Zobrazeno 1 - 10
of 37
pro vyhledávání: '"Pinamonti, Matteo"'
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:
Kunimoto, Michelle, Vanderburg, Andrew, Huang, Chelsea X., Davis, M. Ryleigh, Affer, Laura, Cameron, Andrew Collier, Charbonneau, David, Cosentino, Rosario, Damasso, Mario, Dumusque, Xavier, Fiorenzano, A. F. Martnez, Ghedina, Adriano, Haywood, R. D., Lienhard, Florian, López-Morales, Mercedes, Mayor, Michel, Pepe, Francesco, Pinamonti, Matteo, Poretti, Ennio, Maldonado, Jesús, Rice, Ken, Sozzetti, Alessandro, Wilson, Thomas G., Udry, Stéphane, Baptista, Jay, Barkaoui, Khalid, Becker, Juliette, Benni, Paul, Bieryla, Allyson, Bosch-Cabot, Pau, Ciardi, David R., Collins, Karen A., Collins, Kevin I., Evans, Elise, Dupuy, Trent J., Goliguzova, Maria V., Guerra, Pere, Kraus, Adam, Lissauer, Jack J., Huber, Daniel, Murgas, Felipe, Palle, Enric, Quinn, Samuel N., Safonov, Boris S., Schwarz, Richard P., Shporer, Avi, Stassun, Keivan G., Jenkins, Jon M., Latham, David W., Ricker, George R., Seager, Sara, Vanderspek, Roland, Winn, Joshua, Essack, Zahra, Lewis, Hannah M., Rose, Mark E.
Publikováno v:
AJ, 166, 7 (2023)
We report the confirmation of three exoplanets transiting TOI-4010 (TIC-352682207), a metal-rich K dwarf observed by TESS in Sectors 24, 25, 52, and 58. We confirm these planets with HARPS-N radial velocity observations and measure their masses with
Externí odkaz:
http://arxiv.org/abs/2306.05308
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:
Drimmel, Ronald, Sozzetti, Alessandro, Schroeder, Klaus-Peter, Bastian, Ulrich, Pinamonti, Matteo, Jack, Dennis, Huerta, Missael A. Hernandez
We present a spectroscopic characterisation and a new orbital solution for the binary system beta Cyg Aa/Ac (MCA 55), the primary component (beta Cyg A) of the well-known wide double star Albireo. By matching evolutionary tracks to the physical param
Externí odkaz:
http://arxiv.org/abs/2012.01277
Autor:
Carleo, Ilaria, Desidera, Silvano, Nardiello, Domenico, Malavolta, Luca, Lanza, Antonino F., Livingston, John, Locci, Daniele, Marzari, Francesco, Messina, Sergio, Turrini, Diego, Baratella, Martina, Borsa, Francesco, D'Orazi, Valentina, Nascimbeni, Valerio, Pinamonti, Matteo, Rainer, Monica, Alei, Eleonora, Bignamini, Andrea, Gratton, Raffaele, Micela, Giuseppina, Montalto, Marco, Sozzetti, Alessandro, Squicciarini, Vito, Affer, Laura, Benatti, Serena, Biazzo, Katia, Bonomo, Aldo S., Claudi, Riccardo, Cosentino, Rosario, Covino, Elvira, Damasso, Mario, Esposito, Massimiliano, Fiorenzano, Aldo, Frustagli, Giuseppe, Giacobbe, Paolo, Harutyunyan, Avet, Leto, Giuseppe, Magazzú, Antonio, Maggio, Antonio, Mainella, Giovanni, Maldonado, Jesus, Mallonn, Matthias, Mancini, Luigi, Molinari, Emilio, Molinaro, Marco, Pagano, Isabella, Pedani, Marco, Piotto, Giampaolo, Poretti, Ennio, Redfield, Seth, Scandariato, Gaetano
Publikováno v:
A&A 645, A71 (2021)
Both young stars and multi-planet systems are primary objects that allow us to study, understand and constrain planetary formation and evolution theories. We validate the physical nature of two Neptune-type planets transiting TOI-942 (TYC 5909-319-1)
Externí odkaz:
http://arxiv.org/abs/2011.13795
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:
Cloutier, Ryan, Rodriguez, Joseph E., Irwin, Jonathan, Charbonneau, David, Stassun, Keivan G., Mortier, Annelies, Latham, David W., Isaacson, Howard, Howard, Andrew W., Udry, Stéphane, Wilson, Thomas G., Watson, Christopher A., Pinamonti, Matteo, Lienhard, Florian, Giacobbe, Paolo, Guerra, Pere, Collins, Karen A., Beiryla, Allyson, Esquerdo, Gilbert A., Matthews, Elisabeth, Matson, Rachel A., Howell, Steve B., Furlan, Elise, Crossfield, Ian J. M., Winters, Jennifer G., Nava, Chantanelle, Ment, Kristo, Lopez, Eric D., Ricker, George, Vanderspek, Roland, Seager, Sara, Jenkins, Jon M., Ting, Eric B., Tenenbaum, Peter, Sozzetti, Alessandro, Sha, Lizhou, Ségransan, Damien, Schlieder, Joshua E., Sasselov, Dimitar, Roy, Arpita, Robertson, Paul, Rice, Ken, Poretti, Ennio, Piotto, Giampaolo, Phillips, David, Pepper, Joshua, Pepe, Francesco, Molinari, Emilio, Mocnik, Teo, Micela, Giuseppina, Mayor, Michel, Fiorenzano, Aldo F. Martinez, Mallia, Franco, Lubin, Jack, Lovis, Christophe, López-Morales, Mercedes, Kosiarek, Molly R., Kielkopf, John F., Kane, Stephen R., Jensen, Eric L. N., Isopi, Giovanni, Huber, Daniel, Hill, Michelle L., Harutyunyan, Avet, Gonzales, Erica, Giacalone, Steven, Ghedina, Adriano, Ercolino, Andrea, Dumusque, Xavier, Dressing, Courtney D., Damasso, Mario, Dalba, Paul A., Cosentino, Rosario, Conti, Dennis M., Colón, Knicole D., Collins, Kevin I., Cameron, Andrew Collier, Ciardi, David, Christiansen, Jessie, Chontos, Ashley, Cecconi, Massimo, Caldwell, Douglas A., Burke, Christopher, Buchhave, Lars, Beichman, Charles, Behmard, Aida, Beard, Corey, Murphy, Joseph M. Akana
Small planets on close-in orbits tend to exhibit envelope mass fractions of either effectively zero or up to a few percent depending on their size and orbital period. Models of thermally-driven atmospheric mass loss and of terrestrial planet formatio
Externí odkaz:
http://arxiv.org/abs/2004.06682
Autor:
Cloutier, Ryan, Eastman, Jason D., Rodriguez, Joseph E., Astudillo-Defru, Nicola, Bonfils, Xavier, Mortier, Annelies, Watson, Christopher A., Stalport, Manu, Pinamonti, Matteo, Lienhard, Florian, Harutyunyan, Avet, Damasso, Mario, Latham, David W., Collins, Karen A., Massey, Robert, Irwin, Jonathan, Winters, Jennifer G., Charbonneau, David, Ziegler, Carl, Matthews, Elisabeth, Crossfield, Ian J. M., Kreidberg, Laura, Quinn, Samuel N., Ricker, George, Vanderspek, Roland, Seager, Sara, Winn, Joshua, Jenkins, Jon M., Vezie, Michael, Udry, Stéphane, Twicken, Joseph D., Tenenbaum, Peter, Sozzetti, Alessandro, Ségransan, Damien, Schlieder, Joshua E., Sasselov, Dimitar, Santos, Nuno C., Rice, Ken, Rackham, Benjamin V., Poretti, Ennio, Piotto, Giampaolo, Phillips, David, Pepe, Francesco, Molinari, Emilio, Mignon, Lucile, Micela, Giuseppina, Melo, Claudio, de Medeiros, José R., Mayor, Michel, Matson, Rachel, Fiorenzano, Aldo F. Martinez, Mann, Andrew W., Magazzú, Antonio, Lovis, Christophe, López-Morales, Mercedes, Lopez, Eric, Lissauer, Jack J., Lépine, Sébastien, Law, Nicholas, Kielkopf, John F., Johnson, John A., Jensen, Eric L. N., Howell, Steve B., Gonzales, Erica, Ghedina, Adriano, Forveille, Thierry, Figueira, Pedro, Dumusque, Xavier, Dressing, Courtney D., Doyon, René, Díaz, Rodrigo F., Di Fabrizio, Luca, Delfosse, Xavier, Cosentino, Rosario, Conti, Dennis M., Collins, Kevin I., Cameron, Andrew Collier, Ciardi, David, Caldwell, Douglas A., Burke, Christopher, Buchhave, Lars, Briceño, César, Boyd, Patricia, Bouchy, François, Beichman, Charles, Artigau, Étienne, Almenara, Jose M.
We present the confirmation of two new planets transiting the nearby mid-M dwarf LTT 3780 (TIC 36724087, TOI-732, $V=13.07$, $K_s=8.204$, $R_s$=0.374 R$_{\odot}$, $M_s$=0.401 M$_{\odot}$, d=22 pc). The two planet candidates are identified in a single
Externí odkaz:
http://arxiv.org/abs/2003.01136
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