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  2. DRAFT VERSION MAY 24, 2022Typeset using LATEX twocolumn style ...

    https://people.ast.cam.ac.uk/~wyatt/hcrs22.pdf
    24 May 2022: 2021a). In each setof figures, the left image shows the coronagraphic point spread function for each bandpass, while the middle and right panels show subsequentimage post-processing employing Angular Differential Imaging
  3. 14 Feb 2019: 2. The belt spine (Fig. 3, middle) presents little verti-. cal displacement along the midplane and is largely. ... Nonetheless, we test whether we can. detect a radial dependence of the vertical aspect ratio.
  4. https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_050916.txt

    https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_050916.txt
    22 Sep 2005: The only sensible long term (ie. economic) option is to use internet transfers. ... results. Further tests are still ongoing in conjunction with Omar Almaini the UDS PI.
  5. 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.
  6. arX iv:1 208. 1759 v1 [ astr o-ph .EP ...

    https://people.ast.cam.ac.uk/~wyatt/kwsp12.pdf
    9 Oct 2012: 33. 0.00. 1.33. 2.67. 4.00. Figure 6. Residuals after the resolved model ofα CrB is subtracted from the observations at 70µm (left) 100µm (middle) and 160µm (right). ... 1.33. 0.00. 1.33. 2.67. 4.00. Figure 8. Residuals after the resolved model ofβ
  7. Searching for Saturn's Irregular Satellite Swarm with Spitzer

    https://people.ast.cam.ac.uk/~wyatt/kwss11.pdf
    29 Jun 2012: Our aim here is to test this prediction for Saturn’s dustcloud using the 24µm Spitzer Space Telescope observationsused to discover the Phoebe ring. ... The ON scans are easily identifiable by thelarge bump in the middle due to the Phoebe ring.
  8. 29 Apr 2008: 2000)? Or are we witnessing the colli-sional destruction of massive asteroid belts or the sublimationof comets in the middle of fully formed planetary systems? ... show three different models:Top: Face-on, large radiusr; middle: Face-on small radiusr;
  9. Draft version April 5, 2018Typeset using LATEX twocolumn style ...

    https://people.ast.cam.ac.uk/~wyatt/mmkw18.pdf
    5 Apr 2018: We here test the hypothesis that these selection ef-. fects alone applied to a population uncorrelated in. ... vant for its formation, which depends on which theory. we are trying to test (see discussion in 4).
  10. vpfit10.4.dvi

    https://people.ast.cam.ac.uk/~rfc/vpfit10.4.pdf
    5 Oct 2016: 3. statistics for whole fit:. Runs test K-S test Chi-squared Chans ndf APr Xp(.68) Xp(.95) Xp(.99). ... Runs test K-S test Chi-squared Chans ndf APr Xp(.68) Xp(.95) Xp(.99).
  11. 20 Feb 2024: We use both parametric and non-parametric modelling to test if their inner edges are shallow and consistent with collisional evolution.

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