A Neptune-mass Free-floating Planet Candidate Discovered by Microlensing Surveys
Przemek Mróz,Yoon-Hyun Ryu,Jan Skowron,Andrzej Udalski,Andrew Gould,Michał K. Szymański,Igor Soszyński,Radosław Poleski,Paweł Pietrukowicz,Szymon Kozłowski,Michał Pawlak,K. Ulaczyk,Michael D. Albrow,S. J. Chung,Youn Kil Jung,C. Han,K. H. Hwang,In-Gu Shin,Jennifer C. Yee,Wei Zhu,Sang-Mok Cha,Dong-Jin Kim,Hyoun-Woo Kim,Seung-Lee Kim,Chung-Uk Lee,D. J. Lee,Yongseok Lee,B. G. Park,Richard W. Pogge +28 more
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TLDR
In this paper, the authors presented the discovery of a Neptune-mass free-floating planet candidate in the ultrashort OGLE-2016-BLG-1540 microlensing event.Abstract:
Current microlensing surveys are sensitive to free-floating planets down to Earth-mass objects. All published microlensing events attributed to unbound planets were identified based on their short timescale (below two days), but lacked an angular Einstein radius measurement (and hence lacked a significant constraint on the lens mass). Here, we present the discovery of a Neptune-mass free-floating planet candidate in the ultrashort ($t_{\\rm E}=0.320\\pm0.003$ days) microlensing event OGLE-2016-BLG-1540. The event exhibited strong finite-source effects, which allowed us to measure its angular Einstein radius of $\\theta_{\\rm E}=9.2\\pm0.5\\,\\mu$as. There remains, however, a degeneracy between the lens mass and distance. The combination of the source proper motion and source-lens relative proper motion measurements favors a Neptune-mass lens located in the Galactic disk. However, we cannot rule out that the lens is a Saturn-mass object belonging to the bulge population. We exclude stellar companions up to 15 au.read more
Citations
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Detecting Earth-Mass Planets with Gravitational Microlensing
TL;DR: In this paper, it was shown that Earth mass planets orbiting stars in the Galactic disk and bulge can be detected by monitoring microlensed stars in a Galactic bulge, and that the planetary signal remains detectable for planetary masses as small as an Earth mass when realistic source star sizes are included in the lightcurve calculation.
Journal ArticleDOI
The Optical Gravitational Lensing Experiment. OGLE #7: Binary Microlens or a New Unusual Variable?
Andrzej Udalski,Michał K. Szymański,Shude Mao,R. Di Stefano,Janusz Kaluzny,M. Kubiak,Mario Mateo,Wojtek Krzeminski +7 more
TL;DR: In this article, the authors presented the light curve of OGLE #7, an unusual variable object, detected during the OGLE search for microlensing events, and showed that the star brightened by more than 2~mag with a characteristic double-maximum shape and returned to normal brightness after 60 days.
Journal ArticleDOI
Predictions of the Nancy Grace Roman Space Telescope Galactic Exoplanet Survey II: Free-Floating Planet Detection Rates
Samson A. Johnson,Matthew T. Penny,B. Scott Gaudi,Eamonn Kerins,Nicholas J. Rattenbury,Annie C. Robin,Sebastiano Calchi Novati,Calen B. Henderson +7 more
TL;DR: The Nancy Grace Roman Space Telescope (Roman) will perform a Galactic Exoplanet Survey (RGES) to discover bound exoplanets with semi-major axes greater than 1 au using gravitational microlensing as discussed by the authors.
Journal ArticleDOI
Two new free-floating or wide-orbit planets from microlensing
Przemek Mróz,Andrzej Udalski,David P. Bennett,Yoon-Hyun Ryu,Takahiro Sumi,Yossi Shvartzvald,Jan Skowron,Radosław Poleski,Paweł Pietrukowicz,Szymon Kozłowski,Michał K. Szymański,Łukasz Wyrzykowski,Igor Soszyński,Krzysztof Ulaczyk,K. A. Rybicki,Patryk Iwanek,Michael D. Albrow,Sun-Ju Chung,Andrew Gould,C. Han,K. H. Hwang,Youn Kil Jung,In-Gu Shin,Jennifer C. Yee,W. Zang,Sang-Mok Cha,Dong-Jin Kim,Hyoun-Woo Kim,Seung-Lee Kim,Chung-Uk Lee,D. J. Lee,Yongseok Lee,B. G. Park,Richard W. Pogge,Fumio Abe,Richard Barry,Aparna Bhattacharya,Ian A. Bond,Martin Donachie,Akihiko Fukui,Yuki Hirao,Yoshitaka Itow,K. Kawasaki,Iona Kondo,Naoki Koshimoto,Man Cheung Alex Li,Yutaka Matsubara,Yasushi Muraki,S. Miyazaki,Masayuki Nagakane,Clément Ranc,Nicholas J. Rattenbury,Haruno Suematsu,Denis J. Sullivan,Daisuke Suzuki,Paul J. Tristram,Atsunori Yonehara,D. Maoz,Shai Kaspi,M. Friedmann +59 more
TL;DR: In this article, the authors presented the discovery and characterization of two ultra-short microlensing events identified in data from the Optical Gravitational Lensing Experiment (OGLE) survey, which may have been caused by free-floating or wide-orbit planets.
Journal ArticleDOI
Two new free-floating or wide-orbit planets from microlensing
Przemek Mróz,Andrzej Udalski,David P. Bennett,Yoon-Hyun Ryu,Takahiro Sumi,Yossi Shvartzvald,Jan Skowron,Radosław Poleski,P. Pietrukowicz,S. Kozlowski,Michał K. Szymański,L. Wyrzykowski,Igor Soszyński,K. Ulaczyk,K. A. Rybicki,Patryk Iwanek,Michael D. Albrow,Sun-Ju Chung,Andrew Gould,C. Han,K.-H. Hwang,Y. K. Jung,In-Gu Shin,Jennifer C. Yee,W. Zang,Sang-Mok Cha,D.-J. Kim,H.-W. Kim,S. L. Kim,C.-U. Lee,Duk-Hang Lee,Y. Lee,Byeong-Gon Park,Richard W. Pogge,Fumio Abe,Richard Barry,Aparna Bhattacharya,Ian A. Bond,Martin Donachie,Akihiko Fukui,Yuki Hirao,Yoshitaka Itow,K. Kawasaki,Iona Kondo,Naoki Koshimoto,M. C. A. Li,Yutaka Matsubara,Yasushi Muraki,Satoshi Miyazaki,Masayuki Nagakane,Clément Ranc,Nicholas J. Rattenbury,Haruno Suematsu,Denis J. Sullivan,Daisuke Suzuki,Paul J. Tristram,Atsunori Yonehara,D. Maoz,Shai Kaspi,M. Friedmann +59 more
TL;DR: In this article, the authors presented the discovery and characterization of two ultra-short microlensing events identified in data from the Optical Gravitational Lensing Experiment (OGLE) survey, which may have been caused by free-floating or wide-orbit planets.
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