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  1. Results that match 2 of 3 words

  2. MNRAS 000, 1–14 (2018) Preprint 8 January 2019 Compiled ...

    https://people.ast.cam.ac.uk/~wyatt/mybf19.pdf
    8 Jan 2019: Middle:Comparison between opposite wedges with a mean PA of 45 (NE,green) and 225 (SW, orange). ... 12 au for the topand bottom panels and 20 au for the middle panel approximately.
  3. mnr_20522_LR

    https://people.ast.cam.ac.uk/~wyatt/vw12.pdf
    30 Oct 2012: 5). In con-trast, the initial conditions which lead to instability for the η =0.5 simulations (middle panel of Fig. ... The middle and bottom panels of Fig. 10 indicate that the frac-tion of bodies which escape does not necessarily scale with a0;.
  4. MNRAS 000, 1–12 (2015) Preprint 12 May 2016 Compiled ...

    https://people.ast.cam.ac.uk/~wyatt/mmsw16.pdf
    17 May 2016: The marginaliseddistributions ofr, h = H/r and r0 are presented in the top, middle right andbottom right panel, respectively. ... Left middle panel: marginaliseddistribution of MCO and r0. Left bottom panel: marginalised distribution ofr and MCO.
  5. Project Reassessment Start Date

    https://people.ast.cam.ac.uk/~optics/cirsi/docs/review/review.doc
    16 Jun 2015: 6.2.28 Multiplexor Electrical tests GOTOBUTTON _Toc361307210 PAGEREF _Toc361307210 34. 6.2.29 Install engineering grade detector and test GOTOBUTTON _Toc361307211 PAGEREF _Toc361307211 34. ... 6.2.35 Tests with 4100 standard system GOTOBUTTON
  6. DRAFT VERSION OCTOBER 25, 2022Typeset using LATEX default style ...

    https://people.ast.cam.ac.uk/~wyatt/hmsu22.pdf
    25 Oct 2022: DRAFT VERSION OCTOBER 25, 2022Typeset using LATEX default style in AASTeX63. ALMA Observations of the HD 110058 debris diskANTONIO S. HALES,1,2 SEBASTIÁN MARINO,3,4 PATRICK D. SHEEHAN,5,2 SILVIO ULLOA,6 SEBASTIÁN PÉREZ,7,8,9 LUCA MATRÀ,10,11.
  7. arX iv:1 801. 0542 9v1 [as tro- ph.E P] ...

    https://people.ast.cam.ac.uk/~wyatt/kmmp18.pdf
    18 Jan 2018: These tests were however not exhaustive. Formally, we can use the Schwarz criterion (Bayesian In-. ... formation Criterion, or BIC) to test which among our models. should be preferred (Schwarz 1978).
  8. Circumstellar discs: What will be next? Quentin Kral, Cathie ...

    https://people.ast.cam.ac.uk/~wyatt/kcw17.pdf
    13 Nov 2017: Currently efforts to test this scenario observationallyare in their infancy and over-lap with efforts to test models for photoevaporation(see below).
  9. mnr_21298_LR

    https://people.ast.cam.ac.uk/~wyatt/wksm12.pdf
    7 Nov 2012: left – 70 µm; top middle – 100 µm; top right – 160 µm; bottom left – 250 µm; bottom middle – 350 µm and bottom right – 500 µm. ... 3 (middle) indicating a double-lobed structure. Fitting this as two Gaussians gives 8.0 mJy forthe
  10. MNRAS 000, 1–11 (2018) Preprint 27 June 2018 Compiled ...

    https://people.ast.cam.ac.uk/~wyatt/sbbc18.pdf
    31 Jul 2018: E-mail: schaefer@lsu.edu. 1 INTRODUCTION. The star KIC 8462852 (Boyajian’s Star) is a perfectly or-dinary, isolated, and middle-aged F3 main sequence star in. ... This demonstrates that thesecular decline from 1890 until the end of the Kepler run
  11. 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.

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