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  2. MNRAS 000, 1–22 (2019) Preprint 30 January 2020 Compiled ...

    https://people.ast.cam.ac.uk/~wyatt/mfhk20.pdf
    30 Jan 2020: Middle: high viscosity and high CO input rate. Bottom:low viscosity and high CO input rate. ... In the middle panels, the CO mass input rate is now 100times higher.
  3. 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.
  4. Mon. Not. R. Astron. Soc. 000, 1–8 (2016) Printed ...

    https://people.ast.cam.ac.uk/~wyatt/ghmm16.pdf
    21 Jul 2016: Middle:spectrum after subtracting the 3rd-order polynomial shown in red in the toppanel. ... 10 100. 1.0. 8. 6. 4. 2. 0. KS–Test Comparison Cumulative Fraction Plot.
  5. MNRAS 000, 1–19 (2015) Preprint 4 July 2018 Compiled ...

    https://people.ast.cam.ac.uk/~wyatt/mcwb18.pdf
    31 Jul 2018: The residuals of band 6 (middle row). and band 7 (12mACA, bottom row) are computed using natural.
  6. Draft version May 29, 2015Preprint typeset using LATEX style ...

    https://people.ast.cam.ac.uk/~wyatt/cwmm15.pdf
    14 Sep 2015: 2013; van der Marel et al. 2013; Pérez et al. 2014)could not test the trapping predictions. ... Top: cross-correlation before out-lier filtering. Middle: after outlier filtering, but before as-trometric WCS correction.
  7. MNRAS 000, 1-30 (2020) Preprint 12 October 2020 Compiled ...

    https://people.ast.cam.ac.uk/~wyatt/swmn20.pdf
    15 Oct 2020: 2017) as a test of its validity. The prescriptionpresented by Cataldi et al. ... For each test population, we calculate, using equations 9 11in Wyatt et al.
  8. arX iv:0 810. 5087 v1 [ astr o-ph ] ...

    https://people.ast.cam.ac.uk/~wyatt/scwm08.pdf
    3 Nov 2008: For eachmodel described below a range of parameters was tried and aχ2 goodness-of-fit test applied to find the best fitting parametersand confidence limits (errors from background statistical error).In ... To test whether more complicated models are
  9. arX iv:1 701. 0656 8v1 [as tro- ph.S R] ...

    https://people.ast.cam.ac.uk/~wyatt/kkpr17.pdf
    5 May 2017: By repeatingthis prescription for synthetic data we are able to test different scenarios for how the occultationsdo or do not repeat. ... We leave the development of a quantitative study of thisscenario for the future, noting that tests of such a model
  10. MNRAS 000, 1–15 (2020) Preprint 29April 2021 Compiled…

    https://people.ast.cam.ac.uk/~wyatt/ckkm21.pdf
    29 Apr 2021: To test this hypothesis S14 conduct N-body simulations withrandomly sampled initial separations and eccentricities of the ACbinary; B is generated at a random location within the Hill sphereof the system ... From examination of the residuals for this
  11. 11626.dvi

    https://people.ast.cam.ac.uk/~wyatt/swh09.pdf
    23 Jun 2009: This image acts as a PSF reference. Middle: The final image of HD69830. ... The residual image shows no evidencefor emission beyond the PSF. Further tests comparing the pro-files of the observations, Gaussian and Moffat profile fits to theimages and

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