Combining Spitzer parallax and Keck II adaptive optics imaging to measure the mass of a solar-like s...
Combining Spitzer parallax and Keck II adaptive optics imaging to measure the mass of a solar-like star orbited by a cold gaseous planet discovered by microlensing
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J -P Beaulieu , Batista, V , Bennett, D P , J -B Marquette , Blackman, J W , Cole, A A , Coutures, C , Danielski, C , D Dominis-Prester , Donatowicz, J , Fukui, A , Koshimoto, N , Loncaric, C , Morales, J C , Sumi, T , Suzuki, D , Henderson, C , Shvartzvald, Y and Beichman, C
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Ithaca: Cornell University Library, arXiv.org
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English
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Ithaca: Cornell University Library, arXiv.org
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To obtain accurate mass measurements for cold planets discovered by microlensing, it is usually necessary to combine light curve modeling with at least two lens mass-distance relations. Often, a constraint on the Einstein ring radius measurement is obtained from the caustic crossing time: This is supplemented by secondary constraints such as precis...
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Full title
Combining Spitzer parallax and Keck II adaptive optics imaging to measure the mass of a solar-like star orbited by a cold gaseous planet discovered by microlensing
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TN_cdi_proquest_journals_2071313633
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https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2071313633
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E-ISSN
2331-8422
DOI
10.48550/arxiv.1709.00806
