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Mon. Not. R. Astron. Soc. 000, 1–17 (2002) Printed ...
https://people.ast.cam.ac.uk/~wyatt/pwk13.pdf29 Oct 2013: Le Bouquin et al. 2009; Watson et al.2011; Kennedy et al. -
arX iv:1 701. 0656 8v1 [as tro- ph.S R] ...
https://people.ast.cam.ac.uk/~wyatt/kkpr17.pdf5 May 2017: arX. iv:1. 701. 0656. 8v1. [as. tro-. ph.S. R]. 23. Jan. 2017. rsos.royalsocietypublishing.org. Research. Article submitted to journal. Subject Areas:. astrophysics, extrasolar planets, stars. Keywords:. variable stars, protoplanetary disks,. debris -
arX iv:1 403. 6186 v1 [ astr o-ph .EP ...
https://people.ast.cam.ac.uk/~wyatt/mmek14.pdf2 Jul 2014: arX. iv:1. 403. 6186. v1 [. astr. o-ph. EP. ] 24. Mar. 201. 4Astronomy & Astrophysicsmanuscript no. dunes˙debris˙exoplanets˙v18 c ESO 2014March 26, 2014. Correlations between the stellar, planetary and debris componentsof exoplanet systems -
Observations, Modeling and Theory of Debris Disks Brenda C. ...
https://people.ast.cam.ac.uk/~wyatt/mkwb14.pdf7 Jan 2014: Observations, Modeling and Theory of Debris Disks. Brenda C. MatthewsNational Research Council of Canada – Herzberg Astronomy & Astrophysics. Alexander V. KrivovFriedrich-Schiller-Universität Jena. Mark C. WyattUniversity of Cambridge. Geoffrey -
arX iv:1 610. 0071 4v1 [as tro- ph.E P] ...
https://people.ast.cam.ac.uk/~wyatt/wbjm16.pdf7 Oct 2016: arX. iv:1. 610. 0071. 4v1. [as. tro-. ph.E. P] 3. Oct. 201. 6. MNRAS 000, 1–25 (2016) Preprint 5 October 2016 Compiled using MNRAS LATEX style file v3.0. How to design a planetary system for different scattering. outcomes: giant impact sweet spot, -
https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_090923.txt
https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_090923.txt28 Sep 2009: MJI is in communication with Watson Varricatt regarding the low light level non-linearity tests and also a revisit of the normal non-linearity tests. ... Watson and MJI will also be comparing dome flats with twilight sky flats. -
ESO Public Surveys Proposal Form Phase 1 1 Title: ...
https://people.ast.cam.ac.uk/~rgm/vhs/v4/PS-VHS-v4p0.pdf5 Jun 2007: Venemans(Cam),F. Walter(MPIA), N. Walton(Cam), S. Warren(IC), M. Watson(Leic), N. Webb(Toulouse),C. Wolf(Oxf), H. -
Mon. Not. R. Astron. Soc. 000, 1–20 (2010) Printed ...
https://people.ast.cam.ac.uk/~wyatt/cwds11.pdf5 Jul 2011: Mon. Not. R. Astron. Soc. 000, 1–20 (2010) Printed July 5, 2011 (MN LATEX style file v2.2). Multi-Wavelength Modelling of the β Leo Debris Disc: 1, 2 or 3planetesimal populations? L J Churcher 1†, M.C. Wyatt1, G. Duchêne2,3, B. Sibthorpe4, G. -
https://people.ast.cam.ac.uk/~xmmssc/xidops/xidobs/ukirt0210/almanac.t…
https://people.ast.cam.ac.uk/~xmmssc/xidops/xidobs/ukirt0210/almanac.txt25 Sep 2002: ac.uk To: Weimin Yuan wmy@ast.cam.ac.uk, Jonathan Tedds jat@star.le.ac.uk, Mike Watson mgw@star.le.ac.uk Subject: Almanac Info for Dates of UKIRT -
Publications of the Astronomical Society of Australia (PASA)doi:…
https://people.ast.cam.ac.uk/~wyatt/khna21.pdf23 Nov 2021: Publications of the Astronomical Society of Australia (PASA)doi: 10.1017/pas.2021.xxx. The formation of planetary systems with SPICA. Kamp, I.1, Honda, M.2, Nomura, H.3, Audard, M.4, Fedele, D.5, Waters, L.B.F.M.6,7, Aikawa,Y.8, Banzatti, A.9, Bowey,
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