Search Results - "Burdullis, Todd"

All planetesimals born near the Kuiper belt formed as binaries by Fraser, Wesley C., Bannister, Michele T., Pike, Rosemary E., Marsset, Michael, Schwamb, Megan E., Kavelaars, J. J., Lacerda, Pedro, Nesvorný, David, Volk, Kathryn, Delsanti, Audrey, Benecchi, Susan, Lehner, Matthew J., Noll, Keith, Gladman, Brett, Petit, Jean-Marc, Gwyn, Stephen, Chen, Ying-Tung, Wang, Shiang-Yu, Alexandersen, Mike, Burdullis, Todd, Sheppard, Scott, Trujillo, Chad

“…The cold classical Kuiper belt objects have low inclinations and eccentricities 1 , 2 and are the only Kuiper belt population suspected to have formed in situ…”
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Correction: Corrigendum: All planetesimals born near the Kuiper belt formed as binaries by Fraser, Wesley C., Bannister, Michele T., Pike, Rosemary E., Marsset, Michael, Schwamb, Megan E., Kavelaars, J. J., Lacerda, Pedro, Nesvorný, David, Volk, Kathryn, Delsanti, Audrey, Benecchi, Susan, Lehner, Matthew J., Noll, Keith, Gladman, Brett, Petit, Jean-Marc, Gwyn, Stephen, Chen, Ying-Tung, Wang, Shiang-Yu, Alexandersen, Mike, Burdullis, Todd, Sheppard, Scott, Trujillo, Chad

“…Nature Astronomy 1, 0088 (2017); published 4 April 2017; corrected 24 April 2017. In the version of the Supplementary Information originally published the 2001…”
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MOA-2020-BLG-135Lb: A New Neptune-class Planet for the Extended MOA-II Exoplanet Microlens Statistical Analysis by Ishitani Silva, Stela, Ranc, Clément, Bennett, David P., Bond, Ian A., Zang, Weicheng, Abe, Fumio, Barry, Richard K., Bhattacharya, Aparna, Fujii, Hirosane, Fukui, Akihiko, Hirao, Yuki, Itow, Yoshitaka, Kirikawa, Rintaro, Kondo, Iona, Koshimoto, Naoki, Matsubara, Yutaka, Matsumoto, Sho, Miyazaki, Shota, Muraki, Yasushi, Olmschenk, Greg, Okamura, Arisa, Rattenbury, Nicholas J., Satoh, Yuki, Sumi, Takahiro, Suzuki, Daisuke, Toda, Taiga, Tristram, Paul. J., Vandorou, Aikaterini, Yama, Hibiki, Petric, Andreea, Burdullis, Todd, Fouqué, Pascal, Mao, Shude, Penny, Matthew T., Zhu, Wei, Rau, Gioia

“…We report the light-curve analysis for the event MOA-2020-BLG-135, which leads to the discovery of a new Neptune-class planet, MOA-2020-BLG-135Lb. With a…”
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MOA-2020-BLG-135Lb: A New Neptune-class Planet for the Extended MOA-II Exoplanet Microlens Statistical Analysis by Silva, Stela Ishitani, Ranc, Clément, Bennett, David P, Bond, Ian A, Zang, Weicheng, Abe, Fumio, Barry, Richard K, Bhattacharya, Aparna, Fujii, Hirosane, Fukui, Akihiko, Hirao, Yuki, Itow, Yoshitaka, Kirikawa, Rintaro, Kondo, Iona, Koshimoto, Naoki, Matsubara, Yutaka, Matsumoto, Sho, Miyazaki, Shota, Muraki, Yasushi, Olmschenk, Greg, Okamura, Arisa, Rattenbury, Nicholas J, Satoh, Yuki, Sumi, Takahiro, Suzuki, Daisuke, Toda, Taiga, Tristram, Paul . J, Vandorou, Aikaterini, Yama, Hibiki, Petric, Andreea, Burdullis, Todd, Fouqué, Pascal, Mao, Shude, Penny, Matthew T, Zhu, Wei, Rau, Gioia

“…We report the light-curve analysis for the event MOA-2020-BLG-135, which leads to the discovery of a new Neptune-class planet, MOA-2020-BLG-135Lb. With a…”
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The Effects of Superoutbursts onTOADs by Szkody, Paula, Desai, Vandana, Burdullis, Todd, Hoard, D. W., Fried, Robert, Garnavich, Peter, Gansicke, Boris

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The Effects of Superoutbursts on TOADs by Szkody, Paula, Desai, Vandana, Burdullis, Todd, Hoard, D. W, Fried, Robert, Garnavich, Peter, Gänsicke, Boris

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KMT-2018-BLG-0029Lb: A Very Low Mass-Ratio Spitzer Microlens Planet by Gould, Andrew, Ryu, Yoon-Hyun, Novati, Sebastiano Calchi, Zang, Weicheng, Albrow, Michael D, Chung, Sun-Ju, Han, Cheongho, Hwang, Kyu-Ha, Jung, Youn Kil, 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, Beichman, Charles, Bryden, Geoff, Carey, Sean, Gaudi, B. Scott, Henderson, Calen B, Zhu, Wei, Fouqué, Pascal, Penny, Matthew T, Petric, Andreea, Burdullis, Todd, Mao, Shude

“…At $q=1.81\pm 0.20 \times 10^{-5}$, KMT-2018-BLG-0029Lb has the lowest planet-host mass ratio $q$ of any microlensing planet to date by more than a factor of…”
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All planetesimals born near the Kuiper Belt formed as binaries by Fraser, Wesley C, Bannister, Michele t, Pike, Rosemary E, Marsset, Michael, Schwamb, Megan E, Kavelaars, J. J, Lacerda, Pedro, Nesvornyy, David, Volk, Kathryn, Delsanti, audrey, Benecchi, Susan, Lehner, Matthew J, Noll, Keith, Gladman, Brett, Petit, Jean-Marc, Gwyn, Stephen, Chen, Ying-tung, Wang, Shiang-Yu, Alexandersen, Mike, Burdullis, Todd, Sheppard, Scott, Trujillo, Chad

“…The cold classical Kuiper belt objects have low inclinations and eccentricities and are the only Kuiper belt population suspected to have formed in situ…”
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