A Wide Orbit Exoplanet OGLE-2012-BLG-0838Lb

التفاصيل البيبلوغرافية
العنوان: A Wide Orbit Exoplanet OGLE-2012-BLG-0838Lb
المؤلفون: R., Poleski, D., Suzuki, A., Udalski, X., Xie, C., Yee J., N., Koshimoto, S., Gaudi B., A., Gould, J., Skowron, K., Szymanski M., I., Soszynski, P., Pietrukowicz, S., Kozlowski, L., Wyrzykowski, K., Ulaczyk, F., Abe, K., Barry R., P., Bennett D., A., Bhattacharya, A., Bond I., M., Donachie, H., Fujii, A., Fukui, Y., Itow, Y., Hirao, Y., Kamei, I., Kondo, A., Li M. C., Y., Matsubara, S., Miyazaki, Y., Muraki, M., Nagakane, C., Ranc, J., Rattenbury N., K., Satoh Y., H., Shoji, H., Suematsu, J., Sullivan D., T., Sumi, J., Tristram P., T., Yamakawa, T., Yamawaki, A., Yonehara, C., Han, S., Dong, M., Morzinski K., R., Males J., M., Close L., W., Pogge R., -P., Beaulieu J., -B, Marquette J.
المصدر: Astronomical Journal, Volume 159, Issue 6, id.261, 16 pp. (2020)
سنة النشر: 2019
المجموعة: Astrophysics
مصطلحات موضوعية: Astrophysics - Earth and Planetary Astrophysics
الوصف: We present the discovery of a planet on a very wide orbit in the microlensing event OGLE-2012-BLG-0838. The signal of the planet is well separated from the main peak of the event and the planet-star projected separation is found to be twice larger than the Einstein ring radius, which roughly corresponds to a projected separation of ~4 AU. Similar planets around low-mass stars are very hard to find using any technique other than microlensing. We discuss microlensing model fitting in detail and discuss the prospects for measuring the mass and distance of lens system directly.
Comment: 26 pages, 11 figures
نوع الوثيقة: Working Paper
DOI: 10.3847/1538-3881/ab8a49
URL الوصول: http://arxiv.org/abs/1901.05466
رقم الأكسشن: edsarx.1901.05466
قاعدة البيانات: arXiv
الوصف
DOI:10.3847/1538-3881/ab8a49