Zobrazeno 1 - 10
of 781
pro vyhledávání: '"Berlind, P."'
This paper considers how heterogeneous multi-agent teams can leverage their different capabilities to mutually improve individual agent performance. We present Capability-Augmenting Tasks (CATs), which encode how agents can augment their capabilities
Externí odkaz:
http://arxiv.org/abs/2409.09285
Autor:
Jenkins, Sydney, Vanderburg, Andrew, Bieryla, Allyson, Latham, David W., Badenas-Agusti, Mariona, Berlind, Perry, Blouin, Simon, Buchhave, Lars A., Calkins, Michael L., Esquerdo, Gilbert A., Viaña, Javier
Over a quarter of white dwarfs have photospheric metal pollution, which is evidence for recent accretion of exoplanetary material. While a wide range of mechanisms have been proposed to account for this pollution, there are currently few observationa
Externí odkaz:
http://arxiv.org/abs/2406.18638
Autor:
Šubjak, Ján, Latham, David W., Quinn, Samuel N., Berlind, Perry, Calkins, Michael L., Esquerdo, Gilbert A., Brahm, Rafael, Guenther, Eike, Janík, Jan, Kabáth, Petr, Vanzi, Leonardo, Caballero, José A., Jenkins, Jon M., Mireles, Ismael, Seager, Sara, Shporer, Avi, Striegel, Stephanie, Winn, Joshua N.
Publikováno v:
A&A 688, A120 (2024)
The present study reports the confirmation of BD-14 3065b, a transiting planet/brown dwarf in a triple-star system, with a mass near the deuterium burning boundary. BD-14 3065b has the largest radius observed within the sample of giant planets and br
Externí odkaz:
http://arxiv.org/abs/2403.12311
Autor:
Pass, Emily K., Charbonneau, David, Latham, David W., Berlind, Perry, Calkins, Michael L., Esquerdo, Gilbert A., Mink, Jessica
Fully convective M dwarfs typically remain rapidly rotating and magnetically active for billions of years, followed by an abrupt and mass-dependent transition to slow rotation and quiescence. A robust understanding of this process is complicated by d
Externí odkaz:
http://arxiv.org/abs/2401.10167
Autor:
Bieryla, Allyson, Zhou, George, García-Mejía, Juliana, Farnington, Tyler R., Latham, David W., Carter, Brad, Dong, Jiayin, Huang, Chelsea X., Murphy, Simon J., Shporer, Avi, Collins, Karen A., Quinn, Samuel N., Everett, Mark E., Buchhave, Lars A., Tronsgaard, René, Charbonneau, David, Johnson, Marshall C., Esquerdo, Gilbert A., Calkins, Michael, Berlind, Perry, Jenkins, Jon M., Ricker, George R., Seager, Sara, Winn, Joshua N., Barclay, Thomas, Mireles, Ismael, Paegert, Martin, Twicken, Joseph D.
We report the discovery of TOI-4641b, a warm Jupiter transiting a rapidly rotating F-type star with a stellar effective temperature of 6560 K. The planet has a radius of 0.73 $R_{Jup}$, a mass smaller than 3.87 $M_{Jup}$ $(3\sigma)$, and a period of
Externí odkaz:
http://arxiv.org/abs/2312.03971
Autor:
Carleo, I., Malavolta, L., Desidera, S., Nardiello, D., Wang, S., Turrini, D., Lanza, A. F., Baratella, M., Marzari, F., Benatti, S., Biazzo, K., Bieryla, A., Brahm, R., Bonavita, M., Collins, K. A., Hellier, C., Locci, D., Hobson, M. J., Maggio, A., Mantovan, G., Pinamonti, S. Messina M., Rodriguez, J. E., Sozzetti, A., Stassun, K., Wang, X. Y., Ziegler, C., Damasso, M., Giacobbe, P., Murgas, F., Parviainen, H., Andreuzzi, G., Barkaoui, K., Berlind, P., Bignamini, A., Borsa, F., Briceño, C., Brogi, M., Cabona, L., Calkins, M. L., Capuzzo-Dolcetta, R., Cecconi, M., Colon, K. D., Cosentino, R., Dragomir, D., Esquerdo, G. A., Henning, T., Ghedina, A., Goeke, R. F., Gratton, R., Horta, F. Grau, Gupta, A. F., Jenkins, J. M., Jordán, A., Knapic, C., Latham, D. W., Mireles, I., Law, N., Lorenzi, V., Lund, M. B., Maldonado, J., Mann, A. W., Molinari, E., Pallé, E., Paegert, M., Pedani, M., Quinn, S. N., Scandariato, G., Seager, S., Winn, J. N., Wohler, B., Zingales, T.
Context. Different theories have been developed to explain the origins and properties of close-in giant planets, but none of them alone can explain all of the properties of the warm Jupiters (WJs, Porb = 10 - 200 days). One of the most intriguing cha
Externí odkaz:
http://arxiv.org/abs/2311.11903
Autor:
Porras-Valverde, Antonio J., Forbes, John C., Somerville, Rachel S., Stevens, Adam R. H., Holley-Bockelmann, Kelly, Berlind, Andreas A., Genel, Shy
Semi-analytic models (SAMs) systematically predict higher stellar-mass scatter at a given halo mass than hydrodynamical simulations and most empirical models. Our goal is to investigate the physical origin of this scatter by exploring modifications t
Externí odkaz:
http://arxiv.org/abs/2310.11507
Autor:
Yoshida, Stephanie, Vissapragada, Shreyas, Latham, David W., Bieryla, Allyson, Thorngren, Daniel P., Eastman, Jason D., López-Morales, Mercedes, Barkaoui, Khalid, Beichmam, Charles, Berlind, Perry, Buchave, Lars A., Calkins, Michael L., Ciardi, David R., Collins, Karen A., Cosentino, Rosario, Crossfield, Ian J. M., Dai, Fei, DiTomasso, Victoria, Dowling, Nicholas, Esquerdo, Gilbert A., Forés-Toribio, Raquel, Ghedina, Adriano, Goliguzova, Maria V., Golub, Eli, Gonzales, Erica J., Horta, Ferran Grau, Higuera, Jesus, Hoch, Nora, Horne, Keith, Howell, Steve B., Jenkins, Jon M., Klusmeyer, Jessica, Laloum, Didier, Lissauer, Jack J., Logsdon, Sarah E., Malavolta, Luca, Matson, Rachel A., Matthews, Elisabeth C., McLeod, Kim K., Medina, Jennifer V., Muñoz, Jose A., Osborn, Hugh P., Safonov, Boris, Schlieder, Joshua, Schmidt, Michael, Schweiker, Heidi, Seager, Sara, Sozzetti, Alessandro, Srdoc, Gregor, Stefánsson, Guđmundur, Strakhov, Ivan A., Striegel, Stephanie, Villaseñor, Joel, Winn, Joshua N.
We present the discovery of TOI-1420b, an exceptionally low-density ($\rho = 0.08\pm0.02$ g cm$^{-3}$) transiting planet in a $P = 6.96$ day orbit around a late G dwarf star. Using transit observations from TESS, LCOGT, OPM, Whitin, Wendelstein, OAUV
Externí odkaz:
http://arxiv.org/abs/2309.09945
Autor:
Pass, Emily K, Winters, Jennifer G, Charbonneau, David, Irwin, Jonathan M, Latham, David W, Berlind, Perry, Calkins, Michael L, Esquerdo, Gilbert A, Mink, Jessica
Cold Jovian planets play an important role in sculpting the dynamical environment in which inner terrestrial planets form. The core accretion model predicts that giant planets cannot form around low-mass M dwarfs, although this idea has been challeng
Externí odkaz:
http://arxiv.org/abs/2305.19357
Autor:
Incha, Elyse, Vanderburg, Andrew, Jacobs, Tom, LaCourse, Daryll, Bieryla, Allyson, Pass, Emily, Howell, Steve B., Berlind, Perry, Calkins, Michael, Esquerdo, Gilbert, Latham, David W., Mann, Andrew W.
The Kepler space telescope was responsible for the discovery of over 2,700 confirmed exoplanets, more than half of the total number of exoplanets known today. These discoveries took place during both Kepler's primary mission, when it spent 4 years st
Externí odkaz:
http://arxiv.org/abs/2305.18516