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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 Acesso26 abr. 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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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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 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
Arranjourlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAS > OGLE-2011-BLG-0265Lb: a jovian...
Conteúdo da Pasta docacessar
Conteúdo da Pasta sourcenão têm arquivos
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4. Condições de acesso e uso
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5. Fontes relacionadas
Vinculação8JMKD3MGP7W/3D7EQNH
Repositório Espelhourlib.net/www/2011/03.29.20.55
Unidades Imediatamente Superiores8JMKD3MGPCW/3ETR8EH
Lista de Itens Citando
DivulgaçãoWEBSCI; PORTALCAPES; COMPENDEX; SCOPUS.
Acervo Hospedeirosid.inpe.br/mtc-m21b/2013/09.26.14.25.20
6. Notas
Campos Vaziosalternatejournal archivist callnumber copyholder copyright creatorhistory descriptionlevel e-mailaddress format isbn label lineage mark month nextedition notes orcid pages parameterlist parentrepositories previousedition previouslowerunit progress project rightsholder schedulinginformation secondarydate secondarykey session shorttitle sponsor subject targetfile tertiarytype url
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1. Identificação
Tipo de ReferênciaArtigo em Revista Científica (Journal Article)
Sitemtc-m16d.sid.inpe.br
Código do Detentorisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identificador8JMKD3MGP7W/3A67FCB
Repositóriosid.inpe.br/mtc-m19/2011/07.26.11.48
Última Atualização2011:12.27.17.26.54 (UTC) administrator
Repositório de Metadadossid.inpe.br/mtc-m19/2011/07.26.11.48.35
Última Atualização dos Metadados2018:06.05.04.24.37 (UTC) administrator
Chave SecundáriaINPE--PRE/
DOI10.1051/0004-6361/201016111
ISSN0004-6361
1432-0746
Chave de CitaçãoJablonskiBGDDBBMMCMAHTBNSCKKGHBAABDFFFHHIKKLLMMMMMNNOOPRSSSSTVYBCCCCCPDGHKKMMMMMPPSVWWWZABBDDEGGHJKLMMMMMNOPPPSSSTYBBDDFGGHHHHJLMMMRRSSSZABSSS:2011:MaPlOr
TítuloMOA-2009-BLG-387Lb: a massive planet orbiting an M dwarf
Ano2011
MêsMay
Data de Acesso26 abr. 2024
Tipo SecundárioPRE PI
Número de Arquivos1
Tamanho7570 KiB
2. Contextualização
Autor  1 Jablonski, F
  2 Batista, V.
  3 Gould, A.
  4 Dieters, S.
  5 Dong, S.
  6 Bond, I.
  7 Beaulieu, J. P.
  8 Maoz, D.
  9 Monard, B.
 10 Christie, G. W
 11 McCormick, J.
 12 Albrow, M. D.
 13 Horne, K.
 14 Tsapras, Y.
 15 Burgdorf, M. J.
 16 Novati, S. Calchi
 17 Skottfelt, J.
 18 Caldwell, J.
 19 Kozlowski, S.
 20 Kubas, D.
 21 Gaudi, B. S.
 22 Han, C.
 23 Bennett, D. P.
 24 An, J.
 25 Abe, F.
 26 Botzler, C. S.
 27 Douchin, D.
 28 Freeman, M.
 29 Fukui, A.
 30 Furusawa, K.
 31 Hearnshaw, J. B.
 32 Hosaka, S.
 33 Itow, Y.
 34 Kamiya, K.
 35 Kilmartin, P. M.
 36 Korpela
 37 Lin, W.
 38 Ling, C. H.
 39 Makita, S.
 40 Masuda, K.
 41 Matsubara, Y.
 42 Miyake, N.
 43 Muraki, Y.
 44 Nagaya, M.
 45 Nishimoto, K.
 46 Ohnishi, K.
 47 Okumura, T.
 48 Perrott, Y. C.
 49 Rattenbury, N.
 50 Saito, To.
 51 Sullivan, D. J.
 52 Sumi, T.
 53 Sweatman, W. L.
 54 Tristram, P. J.
 55 Von Seggern, E.
 56 Yock, P. C. M.
 57 Brillant, S.
 58 Calitz, J. J.
 59 Cassan, A.
 60 Cole, A.
 61 Cook, K.
 62 Coutures, C.
 63 Prester, D. Dominis
 64 Donatowicz, J.
 65 Greenhill, J.
 66 Hoffman, M.
 67 Kane, S. R.
 68 Kains, N.
 69 Marquette, J. -B.
 70 Martin, R.
 71 Martioli, Eder
 72 Meintjes, P.
 73 Menzies, J.
 74 Pedretti, E.
 75 Pollard, K.
 76 Sahu, K. C.
 77 Vinter, C.
 78 Wambsganss, J.
 79 Watson, R.
 80 Williams, A.
 81 Zub, M.
 82 Allen, W.
 83 Bolt, G.
 84 Bos, M.
 85 Depoy, D. L.
 86 Drummond, J.
 87 Eastman, J. D.
 88 Gal-Yam, A.
 89 Gorbikov, E.
 90 Higgins, D.
 91 Janczak, J.
 92 Kaspi, S.
 93 Lee, C. -U.
 94 Mallia, F.
 95 Maury, A.
 96 Monard, L. A. G.
 97 Moorhouse, D.
 98 Morgan, N.
 99 Natusch, T.
100 Ofek, E. O.
101 Park, B. -G.
102 Pogge, R. W.
103 Polishook, D.
104 Santallo, R.
105 Shporer, A.
106 Spector, O.
107 Thornley, G.
108 Yee, J. C.
109 Bozza, V.
110 Browne, P.
111 Dominik, M.
112 Dreizler, S.
113 Finet, F.
114 Glitrup, M.
115 Grundahl, F.
116 Harpsoe, K.
117 Hessman, F. V.
118 Hinse, T. C.
119 Hundertmark, M.
120 Jorgensen, U. G.
121 Liebig, C.
122 Maier, G.
123 Mancini, L.
124 Mathiasen, M.
125 Rahvar, S.
126 Ricci, D.
127 Scarpetta, G.
128 Southworth, J.
129 Surdej, J.
130 Zimmer, F.
131 Allan, A.
132 Bramich, D. M.
133 Snodgrass, C.
134 Steele, I. A.
135 Street, R. A.
Grupo  1 DAS-CEA-INPE-MCT-BR
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 71 DAS-CEA-INPE-MCT-BR
Afiliação  1 Instituto Nacional de Pesquisas Espaciais (INPE)
  2 Probing Lensing Anomalies NETwork PLANET, Chicago, IL USA
  3 Ohio State Univ, Dept Astron, Columbus, OH 43210 USA
  4 Probing Lensing Anomalies NETwork PLANET, Chicago, IL USA
  5 Inst Adv Study, Princeton, NJ 08540 USA
  6 MOA, Notre Dame, IN USA
  7 Probing Lensing Anomalies NETwork PLANET, Chicago, IL USA
  8 Tel Aviv Univ, Wise Observ, IL-69978 Tel Aviv, Israel
  9 Ctr Backyard Astrophys, Bronberg Observ, Pretoria, South Africa
 10 Auckland Observ, Auckland, New Zealand
 11 Ctr Backyard Astrophys, Farm Cove Observ, Auckland, New Zealand
 12 Univ Canterbury, Dept Phys & Astron, Christchurch 8020, New Zealand
 13 Probing Lensing Anomalies NETwork PLANET, Chicago, IL USA
 14 Probing Lensing Anomalies NETwork PLANET, Chicago, IL USA
 15 Microlensing Network Detect Small Terr Exoplanets, Les Ulis, France
 16 Microlensing Network Detect Small Terr Exoplanets, Les Ulis, France
 17 Microlensing Network Detect Small Terr Exoplanets, Les Ulis, France
 18 Probing Lensing Anomalies NETwork PLANET, Chicago, IL USA
 19 Ohio State Univ, Dept Astron, Columbus, OH 43210 USA
 20 Probing Lensing Anomalies NETwork PLANET, Chicago, IL USA
 21 Ohio State Univ, Dept Astron, Columbus, OH 43210 USA
 22 Microlensing Follow Network FUN, New York, NY USA.
 23 Probing Lensing Anomalies NETwork PLANET, Chicago, IL USA
 24 Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China
 25 Nagoya Univ, Solar Terr Environm Lab, Nagoya
 26 Univ Auckland, Dept Phys, Auckland, New Zealand
 27 Univ Auckland, Dept Phys, Auckland
 28 Univ Auckland, Dept Phys, Auckland
 29 Nagoya Univ, Solar Terr Environm Lab, Nagoya
 30 Nagoya Univ, Solar Terr Environm Lab, Nagoya
 31 Univ Canterbury, Dept Phys & Astron, Christchurch 8020, New Zealand
 32 Nagoya Univ, Solar Terr Environm Lab, Nagoya
 33 Nagoya Univ, Solar Terr Environm Lab, Nagoya
 34 Nagoya Univ, Solar Terr Environm Lab, Nagoya
 35 Mt John Observ, Lake Tekapo 8780, New Zealand
 36 Victoria Univ, Sch Chem & Phys Sci, Wellington, New Zealand.
 37 Massey Univ, Inst Informat & Math Sci, N Shore Mail Ctr, Auckland, New Zealand
 38 Massey Univ, Inst Informat & Math Sci, N Shore
 39 Nagoya Univ, Solar Terr Environm Lab, Nagoya
 40 Nagoya Univ, Solar Terr Environm Lab, Nagoya
 41 Nagoya Univ, Solar Terr Environm Lab, Nagoya
 42 Nagoya Univ, Solar Terr Environm Lab, Nagoya
 43 Konan Univ, Dept Phys, Kobe, Hyogo
 44 Nagoya Univ, Solar Terr Environm Lab, Nagoya
 45 Nagoya Univ, Solar Terr Environm Lab, Nagoya
 46 Nagano Natl Coll Technol, Nagano
 47 Nagoya Univ, Solar Terr Environm Lab, Nagoya
 48 Univ Auckland, Dept Phys, Auckland, New Zealand
 49 Univ Auckland, Dept Phys, Auckland, New Zealand
 50 Tokyo Metropolitan Coll Ind Technol, Tokyo
 51 Massey Univ, Inst Informat & Math Sci, N Shore Mail Ctr, Auckland, New Zealand
 52 Nagoya Univ, Solar Terr Environm Lab, Nagoya
 53 Massey Univ, Inst Informat & Math Sci, N Shore Mail Ctr, Auckland, New Zealand
 54 Mt John Observ, Lake Tekapo, New Zealand
 55 Univ Auckland, Dept Phys, Auckland, New Zealand
 56 Univ Auckland, Dept Phys, Auckland, New Zealand
 57 European So Observ, Santiago, Chile
 58 Univ Free State, Fac Nat & Agr Sci, Dept Phys, ZA-9300 Bloemfontein, South Africa.
 59 Univ Paris 06, Inst Astrophys Paris, CNRS
 60 Univ Tasmania, Sch Math & Phys, Hobart, Tas 7001, Australia.
 61 Lawrence Livermore Natl Lab, Inst Geophys & Planetary Phys, Livermore, CA 94551 USA.
 62 CEA Saclay, F-91191 Gif Sur Yvette, France.
 63 Univ Rijeka, Dept Phys, Rijeka 51000, Croatia.
 64 Vienna Univ Technol, A-1040 Vienna, Austria.
 65 Univ Tasmania, Sch Math & Phys, Hobart, Tas 7001, Australia.
 66 Univ St Andrews, SUPA Sch Phys & Astron, St Andrews KY16 9SS, Fife, Scotland
 67 CALTECH, NASA Exoplanet Sci Inst, Pasadena
 68 European So Observ, D-85748 Garching, Germany
 69 Univ Paris 06, Inst Astrophys Paris, CNRS UMR7095, F-75014 Paris, France.
 70 Perth Observ, Perth, WA 6076, Australia
 71 Instituto Nacional de Pesquisas Espaciais (INPE)
 72 Univ St Andrews, SUPA Sch Phys & Astron, St Andrews KY16 9SS, Fife, Scotland
 73 Univ Canterbury, Dept Phys & Astron, Christchurch 8020, New Zealand
 74 Univ St Andrews, SUPA Sch Phys & Astron, St Andrews KY16 9SS, Fife, Scotland.
 75 Univ Canterbury, Dept Phys & Astron, Christchurch 8020, New Zealand.
 76 Space Telescope Sci Inst, Baltimore, MD
 77 Univ Copenhagen, Niels Bohr Inst, DK-2100 Copenhagen
 78 Univ Western Australia, Sch Phys, Perth, WA 6009, Australia
 79 Univ Tasmania, Sch Math & Phys, Hobart, Tas 7001, Australia.
 80 Univ Western Australia, Sch Phys, Perth, WA 6009, Australia
 81 Univ Heidelberg ZAH, Astron Rechen Inst, Zentrum Astron, D-69120 Heidelberg, Germany.
 82 Vintage Lane Observ, Blenheim, New Zealand.
 83 Perth ustralia
 84 Molehill Astron Observ, Auckland, New Zealand.
 85 Ohio State Univ, Dept Astron, Columbus, OH 43210 USA
 86 Possum Observ, Patutahi, New Zealand
 87 Tel Aviv Univ, Wise Observ, IL-69978 Tel Aviv, Israel
 88 Weizmann Inst Sci, Dept Particle Phys & Astrophys,Israel
 89 Ohio State Univ, Dept Astron, Columbus, OH 43210 USA
 90 Tel Aviv Univ, Wise Observ, IL-69978 Tel Aviv, Israel
 91 Ohio State University Dep Astronomy
 92 Tel Aviv Univ, Sch Phys & Astron, IL-69978 Tel Aviv, Israel.
 93 Korea Astron & Space Sci Inst, Taejon
 94 Ctr Backyard Astrophys, Bronberg Observ, Pretoria, South Africa
 95 Campo Catino Austral Observ, San Pedro De Atacama, Chile.
 96 Ohio State Univ, Dept Astron, Columbus, OH 43210 USA
 97 Kumeu Observ, Kumeu, New Zealand.
 98 Ohio State Univ, Dept Astron, Columbus
 99 AUT Univ, Auckland, New Zealand
100 Ohio State Univ, Dept Astron, Columbus, OH 43210 USA
101 Tel Aviv Univ, Wise Observ, IL-69978 Tel Aviv, Israel
102 Ohio State Univ, Dept Astron, Columbus
103 Tel Aviv Univ, Wise Observ, IL-69978 Tel Aviv, Israel
104 Tel Aviv Univ, Wise Observ, IL-69978 Tel Aviv, Israel
105 Tel Aviv Univ, Sch Phys & Astron, IL-69978 Tel Aviv, Israel.
106 Ohio State Univ, Dept Astron, Columbus, OH 43210 USA
107 Ist Nazl Fis Nucl, Grp Collegato Salerno, Sez Napoli, Catania, Italy
108 Univ St Andrews, SUPA Sch Phys & Astron, St Andrews KY16 9SS, Fife, Scotland
109 Univ St Andrews, SUPA Sch Phys & Astron, St Andrews KY16 9SS, Fife, Scotland
110 Univ Gottingen, Inst Astrophys, D-37077 Gottingen, Germany
111 Inst Astrophys & Geophys, B-4000 Liege, Belgium
112 Aarhus Univ, Dept Phys & Astron, DK-8000 Aarhus C, Denmark
113 Inst Astrophys & Geophys, B-4000 Liege, Belgium
114 Aarhus Univ, Dept Phys & Astron, DK-8000 Aarhus C, Denmark.
115 Univ Gottingen, Inst Astrophys, D-37077 Gottingen, Germany
116 Observ, Armagh BT61 9DG, North Ireland
117 Univ Gottingen, Inst Astrophys, D-37077 Gottingen, Germany
118 Armagh Observ, Armagh BT61 9DG, North Ireland
119 Univ St Andrews, SUPA Sch Phys & Astron, St Andrews KY16 9SS, Fife, Scotland
120 Univ Copenhagen, Niels Bohr Inst, DK-2100 Copenhagen
121 Univ Sannio, Dipartimento Ingn, I-82100 Benevento, Italy
122 Univ Heidelberg ZAH, Astron Rechen Inst, Zentrum Astron, D-69120 Heidelberg, Germany.
123 IPM Inst Studies Theoret Phys & Math, Sch Astron, Tehran, Iran
124 Inst Astrophys & Geophys, B-4000 Liege, Belgium
125 Ist Nazl Fis Nucl, Grp Collegato Salerno, Sez Napoli, Catania, Italy
126 Keele Univ, Astrophys Grp, Keele ST5 5BG, Staffs, England
127 Inst Astrophys & Geophys, B-4000 Liege, Belgium
128 Keele Univ, Astrophys Grp, Keele ST5 5BG, Staffs, England
129 Inst Astrophys & Geophys, B-4000 Liege, Belgium
130 Probing Lensing Anomalies NETwork PLANET, Chicago, IL USA
131 Univ Exeter, Sch Phys, Exeter EX4 4QL, Devon, England
132 European So Observ, D-85748 Garching, Germany.
133 Max Planck Inst Solar Syst Res, D-37191 Katlenburg Lindau, Germany.
134 Liverpool John Moores Univ, Astrophys Res Inst
135 Las Cumbres Observ Global Telescope Network, Goleta
Endereço de e-Mailtereza@sid.inpe.br
RevistaAstronomy & Astrophysics
Volume529
NúmeroAR A102
Páginas16
Histórico (UTC)2011-07-26 11:50:46 :: marciana -> administrator :: 2011
2011-07-26 19:24:53 :: administrator -> marciana :: 2011
2011-11-01 11:45:46 :: marciana -> banon :: 2011
2011-11-23 13:47:12 :: banon -> tereza@sid.inpe.br :: 2011
2011-12-27 17:27:51 :: tereza@sid.inpe.br -> administrator :: 2011
2012-07-15 02:58:45 :: administrator -> banon :: 2011
2012-09-21 14:37:52 :: banon -> administrator :: 2011
2018-06-05 04:24:37 :: administrator -> tereza@sid.inpe.br :: 2011
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
methods: data analysis
planets and satellites: detection
methods: numerical
instrumentation: adaptive optics
instrumentation: photometers
GALACTIC BULGE
MICROLENSING EVENT
JUPITER/SATURN ANALOG
GIANT PLANETS
SNOW LINE
STARS
MASSES
PHOTOMETRY
COOL
LUMINOSITY
ResumoAims. We report the discovery of a planet with a high planet-to-star mass ratio in the microlensing event MOA-2009-BLG-387, which exhibited pronounced deviations over a 12-day interval, one of the longest for any planetary event. The host is an M dwarf, with a mass in the range 0.07 M(circle dot) < M(host) < 0.49 M(circle dot) at 90% confidence. The planet-star mass ratio q = 0.0132 +/- 0.003 has been measured extremely well, so at the best-estimated host mass, the planet mass is m(p) = 2.6 Jupiter masses for the median host mass, M = 0.19 M(circle dot). Methods. The host mass is determined from two "higher order" microlensing parameters. One of these, the angular Einstein radius theta(E) = 0.31 +/- 0.03 mas has been accurately measured, but the other (the microlens parallax pi(E), which is due to the Earth's orbital motion) is highly degenerate with the orbital motion of the planet. We statistically resolve the degeneracy between Earth and planet orbital effects by imposing priors from a Galactic model that specifies the positions and velocities of lenses and sources and a Kepler model of orbits. Results. The 90% confidence intervals for the distance, semi-major axis, and period of the planet are 3.5 kpc < D(L) < 7.9 kpc, 1.1 AU < a < 2.7 AU, and 3.8 yr < P < 7.6 yr, respectively.
ÁreaCEA
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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
Identificador8JMKD3MGP5W34M/3FA7RCT
Repositóriosid.inpe.br/mtc-m21b/2013/11.27.13.21.25
Última Atualização2013:12.05.13.46.57 (UTC) administrator
Repositório de Metadadossid.inpe.br/mtc-m21b/2013/11.27.13.21.26
Última Atualização dos Metadados2018:06.04.03.14.14 (UTC) administrator
DOI10.1051/0004-6361/201220626
ISSN0004-6361
1432-0746
Rótuloisi 2013-11
Chave de CitaçãoKainsSCHUAJTJSKPSPKPUWSABBBNDDDFGGHHHHHHJKLLLMMPRRSSSSSSTWWBBHISTABBBCFFFILMMMMORSSSSSSTWYABCCDDGGHJKLMMMNNPPSYABBBCCCCCDPDFGKKMMMMPWWZCCCCCC:2013:GiPlBe
TítuloA giant planet beyond the snow line in microlensing event OGLE-2011-BLG-0251
Ano2013
MêsApr.
Data de Acesso26 abr. 2024
Tipo de Trabalhojournal article
Tipo SecundárioPRE PI
Número de Arquivos1
Tamanho3380 KiB
2. Contextualização
Autor  1 Kains, N.
  2 Street, R. A.
  3 Choi, J. -Y.
  4 Han, C.
  5 Udalski, A.
  6 Almeida, L. A.
  7 Jablonski, Francisco Jose
  8 Tristram, P. J.
  9 Jorgensen, U. G.
 10 Szymanski, M. K.
 11 Kubiak, M.
 12 Pietrzynski, G.
 13 Soszynski, I.
 14 Poleski, R.
 15 Kozlowski, S.
 16 Pietrukowicz, P.
 17 Ulaczyk, K.
 18 Wyrzykowski, L.
 19 Skowron, J.
 20 Alsubai, K. A.
 21 Bozza, V.
 22 Browne, P.
 23 Burgdorf, M. J.
 24 Novati, S. Calchi
 25 Dodds, P.
 26 Dominik, M.
 27 Dreizler, S.
 28 Fang, X. -S.
 29 Grundahl, F.
 30 Gu, C-H.
 31 Hardis, S.
 32 Harpsoe, K.
 33 Hessman, F. V.
 34 Hinse, T. C.
 35 Hornstrup, A.
 36 Hundertmark, M.
 37 Jessen-Hansen, J.
 38 Kerins, E.
 39 Liebig, C.
 40 Lund, M.
 41 Lundkvist, M.
 42 Mancini, L.
 43 Mathiasen, M.
 44 Penny, M. T.
 45 Rahvar, S.
 46 Ricci, D.
 47 Sahu, K. C.
 48 Scarpetta, G.
 49 Skottfelt, J.
 50 Snodgrass, C.
 51 Southworth, J.
 52 Surdej, J.
 53 Tregloan-Reed, J.
 54 Wambsganss, J.
 55 Wertz, O.
 56 Bajek, D.
 57 Bramich, D. M.
 58 Horne, K.
 59 Ipatov, S.
 60 Steele, I. A.
 61 Tsapras, Y.
 62 Abe, F.
 63 Bennett, D. P.
 64 Bond, I. A.
 65 Botzler, C. S.
 66 Chote, P.
 67 Freeman, M.
 68 Fukui, A.
 69 Furusawa, K.
 70 Itow, Y.
 71 Ling, C. H.
 72 Masuda, K.
 73 Matsubara, Y.
 74 Miyake, N.
 75 Muraki, Y.
 76 Ohnishi, K.
 77 Rattenbury, N.
 78 Saito, T.
 79 Sullivan, D. J.
 80 Sumi, T.
 81 Suzuki, D.
 82 Suzuki, K.
 83 Sweatman, W. L.
 84 Takino, S.
 85 Wada, K.
 86 Yock, P. C. M.
 87 Allen, W.
 88 Batista, V.
 89 Chung, S. -J.
 90 Christie, G.
 91 DePoy, D. L.
 92 Drummond, J.
 93 Gaudi, B. S.
 94 Gould, A.
 95 Henderson, C.
 96 Jung, Y. -K.
 97 Koo, J. -R.
 98 Lee, C. -U.
 99 McCormick, J.
100 McGregor, D.
101 Munoz, J. A.
102 Natusch, T.
103 Ngan, H.
104 Park, H.
105 Pogge, R. W.
106 Shin, I. -G.
107 Yee, J.
108 Albrow, M. D.
109 Bachelet, E.
110 Beaulieu, J. -P.
111 Brillant, S.
112 Caldwell, J. A. R.
113 Cassan, A.
114 Cole, A.
115 Corrales, E.
116 Coutures, Ch.
117 Dieters, S.
118 Prester, D. Dominis
119 Donatowicz, J.
120 Fouque, P.
121 Greenhill, J.
122 Kane, S. R.
123 Kubas, D.
124 Marquette, J. -B.
125 Martin, R.
126 Meintjes, P.
127 Menzies, J.
128 Pollard, K. R.
129 Williams, A.
130 Wouters, D.
131 Zub, Andm.
132 Collaboration, OGLE
133 Consortium, MiNDSTEp
134 Collaboration, RoboNet
135 Collaboration, MOA
136 Collaboration, FUN
137 Collaboration, PLANET
Identificador de Curriculo  1
  2
  3
  4
  5
  6
  7 8JMKD3MGP5W/3C9JH4Q
Grupo  1
  2
  3
  4
  5
  6
  7 DAS-CEA-INPE-MCTI-GOV-BR
Afiliação  1 European So Observ, D-85748 Garching, Germany.
  2 Las Cumbres Observ Global Telescope Network, Goleta, CA 93117 USA.
  3 Chungbuk Natl Univ, Inst Astrophys, Dept Phys, Chonju 371763, South Korea.
  4 Chungbuk Natl Univ, Inst Astrophys, Dept Phys, Chonju 371763, South Korea.
  5 Univ Warsaw Observ, PL-00478 Warsaw, Poland.
  6 Inst Nacl Pesquisas Espaciais, Div Astrofis, BR-12227010 Sao Jose Dos Campos, SP, Brazil.
  7 Instituto Nacional de Pesquisas Espaciais (INPE)
  8 Victoria Univ, Sch Chem & Phys Sci, Wellington, New Zealand.
  9 Univ Copenhagen, Niels Bohr Inst, DK-2100 Copenhagen, Denmark.; Geol Museum, Ctr Star & Planet Format, DK-1350 Copenhagen, Denmark.
 10 Univ Warsaw Observ, PL-00478 Warsaw, Poland.
 11 Univ Warsaw Observ, PL-00478 Warsaw, Poland.
 12 Univ Warsaw Observ, PL-00478 Warsaw, Poland.; Univ Concepcion, Dept Astron, Concepcion, Chile.
 13 Univ Warsaw Observ, PL-00478 Warsaw, Poland.
 14 Univ Warsaw Observ, PL-00478 Warsaw, Poland.; Ohio State Univ, Dept Astron, Columbus, OH 43210 USA.
 15 Univ Warsaw Observ, PL-00478 Warsaw, Poland.
 16 Univ Warsaw Observ, PL-00478 Warsaw, Poland.
 17 Univ Warsaw Observ, PL-00478 Warsaw, Poland.
 18 Univ Warsaw Observ, PL-00478 Warsaw, Poland.; Univ Cambridge, Inst Astron, Cambridge CB3 0HA, England.
 19 Univ Warsaw Observ, PL-00478 Warsaw, Poland.; Ohio State Univ, Dept Astron, Columbus, OH 43210 USA.
 20 Qatar Fdn, Doha, Qatar.
 21 Univ Salerno, Dipartimento Fis ER Caianiello, I-84084 Fisciano, Italy.; Ist Nazl Fis Nucl, Sez Napoli, Naples, Italy.
 22 Univ St Andrews, SUPA Sch Phys & Astron, St Andrews KY16 9SS, Fife, Scotland.
 23 Univ Stuttgart, Deutsch SOFIA Inst, D-70569 Stuttgart, Germany.; NASA, Ames Res Ctr, SOFIA Sci Ctr, Moffett Field, CA 94035 USA.
 24 Univ Salerno, Dipartimento Fis ER Caianiello, I-84084 Fisciano, Italy.; IIASS, Vietri Sul Mare, SA, Italy.
 25 Univ St Andrews, SUPA Sch Phys & Astron, St Andrews KY16 9SS, Fife, Scotland.
 26 Univ St Andrews, SUPA Sch Phys & Astron, St Andrews KY16 9SS, Fife, Scotland.
 27 Univ Gottingen, Inst Astrophys, D-37077 Gottingen, Germany.
 28 Chinese Acad Sci, Yunnan Observ, Natl Astron Observ, Joint Lab Opt Astron, Kunming 650011, Peoples R China.
 29 Aarhus Univ, Dept Phys & Astron, DK-8000 Aarhus C, Denmark.
 30 Chinese Acad Sci, Yunnan Observ, Natl Astron Observ, Joint Lab Opt Astron, Kunming 650011, Peoples R China.
 31 Univ Copenhagen, Niels Bohr Inst, DK-2100 Copenhagen, Denmark.
 32 Univ Copenhagen, Niels Bohr Inst, DK-2100 Copenhagen, Denmark.; Geol Museum, Ctr Star & Planet Format, DK-1350 Copenhagen, Denmark.
 33 Univ Gottingen, Inst Astrophys, D-37077 Gottingen, Germany.
 34 Univ Copenhagen, Niels Bohr Inst, DK-2100 Copenhagen, Denmark.; Korea Astron & Space Sci Inst, Taejon 305348, South Korea.; Armagh Observ, Armagh BT61 9DG, North Ireland.
 35 Univ Manchester, Jodrell Bank Ctr Astrophys, Oxford M13 9PL, England.
 36 Univ St Andrews, SUPA Sch Phys & Astron, St Andrews KY16 9SS, Fife, Scotland.; Univ Gottingen, Inst Astrophys, D-37077 Gottingen, Germany.
 37 Aarhus Univ, Dept Phys & Astron, DK-8000 Aarhus C, Denmark.
 38 Univ Manchester, Jodrell Bank Ctr Astrophys, Oxford M13 9PL, England.
 39 Univ St Andrews, SUPA Sch Phys & Astron, St Andrews KY16 9SS, Fife, Scotland.
 40 Aarhus Univ, Dept Phys & Astron, DK-8000 Aarhus C, Denmark.
 41 Aarhus Univ, Dept Phys & Astron, DK-8000 Aarhus C, Denmark.
 42 Max Planck Inst Astron, D-69117 Heidelberg, Germany.
 43 Univ Copenhagen, Niels Bohr Inst, DK-2100 Copenhagen, Denmark.
 44 Univ Manchester, Jodrell Bank Ctr Astrophys, Oxford M13 9PL, England.; Ohio State Univ, Dept Astron, Columbus, OH 43210 USA.
 45 Sharif Univ Technol, Dept Phys, Tehran, Iran.; Perimeter Inst Theoret Phys, Waterloo, ON N2L 2Y5, Canada.
 46 Inst Astrophys & Geophys, B-4000 Liege, Belgium.
 47 Space Telescope Sci Inst, Baltimore, MD 21218 USA.
 48 Univ Salerno, Dipartimento Fis ER Caianiello, I-84084 Fisciano, Italy.; Ist Nazl Fis Nucl, Grp Collegato Salerno, Sez Napoli, Naples, Italy.
 49 Univ Copenhagen, Niels Bohr Inst, DK-2100 Copenhagen, Denmark.
 50 Max Planck Inst Solar Syst Res, D-37191 Katlenburg Lindau, Germany.
 51 Keele Univ, Astrophys Grp, Keele ST5 5BG, Staffs, England.
 52 Inst Astrophys & Geophys, B-4000 Liege, Belgium.
 53 Keele Univ, Astrophys Grp, Keele ST5 5BG, Staffs, England.
 54 Univ Heidelberg ZAH, Zentrum Astron, Astron Rechen Inst, D-69120 Heidelberg, Germany.
 55 Inst Astrophys & Geophys, B-4000 Liege, Belgium.
 56 Univ St Andrews, SUPA Sch Phys & Astron, St Andrews KY16 9SS, Fife, Scotland.
 57 European So Observ, D-85748 Garching, Germany.
 58 Univ St Andrews, SUPA Sch Phys & Astron, St Andrews KY16 9SS, Fife, Scotland.
 59 Alsubais Estab Sci Studies, Doha, Qatar.
 60 Liverpool John Moores Univ, Astrophys Res Inst, Birkenhead CH41 1LD, Wirral, England.
 61 Las Cumbres Observ Global Telescope Network, Goleta, CA 93117 USA.; Univ London, Sch Math Sci, London E1 4NS, England.
 62 Nagoya Univ, Solar Terr Environm Lab, Nagoya, Aichi 4648601, Japan.
 63 Univ Notre Dame, Dept Phys, Notre Dame, IN 46556 USA.
 64 Massey Univ, Inst Informat & Math Sci, North Shore Mail Ctr, Auckland, New Zealand.
 65 Univ Auckland, Dept Phys, Auckland, New Zealand.
 66 Victoria Univ, Sch Chem & Phys Sci, Wellington, New Zealand.
 67 Univ Auckland, Dept Phys, Auckland, New Zealand.
 68 Natl Astron Observ Japan, Okayama Astrophys Observ, Okayama 7190232, Japan.
 69 Nagoya Univ, Solar Terr Environm Lab, Nagoya, Aichi 4648601, Japan.
 70 Nagoya Univ, Solar Terr Environm Lab, Nagoya, Aichi 4648601, Japan.
 71 Massey Univ, Inst Informat & Math Sci, North Shore Mail Ctr, Auckland, New Zealand.
 72 Nagoya Univ, Solar Terr Environm Lab, Nagoya, Aichi 4648601, Japan.
 73 Nagoya Univ, Solar Terr Environm Lab, Nagoya, Aichi 4648601, Japan.
 74 Nagoya Univ, Solar Terr Environm Lab, Nagoya, Aichi 4648601, Japan.
 75 Konan Univ, Dept Phys, Kobe, Hyogo 6588501, Japan.
 76 Nagano Natl Coll Technol, Nagano 3818550, Japan.
 77 Univ Auckland, Dept Phys, Auckland, New Zealand.
 78 Tokyo Metropolitan Coll Ind Technol, Tokyo 1168523, Japan.
 79 Victoria Univ, Sch Chem & Phys Sci, Wellington, New Zealand.
 80 Osaka Univ, Grad Sch Sci, Dept Earth & Space Sci, Toyonaka, Osaka 5600043, Japan.
 81 Osaka Univ, Grad Sch Sci, Dept Earth & Space Sci, Toyonaka, Osaka 5600043, Japan.
 82 Nagoya Univ, Solar Terr Environm Lab, Nagoya, Aichi 4648601, Japan.
 83 Massey Univ, Inst Informat & Math Sci, North Shore Mail Ctr, Auckland, New Zealand.
 84 Nagoya Univ, Solar Terr Environm Lab, Nagoya, Aichi 4648601, Japan.
 85 Osaka Univ, Grad Sch Sci, Dept Earth & Space Sci, Toyonaka, Osaka 5600043, Japan.
 86 Univ Auckland, Dept Phys, Auckland, New Zealand.
 87 Vintage Lane Observ, Blenheim, New Zealand.
 88 Ohio State Univ, Dept Astron, Columbus, OH 43210 USA.
 89 Korea Astron & Space Sci Inst, Taejon 305348, South Korea.
 90 Auckland Observ, Auckland 1023, New Zealand.
 91 Texas A&M Univ, Dept Phys & Astron, College Stn, TX 77843 USA.
 92 Possum Observ, Patutahi, Gisbourne, New Zealand.
 93 Ohio State Univ, Dept Astron, Columbus, OH 43210 USA.
 94 Ohio State Univ, Dept Astron, Columbus, OH 43210 USA.
 95 Ohio State Univ, Dept Astron, Columbus, OH 43210 USA.
 96 Chungbuk Natl Univ, Inst Astrophys, Dept Phys, Chonju 371763, South Korea.
 97 Korea Astron & Space Sci Inst, Taejon 305348, South Korea.
 98 Korea Astron & Space Sci Inst, Taejon 305348, South Korea.
 99 Ctr Backyard Astrophys, Farm Cove Observ, Auckland, New Zealand.
100 Ohio State Univ, Dept Astron, Columbus, OH 43210 USA.
101 Univ Valencia, Dept Astron & Astrofis, E-46100 Valencia, Spain.
102 Auckland Observ, Auckland 1023, New Zealand.; AUT Univ, Inst Radiophys & Space Res, Auckland, New Zealand.
103 Auckland Observ, Auckland 1023, New Zealand.
104 Chungbuk Natl Univ, Inst Astrophys, Dept Phys, Chonju 371763, South Korea.
105 Ohio State Univ, Dept Astron, Columbus, OH 43210 USA.
106 Chungbuk Natl Univ, Inst Astrophys, Dept Phys, Chonju 371763, South Korea.
107 Ohio State Univ, Dept Astron, Columbus, OH 43210 USA.
108 Univ Canterbury, Dept Phys & Astron, Christchurch 8020, New Zealand.
109 Univ Toulouse, UPS OMP, IRAP, F-31400 Toulouse, France.; CNRS, IRAP, F-31400 Toulouse, France.
110 UPMC CNRS, UMR7095, Inst Astrophys Paris, F-75014 Paris, France.
111 ESO, Santiago 19, Chile.
112 McDonald Observ, Ft Davis, TX 79734 USA.
113 UPMC CNRS, UMR7095, Inst Astrophys Paris, F-75014 Paris, France.
114 Univ Tasmania, Sch Math & Phys, Gpo Hobart, Tas 7001, Australia.
115 UPMC CNRS, UMR7095, Inst Astrophys Paris, F-75014 Paris, France.
116 UPMC CNRS, UMR7095, Inst Astrophys Paris, F-75014 Paris, France.
117 Univ Toulouse, UPS OMP, IRAP, F-31400 Toulouse, France.
118 Univ Rijeka, Fac Arts & Sci, Dept Phys, Rijeka 51000, Croatia.
119 Vienna Univ Technol, Dept Comp, A-1060 Vienna, Austria.
120 Univ Toulouse, UPS OMP, IRAP, F-31400 Toulouse, France.; CNRS, IRAP, F-31400 Toulouse, France.
121 Univ Tasmania, Sch Math & Phys, Gpo Hobart, Tas 7001, Australia.
122 CALTECH, NASA Exoplanet Sci Inst, Pasadena, CA 91125 USA.
123 ESO, Santiago 19, Chile.; UPMC CNRS, UMR7095, Inst Astrophys Paris, F-75014 Paris, France.
124 UPMC CNRS, UMR7095, Inst Astrophys Paris, F-75014 Paris, France.
125 Perth Observ, Perth, WA 6076, Australia.
126 Univ Free State, Fac Nat & Agr Sci, Dept Phys, ZA-9300 Bloemfontein, South Africa.
127 S African Astron Observ, ZA-7935 Observatory, South Africa.
128 Univ Canterbury, Dept Phys & Astron, Christchurch 8020, New Zealand.
129 Univ Heidelberg ZAH, Zentrum Astron, Astron Rechen Inst, D-69120 Heidelberg, Germany.
130 UPMC CNRS, UMR7095, Inst Astrophys Paris, F-75014 Paris, France.
131 Univ Heidelberg ZAH, Zentrum Astron, Astron Rechen Inst, D-69120 Heidelberg, Germany.
Endereço de e-Mail do Autor  1
  2
  3
  4
  5
  6
  7 chico@das.inpe.br
Endereço de e-Mailmarcelo.pazos@inpe.br
RevistaAstronomy & Astrophysics
Volume552
Histórico (UTC)2018-06-04 03:14:14 :: administrator -> marcelo.pazos@inpe.br :: 2013
3. Conteúdo e estrutura
É a matriz ou uma cópia?é a matriz
Estágio do Conteúdoconcluido
Transferível1
Tipo do ConteúdoExternal Contribution
Palavras-Chavegravitational lensing: weak
planets and satellites: detection
planetary systems
Galaxy: bulge
ResumoAims. 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 two masses with a mass ratio q = 1.9 x 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 M-J orbiting an M dwarf host star with a mass of 0.26 +/- 0.11 M-circle dot. 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 similar to 1-1.5 AU.
ÁreaCEA
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Arquivo Alvo1303.1184v1.pdf
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1. Identificação
Tipo de ReferênciaArtigo em Revista Científica (Journal Article)
Siteplutao.sid.inpe.br
Código do Detentorisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
IdentificadorJ8LNKAN8RW/3D543J5
Repositóriodpi.inpe.br/plutao/2012/11.28.18.48.39
Última Atualização2013:01.28.16.08.52 (UTC) administrator
Repositório de Metadadosdpi.inpe.br/plutao/2012/11.28.18.48.40
Última Atualização dos Metadados2018:06.05.00.02.12 (UTC) administrator
Chave SecundáriaINPE--PRE/
DOI10.1088/0004-637X/755/2/102
ISSN0004-637X
1538-4357
Rótulolattes: 7812463045514059 45 YeeSGBUKHGSSABBCFFFIKLMMMMOORSSSSSTTWSKPSPUWPAABBCDDDFGGHHJKMMMMMMMNNOPSTTSCPLK:2012:TEPUSU
Chave de CitaçãoYeeSGBUKHGSSABBCFFFIKLMMMMOORSSSSSTTWSKPSPUWPAABBCDDDFGGHHJKMMMMMMMNNOPSTTSCPLK:2012:TePuSu
TítuloMOA-2011-BLG-293Lb: A test of pure survey microlensing planet detections
Ano2012
MêsAug.
Data de Acesso26 abr. 2024
Tipo SecundárioPRE PI
Número de Arquivos1
Tamanho872 KiB
2. Contextualização
Autor 1 Yee, J. C.
 2 Shvartzvald, Y.
 3 Gal-Yam, A.
 4 Bond, I. A.
 5 Udalski, A.
 6 Koz owski, S.
 7 Han, C.
 8 Gould, A.
 9 Skowron, J.
10 Suzuki, D.
11 Abe, F.
12 Bennett, D. P.
13 Botzler, C. S.
14 Chote, P.
15 Freeman, M.
16 Fukui, A.
17 Furusawa, K.
18 Itow, Y.
19 Kobara, S.
20 Ling, C. H.
21 Masuda, K.
22 Matsubara, Y.
23 Miyake, N.
24 Muraki, Y.
25 Ohmori, K.
26 Ohnishi, K.
27 Rattenbury, N. J.
28 Saito, To.
29 Sullivan, D. J.
30 Sumi, T.
31 Suzuki, K.
32 Sweatman, W. L.
33 Takino, S.
34 Tristram, P. J.
35 Wada, K.
36 Szyma ski, M. K.
37 Kubiak, M.
38 Pietrzy ski, G.
39 Soszy ski, I.
40 Poleski, R.
41 Ulaczyk, K.
42 Wyrzykowski, .
43 Pietrukowicz, P.
44 Allen, W.
45 Almeida, Leonardo Andrade de
46 Batista, V.
47 Bos, M.
48 Christie, G.
49 Depoy, D. L.
50 Dong, Subo
51 Drummond, J.
52 Finkelman, I.
53 Gaudi, B. S.
54 Gorbikov, E.
55 Henderson, C.
56 Higgins, D.
57 Jablonski, Francisco
58 Kaspi, S.
59 Manulis, I.
60 Maoz, D.
61 McCormick, J.
62 McGregor, D.
63 Monard, L. A. G.
64 Moorhouse, D.
65 Muñoz, J. A.
66 Natusch, T.
67 Ngan, H.
68 Ofek, E.
69 Pogge, R. W.
70 Santallo, R.
71 Tan, T. -G.
72 Thornley, G.
73 Shin, I. -G.
74 Choi, J. -Y.
75 Park, S. -Y.
76 Lee, C. -U.
77 Koo, J. -R.
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Endereço de e-Mail do Autor 1
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45 leonardo@das.inpe.br
Endereço de e-Mailleonardo@das.inpe.br
RevistaAstrophysical Journal
Volume755
Número2
Páginas102 (14 pp)
Nota SecundáriaA1_ASTRONOMIA_/_FÍSICA A2_ENGENHARIAS_IV A1_GEOCIÊNCIAS
Histórico (UTC)2012-11-28 23:06:34 :: lattes -> administrator :: 2012
2012-11-30 02:02:19 :: administrator -> marciana :: 2012
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3. Conteúdo e estrutura
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Estágio do Conteúdoconcluido
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Tipo do ConteúdoExternal Contribution
Tipo de Versãopublisher
Palavras-Chavegravitational microlensing
detection
individual (MOA-2011-BLG-293Lb) Jovian-Mass planet
galactic bulge
event MOA-2007-BLG-192
dwarf stars
photometry
systems
lens
companions
frequency
jupiter
ResumoBecause of the development of large-format, wide-field cameras, microlensing surveys are now able to monitor millions of stars with sufficient cadence to detect planets. These new discoveries will span the full range of significance levels including planetary signals too small to be distinguished from the noise. At present, we do not understand where the threshold is for detecting planets. MOA-2011-BLG-293Lb is the first planet to be published from the new surveys, and it also has substantial follow-up observations. This planet is robustly detected in survey+follow-up data (Delta chi(2) similar to 5400). The planet/host mass ratio is q = (5.3 similar to 0.2) x 10(-3). The best-fit projected separation is s = 0.548 +/- 0.005 Einstein radii. However, due to the s <-> s(-1) degeneracy, projected separations of s-1 are only marginally disfavored at Delta chi(2) = 3. A Bayesian estimate of the host mass gives M-L = 0.43(-0.17)(+0.27) M-circle dot, with a sharp upper limit of M-L < 1.2 M-circle dot from upper limits on the lens flux. Hence, the planet mass is m(p) = 2.4(-0.9)(+1.5) M-Jup, and the physical projected separation is either r(perpendicular to) similar or equal to 1.0 AU or r(perpendicular to) similar or equal to 3.4 AU. We show that survey data alone predict this solution and are able to characterize the planet, but the Delta chi(2) is much smaller (Delta chi(2) similar to 500) than with the follow-up data. The Delta chi(2) for the survey data alone is smaller than for any other securely detected planet. This event suggests a means to probe the detection threshold, by analyzing a large sample of events like MOA-2011-BLG-293, which have both follow-up data and high-cadence survey data, to provide a guide for the interpretation of pure survey microlensing data.
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Arquivo Alvo0004-637X_755_2_102.pdf
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DivulgaçãoWEBSCI; PORTALCAPES; MGA; COMPENDEX.
Acervo Hospedeirodpi.inpe.br/plutao@80/2008/08.19.15.01
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Campos Vaziosalternatejournal archivist callnumber copyholder copyright creatorhistory descriptionlevel format isbn lineage mark mirrorrepository nextedition notes orcid parameterlist parentrepositories previousedition previouslowerunit progress project readergroup resumeid rightsholder schedulinginformation secondarydate session shorttitle sponsor subject tertiarymark tertiarytype typeofwork url
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1. Identificação
Tipo de ReferênciaArtigo em Revista Científica (Journal Article)
Siteplutao.sid.inpe.br
Código do Detentorisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
IdentificadorJ8LNKAN8RW/3D543HU
Repositóriodpi.inpe.br/plutao/2012/11.28.18.48.35
Última Atualização2013:01.17.13.36.10 (UTC) administrator
Repositório de Metadadosdpi.inpe.br/plutao/2012/11.28.18.48.36
Última Atualização dos Metadados2018:06.05.00.02.12 (UTC) administrator
Chave SecundáriaINPE--PRE/
DOI10.1088/0004-637X/754/1/73
ISSN0004-637X
1538-4357
Rótulolattes: 7812463045514059 41 BacheletSHFGMBBBDHMMSSSUAAAABBBCCCCDDDGGHHHHJJKA:2012:COMAMI
Chave de CitaçãoBacheletSHFGMBBBDHMMSSSUAAAABBBCCCCDDDGGHHHHJJKAJ:2012:COMAMI
TítuloMOA 2010-BLG-477Lb: CONSTRAINING THE MASS OF A MICROLENSING PLANET FROM MICROLENSING PARALLAX, ORBITAL MOTION, AND DETECTION OF BLENDED LIGHT
ProjetoNational Research Foundation of Korea [2009-0081561]; MOA [JSPS20340052, JSPS22403003]; Czech Science Foundation [GACR P209/10/1318]; French Polar Institute (IPEV); European Research Council under the European Community's Seventh Framework Programme/ERC [246678]; CALMIP [2011-P1131]; NSF [AST-1103471, 2009068160]; NASA [NNG04GL51G]; KRCF Young Scientist Research Fellowship Program in South Korea; ANR; CNRS; Observatoire de la Cote d'Azur; California Institute of Technology (Caltech); NASA; ANR HOLMES; ANR PNPS
Ano2012
MêsJuly
Data de Acesso26 abr. 2024
Tipo SecundárioPRE PI
Número de Arquivos1
Tamanho2154 KiB
2. Contextualização
Autor 1 Bachelet, E.
 2 Shin, I. -G.
 3 Han, C.
 4 Fouqué, P.
 5 Gould, A.
 6 Menzies, J. W.
 7 Beaulieu, J. -P.
 8 Bennett, D. P.
 9 Bond, I. A.
10 Dong, Subo
11 Heyrovsk, D.
12 Marquette, J. -B.
13 Marshall, J.
14 Skowron, J.
15 Street, R. A.
16 Sumi, T.
17 Udalski, A.
18 Abe, L.
19 Agabi, K.
20 Albrow, M. D.
21 Allen, W.
22 Bertin, E.
23 Bos, M.
24 Bramich, D. M.
25 Chavez, J.
26 Christie, G. W.
27 Cole, A. A.
28 Crouzet, N.
29 Dieters, S.
30 Dominik, M.
31 Drummond, J.
32 Greenhill, J.
33 Guillot, T.
34 Henderson, C. B.
35 Hessman, F. V.
36 Horne, K.
37 Hundertmark, M.
38 Johnson, J. A.
39 Jrgensen, U. G.
40 Kandori, R.
41 Almeida, Leonardo Andrade
42 Jablonski, F.
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Afiliação 1 IRAP, Université de Toulouse, CNRS, 14 Avenue Edouard Belin, 31400 Toulouse, France
 2 Department of Physics, Chungbuk National University, Cheongju 361-763, Republic of Korea
 3 Department of Physics, Chungbuk National University, Cheongju 361-763, Republic of Korea
 4 IRAP, Université de Toulouse, CNRS, 14 Avenue Edouard Belin, 31400 Toulouse, France
 5 Department of Astronomy, Ohio State University, 140 West 18th Avenue, Columbus, OH 43210, USA
 6 South African Astronomical Observatory, P.O. Box 9, Observatory 7925, South Africa
 7 UPMC-CNRS, UMR 7095, Institut d'Astrophysique de Paris, 98bis boulevard Arago, F-75014 Paris, France
 8 Department of Physics, 225 Nieuwland Science Hall, University of Notre Dame, Notre Dame, IN 46556, USA
 9 Institute for Information and Mathematical Sciences, Massey University, Private Bag 102-904, Auckland 1330, New Zealand
10 Institute for Advanced Study, Einstein Drive, Princeton, NJ 08540, USA
11 Institute of Theoretical Physics, Charles University, V Holešovičkách 2, 18000 Prague, Czech Republic
12 UPMC-CNRS, UMR 7095, Institut d'Astrophysique de Paris, 98bis boulevard Arago, F-75014 Paris, France
13 Department of Astronomy, Ohio State University, 140 West 18th Avenue, Columbus, OH 43210, USA
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42 Instituto Nacional de Pesquisas Espaciais (INPE)
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41 leonardo@das.inpe.br
Endereço de e-Mailleonardo@das.inpe.br
RevistaAstrophysical Journal
Volume754
Número1
Páginas73
Nota SecundáriaA1_ASTRONOMIA_/_FÍSICA A2_ENGENHARIAS_IV A1_GEOCIÊNCIAS
Histórico (UTC)2012-11-28 23:06:34 :: lattes -> administrator :: 2012
2012-11-30 03:42:16 :: administrator -> marciana :: 2012
2013-02-01 10:18:42 :: marciana -> administrator :: 2012
2018-06-05 00:02:12 :: administrator -> marciana :: 2012
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
ResumoMicrolensing detections of cool planets are important for the construction of an unbiased sample to estimate the frequency of planets beyond the snow line, which is where giant planets are thought to form according to the core accretion theory of planet formation. In this paper, we report the discovery of a giant planet detected from the analysis of the light curve of a high-magnification microlensing event MOA 2010-BLG-477. The measured planet-star mass ratio is q = (2.181 +/- 0.004) x 10(-3) and the projected separation is s = 1.1228 +/- 0.0006 in units of the Einstein radius. The angular Einstein radius is unusually large theta(E) = 1.38 +/- 0.11 mas. Combining this measurement with constraints on the "microlens parallax" and the lens flux, we can only limit the host mass to the range 0.13 < M/M-circle dot < 1.0. In this particular case, the strong degeneracy between microlensing parallax and planet orbital motion prevents us from measuring more accurate host and planet masses. However, we find that adding Bayesian priors from two effects (Galactic model and Keplerian orbit) each independently favors the upper end of this mass range, yielding star and planet masses of M-* = 0.67(-0.13)(+0.33) M-circle dot and m(p) = 1.5(-0.3)(+0.8) M-JUP at a distance of D = 2.3 +/- 0.6 kpc, and with a semi-major axis of a = 2(-1)(+3) AU. Finally, we show that the lens mass can be determined from future high-resolution near-IR adaptive optics observations independently from two effects, photometric and astrometric.
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URL dos dados zipadoshttp://urlib.net/zip/J8LNKAN8RW/3D543HU
Idiomapt
Arquivo Alvo0004-637X_754_1_73.pdf
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Visibilidadeshown
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5. Fontes relacionadas
Unidades Imediatamente Superiores8JMKD3MGPCW/3ETR8EH
DivulgaçãoWEBSCI; PORTALCAPES; MGA; COMPENDEX.
Acervo Hospedeirodpi.inpe.br/plutao@80/2008/08.19.15.01
6. Notas
Campos Vaziosalternatejournal archivist callnumber copyholder copyright creatorhistory descriptionlevel format isbn lineage mark mirrorrepository nextedition notes orcid parameterlist parentrepositories previousedition previouslowerunit progress resumeid rightsholder schedulinginformation secondarydate session shorttitle sponsor subject tertiarymark tertiarytype typeofwork url
7. Controle da descrição
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1. Identificação
Tipo de ReferênciaArtigo em Revista Científica (Journal Article)
Siteplutao.sid.inpe.br
Código do Detentorisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
IdentificadorJ8LNKAN8RW/3E8265S
Repositóriodpi.inpe.br/plutao/2013/05.31.21.04   (acesso restrito)
Última Atualização2013:07.05.12.31.16 (UTC) administrator
Repositório de Metadadosdpi.inpe.br/plutao/2013/05.31.21.04.15
Última Atualização dos Metadados2018:06.04.23.39.11 (UTC) administrator
DOI10.1088/2041-8205/762/2/L28
ISSN2041-8205
2041-8213
Rótulolattes: 5605590098640584 26 HanAUCYGCTSKSPPUPKSWABDDDGHJJLKMMNNPPPS:2013:OGCPA
Chave de CitaçãoHanUCYGCTSKSPPUPKSWABDDDGHJJLKMMNNPPPS:2013:OGC—Pa
TítuloThe second multiple-planet system discovered by microlensing: OGLE-2012-BLG-0026Lb, c—A pair of jovian planets beyond the snow line
Ano2013
Data de Acesso26 abr. 2024
Tipo de Trabalhojournal article
Tipo SecundárioPRE PI
Número de Arquivos1
Tamanho699 KiB
2. Contextualização
Autor 1 Han, C.
 2 Udalski, A.
 3 Choi, J. -Y.
 4 Yee, J. C.
 5 Gould, A.
 6 Christie, G.
 7 Tan, T. -G.
 8 Szymanski, M. K.
 9 Kubiak, M.
10 Soszynski, I.
11 Pietrzy ski, G.
12 Poleski, R.
13 Ulaczyk, K.
14 Pietrukowicz, P.
15 Kozowski, S.
16 Skowron, J.
17 Wyrzykowski, L.
18 Almeida, Leonardo Andrade de
19 Batista, V.
20 Depoy, D. L.
21 Dong, S.
22 Drummond, J.
23 Gaudi, B. S.
24 Hwang, K. -H
25 Jablonski, Francisco Jose
26 Jung, Y. -K.
27 Lee, C. -U.
28 Koo, J. -R.
29 McCormick, J.
30 Monard, L. A. G.
31 Natusch, T.
32 Ngan, H.
33 Park, H.
34 Pogge, R. W.
35 Porritt, Ian
36 Shin, I. -G.
Identificador de Curriculo 1
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Afiliação 1
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18 Instituto Nacional de Pesquisas Espaciais (INPE)
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25 Instituto Nacional de Pesquisas Espaciais (INPE)
26 Chungbuk Natl Univ, Inst Astrophys, Dept Phys, Cheongju 371763, South Korea.
Endereço de e-Mail do Autor 1
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18 leonardodealmeida.andrade@gmail.com
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25 chico@das.inpe.br
Endereço de e-Mailchico@das.inpe.br
RevistaAstrophysical Journal Letters
Volume762
Número2
PáginasL28
Histórico (UTC)2013-05-31 21:57:05 :: lattes -> administrator :: 2013
2018-06-04 23:39:11 :: administrator -> :: 2013
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
planetary systems
snow line
ResumoWe report the discovery of a planetary system from observation of the high-magnification microlensing event OGLE-2012-BLG-0026. The lensing light curve exhibits a complex central perturbation with multiple features. We find that the perturbation was produced by two planets located near the Einstein ring of the planet host star. We identify four possible solutions resulting from the well-known close/wide degeneracy. By measuring both the lens parallax and the Einstein radius, we estimate the physical parameters of the planetary system. According to the best-fit model, the two planet masses are ~0.11MJ and 0.68MJ and they are orbiting a G-type main-sequence star with a mass ~0.82M. The projected separations of the individual planets are beyond the snow line in all four solutions, being ~3.8AU and 4.6AU in the best-fit solution. The deprojected separations are both individually larger and possibly reversed in order. This is the second multi-planet system with both planets beyond the snow line discovered by microlensing. This is the only such system (other than the solar system) with measured planet masses without sin i degeneracy. The planetary system is located at a distance 4.1 kpc from the Earth toward the Galactic center. It is very likely that extra light from stars other than the lensed star comes from the lens itself. If this is correct, it will be possible to obtain detailed information about the planet host star from follow-up observation.
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VinculaçãoTrabalho Vinculado à Tese/Dissertação
Repositório Espelhoiconet.com.br/banon/2006/11.26.21.31
Unidades Imediatamente Superiores8JMKD3MGPCW/3ETR8EH
URL (dados não confiáveis)http://iopscience.iop.org/2041-8205/762/2/L28/
DivulgaçãoWEBSCI; PORTALCAPES; SCOPUS.
Acervo Hospedeirodpi.inpe.br/plutao@80/2008/08.19.15.01
6. Notas
Campos Vaziosalternatejournal archivist callnumber copyholder copyright creatorhistory descriptionlevel format isbn lineage mark month nextedition notes orcid parameterlist parentrepositories previousedition previouslowerunit progress project rightsholder schedulinginformation secondarydate secondarykey secondarymark session shorttitle sponsor subject tertiarytype

1. Identificação
Tipo de ReferênciaArtigo em Revista Científica (Journal Article)
Sitemtc-m21b.sid.inpe.br
Código do Detentorisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identificador8JMKD3MGP3W34P/3KMH8S8
Repositóriosid.inpe.br/mtc-m21b/2015/12.01.15.46
Última Atualização2015:12.01.15.50.54 (UTC) administrator
Repositório de Metadadossid.inpe.br/mtc-m21b/2015/12.01.15.46.11
Última Atualização dos Metadados2018:06.04.02.55.54 (UTC) administrator
DOI10.1088/0004-637X/812/2/136
ISSN0004-637X
1538-4357
Chave de CitaçãoBacheletBHGSGDADJHHKSSTABBBBCCCCDPDFHMMPRWWACDDHHJJKKLMMNPPPSSYABBBFFIKLMMMOPRSSSSTYBCCGGHHJJKMMPPRRSSSSSSWW:2015:ReNoVe
TítuloRed noise versus planetary interpretations in the microlensing event ogle-2013-BLG-446
Ano2015
MêsOct.
Data de Acesso26 abr. 2024
Tipo de Trabalhojournal article
Tipo SecundárioPRE PI
Número de Arquivos1
Tamanho1296 KiB
2. Contextualização
Autor  1 Bachelet, E.
  2 Bramich, D. M.
  3 Han, C.
  4 Greenhill, J.
  5 Street, R. A.
  6 Gould, A.
  7 D'Ago, G.
  8 Alsubai, K.
  9 Dominik, M.
 10 Jaimes, R. F.
 11 Horne, K.
 12 Hundertmark, M.
 13 Kains, N.
 14 Snodgrass, C.
 15 Steele, I. A.
 16 Tsapras, Y.
 17 Albrow, M. D.
 18 Batista, V.
 19 Beaulieu, J. -P.
 20 Bennett, D. P.
 21 Brillant, S.
 22 Caldwell, J. A. R.
 23 Cassan, A.
 24 Cole, A.
 25 Coutures, C.
 26 Dieters, S.
 27 Prester, D. D.
 28 Donatowicz, J.
 29 Fouqué, P.
 30 Hill, K.
 31 Marquette, J. -B.
 32 Menzies, J.
 33 Pere, C.
 34 Ranc, C.
 35 Wambsganss, J.
 36 Warren, D.
 37 Almeida, Leonardo Andrade de
 38 Choi, J. -Y.
 39 Depoy, D. L.
 40 Dong, S.
 41 Hung, L. -W.
 42 Hwang, K. -H.
 43 Jablonski, Francisco José
 44 Jung, Y. K.
 45 Kaspi, S.
 46 Klein, N.
 47 Lee, C. -U.
 48 Maoz, D.
 49 Muñoz, José Antonio
 50 Nataf, D.
 51 Park, H.
 52 Pogge, R. W.
 53 Polishook, D.
 54 Shin, I. -G.
 55 Shporer, A.
 56 Yee, J. C.
 57 Abe, F.
 58 Bhattacharya, A.
 59 Bond, I. A.
 60 Botzler, C. S.
 61 Freeman, M.
 62 Fukui, A.
 63 Itow, Y.
 64 Koshimoto, N.
 65 Ling, C. H.
 66 Masuda, K.
 67 Matsubara, Y.
 68 Muraki, Y.
 69 Ohnishi, K.
 70 Philpott, L. C.
 71 Rattenbury, N.
 72 Saito, T.
 73 Sullivan, D. J.
 74 Sumi, T.
 75 Suzuki, D.
 76 Tristram, P. J.
 77 Yonehara, A.
 78 Bozza, V.
 79 Calchi Novati, S.
 80 Ciceri, S.
 81 Galianni, P.
 82 Gu, S. -H.
 83 Harpsøe, K.
 84 Hinse, T. C.
 85 Jørgensen, U. G.
 86 Juncher, D.
 87 Korhonen, H.
 88 Mancini, L.
 89 Melchiorre, C.
 90 Popovas, A.
 91 Postiglione, A.
 92 Rabus, M.
 93 Rahvar, S.
 94 Schmidt, R. W.
 95 Scarpetta, G.
 96 Skottfelt, J.
 97 Southworth, J.
 98 Stabile, A.
 99 Surdej, J.
100 Wang, X. -B.
101 Wertz, O.
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 49 Instituto Nacional de Pesquisas Espaciais (INPE)
Endereço de e-Mail do Autor  1
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RevistaAstrophysical Journal
Volume812
Número2
Páginas136
Histórico (UTC)2015-12-01 15:46:11 :: simone -> administrator ::
2018-06-04 02:55:54 :: 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
techniques: photometric
ResumoFor all exoplanet candidates, the reliability of a claimed detection needs to be assessed through a careful study of systematic errors in the data to minimize the false positives rate. We present a method to investigate such systematics in microlensing data sets using the microlensing event OGLE-2013-BLG-0446 as a case study. The event was observed from multiple sites around the world and its high magnification (Amax ∼ 3000) allowed us to investigate the effects of terrestrial and annual parallax. Real-time modeling of the event while it was still ongoing suggested the presence of an extremely low-mass companion (∼3M) to the lensing star, leading to substantial follow-up coverage of the light curve. We test and compare different models for the light curve and conclude that the data do not favor the planetary interpretation when systematic errors are taken into account.
ÁreaCEA
Arranjourlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAS > Red noise versus...
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4. Condições de acesso e uso
URL dos dadoshttp://urlib.net/ibi/8JMKD3MGP3W34P/3KMH8S8
URL dos dados zipadoshttp://urlib.net/zip/8JMKD3MGP3W34P/3KMH8S8
Idiomaen
Arquivo Alvo2015_bachelet.pdf
Grupo de Usuáriossimone
Grupo de Leitoresadministrator
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Visibilidadeshown
Política de Arquivamentoallowpublisher allowfinaldraft
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5. Fontes relacionadas
Repositório Espelhourlib.net/www/2011/03.29.20.55
Unidades Imediatamente Superiores8JMKD3MGPCW/3ETR8EH
Lista de Itens Citando
DivulgaçãoWEBSCI; PORTALCAPES; COMPENDEX; SCOPUS.
Acervo Hospedeirosid.inpe.br/mtc-m21b/2013/09.26.14.25.20
6. Notas
Campos Vaziosalternatejournal archivist callnumber copyholder copyright creatorhistory descriptionlevel e-mailaddress format isbn label lineage mark nextedition notes orcid parameterlist parentrepositories previousedition previouslowerunit progress project readpermission resumeid rightsholder schedulinginformation secondarydate secondarykey secondarymark session shorttitle sponsor subject tertiarymark tertiarytype url
7. Controle da descrição
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1. Identificação
Tipo de ReferênciaArtigo em Revista Científica (Journal Article)
Sitemtc-m21d.sid.inpe.br
Código do Detentorisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identificador8JMKD3MGP3W34T/47UCED8
Repositóriosid.inpe.br/mtc-m21d/2022/11.07.18.01   (acesso restrito)
Última Atualização2022:11.07.18.01.11 (UTC) simone
Repositório de Metadadossid.inpe.br/mtc-m21d/2022/11.07.18.01.11
Última Atualização dos Metadados2023:01.03.16.46.23 (UTC) administrator
DOI10.3390/sym14102001
ISSN2073-8994
Chave de CitaçãoAlmeidaJúniorGomePrad:2022:LiExOr
TítuloLifetimes of an Exomoon Orbiting a Jupiter-Like Planet in a Double Star System with the Mass of the Sun
Ano2022
MêsOct.
Data de Acesso26 abr. 2024
Tipo de Trabalhojournal article
Tipo SecundárioPRE PI
Número de Arquivos1
Tamanho11718 KiB
2. Contextualização
Autor1 Almeida Júnior, Allan Kardec de
2 Gomes, Vivian Martins
3 Prado, Antonio Fernando Bertachini de Almeida
Identificador de Curriculo1
2
3 8JMKD3MGP5W/3C9JGJA
ORCID1 0000-0002-9488-4462
Grupo1 CMC-ETES-DIPGR-INPE-MCTI-GOV-BR
2
3 DIMEC-CGCE-INPE-MCTI-GOV-BR
Afiliação1 Instituto Nacional de Pesquisas Espaciais (INPE)
2 Universidade Estadual Paulista (UNESP)
3 Instituto Nacional de Pesquisas Espaciais (INPE)
Endereço de e-Mail do Autor1 fenixcinza@yahoo.com.br
2
3 antonio.prado@inpe.br
RevistaSymmetry
Volume14
Número10
Páginase2001
Nota SecundáriaB4_CIÊNCIA_DA_COMPUTAÇÃO B5_MATEMÁTICA_/_PROBABILIDADE_E_ESTATÍSTICA
Histórico (UTC)2022-11-07 18:01:54 :: simone -> administrator :: 2022
2023-01-03 16:46:23 :: administrator -> simone :: 2022
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-Chavecelestial mechanics
exomoons
exoplanets
habitability zone
planetary evolution
ResumoThe search for life outside Earth has been a popular topic for a long time in the scientific literature, but it gained more possibilities with the discovery of planets around other stars besides our Sun. In this sense, similarly to what happens in our Solar System, moons of planets sometimes offer good conditions for life if stable orbits for those moons exist. Thus, the present paper analyzes a system composed of a moon (with the mass of the Earth) orbiting a planet (with the mass of Jupiter), which is orbiting a double star system (whose total mass is equal to the mass of the Sun). It is an important topic because there is a large proportion of double stars in the universe. The initial conditions are given by a symmetric configuration of two circular orbits. Although this symmetry is broken due to the four body dynamics, the conditions in which the moon remains bound with the planet are investigated. The stability of the system is given by the survival of the orbit of the moon for an integration time of the order of 10,000 revolutions of the satellite around its mother planet. The regions of stable, unstable, and collision orbits are mapped, and empirical linear equations that separate those regions are obtained from the maps.
ÁreaETES
Arranjo 1urlib.net > BDMCI > Fonds > Produção pgr ATUAIS > CMC > Lifetimes of an...
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4. Condições de acesso e uso
Idiomaen
Arquivo Alvosymmetry-14-02001-v2.pdf
Grupo de Usuáriossimone
Grupo de Leitoresadministrator
simone
Visibilidadeshown
Permissão de Leituradeny from all and allow from 150.163
Permissão de Atualizaçãonão transferida
5. Fontes relacionadas
Unidades Imediatamente Superiores8JMKD3MGPCW/3F2UALS
8JMKD3MGPCW/46KTFK8
Lista de Itens Citandosid.inpe.br/mtc-m21/2012/07.13.14.40.20 1
DivulgaçãoPORTALCAPES; SCOPUS.
Acervo Hospedeirourlib.net/www/2021/06.04.03.40
6. Notas
Campos Vaziosalternatejournal archivingpolicy archivist callnumber copyholder copyright creatorhistory descriptionlevel e-mailaddress format isbn label lineage mark mirrorrepository nextedition notes parameterlist parentrepositories previousedition previouslowerunit progress project rightsholder schedulinginformation secondarydate secondarykey session shorttitle sponsor subject tertiarymark tertiarytype url
7. Controle da descrição
e-Mail (login)simone
atualizar 

1. Identificação
Tipo de ReferênciaArtigo em Revista Científica (Journal Article)
Siteplutao.sid.inpe.br
Código do Detentorisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
IdentificadorJ8LNKAN8RW/3D543JD
Repositóriodpi.inpe.br/plutao/2012/11.28.18.48.47
Última Atualização2013:01.23.12.08.46 (UTC) administrator
Repositório de Metadadosdpi.inpe.br/plutao/2012/11.28.18.48.48
Última Atualização dos Metadados2018:06.05.00.02.12 (UTC) administrator
Chave SecundáriaINPE--PRE/
DOI10.1088/0004-637X/756/1/48
ISSN0004-637X
1538-4357
Rótulolattes: 7812463045514059 86 ChoiSHUSGBDFHSKSPPUPKSWABBBCFFFIKLMMMMOORSSSSSTTWYBSSSTABBCDDFGGHHHHHJJKKLLLMMPRRSSSSTWWABCDDGHJLMMMNNPTTYABBBCCCCDDDGKMMSZ:2012:NETYAM
Chave de CitaçãoChoiSHUSGBDFHSKSPPUPKSWABBBCFFFIKLMMMMOORSSSSSTTWYBSSSTABBCDDFGGHHHHHJJKKLLLMMPRRSSSSTWWABCDDGHJLMMMNNPTTYABBBCCCCDDDGKMMSZ:2012:NeTyAm
TítuloA new type of ambiguity in the planet and binary interpretations of central perturbations of high-magnification gravitational microlensing events
Ano2012
MêsSep.
Data de Acesso26 abr. 2024
Tipo SecundárioPRE PI
Número de Arquivos1
Tamanho2106 KiB
2. Contextualização
Autor  1 Choi, J. -Y.
  2 Shin, I. -G.
  3 Han, C.
  4 Udalski, A.
  5 Sumi, T.
  6 Gould, A.
  7 Bozza, V.
  8 Dominik, M.
  9 Fouqué, P.
 10 Horne, K.
 11 Szyma ski, M. K.
 12 Kubiak, M.
 13 Soszy ski, I.
 14 Pietrzy ski, G.
 15 Poleski, R.
 16 Ulaczyk, K.
 17 Pietrukowicz, P.
 18 Koz owski, S.
 19 Skowron, J.
 20 Wyrzykowski, .
 21 Abe, F.
 22 Bennett, D. P.
 23 Bond, I. A.
 24 Botzler, C. S.
 25 Chote, P.
 26 Freeman, M.
 27 Fukui, A.
 28 Furusawa, K.
 29 Itow, Y.
 30 Kobara, S.
 31 Ling, C. H.
 32 Masuda, K.
 33 Matsubara, Y.
 34 Miyake, N.
 35 Muraki, Y.
 36 Ohmori, K.
 37 Ohnishi, K.
 38 Rattenbury, N. J.
 39 Saito, To.
 40 Sullivan, D. J.
 41 Suzuki, D.
 42 Suzuki, K.
 43 Sweatman, W. L.
 44 Takino, S.
 45 Tristram, P. J.
 46 Wada, K.
 47 Yock, P. C. M.
 48 Bramich, D. M.
 49 Snodgrass, C.
 50 Steele, I. A.
 51 Street, R. A.
 52 Tsapras, Y.
 53 Alsubai, K. A.
 54 Browne, P.
 55 Burgdorf, M. J.
 56 Calchi Novati, S.
 57 Dodds, P.
 58 Dreizler, S.
 59 Fang, X. -S.
 60 Grundahl, F.
 61 Gu, C. -H.
 62 Hardis, S.
 63 Harps e, K.
 64 Hinse, T. C.
 65 Hornstrup, A.
 66 Hundertmark, M.
 67 Jessen-Hansen, J.
 68 J rgensen, U. G.
 69 Kains, N.
 70 Kerins, E.
 71 Liebig, C.
 72 Lund, M.
 73 Lunkkvist, M.
 74 Mancini, L.
 75 Mathiasen, M.
 76 Penny, M. T.
 77 Rahvar, S.
 78 Ricci, D.
 79 Scarpetta, G.
 80 Skottfelt, J.
 81 Southworth, J.
 82 Surdej, J.
 83 Tregloan-Reed, J.
 84 Wambsganss, J.
 85 Wertz, O.
 86 Almeida, Leonardo Andrade de
 87 Batista, V.
 88 Christie, G.
 89 Depoy, D. L.
 90 Dong, Subo
 91 Gaudi, B. S.
 92 Henderson, C.
 93 Jablonski, Francisco
 94 Lee, C. -U.
 95 McCormick, J.
 96 McGregor, D.
 97 Moorhouse, D.
 98 Natusch, T.
 99 Ngan, H.
100 Pogge, R. W.
101 Tan, T. -G.
102 Thornley, G.
103 Yee, J. C.
104 Albrow, M. D.
105 Bachelet, E.
106 Beaulieu, J. -P.
107 Brillant, S.
108 Cassan, A.
109 Cole, A. A.
110 Corrales, E.
111 Coutures, C.
112 Dieters, S.
113 Dominis Prester, D.
114 Donatowicz, J.
115 Greenhill, J.
116 Kubas, D.
117 Marquette, J. -B.
118 Menzies, J. W.
119 Sahu, K. C.
120 Zub, M.
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 86 Instituto Nacional de Pesquisas Espaciais (INPE)
Endereço de e-Mail do Autor  1
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 86 leonardo@das.inpe.br
Endereço de e-Mailleonardo@das.inpe.br
RevistaAstrophysical Journal
Volume756
Número1
Páginas48 (9pp)
Nota SecundáriaA1_ASTRONOMIA_/_FÍSICA A2_ENGENHARIAS_IV A1_GEOCIÊNCIAS
Histórico (UTC)2012-11-28 23:06:34 :: lattes -> marciana :: 2012
2012-12-05 17:56:24 :: marciana -> administrator :: 2012
2012-12-07 00:39:35 :: administrator -> marciana :: 2012
2013-02-01 10:17:42 :: marciana -> administrator :: 2012
2018-06-05 00:02:12 :: administrator -> marciana :: 2012
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-Chavegalactic bulge
gravitational microlensing
ResumoHigh-magnification microlensing events provide an important channel to detect planets. Perturbations near the peak of a high-magnification event can be produced either by a planet or a binary companion. It is known that central perturbations induced by both types of companions can be generally distinguished due to the essentially different magnification pattern around caustics. In this paper, we present a case of central perturbations for which it is difficult to distinguish the planetary and binary interpretations. The peak of a lensing light curve affected by this perturbation appears to be blunt and flat. For a planetary case, this perturbation occurs when the source trajectory passes the negative perturbation region behind the back end of an arrowhead-shaped central caustic. For a binary case, a similar perturbation occurs for a source trajectory passing through the negative perturbation region between two cusps of an astroid-shaped caustic. We demonstrate the degeneracy for two high-magnification events of OGLE-2011-BLG-0526 and OGLE-2011-BLG-0950/MOA-2011-BLG-336. For OGLE-2011-BLG-0526, the χ2 difference between the planetary and binary model is ∼3, implying that the degeneracy is very severe. For OGLE- 2011-BLG-0950/MOA-2011-BLG-336, the stellar binary model is formally excluded with Δχ2 ∼ 105 and the planetary model is preferred. However, it is difficult to claim a planet discovery because systematic residuals of data from the planetary model are larger than the difference between the planetary and binary models. Considering that two events observed during a single season suffer from such a degeneracy, it is expected that central perturbations experiencing this type of degeneracy is common.
ÁreaCEA
Arranjourlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAS > A new type...
Conteúdo da Pasta docacessar
Conteúdo da Pasta sourcenão têm arquivos
Conteúdo da Pasta agreementnão têm arquivos
4. Condições de acesso e uso
URL dos dadoshttp://urlib.net/ibi/J8LNKAN8RW/3D543JD
URL dos dados zipadoshttp://urlib.net/zip/J8LNKAN8RW/3D543JD
Idiomapt
Grupo de Usuáriosadministrator
lattes
marciana
Visibilidadeshown
Política de Arquivamentoallowpublisher allowfinaldraft
Permissão de Leituraallow from all
Permissão de Atualizaçãonão transferida
5. Fontes relacionadas
Unidades Imediatamente Superiores8JMKD3MGPCW/3ETR8EH
DivulgaçãoWEBSCI; PORTALCAPES; MGA; COMPENDEX.
Acervo Hospedeirodpi.inpe.br/plutao@80/2008/08.19.15.01
6. Notas
Campos Vaziosalternatejournal archivist callnumber copyholder copyright creatorhistory descriptionlevel format isbn lineage mark mirrorrepository nextedition notes orcid parameterlist parentrepositories previousedition previouslowerunit progress project readergroup resumeid rightsholder schedulinginformation secondarydate session shorttitle sponsor subject targetfile tertiarymark tertiarytype typeofwork url
7. Controle da descrição
e-Mail (login)marciana
atualizar