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pro vyhledávání: '"Guenther, David A."'
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Autor:
Siwak, Michal, Winiarski, Maciej, Ogloza, Waldemar, Drozdz, Marek, Zola, Stanislaw, Moffat, Anthony F. J., Stachowski, Grzegorz, Rucinski, Slavek M., Cameron, Chris, Matthews, Jaymie M., Weiss, Werner W., Kuschnig, Rainer, Rowe, Jason F., Guenther, David B., Sasselov, Dimitar
Publikováno v:
A&A 618, A79 (2018)
Context. We investigate small-amplitude light variations in FU Ori occurring in timescales of days and weeks. Aims. We seek to determine the mechanisms that lead to these light changes. Methods. The visual light curve of FU Ori gathered by the MOST s
Externí odkaz:
http://arxiv.org/abs/1807.09134
Autor:
Guenther, David A.1 (AUTHOR), Peterson, Kyle1 (AUTHOR), Searcy, Jake1 (AUTHOR), Williams, Brian M.2 (AUTHOR)
Publikováno v:
Accounting Review. Sep2023, Vol. 98 Issue 5, p297-322. 26p. 7 Charts, 3 Graphs.
Autor:
Kipping, David M., Cameron, Chris, Hartman, Joel D., Davenport, James R. A., Matthews, Jaymie M., Sasselov, Dimitar, Rowe, Jason, Siverd, Robert J., Chen, Jingjing, Sandford, Emily, Bakos, Gáspár Á., Jordan, Andres, Bayliss, Daniel, Henning, Thomas, Mancini, Luigi, Penev, Kaloyan, Csubry, Zoltan, Bhatti, Waqas, Bento, Joao Da Silva, Guenther, David B., Kuschnig, Rainer, Moffat, Anthony F. J., Rucinski, Slavek M., Weiss, Werner W.
The analysis of Proxima Centauri's radial velocities recently led Anglada-Escud\'e et al. (2016) to claim the presence of a low mass planet orbiting the Sun's nearest star once every 11.2 days. Although the a-priori probability that Proxima b transit
Externí odkaz:
http://arxiv.org/abs/1609.08718
Autor:
Siwak, Michal, Ogloza, Waldemar, Rucinski, Slavek M., Moffat, Anthony F. J., Matthews, Jaymie M., Cameron, Chris, Guenther, David B., Kuschnig, Rainer, Rowe, Jason F., Sasselov, Dimitar, Weiss, Werner W.
Results of the time variability monitoring of the two classical T Tauri stars, RU Lup and IM Lup, are presented. Three photometric data sets were utilised: (1) simultaneous (same field) MOST satellite observations over four weeks in each of the years
Externí odkaz:
http://arxiv.org/abs/1512.01992
Publikováno v:
In European Journal of Radiology Open 2021 8
Spectroscopy, MOST Photometry, and Interferometry of MWC 314: Is it an LBV or an interacting binary?
Autor:
Richardson, Noel D., Moffat, Anthony F. J., Maltais-Tariant, Raphaël, Pablo, Herbert, Gies, Douglas R., Saio, Hideyuki, St-Louis, Nicole, Schaefer, Gail, Miroshnichenko, Anatoly S., Farrington, Chris, Aldoretta, Emily J., Artigau, Étienne, Boyajian, Tabetha S., Gordon, Kathryn, Jones, Jeremy, Matson, Rachel, McAlister, Harold A., O'Brien, David, Raghavan, Deepak, Ramiaramanantsoa, Tahina, Ridgway, Stephen T., Scott, Nic, Sturmann, Judit, Sturmann, Laszlo, Brummelaar, Theo ten, Thomas, Joshua D., Turner, Nils, Vargas, Norm, Zharikov, Sergey, Matthews, Jaymie, Cameron, Chris, Guenther, David, Kuschnig, Rainer, Rowe, Jason, Rucinski, Slavek, Sasselov, Dimitar, Weiss, Werner
MWC 314 is a bright candidate luminous blue variable that resides in a fairly close binary system, with an orbital period of 60.753$\pm$0.003 d. We observed MWC 314 with a combination of optical spectroscopy, broad-band ground- and space-based photom
Externí odkaz:
http://arxiv.org/abs/1510.00324
Autor:
Pablo, Herbert, Richardson, Noel D., Moffat, Anthony F. J., Corcoran, Michael, Shenar, Tomer, Benvenuto, Omar, Fuller, Jim, Naze, Yael, Hoffman, Jennifer L., Miroshnichenko, Anatoly, Apellaniz, Jesus Maiz, Evans, Nancy, Eversberg, Thomas, Gayley, Ken, Gull, Ted, Hamaguch, Kenji, Hamann, Wolf-Rainer, Henrichs, Huib, Hole, Tabetha, Ignace, Richard, Iping, Rosina, Lauer, Jennifer, Leutenegger, Maurice, Lomax, Jamie, Nichols, Joy, Oskinova, Lida, Owocki, Stan, Pollock, Andy, Russell, Christopher M. P., Waldron, Wayne, Buil, Christian, Garrel, Thierry, Graham, Keith, Heathcote, Bernard, Lemoult, Thierry, Li, Dong, Mauclaire, Benjamin, Potter, Mike, Ribeiro, Jose, Matthews, Jaymie, Cameron, Chris, Guenther, David, Kuschnig, Rainer, Rowe, Jason, Rucinski, Slavek, Sasselov, Dimitar, Weiss, Werner
Publikováno v:
ApJ, 809, 134 (11p,2015)
We report on both high-precision photometry from the MOST space telescope and ground-based spectroscopy of the triple system delta Ori A consisting of a binary O9.5II+early-B (Aa1 and Aa2) with P = 5.7d, and a more distant tertiary (O9 IV P > 400 yrs
Externí odkaz:
http://arxiv.org/abs/1504.08002
Autor:
Vanderburg, Andrew, Montet, Benjamin T., Johnson, John Asher, Buchhave, Lars A., Zeng, Li, Pepe, Francesco, Cameron, Andrew Collier, Latham, David W., Molinari, Emilio, Udry, Stephane, Lovis, Christophe, Matthews, Jaymie M., Cameron, Chris, Law, Nicholas, Bowler, Brendan P., Angus, Ruth, Baranec, Christoph, Bieryla, Allyson, Boschin, Walter, Charbonneau, David, Cosentino, Rosario, Dumusque, Xavier, Figueira, Pedro, Guenther, David B., Harutyunyan, Avet, Hellier, Coel, Kuschnig, Rainer, Lopez-Morales, Mercedes, Mayor, Michel, Micela, Giusi, Moffat, Anthony F. J., Pedani, Marco, Phillips, David F., Piotto, Giampaolo, Pollacco, Don, Queloz, Didier, Rice, Ken, Riddle, Reed, Rowe, Jason F., Rucinski, Slavek M., Sasselov, Dimitar, Segransan, Damien, Sozzetti, Alessandro, Szentgyorgyi, Andrew, Watson, Chris, Weiss, Werner W.
We report the first planet discovery from the two-wheeled Kepler (K2) mission: HIP 116454 b. The host star HIP 116454 is a bright (V = 10.1, K = 8.0) K1-dwarf with high proper motion, and a parallax-based distance of 55.2 +/- 5.4 pc. Based on high-re
Externí odkaz:
http://arxiv.org/abs/1412.5674
Autor:
Guenther, David A.
Publikováno v:
Classical Philology; Jul2024, Vol. 119 Issue 3, p421-426, 6p