Systematic KMTNet Planetary Anomaly Search, Paper III: One Wide-Orbit Planet And Two Stellar Binaries
Only a few wide-orbit planets around old stars have been detected, which limits our statistical understanding of this planet population. Following the systematic search for planetary anomalies in microlensing events found by the Korea Microlensing Telescope Network (KMTNet), we present the discovery...
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creator | Wang, Hanyue Zang, Weicheng Zhu, Wei Kyu-Ha Hwang Udalski, Andrzej Gould, Andrew Han, Cheongho Albrow, Michael D Sun-Ju, Chung Jung, Youn Kil Kim, Doeon Yoon-Hyun, Ryu Shin, In-Gu Shvartzvald, Yossi Yee, Jennifer C Sang-Mok Cha Dong-Jin, Kim Hyoun-Woo, Kim Seung-Lee, Kim Chung-Uk, Lee Dong-Joo, Lee Lee, Yongseok Park, Byeong-Gon Pogge, Richard W Poleski, Radoslaw Mróz, Przemek Skowron, Jan Szymański, Michał K Soszyński, Igor Pietrukowicz, Paweł Kozłowski, Szymon Ulaczyk, Krzysztof Rybicki, Krzysztof A Iwanek, Patryk Wrona, Marcin Gromadzki, Mariusz Yang, Hongjing Mao, Shude Zhang, Xiangyu |
description | Only a few wide-orbit planets around old stars have been detected, which limits our statistical understanding of this planet population. Following the systematic search for planetary anomalies in microlensing events found by the Korea Microlensing Telescope Network (KMTNet), we present the discovery and analysis of three events that were initially thought to contain wide-orbit planets. The anomalous feature in the light curve of OGLE-2018-BLG-0383 is caused by a planet with mass ratio \(q=2.1\times 10^{-4}\) and a projected separation \(s=2.45\). This makes it the lowest mass-ratio microlensing planet at such wide orbits. The other two events, KMT-2018-BLG-0998 and OGLE-2018-BLG-0271, are shown to be stellar binaries (\(q>0.1\)) with rather close (\(s |
doi_str_mv | 10.48550/arxiv.2112.02414 |
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Following the systematic search for planetary anomalies in microlensing events found by the Korea Microlensing Telescope Network (KMTNet), we present the discovery and analysis of three events that were initially thought to contain wide-orbit planets. The anomalous feature in the light curve of OGLE-2018-BLG-0383 is caused by a planet with mass ratio \(q=2.1\times 10^{-4}\) and a projected separation \(s=2.45\). This makes it the lowest mass-ratio microlensing planet at such wide orbits. The other two events, KMT-2018-BLG-0998 and OGLE-2018-BLG-0271, are shown to be stellar binaries (\(q>0.1\)) with rather close (\(s<1\)) separations. We briefly discuss the properties of known wide-orbit microlensing planets and show that the survey observations are crucial in discovering and further statistically constraining such a planet population.</description><identifier>EISSN: 2331-8422</identifier><identifier>DOI: 10.48550/arxiv.2112.02414</identifier><language>eng</language><publisher>Ithaca: Cornell University Library, arXiv.org</publisher><subject>Anomalies ; Binary stars ; Light curve ; Microlenses ; Physics - Astrophysics of Galaxies ; Physics - Earth and Planetary Astrophysics ; Planetary orbits ; Planets ; Population (statistical)</subject><ispartof>arXiv.org, 2021-12</ispartof><rights>2021. This work is published under http://creativecommons.org/publicdomain/zero/1.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License.</rights><rights>http://creativecommons.org/publicdomain/zero/1.0</rights><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>228,230,776,780,881,27904</link.rule.ids><backlink>$$Uhttps://doi.org/10.1093/mnras/stab3581$$DView published paper (Access to full text may be restricted)$$Hfree_for_read</backlink><backlink>$$Uhttps://doi.org/10.48550/arXiv.2112.02414$$DView paper in arXiv$$Hfree_for_read</backlink></links><search><creatorcontrib>Wang, Hanyue</creatorcontrib><creatorcontrib>Zang, Weicheng</creatorcontrib><creatorcontrib>Zhu, Wei</creatorcontrib><creatorcontrib>Kyu-Ha Hwang</creatorcontrib><creatorcontrib>Udalski, Andrzej</creatorcontrib><creatorcontrib>Gould, Andrew</creatorcontrib><creatorcontrib>Han, Cheongho</creatorcontrib><creatorcontrib>Albrow, Michael D</creatorcontrib><creatorcontrib>Sun-Ju, Chung</creatorcontrib><creatorcontrib>Jung, Youn Kil</creatorcontrib><creatorcontrib>Kim, Doeon</creatorcontrib><creatorcontrib>Yoon-Hyun, Ryu</creatorcontrib><creatorcontrib>Shin, In-Gu</creatorcontrib><creatorcontrib>Shvartzvald, Yossi</creatorcontrib><creatorcontrib>Yee, Jennifer C</creatorcontrib><creatorcontrib>Sang-Mok Cha</creatorcontrib><creatorcontrib>Dong-Jin, Kim</creatorcontrib><creatorcontrib>Hyoun-Woo, Kim</creatorcontrib><creatorcontrib>Seung-Lee, Kim</creatorcontrib><creatorcontrib>Chung-Uk, Lee</creatorcontrib><creatorcontrib>Dong-Joo, Lee</creatorcontrib><creatorcontrib>Lee, Yongseok</creatorcontrib><creatorcontrib>Park, Byeong-Gon</creatorcontrib><creatorcontrib>Pogge, Richard W</creatorcontrib><creatorcontrib>Poleski, Radoslaw</creatorcontrib><creatorcontrib>Mróz, Przemek</creatorcontrib><creatorcontrib>Skowron, Jan</creatorcontrib><creatorcontrib>Szymański, Michał K</creatorcontrib><creatorcontrib>Soszyński, Igor</creatorcontrib><creatorcontrib>Pietrukowicz, Paweł</creatorcontrib><creatorcontrib>Kozłowski, Szymon</creatorcontrib><creatorcontrib>Ulaczyk, Krzysztof</creatorcontrib><creatorcontrib>Rybicki, Krzysztof A</creatorcontrib><creatorcontrib>Iwanek, Patryk</creatorcontrib><creatorcontrib>Wrona, Marcin</creatorcontrib><creatorcontrib>Gromadzki, Mariusz</creatorcontrib><creatorcontrib>Yang, Hongjing</creatorcontrib><creatorcontrib>Mao, Shude</creatorcontrib><creatorcontrib>Zhang, Xiangyu</creatorcontrib><title>Systematic KMTNet Planetary Anomaly Search, Paper III: One Wide-Orbit Planet And Two Stellar Binaries</title><title>arXiv.org</title><description>Only a few wide-orbit planets around old stars have been detected, which limits our statistical understanding of this planet population. Following the systematic search for planetary anomalies in microlensing events found by the Korea Microlensing Telescope Network (KMTNet), we present the discovery and analysis of three events that were initially thought to contain wide-orbit planets. The anomalous feature in the light curve of OGLE-2018-BLG-0383 is caused by a planet with mass ratio \(q=2.1\times 10^{-4}\) and a projected separation \(s=2.45\). This makes it the lowest mass-ratio microlensing planet at such wide orbits. The other two events, KMT-2018-BLG-0998 and OGLE-2018-BLG-0271, are shown to be stellar binaries (\(q>0.1\)) with rather close (\(s<1\)) separations. We briefly discuss the properties of known wide-orbit microlensing planets and show that the survey observations are crucial in discovering and further statistically constraining such a planet population.</description><subject>Anomalies</subject><subject>Binary stars</subject><subject>Light curve</subject><subject>Microlenses</subject><subject>Physics - Astrophysics of Galaxies</subject><subject>Physics - Earth and Planetary Astrophysics</subject><subject>Planetary orbits</subject><subject>Planets</subject><subject>Population (statistical)</subject><issn>2331-8422</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2021</creationdate><recordtype>article</recordtype><sourceid>ABUWG</sourceid><sourceid>AFKRA</sourceid><sourceid>AZQEC</sourceid><sourceid>BENPR</sourceid><sourceid>CCPQU</sourceid><sourceid>DWQXO</sourceid><sourceid>GOX</sourceid><recordid>eNo1kMtOwzAURC0kJKrSD2CFJbak2I7tOOxKxSOi0EqpxDK6tW-EqzQpTgr07wktrGYzM5o5hFxwNpZGKXYD4dt_jgXnYsyE5PKEDEQc88hIIc7IqG3XjDGhE6FUPCCY79sON9B5S59flq_Y0UUFNXYQ9nRSNxuo9jRHCPb9mi5gi4FmWXZL5zXSN-8wmoeV_8_0AUeXXw3NO6wqCPTO1xA8tufktISqxdGfDkn-cL-cPkWz-WM2ncwiUEJGaSKkARBOq7Q0JokTJRmzkHKnEy3dyiKI0mpeljq1K3TGMq4QDXNapjoekstj6wFBsQ1-078oflEUBxS94-ro2IbmY4dtV6ybXaj7SYXQLJHaSC3jHzmZYBI</recordid><startdate>20211204</startdate><enddate>20211204</enddate><creator>Wang, Hanyue</creator><creator>Zang, Weicheng</creator><creator>Zhu, Wei</creator><creator>Kyu-Ha Hwang</creator><creator>Udalski, Andrzej</creator><creator>Gould, Andrew</creator><creator>Han, Cheongho</creator><creator>Albrow, Michael D</creator><creator>Sun-Ju, Chung</creator><creator>Jung, Youn Kil</creator><creator>Kim, Doeon</creator><creator>Yoon-Hyun, Ryu</creator><creator>Shin, In-Gu</creator><creator>Shvartzvald, Yossi</creator><creator>Yee, Jennifer C</creator><creator>Sang-Mok Cha</creator><creator>Dong-Jin, Kim</creator><creator>Hyoun-Woo, Kim</creator><creator>Seung-Lee, Kim</creator><creator>Chung-Uk, Lee</creator><creator>Dong-Joo, Lee</creator><creator>Lee, Yongseok</creator><creator>Park, Byeong-Gon</creator><creator>Pogge, Richard W</creator><creator>Poleski, Radoslaw</creator><creator>Mróz, Przemek</creator><creator>Skowron, Jan</creator><creator>Szymański, Michał K</creator><creator>Soszyński, Igor</creator><creator>Pietrukowicz, Paweł</creator><creator>Kozłowski, Szymon</creator><creator>Ulaczyk, Krzysztof</creator><creator>Rybicki, Krzysztof A</creator><creator>Iwanek, Patryk</creator><creator>Wrona, Marcin</creator><creator>Gromadzki, Mariusz</creator><creator>Yang, Hongjing</creator><creator>Mao, Shude</creator><creator>Zhang, Xiangyu</creator><general>Cornell University Library, arXiv.org</general><scope>8FE</scope><scope>8FG</scope><scope>ABJCF</scope><scope>ABUWG</scope><scope>AFKRA</scope><scope>AZQEC</scope><scope>BENPR</scope><scope>BGLVJ</scope><scope>CCPQU</scope><scope>DWQXO</scope><scope>HCIFZ</scope><scope>L6V</scope><scope>M7S</scope><scope>PIMPY</scope><scope>PQEST</scope><scope>PQQKQ</scope><scope>PQUKI</scope><scope>PRINS</scope><scope>PTHSS</scope><scope>GOX</scope></search><sort><creationdate>20211204</creationdate><title>Systematic KMTNet Planetary Anomaly Search, Paper III: One Wide-Orbit Planet And Two Stellar Binaries</title><author>Wang, Hanyue ; Zang, Weicheng ; Zhu, Wei ; Kyu-Ha Hwang ; Udalski, Andrzej ; Gould, Andrew ; Han, Cheongho ; Albrow, Michael D ; Sun-Ju, Chung ; Jung, Youn Kil ; Kim, Doeon ; Yoon-Hyun, Ryu ; Shin, In-Gu ; Shvartzvald, Yossi ; Yee, Jennifer C ; Sang-Mok Cha ; Dong-Jin, Kim ; Hyoun-Woo, Kim ; Seung-Lee, Kim ; Chung-Uk, Lee ; Dong-Joo, Lee ; Lee, Yongseok ; Park, Byeong-Gon ; Pogge, Richard W ; Poleski, Radoslaw ; Mróz, Przemek ; Skowron, Jan ; Szymański, Michał K ; Soszyński, Igor ; Pietrukowicz, Paweł ; Kozłowski, Szymon ; Ulaczyk, Krzysztof ; Rybicki, Krzysztof A ; Iwanek, Patryk ; Wrona, Marcin ; Gromadzki, Mariusz ; Yang, Hongjing ; Mao, Shude ; Zhang, Xiangyu</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-a524-97248aa2d659f887375400ca91d6764dbcea2fc61ff69cbed8c015ee80d64963</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2021</creationdate><topic>Anomalies</topic><topic>Binary stars</topic><topic>Light curve</topic><topic>Microlenses</topic><topic>Physics - 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Following the systematic search for planetary anomalies in microlensing events found by the Korea Microlensing Telescope Network (KMTNet), we present the discovery and analysis of three events that were initially thought to contain wide-orbit planets. The anomalous feature in the light curve of OGLE-2018-BLG-0383 is caused by a planet with mass ratio \(q=2.1\times 10^{-4}\) and a projected separation \(s=2.45\). This makes it the lowest mass-ratio microlensing planet at such wide orbits. The other two events, KMT-2018-BLG-0998 and OGLE-2018-BLG-0271, are shown to be stellar binaries (\(q>0.1\)) with rather close (\(s<1\)) separations. We briefly discuss the properties of known wide-orbit microlensing planets and show that the survey observations are crucial in discovering and further statistically constraining such a planet population.</abstract><cop>Ithaca</cop><pub>Cornell University Library, arXiv.org</pub><doi>10.48550/arxiv.2112.02414</doi><oa>free_for_read</oa></addata></record> |
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subjects | Anomalies Binary stars Light curve Microlenses Physics - Astrophysics of Galaxies Physics - Earth and Planetary Astrophysics Planetary orbits Planets Population (statistical) |
title | Systematic KMTNet Planetary Anomaly Search, Paper III: One Wide-Orbit Planet And Two Stellar Binaries |
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