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Information about sources of funding available to postgraduates at Cambridge.
www.student-funding.cam.ac.uk/
Cambridge Bursary Scheme
The Bursary is free financial support of generally up to £3,500 a year for full-time undergraduate students, to help with your Cambridge fees or living costs. Like a scholarship or grant, the payment is non-refundable – you don’t need to pay it back.
Higher amounts are available for medical students in their clinical years, independent students including care leavers, and students who were eligible for free school meals.
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The role of impacts on the atmospheres on the moons of outer giants
https://people.ast.cam.ac.uk/~wyatt/sw21.pdf14 Feb 2022: In this work, we follow the approach described in. MNRAS 509, 345–366 (2022). ... ambridge user on 14 February 2022. Impacts and atmospheres of the outer giant’s moons 349. -
MNRAS 000, 1–22 (2021) Preprint 29 September 2023 Compiled ...
https://people.ast.cam.ac.uk/~wyatt/yw23.pdf29 Sep 2023: 2015; Han et al. 2022) as well as N-bodysimulations of mutual planetesimal scattering (Ida & Makino 1992),though in our model a companion star is perturbing the disc so thecharacteristic eccentricity ... 2021). Γ = 2.92(𝐿𝐿. )0.13, (26). and, for -
DRAFT VERSION OCTOBER 25, 2022Typeset using LATEX default style ...
https://people.ast.cam.ac.uk/~wyatt/hmsu22.pdf25 Oct 2022: Accepted on October 21 2022). ABSTRACTWe present Atacama Large Millimeter Array (ALMA) observations of the young, gas-rich debris. ... 2022) that allows to create disk models and uses RADMC-3D 3 (Dullemond et al. -
Draft version March 24, 2022Typeset using LATEX twocolumn style ...
https://people.ast.cam.ac.uk/~wyatt/hycd22.pdf22 Mar 2024: Received 21 Jan 2022; Revised 10 Mar 2022; Accepted 21 Mar 2022). -
DRAFT VERSION JULY 17, 2023Typeset using LATEX twocolumn style ...
https://people.ast.cam.ac.uk/~wyatt/srw23.pdf22 Mar 2024: 2018; Marino 2022, and references therein).This is so because millimeter observations trace mm-sizedgrains that are largely unaffected by non-gravitational radi-ation forces (Burns et al. ... 2022)). 30 50 70 90 110 130 150-2. -1.5. -1. -0.5. 0. -
MNRAS 000, 000–000 (2018) Preprint 21 February 2019 Compiled ...
https://people.ast.cam.ac.uk/~wyatt/mphp19.pdf21 Feb 2019: MNRAS 000, 000–000 (2018) Preprint 21 February 2019 Compiled using MNRAS LATEX style file v3.0. Asymmetric mid-plane gas in ALMA images of HD 100546. J. M. Miley1?, O. Panić 1, T. J. Haworth 2, I. Pascucci 3, M. Wyatt 4, C. Clarke 4,. A. M. S. -
DRAFT VERSION MAY 24, 2022Typeset using LATEX twocolumn style ...
https://people.ast.cam.ac.uk/~wyatt/hcrs22.pdf24 May 2022: 2022), including obtaining direct spec-troscopy for widely separated companions. NIRISS (Doyonet al. ... 2011; Ruane et al. 2019; Sanghi et al. 2022),and labelled “ADIRDI” in the figure. -
Astronomy & Astrophysics manuscript no. LIFE_paper_1_FINAL_EDITED …
https://people.ast.cam.ac.uk/~wyatt/qofk22.pdf18 Apr 2022: Astronomy & Astrophysics manuscript no. LIFE_paper_1_FINAL_EDITED ESO 2022April 11, 2022. Large Interferometer For Exoplanets (LIFE):. ... vided in Dannert et al. (2022), but we refer the reader to Defrèreet al. -
cv.dvi
https://people.ast.cam.ac.uk/~gpe/cv.pdf24 Jan 2012: R236] Planck Early Results: The Planck mission, Planck Collaboration, 2011,arXiv:1101.2022. 6. -
MNRAS 000, 1–24 (2020) Preprint 7 July 2020 Compiled ...
https://people.ast.cam.ac.uk/~wyatt/xw20.pdf7 Jul 2020: MNRAS 000, 1–24 (2020) Preprint 7 July 2020 Compiled using MNRAS LATEX style file v3.0. Evidence for a high mutual inclination between the coldJupiter and transiting super Earth orbiting π Men. Jerry W. Xuan,? and Mark C. WyattInstitute of -
The Astrophysical Journal, 701:2019–2032, 2009 August 20…
https://people.ast.cam.ac.uk/~wyatt/lcwm09.pdf1 Aug 2012: 2022 LISSE ET AL. Vol. 701. Figure 4. Spitzer IRS emissivity spectrum of the HD172555 circumstellar excess, and best-fit compositional model. -
https://people.ast.cam.ac.uk/~optics/dazle/sky-data/sky_h20_absorption…
https://people.ast.cam.ac.uk/~optics/dazle/sky-data/sky_h20_absorption.txt16 Jun 2015: 0.2022 0.1240 0.0794 0.0523 0.0351 713. 0.2309 0.1451 0.0949 0.0636 0.0434 714. -
arX iv:0 911. 3426 v1 [ astr o-ph .SR ...
https://people.ast.cam.ac.uk/~wyatt/pgdm09.pdf19 Nov 2009: arX. iv:0. 911. 3426. v1 [. astr. o-ph. SR. ] 1. 8 N. ov 2. 009. Mon. Not. R. Astron. Soc. 000, 1–? (2009) Printed 19 November 2009 (MN LATEX style file v2.2). Target selection for the SUNS and DEBRIS surveys for. debris discs in the solar
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