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11 - 13 of 13 search results for KaKaoTalk:ZA31 24 24 |u:people.ast.cam.ac.uk where 0 match all words and 13 match some words.

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  2. Quanz_et_al_ESA_white_paper_MIR_interferometry_revised

    https://people.ast.cam.ac.uk/~wyatt/qabb22.pdf
    22 Mar 2024: 1. Atmospheric characterization of terrestrial exoplanets in the mid-infrared: biosignatures, habitability, and diversity. Corresponding author: Sascha P. Quanz, ETH Zurich, Institute for Particle Physics and Astrophysics, Zurich, Switzerland Contact

  3. MNRAS 000, 1–17 (2033) Preprint 19 June 2023 Compiled ...

    https://people.ast.cam.ac.uk/~wyatt/tmbh23.pdf
    22 Mar 2024: M = H(q)𝑇 N1H(q), (23). j = H𝑇 N1V. (24). Finally, I𝑠 = 𝝁 is used as the inferred brightness. ... 2). (27). This change to H(q) is used in Equations 21–24 or when comput-ing the model visibilities (Equation 18), with the code

  4. MNRAS 000, 1–14 (2022) Preprint 18 January 2023 Compiled ...

    https://people.ast.cam.ac.uk/~wyatt/hwd22.pdf
    22 Mar 2024: MNRAS 000, 1–14 (2022) Preprint 18 January 2023 Compiled usingMNRASLATEXstyle file v3.0. Has the dust clump in the debris disk of Beta Pictoris moved? Y.Han,1 M.C.Wyatt,1 W.R. F.Dent,21Institute of Astronomy, University of Cambridge, Madingley Road

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