A giant planet beyond the snow line in microlensing event OGLE-2011-BLG-0251
Aims. We present the analysis of the gravitational microlensing event OGLE-2011-BLG-0251. This anomalous event was observed by several survey and follow-up collaborations conducting microlensing observations towards the Galactic bulge.Methods. Based on detailed modelling of the observed light curve,...
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| Format: | Journal Article |
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EDP Sciences
2013
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| Online Access: | http://www.aanda.org/articles/aa/abs/2013/04/aa20626-12/aa20626-12.html http://hdl.handle.net/20.500.11937/46406 |
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| author | Kains, N. Street, R. Choi, J. Han, C. Udalski, A. Almeida, L. Jablonski, F. Tristram, P. Jorgensen, U. Szymanski, M. Kubiak, M. Pietrzynski, G. Soszynski, I. Poleski, R. Kozlowski, S. Pietrukowicz, P. Ulaczyk, K. Wyrzykowski, L. Skowron, J. Alsubai, K. Bozza, V. Browne, P. Burgdorf, M. Calchi Novati, S. Dodds, P. Dominik, M. Dreizler, S. Fang, X. Grundahl, F. Gu, C. Hardis, S. Harpsoe, K. Hessman, F. Hinse, T. Hornstrup, A. Hundertmark, M. Jessen-Hansen, J. Kerins, E. Liebig, C. Lund, M. Lundkvist, M. Mancini, L. Mathiasen, M. Penny, M. Rahvar, S. Ricci, D. Sahu, K. Scarpetta, G. Skottfelt, J. Snodgrass, C. Southworth, J. Surdej, J. Tregloan-Reed, J. Wambsganss, J. Wertz, O. Bajek, D. Bramich, D. Horne, K. Ipatov, S. Steele, I. Tsapras, Y. Abe, F. Bennett, D. Bond, I. Botzler, C. Chote, P. Freeman, M. Fukui, A. Furusawa, K. Itow, Y. Ling, C. Masuda, K. Matsubara, Y. Miyake, N. Muraki, Y. Ohnishi, K. Rattenbury, N. Saito, T. Sullivan, D. Sumi, T. Suzuki, D. Suzuki, K. Sweatman, W. Takino, S. Wada, K. Yock, P. Allen, W. Batista, V. Chung, S. Christie, G. DePoy, D. Drummond, J. Gaudi, B. Gould, A. Henderson, C. Jung, Y. Koo, J. Lee, C. McCormick, J. McGregor, D. Munoz, J. Natusch, T. Ngan, H. Park, H. Pogge, R. Shin, I. Yee, J. Albrow, M. Bachelet, E. Beaulieu, J. Brillant, S. Caldwell, J. Cassan, A. Cole, A. Corrales, E. Coutures, C. Dieters, S. Dominis Prester, D. Donatowicz, J. Fouque, P. Greenhill, J. Kane, S. Kubas, D. Marquette, J. Martin, R. Meintjes, P. Menzies, J. Pollard, K. Williams, Andrew Wouters, D. Zub, M. |
| author_facet | Kains, N. Street, R. Choi, J. Han, C. Udalski, A. Almeida, L. Jablonski, F. Tristram, P. Jorgensen, U. Szymanski, M. Kubiak, M. Pietrzynski, G. Soszynski, I. Poleski, R. Kozlowski, S. Pietrukowicz, P. Ulaczyk, K. Wyrzykowski, L. Skowron, J. Alsubai, K. Bozza, V. Browne, P. Burgdorf, M. Calchi Novati, S. Dodds, P. Dominik, M. Dreizler, S. Fang, X. Grundahl, F. Gu, C. Hardis, S. Harpsoe, K. Hessman, F. Hinse, T. Hornstrup, A. Hundertmark, M. Jessen-Hansen, J. Kerins, E. Liebig, C. Lund, M. Lundkvist, M. Mancini, L. Mathiasen, M. Penny, M. Rahvar, S. Ricci, D. Sahu, K. Scarpetta, G. Skottfelt, J. Snodgrass, C. Southworth, J. Surdej, J. Tregloan-Reed, J. Wambsganss, J. Wertz, O. Bajek, D. Bramich, D. Horne, K. Ipatov, S. Steele, I. Tsapras, Y. Abe, F. Bennett, D. Bond, I. Botzler, C. Chote, P. Freeman, M. Fukui, A. Furusawa, K. Itow, Y. Ling, C. Masuda, K. Matsubara, Y. Miyake, N. Muraki, Y. Ohnishi, K. Rattenbury, N. Saito, T. Sullivan, D. Sumi, T. Suzuki, D. Suzuki, K. Sweatman, W. Takino, S. Wada, K. Yock, P. Allen, W. Batista, V. Chung, S. Christie, G. DePoy, D. Drummond, J. Gaudi, B. Gould, A. Henderson, C. Jung, Y. Koo, J. Lee, C. McCormick, J. McGregor, D. Munoz, J. Natusch, T. Ngan, H. Park, H. Pogge, R. Shin, I. Yee, J. Albrow, M. Bachelet, E. Beaulieu, J. Brillant, S. Caldwell, J. Cassan, A. Cole, A. Corrales, E. Coutures, C. Dieters, S. Dominis Prester, D. Donatowicz, J. Fouque, P. Greenhill, J. Kane, S. Kubas, D. Marquette, J. Martin, R. Meintjes, P. Menzies, J. Pollard, K. Williams, Andrew Wouters, D. Zub, M. |
| author_sort | Kains, N. |
| building | Curtin Institutional Repository |
| collection | Online Access |
| description | Aims. We present the analysis of the gravitational microlensing event OGLE-2011-BLG-0251. This anomalous event was observed by several survey and follow-up collaborations conducting microlensing observations towards the Galactic bulge.Methods. Based on detailed modelling of the observed light curve, we find that the lens is composed of twomasses with a mass ratio q = 1.9 × 10-3. Thanks to our detection of higher-order effects on the light curve due to the Earth’s orbital motion and the finite size of source, we are able to measure the mass and distance to the lens unambiguously.Results. We find that the lens is made up of a planet of mass 0.53 ± 0.21 MJ orbiting an M dwarf host star with a mass of 0.26 ± 0.11 M. The planetary system is located at a distance of 2.57 ± 0.61 kpc towards the Galactic centre. The projected separation of the planet from its host star is d = 1.408 ± 0.019, in units of the Einstein radius, which corresponds to 2.72 ± 0.75 AU in physical units. We also identified a competitive model with similar planet and host star masses, but with a smaller orbital radius of 1.50 ± 0.50 AU. The planet is therefore located beyond the snow line of its host star, which we estimate to be around ~1-1.5 AU. |
| first_indexed | 2025-11-14T09:29:50Z |
| format | Journal Article |
| id | curtin-20.500.11937-46406 |
| institution | Curtin University Malaysia |
| institution_category | Local University |
| last_indexed | 2025-11-14T09:29:50Z |
| publishDate | 2013 |
| publisher | EDP Sciences |
| recordtype | eprints |
| repository_type | Digital Repository |
| spelling | curtin-20.500.11937-464062017-02-28T01:44:37Z A giant planet beyond the snow line in microlensing event OGLE-2011-BLG-0251 Kains, N. Street, R. Choi, J. Han, C. Udalski, A. Almeida, L. Jablonski, F. Tristram, P. Jorgensen, U. Szymanski, M. Kubiak, M. Pietrzynski, G. Soszynski, I. Poleski, R. Kozlowski, S. Pietrukowicz, P. Ulaczyk, K. Wyrzykowski, L. Skowron, J. Alsubai, K. Bozza, V. Browne, P. Burgdorf, M. Calchi Novati, S. Dodds, P. Dominik, M. Dreizler, S. Fang, X. Grundahl, F. Gu, C. Hardis, S. Harpsoe, K. Hessman, F. Hinse, T. Hornstrup, A. Hundertmark, M. Jessen-Hansen, J. Kerins, E. Liebig, C. Lund, M. Lundkvist, M. Mancini, L. Mathiasen, M. Penny, M. Rahvar, S. Ricci, D. Sahu, K. Scarpetta, G. Skottfelt, J. Snodgrass, C. Southworth, J. Surdej, J. Tregloan-Reed, J. Wambsganss, J. Wertz, O. Bajek, D. Bramich, D. Horne, K. Ipatov, S. Steele, I. Tsapras, Y. Abe, F. Bennett, D. Bond, I. Botzler, C. Chote, P. Freeman, M. Fukui, A. Furusawa, K. Itow, Y. Ling, C. Masuda, K. Matsubara, Y. Miyake, N. Muraki, Y. Ohnishi, K. Rattenbury, N. Saito, T. Sullivan, D. Sumi, T. Suzuki, D. Suzuki, K. Sweatman, W. Takino, S. Wada, K. Yock, P. Allen, W. Batista, V. Chung, S. Christie, G. DePoy, D. Drummond, J. Gaudi, B. Gould, A. Henderson, C. Jung, Y. Koo, J. Lee, C. McCormick, J. McGregor, D. Munoz, J. Natusch, T. Ngan, H. Park, H. Pogge, R. Shin, I. Yee, J. Albrow, M. Bachelet, E. Beaulieu, J. Brillant, S. Caldwell, J. Cassan, A. Cole, A. Corrales, E. Coutures, C. Dieters, S. Dominis Prester, D. Donatowicz, J. Fouque, P. Greenhill, J. Kane, S. Kubas, D. Marquette, J. Martin, R. Meintjes, P. Menzies, J. Pollard, K. Williams, Andrew Wouters, D. Zub, M. detection gravitational lensing weak – planets and satellites Galaxy planetary systems bulge Aims. We present the analysis of the gravitational microlensing event OGLE-2011-BLG-0251. This anomalous event was observed by several survey and follow-up collaborations conducting microlensing observations towards the Galactic bulge.Methods. Based on detailed modelling of the observed light curve, we find that the lens is composed of twomasses with a mass ratio q = 1.9 × 10-3. Thanks to our detection of higher-order effects on the light curve due to the Earth’s orbital motion and the finite size of source, we are able to measure the mass and distance to the lens unambiguously.Results. We find that the lens is made up of a planet of mass 0.53 ± 0.21 MJ orbiting an M dwarf host star with a mass of 0.26 ± 0.11 M. The planetary system is located at a distance of 2.57 ± 0.61 kpc towards the Galactic centre. The projected separation of the planet from its host star is d = 1.408 ± 0.019, in units of the Einstein radius, which corresponds to 2.72 ± 0.75 AU in physical units. We also identified a competitive model with similar planet and host star masses, but with a smaller orbital radius of 1.50 ± 0.50 AU. The planet is therefore located beyond the snow line of its host star, which we estimate to be around ~1-1.5 AU. 2013 Journal Article http://hdl.handle.net/20.500.11937/46406 http://www.aanda.org/articles/aa/abs/2013/04/aa20626-12/aa20626-12.html EDP Sciences restricted |
| spellingShingle | detection gravitational lensing weak – planets and satellites Galaxy planetary systems bulge Kains, N. Street, R. Choi, J. Han, C. Udalski, A. Almeida, L. Jablonski, F. Tristram, P. Jorgensen, U. Szymanski, M. Kubiak, M. Pietrzynski, G. Soszynski, I. Poleski, R. Kozlowski, S. Pietrukowicz, P. Ulaczyk, K. Wyrzykowski, L. Skowron, J. Alsubai, K. Bozza, V. Browne, P. Burgdorf, M. Calchi Novati, S. Dodds, P. Dominik, M. Dreizler, S. Fang, X. Grundahl, F. Gu, C. Hardis, S. Harpsoe, K. Hessman, F. Hinse, T. Hornstrup, A. Hundertmark, M. Jessen-Hansen, J. Kerins, E. Liebig, C. Lund, M. Lundkvist, M. Mancini, L. Mathiasen, M. Penny, M. Rahvar, S. Ricci, D. Sahu, K. Scarpetta, G. Skottfelt, J. Snodgrass, C. Southworth, J. Surdej, J. Tregloan-Reed, J. Wambsganss, J. Wertz, O. Bajek, D. Bramich, D. Horne, K. Ipatov, S. Steele, I. Tsapras, Y. Abe, F. Bennett, D. Bond, I. Botzler, C. Chote, P. Freeman, M. Fukui, A. Furusawa, K. Itow, Y. Ling, C. Masuda, K. Matsubara, Y. Miyake, N. Muraki, Y. Ohnishi, K. Rattenbury, N. Saito, T. Sullivan, D. Sumi, T. Suzuki, D. Suzuki, K. Sweatman, W. Takino, S. Wada, K. Yock, P. Allen, W. Batista, V. Chung, S. Christie, G. DePoy, D. Drummond, J. Gaudi, B. Gould, A. Henderson, C. Jung, Y. Koo, J. Lee, C. McCormick, J. McGregor, D. Munoz, J. Natusch, T. Ngan, H. Park, H. Pogge, R. Shin, I. Yee, J. Albrow, M. Bachelet, E. Beaulieu, J. Brillant, S. Caldwell, J. Cassan, A. Cole, A. Corrales, E. Coutures, C. Dieters, S. Dominis Prester, D. Donatowicz, J. Fouque, P. Greenhill, J. Kane, S. Kubas, D. Marquette, J. Martin, R. Meintjes, P. Menzies, J. Pollard, K. Williams, Andrew Wouters, D. Zub, M. A giant planet beyond the snow line in microlensing event OGLE-2011-BLG-0251 |
| title | A giant planet beyond the snow line in microlensing event OGLE-2011-BLG-0251 |
| title_full | A giant planet beyond the snow line in microlensing event OGLE-2011-BLG-0251 |
| title_fullStr | A giant planet beyond the snow line in microlensing event OGLE-2011-BLG-0251 |
| title_full_unstemmed | A giant planet beyond the snow line in microlensing event OGLE-2011-BLG-0251 |
| title_short | A giant planet beyond the snow line in microlensing event OGLE-2011-BLG-0251 |
| title_sort | giant planet beyond the snow line in microlensing event ogle-2011-blg-0251 |
| topic | detection gravitational lensing weak – planets and satellites Galaxy planetary systems bulge |
| url | http://www.aanda.org/articles/aa/abs/2013/04/aa20626-12/aa20626-12.html http://hdl.handle.net/20.500.11937/46406 |