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    Interpretation of a short-term anomaly in the gravitational microlensing event MOA-2012-BLG-486

    Access Status
    Fulltext not available
    Authors
    Hwang, K.
    Choi, J.
    Bond, I.
    Sumi, T.
    Han, C.
    Gaudi, B.
    Gould, A.
    Bozza, V.
    Beaulieu, J.
    Tsapras, Y.
    Abe, F.
    Bennett, D.
    Botzler, C.
    Chote, P.
    Freeman, M.
    Fukui, A.
    Fukunaga, D.
    Harris, P.
    Itow, Y.
    Koshimoto, N.
    Ling, C.
    Masuda, K.
    Matsubara, M.
    Muraki, Y.
    Namba, S.
    Ohnishi, K.
    Rattenbury, N.
    Saito, T.
    Sullivan, D.
    Sweatman, W.
    Suzuki, D.
    Tristram, P.
    Wada, K.
    Yamai, N.
    Yock, P.
    Yonehara, A.
    Andrade de Almeida, L.
    DePoy, D.
    Dong, S.
    Jablonski, F.
    Jung, Y.
    Kavka, A.
    Lee, C.
    Park, H.
    Pogge, R.
    Shin, I.
    Yee, J.
    Albrow, M.
    Bachelet, E.
    Batista, V.
    Brillant, S.
    Caldwell, J.
    Cassan, A.
    Cole, A.
    Corrales, E.
    Coutures, C.
    Dieters, S.
    Dominis Prester, D.
    Donatowicz, J.
    Fouque, P.
    Greenhill, J.
    Jorgensen, U.
    Kane, S.
    Kubas, D.
    Marquette, J.
    Martin, R.
    Meintjes, P.
    Menzies, J.
    Pollard, K.
    Williams, Andrew
    Wouters, D.
    Bramich, D.
    Dominik, M.
    Horne, K.
    Browne, P.
    Hundertmark, M.
    Ipatov, S.
    Kains, N.
    Snodgrass, C.
    Steele, I.
    Street, R.
    Date
    2013
    Type
    Journal Article
    
    Metadata
    Show full item record
    Citation
    Hwang, K. and Choi, J. and Bond, I. and Sumi, T. and Han, C. and Gaudi, B. and Gould, A. et al. 2013. Interpretation of a short-term anomaly in the gravitational microlensing event MOA-2012-BLG-486. The Astrophysical Journal. 778.
    Source Title
    The Astrophysical Journal
    Additional URLs
    http://iopscience.iop.org/0004-637X/778/1/55/pdf/0004-637X_778_1_55.pdf
    ISSN
    0004-637X
    URI
    http://hdl.handle.net/20.500.11937/14093
    Collection
    • Curtin Research Publications
    Abstract

    A planetary microlensing signal is generally characterized by a short-term perturbation to the standard single lensing light curve. A subset of binary-source events can produce perturbations that mimic planetary signals, thereby introducing an ambiguity between the planetary and binary-source interpretations. In this paper, we present the analysis of the microlensing event MOA-2012-BLG-486, for which the light curve exhibits a short-lived perturbation. Routine modeling not considering data taken in different passbands yields a best-fit planetary model that is slightly preferred over the best-fit binary-source model. However, when allowed for a change in the color during the perturbation, we find that the binary-source model yields a significantly better fit and thus the degeneracy is clearlyresolved. This event not only signifies the importance of considering various interpretations of short-term anomalies, but also demonstrates the importance of multi-band data for checking the possibility of false-positive planetary signals.

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