Zobrazeno 1 - 10
of 35
pro vyhledávání: '"Chew, Yilen Gomez Maqueo"'
Autor:
Gillon, Michaël, Pedersen, Peter P., Rackham, Benjamin V., Dransfield, Georgina, Ducrot, Elsa, Barkaoui, Khalid, Burdanov, Artem Y., Schroffenegger, Urs, Chew, Yilen Gómez Maqueo, Lederer, Susan M., Alonso, Roi, Burgasser, Adam J., Howell, Steve B., Narita, Norio, de Wit, Julien, Demory, Brice-Olivier, Queloz, Didier, Triaud, Amaury H. M. J., Delrez, Laetitia, Jehin, Emmanuël, Hooton, Matthew J., Garcia, Lionel J., Muñoz, Clàudia Jano, Murray, Catriona A., Pozuelos, Francisco J., Sebastian, Daniel, Timmermans, Mathilde, Thompson, Samantha J., Aceituno, Jesús, Aganze, Christian, Amado, Pedro J., Baycroft, Thomas, Benkhaldoun, Zouhair, Berardo, David, Bolmont, Emeline, Clark, Catherine A., Davis, Yasmin T., Davoudi, Fatemeh, de Beurs, Zoë L., de Leon, Jerome P., Ikoma, Masahiro, Ikuta, Kai, Isogai, Keisuke, Fukuda, Izuru, Fukui, Akihiko, Gerasimov, Roman, Ghachoui, Mourad, Günther, Maximilian N., Hasler, Samantha, Hayashi, Yuya, Heng, Kevin, Hu, Renyu, Kagetani, Taiki, Kawai, Yugo, Kawauchi, Kiyoe, Kitzmann, Daniel, Koll, Daniel D. B., Lendl, Monika, Livingston, John H., Lyu, Xintong, Valdés, Erik A. Meier, Mori, Mayuko, McCormac, James J., Murgas, Felipe, Niraula, Prajwal, Pallé, Enric, Plauchu-Frayn, Ilse, Rebolo, Rafael, Sabin, Laurence, Schackey, Yannick, Schanche, Nicole, Selsis, Franck, Sota, Alfredo, Stalport, Manu, Standing, Matthew R., Stassun, Keivan G., Tamura, Motohide, Theissen, Christopher A., Turbet, Martin, Van Grootel, Valérie, Varas, Roberto, Watanabe, Noriharu, Lang, Francis Zong
Located at the bottom of the main sequence, ultracool dwarf stars are widespread in the solar neighbourhood. Nevertheless, their extremely low luminosity has left their planetary population largely unexplored, and only one of them, TRAPPIST-1, has so
Externí odkaz:
http://arxiv.org/abs/2406.00794
Autor:
Petrucci, Romina P., Chew, Yilen Gómez Maqueo, Jofré, Emiliano, Segura, Antígona, Ferrero, Leticia V.
We present a photometric characterization of 208 ultra-cool dwarfs (UCDs) with spectral types between M4 and L4, from 20-second and 2-minute cadence TESS light curves. We determine rotation periods for 87 objects (42 percent) and identify 778 flare e
Externí odkaz:
http://arxiv.org/abs/2311.13591
Autor:
Albareti, Franco D., Prieto, Carlos Allende, Almeida, Andres, Anders, Friedrich, Anderson, Scott, Andrews, Brett H., Aragón-Salamanca, Alfonso, Argudo-Fernández, Maria, Armengaud, Eric, Aubourg, Eric, Avila-Reese, Vladimir, Badenes, Carles, Bailey, Stephen, Barbuy, Beatriz, Barger, Kat, Barrera-Ballesteros, Jorge, Bartosz, Curtis, Basu, Sarbani, Bates, Dominic, Battaglia, Giuseppina, Baumgarten, Falk, Baur, Julien, Bautista, Julian, Beers, Timothy C., Belfiore, Francesco, Bershady, Matthew, de Lis, Sara Bertran, Bird, Jonathan C., Bizyaev, Dmitry, Blanc, Guillermo A., Blanton, Michael, Blomqvist, Michael, Bolton, Adam S., Borissova, J., Bovy, Jo, Brandt, William Nielsen, Brinkmann, Jonathan, Brownstein, Joel R., Bundy, Kevin, Burtin, Etienne, Busca, Nicolás G., Chavez, Hugo Orlando Camacho, Díaz, M. Cano, Cappellari, Michele, Carrera, Ricardo, Chen, Yanping, Cherinka, Brian, Cheung, Edmond, Chiappini, Cristina, Chojnowski, Drew, Chuang, Chia-Hsun, Chung, Haeun, Cirolini, Rafael Fernando, Clerc, Nicolas, Cohen, Roger E., Comerford, Julia M., Comparat, Johan, Correa do Nascimento, Janaina, Cousinou, Marie-Claude, Covey, Kevin, Crane, Jeffrey D., Croft, Rupert, Cunha, Katia, Darling, Jeremy, Davidson, James W., Dawson, Kyle, Da Costa, Luiz, Da Silva Ilha, Gabriele, Machado, Alice Deconto, Delubac, Timothée, De Lee, Nathan, De la Macorra, Axel, De la Torre, Sylvain, Diamond-Stanic, Aleksandar M., Donor, John, Downes, Juan Jose, Drory, Niv, Du, Cheng, Du Mas des Bourboux, Hélion, Dwelly, Tom, Ebelke, Garrett, Eigenbrot, Arthur, Eisenstein, Daniel J., Elsworth, Yvonne P., Emsellem, Eric, Eracleous, Michael, Escoffier, Stephanie, Evans, Michael L., Falcón-Barroso, Jesús, Fan, Xiaohui, Favole, Ginevra, Fernandez-Alvar, Emma, Fernandez-Trincado, J. G., Feuillet, Diane, Fleming, Scott W., Font-Ribera, Andreu, Freischlad, Gordon, Frinchaboy, Peter, Fu, Hai, Gao, Yang, Garcia, Rafael A., Garcia-Dias, R., Garcia-Hernández, D. A., Pérez, Ana E. Garcia, Gaulme, Patrick, Ge, Junqiang, Geisler, Douglas, Gillespie, Bruce, Marin, Hector Gil, Girardi, Léo, Goddard, Daniel, Chew, Yilen Gomez Maqueo, Gonzalez-Perez, Violeta, Grabowski, Kathleen, Green, Paul, Grier, Catherine J., Grier, Thomas, Guo, Hong, Guy, Julien, Hagen, Alex, Hall, Matt, Harding, Paul, Harley, R. E., Hasselquist, Sten, Hawley, Suzanne, Hayes, Christian R., Hearty, Fred, Hekker, Saskia, Toledo, Hector Hernandez, Ho, Shirley, Hogg, David W., Holley-Bockelmann, Kelly, Holtzman, Jon A., Holzer, Parker H., Hu, Jian, Huber, Daniel, Hutchinson, Timothy Alan, Hwang, Ho Seong, Ibarra-Medel, Héctor J., Ivans, Inese I., Ivory, KeShawn, Jaehnig, Kurt, Jensen, Trey W., Johnson, Jennifer A., Jones, Amy, Jullo, Eric, Kallinger, T., Kinemuchi, Karen, Kirkby, David, Klaene, Mark, Kneib, Jean-Paul, Kollmeier, Juna A., Lacerna, Ivan, Lane, Richard R., Lang, Dustin, Laurent, Pierre, Law, David R., Leauthaud, Alexie, Le Goff, Jean-Marc, Li, Chen, Li, Cheng, Li, Niu, Li, Ran, Liang, Fu-Heng, Liang, Yu, Lima, Marcos, Lin, Lihwai, Lin, Lin, Lin, Yen-Ting, Liu, Chao, Long, Dan, Lucatello, Sara, MacDonald, Nicholas, MacLeod, Chelsea L., Mackereth, J. Ted, Mahadevan, Suvrath, Maia, Marcio Antonio Geimba, Maiolino, Roberto, Majewski, Steven R., Malanushenko, Olena, Malanushenko, Viktor, Mallmann, Nícolas Dullius, Manchado, Arturo, Maraston, Claudia, Marques-Chaves, Rui, Valpuesta, Inma Martinez, Masters, Karen L., Mathur, Savita, McGreer, Ian D., Merloni, Andrea, Merrifield, Michael R., Meszáros, Szabolcs, Meza, Andres, Miglio, Andrea, Minchev, Ivan, Molaverdikhani, Karan, Montero-Dorta, Antonio D., Mosser, Benoit, Muna, Demitri, Myers, Adam, Nair, Preethi, Nandra, Kirpal, Ness, Melissa, Newman, Jeffrey A., Nichol, Robert C., Nidever, David L., Nitschelm, Christian, O’Connell, Julia, Oravetz, Audrey, Oravetz, Daniel J., Pace, Zachary, Padilla, Nelson, Palanque-Delabrouille, Nathalie, Pan, Kaike, Parejko, John, Paris, Isabelle, Park, Changbom, Peacock, John A., Peirani, Sebastien, Pellejero-Ibanez, Marcos, Penny, Samantha, Percival, Will J., Percival, Jeffrey W., Perez-Fournon, Ismael, Petitjean, Patrick, Pieri, Matthew, Pinsonneault, Marc H., Pisani, Alice, Prada, Francisco, Prakash, Abhishek, Price-Jones, Natalie, Raddick, M. Jordan, Rahman, Mubdi, Raichoor, Anand, Rembold, Sandro Barboza, Reyna, A. M., Rich, James, Richstein, Hannah, Ridl, Jethro, Riffel, Rogemar A., Riffel, Rogério, Rix, Hans-Walter, Robin, Annie C., Rockosi, Constance M., Rodríguez-Torres, Sergio, Rodrigues, Thaíse S., Roe, Natalie, Lopes, A. Roman, Román-Zúñiga, Carlos, Ross, Ashley J., Rossi, Graziano, Ruan, John, Ruggeri, Rossana, Runnoe, Jessie C., Salazar-Albornoz, Salvador, Salvato, Mara, Sanchez, Sebastian F., Sanchez, Ariel G., Sanchez-Gallego, José R., Santiago, Basílio Xavier, Schiavon, Ricardo, Schimoia, Jaderson S., Schlafly, Eddie, Schlegel, David J., Schneider, Donald P., Schönrich, Ralph, Schultheis, Mathias, Schwope, Axel, Seo, Hee-Jong, Serenelli, Aldo, Sesar, Branimir, Shao, Zhengyi, Shetrone, Matthew, Shull, Michael, Aguirre, Victor Silva, Skrutskie, M. F., Slosar, Anže, Smith, Michael, Smith, Verne V., Sobeck, Jennifer, Somers, Garrett, Souto, Diogo, Stark, David V., Stassun, Keivan G., Steinmetz, Matthias, Stello, Dennis, Bergmann, Thaisa Storchi, Strauss, Michael A., Streblyanska, Alina, Stringfellow, Guy S., Suarez, Genaro, Sun, Jing, Taghizadeh-Popp, Manuchehr, Tang, Baitian, Tao, Charling, Tayar, Jamie, Tembe, Mita, Thomas, Daniel, Tinker, Jeremy, Tojeiro, Rita, Tremonti, Christy, Troup, Nicholas, Trump, Jonathan R., Unda-Sanzana, Eduardo, Valenzuela, O., Van den Bosch, Remco, Vargas-Magaña, Mariana, Vazquez, Jose Alberto, Villanova, Sandro, Vivek, M., Vogt, Nicole, Wake, David, Walterbos, Rene, Wang, Yuting, Wang, Enci, Weaver, Benjamin Alan, Weijmans, Anne-Marie, Weinberg, David H., Westfall, Kyle B., Whelan, David G., Wilcots, Eric, Wild, Vivienne, Williams, Rob A., Wilson, John, Wood-Vasey, W. M., Wylezalek, Dominika, Xiao, Ting, Yan, Renbin, Yang, Meng, Ybarra, Jason E., Yeche, Christophe, Yuan, Fang-Ting, Zakamska, Nadia, Zamora, Olga, Zasowski, Gail, Zhang, Kai, Zhao, Cheng, Zhao, Gong-Bo, Zheng, Zheng, Zhou, Zhi-Min, Zhu, Guangtun, Zinn, Joel C., Zou, Hu
The fourth generation of the Sloan Digital Sky Survey (SDSS-IV) began observations in 2014 July. It pursues three core programs: the Apache Point Observatory Galactic Evolution Experiment 2 (APOGEE-2), Mapping Nearby Galaxies at APO (MaNGA), and the
Externí odkaz:
http://hdl.handle.net/10150/626420
http://arizona.openrepository.com/arizona/handle/10150/626420
http://arizona.openrepository.com/arizona/handle/10150/626420
Autor:
Triaud, Amaury H. M. J., Dransfield, Georgina, Kagetani, Taiki, Timmermans, Mathilde, Narita, Norio, Barkaoui, Khalid, Hirano, Teruyuki, Rackham, Benjamin V., Mori, Mayuko, Baycroft, Thomas, Benkhaldoun, Zouhair, Burgasser, Adam J., Caldwell, Douglas A., Collins, Karen A., Davis, Yasmin T., Delrez, Laetitia, Demory, Brice-Oliver, Ducrot, Elsa, Fukui, Akihiko, Muñoz, Clàudia Jano, Jehin, Emmanuël, García, Lionel J., Ghachoui, Mourad, Gillon, Michaël, Chew, Yilen Gómez Maqueo, Hooton, Matthew J., Ikoma, Masahiro, Kawauchi, Kiyoe, Kotani, Takayuki, Levine, Alan M., Pallé, Enric, Pedersen, Peter P., Pozuelos, Francisco J., Queloz, Didier, Scutt, Owen J., Seager, Sara, Sebastian, Daniel, Tamura, Motohide, Thompson, Samantha, Watanabe, Noriharu, de Wit, Julien, Winn, Joshua N., Zúñiga-Fernández, Sebastián
In the last decade, a dozen close-in giant planets have been discovered orbiting stars with spectral types ranging from M0 to M4, a mystery since known formation pathways do not predict the existence of such systems. Here, we confirm TOI-4860 b, a Ju
Externí odkaz:
http://arxiv.org/abs/2308.02253
A 1.55 R$_{\oplus}$ habitable-zone planet hosted by TOI-715, an M4 star near the ecliptic South Pole
Autor:
Dransfield, Georgina, Timmermans, Mathilde, Triaud, Amaury H. M. J., Dévora-Pajares, Martín, Aganze, Christian, Barkaoui, Khalid, Burgasser, Adam J., Collins, Karen A., Cointepas, Marion, Ducrot, Elsa, Günther, Maximilian N., Howell, Steve B., Murray, Catriona A., Niraula, Prajwal, Rackham, Benjamin V., Sebastian, Daniel, Stassun, Keivan G., Zúñiga-Fernández, Sebastián, Almenara, José Manuel, Bonfils, Xavier, Bouchy, François, Burke, Christopher J., Charbonneau, David, Christiansen, Jessie L., Delrez, Laetitia, Gan, Tianjun, García, Lionel J., Gillon, Michaël, Chew, Yilen Gómez Maqueo, Hesse, Katharine M., Hooton, Matthew J., Isopi, Giovanni, Jehin, Emmanuël, Jenkins, Jon M., Latham, David W., Mallia, Franco, Murgas, Felipe, Pedersen, Peter P., Pozuelos, Francisco J., Queloz, Didier, Rodriguez, David R., Schanche, Nicole, Seager, Sara, Srdoc, Gregor, Stockdale, Chris, Twicken, Joseph D., Vanderspek, Roland, Wells, Robert, Winn, Joshua N., de Wit, Julien, Zapparata, Aldo
A new generation of observatories is enabling detailed study of exoplanetary atmospheres and the diversity of alien climates, allowing us to seek evidence for extraterrestrial biological and geological processes. Now is therefore the time to identify
Externí odkaz:
http://arxiv.org/abs/2305.06206
Autor:
Osborn, Hugh P., Bonfanti, Andrea, Gandolfi, Davide, Hedges, Christina, Leleu, Adrien, Fortier, Andrea, Futyan, David, Gutermann, Pascal, Maxted, Pierre F. L., Borsato, Luca, Collins, Karen A., da Silva, J. Gomes, Chew, Yilen Gómez Maqueo, Hooton, Matthew J., Lendl, Monika, Parviainen, Hannu, Salmon, Sébastien, Schanche, Nicole, Serrano, Luisa M., Sousa, Sergio G., Tuson, Amy, Ulmer-Moll, Solène, Van Grootel, Valerie, Wells, R. D., Wilson, Thomas G., Alibert, Yann, Alonso, Roi, Anglada, Guillem, Asquier, Joel, Navascues, David Barrado y, Baumjohann, Wolfgang, Beck, Thomas, Benz, Willy, Biondi, Federico, Bonfils, Xavier, Bouchy, Francois, Brandeker, Alexis, Broeg, Christopher, Bárczy, Tamas, Barros, S. C. C., Cabrera, Juan, Charnoz, Sébastien, Cameron, Andrew Collier, Csizmadia, Szilard, Davies, Melvyn B., Deleuil, Magali, Delrez, Laetitia, Demory, Brice-Olivier, Ehrenreich, David, Erikson, Anders, Fossati, Luca, Fridlund, Malcolm, Gillon, Michaël, Gómez-Muñoz, M. A., Güdel, Manuel, Heng, Kevin, Hoyer, Sergio, Isaak, Kate G., Kiss, Laszlo, Laskar, Jacques, Etangs, Alain Lecavelier des, Lovis, Christophe, Magrin, Demetrio, Malavolta, Luca, McCormac, James, Nascimbeni, Valerio, Olofsson, Göran, Ottensamer, Roland, Pagano, Isabella, Pallé, Enric, Peter, Gisbert, Piazza, Daniele, Piotto, Giampaolo, Pollacco, Don, Queloz, Didier, Ragazzoni, Roberto, Rando, Nicola, Rauer, Heike, Reimers, Christian, Ribas, Ignasi, Demangeon, Olivier D. S., Smith, Alexis M. S., Sabin, L., Santos, Nuno, Scandariato, Gaetano, Schroffenegger, U., Schwarz, Rick P., Shporer, Avi, Simon, Attila E., Steller, Manfred, Szabó, Gyula M., Ségransan, Damien, Thomas, Nicolas, Udry, Stéphane, Walter, Ingo, Walton, Nicholas
Publikováno v:
A&A 664, A156 (2022)
Context: TOI-2076 is a transiting three-planet system of sub-Neptunes orbiting a bright (G = 8.9 mag), young ($340\pm80$ Myr) K-type star. Although a validated planetary system, the orbits of the two outer planets were unconstrained as only two non-c
Externí odkaz:
http://arxiv.org/abs/2203.03194
Autor:
Gan, Tianjun, Soubkiou, Abderahmane, Wang, Sharon X., Benkhaldoun, Zouhair, Mao, Shude, Artigau, Étienne, Fouqué, Pascal, Giacalone, Steven, Theissen, Christopher A., Aganze, Christian, Collins, Karen A., Shporer, Avi, Barkaoui, Khalid, Ghachoui, Mourad, Howell, Steve B., Lamman, Claire, Demangeon, Olivier D. S., Burdanov, Artem, Cadieux, Charles, Chouqar, Jamila, Collins, Kevin I., Cook, Neil J., Delrez, Laetitia, Demory, Brice-Olivier, Doyon, René, Dransfield, Georgina, Dressing, Courtney D., Ducrot, Elsa, Fan, Jiahao, Garcia, Lionel, Gill, Holden, Gillon, Michaël, Gnilka, Crystal L., Chew, Yilen Gómez Maqueo, Günther, Maximilian N., Henze, Christopher E., Huang, Chelsea X., Jehin, Emmanuel, Jensen, Eric L. N., Lin, Zitao, McCormac, James, Murray, Catriona A., Niraula, Prajwal, Pedersen, Peter P., Pozuelos, Francisco J., Queloz, Didier, Rackham, Benjamin V., Savel, Arjun B., Schanche, Nicole, Schwarz, Richard P., Sebastian, Daniel, Thompson, Samantha, Timmermans, Mathilde, Triaud, Amaury H. M. J., Vezie, Michael, Wells, Robert D., de Wit, Julien, Ricker, George R., Vanderspek, Roland, Latham, David W., Seager, Sara, Winn, Joshua N., Jenkins, Jon M.
We present the discovery of TOI-2136b, a sub-Neptune planet transiting every 7.85 days a nearby M4.5V-type star, identified through photometric measurements from the TESS mission. The host star is located $33$ pc away with a radius of $R_{\ast} = 0.3
Externí odkaz:
http://arxiv.org/abs/2202.10024
Transit Timing Variations (TTVs) is currently the most successful method to determine dynamical masses and orbital elements for Earth-sized transiting planets. Precise mass determination is fundamental to restrict planetary densities and thus infer p
Externí odkaz:
http://arxiv.org/abs/2110.03830
Autor:
Jofré, Emiliano, Petrucci, Romina, Chew, Yilen Gómez Maqueo, Ramírez, Ivan, Saffe, Carlos, Martioli, Eder, Buccino, Andrea, Mašek, Martin, García, Luciano, Canul, Eliab, Gómez, Mercedes
Wide binary stars with similar components hosting planets provide a favorable opportunity for exploring the star-planet chemical connection. We perform a detailed characterization of the solar-type stars in the WASP-160 binary system. No planet has b
Externí odkaz:
http://arxiv.org/abs/2109.04590
Autor:
Niraula, Prajwal, de Wit, Julien, Rackham, Benjamin V., Ducrot, Elsa, Burdanov, Artem, Crossfield, Ian J. M., Van Grootel, Valerie, Murray, Catriona, Garcia, Lionel J., Alonso, Roi, Beard, Corey, Chew, Yilen Gomez Maqueo, Delrez, Laetitia, Demory, Brice-Olivier, Fulton, Benjamin J., Gillon, Michael, Gunther, Maximilian N., Howard, Andrew W., Issacson, Howard, Jehin, Emmanuel, Pedersen, Peter P., Pozuelos, Francisco J., Queloz, Didier, Rebolo-Lopez, Rafael, Sairam, Lalitha, Sebastian, Daniel, Thompson, Samantha, Triaud, Amaury H. M. J.
We report on the discovery of a transiting Earth-sized (0.95$R_\oplus$) planet around an M3.5 dwarf star at 57$\,$pc, K2-315b. The planet has a period of $\sim$3.14 days, i.e. ${\sim}\pi$, with an instellation of 7.45$\,$S$_{\oplus}$. The detection w
Externí odkaz:
http://arxiv.org/abs/2006.07308