Zobrazeno 1 - 10
of 1 092
pro vyhledávání: '"Schmidt, Stephen"'
Exoplanet systems are thought to evolve on secular timescales over billions of years. This evolution is impossible to directly observe on human timescales in most individual systems. While the availability of accurate and precise age inferences for i
Externí odkaz:
http://arxiv.org/abs/2407.04765
Autor:
Wood, Mackenna L., Mann, Andrew W., Barber, Madyson G., Bush, Jonathan L., Milburn, Reilly P., Thao, Pa Chia, Schmidt, Stephen P., Tofflemire, Benjamin M., Kraus, Adam L.
The dispersed remnants of stellar nurseries, stellar associations provide unparalleled samples of coeval stars critical for studies of stellar and planetary formation and evolution. The Carina Stellar Association is one of the closest stellar associa
Externí odkaz:
http://arxiv.org/abs/2310.16883
Autor:
Schmidt, Stephen P., Schlaufman, Kevin C., Ding, Keyi, Grunblatt, Samuel K., Carmichael, Theron, Bieryla, Allyson, Rodriguez, Joseph E., Schulte, Jack, Vowell, Noah, Zhou, George, Quinn, Samuel N., Yee, Samuel W., Winn, Joshua N., Hartman, Joel D., Latham, David W., Caldwell, Douglas A., Fausnaugh, M. M., Hedges, Christina, Jenkins, Jon M., Osborn, Hugh P., Seager, S.
While secondary mass inferences based on single-lined spectroscopic binary (SB1) solutions are subject to $\sin{i}$ degeneracies, this degeneracy can be lifted through the observations of eclipses. We combine the subset of Gaia Data Release (DR) 3 SB
Externí odkaz:
http://arxiv.org/abs/2310.07936
Autor:
Wood, Mackenna L., Mann, Andrew W., Barber, Madyson G., Bush, Jonathan L., Kraus, Adam L., Tofflemire, Benjamin M., Vanderburg, Andrew, Newton, Elisabeth R., Feiden, Gregory A., Zhou, George, Bouma, Luke G., Quinn, Samuel N., Armstrong, David J., Osborn, Ares, Adibekyan, Vardan, Mena, Elisa Delgado, Sousa, Sergio G., Gagné, Jonathan, Fields, Matthew J., Milburn, Reilly P., Thao, Pa Chia, Schmidt, Stephen P., Gnilka, Crystal L., Howell, Steve B., Law, Nicholas M., Ziegler, Carl, Briceño, César, Ricker, George R., Vanderspek, Roland, Latham, David W., Seager, Sara, Winn, Joshua N., Jenkins, Jon M., Schlieder, Joshua E., Osborn, Hugh P., Twicken, Joseph D., Ciardi, David R., Huang, Chelsea X.
We report the discovery and characterization of a nearby (~ 85 pc), older (27 +/- 3 Myr), distributed stellar population near Lower-Centaurus-Crux (LCC), initially identified by searching for stars co-moving with a candidate transiting planet from TE
Externí odkaz:
http://arxiv.org/abs/2212.03266
Autor:
Mann, Andrew W., Wood, Mackenna L., Schmidt, Stephen P., Barber, Madyson G., Owen, James E., Tofflemire, Benjamin M., Newton, Elisabeth R., Mamajek, Eric E., Bush, Jonathan L., Mace, Gregory N., Kraus, Adam L., Thao, Pa Chia, Vanderburg, Andrew, Llama, Joe, Johns-Krull, Christopher M., Prato, L., Stahl, Asa G., Tang, Shih-Yun, Fields, Matthew J., Collins, Karen A., Collins, Kevin I., Gan, Tianjun, Jensen, Eric L. N., Kamler, Jacob, Schwarz, Richard P., Furlan, Elise, Gnilka, Crystal L., Howell, Steve B., Lester, Kathryn V., Owens, Dylan A., Suarez, Olga, Mekarnia, Djamel, Guillot, Tristan, Abe, Lyu, Triaud, Amaury H. M. J., Johnson, Marshall C., Milburn, Reilly P., Rizzuto, Aaron C., Quinn, Samuel N., Kerr, Ronan, Ricker, George R., Vanderspek, Roland, Latham, David W., Seager, Sara, Winn, Joshua N., Jenkins, Jon M., Guerrero, Natalia M., Shporer, Avi, Schlieder, Joshua E., McLean, Brian, Wohler, Bill
Publikováno v:
AJ 163 156 (2022)
Mature super-Earths and sub-Neptunes are predicted to be $\simeq$Jovian radius when younger than 10 Myr. Thus, we expect to find 5-15$R_\oplus$ planets around young stars even if their older counterparts harbor none. We report the discovery and valid
Externí odkaz:
http://arxiv.org/abs/2110.09531
Autor:
Palopoli-Trojani, Kay, Schmidt, Stephen L., Baringer, Karley D., Slotkin, Theodore A., Peters, Jennifer J., Turner, Dennis A., Grill, Warren M.
Publikováno v:
In Brain Stimulation November-December 2023 16(6):1630-1642
Autor:
Schmidt, Stephen J.
Publikováno v:
AEA Papers and Proceedings, 2021 May 01. 111, 107-111.
Externí odkaz:
https://www.jstor.org/stable/27042281
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.