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  2. Draft version March 24, 2022Typeset using LATEX twocolumn style ...

    https://people.ast.cam.ac.uk/~wyatt/hycd22.pdf
    22 Mar 2024: 3.2. Polarized dust emission in the middle versus outerregions of β Pic. ... Thebox has dimensions of 12130 pixels, corresponding toa box size of 1.′′718.′′2 or 32.7 au354 au.Our first test is to analyze the middle half of the disk.

  3. M. Pettini: Structure and Evolution of Stars — Lecture ...

    https://people.ast.cam.ac.uk/~pettini/Stellar%20Structure%20Evolution/Lecture16.pdf
    24 Nov 2023: This is fundamental work, providing empirical tests ofour theories of stellar evolution for massive stars. ... Middle pair: SN2005cs in M51 ata distance of 7 Mpc. Bottom pair: SN2003gd in the face-on spiral galaxy M74 at adistance of 9 Mpc.

  4. MNRAS 000, 1–16 (2022) Preprint 6 July 2023 Compiled ...

    https://people.ast.cam.ac.uk/~wyatt/bwmd23.pdf
    11 Jul 2023: ted lines) at various epochs. The middle panel shows the volatilecontent of planetesimals as a function of diameter. ... order of magnitude.This is plausibly an important test of whether large planetes-imals.

  5. MNRAS 000, 1–24 (2023) Preprint 9 November 2023 Compiled ...

    https://people.ast.cam.ac.uk/~wyatt/pksj23.pdf
    22 Mar 2024: so we can test different initial surface-density profiles; weconsider initial surface-density profiles between 𝑟0 and 𝑟1.5.

  6. Inner edges of planetesimal belts: collisionally eroded or truncated?

    https://people.ast.cam.ac.uk/~wyatt/immb23.pdf
    20 Feb 2024: We use both parametric and non-parametric modelling to test if their inner edges are shallow and consistent with collisional evolution.

  7. Astronomy & Astrophysics manuscript no. SHARDDS ©ESO 2022August…

    https://people.ast.cam.ac.uk/~wyatt/dmac22.pdf
    22 Mar 2024: The PSO framework was chosen as it showed, during tests,a higher convergence rate than Bayesian optimisation and al-lowed multi-core estimation7, reducing the computation time.More standard minimisation frameworks

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