Zobrazeno 1 - 6
of 6
pro vyhledávání: '"Eigmüller, Phillip"'
Autor:
Psaridi, Angelica, Bouchy, François, Lendl, Monika, Akinsanmi, Babatunde, Stassun, Keivan G., Smalley, Barry, Armstrong, David J., Howard, Saburo, Ulmer-Moll, Solène, Grieves, Nolan, Barkaoui, Khalid, Rodriguez, Joseph E., Bryant, Edward M., Suárez, Olga, Guillot, Tristan, Evans, Phil, Attia, Omar, Wittenmyer, Robert A., Yee, Samuel W., Collins, Karen A., Zhou, George, Galland, Franck, Parc, Léna, Udry, Stéphane, Figueira, Pedro, Ziegler, Carl, Mordasini, Christoph, Winn, Joshua N., Seager, Sara, Jenkins, Jon M., Twicken, Joseph D., Brahm, Rafael, Jones, Matías I., Abe, Lyu, Addison, Brett, Briceño, César, Briegal, Joshua T., Collins, Kevin I., Daylan, Tansu, Eigmüller, Phillip, Furesz, Gabor, Guerrero, Natalia M., Hagelberg, Janis, Heitzmann, Alexis, Hounsell, Rebekah, Huang, Chelsea X., Krenn, Andreas, Law, Nicholas M., Mann, Andrew W., McCormac, James, Mékarnia, Djamel, Mounzer, Dany, Nielsen, Louise D., Osborn, Ares, Reinarz, Yared, Sefako, Ramotholo R., Steiner, Michal, Strøm, Paul A., Triaud, Amaury H. M. J., Vanderspek, Roland, Vanzi, Leonardo, Vines, Jose I., Watson, Christopher A., Wright, Duncan J., Zapata, Abner
Publikováno v:
A&A 675, A39 (2023)
While the sample of confirmed exoplanets continues to increase, the population of transiting exoplanets around early-type stars is still limited. These planets allow us to investigate the planet properties and formation pathways over a wide range of
Externí odkaz:
http://arxiv.org/abs/2303.15080
Autor:
Jackson, David G., Watson, Christopher A., de Mooij, Ernst J. W., Acton, Jack S., Alves, Douglas R., Anderson, David R., Armstrong, David J., Bayliss, Daniel, Belardi, Claudia, Bouchy, François, Bryant, Edward M., Burleigh, Matthew R., Casewell, Sarah L., Costes, Jean C., Eigmüller, Phillip, Goad, Michael R., Gill, Samuel, Gillen, Edward, Günther, Maximilian N., Hawthorn, Faith, Henderson, Beth A., Jackman, James A. G., Jenkins, James S., Lendl, Monika, Kendall, Alicia, McCormac, James, Moyano, Maximiliano, Nielsen, Louise. D., Osborn, Ares, Sefako, Ramotholo R., Smith, Alexis M. S., Tilbrook, Rosanna H., Turner, Oliver, Udry, Stéphane, Vines, Jose I., West, Richard G., Wheatley, Peter J., Worters, Hannah
We report the discovery of three new hot Jupiters with the Next Generation Transit Survey (NGTS) as well as updated parameters for HATS-54b, which was independently discovered by NGTS. NGTS-23b, NGTS-24b and NGTS-25b have orbital periods of 4.076, 3.
Externí odkaz:
http://arxiv.org/abs/2211.01044
Autor:
Acton, Jack S., Goad, Michael R., Burleigh, Matthew R., Casewell, Sarah L., Breytenbach, Hannes, Nielsen, Louise D., Smith, Gareth, Anderson, David R., Battley, Matthew P., Bayliss, Daniel, Bouchy, François, Bryant, Edward M., Csizmadia, Szilárd, Eigmüller, Phillip, Gill, Samuel, Gillen, Edward, Grieves, Nolan, Günther, Maximilian N., Henderson, Beth A., Hodgkin, Simon T., Jackman, James A. G., Jenkins, James S., Lendl, Monika, McCormac, James, Moyano, Maximiliano, Nelson, Richard P., Sefako, Ramotholo R., Smith, Alexis M. S., Stalport, Manu, Thomas, Jessymol K., Tilbrook, Rosanna H., Udry, Stéphane, West, Richard G., Wheatley, Peter J., Worters, Hannah L., Vines, Jose I., Alves, Douglas R.
We present the discovery of NGTS-19b, a high mass transiting brown dwarf discovered by the Next Generation Transit Survey (NGTS). We investigate the system using follow up photometry from the South African Astronomical Observatory, as well as sector
Externí odkaz:
http://arxiv.org/abs/2105.08574
Autor:
Acton, Jack S., Goad, Michael R., Casewell, Sarah L., Vines, José I., Burleigh, Matthew R., Eigmüller, Phillip, Nielsen, Louise D., Gänsicke, Boris T., Bayliss, Daniel, Bouchy, François, Bryant, Edward M., Gill, Samuel, Gillen, Edward, Günther, Maximilian N., Jenkins, James S., McCormac, James, Moyano, Maximiliano, Raynard, Liam R., Tilbrook, Rosanna H., Udry, Stéphane, Watson, Christopher A., West, Richard G., Wheatley, Peter J.
We present the discovery of NGTS J0930-18, an extreme mass ratio eclipsing M-dwarf binary system with an early M-dwarf primary and a late M-dwarf secondary close to the hydrogen burning limit. Global modelling of photometry and radial velocities reve
Externí odkaz:
http://arxiv.org/abs/2008.07354
Autor:
Acton, Jack S., Goad, Michael R., Raynard, Liam, Casewell, Sarah L., Jackman, James A. G., Alexander, Richard D., Anderson, David R., Bayliss, Daniel, Bryant, Edward M., Burleigh, Matthew R., Belardi, Claudia, Cooke, Benjamin F., Eigmüller, Phillip, Gill, Samuel, Jenkins, James S., Lendl, Monika, Louden, Tom, McCormac, James, Moyano, Maximiliano, Nielsen, Louise D., Tilbrook, Rosanna H., Udry, Stéphane, Watson, Christopher A., West, Richard G., Wheatley, Peter J., Vines, Jose I.
We present the discovery of NGTS J214358.5-380102, an eccentric M-dwarf binary discovered by the Next Generation Transit Survey. The system period of 7.618 days is greater than many known eclipsing M-dwarf binary systems. Its orbital eccentricity of
Externí odkaz:
http://arxiv.org/abs/2003.14314
Autor:
Jackson, David G, Watson, Christopher A, de Mooij, Ernst J W, Acton, Jack S, Alves, Douglas R, Anderson, David R, Armstrong, David J, Bayliss, Daniel, Belardi, Claudia, Bouchy, François, Bryant, Edward M, Burleigh, Matthew R, Casewell, Sarah L, Costes, Jean C, Eigmüller, Phillip, Goad, Michael R, Gill, Samuel, Gillen, Edward, Günther, Maximilian N, Hawthorn, Faith
Publikováno v:
Monthly Notices of the Royal Astronomical Society; Feb2023, Vol. 518 Issue 4, p4845-4860, 16p
