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• W3100785802 abstract "Aims. We conducted a multi-wavelength, multi-instrument observational characterisation of the candidate free-floating planet CFBDSIR J214947.2−040308.9, a late T-dwarf with possible low-gravity features, in order to constrain its physical properties. Methods. We analysed nine hours of X-shooter spectroscopy with signal detectable from 0.8 to 2.3 μ m, as well as additional photometry in the mid-infrared using the Spitzer Space Telescope. Combined with a VLT/HAWK-I astrometric parallax, this enabled a full characterisation of the absolute flux from the visible to 5 μ m, encompassing more than 90% of the expected energy emitted by such a cool late T-type object. Our analysis of the spectrum also provided the radial velocity and therefore the determination of its full 3D kinematics. Results. While our new spectrum confirms the low gravity and/or high metallicity of CFBDSIR 2149, the parallax and kinematics safely rule out membership to any known young moving group, including AB Doradus. We use the equivalent width of the K i doublet at 1.25 μ m as a promising tool to discriminate the effects of low-gravity from the effects of high-metallicity on the emission spectra of cool atmospheres. In the case of CFBDSIR 2149, the observed K i doublet clearly favours the low-gravity solution. Conclusions. CFBDSIR 2149 is therefore a peculiar late-T dwarf that is probably a young, planetary-mass object (2–13 M Jup , <500 Myr) possibly similar to the exoplanet 51 Eri b, or perhaps a 2–40 M Jup brown dwarf with super-solar metallicity." @default.
• W3100785802 created "2020-11-23" @default.
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• W3100785802 date "2017-06-01" @default.
• W3100785802 modified "2023-10-18" @default.
• W3100785802 title "CFBDSIR 2149-0403: young isolated planetary-mass object or high-metallicity low-mass brown dwarf?" @default.
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• W3100785802 cites W1980371628 @default.
• W3100785802 cites W1985663566 @default.
• W3100785802 cites W1997008272 @default.
• W3100785802 cites W2002156484 @default.
• W3100785802 cites W2010509088 @default.
• W3100785802 cites W2015097457 @default.
• W3100785802 cites W2020890029 @default.
• W3100785802 cites W2030663701 @default.
• W3100785802 cites W2033954023 @default.
• W3100785802 cites W2035525551 @default.
• W3100785802 cites W2074044119 @default.
• W3100785802 cites W2075779114 @default.
• W3100785802 cites W2077265829 @default.
• W3100785802 cites W2078792426 @default.
• W3100785802 cites W2082846968 @default.
• W3100785802 cites W2083456831 @default.
• W3100785802 cites W2090902729 @default.
• W3100785802 cites W2100833883 @default.
• W3100785802 cites W2106185107 @default.
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• W3100785802 cites W2111817932 @default.
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• W3100785802 cites W2113933657 @default.
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• W3100785802 cites W2114592647 @default.
• W3100785802 cites W2122941696 @default.
• W3100785802 cites W2127810294 @default.
• W3100785802 cites W2135655113 @default.
• W3100785802 cites W2136610436 @default.
• W3100785802 cites W2137802640 @default.
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• W3100785802 cites W2153696725 @default.
• W3100785802 cites W2171437022 @default.
• W3100785802 cites W2182323948 @default.
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• W3100785802 cites W2261573924 @default.
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• W3100785802 cites W3097996452 @default.
• W3100785802 cites W3098029385 @default.
• W3100785802 cites W3098283280 @default.
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• W3100785802 cites W3098704547 @default.
• W3100785802 cites W3098854266 @default.
• W3100785802 cites W3099295996 @default.
• W3100785802 cites W3099430025 @default.
• W3100785802 cites W3099504888 @default.
• W3100785802 cites W3099545547 @default.
• W3100785802 cites W3099926194 @default.
• W3100785802 cites W3100646721 @default.
• W3100785802 cites W3100706962 @default.
• W3100785802 cites W3100763381 @default.
• W3100785802 cites W3101303406 @default.
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• W3100785802 cites W3102938219 @default.
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• W3100785802 doi "https://doi.org/10.1051/0004-6361/201629633" @default.
• W3100785802 hasPublicationYear "2017" @default.
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