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  2. MNRAS 000, 1–24 (2020) Preprint 2 July 2020 Compiled ...

    https://people.ast.cam.ac.uk/~wyatt/rw20.pdf
    2 Jul 2020: MNRAS 000, 1–24 (2020). 8 J. K. Rigley et al. Figure 2. ... MNRAS 000, 1–24 (2020). 10 J. K. Rigley et al. 10-18.
  3. MNRAS 000, 1–24 (2020) Preprint 7 July 2020 Compiled ...

    https://people.ast.cam.ac.uk/~wyatt/xw20.pdf
    7 Jul 2020: MNRAS 000, 1–24 (2020). Mutual inclination between π Men b and c 3. ... The. 1 https://gaia.esac.esa.int/gost/. MNRAS 000, 1–24 (2020).
  4. M. Pettini: Introduction to Cosmology — Lecture 15 CLUSTERS ...

    https://people.ast.cam.ac.uk/~pettini/Intro%20Cosmology/Lecture15.pdf
    28 Jun 2020: 15.24). The virial theorem for bound objects tells us that:. v2 =GM.
  5. The Dynamics of Scarlet Fever Epidemics in England and Wales in the…

    https://people.ast.cam.ac.uk/~vasily/data/scarlet.pdf
    18 Oct 2020: both in England in the 17th century [22] and in the Dutch hunger winter between September 1944 and May 1945 [24, 25]. ... London: Batsford Aca? demic, 1984: 79-101. 24. Stein Z, Susser M, Saenger G, Marolla F.
  6. MNRAS 000, 1–7 (2019) Preprint 28 January 2020 Compiled ...

    https://people.ast.cam.ac.uk/~wyatt/mwkk19.pdf
    28 Jan 2020: 2010) and MIPS 24 µm observations(0.2 mJy, which are limited by calibration uncertainties of 5%, Gautier et al. ... Fν,? [mJy]. 0.21 0.22 0.23 0.24 0.25. MJD 58350. 1. 0.
  7. Mon. Not. R. Astron. Soc. 000, 1–21 (2002) Printed ...

    https://people.ast.cam.ac.uk/~wyatt/kmkm20.pdf
    8 Jul 2020: 0.00. 0.04. 0.08. 0.12. 0.16. 0.20. 0.24. Fν. [mJy. /bea. m]. ... 72 75 78 81. R0. 0.08. 0.16. 0.24. 0.32. h. 0.51.
  8. MNRAS 000, 1–14 (2020) Preprint 8October 2020 Compiled…

    https://people.ast.cam.ac.uk/~wyatt/xkwy20.pdf
    8 Oct 2020: Themasses from the two age solutionsare consistentwithin 1𝜎 (see 2). is because the reflex motion due to a wide-orbiting companion isessentially linear and constant on the 24.25 yr
  9. MNRAS 000, 1–11 (2020) Preprint 26November 2020 Compiled…

    https://people.ast.cam.ac.uk/~wyatt/zcac20.pdf
    26 Nov 2020: Sz65B (Sz66) 234.8656 -34.7715 II 155 983 97 0.46 0.21 Res 0.1 L2MASS J15430624-3920194B 235.7760 -39.3387 III 165 24 -16 0.99 - ND <
  10. Draft version March 10, 2020Typeset using LATEX twocolumn style ...

    https://people.ast.cam.ac.uk/~wyatt/edhm20.pdf
    10 Mar 2020: Draft version March 10, 2020Typeset using LATEX twocolumn style in AASTeX62. The HOSTS survey for exozodiacal dust: Observational results from the complete survey. Ertel, S.,1, 2 Defrère, D.,3 Hinz, P.,2 Mennesson, B.,4 Kennedy, G. M.,5 Danchi, W.
  11. MNRAS 000, 1–19 (2019) Preprint 20 December 2019 Compiled ...

    https://people.ast.cam.ac.uk/~wyatt/aght19.pdf
    17 Jan 2020: Thus we uniformly (re)derive the inclinations of 24 dipperdiscs resolved with (sub-)mm interferometry from ALMA. ... 88 2016.1.00545.S. 203770559d J16250208-2459323 WSB 19B. 33.214.9 C18 43.74.24.5 12665 2016.1.00545.S.
  12. MNRAS 000, 1–20 (2020) Preprint 18 August 2020 Compiled ...

    https://people.ast.cam.ac.uk/~wyatt/kw20.pdf
    18 Aug 2020: 8.1 1.6 23 100.0 100.0 24.3 2.1e-03 7.9e-02 1.2e03 4.1e03 0.3 5.5. ... 24). purposes, as we only wish to demonstrate that the Kuiperbelt is not affected by the mass problem.
  13. Draft version June 29, 2020Typeset using LATEX twocolumn style ...

    https://people.ast.cam.ac.uk/~wyatt/mdwm20.pdf
    29 Jun 2020: 1984). It is now. recognised that at least 24% of A-type stars harbour.
  14. MNRAS 000, 1–22 (2019) Preprint 30 January 2020 Compiled ...

    https://people.ast.cam.ac.uk/~wyatt/mfhk20.pdf
    30 Jan 2020: 2007b) to fit the infrared excess evolution at 24 and70 µm in nearby A stars (Rieke et al. ... Wyatt et al. used the distri-bution of observed 24 and 70 µm excess as a function ofage to constrain the initial distribution of disc radii (ap-proximating
  15. MNRAS 000, 1-30 (2020) Preprint 12 October 2020 Compiled ...

    https://people.ast.cam.ac.uk/~wyatt/swmn20.pdf
    15 Oct 2020: vimppξq “b. v2esc. ξvpl˘2. (24). These test impactor properties, labelled by the outcome they haveon the atmosphere, are shown in Table 1.

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