Zobrazeno 1 - 10
of 595
pro vyhledávání: '"Gaudi, B. Scott"'
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, Radoslaw, Szymański, Michaeł K., Soszynśki, 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:
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
Autor:
Malpas, Amber, Albrow, Michael D., Yee, Jennifer C., Gould, Andrew, Udalski, Andrzej, Martin, Antonio Herrera, Team, Spitzer, Beichman, Charles A., Bryden, Geoffery, Novati, Sebastiano Calchi, Carey, Sean, Henderson, Calen B., Gaudi, B. Scott, Shvartzvald, Yossi, Zhu, Wei, Collaboration, KMTNet, Cha, Sang-Mok, Chung, Sun-Ju, Han, Cheongho, Hwang, Kyu-Ha, Jung, Youn Kil, Kim, Dong-Jin, Kim, Hyoun-Woo, Kim, Seung-Lee, Lee, Chung-Uk, Lee, Dong-Joo, Lee, Yongseok, Park, Byeong-Gon, Pogge, Richard W., Ryu, Yoon-Hyun, Shin, In-Gu, Zang, Weicheng, Collaboration, OGLE, Iwanek, Patryk, Kozlowski, Szymon, Mróz, Przemek, Pietrukowicz, Pawel, Poleski, Radoslaw, Rybicki, Krzysztof A., Skowron, Jan, Soszyński, Igor, Szymański, Michal K., Ulaczyk, Krzysztof
Publikováno v:
AJ 164 (2022) 102
We report the analysis of microlensing event OGLE-2017-BLG-1038, observed by the Optical Gravitational Lensing Experiment, Korean Microlensing Telescope Network, and Spitzer telescopes. The event is caused by a giant source star in the Galactic Bulge
Externí odkaz:
http://arxiv.org/abs/2302.07497
Autor:
Phillips, Caprice, Wang, Ji, Edwards, Billy, Martinez, Romy Rodriguez, Asnodkar, Anusha Pai, Gaudi, B. Scott
We explore the prospects for Twinkle to determine the atmospheric composition of the nearby terrestrial-like planet LTT 1445 Ab, including the possibility of detecting the potential biosignature ammonia (NH$_{3}$). At a distance of 6.9 pc, this syste
Externí odkaz:
http://arxiv.org/abs/2209.12919
Transiting planet systems offer the best opportunity to measure the masses and radii of a large sample of planets and their host stars. However, relative photometry and radial velocity measurements alone only constrain the density of the host star. T
Externí odkaz:
http://arxiv.org/abs/2209.09266
Autor:
Duck, Alison, Martin, David V., Gill, Sam, Armitage, Tayt, Martínez, Romy Rodríguez, Maxted, Pierre F. L., Sebastian, Daniel, Sethi, Ritika, Swayne, Matthew I., Cameron, Andrew Collier, Dransfield, Georgina, Gaudi, B. Scott, Gillon, Michael, Hellier, Coel, Kunovac, Vedad, Lovis, Christophe, McCormac, James, Pepe, Francesco A., Pollacco, Don, Sairam, Lalitha, Santerne, Alexandre, Ségransan, Damien, Standing, Matthew R., Southworth, John, Triaud, Amaury H. M. J., Udry, Stephane
M-dwarfs are the most abundant stars in the galaxy and popular targets for exoplanet searches. However, their intrinsic faintness and complex spectra inhibit precise characterisation. We only know of dozens of M-dwarfs with fundamental parameters of
Externí odkaz:
http://arxiv.org/abs/2208.10534