Zobrazeno 1 - 10
of 214
pro vyhledávání: '"Molinari, Emilio"'
Autor:
Cloutier, Ryan, Greklek-McKeon, Michael, Wurmser, Serena, Cherubim, Collin, Gillis, Erik, Vanderburg, Andrew, Hadden, Sam, Cadieux, Charles, Artigau, Étienne, Vissapragada, Shreyas, Mortier, Annelies, López-Morales, Mercedes, Latham, David W., Knutson, Heather, Haywood, Raphaëlle D., Pallé, Enric, Doyon, René, Cook, Neil, Andreuzzi, Gloria, Cecconi, Massimo, Cosentino, Rosario, Ghedina, Adriano, Harutyunyan, Avet, Pinamonti, Matteo, Stalport, Manu, Damasso, Mario, Rescigno, Federica, Wilson, Thomas G., Buchhave, Lars A., Charbonneau, David, Cameron, Andrew Collier, Dumusque, Xavier, Lovis, Christophe, Mayor, Michel, Molinari, Emilio, Pepe, Francesco, Piotto, Giampaolo, Rice, Ken, Sasselov, Dimitar, Ségransan, Damien, Sozzetti, Alessandro, Udry, Stéphane, Watson, Chris A.
Is the population of close-in planets orbiting M dwarfs sculpted by thermally driven escape or is it a direct outcome of the planet formation process? A number of recent empirical results strongly suggest the latter. However, the unique architecture
Externí odkaz:
http://arxiv.org/abs/2310.13496
Autor:
Christiansen, Jessie L., Vanderburg, Andrew, Burt, Jennifer, Fulton, B. J., Batygin, Konstantin, Benneke, Björn, Brewer, John M., Charbonneau, David, Ciardi, David R., Cameron, Andrew Collier, Coughlin, Jeffrey L., Crossfield, Ian J. M., Dressing, Courtney, Greene, Thomas P., Howard, Andrew W., Latham, David W., Molinari, Emilio, Mortier, Annelies, Mullally, Fergal, Pepe, Francesco, Rice, Ken, Sinukoff, Evan, Sozzetti, Alessandro, Thompson, Susan E., Udry, Stéphane, Vogt, Steven S., Barman, Travis S., Batalha, Natasha E., Bouchy, François, Buchhave, Lars A., Butler, R. Paul, Cosentino, Rosario, Dupuy, Trent J., Ehrenreich, David, Fiorenzano, Aldo, Hansen, Brad M. S., Henning, Thomas, Hirsch, Lea, Holden, Bradford P., Isaacson, Howard T., Johnson, John A., Knutson, Heather A., Kosiarek, Molly, López-Morales, Mercedes, Lovis, Christophe, Malavolta, Luca, Mayor, Michel, Micela, Giuseppina, Motalebi, Fatemeh, Petigura, Erik, Phillips, David F., Piotto, Giampaolo, Rogers, Leslie A., Sasselov, Dimitar, Schlieder, Joshua E., Ségransan, Damien, Watson, Christopher A., Weiss, Lauren M.
HD 3167 is a bright (V = 8.9), nearby KO star observed by the NASA K2 mission (EPIC 220383386), hosting two small, short-period transiting planets. Here we present the results of a multi-site, multi-instrument radial-velocity campaign to characterize
Externí odkaz:
http://hdl.handle.net/10150/625817
http://arizona.openrepository.com/arizona/handle/10150/625817
http://arizona.openrepository.com/arizona/handle/10150/625817
Autor:
Mayo, Andrew W., Dressing, Courtney D., Vanderburg, Andrew, Fortenbach, Charles D., Lienhard, Florian, Malavolta, Luca, Mortier, Annelies, Núñez, Alejandro, Richey-Yowell, Tyler, Turtelboom, Emma V., Bonomo, Aldo S., Latham, David W., López-Morales, Mercedes, Shkolnik, Evgenya, Sozzetti, Alessandro, Agüeros, Marcel A., Borsato, Luca, Charbonneau, David, Cosentino, Rosario, Douglas, Stephanie T., Dumusque, Xavier, Ghedina, Adriano, Gibson, Rose, Granata, Valentina, Harutyunyan, Avet, Haywood, R. D., Lacedelli, Gaia, Lorenzi, Vania, Magazzù, Antonio, Fiorenzano, A. F. Martinez, Micela, Giuseppina, Molinari, Emilio, Montalto, Marco, Nardiello, Domenico, Nascimbeni, Valerio, Pagano, Isabella, Piotto, Giampaolo, Pino, Lorenzo, Poretti, Ennio, Scandariato, Gaetano, Udry, Stephane, Buchhave, Lars A.
K2-136 is a late-K dwarf ($0.742\pm0.039$ M$_\odot$) in the Hyades open cluster with three known, transiting planets and an age of $650\pm70$ Myr. Analyzing K2 photometry, we found that planets K2-136b, c, and d have periods of $8.0$, $17.3$, and $25
Externí odkaz:
http://arxiv.org/abs/2304.02779
Autor:
Jin, Shoko, Trager, Scott C., Dalton, Gavin B., Aguerri, J. Alfonso L., Drew, J. E., Falcón-Barroso, Jesús, Gänsicke, Boris T., Hill, Vanessa, Iovino, Angela, Pieri, Matthew M., Poggianti, Bianca M., Smith, D. J. B., Vallenari, Antonella, Abrams, Don Carlos, Aguado, David S., Antoja, Teresa, Aragón-Salamanca, Alfonso, Ascasibar, Yago, Babusiaux, Carine, Balcells, Marc, Barrena, R., Battaglia, Giuseppina, Belokurov, Vasily, Bensby, Thomas, Bonifacio, Piercarlo, Bragaglia, Angela, Carrasco, Esperanza, Carrera, Ricardo, Cornwell, Daniel J., Domínguez-Palmero, Lilian, Duncan, Kenneth J., Famaey, Benoit, Fariña, Cecilia, Gonzalez, Oscar A., Guest, Steve, Hatch, Nina A., Hess, Kelley M., Hoskin, Matthew J., Irwin, Mike, Knapen, Johan H., Koposov, Sergey E., Kuchner, Ulrike, Laigle, Clotilde, Lewis, Jim, Longhetti, Marcella, Lucatello, Sara, Méndez-Abreu, Jairo, Mercurio, Amata, Molaeinezhad, Alireza, Monguió, Maria, Morrison, Sean, Murphy, David N. A., de Arriba, Luis Peralta, Pérez, Isabel, Pérez-Ràfols, Ignasi, Picó, Sergio, Raddi, Roberto, Romero-Gómez, Mercè, Royer, Frédéric, Siebert, Arnaud, Seabroke, George M., Som, Debopam, Terrett, David, Thomas, Guillaume, Wesson, Roger, Worley, C. Clare, Alfaro, Emilio J., Prieto, Carlos Allende, Alonso-Santiago, Javier, Amos, Nicholas J., Ashley, Richard P., Balaguer-Núñez, Lola, Balbinot, Eduardo, Bellazzini, Michele, Benn, Chris R., Berlanas, Sara R., Bernard, Edouard J., Best, Philip, Bettoni, Daniela, Bianco, Andrea, Bishop, Georgia, Blomqvist, Michael, Boeche, Corrado, Bolzonella, Micol, Bonoli, Silvia, Bosma, Albert, Britavskiy, Nikolay, Busarello, Gianni, Caffau, Elisabetta, Cantat-Gaudin, Tristan, Castro-Ginard, Alfred, Couto, Guilherme, Carbajo-Hijarrubia, Juan, Carter, David, Casamiquela, Laia, Conrado, Ana M., Corcho-Caballero, Pablo, Costantin, Luca, Deason, Alis, de Burgos, Abel, De Grandi, Sabrina, Di Matteo, Paola, Domínguez-Gómez, Jesús, Dorda, Ricardo, Drake, Alyssa, Dutta, Rajeshwari, Erkal, Denis, Feltzing, Sofia, Ferré-Mateu, Anna, Feuillet, Diane, Figueras, Francesca, Fossat, Matteo, Franciosin, Elena, Frasca, Antonio, Fumagalli, Michele, Gallazzi, Anna, García-Benito, Rubén, Fusillo, Nicola Gentile, Gebran, Marwan, Gilbert, James, Gledhill, T. M., Delgado, Rosa M. González, Greimel, Robert, Guarcello, Mario Giuseppe, Guerra, Jose, Gullieuszik, Marco, Haines, Christopher P., Hardcastle, Martin J., Harris, Amy, Haywood, Misha, Helmi, Amina, Hernandez, Nauzet, Herrero, Artemio, Hughes, Sarah, Irsic, Vid, Jablonka, Pascale, Jarvis, Matt J., Jordi, Carme, Kondapally, Rohit, Kordopatis, Georges, Krogager, Jens-Kristian, La Barbera, Francesco, Lam, Man I, Larsen, Søren S., Lemasle, Bertrand, Lewis, Ian J., Lhomé, Emilie, Lind, Karin, Lodi, Marcello, Longobardi, Alessia, Lonoce, Ilaria, Magrin, Laura, Apellániz, Jesús Maíz, Marchal, Olivier, Marco, Amparo, Martin, Nicolas F., Matsuno, Tadafumi, Maurogordato, Sophie, Merluzzi, Paola, Miralda-Escudé, Jordi, Molinari, Emilio, Monari, Giacomo, Morelli, Lorenzo, Mottram, Christopher J., Naylor, Tim, Negueruela, Ignacio, Oñorbe, Jose, Pancino, Elena, Peirani, Sébastien, Peletier, Reynier F., Pozzetti, Lucia, Rainer, Monica, Ramos, Pau, Read, Shaun C., Rossi, Elena Maria, Röttgering, Huub J. A., Rubiño-Martín, Jose Alberto, Montes, Jose Sabater, Juan, José San, Sanna, Nicoletta, Schallig, Ellen, Schiavon, Ricardo P., Schultheis, Mathias, Serra, Paolo, Shimwell, Timothy W., Simón-Díaz, Sergio, Smith, Russell J., Sordo, Rosanna, Sorini, Daniele, Soubiran, Caroline, Starkenburg, Else, Steele, Iain A., Stott, John, Stuik, Remko, Tolstoy, Eline, Tortora, Crescenzo, Tsantaki, Maria, Van der Swaelmen, Mathieu, van Weeren, Reinout J., Vergani, Daniela, Verheijen, Marc A. W., Verro, Kristiina, Vink, Jorick S., Vioque, Miguel, Walcher, C. Jakob, Walton, Nicholas A., Wegg, Christopher, Weijmans, Anne-Marie, Williams, Wendy L., Wilson, Andrew J., Wright, Nicholas J., Xylakis-Dornbusch, Theodora, Youakim, Kris, Zibetti, Stefano, Zurita, Cristina
WEAVE, the new wide-field, massively multiplexed spectroscopic survey facility for the William Herschel Telescope, will see first light in late 2022. WEAVE comprises a new 2-degree field-of-view prime-focus corrector system, a nearly 1000-multiplex f
Externí odkaz:
http://arxiv.org/abs/2212.03981
Autor:
Cherubim, Collin, Cloutier, Ryan, Charbonneau, David, Wohler, Bill, Stockdale, Chris, Stassun, Keivan G., Schwarz, Richard P., Safonov, Boris, Mortier, Annelies, Latham, David W., Horne, Keith, Haywood, Raphaëlle D., Gonzales, Erica, Goliguzova, Maria V., Collins, Karen A., Ciardi, David R., Bieryla, Allyson, Belinski, Alexander A., Watson, Christopher A., Vanderspek, Rolands, Udry, Stéphane, Sozzetti, Alessandro, Ségransan, Damien, Sasselov, Dimitar, Ricker, George R., Rice, Ken, Poretti, Ennio, Piotto, Giampaolo, Pepe, Francesco, Molinari, Emilio, Micela, Giuseppina, Mayor, Michel, Lovis, Christophe, López-Morales, Mercedes, Jenkins, Jon M., Essack, Zahra, Dumusque, Xavier, Doty, John P., Colón, Knicole D., Cameron, Andrew Collier, Buchhave, Lars A.
Characterizing the bulk compositions of transiting exoplanets within the M dwarf radius valley offers a unique means to establish whether the radius valley emerges from an atmospheric mass loss process or is imprinted by planet formation itself. We p
Externí odkaz:
http://arxiv.org/abs/2211.06445
Autor:
Brinkman, Casey, Cadman, James, Weiss, Lauren, Gaidos, Eric, Rice, Ken, Huber, Daniel, Claytor, Zachary R., Bonomo, Aldo S., Buchhave, Lars A., Cameron, Andrew Collier, Cosentino, Rosario, Dumusque, Xavier, Fiorenzano, Aldo F Martinez, Ghedina, Adriano, Harutyunyan, Avet, Howard, Andrew, Isaacson, Howard, Latham, David W., Lopez-Morales, Mercedes, Malavolta, Luca, Micela, Giuseppina, Molinari, Emilio, Pepe, Francesco, Philips, David F, Poretti, Ennio, Sozzetti, Alessandro, Udry, Stephane
Radial velocity (RV) measurements of transiting multiplanet systems allow us to understand the densities and compositions of planets unlike those in the Solar System. Kepler-102, which consists of 5 tightly packed transiting planets, is a particularl
Externí odkaz:
http://arxiv.org/abs/2211.05196
Autor:
DiTomasso, Victoria, Nava, Chantanelle, López-Morales, Mercedes, Bieryla, Allyson, Cloutier, Ryan, Malavolta, Luca, Mortier, Annelies, Buchhave, Lars A., Stassun, Keivan G., Sozzetti, Alessandro, Bonomo, Aldo Stefano, Charbonneau, David, Cameron, Andrew Collier, Cosentino, Rosario, Damasso, Mario, Dumusque, Xavier, Fiorenzano, A. F. Martínez, Ghedina, Adriano, Harutyunyan, Avet, Haywood, R. D., Latham, David, Molinari, Emilio, Pepe, Francesco A., Pinamonti, Matteo, Poretti, Ennio, Rice, Ken, Sasselov, Dimitar, Stalport, Manu, Udry, Stéphane, Watson, Christopher, Wilson, Thomas G.
We present high-precision radial velocities (RVs) from the HARPS-N spectrograph for HD79210 and HD79211, two M0V members of a gravitationally-bound binary system. We detect a planet candidate with a period of $24.421^{+0.016}_{-0.017}$ days around HD
Externí odkaz:
http://arxiv.org/abs/2210.12211
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:
Nava, Chantanelle, López-Morales, Mercedes, Mortier, Annelies, Zeng, Li, Giles, Helen A. C., Bieryla, Allyson, Vanderburg, Andrew, Buchhave, Lars A., Poretti, Ennio, Saar, Steven H., Dumusque, Xavier, Latham, David W., Charbonneau, David, Damasso, Mario, Bonomo, Aldo S., Lovis, Christophe, Cameron, Andrew Collier, Eastman, Jason D., Sozzetti, Alessandro, Cosentino, Rosario, Pedani, Marco, Pepe, Francesco, Molinari, Emilio, Sasselov, Dimitar, Mayor, Michel, Stalport, Manu, Malavolta, Luca, Rice, Ken, Watson, Christopher A., Fiorenzano, A. F. Martinez, Di Fabrizio, Luca
We present mass and radius measurements of K2-79b and K2-222b, two transiting exoplanets orbiting active G-type stars. Their respective 10.99d and 15.39d orbital periods fall near periods of signals induced by stellar magnetic activity. The two signa
Externí odkaz:
http://arxiv.org/abs/2111.02608
Autor:
Polanski, Alex S., Crossfield, Ian J. M., Burt, Jennifer A., Nowak, Grzegorz, López-Morales, Mercedes, Mortier, Annelies, Poretti, Ennio, Behmard, Aida, Benneke, Björn, Blunt, Sarah, Bonomo, Aldo S., Butler, R. Paul, Chontos, Ashley, Cosentino, Rosario, Crane, Jeffrey D., Dumusque, Xavier, Fulton, Benjamin J., Ghedina, Adriano, Gorjian, Varoujan, Grunblatt, Samuel K., Harutyunyan, Avet, Howard, Andrew W., Isaacson, Howard, Kosiarek, Molly R., Latham, David W., Luque, Rafael, Fiorenzano, Aldo F. Martinez, Mayor, Michel, Mills, Sean M., Molinari, Emilio, Nagel, Evangelos, Pallé, Enric, Petigura, Erik A., Shectman, Stephen A., Sozzetti, Alessandro, Teske, Johanna K., Wang, Sharon Xuesong, Weiss, Lauren M.
Using radial velocity measurements from four instruments, we report the mass and density of a $2.043\pm0.069 ~\rm{R}_{\oplus}$ sub-Neptune orbiting the quiet K-dwarf Wolf 503 (HIP 67285). In addition, we present improved orbital and transit parameter
Externí odkaz:
http://arxiv.org/abs/2107.08092