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1. Identificação
Tipo de ReferênciaArtigo em Revista Científica (Journal Article)
Sitemtc-m21b.sid.inpe.br
Código do Detentorisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identificador8JMKD3MGP3W34P/3JLDG5P
Repositóriosid.inpe.br/mtc-m21b/2015/06.11.13.56
Última Atualização2015:07.06.13.49.03 (UTC) administrator
Repositório de Metadadossid.inpe.br/mtc-m21b/2015/06.11.13.56.44
Última Atualização dos Metadados2018:06.04.02.55.27 (UTC) administrator
DOI10.1088/0004-637X/804/1/33
ISSN0004-637X
Chave de CitaçãoSkowronSUHSSGPSJBBSKPSPKPUWABBBFFFILKMMMNOPRSSSTYMKFABCCDGHHJJLMNNPPYABBBCCCCCDDFGKKKMMMPRSWWWTBHHSSABBNDDDFGHHHHJKLLLMMPRRSSSSTW:2015:JoMiPl
TítuloOGLE-2011-BLG-0265Lb: a jovian microlensing planet orbiting an M DWARF
Ano2015
Data de Acesso09 maio 2024
Tipo de Trabalhojournal article
Tipo SecundárioPRE PI
Número de Arquivos1
Tamanho979 KiB
2. Contextualização
Autor  1 Skowron, J.
  2 Shin, I-G.
  3 Udalski, A.
  4 Han, C.
  5 Sumi, T.
  6 Shvartzvald, Y.
  7 Gould, A.
  8 Prester, D. Dominis
  9 Street, R. A.
 10 Jorgensen, U. G.
 11 Bennett, D. P.
 12 Bozza, V.
 13 Szymanski, M. K.
 14 Kubiak, M.
 15 Pietrzynski, G.
 16 Soszynski, I.
 17 Poleski, R.
 18 Kozlowski, S.
 19 Pietrukowicz, P.
 20 Ulaczyk, K.
 21 Wyrzykowski, L.
 22 Abe, F.
 23 Bhattacharya, A.
 24 Bond, I. A.
 25 Botzler, C. S.
 26 Freeman, M.
 27 Fukui, A.
 28 Fukunaga, D.
 29 Itow, Y.
 30 Ling, C. H.
 31 Koshimoto, N.
 32 Masuda, K.
 33 Matsubara, Y.
 34 Muraki, Y.
 35 Namba, S.
 36 Ohnishi, K.
 37 Philpott, L. C.
 38 Rattenbury, N.
 39 Saito, T.
 40 Sullivan, D. J.
 41 Suzuki, D.
 42 Tristam, P. J.
 43 Yock, P. C. M.
 44 Maoz, D.
 45 Kaspi, S.
 46 Friedmann, M.
 47 Almeida, Leonardo Andrade de
 48 Batista, V.
 49 Christie, G.
 50 Choi, J. Y.
 51 DePoy, D. L.
 52 Gaudi, B. S.
 53 Henderson, C.
 54 Hwang, K. H.
 55 Jablonski, Francisco José
 56 Jung, Y. K.
 57 Lee, C. U.
 58 McCormick, J.
 59 Natusch, T.
 60 Ngan, H.
 61 Park, H.
 62 Pogge, R. W.
 63 Yee, J. C.
 64 Albrow, M. D.
 65 Bachelet, E.
 66 Beaulieu, J. P.
 67 Brillant, S.
 68 Caldwell, J. A. R.
 69 Cassan, A.
 70 Cole, A.
 71 Corrales, E.
 72 Coutures, Ch.
 73 Dieters, S.
 74 Donatowicz, J.
 75 Fouqué, P.
 76 Greenhill, J.
 77 Kains, N.
 78 Kane, S. R.
 79 Kubas, D.
 80 Marquette, J. B.
 81 Martin, R.
 82 Menzies, J.
 83 Pollard, K. R.
 84 Ranc, C.
 85 Sahu, K. C.
 86 Wambganss, J.
 87 Williams, A.
 88 Wouters, D.
 89 Tsapras, Y.
 90 Bramich, D. M.
 91 Horne, K.
 92 Hundertmark, M.
 93 Snodgrass, C.
 94 Steele, I. A.
 95 Alsubai, K. A.
 96 Browne, P.
 97 Burgdorf, M. J.
 98 Novati, S. Calchi
 99 Dodds, P.
100 Dominik, M.
101 Dreizler, S.
102 Fang, X. S.
103 Gu, C. H.
104 Hardis
105 Harpsoe, K.
106 Hessman, F. V.
107 Hinse, T. C.
108 Hornstrup, A.
109 Jessen-Hansen, J.
110 Kerins, E.
111 Liebig, C.
112 Lund, M.
113 Lundkvist, M.
114 Mancini, L.
115 Mathiasen, M.
116 Penny, M. T.
117 Rahvar, S.
118 Ricci, D.
119 Scarpetta, G.
120 Skottfelt, J.
121 Southworth, J.
122 Surdej, J.
123 Tregolan-Reed, J.
124 Wertz, O.
Identificador de Curriculo  1
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Grupo  1
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 55 DAS-CEA-INPE-MCTI-GOV-BR
Afiliação  1 Warsaw University Observatory
  2 Chungbuk National University
  3 Warsaw University Observatory
  4 Chungbuk National University
  5 Osaka University
  6 Tel-Aviv University
  7 Ohio State University
  8 University of Rijeka
  9 Las Cumbres Observatory Global Telescope Network
 10 University of Copenhagen
 11 University of Notre Dame
 12 Università degli Studi di Salerno
 13 Warsaw University Observatory
 14 Warsaw University Observatory
 15 Warsaw University Observatory
 16 Warsaw University Observatory
 17 Warsaw University Observatory
 18 Warsaw University Observatory
 19 Warsaw University Observatory
 20 Warsaw University Observatory
 21 University of Cambridge
 22 Nagoya University
 23 University of Notre Dame
 24 Massey University
 25 University of Auckland
 26 University of Auckland
 27 National Astronomical Observatory of Japan
 28 Nagoya University
 29 Nagoya University
 30 Massey University
 31 Osaka University
 32 Nagoya University
 33 Nagoya University
 34 Konan University
 35 Osaka University
 36 Nagano National College of Technology
 37 University of British Columbia
 38 University of Auckland
 39 Tokyo Metropolitan College of Industrial Technology
 40 Victoria University
 41 Osaka University
 42 Victoria University
 43 University of Auckland
 44 Tel-Aviv University
 45 Tel-Aviv University
 46 Tel-Aviv University
 47 Instituto Nacional de Pesquisas Espaciais (INPE)
 48 Ohio State University
 49 Auckland Observatory
 50 Chungbuk National University
 51 Texas A&M University College Station
 52 Ohio State University
 53 Ohio State University
 54 Chungbuk National University
 55 Instituto Nacional de Pesquisas Espaciais (INPE)
 56 Chungbuk National University
 57 Korea Astronomy and Space Science Institute
 58 Centre for Backyard Astrophysics
 59 Auckland Observatory
 60 Auckland Observatory
 61 Chungbuk National University
 62 Ohio State University
 63 Ohio State University
 64 University of Canterbury
 65 Université de Toulouse
 66 Institut d’Astrophysique de Paris
 67 European Southern Observatory (ESO)
 68 McDonald Observatory
 69 Institut d’Astrophysique de Paris
 70 University of Tasmania
 71 Institut d’Astrophysique de Paris
 72 Institut d’Astrophysique de Paris
 73 Université de Toulouse
 74 Technical University of Vienna
 75 Université de Toulouse
 76 University of Tasmania
 77 European Southern Observatory
 78 NASA Exoplanet Science Institute
 79 Institut d’Astrophysique de Paris
 80 Institut d’Astrophysique de Paris
 81 Perth Observatory
 82 South African Astronomical Observatory
 83 University of Canterbury
 84 Institut d’Astrophysique de Paris
 85 Space Telescope Science Institute
 86 Zentrum für Astronomie der Universität Heidelberg (ZAH)
 87 Zentrum für Astronomie der Universität Heidelberg (ZAH)
 88 Institut d’Astrophysique de Paris
 89 Las Cumbres Observatory Global Telescope Network
 90 Qatar Foundation
 91 University of St Andrews
 92 University of St Andrews
 93 Max Planck Institute for Solar System Research
 94 Liverpool John Moores University
 95 Qatar Foundation
 96 University of St Andrews
 97 HE Space Operations GmbH
 98 NASA Exoplanet Science Institute
 99 University of St Andrews
100 University of St Andrews
101 Georg-August-Universität
102 Chinese Academy of Sciences
103 Chinese Academy of Sciences
104 University of Copenhagen
105 University of Copenhagen
106 Georg-August-Universität
107 Korea Astronomy and Space Science Institute
108 University of Manchester
109 Aarhus University
110 University of Manchester
111 University of St Andrews
112 Aarhus University
113 Aarhus University
114 Max Planck Institute for Astronomy
115 University of Copenhagen
116 University of Manchester
117 Sharif University of Technology
118 Institut d’Astrophysique et de Géophysique
119 Università degli Studi di Salerno
120 University of Copenhagen
121 Keele University
122 Institut d’Astrophysique et de Géophysique
123 NASA Ames Research Center
124 NASA Ames Research Center
Endereço de e-Mail do Autor  1
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 47 leonardo@das.inpe.br
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 55 chico@das.inpe.br
RevistaThe Astrophysical Journal
Volume804
Número33
Nota SecundáriaA1_QUÍMICA A1_INTERDISCIPLINAR A1_GEOCIÊNCIAS A1_ENGENHARIAS_III A1_ASTRONOMIA_/_FÍSICA A2_ENGENHARIAS_IV B2_ENSINO
Histórico (UTC)2015-06-11 13:56:44 :: simone -> administrator ::
2018-06-04 02:55:27 :: administrator -> simone :: 2015
3. Conteúdo e estrutura
É a matriz ou uma cópia?é a matriz
Estágio do Conteúdoconcluido
Transferível1
Tipo do ConteúdoExternal Contribution
Tipo de Versãopublisher
Palavras-Chavegravitational lensing: micro – planetary systems
ResumoWe report the discovery of a Jupiter-mass planet orbiting an M-dwarf star that gave rise to the microlensing event OGLE-2011-BLG-0265. Such a system is very rare among known planetary systems and thus the discovery is important for theoretical studies of planetary formation and evolution. High-cadence temporal coverage of the planetary signal, combined with extended observations throughout the event, allows us to accurately model the observed light curve. However, the final microlensing solution remains degenerate, yielding two possible configurations of the planet and the host star. In the case of the preferred solution, the mass of the planet is M M p J = +- 0.9 0.3 , and the planet is orbiting a star with a mass M M = +- 0.22 0.06 M.The second possible configuration (2σ away) consists of a planet with M M p J = +- 0.6 0.3 and host star with M M = +- 0.14 0.06 M. The system is located in the Galactic disk 34 kpc toward the Galactic bulge. In both cases, with an orbit size of 1.52.0 AU, the planet is a cold Jupiterlocated well beyond the snow line of the host star. Currently available data make the secure selection of the correct solution difficult, but there are prospects for lifting the degeneracy with additional follow-up observations in the future, when the lens and source star separate.
ÁreaCEA
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