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| Verfasst von: | Janczak, Julia [VerfasserIn]  |
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| | Fukui, A. [VerfasserIn] |
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| | Dong, Subo [VerfasserIn] |
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| | Monard, L. A. G. [VerfasserIn] |
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| | Kozłowski, Szymon [VerfasserIn] |
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| | Gould, A. [VerfasserIn] |
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| | Beaulieu, J. P. [VerfasserIn] |
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| | Kubas, Daniel [VerfasserIn] |
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| | Marquette, J. B. [VerfasserIn] |
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| | Sumi, T. [VerfasserIn] |
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| | Bond, I. A. [VerfasserIn] |
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| | Bennett, D. P. [VerfasserIn] |
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| | Abe, F. [VerfasserIn] |
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| | Furusawa, K. [VerfasserIn] |
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| | Hearnshaw, J. B. [VerfasserIn] |
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| | Hosaka, S. [VerfasserIn] |
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| | Itow, Y. [VerfasserIn] |
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| | Kamiya, K. [VerfasserIn] |
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| | Korpela, A. V. [VerfasserIn] |
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| | Kilmartin, P. M. [VerfasserIn] |
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| | Lin, W. [VerfasserIn] |
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| | Ling, C. H. [VerfasserIn] |
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| | Makita, S. [VerfasserIn] |
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| | Masuda, K. [VerfasserIn] |
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| | Matsubara, Y. [VerfasserIn] |
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| | Miyake, N. [VerfasserIn] |
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| | Muraki, Y. [VerfasserIn] |
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| | Nagaya, M. [VerfasserIn] |
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| | Nagayama, T. [VerfasserIn] |
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| | Nishimoto, K. [VerfasserIn] |
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| | Ohnishi, K. [VerfasserIn] |
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| | Perrott, Y. C. [VerfasserIn] |
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| | Rattenbury, N. J. [VerfasserIn] |
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| | Sako, T. [VerfasserIn] |
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| | Saito, To [VerfasserIn] |
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| | Skuljan, L. [VerfasserIn] |
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| | Sullivan, D. J. [VerfasserIn] |
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| | Sweatman, W. L. [VerfasserIn] |
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| | Tristram, P. J. [VerfasserIn] |
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| | Yock, P. C. M. [VerfasserIn] |
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| | An, Jin H. [VerfasserIn] |
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| | Christie, G. W. [VerfasserIn] |
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| | Chung, Sun-Ju [VerfasserIn] |
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| | DePoy, D. L. [VerfasserIn] |
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| | Gaudi, B. S. [VerfasserIn] |
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| | Han, C. [VerfasserIn] |
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| | Lee, C.-U. [VerfasserIn] |
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| | Mallia, F. [VerfasserIn] |
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| | Natusch, T. [VerfasserIn] |
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| | Park, B.-G. [VerfasserIn] |
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| | Pogge, R. W. [VerfasserIn] |
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| | Anguita, Timo [VerfasserIn] |
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| | Novati, S. Calchi [VerfasserIn] |
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| | Dominik, M. [VerfasserIn] |
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| | Jørgensen, U. G. [VerfasserIn] |
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| | Masi, G. [VerfasserIn] |
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| | Mathiasen, M. [VerfasserIn] |
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| | Batista, V. [VerfasserIn] |
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| | Brillant, S. [VerfasserIn] |
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| | Cassan, Arnaud [VerfasserIn] |
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| | Cole, A. [VerfasserIn] |
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| | Corrales, E. [VerfasserIn] |
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| | Coutures, Ch [VerfasserIn] |
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| | Dieters, S. [VerfasserIn] |
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| | Fouqué, and P. [VerfasserIn] |
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| | Greenhill, J. [VerfasserIn] |
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| Titel: | Sub-Saturn Planet MOA-2008-BLG-310Lb |
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| Titelzusatz: | likely to be in the galactic bulge |
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| Verf.angabe: | Julia Janczak, A. Fukui, Subo Dong, L. A. G. Monard, Szymon Kozłowski, A. Gould, J. P. Beaulieu, Daniel Kubas, J. B. Marquette, T. Sumi, I. A. Bond, D. P. Bennett, F. Abe, K. Furusawa, J. B. Hearnshaw, S. Hosaka, Y. Itow, K. Kamiya, A. V. Korpela, P. M. Kilmartin, W. Lin, C. H. Ling, S. Makita, K. Masuda, Y. Matsubara, N. Miyake, Y. Muraki, M. Nagaya, T. Nagayama, K. Nishimoto, K. Ohnishi, Y. C. Perrott, N. J. Rattenbury, T. Sako, To Saito, L. Skuljan, D. J. Sullivan, W. L. Sweatman, P. J. Tristram, P. C. M. Yock, (The MOA Collaboration), Jin H. An, G. W. Christie, Sun-Ju Chung, D. L. DePoy, B. S. Gaudi, C. Han, C.-U. Lee, F. Mallia, T. Natusch, B.-G. Park, R. W. Pogge, (The [Mu]FUN Collaboration), T. Anguita, S. Calchi Novati, M. Dominik, U. G. Jørgensen, G. Masi, M. Mathiasen, (The MiNDSTEp Collaboration), V. Batista, S. Brillant, A. Cassan, A. Cole, E. Corrales, Ch Coutures, S. Dieters, and P. Fouqué, J. Greenhill, (The PLANET Collaboration) |
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| E-Jahr: | 2010 |
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| Jahr: | 2010 March 10 |
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| Umfang: | 13 S. |
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| Illustrationen: | Diagramme |
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| Fussnoten: | Gesehen am 14.07.2023 ; Das Mu in The [Mu]FUN Collaboration ist als griechischer Buchstabe dargestellt |
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| Titel Quelle: | Enthalten in: The astrophysical journal / 1 |
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| Ort Quelle: | London : Institute of Physics Publ., 1995 |
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| Jahr Quelle: | 2010 |
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| Band/Heft Quelle: | 711(2010), 2 vom: März, Seite 731-743 |
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| ISSN Quelle: | 1538-4357 |
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| Abstract: | We report the detection of sub-Saturn-mass planet MOA-2008-BLG-310Lb and argue that it is the strongest candidate yet for a bulge planet. Deviations from the single-lens fit are smoothed out by finite-source effects and therefore are not immediately apparent from the light curve. Nevertheless, we find that a model in which the primary has a planetary companion is favored over the single-lens model by Δχ2 ∼ 880 for an additional 3 degrees of freedom. Detailed analysis yields a planet/star mass ratio q = (3.3 ± 0.3) × 10−4 and an angular separation between the planet and star within 10% of the angular Einstein radius. The small angular Einstein radius, θE = 0.155 ± 0.011 mas, constrains the distance to the lens to be DL>6.0 kpc if it is a star (ML>0.08 M☉). This is the only microlensing exoplanet host discovered so far that must be in the bulge if it is a star. By analyzing VLT NACO adaptive optics images taken near the baseline of the event, we detect additional blended light that is aligned to within 130 mas of the lensed source. This light is plausibly from the lens, but could also be due to a companion to the lens or source, or possibly an unassociated star. If the blended light is indeed due to the lens, we can estimate the mass of the lens, ML = 0.67 ± 0.14 M☉, planet mass m = 74 ± 17 M⊕, and projected separation between the planet and host, 1.25 ± 0.10 AU, putting it right on the “snow line.” If not, then the planet has lower mass, is closer to its host and is colder. To distinguish among these possibilities on reasonable timescales would require obtaining Hubble Space Telescope images almost immediately, before the source-lens relative motion of causes them to separate substantially. |
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| DOI: | doi:10.1088/0004-637X/711/2/731 |
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| URL: | Bitte beachten Sie: Dies ist ein Bibliographieeintrag. Ein Volltextzugriff für Mitglieder der Universität besteht hier nur, falls für die entsprechende Zeitschrift/den entsprechenden Sammelband ein Abonnement besteht oder es sich um einen OpenAccess-Titel handelt.
Volltext: https://doi.org/10.1088/0004-637X/711/2/731 |
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| | Volltext: https://dx.doi.org/10.1088/0004-637X/711/2/731 |
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| | DOI: https://doi.org/10.1088/0004-637X/711/2/731 |
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| Datenträger: | Online-Ressource |
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| Sprache: | eng |
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| K10plus-PPN: | 1852736208 |
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| Verknüpfungen: | → Zeitschrift |
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Sub-Saturn Planet MOA-2008-BLG-310Lb / Janczak, Julia [VerfasserIn]; 2010 March 10 (Online-Ressource)
