تقرير
HD 202772A B: A Transiting Hot Jupiter Around A Bright, Mildly Evolved Star In A Visual Binary Discovered By Tess
| العنوان: | HD 202772A B: A Transiting Hot Jupiter Around A Bright, Mildly Evolved Star In A Visual Binary Discovered By Tess |
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| المؤلفون: | Wang, Songhu, Jones, Matias, Shporer, Avi, Fulton, Benjamin J., Paredes, Leonardo A., Trifonov, Trifon, Kossakowski, Diana, Eastman, Jason, Gunther, Maximilian N., Huang, Chelsea X., Millholland, Sarah, Seligman, Darryl, Fischer, Debra, Brahm, Rafael, Wang, Xian-Yu, Cruz, Bryndis, James, Hodari-Sadiki, Addison, Brett, Henry, Todd, Liang, En-Si, Davis, Allen B., Tronsgaard, Rene, Worku, Keduse, Brewer, John, Kurster, Martin, Beichman, Charles A., Bieryla, Allyson, Brown, Timothy M., Christiansen, Jessie L., Ciardi, David R., Collins, Karen A., Esquerdo, Gilbert A., Howard, Andrew W., Isaacson, Howard, Latham, David W., Mazeh, Tsevi, Petigura, Erik A., Quinn, Samuel N., Shahaf, Sahar, Siverd, Robert J., Ricker, George R., Vanderspek, Roland, Seager, Sara, Winn, Joshua N., Jenkins, Jon M., Boyd, Patricia T., Furesz, Gabor, Henze, Christopher, Levine, Alen M., Morris, Robert, Paegert, Martin, Stassun, Keivan G., Ting, Eric B., Vezie, Michael, Laughlin, Gregory |
| سنة النشر: | 2018 |
| المجموعة: | Astrophysics |
| مصطلحات موضوعية: | Astrophysics - Earth and Planetary Astrophysics |
| الوصف: | We report the first confirmation of a hot Jupiter discovered by the Transiting Exoplanet Survey Satellite (TESS) mission: HD 202772A b. The transit signal was detected in the data from TESS Sector 1, and was confirmed to be of planetary origin through radial-velocity measurements. HD 202772A b is orbiting a mildly evolved star with a period of 3.3 days. With an apparent magnitude of V = 8.3, the star is among the brightest known to host a hot Jupiter. Based on the 27days of TESS photometry, and radial velocity data from the CHIRON and HARPS spectrographs, the planet has a mass of 1.008+/-0.074 M_J and radius of 1.562+/-0.053 R_J , making it an inflated gas giant. HD 202772A b is a rare example of a transiting hot Jupiter around a quickly evolving star. It is also one of the most strongly irradiated hot Jupiters currently known. Comment: Submitted to AAS Journal |
| نوع الوثيقة: | Working Paper |
| DOI: | 10.3847/1538-3881/aaf1b7 |
| URL الوصول: | http://arxiv.org/abs/1810.02341 |
| رقم الأكسشن: | edsarx.1810.02341 |
| قاعدة البيانات: | arXiv |
| DOI: | 10.3847/1538-3881/aaf1b7 |
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