz, S., Jessen, N. Christian, Ciaravella, A., Claret, A., Claudi, R., Coates, A., Cole, R., Collura, A., Cordier, D., Covino, E., Danielski, C., Damasso, M., Deeg, H. J., Delgado-Mena, E., Del Vecchio, C., Demangeon, O., De Sio, A., De Wit, J., Dobrijévic, M., Doel, P., Dominic, C., Dorfi, E., Eales, S., Eiroa, C., Contreras, M. Espinoza, Esposito, M., Eymet, V., Fabrizio, N., Fernández, M., Castella, B. Femenía, Figueira, P., Filacchione, G., Fletcher, L., Focardi, M., Fossey, S., Fouqué, P., Frith, J., Galand, M., Gambicorti, L., Gaulme, P., López, R. J. García, Garcia-Piquer, A., Gear, W., Gerard, J. -C., Gesa, L., Giani, E., Gianotti, F., Gillon, M., Giro, E., Giuranna, M., Gomez, H., Gomez-Leal, I., Hernandez, J. Gonzalez, Merino, B. González, Graczyk, R., Grassi, D., Guardia, J., Guio, P., Gustin, J., Hargrave, P., Haigh, J., Hébrard, E., Heiter, U., Heredero, R. L., Herrero, E., Hersant, F., Heyrovsky, D., Hollis, M., Hubert, B., Hueso, R., Israelian, G., Iro, N., Irwin, P., Jacquemoud, S., Jones, G., Jones, H., Justtanont, K., Kehoe, T., Kerschbaum, F., Kerins, E., Kervella, P., Kipping, D., Koskinen, T., Krupp, N., Lahav, O., Laken, B., Lanza, N., Lellouch, E., Leto, G., Goldaracena, J. Licandro, Lithgow-Bertelloni, C., Liu, S. J., Cicero, U. Lo, Lodieu, N., Lognonné, P., Lopez-Puertas, M., Lopez-Valverde, M. A., Rasmussen, I. Lundgaard, Luntzer, A., Machado, P., MacTavish, C., Maggio, A., Maillard, J. -P., Magnes, W., Maldonado, J., Mall, U., Marquette, J. -B., Mauskopf, P., Massi, F., Maurin, A. -S., Medvedev, A., Michaut, C., Miles-Paez, P., Montalto, M., Rodríguez, P. Montañés, Monteiro, M., Montes, D., Morais, H., Morales, J. C., Morales-Calderón, M., Morello, G., Martín, A. Moro, Moses, J., Bedon, A. Moya, Alcaino, F. Murgas, Oliva, E., Orton, G., Palla, F., Pancrazzi, M., Pantin, E., Parmentier, V., Parviainen, H., Ramírez, K. Y. Peña, Peralta, J., Perez-Hoyos, S., Petrov, R., Pezzuto, S., Pietrzak, R., Pilat-Lohinger, E., Piskunov, N., Prinja, R., Prisinzano, L., Polichtchouk, I., Poretti, E., Radioti, A., Ramos, A. A., Rank-Lüftinger, T., Read, P., Readorn, K., López, R. Rebolo, Rebordão, J., Rengel, M., Rezac, L., Rocchetto, M., Rodler, F., Béjar, V. J. Sánchez, Lavega, A. Sanchez, Sanromá, E., Santos, N., Forcada, J. Sanz, Scandariato, G., Schmider, F. -X., Scholz, A., Scuderi, S., Sethenadh, J., Shore, S., Showman, A., Sicardy, B., Sitek, P., Smith, A., Soret, L., Sousa, S., Stiepen, A., Stolarski, M., Strazzulla, G., Tabernero, H. M, Tanga, P., Tecsa, M., Temple, J., Terenzi, L., Tessenyi, M., Testi, L., Thompson, S., Thrastarson, H., Tingley, B. W., Trifoglio, M., Torres, J. Martín, Tozzi, A., Turrini, D., Varley, R., Vakili, F., de Val-Borro, M., Valdivieso, M. L., Venot, O., Villaver, E., Vinatier, S., Viti, S., Waldmann, I., Waltham, D., Ward-Thompson, D., Waters, R., Watkins, C., Watson, D., Wawer, P., Wawrzaszk, A., White, G., Widemann, T., Winek, W., Wiśniowski, T., Yelle, R., Yung, Y., Yurchenko, S. N.
The discovery of almost 2000 exoplanets has revealed an unexpectedly diverse planet population. Observations to date have shown that our Solar System is certainly not representative of the general population of planets in our Milky Way. The key scien
Externí odkaz:
http://arxiv.org/abs/1502.05747
Autor:
Tozzi, A., Oliva, E., Origlia, L., Baffa, C., Biliotti, V., Falcini, G., Giani, E., Iuzzolino, M., Massi, F., Sanna, N., Scuderi, S., Sozzi, M.
Giano is a Cryogenic Spectrograph located in T.N.G. (Spain) and commisioned in 2013. It works in the range 950-2500 nm with a resolving power of 50000. This instrument was designed and built for direct feeding from the telescope [2]. However, due to
Externí odkaz:
http://arxiv.org/abs/1407.3126