MOA-2013-BLG-220Lb: massive planetary companion to galactic-disk host

J.C. Yee; C. Han; A. Gould; J. Skowron; I.A. Bond; A. Udalski; M. Hundertmark; L.A.G. Monard; I. Porritt; P. Nelson; V. Bozza; M.D. Albrow; J.-Y. Choi; G.W. Christie; D.L. Depoy; B.S. Gaudi; K.-H. Hwang; Y.K. Jung; C.-U. Lee; J. McCormick; T. Natusch; H. Ngan; H. Park; R.W. Pogge; I.-G. Shin; T.-G. Tan; F. Abe; D.P. Bennett; C.S. Botzler; M. Freeman; A. Fukui; D. Fukunaga; Y. Itow; N. Koshimoto; P. Larsen; C.H. Ling; K. Masuda; Y. Matsubara; Y. Muraki; S. Namba; K. Ohnishi; L. Philpott; N.J. Rattenbury; T. Saito; D.J. Sullivan; T. Sumi; W.L. Sweatman; D. Suzuki; P.J. Tristram; N. Tsurumi; K. Wada; N. Yamai; P.C.M. Yock; A. Yonehara; M.K. Szymański; K. Ulaczyk; S. Kozłowski; R. Poleski; Ł. Wyrzykowski; M. Kubiak; P. Pietrukowicz; G. Pietrzyński; I. Soszyński; D.M. Bramich; P. Browne; R. Figuera Jaimes; K. Horne; S. Ipatov; N. Kains; C. Snodgrass; I.A. Steele; R. Street; Y. Tsapras

doi:10.1088/0004-637X/790/1/14

MOA-2013-BLG-220Lb: massive planetary companion to galactic-disk host

J.C. Yee, C. Han, A. Gould, J. Skowron, I.A. Bond, A. Udalski, M. Hundertmark, L.A.G. Monard, I. Porritt, P. Nelson, V. Bozza, M.D. Albrow, J.-Y. Choi, G.W. Christie, D.L. Depoy, B.S. Gaudi, K.-H. Hwang, Y.K. Jung, C.-U. Lee, J. McCormickT. Natusch, H. Ngan, H. Park, R.W. Pogge, I.-G. Shin, T.-G. Tan, F. Abe, D.P. Bennett, C.S. Botzler, M. Freeman, A. Fukui, D. Fukunaga, Y. Itow, N. Koshimoto, P. Larsen, C.H. Ling, K. Masuda, Y. Matsubara, Y. Muraki, S. Namba, K. Ohnishi, L. Philpott, N.J. Rattenbury, T. Saito, D.J. Sullivan, T. Sumi, W.L. Sweatman, D. Suzuki, P.J. Tristram, N. Tsurumi, K. Wada, N. Yamai, P.C.M. Yock, A. Yonehara, M.K. Szymański, K. Ulaczyk, S. Kozłowski, R. Poleski, Ł. Wyrzykowski, M. Kubiak, P. Pietrukowicz, G. Pietrzyński, I. Soszyński, D.M. Bramich, P. Browne, R. Figuera Jaimes, K. Horne, S. Ipatov, N. Kains, C. Snodgrass, I.A. Steele, R. Street, Y. Tsapras

School of Physics and Astronomy

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Abstract

We report the discovery of MOA-2013-BLG-220Lb, which has a super-Jupiter mass ratio q = 3.01 ± 0.02 × 10^-3 relative to its host. The proper motion, μ = 12.5 ± 1 mas yr^-1, is one of the highest for microlensing planets yet discovered, implying that it will be possible to separately resolve the host within ∼7 yr. Two separate lines of evidence imply that the planet and host are in the Galactic disk. The planet could have been detected and characterized purely with follow-up data, which has important implications for microlensing surveys, both current and into the Large Synoptic Survey Telescope (LSST) era.

Original language	English
Number of pages	7
Journal	Astrophysical Journal
Volume	790
Issue number	1
DOIs	https://doi.org/10.1088/0004-637X/790/1/14
Publication status	Published - 20 Jul 2014

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10.1088/0004-637X/790/1/14

Yee_2014_TAJ_MOA
© 2014. The American Astronomical Society. All rights reserved.
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Astrophysics at St Andrews:2012 - 2014: Astrophysics at St Andrews: 2012 - 2014
Horne, K. D. (PI)
Science & Technology Facilities Council
1/10/11 → 31/03/12
Project: Standard

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Yee, J. C., Han, C., Gould, A., Skowron, J., Bond, I. A., Udalski, A., Hundertmark, M., Monard, L. A. G., Porritt, I., Nelson, P., Bozza, V., Albrow, M. D., Choi, J.-Y., Christie, G. W., Depoy, D. L., Gaudi, B. S., Hwang, K.-H., Jung, Y. K., Lee, C.-U., ... Tsapras, Y. (2014). MOA-2013-BLG-220Lb: massive planetary companion to galactic-disk host. Astrophysical Journal, 790(1). https://doi.org/10.1088/0004-637X/790/1/14

@article{19a29264d57d4713af71ea2136c0b268,

title = "MOA-2013-BLG-220Lb: massive planetary companion to galactic-disk host",

abstract = "We report the discovery of MOA-2013-BLG-220Lb, which has a super-Jupiter mass ratio q = 3.01 ± 0.02 × 10-3 relative to its host. The proper motion, μ = 12.5 ± 1 mas yr-1, is one of the highest for microlensing planets yet discovered, implying that it will be possible to separately resolve the host within ∼7 yr. Two separate lines of evidence imply that the planet and host are in the Galactic disk. The planet could have been detected and characterized purely with follow-up data, which has important implications for microlensing surveys, both current and into the Large Synoptic Survey Telescope (LSST) era.",

author = "J.C. Yee and C. Han and A. Gould and J. Skowron and I.A. Bond and A. Udalski and M. Hundertmark and L.A.G. Monard and I. Porritt and P. Nelson and V. Bozza and M.D. Albrow and J.-Y. Choi and G.W. Christie and D.L. Depoy and B.S. Gaudi and K.-H. Hwang and Y.K. Jung and C.-U. Lee and J. McCormick and T. Natusch and H. Ngan and H. Park and R.W. Pogge and I.-G. Shin and T.-G. Tan and F. Abe and D.P. Bennett and C.S. Botzler and M. Freeman and A. Fukui and D. Fukunaga and Y. Itow and N. Koshimoto and P. Larsen and C.H. Ling and K. Masuda and Y. Matsubara and Y. Muraki and S. Namba and K. Ohnishi and L. Philpott and N.J. Rattenbury and T. Saito and D.J. Sullivan and T. Sumi and W.L. Sweatman and D. Suzuki and P.J. Tristram and N. Tsurumi and K. Wada and N. Yamai and P.C.M. Yock and A. Yonehara and M.K. Szyma{\'n}ski and K. Ulaczyk and S. Koz{\l}owski and R. Poleski and {\L}. Wyrzykowski and M. Kubiak and P. Pietrukowicz and G. Pietrzy{\'n}ski and I. Soszy{\'n}ski and D.M. Bramich and P. Browne and {Figuera Jaimes}, R. and K. Horne and S. Ipatov and N. Kains and C. Snodgrass and I.A. Steele and R. Street and Y. Tsapras",

note = "Work by J. C. Yee was supported in part by a Distinguished University Fellowship from The Ohio State University and in part under contract with the California Institute of Technology (Caltech) funded by NASA through the Sagan Fellowship Program. Work by CH was supported by the Creative Research Initiative Program (2009-0081561) of the National Research Foundation of Korea. Work by A.G. and B.S.G. was supported by NSF grant AST 1103471. Work by A.G., B.S.G., and R.W.P. was supported by NASA grant NNX12AB99G. T.S. acknowledges the support from the grant JSPS23340044 and JSPS24253004. The OGLE project has received funding from the European Research Council under the European Community's Seventh Framework Programme (FP7/2007-2013)/ERC grant agreement no. 246678 to AU. This publication was made possible by NPRP grant X-019-1-006 from the Qatar National Research Fund (a member of Qatar Foundation).",

year = "2014",

month = jul,

day = "20",

doi = "10.1088/0004-637X/790/1/14",

language = "English",

volume = "790",

journal = "Astrophysical Journal",

issn = "0004-637X",

publisher = "American Astronomical Society",

number = "1",

}

Yee, JC, Han, C, Gould, A, Skowron, J, Bond, IA, Udalski, A, Hundertmark, M, Monard, LAG, Porritt, I, Nelson, P, Bozza, V, Albrow, MD, Choi, J-Y, Christie, GW, Depoy, DL, Gaudi, BS, Hwang, K-H, Jung, YK, Lee, C-U, McCormick, J, Natusch, T, Ngan, H, Park, H, Pogge, RW, Shin, I-G, Tan, T-G, Abe, F, Bennett, DP, Botzler, CS, Freeman, M, Fukui, A, Fukunaga, D, Itow, Y, Koshimoto, N, Larsen, P, Ling, CH, Masuda, K, Matsubara, Y, Muraki, Y, Namba, S, Ohnishi, K, Philpott, L, Rattenbury, NJ, Saito, T, Sullivan, DJ, Sumi, T, Sweatman, WL, Suzuki, D, Tristram, PJ, Tsurumi, N, Wada, K, Yamai, N, Yock, PCM, Yonehara, A, Szymański, MK, Ulaczyk, K, Kozłowski, S, Poleski, R, Wyrzykowski, Ł, Kubiak, M, Pietrukowicz, P, Pietrzyński, G, Soszyński, I, Bramich, DM, Browne, P, Figuera Jaimes, R, Horne, K, Ipatov, S, Kains, N, Snodgrass, C, Steele, IA, Street, R & Tsapras, Y 2014, 'MOA-2013-BLG-220Lb: massive planetary companion to galactic-disk host', Astrophysical Journal, vol. 790, no. 1. https://doi.org/10.1088/0004-637X/790/1/14

TY - JOUR

T1 - MOA-2013-BLG-220Lb

T2 - massive planetary companion to galactic-disk host

AU - Yee, J.C.

AU - Han, C.

AU - Gould, A.

AU - Skowron, J.

AU - Bond, I.A.

AU - Udalski, A.

AU - Hundertmark, M.

AU - Monard, L.A.G.

AU - Porritt, I.

AU - Nelson, P.

AU - Bozza, V.

AU - Albrow, M.D.

AU - Choi, J.-Y.

AU - Christie, G.W.

AU - Depoy, D.L.

AU - Gaudi, B.S.

AU - Hwang, K.-H.

AU - Jung, Y.K.

AU - Lee, C.-U.

AU - McCormick, J.

AU - Natusch, T.

AU - Ngan, H.

AU - Park, H.

AU - Pogge, R.W.

AU - Shin, I.-G.

AU - Tan, T.-G.

AU - Abe, F.

AU - Bennett, D.P.

AU - Botzler, C.S.

AU - Freeman, M.

AU - Fukui, A.

AU - Fukunaga, D.

AU - Itow, Y.

AU - Koshimoto, N.

AU - Larsen, P.

AU - Ling, C.H.

AU - Masuda, K.

AU - Matsubara, Y.

AU - Muraki, Y.

AU - Namba, S.

AU - Ohnishi, K.

AU - Philpott, L.

AU - Rattenbury, N.J.

AU - Saito, T.

AU - Sullivan, D.J.

AU - Sumi, T.

AU - Sweatman, W.L.

AU - Suzuki, D.

AU - Tristram, P.J.

AU - Tsurumi, N.

AU - Wada, K.

AU - Yamai, N.

AU - Yock, P.C.M.

AU - Yonehara, A.

AU - Szymański, M.K.

AU - Ulaczyk, K.

AU - Kozłowski, S.

AU - Poleski, R.

AU - Wyrzykowski, Ł.

AU - Kubiak, M.

AU - Pietrukowicz, P.

AU - Pietrzyński, G.

AU - Soszyński, I.

AU - Bramich, D.M.

AU - Browne, P.

AU - Figuera Jaimes, R.

AU - Horne, K.

AU - Ipatov, S.

AU - Kains, N.

AU - Snodgrass, C.

AU - Steele, I.A.

AU - Street, R.

AU - Tsapras, Y.

N1 - Work by J. C. Yee was supported in part by a Distinguished University Fellowship from The Ohio State University and in part under contract with the California Institute of Technology (Caltech) funded by NASA through the Sagan Fellowship Program. Work by CH was supported by the Creative Research Initiative Program (2009-0081561) of the National Research Foundation of Korea. Work by A.G. and B.S.G. was supported by NSF grant AST 1103471. Work by A.G., B.S.G., and R.W.P. was supported by NASA grant NNX12AB99G. T.S. acknowledges the support from the grant JSPS23340044 and JSPS24253004. The OGLE project has received funding from the European Research Council under the European Community's Seventh Framework Programme (FP7/2007-2013)/ERC grant agreement no. 246678 to AU. This publication was made possible by NPRP grant X-019-1-006 from the Qatar National Research Fund (a member of Qatar Foundation).

PY - 2014/7/20

Y1 - 2014/7/20

N2 - We report the discovery of MOA-2013-BLG-220Lb, which has a super-Jupiter mass ratio q = 3.01 ± 0.02 × 10-3 relative to its host. The proper motion, μ = 12.5 ± 1 mas yr-1, is one of the highest for microlensing planets yet discovered, implying that it will be possible to separately resolve the host within ∼7 yr. Two separate lines of evidence imply that the planet and host are in the Galactic disk. The planet could have been detected and characterized purely with follow-up data, which has important implications for microlensing surveys, both current and into the Large Synoptic Survey Telescope (LSST) era.

AB - We report the discovery of MOA-2013-BLG-220Lb, which has a super-Jupiter mass ratio q = 3.01 ± 0.02 × 10-3 relative to its host. The proper motion, μ = 12.5 ± 1 mas yr-1, is one of the highest for microlensing planets yet discovered, implying that it will be possible to separately resolve the host within ∼7 yr. Two separate lines of evidence imply that the planet and host are in the Galactic disk. The planet could have been detected and characterized purely with follow-up data, which has important implications for microlensing surveys, both current and into the Large Synoptic Survey Telescope (LSST) era.

U2 - 10.1088/0004-637X/790/1/14

DO - 10.1088/0004-637X/790/1/14

M3 - Article

AN - SCOPUS:84904174369

SN - 0004-637X

VL - 790

JO - Astrophysical Journal

JF - Astrophysical Journal

IS - 1

ER -

MOA-2013-BLG-220Lb: massive planetary companion to galactic-disk host

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