Zobrazeno 1 - 5
of 5
pro vyhledávání: '"Olmschenk, Greg"'
Autor:
Yang, Hongjing, Zang, Weicheng, Gould, Andrew, Yee, Jennifer C., Hwang, Kyu-Ha, Christie, Grant, Sumi, Takahiro, Zhang, Jiyuan, Mao, Shude, Albrow, Michael D., Chung, Sun-Ju, Han, Cheongho, Jung, Youn Kil, Ryu, Yoon-Hyun, Shin, In-Gu, Shvartzvald, Yossi, Cha, Sang-Mok, Kim, Dong-Jin, Kim, Hyoun-Woo, Kim, Seung-Lee, Lee, Chung-Uk, Lee, Dong-Joo, Lee, Yongseok, Park, Byeong-Gon, Pogge, Richard W., Drummond, John, Maoz, Dan, McCormick, Jennie, Natusch, Tim, Penny, Matthew T., Zhu, Wei, Bond, Ian A., Abe, Fumio, Barry, Richard, Bennett, David P., Bhattacharya, Aparna, Donachie, Martin, Fujii, Hirosane, Fukui, Akihiko, Hirao, Yuki, Itow, Yoshitaka, Kirikawa, Rintaro, Kondo, Iona, Koshimoto, Naoki, Li, Man Cheung Alex, Matsubara, Yutaka, Muraki, Yasushi, Miyazaki, Shota, Olmschenk, Greg, Ranc, Clément, Rattenbury, Nicholas J., Satoh, Yuki, Shoji, Hikaru, Silva, Stela Ishitani, Suzuki, Daisuke, Tanaka, Yuzuru, Tristram, Paul J., Yamawaki, Tsubasa, Yonehara, Atsunori
Follow-up observations of high-magnification gravitational microlensing events can fully exploit their intrinsic sensitivity to detect extrasolar planets, especially those with small mass ratios. To make followup more uniform and efficient, we develo
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0b8369ebc93a579cbcf6d490b1d4047a
http://arxiv.org/abs/2205.12584
http://arxiv.org/abs/2205.12584
Autor:
Han, Cheongho, Kim, Doeon, Gould, Andrew, Udalski, Andrzej, Bond, Ian A., Bozza, Valerio, Jung, Youn Kil, Albrow, Michael D., Chung, Sun-Ju, Hwang, Kyu-Ha, Ryu, Yoon-Hyun, Shin, In-Gu, Shvartzvald, Yossi, Yee, Jennifer C., Zang, Weicheng, Cha, Sang-Mok, Kim, Dong-Jin, Kim, Seung-Lee, Lee, Chung-Uk, Lee, Dong-Joo, Lee, Yongseok, Park, Byeong-Gon, Pogge, Richard W., Mróz, Przemek, Szymański, Michał K., Skowron, Jan, Poleski, Radosław, Soszyński, Igor, Pietrukowicz, Paweł, Kozłowski, Szymon, Ulaczyk, Krzysztof, Rybicki, Krzysztof A., Iwanek, Patryk, Abe, Fumio, Barry, Richard K., Bennett, David P., Bhattacharya, Aparna, Fujii, Hirosane, Fukui, Akihiko, Hirao, Yuki, Itow, Yoshitaka, Kirikawa, Rintaro, Koshimoto, Naoki, Kondo, Iona, Matsubara, Yutaka, Matsumoto, Sho, Miyazaki, Shota, Muraki, Yasushi, Olmschenk, Greg, Okamura, Arisa, Ranc, Clément, Rattenbury, Nicholas J., Satoh, Yuki, Silva, Stela Ishitani, Sumi, Takahiro, Suzuki, Daisuke, Toda, Taiga, Tristram, Paul J., Vandorou, Aikaterini, Yama, Hibiki
With the aim of finding short-term planetary signals, we investigated the data collected from the high-cadence microlensing surveys. From this investigation, we found four planetary systems with low planet-to-host mass ratios, including OGLE-2017-BLG
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::486f6cb8e315df5186f83df22de5948e
http://arxiv.org/abs/2205.10510
http://arxiv.org/abs/2205.10510
Autor:
Gould, Andrew, Han, Cheongho, Zang, Weicheng, Yang, Hongjing, Hwang, Kyu-Ha, Udalski, Andrzej, Bond, Ian A., Albrow, Michael D., Chung, Sun-Ju, Jung, Youn Kil, Ryu, Yoon-Hyun, Shin, In-Gu, Shvartzvald, Yossi, Yee, Jennifer C., Cha, Sang-Mok, Kim, Dong-Jin, Kim, Hyoun-Woo, Kim, Seung-Lee, Lee, Chung-Uk, Lee, Dong-Joo, Lee, Yongseok, Park, Byeong-Gon, Pogge, Richard W., Mróz, Przemek, Szymański, Michał K., Skowron, Jan, Poleski, Radek, Soszyński, Igor, Pietrukowicz, Paweł, Kozłowski, Szymon, Ulaczyk, Krzysztof, Rybicki, Krzysztof A., Iwanek, Patryk, Wrona, Marcin, Abe, Fumio, Barry, Richard, Bennett, David P., Bhattacharya, Aparna, Fujii, Hirosame, Fukui, Akihiko, Hirao, Yuki, Silva, Stela Ishitani, Kirikawa, Rintaro, Kondo, Iona, Koshimoto, Naoki, Matsubara, Yutaka, Matsumoto, Sho, Miyazaki, Shota, Muraki, Yasushi, Okamura, Arisa, Olmschenk, Greg, Ranc, Clément, Rattenbury, Nicholas J., Satoh, Yuki, Sumi, Takahiro, Suzuki, Daisuke, Toda, Taiga, Tristram, Paul J., Vandorou, Aikaterini, Yama, Hibiki, Beichman, Charles, Bryden, Geoffry, Novati, Sebastiano Calchi, Gaudi, B. Scott, Henderson, Calen B., Penny, MatthewT., Jacklin, Savannah, Stassun, Keivan G.
We complete the analysis of all 2018 prime-field microlensing planets identified by the KMTNet AnomalyFinder. Among the 10 previously unpublished events with clear planetary solutions, 8 are either unambiguously planetary or are very likely to be pla
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d5f7fc6aa4b713f61a6abd7a84360785
Autor:
Han, Cheongho, Gould, Andrew, Bond, Ian A., Jung, Youn Kil, Albrow, Michael D., Chung, Sun-Ju, Hwang, Kyu-Ha, Ryu, Yoon-Hyun, Shin, In-Gu, Shvartzvald, Yossi, Yee, Jennifer C., Zang, Weicheng, Cha, Sang-Mok, Kim, Dong-Jin, Kim, Seung-Lee, Lee, Chung-Uk, Lee, Dong-Joo, Lee, Yongseok, Park, Byeong-Gon, Pogge, Richard W., Kim, Doeon, Abe, Fumio, Barry, Richard K., Bennett, David P., Bhattacharya, Aparna, Fujii, Hirosane, Fukui, Akihiko, Hirao, Yuki, Itow, Yoshitaka, Kirikawa, Rintaro, Koshimoto, Naoki, Kondo, Iona, Matsubara, Yutaka, Matsumoto, Sho, Miyazaki, Shota, Muraki, Yasushi, Olmschenk, Greg, Okamura, Arisa, Ranc, Clément, Rattenbury, Nicholas J., Satoh, Yuki, Silva, Stela Ishitani, Sumi, Takahiro, Suzuki, Daisuke, Toda, Taiga, Tristram, Paul J., Vandorou, Aikaterini, Yama, Hibiki
Publikováno v:
Astronomy & Astrophysics. 662:A70
The high-magnification microlensing event KMT-2021-BLG-1077 exhibits a subtle and complex anomaly pattern in the region around the peak. We analyze the lensing light curve of the event with the aim of revealing the nature of the anomaly. We test vari
Autor:
Miyazaki, Shota, Suzuki, Daisuke, Udalski, Andrzej, Koshimoto, Naoki, Bennett, David P., Sumi, Takahiro, Rattenbury, Nicholas, Cheongho, Han, Abe, Fumio, Barry, Richard K., Bhattacharya, Aparna, Bond, Ian A., Fukui, Akihiko, Fujii, Hirosane, Hirao, Yuki, Silva, Stela Ishitani, Itow, Yoshitaka, Kirikawa, Rintaro, Kondo, Iona, Munford, Brandon, Matsubara, Yutaka, Matsumoto, Sho, Muraki, Yasushi, Okamura, Arisa, Olmschenk, Greg, Ranc, Clément, Satoh, Yuki K., Toda, Taiga, Tristram, Paul J., Yama, Hibiki, Yonehara, Atsunori, Poleski, Radek, Mróz, Przemek, Skowron, Jan, Szymański, Michal K., Soszyński, Igor, Pietrukowicz, Pawel, Kozłowski, Syzmon, Ulaczyk, Krzysztof, Wyrzykowski, Łukasz, HASH(0x5651c9725458), HASH(0x5651c991ba80)
We report the discovery of a sub-Jovian-mass planet, OGLE-2014-BLG-0319Lb. The characteristics of this planet will be added into a future extended statistical analysis of the Microlensing Observations in Astrophysics (MOA) collaboration. The planetar
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::63d35accdfe9f438044669568bb1c3b4