Zobrazeno 1 - 10
of 88
pro vyhledávání: '"Carter, Brad D"'
Autor:
Tristan, Isaiah I., Notsu, Yuta, Kowalski, Adam F., Brown, Alexander, Wisniewski, John P., Osten, Rachel A., Vrijmoet, Eliot H., White, Graeme L., Carter, Brad D., Grady, Carol A., Henry, Todd J., Hinojosa, Rodrigo H., Lomax, Jamie R., Neff, James E., Paredes, Leonardo A., Soutter, Jack
We present light curves and flares from a seven day, multi-wavelength observational campaign of AU Mic, a young and active dM1e star with exoplanets and a debris disk. We report on 73 unique flares between the X-ray to optical data. We use high-time
Externí odkaz:
http://arxiv.org/abs/2304.05692
Autor:
Clark, Jake T., Wright, Duncan J., Wittenmyer, Robert A., Horner, Jonathan, Hinkel, Natalie R., Clerté, Mathieu, Carter, Brad D., Buder, Sven, Hayden, Michael R., Bland-Hawthorn, Joss, Casey, Andrew R., De Silva, Gayandhi M., D'Orazi, Valentina, Freeman, Ken C., Kos, Janez, Lewis, Geraint F., Lin, Jane, Lind, Karin, Martell, Sarah L., Schlesinger, Katharine J., Sharma, Sanjib, Simpson, Jeffrey D., Stello, Dennis, Zucker, Daniel B., Zwitter, Tomaž, Munari, Ulisse, Nordlander, Thomas
Pioneering photometric, astrometric, and spectroscopic surveys are helping exoplanetary scientists better constrain the fundamental properties of stars within our galaxy, and the planets these stars host. In this study, we use the third data release
Externí odkaz:
http://arxiv.org/abs/2111.14883
Autor:
Holt, Timothy R., Horner, Jonathan, Nesvorný, David, King, Rachel, Popescu, Marcel, Carter, Brad D., Tylor, Christopher C. E.
The Jovian Trojans are two swarms of small objects that share Jupiter's orbit, clustered around the leading and trailing Lagrange points, L$_4$ and L$_5$. In this work, we investigate the Jovian Trojan population using the technique of astrocladistic
Externí odkaz:
http://arxiv.org/abs/2103.10967
Autor:
Kane, Stephen R., Yalçınkaya, Selçuk, Osborn, Hugh P., Dalba, Paul A., Nielsen, Louise D., Vanderburg, Andrew, Močnik, Teo, Hinkel, Natalie R., Ostberg, Colby, Esmer, Ekrem Murat, Udry, Stéphane, Fetherolf, Tara, Baştürk, Özgür, Ricker, George R., Vanderspek, Roland, Latham, David W., Seager, Sara, Winn, Joshua N., Jenkins, Jon M., Allart, Romain, Bailey, Jeremy, Bean, Jacob L., Bouchy, Francois, Butler, R. Paul, Campante, Tiago L., Carter, Brad D., Daylan, Tansu, Deleuil, Magali, Diaz, Rodrigo F., Dumusque, Xavier, Ehrenreich, David, Horner, Jonathan, Howard, Andrew W., Isaacson, Howard, Jones, Hugh R. A., Kristiansen, Martti H., Lovis, Christophe, Marcy, Geoffrey W., Marmier, Maxime, O'Toole, Simon J., Pepe, Francesco, Ragozzine, Darin, Ségransan, Damien, Tinney, C. G., Turnbull, Margaret C., Wittenmyer, Robert A., Wright, Duncan J., Wright, Jason T.
Some of the most scientifically valuable transiting planets are those that were already known from radial velocity (RV) surveys. This is primarily because their orbits are well characterized and they preferentially orbit bright stars that are the tar
Externí odkaz:
http://arxiv.org/abs/2007.10995
Autor:
Kane, Stephen R., Dalba, Paul A., Li, Zhexing, Horch, Elliott P., Hirsch, Lea A., Horner, Jonathan, Wittenmyer, Robert A., Howell, Steve B., Everett, Mark E., Butler, R. Paul, Tinney, Christopher G., Carter, Brad D., Wright, Duncan J., Jones, Hugh R. A., Bailey, Jeremy, O'Toole, Simon J.
The sensitivity of radial velocity (RV) surveys for exoplanet detection are extending to increasingly long orbital periods, where companions with periods of several years are now being regularly discovered. Companions with orbital periods that exceed
Externí odkaz:
http://arxiv.org/abs/1904.12931
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Autor:
Wittenmyer, Robert A, Horner, Jonathan, Carter, Brad D, Kane, Stephen R, Plavchan, Peter, Ciardi, David, consortium, the MINERVA-Australis
Super Earths, planets between 5-10 Earth masses, are the most common type of exoplanet known, yet are completely absent from our Solar system. As a result, their detailed properties, compositions, and formation mechanisms are poorly understood. NASA'
Externí odkaz:
http://arxiv.org/abs/1806.09282
Autor:
Kane, Stephen R., Wittenmyer, Robert A., Hinkel, Natalie R., Roy, Arpita, Mahadevan, Suvrath, Dragomir, Diana, Matthews, Jaymie M., Henry, Gregory W., Chakraborty, Abhijit, Boyajian, Tabetha S., Wright, Jason T., Ciardi, David R., Fischer, Debra A., Butler, R. Paul, Tinney, C. G., Carter, Brad D., Jones, Hugh R. A., Bailey, Jeremy, O'Toole, Simon J.
Planets in highly eccentric orbits form a class of objects not seen within our Solar System. The most extreme case known amongst these objects is the planet orbiting HD~20782, with an orbital period of 597~days and an eccentricity of 0.96. Here we pr
Externí odkaz:
http://arxiv.org/abs/1511.08679
Autor:
Jenkins, James S., Díaz, Matias, Jones, Hugh R. A., Butler, R. Paul, Tinney, Chris G., O'Toole, Simon J., Carter, Brad D., Wittenmyer, Robert A., Pinfield, David J.
We report the detection of sixteen binary systems from the Anglo-Australian Planet Search. Solutions to the radial velocity data indicate that the stars have companions orbiting with a wide range of masses, eccentricities and periods. Three of the sy
Externí odkaz:
http://arxiv.org/abs/1507.04749
Autor:
Tuomi, Mikko, Jones, Hugh R. A., Jenkins, James S., Tinney, Chris G., Butler, R. Paul, Vogt, Steve S., Barnes, John R., Wittenmyer, Robert A., O'Toole, Simon, Horner, Jonathan, Bailey, Jeremy, Carter, Brad D., Wright, Duncan J., Salter, Graeme S., Pinfield, David
The abilities of radial velocity exoplanet surveys to detect the lowest-mass extra-solar planets are currently limited by a combination of instrument precision, lack of data, and "jitter". Jitter is a general term for any unknown features in the nois
Externí odkaz:
http://arxiv.org/abs/1212.4277