Zobrazeno 1 - 10
of 197
pro vyhledávání: '"Lòpez, Eric"'
Autor:
Cereceda-López, Eric, De Corato, Marco, Pagonabarraga, Ignacio, Meng, Fanlong, Tierno, Pietro, Ortiz-Ambriz, Antonio
The effect of curvature and how it induces and enhances the transport of colloidal particles driven through narrow channels represent an unexplored research avenue. Here we combine experiments and simulations to investigate the dynamics of magnetical
Externí odkaz:
http://arxiv.org/abs/2409.07661
Autor:
Nabbie, Emma, Huang, Chelsea X., Burt, Jennifer A., Armstrong, David J., Mamajek, Eric E., Adibekyan, Vardan, Sousa, Sérgio G., Lopez, Eric D., Thorngren, Daniel P., Fernández, Jorge, Li, Gongjie, Jenkins, James S., Vines, Jose I., da Silva, João Gomes, Wittenmyer, Robert A., Bayliss, Daniel, Briceño, César, Collins, Karen A., Dumusque, Xavier, Horne, Keith D., Keniger, Marcelo F., Law, Nicholas, Lillo-Box, Jorge, Liu, Shang-Fei, Mann, Andrew W., Nielsen, Louise Dyregaard, Osborn, Ares, Relles, Howard M., Rodrigues, José J., Bell, Juan, Srdoc, Gregor, Stockdale, Chris, Strøm, Paul A., Gardner-Watkins, Cristilyn N., Wheatley, Peter J., Wright, Duncan J., Zhou, George, Ziegler, Carl, Ricker, George R., Seager, Sara, Vanderspek, Roland, Winn, Joshua W., Jenkins, Jon M., Fausnaugh, Michael, Kunimoto, Michelle, Osborn, Hugh P., Quinn, Samuel N., Wohler, Bill
The recent discoveries of Neptune-sized ultra-short period planets (USPs) challenge existing planet formation theories. It is unclear whether these residents of the Hot Neptune Desert have similar origins to smaller, rocky USPs, or if this discrete p
Externí odkaz:
http://arxiv.org/abs/2407.04225
Autor:
Quintana, Elisa V., Gilbert, Emily A., Barclay, Thomas, Silverstein, Michele L., Schlieder, Joshua E., Cloutier, Ryan, Quinn, Samuel N., Rodriguez, Joseph E., Vanderburg, Andrew, Hord, Benjamin J., Louie, Dana R., Ostberg, Colby, Kane, Stephen R., Hoffman, Kelsey, Rowe, Jason F., Arney, Giada N., Saxena, Prabal, Richardson, Taran, Clement, Matthew S., Kartvedt, Nicholas M., Adams, Fred C., Alfred, Marcus, Berger, Travis, Bieryla, Allyson, Bonney, Paul, Boyd, Patricia, Cadieux, Charles, Caldwell, Douglas, Ciardi, David R., Charbonneau, David, Collins, Karen A., Colon, Knicole D., Conti, Dennis M., Di Sora, Mario, Domagal-Goldman, Shawn, Dotson, Jessie, Fauchez, Thomas, Günther, Maximilian N., Hedges, Christina, Isopi, Giovanni, Kohler, Erika, Kopparapu, Ravi, Kostov, Veselin B., Larsen, Jeffrey A., Lopez, Eric, Mallia, Franco, Mandell, Avi, Mullally, Susan E., Paudel, Rishi R., Powell, Brian P., Ricker, George R., Safonov, Boris S., Schwarz, Richard P., Sefako, Ramotholo, Stassun, Keivan G., Wilson, Robert, Winn, Joshua N., Vanderspek, Roland K.
We report the detection and validation of two planets orbiting TOI-2095 (TIC 235678745). The host star is a 3700K M1V dwarf with a high proper motion. The star lies at a distance of 42 pc in a sparsely populated portion of the sky and is bright in th
Externí odkaz:
http://arxiv.org/abs/2304.09189
Autor:
Krishnamurthy, Vigneshwaran, Hirano, Teruyuki, Gaidos, Eric, Sato, Bunei, Kopparapu, Ravi, Barclay, Thomas, Garcia-Sage, Katherine, Harakawa, Hiroki, Hodapp, Klaus, Jacobson, Shane, Konishi, Mihoko, Kotani, Takayuki, Kudo, Tomoyuki, Kurokawa, Takashi, Kuzuhara, Masayuki, Lopez, Eric, Nishikawa, Jun, Omiya, Masashi, Schlieder, Joshua E., Serizawa, Takuma, Tamura, Motohide, Ueda, Akitoshi, Vievard, Sebastien
\textit{Kepler} showed a paucity of planets with radii of 1.5 - 2 $\mathrm R_{\oplus}$ around solar mass stars but this radius-gap has not been well studied for low-mass star planets. Energy-driven escape models like photoevaporation and core-powered
Externí odkaz:
http://arxiv.org/abs/2302.01479
Autor:
Barclay, Thomas, Sheppard, Kyle B., Latouf, Natasha, Mandell, Avi M., Quintana, Elisa V., Gilbert, Emily A., Liuzzi, Giuliano, Villanueva, Geronimo L., Arney, Giada, Brande, Jonathan, Colón, Knicole D., Covone, Giovanni, Crossfield, Ian J. M., Damiano, Mario, Domagal-Goldman, Shawn D., Fauchez, Thomas J., Fiscale, Stefano, Gallo, Francesco, Hedges, Christina L., Hu, Renyu, Kite, Edwin S., Koll, Daniel, Kopparapu, Ravi K., Kostov, Veselin B., Kreidberg, Laura, Lopez, Eric D., Mang, James, Morley, Caroline V., Mullally, Fergal, Mullally, Susan E., Pidhorodetska, Daria, Schlieder, Joshua E., Vega, Laura D., Youngblood, Allison, Zieba, Sebastian
We present observations of the 1.35+/-0.07 Earth-radius planet L 98-59 c using Wide Field Camera~3 on the Hubble Space Telescope. L 98-59 is a nearby (10.6 pc), bright (H=7.4 mag), M3V star that harbors three small, transiting planets. As one of the
Externí odkaz:
http://arxiv.org/abs/2301.10866
The hot Saturn population exhibits a boundary in mass-radius space, such that no planets are observed at a density less than $\sim$0.1 g cm$^{-3}$. Yet, planet interior structure models can readily construct such objects as the natural result of radi
Externí odkaz:
http://arxiv.org/abs/2211.11770
Autor:
Renaud, Joe P., Lopez, Eric, Brande, Jonathan, Cruz-Arce, Carlos E., Kelahan, Cameron, Susemiehl, Nicholas, Cristy, Dylan, Hostetter, Carl, Moore, Michael Dane, Patel, Apexa, Mandell, Avi M.
Publikováno v:
Res. Notes AAS, 6: 185 (2022)
The Exoplanet Modeling and Analysis Center (EMAC) at NASA Goddard Space Flight Center is a web-based catalog, repository, and integration platform for modeling and analysis resources focused on the study of exoplanet characteristics and environments.
Externí odkaz:
http://arxiv.org/abs/2209.04005
Autor:
Lips, Dominik, Cereceda-López, Eric, Ortiz-Ambriz, Antonio, Tierno, Pietro, Ryabov, Artem, Maass, Philipp
Publikováno v:
Soft Matter, 2022
The flow-driven transport of interacting micron-sized particles occurs in many soft matter systems spanning from the translocation of proteins to moving emulsions in microfluidic devices. Here we combine experiments and theory to investigate the coll
Externí odkaz:
http://arxiv.org/abs/2208.10798
Autor:
Cereceda-López, Eric, Lips, Dominik, Ortiz-Ambriz, Antonio, Ryabov, Artem, Maass, Philipp, Tierno, Pietro
Publikováno v:
Phys. Rev. Lett. 127, 214501 (2021)
Hydrodynamic interactions between fluid-dispersed particles are ubiquitous in soft matter and biological systems and they give rise to intriguing collective phenomena. While it was reported that these interactions can facilitate force-driven particle
Externí odkaz:
http://arxiv.org/abs/2110.05097
Publikováno v:
ApJ 876, 22 (2019)
Short-period sub-Neptunes with substantial volatile envelopes are among the most common type of known exoplanets. However, recent studies of the Kepler population have suggested a dearth of sub-Neptunes on highly irradiated orbits, where they are vul
Externí odkaz:
http://arxiv.org/abs/2105.00142