Zobrazeno 1 - 10
of 115
pro vyhledávání: '"Henderson, Calen B"'
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:
Ryu, Yoon-Hyun, Udalski, Andrzej, Yee, Jennifer C., Zang, Weicheng, Shvartzvald, Yossi, Han, Cheongho, Gould, Andrew, Albrow, Michael D., Chung, Sun-Ju, Hwang, Kyu-Ha, Jung, Youn Kil, Shin, In-Gu, Yang, Hongjing, Cha, Sang-Mok, Kim, Dong-Jin, Kim, Seung-Lee, Lee, Chung-Uk, Lee, Dong-Joo, Lee, Yongseok, Park, Byeong-Gon, Pogge, Richard W., Wang, Hanyue, Mróz, Przemek, Szymański, Michał K., Skowron, Jan, Poleski, Radek, Soszyński, Igor, Pietrukowicz, Paweł, Kozłowski, Szymon, Ulaczyk, Krzysztof, Rybicki, Krzysztof A., Iwanek, Patryk, Wrona, Marcin, Beichman, Charles, Bryden, Geoffry, Carey, Sean, Henderson, Calen B., Novati, Sebastiano Calchi, Zhu, Wei, Jacklin, Savannah, Penny, Matthew T.
We complete the analysis of planetary candidates found by the KMT AnomalyFinder for the 2017 prime fields that cover $\sim 13\,{\rm deg}^2$. We report 3 unambiguous planets: OGLE-2017-BLG-0640, OGLE-2017-BLG-1275, and OGLE-2017-BLG-1237. The first tw
Externí odkaz:
http://arxiv.org/abs/2307.13359
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:
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:
http://arxiv.org/abs/2204.04354
Autor:
Shin, In-Gu, Yee, Jennifer C., Hwang, Kyu-Ha, Gould, Andrew, Udalski, Andrzej, Bond, Ian A., Albrow, Michael D., Chung, Sun-Ju, Han, Cheongho, Jung, Youn Kil, Kim, Hyoun Woo, Ryu, Yoon-Hyun, Shvartzvald, Yossi, 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, Radek, Soszyński, Igor, Pietrukowicz, Paweł, Kozłowski, Szymon, Ulaczyk, Krzysztof, Beichman, Charles A., Bryden, Geoffery, Novati, Sebastiano Calchi, Carey, Sean, Gaudi, B. Scott, Henderson, Calen B., Zhu, Wei, 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
OGLE-2016-BLG-1093 is a planetary microlensing event that is part of the statistical $Spitzer$ microlens parallax sample. The precise measurement of the microlens parallax effect for this event, combined with the measurement of finite source effects,
Externí odkaz:
http://arxiv.org/abs/2201.04312
Autor:
Xie, Xiao-Jia, Dong, Subo, Shvartzvald, Yossi, Gould, Andrew, Udalski, Andrzej, Beaulieu, Jean-Philippe, Beichman, Charles, Close, Laird Miller, Henderson, Calen B., Males, Jared R., Marquette, Jean-Baptiste, Morzinski, Katie M., Gelino, Christopher R.
Publikováno v:
RAA, 2021, 21, 303
We constrain the host-star flux of the microlensing planet OGLE-2014-BLG-0676Lb using adaptive optics (AO) images taken by the Magellan and Keck telescopes. We measure the flux of the light blended with the microlensed source to be K = 16.79 +/- 0.04
Externí odkaz:
http://arxiv.org/abs/2112.08030
Autor:
Chen, Tracy X., Schmitz, Marion, Mazzarella, Joseph M., Wu, Xiuqin, van Eyken, Julian C., Accomazzi, Alberto, Akeson, Rachel L., Allen, Mark, Beaton, Rachael, Berriman, G. Bruce, Boyle, Andrew W., Brouty, Marianne, Chan, Ben, Christiansen, Jessie L., Ciardi, David R., Cook, David, D'Abrusco, Raffaele, Ebert, Rick, Frayer, Cren, Fulton, Benjamin J., Gelino, Christopher, Helou, George, Henderson, Calen B., Howell, Justin, Kim, Joyce, Landais, Gilles, Lo, Tak, Loup, Cecile, Madore, Barry, Monari, Giacomo, Muench, August, Oberto, Anais, Ocvirk, Pierre, Peek, Joshua E. G., Perret, Emmanuelle, Pevunova, Olga, Ramirez, Solange V., Rebull, Luisa, Shemmer, Ohad, Smale, Alan, Tam, Raymond, Terek, Scott, Van Orsow, Doug, Vannier, Patricia, Wang, Shin-Ywan
We present an overview of best practices for publishing data in astronomy and astrophysics journals. These recommendations are intended as a reference for authors to help prepare and publish data in a way that will better represent and support scienc
Externí odkaz:
http://arxiv.org/abs/2106.01477
Autor:
Zang, Weicheng, Hwang, Kyu-Ha, Udalski, Andrzej, Wang, Tianshu, Zhu, Wei, Sumi, Takahiro, Yee, Jennifer C., Gould, Andrew, Mao, Shude, Zhang, Xiangyu, 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., Mróz, Przemek, Skowron, Jan, Szymański, Michał K., Soszyński, Igor, Pietrukowicz, Paweł, Kozłowski, Szymon, Ulaczyk, Krzysztof, Rybicki, Krzysztof A., Iwanek, Patryk, Wrona, Marcin, Gromadzki, Mariusz, 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, Beichman, Charles A., Bryden, Geoffery, Novati, Sebastiano Calchi, Carey, Sean, Gaudi, B. Scott, Henderson, Calen B., Johnson, Samson
In order to exhume the buried signatures of "missing planetary caustics" in the KMTNet data, we conducted a systematic anomaly search to the residuals from point-source point-lens fits, based on a modified version of the KMTNet EventFinder algorithm.
Externí odkaz:
http://arxiv.org/abs/2103.11880
Autor:
Yee, Jennifer C., Zang, Weicheng, Udalski, Andrzej, Ryu, Yoon-Hyun, Green, Jonathan, Hennerley, Steve, Marmont, Andrew, Sumi, Takahiro, Mao, Shude, Gromadzki, Mariusz, Mróz, Przemek, Skowron, Jan, Poleski, Radoslaw, Szymański, Michał K., Soszyński, Igor, Pietrukowicz, Paweł, Kozłowski, Szymon, Ulaczyk, Krzysztof, Rybicki, Krzysztof A., Iwanek, Patryk, Wrona, Marcin, Albrow, Michael D., Chung, Sun-Ju, Gould, Andrew, Han, Cheongho, Hwang, Kyu-Ha, Jung, Youn Kil, Kim, Hyoun-Woo, Shin, In-Gu, Shvartzvald, Yossi, Cha, Sang-Mok, Kim, Dong-Jin, Kim, Seung-Lee, Lee, Chung-Uk, Lee, Dong-Joo, Lee, Yongseok, Park, Byeong-Gon, Pogge, Richard W., Bachelet, Etienne, Christie, Grant, Hundertmark, Markus P. G., Maoz, Dan, McCormick, Jennie, Natusch, Tim, Penny, Matthew T., Street, Rachel A., Tsapras, Yiannis, Beichman, Charles A., Bryden, Geoffery, Novati, Sebastiano Calchi, Carey, Sean, Gaudi, B. Scott, Henderson, Calen B., Johnson, Samson, Zhu, Wei, Bond, Ian A., Abe, Fumio, Barry, Richard, Bennett, David P., Bhattacharya, Aparna, Donachie, Martin, Fujii, Hirosane, Fukui, Akihiko, Hirao, Yuki, Silva, Stela Ishitani, 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, Suzuki, Daisuke, Tanaka, Yuzuru, Tristram, Paul J., Yamawaki, Tsubasa, Yonehara, Atsunori
We report the analysis of OGLE-2019-BLG-0960, which contains the smallest mass-ratio microlensing planet found to date (q = 1.2--1.6 x 10^{-5} at 1-sigma). Although there is substantial uncertainty in the satellite parallax measured by Spitzer, the m
Externí odkaz:
http://arxiv.org/abs/2101.04696
Autor:
Zang, Weicheng, Shvartzvald, Yossi, Udalski, Andrzej, Yee, Jennifer C., Lee, Chung-Uk, Sumi, Takahiro, Zhang, Xiangyu, Yang, Hongjing, Mao, Shude, Novati, Sebastiano Calchi, Gould, Andrew, Zhu, Wei, Beichman, Charles A., Bryden, Geoffery, Carey, Sean, Gaudi, B. Scott, Henderson, Calen B., Mróz, Przemek, Skowron, Jan, Poleski, Radoslaw, Szymański, Michał K., Soszyński, Igor, Pietrukowicz, Paweł, Kozłowski, Szymon, Ulaczyk, Krzysztof, Rybicki, Krzysztof A., Iwanek, Patryk, Wrona, Marcin, Albrow, Michael D., Chung, Sun-Ju, Han, Cheongho, Hwang, Kyu-Ha, Jung, Youn Kil, Ryu, Yoon-Hyun, Shin, In-Gu, Cha, Sang-Mok, Kim, Dong-Jin, Kim, Hyoun-Woo, Kim, Seung-Lee, Lee, Dong-Joo, Lee, Yongseok, Park, Byeong-Gon, Pogge, Richard W., 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, Ranc, Clément, Rattenbury, Nicholas J., Satoh, Yuki, Shoji, Hikaru, Suzuki, Daisuke, Tanaka, Yuzuru, Tristram, Paul J., Yamawaki, Tsubasa, Yonehara, Atsunori, Bachelet, Etienne, Hundertmark, Markus P. G., Jaimes, R. Figuera, Maoz, Dan, Penny, Matthew T., Street, Rachel A., Tsapras, Yiannis
We report the discovery and analysis of a planet in the microlensing event OGLE-2018-BLG-0799. The planetary signal was observed by several ground-based telescopes, and the planet-host mass ratio is $q = (2.65 \pm 0.16) \times 10^{-3}$. The ground-ba
Externí odkaz:
http://arxiv.org/abs/2010.08732