Zobrazeno 1 - 10
of 120
pro vyhledávání: '"Micela, Giusi"'
Autor:
Kashyap, Vinay L., Guarcello, Mario G., Wright, Nicholas J., Drake, Jeremy J., Flaccomio, Ettore, Aldcroft, Tom L., Colombo, Juan F. Albacete, Briggs, Kevin, Damiani, Francesco, Drew, Janet E., Martin, Eduardo L., Micela, Giusi, Naylor, Tim, Sciortino, Salvatore
We have devised a predominantly Naive Bayes method to classify the optical/IR matches to X-ray sources detected by Chandra in the Cygnus OB2 association into foreground, member, and background objects. We employ a variety of X-ray, optical, and infra
Externí odkaz:
http://arxiv.org/abs/2306.06832
Autor:
Crepp, Justin R., Crass, Jonathan, King, David, Bechter, Andrew, Bechter, Eric, Ketterer, Ryan, Reynolds, Robert, Hinz, Philip, Kopon, Derek, Cavalieri, David, Fantano, Louis, Koca, Corina, Onuma, Eleanya, Stapelfeldt, Karl, Thomes, Joseph, Wall, Sheila, Macenka, Steven, McGuire, James, Korniski, Ronald, Zugby, Leonard, Eisner, Joshua, Gaudi, B S., Hearty, Fred, Kratter, Kaitlin, Kuchner, Marc, Micela, Giusi, Nelson, Matthew, Pagano, Isabella, Quirrenbach, Andreas, Schwab, Christian, Skrutskie, Michael, Sozzetti, Alessandro, Woodward, Charles, Zhao, Bo
We are developing a stable and precise spectrograph for the Large Binocular Telescope (LBT) named "iLocater." The instrument comprises three principal components: a cross-dispersed echelle spectrograph that operates in the YJ-bands (0.97-1.30 mu m),
Externí odkaz:
http://hdl.handle.net/10150/622805
http://arizona.openrepository.com/arizona/handle/10150/622805
http://arizona.openrepository.com/arizona/handle/10150/622805
Autor:
Carleo, Ilaria, Giacobbe, Paolo, Guilluy, Gloria, Cubillos, Patricio E., Bonomo, Aldo S., Sozzetti, Alessandro, Brogi, Matteo, Gandhi, Siddharth, Fossati, Luca, Turrini, Diego, Biazzo, Katia, Borsa, Francesco, Lanza, Antonino F., Malavolta, Luca, Maggio, Antonio, Mancini, Luigi, Micela, Giusi, Pino, Lorenzo, Poretti, Ennio, Rainer, Monica, Scandariato, Gaetano, Schisano, Eugenio, Andreuzzi, Gloria, Bignamini, Andrea, Cosentino, Rosario, Fiorenzano, Aldo, Harutyunyan, Avet, Molinari, Emilio, Pedani, Marco, Redfield, Seth, Stoev, Hristo
Detections of molecules in the atmosphere of gas giant exoplanets allow us to investigate the physico-chemical properties of the atmospheres. Their inferred chemical composition is used as tracer of planet formation and evolution mechanisms. Currentl
Externí odkaz:
http://arxiv.org/abs/2207.09761
Autor:
Tinetti, Giovanna, Eccleston, Paul, Haswell, Carole, Lagage, Pierre-Olivier, Leconte, Jérémy, Lüftinger, Theresa, Micela, Giusi, Min, Michel, Pilbratt, Göran, Puig, Ludovic, Swain, Mark, Testi, Leonardo, Turrini, Diego, Vandenbussche, Bart, Osorio, Maria Rosa Zapatero, Aret, Anna, Beaulieu, Jean-Philippe, Buchhave, Lars, Ferus, Martin, Griffin, Matt, Guedel, Manuel, Hartogh, Paul, Machado, Pedro, Malaguti, Giuseppe, Pallé, Enric, Rataj, Mirek, Ray, Tom, Ribas, Ignasi, Szabó, Robert, Tan, Jonathan, Werner, Stephanie, Ratti, Francesco, Scharmberg, Carsten, Salvignol, Jean-Christophe, Boudin, Nathalie, Halain, Jean-Philippe, Haag, Martin, Crouzet, Pierre-Elie, Kohley, Ralf, Symonds, Kate, Renk, Florian, Caldwell, Andrew, Abreu, Manuel, Alonso, Gustavo, Amiaux, Jerome, Berthé, Michel, Bishop, Georgia, Bowles, Neil, Carmona, Manuel, Coffey, Deirdre, Colomé, Josep, Crook, Martin, Désjonqueres, Lucile, Díaz, José J., Drummond, Rachel, Focardi, Mauro, Gómez, Jose M., Holmes, Warren, Krijger, Matthijs, Kovacs, Zsolt, Hunt, Tom, Machado, Richardo, Morgante, Gianluca, Ollivier, Marc, Ottensamer, Roland, Pace, Emanuele, Pagano, Teresa, Pascale, Enzo, Pearson, Chris, Pedersen, Søren Møller, Pniel, Moshe, Roose, Stéphane, Savini, Giorgio, Stamper, Richard, Szirovicza, Peter, Szoke, Janos, Tosh, Ian, Vilardell, Francesc, Barstow, Joanna, Borsato, Luca, Casewell, Sarah, Changeat, Quentin, Charnay, Benjamin, Civiš, Svatopluk, Foresto, Vincent Coudé du, Coustenis, Athena, Cowan, Nicolas, Danielski, Camilla, Demangeon, Olivier, Drossart, Pierre, Edwards, Billy N., Gilli, Gabriella, Encrenaz, Therese, Kiss, Csaba, Kokori, Anastasia, Ikoma, Masahiro, Morales, Juan Carlos, Mendonça, João, Moneti, Andrea, Mugnai, Lorenzo, Muñoz, Antonio García, Helled, Ravit, Kama, Mihkel, Miguel, Yamila, Nikolaou, Nikos, Pagano, Isabella, Panic, Olja, Rengel, Miriam, Rickman, Hans, Rocchetto, Marco, Sarkar, Subhajit, Selsis, Franck, Tennyson, Jonathan, Tsiaras, Angelos, Venot, Olivia, Vida, Krisztián, Waldmann, Ingo P., Yurchenko, Sergey, Szabó, Gyula, Zellem, Rob, Al-Refaie, Ahmed, Alvarez, Javier Perez, Anisman, Lara, Arhancet, Axel, Ateca, Jaume, Baeyens, Robin, Barnes, John R., Bell, Taylor, Benatti, Serena, Biazzo, Katia, Błęcka, Maria, Bonomo, Aldo Stefano, Bosch, José, Bossini, Diego, Bourgalais, Jeremy, Brienza, Daniele, Brucalassi, Anna, Bruno, Giovanni, Caines, Hamish, Calcutt, Simon, Campante, Tiago, Canestrari, Rodolfo, Cann, Nick, Casali, Giada, Casas, Albert, Cassone, Giuseppe, Cara, Christophe, Carone, Ludmila, Carrasco, Nathalie, Chioetto, Paolo, Cortecchia, Fausto, Czupalla, Markus, Chubb, Katy L., Ciaravella, Angela, Claret, Antonio, Claudi, Riccardo, Codella, Claudio, Comas, Maya Garcia, Cracchiolo, Gianluca, Cubillos, Patricio, Da Peppo, Vania, Decin, Leen, Dejabrun, Clemence, Delgado-Mena, Elisa, Di Giorgio, Anna, Diolaiti, Emiliano, Dorn, Caroline, Doublier, Vanessa, Doumayrou, Eric, Dransfield, Georgina, Dumaye, Luc, Dunford, Emma, Escobar, Antonio Jimenez, Van Eylen, Vincent, Farina, Maria, Fedele, Davide, Fernández, Alejandro, Fleury, Benjamin, Fonte, Sergio, Fontignie, Jean, Fossati, Luca, Funke, Bernd, Galy, Camille, Garai, Zoltán, García, Andrés, García-Rigo, Alberto, Garufi, Antonio, Sacco, Giuseppe Germano, Giacobbe, Paolo, Gómez, Alejandro, Gonzalez, Arturo, Gonzalez-Galindo, Francisco, Grassi, Davide, Griffith, Caitlin, Guarcello, Mario Giuseppe, Goujon, Audrey, Gressier, Amélie, Grzegorczyk, Aleksandra, Guillot, Tristan, Guilluy, Gloria, Hargrave, Peter, Hellin, Marie-Laure, Herrero, Enrique, Hills, Matt, Horeau, Benoit, Ito, Yuichi, Jessen, Niels Christian, Kabath, Petr, Kálmán, Szilárd, Kawashima, Yui, Kimura, Tadahiro, Knížek, Antonín, Kreidberg, Laura, Kruid, Ronald, Kruijssen, Diederik J. M., Kubelík, Petr, Lara, Luisa, Lebonnois, Sebastien, Lee, David, Lefevre, Maxence, Lichtenberg, Tim, Locci, Daniele, Lombini, Matteo, Lopez, Alejandro Sanchez, Lorenzani, Andrea, MacDonald, Ryan, Magrini, Laura, Maldonado, Jesus, Marcq, Emmanuel, Migliorini, Alessandra, Modirrousta-Galian, Darius, Molaverdikhani, Karan, Molinari, Sergio, Mollière, Paul, Moreau, Vincent, Morello, Giuseppe, Morinaud, Gilles, Morvan, Mario, Moses, Julianne I., Mouzali, Salima, Nakhjiri, Nariman, Naponiello, Luca, Narita, Norio, Nascimbeni, Valerio, Nikolaou, Athanasia, Noce, Vladimiro, Oliva, Fabrizio, Palladino, Pietro, Papageorgiou, Andreas, Parmentier, Vivien, Peres, Giovanni, Pérez, Javier, Perez-Hoyos, Santiago, Perger, Manuel, Pestellini, Cesare Cecchi, Petralia, Antonino, Philippon, Anne, Piccialli, Arianna, Pignatari, Marco, Piotto, Giampaolo, Podio, Linda, Polenta, Gianluca, Preti, Giampaolo, Pribulla, Theodor, Puertas, Manuel Lopez, Rainer, Monica, Reess, Jean-Michel, Rimmer, Paul, Robert, Séverine, Rosich, Albert, Rossi, Loic, Rust, Duncan, Saleh, Ayman, Sanna, Nicoletta, Schisano, Eugenio, Schreiber, Laura, Schwartz, Victor, Scippa, Antonio, Seli, Bálint, Shibata, Sho, Simpson, Caroline, Shorttle, Oliver, Skaf, N., Skup, Konrad, Sobiecki, Mateusz, Sousa, Sergio, Sozzetti, Alessandro, Šponer, Judit, Steiger, Lukas, Tanga, Paolo, Tackley, Paul, Taylor, Jake, Tecza, Matthias, Terenzi, Luca, Tremblin, Pascal, Tozzi, Andrea, Triaud, Amaury, Trompet, Loïc, Tsai, Shang-Min, Tsantaki, Maria, Valencia, Diana, Vandaele, Ann Carine, Van der Swaelmen, Mathieu, Vardan, Adibekyan, Vasisht, Gautam, Vazan, Allona, Del Vecchio, Ciro, Waltham, Dave, Wawer, Piotr, Widemann, Thomas, Wolkenberg, Paulina, Yip, Gordon Hou, Yung, Yuk, Zilinskas, Mantas, Zingales, Tiziano, Zuppella, Paola
Ariel, the Atmospheric Remote-sensing Infrared Exoplanet Large-survey, was adopted as the fourth medium-class mission in ESA's Cosmic Vision programme to be launched in 2029. During its 4-year mission, Ariel will study what exoplanets are made of, ho
Externí odkaz:
http://arxiv.org/abs/2104.04824
Autor:
de Beurs, Zoe L., Vanderburg, Andrew, Shallue, Christopher J., Dumusque, Xavier, Cameron, Andrew Collier, Leet, Christopher, Buchhave, Lars A., Cosentino, Rosario, Ghedina, Adriano, Haywood, Raphaëlle D., Langellier, Nicholas, Latham, David W., López-Morales, Mercedes, Mayor, Michel, Micela, Giusi, Milbourne, Timothy W., Mortier, Annelies, Molinari, Emilio, Pepe, Francesco, Phillips, David F., Pinamonti, Matteo, Piotto, Giampaolo, Rice, Ken, Sasselov, Dimitar, Sozzetti, Alessandro, Udry, Stéphane, Watson, Christopher A.
Exoplanet detection with precise radial velocity (RV) observations is currently limited by spurious RV signals introduced by stellar activity. We show that machine learning techniques such as linear regression and neural networks can effectively remo
Externí odkaz:
http://arxiv.org/abs/2011.00003
Autor:
Ehrenreich, David, Lovis, Christophe, Allart, Romain, Osorio, María Rosa Zapatero, Pepe, Francesco, Cristiani, Stefano, Rebolo, Rafael, Santos, Nuno C., Borsa, Francesco, Demangeon, Olivier, Dumusque, Xavier, Hernández, Jonay I. González, Casasayas-Barris, Núria, Ségransan, Damien, Sousa, Sérgio, Abreu, Manuel, Adibekyan, Vardan, Affolter, Michael, Prieto, Carlos Allende, Alibert, Yann, Aliverti, Matteo, Alves, David, Amate, Manuel, Avila, Gerardo, Baldini, Veronica, Bandy, Timothy, Benz, Willy, Bianco, Andrea, Bolmont, Émeline, Bouchy, François, Bourrier, Vincent, Broeg, Christopher, Cabral, Alexandre, Calderone, Giorgio, Pallé, Enric, Cegla, H. M., Cirami, Roberto, Coelho, João M. P., Conconi, Paolo, Coretti, Igor, Cumani, Claudio, Cupani, Guido, Dekker, Hans, Delabre, Bernard, Deiries, Sebastian, D'Odorico, Valentina, Di Marcantonio, Paolo, Figueira, Pedro, Fragoso, Ana, Genolet, Ludovic, Genoni, Matteo, Santos, Ricardo Génova, Hara, Nathan, Hughes, Ian, Iwert, Olaf, Kerber, Florian, Knudstrup, Jens, Landoni, Marco, Lavie, Baptiste, Lizon, Jean-Louis, Lendl, Monika, Curto, Gaspare Lo, Maire, Charles, Manescau, Antonio, Martins, C. J. A. P., Mégevand, Denis, Mehner, Andrea, Micela, Giusi, Modigliani, Andrea, Molaro, Paolo, Monteiro, Manuel, Monteiro, Mario, Moschetti, Manuele, Müller, Eric, Nunes, Nelson, Oggioni, Luca, Oliveira, António, Pariani, Giorgio, Pasquini, Luca, Poretti, Ennio, Rasilla, José Luis, Redaelli, Edoardo, Riva, Marco, Tschudi, Samuel Santana, Santin, Paolo, Santos, Pedro, Milla, Alex Segovia, Seidel, Julia V., Sosnowska, Danuta, Sozzetti, Alessandro, Spanò, Paolo, Mascareño, Alejandro Suárez, Tabernero, Hugo, Tenegi, Fabio, Udry, Stéphane, Zanutta, Alessio, Zerbi, Filippo
Ultra-hot giant exoplanets receive thousands of times Earth's insolation. Their high-temperature atmospheres (>2,000 K) are ideal laboratories for studying extreme planetary climates and chemistry. Daysides are predicted to be cloud-free, dominated b
Externí odkaz:
http://arxiv.org/abs/2003.05528
Autor:
Dubber, Sophie C., Mortier, Annelies, Rice, Ken, Nava, Chantanelle, Malavolta, Luca, Giles, Helen, Coffinet, Adrien, Charbonneau, David, Vanderburg, Andrew, Bonomo, Aldo S., Boschin, Walter, Buchhave, Lars A., Cameron, Andrew Collier, Cosentino, Rosario, Dumusque, Xavier, Ghedina, Adriano, Harutyunyan, Avet, Haywood, Raphaelle D., Latham, David, Lopez-Morales, Mercedes, Micela, Giusi, Molinari, Emilio, Pepe, Francesco A., Phillips, David, Piotto, Giampaolo, Poretti, Ennio, Sasselov, Dimitar, Sozzetti, Alessandro, Udry, Stephane
We present confirmation of the planetary nature of PH-2b, as well as the first mass estimates for the two planets in the Kepler-103 system. PH-2b and Kepler-103c are both long-period and transiting, a sparsely-populated category of exoplanet. We use
Externí odkaz:
http://arxiv.org/abs/1910.03518
Autor:
Mayo, Andrew W., Rajpaul, Vinesh M., Buchhave, Lars A., Dressing, Courtney D., Mortier, Annelies, Zeng, Li, Fortenbach, Charles D., Aigrain, Suzanne, Bonomo, Aldo S., Cameron, Andrew Collier, Charbonneau, David, Coffinet, Adrien, Cosentino, Rosario, Damasso, Mario, Dumusque, Xavier, Fiorenzano, A. F. Martinez, Haywood, Raphaëlle D., Latham, David W., López-Morales, Mercedes, Malavolta, Luca, Micela, Giusi, Molinari, Emilio, Pearce, Logan, Pepe, Francesco, Phillips, David, Piotto, Giampaolo, Poretti, Ennio, Rice, Ken, Sozzetti, Alessandro, Udry, Stephane
Publikováno v:
2019 AJ 158 4
Although several thousands of exoplanets have now been detected and characterized, observational biases have led to a paucity of long-period, low-mass exoplanets with measured masses and a corresponding lag in our understanding of such planets. In th
Externí odkaz:
http://arxiv.org/abs/1908.08585
Autor:
Pizzocaro, Daniele, Stelzer, Beate, Poretti, Ennio, Raetz, Stefanie, Micela, Giusi, Belfiore, Andrea, Marelli, Martino, Salvetti, David, De Luca, Andrea
The relation between magnetic activity and rotation in late-type stars provides fundamental information on stellar dynamos and angular momentum evolution. Rotation/activity studies found in the literature suffer from inhomogeneity in the measure of a
Externí odkaz:
http://arxiv.org/abs/1906.05587
Autor:
Drake, Jeremy J., Alvarado-Gómez, Julián D., Airapetian, Vladimir, Cauley, P. Wilson, Argiroffi, Costanza, Browning, Matthew K., Christian, Damian J., Cohen, Ofer, Corrales, Lia, Danchi, William, de Val-Borro, Miguel, Dong, Chuanfei, Forman, William, France, Kevin, Gallo, Elena, Garcia-Sage, Katherine, Garraffo, Cecilia, Gelino, Dawn M., Gronoff, Guillaume, Günther, H. Moritz, Harper, Graham M., Haywood, Raphaëlle D., Karovska, Margarita, Kashyap, Vinay, Kastner, Joel, Kim, Jinyoung Serena, Leutenegger, Maurice A., Linsky, Jeffrey, López-Morales, Mercedes, Micela, Giusi, Moschou, Sofia-Paraskevi, Oskinova, Lidia, Osten, Rachel A., Owen, James E., Poppenhaeger, Katja, Principe, David A., Pye, John P., Sciortino, Salvatore, Tzanavaris, Panayiotis, Wargelin, Brad, Wheatley, Peter J., Williams, Peter K. G., Winston, Elaine, Wolk, Scott J.
It is now recognized that energetic stellar photon and particle radiation evaporates and erodes planetary atmospheres and controls upper atmospheric chemistry. Key exoplanet host stars will be too faint at X-ray wavelengths for accurate characterizat
Externí odkaz:
http://arxiv.org/abs/1903.12338