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  2. panstarrs.eps

    https://people.ast.cam.ac.uk/~wyatt/sjw19.pdf
    13 Mar 2019: In both Tack. cases, we do not simulate test particles beyond 14 au, but instead. ... the fraction of test particles that are ever members of the Oort cloud.
  3. 17 Jan 2019: in Figure 3. To further test this hypothesis, we simulated the response of the disc to perturbations from. ... simulations (see Methods). The main conclusion from the n-body simulations is that test particles.
  4. A planetesimal orbiting within the debris discaround a white ...

    https://people.ast.cam.ac.uk/~wyatt/mgeh19.pdf
    25 Apr 2019: Manual, http://pencil-code.nordita.org/doc/manual.pdf. 96. C. P. McNally, W. Lyra, J.-C. Passy, A Well-posed Kelvin-Helmholtz Instability Test and. ... S6 &. S7 can be found in the directory pencil-code/samples/2d-tests/WhiteDwarfDisk, using version.
  5. 1911.05131

    https://people.ast.cam.ac.uk/~wyatt/tw19.pdf
    20 Nov 2019: This new survey therefore presents a unique oppor-tunity to test prospective models statistically against a largesample. ... Instead, here we estimate a simple detec-tion threshold to test its significance.
  6. MNRAS 000, 1–21 (2018) Preprint 11 July 2019 Compiled ...

    https://people.ast.cam.ac.uk/~wyatt/yksw19.pdf
    11 Jul 2019: However, us-ing a Kolmogorov-Smirnov (KS) test, they demonstratedthat the period distributions of their disc-bearing anddisc-free binaries and multiples were not, in fact, differ-ent in a statistically
  7. 1906.08797

    https://people.ast.cam.ac.uk/~wyatt/smkb19.pdf
    20 Nov 2019: 4.3. Exploring Hypothetical Exoplanetary SystemArchitecture. Stars that host both a debris disk and one or more exo-planets serve as critical test beds for studying the forma-tion and evolution
  8. 14 Feb 2019: Nonetheless, we test whether we can. detect a radial dependence of the vertical aspect ratio. ... the two datasets do not allow us to test this hypothe-.
  9. Draft version April 2, 2019Typeset using LATEX twocolumn style ...

    https://people.ast.cam.ac.uk/~wyatt/dhcf19.pdf
    3 Apr 2019: Draft version April 2, 2019Typeset using LATEX twocolumn style in AASTeX62. The Mass of Stirring Bodies in the AU Mic Debris Disk Inferred from Resolved Vertical Structure. Cail Daley,1, 2 A. Meredith Hughes,1 Evan S. Carter,1 Kevin Flaherty,1, 3
  10. MNRAS 000, 000–000 (2018) Preprint 21 February 2019 Compiled ...

    https://people.ast.cam.ac.uk/~wyatt/mphp19.pdf
    21 Feb 2019: 5.3.2 Temperature Scenario. To test the possibility of temperature variation as the causeof asymmetry in the outer C18O disc, we measure the av-erage flux in different segments of
  11. MNRAS 000, 1–14 (2018) Preprint 8 January 2019 Compiled ...

    https://people.ast.cam.ac.uk/~wyatt/mybf19.pdf
    8 Jan 2019: This small difference in χ2 there-fore favours the SR model when compared against the fulleccentric disc model presented in 3 because it has fewerparameters (based on a χ2 difference test

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