Zobrazeno 1 - 10
of 8 153
pro vyhledávání: '"B Scott"'
Autor:
Crepp, Justin R., Crass, Jonathan, Bechter, Andrew J., Sands, Brian L., Ketterer, Ryan, King, David, Kopon, Derek, Hamper, Randall, Engstrom, Matthew, Smous, James E., Bechter, Eric B., Harris, Robert, Johnson, Marshall C., Baggett, Nicholas, Dulz, Shannon, Vansickle, Michael, Conrad, Al, Ertel, Steve, Gaudi, B. Scott, Hinz, Philip, Kuchner, Marc, Montoya, Manny, Onuma, Eleanya, Ott, Melanie, Pogge, Richard, Rahmer, Gustavo, Reynolds, Robert, Schwab, Christian, Stapelfeldt, Karl, Thomes, Joseph, Vaz, Amali, Wang, Ji, Woodward, Charles E.
Precision radial velocity (RV) spectrographs that use adaptive optics (AO) show promise to advance telescope observing capabilities beyond those of seeing-limited designs. We are building a spectrograph for the Large Binocular Telescope (LBT) named i
Externí odkaz:
http://arxiv.org/abs/2412.06982
Autor:
Basinger, Connor, Pinsonneault, Marc, Bastelberger, Sandra T., Gaudi, B. Scott, Domagal-Goldman, Shawn
Stellar evolution theory predicts that the Sun was fainter in the past, which can pose difficulties for understanding Earth's climate history. One proposed solution to this Faint Young Sun problem is a more luminous Sun in the past. In this paper, we
Externí odkaz:
http://arxiv.org/abs/2409.03823
Autor:
Zhang, Keming, Zang, Weicheng, El-Badry, Kareem, Lu, Jessica R., Bloom, Joshua S., Agol, Eric, Gaudi, B. Scott, Konopacky, Quinn, LeBaron, Natalie, Mao, Shude, Terry, Sean
Publikováno v:
Nat Astron (2024)
Terrestrial planets born beyond 1-3 AU have been theorized to avoid being engulfed during the red-giant phases of their host stars. Nevertheless, only a few gas-giant planets have been observed around white dwarfs (WDs) -- the end product left behind
Externí odkaz:
http://arxiv.org/abs/2409.02157
Autor:
Hu, Zhecheng, Zhu, Wei, Gould, Andrew, Udalski, Andrzej, Sumi, Takahiro, Chen, Ping, Novati, Sebastiano Calchi, Yee, Jennifer C., Beichman, Charles A., Bryden, Geoffery, Carey, Sean, Fausnaugh, Michael, Gaudi, B. Scott, Henderson, Calen B., Shvartzvald, Yossi, Wibking, Benjamin, Mróz, Przemek, Skowron, Jan, Poleski, Radosław, Szymański, Michał K., Soszyński, Igor, Pietrukowicz, Paweł, Kozłowski, Szymon, Ulaczyk, Krzysztof, Rybicki, Krzysztof A., Iwanek, Patryk, Wrona, Marcin, Gromadzki, Mariusz, Abe, Fumio, Barry, Richard, Bennett, David P., Bhattacharya, Aparna, Bond, Ian A., Fujii, Hirosane, Fukui, Akihiko, Hamada, Ryusei, Hirao, Yuki, Silva, Stela Ishitani, Itow, Yoshitaka, Kirikawa, Rintaro, Koshimoto, Naoki, Matsubara, Yutaka, Miyazaki, Shota, Muraki, Yasushi, Olmschenk, Greg, Ranc, Clément, Rattenbury, Nicholas J., Satoh, Yuki, Suzuki, Daisuke, Tomoyoshi, Mio, Tristram, Paul. J., Vandorou, Aikaterini, Yama, Hibiki, Yamashita, Kansuke
We present the analysis of the microlensing event OGLE-2015-BLG-0845, which was affected by both the microlensing parallax and xallarap effects. The former was detected via the simultaneous observations from the ground and Spitzer, and the latter was
Externí odkaz:
http://arxiv.org/abs/2404.13031
Autor:
Amy L. Toth, Christopher D. R. Wyatt, Rick E. Masonbrink, Katherine S. Geist, Ryan Fortune, Sarah B. Scott, Emeline Favreau, Sandra M. Rehan, Seirian Sumner, Mary M. Gardiner, Frances S. Sivakoff
Publikováno v:
BMC Genomics, Vol 25, Iss 1, Pp 1-13 (2024)
Abstract Background The common Eastern bumble bee Bombus impatiens is native to North America and is the main commercially reared pollinator in the Americas. There has been extensive research on this species related to its social biology, applied pol
Externí odkaz:
https://doaj.org/article/d3eaa7d32c304cd5b06b4659e06a3c91
Autor:
Petz, Sydney, Johnson, Marshall C., Asnodkar, Anusha Pai, Wang, Ji, Gaudi, B. Scott, Henning, Thomas, Keles, Engin, Molaverdikhani, Karan, Poppenhaeger, Katja, Scandariato, Gaetano, Shkolnik, Evgenya K., Sicilia, Daniela, Strassmeier, Klaus G., Yan, Fei
Most ultra hot Jupiters (UHJs) show evidence of temperature inversions, in which temperature increases with altitude over a range of pressures. Temperature inversions can occur when there is a species that absorbs the stellar irradiation at a relativ
Externí odkaz:
http://arxiv.org/abs/2310.09352
Autor:
Martínez, Romy Rodríguez, Martin, David V., Gaudi, B. Scott, Schulze, Joseph G., Asnodkar, Anusha Pai, Boley, Kiersten M., Ballard, Sarah
We investigate and compare the composition of M-dwarf planets in systems with only one known planet (``singles") to those residing in multi-planet systems (``multis") and the fundamental properties of their host stars. We restrict our analysis to pla
Externí odkaz:
http://arxiv.org/abs/2307.13034
Autor:
Grunblatt, Samuel K., Wilson, Robert F., Winter, Andrew, Gaudi, B. Scott, Huber, Daniel, Yahalomi, Daniel A., Bellini, Andrea, Claytor, Zachary R., Palomera, Jorge Martinez, Barclay, Thomas, Fu, Guangwei, Price-Whelan, Adrian
Despite multiple previous searches, no transiting planets have yet been identified within a globular cluster. This is believed to be due to a combination of factors: the low metallicities of most globular clusters suggests that there is significantly
Externí odkaz:
http://arxiv.org/abs/2306.10647
Autor:
Wehrle, Ann E., Carini, Michael, Wiita, Paul J., Pepper, Joshua, Gaudi, B. Scott, Pogge, Richard W., Stassun, Keivan G., Villaneuva, Jr., Steven
We present second observations by K2 of OJ~287 and 7 other $\gamma$-ray AGNs obtained in 2017-2018, second and third observations of the lobe-dominated, steep spectrum quasar 3C~207, and observations of 9 additional blazars not previously observed wi
Externí odkaz:
http://arxiv.org/abs/2305.17060
Autor:
Stephan, Alexander P., Gaudi, B. Scott
For the majority of short period exoplanets transiting massive stars with radiative envelopes, the spin angular momentum of the host star is greater than the planetary orbital angular momentum. In this case, the orbits of the planets will undergo nod
Externí odkaz:
http://arxiv.org/abs/2304.09890