A super-Jupiter orbiting a late-type star: a refined analysis of microlensing event OGLE-2012-BLG-0406

Y. Tsapras; J.-Y. Choi; R.A. Street; C. Han; V. Bozza; A. Gould; M. Dominik; J.-P. Beaulieu; A. Udalski; U.G. Jørgensen; T. Sumi; D.M. Bramich; P. Browne; K. Horne; M. Hundertmark; S. Ipatov; N. Kains; C. Snodgrass; I.A. Steele; K.A. Alsubai; J.M. Andersen; S.C. Novati; Y. Damerdji; C. Diehl; A. Elyiv; E. Giannini; S. Hardis; K. Harpsøe; T.C. Hinse; D. Juncher; E. Kerins; H. Korhonen; C. Liebig; L. Mancini; M. Mathiasen; M.T. Penny; M. Rabus; S. Rahvar; G. Scarpetta; J. Skottfelt; J. Southworth; J. Surdej; J. Tregloan-Reed; C. Vilela; J. Wambsganss; J. Skowron; R. Poleski; S. Kozłowski; Ł. Wyrzykowski; M.K. Szymański; M. Kubiak; P. Pietrukowicz; G. Pietrzyński; I. Soszyński; K. Ulaczyk; M.D. Albrow; E. Bachelet; R. Barry; V. Batista; A. Bhattacharya; S. Brillant; J.A.R. Caldwell; A. Cassan; A. Cole; E. Corrales; C. Coutures; S. Dieters; D. Dominis Prester; J. Donatowicz; P. Fouqué; J. Greenhill; S.R. Kane; D. Kubas; J.-B. Marquette; J. Menzies; C. Père; K.R. Pollard; M. Zub; G. Christie; D.L. Depoy; S. Dong; J. Drummond; B.S. Gaudi; C.B. Henderson; K.H. Hwang; Y.K. Jung; A. Kavka; J.-R. Koo; C.-U. Lee; D. Maoz; L.A.G. Monard; T. Natusch; H. Ngan; H. Park; R.W. Pogge; I. Porritt; I.-G. Shin; Y. Shvartzvald; T.G. Tan; J.C. Yee; F. Abe; D.P. Bennett; I.A. Bond; C.S. Botzler; M. Freeman; A. Fukui; D. Fukunaga; Y. Itow; N. Koshimoto; C.H. Ling; K. Masuda; Y. Matsubara; Y. Muraki; S. Namba; K. Ohnishi; N.J. Rattenbury; T. Saito; D.J. Sullivan; W.L. Sweatman; D. Suzuki; P.J. Tristram; N. Tsurumi; K. Wada; N. Yamai; P.C.M. Yock; A. Yonehara

doi:10.1088/0004-637X/782/1/48

A super-Jupiter orbiting a late-type star: a refined analysis of microlensing event OGLE-2012-BLG-0406

Y. Tsapras, J.-Y. Choi, R.A. Street, C. Han, V. Bozza, A. Gould, M. Dominik, J.-P. Beaulieu, A. Udalski, U.G. Jørgensen, T. Sumi, D.M. Bramich, P. Browne, K. Horne, M. Hundertmark, S. Ipatov, N. Kains, C. Snodgrass, I.A. Steele, K.A. AlsubaiJ.M. Andersen, S.C. Novati, Y. Damerdji, C. Diehl, A. Elyiv, E. Giannini, S. Hardis, K. Harpsøe, T.C. Hinse, D. Juncher, E. Kerins, H. Korhonen, C. Liebig, L. Mancini, M. Mathiasen, M.T. Penny, M. Rabus, S. Rahvar, G. Scarpetta, J. Skottfelt, J. Southworth, J. Surdej, J. Tregloan-Reed, C. Vilela, J. Wambsganss, J. Skowron, R. Poleski, S. Kozłowski, Ł. Wyrzykowski, M.K. Szymański, M. Kubiak, P. Pietrukowicz, G. Pietrzyński, I. Soszyński, K. Ulaczyk, M.D. Albrow, E. Bachelet, R. Barry, V. Batista, A. Bhattacharya, S. Brillant, J.A.R. Caldwell, A. Cassan, A. Cole, E. Corrales, C. Coutures, S. Dieters, D. Dominis Prester, J. Donatowicz, P. Fouqué, J. Greenhill, S.R. Kane, D. Kubas, J.-B. Marquette, J. Menzies, C. Père, K.R. Pollard, M. Zub, G. Christie, D.L. Depoy, S. Dong, J. Drummond, B.S. Gaudi, C.B. Henderson, K.H. Hwang, Y.K. Jung, A. Kavka, J.-R. Koo, C.-U. Lee, D. Maoz, L.A.G. Monard, T. Natusch, H. Ngan, H. Park, R.W. Pogge, I. Porritt, I.-G. Shin, Y. Shvartzvald, T.G. Tan, J.C. Yee, F. Abe, D.P. Bennett, I.A. Bond, C.S. Botzler, M. Freeman, A. Fukui, D. Fukunaga, Y. Itow, N. Koshimoto, C.H. Ling, K. Masuda, Y. Matsubara, Y. Muraki, S. Namba, K. Ohnishi, N.J. Rattenbury, T. Saito, D.J. Sullivan, W.L. Sweatman, D. Suzuki, P.J. Tristram, N. Tsurumi, K. Wada, N. Yamai, P.C.M. Yock, A. Yonehara

School of Physics and Astronomy

Research output: Contribution to journal › Article › peer-review

Abstract

We present a detailed analysis of survey and follow-up observations of microlensing event OGLE-2012-BLG-0406 based on data obtained from 10 different observatories. Intensive coverage of the light curve, especially the perturbation part, allowed us to accurately measure the parallax effect and lens orbital motion. Combining our measurement of the lens parallax with the angular Einstein radius determined from finite-source effects, we estimate the physical parameters of the lens system. We find that the event was caused by a 2.73 ± 0.43 M _J planet orbiting a 0.44 ± 0.07 M _☉ early M-type star. The distance to the lens is 4.97 ± 0.29 kpc and the projected separation between the host star and its planet at the time of the event is 3.45 ± 0.26 AU. We find that the additional coverage provided by follow-up observations, especially during the planetary perturbation, leads to a more accurate determination of the physical parameters of the lens.

Original language	English
Article number	48
Number of pages	9
Journal	Astrophysical Journal
Volume	782
Issue number	1
Early online date	27 Jan 2014
DOIs	https://doi.org/10.1088/0004-637X/782/1/48
Publication status	Published - 10 Feb 2014

Keywords

Binaries: general
Gravitational lensing: micro
Planetary systems

Access to Document

10.1088/0004-637X/782/1/48

Dominik_2014_TAJ_ASuper
© 2014. The American Astronomical Society. All rights reserved.
Final published version, 1.97 MB

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
Planet population statistics: Planet population statistics from fully-deterministic microlensing campaigns
Dominik, M. (PI)
The Royal Society
1/10/11 → 30/09/15
Project: Fellowship

Cite this

Tsapras, Y., Choi, J.-Y., Street, R. A., Han, C., Bozza, V., Gould, A., Dominik, M., Beaulieu, J.-P., Udalski, A., Jørgensen, U. G., Sumi, T., Bramich, D. M., Browne, P., Horne, K., Hundertmark, M., Ipatov, S., Kains, N., Snodgrass, C., Steele, I. A., ... Yonehara, A. (2014). A super-Jupiter orbiting a late-type star: a refined analysis of microlensing event OGLE-2012-BLG-0406. Astrophysical Journal, 782(1), Article 48. https://doi.org/10.1088/0004-637X/782/1/48

@article{666c43280e2143028ebdc08fffd76b10,

title = "A super-Jupiter orbiting a late-type star: a refined analysis of microlensing event OGLE-2012-BLG-0406",

abstract = "We present a detailed analysis of survey and follow-up observations of microlensing event OGLE-2012-BLG-0406 based on data obtained from 10 different observatories. Intensive coverage of the light curve, especially the perturbation part, allowed us to accurately measure the parallax effect and lens orbital motion. Combining our measurement of the lens parallax with the angular Einstein radius determined from finite-source effects, we estimate the physical parameters of the lens system. We find that the event was caused by a 2.73 ± 0.43 M J planet orbiting a 0.44 ± 0.07 M ☉ early M-type star. The distance to the lens is 4.97 ± 0.29 kpc and the projected separation between the host star and its planet at the time of the event is 3.45 ± 0.26 AU. We find that the additional coverage provided by follow-up observations, especially during the planetary perturbation, leads to a more accurate determination of the physical parameters of the lens.",

keywords = "Binaries: general, Gravitational lensing: micro, Planetary systems",

author = "Y. Tsapras and J.-Y. Choi and R.A. Street and C. Han and V. Bozza and A. Gould and M. Dominik and J.-P. Beaulieu and A. Udalski and U.G. J{\o}rgensen and T. Sumi and D.M. Bramich and P. Browne and K. Horne and M. Hundertmark and S. Ipatov and N. Kains and C. Snodgrass and I.A. Steele and K.A. Alsubai and J.M. Andersen and S.C. Novati and Y. Damerdji and C. Diehl and A. Elyiv and E. Giannini and S. Hardis and K. Harps{\o}e and T.C. Hinse and D. Juncher and E. Kerins and H. Korhonen and C. Liebig and L. Mancini and M. Mathiasen and M.T. Penny and M. Rabus and S. Rahvar and G. Scarpetta and J. Skottfelt and J. Southworth and J. Surdej and J. Tregloan-Reed and C. Vilela and J. Wambsganss and J. Skowron and R. Poleski and S. Koz{\l}owski and {\L}. Wyrzykowski and M.K. Szyma{\'n}ski and M. Kubiak and P. Pietrukowicz and G. Pietrzy{\'n}ski and I. Soszy{\'n}ski and K. Ulaczyk and M.D. Albrow and E. Bachelet and R. Barry and V. Batista and A. Bhattacharya and S. Brillant and J.A.R. Caldwell and A. Cassan and A. Cole and E. Corrales and C. Coutures and S. Dieters and {Dominis Prester}, D. and J. Donatowicz and P. Fouqu{\'e} and J. Greenhill and S.R. Kane and D. Kubas and J.-B. Marquette and J. Menzies and C. P{\`e}re and K.R. Pollard and M. Zub and G. Christie and D.L. Depoy and S. Dong and J. Drummond and B.S. Gaudi and C.B. Henderson and K.H. Hwang and Y.K. Jung and A. Kavka and J.-R. Koo and C.-U. Lee and D. Maoz and L.A.G. Monard and T. Natusch and H. Ngan and H. Park and R.W. Pogge and I. Porritt and I.-G. Shin and Y. Shvartzvald and T.G. Tan and J.C. Yee and F. Abe and D.P. Bennett and I.A. Bond and C.S. Botzler and M. Freeman and A. Fukui and D. Fukunaga and Y. Itow and N. Koshimoto and C.H. Ling and K. Masuda and Y. Matsubara and Y. Muraki and S. Namba and K. Ohnishi and N.J. Rattenbury and T. Saito and D.J. Sullivan 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",

note = "D.M.B., M.D., K.H., C.S., R.A.S., K.A.A., M.H., and Y.T. are supported by NPRP grant NPRP-09-476-1-78 from the Qatar National Research Fund (a member of Qatar Foundation). C.S. received funding from the European Union Seventh Framework Programme (FP7/2007-2013) under grant agreement No. 268421. K.H. is supported by a Royal Society Leverhulme Trust Senior Research Fellowship. J.P.B. and P.F. acknowledge the financial support of Programme National de Plantologie and of IAP. 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. Work by C.H. was supported by Creative Research Initiative Program (2009-0081561) of National Research Foundation of Korea. The MOA experiment was supported by grants JSPS22403003 and JSPS23340064. T.S. acknowledges the support JSPS24253004. T.S. is supported by the grant JSPS23340044. T.C.H. acknowledges support from KRCF via the KRCF Young Scientist Fellowship program and financial support from KASI grant number 2013-9-400-00. Y.M. acknowledges support from JSPS grants JSPS23540339 and JSPS19340058. A.G. and B.S.G. acknowledge support from NSF AST-1103471. M.R. acknowledges support from FONDECYT postdoctoral fellowship No3120097. B.S.G., A.G., and R.W.P. acknowledge support from NASA grant NNX12AB99G. Y.D., A.E., and J.S. acknowledge support from the Communaute francaise de Belgique—Actions de recherche concertees—Academie Wallonie-Europe. ",

year = "2014",

month = feb,

day = "10",

doi = "10.1088/0004-637X/782/1/48",

language = "English",

volume = "782",

journal = "Astrophysical Journal",

issn = "0004-637X",

publisher = "American Astronomical Society",

number = "1",

}

Tsapras, Y, Choi, J-Y, Street, RA, Han, C, Bozza, V, Gould, A, Dominik, M, Beaulieu, J-P, Udalski, A, Jørgensen, UG, Sumi, T, Bramich, DM, Browne, P, Horne, K, Hundertmark, M, Ipatov, S, Kains, N, Snodgrass, C, Steele, IA, Alsubai, KA, Andersen, JM, Novati, SC, Damerdji, Y, Diehl, C, Elyiv, A, Giannini, E, Hardis, S, Harpsøe, K, Hinse, TC, Juncher, D, Kerins, E, Korhonen, H, Liebig, C, Mancini, L, Mathiasen, M, Penny, MT, Rabus, M, Rahvar, S, Scarpetta, G, Skottfelt, J, Southworth, J, Surdej, J, Tregloan-Reed, J, Vilela, C, Wambsganss, J, Skowron, J, Poleski, R, Kozłowski, S, Wyrzykowski, Ł, Szymański, MK, Kubiak, M, Pietrukowicz, P, Pietrzyński, G, Soszyński, I, Ulaczyk, K, Albrow, MD, Bachelet, E, Barry, R, Batista, V, Bhattacharya, A, Brillant, S, Caldwell, JAR, Cassan, A, Cole, A, Corrales, E, Coutures, C, Dieters, S, Dominis Prester, D, Donatowicz, J, Fouqué, P, Greenhill, J, Kane, SR, Kubas, D, Marquette, J-B, Menzies, J, Père, C, Pollard, KR, Zub, M, Christie, G, Depoy, DL, Dong, S, Drummond, J, Gaudi, BS, Henderson, CB, Hwang, KH, Jung, YK, Kavka, A, Koo, J-R, Lee, C-U, Maoz, D, Monard, LAG, Natusch, T, Ngan, H, Park, H, Pogge, RW, Porritt, I, Shin, I-G, Shvartzvald, Y, Tan, TG, Yee, JC, Abe, F, Bennett, DP, Bond, IA, Botzler, CS, Freeman, M, Fukui, A, Fukunaga, D, Itow, Y, Koshimoto, N, Ling, CH, Masuda, K, Matsubara, Y, Muraki, Y, Namba, S, Ohnishi, K, Rattenbury, NJ, Saito, T, Sullivan, DJ, Sweatman, WL, Suzuki, D, Tristram, PJ, Tsurumi, N, Wada, K, Yamai, N, Yock, PCM & Yonehara, A 2014, 'A super-Jupiter orbiting a late-type star: a refined analysis of microlensing event OGLE-2012-BLG-0406', Astrophysical Journal, vol. 782, no. 1, 48. https://doi.org/10.1088/0004-637X/782/1/48

TY - JOUR

T1 - A super-Jupiter orbiting a late-type star

T2 - a refined analysis of microlensing event OGLE-2012-BLG-0406

AU - Tsapras, Y.

AU - Choi, J.-Y.

AU - Street, R.A.

AU - Han, C.

AU - Bozza, V.

AU - Gould, A.

AU - Dominik, M.

AU - Beaulieu, J.-P.

AU - Udalski, A.

AU - Jørgensen, U.G.

AU - Sumi, T.

AU - Bramich, D.M.

AU - Browne, P.

AU - Horne, K.

AU - Hundertmark, M.

AU - Ipatov, S.

AU - Kains, N.

AU - Snodgrass, C.

AU - Steele, I.A.

AU - Alsubai, K.A.

AU - Andersen, J.M.

AU - Novati, S.C.

AU - Damerdji, Y.

AU - Diehl, C.

AU - Elyiv, A.

AU - Giannini, E.

AU - Hardis, S.

AU - Harpsøe, K.

AU - Hinse, T.C.

AU - Juncher, D.

AU - Kerins, E.

AU - Korhonen, H.

AU - Liebig, C.

AU - Mancini, L.

AU - Mathiasen, M.

AU - Penny, M.T.

AU - Rabus, M.

AU - Rahvar, S.

AU - Scarpetta, G.

AU - Skottfelt, J.

AU - Southworth, J.

AU - Surdej, J.

AU - Tregloan-Reed, J.

AU - Vilela, C.

AU - Wambsganss, J.

AU - Skowron, J.

AU - Poleski, R.

AU - Kozłowski, S.

AU - Wyrzykowski, Ł.

AU - Szymański, M.K.

AU - Kubiak, M.

AU - Pietrukowicz, P.

AU - Pietrzyński, G.

AU - Soszyński, I.

AU - Ulaczyk, K.

AU - Albrow, M.D.

AU - Bachelet, E.

AU - Barry, R.

AU - Batista, V.

AU - Bhattacharya, A.

AU - Brillant, S.

AU - Caldwell, J.A.R.

AU - Cassan, A.

AU - Cole, A.

AU - Corrales, E.

AU - Coutures, C.

AU - Dieters, S.

AU - Dominis Prester, D.

AU - Donatowicz, J.

AU - Fouqué, P.

AU - Greenhill, J.

AU - Kane, S.R.

AU - Kubas, D.

AU - Marquette, J.-B.

AU - Menzies, J.

AU - Père, C.

AU - Pollard, K.R.

AU - Zub, M.

AU - Christie, G.

AU - Depoy, D.L.

AU - Dong, S.

AU - Drummond, J.

AU - Gaudi, B.S.

AU - Henderson, C.B.

AU - Hwang, K.H.

AU - Jung, Y.K.

AU - Kavka, A.

AU - Koo, J.-R.

AU - Lee, C.-U.

AU - Maoz, D.

AU - Monard, L.A.G.

AU - Natusch, T.

AU - Ngan, H.

AU - Park, H.

AU - Pogge, R.W.

AU - Porritt, I.

AU - Shin, I.-G.

AU - Shvartzvald, Y.

AU - Tan, T.G.

AU - Yee, J.C.

AU - Abe, F.

AU - Bennett, D.P.

AU - Bond, I.A.

AU - Botzler, C.S.

AU - Freeman, M.

AU - Fukui, A.

AU - Fukunaga, D.

AU - Itow, Y.

AU - Koshimoto, N.

AU - Ling, C.H.

AU - Masuda, K.

AU - Matsubara, Y.

AU - Muraki, Y.

AU - Namba, S.

AU - Ohnishi, K.

AU - Rattenbury, N.J.

AU - Saito, T.

AU - Sullivan, D.J.

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.

N1 - D.M.B., M.D., K.H., C.S., R.A.S., K.A.A., M.H., and Y.T. are supported by NPRP grant NPRP-09-476-1-78 from the Qatar National Research Fund (a member of Qatar Foundation). C.S. received funding from the European Union Seventh Framework Programme (FP7/2007-2013) under grant agreement No. 268421. K.H. is supported by a Royal Society Leverhulme Trust Senior Research Fellowship. J.P.B. and P.F. acknowledge the financial support of Programme National de Plantologie and of IAP. 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. Work by C.H. was supported by Creative Research Initiative Program (2009-0081561) of National Research Foundation of Korea. The MOA experiment was supported by grants JSPS22403003 and JSPS23340064. T.S. acknowledges the support JSPS24253004. T.S. is supported by the grant JSPS23340044. T.C.H. acknowledges support from KRCF via the KRCF Young Scientist Fellowship program and financial support from KASI grant number 2013-9-400-00. Y.M. acknowledges support from JSPS grants JSPS23540339 and JSPS19340058. A.G. and B.S.G. acknowledge support from NSF AST-1103471. M.R. acknowledges support from FONDECYT postdoctoral fellowship No3120097. B.S.G., A.G., and R.W.P. acknowledge support from NASA grant NNX12AB99G. Y.D., A.E., and J.S. acknowledge support from the Communaute francaise de Belgique—Actions de recherche concertees—Academie Wallonie-Europe.

PY - 2014/2/10

Y1 - 2014/2/10

N2 - We present a detailed analysis of survey and follow-up observations of microlensing event OGLE-2012-BLG-0406 based on data obtained from 10 different observatories. Intensive coverage of the light curve, especially the perturbation part, allowed us to accurately measure the parallax effect and lens orbital motion. Combining our measurement of the lens parallax with the angular Einstein radius determined from finite-source effects, we estimate the physical parameters of the lens system. We find that the event was caused by a 2.73 ± 0.43 M J planet orbiting a 0.44 ± 0.07 M ☉ early M-type star. The distance to the lens is 4.97 ± 0.29 kpc and the projected separation between the host star and its planet at the time of the event is 3.45 ± 0.26 AU. We find that the additional coverage provided by follow-up observations, especially during the planetary perturbation, leads to a more accurate determination of the physical parameters of the lens.

AB - We present a detailed analysis of survey and follow-up observations of microlensing event OGLE-2012-BLG-0406 based on data obtained from 10 different observatories. Intensive coverage of the light curve, especially the perturbation part, allowed us to accurately measure the parallax effect and lens orbital motion. Combining our measurement of the lens parallax with the angular Einstein radius determined from finite-source effects, we estimate the physical parameters of the lens system. We find that the event was caused by a 2.73 ± 0.43 M J planet orbiting a 0.44 ± 0.07 M ☉ early M-type star. The distance to the lens is 4.97 ± 0.29 kpc and the projected separation between the host star and its planet at the time of the event is 3.45 ± 0.26 AU. We find that the additional coverage provided by follow-up observations, especially during the planetary perturbation, leads to a more accurate determination of the physical parameters of the lens.

KW - Binaries: general

KW - Gravitational lensing: micro

KW - Planetary systems

U2 - 10.1088/0004-637X/782/1/48

DO - 10.1088/0004-637X/782/1/48

M3 - Article

AN - SCOPUS:84893176264

SN - 0004-637X

VL - 782

JO - Astrophysical Journal

JF - Astrophysical Journal

IS - 1

M1 - 48

ER -

A super-Jupiter orbiting a late-type star: a refined analysis of microlensing event OGLE-2012-BLG-0406

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Astrophysics at St Andrews:2012 - 2014: Astrophysics at St Andrews: 2012 - 2014

Planet population statistics: Planet population statistics from fully-deterministic microlensing campaigns

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